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Message-ID: <5C540AC6.9040806@posteo.de>
Date: Fri, 01 Feb 2019 10:00:54 +0100
From: DK7FC <selberdenken@posteo.de>
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To: rsgb_lf_group@blacksheep.org
References: <1UTCZw4Jzr.F7dZYpniNns@optiplex980-pc> <5C52F3F6.5080906@posteo.de> <D9D627C726E24B02BF4C53DAD9F06AE8@DELL4>
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 Content preview:  Hi Jay, Joe, LF, Good copy of VO1NA here as well, see attachment.
    73, Stefan 
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Subject: Re: LF: VO1NA EbNaut
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Hi Jay, Joe, LF,

Good copy of VO1NA here as well, see attachment.

73, Stefan



Am 31.01.2019 16:34, schrieb jrusgrove@comcast.net:
> Stefan
> VO1NA 137477 8K19A CRC16 Symper 3.0 Char 7
> Jay W1VD
>
>     ----- Original Message -----
>     *From:* DK7FC <mailto:selberdenken@posteo.de>
>     *To:* rsgb_lf_group@blacksheep.org
>     <mailto:rsgb_lf_group@blacksheep.org>
>     *Sent:* Thursday, January 31, 2019 8:11 AM
>     *Subject:* Re: LF: VO1NA EbNaut
>
>     Jay, Joe, LF,
>
>     Interesting. And thanks for reminding that Joe has been on the
>     air. What were the parameters of the transmission? I can't find
>     the message announcement...
>
>     73, Stefan
>
>
>
>     Am 31.01.2019 12:29, schrieb jrusgrove@comcast.net:
>>     Joe & EbNaut-eers
>>     Had not checked in on VO1NA LF EbNaut for some time so decided to
>>     have a look. Immediately noticed the unusually large spread
>>     between car Eb/N0 and Eb/N0. Inspection of the phase plots
>>     revealed the problem ... there were two minute periods of
>>     'disruption' on an otherwise clean phase plots. By matching up
>>     the observed 'disruption' times with the WSPR database I was able
>>     to determine the interfering signal was WSPR and belonged to
>>     K3RWR (one of the strongest LF signals at this
>>     location). Considering K3RWR's signal is outside the SpecLab FFT
>>     bandwidth the problem is most likely happening at the receiver
>>     ... a Cubic SMA-2400. AGC was turned on at the time to prevent
>>     audio distortion from the stronger WSPR signals. When time
>>     permits I'll run another test with AGC turned off.
>>     Last night's reception list:
>>     0130 Rank 0 car Eb/N0 16.2 Eb/N0   8.9 *******
>>     0200 Rank 0 car Eb/N0 20.1 Eb/N0 12.3 **VO1NA
>>     0230 Rank 0 car Eb/N0 29.1 Eb/N0 15.3 *******
>>     0300 Rank 0 car Eb/N0 27.9 Eb/N0 15.6 **VO1NA
>>     0330 Rank 0 car Eb/N0 28.0 Eb/N0 13.3 *******
>>     0400 Rank 0 car Eb/N0 28.7 Eb/N0 11.9 **VO1NA
>>     Phase plot below.
>>     Jay W1VD
>

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<body bgcolor="#ffffff" text="#000000">
Hi Jay, Joe, LF,<br>
<br>
Good copy of VO1NA here as well, see attachment.<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 31.01.2019 16:34, schrieb <a class="moz-txt-link-abbreviated" href="mailto:jrusgrove@comcast.net:">jrusgrove@comcast.net:</a>
<blockquote cite="mid:D9D627C726E24B02BF4C53DAD9F06AE8@DELL4"
 type="cite">
  <meta http-equiv="Content-Type" content="text/html; charset=UTF-8">
  <meta content="MSHTML 6.00.2900.5512" name="GENERATOR">
  <div><font face="Arial" size="2">Stefan</font></div>
  <div> </div>
  <div><font face="Arial" size="2">VO1NA 137477 8K19A CRC16 Symper 3.0
Char 7</font></div>
  <div> </div>
  <div><font face="Arial" size="2">Jay W1VD</font></div>
  <blockquote dir="ltr"
 style="border-left: 2px solid rgb(0, 0, 0); padding-right: 0px; padding-left: 5px; margin-left: 5px; margin-right: 0px;">
    <div
 style="font-family: arial; font-style: normal; font-variant: normal; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adjust: none; font-stretch: normal; -x-system-font: none;">-----
Original Message ----- </div>
    <div
 style="background: rgb(228, 228, 228) none repeat scroll 0% 0%; -moz-background-clip: border; -moz-background-origin: padding; -moz-background-inline-policy: continuous; font-family: arial; font-style: normal; font-variant: normal; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adjust: none; font-stretch: normal; -x-system-font: none;"><b>From:</b>
    <a moz-do-not-send="true" title="selberdenken@posteo.de"
 href="mailto:selberdenken@posteo.de">DK7FC</a> </div>
    <div
 style="font-family: arial; font-style: normal; font-variant: normal; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adjust: none; font-stretch: normal; -x-system-font: none;"><b>To:</b>
    <a moz-do-not-send="true" title="rsgb_lf_group@blacksheep.org"
 href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org</a>
    </div>
    <div
 style="font-family: arial; font-style: normal; font-variant: normal; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adjust: none; font-stretch: normal; -x-system-font: none;"><b>Sent:</b>
Thursday, January 31, 2019 8:11 AM</div>
    <div
 style="font-family: arial; font-style: normal; font-variant: normal; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adjust: none; font-stretch: normal; -x-system-font: none;"><b>Subject:</b>
Re: LF: VO1NA EbNaut</div>
    <div><br>
    </div>
Jay, Joe, LF,<br>
    <br>
Interesting. And thanks for reminding that Joe has been on the air.
What were the parameters of the transmission? I can't find the message
announcement... <br>
    <br>
73, Stefan<br>
    <br>
    <br>
    <br>
Am 31.01.2019 12:29, schrieb <a moz-do-not-send="true"
 class="moz-txt-link-abbreviated" href="mailto:jrusgrove@comcast.net:">jrusgrove@comcast.net:</a>
    <blockquote cite="mid:1UTCZw4Jzr.F7dZYpniNns@optiplex980-pc"
 type="cite">
      <style type="text/css">BODY {
	MARGIN: 0.7em
}
BODY.OECFntDef {
	FONT-SIZE: 10pt; FONT-FAMILY: Arial,"Segoe UI",Tahoma,Verdana,Helvetica,sans-serif
}
BODY.OECFntDef DIV {
	FONT-SIZE: 10pt; FONT-FAMILY: Arial,"Segoe UI",Tahoma,Verdana,Helvetica,sans-serif
}
      </style>
      <meta content="MSHTML 11.00.9600.18450" name="GENERATOR">
      <div>Joe &amp; EbNaut-eers</div>
      <div> </div>
      <div>Had not checked in on VO1NA LF EbNaut for some time so
decided to have a look. Immediately noticed the unusually large spread
between car Eb/N0 and Eb/N0. Inspection of the phase plots revealed the
problem ... there were two minute periods of 'disruption' on an
otherwise clean phase plots. By matching up the observed 'disruption'
times with the WSPR database I was able to determine the interfering
signal was WSPR and belonged to K3RWR (one of the strongest LF signals
at this location). Considering K3RWR's signal is outside the SpecLab
FFT bandwidth the problem is most likely happening at the receiver ...
a Cubic SMA-2400. AGC was turned on at the time to prevent audio
distortion from the stronger WSPR signals. When time permits I'll run
another test with AGC turned off.</div>
      <div> </div>
      <div>Last night's reception list:     </div>
      <div> </div>
      <div>0130 Rank 0 car Eb/N0 16.2 Eb/N0   8.9 *******</div>
      <div>
      <div>0200 Rank 0 car Eb/N0 20.1 Eb/N0 12.3 **VO1NA</div>
      <div>
      <div>0230 Rank 0 car Eb/N0 29.1 Eb/N0 15.3 *******</div>
      <div>0300 Rank 0 car Eb/N0 27.9 Eb/N0 15.6 **VO1NA</div>
      <div>0330 Rank 0 car Eb/N0 28.0 Eb/N0 13.3 *******</div>
      <div>0400 Rank 0 car Eb/N0 28.7 Eb/N0 11.9 **VO1NA</div>
      <div> </div>
      <div>Phase plot below.</div>
      <div> </div>
      <div><img alt="" src="cid:part1.07050802.01020301@posteo.de"
 align="baseline" border="0" hspace="0"></div>
      <div> </div>
      <div>Jay W1VD</div>
      </div>
      </div>
    </blockquote>
  </blockquote>
</blockquote>
</body>
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 Content preview:  On 31/01/2019 21:30, DK7FC wrote: > Hello Nick, > > Thank
   you. Good to know that it works for someone. And you're also using > a NEO-7M,
    right? > /dev/ttyACM0, is that an usb-to-serial converter? I'm [...] 
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On 31/01/2019 21:30, DK7FC wrote:
> Hello Nick,
> 
> Thank you. Good to know that it works for someone. And you're also using
> a NEO-7M, right?
> /dev/ttyACM0, is that an usb-to-serial converter? I'm using /dev/AMA0,
> which is the TXD/RXD pins on the GPIO port. So i just need to use 4
> wires and connect the module to the Raspi...
> I could try to use the usb-to-serial adapter connected to the Raspi but
> that is a rather uncomfortable work-arround and even more power
> consuming...
> 
> ...would like to try to transmit EbNaut on 137 kHz directly from such a
> module.
> 
> 73, Stefan
> 

Stephan,

Yes, NEO 7M, and yes a usb-rs232 (on a desktop not a Pi)

Good luck, it is also on my list ...

:-)

Regards

Nick
M0HGU
-- 
Worlds of belief, she [Susan] thought. Just like oysters. A little piece
of shit gets in and then a pearl grows around it.
(Hogfather)
09:30:02 up 13 days, 21:24, 8 users, load average: 1.84, 0.81, 0.63

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From: Rik Strobbe <rik.strobbe@kuleuven.be>
To: "rsgb-lf-group@groups.io" <rsgb-lf-group@groups.io>
CC: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>,
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Thread-Topic: [rsgb-lf-group] SlowJT9 update (v0.9.15.0)
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 Content preview:  Hello Les, all, WX permitting I will be QRV on Saturday (here
    in Europe) starting 5h30 UTC. I will monitor JT9, JT9-2 and JT9-5 all night.
    73, Rik ON7YD - OR7T 
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Subject: LF: Re: [rsgb-lf-group] SlowJT9 update (v0.9.15.0)
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Hello Les, all,

WX permitting I will be QRV on Saturday (here in Europe) starting 5h30 UTC.
I will monitor JT9, JT9-2 and JT9-5 all night.

73, Rik   ON7YD - OR7T

________________________________________
Van: rsgb-lf-group@groups.io <rsgb-lf-group@groups.io> namens Les Peters, N1SV <n1sv@comcast.net>
Verzonden: donderdag 31 januari 2019 23:38
Aan: rsgb-lf-group@groups.io
CC: rsgb_lf_group@blacksheep.org; 600MRG@mailman.qth.net
Onderwerp: Re: [rsgb-lf-group] SlowJT9 update (v0.9.15.0)

I plan to be on 475 Friday and Saturday so yes would like to try!

Les, N1SV
> On Jan 31, 2019, at 5:04 PM, Rik Strobbe <rik.strobbe@kuleuven.be> wrote:
>
> Hi Paul, all,
>
> SlowJT9 vs WSJT-X: as I mentioned it was pure luck that SlowJT9 performed better that night.
> But as the only reason I can think of is a small timing difference between both it might be worth to time-shift the incoming audio by small steps, then try to decode each step nd take a "best off" as result.
>
> Frequency conversion: I will investigate that furher. Anyway, if I implement this it will be optional (can be switched off).
>
> For the moment WX is rather bad here, so the antenna is lowered. But in a few days, when the  WX permits I would like to try some TA QSO's on 475 kHz using the slower JT9 modes.
> Any takers at the other side of the pond?
> I worked Paul, N1BUG and Eric, NO3M, mid February last year.
>
> 73, Rik  ON7YD - OR7T
>
> ________________________________________
> Van: rsgb-lf-group@groups.io <rsgb-lf-group@groups.io> namens N1BUG <paul@n1bug.com>
> Verzonden: donderdag 31 januari 2019 21:43
> Aan: rsgb-lf-group@groups.io; rsgb_lf_group@blacksheep.org; 600MRG@mailman.qth.net
> Onderwerp: Re: [rsgb-lf-group] SlowJT9 update (v0.9.15.0)
>
> Hello Rik, all,
>
> Two comments, see below.
>
>> Interestingly Rik's SlowJT9 which was running in parallel,
>> managed to decode a couple of more transmissions than WSJT-X."
>
> I have seen this work both ways. Sometimes SlowJT9 will decode
> something WSJT-X does not. Other times WSJT-X will decode something
> SlowJT9 does not. Usually they are equal.
>
>> 2. Add optional internal frequency conversion to allow reception
>> at higher frequencies I have done some preliminary tests (based
>> on the code snippet Wolf, DL4YHF, sent me) and it seems to work
>> fine. But I am not sure that it will be very useful as frequency
>> conversion will not increase the usable frequeny range, but just
>> shit it. Eg: now JT9-10 can be received from 100 Hz to 415 Hz
>> audio. After USB downconversion with a 1 kHz carrier the range
>> will be 1100 Hz to 1415 Hz. The only reason I can think of to
>> want frequency conversion is if you use a fixed frequency (ofen
>> 800Hz) CW filter, so you can fit the JT9-5 or JT9-10 frequency
>> range into the filter passband. But this downconversion requires
>> a Hilbert transform (90 degrees all pass filter) that never can
>> be perfect and this will cause some distortion (in particular at
>> the lower and of the passband). So before I start the effort to
>> implement this in SlowJT9 I would like to know if there is an
>> audience for it.
>
> I think there is justification for it on 2200m if it comes without
> too high cost in lost sensitivity. Some people cannot easily tune
> antennas down to 136.4 or so. But if we operate at 137.x then
> listening stations must adjust their receiver because the usual
> 136.000 'dial' frequency will not allow receiving JT9-5 or JT9-10.
> This is not the usual setting for most who also want to monitor WSPR
> or other modes. For pre-arranged QSOs this will not matter, but for
> calling CQ it is good to operate where we can be heard without
> special receiver settings.
>
> However, if this feature comes with significant loss of decoding
> sensitivity, then I would vote to stay as we are.
>
> 73,
> Paul N1BUG
>
>
>
>
>
>


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From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Fri, 1 Feb 2019 21:55:13 +0100
Message-ID: <CANA3B6Vv89cy_LEii6wyBzJ9M-U4aJAp3dyBTyTjdTf_L_oSOw@mail.gmail.com>
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 Content preview:  LF, Tonite I've scheduled some transmissions with these parameters:
    *QRG: 137546.2 Hz* *Coding 8K19A* *CRC 14* *3 sec./sym.* *7 characters* *Duration:
    29' 36"* *Every 30 min., 1st on 2100z, last on 0800z* 
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  pts rule name              description
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                             no trust
                             [2a00:1450:4864:20:0:0:0:533 listed in]
                             [list.dnswl.org]
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  0.0 FREEMAIL_FROM          Sender email is commonly abused enduser mail
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Subject: LF: EbNaut on 137546.2 Hz
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--000000000000b4266f0580db5c72
Content-Type: text/plain; charset="UTF-8"

LF,

Tonite I've scheduled some transmissions with these parameters:

*QRG: 137546.2 Hz*
*Coding 8K19A*
*CRC 14*
*3 sec./sym.*
*7 characters*
*Duration: 29' 36"*
*Every 30 min., 1st on 2100z, last on 0800z*

Reports are welcome.


All the best

73 de Riccardo IW4DXW

--000000000000b4266f0580db5c72
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"auto"><div dir=3D"auto"><br></div><div dir=3D"auto">LF,</div><d=
iv dir=3D"auto"><br></div><div dir=3D"auto">Tonite I&#39;ve scheduled some =
transmissions with these parameters:</div><div dir=3D"auto"><br></div><div =
dir=3D"auto"><b>QRG: 137546.2 Hz</b></div><div dir=3D"auto"><b>Coding 8K19A=
</b></div><div dir=3D"auto"><b>CRC 14</b></div><div dir=3D"auto"><b>3 sec./=
sym.</b></div><div dir=3D"auto"><b>7 characters</b></div><div dir=3D"auto">=
<b>Duration: 29&#39; 36&quot;</b></div><div dir=3D"auto"><b>Every 30 min., =
1st on 2100z, last on 0800z</b></div><div dir=3D"auto"><br></div><div dir=
=3D"auto">Reports are welcome.</div><div dir=3D"auto"><br></div><div dir=3D=
"auto"><br></div><div dir=3D"auto">All the best</div><div dir=3D"auto"><br>=
</div><div dir=3D"auto">73 de Riccardo IW4DXW</div><div dir=3D"auto"><br></=
div></div>

--000000000000b4266f0580db5c72--

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 Content preview:  Riccardo, Sorry, but no decodes overnight. 73, Rob - K3RWR
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Subject: Re: LF: EbNaut on 137546.2 Hz
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------=_NextPart_000_000C_01D4BAF3.48D40220
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	charset="utf-8"
Content-Transfer-Encoding: quoted-printable

Riccardo,

Sorry, but no decodes overnight.

73,
Rob - K3RWR

From: Riccardo Zoli=20
Sent: Friday, February 01, 2019 8:55 PM
To: LF Group=20
Subject: LF: EbNaut on 137546.2 Hz


LF,

Tonite I've scheduled some transmissions with these parameters:

QRG: 137546.2 Hz
Coding 8K19A
CRC 14
3 sec./sym.
7 characters
Duration: 29' 36"
Every 30 min., 1st on 2100z, last on 0800z

Reports are welcome.


All the best

73 de Riccardo IW4DXW

------=_NextPart_000_000C_01D4BAF3.48D40220
Content-Type: text/html;
	charset="utf-8"
Content-Transfer-Encoding: quoted-printable

<HTML><HEAD></HEAD>
<BODY dir=3Dltr>
<DIV dir=3Dltr>
<DIV style=3D"FONT-SIZE: 12pt; FONT-FAMILY: 'Calibri'; COLOR: #000000">
<DIV>Riccardo,</DIV>
<DIV>&nbsp;</DIV>
<DIV>Sorry, but no decodes overnight.</DIV>
<DIV>&nbsp;</DIV>
<DIV>73,</DIV>
<DIV>Rob - K3RWR</DIV>
<DIV=20
style=3D'FONT-SIZE: small; TEXT-DECORATION: none; FONT-FAMILY: =
"Calibri"; FONT-WEIGHT: normal; COLOR: #000000; FONT-STYLE: normal; =
DISPLAY: inline'>
<DIV style=3D"FONT: 10pt tahoma">
<DIV>&nbsp;</DIV>
<DIV style=3D"BACKGROUND: #f5f5f5">
<DIV style=3D"font-color: black"><B>From:</B> <A=20
title=3Driccardozoli80@gmail.com>Riccardo Zoli</A> </DIV>
<DIV><B>Sent:</B> Friday, February 01, 2019 8:55 PM</DIV>
<DIV><B>To:</B> <A title=3Drsgb_lf_group@blacksheep.org>LF Group</A> =
</DIV>
<DIV><B>Subject:</B> LF: EbNaut on 137546.2 Hz</DIV></DIV></DIV>
<DIV>&nbsp;</DIV></DIV>
<DIV=20
style=3D'FONT-SIZE: small; TEXT-DECORATION: none; FONT-FAMILY: =
"Calibri"; FONT-WEIGHT: normal; COLOR: #000000; FONT-STYLE: normal; =
DISPLAY: inline'>
<DIV>
<DIV>&nbsp;</DIV>
<DIV>LF,</DIV>
<DIV>&nbsp;</DIV>
<DIV>Tonite I've scheduled some transmissions with these =
parameters:</DIV>
<DIV>&nbsp;</DIV>
<DIV><B>QRG: 137546.2 Hz</B></DIV>
<DIV><B>Coding 8K19A</B></DIV>
<DIV><B>CRC 14</B></DIV>
<DIV><B>3 sec./sym.</B></DIV>
<DIV><B>7 characters</B></DIV>
<DIV><B>Duration: 29' 36"</B></DIV>
<DIV><B>Every 30 min., 1st on 2100z, last on 0800z</B></DIV>
<DIV>&nbsp;</DIV>
<DIV>Reports are welcome.</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>All the best</DIV>
<DIV>&nbsp;</DIV>
<DIV>73 de Riccardo IW4DXW</DIV>
<DIV>&nbsp;</DIV></DIV></DIV></DIV></DIV></BODY></HTML>

------=_NextPart_000_000C_01D4BAF3.48D40220--


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Date: Sat, 2 Feb 2019 12:46:21 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
Message-ID: <1853806007.1845781.1549111581841@mail.yahoo.com>
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 Content preview:  Think I have tamed my u-blox LEA-6T module well enough, so
    will try to send an EbNaut test this afternoon: Frequency 137536 Hz, Start
    times: 13:00 and 13:30 UT, 6 char, 3 sec symbols,  8k19A, crc 16. 
 Content analysis details:   (0.0 points, 5.0 required)
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Subject: LF: EbNaut test from u-blox module
Content-Type: multipart/alternative; 
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Sender: owner-rsgb_lf_group@blacksheep.org
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------=_Part_1845780_1410746881.1549111581840
Content-Type: text/plain; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

Think I have=C2=A0tamed my u-blox LEA-6T module well enough, so will try to=
=C2=A0send an EbNaut test this afternoon:

Frequency 137536 Hz,
Start times: 13:00 and 13:30 UT,
6 char, 3 sec symbols, =C2=A08k19A, crc 16.

Experimental scripts to control the timepulse-2 output are at=20
http://df6nm.bplaced.net/LF/u-blox_ebnaut/=C2=A0
and I intend to=C2=A0explain some details later this weekend.

Best 73,
Markus (DF6NM)

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Do, 31. Jan. 2019 22:32
Betreff: Re: LF: NEO-7M as a frequency source

...
...would like to try to transmit EbNaut on 137 kHz directly from such a=20
module.

73, Stefan



------=_Part_1845780_1410746881.1549111581840
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"300">Think I have&nbsp;tamed my u-blox LEA-6T mod=
ule well enough, so will try to&nbsp;send an EbNaut test this afternoon:<br=
><br>Frequency 137536 Hz,<br>Start times: 13:00 and 13:30 UT,<br>6 char, 3 =
sec symbols, &nbsp;8k19A, crc 16.<br><br>Experimental scripts to control th=
e timepulse-2 output are at <br>http://df6nm.bplaced.net/LF/u-blox_ebnaut/&=
nbsp;<br>and I intend to&nbsp;explain some details later this weekend.<br><=
br>Best 73,<br>Markus (DF6NM)<br abp=3D"302"><br abp=3D"303">-----Urspr=C3=
=BCngliche Mitteilung-----<br abp=3D"304">Von: DK7FC &lt;selberdenken@poste=
o.de&gt;<br abp=3D"305">An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&=
gt;<br abp=3D"306">Verschickt: Do, 31. Jan. 2019 22:32<br abp=3D"307">Betre=
ff: Re: LF: NEO-7M as a frequency source<br abp=3D"308"><br abp=3D"309">...=
<br clear=3D"none" abp=3D"320">...would like to try to transmit EbNaut on 1=
37 kHz directly from such a <br clear=3D"none" abp=3D"321">module.<br clear=
=3D"none" abp=3D"322"><br clear=3D"none" abp=3D"323">73, Stefan<br clear=3D=
"none" abp=3D"324"><br clear=3D"none" abp=3D"325"><br clear=3D"none" abp=3D=
"373"></div></div>
------=_Part_1845780_1410746881.1549111581840--

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Date: Sat, 02 Feb 2019 14:30:54 +0100
From: DK7FC <selberdenken@posteo.de>
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References: <CANA3B6Vv89cy_LEii6wyBzJ9M-U4aJAp3dyBTyTjdTf_L_oSOw@mail.gmail.com> <72260FC83F8D405D837689890C0FB310@Rob64PC>
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 Content preview:  Hi Riccardo, Rob, LF, Probably just a consolation for you,
    but here you are very strong :-) The phase was changing during that time.
    The srpring is coming slowly!!! 73, Stefan 
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Subject: Re: LF: EbNaut on 137546.2 Hz
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This is a multi-part message in MIME format.
--------------020804020902020703060309
Content-Type: multipart/alternative;
 boundary="------------050708090104050003020604"


--------------050708090104050003020604
Content-Type: text/plain; charset=UTF-8; format=flowed
Content-Transfer-Encoding: 7bit

Hi Riccardo, Rob, LF,

Probably just a consolation for you, but here you are very strong :-)
The phase was changing during that time. The srpring is coming slowly!!!

73, Stefan

Am 02.02.2019 13:31, schrieb Rob Renoud:
> Riccardo,
> Sorry, but no decodes overnight.
> 73,
> Rob - K3RWR
> *From:* Riccardo Zoli
> *Sent:* Friday, February 01, 2019 8:55 PM
> *To:* LF Group
> *Subject:* LF: EbNaut on 137546.2 Hz
> LF,
> Tonite I've scheduled some transmissions with these parameters:
> *QRG: 137546.2 Hz*
> *Coding 8K19A*
> *CRC 14*
> *3 sec./sym.*
> *7 characters*
> *Duration: 29' 36"*
> *Every 30 min., 1st on 2100z, last on 0800z*
> Reports are welcome.
> All the best
> 73 de Riccardo IW4DXW

--------------050708090104050003020604
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 8bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
  <title></title>
</head>
<body bgcolor="#ffffff" text="#000000">
Hi Riccardo, Rob, LF, <br>
<br>
Probably just a consolation for you, but here you are very strong :-)<br>
The phase was changing during that time. The srpring is coming slowly!!!<br>
<br>
73, Stefan<br>
<br>
Am 02.02.2019 13:31, schrieb Rob Renoud:
<blockquote cite="mid:72260FC83F8D405D837689890C0FB310@Rob64PC"
 type="cite">
  <div dir="ltr">
  <div
 style="font-size: 12pt; font-family: 'Calibri'; color: rgb(0, 0, 0);">
  <div>Riccardo,</div>
  <div> </div>
  <div>Sorry, but no decodes overnight.</div>
  <div> </div>
  <div>73,</div>
  <div>Rob - K3RWR</div>
  <div
 style="font-size: small; text-decoration: none; font-family: &quot;Calibri&quot;; font-weight: normal; color: rgb(0, 0, 0); font-style: normal; display: inline;">
  <div
 style="font-family: tahoma; font-style: normal; font-variant: normal; font-weight: normal; font-size: 10pt; line-height: normal; font-size-adjust: none; font-stretch: normal; -x-system-font: none;">
  <div> </div>
  <div
 style="background: rgb(245, 245, 245) none repeat scroll 0% 0%; -moz-background-clip: border; -moz-background-origin: padding; -moz-background-inline-policy: continuous;">
  <div style=""><b>From:</b> <a moz-do-not-send="true"
 title="riccardozoli80@gmail.com">Riccardo Zoli</a> </div>
  <div><b>Sent:</b> Friday, February 01, 2019 8:55 PM</div>
  <div><b>To:</b> <a moz-do-not-send="true"
 title="rsgb_lf_group@blacksheep.org">LF Group</a> </div>
  <div><b>Subject:</b> LF: EbNaut on 137546.2 Hz</div>
  </div>
  </div>
  <div> </div>
  </div>
  <div
 style="font-size: small; text-decoration: none; font-family: &quot;Calibri&quot;; font-weight: normal; color: rgb(0, 0, 0); font-style: normal; display: inline;">
  <div>
  <div> </div>
  <div>LF,</div>
  <div> </div>
  <div>Tonite I've scheduled some transmissions with these parameters:</div>
  <div> </div>
  <div><b>QRG: 137546.2 Hz</b></div>
  <div><b>Coding 8K19A</b></div>
  <div><b>CRC 14</b></div>
  <div><b>3 sec./sym.</b></div>
  <div><b>7 characters</b></div>
  <div><b>Duration: 29' 36"</b></div>
  <div><b>Every 30 min., 1st on 2100z, last on 0800z</b></div>
  <div> </div>
  <div>Reports are welcome.</div>
  <div> </div>
  <div> </div>
  <div>All the best</div>
  <div> </div>
  <div>73 de Riccardo IW4DXW</div>
  <div> </div>
  </div>
  </div>
  </div>
  </div>
</blockquote>
</body>
</html>

--------------050708090104050003020604--

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 Content preview:  Hi Markus, Great work! It seems to work well. There are some
    dynamic changes in the phase. Would you think it is propagation? So this
   is a Windows solution without the need to use an upconverter. Let's see if
    th [...] 
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Subject: Re: LF: EbNaut test from u-blox module
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Hi Markus,

Great work! It seems to work well. There are some dynamic changes in the 
phase. Would you think it is propagation?
So this is a Windows solution without the need to use an upconverter. 
Let's see if this will help to make the mode more popular, or not.
How did you connect the module to the PA, which kind of exciter? I would 
know how to do it, just beeing curious...

73, Stefan


Am 02.02.2019 13:46, schrieb Markus Vester:
> Think I have tamed my u-blox LEA-6T module well enough, so will try 
> to send an EbNaut test this afternoon:
>
> Frequency 137536 Hz,
> Start times: 13:00 and 13:30 UT,
> 6 char, 3 sec symbols,  8k19A, crc 16.
>
> Experimental scripts to control the timepulse-2 output are at
> http://df6nm.bplaced.net/LF/u-blox_ebnaut/
> and I intend to explain some details later this weekend.
>
> Best 73,
> Markus (DF6NM)
>
> -----Ursprüngliche Mitteilung-----
> Von: DK7FC <selberdenken@posteo.de>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Do, 31. Jan. 2019 22:32
> Betreff: Re: LF: NEO-7M as a frequency source
>
> ...
> ...would like to try to transmit EbNaut on 137 kHz directly from such a
> module.
>
> 73, Stefan
>
>

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Hi Markus, <br>
<br>
Great work! It seems to work well. There are some dynamic changes in
the phase. Would you think it is propagation?<br>
So this is a Windows solution without the need to use an upconverter.
Let's see if this will help to make the mode more popular, or not.<br>
How did you connect the module to the PA, which kind of exciter? I
would know how to do it, just beeing curious...<br>
<br>
73, Stefan<br>
<br>
<br>
Am 02.02.2019 13:46, schrieb Markus Vester:
<blockquote cite="mid:1853806007.1845781.1549111581841@mail.yahoo.com"
 type="cite">
  <div
 style="font-size: 10pt; font-family: arial,helvetica,sans-serif; color: black;">
  <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;"
 abp="300">Think I have tamed my u-blox LEA-6T module well enough, so
will try to send an EbNaut test this afternoon:<br>
  <br>
Frequency 137536 Hz,<br>
Start times: 13:00 and 13:30 UT,<br>
6 char, 3 sec symbols,  8k19A, crc 16.<br>
  <br>
Experimental scripts to control the timepulse-2 output are at <br>
<a class="moz-txt-link-freetext" href="http://df6nm.bplaced.net/LF/u-blox_ebnaut/">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</a> <br>
and I intend to explain some details later this weekend.<br>
  <br>
Best 73,<br>
Markus (DF6NM)<br abp="302">
  <br abp="303">
-----Ursprüngliche Mitteilung-----<br abp="304">
Von: DK7FC <a class="moz-txt-link-rfc2396E" href="mailto:selberdenken@posteo.de">&lt;selberdenken@posteo.de&gt;</a><br abp="305">
An: rsgb_lf_group <a class="moz-txt-link-rfc2396E" href="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br abp="306">
Verschickt: Do, 31. Jan. 2019 22:32<br abp="307">
Betreff: Re: LF: NEO-7M as a frequency source<br abp="308">
  <br abp="309">
...<br abp="320" clear="none">
...would like to try to transmit EbNaut on 137 kHz directly from such a
  <br abp="321" clear="none">
module.<br abp="322" clear="none">
  <br abp="323" clear="none">
73, Stefan<br abp="324" clear="none">
  <br abp="325" clear="none">
  <br abp="373" clear="none">
  </div>
  </div>
</blockquote>
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--------------050109000101050903070205--

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 Content preview:  Riccardo No decodes here. DCF39 on the weak side again last
    night. Jay W1VD 
 Content analysis details:   (-0.7 points, 5.0 required)
  pts rule name              description
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Subject: Re: LF: EbNaut on 137546.2 Hz
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Riccardo

No decodes here. DCF39 on the weak side again last night.

Jay W1VD





----- Original Message -----
From: Rob Renoud <k3rwr@md.metrocast.net>
Reply-To: <rsgb_lf_group@blacksheep.org>
To: <rsgb_lf_group@blacksheep.org>
Sent: 2/2/2019 7:31:56 AM
Subject: Re: LF: EbNaut on 137546.2 Hz



Riccardo,

Sorry, but no decodes overnight.

73,
Rob - K3RWR

From: Riccardo Zoli=20
Sent: Friday, February 01, 2019 8:55 PM
To: LF Group=20
Subject: LF: EbNaut on 137546.2 Hz


LF,

Tonite=20
I've scheduled some transmissions with these parameters:

QRG: 137546.2 Hz
Coding 8K19A
CRC 14
3 sec./sym.
7 characters
Duration: 29'=20
36"
Every 30 min., 1st on 2100z, last on 0800z

Reports are welcome.


All the best

73 de Riccardo IW4DXW

--Hn51SXykYf3JlHvcDk=_mIguIGQfnNIfTv
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Content-Transfer-Encoding: quoted-printable
Content-Disposition: inline

<HTML><HEAD>
<STYLE type=3Dtext/css> body { margin:0.7em; } body.OECFntDef, body.OE=
CFntDef div { font-family:Arial,"Segoe UI",Tahoma,Verdana,Helvetica,sa=
ns-serif;font-size:10pt; }</STYLE>

<META name=3DGENERATOR content=3D"MSHTML 11.00.9600.18450"></HEAD>
<BODY spellcheck=3Dtrue class=3DOECFntDef>
<DIV>Riccardo</DIV>
<DIV>&nbsp;</DIV>
<DIV>No decodes here. DCF39 on the weak side again&nbsp;last night.</D=
IV>
<DIV>&nbsp;</DIV>
<DIV>Jay W1VD</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE style=3D"PADDING-BOTTOM: 0px; PADDING-TOP: 0px; PADDING-LE=
FT: 0.5em; MARGIN: 0px 0px 0px 0.5em; BORDER-LEFT: #c7e5ff 1px solid; =
PADDING-RIGHT: 0px">
<DIV><B>----- Original Message -----</B></DIV>
<DIV><B>From:</B> Rob Renoud &lt;<A href=3D"mailto:k3rwr@md.metrocast.=
net">k3rwr@md.metrocast.net</A>&gt;</DIV>
<DIV><B>Reply-To:</B> &lt;<A href=3D"mailto:rsgb_lf_group@blacksheep.o=
rg">rsgb_lf_group@blacksheep.org</A>&gt;</DIV>
<DIV><B>To:</B> &lt;<A href=3D"mailto:rsgb_lf_group@blacksheep.org">rs=
gb_lf_group@blacksheep.org</A>&gt;</DIV>
<DIV><B>Sent:</B> 2/2/2019 7:31:56 AM</DIV>
<DIV><B>Subject:</B> Re: LF: EbNaut on 137546.2 Hz</DIV>
<HR style=3D"BORDER-TOP: medium none; HEIGHT: 1px; BORDER-RIGHT: mediu=
m none; BORDER-BOTTOM: medium none; COLOR: #ccc; BORDER-LEFT: medium n=
one; BACKGROUND-COLOR: #ccc">

<DIV dir=3Dltr>
<DIV style=3D"FONT-SIZE: 12pt; FONT-FAMILY: 'Calibri'; COLOR: #000000"=
>
<DIV>Riccardo,</DIV>
<DIV>&nbsp;</DIV>
<DIV>Sorry, but no decodes overnight.</DIV>
<DIV>&nbsp;</DIV>
<DIV>73,</DIV>
<DIV>Rob - K3RWR</DIV>
<DIV style=3D'FONT-SIZE: small; TEXT-DECORATION: none; FONT-FAMILY: "C=
alibri"; FONT-WEIGHT: normal; COLOR: #000000; FONT-STYLE: normal; DISP=
LAY: inline'>
<DIV style=3D"FONT: 10pt tahoma">
<DIV>&nbsp;</DIV>
<DIV style=3D"BACKGROUND: #f5f5f5">
<DIV style=3D"font-color: black"><B>From:</B> <A title=3Driccardozoli8=
0@gmail.com>Riccardo Zoli</A> </DIV>
<DIV><B>Sent:</B> Friday, February 01, 2019 8:55 PM</DIV>
<DIV><B>To:</B> <A title=3Drsgb_lf_group@blacksheep.org>LF Group</A> <=
/DIV>
<DIV><B>Subject:</B> LF: EbNaut on 137546.2 Hz</DIV></DIV></DIV>
<DIV>&nbsp;</DIV></DIV>
<DIV style=3D'FONT-SIZE: small; TEXT-DECORATION: none; FONT-FAMILY: "C=
alibri"; FONT-WEIGHT: normal; COLOR: #000000; FONT-STYLE: normal; DISP=
LAY: inline'>
<DIV>
<DIV>&nbsp;</DIV>
<DIV>LF,</DIV>
<DIV>&nbsp;</DIV>
<DIV>Tonite I've scheduled some transmissions with these parameters:</=
DIV>
<DIV>&nbsp;</DIV>
<DIV><B>QRG: 137546.2 Hz</B></DIV>
<DIV><B>Coding 8K19A</B></DIV>
<DIV><B>CRC 14</B></DIV>
<DIV><B>3 sec./sym.</B></DIV>
<DIV><B>7 characters</B></DIV>
<DIV><B>Duration: 29' 36"</B></DIV>
<DIV><B>Every 30 min., 1st on 2100z, last on 0800z</B></DIV>
<DIV>&nbsp;</DIV>
<DIV>Reports are welcome.</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>All the best</DIV>
<DIV>&nbsp;</DIV>
<DIV>73 de Riccardo IW4DXW</DIV>
<DIV>&nbsp;</DIV></DIV></DIV></DIV></DIV></BLOCKQUOTE></BODY></HTML>

--Hn51SXykYf3JlHvcDk=_mIguIGQfnNIfTv--


From owner-rsgb_lf_group@blacksheep.org  Sat Feb  2 16:46:34 2019
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To: RSGB LF group <rsgb_lf_group@blacksheep.org>
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References: <CAA8k23Qe5rgZ=0WTbnQksH0Dpd3EqtW5ZHHE+CO0AobJtwoLmQ@mail.gmail.com> <7e1ee234-21b9-d8b1-f0e1-e2eace39a968@usa.net> <CAA8k23QySVguYTpmfnp=xL4j_8Vgiqm_Ts1FT+1mQyGXZmpgqA@mail.gmail.com> <71d8e1d2-69cb-4ecb-0205-028cb5a81ff9@usa.net>
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 Content preview:  some time ago the yahoo group was formed because of two problems:
    lack of archives and problems getting mail from/to blacksheep. both are solved.
    the problems in getting mail from/to blacksheep were usually due to the mail
    provider's servers being misconfigured (not blacksheep's). i think this is
    less of a problem now. 
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Subject: Re: Re: LF: Re: [rsgb-lf-group] SMT PA0RDT Board
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--17435139-1238230729-1549122052=:725
Content-Type: TEXT/PLAIN; charset=ISO-8859-15; format=flowed
Content-Transfer-Encoding: 8BIT

some time ago the yahoo group was formed because of two problems: lack of 
archives and problems getting mail from/to blacksheep. both are solved.


the problems in getting mail from/to blacksheep were usually due to the 
mail provider's servers being misconfigured (not blacksheep's). i think 
this is less of a problem now.

the first problem is solved too, the list has an unofficial archive here:
https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/

btw the archive dates from july 2014, if anyone has an archive of earlier 
emails in mbox format, i'd be glad to add them to the archive.


i don't think there are any more valid reasons, apart from the fact that 
that mailing lists are not "modern" (no shiny webpage that can dissapear 
anytime the owner choses so).

VY 73

Jacek / SQ5BPF



On Thu, 31 Jan 2019, dhchurch wrote:

> Date: Thu, 31 Jan 2019 10:58:12 +0000
> From: dhchurch <dhchurch@lineone.net>
> Reply-To: rsgb_lf_group@blacksheep.org
> To: RSGB LF group <rsgb_lf_group@blacksheep.org>
> Subject: Re: Re: LF: Re: [rsgb-lf-group] SMT PA0RDT Board
> 
> Hello�All
> �
> I simply dislike Yahoo and many others because they have been known to collect personal data. It's bad
> enough trying to avoid Google but there are other sites�like Facebook which�really are both annoying and
> worrying.
> �
> 73, Hugh, M0DS�
> �
>       ----- Receiving the following content -----
> From: DK7FC
> Receiver: rsgb_lf_group
> Time: 2019-01-30, 14:58:33
> Subject: Re: LF: Re: [rsgb-lf-group] SMT PA0RDT Board
> 
> Mal,
> 
> why are you subscribed to that .io list at all? I don't care about it completely. It is simply not
> existing. Tomorrow it will be groups.to and then lists.li and then mail.vt, of course always with
> new features and advantages. Each few years the same story. It is so boring!!!
> 
> My car becomes 30 years old in a few weeks and i still like it as in the first week (i bought it 16
> years ago, for just 800 EUR). People told me that it would be better to change it to a NEWer
> version, think of all the advantages, oh and the SAFETY!!! ;-) And then the advertisement. More,
> better, faster, efficient... uuuh.
> 
> You know, there are those people who somehow like to shutdown blacksheep. Why do they have that
> motivation? I observed the effect in 2012, when the super-yahoo advanced group came up. It wasn't
> enough for them to move to the other group, which is their free decision of course. Why aren't they
> just happy with all the new advantages? What is going on into their minds that they feel motivated
> to destroy the group which other people still like? Coexistence unwanted? Simple-minded, indeed.
> But dangerous.
> 
> 73, Stefan
> 
> 
> 
> 
> 
> 
> Am 30.01.2019 15:25, schrieb mal hamilton:
>       BLACKSHEEP has stood the test of TIME, others have been and gone. People use Blacksheep
>       because it is reliable and has been going for over 20 years.
> How long will groups.ie last ? Some people like Choice
> G3KEV
> ?
> ?
> From: Alberto di Bene
> Sent: Tuesday, January 29, 2019 5:44 PM
> To: rsgb-lf-group@groups.io
> Subject: Re: [rsgb-lf-group] SMT PA0RDT Board
> ?
> On 2019-01-29 18:12, Andy TALBOT wrote:
>       Pity the Blacksheep only subscribers can't get at it :-)
> 
> 
> I don't understand why the group duplication still exists... when the group was hosted by
> Yahoo, all the Yahoo-haters had a valid reason to refuge themselves in the reassuring wool of
> a black sheep... but now that the main group has migrated to groups.io, frankly I don't see
> the reason why the blacksheep list should continue to exist... but I am a simple-minded
> person, maybe those reasons are escaping my understanding... :-)
> 
> 73? Alberto? I2PHD
> 
> ?
> _._,_._,_
> 
> _________________________________________________________________________________________________________
> Groups.io Links:
> 
> You receive all messages sent to this group.
> 
> View/Reply Online (#8542) | Reply To Group | Reply To Sender | Mute This Topic | New Topic
> 
> Your Subscription | Contact Group Owner | Unsubscribe [g3kevmal@talktalk.net]
> 
> _._,_._,_
> 
> 
>
--17435139-1238230729-1549122052=:725--

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To: "(rsgb_lf_group@blacksheep.org)" <rsgb_lf_group@blacksheep.org>
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 Content preview:  Joe Decodes from this morning ... just checking spread between
    car Eb/N0 and Eb/N0 without interference. Curious if the LF beacon runs 24
    hours or is switched off during the day. 1100 Rank 0 car Eb/N0 21.6 dB Eb/N0
    15.3 dB VO1NA** 1130 Rank 0 car Eb/N0 14.6 dB Eb/N0 12.3 dB ******* 1200
   - 1230 - 1300 - 
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                             low trust
                             [2001:558:fe21:29:69:252:207:38 listed in]
                             [list.dnswl.org]
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Subject: LF: VO1NA EbNaut
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--cJLWd=_Hmk2CXEfVvdaHVA6lKfrViYodkW
Content-Type: text/plain; charset="utf-8"
Content-Transfer-Encoding: quoted-printable
Content-Disposition: inline

Joe

Decodes from this morning ... just checking spread between car Eb/N0 a=
nd Eb/N0=20
without interference. Curious if the LF beacon runs 24 hours or is swi=
tched off=20
during the day.=20

1100 Rank 0 car Eb/N0 21.6 dB Eb/N0 15.3 dB VO1NA**
1130 Rank 0 car Eb/N0 14.6 dB Eb/N0 12.3 dB *******
1200 -
1230 -
1300 -

Jay W1VD

--cJLWd=_Hmk2CXEfVvdaHVA6lKfrViYodkW
Content-Type: text/html; charset="utf-8"
Content-Transfer-Encoding: quoted-printable
Content-Disposition: inline

<HTML><HEAD>
<STYLE type=3Dtext/css> body { margin:0.7em; } body.OECFntDef, body.OE=
CFntDef div { font-family:Arial,"Segoe UI",Tahoma,Verdana,Helvetica,sa=
ns-serif;font-size:10pt; }</STYLE>

<META name=3DGENERATOR content=3D"MSHTML 11.00.9600.18450"></HEAD>
<BODY spellcheck=3Dtrue class=3DOECFntDef>
<DIV>
<DIV>Joe</DIV>
<DIV>&nbsp;</DIV>
<DIV>Decodes&nbsp;from this morning ... just checking spread between c=
ar Eb/N0 and Eb/N0 without interference. Curious if the LF beacon&nbsp=
;runs 24 hours or is switched off during the day.&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>1100 Rank 0 car Eb/N0&nbsp;21.6 dB Eb/N0&nbsp;15.3 dB&nbsp;VO1NA*=
*</DIV>
<DIV>
<DIV>1130 Rank 0 car Eb/N0&nbsp;14.6 dB&nbsp;Eb/N0&nbsp;12.3 dB ******=
*</DIV>
<DIV>
<DIV>1200 -</DIV>
<DIV>1230 -</DIV>
<DIV>1300 -</DIV>
<DIV>&nbsp;</DIV>
<DIV>Jay W1VD</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>
<DIV>&nbsp;</DIV></DIV></DIV></DIV></DIV></BODY></HTML>

--cJLWd=_Hmk2CXEfVvdaHVA6lKfrViYodkW--


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From: "jrusgrove@comcast.net" <jrusgrove@comcast.net>
To: "(rsgb_lf_group@blacksheep.org)" <rsgb_lf_group@blacksheep.org>
MIME-Version: 1.0
Date: Sat, 2 Feb 2019 13:54:20 -0500
Message-ID: <1UTDpVxH4o.6QUhea15UOe@optiplex980-pc>
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 Content preview:  EbNaut enthusiasts Recent LF EbNaut decodes added to the list
    ... http://www.w1vd.com/EbNaut.html . Jay W1VD 
 Content analysis details:   (-0.7 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -0.7 RCVD_IN_DNSWL_LOW      RBL: Sender listed at http://www.dnswl.org/,
                             low trust
                             [2001:558:fe21:29:69:252:207:40 listed in]
                             [list.dnswl.org]
 -0.0 SPF_PASS               SPF: sender matches SPF record
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                             provider (jrusgrove[at]comcast.net)
  0.0 HTML_MESSAGE           BODY: HTML included in message
X-Scan-Signature: 739d4fb39bd02fc5a2de5437a39bb056
Subject: LF: LF EbNaut
Content-Type: multipart/alternative; boundary="QheXsjRGgLQ3vH=_SY7bw3mTIO6jg0yHBn"
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This is a multi-part message in MIME format

--QheXsjRGgLQ3vH=_SY7bw3mTIO6jg0yHBn
Content-Type: text/plain; charset="utf-8"
Content-Transfer-Encoding: quoted-printable
Content-Disposition: inline

EbNaut enthusiasts

Recent LF EbNaut decodes added to the list ... http://www.w1vd.com/EbN=
aut.html .

Jay W1VD

--QheXsjRGgLQ3vH=_SY7bw3mTIO6jg0yHBn
Content-Type: text/html; charset="utf-8"
Content-Transfer-Encoding: quoted-printable
Content-Disposition: inline

<HTML><HEAD>
<STYLE type=3Dtext/css> body { margin:0.7em; } body.OECFntDef, body.OE=
CFntDef div { font-family:Arial,"Segoe UI",Tahoma,Verdana,Helvetica,sa=
ns-serif;font-size:10pt; }</STYLE>

<META name=3DGENERATOR content=3D"MSHTML 11.00.9600.18450"></HEAD>
<BODY spellcheck=3Dtrue class=3DOECFntDef>
<DIV>EbNaut enthusiasts</DIV>
<DIV>&nbsp;</DIV>
<DIV>Recent LF EbNaut&nbsp;decodes added to the list ... <A href=3D"ht=
tp://www.w1vd.com/EbNaut.html">http://www.w1vd.com/EbNaut.html</A>&nbs=
p;.</DIV>
<DIV>&nbsp;</DIV>
<DIV>Jay W1VD</DIV></BODY></HTML>

--QheXsjRGgLQ3vH=_SY7bw3mTIO6jg0yHBn--


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From: Domenico IZ7SLZ <iz7slz.domenico@gmail.com>
Date: Sat, 2 Feb 2019 20:58:18 +0100
Message-ID: <CAC+C6w4u7q+d2aaTHZMVNqVsGTH2oD26RB6YuDdcknmd6CbzpQ@mail.gmail.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  Hi EbNaut-eers at the link https://drive.google.com/file/d/1kpuFi9yDsXygNLNhnp3yAXOnvv-GYtCR/view?usp=sharing
 Content analysis details:   (0.0 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -0.0 RCVD_IN_DNSWL_NONE     RBL: Sender listed at http://www.dnswl.org/,
                             no trust
                             [2607:f8b0:4864:20:0:0:0:235 listed in]
                             [list.dnswl.org]
 -0.0 SPF_PASS               SPF: sender matches SPF record
  0.0 FREEMAIL_FROM          Sender email is commonly abused enduser mail
                             provider (iz7slz.domenico[at]gmail.com)
  0.0 HTML_MESSAGE           BODY: HTML included in message
X-Scan-Signature: 1708620d3ce65bee0beaaede7929769a
Subject: LF: Ebnaut instructions for Windows's user
Content-Type: multipart/alternative; boundary="00000000000086c3ce0580eeb0f4"
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--00000000000086c3ce0580eeb0f4
Content-Type: text/plain; charset="UTF-8"

Hi EbNaut-eers

at the link

https://drive.google.com/file/d/1kpuFi9yDsXygNLNhnp3yAXOnvv-GYtCR/view?usp=sharing

i have uploaded a paper written by me with some notes and instructions for
operate EbNaut decoder under Windows o.s.

Many thanks to Markus DF6NM,  who has added in this paper,  many other
important notes.

We hope to have produced an useful manual for the community of the EbNaut
operator and we hope that many others can approach this technique.

I wish you good reading and of course, i am at disposal for any further
informations.

73, Domenico IZ7SLZ

--00000000000086c3ce0580eeb0f4
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr">Hi EbNa=
ut-eers<div><br></div><div>at the link=C2=A0</div><div><br></div><div><a hr=
ef=3D"https://drive.google.com/file/d/1kpuFi9yDsXygNLNhnp3yAXOnvv-GYtCR/vie=
w?usp=3Dsharing">https://drive.google.com/file/d/1kpuFi9yDsXygNLNhnp3yAXOnv=
v-GYtCR/view?usp=3Dsharing</a><br></div><div><br></div><div>i have uploaded=
 a paper written by me with some notes and instructions for operate EbNaut =
decoder under Windows o.s.</div><div><br></div><div>Many thanks to Markus D=
F6NM,=C2=A0 who has added in this paper,=C2=A0 many other important notes.<=
/div><div><br></div><div>We hope to have produced an useful manual for the =
community of the EbNaut operator and we hope that many others can approach =
this technique.</div><div><br></div><div>I wish you good reading and of cou=
rse, i am at disposal for any further informations.</div><div><br></div><di=
v>73, Domenico IZ7SLZ</div></div></div></div></div>

--00000000000086c3ce0580eeb0f4--

From owner-rsgb_lf_group@blacksheep.org  Sat Feb  2 21:32:55 2019
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 Content preview:  Hi Jay, Thanks for the report. Normally it is off during the
    day. Let's leave it on until Monday morning and see what happens. 73 Joe 
 Content analysis details:   (0.0 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
X-Scan-Signature: bb61bee384896e075004ae5ec954ddd2
Subject: Re: LF: VO1NA EbNaut
Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed
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Hi Jay,

Thanks for the report.  Normally it is off during the day.  Let's
leave it on until Monday morning and see what happens.

73
Joe

On Sat, 2 Feb 2019, jrusgrove@comcast.net wrote:

> Joe
>
> Decodes from this morning ... just checking spread between car Eb/N0 and Eb/N0
> without interference. Curious if the LF beacon runs 24 hours or is switched off
> during the day.
>
> 1100 Rank 0 car Eb/N0 21.6 dB Eb/N0 15.3 dB VO1NA**
> 1130 Rank 0 car Eb/N0 14.6 dB Eb/N0 12.3 dB *******
> 1200 -
> 1230 -
> 1300 -
>
> Jay W1VD
>

From owner-rsgb_lf_group@blacksheep.org  Sat Feb  2 22:20:08 2019
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 <72260FC83F8D405D837689890C0FB310@Rob64PC> <1UTDpTCfJH.3TN4CxnaHJt@optiplex980-pc>
In-Reply-To: <1UTDpTCfJH.3TN4CxnaHJt@optiplex980-pc>
From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Sat, 2 Feb 2019 22:05:53 +0100
Message-ID: <CANA3B6WwFmskn2w+SK2j4d6uVEkUByJ70AR2qHpCeVf3gPXSuQ@mail.gmail.com>
To: LF Group <rsgb_lf_group@blacksheep.org>
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 Content preview:  Rob, Jay many thanks for your attempts. Yes: last night the
    propagation was not so good. Stefan, thanks so much for your detailed and
    comfortable report for me. Good decodes with stable phase from Domenico as
    well. 
 Content analysis details:   (0.3 points, 5.0 required)
  pts rule name              description
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Subject: Re: LF: EbNaut on 137546.2 Hz
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--000000000000a6dd560580efa0c1
Content-Type: text/plain; charset="UTF-8"

Rob, Jay
many thanks for your attempts.
Yes: last night the propagation was not so good.

Stefan,
thanks so much for your detailed and comfortable report for me. Good
decodes with stable phase from Domenico as well.

So this is my last TX setup:
- PC with Spectrum Lab (configured as I/Q out), EbNaut_sender and rsNTP.
- SDR "Softrock style" (modified for phase reference restore),
- ring modulator on RF before driver (and PA),
- U-blox NEO-M8T for 1PPS reference and ftx*4 source for SDR clock.

All the best


73 de Riccardo IW4DXW







Il giorno Sab 2 Feb 2019, 15:51 jrusgrove@comcast.net <jrusgrove@comcast.net>
ha scritto:

> Riccardo
>
> No decodes here. DCF39 on the weak side again last night.
>
> Jay W1VD
>
>
>
> *----- Original Message -----*
> *From:* Rob Renoud <k3rwr@md.metrocast.net>
> *Reply-To:* <rsgb_lf_group@blacksheep.org>
> *To:* <rsgb_lf_group@blacksheep.org>
> *Sent:* 2/2/2019 7:31:56 AM
> *Subject:* Re: LF: EbNaut on 137546.2 Hz
> ------------------------------
> Riccardo,
>
> Sorry, but no decodes overnight.
>
> 73,
> Rob - K3RWR
>
> *From:* Riccardo Zoli
> *Sent:* Friday, February 01, 2019 8:55 PM
> *To:* LF Group
> *Subject:* LF: EbNaut on 137546.2 Hz
>
>
> LF,
>
> Tonite I've scheduled some transmissions with these parameters:
>
> *QRG: 137546.2 Hz*
> *Coding 8K19A*
> *CRC 14*
> *3 sec./sym.*
> *7 characters*
> *Duration: 29' 36"*
> *Every 30 min., 1st on 2100z, last on 0800z*
>
> Reports are welcome.
>
>
> All the best
>
> 73 de Riccardo IW4DXW
>
>
>

--000000000000a6dd560580efa0c1
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"auto"><div dir=3D"auto"><br></div>Rob, Jay=C2=A0<div dir=3D"aut=
o">many thanks for your attempts.<div dir=3D"auto">Yes: last night the prop=
agation was not so good.</div><div dir=3D"auto"><br></div><div dir=3D"auto"=
>Stefan,=C2=A0</div><div dir=3D"auto">thanks so much for your detailed and =
comfortable report for me. Good decodes with stable phase from Domenico as =
well.</div><div dir=3D"auto"><br></div><div dir=3D"auto">So this is my last=
 TX setup:=C2=A0</div><div dir=3D"auto">- PC with Spectrum Lab (configured =
as I/Q out), EbNaut_sender and rsNTP.</div><div dir=3D"auto">- SDR &quot;So=
ftrock style&quot; (modified for phase reference restore),</div><div dir=3D=
"auto">- ring modulator on RF before driver (and PA),</div><div dir=3D"auto=
">- U-blox NEO-M8T for 1PPS reference and ftx*4 source for SDR clock.</div>=
<div dir=3D"auto"><br></div><div dir=3D"auto">All the best</div><div dir=3D=
"auto"><br></div><div dir=3D"auto"><br></div><div dir=3D"auto">73 de Riccar=
do IW4DXW</div><div dir=3D"auto"><br></div><div dir=3D"auto"><br></div><div=
 dir=3D"auto"><br></div><div dir=3D"auto"><br></div><div dir=3D"auto"><br><=
/div><div dir=3D"auto"><br></div></div></div><br><div class=3D"gmail_quote"=
><div dir=3D"ltr">Il giorno Sab 2 Feb 2019, 15:51 <a href=3D"mailto:jrusgro=
ve@comcast.net" target=3D"_blank" rel=3D"noreferrer">jrusgrove@comcast.net<=
/a> &lt;<a href=3D"mailto:jrusgrove@comcast.net" target=3D"_blank" rel=3D"n=
oreferrer">jrusgrove@comcast.net</a>&gt; ha scritto:<br></div><blockquote c=
lass=3D"gmail_quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc solid;=
padding-left:1ex">



<div class=3D"m_-804179810947390431m_-2625399685667482187OECFntDef">
<div>Riccardo</div>
<div>=C2=A0</div>
<div>No decodes here. DCF39 on the weak side again=C2=A0last night.</div>
<div>=C2=A0</div>
<div>Jay W1VD</div>
<div>=C2=A0</div>
<div>=C2=A0</div>
<blockquote style=3D"PADDING-BOTTOM:0px;PADDING-TOP:0px;PADDING-LEFT:0.5em;=
MARGIN:0px 0px 0px 0.5em;BORDER-LEFT:#c7e5ff 1px solid;PADDING-RIGHT:0px">
<div><b>----- Original Message -----</b></div>
<div><b>From:</b> Rob Renoud &lt;<a href=3D"mailto:k3rwr@md.metrocast.net" =
rel=3D"noreferrer noreferrer" target=3D"_blank">k3rwr@md.metrocast.net</a>&=
gt;</div>
<div><b>Reply-To:</b> &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" r=
el=3D"noreferrer noreferrer" target=3D"_blank">rsgb_lf_group@blacksheep.org=
</a>&gt;</div>
<div><b>To:</b> &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" rel=3D"=
noreferrer noreferrer" target=3D"_blank">rsgb_lf_group@blacksheep.org</a>&g=
t;</div>
<div><b>Sent:</b> 2/2/2019 7:31:56 AM</div>
<div><b>Subject:</b> Re: LF: EbNaut on 137546.2 Hz</div>
<hr style=3D"BORDER-TOP:medium none;HEIGHT:1px;BORDER-RIGHT:medium none;BOR=
DER-BOTTOM:medium none;COLOR:#ccc;BORDER-LEFT:medium none;BACKGROUND-COLOR:=
#ccc">

<div dir=3D"ltr">
<div style=3D"FONT-SIZE:12pt;FONT-FAMILY:&#39;Calibri&#39;;COLOR:#000000">
<div>Riccardo,</div>
<div>=C2=A0</div>
<div>Sorry, but no decodes overnight.</div>
<div>=C2=A0</div>
<div>73,</div>
<div>Rob - K3RWR</div>
<div style=3D"FONT-SIZE:small;TEXT-DECORATION:none;FONT-FAMILY:&quot;Calibr=
i&quot;;FONT-WEIGHT:normal;COLOR:#000000;FONT-STYLE:normal;DISPLAY:inline">
<div style=3D"FONT:10pt tahoma">
<div>=C2=A0</div>
<div style=3D"BACKGROUND:#f5f5f5">
<div><b>From:</b> <a title=3D"riccardozoli80@gmail.com" rel=3D"noreferrer n=
oreferrer">Riccardo Zoli</a> </div>
<div><b>Sent:</b> Friday, February 01, 2019 8:55 PM</div>
<div><b>To:</b> <a title=3D"rsgb_lf_group@blacksheep.org" rel=3D"noreferrer=
 noreferrer">LF Group</a> </div>
<div><b>Subject:</b> LF: EbNaut on 137546.2 Hz</div></div></div>
<div>=C2=A0</div></div>
<div style=3D"FONT-SIZE:small;TEXT-DECORATION:none;FONT-FAMILY:&quot;Calibr=
i&quot;;FONT-WEIGHT:normal;COLOR:#000000;FONT-STYLE:normal;DISPLAY:inline">
<div>
<div>=C2=A0</div>
<div>LF,</div>
<div>=C2=A0</div>
<div>Tonite I&#39;ve scheduled some transmissions with these parameters:</d=
iv>
<div>=C2=A0</div>
<div><b>QRG: 137546.2 Hz</b></div>
<div><b>Coding 8K19A</b></div>
<div><b>CRC 14</b></div>
<div><b>3 sec./sym.</b></div>
<div><b>7 characters</b></div>
<div><b>Duration: 29&#39; 36&quot;</b></div>
<div><b>Every 30 min., 1st on 2100z, last on 0800z</b></div>
<div>=C2=A0</div>
<div>Reports are welcome.</div>
<div>=C2=A0</div>
<div>=C2=A0</div>
<div>All the best</div>
<div>=C2=A0</div>
<div>73 de Riccardo IW4DXW</div>
<div>=C2=A0</div></div></div></div></div></blockquote></div>
</blockquote></div>

--000000000000a6dd560580efa0c1--

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Date: Sun, 3 Feb 2019 00:15:53 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  Thanks Stefan and Michel (F5WK) for your excellent reports!
    The residual phase variation was surely from the antenna moving in the wind.
    I haven't been using the automatic tuner, and also did some manual tweaking near
    the beginning. Interestingly Michel's [...] 
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Subject: Re: LF: EbNaut test from u-blox module
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Thanks Stefan and Michel (F5WK) for your excellent reports!=20

The=C2=A0residual phase variation was surely from the antenna moving in the=
 wind. I haven't been using the=C2=A0automatic tuner, and also did some man=
ual tweaking=C2=A0near the beginning.=C2=A0Interestingly Michel's phase tra=
ce was a perfect copy of yours.

The exciter and 250 W PA are the same as=C2=A0in my usual LF setup, except =
that the feed from the SSB=C2=A0exciter has been replaced by the TP2 output=
 from the GPS device,=C2=A0connected=C2=A0through 470 ohm and a piece of co=
ax. The=C2=A0LEA-6T module came=C2=A0from Hongkong for=C2=A027 =E2=82=AC an=
d is very similar to the one described here
http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardow=
n-and-initial-test/

I=C2=A0am now repeating the same=C2=A0pair of transmissions=C2=A0at 0:00 an=
d 0:30 UT, but moved to=C2=A0137545 Hz to fit inside=C2=A0Jay's narrowband =
recording.=20

Best 73,
Markus=C2=A0=C2=A0(DF6NM)

=C2=A0=C2=A0

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Sa, 2. Feb. 2019 14:52
Betreff: Re: LF: EbNaut test from u-blox module

Hi Markus,=20

Great work! It seems to work well. There are some dynamic changes inthe pha=
se. Would you think it is propagation?
So this is a Windows solution without the need to use an upconverter.Let's =
see if this will help to make the mode more popular, or not.
How did you connect the module to the PA, which kind of exciter? Iwould kno=
w how to do it, just beeing curious...

73, Stefan


Am 02.02.2019 13:46, schrieb Markus Vester:
  Think I have=C2=A0tamed my u-blox LEA-6T module well enough, sowill try t=
o=C2=A0send an EbNaut test this afternoon:
=20
Frequency 137536 Hz,
Start times: 13:00 and 13:30 UT,
6 char, 3 sec symbols, =C2=A08k19A, crc 16.
=20
Experimental scripts to control the timepulse-2 output are at=20
http://df6nm.bplaced.net/LF/u-blox_ebnaut/=C2=A0
and I intend to=C2=A0explain some details later this weekend.
=20
Best 73,
Markus (DF6NM)
=20
-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Do, 31. Jan. 2019 22:32
Betreff: Re: LF: NEO-7M as a frequency source
=20
...
...would like to try to transmit EbNaut on 137 kHz directly from such a=20
module.
=20
73, Stefan
=20
=20
 =20


------=_Part_2047109_2141085363.1549152953582
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div id=3D"yiv2990111096" abp=3D"2819"><div abp=3D"2820"><div style=
=3D"color: black; font-family: arial, helvetica, sans-serif; font-size: 10p=
t;" abp=3D"2821"><div style=3D"color: black; font-family: arial, helvetica,=
 sans-serif; font-size: 10pt;" abp=3D"2822">Thanks Stefan and Michel (F5WK)=
 for your excellent reports! <br clear=3D"none" abp=3D"2823"><br clear=3D"n=
one" abp=3D"2824">The&nbsp;residual phase variation was surely from the ant=
enna moving in the wind. I haven't been using the&nbsp;automatic tuner, and=
 also did some manual tweaking&nbsp;near the beginning.&nbsp;Interestingly =
Michel's phase trace was a perfect copy of yours.<br clear=3D"none" abp=3D"=
2825"><br clear=3D"none" abp=3D"2826">The exciter and 250 W PA are the same=
 as&nbsp;in my usual LF setup, except that the feed from the SSB&nbsp;excit=
er has been replaced by the TP2 output from the GPS device,&nbsp;connected&=
nbsp;through 470 ohm and a piece of coax. The&nbsp;LEA-6T module came&nbsp;=
from Hongkong for&nbsp;27 =E2=82=AC and is very similar to the one describe=
d here<br>http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-modu=
le-teardown-and-initial-test/<br clear=3D"none" abp=3D"2827"><br clear=3D"n=
one" abp=3D"2828">I&nbsp;am now repeating the same&nbsp;pair of transmissio=
ns&nbsp;at<strong> 0:00</strong> and<strong> 0:30 UT</strong>, but moved to=
&nbsp;<strong>137545 Hz</strong> to fit inside&nbsp;Jay's narrowband record=
ing. <br clear=3D"none" abp=3D"2829"><br clear=3D"none" abp=3D"2830">Best 7=
3,<br clear=3D"none" abp=3D"2831">Markus&nbsp;&nbsp;(DF6NM)<br clear=3D"non=
e" abp=3D"2832"><br clear=3D"none" abp=3D"2833">&nbsp;&nbsp;<br clear=3D"no=
ne" abp=3D"2834"><br clear=3D"none" abp=3D"2835">-----Urspr=C3=BCngliche Mi=
tteilung-----<br clear=3D"none" abp=3D"2836">Von: DK7FC &lt;selberdenken@po=
steo.de&gt;<br clear=3D"none" abp=3D"2837">An: rsgb_lf_group &lt;rsgb_lf_gr=
oup@blacksheep.org&gt;<br clear=3D"none" abp=3D"2838">Verschickt: Sa, 2. Fe=
b. 2019 14:52<br clear=3D"none" abp=3D"2839">Betreff: Re: LF: EbNaut test f=
rom u-blox module<br clear=3D"none" abp=3D"2840"><br clear=3D"none" abp=3D"=
2841"></div><div class=3D"yiv2990111096yqt2807499086" id=3D"yiv2990111096yq=
t91517" abp=3D"2842"><div id=3D"yiv2990111096" abp=3D"2843"><div abp=3D"284=
4">
Hi Markus, <br clear=3D"none" abp=3D"2845">
<br clear=3D"none" abp=3D"2846">
Great work! It seems to work well. There are some dynamic changes in
the phase. Would you think it is propagation?<br clear=3D"none" abp=3D"2847=
">
So this is a Windows solution without the need to use an upconverter.
Let's see if this will help to make the mode more popular, or not.<br clear=
=3D"none" abp=3D"2848">
How did you connect the module to the PA, which kind of exciter? I
would know how to do it, just beeing curious...<br clear=3D"none" abp=3D"28=
49">
<br clear=3D"none" abp=3D"2850">
73, Stefan<br clear=3D"none" abp=3D"2851">
<br clear=3D"none" abp=3D"2852">
<br clear=3D"none" abp=3D"2853">
Am 02.02.2019 13:46, schrieb Markus Vester:
<div class=3D"yiv2990111096yqt0945518385" id=3D"yiv2990111096yqt44022" abp=
=3D"2854"><blockquote abp=3D"2855" type=3D"cite">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;" abp=3D"2856">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;" abp=3D"2857">Think I have&nbsp;tamed my u-blox LEA-6T modul=
e well enough, so
will try to&nbsp;send an EbNaut test this afternoon:<br clear=3D"none" abp=
=3D"2858">
  <br clear=3D"none" abp=3D"2859">
Frequency 137536 Hz,<br clear=3D"none" abp=3D"2860">
Start times: 13:00 and 13:30 UT,<br clear=3D"none" abp=3D"2861">
<strong>6 char, 3 sec symbols, &nbsp;8k19A, crc 16.</strong><br clear=3D"no=
ne" abp=3D"2862">
  <br clear=3D"none" abp=3D"2863">
Experimental scripts to control the timepulse-2 output are at <br clear=3D"=
none" abp=3D"2864">
<a class=3D"yiv2990111096moz-txt-link-freetext" href=3D"http://df6nm.bplace=
d.net/LF/u-blox_ebnaut/" target=3D"_blank" rel=3D"nofollow" shape=3D"rect" =
abp=3D"2865">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</a>&nbsp;<br clear=
=3D"none" abp=3D"2866">
and I intend to&nbsp;explain some details later this weekend.<br clear=3D"n=
one" abp=3D"2867">
  <br clear=3D"none" abp=3D"2868">
Best 73,<br clear=3D"none" abp=3D"2869">
Markus (DF6NM)<br clear=3D"none" abp=3D"2870">
  <br clear=3D"none" abp=3D"2871">
-----Urspr=C3=BCngliche Mitteilung-----<br clear=3D"none" abp=3D"2872">
Von: DK7FC <a class=3D"yiv2990111096moz-txt-link-rfc2396E" href=3D"mailto:s=
elberdenken@posteo.de" target=3D"_blank" rel=3D"nofollow" shape=3D"rect" ab=
p=3D"2873" ymailto=3D"mailto:selberdenken@posteo.de">&lt;selberdenken@poste=
o.de&gt;</a><br clear=3D"none" abp=3D"2874">
An: rsgb_lf_group <a class=3D"yiv2990111096moz-txt-link-rfc2396E" href=3D"m=
ailto:rsgb_lf_group@blacksheep.org" target=3D"_blank" rel=3D"nofollow" shap=
e=3D"rect" abp=3D"2875" ymailto=3D"mailto:rsgb_lf_group@blacksheep.org">&lt=
;rsgb_lf_group@blacksheep.org&gt;</a><br clear=3D"none" abp=3D"2876">
Verschickt: Do, 31. Jan. 2019 22:32<br clear=3D"none" abp=3D"2877">
Betreff: Re: LF: NEO-7M as a frequency source<br clear=3D"none" abp=3D"2878=
">
  <br clear=3D"none" abp=3D"2879">
...<br clear=3D"none" abp=3D"2880">
...would like to try to transmit EbNaut on 137 kHz directly from such a
  <br clear=3D"none" abp=3D"2881">
module.<br clear=3D"none" abp=3D"2882">
  <br clear=3D"none" abp=3D"2883">
73, Stefan<br clear=3D"none" abp=3D"2884">
  <br clear=3D"none" abp=3D"2885">
  <br clear=3D"none" abp=3D"2886">
  </div>
  </div>
</blockquote></div>
</div></div></div>
<br clear=3D"none" abp=3D"2887"></div></div></div></div>
------=_Part_2047109_2141085363.1549152953582--

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Date: Sun, 3 Feb 2019 00:34:22 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
Message-ID: <1272243865.2050719.1549154062237@mail.yahoo.com>
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 Content preview:  The first transmission at midnight went out ok, but the second
    one at 0:30 was aborted due to beginning rain. 73, Markus -----Ursprüngliche
    Mitteilung----- Von: Markus Vester An: rsgb_lf_group Verschickt: So, 3. Feb.
    2019 1:18 Betreff: Re: LF: EbNaut test from u-blox module 
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Subject: Re: LF: EbNaut test from u-blox module
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The first transmission at midnight went out ok, but the second one at 0:30 =
was aborted due to beginning rain.

73, Markus


-----Urspr=C3=BCngliche Mitteilung-----
Von: Markus Vester <markusvester@aol.com>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: So, 3. Feb. 2019 1:18
Betreff: Re: LF: EbNaut test from u-blox module

Thanks Stefan and Michel (F5WK) for your excellent reports!=20

The=C2=A0residual phase variation was surely from the antenna moving in the=
 wind. I haven't been using the=C2=A0automatic tuner, and also did some man=
ual tweaking=C2=A0near the beginning.=C2=A0Interestingly Michel's phase tra=
ce was a perfect copy of yours.

The exciter and 250 W PA are the same as=C2=A0in my usual LF setup, except =
that the feed from the SSB=C2=A0exciter has been replaced by the TP2 output=
 from the GPS device,=C2=A0connected=C2=A0through 470 ohm and a piece of co=
ax. The=C2=A0LEA-6T module came=C2=A0from Hongkong for=C2=A027 =E2=82=AC an=
d is very similar to the one described here
http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardow=
n-and-initial-test/

I=C2=A0am now repeating the same=C2=A0pair of transmissions=C2=A0at 0:00 an=
d 0:30 UT, but moved to=C2=A0137545 Hz to fit inside=C2=A0Jay's narrowband =
recording.=20

Best 73,
Markus=C2=A0=C2=A0(DF6NM)

=C2=A0=C2=A0

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Sa, 2. Feb. 2019 14:52
Betreff: Re: LF: EbNaut test from u-blox module

Hi Markus,=20

Great work! It seems to work well. There are some dynamic changes inthe pha=
se. Would you think it is propagation?
So this is a Windows solution without the need to use an upconverter.Let's =
see if this will help to make the mode more popular, or not.
How did you connect the module to the PA, which kind of exciter? Iwould kno=
w how to do it, just beeing curious...

73, Stefan


Am 02.02.2019 13:46, schrieb Markus Vester:
  Think I have=C2=A0tamed my u-blox LEA-6T module well enough, sowill try t=
o=C2=A0send an EbNaut test this afternoon:
=20
Frequency 137536 Hz,
Start times: 13:00 and 13:30 UT,
6 char, 3 sec symbols, =C2=A08k19A, crc 16.
=20
Experimental scripts to control the timepulse-2 output are at=20
http://df6nm.bplaced.net/LF/u-blox_ebnaut/=C2=A0
and I intend to=C2=A0explain some details later this weekend.
=20
Best 73,
Markus (DF6NM)
=20
-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Do, 31. Jan. 2019 22:32
Betreff: Re: LF: NEO-7M as a frequency source
=20
...
...would like to try to transmit EbNaut on 137 kHz directly from such a=20
module.
=20
73, Stefan
=20
=20
 =20


------=_Part_2050718_480173661.1549154062236
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;">The first transmission at midnight went out ok, but the =
second one at 0:30 was aborted due to beginning rain.<br><br>73, Markus<br>=
<br><br>-----Urspr=C3=BCngliche Mitteilung-----<br>Von: Markus Vester &lt;m=
arkusvester@aol.com&gt;<br>An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.o=
rg&gt;<br>Verschickt: So, 3. Feb. 2019 1:18<br>Betreff: Re: LF: EbNaut test=
 from u-blox module<br><br></div><div id=3D"yiv4882573415"><div style=3D"co=
lor: black; font-family: arial, helvetica, sans-serif; font-size: 10pt;"><d=
iv id=3D"yiv4882573415"><div><div style=3D"color: black; font-family: arial=
, helvetica, sans-serif; font-size: 10pt;"><div style=3D"color: black; font=
-family: arial, helvetica, sans-serif; font-size: 10pt;">Thanks Stefan and =
Michel (F5WK) for your excellent reports! <br clear=3D"none"><br clear=3D"n=
one">The&nbsp;residual phase variation was surely from the antenna moving i=
n the wind. I haven't been using the&nbsp;automatic tuner, and also did som=
e manual tweaking&nbsp;near the beginning.&nbsp;Interestingly Michel's phas=
e trace was a perfect copy of yours.<br clear=3D"none"><br clear=3D"none">T=
he exciter and 250 W PA are the same as&nbsp;in my usual LF setup, except t=
hat the feed from the SSB&nbsp;exciter has been replaced by the TP2 output =
from the GPS device,&nbsp;connected&nbsp;through 470 ohm and a piece of coa=
x. The&nbsp;LEA-6T module came&nbsp;from Hongkong for&nbsp;27 =E2=82=AC and=
 is very similar to the one described here<br>http://www.eevblog.com/forum/=
projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/<br clear=
=3D"none"><br clear=3D"none">I&nbsp;am now repeating the same&nbsp;pair of =
transmissions&nbsp;at<strong> 0:00</strong> and<strong> 0:30 UT</strong>, b=
ut moved to&nbsp;<strong>137545 Hz</strong> to fit inside&nbsp;Jay's narrow=
band recording. <br clear=3D"none"><br clear=3D"none">Best 73,<br clear=3D"=
none">Markus&nbsp;&nbsp;(DF6NM)<br clear=3D"none"><br clear=3D"none">&nbsp;=
&nbsp;<br clear=3D"none"><br clear=3D"none">-----Urspr=C3=BCngliche Mitteil=
ung-----<br clear=3D"none">Von: DK7FC &lt;selberdenken@posteo.de&gt;<br cle=
ar=3D"none">An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br clear=
=3D"none">Verschickt: Sa, 2. Feb. 2019 14:52<br clear=3D"none">Betreff: Re:=
 LF: EbNaut test from u-blox module<br clear=3D"none"><br clear=3D"none"></=
div><div class=3D"yiv4882573415yqt2807499086" id=3D"yiv4882573415yqt91517">=
<div id=3D"yiv4882573415"><div>
Hi Markus, <br clear=3D"none">
<br clear=3D"none">
Great work! It seems to work well. There are some dynamic changes in
the phase. Would you think it is propagation?<br clear=3D"none">
So this is a Windows solution without the need to use an upconverter.
Let's see if this will help to make the mode more popular, or not.<br clear=
=3D"none">
How did you connect the module to the PA, which kind of exciter? I
would know how to do it, just beeing curious...<br clear=3D"none">
<br clear=3D"none">
73, Stefan<br clear=3D"none">
<br clear=3D"none">
<br clear=3D"none">
Am 02.02.2019 13:46, schrieb Markus Vester:
<div class=3D"yiv4882573415yqt0945518385" id=3D"yiv4882573415yqt44022"><blo=
ckquote type=3D"cite">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;">Think I have&nbsp;tamed my u-blox LEA-6T module well enough=
, so
will try to&nbsp;send an EbNaut test this afternoon:<br clear=3D"none">
  <br clear=3D"none">
Frequency 137536 Hz,<br clear=3D"none">
Start times: 13:00 and 13:30 UT,<br clear=3D"none">
<strong>6 char, 3 sec symbols, &nbsp;8k19A, crc 16.</strong><br clear=3D"no=
ne">
  <br clear=3D"none">
Experimental scripts to control the timepulse-2 output are at <br clear=3D"=
none">
<a class=3D"yiv4882573415moz-txt-link-freetext" href=3D"http://df6nm.bplace=
d.net/LF/u-blox_ebnaut/" target=3D"_blank" rel=3D"noopener noreferrer" shap=
e=3D"rect">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</a>&nbsp;<br clear=3D=
"none">
and I intend to&nbsp;explain some details later this weekend.<br clear=3D"n=
one">
  <br clear=3D"none">
Best 73,<br clear=3D"none">
Markus (DF6NM)<br clear=3D"none">
  <br clear=3D"none">
-----Urspr=C3=BCngliche Mitteilung-----<br clear=3D"none">
Von: DK7FC <a class=3D"yiv4882573415moz-txt-link-rfc2396E" href=3D"mailto:s=
elberdenken@posteo.de" target=3D"_blank" rel=3D"noopener noreferrer" shape=
=3D"rect" ymailto=3D"mailto:selberdenken@posteo.de">&lt;selberdenken@posteo=
.de&gt;</a><br clear=3D"none">
An: rsgb_lf_group <a class=3D"yiv4882573415moz-txt-link-rfc2396E" href=3D"m=
ailto:rsgb_lf_group@blacksheep.org" target=3D"_blank" rel=3D"noopener noref=
errer" shape=3D"rect" ymailto=3D"mailto:rsgb_lf_group@blacksheep.org">&lt;r=
sgb_lf_group@blacksheep.org&gt;</a><br clear=3D"none">
Verschickt: Do, 31. Jan. 2019 22:32<br clear=3D"none">
Betreff: Re: LF: NEO-7M as a frequency source<br clear=3D"none">
  <br clear=3D"none">
...<br clear=3D"none">
...would like to try to transmit EbNaut on 137 kHz directly from such a
  <br clear=3D"none">
module.<br clear=3D"none">
  <br clear=3D"none">
73, Stefan<br clear=3D"none">
  <br clear=3D"none">
  <br clear=3D"none">
  </div>
  </div>
</blockquote></div>
</div></div></div>
<br clear=3D"none"></div></div></div></div></div></div>
------=_Part_2050718_480173661.1549154062236--

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 Content preview:  Hi Markus, Snow-rain here, not the most inviting climate for
    outdoor experiments, although i would like to climb the tree to repair my
    VLF E-field :-) I just thought about your latest tool and wonder if it is
    possible to do the same for WSPR-2 or WSPR-15, all without a transceiver
   or upconverter or the whole dial stuff ;-) It would be comfortable an [...]
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Subject: Re: LF: EbNaut test from u-blox module - and what about WSPR?
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Hi Markus,

Snow-rain here, not the most inviting climate for outdoor experiments, 
although i would like to climb the tree to repair my VLF E-field :-)

I just thought about your latest tool and wonder if it is possible to do 
the same for WSPR-2 or WSPR-15, all without a transceiver or upconverter 
or the whole dial stuff ;-) It would be comfortable and power saving. So 
much can be done...

73, Stefan

Am 03.02.2019 01:15, schrieb Markus Vester:
> Thanks Stefan and Michel (F5WK) for your excellent reports!
>
> The residual phase variation was surely from the antenna moving in the 
> wind. I haven't been using the automatic tuner, and also did some 
> manual tweaking near the beginning. Interestingly Michel's phase trace 
> was a perfect copy of yours.
>
> The exciter and 250 W PA are the same as in my usual LF setup, except 
> that the feed from the SSB exciter has been replaced by the TP2 output 
> from the GPS device, connected through 470 ohm and a piece of coax. 
> The LEA-6T module came from Hongkong for 27 € and is very similar to 
> the one described here
> http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/
>
> I am now repeating the same pair of transmissions at* 0:00* and* 0:30 
> UT*, but moved to *137545 Hz* to fit inside Jay's narrowband recording.
>
> Best 73,
> Markus  (DF6NM)
>
>
>
> -----Ursprüngliche Mitteilung-----
> Von: DK7FC <selberdenken@posteo.de>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Sa, 2. Feb. 2019 14:52
> Betreff: Re: LF: EbNaut test from u-blox module
>
> Hi Markus,
>
> Great work! It seems to work well. There are some dynamic changes in 
> the phase. Would you think it is propagation?
> So this is a Windows solution without the need to use an upconverter. 
> Let's see if this will help to make the mode more popular, or not.
> How did you connect the module to the PA, which kind of exciter? I 
> would know how to do it, just beeing curious...
>
> 73, Stefan
>
>
> Am 02.02.2019 13:46, schrieb Markus Vester:
>> Think I have tamed my u-blox LEA-6T module well enough, so will try 
>> to send an EbNaut test this afternoon:
>>
>> Frequency 137536 Hz,
>> Start times: 13:00 and 13:30 UT,
>> *6 char, 3 sec symbols,  8k19A, crc 16.*
>>
>> Experimental scripts to control the timepulse-2 output are at
>> http://df6nm.bplaced.net/LF/u-blox_ebnaut/
>> and I intend to explain some details later this weekend.
>>
>> Best 73,
>> Markus (DF6NM)
>>
>> -----Ursprüngliche Mitteilung-----
>> Von: DK7FC <selberdenken@posteo.de> <mailto:selberdenken@posteo.de>
>> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org> 
>> <mailto:rsgb_lf_group@blacksheep.org>
>> Verschickt: Do, 31. Jan. 2019 22:32
>> Betreff: Re: LF: NEO-7M as a frequency source
>>
>> ...
>> ...would like to try to transmit EbNaut on 137 kHz directly from such a
>> module.
>>
>> 73, Stefan
>>
>>
>

--------------090907000709040001070605
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Hi Markus, <br>
<br>
Snow-rain here, not the most inviting climate for outdoor experiments,
although i would like to climb the tree to repair my VLF E-field :-)<br>
<br>
I just thought about your latest tool and wonder if it is possible to
do the same for WSPR-2 or WSPR-15, all without a transceiver or
upconverter or the whole dial stuff ;-) It would be comfortable and
power saving. So much can be done...<br>
<br>
73, Stefan<br>
<br>
Am 03.02.2019 01:15, schrieb Markus Vester:
<blockquote cite="mid:114026853.2047110.1549152953584@mail.yahoo.com"
 type="cite">
  <div
 style="font-size: 10pt; font-family: arial,helvetica,sans-serif; color: black;">
  <div id="yiv2990111096" abp="2819">
  <div abp="2820">
  <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;"
 abp="2821">
  <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;"
 abp="2822">Thanks Stefan and Michel (F5WK) for your excellent reports!
  <br abp="2823" clear="none">
  <br abp="2824" clear="none">
The residual phase variation was surely from the antenna moving in the
wind. I haven't been using the automatic tuner, and also did some
manual tweaking near the beginning. Interestingly Michel's phase trace
was a perfect copy of yours.<br abp="2825" clear="none">
  <br abp="2826" clear="none">
The exciter and 250 W PA are the same as in my usual LF setup, except
that the feed from the SSB exciter has been replaced by the TP2 output
from the GPS device, connected through 470 ohm and a piece of coax.
The LEA-6T module came from Hongkong for 27 € and is very similar to
the one described here<br>
<a class="moz-txt-link-freetext" href="http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/">http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/</a><br
 abp="2827" clear="none">
  <br abp="2828" clear="none">
I am now repeating the same pair of transmissions at<strong> 0:00</strong>
and<strong> 0:30 UT</strong>, but moved to <strong>137545 Hz</strong>
to fit inside Jay's narrowband recording. <br abp="2829" clear="none">
  <br abp="2830" clear="none">
Best 73,<br abp="2831" clear="none">
Markus  (DF6NM)<br abp="2832" clear="none">
  <br abp="2833" clear="none">
  <br abp="2834" clear="none">
  <br abp="2835" clear="none">
-----Ursprüngliche Mitteilung-----<br abp="2836" clear="none">
Von: DK7FC <a class="moz-txt-link-rfc2396E" href="mailto:selberdenken@posteo.de">&lt;selberdenken@posteo.de&gt;</a><br abp="2837" clear="none">
An: rsgb_lf_group <a class="moz-txt-link-rfc2396E" href="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br abp="2838"
 clear="none">
Verschickt: Sa, 2. Feb. 2019 14:52<br abp="2839" clear="none">
Betreff: Re: LF: EbNaut test from u-blox module<br abp="2840"
 clear="none">
  <br abp="2841" clear="none">
  </div>
  <div class="yiv2990111096yqt2807499086" id="yiv2990111096yqt91517"
 abp="2842">
  <div id="yiv2990111096" abp="2843">
  <div abp="2844">Hi Markus, <br abp="2845" clear="none">
  <br abp="2846" clear="none">
Great work! It seems to work well. There are some dynamic changes in
the phase. Would you think it is propagation?<br abp="2847" clear="none">
So this is a Windows solution without the need to use an upconverter.
Let's see if this will help to make the mode more popular, or not.<br
 abp="2848" clear="none">
How did you connect the module to the PA, which kind of exciter? I
would know how to do it, just beeing curious...<br abp="2849"
 clear="none">
  <br abp="2850" clear="none">
73, Stefan<br abp="2851" clear="none">
  <br abp="2852" clear="none">
  <br abp="2853" clear="none">
Am 02.02.2019 13:46, schrieb Markus Vester:
  <div class="yiv2990111096yqt0945518385" id="yiv2990111096yqt44022"
 abp="2854">
  <blockquote abp="2855" type="cite">
    <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;"
 abp="2856">
    <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;"
 abp="2857">Think I have tamed my u-blox LEA-6T module well enough, so
will try to send an EbNaut test this afternoon:<br abp="2858"
 clear="none">
    <br abp="2859" clear="none">
Frequency 137536 Hz,<br abp="2860" clear="none">
Start times: 13:00 and 13:30 UT,<br abp="2861" clear="none">
    <strong>6 char, 3 sec symbols,  8k19A, crc 16.</strong><br
 abp="2862" clear="none">
    <br abp="2863" clear="none">
Experimental scripts to control the timepulse-2 output are at <br
 abp="2864" clear="none">
    <a moz-do-not-send="true" class="yiv2990111096moz-txt-link-freetext"
 href="http://df6nm.bplaced.net/LF/u-blox_ebnaut/" target="_blank"
 rel="nofollow" shape="rect" abp="2865">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</a> <br
 abp="2866" clear="none">
and I intend to explain some details later this weekend.<br abp="2867"
 clear="none">
    <br abp="2868" clear="none">
Best 73,<br abp="2869" clear="none">
Markus (DF6NM)<br abp="2870" clear="none">
    <br abp="2871" clear="none">
-----Ursprüngliche Mitteilung-----<br abp="2872" clear="none">
Von: DK7FC <a moz-do-not-send="true"
 class="yiv2990111096moz-txt-link-rfc2396E"
 href="mailto:selberdenken@posteo.de" target="_blank" rel="nofollow"
 shape="rect" abp="2873" ymailto="mailto:selberdenken@posteo.de">&lt;selberdenken@posteo.de&gt;</a><br
 abp="2874" clear="none">
An: rsgb_lf_group <a moz-do-not-send="true"
 class="yiv2990111096moz-txt-link-rfc2396E"
 href="mailto:rsgb_lf_group@blacksheep.org" target="_blank"
 rel="nofollow" shape="rect" abp="2875"
 ymailto="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br
 abp="2876" clear="none">
Verschickt: Do, 31. Jan. 2019 22:32<br abp="2877" clear="none">
Betreff: Re: LF: NEO-7M as a frequency source<br abp="2878" clear="none">
    <br abp="2879" clear="none">
...<br abp="2880" clear="none">
...would like to try to transmit EbNaut on 137 kHz directly from such a
    <br abp="2881" clear="none">
module.<br abp="2882" clear="none">
    <br abp="2883" clear="none">
73, Stefan<br abp="2884" clear="none">
    <br abp="2885" clear="none">
    <br abp="2886" clear="none">
    </div>
    </div>
  </blockquote>
  </div>
  </div>
  </div>
  </div>
  <br abp="2887" clear="none">
  </div>
  </div>
  </div>
  </div>
</blockquote>
</body>
</html>

--------------090907000709040001070605--

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 Content preview:  ...indeed! Since more than 72 hours i'm running the WSPR transmission
    in 25% duty cycle (each 8 minutes). First i tuned to 20 A antenna current
    and the temperature / antenna current changes were much [...] 
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Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2
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...indeed! Since more than 72 hours i'm running the WSPR transmission in
25% duty cycle (each 8 minutes). First i tuned to 20 A antenna current
and the temperature / antenna current changes were much smaller. But
there was a certain click, or krrrrkkrt audible from the Cs. It was
likely that there were indeed internal voltage breakthroughs, which were
self-healing. Now after 3 days the current dropped again to 14 A,
meaning that the capacity dropped, so the loop became detuned and so the
RF current and voltages dropped to a level which is accepted by the
capacitors.

So my conclusion is, the derating curves actually should be considered.

I wonder if the effect is still happening if one keeps the temperatures
down at 25 C or even lower. When placing the capacitors in de-ionised
iced water, it should be possible to keep the temperatures down, also in
the internal of the capacitor.

But all in all this is not a good solution. Fortunately i have another
antenna which is more efficient :-)

73, Stefan


Am 31.01.2019 11:54, schrieb dhchurch:
> Hello Dimitrios
> Polypropylene capacitors can actually self-heal to such an extent that
> there's little left of them. The melting point of polypropylene is not
> very high and they can end up as just a liitle blob of plastic.
> Don't worry though, I still use them suitably rated for the frequency
> in use and most of them are 600Vac or more.
> 73, Hugh, M0DSZ
>
>     ----- Receiving the following content -----
>     *From:* Dimitrios Tsifakis <mailto:dtsifakis@gmail.com>
>     *Receiver:* rsgb_lf_group <mailto:rsgb_lf_group@blacksheep.org>
>     *Time:* 2019-01-31, 00:25:55
>     *Subject:* Re: LF: TXing WSPR/MF on an indoor loop, part 2
>
>     Hi Stefan,
>
>     In my experience these polypropylene capacitors when they fail, they
>     just lose some capacitance. I think they call it 'self healing', maybe
>     they imply that when they fail there is no short circuit?
>
>     I have some really nice silver mica capacitors (ex MW broadcast stuff)
>     that would be perfect for this task...
>
>     Anyway, I am slowly gearing up for some VLF action over here. The
>     other day I did some tests at 16.72 kHz into an ugly loop (very
>     roughly 120 metres by 3 metres, single turn) and I was able to receive
>     my signals using an unoptimise ferrite antenna at a bit over 2 km from
>     the TX. I don't think I am in the near field at that distance, am I?
>     :-)
>
>     73, Dimitris VK2COW
>
>     >
>

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...indeed! Since more than 72 hours i'm running the WSPR transmission
in 25% duty cycle (each 8 minutes). First i tuned to 20 A antenna
current and the temperature / antenna current changes were much
smaller. But there was a certain click, or krrrrkkrt audible from the
Cs. It was likely that there were indeed internal voltage
breakthroughs, which were self-healing. Now after 3 days the current
dropped again to 14 A, meaning that the capacity dropped, so the loop
became detuned and so the RF current and voltages dropped to a level
which is accepted by the capacitors.<br>
<br>
So my conclusion is, the derating curves actually should be considered.<br>
<br>
I wonder if the effect is still happening if one keeps the temperatures
down at 25 C or even lower. When placing the capacitors in de-ionised
iced water, it should be possible to keep the temperatures down, also
in the internal of the capacitor.<br>
<br>
But all in all this is not a good solution. Fortunately i have another
antenna which is more efficient :-)<br>
<br>
73, Stefan<br>
<br>
<br>
Am 31.01.2019 11:54, schrieb dhchurch:
<blockquote cite="mid:DM__190131105008_42113600808@smtp.eclipse.co.uk"
 type="cite">
  <title></title>
  <meta
 content="KsDHTMLEDLib.ocx, FreeWare HTML Editor 1.164.2, &copy; Kurt Senfer"
 name="GENERATOR">
  <meta http-equiv="Content-Type" content="text/html; charset=GB2312">
  <div>Hello Dimitrios</div>
  <div>&nbsp;</div>
  <div>Polypropylene capacitors can actually self-heal to such an
extent that there's little left of them. The melting point of
polypropylene is not very high&nbsp;and they can end up as just a liitle
blob of plastic.&nbsp;</div>
  <div>&nbsp;</div>
  <div>Don't worry though, I still use them suitably rated for the
frequency in use and most of them are 600Vac or more.</div>
  <div>&nbsp;</div>
  <div>73, Hugh, M0DSZ</div>
  <blockquote
 style="border-left: 2px solid rgb(0, 0, 0); padding-right: 0px; padding-left: 5px; margin-left: 5px; margin-right: 0px;">
    <div
 style="font-weight: normal; font-size: 9pt; line-height: normal; font-style: normal; font-variant: normal;">-----
Receiving the following content ----- </div>
    <div
 style="background: rgb(228, 228, 228) none repeat scroll 0% 0%; font-weight: normal; font-size: 9pt; -moz-background-clip: border; -moz-background-origin: padding; -moz-background-inline-policy: continuous; line-height: normal; font-style: normal; font-variant: normal;"><b>From:</b>
    <a moz-do-not-send="true" href="mailto:dtsifakis@gmail.com">Dimitrios
Tsifakis</a> </div>
    <div
 style="font-weight: normal; font-size: 9pt; line-height: normal; font-style: normal; font-variant: normal;"><b>Receiver:</b>
    <a moz-do-not-send="true" href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group</a>
    </div>
    <div
 style="font-weight: normal; font-size: 9pt; line-height: normal; font-style: normal; font-variant: normal;"><b>Time:</b>
2019-01-31, 00:25:55</div>
    <div
 style="font-weight: normal; font-size: 9pt; line-height: normal; font-style: normal; font-variant: normal;"><b>Subject:</b>
Re: LF: TXing WSPR/MF on an indoor loop, part 2</div>
    <div><br>
    </div>
    <div>
    <div>Hi Stefan,<br>
    <br>
In my experience these polypropylene capacitors when they fail, they<br>
just lose some capacitance. I think they call it 'self healing', maybe<br>
they imply that when they fail there is no short circuit?<br>
    <br>
I have some really nice silver mica capacitors (ex MW broadcast stuff)<br>
that would be perfect for this task...<br>
    <br>
Anyway, I am slowly gearing up for some VLF action over here. The<br>
other day I did some tests at 16.72 kHz into an ugly loop (very<br>
roughly 120 metres by 3 metres, single turn) and I was able to receive<br>
my signals using an unoptimise ferrite antenna at a bit over 2 km from<br>
the TX. I don't think I am in the near field at that distance, am I?<br>
:-)<br>
    <br>
73, Dimitris VK2COW<br>
    <br>
&gt;<br>
    <br>
    </div>
    </div>
  </blockquote>
</blockquote>
</body>
</html>

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 Content preview:  LF, Good copy of 'R'. Nice to see some activity in DFCW on
    LF. Grabber as usual under: http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_LF_DX_Grabber.html
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LF,

Good copy of 'R'.


Nice to see some activity in DFCW on LF.
Grabber as usual under: 
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_LF_DX_Grabber.html

73, Stefan

--------------010401040504030809010404
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LF, <br>
<br>
Good copy of 'R'. <br>
<img src="cid:part1.01020906.03000602@posteo.de" alt=""><br>
<br>
Nice to see some activity in DFCW on LF.<br>
Grabber as usual under:
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_LF_DX_Grabber.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_LF_DX_Grabber.html</a><br>
<br>
73, Stefan<br>
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--------------010004090403060908080803--

--------------010401040504030809010404--

From owner-rsgb_lf_group@blacksheep.org  Sun Feb  3 18:25:42 2019
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From: <hvanesce@comcast.net>
To: <rsgb_lf_group@blacksheep.org>
References: <168a5557287.marcocadeddu@tin.it>
In-Reply-To: <168a5557287.marcocadeddu@tin.it>
Date: Sun, 3 Feb 2019 12:20:24 -0500
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 Content preview:  Thanks Marco, I added the 940C to my list. I don’t know
   if the ESRs in the 940C data sheet are specified at 120 Hz or 1 kHz, but in
    any case the 940C ESR and other specifications look good. 
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Subject: RE: RE: LF: TXing on indoor/outdoor loops and Silver mica caps
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Thanks Marco,

=20

I added the 940C to my list. =20

=20

I don=E2=80=99t know if the ESRs in the 940C data sheet are specified at =
120 Hz or 1 kHz, but in any case the 940C ESR and other specifications =
look good.

=20

Looking at the 940C package brings to mind that I have been =
series/parallel stacking the rectangular PHE450 capacitors incorrectly: =
no air gap for cooling. I wonder if a stack of 940Cs would be better =
than rectangular capacitors (PHE450 etc.) in a forced-air configuration. =
Or in de-ionized ice water as Stefan mentioned.

=20

73,

=20

Jim AA5BW    =20

=20

From: owner-rsgb_lf_group@blacksheep.org =
[mailto:owner-rsgb_lf_group@blacksheep.org] On Behalf Of =
marcocadeddu@tin.it
Sent: Thursday, January 31, 2019 2:14 PM
To: rsgb_lf_group@blacksheep.org
Subject: R: RE: LF: TXing on indoor/outdoor loops and Silver mica caps

=20

Hi Jim,
just to share my feelings / thoughs ...
Since I started to play with LF I collected a number of R.I.P. caps ;-) =
and failure reason, on my opinion, was that the current was exceeding =
the capability of the cap.
I was used to refer to the insulation voltage and thus seen the =
trepassing of a lot of caps, the found this serie=20

http://www.cde.com/resources/catalogs/940C.pdf

and never had further trespassing at least in low impedance, relative =
high power: for instance for the caps insulating the dc component and =
carrying the RF power from a 500W pushpull @28Vdc.
For other similar application like for instance the caps in the output =
LC of Decca style PA or Class E PA I used succesfully either the above =
CDE caps or WIMA FKP1 combining series /parallel in order to have the =
wished capacitance / voltage insulation and current capability.

I guess should be nice organize a day to remember all our ex-devices ;-)

73, Marco IK1HSS


----Messaggio originale----
Da: hvanesce@comcast.net
Data: 31-gen-2019 18.55
A: <rsgb_lf_group@blacksheep.org>
Ogg: RE: LF: TXing on indoor/outdoor loops and Silver mica caps

=20

I have been using what appear to be similar polypropylene capacitors =
[data sheet specifications (see below) including spectral loss tangent =
seem very similar] for multi-turn indoor and outdoor (35 meter x 35 =
meter) single-turn VLF transmitting loops for about five years (when =
time is available) and have found the following:

1) Temperature rise has been roughly consistent with the spectral loss =
tangent table

2) No change noticed in capacitance after approximately 200 of hours of =
transmitter operation at capacitor case temperature of 115 F (46 C)

=20

Used 80-PHE450HD6470JR6L2 (0.47 uF) and also used 0.1 uF through 1.0 uF =
from the same PHE450 product line; always series/parallel stacking =
capacitors of the same value to enable higher current and/or voltage at =
a given capacitance.

=20

Data sheet:

https://www.mouser.com/datasheet/2/212/KEM_F3033_PHE450-1104182.pdf

=20

Reached somewhat of a practical limit of series/parallel stacking of =
these capacitors, for indoor multi-turn loops from 1 meter diameter to =
ten square meters, and outdoor loop 35 m x 35 m; and have hoped to find =
capacitors that would allow more current and voltage. I thought I had =
investigated (through calculations, not on the workbench) silver micas =
and found these polypropylene capacitors to be better based on =
calculations, but based on the messages between Stefan, Dimitris and =
Marko I must have missed something (perhaps temperature rating?); thanks =
for the inputs on this topic; looking forward to silver micas.

=20

73,

=20

Jim AA5BW       =20

=20

From: owner-rsgb_lf_group@blacksheep.org =
[mailto:owner-rsgb_lf_group@blacksheep.org] On Behalf Of dhchurch
Sent: Thursday, January 31, 2019 5:55 AM
To: RSGB LF group
Subject: Re: Re: LF: TXing WSPR/MF on an indoor loop, part 2

=20

Hello Dimitrios

=20

Polypropylene capacitors can actually self-heal to such an extent that =
there's little left of them. The melting point of polypropylene is not =
very high and they can end up as just a liitle blob of plastic.=20

=20

Don't worry though, I still use them suitably rated for the frequency in =
use and most of them are 600Vac or more.

=20

73, Hugh, M0DSZ

----- Receiving the following content -----=20

From: Dimitrios Tsifakis <mailto:dtsifakis@gmail.com> =20

Receiver: rsgb_lf_group <mailto:rsgb_lf_group@blacksheep.org> =20

Time: 2019-01-31, 00:25:55

Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2

=20

Hi Stefan,

In my experience these polypropylene capacitors when they fail, they
just lose some capacitance. I think they call it 'self healing', maybe
they imply that when they fail there is no short circuit?

I have some really nice silver mica capacitors (ex MW broadcast stuff)
that would be perfect for this task...

Anyway, I am slowly gearing up for some VLF action over here. The
other day I did some tests at 16.72 kHz into an ugly loop (very
roughly 120 metres by 3 metres, single turn) and I was able to receive
my signals using an unoptimise ferrite antenna at a bit over 2 km from
the TX. I don't think I am in the near field at that distance, am I?
:-)

73, Dimitris VK2COW

>

=20


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<o:idmap v:ext=3D"edit" data=3D"1" />
</o:shapelayout></xml><![endif]--></head><body lang=3DEN-US link=3Dblue =
vlink=3Dpurple><div class=3DWordSection1><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Thanks Marco,<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>I added the 940C to my list.=C2=A0 <o:p></o:p></span></p><p =
class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>I don=E2=80=99t know if the ESRs in the 940C data sheet are specified =
at 120 Hz or 1 kHz, but in any case the 940C ESR and other =
specifications look good.<o:p></o:p></span></p><p =
class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Looking at the 940C package brings to mind that I have been =
series/parallel stacking the rectangular </span><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>PHE450 capacitors incorrectly: no air gap for cooling. I wonder if a =
stack of 940Cs would be better than rectangular capacitors (PHE450 etc.) =
in a forced-air configuration. Or in de-ionized ice water as Stefan =
mentioned.<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>73,<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Jim AA5BW =C2=A0=C2=A0</span><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>=C2=A0=C2=A0<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><b><span =
style=3D'font-size:10.0pt;font-family:"Tahoma","sans-serif"'>From:</span>=
</b><span style=3D'font-size:10.0pt;font-family:"Tahoma","sans-serif"'> =
owner-rsgb_lf_group@blacksheep.org =
[mailto:owner-rsgb_lf_group@blacksheep.org] <b>On Behalf Of =
</b>marcocadeddu@tin.it<br><b>Sent:</b> Thursday, January 31, 2019 2:14 =
PM<br><b>To:</b> rsgb_lf_group@blacksheep.org<br><b>Subject:</b> R: RE: =
LF: TXing on indoor/outdoor loops and Silver mica =
caps<o:p></o:p></span></p><p class=3DMsoNormal><o:p>&nbsp;</o:p></p><p =
class=3DMsoNormal style=3D'margin-bottom:12.0pt'>Hi Jim,<br>just to =
share my feelings / thoughs ...<br>Since I started to play with LF I =
collected a number of R.I.P. caps ;-) and failure reason, on my opinion, =
was that the current was exceeding the capability of the cap.<br>I was =
used to refer to the insulation voltage and thus seen the trepassing of =
a lot of caps, the found this serie <br><br><a =
href=3D"http://www.cde.com/resources/catalogs/940C.pdf">http://www.cde.co=
m/resources/catalogs/940C.pdf</a><br><br>and never had further =
trespassing at least in low impedance, relative high power: for instance =
for the caps insulating the dc component and carrying the RF power from =
a 500W pushpull @28Vdc.<br>For other similar application like for =
instance the caps in the output LC of Decca style PA or Class E PA I =
used succesfully either the above CDE caps or WIMA FKP1 combining series =
/parallel in order to have the wished capacitance / voltage insulation =
and current capability.<br><br>I guess should be nice organize a day to =
remember all our ex-devices ;-)<br><br>73, Marco =
IK1HSS<br><br><br>----Messaggio originale----<br>Da: <a =
href=3D"mailto:hvanesce@comcast.net">hvanesce@comcast.net</a><br>Data: =
31-gen-2019 18.55<br>A: &lt;<a =
href=3D"mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org=
</a>&gt;<br>Ogg: RE: LF: TXing on indoor/outdoor loops and Silver mica =
caps<o:p></o:p></p><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>&nbsp;</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>I have been using what appear to be similar polypropylene capacitors =
[data sheet specifications (see below) including spectral loss tangent =
seem very similar] for multi-turn indoor and outdoor (35 meter x 35 =
meter) single-turn VLF transmitting loops for about five years (when =
time is available) and have found the following:</span><o:p></o:p></p><p =
class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>1) Temperature rise has been roughly consistent with the spectral =
loss tangent table</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>2) No change noticed in capacitance after approximately 200 of hours =
of transmitter operation at capacitor case temperature of 115 F (46 =
C)</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>&nbsp;</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Used 80-PHE450HD6470JR6L2 (0.47 uF) and also used 0.1 uF through 1.0 =
uF from the same PHE450 product line; always series/parallel stacking =
capacitors of the same value to enable higher current and/or voltage at =
a given capacitance.</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:10.0pt;font-family:"Arial","sans-serif";color:#333333'=
>&nbsp;</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:10.0pt;font-family:"Arial","sans-serif";color:#333333'=
>Data sheet:</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><a =
href=3D"https://www.mouser.com/datasheet/2/212/KEM_F3033_PHE450-1104182.p=
df">https://www.mouser.com/datasheet/2/212/KEM_F3033_PHE450-1104182.pdf</=
a></span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>&nbsp;</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Reached somewhat of a practical limit of series/parallel stacking of =
these capacitors, for indoor multi-turn loops from 1 meter diameter to =
ten square meters, and outdoor loop 35 m x 35 m; and have hoped to find =
capacitors that would allow more current and voltage. I thought I had =
investigated (through calculations, not on the workbench) silver micas =
and found these polypropylene capacitors to be better based on =
calculations, but based on the messages between Stefan, Dimitris and =
Marko I must have missed something (perhaps temperature rating?); thanks =
for the inputs on this topic; looking forward to silver =
micas.</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>&nbsp;</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>73,</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>&nbsp;</span><o:p></o:p></p><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Jim AA5BW =
&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;</span><o:p></o:p></p><p =
class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>&nbsp;</span><o:p></o:p></p><div><div =
style=3D'border:none;border-top:solid #B5C4DF 1.0pt;padding:3.0pt 0in =
0in 0in'><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><b><span =
style=3D'font-size:10.0pt;font-family:"Tahoma","sans-serif"'>From:</span>=
</b><span style=3D'font-size:10.0pt;font-family:"Tahoma","sans-serif"'> =
<a =
href=3D"mailto:owner-rsgb_lf_group@blacksheep.org">owner-rsgb_lf_group@bl=
acksheep.org</a> [<a =
href=3D"mailto:owner-rsgb_lf_group@blacksheep.org">mailto:owner-rsgb_lf_g=
roup@blacksheep.org</a>] <b>On Behalf Of </b>dhchurch<br><b>Sent:</b> =
Thursday, January 31, 2019 5:55 AM<br><b>To:</b> RSGB LF =
group<br><b>Subject:</b> Re: Re: LF: TXing WSPR/MF on an indoor loop, =
part 2</span><o:p></o:p></p></div></div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'>&nbsp;<o:p><=
/o:p></p><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>Hello =
Dimitrios</span><o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>&nbsp;</span>=
<o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>Polypropylene=
 capacitors can actually self-heal to such an extent that there's little =
left of them. The melting point of polypropylene is not very =
high&nbsp;and they can end up as just a liitle blob of =
plastic.&nbsp;</span><o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>&nbsp;</span>=
<o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>Don't worry =
though, I still use them suitably rated for the frequency in use and =
most of them are 600Vac or more.</span><o:p></o:p></p></div><div><p =
class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>&nbsp;</span>=
<o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>73, Hugh, =
M0DSZ</span><o:p></o:p></p></div><blockquote =
style=3D'border:none;border-left:solid black 1.5pt;padding:0in 0in 0in =
4.0pt;margin-left:3.75pt;margin-top:5.0pt;margin-right:0in;margin-bottom:=
5.0pt'><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'>----- =
Receiving the following content ----- =
</span><o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto;background:#E=
4E4E4'><b><span =
style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'>From:</span><=
/b><span style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'> <a =
href=3D"mailto:dtsifakis@gmail.com">Dimitrios Tsifakis</a> =
</span><o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><b><span =
style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'>Receiver:</sp=
an></b><span =
style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'> <a =
href=3D"mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group</a> =
</span><o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><b><span =
style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'>Time:</span><=
/b><span style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'> =
2019-01-31, 00:25:55</span><o:p></o:p></p></div><div><p =
class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><b><span =
style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'>Subject:</spa=
n></b><span style=3D'font-size:9.0pt;font-family:"Tahoma","sans-serif"'> =
Re: LF: TXing WSPR/MF on an indoor loop, part =
2</span><o:p></o:p></p></div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>&nbsp;</span>=
<o:p></o:p></p></div><div><div><p class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;margin-bottom:12.0pt'><span =
style=3D'font-size:8.0pt;font-family:"Tahoma","sans-serif"'>Hi =
Stefan,<br><br>In my experience these polypropylene capacitors when they =
fail, they<br>just lose some capacitance. I think they call it 'self =
healing', maybe<br>they imply that when they fail there is no short =
circuit?<br><br>I have some really nice silver mica capacitors (ex MW =
broadcast stuff)<br>that would be perfect for this =
task...<br><br>Anyway, I am slowly gearing up for some VLF action over =
here. The<br>other day I did some tests at 16.72 kHz into an ugly loop =
(very<br>roughly 120 metres by 3 metres, single turn) and I was able to =
receive<br>my signals using an unoptimise ferrite antenna at a bit over =
2 km from<br>the TX. I don't think I am in the near field at that =
distance, am I?<br>:-)<br><br>73, Dimitris =
VK2COW<br><br>&gt;</span><o:p></o:p></p></div></div></blockquote></div><p=
 class=3DMsoNormal =
style=3D'margin-bottom:12.0pt'><o:p>&nbsp;</o:p></p></div></body></html>
------=_NextPart_000_0120_01D4BBBA.DC7DCC50--


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From: Alex R7NT <r7nt.73@gmail.com>
Date: Sun, 3 Feb 2019 20:40:26 +0300
Message-ID: <CAL-VeeMOPJxNDccNtgRDCzUOE8+A6PgfGTzCuO_hZVun_ey7jA@mail.gmail.com>
To: rsgb_lf_group@blacksheep.org, eb8arz@hotmail.com,
        Riccardo Zoli <riccardozoli80@gmail.com>, k3rwr@md.metrocast.net,
        no3m@no3m.net
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 Content preview:  Dear LF enthusiasts, AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
    * 1. New database records have been added :* #668 QRB=5863,6 2019-02-01 NO3M
    -> EB8ARX WSPR2 #667 QRB=7038,8 2019-01-27 IW4DXW -> K3RWR EbNaut 
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Subject: LF: AWLF Updated 2019-02-03
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--000000000000e1ff15058100df8d
Content-Type: text/plain; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

Dear LF enthusiasts,
 AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
* 1. New database records have been added :*

#668  QRB=3D5863,6  2019-02-01  NO3M     -> EB8ARX WSPR2

#667  QRB=3D7038,8  2019-01-27  IW4DXW   -> K3RWR  EbNaut



*2. Ratings have been updated :*
*K3RWR   *AWLF 4 Rating 3 =E2=86=91 2
        AWLF 1 RX Rating 48 =E2=86=91 26

*EB8ARZ  *AWLF 2 Rating 17 =E2=86=91 14
        AWLF 2 RX Rating 9 =E2=86=91 7

*IW4DXW  *AWLF 1 Rating 64 =E2=86=91 44
        AWLF 1 TX Rating 30 =E2=86=91 25

*NO3M    *AWLF 1 Rating 67 =E2=86=91 49
        AWLF 1 TX Rating 38 =E2=86=91 28



*3. Some personal pdf files have been updated in "AWLF Data by Calls":*
*EB8ARZ* *AWLF RX*   *IW4DXW** AWLF, **AWLF TX**   K3RWR* *AWLF, **AWLF RX*=
*
  NO3M** AWLF, **AWLF TX*


*4. "Best QSOs" have been updated : *sorted in *QRB/Date* , *Chronological
order* , *Mode(Cat)/Date*
*http://136.73.ru/h_qso <http://136.73.ru/h_qso>*     (maybe refresh frame)

73! Alex R7NT  *http://136.73.ru <http://136.73.ru/>*

--000000000000e1ff15058100df8d
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;li=
ne-height:normal;background-image:initial;background-position:initial;backg=
round-size:initial;background-repeat:initial;background-origin:initial;back=
ground-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif">Dear LF e=
nthusiasts,<br>
=C2=A0AWLF=C2=A0</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-=
family:Arial,sans-serif;color:blue"><a href=3D"http://136.73.ru/h_aw" style=
=3D"color:blue" target=3D"_blank">http://136.73.ru/h_aw</a></span></u><span=
 lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif">=C2=A0=
=C2=A0</span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&qu=
ot;Courier New&quot;"><br>
<u>1. New database records have been added :</u></span></b><u><span lang=3D=
"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif"></span></u></p=
>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#668=C2=A0=C2=A0QRB=
=3D5863,6=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-01=C2=A0 NO3M=
=C2=A0 =C2=A0=C2=A0=C2=A0-&gt; EB8ARX=C2=A0WSPR2</span><span lang=3D"EN-US"=
 style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(23,59=
,211)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#667=C2=A0=C2=A0QRB=
=3D7038,8=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,102,0)">2019-01-27=C2=A0 IW4DX=
W=C2=A0=C2=A0 -&gt; K3RWR
=C2=A0EbNaut</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:rgb(23,59,211)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">2.=C2=A0Ratin=
gs have been
updated :</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"><br>
<b>K3RWR=C2=A0 =C2=A0</b>AWLF 4 Rating 3</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">=
=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;=
Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;;color:black">=C2=A02<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
48</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A026</span><=
b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New=
&quot;;color:black"></span></b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">EB8A=
RZ =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;;color:black">AWLF 2 Rating 17</span><span lang=3D"=
EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb=
(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=
=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">=C2=A014<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 2 RX Rating
9</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Couri=
er New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;background:r=
gb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;=
font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A07</span><b><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;;color:black"></span></b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">IW4D=
XW =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;;color:black">AWLF 1 Rating 64</span><span lang=3D"=
EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb=
(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=
=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">=C2=A044<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;;color:rgb(192,0,0)">=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0 =
AWLF 1
TX Rating 30 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</=
span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier =
New&quot;;color:red">=C2=A025</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">NO3M=
=C2=A0 =C2=A0=C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black">AWLF 1 Rating 67</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211=
)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black">=C2=A049<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;;color:rgb(192,0,0)">=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0 =
AWLF 1
TX Rating 38 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</=
span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier =
New&quot;;color:red">=C2=A028</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">=C2=
=A0</span></b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">3.=C2=
=A0Some personal pdf files have been updated in
&quot;AWLF Data by Calls&quot;:</span></u></b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;"><br>
</span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">EB8ARZ</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =C2=A0=
=C2=A0</span></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;">IW4DXW</span></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:black">=C2=A0AW=
LF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;f=
ont-family:&quot;Courier New&quot;;color:rgb(192,0,0)">AWLF TX</span></i></=
b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier =
New&quot;;color:black">=C2=A0=C2=A0 K3RWR</span></b><b><span lang=3D"EN-US"=
 style=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b=
><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier N=
ew&quot;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" =
style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,=
0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;fo=
nt-family:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0NO3M</span></b>=
<b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier=
 New&quot;;color:black">=C2=A0AWLF,=C2=A0</span></i></b><b><i><span lang=3D=
"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rg=
b(192,0,0)">AWLF TX</span></i></b><b><span lang=3D"EN-US" style=3D"font-siz=
e:9pt;font-family:&quot;Courier New&quot;;color:black">=C2=A0=C2=A0 </span>=
</b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;">4. &quot;Best QSO=
s&quot; have been updated :<br>
</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">sorted in=C2=A0</span><b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">QRB/=
Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" style=3D"f=
ont-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">Chrono=
logical order</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0=
)">Mode(Cat)/Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:black"><br>
</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,san=
s-serif;color:blue"><a href=3D"http://136.73.ru/h_qso" style=3D"color:blue"=
 target=3D"_blank">http://136.73.ru/h_qso</a></span></u><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0=
 =C2=A0(maybe refresh frame)</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:Arial,sans-serif">73! Alex R7NT=C2=A0=C2=A0</spa=
n><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-ser=
if;color:blue"><a href=3D"http://136.73.ru/" style=3D"color:blue" target=3D=
"_blank">http://136.73.ru</a></span></u><span lang=3D"EN-US" style=3D"font-=
size:9pt;font-family:Arial,sans-serif"></span></p></div>

--000000000000e1ff15058100df8d--

From owner-rsgb_lf_group@blacksheep.org  Sun Feb  3 19:11:02 2019
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Date: Sun, 3 Feb 2019 18:06:41 +0000 (GMT)
From: DAVE PICK <daveyxm@virginmedia.com>
To: rsgb_lf_group@blacksheep.org, Jacek Lipkowski <sq5bpf@lipkowski.org>
Message-ID: <1097725691.481056.1549217201654@mail2.virginmedia.com>
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 Content preview:  Jacek I have an archive of the LF reflector from 1999 to early
    2006. It's in a Thunderbird archive folder which is readable by Thunderbird
    if you have it. I don't know how to convert the emails into the for [...]
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  pts rule name              description
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Subject: LF: LF Reflector archive
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------=_Part_481055_1325520213.1549217201652
MIME-Version: 1.0
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Content-Transfer-Encoding: 7bit

Jacek


I have an archive of the LF reflector from 1999 to early 2006. It's in a Thunderbird archive folder which is readable by Thunderbird if you have it. I don't know how to convert the emails into the format you asked for in bulk and I'm certainly not going to do them one by one! If it's any use I'll send you a link to it. It's about 126MB.

I may find some more if I keep looking!

73

Dave G3YXM


------=_Part_481055_1325520213.1549217201652
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<!DOCTYPE html>
<html><head>
    <meta charset="UTF-8">
</head><body><p class="default-style">Jacek<br></p><p class="default-style"><br></p><p class="default-style">I have an archive of the LF reflector from 1999 to early 2006. It&#39;s in a Thunderbird archive folder which is readable by Thunderbird if you have it. I don&#39;t know how to convert the emails into the format you asked for in bulk and I&#39;m certainly not going to do them one by one! If it&#39;s any use I&#39;ll send you a link to it. It&#39;s about 126MB.<br></p><p class="default-style">I may find some more if I keep looking!<br></p><p class="default-style">73<br></p><p class="default-style">Dave G3YXM<br></p><p class="default-style"><br></p></body></html>
 
------=_Part_481055_1325520213.1549217201652--

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 <alpine.DEB.2.11.1902021559010.725@mailn.lipkowski.org> <1097725691.481056.1549217201654@mail2.virginmedia.com>
In-Reply-To: <1097725691.481056.1549217201654@mail2.virginmedia.com>
From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Sun, 3 Feb 2019 18:10:52 +0000
Message-ID: <CAA8k23TVTXchMtTRBsmnOB9fJFj+eKq05N3g7JFYSyW6BL=h1w@mail.gmail.com>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
X-Spam-Score: 0.0 (/)
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 Content preview:  You could place the archive on the groups.io files section
    IGMC ! Andy www.g4jnt.com 
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                             no trust
                             [2607:f8b0:4864:20:0:0:0:e2a listed in]
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Subject: Re: LF: LF Reflector archive
Content-Type: multipart/alternative; boundary="00000000000073578b0581014ed2"
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--00000000000073578b0581014ed2
Content-Type: text/plain; charset="UTF-8"

You could place the archive on the groups.io files section

IGMC !

Andy
www.g4jnt.com



On Sun, 3 Feb 2019 at 18:09, DAVE PICK <daveyxm@virginmedia.com> wrote:

> Jacek
>
>
> I have an archive of the LF reflector from 1999 to early 2006. It's in a
> Thunderbird archive folder which is readable by Thunderbird if you have it.
> I don't know how to convert the emails into the format you asked for in
> bulk and I'm certainly not going to do them one by one! If it's any use
> I'll send you a link to it. It's about 126MB.
>
> I may find some more if I keep looking!
>
> 73
>
> Dave G3YXM
>
>
>

--00000000000073578b0581014ed2
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">You could place the archive on the <a href=3D"ht=
tp://groups.io">groups.io</a> files section=C2=A0</div><div class=3D"gmail_=
default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br></div>=
<div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-si=
ze:small">IGMC !</div><div class=3D"gmail_default" style=3D"font-family:tah=
oma,sans-serif;font-size:small"><br></div><div><div dir=3D"ltr" class=3D"gm=
ail_signature" data-smartmail=3D"gmail_signature"><div dir=3D"ltr"><div><di=
v dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"=
ltr">Andy<div><span style=3D"font-size:12.8px"><a href=3D"http://www.g4jnt.=
com" target=3D"_blank">www.g4jnt.com</a></span><br></div><div><br></div></d=
iv></div></div></div></div></div></div></div></div></div></div><br></div><b=
r><div class=3D"gmail_quote"><div dir=3D"ltr" class=3D"gmail_attr">On Sun, =
3 Feb 2019 at 18:09, DAVE PICK &lt;<a href=3D"mailto:daveyxm@virginmedia.co=
m">daveyxm@virginmedia.com</a>&gt; wrote:<br></div><blockquote class=3D"gma=
il_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,2=
04,204);padding-left:1ex"><u></u>

   =20
<div><p class=3D"gmail-m_-9025933769200115931default-style">Jacek<br></p><p=
 class=3D"gmail-m_-9025933769200115931default-style"><br></p><p class=3D"gm=
ail-m_-9025933769200115931default-style">I have an archive of the LF reflec=
tor from 1999 to early 2006. It&#39;s in a Thunderbird archive folder which=
 is readable by Thunderbird if you have it. I don&#39;t know how to convert=
 the emails into the format you asked for in bulk and I&#39;m certainly not=
 going to do them one by one! If it&#39;s any use I&#39;ll send you a link =
to it. It&#39;s about 126MB.<br></p><p class=3D"gmail-m_-902593376920011593=
1default-style">I may find some more if I keep looking!<br></p><p class=3D"=
gmail-m_-9025933769200115931default-style">73<br></p><p class=3D"gmail-m_-9=
025933769200115931default-style">Dave G3YXM<br></p><p class=3D"gmail-m_-902=
5933769200115931default-style"><br></p></div>
 </blockquote></div>

--00000000000073578b0581014ed2--

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Date: Sun, 3 Feb 2019 18:26:40 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
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References: <1853806007.1845781.1549111581841.ref@mail.yahoo.com> <1853806007.1845781.1549111581841@mail.yahoo.com> <1688162151.2205988.1549206383504@mail.yahoo.com>
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 Content preview:  Here's a short summary of my recent experiments and conclusions.
    LEA-6T hardware: At around 27 €, this LEA-6T module is perhaps one of the
    cheapest solutione with two timing outputs - see http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardow
    [...] 
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Subject: LF: Generating EbNaut from u-blox GPS timepulse
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------=_Part_2252902_26065457.1549218400560
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Here's a short summary of my recent experiments and conclusions.

LEA-6T hardware:
At around 27 =E2=82=AC, this LEA-6T module is perhaps one of the cheapest s=
olutione with two timing outputs - see
http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardow=
n-and-initial-test/Although the LEA series has been superseded by NEO-7 and=
 -8 with GLONASS and Galileo capabilities, but these tend to be much more e=
xpensive.

My unit arrived within about a week, and started up fine through the includ=
ed USB adapter board. Unfortunately my device did not remember settings aft=
er powerdown, which turned out to be due to a missing flash eeprom chip, an=
d also (believe it or not) a faulty solder joint on backup-battery charging=
 resistor. In fact all the solder joints looked as if they had been hand so=
ldered in a Chinese garage factory but that's fine with me.
=C2=A0
Then I connected the timepulse outputs through 470 ohm protection resistors=
 and separate coax cables. With 3.3 Vpp behind the resistor we get ~ 1 mW a=
vailable power. However connecting the little ublox module barefoot to the =
antenna produced good carrier traces and successful EbNaut decodes at the D=
L0AO MF-Grabber, 48 km from here. For PA switching, I later employed a simp=
le VOX circuit fed by TP2 output signal.
The frequency can be set at any integer Hz from 1 to 24 MHz. The stepsize i=
s fine for LF and MF but perhaps inconvenient at VLF where we would rather =
avoitd integer Hz frequencies. But it may be possible to create small and p=
recise sub-Hz offsets by regularly advancing phase, using the user-delay fi=
eld. Note that at higher HF frequencies, a noticable degradation of GPS sen=
sitivity occured presumably due to interference to the on-board ceramic ant=
enna.
EbNaut generation:
The idea for ebnaut is to generate PSK by using ublox commands to change po=
larity of timepulse, minimizing hardware and doing away with audio mixers o=
r external phase switches. I started by monitoring the 40-byte TP5 commands=
 in in the binary message display. Then based on the specificaton on the u-=
blox website,
https://www.u-blox.com/sites/default/files/products/documents/u-blox6_Recei=
verDescrProtSpec_%28GPS.G6-SW-10018%29_Public.pdf
(chapters 23 and 31.24.3), I wrote a small Basic executable setubx.exe whic=
h reads a template and=C2=A0patches the frequency, flag and checksum fields=
. The output can be redirected to the virtual com-port of the USB device (e=
.g. >com6).
Note that any changes are not executed immediately but only at the start th=
e next second. If a command has been issued as early as 1 to 0.1 s before, =
the output inversion happens about 50 ms after the tick (implying a negligi=
ble 0.05 s extra symbol delay). The advantage is that no subsecond timing i=
s required for the issuing of commands, enabling the use of simple DOS time=
out or sleep functions. On the other hand, the maximum signalling speed is =
thus limited to 1 second per symbol.
As mentioned before, I have created a directory for Windows scripts and a f=
ew screenshots, and also this email:
http://df6nm.bplaced.net/LF/u-blox_ebnaut/
To prepare an EbNaut transmission, you'd go through the following steps:
- download and unpack ebnaut_ublox.zip=20
- use Paul's ebnaut-tx.exe and "write lines" to produce a pskln_xxx.txt out=
put file,
- edit the file with notepad to replace "1" by "call 1" (same for 0) and sa=
ve as a .bat file,
- right-click and edit frequency and delay functions in 1.bat and 0.bat=C2=
=A0=C2=A0=20
- edit the send_ebnaut...bat according to your desired transmit schedule.
BTW I did struggle with strange peculiarities in batch scripting... We need=
 to wait until the second before the next of 3-second-multiple, but why thi=
s cryptic notation:
@set /a waittime=3D2-(3%time:~6,2%%%3)
- set /a is for arithmetic calculations for a variable,
- %time:~6,2% provides two digits for the seconds in a minute,
- %% is an expansion of the % modulo operator which is required in a batch =
script,=C2=A0=C2=A0=20
- 3%time:~6,2% expands xx to 3xx, only to avoid 08 being interpreted as an =
invalid octal number.=20
Spectral purity:
Originally I had hoped for relatively low jitter, as little as 21 ns from t=
he 48 MHz clock. But it turned out that on most output frequencies the jitt=
er is really much larger, leading to relatively strong 1 kHz spaced spuriou=
s sidelines. It looks as if frequencies were internally generated on a rela=
tively coarse raster, and then the phase is being pulled in periodically ea=
ch millisecond. But some preferred frequencies are much cleaner than others=
, specifically
=C2=A0- integer divisors of 48 MHz (well-known and easy to understand),=20
=C2=A0- but also all multiples of 366.2155 Hz. This raster happens to be 48=
000.34 kHz/2^17, so I speculate that this may be a "DDS"-like architecture,=
 clocked by my particular 48 MHz crystal, and outputting the msb of an over=
flowing 17-bit-counter.
When the output frequency is set slightly above one of these sweet spots, t=
he level of 1 kHz sidelines gradually increases. But going only 1 Hz below =
the spot produces a sharp detoriation to the worst levels. For example:
=C2=A0137330 Hz -15 dB, 137331 Hz -54 dB,
=C2=A0137536 Hz =3D 48 MHz/349: -54 dB,
=C2=A0475710 Hz -5 dB(!), 475712 Hz -47 dB.

When sweeping through frequencies, a "sawtooth-like" dependence of spurious=
 levels can be observed (screenshot lea-6t_sweep_474-480.5kHz.png).=20
Hope this may be useful=E2=80=A6
Best 73,
Markus (DF6NM)



------=_Part_2252902_26065457.1549218400560
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;">Here's a short summary of my recent experiments and conc=
lusions.<br clear=3D"none"><br clear=3D"none">LEA-6T hardware:<br clear=3D"=
none"></div><div id=3D"yiv4854928327"><div><div style=3D"color: black; font=
-family: arial, helvetica, sans-serif; font-size: 10pt;"><div style=3D"colo=
r: black; font-family: arial, helvetica, sans-serif; font-size: 10pt;">At a=
round 27 =E2=82=AC, this LEA-6T module is perhaps one of the cheapest solut=
ione with two timing outputs - see<br clear=3D"none">http://www.eevblog.com=
/forum/projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/</d=
iv><div style=3D"color: black; font-family: arial, helvetica, sans-serif; f=
ont-size: 10pt;">Although the LEA series has been superseded by NEO-7 and -=
8 with GLONASS and Galileo capabilities, but these tend to be much more exp=
ensive.<br clear=3D"none"><br clear=3D"none">My unit arrived within about a=
 week, and started up fine through the included USB adapter board. Unfortun=
ately my device did not remember settings after powerdown, which turned out=
 to be due to a missing flash eeprom chip, and also (believe it or not) a f=
aulty solder joint on backup-battery charging resistor. In fact all the sol=
der joints looked as if they had been hand soldered in a Chinese garage fac=
tory but that's fine with me.<br clear=3D"none">&nbsp;<br clear=3D"none">Th=
en I connected the timepulse outputs through 470 ohm protection resistors a=
nd separate coax cables. With 3.3 Vpp behind the resistor we get ~ 1 mW ava=
ilable power. However connecting the little ublox module barefoot to the an=
tenna produced good carrier traces and successful EbNaut decodes at the DL0=
AO MF-Grabber, 48 km from here. For PA switching, I later employed a simple=
 VOX circuit fed by TP2 output signal.</div><div style=3D"color: black; fon=
t-family: arial, helvetica, sans-serif; font-size: 10pt;"><br clear=3D"none=
">The frequency can be set at any integer Hz from 1 to 24 MHz. The stepsize=
 is fine for LF and MF but perhaps inconvenient at VLF where we would rathe=
r avoitd integer Hz frequencies. But it may be possible to create small and=
 precise sub-Hz offsets by regularly advancing phase, using the user-delay =
field. Note that at higher HF frequencies, a noticable degradation of GPS s=
ensitivity occured presumably due to interference to the on-board ceramic a=
ntenna.</div><div style=3D"color: black; font-family: arial, helvetica, san=
s-serif; font-size: 10pt;"><br clear=3D"none">EbNaut generation:</div><div =
style=3D"color: black; font-family: arial, helvetica, sans-serif; font-size=
: 10pt;"><br clear=3D"none">The idea for ebnaut is to generate PSK by using=
 ublox commands to change polarity of timepulse, minimizing hardware and do=
ing away with audio mixers or external phase switches. I started by monitor=
ing the 40-byte TP5 commands in in the binary message display. Then based o=
n the specificaton on the u-blox website,<br clear=3D"none">https://www.u-b=
lox.com/sites/default/files/products/documents/u-blox6_ReceiverDescrProtSpe=
c_%28GPS.G6-SW-10018%29_Public.pdf<br clear=3D"none">(chapters 23 and 31.24=
.3), I wrote a small Basic executable setubx.exe which reads a template and=
&nbsp;patches the frequency, flag and checksum fields. The output can be re=
directed to the virtual com-port of the USB device (e.g. &gt;com6).</div><d=
iv style=3D"color: black; font-family: arial, helvetica, sans-serif; font-s=
ize: 10pt;"><br clear=3D"none">Note that any changes are not executed immed=
iately but only at the start the next second. If a command has been issued =
as early as 1 to 0.1 s before, the output inversion happens about 50 ms aft=
er the tick (implying a negligible 0.05 s extra symbol delay). The advantag=
e is that no subsecond timing is required for the issuing of commands, enab=
ling the use of simple DOS timeout or sleep functions. On the other hand, t=
he maximum signalling speed is thus limited to 1 second per symbol.</div><d=
iv style=3D"color: black; font-family: arial, helvetica, sans-serif; font-s=
ize: 10pt;"><br clear=3D"none">As mentioned before, I have created a direct=
ory for Windows scripts and a few screenshots, and also this email:<br clea=
r=3D"none">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</div><div style=3D"co=
lor: black; font-family: arial, helvetica, sans-serif; font-size: 10pt;"><b=
r clear=3D"none">To prepare an EbNaut transmission, you'd go through the fo=
llowing steps:<br clear=3D"none">- download and unpack ebnaut_ublox.zip <br=
 clear=3D"none">- use Paul's ebnaut-tx.exe and "write lines" to produce a p=
skln_xxx.txt output file,<br clear=3D"none">- edit the file with notepad to=
 replace "1" by "call 1" (same for 0) and save as a .bat file,<br clear=3D"=
none">- right-click and edit frequency and delay functions in 1.bat and 0.b=
at&nbsp;&nbsp; <br clear=3D"none">- edit the send_ebnaut...bat according to=
 your desired transmit schedule.</div><div style=3D"color: black; font-fami=
ly: arial, helvetica, sans-serif; font-size: 10pt;"><br clear=3D"none">BTW =
I did struggle with strange peculiarities in batch scripting... We need to =
wait until the second before the next of 3-second-multiple, but why this cr=
yptic notation:<br clear=3D"none">@set /a waittime=3D2-(3%time:~6,2%%%3)<br=
 clear=3D"none">- set /a is for arithmetic calculations for a variable,<br =
clear=3D"none">- %time:~6,2% provides two digits for the seconds in a minut=
e,<br clear=3D"none">- %% is an expansion of the % modulo operator which is=
 required in a batch script,&nbsp;&nbsp; <br clear=3D"none">- 3%time:~6,2% =
expands xx to 3xx, only to avoid 08 being interpreted as an invalid octal n=
umber. </div><div style=3D"color: black; font-family: arial, helvetica, san=
s-serif; font-size: 10pt;"><br clear=3D"none">Spectral purity:</div><div st=
yle=3D"color: black; font-family: arial, helvetica, sans-serif; font-size: =
10pt;"><br clear=3D"none">Originally I had hoped for relatively low jitter,=
 as little as 21 ns from the 48 MHz clock. But it turned out that on most o=
utput frequencies the jitter is really much larger, leading to relatively s=
trong 1 kHz spaced spurious sidelines. It looks as if frequencies were inte=
rnally generated on a relatively coarse raster, and then the phase is being=
 pulled in periodically each millisecond. But some preferred frequencies ar=
e much cleaner than others, specifically<br clear=3D"none">&nbsp;- integer =
divisors of 48 MHz (well-known and easy to understand), <br clear=3D"none">=
&nbsp;- but also all multiples of 366.2155 Hz. This raster happens to be 48=
000.34 kHz/2^17, so I speculate that this may be a "DDS"-like architecture,=
 clocked by my particular 48 MHz crystal, and outputting the msb of an over=
flowing 17-bit-counter.</div><div style=3D"color: black; font-family: arial=
, helvetica, sans-serif; font-size: 10pt;"><br clear=3D"none">When the outp=
ut frequency is set slightly above one of these sweet spots, the level of 1=
 kHz sidelines gradually increases. But going only 1 Hz below the spot prod=
uces a sharp detoriation to the worst levels. For example:<br clear=3D"none=
">&nbsp;137330 Hz -15 dB, 137331 Hz -54 dB,<br clear=3D"none">&nbsp;137536 =
Hz =3D 48 MHz/349: -54 dB,<br clear=3D"none">&nbsp;475710 Hz -5 dB(!), 4757=
12 Hz -47 dB.<br clear=3D"none"><br clear=3D"none">When sweeping through fr=
equencies, a "sawtooth-like" dependence of spurious levels can be observed =
(screenshot lea-6t_sweep_474-480.5kHz.png). </div><div style=3D"color: blac=
k; font-family: arial, helvetica, sans-serif; font-size: 10pt;"><br clear=
=3D"none">Hope this may be useful=E2=80=A6</div><div class=3D"yiv4854928327=
yqt6450327648" id=3D"yiv4854928327yqtfd82931"><div style=3D"color: black; f=
ont-family: arial, helvetica, sans-serif; font-size: 10pt;"><br clear=3D"no=
ne">Best 73,<br clear=3D"none">Markus (DF6NM)<br clear=3D"none"><br clear=
=3D"none"><br clear=3D"none"></div></div></div></div></div></div>
------=_Part_2252902_26065457.1549218400560--

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Date: Sun, 3 Feb 2019 18:48:53 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
Message-ID: <1612939286.2266215.1549219733177@mail.yahoo.com>
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 Content preview:  Hi Stefan, WSPR - no, timing and frequency spacing won't
    fit what u-blox can do. Well, unless we defined a new "WSPR-3" submode,
   using exactly 1 second symbols and 1 Hz tone spacing. Thinking again, maybe it's
    not such a bad idea in some respects… 
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Subject: Re: LF: EbNaut test from u-blox module - and what about WSPR?
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------=_Part_2266214_1114858869.1549219733175
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Hi Stefan,

WSPR=C2=A0- no,=C2=A0timing and frequency spacing won't fit what=C2=A0u-blo=
x can do.=20

Well, unless we defined a new "WSPR-3" submode, using exactly 1 second symb=
ols and 1 Hz tone spacing. Thinking again, maybe=C2=A0it's not such a bad i=
dea in some respects=E2=80=A6=20

Best 73,
Markus



=C2=A0

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: So, 3. Feb. 2019 14:42
Betreff: Re: LF: EbNaut test from u-blox module - and what about WSPR?

Hi Markus,=20

Snow-rain here, not the most inviting climate for outdoor experiments,altho=
ugh i would like to climb the tree to repair my VLF E-field :-)

I just thought about your latest tool and wonder if it is possible todo the=
 same for WSPR-2 or WSPR-15, all without a transceiver orupconverter or the=
 whole dial stuff ;-) It would be comfortable andpower saving. So much can =
be done...

73, Stefan

Am 03.02.2019 01:15, schrieb Markus Vester:
     Thanks Stefan and Michel (F5WK) for your excellent reports!=20
=20
The=C2=A0residual phase variation was surely from the antenna moving in the=
wind. I haven't been using the=C2=A0automatic tuner, and also did somemanua=
l tweaking=C2=A0near the beginning.=C2=A0Interestingly Michel's phase trace=
was a perfect copy of yours.
=20
The exciter and 250 W PA are the same as=C2=A0in my usual LF setup, exceptt=
hat the feed from the SSB=C2=A0exciter has been replaced by the TP2 outputf=
rom the GPS device,=C2=A0connected=C2=A0through 470 ohm and a piece of coax=
.The=C2=A0LEA-6T module came=C2=A0from Hongkong for=C2=A027 =E2=82=AC and i=
s very similar tothe one described here
http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardow=
n-and-initial-test/
=20
I=C2=A0am now repeating the same=C2=A0pair of transmissions=C2=A0at 0:00and=
 0:30 UT, but moved to=C2=A0137545 Hzto fit inside=C2=A0Jay's narrowband re=
cording.=20
=20
Best 73,
Markus=C2=A0=C2=A0(DF6NM)
=20
=C2=A0=C2=A0
=20
-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Sa, 2. Feb. 2019 14:52
Betreff: Re: LF: EbNaut test from u-blox module
=20
    Hi Markus,=20
=20
Great work! It seems to work well. There are some dynamic changes inthe pha=
se. Would you think it is propagation?
So this is a Windows solution without the need to use an upconverter.Let's =
see if this will help to make the mode more popular, or not.
How did you connect the module to the PA, which kind of exciter? Iwould kno=
w how to do it, just beeing curious...
=20
73, Stefan
=20
=20
Am 02.02.2019 13:46, schrieb Markus Vester: =20
  Think I have=C2=A0tamed my u-blox LEA-6T module well enough, sowill try t=
o=C2=A0send an EbNaut test this afternoon:
=20
Frequency 137536 Hz,
Start times: 13:00 and 13:30 UT,
 6 char, 3 sec symbols, =C2=A08k19A, crc 16.
=20
Experimental scripts to control the timepulse-2 output are at=20
 http://df6nm.bplaced.net/LF/u-blox_ebnaut/=C2=A0
and I intend to=C2=A0explain some details later this weekend.
=20
Best 73,
Markus (DF6NM)
=20
-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Do, 31. Jan. 2019 22:32
Betreff: Re: LF: NEO-7M as a frequency source
=20
...
...would like to try to transmit EbNaut on 137 kHz directly from such a=20
module.
=20
73, Stefan
=20
=20
  =20
    =20
   =20

------=_Part_2266214_1114858869.1549219733175
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;">Hi Stefan,<br><br>WSPR&nbsp;- no,&nbsp;timing and freque=
ncy spacing won't fit what&nbsp;u-blox can do. <br><br>Well, unless we defi=
ned a new "WSPR-3" submode, using exactly 1 second symbols and 1 Hz tone sp=
acing. Thinking again, maybe&nbsp;it's not such a bad idea in some respects=
=E2=80=A6 <br><br>Best 73,<br>Markus<br><br><br><br>&nbsp;<br><br>-----Ursp=
r=C3=BCngliche Mitteilung-----<br>Von: DK7FC &lt;selberdenken@posteo.de&gt;=
<br>An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br>Verschickt: S=
o, 3. Feb. 2019 14:42<br>Betreff: Re: LF: EbNaut test from u-blox module - =
and what about WSPR?<br><br></div><div id=3D"yiv1940968262"><div>
Hi Markus, <br clear=3D"none">
<br clear=3D"none">
Snow-rain here, not the most inviting climate for outdoor experiments,
although i would like to climb the tree to repair my VLF E-field :-)<br cle=
ar=3D"none">
<br clear=3D"none">
I just thought about your latest tool and wonder if it is possible to
do the same for WSPR-2 or WSPR-15, all without a transceiver or
upconverter or the whole dial stuff ;-) It would be comfortable and
power saving. So much can be done...<br clear=3D"none">
<br clear=3D"none">
73, Stefan<br clear=3D"none">
<br clear=3D"none">
Am 03.02.2019 01:15, schrieb Markus Vester:
<div class=3D"yiv1940968262yqt9084460399" id=3D"yiv1940968262yqt36684"><blo=
ckquote type=3D"cite">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;">
  <div id=3D"yiv1940968262">
  <div>
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;">Thanks Stefan and Michel (F5WK) for your excellent reports!
  <br clear=3D"none">
  <br clear=3D"none">
The&nbsp;residual phase variation was surely from the antenna moving in the
wind. I haven't been using the&nbsp;automatic tuner, and also did some
manual tweaking&nbsp;near the beginning.&nbsp;Interestingly Michel's phase =
trace
was a perfect copy of yours.<br clear=3D"none">
  <br clear=3D"none">
The exciter and 250 W PA are the same as&nbsp;in my usual LF setup, except
that the feed from the SSB&nbsp;exciter has been replaced by the TP2 output
from the GPS device,&nbsp;connected&nbsp;through 470 ohm and a piece of coa=
x.
The&nbsp;LEA-6T module came&nbsp;from Hongkong for&nbsp;27 =E2=82=AC and is=
 very similar to
the one described here<br clear=3D"none">
<a class=3D"yiv1940968262moz-txt-link-freetext" href=3D"http://www.eevblog.=
com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/=
" target=3D"_blank" rel=3D"noopener noreferrer" shape=3D"rect">http://www.e=
evblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardown-and-initia=
l-test/</a><br clear=3D"none">
  <br clear=3D"none">
I&nbsp;am now repeating the same&nbsp;pair of transmissions&nbsp;at<strong>=
 0:00</strong>
and<strong> 0:30 UT</strong>, but moved to&nbsp;<strong>137545 Hz</strong>
to fit inside&nbsp;Jay's narrowband recording. <br clear=3D"none">
  <br clear=3D"none">
Best 73,<br clear=3D"none">
Markus&nbsp;&nbsp;(DF6NM)<br clear=3D"none">
  <br clear=3D"none">
&nbsp;&nbsp;<br clear=3D"none">
  <br clear=3D"none">
-----Urspr=C3=BCngliche Mitteilung-----<br clear=3D"none">
Von: DK7FC <a class=3D"yiv1940968262moz-txt-link-rfc2396E" href=3D"mailto:s=
elberdenken@posteo.de" target=3D"_blank" rel=3D"noopener noreferrer" shape=
=3D"rect" ymailto=3D"mailto:selberdenken@posteo.de">&lt;selberdenken@posteo=
.de&gt;</a><br clear=3D"none">
An: rsgb_lf_group <a class=3D"yiv1940968262moz-txt-link-rfc2396E" href=3D"m=
ailto:rsgb_lf_group@blacksheep.org" target=3D"_blank" rel=3D"noopener noref=
errer" shape=3D"rect" ymailto=3D"mailto:rsgb_lf_group@blacksheep.org">&lt;r=
sgb_lf_group@blacksheep.org&gt;</a><br clear=3D"none">
Verschickt: Sa, 2. Feb. 2019 14:52<br clear=3D"none">
Betreff: Re: LF: EbNaut test from u-blox module<br clear=3D"none">
  <br clear=3D"none">
  </div>
  <div class=3D"yiv1940968262yqt2807499086" id=3D"yiv1940968262yqt91517">
  <div id=3D"yiv1940968262">
  <div>Hi Markus, <br clear=3D"none">
  <br clear=3D"none">
Great work! It seems to work well. There are some dynamic changes in
the phase. Would you think it is propagation?<br clear=3D"none">
So this is a Windows solution without the need to use an upconverter.
Let's see if this will help to make the mode more popular, or not.<br clear=
=3D"none">
How did you connect the module to the PA, which kind of exciter? I
would know how to do it, just beeing curious...<br clear=3D"none">
  <br clear=3D"none">
73, Stefan<br clear=3D"none">
  <br clear=3D"none">
  <br clear=3D"none">
Am 02.02.2019 13:46, schrieb Markus Vester:
  <div class=3D"yiv1940968262yqt0945518385" id=3D"yiv1940968262yqt44022">
  <blockquote type=3D"cite">
    <div style=3D"color: black; font-family: arial, helvetica, sans-serif; =
font-size: 10pt;">
    <div style=3D"color: black; font-family: arial, helvetica, sans-serif; =
font-size: 10pt;">Think I have&nbsp;tamed my u-blox LEA-6T module well enou=
gh, so
will try to&nbsp;send an EbNaut test this afternoon:<br clear=3D"none">
    <br clear=3D"none">
Frequency 137536 Hz,<br clear=3D"none">
Start times: 13:00 and 13:30 UT,<br clear=3D"none">
    <strong>6 char, 3 sec symbols, &nbsp;8k19A, crc 16.</strong><br clear=
=3D"none">
    <br clear=3D"none">
Experimental scripts to control the timepulse-2 output are at <br clear=3D"=
none">
    <a class=3D"yiv1940968262moz-txt-link-freetext" href=3D"http://df6nm.bp=
laced.net/LF/u-blox_ebnaut/" target=3D"_blank" rel=3D"noopener noreferrer" =
shape=3D"rect">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</a>&nbsp;<br clea=
r=3D"none">
and I intend to&nbsp;explain some details later this weekend.<br clear=3D"n=
one">
    <br clear=3D"none">
Best 73,<br clear=3D"none">
Markus (DF6NM)<br clear=3D"none">
    <br clear=3D"none">
-----Urspr=C3=BCngliche Mitteilung-----<br clear=3D"none">
Von: DK7FC <a class=3D"yiv1940968262moz-txt-link-rfc2396E" href=3D"mailto:s=
elberdenken@posteo.de" target=3D"_blank" rel=3D"noopener noreferrer" shape=
=3D"rect" ymailto=3D"mailto:selberdenken@posteo.de">&lt;selberdenken@posteo=
.de&gt;</a><br clear=3D"none">
An: rsgb_lf_group <a class=3D"yiv1940968262moz-txt-link-rfc2396E" href=3D"m=
ailto:rsgb_lf_group@blacksheep.org" target=3D"_blank" rel=3D"noopener noref=
errer" shape=3D"rect" ymailto=3D"mailto:rsgb_lf_group@blacksheep.org">&lt;r=
sgb_lf_group@blacksheep.org&gt;</a><br clear=3D"none">
Verschickt: Do, 31. Jan. 2019 22:32<br clear=3D"none">
Betreff: Re: LF: NEO-7M as a frequency source<br clear=3D"none">
    <br clear=3D"none">
...<br clear=3D"none">
...would like to try to transmit EbNaut on 137 kHz directly from such a
    <br clear=3D"none">
module.<br clear=3D"none">
    <br clear=3D"none">
73, Stefan<br clear=3D"none">
    <br clear=3D"none">
    <br clear=3D"none">
    </div>
    </div>
  </blockquote>
  </div>
  </div>
  </div>
  </div>
  <br clear=3D"none">
  </div>
  </div>
  </div>
  </div>
</blockquote></div>
</div></div></div>
------=_Part_2266214_1114858869.1549219733175--

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Date: Sun, 3 Feb 2019 22:44:44 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
Message-ID: <515975858.2340956.1549233884518@mail.yahoo.com>
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 Content preview:  A little snapshot from the DL0AO LF/MF-grabber... 73, Markus
    -----Ursprüngliche Mitteilung----- Von: DK7FC An: rsgb_lf_group Verschickt:
    So, 3. Feb. 2019 15:00 Betreff: Re: LF: TXing WSPR/MF on an indoor loop,
   part 2 
 Content analysis details:   (0.0 points, 5.0 required)
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Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2
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Content-Transfer-Encoding: quoted-printable

A little snapshot from the DL0AO LF/MF-grabber...

73, Markus


-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: So, 3. Feb. 2019 15:00
Betreff: Re: LF: TXing WSPR/MF on an indoor loop, part 2

...indeed! Since more than 72 hours i'm running the WSPR transmissionin 25%=
 duty cycle (each 8 minutes). First i tuned to 20 A antennacurrent and the =
temperature / antenna current changes were muchsmaller. But there was a cer=
tain click, or krrrrkkrt audible from theCs. It was likely that there were =
indeed internal voltagebreakthroughs, which were self-healing. Now after 3 =
days the currentdropped again to 14 A, meaning that the capacity dropped, s=
o the loopbecame detuned and so the RF current and voltages dropped to a le=
velwhich is accepted by the capacitors.

So my conclusion is, the derating curves actually should be considered.

I wonder if the effect is still happening if one keeps the temperaturesdown=
 at 25 C or even lower. When placing the capacitors in de-ionisediced water=
, it should be possible to keep the temperatures down, alsoin the internal =
of the capacitor.

But all in all this is not a good solution. Fortunately i have anotheranten=
na which is more efficient :-)

73, Stefan
...=20
------=_Part_2340954_1929269339.1549233884517
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"151">A little snapshot from the DL0AO LF/MF-grabb=
er...<br><br>73, Markus<br abp=3D"152"><br abp=3D"153"><br abp=3D"154">----=
-Urspr=C3=BCngliche Mitteilung-----<br abp=3D"155">Von: DK7FC &lt;selberden=
ken@posteo.de&gt;<br abp=3D"156">An: rsgb_lf_group &lt;rsgb_lf_group@blacks=
heep.org&gt;<br abp=3D"157">Verschickt: So, 3. Feb. 2019 15:00<br abp=3D"15=
8">Betreff: Re: LF: TXing WSPR/MF on an indoor loop, part 2<br abp=3D"159">=
<br abp=3D"160"></div><div id=3D"yiv6719322957" abp=3D"161"><div abp=3D"162=
">
...indeed! Since more than 72 hours i'm running the WSPR transmission
in 25% duty cycle (each 8 minutes). First i tuned to 20 A antenna
current and the temperature / antenna current changes were much
smaller. But there was a certain click, or krrrrkkrt audible from the
Cs. It was likely that there were indeed internal voltage
breakthroughs, which were self-healing. Now after 3 days the current
dropped again to 14 A, meaning that the capacity dropped, so the loop
became detuned and so the RF current and voltages dropped to a level
which is accepted by the capacitors.<br clear=3D"none" abp=3D"163">
<br clear=3D"none" abp=3D"164">
So my conclusion is, the derating curves actually should be considered.<br =
clear=3D"none" abp=3D"165">
<br clear=3D"none" abp=3D"166">
I wonder if the effect is still happening if one keeps the temperatures
down at 25 C or even lower. When placing the capacitors in de-ionised
iced water, it should be possible to keep the temperatures down, also
in the internal of the capacitor.<br clear=3D"none" abp=3D"167">
<br clear=3D"none" abp=3D"168">
But all in all this is not a good solution. Fortunately i have another
antenna which is more efficient :-)<br clear=3D"none" abp=3D"169">
<br clear=3D"none" abp=3D"170">
73, Stefan<br clear=3D"none" abp=3D"171">
...</div>
   =20
 =20

</div></div>
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 Content preview:  Hi Markus, What a surprise, many thanks :-) This was just
   a short test. I just transmitted my call 4 times without an announcement and
    you picked it up. Very attentive :-) I never thought that someone will pick
    [...] 
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Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2
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Hi Markus,

What a surprise, many thanks :-) This was just a short test. I just 
transmitted my call 4 times without an announcement and you picked it 
up. Very attentive :-) I never thought that someone will pick it up :-)
That QRSS was generated by the Raspi using a tool written by VK2COW.

I had a look at http://www.472khz.org/pages/on-the-air/grabbers.php and 
searched for grabberson-line grabbers (excluding my own). DL0AO is not 
yet listed on that page. Just a few MF grabbers that are actually running...

73, Stefan



Am 03.02.2019 23:44, schrieb Markus Vester:
> A little snapshot from the DL0AO LF/MF-grabber...
>
> 73, Markus
>
>
> -----Ursprüngliche Mitteilung-----
> Von: DK7FC <selberdenken@posteo.de>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: So, 3. Feb. 2019 15:00
> Betreff: Re: LF: TXing WSPR/MF on an indoor loop, part 2
>
> ...indeed! Since more than 72 hours i'm running the WSPR transmission 
> in 25% duty cycle (each 8 minutes). First i tuned to 20 A antenna 
> current and the temperature / antenna current changes were much 
> smaller. But there was a certain click, or krrrrkkrt audible from the 
> Cs. It was likely that there were indeed internal voltage 
> breakthroughs, which were self-healing. Now after 3 days the current 
> dropped again to 14 A, meaning that the capacity dropped, so the loop 
> became detuned and so the RF current and voltages dropped to a level 
> which is accepted by the capacitors.
>
> So my conclusion is, the derating curves actually should be considered.
>
> I wonder if the effect is still happening if one keeps the 
> temperatures down at 25 C or even lower. When placing the capacitors 
> in de-ionised iced water, it should be possible to keep the 
> temperatures down, also in the internal of the capacitor.
>
> But all in all this is not a good solution. Fortunately i have another 
> antenna which is more efficient :-)
>
> 73, Stefan
> ...

--------------020602070708070601010005
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<body bgcolor="#ffffff" text="#000000">
Hi Markus, <br>
<br>
What a surprise, many thanks :-) This was just a short test. I just
transmitted my call 4 times without an announcement and you picked it
up. Very attentive :-) I never thought that someone will pick it up :-)<br>
That QRSS was generated by the Raspi using a tool written by VK2COW.<br>
<br>
I had a look at <a class="moz-txt-link-freetext" href="http://www.472khz.org/pages/on-the-air/grabbers.php">http://www.472khz.org/pages/on-the-air/grabbers.php</a> and
searched for grabberson-line grabbers (excluding my own). DL0AO is not
yet listed on that page. Just a few MF grabbers that are actually
running...<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 03.02.2019 23:44, schrieb Markus Vester:
<blockquote cite="mid:515975858.2340956.1549233884518@mail.yahoo.com"
 type="cite">
  <div
 style="font-size: 10pt; font-family: arial,helvetica,sans-serif; color: black;">
  <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;"
 abp="151">A little snapshot from the DL0AO LF/MF-grabber...<br>
  <br>
73, Markus<br abp="152">
  <br abp="153">
  <br abp="154">
-----Ursprüngliche Mitteilung-----<br abp="155">
Von: DK7FC <a class="moz-txt-link-rfc2396E" href="mailto:selberdenken@posteo.de">&lt;selberdenken@posteo.de&gt;</a><br abp="156">
An: rsgb_lf_group <a class="moz-txt-link-rfc2396E" href="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br abp="157">
Verschickt: So, 3. Feb. 2019 15:00<br abp="158">
Betreff: Re: LF: TXing WSPR/MF on an indoor loop, part 2<br abp="159">
  <br abp="160">
  </div>
  <div id="yiv6719322957" abp="161">
  <div abp="162">...indeed! Since more than 72 hours i'm running the
WSPR transmission
in 25% duty cycle (each 8 minutes). First i tuned to 20 A antenna
current and the temperature / antenna current changes were much
smaller. But there was a certain click, or krrrrkkrt audible from the
Cs. It was likely that there were indeed internal voltage
breakthroughs, which were self-healing. Now after 3 days the current
dropped again to 14 A, meaning that the capacity dropped, so the loop
became detuned and so the RF current and voltages dropped to a level
which is accepted by the capacitors.<br abp="163" clear="none">
  <br abp="164" clear="none">
So my conclusion is, the derating curves actually should be considered.<br
 abp="165" clear="none">
  <br abp="166" clear="none">
I wonder if the effect is still happening if one keeps the temperatures
down at 25 C or even lower. When placing the capacitors in de-ionised
iced water, it should be possible to keep the temperatures down, also
in the internal of the capacitor.<br abp="167" clear="none">
  <br abp="168" clear="none">
But all in all this is not a good solution. Fortunately i have another
antenna which is more efficient :-)<br abp="169" clear="none">
  <br abp="170" clear="none">
73, Stefan<br abp="171" clear="none">
...</div>
  </div>
  </div>
</blockquote>
</body>
</html>

--------------020602070708070601010005--

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Mon, 4 Feb 2019 16:54:35 +1100
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 Content preview:  Hi all, I have a few mica capacitors that came from a MW broadcaster,
    similar to this one (in fact I have one that it bigger than this one). Stefan,
    I think this is probably your best bet and pity you are not closer otherwise
    I would be happy to lend you a couple to do your experiments :-) 
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Subject: Re: Re: LF: TXing WSPR/MF on an indoor loop, part 2
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Hi all,

I have a few mica capacitors that came from a MW broadcaster, similar
to this one (in fact I have one that it bigger than this one).

Stefan, I think this is probably your best bet and pity you are not
closer otherwise I would be happy to lend you a couple to do your
experiments :-)

https://rustys.net.au/products/large-ducon-transmitter-honey-pot-capacitor

(this is smaller than the ones I have, most are about 1 nF capacitance)

73, Dimitris VK2COW

Στις Πέμ, 31 Ιαν 2019 στις 10:01 μ.μ., ο/η dhchurch
<dhchurch@lineone.net> έγραψε:
>
> Hello Dimitrios
>
> Polypropylene capacitors can actually self-heal to such an extent that there's little left of them. The melting point of polypropylene is not very high and they can end up as just a liitle blob of plastic.
>
> Don't worry though, I still use them suitably rated for the frequency in use and most of them are 600Vac or more.
>
> 73, Hugh, M0DSZ
>
> ----- Receiving the following content -----
> From: Dimitrios Tsifakis
> Receiver: rsgb_lf_group
> Time: 2019-01-31, 00:25:55
> Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2
>
> Hi Stefan,
>
> In my experience these polypropylene capacitors when they fail, they
> just lose some capacitance. I think they call it 'self healing', maybe
> they imply that when they fail there is no short circuit?
>
> I have some really nice silver mica capacitors (ex MW broadcast stuff)
> that would be perfect for this task...
>
> Anyway, I am slowly gearing up for some VLF action over here. The
> other day I did some tests at 16.72 kHz into an ugly loop (very
> roughly 120 metres by 3 metres, single turn) and I was able to receive
> my signals using an unoptimise ferrite antenna at a bit over 2 km from
> the TX. I don't think I am in the near field at that distance, am I?
> :-)
>
> 73, Dimitris VK2COW
>
> >
>


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 Content preview:  Hi Dimitris, Thanks, very kind. If your's is even larger and
    has just 1 nF, then it will be just adequate :-) Another radio amateur from
    Germany offered me two capacitors wich will be suitable. They seem to be
   alr [...] 
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Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2 / VLF in VK?
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Hi Dimitris,

Thanks, very kind. If your's is even larger and has just 1 nF, then it 
will be just adequate :-)
Another radio amateur from Germany offered me two capacitors wich will 
be suitable. They seem to be already on the way in the post.

I wonder how this indoor loop performs as an RX antenna.  Of course it 
will depend on the neighbours QRM but maybe it is not as bad as 
expected. Then, i could try to arrange a JT9 QSO or maybe QRSS... If the 
other station is 20 dB stronger, then i could have a higher QRM level...

What about your VLF experiments, what is the next step? What was the 
locator of your 120m antenna? Could you build a longer antenna? Maybe 
you like to try a ground loop? Did you follow the recent experiments 
from my 900m long antenna on 8270 Hz? It is the best experimentation 
field that VLF amateur radio offers these days :-) My recommendation :-)

73, Stefan


Am 04.02.2019 06:54, schrieb Dimitrios Tsifakis:
> Hi all,
>
> I have a few mica capacitors that came from a MW broadcaster, similar
> to this one (in fact I have one that it bigger than this one).
>
> Stefan, I think this is probably your best bet and pity you are not
> closer otherwise I would be happy to lend you a couple to do your
> experiments :-)
>
> https://rustys.net.au/products/large-ducon-transmitter-honey-pot-capacitor
>
> (this is smaller than the ones I have, most are about 1 nF capacitance)
>
> 73, Dimitris VK2COW
>
> Στις Πέμ, 31 Ιαν 2019 στις 10:01 μ.μ., ο/η dhchurch
> <dhchurch@lineone.net>  έγραψε:
>    
>> Hello Dimitrios
>>
>> Polypropylene capacitors can actually self-heal to such an extent that there's little left of them. The melting point of polypropylene is not very high and they can end up as just a liitle blob of plastic.
>>
>> Don't worry though, I still use them suitably rated for the frequency in use and most of them are 600Vac or more.
>>
>> 73, Hugh, M0DSZ
>>
>> ----- Receiving the following content -----
>> From: Dimitrios Tsifakis
>> Receiver: rsgb_lf_group
>> Time: 2019-01-31, 00:25:55
>> Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2
>>
>> Hi Stefan,
>>
>> In my experience these polypropylene capacitors when they fail, they
>> just lose some capacitance. I think they call it 'self healing', maybe
>> they imply that when they fail there is no short circuit?
>>
>> I have some really nice silver mica capacitors (ex MW broadcast stuff)
>> that would be perfect for this task...
>>
>> Anyway, I am slowly gearing up for some VLF action over here. The
>> other day I did some tests at 16.72 kHz into an ugly loop (very
>> roughly 120 metres by 3 metres, single turn) and I was able to receive
>> my signals using an unoptimise ferrite antenna at a bit over 2 km from
>> the TX. I don't think I am in the near field at that distance, am I?
>> :-)
>>
>> 73, Dimitris VK2COW
>>
>>      
>>>        
>>      
>    

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 Content preview:  On Sun, 3 Feb 2019, DAVE PICK wrote: > I have an archive of
    the LF reflector from 1999 to early 2006. It's in a Thunderbird archive folder
    which > is readable by Thunderbird if you have it. thanks. i think this is
    either mbox format, or something that should be easy to convert. 
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On Sun, 3 Feb 2019, DAVE PICK wrote:

> I have an archive of the LF reflector from 1999 to early 2006. It's in a Thunderbird archive folder which
> is readable by Thunderbird if you have it.

thanks. i think this is either mbox format, or something that should be 
easy to convert.

later archives would also be very interesting, since they contain the 
early VLF work. i think it should be preserved.

VY 73

Jacek / SQ5BPF


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References: <1UTDpVl7g1.4QjadrkFEvr@optiplex980-pc> <Pine.LNX.4.64.1902021656100.11708@plato.ucs.mun.ca>
In-Reply-To: <Pine.LNX.4.64.1902021656100.11708@plato.ucs.mun.ca>
From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Mon, 4 Feb 2019 10:42:45 +0100
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 Content preview:  Joe, I've some decodes in JN64, see attachement. Thank you
    so much for your transmissions. Condx here: SDR setup clocked and referenced
    entirely with a NEO-M8T. UTC carrier S/N Eb/N0 mess. 0000 18.61 -0.3 VO1NA-*
    0230 23.10 5.2 ******* 0530 25.54 8.0 ******* 
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--000000000000931c0405810e5139
Content-Type: multipart/alternative; boundary="000000000000931c0105810e5137"

--000000000000931c0105810e5137
Content-Type: text/plain; charset="UTF-8"

Joe,

I've some decodes in JN64, see attachement. Thank you so much for your
transmissions.
Condx here: SDR setup clocked and referenced entirely with a NEO-M8T.

UTC     carrier S/N     Eb/N0      mess.
0000     18.61            -0.3         VO1NA-*
0230     23.10             5.2         *******
0530     25.54             8.0         *******


All the best

73 de Riccardo IW4DXW






Il giorno Sab 2 Feb 2019, 21:31 <jcraig@mun.ca> ha scritto:

> Hi Jay,
>
> Thanks for the report.  Normally it is off during the day.  Let's
> leave it on until Monday morning and see what happens.
>
> 73
> Joe
>
> On Sat, 2 Feb 2019, jrusgrove@comcast.net wrote:
>
> > Joe
> >
> > Decodes from this morning ... just checking spread between car Eb/N0 and
> Eb/N0
> > without interference. Curious if the LF beacon runs 24 hours or is
> switched off
> > during the day.
> >
> > 1100 Rank 0 car Eb/N0 21.6 dB Eb/N0 15.3 dB VO1NA**
> > 1130 Rank 0 car Eb/N0 14.6 dB Eb/N0 12.3 dB *******
> > 1200 -
> > 1230 -
> > 1300 -
> >
> > Jay W1VD
> >
>
>

--000000000000931c0105810e5137
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"auto"><div dir=3D"auto"><br></div><div dir=3D"=
auto">Joe,</div><div dir=3D"auto"><br></div><div dir=3D"auto">I&#39;ve some=
 decodes in JN64, see attachement. Thank you so much for your transmissions=
.</div><div>Condx here: SDR setup clocked and referenced entirely with a NE=
O-M8T.</div><div dir=3D"auto"><br></div><div dir=3D"auto">UTC=C2=A0 =C2=A0 =
=C2=A0carrier S/N=C2=A0 =C2=A0 =C2=A0Eb/N0 =C2=A0 =C2=A0 =C2=A0mess.</div><=
div>0000 =C2=A0 =C2=A0 18.61 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0-0.3 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 VO1NA-*</div>0230 =C2=A0 =C2=A0 23.10 =C2=A0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 5.2 =C2=A0 =C2=A0 =C2=A0 =C2=A0 *******<=
br>0530 =C2=A0 =C2=A0 25.54 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 8.0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 *******</div><div dir=3D"auto"><br><br>All the =
best</div><div dir=3D"auto"><br></div><div>73 de Riccardo IW4DXW</div><div>=
<br></div><div><br></div><div dir=3D"auto"><br></div><div dir=3D"auto"><br>=
</div><div dir=3D"auto"><br><br><div class=3D"gmail_quote" dir=3D"auto"><di=
v dir=3D"ltr">Il giorno Sab 2 Feb 2019, 21:31  &lt;<a href=3D"mailto:jcraig=
@mun.ca" rel=3D"noreferrer noreferrer" target=3D"_blank">jcraig@mun.ca</a>&=
gt; ha scritto:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:=
0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex">Hi Jay,<br>
<br>
Thanks for the report.=C2=A0 Normally it is off during the day.=C2=A0 Let&#=
39;s<br>
leave it on until Monday morning and see what happens.<br>
<br>
73<br>
Joe<br>
<br>
On Sat, 2 Feb 2019, <a href=3D"mailto:jrusgrove@comcast.net" rel=3D"norefer=
rer noreferrer noreferrer" target=3D"_blank">jrusgrove@comcast.net</a> wrot=
e:<br>
<br>
&gt; Joe<br>
&gt;<br>
&gt; Decodes from this morning ... just checking spread between car Eb/N0 a=
nd Eb/N0<br>
&gt; without interference. Curious if the LF beacon runs 24 hours or is swi=
tched off<br>
&gt; during the day.<br>
&gt;<br>
&gt; 1100 Rank 0 car Eb/N0 21.6 dB Eb/N0 15.3 dB VO1NA**<br>
&gt; 1130 Rank 0 car Eb/N0 14.6 dB Eb/N0 12.3 dB *******<br>
&gt; 1200 -<br>
&gt; 1230 -<br>
&gt; 1300 -<br>
&gt;<br>
&gt; Jay W1VD<br>
&gt;<br>
<br>
</blockquote></div>
</div>
</div>

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 <alpine.DEB.2.11.1902041006480.725@mailn.lipkowski.org>
From: Paul Nicholson <vlf0403@abelian.org>
Message-ID: <91ad4456-4056-3166-18f9-22a252f3edf0@abelian.org>
Date: Mon, 4 Feb 2019 10:18:04 +0000
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 Content preview:  The archive of blacksheep maintained at https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/
    works well, is at least partially indexed by Google, and the archive is downloadable
    in the long-established and well known mbox format. 
 Content analysis details:   (-0.7 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
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Subject: Re: LF: LF Reflector archive
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X-SA-Exim-Rcpt-To: rs_out_1@blacksheep.org
X-SA-Exim-Scanned: No; SAEximRunCond expanded to false


The archive of blacksheep maintained at

  https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/

works well, is at least partially indexed by Google, and the
archive is downloadable in the long-established and well known
mbox format.

The old Yahoo group and its migration to groups.io does not
have a public archive, therefore messages posted are lost
forever.   Without an archive, there is no enduring history
of LF and VLF developments.

When blacksheep eventually fails, the RSGB LF group will at that
moment disappear from history unless a new non-secret group is
created on groups.io

Apart from the unwarranted secrecy, groups.io provides an ideal
platform for a forum, there are no privacy or security issues.

--
Paul Nicholson
--

From owner-rsgb_lf_group@blacksheep.org  Mon Feb  4 12:18:57 2019
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In-Reply-To: <91ad4456-4056-3166-18f9-22a252f3edf0@abelian.org>
From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Mon, 4 Feb 2019 11:14:07 +0000
Message-ID: <CAA8k23TGN=orhMbcoOjU4M_dumDuft4VwsdWAraFjG+SHoYzxg@mail.gmail.com>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
X-Spam-Score: 0.0 (/)
X-Spam-Report: Spam detection software, running on the system "relay1.thorcom.net",
 has NOT identified this incoming email as spam.  The original
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 similar future email.  If you have any questions, see
 the administrator of that system for details.
 Content preview:  There is no secrecy with the groups.io You just register All
    messages are there in the archive Andy www.g4jnt.com (owner of two other
   groups.io) 
 Content analysis details:   (0.0 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -0.0 RCVD_IN_DNSWL_NONE     RBL: Sender listed at http://www.dnswl.org/,
                             no trust
                             [2607:f8b0:4864:20:0:0:0:e29 listed in]
                             [list.dnswl.org]
 -0.0 SPF_PASS               SPF: sender matches SPF record
  0.0 FREEMAIL_FROM          Sender email is commonly abused enduser mail
                             provider (andy.g4jnt[at]gmail.com)
  0.0 HTML_MESSAGE           BODY: HTML included in message
X-Scan-Signature: 3d0ae5b4ae8b74dc4bf5c1dbe3fef430
Subject: Re: LF: LF Reflector archive
Content-Type: multipart/alternative; boundary="000000000000080f0c05810f98b1"
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--000000000000080f0c05810f98b1
Content-Type: text/plain; charset="UTF-8"

There is no secrecy with the groups.io
You just register

All messages are there in the archive

Andy
www.g4jnt.com
(owner of two other groups.io)



On Mon, 4 Feb 2019 at 10:22, Paul Nicholson <vlf0403@abelian.org> wrote:

>
> The archive of blacksheep maintained at
>
>   https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/
>
> works well, is at least partially indexed by Google, and the
> archive is downloadable in the long-established and well known
> mbox format.
>
> The old Yahoo group and its migration to groups.io does not
> have a public archive, therefore messages posted are lost
> forever.   Without an archive, there is no enduring history
> of LF and VLF developments.
>
> When blacksheep eventually fails, the RSGB LF group will at that
> moment disappear from history unless a new non-secret group is
> created on groups.io
>
> Apart from the unwarranted secrecy, groups.io provides an ideal
> platform for a forum, there are no privacy or security issues.
>
> --
> Paul Nicholson
> --
>
>

--000000000000080f0c05810f98b1
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">There is no secrecy with the <a href=3D"http://g=
roups.io">groups.io</a></div><div class=3D"gmail_default" style=3D"font-fam=
ily:tahoma,sans-serif;font-size:small">You just register</div><div class=3D=
"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br=
></div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;=
font-size:small">All messages are there in the archive</div><div class=3D"g=
mail_default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br><=
/div><div><div dir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"gmai=
l_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><=
div><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=3D"font-siz=
e:12.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank">www.g4jnt.com<=
/a></span><br></div><div><div class=3D"gmail_default" style=3D"font-family:=
tahoma,sans-serif;font-size:small">(owner of two other <a href=3D"http://gr=
oups.io">groups.io</a>)</div><br></div></div></div></div></div></div></div>=
</div></div></div></div></div><br></div><br><div class=3D"gmail_quote"><div=
 dir=3D"ltr" class=3D"gmail_attr">On Mon, 4 Feb 2019 at 10:22, Paul Nichols=
on &lt;<a href=3D"mailto:vlf0403@abelian.org">vlf0403@abelian.org</a>&gt; w=
rote:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0p=
x 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><br>
The archive of blacksheep maintained at<br>
<br>
=C2=A0 <a href=3D"https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_gro=
up/" rel=3D"noreferrer" target=3D"_blank">https://klubnl.pl/rsgb_lf_group-a=
rchives/html/rsgb_lf_group/</a><br>
<br>
works well, is at least partially indexed by Google, and the<br>
archive is downloadable in the long-established and well known<br>
mbox format.<br>
<br>
The old Yahoo group and its migration to <a href=3D"http://groups.io" rel=
=3D"noreferrer" target=3D"_blank">groups.io</a> does not<br>
have a public archive, therefore messages posted are lost<br>
forever.=C2=A0 =C2=A0Without an archive, there is no enduring history<br>
of LF and VLF developments.<br>
<br>
When blacksheep eventually fails, the RSGB LF group will at that<br>
moment disappear from history unless a new non-secret group is<br>
created on <a href=3D"http://groups.io" rel=3D"noreferrer" target=3D"_blank=
">groups.io</a><br>
<br>
Apart from the unwarranted secrecy, <a href=3D"http://groups.io" rel=3D"nor=
eferrer" target=3D"_blank">groups.io</a> provides an ideal<br>
platform for a forum, there are no privacy or security issues.<br>
<br>
--<br>
Paul Nicholson<br>
--<br>
<br>
</blockquote></div>

--000000000000080f0c05810f98b1--

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Date: Mon, 4 Feb 2019 12:21:51 +0000
From: Chris Wilson <dead.fets@gmail.com>
X-Priority: 3 (Normal)
Message-ID: <1771146765.20190204122151@gmail.com>
To: LF Group <rsgb_lf_group@blacksheep.org>
MIME-Version: 1.0
X-Spam-Score: 0.0 (/)
X-Spam-Report: Spam detection software, running on the system "relay1.thorcom.net",
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 similar future email.  If you have any questions, see
 the administrator of that system for details.
 Content preview:  Hello LF, A naive question re WSPR15 please? Assuming the
   source code is available how hard would it be for a clever person to add X2
    functionality to it? Thanks. -- Best regards, Chris mailto:dead.fets@gmail.com
 Content analysis details:   (0.0 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -0.0 RCVD_IN_DNSWL_NONE     RBL: Sender listed at http://www.dnswl.org/,
                             no trust
                             [2a00:1450:4864:20:0:0:0:42d listed in]
                             [list.dnswl.org]
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  0.0 FREEMAIL_FROM          Sender email is commonly abused enduser mail
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Subject: LF: Naive WSPR15 question
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Hello  LF,

  A  naive  question  re  WSPR15  please?  Assuming the source code is
  available  how  hard  would  it  be  for  a  clever person to add X2
  functionality to it? Thanks.

-- 
Best regards,
 Chris                          mailto:dead.fets@gmail.com


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 Content preview:  Hello Chris, For a clever person it is very easy :-) It will
    depend on which way you want to generate WSPR. Here, for example, i have
   a Raspi which generates my WSPR (2) for MF. I modified the c source code so
    tha [...] 
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Subject: Re: LF: Naive WSPR15 question
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Hello Chris,

For a clever person it is very easy :-)
It will depend on which way you want to generate WSPR.
Here, for example, i have a Raspi which generates my WSPR (2) for MF. I 
modified the c source code so that the frequency is 4 times higher and 
the frequency shift is 4 times higher too. In my PA, probably like in 
yours, there is a frequency divider using CD4013 ICs which reproduce the 
desired frequency and frequency shift. Of course this can be done with a 
factor 2 too.
For Windows solutions, there is DF6NMs tool for slow WSPR which works 
very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be 
modified for twice the frequency shift but then you will need an 
upconverter to convert it to LF or MF...

73, Stefan

Am 04.02.2019 13:21, schrieb Chris Wilson:
>
> Hello  LF,
>
>    A  naive  question  re  WSPR15  please?  Assuming the source code is
>    available  how  hard  would  it  be  for  a  clever person to add X2
>    functionality to it? Thanks.
>
>    

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 Content preview:  ...i checked some files from the slow_WSPR tool. I think i
    would be able to solve the problem. Maybe Markus likes to confirm that this
    could work (getting a factor 2 in the frequency shift)? Chris, it [...] 
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...i checked some files from the slow_WSPR tool. I think i would be able 
to solve the problem. Maybe Markus likes to confirm that this could work 
(getting a factor 2 in the frequency shift)?
Chris, it would then be worth to try the normal tool first.

73, Stefan

Am 04.02.2019 20:25, schrieb DK7FC:
> Hello Chris,
>
> For a clever person it is very easy :-)
> It will depend on which way you want to generate WSPR.
> Here, for example, i have a Raspi which generates my WSPR (2) for MF. 
> I modified the c source code so that the frequency is 4 times higher 
> and the frequency shift is 4 times higher too. In my PA, probably like 
> in yours, there is a frequency divider using CD4013 ICs which 
> reproduce the desired frequency and frequency shift. Of course this 
> can be done with a factor 2 too.
> For Windows solutions, there is DF6NMs tool for slow WSPR which works 
> very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be 
> modified for twice the frequency shift but then you will need an 
> upconverter to convert it to LF or MF...
>
> 73, Stefan
>
> Am 04.02.2019 13:21, schrieb Chris Wilson:
>>
>> Hello  LF,
>>
>>    A  naive  question  re  WSPR15  please?  Assuming the source code is
>>    available  how  hard  would  it  be  for  a  clever person to add X2
>>    functionality to it? Thanks.
>>
>

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Date: Mon, 4 Feb 2019 21:08:35 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  Hi Stefan, Chris, in principle yes… (R. Eriwan) The old
   tools from 2012 are here  http://df6nm.bplaced.net/wspr/slowWSPR.zip But
   they used a homemade 16-bit-utility "waitraster" for timing, which is no
   longer supported by 64-bit Win-7 and Win 10. [...] 
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Subject: Re: LF: Naive WSPR15 question
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Hi Stefan, Chris,

in principle yes=E2=80=A6 (R. Eriwan)

The old tools from 2012 are here=C2=A0
http://df6nm.bplaced.net/wspr/slowWSPR.zip=20
But they used a homemade=C2=A016-bit-utility "waitraster" for timing, which=
 is no longer supported by 64-bit Win-7 and Win 10. This=C2=A0can be replac=
ed by simple DOS commands, which=C2=A0has so far been implemented for=C2=A0=
receiving WSPR-15
https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg0031=
8.html
but not yet for transmitting.=C2=A0So a little more work=C2=A0will be neede=
d.

On the other hand, I'm asking myself=C2=A0why=C2=A0so many people=C2=A0stil=
l insist on=C2=A0having=C2=A0dividers before their PA's.=C2=A0It only makes=
 life more difficult, and=C2=A0undermines coherent=C2=A0EbNaut or Opera sig=
nal transmissions.=C2=A0

Best 73,
Markus (DF6NM)

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Mo, 4. Feb. 2019 21:11
Betreff: Re: LF: Naive WSPR15 question

...i checked some files from the slow_WSPR tool. I think i would be able=20
to solve the problem. Maybe Markus likes to confirm that this could work=20
(getting a factor 2 in the frequency shift)?
Chris, it would then be worth to try the normal tool first.

73, Stefan

Am 04.02.2019 20:25, schrieb DK7FC:
> Hello Chris,
>
> For a clever person it is very easy :-)
> It will depend on which way you want to generate WSPR.
> Here, for example, i have a Raspi which generates my WSPR (2) for MF.=20
> I modified the c source code so that the frequency is 4 times higher=20
> and the frequency shift is 4 times higher too. In my PA, probably like=20
> in yours, there is a frequency divider using CD4013 ICs which=20
> reproduce the desired frequency and frequency shift. Of course this=20
> can be done with a factor 2 too.
> For Windows solutions, there is DF6NMs tool for slow WSPR which works=20
> very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be=20
> modified for twice the frequency shift but then you will need an=20
> upconverter to convert it to LF or MF...
>
> 73, Stefan
>
> Am 04.02.2019 13:21, schrieb Chris Wilson:
>>
>> Hello=C2=A0 LF,
>>
>>=C2=A0 =C2=A0 A=C2=A0 naive=C2=A0 question=C2=A0 re=C2=A0 WSPR15=C2=A0 pl=
ease?=C2=A0 Assuming the source code is
>>=C2=A0 =C2=A0 available=C2=A0 how=C2=A0 hard=C2=A0 would=C2=A0 it=C2=A0 b=
e=C2=A0 for=C2=A0 a=C2=A0 clever person to add X2
>>=C2=A0 =C2=A0 functionality to it? Thanks.
>>
>


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<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;">Hi Stefan, Chris,<br><br>in principle yes=E2=80=A6 (R. E=
riwan)<br><br>The old tools from 2012 are here&nbsp;<br>http://df6nm.bplace=
d.net/wspr/slowWSPR.zip <br>But they used a homemade&nbsp;16-bit-utility "w=
aitraster" for timing, which is no longer supported by 64-bit Win-7 and Win=
 10. This&nbsp;can be replaced by simple DOS commands, which&nbsp;has so fa=
r been implemented for&nbsp;receiving WSPR-15<br>https://klubnl.pl/rsgb_lf_=
group-archives/html/rsgb_lf_group/2018-11/msg00318.html<br>but not yet for =
transmitting.&nbsp;So a little more work&nbsp;will be needed.<br><br>On the=
 other hand, I'm asking myself&nbsp;why&nbsp;so many people&nbsp;still insi=
st on&nbsp;having&nbsp;dividers before their PA's.&nbsp;It only makes life =
more difficult, and&nbsp;undermines coherent&nbsp;EbNaut or Opera signal tr=
ansmissions.&nbsp;<br><br>Best 73,<br>Markus (DF6NM)<br><br>-----Urspr=C3=
=BCngliche Mitteilung-----<br>Von: DK7FC &lt;selberdenken@posteo.de&gt;<br>=
An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br>Verschickt: Mo, 4=
. Feb. 2019 21:11<br>Betreff: Re: LF: Naive WSPR15 question<br><br></div><d=
iv dir=3D"ltr">...i checked some files from the slow_WSPR tool. I think i w=
ould be able <br clear=3D"none">to solve the problem. Maybe Markus likes to=
 confirm that this could work <br clear=3D"none">(getting a factor 2 in the=
 frequency shift)?<br clear=3D"none">Chris, it would then be worth to try t=
he normal tool first.<br clear=3D"none"><br clear=3D"none">73, Stefan<br cl=
ear=3D"none"><div class=3D"yqt7610097017" id=3D"yqtfd93454"><br clear=3D"no=
ne">Am 04.02.2019 20:25, schrieb DK7FC:<br clear=3D"none">&gt; Hello Chris,=
<br clear=3D"none">&gt;<br clear=3D"none">&gt; For a clever person it is ve=
ry easy :-)<br clear=3D"none">&gt; It will depend on which way you want to =
generate WSPR.<br clear=3D"none">&gt; Here, for example, i have a Raspi whi=
ch generates my WSPR (2) for MF. <br clear=3D"none">&gt; I modified the c s=
ource code so that the frequency is 4 times higher <br clear=3D"none">&gt; =
and the frequency shift is 4 times higher too. In my PA, probably like <br =
clear=3D"none">&gt; in yours, there is a frequency divider using CD4013 ICs=
 which <br clear=3D"none">&gt; reproduce the desired frequency and frequenc=
y shift. Of course this <br clear=3D"none">&gt; can be done with a factor 2=
 too.<br clear=3D"none">&gt; For Windows solutions, there is DF6NMs tool fo=
r slow WSPR which works <br clear=3D"none">&gt; very reliable here, for WSP=
R-2 and WSPR-15. I'm sure this can be <br clear=3D"none">&gt; modified for =
twice the frequency shift but then you will need an <br clear=3D"none">&gt;=
 upconverter to convert it to LF or MF...<br clear=3D"none">&gt;<br clear=
=3D"none">&gt; 73, Stefan<br clear=3D"none">&gt;<br clear=3D"none">&gt; Am =
04.02.2019 13:21, schrieb Chris Wilson:<br clear=3D"none">&gt;&gt;<br clear=
=3D"none">&gt;&gt; Hello&nbsp; LF,<br clear=3D"none">&gt;&gt;<br clear=3D"n=
one">&gt;&gt;&nbsp; &nbsp; A&nbsp; naive&nbsp; question&nbsp; re&nbsp; WSPR=
15&nbsp; please?&nbsp; Assuming the source code is<br clear=3D"none">&gt;&g=
t;&nbsp; &nbsp; available&nbsp; how&nbsp; hard&nbsp; would&nbsp; it&nbsp; b=
e&nbsp; for&nbsp; a&nbsp; clever person to add X2<br clear=3D"none">&gt;&gt=
;&nbsp; &nbsp; functionality to it? Thanks.<br clear=3D"none">&gt;&gt;<br c=
lear=3D"none">&gt;<br clear=3D"none"><br clear=3D"none"></div></div></div>
------=_Part_2898207_809954970.1549314515046--

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From: Roman <rw3adb@yandex.ru>
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In-Reply-To: <1615191474.2898208.1549314515047@mail.yahoo.com>
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 Content preview:  Hello, Genossen Lfers! RN3AUS DDS generate WSPR-15, but own
    forum in fault up to now(( Email him personaly if you want - rn3aus@mail.ru
    73! Roman 
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Subject: Re: LF: Naive WSPR15 question
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Hello, Genossen Lfers!

RN3AUS DDS generate WSPR-15, but own forum in fault up to now((
Email him personaly if you want - rn3aus@mail.ru

73!
Roman

> Hi Stefan, Chris,
> 
> in principle yes… (R. Eriwan)
> 
> The old tools from 2012 are here
> http://df6nm.bplaced.net/wspr/slowWSPR.zip
> But they used a homemade 16-bit-utility "waitraster" for timing, which is no longer supported by 64-bit Win-7 and Win 10. This can be replaced by simple DOS commands, which has so far been implemented for receiving WSPR-15
> https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg00318.html
> but not yet for transmitting. So a little more work will be needed.
> 
> On the other hand, I'm asking myself why so many people still insist on having dividers before their PA's. It only makes life more difficult, and undermines coherent EbNaut or Opera signal transmissions.
> 
> Best 73,
> Markus (DF6NM)
> 
> -----Ursprüngliche Mitteilung-----
> Von: DK7FC <selberdenken@posteo.de>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Mo, 4. Feb. 2019 21:11
> Betreff: Re: LF: Naive WSPR15 question
> 
> ...i checked some files from the slow_WSPR tool. I think i would be able
> to solve the problem. Maybe Markus likes to confirm that this could work
> (getting a factor 2 in the frequency shift)?
> Chris, it would then be worth to try the normal tool first.
> 
> 73, Stefan
> 
> Am 04.02.2019 20:25, schrieb DK7FC:
>> Hello Chris,
>>
>> For a clever person it is very easy :-)
>> It will depend on which way you want to generate WSPR.
>> Here, for example, i have a Raspi which generates my WSPR (2) for MF.
>> I modified the c source code so that the frequency is 4 times higher
>> and the frequency shift is 4 times higher too. In my PA, probably like
>> in yours, there is a frequency divider using CD4013 ICs which
>> reproduce the desired frequency and frequency shift. Of course this
>> can be done with a factor 2 too.
>> For Windows solutions, there is DF6NMs tool for slow WSPR which works
>> very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be
>> modified for twice the frequency shift but then you will need an
>> upconverter to convert it to LF or MF...
>>
>> 73, Stefan
>>
>> Am 04.02.2019 13:21, schrieb Chris Wilson:
>>>
>>> Hello LF,
>>>
>>> A naive question re WSPR15 please? Assuming the source code is
>>> available how hard would it be for a clever person to add X2
>>> functionality to it? Thanks.
>>>
>>
-- 
73!
Roman, RW3ADB

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 Content preview:  Hi Riccardo, Thanks for the report. It seems that transmission
    just made it through! Best 73 Joe VO1NA 
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Subject: Re: LF: VO1NA EbNaut
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Hi Riccardo,

Thanks for the report.  It seems that transmission just made it through!

Best 73
Joe VO1NA

On Mon, 4 Feb 2019, Riccardo Zoli wrote:

> Joe,
>
> I've some decodes in JN64, see attachement. Thank you so much for your
> transmissions.
> Condx here: SDR setup clocked and referenced entirely with a NEO-M8T.
>
> UTC     carrier S/N     Eb/N0      mess.
> 0000     18.61            -0.3         VO1NA-*
> 0230     23.10             5.2         *******
> 0530     25.54             8.0         *******
>
>
> All the best
>
> 73 de Riccardo IW4DXW
>
>
>
>
>
>
> Il giorno Sab 2 Feb 2019, 21:31 <jcraig@mun.ca> ha scritto:
>
>> Hi Jay,
>>
>> Thanks for the report.  Normally it is off during the day.  Let's
>> leave it on until Monday morning and see what happens.
>>
>> 73
>> Joe
>>
>> On Sat, 2 Feb 2019, jrusgrove@comcast.net wrote:
>>
>>> Joe
>>>
>>> Decodes from this morning ... just checking spread between car Eb/N0 and
>> Eb/N0
>>> without interference. Curious if the LF beacon runs 24 hours or is
>> switched off
>>> during the day.
>>>
>>> 1100 Rank 0 car Eb/N0 21.6 dB Eb/N0 15.3 dB VO1NA**
>>> 1130 Rank 0 car Eb/N0 14.6 dB Eb/N0 12.3 dB *******
>>> 1200 -
>>> 1230 -
>>> 1300 -
>>>
>>> Jay W1VD
>>>
>>
>>
>

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In-Reply-To: <5C57FC38.3020203@posteo.de>
From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Tue, 5 Feb 2019 11:16:34 +1100
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To: rsgb_lf_group@blacksheep.org
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 Content preview:  Hi Stefan, I am working on both making a portable VLF magnetic
    field antenna (tuned) and a transmit antenna which perhaps will be better
    than the existing 120 m by 3 m (average height) loop. The resistance of th
    [...] 
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Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2 / VLF in VK?
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Hi Stefan,

I am working on both making a portable VLF magnetic field antenna
(tuned) and a transmit antenna which perhaps will be better than the
existing 120 m by 3 m (average height) loop. The resistance of this
loop isn't stellar (about 11 ohm DCR) and half of it is aluminium
welding wire. Anyway, it's there and it is my reference antenna. The
new loop antenna will be better but it is still under construction.
Heavy copper cabling is surprisingly difficult to put up in the air
with limited resources. Anyway, once all that is in place, I will do
some local tests (without rubidium or GPS locked oscillators) and
we'll take it from there. My QTH locator is QF44OX (very close to
QF44nx). I have plenty of space but it's undulating and kangaroos
always make a mess with low hanging wires!

Is there a web page with your 8270 Hz experiments? I'd love to read up
a bit of inspiring material of what others have achieved as it can be
quite lonely doing experiments like that where I am. How much radiated
power have you achieved?

73, Dimitris VK2COW


Στις Δευ, 4 Φεβ 2019 στις 7:57 μ.μ., ο/η DK7FC <selberdenken@posteo.de> έγραψε:
>
> Hi Dimitris,
>
> Thanks, very kind. If your's is even larger and has just 1 nF, then it
> will be just adequate :-)
> Another radio amateur from Germany offered me two capacitors wich will
> be suitable. They seem to be already on the way in the post.
>
> I wonder how this indoor loop performs as an RX antenna.  Of course it
> will depend on the neighbours QRM but maybe it is not as bad as
> expected. Then, i could try to arrange a JT9 QSO or maybe QRSS... If the
> other station is 20 dB stronger, then i could have a higher QRM level...
>
> What about your VLF experiments, what is the next step? What was the
> locator of your 120m antenna? Could you build a longer antenna? Maybe
> you like to try a ground loop? Did you follow the recent experiments
> from my 900m long antenna on 8270 Hz? It is the best experimentation
> field that VLF amateur radio offers these days :-) My recommendation :-)
>
> 73, Stefan
>
>
> Am 04.02.2019 06:54, schrieb Dimitrios Tsifakis:
> > Hi all,
> >
> > I have a few mica capacitors that came from a MW broadcaster, similar
> > to this one (in fact I have one that it bigger than this one).
> >
> > Stefan, I think this is probably your best bet and pity you are not
> > closer otherwise I would be happy to lend you a couple to do your
> > experiments :-)
> >
> > https://rustys.net.au/products/large-ducon-transmitter-honey-pot-capacitor
> >
> > (this is smaller than the ones I have, most are about 1 nF capacitance)
> >
> > 73, Dimitris VK2COW
> >
> > Στις Πέμ, 31 Ιαν 2019 στις 10:01 μ.μ., ο/η dhchurch
> > <dhchurch@lineone.net>  έγραψε:
> >
> >> Hello Dimitrios
> >>
> >> Polypropylene capacitors can actually self-heal to such an extent that there's little left of them. The melting point of polypropylene is not very high and they can end up as just a liitle blob of plastic.
> >>
> >> Don't worry though, I still use them suitably rated for the frequency in use and most of them are 600Vac or more.
> >>
> >> 73, Hugh, M0DSZ
> >>
> >> ----- Receiving the following content -----
> >> From: Dimitrios Tsifakis
> >> Receiver: rsgb_lf_group
> >> Time: 2019-01-31, 00:25:55
> >> Subject: Re: LF: TXing WSPR/MF on an indoor loop, part 2
> >>
> >> Hi Stefan,
> >>
> >> In my experience these polypropylene capacitors when they fail, they
> >> just lose some capacitance. I think they call it 'self healing', maybe
> >> they imply that when they fail there is no short circuit?
> >>
> >> I have some really nice silver mica capacitors (ex MW broadcast stuff)
> >> that would be perfect for this task...
> >>
> >> Anyway, I am slowly gearing up for some VLF action over here. The
> >> other day I did some tests at 16.72 kHz into an ugly loop (very
> >> roughly 120 metres by 3 metres, single turn) and I was able to receive
> >> my signals using an unoptimise ferrite antenna at a bit over 2 km from
> >> the TX. I don't think I am in the near field at that distance, am I?
> >> :-)
> >>
> >> 73, Dimitris VK2COW
> >>
> >>
> >>>
> >>
> >
>


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 Content preview:  naaaaa I cant believe that you too remember it Markus!! :-)))(I
    mean of course the reference to Radio Yerivan ;-)) ) have a nice day! Marco
    IK1HSS ----Messaggio originale---- Da: markusvester@aol.com 
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Subject: R: Re: LF: Naive WSPR15 question - Radio Erivan
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naaaaa I cant believe that you too remember it Markus!! :-)))(I mean of cou=
rse the reference to Radio Yerivan ;-)) )
have a nice day!
Marco IK1HSS



----Messaggio originale----

Da: markusvester@aol.com

Data: 4-feb-2019 22.08

A: <rsgb_lf_group@blacksheep.org>

Ogg: Re: LF: Naive WSPR15 question



Hi Stefan, Chris,

in principle yes=E2=80=A6 (R. Eriwan)

The old tools from 2012 are here=20
http://df6nm.bplaced.net/wspr/slowWSPR.zip=20
But they used a homemade 16-bit-utility "waitraster" for timing, which is n=
o longer supported by 64-bit Win-7 and Win 10. This can be replaced by simp=
le DOS commands, which has so far been implemented for receiving WSPR-15
https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg0031=
8.html
but not yet for transmitting. So a little more work will be needed.

On the other hand, I'm asking myself why so many people still insist on hav=
ing dividers before their PA's. It only makes life more difficult, and unde=
rmines coherent EbNaut or Opera signal transmissions.=20

Best 73,
Markus (DF6NM)

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Mo, 4. Feb. 2019 21:11
Betreff: Re: LF: Naive WSPR15 question

...i checked some files from the slow_WSPR tool. I think i would be able to=
 solve the problem. Maybe Markus likes to confirm that this could work (get=
ting a factor 2 in the frequency shift)?Chris, it would then be worth to tr=
y the normal tool first.73, StefanAm 04.02.2019 20:25, schrieb DK7FC:> Hell=
o Chris,>> For a clever person it is very easy :-)> It will depend on which=
 way you want to generate WSPR.> Here, for example, i have a Raspi which ge=
nerates my WSPR (2) for MF. > I modified the c source code so that the freq=
uency is 4 times higher > and the frequency shift is 4 times higher too. In=
 my PA, probably like > in yours, there is a frequency divider using CD4013=
 ICs which > reproduce the desired frequency and frequency shift. Of course=
 this > can be done with a factor 2 too.> For Windows solutions, there is D=
F6NMs tool for slow WSPR which works > very reliable here, for WSPR-2 and W=
SPR-15. I'm sure this can be > modified for twice the frequency shift but t=
hen you will need an > upconverter to convert it to LF or MF...>> 73, Stefa=
n>> Am 04.02.2019 13:21, schrieb Chris Wilson:>>>> Hello  LF,>>>>    A  nai=
ve  question  re  WSPR15  please?  Assuming the source code is>>    availab=
le  how  hard  would  it  be  for  a  clever person to add X2>>    function=
ality to it? Thanks.>>>




------=_Part_62256_6977437.1549354260455
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div>naaaaa I cant believe that you too remember it Markus!! :-)))</div><di=
v>(I mean of course the reference to Radio Yerivan ;-)) )</div><div><br></d=
iv><div>have a nice day!</div><div><br></div><div>Marco IK1HSS<br></div>
<br>
----Messaggio originale----<br>
Da: markusvester@aol.com<br>
Data: 4-feb-2019 22.08<br>
A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Ogg: Re: LF: Naive WSPR15 question<br>
<br>
<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;">Hi Stefan, Chris,<br><br>in principle yes=E2=80=A6 (R. E=
riwan)<br><br>The old tools from 2012 are here&nbsp;<br>http://df6nm.bplace=
d.net/wspr/slowWSPR.zip <br>But they used a homemade&nbsp;16-bit-utility "w=
aitraster" for timing, which is no longer supported by 64-bit Win-7 and Win=
 10. This&nbsp;can be replaced by simple DOS commands, which&nbsp;has so fa=
r been implemented for&nbsp;receiving WSPR-15<br>https://klubnl.pl/rsgb_lf_=
group-archives/html/rsgb_lf_group/2018-11/msg00318.html<br>but not yet for =
transmitting.&nbsp;So a little more work&nbsp;will be needed.<br><br>On the=
 other hand, I'm asking myself&nbsp;why&nbsp;so many people&nbsp;still insi=
st on&nbsp;having&nbsp;dividers before their PA's.&nbsp;It only makes life =
more difficult, and&nbsp;undermines coherent&nbsp;EbNaut or Opera signal tr=
ansmissions.&nbsp;<br><br>Best 73,<br>Markus (DF6NM)<br><br>-----Urspr=C3=
=BCngliche Mitteilung-----<br>Von: DK7FC &lt;selberdenken@posteo.de&gt;<br>=
An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br>Verschickt: Mo, 4=
. Feb. 2019 21:11<br>Betreff: Re: LF: Naive WSPR15 question<br><br></div><d=
iv dir=3D"ltr">...i checked some files from the slow_WSPR tool. I think i w=
ould be able <br clear=3D"none">to solve the problem. Maybe Markus likes to=
 confirm that this could work <br clear=3D"none">(getting a factor 2 in the=
 frequency shift)?<br clear=3D"none">Chris, it would then be worth to try t=
he normal tool first.<br clear=3D"none"><br clear=3D"none">73, Stefan<br cl=
ear=3D"none"><div class=3D"yqt7610097017" id=3D"yqtfd93454"><br clear=3D"no=
ne">Am 04.02.2019 20:25, schrieb DK7FC:<br clear=3D"none">&gt; Hello Chris,=
<br clear=3D"none">&gt;<br clear=3D"none">&gt; For a clever person it is ve=
ry easy :-)<br clear=3D"none">&gt; It will depend on which way you want to =
generate WSPR.<br clear=3D"none">&gt; Here, for example, i have a Raspi whi=
ch generates my WSPR (2) for MF. <br clear=3D"none">&gt; I modified the c s=
ource code so that the frequency is 4 times higher <br clear=3D"none">&gt; =
and the frequency shift is 4 times higher too. In my PA, probably like <br =
clear=3D"none">&gt; in yours, there is a frequency divider using CD4013 ICs=
 which <br clear=3D"none">&gt; reproduce the desired frequency and frequenc=
y shift. Of course this <br clear=3D"none">&gt; can be done with a factor 2=
 too.<br clear=3D"none">&gt; For Windows solutions, there is DF6NMs tool fo=
r slow WSPR which works <br clear=3D"none">&gt; very reliable here, for WSP=
R-2 and WSPR-15. I'm sure this can be <br clear=3D"none">&gt; modified for =
twice the frequency shift but then you will need an <br clear=3D"none">&gt;=
 upconverter to convert it to LF or MF...<br clear=3D"none">&gt;<br clear=
=3D"none">&gt; 73, Stefan<br clear=3D"none">&gt;<br clear=3D"none">&gt; Am =
04.02.2019 13:21, schrieb Chris Wilson:<br clear=3D"none">&gt;&gt;<br clear=
=3D"none">&gt;&gt; Hello&nbsp; LF,<br clear=3D"none">&gt;&gt;<br clear=3D"n=
one">&gt;&gt;&nbsp; &nbsp; A&nbsp; naive&nbsp; question&nbsp; re&nbsp; WSPR=
15&nbsp; please?&nbsp; Assuming the source code is<br clear=3D"none">&gt;&g=
t;&nbsp; &nbsp; available&nbsp; how&nbsp; hard&nbsp; would&nbsp; it&nbsp; b=
e&nbsp; for&nbsp; a&nbsp; clever person to add X2<br clear=3D"none">&gt;&gt=
;&nbsp; &nbsp; functionality to it? Thanks.<br clear=3D"none">&gt;&gt;<br c=
lear=3D"none">&gt;<br clear=3D"none"><br clear=3D"none"></div></div></div><=
br>
<br>

------=_Part_62256_6977437.1549354260455--


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To: rsgb_lf_group@blacksheep.org
References: <1615191474.2898208.1549314515047.ref@mail.yahoo.com> <1615191474.2898208.1549314515047@mail.yahoo.com> <14035761549315679@iva1-a2ffb02749cf.qloud-c.yandex.net>
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 Content preview:  MF, Since yesterday, there is some sun in Heidelberg and my
    tree grabber came back. MF reception is possible again (the VLF E field still
    has a problem). http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7F [...] 
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Subject: LF: MF WSPR
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MF,

Since yesterday, there is some sun in Heidelberg and my tree grabber 
came back. MF reception is possible again (the VLF E field still has a 
problem).
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_Grabber.html

Last night i got my best RX distance on MF ever (i think):

Timestamp 	Call 	MHz 	SNR 	Drift 	Grid 	Pwr 	Reporter 	RGrid 	km 	az
  2019-02-05 06:12 	 WA4SZE 	 0.475703 	 -29 	 0 	 EM65 	 0.2 
  DK7FC/P 	 JN49ik 	 7470 	 45


The band still seems to be open for DX.

73, Stefan

--------------070908020005030203040103
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 8bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
MF, <br>
<br>
Since yesterday, there is some sun in Heidelberg and my tree grabber
came back. MF reception is possible again (the VLF E field still has a
problem).<br>
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_Grabber.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_Grabber.html</a><br>
<br>
Last night i got my best RX distance on MF ever (i think):<br>
<br>
<table>
  <tbody>
    <tr>
      <th>Timestamp</th>
      <th>Call</th>
      <th>MHz</th>
      <th>SNR</th>
      <th>Drift</th>
      <th>Grid</th>
      <th>Pwr</th>
      <th>Reporter</th>
      <th>RGrid</th>
      <th>km</th>
      <th>az</th>
    </tr>
    <tr>
      <td align="right"> 2019-02-05 06:12 </td>
      <td align="left"> WA4SZE </td>
      <td align="right"> 0.475703 </td>
      <td align="right"> -29 </td>
      <td align="right"> 0 </td>
      <td align="left"> EM65 </td>
      <td align="right"> 0.2 </td>
      <td align="left"> DK7FC/P </td>
      <td align="left"> JN49ik </td>
      <td align="right"> 7470 </td>
      <td align="right"> 45 </td>
    </tr>
  </tbody>
</table>
<br>
The band still seems to be open for DX.<br>
<br>
73, Stefan<br>
</body>
</html>

--------------070908020005030203040103--

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From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hi Dimitris, Am 04.02.2019 06:54, schrieb Dimitrios Tsifakis:
    > [...] and pity you are not > closer otherwise [...] Indeed. Otherwise we
    could do some VLF experiments together, maybe in that desert close to the
    se [...] 
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Hi Dimitris,

Am 04.02.2019 06:54, schrieb Dimitrios Tsifakis:
> [...] and pity you are not
> closer otherwise [...]
Indeed. Otherwise we could do some VLF experiments together, maybe in 
that desert close to the sea: 
https://www.youtube.com/watch?v=XfR9iY5y94s :-)


Am 05.02.2019 01:16, schrieb Dimitrios Tsifakis:
> Hi Stefan,
>
> I am working on both making a portable VLF magnetic field antenna
> (tuned) and a transmit antenna which perhaps will be better than the
> existing 120 m by 3 m (average height) loop. The resistance of this
> loop isn't stellar (about 11 ohm DCR) and half of it is aluminium
> welding wire. Anyway, it's there and it is my reference antenna.
It could be a good RX antenna for VLF. Did you try to connect a 
soundcard of a notebook and record something or produce a spectrogram?
You know there is Edgar from Tasmania, most probably already following 
the conversation and hoping to receive something of you :-)

>   The
> new loop antenna will be better but it is still under construction.
> Heavy copper cabling is surprisingly difficult to put up in the air
> with limited resources. Anyway, once all that is in place, I will do
> some local tests (without rubidium or GPS locked oscillators) and
> we'll take it from there. My QTH locator is QF44OX (very close to
> QF44nx). I have plenty of space but it's undulating and kangaroos
> always make a mess with low hanging wires!
>    
Wow, exciting! So the RX is in QF44OX and the TX is in QF44NX?
If you have plenty of space, it may be easier to improve the ERP by 
building a larger loop out of thin wire instead of a 'small' one out of 
heavy wire. Maybe you can even bury the wire to avoid collisions with 
kangaroos.

> Is there a web page with your 8270 Hz experiments? I'd love to read up
> a bit of inspiring material of what others have achieved as it can be
> quite lonely doing experiments like that where I am. How much radiated
> power have you achieved?
>    
I must admit that i do not have my own homepage with up to date overview 
of my VLF experiments. There is a list maintained by Paul Nicholson 
giving an impression of what has been done lately on VLF/ULF: 
http://abelian.org/vlf/amateur-radio/
A web page of these experiments would be very large and you could read 
for hours. But i'm rather lazy writing it up, unfortunately. I'm rather 
the one who puts time into winding coils!!! ;-)
Actually the whole story of all experiments is spread over the emails of 
this reflector.

Your next well prepared VLF RX station is Edgar J.T. in QE37PD, see 
http://k7fry.com/grid/?qth=QF44OX&from=QE37PD
With a well prepared loop, it is not unlikely at all to leave a trace on 
his site! The distance is just like the distance between me and Paul 
Nicholson.

But at the moment you are doing some first steps and there are some more 
to be done until you reach that distance. But it is really doable!
At the transmitter site, do you have electricity or do you transmit from 
batteries?
What is the power level?
Can you (temporarely) lay out a wire from here to there: 
http://k7fry.com/grid/?qth=QF44NX86FC&from=QF44NX73XQ :-) This is a good 
length and if configured to a loop, it would point perfectly towards 
Edgar. A simple loudspeaker cable of 0.75mm2 would be fine. And you will 
need some ground rods at the ends.

Sorry, that was maybe a bit much of input :-)
What do you think?

73, Stefan



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 Content preview:  Hi Stefan, MF, the grabber resurrects after the winter rest
    ;-) compliments for good performance.I'm still running 24/24 WSPR beacon
   on MF since almost 3 months without interruptions (only exception s [...] 
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------=_Part_1255_18547744.1549363371769
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Hi Stefan, MF,
the grabber resurrects after the winter rest ;-) compliments for good performance.I'm still running 24/24 WSPR beacon on MF since almost 3 months without interruptions (only exception sometime the windows 10 strike ;-) ) it is a relative low power beacon that anyway was heard sometime beyond the pond but since about a week I had no reports neither from TF3GZ nor from W or VE station.. last night also the reports from EA8 were missing...It is hard to state if it is due to propagation, environment (my location is close to Alps and I remember troubles both TX and RX on 160m ) or maybe speaking of SNR the noise level is higher than one week ago making my sigs not decodable..Anyway it is fun keep such a beacon in function and see what happens
Marco, IK1HSS



----Messaggio originale----

Da: selberdenken@posteo.de

Data: 5-feb-2019 9.25

A: <rsgb_lf_group@blacksheep.org>

Ogg: LF: MF WSPR







MF, 



Since yesterday, there is some sun in Heidelberg and my tree grabber
came back. MF reception is possible again (the VLF E field still has a
problem).

http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_Grabber.html



Last night i got my best RX distance on MF ever (i think):




  
    
      Timestamp
      Call
      MHz
      SNR
      Drift
      Grid
      Pwr
      Reporter
      RGrid
      km
      az
    
    
       2019-02-05 06:12 
       WA4SZE 
       0.475703 
       -29 
       0 
       EM65 
       0.2 
       DK7FC/P 
       JN49ik 
       7470 
       45 
    
  



The band still seems to be open for DX.



73, Stefan








------=_Part_1255_18547744.1549363371769
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: 7bit

<div>Hi Stefan, MF,</div><div><br></div><div>the grabber resurrects after the winter rest ;-) compliments for good performance.</div><div>I'm still running 24/24 WSPR beacon on MF since almost 3 months without interruptions (only exception sometime the windows 10 strike ;-) ) it is a relative low power beacon that anyway was heard sometime beyond the pond but since about a week I had no reports neither from TF3GZ nor from W or VE station.. last night also the reports from EA8 were missing...</div><div>It is hard to state if it is due to propagation, environment (my location is close to Alps and I remember troubles both TX and RX on 160m ) or maybe speaking of SNR the noise level is higher than one week ago making my sigs not decodable..</div><div>Anyway it is fun keep such a beacon in function and see what happens</div><div><br></div><div>Marco, IK1HSS<br></div>
<br>
----Messaggio originale----<br>
Da: selberdenken@posteo.de<br>
Data: 5-feb-2019 9.25<br>
A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Ogg: LF: MF WSPR<br>
<br>


<!--
  
-->

MF, <br>
<br>
Since yesterday, there is some sun in Heidelberg and my tree grabber
came back. MF reception is possible again (the VLF E field still has a
problem).<br>
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_Grabber.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_Grabber.html</a><br>
<br>
Last night i got my best RX distance on MF ever (i think):<br>
<br>
<table>
  <tbody>
    <tr>
      <th>Timestamp</th>
      <th>Call</th>
      <th>MHz</th>
      <th>SNR</th>
      <th>Drift</th>
      <th>Grid</th>
      <th>Pwr</th>
      <th>Reporter</th>
      <th>RGrid</th>
      <th>km</th>
      <th>az</th>
    </tr>
    <tr>
      <td align="right">&nbsp;2019-02-05 06:12&nbsp;</td>
      <td align="left">&nbsp;WA4SZE&nbsp;</td>
      <td align="right">&nbsp;0.475703&nbsp;</td>
      <td align="right">&nbsp;-29&nbsp;</td>
      <td align="right">&nbsp;0&nbsp;</td>
      <td align="left">&nbsp;EM65&nbsp;</td>
      <td align="right">&nbsp;0.2&nbsp;</td>
      <td align="left">&nbsp;DK7FC/P&nbsp;</td>
      <td align="left">&nbsp;JN49ik&nbsp;</td>
      <td align="right">&nbsp;7470&nbsp;</td>
      <td align="right">&nbsp;45&nbsp;</td>
    </tr>
  </tbody>
</table>
<br>
The band still seems to be open for DX.<br>
<br>
73, Stefan<br>


<br>
<br>

------=_Part_1255_18547744.1549363371769--


From owner-rsgb_lf_group@blacksheep.org  Tue Feb  5 12:39:54 2019
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From: "Roelof Bakker" <roelof@ndb.demon.nl>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 05 Feb 2019 12:35:03 +0100
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 Content preview:  Hello Marco, Your observations agree with what I found in
   regard to reception of T/A NDB's. Except for Puerto Rico, reception is very
    poor and northern Canada has been absent as well. On NAVTEX 518 kHz the most
    consistant T/A station has been Miami. 
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Hello Marco,

Your observations agree with what I found in regard to reception of T/A NDB's.
Except for Puerto Rico, reception is very poor and northern Canada has been absent as well.

On NAVTEX 518 kHz the most consistant T/A station has been Miami.

So, yes it is propagation to blame!

73,
Roelof, pa0rdt

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 Content preview:  Hello Roelof, thanks for the feeback! so I have not to plan
    a QTH change ;-) In case will plan to move close to the seaside in a warm
    area thus can enjoy both ham radio and diving :-))) 73, Marco IK1H [...] 
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Hello Roelof,
thanks for the feeback! so I have not to plan a QTH change ;-)
In case will plan to move close to the seaside in a warm area thus can enjoy both ham radio and diving :-)))
73, Marco IK1HSS



----Messaggio originale----
Da: roelof@ndb.demon.nl
Data: 5-feb-2019 12.35
A: <rsgb_lf_group@blacksheep.org>
Ogg: Re: R: LF: MF WSPR

Hello Marco,

Your observations agree with what I found in regard to reception of T/A NDB's.
Except for Puerto Rico, reception is very poor and northern Canada has been absent as well.

On NAVTEX 518 kHz the most consistant T/A station has been Miami.

So, yes it is propagation to blame!

73,
Roelof, pa0rdt





------=_Part_43644_19947591.1549366956289
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<div>Hello Roelof,</div><div><br></div><div>thanks for the feeback! so I have not to plan a QTH change ;-)</div><div><br></div><div>In case will plan to move close to the seaside in a warm area thus can enjoy both ham radio and diving :-)))</div><div><br></div><div>73, Marco IK1HSS<br></div>
<br>
----Messaggio originale----<br>Da: roelof@ndb.demon.nl<br>Data: 5-feb-2019 12.35<br>A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>Ogg: Re: R: LF: MF WSPR<br><br>Hello Marco,<br><br>Your observations agree with what I found in regard to reception of T/A NDB's.<br>Except for Puerto Rico, reception is very poor and northern Canada has been absent as well.<br><br>On NAVTEX 518 kHz the most consistant T/A station has been Miami.<br><br>So, yes it is propagation to blame!<br><br>73,<br>Roelof, pa0rdt<br><br><br><br>

------=_Part_43644_19947591.1549366956289--


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Hi Dimitris and Stefan,

Receiver is ready when you are.

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 Content preview:  Hell Markus, LF, While walking to the tree today (which takes
    at about 30 minutes, you know) i had a thought/idea how the double shift
   keying for WSPR could be made: Let's assume the frequency (audio) is known
    to +- 2 [...] 
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Subject: Re: LF: Naive WSPR15 question
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Hell Markus, LF,

While walking to the tree today (which takes at about 30 minutes, you 
know) i had a thought/idea how the double shift keying for WSPR could be 
made:
Let's assume the frequency (audio) is known to +- 200 mHz maybe, let's 
say 1500 Hz. Then, would it be possible to use a SpecLab instance and 
measure the frequency arround 1500+-3 Hz which has the highest signal 
level? This way one could identify which of the 4 FSK frequencies is 
getting out of the WSPR software in that moment. Then, could we say, 
using the conditional actions, if frequency is higher than x and lower 
than y, that this is identified as '2' (1, 2, 3, 4). And then, if '2' is 
identified, use the signal generator and transmit on another frequency, 
which is then at twice the shift frequency from the center. All in all, 
just 4 lines in the conditional actions window (maybe adding a minimum 
signal level is required also to give a 'true').
So, determine the input frequency and generate another one using the 
internal signal generator?
This must be a fast running spectrogram / FFT, to be fast enough but it 
should be no problem. There must be no significant drift of the TX 
though but that could be possible too.
I expressed myselfe a bit difficult but i guess you know what i mean. 
But i try to make it a bot more clear (for me too ;-) ):
 From the file 'wsptones.txt' i got the information that
0= 1497.803 Hz
1= 1499.268 Hz
2= 1500.732 Hz
3= 1502.197 Hz
The difference between 2 steps is 1.465 Hz, obviously.
So, if the detected frequency from the input is higher than 1500 Hz and 
lower than 1501.465 Hz, then this is '2'. And then, the signal generator 
must produce a frequency of 1501.465 Hz instead, which is '2' with twice 
the offset from the center frequency. And so on...
If this output signal is upconvertred by 272 kHz and then sum is divided 
by 2, we should come out at the normal WSPR spacing at 137.5 kHz.
This would then also work without the slow WSPR tool and should also 
work for WSPR-15...

73, Stefan



Am 04.02.2019 22:08, schrieb Markus Vester:
> Hi Stefan, Chris,
>
> in principle yes… (R. Eriwan)
>
> The old tools from 2012 are here
> http://df6nm.bplaced.net/wspr/slowWSPR.zip
> But they used a homemade 16-bit-utility "waitraster" for timing, which 
> is no longer supported by 64-bit Win-7 and Win 10. This can be 
> replaced by simple DOS commands, which has so far been implemented 
> for receiving WSPR-15
> https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg00318.html
> but not yet for transmitting. So a little more work will be needed.
>
> On the other hand, I'm asking myself why so many people still insist 
> on having dividers before their PA's. It only makes life more 
> difficult, and undermines coherent EbNaut or Opera signal transmissions.
>
> Best 73,
> Markus (DF6NM)
>
> -----Ursprüngliche Mitteilung-----
> Von: DK7FC <selberdenken@posteo.de>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Mo, 4. Feb. 2019 21:11
> Betreff: Re: LF: Naive WSPR15 question
>
> ...i checked some files from the slow_WSPR tool. I think i would be able
> to solve the problem. Maybe Markus likes to confirm that this could work
> (getting a factor 2 in the frequency shift)?
> Chris, it would then be worth to try the normal tool first.
>
> 73, Stefan
>
> Am 04.02.2019 20:25, schrieb DK7FC:
> > Hello Chris,
> >
> > For a clever person it is very easy :-)
> > It will depend on which way you want to generate WSPR.
> > Here, for example, i have a Raspi which generates my WSPR (2) for MF.
> > I modified the c source code so that the frequency is 4 times higher
> > and the frequency shift is 4 times higher too. In my PA, probably like
> > in yours, there is a frequency divider using CD4013 ICs which
> > reproduce the desired frequency and frequency shift. Of course this
> > can be done with a factor 2 too.
> > For Windows solutions, there is DF6NMs tool for slow WSPR which works
> > very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be
> > modified for twice the frequency shift but then you will need an
> > upconverter to convert it to LF or MF...
> >
> > 73, Stefan
> >
> > Am 04.02.2019 13:21, schrieb Chris Wilson:
> >>
> >> Hello  LF,
> >>
> >>    A  naive  question  re  WSPR15  please?  Assuming the source code is
> >>    available  how  hard  would  it  be  for  a  clever person to add X2
> >>    functionality to it? Thanks.
> >>
> >
>

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Hell Markus, LF,<br>
<br>
While walking to the tree today (which takes at about 30 minutes, you
know) i had a thought/idea how the double shift keying for WSPR could
be made:<br>
Let's assume the frequency (audio) is known to +- 200 mHz maybe, let's
say 1500 Hz. Then, would it be possible to use a SpecLab instance and
measure the frequency arround 1500+-3 Hz which has the highest signal
level? This way one could identify which of the 4 FSK frequencies is
getting out of the WSPR software in that moment. Then, could we say,
using the conditional actions, if frequency is higher than x and lower
than y, that this is identified as '2' (1, 2, 3, 4). And then, if '2'
is identified, use the signal generator and transmit on another
frequency, which is then at twice the shift frequency from the center.
All in all, just 4 lines in the conditional actions window (maybe
adding a minimum signal level is required also to give a 'true').<br>
So, determine the input frequency and generate another one using the
internal signal generator?<br>
This must be a fast running spectrogram / FFT, to be fast enough but it
should be no problem. There must be no significant drift of the TX
though but that could be possible too.<br>
I expressed myselfe a bit difficult but i guess you know what i mean.
But i try to make it a bot more clear (for me too ;-) ):<br>
>From the file 'wsptones.txt' i got the information that <br>
0= 1497.803 Hz<br>
1= 1499.268 Hz<br>
2= 1500.732 Hz<br>
3= 1502.197 Hz<br>
The difference between 2 steps is 1.465 Hz, obviously.<br>
So, if the detected frequency from the input is higher than 1500 Hz and
lower than 1501.465 Hz, then this is '2'. And then, the signal
generator must produce a frequency of 1501.465 Hz instead, which is '2'
with twice the offset from the center frequency. And so on...<br>
If this output signal is upconvertred by 272 kHz and then sum is
divided by 2, we should come out at the normal WSPR spacing at 137.5
kHz.<br>
This would then also work without the slow WSPR tool and should also
work for WSPR-15...<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 04.02.2019 22:08, schrieb Markus Vester:
<blockquote cite="mid:1615191474.2898208.1549314515047@mail.yahoo.com"
 type="cite">
  <div
 style="font-size: 10pt; font-family: arial,helvetica,sans-serif; color: black;">
  <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;">Hi
Stefan, Chris,<br>
  <br>
in principle yes… (R. Eriwan)<br>
  <br>
The old tools from 2012 are here <br>
<a class="moz-txt-link-freetext" href="http://df6nm.bplaced.net/wspr/slowWSPR.zip">http://df6nm.bplaced.net/wspr/slowWSPR.zip</a> <br>
But they used a homemade 16-bit-utility "waitraster" for timing, which
is no longer supported by 64-bit Win-7 and Win 10. This can be replaced
by simple DOS commands, which has so far been implemented for receiving
WSPR-15<br>
<a class="moz-txt-link-freetext" href="https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg00318.html">https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg00318.html</a><br>
but not yet for transmitting. So a little more work will be needed.<br>
  <br>
On the other hand, I'm asking myself why so many people still insist
on having dividers before their PA's. It only makes life more
difficult, and undermines coherent EbNaut or Opera signal
transmissions. <br>
  <br>
Best 73,<br>
Markus (DF6NM)<br>
  <br>
-----Ursprüngliche Mitteilung-----<br>
Von: DK7FC <a class="moz-txt-link-rfc2396E" href="mailto:selberdenken@posteo.de">&lt;selberdenken@posteo.de&gt;</a><br>
An: rsgb_lf_group <a class="moz-txt-link-rfc2396E" href="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br>
Verschickt: Mo, 4. Feb. 2019 21:11<br>
Betreff: Re: LF: Naive WSPR15 question<br>
  <br>
  </div>
  <div dir="ltr">...i checked some files from the slow_WSPR tool. I
think i would be able <br clear="none">
to solve the problem. Maybe Markus likes to confirm that this could
work <br clear="none">
(getting a factor 2 in the frequency shift)?<br clear="none">
Chris, it would then be worth to try the normal tool first.<br
 clear="none">
  <br clear="none">
73, Stefan<br clear="none">
  <div class="yqt7610097017" id="yqtfd93454"><br clear="none">
Am 04.02.2019 20:25, schrieb DK7FC:<br clear="none">
&gt; Hello Chris,<br clear="none">
&gt;<br clear="none">
&gt; For a clever person it is very easy :-)<br clear="none">
&gt; It will depend on which way you want to generate WSPR.<br
 clear="none">
&gt; Here, for example, i have a Raspi which generates my WSPR (2) for
MF. <br clear="none">
&gt; I modified the c source code so that the frequency is 4 times
higher <br clear="none">
&gt; and the frequency shift is 4 times higher too. In my PA, probably
like <br clear="none">
&gt; in yours, there is a frequency divider using CD4013 ICs which <br
 clear="none">
&gt; reproduce the desired frequency and frequency shift. Of course
this <br clear="none">
&gt; can be done with a factor 2 too.<br clear="none">
&gt; For Windows solutions, there is DF6NMs tool for slow WSPR which
works <br clear="none">
&gt; very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be <br
 clear="none">
&gt; modified for twice the frequency shift but then you will need an <br
 clear="none">
&gt; upconverter to convert it to LF or MF...<br clear="none">
&gt;<br clear="none">
&gt; 73, Stefan<br clear="none">
&gt;<br clear="none">
&gt; Am 04.02.2019 13:21, schrieb Chris Wilson:<br clear="none">
&gt;&gt;<br clear="none">
&gt;&gt; Hello  LF,<br clear="none">
&gt;&gt;<br clear="none">
&gt;&gt;    A  naive  question  re  WSPR15  please?  Assuming the
source code is<br clear="none">
&gt;&gt;    available  how  hard  would  it  be  for  a  clever person
to add X2<br clear="none">
&gt;&gt;    functionality to it? Thanks.<br clear="none">
&gt;&gt;<br clear="none">
&gt;<br clear="none">
  <br clear="none">
  </div>
  </div>
  </div>
</blockquote>
</body>
</html>

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Wed, 6 Feb 2019 07:14:45 +1100
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 Content preview:  G'day Stefan and Edgar, My house is on QF44OX00OR and the
   property extends to QF44NX (50 acres or 200,000 m^2). I do have permission
    from some neighbours to lay wires into their properties, so an extra large
    (over 1km) groun [...] 
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G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed. I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started. I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen. I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!

Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list. You are clearly not lazy having achieved so
much on MF and below :-)

I have played with ground loops before and had some good results in
LF. Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.

73, Dimitris VK2COW

Στις Τρί, 5 Φεβ 2019 στις 8:09 μ.μ., ο/η DK7FC <selberdenken@posteo.de> έγραψε:
>
> Hi Dimitris,
>
> Am 04.02.2019 06:54, schrieb Dimitrios Tsifakis:
> > [...] and pity you are not
> > closer otherwise [...]
> Indeed. Otherwise we could do some VLF experiments together, maybe in
> that desert close to the sea:
> https://www.youtube.com/watch?v=XfR9iY5y94s :-)
>
>
> Am 05.02.2019 01:16, schrieb Dimitrios Tsifakis:
> > Hi Stefan,
> >
> > I am working on both making a portable VLF magnetic field antenna
> > (tuned) and a transmit antenna which perhaps will be better than the
> > existing 120 m by 3 m (average height) loop. The resistance of this
> > loop isn't stellar (about 11 ohm DCR) and half of it is aluminium
> > welding wire. Anyway, it's there and it is my reference antenna.
> It could be a good RX antenna for VLF. Did you try to connect a
> soundcard of a notebook and record something or produce a spectrogram?
> You know there is Edgar from Tasmania, most probably already following
> the conversation and hoping to receive something of you :-)
>
> >   The
> > new loop antenna will be better but it is still under construction.
> > Heavy copper cabling is surprisingly difficult to put up in the air
> > with limited resources. Anyway, once all that is in place, I will do
> > some local tests (without rubidium or GPS locked oscillators) and
> > we'll take it from there. My QTH locator is QF44OX (very close to
> > QF44nx). I have plenty of space but it's undulating and kangaroos
> > always make a mess with low hanging wires!
> >
> Wow, exciting! So the RX is in QF44OX and the TX is in QF44NX?
> If you have plenty of space, it may be easier to improve the ERP by
> building a larger loop out of thin wire instead of a 'small' one out of
> heavy wire. Maybe you can even bury the wire to avoid collisions with
> kangaroos.
>
> > Is there a web page with your 8270 Hz experiments? I'd love to read up
> > a bit of inspiring material of what others have achieved as it can be
> > quite lonely doing experiments like that where I am. How much radiated
> > power have you achieved?
> >
> I must admit that i do not have my own homepage with up to date overview
> of my VLF experiments. There is a list maintained by Paul Nicholson
> giving an impression of what has been done lately on VLF/ULF:
> http://abelian.org/vlf/amateur-radio/
> A web page of these experiments would be very large and you could read
> for hours. But i'm rather lazy writing it up, unfortunately. I'm rather
> the one who puts time into winding coils!!! ;-)
> Actually the whole story of all experiments is spread over the emails of
> this reflector.
>
> Your next well prepared VLF RX station is Edgar J.T. in QE37PD, see
> http://k7fry.com/grid/?qth=QF44OX&from=QE37PD
> With a well prepared loop, it is not unlikely at all to leave a trace on
> his site! The distance is just like the distance between me and Paul
> Nicholson.
>
> But at the moment you are doing some first steps and there are some more
> to be done until you reach that distance. But it is really doable!
> At the transmitter site, do you have electricity or do you transmit from
> batteries?
> What is the power level?
> Can you (temporarely) lay out a wire from here to there:
> http://k7fry.com/grid/?qth=QF44NX86FC&from=QF44NX73XQ :-) This is a good
> length and if configured to a loop, it would point perfectly towards
> Edgar. A simple loudspeaker cable of 0.75mm2 would be fine. And you will
> need some ground rods at the ends.
>
> Sorry, that was maybe a bit much of input :-)
> What do you think?
>
> 73, Stefan
>
>
>


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 Content preview:  If you want to use SpecLab as a frequency doubler, you could
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Subject: Re: LF: Naive WSPR15 question
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If you want to use SpecLab as a frequency doubler, you could simply employ =
the "amplitude demodulator"=C2=A0e.g. in the L1-L2 blackbox.=C2=A0With high=
 enough output bandwidth (> 5000 Hz), it acts as a full-wave rectifier, pro=
ducing=C2=A0DC, 2xf and=C2=A0higher even-numbered harmonics. These can then=
 be filtered by a bandpass filter around 2xf, and=C2=A0also=C2=A0frequency =
shifted=C2=A0before or after doubling.

BTW I have=C2=A0employed this scheme to frequency-double=C2=A0the MSK-signa=
l=C2=A0from NWC, producing a pair of spectral lines whose=C2=A0absolute=C2=
=A0phase is=C2=A0plotted on the DL0AO VLF-grabber.

Best 73,
Markus (DF6NM)

-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Di, 5. Feb. 2019 21:06
Betreff: Re: LF: Naive WSPR15 question

Hell Markus, LF,

While walking to the tree today (which takes at about 30 minutes, youknow) =
i had a thought/idea how the double shift keying for WSPR couldbe made:
Let's assume the frequency (audio) is known to +- 200 mHz maybe, let'ssay 1=
500 Hz. Then, would it be possible to use a SpecLab instance andmeasure the=
 frequency arround 1500+-3 Hz which has the highest signallevel? This way o=
ne could identify which of the 4 FSK frequencies isgetting out of the WSPR =
software in that moment. Then, could we say,using the conditional actions, =
if frequency is higher than x and lowerthan y, that this is identified as '=
2' (1, 2, 3, 4). And then, if '2'is identified, use the signal generator an=
d transmit on anotherfrequency, which is then at twice the shift frequency =
from the center.All in all, just 4 lines in the conditional actions window =
(maybeadding a minimum signal level is required also to give a 'true').
So, determine the input frequency and generate another one using theinterna=
l signal generator?
This must be a fast running spectrogram / FFT, to be fast enough but itshou=
ld be no problem. There must be no significant drift of the TXthough but th=
at could be possible too.
I expressed myselfe a bit difficult but i guess you know what i mean.But i =
try to make it a bot more clear (for me too ;-) ):
>From the file 'wsptones.txt' i got the information that=20
0=3D 1497.803 Hz
1=3D 1499.268 Hz
2=3D 1500.732 Hz
3=3D 1502.197 Hz
The difference between 2 steps is 1.465 Hz, obviously.
So, if the detected frequency from the input is higher than 1500 Hz andlowe=
r than 1501.465 Hz, then this is '2'. And then, the signalgenerator must pr=
oduce a frequency of 1501.465 Hz instead, which is '2'with twice the offset=
 from the center frequency. And so on...
If this output signal is upconvertred by 272 kHz and then sum isdivided by =
2, we should come out at the normal WSPR spacing at 137.5kHz.
This would then also work without the slow WSPR tool and should alsowork fo=
r WSPR-15...

73, Stefan



Am 04.02.2019 22:08, schrieb Markus Vester:
  HiStefan, Chris,
=20
in principle yes=E2=80=A6 (R. Eriwan)
=20
The old tools from 2012 are here=C2=A0
http://df6nm.bplaced.net/wspr/slowWSPR.zip=20
But they used a homemade=C2=A016-bit-utility "waitraster" for timing, which=
is no longer supported by 64-bit Win-7 and Win 10. This=C2=A0can be replace=
dby simple DOS commands, which=C2=A0has so far been implemented for=C2=A0re=
ceivingWSPR-15
https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg0031=
8.html
but not yet for transmitting.=C2=A0So a little more work=C2=A0will be neede=
d.
=20
On the other hand, I'm asking myself=C2=A0why=C2=A0so many people=C2=A0stil=
l insiston=C2=A0having=C2=A0dividers before their PA's.=C2=A0It only makes =
life moredifficult, and=C2=A0undermines coherent=C2=A0EbNaut or Opera signa=
ltransmissions.=C2=A0
=20
Best 73,
Markus (DF6NM)
=20
-----Urspr=C3=BCngliche Mitteilung-----
Von: DK7FC <selberdenken@posteo.de>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Mo, 4. Feb. 2019 21:11
Betreff: Re: LF: Naive WSPR15 question
=20
  ...i checked some files from the slow_WSPR tool. Ithink i would be able=
=20
to solve the problem. Maybe Markus likes to confirm that this couldwork=20
(getting a factor 2 in the frequency shift)?
Chris, it would then be worth to try the normal tool first.
=20
73, Stefan
=20
Am 04.02.2019 20:25, schrieb DK7FC:
> Hello Chris,
>
> For a clever person it is very easy :-)
> It will depend on which way you want to generate WSPR.
> Here, for example, i have a Raspi which generates my WSPR (2) forMF.=20
> I modified the c source code so that the frequency is 4 timeshigher=20
> and the frequency shift is 4 times higher too. In my PA, probablylike=20
> in yours, there is a frequency divider using CD4013 ICs which=20
> reproduce the desired frequency and frequency shift. Of coursethis=20
> can be done with a factor 2 too.
> For Windows solutions, there is DF6NMs tool for slow WSPR whichworks=20
> very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be=20
> modified for twice the frequency shift but then you will need an=20
> upconverter to convert it to LF or MF...
>
> 73, Stefan
>
> Am 04.02.2019 13:21, schrieb Chris Wilson:
>>
>> Hello=C2=A0 LF,
>>
>>=C2=A0 =C2=A0 A=C2=A0 naive=C2=A0 question=C2=A0 re=C2=A0 WSPR15=C2=A0 pl=
ease?=C2=A0 Assuming thesource code is
>>=C2=A0 =C2=A0 available=C2=A0 how=C2=A0 hard=C2=A0 would=C2=A0 it=C2=A0 b=
e=C2=A0 for=C2=A0 a=C2=A0 clever personto add X2
>>=C2=A0 =C2=A0 functionality to it? Thanks.
>>
>
=20
  =20

------=_Part_3607993_1701696998.1549406541236
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"151">If you want to use SpecLab as a frequency do=
ubler, you could simply employ the "amplitude demodulator"&nbsp;e.g. in the=
 L1-L2 blackbox.&nbsp;With high enough output bandwidth (&gt; 5000 Hz), it =
acts as a full-wave rectifier, producing&nbsp;DC, 2xf and&nbsp;higher even-=
numbered harmonics. These can then be filtered by a bandpass filter around =
2xf, and&nbsp;also&nbsp;frequency shifted&nbsp;before or after doubling.<br=
><br>BTW I have&nbsp;employed this scheme to frequency-double&nbsp;the MSK-=
signal&nbsp;from NWC, producing a pair of spectral lines whose&nbsp;absolut=
e&nbsp;phase is&nbsp;plotted on the DL0AO VLF-grabber.<br abp=3D"152"><br>B=
est 73,<br>Markus (DF6NM)<br abp=3D"153"><br abp=3D"154">-----Urspr=C3=BCng=
liche Mitteilung-----<br abp=3D"155">Von: DK7FC &lt;selberdenken@posteo.de&=
gt;<br abp=3D"156">An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<b=
r abp=3D"157">Verschickt: Di, 5. Feb. 2019 21:06<br abp=3D"158">Betreff: Re=
: LF: Naive WSPR15 question<br abp=3D"159"><br abp=3D"160"></div><div id=3D=
"yiv3605804817" abp=3D"161"><div abp=3D"162">
Hell Markus, LF,<br clear=3D"none" abp=3D"163">
<br clear=3D"none" abp=3D"164">
While walking to the tree today (which takes at about 30 minutes, you
know) i had a thought/idea how the double shift keying for WSPR could
be made:<br clear=3D"none" abp=3D"165">
Let's assume the frequency (audio) is known to +- 200 mHz maybe, let's
say 1500 Hz. Then, would it be possible to use a SpecLab instance and
measure the frequency arround 1500+-3 Hz which has the highest signal
level? This way one could identify which of the 4 FSK frequencies is
getting out of the WSPR software in that moment. Then, could we say,
using the conditional actions, if frequency is higher than x and lower
than y, that this is identified as '2' (1, 2, 3, 4). And then, if '2'
is identified, use the signal generator and transmit on another
frequency, which is then at twice the shift frequency from the center.
All in all, just 4 lines in the conditional actions window (maybe
adding a minimum signal level is required also to give a 'true').<br clear=
=3D"none" abp=3D"166">
So, determine the input frequency and generate another one using the
internal signal generator?<br clear=3D"none" abp=3D"167">
This must be a fast running spectrogram / FFT, to be fast enough but it
should be no problem. There must be no significant drift of the TX
though but that could be possible too.<br clear=3D"none" abp=3D"168">
I expressed myselfe a bit difficult but i guess you know what i mean.
But i try to make it a bot more clear (for me too ;-) ):<br clear=3D"none" =
abp=3D"169">
>From the file 'wsptones.txt' i got the information that <br clear=3D"none" =
abp=3D"170">
0=3D 1497.803 Hz<br clear=3D"none" abp=3D"171">
1=3D 1499.268 Hz<br clear=3D"none" abp=3D"172">
2=3D 1500.732 Hz<br clear=3D"none" abp=3D"173">
3=3D 1502.197 Hz<br clear=3D"none" abp=3D"174">
The difference between 2 steps is 1.465 Hz, obviously.<br clear=3D"none" ab=
p=3D"175">
So, if the detected frequency from the input is higher than 1500 Hz and
lower than 1501.465 Hz, then this is '2'. And then, the signal
generator must produce a frequency of 1501.465 Hz instead, which is '2'
with twice the offset from the center frequency. And so on...<br clear=3D"n=
one" abp=3D"176">
If this output signal is upconvertred by 272 kHz and then sum is
divided by 2, we should come out at the normal WSPR spacing at 137.5
kHz.<br clear=3D"none" abp=3D"177">
This would then also work without the slow WSPR tool and should also
work for WSPR-15...<br clear=3D"none" abp=3D"178">
<br clear=3D"none" abp=3D"179">
73, Stefan<br clear=3D"none" abp=3D"180">
<br clear=3D"none" abp=3D"181">
<br clear=3D"none" abp=3D"182">
<br clear=3D"none" abp=3D"183">
Am 04.02.2019 22:08, schrieb Markus Vester:
<div class=3D"yiv3605804817yqt1216174375" id=3D"yiv3605804817yqt32627" abp=
=3D"184"><blockquote abp=3D"185" type=3D"cite">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;" abp=3D"186">
  <div style=3D"color: black; font-family: arial, helvetica, sans-serif; fo=
nt-size: 10pt;" abp=3D"187">Hi
Stefan, Chris,<br clear=3D"none" abp=3D"188">
  <br clear=3D"none" abp=3D"189">
in principle yes=E2=80=A6 (R. Eriwan)<br clear=3D"none" abp=3D"190">
  <br clear=3D"none" abp=3D"191">
The old tools from 2012 are here&nbsp;<br clear=3D"none" abp=3D"192">
<a class=3D"yiv3605804817moz-txt-link-freetext" href=3D"http://df6nm.bplace=
d.net/wspr/slowWSPR.zip" target=3D"_blank" rel=3D"noopener noreferrer" shap=
e=3D"rect" abp=3D"193">http://df6nm.bplaced.net/wspr/slowWSPR.zip</a> <br c=
lear=3D"none" abp=3D"194">
But they used a homemade&nbsp;16-bit-utility "waitraster" for timing, which
is no longer supported by 64-bit Win-7 and Win 10. This&nbsp;can be replace=
d
by simple DOS commands, which&nbsp;has so far been implemented for&nbsp;rec=
eiving
WSPR-15<br clear=3D"none" abp=3D"195">
<a class=3D"yiv3605804817moz-txt-link-freetext" href=3D"https://klubnl.pl/r=
sgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg00318.html" target=3D"_=
blank" rel=3D"noopener noreferrer" shape=3D"rect" abp=3D"196">https://klubn=
l.pl/rsgb_lf_group-archives/html/rsgb_lf_group/2018-11/msg00318.html</a><br=
 clear=3D"none" abp=3D"197">
but not yet for transmitting.&nbsp;So a little more work&nbsp;will be neede=
d.<br clear=3D"none" abp=3D"198">
  <br clear=3D"none" abp=3D"199">
On the other hand, I'm asking myself&nbsp;why&nbsp;so many people&nbsp;stil=
l insist
on&nbsp;having&nbsp;dividers before their PA's.&nbsp;It only makes life mor=
e
difficult, and&nbsp;undermines coherent&nbsp;EbNaut or Opera signal
transmissions.&nbsp;<br clear=3D"none" abp=3D"200">
  <br clear=3D"none" abp=3D"201">
Best 73,<br clear=3D"none" abp=3D"202">
Markus (DF6NM)<br clear=3D"none" abp=3D"203">
  <br clear=3D"none" abp=3D"204">
-----Urspr=C3=BCngliche Mitteilung-----<br clear=3D"none" abp=3D"205">
Von: DK7FC <a class=3D"yiv3605804817moz-txt-link-rfc2396E" href=3D"mailto:s=
elberdenken@posteo.de" target=3D"_blank" rel=3D"noopener noreferrer" shape=
=3D"rect" abp=3D"206" ymailto=3D"mailto:selberdenken@posteo.de">&lt;selberd=
enken@posteo.de&gt;</a><br clear=3D"none" abp=3D"207">
An: rsgb_lf_group <a class=3D"yiv3605804817moz-txt-link-rfc2396E" href=3D"m=
ailto:rsgb_lf_group@blacksheep.org" target=3D"_blank" rel=3D"noopener noref=
errer" shape=3D"rect" abp=3D"208" ymailto=3D"mailto:rsgb_lf_group@blackshee=
p.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br clear=3D"none" abp=3D"20=
9">
Verschickt: Mo, 4. Feb. 2019 21:11<br clear=3D"none" abp=3D"210">
Betreff: Re: LF: Naive WSPR15 question<br clear=3D"none" abp=3D"211">
  <br clear=3D"none" abp=3D"212">
  </div>
  <div dir=3D"ltr" abp=3D"213">...i checked some files from the slow_WSPR t=
ool. I
think i would be able <br clear=3D"none" abp=3D"214">
to solve the problem. Maybe Markus likes to confirm that this could
work <br clear=3D"none" abp=3D"215">
(getting a factor 2 in the frequency shift)?<br clear=3D"none" abp=3D"216">
Chris, it would then be worth to try the normal tool first.<br clear=3D"non=
e" abp=3D"217">
  <br clear=3D"none" abp=3D"218">
73, Stefan<br clear=3D"none" abp=3D"219">
  <div class=3D"yiv3605804817yqt7610097017" id=3D"yiv3605804817yqtfd93454" =
abp=3D"220"><br clear=3D"none" abp=3D"221">
Am 04.02.2019 20:25, schrieb DK7FC:<br clear=3D"none" abp=3D"222">
&gt; Hello Chris,<br clear=3D"none" abp=3D"223">
&gt;<br clear=3D"none" abp=3D"224">
&gt; For a clever person it is very easy :-)<br clear=3D"none" abp=3D"225">
&gt; It will depend on which way you want to generate WSPR.<br clear=3D"non=
e" abp=3D"226">
&gt; Here, for example, i have a Raspi which generates my WSPR (2) for
MF. <br clear=3D"none" abp=3D"227">
&gt; I modified the c source code so that the frequency is 4 times
higher <br clear=3D"none" abp=3D"228">
&gt; and the frequency shift is 4 times higher too. In my PA, probably
like <br clear=3D"none" abp=3D"229">
&gt; in yours, there is a frequency divider using CD4013 ICs which <br clea=
r=3D"none" abp=3D"230">
&gt; reproduce the desired frequency and frequency shift. Of course
this <br clear=3D"none" abp=3D"231">
&gt; can be done with a factor 2 too.<br clear=3D"none" abp=3D"232">
&gt; For Windows solutions, there is DF6NMs tool for slow WSPR which
works <br clear=3D"none" abp=3D"233">
&gt; very reliable here, for WSPR-2 and WSPR-15. I'm sure this can be <br c=
lear=3D"none" abp=3D"234">
&gt; modified for twice the frequency shift but then you will need an <br c=
lear=3D"none" abp=3D"235">
&gt; upconverter to convert it to LF or MF...<br clear=3D"none" abp=3D"236"=
>
&gt;<br clear=3D"none" abp=3D"237">
&gt; 73, Stefan<br clear=3D"none" abp=3D"238">
&gt;<br clear=3D"none" abp=3D"239">
&gt; Am 04.02.2019 13:21, schrieb Chris Wilson:<br clear=3D"none" abp=3D"24=
0">
&gt;&gt;<br clear=3D"none" abp=3D"241">
&gt;&gt; Hello&nbsp; LF,<br clear=3D"none" abp=3D"242">
&gt;&gt;<br clear=3D"none" abp=3D"243">
&gt;&gt;&nbsp; &nbsp; A&nbsp; naive&nbsp; question&nbsp; re&nbsp; WSPR15&nb=
sp; please?&nbsp; Assuming the
source code is<br clear=3D"none" abp=3D"244">
&gt;&gt;&nbsp; &nbsp; available&nbsp; how&nbsp; hard&nbsp; would&nbsp; it&n=
bsp; be&nbsp; for&nbsp; a&nbsp; clever person
to add X2<br clear=3D"none" abp=3D"245">
&gt;&gt;&nbsp; &nbsp; functionality to it? Thanks.<br clear=3D"none" abp=3D=
"246">
&gt;&gt;<br clear=3D"none" abp=3D"247">
&gt;<br clear=3D"none" abp=3D"248">
  <br clear=3D"none" abp=3D"249">
  </div>
  </div>
  </div>
</blockquote></div>
</div></div></div>
------=_Part_3607993_1701696998.1549406541236--

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 Content preview:  Dimitris, Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
    > G'day Stefan and Edgar, > > My house is on QF44OX00OR and the property
   extends to QF44NX (50 acres > or 200,000 m^2). I do have permission from some
    [...] 
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Dimitris,

Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
> G'day Stefan and Edgar,
>
> My house is on QF44OX00OR and the property extends to QF44NX (50 acres
> or 200,000 m^2). I do have permission from some neighbours to lay
> wires into their properties, so an extra large (over 1km) ground wire
> is entirely doable but not at this point in time.
Wow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!
Not at this time, ok. I would suggest to start in small steps anyway, 
then you can be happy about many improvements, not just a single big one 
:-)
I often imagine to live in Canada or Australia and do such experiments 
exactly!
> The reference loop
> is from the shed, about 100 metres south of the house, to the tractor
> shed.
100m is very close, the far field begins at about 5.7 km distance at 
8.27 kHz. A RX in that distance is only useful to check and observe the 
signal stability and compare levels. A feedback monitor like my tree 
which is 3.5 km distant from my INV-L antenna in the city. From my 
ground loop antenna in JN39WI it is 57.6 km distant, which is already an 
interesting distance and can be challenging below 3 kHz.

>   I have mains in the shed and I also have a 200 W audio linear
> amplifier to get things started.
Excellent, just excellent! Your signal could be the stongest of the 
radio amateurs! 200W is just fine for the first steps. But be careful 
with those audio amplifiers, they do not seem to like to much reactive 
power.
For tuning the antenna you will only need a capacitor in series. For my 
portable VLF system i built a current transformer to produce a small 
voltage that goes to the soundcard. Then, using SpecLab, i can calculate 
the antenna current directly and even keep the phase of the current 
stable, even if there should be a soundcard glitch. For the signal 
generation i also use SpecLab and a cheap GPS module. It all works very 
reliable, there were no problems so far.
With a house at one of the ends of the antenna you are in a very 
comfortable situation! You may already have a ground system there, so 
the effort is at one end only.

>   I can build a class-E kilowatt if
> necessary later. I like the roughly north-south loop configuration as
> it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
> and most importantly Canberra which is only 30 km to the South. I will
> try to get some signals received in Canberra before I start asking
> people further away to have a listen.
Yes, this is a very good distance to observe your own signal. If you 
have internet access there and can leave a small PC/notebook/tablet ... 
then you could build up a webpage and run a grabber from there like i do 
from my tree (still under maintenance). That would be ideal and it just 
feels good to see the own signal very clearly on a real RX in a short 
distance. You are then independent.


>   I currently have assembled an XO
> clocked DDS controlled by an arduino to do the initial tests but later
> when I decide to go QRSSSSSI can dig out and use the old rubidium
> clock as a reference for extra stability. For receiving I use a 24
> bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
> antenna I will use for receive is one of those monster ferrite rods.
> Amplification may not even be necessary, the signals I get when the
> antenna is tuned seem to be already quite good. Once I have a decent
> RX antenna I think I will start gifting these rods (I have a few) to
> interested amateurs in the region and help them get started with
> receiving on VLF. Make a small army of receivers, that would make life
> much easier when evaluating antennas!
>    
Oh yes! Fortunately there are a few arround here. These days this is 
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, 
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar 
J.T. This is about the complete VLF group worldwide, at least those who 
prooved to detect narrow band (sub mHz) signals close to the limits, in 
the last 3 years until now.

> Hey, you should document your experiments even if it is a summary of
> the activities and nothing more. The list is great but perhaps we are
> missing out on many other potentially interested people that may have
> not discovered the list.
Yes, you are right. I had the same thought sometimes. Certainly there 
are many amateurs who would feel like having a new life when starting at 
VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually it 
is not even amateur radio because it is not a spectrum allocated to 
amateur radio. So everyone could operate there.
But there is a risk, you know. There are those people who do not simply 
start to transmit/receive there and feel good. There are those who 
prefer to ask if this is legal at all. And then they ask here and there, 
as long as they find someone who triggers their fears and phobs, and 
then they do nothing at all! Beware of such people, they are 
contaminating your free mind. Concentrate on ideas and wishes, like for 
example detecting your own signal in Canberra. And then the question 
"Will this also work on lower frequencies", for example.
When writing an article in a radio magazine, what will be the result? 
Will it actually lead to more _active_ people on the band, who transmit 
and/or receive_ for a longer time, say at least 5 to 10 years_? Or will 
it rise a short interest only, dominated by people telling it is not 
legal and so on... I'm not sure about that. It could be even better to 
stay in a smaller group who can do what it wants instead causing a 
decision / regulation by an 'authority'.

>   You are clearly not lazy having achieved so
> much on MF and below :-)
>    
Thanks but i'm lazy into a certain spectrum. On the other side, there 
are people who write many articles over the years but it is simply 
impossible for them to even imagine to wind a coil which has more than 
100 turns. Maybe it is good that there is a variety of people, the 
article writers and the coil winders and something inbetween :-) Oh, and 
the programmers! Very important. Without Wolfgang and Paul and Markus we 
would do nothing at all!
Oh BTW maybe i'll transmit on my loop again the next weekend. I can't 
await it, it is more than 2 weeks ago, a very long time!!

> I have played with ground loops before and had some good results in
> LF.
On VLF it should work much better (relative to a vertical E field 
antenna). The idea is that the current runs back in a deep layer (skin 
depth), depending on the ground conductivity. So it should work better 
on poor conducting ground.
>   Once I establish a reference system, I can compare antennas
> including ground loops. Unlike Europe where you have plenty of people
> around you, I have to do both the TXing and the RXing and that
> requires effort and time. The latter is a very scarce resource!
>
> Anyway, looks like a nice day today to do some more outdoor work. We
> had lightning storms and plenty of rain the past few days, so I
> haven't made any progress.
>    
RR, good luck and fun with the new challenges.
Looking forward to your next steps and reports.

73, Stefan



> 73, Dimitris VK2COW
>

--------------040508070400010208040207
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 7bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
Dimitris, <br>
<br>
Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap="">G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. </pre>
</blockquote>
Wow, i'm envious and happy that you have such
possibilities!!!!!!!!!!!!!!<br>
Not at this time, ok. I would suggest to start in small steps anyway,
then you can be happy about many improvements, not just a single big
one :-) <br>
I often imagine to live in Canada or Australia and do such experiments
exactly!<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap="">The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed.</pre>
</blockquote>
100m is very close, the far field begins at about 5.7 km distance at
8.27 kHz. A RX in that distance is only useful to check and observe the
signal stability and compare levels. A feedback monitor like my tree
which is 3.5 km distant from my INV-L antenna in the city. From my
ground loop antenna in JN39WI it is 57.6 km distant, which is already
an interesting distance and can be challenging below 3 kHz.<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap=""> I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started.</pre>
</blockquote>
Excellent, just excellent! Your signal could be the stongest of the
radio amateurs! 200W is just fine for the first steps. But be careful
with those audio amplifiers, they do not seem to like to much reactive
power.<br>
For tuning the antenna you will only need a capacitor in series. For my
portable VLF system i built a current transformer to produce a small
voltage that goes to the soundcard. Then, using SpecLab, i can
calculate the antenna current directly and even keep the phase of the
current stable, even if there should be a soundcard glitch. For the
signal generation i also use SpecLab and a cheap GPS module. It all
works very reliable, there were no problems so far.<br>
With a house at one of the ends of the antenna you are in a very
comfortable situation! You may already have a ground system there, so
the effort is at one end only.<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap=""> I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen.</pre>
</blockquote>
Yes, this is a very good distance to observe your own signal. If you
have internet access there and can leave a small PC/notebook/tablet ...
then you could build up a webpage and run a grabber from there like i
do from my tree (still under maintenance). That would be ideal and it
just feels good to see the own signal very clearly on a real RX in a
short distance. You are then independent.<br>
<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap=""> I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!
  </pre>
</blockquote>
Oh yes! Fortunately there are a few arround here. These days this is
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF,
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar
J.T. This is about the complete VLF group worldwide, at least those who
prooved to detect narrow band (sub mHz) signals close to the limits, in
the last 3 years until now.<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap="">Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list.</pre>
</blockquote>
Yes, you are right. I had the same thought sometimes. Certainly there
are many amateurs who would feel like having a new life when starting
at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually
it is not even amateur radio because it is not a spectrum allocated to
amateur radio. So everyone could operate there.<br>
But there is a risk, you know. There are those people who do not simply
start to transmit/receive there and feel good. There are those who
prefer to ask if this is legal at all. And then they ask here and
there, as long as they find someone who triggers their fears and phobs,
and then they do nothing at all! Beware of such people, they are
contaminating your free mind. Concentrate on ideas and wishes, like for
example detecting your own signal in Canberra. And then the question
"Will this also work on lower frequencies", for example.<br>
When writing an article in a radio magazine, what will be the result?
Will it actually lead to more <u>active</u> people on the band, who
transmit and/or receive<u> for a longer time, say at least 5 to 10 years</u>?
Or will it rise a short interest only, dominated by people telling it
is not legal and so on... I'm not sure about that. It could be even
better to stay in a smaller group who can do what it wants instead
causing a decision / regulation by an 'authority'.<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap=""> You are clearly not lazy having achieved so
much on MF and below :-)
  </pre>
</blockquote>
Thanks but i'm lazy into a certain spectrum. On the other side, there
are people who write many articles over the years but it is simply
impossible for them to even imagine to wind a coil which has more than
100 turns. Maybe it is good that there is a variety of people, the
article writers and the coil winders and something inbetween :-) Oh,
and the programmers! Very important. Without Wolfgang and Paul and
Markus we would do nothing at all!<br>
Oh BTW maybe i'll transmit on my loop again the next weekend. I can't
await it, it is more than 2 weeks ago, a very long time!!<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap="">I have played with ground loops before and had some good results in
LF.</pre>
</blockquote>
On VLF it should work much better (relative to a vertical E field
antenna). The idea is that the current runs back in a deep layer (skin
depth), depending on the ground conductivity. So it should work better
on poor conducting ground.<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap=""> Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.
  </pre>
</blockquote>
RR, good luck and fun with the new challenges. <br>
Looking forward to your next steps and reports.<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
<blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
  <pre wrap="">
73, Dimitris VK2COW</pre>
  <br>
</blockquote>
</body>
</html>

--------------040508070400010208040207--

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Subject: Re: LF: Generating EbNaut from u-blox GPS timepulse - also
 non-integer Hz
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There is now an extension for non-integer Hz frequencies (e.g. 8270.0025 Hz=
):
http://df6nm.bplaced.net/LF/u-blox_ebnaut/setubx2.zip
setubx2 works the same way as setubx did, except that it can take a non-int=
eger frequency as argument.=C2=A0A phase offset is calculated from the=C2=
=A0fractional part of the frequency and the time of day, and it is sent to =
the=C2=A0ublox module as a "user delay".=C2=A0By executing setubx2 periodic=
ally, the phase is slowly advanced,=C2=A0producing the desired fine offset.=
=C2=A0

Absolute phase is referenced to local midnight and maintained over outages =
or restarts. Also setubx2 can simlpy replace setubx=C2=A0in the EbNaut scri=
pts.=C2=A0

Note that the frequency should not be too far from an integer Hz (preferabl=
y closer than +-0.1 Hz), to avoid large phase steps and strong 1 Hz spuriou=
s sidebands.

Best 73,
Markus (DF6NM)

-----Urspr=C3=BCngliche Mitteilung-----
Von: Markus Vester <markusvester@aol.com>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: So, 3. Feb. 2019 19:28
Betreff: LF: Generating EbNaut from u-blox GPS timepulse

Here's a short summary of my recent experiments and conclusions.

LEA-6T hardware:
At around 27 =E2=82=AC, this LEA-6T module is perhaps one of the cheapest s=
olutions with two timing outputs - see
http://www.eevblog.com/forum/projects/ebay-u-blox-lea-6t-gps-module-teardow=
n-and-initial-test/Although the LEA series has been superseded by NEO-7 and=
 -8 with GLONASS and Galileo capabilities, but these tend to be much more e=
xpensive.

My unit arrived within about a week, and started up fine through the includ=
ed USB adapter board. Unfortunately my device did not remember settings aft=
er powerdown, which turned out to be due to a missing flash eeprom chip, an=
d also (believe it or not) a faulty solder joint on backup-battery charging=
 resistor. In fact all the solder joints looked as if they had been hand so=
ldered in a Chinese garage factory, but that's fine with me.
=C2=A0
Then I connected the timepulse outputs through 470 ohm protection resistors=
 and separate coax cables. With 3.3 Vpp behind the resistor we get ~ 1 mW a=
vailable power. However connecting the little ublox module barefoot to the =
antenna produced good carrier traces and successful EbNaut decodes at the D=
L0AO MF-Grabber, 48 km from here. For PA switching, I later employed a simp=
le VOX circuit fed by TP2 output signal.
The frequency can be set at any integer Hz from 1 Hz to 24 MHz. The stepsiz=
e is fine for LF and MF but perhaps inconvenient at VLF where we would rath=
er avoitd integer Hz frequencies. But it may be possible to create small an=
d precise sub-Hz offsets by regularly advancing phase, using the user-delay=
 field. Note that at higher HF frequencies, a noticable degradation of GPS =
sensitivity occured presumably due to interference to the on-board ceramic =
antenna.
EbNaut generation:
The idea for ebnaut is to generate PSK by using ublox commands to change po=
larity of timepulse, minimizing hardware and doing away with audio mixers o=
r external phase switches. I started by monitoring the 40-byte TP5 commands=
 in in the binary message display. Then based on the specificaton on the u-=
blox website,
https://www.u-blox.com/sites/default/files/products/documents/u-blox6_Recei=
verDescrProtSpec_%28GPS.G6-SW-10018%29_Public.pdf
(chapters 23 and 31.24.3), I wrote a small Basic executable setubx.exe whic=
h reads a template and=C2=A0patches the frequency, flag and checksum fields=
. The output can be redirected to the virtual com-port of the USB=C2=A0conn=
ection (e.g. >com6).
Note that any changes are not executed immediately but only at the start th=
e next second. If a command has been issued as early as 1.0 to 0.1 s before=
, the output inversion happens about 50 ms after the next second tick (impl=
ying a negligible 0.05 s extra symbol delay). The advantage is that no subs=
econd timing is required for the issuing of commands, allowing the use of s=
imple DOS timeout or sleep functions. On the other hand, the maximum signal=
ling speed is thus limited to 1 symbol per second.
As mentioned before, I have created a directory for Windows scripts and a f=
ew screenshots, and also this email:
http://df6nm.bplaced.net/LF/u-blox_ebnaut/
To prepare an EbNaut transmission, you'd go through the following steps:
- download and unpack ebnaut_ublox.zip=20
- use Paul's ebnaut-tx.exe and "write lines" to produce a pskln_xxx.txt out=
put file,
- edit the file with notepad to replace "1" by "call 1" (same for 0) and sa=
ve as a .bat file,
- right-click and edit frequency and delay functions in 1.bat and 0.bat=C2=
=A0=C2=A0=20
- edit the send_ebnaut...bat according to your desired transmit schedule.
BTW I did struggle with strange peculiarities in batch scripting... We need=
 to wait until the second before the next of 3-second-multiple, but why thi=
s cryptic notation:
@set /a waittime=3D2-(3%time:~6,2%%%3)
- set /a is for arithmetic calculations for a variable,
- %time:~6,2% provides two digits for the seconds in a minute,
- %% is an expansion of the % modulo operator which is required in a batch =
script,=C2=A0=C2=A0=20
- 3%time:~6,2% expands xx to 3xx, only to avoid 08 or 09 being interpreted =
as an invalid octal numbers.=20
Spectral purity:
Originally I had hoped for relatively low jitter, as little as 21 ns from t=
he 48 MHz clock. But it turned out that on most output frequencies the jitt=
er is really much larger, leading to relatively strong 1 kHz spaced spuriou=
s sidelines. It looks as if frequencies were internally generated on a rela=
tively coarse raster, and then the phase is then being corrected periodical=
ly each millisecond. But some preferred frequencies are much cleaner than o=
thers, specifically
=C2=A0- integer divisors of 48 MHz (well-known and easy to understand),=20
=C2=A0- but also all multiples of 366.2155 Hz. This raster happens to be 48=
000.34 kHz/2^17, so I speculate that this may be a "DDS"-like architecture,=
 clocked by my particular 48 MHz crystal, and outputting the msb of an over=
flowing 17-bit-counter.
When the output frequency is set slightly above one of these sweet spots, t=
he level of 1 kHz sidelines gradually increases. But going only 1 Hz below =
the spot produces a sharp detoriation to the worst levels. For example:
=C2=A0137330 Hz -15 dB, 137331 Hz -54 dB,
=C2=A0137536 Hz =3D 48 MHz/349: -54 dB,
=C2=A0475710 Hz -5 dB(!), 475712 Hz -47 dB.

When sweeping through frequencies, a "sawtooth-like" dependence of spurious=
 levels can be observed (screenshot lea-6t_sweep_474-480.5kHz.png).=20
Hope this may be useful=E2=80=A6
Best 73,
Markus (DF6NM)



------=_Part_3663262_974195683.1549412744351
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"297">There is now an extension for non-integer Hz=
 frequencies (e.g. 8270.0025 Hz):<br>http://df6nm.bplaced.net/LF/u-blox_ebn=
aut/setubx2.zip<br>setubx2 works the same way as setubx did, except that it=
 can take a non-integer frequency as argument.&nbsp;A phase offset is calcu=
lated from the&nbsp;fractional part of the frequency and the time of day, a=
nd it is sent to the&nbsp;ublox module as a "user delay".&nbsp;By executing=
 setubx2 periodically, the phase is slowly advanced,&nbsp;producing the des=
ired fine offset.&nbsp;<br><br>Absolute phase is referenced to local midnig=
ht and maintained over outages or restarts. Also setubx2 can simlpy replace=
 setubx&nbsp;in the EbNaut scripts.&nbsp;<br><br>Note that the frequency sh=
ould not be too far from an integer Hz (preferably closer than +-0.1 Hz), t=
o avoid large phase steps and strong 1 Hz spurious sidebands.<br><br abp=3D=
"298">Best 73,<br>Markus (DF6NM)<br abp=3D"299"><br abp=3D"300">-----Urspr=
=C3=BCngliche Mitteilung-----<br abp=3D"301">Von: Markus Vester &lt;markusv=
ester@aol.com&gt;<br abp=3D"302">An: rsgb_lf_group &lt;rsgb_lf_group@blacks=
heep.org&gt;<br abp=3D"303">Verschickt: So, 3. Feb. 2019 19:28<br abp=3D"30=
4">Betreff: LF: Generating EbNaut from u-blox GPS timepulse<br abp=3D"305">=
<br abp=3D"306"></div><div id=3D"yiv3320327467" abp=3D"307"><div class=3D"y=
iv3320327467yqt0861149263" id=3D"yiv3320327467yqtfd07409" abp=3D"308"><div =
abp=3D"309"><div style=3D"color: black; font-family: arial, helvetica, sans=
-serif; font-size: 10pt;" abp=3D"310"><div style=3D"color: black; font-fami=
ly: arial, helvetica, sans-serif; font-size: 10pt;" abp=3D"311">Here's a sh=
ort summary of my recent experiments and conclusions.<br clear=3D"none" abp=
=3D"312"><br clear=3D"none" abp=3D"313">LEA-6T hardware:<br clear=3D"none" =
abp=3D"314"></div><div id=3D"yiv3320327467" abp=3D"315"><div abp=3D"316"><d=
iv style=3D"color: black; font-family: arial, helvetica, sans-serif; font-s=
ize: 10pt;" abp=3D"317"><div style=3D"color: black; font-family: arial, hel=
vetica, sans-serif; font-size: 10pt;" abp=3D"318">At around 27 =E2=82=AC, t=
his LEA-6T module is perhaps one of the cheapest solutions with two timing =
outputs - see<br clear=3D"none" abp=3D"319">http://www.eevblog.com/forum/pr=
ojects/ebay-u-blox-lea-6t-gps-module-teardown-and-initial-test/</div><div s=
tyle=3D"color: black; font-family: arial, helvetica, sans-serif; font-size:=
 10pt;" abp=3D"320">Although the LEA series has been superseded by NEO-7 an=
d -8 with GLONASS and Galileo capabilities, but these tend to be much more =
expensive.<br clear=3D"none" abp=3D"321"><br clear=3D"none" abp=3D"322">My =
unit arrived within about a week, and started up fine through the included =
USB adapter board. Unfortunately my device did not remember settings after =
powerdown, which turned out to be due to a missing flash eeprom chip, and a=
lso (believe it or not) a faulty solder joint on backup-battery charging re=
sistor. In fact all the solder joints looked as if they had been hand solde=
red in a Chinese garage factory, but that's fine with me.<br clear=3D"none"=
 abp=3D"323">&nbsp;<br clear=3D"none" abp=3D"324">Then I connected the time=
pulse outputs through 470 ohm protection resistors and separate coax cables=
. With 3.3 Vpp behind the resistor we get ~ 1 mW available power. However c=
onnecting the little ublox module barefoot to the antenna produced good car=
rier traces and successful EbNaut decodes at the DL0AO MF-Grabber, 48 km fr=
om here. For PA switching, I later employed a simple VOX circuit fed by TP2=
 output signal.</div><div style=3D"color: black; font-family: arial, helvet=
ica, sans-serif; font-size: 10pt;" abp=3D"325"><br clear=3D"none" abp=3D"32=
6">The frequency can be set at any integer Hz from 1 Hz to 24 MHz. The step=
size is fine for LF and MF but perhaps inconvenient at VLF where we would r=
ather avoitd integer Hz frequencies. But it may be possible to create small=
 and precise sub-Hz offsets by regularly advancing phase, using the user-de=
lay field. Note that at higher HF frequencies, a noticable degradation of G=
PS sensitivity occured presumably due to interference to the on-board ceram=
ic antenna.</div><div style=3D"color: black; font-family: arial, helvetica,=
 sans-serif; font-size: 10pt;" abp=3D"327"><br clear=3D"none" abp=3D"328">E=
bNaut generation:</div><div style=3D"color: black; font-family: arial, helv=
etica, sans-serif; font-size: 10pt;" abp=3D"329"><br clear=3D"none" abp=3D"=
330">The idea for ebnaut is to generate PSK by using ublox commands to chan=
ge polarity of timepulse, minimizing hardware and doing away with audio mix=
ers or external phase switches. I started by monitoring the 40-byte TP5 com=
mands in in the binary message display. Then based on the specificaton on t=
he u-blox website,<br clear=3D"none" abp=3D"331">https://www.u-blox.com/sit=
es/default/files/products/documents/u-blox6_ReceiverDescrProtSpec_%28GPS.G6=
-SW-10018%29_Public.pdf<br clear=3D"none" abp=3D"332">(chapters 23 and 31.2=
4.3), I wrote a small Basic executable setubx.exe which reads a template an=
d&nbsp;patches the frequency, flag and checksum fields. The output can be r=
edirected to the virtual com-port of the USB&nbsp;connection (e.g. &gt;com6=
).</div><div style=3D"color: black; font-family: arial, helvetica, sans-ser=
if; font-size: 10pt;" abp=3D"333"><br clear=3D"none" abp=3D"334">Note that =
any changes are not executed immediately but only at the start the next sec=
ond. If a command has been issued as early as 1.0 to 0.1 s before, the outp=
ut inversion happens about 50 ms after the next second tick (implying a neg=
ligible 0.05 s extra symbol delay). The advantage is that no subsecond timi=
ng is required for the issuing of commands, allowing the use of simple DOS =
timeout or sleep functions. On the other hand, the maximum signalling speed=
 is thus limited to 1 symbol per second.</div><div style=3D"color: black; f=
ont-family: arial, helvetica, sans-serif; font-size: 10pt;" abp=3D"335"><br=
 clear=3D"none" abp=3D"336">As mentioned before, I have created a directory=
 for Windows scripts and a few screenshots, and also this email:<br clear=
=3D"none" abp=3D"337">http://df6nm.bplaced.net/LF/u-blox_ebnaut/</div><div =
style=3D"color: black; font-family: arial, helvetica, sans-serif; font-size=
: 10pt;" abp=3D"338"><br clear=3D"none" abp=3D"339">To prepare an EbNaut tr=
ansmission, you'd go through the following steps:<br clear=3D"none" abp=3D"=
340">- download and unpack ebnaut_ublox.zip <br clear=3D"none" abp=3D"341">=
- use Paul's ebnaut-tx.exe and "write lines" to produce a pskln_xxx.txt out=
put file,<br clear=3D"none" abp=3D"342">- edit the file with notepad to rep=
lace "1" by "call 1" (same for 0) and save as a .bat file,<br clear=3D"none=
" abp=3D"343">- right-click and edit frequency and delay functions in 1.bat=
 and 0.bat&nbsp;&nbsp; <br clear=3D"none" abp=3D"344">- edit the send_ebnau=
t...bat according to your desired transmit schedule.</div><div style=3D"col=
or: black; font-family: arial, helvetica, sans-serif; font-size: 10pt;" abp=
=3D"345"><br clear=3D"none" abp=3D"346">BTW I did struggle with strange pec=
uliarities in batch scripting... We need to wait until the second before th=
e next of 3-second-multiple, but why this cryptic notation:<br clear=3D"non=
e" abp=3D"347">@set /a waittime=3D2-(3%time:~6,2%%%3)<br clear=3D"none" abp=
=3D"348">- set /a is for arithmetic calculations for a variable,<br clear=
=3D"none" abp=3D"349">- %time:~6,2% provides two digits for the seconds in =
a minute,<br clear=3D"none" abp=3D"350">- %% is an expansion of the % modul=
o operator which is required in a batch script,&nbsp;&nbsp; <br clear=3D"no=
ne" abp=3D"351">- 3%time:~6,2% expands xx to 3xx, only to avoid 08 or 09 be=
ing interpreted as an invalid octal numbers. </div><div style=3D"color: bla=
ck; font-family: arial, helvetica, sans-serif; font-size: 10pt;" abp=3D"352=
"><br clear=3D"none" abp=3D"353">Spectral purity:</div><div style=3D"color:=
 black; font-family: arial, helvetica, sans-serif; font-size: 10pt;" abp=3D=
"354"><br clear=3D"none" abp=3D"355">Originally I had hoped for relatively =
low jitter, as little as 21 ns from the 48 MHz clock. But it turned out tha=
t on most output frequencies the jitter is really much larger, leading to r=
elatively strong 1 kHz spaced spurious sidelines. It looks as if frequencie=
s were internally generated on a relatively coarse raster, and then the pha=
se is then being corrected periodically each millisecond. But some preferre=
d frequencies are much cleaner than others, specifically<br clear=3D"none" =
abp=3D"356">&nbsp;- integer divisors of 48 MHz (well-known and easy to unde=
rstand), <br clear=3D"none" abp=3D"357">&nbsp;- but also all multiples of 3=
66.2155 Hz. This raster happens to be 48000.34 kHz/2^17, so I speculate tha=
t this may be a "DDS"-like architecture, clocked by my particular 48 MHz cr=
ystal, and outputting the msb of an overflowing 17-bit-counter.</div><div s=
tyle=3D"color: black; font-family: arial, helvetica, sans-serif; font-size:=
 10pt;" abp=3D"358"><br clear=3D"none" abp=3D"359">When the output frequenc=
y is set slightly above one of these sweet spots, the level of 1 kHz sideli=
nes gradually increases. But going only 1 Hz below the spot produces a shar=
p detoriation to the worst levels. For example:<br clear=3D"none" abp=3D"36=
0">&nbsp;137330 Hz -15 dB, 137331 Hz -54 dB,<br clear=3D"none" abp=3D"361">=
&nbsp;137536 Hz =3D 48 MHz/349: -54 dB,<br clear=3D"none" abp=3D"362">&nbsp=
;475710 Hz -5 dB(!), 475712 Hz -47 dB.<br clear=3D"none" abp=3D"363"><br cl=
ear=3D"none" abp=3D"364">When sweeping through frequencies, a "sawtooth-lik=
e" dependence of spurious levels can be observed (screenshot lea-6t_sweep_4=
74-480.5kHz.png). </div><div style=3D"color: black; font-family: arial, hel=
vetica, sans-serif; font-size: 10pt;" abp=3D"365"><br clear=3D"none" abp=3D=
"366">Hope this may be useful=E2=80=A6</div><div class=3D"yiv3320327467yqt6=
450327648" id=3D"yiv3320327467yqtfd82931" abp=3D"367"><div style=3D"color: =
black; font-family: arial, helvetica, sans-serif; font-size: 10pt;" abp=3D"=
368"><br clear=3D"none" abp=3D"369">Best 73,<br clear=3D"none" abp=3D"370">=
Markus (DF6NM)<br clear=3D"none" abp=3D"371"><br clear=3D"none" abp=3D"372"=
><br clear=3D"none" abp=3D"373"></div></div></div></div></div></div></div><=
/div></div></div>
------=_Part_3663262_974195683.1549412744351--

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 Content preview:  Hi Stefan, Dimitris, room is sure a thing that is not missing
    in VK :-) I remember a vacation I had there some years ago ... a lot of km
    between "adiacent places".. so ideal place for LF, VLF and even close to
   DC frequenc [...] 
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Hi Stefan, Dimitris,

room is sure a thing that is not missing in VK :-)
I remember a vacation I had there some years ago ... a lot of km between "adiacent places".. so ideal place for LF, VLF and even close to DC frequencies!
During my travel, just for fate, I drove close to Holt Navy Base sporting an antenna just a bit larger than your loop ;-)
Anyway you know the grass of the neighbor is more green...
Dimitris has room but not a lot of time..
I have more time but less room
somebody else has room and time but no money...
What an hard life!
But... we all have fun!

73 Marco IK1HSS

P.S. who's looking the legal aspects?? ;-)



----Messaggio originale----

Da: selberdenken@posteo.de

Data: 5-feb-2019 23.40

A: <rsgb_lf_group@blacksheep.org>

Ogg: Re: VLF: in VK?







Dimitris, 



Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:

  G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. 

Wow, i'm envious and happy that you have such
possibilities!!!!!!!!!!!!!!

Not at this time, ok. I would suggest to start in small steps anyway,
then you can be happy about many improvements, not just a single big
one :-) 

I often imagine to live in Canada or Australia and do such experiments
exactly!


  The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed.

100m is very close, the far field begins at about 5.7 km distance at
8.27 kHz. A RX in that distance is only useful to check and observe the
signal stability and compare levels. A feedback monitor like my tree
which is 3.5 km distant from my INV-L antenna in the city. From my
ground loop antenna in JN39WI it is 57.6 km distant, which is already
an interesting distance and can be challenging below 3 kHz.




   I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started.

Excellent, just excellent! Your signal could be the stongest of the
radio amateurs! 200W is just fine for the first steps. But be careful
with those audio amplifiers, they do not seem to like to much reactive
power.

For tuning the antenna you will only need a capacitor in series. For my
portable VLF system i built a current transformer to produce a small
voltage that goes to the soundcard. Then, using SpecLab, i can
calculate the antenna current directly and even keep the phase of the
current stable, even if there should be a soundcard glitch. For the
signal generation i also use SpecLab and a cheap GPS module. It all
works very reliable, there were no problems so far.

With a house at one of the ends of the antenna you are in a very
comfortable situation! You may already have a ground system there, so
the effort is at one end only.




   I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen.

Yes, this is a very good distance to observe your own signal. If you
have internet access there and can leave a small PC/notebook/tablet ...
then you could build up a webpage and run a grabber from there like i
do from my tree (still under maintenance). That would be ideal and it
just feels good to see the own signal very clearly on a real RX in a
short distance. You are then independent.






   I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!
  

Oh yes! Fortunately there are a few arround here. These days this is
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF,
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar
J.T. This is about the complete VLF group worldwide, at least those who
prooved to detect narrow band (sub mHz) signals close to the limits, in
the last 3 years until now.




  Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list.

Yes, you are right. I had the same thought sometimes. Certainly there
are many amateurs who would feel like having a new life when starting
at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually
it is not even amateur radio because it is not a spectrum allocated to
amateur radio. So everyone could operate there.

But there is a risk, you know. There are those people who do not simply
start to transmit/receive there and feel good. There are those who
prefer to ask if this is legal at all. And then they ask here and
there, as long as they find someone who triggers their fears and phobs,
and then they do nothing at all! Beware of such people, they are
contaminating your free mind. Concentrate on ideas and wishes, like for
example detecting your own signal in Canberra. And then the question
"Will this also work on lower frequencies", for example.

When writing an article in a radio magazine, what will be the result?
Will it actually lead to more active people on the band, who
transmit and/or receive for a longer time, say at least 5 to 10 years?
Or will it rise a short interest only, dominated by people telling it
is not legal and so on... I'm not sure about that. It could be even
better to stay in a smaller group who can do what it wants instead
causing a decision / regulation by an 'authority'.




   You are clearly not lazy having achieved so
much on MF and below :-)
  

Thanks but i'm lazy into a certain spectrum. On the other side, there
are people who write many articles over the years but it is simply
impossible for them to even imagine to wind a coil which has more than
100 turns. Maybe it is good that there is a variety of people, the
article writers and the coil winders and something inbetween :-) Oh,
and the programmers! Very important. Without Wolfgang and Paul and
Markus we would do nothing at all!

Oh BTW maybe i'll transmit on my loop again the next weekend. I can't
await it, it is more than 2 weeks ago, a very long time!!




  I have played with ground loops before and had some good results in
LF.

On VLF it should work much better (relative to a vertical E field
antenna). The idea is that the current runs back in a deep layer (skin
depth), depending on the ground conductivity. So it should work better
on poor conducting ground.


   Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.
  

RR, good luck and fun with the new challenges. 

Looking forward to your next steps and reports.



73, Stefan








  73, Dimitris VK2COW
  









------=_Part_66133_17580208.1549478365689
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: 7bit

Hi Stefan, Dimitris,<br><br>room is sure a thing that is not missing in VK :-)<br>I remember a vacation I had there some years ago ... a lot of km between "adiacent places".. so ideal place for LF, VLF and even close to DC frequencies!<br>During my travel, just for fate, I drove close to Holt Navy Base sporting an antenna just a bit larger than your loop ;-)<br>Anyway you know the grass of the neighbor is more green...<br>Dimitris has room but not a lot of time..<br>I have more time but less room<br>somebody else has room and time but no money...<br>What an hard life!<br>But... we all have fun!<br><br>73 Marco IK1HSS<br><br>P.S. who's looking the legal aspects?? ;-)<br>
<br>
----Messaggio originale----<br>
Da: selberdenken@posteo.de<br>
Data: 5-feb-2019 23.40<br>
A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Ogg: Re: VLF: in VK?<br>
<br>


<!--
  
-->

Dimitris, <br>
<br>
Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap="">G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. </pre>
</blockquote>
Wow, i'm envious and happy that you have such
possibilities!!!!!!!!!!!!!!<br>
Not at this time, ok. I would suggest to start in small steps anyway,
then you can be happy about many improvements, not just a single big
one :-) <br>
I often imagine to live in Canada or Australia and do such experiments
exactly!<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap="">The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed.</pre>
</blockquote>
100m is very close, the far field begins at about 5.7 km distance at
8.27 kHz. A RX in that distance is only useful to check and observe the
signal stability and compare levels. A feedback monitor like my tree
which is 3.5 km distant from my INV-L antenna in the city. From my
ground loop antenna in JN39WI it is 57.6 km distant, which is already
an interesting distance and can be challenging below 3 kHz.<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap=""> I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started.</pre>
</blockquote>
Excellent, just excellent! Your signal could be the stongest of the
radio amateurs! 200W is just fine for the first steps. But be careful
with those audio amplifiers, they do not seem to like to much reactive
power.<br>
For tuning the antenna you will only need a capacitor in series. For my
portable VLF system i built a current transformer to produce a small
voltage that goes to the soundcard. Then, using SpecLab, i can
calculate the antenna current directly and even keep the phase of the
current stable, even if there should be a soundcard glitch. For the
signal generation i also use SpecLab and a cheap GPS module. It all
works very reliable, there were no problems so far.<br>
With a house at one of the ends of the antenna you are in a very
comfortable situation! You may already have a ground system there, so
the effort is at one end only.<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap=""> I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen.</pre>
</blockquote>
Yes, this is a very good distance to observe your own signal. If you
have internet access there and can leave a small PC/notebook/tablet ...
then you could build up a webpage and run a grabber from there like i
do from my tree (still under maintenance). That would be ideal and it
just feels good to see the own signal very clearly on a real RX in a
short distance. You are then independent.<br>
<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap=""> I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!
  </pre>
</blockquote>
Oh yes! Fortunately there are a few arround here. These days this is
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF,
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar
J.T. This is about the complete VLF group worldwide, at least those who
prooved to detect narrow band (sub mHz) signals close to the limits, in
the last 3 years until now.<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap="">Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list.</pre>
</blockquote>
Yes, you are right. I had the same thought sometimes. Certainly there
are many amateurs who would feel like having a new life when starting
at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually
it is not even amateur radio because it is not a spectrum allocated to
amateur radio. So everyone could operate there.<br>
But there is a risk, you know. There are those people who do not simply
start to transmit/receive there and feel good. There are those who
prefer to ask if this is legal at all. And then they ask here and
there, as long as they find someone who triggers their fears and phobs,
and then they do nothing at all! Beware of such people, they are
contaminating your free mind. Concentrate on ideas and wishes, like for
example detecting your own signal in Canberra. And then the question
"Will this also work on lower frequencies", for example.<br>
When writing an article in a radio magazine, what will be the result?
Will it actually lead to more <u>active</u> people on the band, who
transmit and/or receive<u> for a longer time, say at least 5 to 10 years</u>?
Or will it rise a short interest only, dominated by people telling it
is not legal and so on... I'm not sure about that. It could be even
better to stay in a smaller group who can do what it wants instead
causing a decision / regulation by an 'authority'.<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap=""> You are clearly not lazy having achieved so
much on MF and below :-)
  </pre>
</blockquote>
Thanks but i'm lazy into a certain spectrum. On the other side, there
are people who write many articles over the years but it is simply
impossible for them to even imagine to wind a coil which has more than
100 turns. Maybe it is good that there is a variety of people, the
article writers and the coil winders and something inbetween :-) Oh,
and the programmers! Very important. Without Wolfgang and Paul and
Markus we would do nothing at all!<br>
Oh BTW maybe i'll transmit on my loop again the next weekend. I can't
await it, it is more than 2 weeks ago, a very long time!!<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap="">I have played with ground loops before and had some good results in
LF.</pre>
</blockquote>
On VLF it should work much better (relative to a vertical E field
antenna). The idea is that the current runs back in a deep layer (skin
depth), depending on the ground conductivity. So it should work better
on poor conducting ground.<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap=""> Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.
  </pre>
</blockquote>
RR, good luck and fun with the new challenges. <br>
Looking forward to your next steps and reports.<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
<blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
  <pre wrap="">73, Dimitris VK2COW</pre>
  <br>
</blockquote>


<br>
<br>

------=_Part_66133_17580208.1549478365689--


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 Content preview:  Hi Marco, Yes, i totally agree with you :-) Fortunately i
   have enough time and money but room, room is never enough if you are as crazy
    as i am.. BTW i've been on the tree again today until it was nearly total
    dark. I took a photo, see http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg
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Hi Marco,

Yes, i totally agree with you :-)
Fortunately i have enough time and money but room, room is never enough 
if you are as crazy as i am..

BTW i've been on the tree again today until it was nearly total dark. I 
took a photo, see 
http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg It 
was below 0 C up there (~ 420m AGL). BUT now my VLF E field is back 
again so the grabber ( 
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html ) 
has full functionality again. I'm just sitting here listening to the E 
field with headphones, i like the deep sferics, the bummph and there are 
some tweaks at higher frequencies.
So now i am ready to receive Dimitris! ;-)

Indeed, Marco, we have our fun, despite the hard life. BTW didn't you 
want to get started with VLF some time? :-)

73, Stefan



Am 06.02.2019 19:39, schrieb marcocadeddu@tin.it:
> Hi Stefan, Dimitris,
>
> room is sure a thing that is not missing in VK :-)
> I remember a vacation I had there some years ago ... a lot of km 
> between "adiacent places".. so ideal place for LF, VLF and even close 
> to DC frequencies!
> During my travel, just for fate, I drove close to Holt Navy Base 
> sporting an antenna just a bit larger than your loop ;-)
> Anyway you know the grass of the neighbor is more green...
> Dimitris has room but not a lot of time..
> I have more time but less room
> somebody else has room and time but no money...
> What an hard life!
> But... we all have fun!
>
> 73 Marco IK1HSS
>
> P.S. who's looking the legal aspects?? ;-)
>
> ----Messaggio originale----
> Da: selberdenken@posteo.de
> Data: 5-feb-2019 23.40
> A: <rsgb_lf_group@blacksheep.org>
> Ogg: Re: VLF: in VK?
>
> Dimitris,
>
> Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
>> G'day Stefan and Edgar,
>>
>> My house is on QF44OX00OR and the property extends to QF44NX (50 acres
>> or 200,000 m^2). I do have permission from some neighbours to lay
>> wires into their properties, so an extra large (over 1km) ground wire
>> is entirely doable but not at this point in time.
> Wow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!
> Not at this time, ok. I would suggest to start in small steps anyway, 
> then you can be happy about many improvements, not just a single big 
> one :-)
> I often imagine to live in Canada or Australia and do such experiments 
> exactly!
>> The reference loop
>> is from the shed, about 100 metres south of the house, to the tractor
>> shed.
> 100m is very close, the far field begins at about 5.7 km distance at 
> 8.27 kHz. A RX in that distance is only useful to check and observe 
> the signal stability and compare levels. A feedback monitor like my 
> tree which is 3.5 km distant from my INV-L antenna in the city. From 
> my ground loop antenna in JN39WI it is 57.6 km distant, which is 
> already an interesting distance and can be challenging below 3 kHz.
>
>>   I have mains in the shed and I also have a 200 W audio linear
>> amplifier to get things started.
> Excellent, just excellent! Your signal could be the stongest of the 
> radio amateurs! 200W is just fine for the first steps. But be careful 
> with those audio amplifiers, they do not seem to like to much reactive 
> power.
> For tuning the antenna you will only need a capacitor in series. For 
> my portable VLF system i built a current transformer to produce a 
> small voltage that goes to the soundcard. Then, using SpecLab, i can 
> calculate the antenna current directly and even keep the phase of the 
> current stable, even if there should be a soundcard glitch. For the 
> signal generation i also use SpecLab and a cheap GPS module. It all 
> works very reliable, there were no problems so far.
> With a house at one of the ends of the antenna you are in a very 
> comfortable situation! You may already have a ground system there, so 
> the effort is at one end only.
>
>>   I can build a class-E kilowatt if
>> necessary later. I like the roughly north-south loop configuration as
>> it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
>> and most importantly Canberra which is only 30 km to the South. I will
>> try to get some signals received in Canberra before I start asking
>> people further away to have a listen.
> Yes, this is a very good distance to observe your own signal. If you 
> have internet access there and can leave a small PC/notebook/tablet 
> ... then you could build up a webpage and run a grabber from there 
> like i do from my tree (still under maintenance). That would be ideal 
> and it just feels good to see the own signal very clearly on a real RX 
> in a short distance. You are then independent.
>
>
>>   I currently have assembled an XO
>> clocked DDS controlled by an arduino to do the initial tests but later
>> when I decide to go QRSSSSSI can dig out and use the old rubidium
>> clock as a reference for extra stability. For receiving I use a 24
>> bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
>> antenna I will use for receive is one of those monster ferrite rods.
>> Amplification may not even be necessary, the signals I get when the
>> antenna is tuned seem to be already quite good. Once I have a decent
>> RX antenna I think I will start gifting these rods (I have a few) to
>> interested amateurs in the region and help them get started with
>> receiving on VLF. Make a small army of receivers, that would make life
>> much easier when evaluating antennas!
>>    
> Oh yes! Fortunately there are a few arround here. These days this is 
> (sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, 
> IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and 
> Edgar J.T. This is about the complete VLF group worldwide, at least 
> those who prooved to detect narrow band (sub mHz) signals close to the 
> limits, in the last 3 years until now.
>
>> Hey, you should document your experiments even if it is a summary of
>> the activities and nothing more. The list is great but perhaps we are
>> missing out on many other potentially interested people that may have
>> not discovered the list.
> Yes, you are right. I had the same thought sometimes. Certainly there 
> are many amateurs who would feel like having a new life when starting 
> at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually 
> it is not even amateur radio because it is not a spectrum allocated to 
> amateur radio. So everyone could operate there.
> But there is a risk, you know. There are those people who do not 
> simply start to transmit/receive there and feel good. There are those 
> who prefer to ask if this is legal at all. And then they ask here and 
> there, as long as they find someone who triggers their fears and 
> phobs, and then they do nothing at all! Beware of such people, they 
> are contaminating your free mind. Concentrate on ideas and wishes, 
> like for example detecting your own signal in Canberra. And then the 
> question "Will this also work on lower frequencies", for example.
> When writing an article in a radio magazine, what will be the result? 
> Will it actually lead to more _active_ people on the band, who 
> transmit and/or receive_ for a longer time, say at least 5 to 10 
> years_? Or will it rise a short interest only, dominated by people 
> telling it is not legal and so on... I'm not sure about that. It could 
> be even better to stay in a smaller group who can do what it wants 
> instead causing a decision / regulation by an 'authority'.
>
>>   You are clearly not lazy having achieved so
>> much on MF and below :-)
>>    
> Thanks but i'm lazy into a certain spectrum. On the other side, there 
> are people who write many articles over the years but it is simply 
> impossible for them to even imagine to wind a coil which has more than 
> 100 turns. Maybe it is good that there is a variety of people, the 
> article writers and the coil winders and something inbetween :-) Oh, 
> and the programmers! Very important. Without Wolfgang and Paul and 
> Markus we would do nothing at all!
> Oh BTW maybe i'll transmit on my loop again the next weekend. I can't 
> await it, it is more than 2 weeks ago, a very long time!!
>
>> I have played with ground loops before and had some good results in
>> LF.
> On VLF it should work much better (relative to a vertical E field 
> antenna). The idea is that the current runs back in a deep layer (skin 
> depth), depending on the ground conductivity. So it should work better 
> on poor conducting ground.
>>   Once I establish a reference system, I can compare antennas
>> including ground loops. Unlike Europe where you have plenty of people
>> around you, I have to do both the TXing and the RXing and that
>> requires effort and time. The latter is a very scarce resource!
>>
>> Anyway, looks like a nice day today to do some more outdoor work. We
>> had lightning storms and plenty of rain the past few days, so I
>> haven't made any progress.
>>    
> RR, good luck and fun with the new challenges.
> Looking forward to your next steps and reports.
>
> 73, Stefan
>
>
>
>> 73, Dimitris VK2COW
>>
>
>

--------------000309060906050808020900
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Content-Transfer-Encoding: 7bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
Hi Marco, <br>
<br>
Yes, i totally agree with you :-) <br>
Fortunately i have enough time and money but room, room is never enough
if you are as crazy as i am..<br>
<br>
BTW i've been on the tree again today until it was nearly total dark. I
took a photo, see
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg">http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg</a>
It was below 0 C up there (~ 420m AGL). BUT now my VLF E field is back
again so the grabber (
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a> )
has full functionality again. I'm just sitting here listening to the E
field with headphones, i like the deep sferics, the bummph and there
are some tweaks at higher frequencies. <br>
So now i am ready to receive Dimitris! ;-)<br>
<br>
Indeed, Marco, we have our fun, despite the hard life. BTW didn't you
want to get started with VLF some time? :-)<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 06.02.2019 19:39, schrieb <a class="moz-txt-link-abbreviated" href="mailto:marcocadeddu@tin.it:">marcocadeddu@tin.it:</a>
<blockquote cite="mid:168c41b89f6.marcocadeddu@tin.it" type="cite">Hi
Stefan, Dimitris,<br>
  <br>
room is sure a thing that is not missing in VK :-)<br>
I remember a vacation I had there some years ago ... a lot of km
between "adiacent places".. so ideal place for LF, VLF and even close
to DC frequencies!<br>
During my travel, just for fate, I drove close to Holt Navy Base
sporting an antenna just a bit larger than your loop ;-)<br>
Anyway you know the grass of the neighbor is more green...<br>
Dimitris has room but not a lot of time..<br>
I have more time but less room<br>
somebody else has room and time but no money...<br>
What an hard life!<br>
But... we all have fun!<br>
  <br>
73 Marco IK1HSS<br>
  <br>
P.S. who's looking the legal aspects?? ;-)<br>
  <br>
----Messaggio originale----<br>
Da: <a class="moz-txt-link-abbreviated" href="mailto:selberdenken@posteo.de">selberdenken@posteo.de</a><br>
Data: 5-feb-2019 23.40<br>
A: <a class="moz-txt-link-rfc2396E" href="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br>
Ogg: Re: VLF: in VK?<br>
  <br>
<!--
  
-->
Dimitris, <br>
  <br>
Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap="">G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. </pre>
  </blockquote>
Wow, i'm envious and happy that you have such
possibilities!!!!!!!!!!!!!!<br>
Not at this time, ok. I would suggest to start in small steps anyway,
then you can be happy about many improvements, not just a single big
one :-) <br>
I often imagine to live in Canada or Australia and do such experiments
exactly!<br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap="">The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed.</pre>
  </blockquote>
100m is very close, the far field begins at about 5.7 km distance at
8.27 kHz. A RX in that distance is only useful to check and observe the
signal stability and compare levels. A feedback monitor like my tree
which is 3.5 km distant from my INV-L antenna in the city. From my
ground loop antenna in JN39WI it is 57.6 km distant, which is already
an interesting distance and can be challenging below 3 kHz.<br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap=""> I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started.</pre>
  </blockquote>
Excellent, just excellent! Your signal could be the stongest of the
radio amateurs! 200W is just fine for the first steps. But be careful
with those audio amplifiers, they do not seem to like to much reactive
power.<br>
For tuning the antenna you will only need a capacitor in series. For my
portable VLF system i built a current transformer to produce a small
voltage that goes to the soundcard. Then, using SpecLab, i can
calculate the antenna current directly and even keep the phase of the
current stable, even if there should be a soundcard glitch. For the
signal generation i also use SpecLab and a cheap GPS module. It all
works very reliable, there were no problems so far.<br>
With a house at one of the ends of the antenna you are in a very
comfortable situation! You may already have a ground system there, so
the effort is at one end only.<br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap=""> I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen.</pre>
  </blockquote>
Yes, this is a very good distance to observe your own signal. If you
have internet access there and can leave a small PC/notebook/tablet ...
then you could build up a webpage and run a grabber from there like i
do from my tree (still under maintenance). That would be ideal and it
just feels good to see the own signal very clearly on a real RX in a
short distance. You are then independent.<br>
  <br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap=""> I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!
  </pre>
  </blockquote>
Oh yes! Fortunately there are a few arround here. These days this is
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF,
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar
J.T. This is about the complete VLF group worldwide, at least those who
prooved to detect narrow band (sub mHz) signals close to the limits, in
the last 3 years until now.<br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap="">Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list.</pre>
  </blockquote>
Yes, you are right. I had the same thought sometimes. Certainly there
are many amateurs who would feel like having a new life when starting
at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually
it is not even amateur radio because it is not a spectrum allocated to
amateur radio. So everyone could operate there.<br>
But there is a risk, you know. There are those people who do not simply
start to transmit/receive there and feel good. There are those who
prefer to ask if this is legal at all. And then they ask here and
there, as long as they find someone who triggers their fears and phobs,
and then they do nothing at all! Beware of such people, they are
contaminating your free mind. Concentrate on ideas and wishes, like for
example detecting your own signal in Canberra. And then the question
"Will this also work on lower frequencies", for example.<br>
When writing an article in a radio magazine, what will be the result?
Will it actually lead to more <u>active</u> people on the band, who
transmit and/or receive<u> for a longer time, say at least 5 to 10 years</u>?
Or
will it rise a short interest only, dominated by people telling it
is not legal and so on... I'm not sure about that. It could be even
better to stay in a smaller group who can do what it wants instead
causing a decision / regulation by an 'authority'.<br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap=""> You are clearly not lazy having achieved so
much on MF and below :-)
  </pre>
  </blockquote>
Thanks but i'm lazy into a certain spectrum. On the other side, there
are people who write many articles over the years but it is simply
impossible for them to even imagine to wind a coil which has more than
100 turns. Maybe it is good that there is a variety of people, the
article writers and the coil winders and something inbetween :-) Oh,
and the programmers! Very important. Without Wolfgang and Paul and
Markus we would do nothing at all!<br>
Oh BTW maybe i'll transmit on my loop again the next weekend. I can't
await it, it is more than 2 weeks ago, a very long time!!<br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap="">I have played with ground loops before and had some good results in
LF.</pre>
  </blockquote>
On VLF it should work much better (relative to a vertical E field
antenna). The idea is that the current runs back in a deep layer (skin
depth), depending on the ground conductivity. So it should work better
on poor conducting ground.<br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap=""> Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.
  </pre>
  </blockquote>
RR, good luck and fun with the new challenges. <br>
Looking forward to your next steps and reports.<br>
  <br>
73, Stefan<br>
  <br>
  <br>
  <br>
  <blockquote
 cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com"
 type="cite">
    <pre wrap="">73, Dimitris VK2COW</pre>
    <br>
  </blockquote>
  <br>
  <br>
</blockquote>
</body>
</html>

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 Content preview:  Hi Stefan, room is never enough by default ;-) Nice picture
    from the tree: would be nice to have a forest close to my city.. My attempts
    to listen (at least) to VLF were frustrated from the city noise but.. never
    say never, I have still to work ar [...] 
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Hi Stefan,

room is never enough by default ;-)

Nice picture from the tree: would be nice to have a forest close to my city..
My attempts to listen (at least) to VLF were frustrated from the city noise but.. never say never, I have still to work around the MF/LF antenna and then I cannot exclude a priori further experiments on VLF ;-) on the other hand I do hope to be retired soon and probably gain more patience to leave the FFT to work hihi I really hate to have the PC running for hours before see a pixel on the screen (specially if it is just noise.. )

Marco, IK1HSS  



----Messaggio originale----

Da: selberdenken@posteo.de

Data: 6-feb-2019 20.11

A: <rsgb_lf_group@blacksheep.org>

Ogg: Re: R: Re: VLF: in VK?







Hi Marco, 



Yes, i totally agree with you :-) 

Fortunately i have enough time and money but room, room is never enough
if you are as crazy as i am..



BTW i've been on the tree again today until it was nearly total dark. I
took a photo, see
http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg
It was below 0 C up there (~ 420m AGL). BUT now my VLF E field is back
again so the grabber (
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html )
has full functionality again. I'm just sitting here listening to the E
field with headphones, i like the deep sferics, the bummph and there
are some tweaks at higher frequencies. 

So now i am ready to receive Dimitris! ;-)



Indeed, Marco, we have our fun, despite the hard life. BTW didn't you
want to get started with VLF some time? :-)



73, Stefan







Am 06.02.2019 19:39, schrieb marcocadeddu@tin.it:
Hi
Stefan, Dimitris,

  

room is sure a thing that is not missing in VK :-)

I remember a vacation I had there some years ago ... a lot of km
between "adiacent places".. so ideal place for LF, VLF and even close
to DC frequencies!

During my travel, just for fate, I drove close to Holt Navy Base
sporting an antenna just a bit larger than your loop ;-)

Anyway you know the grass of the neighbor is more green...

Dimitris has room but not a lot of time..

I have more time but less room

somebody else has room and time but no money...

What an hard life!

But... we all have fun!

  

73 Marco IK1HSS

  

P.S. who's looking the legal aspects?? ;-)

  

----Messaggio originale----

Da: selberdenken@posteo.de

Data: 5-feb-2019 23.40

A: <rsgb_lf_group@blacksheep.org>

Ogg: Re: VLF: in VK?

  


Dimitris, 

  

Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
  
    G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. 
  
Wow, i'm envious and happy that you have such
possibilities!!!!!!!!!!!!!!

Not at this time, ok. I would suggest to start in small steps anyway,
then you can be happy about many improvements, not just a single big
one :-) 

I often imagine to live in Canada or Australia and do such experiments
exactly!

  
    The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed.
  
100m is very close, the far field begins at about 5.7 km distance at
8.27 kHz. A RX in that distance is only useful to check and observe the
signal stability and compare levels. A feedback monitor like my tree
which is 3.5 km distant from my INV-L antenna in the city. From my
ground loop antenna in JN39WI it is 57.6 km distant, which is already
an interesting distance and can be challenging below 3 kHz.

  

  
     I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started.
  
Excellent, just excellent! Your signal could be the stongest of the
radio amateurs! 200W is just fine for the first steps. But be careful
with those audio amplifiers, they do not seem to like to much reactive
power.

For tuning the antenna you will only need a capacitor in series. For my
portable VLF system i built a current transformer to produce a small
voltage that goes to the soundcard. Then, using SpecLab, i can
calculate the antenna current directly and even keep the phase of the
current stable, even if there should be a soundcard glitch. For the
signal generation i also use SpecLab and a cheap GPS module. It all
works very reliable, there were no problems so far.

With a house at one of the ends of the antenna you are in a very
comfortable situation! You may already have a ground system there, so
the effort is at one end only.

  

  
     I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen.
  
Yes, this is a very good distance to observe your own signal. If you
have internet access there and can leave a small PC/notebook/tablet ...
then you could build up a webpage and run a grabber from there like i
do from my tree (still under maintenance). That would be ideal and it
just feels good to see the own signal very clearly on a real RX in a
short distance. You are then independent.

  

  

  
     I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!
  
  
Oh yes! Fortunately there are a few arround here. These days this is
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF,
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar
J.T. This is about the complete VLF group worldwide, at least those who
prooved to detect narrow band (sub mHz) signals close to the limits, in
the last 3 years until now.

  

  
    Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list.
  
Yes, you are right. I had the same thought sometimes. Certainly there
are many amateurs who would feel like having a new life when starting
at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually
it is not even amateur radio because it is not a spectrum allocated to
amateur radio. So everyone could operate there.

But there is a risk, you know. There are those people who do not simply
start to transmit/receive there and feel good. There are those who
prefer to ask if this is legal at all. And then they ask here and
there, as long as they find someone who triggers their fears and phobs,
and then they do nothing at all! Beware of such people, they are
contaminating your free mind. Concentrate on ideas and wishes, like for
example detecting your own signal in Canberra. And then the question
"Will this also work on lower frequencies", for example.

When writing an article in a radio magazine, what will be the result?
Will it actually lead to more active people on the band, who
transmit and/or receive for a longer time, say at least 5 to 10 years?
Or
will it rise a short interest only, dominated by people telling it
is not legal and so on... I'm not sure about that. It could be even
better to stay in a smaller group who can do what it wants instead
causing a decision / regulation by an 'authority'.

  

  
     You are clearly not lazy having achieved so
much on MF and below :-)
  
  
Thanks but i'm lazy into a certain spectrum. On the other side, there
are people who write many articles over the years but it is simply
impossible for them to even imagine to wind a coil which has more than
100 turns. Maybe it is good that there is a variety of people, the
article writers and the coil winders and something inbetween :-) Oh,
and the programmers! Very important. Without Wolfgang and Paul and
Markus we would do nothing at all!

Oh BTW maybe i'll transmit on my loop again the next weekend. I can't
await it, it is more than 2 weeks ago, a very long time!!

  

  
    I have played with ground loops before and had some good results in
LF.
  
On VLF it should work much better (relative to a vertical E field
antenna). The idea is that the current runs back in a deep layer (skin
depth), depending on the ground conductivity. So it should work better
on poor conducting ground.

  
     Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.
  
  
RR, good luck and fun with the new challenges. 

Looking forward to your next steps and reports.

  

73, Stefan

  

  

  

  
    73, Dimitris VK2COW
    

  
  

  









------=_Part_35743_17624788.1549488538363
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: 7bit

Hi Stefan,<br><br>room is never enough by default ;-)<br><br>Nice picture from the tree: would be nice to have a forest close to my city..<br>My attempts to listen (at least) to VLF were frustrated from the city noise but.. never say never, I have still to work around the MF/LF antenna and then I cannot exclude <i>a priori </i>further experiments on VLF ;-) on the other hand I do hope to be retired soon and probably gain more patience to leave the FFT to work hihi I really hate to have the PC running for hours before see a pixel on the screen (specially if it is just noise.. )<br><br>Marco, IK1HSS&nbsp; <br>
<br>
----Messaggio originale----<br>
Da: selberdenken@posteo.de<br>
Data: 6-feb-2019 20.11<br>
A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Ogg: Re: R: Re: VLF: in VK?<br>
<br>


<!--
  
-->

Hi Marco, <br>
<br>
Yes, i totally agree with you :-) <br>
Fortunately i have enough time and money but room, room is never enough
if you are as crazy as i am..<br>
<br>
BTW i've been on the tree again today until it was nearly total dark. I
took a photo, see
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg">http://www.iup.uni-heidelberg.de/schaefer_vlf/VLF/20190206_175937.jpg</a>
It was below 0 C up there (~ 420m AGL). BUT now my VLF E field is back
again so the grabber (
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a> )
has full functionality again. I'm just sitting here listening to the E
field with headphones, i like the deep sferics, the bummph and there
are some tweaks at higher frequencies. <br>
So now i am ready to receive Dimitris! ;-)<br>
<br>
Indeed, Marco, we have our fun, despite the hard life. BTW didn't you
want to get started with VLF some time? :-)<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 06.02.2019 19:39, schrieb <a class="moz-txt-link-abbreviated" href="mailto:marcocadeddu@tin.it:">marcocadeddu@tin.it:</a>
<blockquote cite="mid:168c41b89f6.marcocadeddu@tin.it" type="cite">Hi
Stefan, Dimitris,<br>
  <br>
room is sure a thing that is not missing in VK :-)<br>
I remember a vacation I had there some years ago ... a lot of km
between "adiacent places".. so ideal place for LF, VLF and even close
to DC frequencies!<br>
During my travel, just for fate, I drove close to Holt Navy Base
sporting an antenna just a bit larger than your loop ;-)<br>
Anyway you know the grass of the neighbor is more green...<br>
Dimitris has room but not a lot of time..<br>
I have more time but less room<br>
somebody else has room and time but no money...<br>
What an hard life!<br>
But... we all have fun!<br>
  <br>
73 Marco IK1HSS<br>
  <br>
P.S. who's looking the legal aspects?? ;-)<br>
  <br>
----Messaggio originale----<br>
Da: <a class="moz-txt-link-abbreviated" href="mailto:selberdenken@posteo.de">selberdenken@posteo.de</a><br>
Data: 5-feb-2019 23.40<br>
A: <a class="moz-txt-link-rfc2396E" href="mailto:rsgb_lf_group@blacksheep.org">&lt;rsgb_lf_group@blacksheep.org&gt;</a><br>
Ogg: Re: VLF: in VK?<br>
  <br>
<!--
  
-->
Dimitris, <br>
  <br>
Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap="">G'day Stefan and Edgar,

My house is on QF44OX00OR and the property extends to QF44NX (50 acres
or 200,000 m^2). I do have permission from some neighbours to lay
wires into their properties, so an extra large (over 1km) ground wire
is entirely doable but not at this point in time. </pre>
  </blockquote>
Wow, i'm envious and happy that you have such
possibilities!!!!!!!!!!!!!!<br>
Not at this time, ok. I would suggest to start in small steps anyway,
then you can be happy about many improvements, not just a single big
one :-) <br>
I often imagine to live in Canada or Australia and do such experiments
exactly!<br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap="">The reference loop
is from the shed, about 100 metres south of the house, to the tractor
shed.</pre>
  </blockquote>
100m is very close, the far field begins at about 5.7 km distance at
8.27 kHz. A RX in that distance is only useful to check and observe the
signal stability and compare levels. A feedback monitor like my tree
which is 3.5 km distant from my INV-L antenna in the city. From my
ground loop antenna in JN39WI it is 57.6 km distant, which is already
an interesting distance and can be challenging below 3 kHz.<br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap=""> I have mains in the shed and I also have a 200 W audio linear
amplifier to get things started.</pre>
  </blockquote>
Excellent, just excellent! Your signal could be the stongest of the
radio amateurs! 200W is just fine for the first steps. But be careful
with those audio amplifiers, they do not seem to like to much reactive
power.<br>
For tuning the antenna you will only need a capacitor in series. For my
portable VLF system i built a current transformer to produce a small
voltage that goes to the soundcard. Then, using SpecLab, i can
calculate the antenna current directly and even keep the phase of the
current stable, even if there should be a soundcard glitch. For the
signal generation i also use SpecLab and a cheap GPS module. It all
works very reliable, there were no problems so far.<br>
With a house at one of the ends of the antenna you are in a very
comfortable situation! You may already have a ground system there, so
the effort is at one end only.<br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap=""> I can build a class-E kilowatt if
necessary later. I like the roughly north-south loop configuration as
it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
and most importantly Canberra which is only 30 km to the South. I will
try to get some signals received in Canberra before I start asking
people further away to have a listen.</pre>
  </blockquote>
Yes, this is a very good distance to observe your own signal. If you
have internet access there and can leave a small PC/notebook/tablet ...
then you could build up a webpage and run a grabber from there like i
do from my tree (still under maintenance). That would be ideal and it
just feels good to see the own signal very clearly on a real RX in a
short distance. You are then independent.<br>
  <br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap=""> I currently have assembled an XO
clocked DDS controlled by an arduino to do the initial tests but later
when I decide to go QRSSSSSI can dig out and use the old rubidium
clock as a reference for extra stability. For receiving I use a 24
bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
antenna I will use for receive is one of those monster ferrite rods.
Amplification may not even be necessary, the signals I get when the
antenna is tuned seem to be already quite good. Once I have a decent
RX antenna I think I will start gifting these rods (I have a few) to
interested amateurs in the region and help them get started with
receiving on VLF. Make a small army of receivers, that would make life
much easier when evaluating antennas!
  </pre>
  </blockquote>
Oh yes! Fortunately there are a few arround here. These days this is
(sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF,
IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar
J.T. This is about the complete VLF group worldwide, at least those who
prooved to detect narrow band (sub mHz) signals close to the limits, in
the last 3 years until now.<br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap="">Hey, you should document your experiments even if it is a summary of
the activities and nothing more. The list is great but perhaps we are
missing out on many other potentially interested people that may have
not discovered the list.</pre>
  </blockquote>
Yes, you are right. I had the same thought sometimes. Certainly there
are many amateurs who would feel like having a new life when starting
at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually
it is not even amateur radio because it is not a spectrum allocated to
amateur radio. So everyone could operate there.<br>
But there is a risk, you know. There are those people who do not simply
start to transmit/receive there and feel good. There are those who
prefer to ask if this is legal at all. And then they ask here and
there, as long as they find someone who triggers their fears and phobs,
and then they do nothing at all! Beware of such people, they are
contaminating your free mind. Concentrate on ideas and wishes, like for
example detecting your own signal in Canberra. And then the question
"Will this also work on lower frequencies", for example.<br>
When writing an article in a radio magazine, what will be the result?
Will it actually lead to more <u>active</u> people on the band, who
transmit and/or receive<u> for a longer time, say at least 5 to 10 years</u>?
Or
will it rise a short interest only, dominated by people telling it
is not legal and so on... I'm not sure about that. It could be even
better to stay in a smaller group who can do what it wants instead
causing a decision / regulation by an 'authority'.<br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap=""> You are clearly not lazy having achieved so
much on MF and below :-)
  </pre>
  </blockquote>
Thanks but i'm lazy into a certain spectrum. On the other side, there
are people who write many articles over the years but it is simply
impossible for them to even imagine to wind a coil which has more than
100 turns. Maybe it is good that there is a variety of people, the
article writers and the coil winders and something inbetween :-) Oh,
and the programmers! Very important. Without Wolfgang and Paul and
Markus we would do nothing at all!<br>
Oh BTW maybe i'll transmit on my loop again the next weekend. I can't
await it, it is more than 2 weeks ago, a very long time!!<br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap="">I have played with ground loops before and had some good results in
LF.</pre>
  </blockquote>
On VLF it should work much better (relative to a vertical E field
antenna). The idea is that the current runs back in a deep layer (skin
depth), depending on the ground conductivity. So it should work better
on poor conducting ground.<br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap=""> Once I establish a reference system, I can compare antennas
including ground loops. Unlike Europe where you have plenty of people
around you, I have to do both the TXing and the RXing and that
requires effort and time. The latter is a very scarce resource!

Anyway, looks like a nice day today to do some more outdoor work. We
had lightning storms and plenty of rain the past few days, so I
haven't made any progress.
  </pre>
  </blockquote>
RR, good luck and fun with the new challenges. <br>
Looking forward to your next steps and reports.<br>
  <br>
73, Stefan<br>
  <br>
  <br>
  <br>
  <blockquote cite="mid:CAKvcm2eruQgEambPR+5HBsg6ckjd3ZOFNf5hV7NfTCLuFOy-=g@mail.gmail.com" type="cite">
    <pre wrap="">73, Dimitris VK2COW</pre>
    <br>
  </blockquote>
  <br>
  <br>
</blockquote>


<br>
<br>

------=_Part_35743_17624788.1549488538363--


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Ciao Marco,

yes, the grass is indeed greener on the other side but I am not
complaining about that! If there is no time now, perhaps there will be
later! More things to do when I retire, there is nothing worse that
people that retire and do nothing...By the way I do look at the legal
aspects. We are lucky in Australia our local spectrum authority has
made it clear how much we can radiate in the various parts of the
spectrum. There is a class licence known as LIPD (low interference
potential devices) which tell you how many microwatts you can radiate
on VLF and below and it is very generous I think. Here is what we are
allowed to do:

0 kHz to 14 kHz        200 uW EIRP
14 kHz to 19.95 kHz   50 uW EIRP
20.05 kHz to 70 kHz  7.5 uW EIRP

(note I cannot transmit between 19.95 kHz and 20.05 kHz, not sure why
there is that gap)

I can live with that!

73, Dimitris VK2COW


Στις Πέμ, 7 Φεβ 2019 στις 5:46 π.μ., ο/η marcocadeddu@tin.it
<marcocadeddu@tin.it> έγραψε:
>
> Hi Stefan, Dimitris,
>
> room is sure a thing that is not missing in VK :-)
> I remember a vacation I had there some years ago ... a lot of km between "adiacent places".. so ideal place for LF, VLF and even close to DC frequencies!
> During my travel, just for fate, I drove close to Holt Navy Base sporting an antenna just a bit larger than your loop ;-)
> Anyway you know the grass of the neighbor is more green...
> Dimitris has room but not a lot of time..
> I have more time but less room
> somebody else has room and time but no money...
> What an hard life!
> But... we all have fun!
>
> 73 Marco IK1HSS
>
> P.S. who's looking the legal aspects?? ;-)
>
> ----Messaggio originale----
> Da: selberdenken@posteo.de
> Data: 5-feb-2019 23.40
> A: <rsgb_lf_group@blacksheep.org>
> Ogg: Re: VLF: in VK?
>
> Dimitris,
>
> Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
>
> G'day Stefan and Edgar,
>
> My house is on QF44OX00OR and the property extends to QF44NX (50 acres
> or 200,000 m^2). I do have permission from some neighbours to lay
> wires into their properties, so an extra large (over 1km) ground wire
> is entirely doable but not at this point in time.
>
> Wow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!
> Not at this time, ok. I would suggest to start in small steps anyway, then you can be happy about many improvements, not just a single big one :-)
> I often imagine to live in Canada or Australia and do such experiments exactly!
>
> The reference loop
> is from the shed, about 100 metres south of the house, to the tractor
> shed.
>
> 100m is very close, the far field begins at about 5.7 km distance at 8.27 kHz. A RX in that distance is only useful to check and observe the signal stability and compare levels. A feedback monitor like my tree which is 3.5 km distant from my INV-L antenna in the city. From my ground loop antenna in JN39WI it is 57.6 km distant, which is already an interesting distance and can be challenging below 3 kHz.
>
>  I have mains in the shed and I also have a 200 W audio linear
> amplifier to get things started.
>
> Excellent, just excellent! Your signal could be the stongest of the radio amateurs! 200W is just fine for the first steps. But be careful with those audio amplifiers, they do not seem to like to much reactive power.
> For tuning the antenna you will only need a capacitor in series. For my portable VLF system i built a current transformer to produce a small voltage that goes to the soundcard. Then, using SpecLab, i can calculate the antenna current directly and even keep the phase of the current stable, even if there should be a soundcard glitch. For the signal generation i also use SpecLab and a cheap GPS module. It all works very reliable, there were no problems so far.
> With a house at one of the ends of the antenna you are in a very comfortable situation! You may already have a ground system there, so the effort is at one end only.
>
>  I can build a class-E kilowatt if
> necessary later. I like the roughly north-south loop configuration as
> it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
> and most importantly Canberra which is only 30 km to the South. I will
> try to get some signals received in Canberra before I start asking
> people further away to have a listen.
>
> Yes, this is a very good distance to observe your own signal. If you have internet access there and can leave a small PC/notebook/tablet ... then you could build up a webpage and run a grabber from there like i do from my tree (still under maintenance). That would be ideal and it just feels good to see the own signal very clearly on a real RX in a short distance. You are then independent.
>
>
>  I currently have assembled an XO
> clocked DDS controlled by an arduino to do the initial tests but later
> when I decide to go QRSSSSSI can dig out and use the old rubidium
> clock as a reference for extra stability. For receiving I use a 24
> bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
> antenna I will use for receive is one of those monster ferrite rods.
> Amplification may not even be necessary, the signals I get when the
> antenna is tuned seem to be already quite good. Once I have a decent
> RX antenna I think I will start gifting these rods (I have a few) to
> interested amateurs in the region and help them get started with
> receiving on VLF. Make a small army of receivers, that would make life
> much easier when evaluating antennas!
>
>
> Oh yes! Fortunately there are a few arround here. These days this is (sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar J.T. This is about the complete VLF group worldwide, at least those who prooved to detect narrow band (sub mHz) signals close to the limits, in the last 3 years until now.
>
> Hey, you should document your experiments even if it is a summary of
> the activities and nothing more. The list is great but perhaps we are
> missing out on many other potentially interested people that may have
> not discovered the list.
>
> Yes, you are right. I had the same thought sometimes. Certainly there are many amateurs who would feel like having a new life when starting at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually it is not even amateur radio because it is not a spectrum allocated to amateur radio. So everyone could operate there.
> But there is a risk, you know. There are those people who do not simply start to transmit/receive there and feel good. There are those who prefer to ask if this is legal at all. And then they ask here and there, as long as they find someone who triggers their fears and phobs, and then they do nothing at all! Beware of such people, they are contaminating your free mind. Concentrate on ideas and wishes, like for example detecting your own signal in Canberra. And then the question "Will this also work on lower frequencies", for example.
> When writing an article in a radio magazine, what will be the result? Will it actually lead to more active people on the band, who transmit and/or receive for a longer time, say at least 5 to 10 years? Or will it rise a short interest only, dominated by people telling it is not legal and so on... I'm not sure about that. It could be even better to stay in a smaller group who can do what it wants instead causing a decision / regulation by an 'authority'.
>
>  You are clearly not lazy having achieved so
> much on MF and below :-)
>
>
> Thanks but i'm lazy into a certain spectrum. On the other side, there are people who write many articles over the years but it is simply impossible for them to even imagine to wind a coil which has more than 100 turns. Maybe it is good that there is a variety of people, the article writers and the coil winders and something inbetween :-) Oh, and the programmers! Very important. Without Wolfgang and Paul and Markus we would do nothing at all!
> Oh BTW maybe i'll transmit on my loop again the next weekend. I can't await it, it is more than 2 weeks ago, a very long time!!
>
> I have played with ground loops before and had some good results in
> LF.
>
> On VLF it should work much better (relative to a vertical E field antenna). The idea is that the current runs back in a deep layer (skin depth), depending on the ground conductivity. So it should work better on poor conducting ground.
>
>  Once I establish a reference system, I can compare antennas
> including ground loops. Unlike Europe where you have plenty of people
> around you, I have to do both the TXing and the RXing and that
> requires effort and time. The latter is a very scarce resource!
>
> Anyway, looks like a nice day today to do some more outdoor work. We
> had lightning storms and plenty of rain the past few days, so I
> haven't made any progress.
>
>
> RR, good luck and fun with the new challenges.
> Looking forward to your next steps and reports.
>
> 73, Stefan
>
>
>
> 73, Dimitris VK2COW
>
>
>
>


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 Content preview:  Kalispera Dimitris, I guess (almost) nobody here is complaining
    for something lacking ;-) but of course we all have some dream :-) Leaving
    the jokes, recalling the HAM decalog, we do respect laws and [...] 
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Kalispera Dimitris,
I guess (almost) nobody here is complaining for something lacking ;-) but o=
f course we all have some dream :-)
Leaving the jokes, recalling the HAM decalog, we do respect laws and take c=
are of the legal aspects even if laws have today the trend to became not ve=
ry simple to understand, sometime even to know and some point could be even=
 hard to full respect for an "amateur"
For instance, I admit my lack, here in EU below 9 kHz, provided no interfer=
ence with other services, the use of the band should be free: am I wrong?It=
 is amazing the limit you have.. uW allowed.. we know how far Stefan was de=
tected with few uW but how can an average amateur be sure to comply such li=
mits?
Maybe 20 kHz is the Holt qrg? ;-))
73, Marco IK1HSS



----Messaggio originale----
Da: dtsifakis@gmail.com
Data: 7-feb-2019 1.52
A: <rsgb_lf_group@blacksheep.org>
Ogg: Re: Re: VLF: in VK?

Ciao Marco,

yes, the grass is indeed greener on the other side but I am not
complaining about that! If there is no time now, perhaps there will be
later! More things to do when I retire, there is nothing worse that
people that retire and do nothing...By the way I do look at the legal
aspects. We are lucky in Australia our local spectrum authority has
made it clear how much we can radiate in the various parts of the
spectrum. There is a class licence known as LIPD (low interference
potential devices) which tell you how many microwatts you can radiate
on VLF and below and it is very generous I think. Here is what we are
allowed to do:

0 kHz to 14 kHz        200 uW EIRP
14 kHz to 19.95 kHz   50 uW EIRP
20.05 kHz to 70 kHz  7.5 uW EIRP

(note I cannot transmit between 19.95 kHz and 20.05 kHz, not sure why
there is that gap)

I can live with that!

73, Dimitris VK2COW


=CE=A3=CF=84=CE=B9=CF=82 =CE=A0=CE=AD=CE=BC, 7 =CE=A6=CE=B5=CE=B2 2019 =CF=
=83=CF=84=CE=B9=CF=82 5:46 =CF=80.=CE=BC., =CE=BF/=CE=B7 marcocadeddu@tin.i=
t
<marcocadeddu@tin.it> =CE=AD=CE=B3=CF=81=CE=B1=CF=88=CE=B5:
>
> Hi Stefan, Dimitris,
>
> room is sure a thing that is not missing in VK :-)
> I remember a vacation I had there some years ago ... a lot of km between =
"adiacent places".. so ideal place for LF, VLF and even close to DC frequen=
cies!
> During my travel, just for fate, I drove close to Holt Navy Base sporting=
 an antenna just a bit larger than your loop ;-)
> Anyway you know the grass of the neighbor is more green...
> Dimitris has room but not a lot of time..
> I have more time but less room
> somebody else has room and time but no money...
> What an hard life!
> But... we all have fun!
>
> 73 Marco IK1HSS
>
> P.S. who's looking the legal aspects?? ;-)
>
> ----Messaggio originale----
> Da: selberdenken@posteo.de
> Data: 5-feb-2019 23.40
> A: <rsgb_lf_group@blacksheep.org>
> Ogg: Re: VLF: in VK?
>
> Dimitris,
>
> Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
>
> G'day Stefan and Edgar,
>
> My house is on QF44OX00OR and the property extends to QF44NX (50 acres
> or 200,000 m^2). I do have permission from some neighbours to lay
> wires into their properties, so an extra large (over 1km) ground wire
> is entirely doable but not at this point in time.
>
> Wow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!
> Not at this time, ok. I would suggest to start in small steps anyway, the=
n you can be happy about many improvements, not just a single big one :-)
> I often imagine to live in Canada or Australia and do such experiments ex=
actly!
>
> The reference loop
> is from the shed, about 100 metres south of the house, to the tractor
> shed.
>
> 100m is very close, the far field begins at about 5.7 km distance at 8.27=
 kHz. A RX in that distance is only useful to check and observe the signal =
stability and compare levels. A feedback monitor like my tree which is 3.5 =
km distant from my INV-L antenna in the city. From my ground loop antenna i=
n JN39WI it is 57.6 km distant, which is already an interesting distance an=
d can be challenging below 3 kHz.
>
>  I have mains in the shed and I also have a 200 W audio linear
> amplifier to get things started.
>
> Excellent, just excellent! Your signal could be the stongest of the radio=
 amateurs! 200W is just fine for the first steps. But be careful with those=
 audio amplifiers, they do not seem to like to much reactive power.
> For tuning the antenna you will only need a capacitor in series. For my p=
ortable VLF system i built a current transformer to produce a small voltage=
 that goes to the soundcard. Then, using SpecLab, i can calculate the anten=
na current directly and even keep the phase of the current stable, even if =
there should be a soundcard glitch. For the signal generation i also use Sp=
ecLab and a cheap GPS module. It all works very reliable, there were no pro=
blems so far.
> With a house at one of the ends of the antenna you are in a very comforta=
ble situation! You may already have a ground system there, so the effort is=
 at one end only.
>
>  I can build a class-E kilowatt if
> necessary later. I like the roughly north-south loop configuration as
> it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
> and most importantly Canberra which is only 30 km to the South. I will
> try to get some signals received in Canberra before I start asking
> people further away to have a listen.
>
> Yes, this is a very good distance to observe your own signal. If you have=
 internet access there and can leave a small PC/notebook/tablet ... then yo=
u could build up a webpage and run a grabber from there like i do from my t=
ree (still under maintenance). That would be ideal and it just feels good t=
o see the own signal very clearly on a real RX in a short distance. You are=
 then independent.
>
>
>  I currently have assembled an XO
> clocked DDS controlled by an arduino to do the initial tests but later
> when I decide to go QRSSSSSI can dig out and use the old rubidium
> clock as a reference for extra stability. For receiving I use a 24
> bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
> antenna I will use for receive is one of those monster ferrite rods.
> Amplification may not even be necessary, the signals I get when the
> antenna is tuned seem to be already quite good. Once I have a decent
> RX antenna I think I will start gifting these rods (I have a few) to
> interested amateurs in the region and help them get started with
> receiving on VLF. Make a small army of receivers, that would make life
> much easier when evaluating antennas!
>
>
> Oh yes! Fortunately there are a few arround here. These days this is (sor=
ted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, IK1QFK, Paul =
Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar J.T. This is abo=
ut the complete VLF group worldwide, at least those who prooved to detect n=
arrow band (sub mHz) signals close to the limits, in the last 3 years until=
 now.
>
> Hey, you should document your experiments even if it is a summary of
> the activities and nothing more. The list is great but perhaps we are
> missing out on many other potentially interested people that may have
> not discovered the list.
>
> Yes, you are right. I had the same thought sometimes. Certainly there are=
 many amateurs who would feel like having a new life when starting at VLF, =
It is an unknown spectrum for 99.9 % of the amateurs. Actually it is not ev=
en amateur radio because it is not a spectrum allocated to amateur radio. S=
o everyone could operate there.
> But there is a risk, you know. There are those people who do not simply s=
tart to transmit/receive there and feel good. There are those who prefer to=
 ask if this is legal at all. And then they ask here and there, as long as =
they find someone who triggers their fears and phobs, and then they do noth=
ing at all! Beware of such people, they are contaminating your free mind. C=
oncentrate on ideas and wishes, like for example detecting your own signal =
in Canberra. And then the question "Will this also work on lower frequencie=
s", for example.
> When writing an article in a radio magazine, what will be the result? Wil=
l it actually lead to more active people on the band, who transmit and/or r=
eceive for a longer time, say at least 5 to 10 years? Or will it rise a sho=
rt interest only, dominated by people telling it is not legal and so on... =
I'm not sure about that. It could be even better to stay in a smaller group=
 who can do what it wants instead causing a decision / regulation by an 'au=
thority'.
>
>  You are clearly not lazy having achieved so
> much on MF and below :-)
>
>
> Thanks but i'm lazy into a certain spectrum. On the other side, there are=
 people who write many articles over the years but it is simply impossible =
for them to even imagine to wind a coil which has more than 100 turns. Mayb=
e it is good that there is a variety of people, the article writers and the=
 coil winders and something inbetween :-) Oh, and the programmers! Very imp=
ortant. Without Wolfgang and Paul and Markus we would do nothing at all!
> Oh BTW maybe i'll transmit on my loop again the next weekend. I can't awa=
it it, it is more than 2 weeks ago, a very long time!!
>
> I have played with ground loops before and had some good results in
> LF.
>
> On VLF it should work much better (relative to a vertical E field antenna=
). The idea is that the current runs back in a deep layer (skin depth), dep=
ending on the ground conductivity. So it should work better on poor conduct=
ing ground.
>
>  Once I establish a reference system, I can compare antennas
> including ground loops. Unlike Europe where you have plenty of people
> around you, I have to do both the TXing and the RXing and that
> requires effort and time. The latter is a very scarce resource!
>
> Anyway, looks like a nice day today to do some more outdoor work. We
> had lightning storms and plenty of rain the past few days, so I
> haven't made any progress.
>
>
> RR, good luck and fun with the new challenges.
> Looking forward to your next steps and reports.
>
> 73, Stefan
>
>
>
> 73, Dimitris VK2COW
>
>
>
>





------=_Part_7358_13888973.1549527045662
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div>Kalispera Dimitris,</div><div><br></div><div>I guess (almost) nobody h=
ere is complaining for something lacking ;-) but of course we all have some=
 dream :-)</div><div><br></div><div>Leaving the jokes, recalling the HAM de=
calog, we do respect laws and take care of the legal aspects even if laws h=
ave today the trend to became not very simple to understand, sometime even =
to know and some point could be even hard to full respect for an "amateur"<=
/div><div><br></div><div>For instance, I admit my lack, here in EU below 9 =
kHz, provided no interference with other services, the use of the band shou=
ld be free: am I wrong?</div><div>It is amazing the limit you have.. uW all=
owed.. we know how far Stefan was detected with few uW but how can an avera=
ge amateur be sure to comply such limits?</div><div><br></div><div>Maybe 20=
 kHz is the Holt qrg? ;-))</div><div><br></div><div>73, Marco IK1HSS<br></d=
iv>
<br>
----Messaggio originale----<br>Da: dtsifakis@gmail.com<br>Data: 7-feb-2019 =
1.52<br>A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>Ogg: Re: Re: VLF: in VK?=
<br><br>Ciao Marco,<br><br>yes, the grass is indeed greener on the other si=
de but I am not<br>complaining about that! If there is no time now, perhaps=
 there will be<br>later! More things to do when I retire, there is nothing =
worse that<br>people that retire and do nothing...By the way I do look at t=
he legal<br>aspects. We are lucky in Australia our local spectrum authority=
 has<br>made it clear how much we can radiate in the various parts of the<b=
r>spectrum. There is a class licence known as LIPD (low interference<br>pot=
ential devices) which tell you how many microwatts you can radiate<br>on VL=
F and below and it is very generous I think. Here is what we are<br>allowed=
 to do:<br><br>0 kHz to 14 kHz&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 20=
0 uW EIRP<br>14 kHz to 19.95 kHz&nbsp;&nbsp; 50 uW EIRP<br>20.05 kHz to 70 =
kHz&nbsp; 7.5 uW EIRP<br><br>(note I cannot transmit between 19.95 kHz and =
20.05 kHz, not sure why<br>there is that gap)<br><br>I can live with that!<=
br><br>73, Dimitris VK2COW<br><br><br>=CE=A3=CF=84=CE=B9=CF=82 =CE=A0=CE=AD=
=CE=BC, 7 =CE=A6=CE=B5=CE=B2 2019 =CF=83=CF=84=CE=B9=CF=82 5:46 =CF=80.=CE=
=BC., =CE=BF/=CE=B7 marcocadeddu@tin.it<br>&lt;marcocadeddu@tin.it&gt; =CE=
=AD=CE=B3=CF=81=CE=B1=CF=88=CE=B5:<br>&gt;<br>&gt; Hi Stefan, Dimitris,<br>=
&gt;<br>&gt; room is sure a thing that is not missing in VK :-)<br>&gt; I r=
emember a vacation I had there some years ago ... a lot of km between "adia=
cent places".. so ideal place for LF, VLF and even close to DC frequencies!=
<br>&gt; During my travel, just for fate, I drove close to Holt Navy Base s=
porting an antenna just a bit larger than your loop ;-)<br>&gt; Anyway you =
know the grass of the neighbor is more green...<br>&gt; Dimitris has room b=
ut not a lot of time..<br>&gt; I have more time but less room<br>&gt; someb=
ody else has room and time but no money...<br>&gt; What an hard life!<br>&g=
t; But... we all have fun!<br>&gt;<br>&gt; 73 Marco IK1HSS<br>&gt;<br>&gt; =
P.S. who's looking the legal aspects?? ;-)<br>&gt;<br>&gt; ----Messaggio or=
iginale----<br>&gt; Da: selberdenken@posteo.de<br>&gt; Data: 5-feb-2019 23.=
40<br>&gt; A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>&gt; Ogg: Re: VLF: in=
 VK?<br>&gt;<br>&gt; Dimitris,<br>&gt;<br>&gt; Am 05.02.2019 21:14, schrieb=
 Dimitrios Tsifakis:<br>&gt;<br>&gt; G'day Stefan and Edgar,<br>&gt;<br>&gt=
; My house is on QF44OX00OR and the property extends to QF44NX (50 acres<br=
>&gt; or 200,000 m^2). I do have permission from some neighbours to lay<br>=
&gt; wires into their properties, so an extra large (over 1km) ground wire<=
br>&gt; is entirely doable but not at this point in time.<br>&gt;<br>&gt; W=
ow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!<br=
>&gt; Not at this time, ok. I would suggest to start in small steps anyway,=
 then you can be happy about many improvements, not just a single big one :=
-)<br>&gt; I often imagine to live in Canada or Australia and do such exper=
iments exactly!<br>&gt;<br>&gt; The reference loop<br>&gt; is from the shed=
, about 100 metres south of the house, to the tractor<br>&gt; shed.<br>&gt;=
<br>&gt; 100m is very close, the far field begins at about 5.7 km distance =
at 8.27 kHz. A RX in that distance is only useful to check and observe the =
signal stability and compare levels. A feedback monitor like my tree which =
is 3.5 km distant from my INV-L antenna in the city. From my ground loop an=
tenna in JN39WI it is 57.6 km distant, which is already an interesting dist=
ance and can be challenging below 3 kHz.<br>&gt;<br>&gt;&nbsp; I have mains=
 in the shed and I also have a 200 W audio linear<br>&gt; amplifier to get =
things started.<br>&gt;<br>&gt; Excellent, just excellent! Your signal coul=
d be the stongest of the radio amateurs! 200W is just fine for the first st=
eps. But be careful with those audio amplifiers, they do not seem to like t=
o much reactive power.<br>&gt; For tuning the antenna you will only need a =
capacitor in series. For my portable VLF system i built a current transform=
er to produce a small voltage that goes to the soundcard. Then, using SpecL=
ab, i can calculate the antenna current directly and even keep the phase of=
 the current stable, even if there should be a soundcard glitch. For the si=
gnal generation i also use SpecLab and a cheap GPS module. It all works ver=
y reliable, there were no problems so far.<br>&gt; With a house at one of t=
he ends of the antenna you are in a very comfortable situation! You may alr=
eady have a ground system there, so the effort is at one end only.<br>&gt;<=
br>&gt;&nbsp; I can build a class-E kilowatt if<br>&gt; necessary later. I =
like the roughly north-south loop configuration as<br>&gt; it favours many =
large cities (Melbourne, Sydney, Brisbane and Tassie)<br>&gt; and most impo=
rtantly Canberra which is only 30 km to the South. I will<br>&gt; try to ge=
t some signals received in Canberra before I start asking<br>&gt; people fu=
rther away to have a listen.<br>&gt;<br>&gt; Yes, this is a very good dista=
nce to observe your own signal. If you have internet access there and can l=
eave a small PC/notebook/tablet ... then you could build up a webpage and r=
un a grabber from there like i do from my tree (still under maintenance). T=
hat would be ideal and it just feels good to see the own signal very clearl=
y on a real RX in a short distance. You are then independent.<br>&gt;<br>&g=
t;<br>&gt;&nbsp; I currently have assembled an XO<br>&gt; clocked DDS contr=
olled by an arduino to do the initial tests but later<br>&gt; when I decide=
 to go QRSSSSSI can dig out and use the old rubidium<br>&gt; clock as a ref=
erence for extra stability. For receiving I use a 24<br>&gt; bit, 192 kHz U=
SB sound card and spectrum lab (thanks Wolf!). The<br>&gt; antenna I will u=
se for receive is one of those monster ferrite rods.<br>&gt; Amplification =
may not even be necessary, the signals I get when the<br>&gt; antenna is tu=
ned seem to be already quite good. Once I have a decent<br>&gt; RX antenna =
I think I will start gifting these rods (I have a few) to<br>&gt; intereste=
d amateurs in the region and help them get started with<br>&gt; receiving o=
n VLF. Make a small army of receivers, that would make life<br>&gt; much ea=
sier when evaluating antennas!<br>&gt;<br>&gt;<br>&gt; Oh yes! Fortunately =
there are a few arround here. These days this is (sorted by distance to my =
VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, IK1QFK, Paul Nicholson, SQ5BPF and =
RN3AUS. Oh and W1VD, K3SIW and Edgar J.T. This is about the complete VLF gr=
oup worldwide, at least those who prooved to detect narrow band (sub mHz) s=
ignals close to the limits, in the last 3 years until now.<br>&gt;<br>&gt; =
Hey, you should document your experiments even if it is a summary of<br>&gt=
; the activities and nothing more. The list is great but perhaps we are<br>=
&gt; missing out on many other potentially interested people that may have<=
br>&gt; not discovered the list.<br>&gt;<br>&gt; Yes, you are right. I had =
the same thought sometimes. Certainly there are many amateurs who would fee=
l like having a new life when starting at VLF, It is an unknown spectrum fo=
r 99.9 % of the amateurs. Actually it is not even amateur radio because it =
is not a spectrum allocated to amateur radio. So everyone could operate the=
re.<br>&gt; But there is a risk, you know. There are those people who do no=
t simply start to transmit/receive there and feel good. There are those who=
 prefer to ask if this is legal at all. And then they ask here and there, a=
s long as they find someone who triggers their fears and phobs, and then th=
ey do nothing at all! Beware of such people, they are contaminating your fr=
ee mind. Concentrate on ideas and wishes, like for example detecting your o=
wn signal in Canberra. And then the question "Will this also work on lower =
frequencies", for example.<br>&gt; When writing an article in a radio magaz=
ine, what will be the result? Will it actually lead to more active people o=
n the band, who transmit and/or receive for a longer time, say at least 5 t=
o 10 years? Or will it rise a short interest only, dominated by people tell=
ing it is not legal and so on... I'm not sure about that. It could be even =
better to stay in a smaller group who can do what it wants instead causing =
a decision / regulation by an 'authority'.<br>&gt;<br>&gt;&nbsp; You are cl=
early not lazy having achieved so<br>&gt; much on MF and below :-)<br>&gt;<=
br>&gt;<br>&gt; Thanks but i'm lazy into a certain spectrum. On the other s=
ide, there are people who write many articles over the years but it is simp=
ly impossible for them to even imagine to wind a coil which has more than 1=
00 turns. Maybe it is good that there is a variety of people, the article w=
riters and the coil winders and something inbetween :-) Oh, and the program=
mers! Very important. Without Wolfgang and Paul and Markus we would do noth=
ing at all!<br>&gt; Oh BTW maybe i'll transmit on my loop again the next we=
ekend. I can't await it, it is more than 2 weeks ago, a very long time!!<br=
>&gt;<br>&gt; I have played with ground loops before and had some good resu=
lts in<br>&gt; LF.<br>&gt;<br>&gt; On VLF it should work much better (relat=
ive to a vertical E field antenna). The idea is that the current runs back =
in a deep layer (skin depth), depending on the ground conductivity. So it s=
hould work better on poor conducting ground.<br>&gt;<br>&gt;&nbsp; Once I e=
stablish a reference system, I can compare antennas<br>&gt; including groun=
d loops. Unlike Europe where you have plenty of people<br>&gt; around you, =
I have to do both the TXing and the RXing and that<br>&gt; requires effort =
and time. The latter is a very scarce resource!<br>&gt;<br>&gt; Anyway, loo=
ks like a nice day today to do some more outdoor work. We<br>&gt; had light=
ning storms and plenty of rain the past few days, so I<br>&gt; haven't made=
 any progress.<br>&gt;<br>&gt;<br>&gt; RR, good luck and fun with the new c=
hallenges.<br>&gt; Looking forward to your next steps and reports.<br>&gt;<=
br>&gt; 73, Stefan<br>&gt;<br>&gt;<br>&gt;<br>&gt; 73, Dimitris VK2COW<br>&=
gt;<br>&gt;<br>&gt;<br>&gt;<br><br><br><br>

------=_Part_7358_13888973.1549527045662--


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Message-ID: <5C5BE905.2010904@posteo.de>
Date: Thu, 07 Feb 2019 09:15:01 +0100
From: DK7FC <selberdenken@posteo.de>
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References: <168c41b89f6.marcocadeddu@tin.it> <CAKvcm2eoZZOrjQ6zZ6Tx3zxHfahEL6eJ2jrcHELgsVdecfLA2g@mail.gmail.com>
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 Content preview:  Hi Dimitris, Interesting, theat LIPD class. So you could even
    try higher frequencies than 8.3 kHz. Here we are not allowed to transmit
   above 8.3 kHz. However, i have a special licence to transmit arround 17.47
    kHz [...] 
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Subject: Re: VLF: in VK?
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Hi Dimitris,

Interesting, theat LIPD class. So you could even try higher frequencies 
than 8.3 kHz. Here we are not allowed to transmit above 8.3 kHz.
However, i have a special licence to transmit arround 17.47 kHz, with 5 
mW ERP. On that frequency i have been received by Edgar and we 
transferred a 3 character message successfully some months ago. A 5 
character message almost decoded but in the end we failed.

Why is there is a  gap between 19.95...20.05 kHz? No idea but i would 
have expected a gap arround 19.8 kHz, because of NWC 
https://en.wikipedia.org/wiki/Naval_Communication_Station_Harold_E._Holt

200 uW on 8.27 kHz is a good signal but with the space you have, you 
could get up to 20 dB more so it is a pity. But anyway, many people 
could detect you at 200 uW, at least in a radius a few 1000 km.

73, Stefan



Am 07.02.2019 01:52, schrieb Dimitrios Tsifakis:
> Ciao Marco,
>
> yes, the grass is indeed greener on the other side but I am not
> complaining about that! If there is no time now, perhaps there will be
> later! More things to do when I retire, there is nothing worse that
> people that retire and do nothing...By the way I do look at the legal
> aspects. We are lucky in Australia our local spectrum authority has
> made it clear how much we can radiate in the various parts of the
> spectrum. There is a class licence known as LIPD (low interference
> potential devices) which tell you how many microwatts you can radiate
> on VLF and below and it is very generous I think. Here is what we are
> allowed to do:
>
> 0 kHz to 14 kHz        200 uW EIRP
> 14 kHz to 19.95 kHz   50 uW EIRP
> 20.05 kHz to 70 kHz  7.5 uW EIRP
>
> (note I cannot transmit between 19.95 kHz and 20.05 kHz, not sure why
> there is that gap)
>
> I can live with that!
>
> 73, Dimitris VK2COW
>
>
> Στις Πέμ, 7 Φεβ 2019 στις 5:46 π.μ., ο/η marcocadeddu@tin.it
> <marcocadeddu@tin.it>  έγραψε:
>    
>> Hi Stefan, Dimitris,
>>
>> room is sure a thing that is not missing in VK :-)
>> I remember a vacation I had there some years ago ... a lot of km between "adiacent places".. so ideal place for LF, VLF and even close to DC frequencies!
>> During my travel, just for fate, I drove close to Holt Navy Base sporting an antenna just a bit larger than your loop ;-)
>> Anyway you know the grass of the neighbor is more green...
>> Dimitris has room but not a lot of time..
>> I have more time but less room
>> somebody else has room and time but no money...
>> What an hard life!
>> But... we all have fun!
>>
>> 73 Marco IK1HSS
>>
>> P.S. who's looking the legal aspects?? ;-)
>>
>> ----Messaggio originale----
>> Da: selberdenken@posteo.de
>> Data: 5-feb-2019 23.40
>> A:<rsgb_lf_group@blacksheep.org>
>> Ogg: Re: VLF: in VK?
>>
>> Dimitris,
>>
>> Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
>>
>> G'day Stefan and Edgar,
>>
>> My house is on QF44OX00OR and the property extends to QF44NX (50 acres
>> or 200,000 m^2). I do have permission from some neighbours to lay
>> wires into their properties, so an extra large (over 1km) ground wire
>> is entirely doable but not at this point in time.
>>
>> Wow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!
>> Not at this time, ok. I would suggest to start in small steps anyway, then you can be happy about many improvements, not just a single big one :-)
>> I often imagine to live in Canada or Australia and do such experiments exactly!
>>
>> The reference loop
>> is from the shed, about 100 metres south of the house, to the tractor
>> shed.
>>
>> 100m is very close, the far field begins at about 5.7 km distance at 8.27 kHz. A RX in that distance is only useful to check and observe the signal stability and compare levels. A feedback monitor like my tree which is 3.5 km distant from my INV-L antenna in the city. From my ground loop antenna in JN39WI it is 57.6 km distant, which is already an interesting distance and can be challenging below 3 kHz.
>>
>>   I have mains in the shed and I also have a 200 W audio linear
>> amplifier to get things started.
>>
>> Excellent, just excellent! Your signal could be the stongest of the radio amateurs! 200W is just fine for the first steps. But be careful with those audio amplifiers, they do not seem to like to much reactive power.
>> For tuning the antenna you will only need a capacitor in series. For my portable VLF system i built a current transformer to produce a small voltage that goes to the soundcard. Then, using SpecLab, i can calculate the antenna current directly and even keep the phase of the current stable, even if there should be a soundcard glitch. For the signal generation i also use SpecLab and a cheap GPS module. It all works very reliable, there were no problems so far.
>> With a house at one of the ends of the antenna you are in a very comfortable situation! You may already have a ground system there, so the effort is at one end only.
>>
>>   I can build a class-E kilowatt if
>> necessary later. I like the roughly north-south loop configuration as
>> it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
>> and most importantly Canberra which is only 30 km to the South. I will
>> try to get some signals received in Canberra before I start asking
>> people further away to have a listen.
>>
>> Yes, this is a very good distance to observe your own signal. If you have internet access there and can leave a small PC/notebook/tablet ... then you could build up a webpage and run a grabber from there like i do from my tree (still under maintenance). That would be ideal and it just feels good to see the own signal very clearly on a real RX in a short distance. You are then independent.
>>
>>
>>   I currently have assembled an XO
>> clocked DDS controlled by an arduino to do the initial tests but later
>> when I decide to go QRSSSSSI can dig out and use the old rubidium
>> clock as a reference for extra stability. For receiving I use a 24
>> bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
>> antenna I will use for receive is one of those monster ferrite rods.
>> Amplification may not even be necessary, the signals I get when the
>> antenna is tuned seem to be already quite good. Once I have a decent
>> RX antenna I think I will start gifting these rods (I have a few) to
>> interested amateurs in the region and help them get started with
>> receiving on VLF. Make a small army of receivers, that would make life
>> much easier when evaluating antennas!
>>
>>
>> Oh yes! Fortunately there are a few arround here. These days this is (sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar J.T. This is about the complete VLF group worldwide, at least those who prooved to detect narrow band (sub mHz) signals close to the limits, in the last 3 years until now.
>>
>> Hey, you should document your experiments even if it is a summary of
>> the activities and nothing more. The list is great but perhaps we are
>> missing out on many other potentially interested people that may have
>> not discovered the list.
>>
>> Yes, you are right. I had the same thought sometimes. Certainly there are many amateurs who would feel like having a new life when starting at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually it is not even amateur radio because it is not a spectrum allocated to amateur radio. So everyone could operate there.
>> But there is a risk, you know. There are those people who do not simply start to transmit/receive there and feel good. There are those who prefer to ask if this is legal at all. And then they ask here and there, as long as they find someone who triggers their fears and phobs, and then they do nothing at all! Beware of such people, they are contaminating your free mind. Concentrate on ideas and wishes, like for example detecting your own signal in Canberra. And then the question "Will this also work on lower frequencies", for example.
>> When writing an article in a radio magazine, what will be the result? Will it actually lead to more active people on the band, who transmit and/or receive for a longer time, say at least 5 to 10 years? Or will it rise a short interest only, dominated by people telling it is not legal and so on... I'm not sure about that. It could be even better to stay in a smaller group who can do what it wants instead causing a decision / regulation by an 'authority'.
>>
>>   You are clearly not lazy having achieved so
>> much on MF and below :-)
>>
>>
>> Thanks but i'm lazy into a certain spectrum. On the other side, there are people who write many articles over the years but it is simply impossible for them to even imagine to wind a coil which has more than 100 turns. Maybe it is good that there is a variety of people, the article writers and the coil winders and something inbetween :-) Oh, and the programmers! Very important. Without Wolfgang and Paul and Markus we would do nothing at all!
>> Oh BTW maybe i'll transmit on my loop again the next weekend. I can't await it, it is more than 2 weeks ago, a very long time!!
>>
>> I have played with ground loops before and had some good results in
>> LF.
>>
>> On VLF it should work much better (relative to a vertical E field antenna). The idea is that the current runs back in a deep layer (skin depth), depending on the ground conductivity. So it should work better on poor conducting ground.
>>
>>   Once I establish a reference system, I can compare antennas
>> including ground loops. Unlike Europe where you have plenty of people
>> around you, I have to do both the TXing and the RXing and that
>> requires effort and time. The latter is a very scarce resource!
>>
>> Anyway, looks like a nice day today to do some more outdoor work. We
>> had lightning storms and plenty of rain the past few days, so I
>> haven't made any progress.
>>
>>
>> RR, good luck and fun with the new challenges.
>> Looking forward to your next steps and reports.
>>
>> 73, Stefan
>>
>>
>>
>> 73, Dimitris VK2COW
>>
>>
>>
>>
>>      
>    

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From: Domenico IZ7SLZ <iz7slz.domenico@gmail.com>
Date: Thu, 7 Feb 2019 16:38:05 +0100
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 Content preview:  Joe, LF in my EbNaut log *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
    <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>* there are some decodes of your
    EbNaut of last nights (QRB=5426 km). Seems that since ye [...] 
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Subject: LF: VO1NA Ebnaut recently decodes
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--0000000000005e328505814fa3cf
Content-Type: text/plain; charset="UTF-8"

Joe, LF
in my EbNaut log
*https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
<https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
there are some decodes of your EbNaut of last nights (QRB=5426 km). Seems
that since yesterday, only carrier is sent on usual qrg 137477 Hz.
Autodecoder here is now running, every XX:00 and XX:30 on Joe's parameters:

137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s
T_OFFSET=0.0s F_OFFSET=0.000Hz

73, Domenico IZ7SLZ / JN80nu

--0000000000005e328505814fa3cf
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div>Joe, LF<br></div><div>in my EbNaut l=
og</div><div> <b><a href=3D"https://qsl.net/iz7slz/EBNAUT/DECODED.TXT">http=
s://qsl.net/iz7slz/EBNAUT/DECODED.TXT</a></b></div><div>there are some deco=
des of your EbNaut of last nights (QRB=3D5426 km). Seems that since yesterd=
ay, only carrier is sent on usual qrg 137477 Hz.</div><div>Autodecoder here=
 is now running, every XX:00 and XX:30 on Joe&#39;s parameters:</div><div>
<pre>137477.000Hz N=3D7 T=3D3s 8K19A CRC=3D16 list=3D2000 sym=3D608 Duratio=
n=3D1824s
T_OFFSET=3D0.0s F_OFFSET=3D0.000Hz<br>
</pre><pre><font face=3D"arial,helvetica,sans-serif">73, Domenico IZ7SLZ / =
JN80nu</font><br>
</pre></div></div></div>

--0000000000005e328505814fa3cf--

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 Content preview:  Hi ELF ;-) I'm glad to announce that since 15:46 UTC i am
   transmitting on ELF (the real ELF, i.e. into the range of 3...30 Hz, ITU radio
    band 1 <https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first
    [...] 
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Subject: ELF: Carrier on 22.97 Hz
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This is a multi-part message in MIME format.
--------------090806040903080706070406
Content-Type: text/plain; charset=ISO-8859-15; format=flowed
Content-Transfer-Encoding: 7bit

Hi ELF ;-)

I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the 
real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 
<https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first time 
ever.

Here are the parameters:

TX frequency: *22.970 Hz*
Wavelength of that frequency: *13060 km*
Antenna voltage: *4.8 kV rms* (+ a DC component of 7.5 kV)
Antenna current: *325 uA*
ERP: 600 aW, or *6E-16 W*

Call it QRP!
The goal is to detect the signal on my 3.5 km distant tree grabber, 
whose E field is now working again. Since the E field probe is not to 
far above the tree, the effective height is not as much as it should 
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can 
see the Schumann resonances and the 60 Hz power grid. So i hope it will 
work.

A spectrogram which is centered on the frequency of interest in now 
shown at 
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html 
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In 
a few minutes we'll see more :-) It takes about 40 minutes until a peak 
could have fully developed...

73, Stefan


--------------090806040903080706070406
Content-Type: text/html; charset=ISO-8859-15
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<body bgcolor="#ffffff" text="#000000">
Hi ELF ;-)<br>
<br>
I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a
 href="https://en.wikipedia.org/wiki/Radio_spectrum#ITU">ITU radio band
1</a> ) for the first time ever.<br>
<br>
Here are the parameters: <br>
<br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
<br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
<br>
A spectrogram which is centered on the frequency of interest in now
shown at
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
<br>
73, Stefan<br>
<br>
</body>
</html>

--------------090806040903080706070406--

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 Content preview:  Dominico, Thanks to you and Markus and Domenico for the autodecoder
    service. I will check the modulator and try again tonight. Some antenna work
    is planned as well when the wx improves so there should be some m [...] 
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X-Scan-Signature: e09cca6d8e44a91eadbdfb3e1b8aec09
Subject: Re: LF: VO1NA Ebnaut recently decodes
Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed
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Dominico,

Thanks to you and Markus and Domenico for the autodecoder service.
I will check the modulator and try again tonight. Some antenna work
is planned as well when the wx improves so there should be some more
dB available soon.

73
Joe

On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:

> Joe, LF
> in my EbNaut log
> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
> there are some decodes of your EbNaut of last nights (QRB=5426 km). Seems
> that since yesterday, only carrier is sent on usual qrg 137477 Hz.
> Autodecoder here is now running, every XX:00 and XX:30 on Joe's parameters:
>
> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s
> T_OFFSET=0.0s F_OFFSET=0.000Hz
>
> 73, Domenico IZ7SLZ / JN80nu
>

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 Content preview:  Apologies: I misspelt Domenico and did not acknowledge Riccardo's
    autodetector. 73 Joe On Thu, 7 Feb 2019, jcraig@mun.ca wrote: > Dominico,
    > > Thanks to you and Markus and Domenico for the autodecoder service. >
   I will check the modulator and try again tonight. Some antenna work > is planned
    as well when the wx improves so th [...] 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Apologies: I misspelt Domenico and did not acknowledge Riccardo's 
autodetector.
73
Joe

On Thu, 7 Feb 2019, jcraig@mun.ca wrote:

> Dominico,
>
> Thanks to you and Markus and Domenico for the autodecoder service.
> I will check the modulator and try again tonight. Some antenna work
> is planned as well when the wx improves so there should be some more
> dB available soon.
>
> 73
> Joe
>
> On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>
>> Joe, LF
>> in my EbNaut log
>> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>> there are some decodes of your EbNaut of last nights (QRB=5426 km). Seems
>> that since yesterday, only carrier is sent on usual qrg 137477 Hz.
>> Autodecoder here is now running, every XX:00 and XX:30 on Joe's parameters:
>> 
>> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s
>> T_OFFSET=0.0s F_OFFSET=0.000Hz
>> 
>> 73, Domenico IZ7SLZ / JN80nu
>> 
>
>

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Date: Thu, 07 Feb 2019 19:54:49 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  ...wow, after analysing the first 90 minutes of the transmission
    i found that the best SNR is achieved without sferic blanking! So then the
    hum filter and the low pass filter can be disabled too. So f [...] 
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Subject: Re: ELF: Carrier on 22.97 Hz
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...wow, after analysing the first 90 minutes of the transmission i found 
that the best SNR is achieved without sferic blanking! So then the hum 
filter and the low pass filter can be disabled too.
So far, during that noisy evening period, i'm getting about *14 dB SNR 
in 185 uHz.*
Unfortunately i temporarely overloaded the PC while doing the analysis, 
which caused an interruption of the stream and then all SpecLab 
instances did a restart.

Now the spectrogram is generated from the unfiltered and unblanked 
stream and now we can already see a clear peak right on the expected 
frequency, showing about 10 dB SNR.

I intend to run the carrier at least for 24 hours, if all works well. 
Not sure if and how the antenna current will drop when it starts to 
rain. It would have been better to decouple the DC component from the 
antenna by using a big series capacitor but id didn't have one that 
holds 20 kV or so.

More later...

73, Stefan



Am 07.02.2019 17:05, schrieb DK7FC:
> Hi ELF ;-)
>
> I'm glad to announce that since 15:46 UTC i am transmitting on ELF 
> (the real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 
> <https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first 
> time ever.
>
> Here are the parameters:
>
> TX frequency: *22.970 Hz*
> Wavelength of that frequency: *13060 km*
> Antenna voltage: *4.8 kV rms* (+ a DC component of 7.5 kV)
> Antenna current: *325 uA*
> ERP: 600 aW, or *6E-16 W*
>
> Call it QRP!
> The goal is to detect the signal on my 3.5 km distant tree grabber, 
> whose E field is now working again. Since the E field probe is not to 
> far above the tree, the effective height is not as much as it should 
> ideally be, at this frequency, so the RX is somewhat deaf. Anyway i 
> can see the Schumann resonances and the 60 Hz power grid. So i hope it 
> will work.
>
> A spectrogram which is centered on the frequency of interest in now 
> shown at 
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html 
> (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! 
> In a few minutes we'll see more :-) It takes about 40 minutes until a 
> peak could have fully developed...
>
> 73, Stefan
>

--------------010205070004020504000400
Content-Type: text/html; charset=ISO-8859-15
Content-Transfer-Encoding: 7bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=ISO-8859-15"
 http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
...wow, after analysing the first 90 minutes of the transmission i
found that the best SNR is achieved without sferic blanking! So then
the hum filter and the low pass filter can be disabled too.<br>
So far, during that noisy evening period, i'm getting about <b>14 dB
SNR in 185 uHz.</b><br>
Unfortunately i temporarely overloaded the PC while doing the analysis,
which caused an interruption of the stream and then all SpecLab
instances did a restart.<br>
<br>
Now the spectrogram is generated from the unfiltered and unblanked
stream and now we can already see a clear peak right on the expected
frequency, showing about 10 dB SNR.<br>
<br>
I intend to run the carrier at least for 24 hours, if all works well.
Not sure if and how the antenna current will drop when it starts to
rain. It would have been better to decouple the DC component from the
antenna by using a big series capacitor but id didn't have one that
holds 20 kV or so.<br>
<br>
More later...<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 07.02.2019 17:05, schrieb DK7FC:
<blockquote cite="mid:5C5C5757.5080906@posteo.de" type="cite">
  <meta http-equiv="content-type"
 content="text/html; charset=ISO-8859-15">
Hi ELF ;-)<br>
  <br>
I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a moz-do-not-send="true"
 href="https://en.wikipedia.org/wiki/Radio_spectrum#ITU">ITU radio band
1</a> ) for the first time ever.<br>
  <br>
Here are the parameters: <br>
  <br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
  <br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
  <br>
A spectrogram which is centered on the frequency of interest in now
shown at
  <a moz-do-not-send="true" class="moz-txt-link-freetext"
 href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
  <br>
73, Stefan<br>
  <br>
</blockquote>
</body>
</html>

--------------010205070004020504000400--

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 Content preview:  ! ! ! :-)) no words Stefan but... big smail ;-) I figure that
    next step is collecting a bulk of batteries and a shaker to go down to 0,001
    Hz ;-))) amazing.. simply amazing Marco Ik1HSS 
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Subject: R: Re: ELF: Carrier on 22.97 Hz
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------=_Part_69226_6006324.1549569933639
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!
!
!
:-))
no words Stefan but... big smail ;-)
I figure that next step is collecting a bulk of batteries and a shaker to go down to 0,001 Hz ;-)))

amazing.. simply amazing

Marco Ik1HSS



----Messaggio originale----

Da: selberdenken@posteo.de

Data: 7-feb-2019 19.54

A: <rsgb_lf_group@blacksheep.org>

Ogg: Re: ELF: Carrier on 22.97 Hz







...wow, after analysing the first 90 minutes of the transmission i
found that the best SNR is achieved without sferic blanking! So then
the hum filter and the low pass filter can be disabled too.

So far, during that noisy evening period, i'm getting about 14 dB
SNR in 185 uHz.

Unfortunately i temporarely overloaded the PC while doing the analysis,
which caused an interruption of the stream and then all SpecLab
instances did a restart.



Now the spectrogram is generated from the unfiltered and unblanked
stream and now we can already see a clear peak right on the expected
frequency, showing about 10 dB SNR.



I intend to run the carrier at least for 24 hours, if all works well.
Not sure if and how the antenna current will drop when it starts to
rain. It would have been better to decouple the DC component from the
antenna by using a big series capacitor but id didn't have one that
holds 20 kV or so.



More later...



73, Stefan







Am 07.02.2019 17:05, schrieb DK7FC:

  
Hi ELF ;-)

  

I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, ITU radio band
1 ) for the first time ever.

  

Here are the parameters: 

  

TX frequency: 22.970 Hz

Wavelength of that frequency: 13060 km

Antenna voltage: 4.8 kV rms (+ a DC component of 7.5 kV)

Antenna current: 325 uA 

ERP: 600 aW, or 6E-16 W

  

Call it QRP!

The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.

  

A spectrogram which is centered on the frequency of interest in now
shown at
  http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...

  

73, Stefan

  









------=_Part_69226_6006324.1549569933639
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: 7bit

!<br>!<br>!<br>:-))<br>no words Stefan but... big smail ;-)<br>I figure that next step is collecting a bulk of batteries and a shaker to go down to 0,001 Hz ;-)))<br><br>amazing.. simply amazing<br><br>Marco Ik1HSS<br>
<br>
----Messaggio originale----<br>
Da: selberdenken@posteo.de<br>
Data: 7-feb-2019 19.54<br>
A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Ogg: Re: ELF: Carrier on 22.97 Hz<br>
<br>


<!--
  
-->

...wow, after analysing the first 90 minutes of the transmission i
found that the best SNR is achieved without sferic blanking! So then
the hum filter and the low pass filter can be disabled too.<br>
So far, during that noisy evening period, i'm getting about <b>14 dB
SNR in 185 uHz.</b><br>
Unfortunately i temporarely overloaded the PC while doing the analysis,
which caused an interruption of the stream and then all SpecLab
instances did a restart.<br>
<br>
Now the spectrogram is generated from the unfiltered and unblanked
stream and now we can already see a clear peak right on the expected
frequency, showing about 10 dB SNR.<br>
<br>
I intend to run the carrier at least for 24 hours, if all works well.
Not sure if and how the antenna current will drop when it starts to
rain. It would have been better to decouple the DC component from the
antenna by using a big series capacitor but id didn't have one that
holds 20 kV or so.<br>
<br>
More later...<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 07.02.2019 17:05, schrieb DK7FC:
<blockquote cite="mid:5C5C5757.5080906@posteo.de" type="cite">
  
Hi ELF ;-)<br>
  <br>
I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a moz-do-not-send="true" href="https://en.wikipedia.org/wiki/Radio_spectrum#ITU">ITU radio band
1</a> ) for the first time ever.<br>
  <br>
Here are the parameters: <br>
  <br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
  <br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
  <br>
A spectrogram which is centered on the frequency of interest in now
shown at
  <a moz-do-not-send="true" class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
  <br>
73, Stefan<br>
  <br>
</blockquote>


<br>
<br>

------=_Part_69226_6006324.1549569933639--


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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Fri, 8 Feb 2019 08:59:12 +1100
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 Content preview:  Hi Marco and Stefan, Competing with NWC Harold Holt would
   be insanity, regardless of the regulation, that's a frequency to certainly
    avoid :-) You must have a much larger antenna than me as in my current 140
    m^2, 3-turn loop, I can reach a bit over a 1 uW with a 1 kW input! There
   are many physical limitation that cannot be exceeded that will [...] 
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Subject: Re: VLF: in VK?
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Hi Marco and Stefan,

Competing with NWC Harold Holt would be insanity, regardless of the
regulation, that's a frequency to certainly avoid :-)

You must have a much larger antenna than me as in my current 140 m^2,
3-turn loop, I can reach a bit over a 1 uW with a 1 kW input! There
are many physical limitation that cannot be exceeded that will never
allow me 200 uW with this antenna. Of course, that's just the start,
once I get some success, I will be looking for larger antennas (and I
do have some ideas which extend past my fence). You know the
addiction!

Anyway, my plan is to start at 29.999 kHz (the entrance to VLF!)
first. My antenna works a lot better on that frequency. I will them
move down in frequency. For the legal limit of 7.5 uW, what distance
would you expect a QRSS10 signal to cover at 29.99 kHz? We'll find out
this weekend but I can start taking bets today! :-)

73, Dimitris VK2COW

Στις Πέμ, 7 Φεβ 2019 στις 7:21 μ.μ., ο/η DK7FC <selberdenken@posteo.de> έγραψε:
>
> Hi Dimitris,
>
> Interesting, theat LIPD class. So you could even try higher frequencies
> than 8.3 kHz. Here we are not allowed to transmit above 8.3 kHz.
> However, i have a special licence to transmit arround 17.47 kHz, with 5
> mW ERP. On that frequency i have been received by Edgar and we
> transferred a 3 character message successfully some months ago. A 5
> character message almost decoded but in the end we failed.
>
> Why is there is a  gap between 19.95...20.05 kHz? No idea but i would
> have expected a gap arround 19.8 kHz, because of NWC
> https://en.wikipedia.org/wiki/Naval_Communication_Station_Harold_E._Holt
>
> 200 uW on 8.27 kHz is a good signal but with the space you have, you
> could get up to 20 dB more so it is a pity. But anyway, many people
> could detect you at 200 uW, at least in a radius a few 1000 km.
>
> 73, Stefan
>
>
>
> Am 07.02.2019 01:52, schrieb Dimitrios Tsifakis:
> > Ciao Marco,
> >
> > yes, the grass is indeed greener on the other side but I am not
> > complaining about that! If there is no time now, perhaps there will be
> > later! More things to do when I retire, there is nothing worse that
> > people that retire and do nothing...By the way I do look at the legal
> > aspects. We are lucky in Australia our local spectrum authority has
> > made it clear how much we can radiate in the various parts of the
> > spectrum. There is a class licence known as LIPD (low interference
> > potential devices) which tell you how many microwatts you can radiate
> > on VLF and below and it is very generous I think. Here is what we are
> > allowed to do:
> >
> > 0 kHz to 14 kHz        200 uW EIRP
> > 14 kHz to 19.95 kHz   50 uW EIRP
> > 20.05 kHz to 70 kHz  7.5 uW EIRP
> >
> > (note I cannot transmit between 19.95 kHz and 20.05 kHz, not sure why
> > there is that gap)
> >
> > I can live with that!
> >
> > 73, Dimitris VK2COW
> >
> >
> > Στις Πέμ, 7 Φεβ 2019 στις 5:46 π.μ., ο/η marcocadeddu@tin.it
> > <marcocadeddu@tin.it>  έγραψε:
> >
> >> Hi Stefan, Dimitris,
> >>
> >> room is sure a thing that is not missing in VK :-)
> >> I remember a vacation I had there some years ago ... a lot of km between "adiacent places".. so ideal place for LF, VLF and even close to DC frequencies!
> >> During my travel, just for fate, I drove close to Holt Navy Base sporting an antenna just a bit larger than your loop ;-)
> >> Anyway you know the grass of the neighbor is more green...
> >> Dimitris has room but not a lot of time..
> >> I have more time but less room
> >> somebody else has room and time but no money...
> >> What an hard life!
> >> But... we all have fun!
> >>
> >> 73 Marco IK1HSS
> >>
> >> P.S. who's looking the legal aspects?? ;-)
> >>
> >> ----Messaggio originale----
> >> Da: selberdenken@posteo.de
> >> Data: 5-feb-2019 23.40
> >> A:<rsgb_lf_group@blacksheep.org>
> >> Ogg: Re: VLF: in VK?
> >>
> >> Dimitris,
> >>
> >> Am 05.02.2019 21:14, schrieb Dimitrios Tsifakis:
> >>
> >> G'day Stefan and Edgar,
> >>
> >> My house is on QF44OX00OR and the property extends to QF44NX (50 acres
> >> or 200,000 m^2). I do have permission from some neighbours to lay
> >> wires into their properties, so an extra large (over 1km) ground wire
> >> is entirely doable but not at this point in time.
> >>
> >> Wow, i'm envious and happy that you have such possibilities!!!!!!!!!!!!!!
> >> Not at this time, ok. I would suggest to start in small steps anyway, then you can be happy about many improvements, not just a single big one :-)
> >> I often imagine to live in Canada or Australia and do such experiments exactly!
> >>
> >> The reference loop
> >> is from the shed, about 100 metres south of the house, to the tractor
> >> shed.
> >>
> >> 100m is very close, the far field begins at about 5.7 km distance at 8.27 kHz. A RX in that distance is only useful to check and observe the signal stability and compare levels. A feedback monitor like my tree which is 3.5 km distant from my INV-L antenna in the city. From my ground loop antenna in JN39WI it is 57.6 km distant, which is already an interesting distance and can be challenging below 3 kHz.
> >>
> >>   I have mains in the shed and I also have a 200 W audio linear
> >> amplifier to get things started.
> >>
> >> Excellent, just excellent! Your signal could be the stongest of the radio amateurs! 200W is just fine for the first steps. But be careful with those audio amplifiers, they do not seem to like to much reactive power.
> >> For tuning the antenna you will only need a capacitor in series. For my portable VLF system i built a current transformer to produce a small voltage that goes to the soundcard. Then, using SpecLab, i can calculate the antenna current directly and even keep the phase of the current stable, even if there should be a soundcard glitch. For the signal generation i also use SpecLab and a cheap GPS module. It all works very reliable, there were no problems so far.
> >> With a house at one of the ends of the antenna you are in a very comfortable situation! You may already have a ground system there, so the effort is at one end only.
> >>
> >>   I can build a class-E kilowatt if
> >> necessary later. I like the roughly north-south loop configuration as
> >> it favours many large cities (Melbourne, Sydney, Brisbane and Tassie)
> >> and most importantly Canberra which is only 30 km to the South. I will
> >> try to get some signals received in Canberra before I start asking
> >> people further away to have a listen.
> >>
> >> Yes, this is a very good distance to observe your own signal. If you have internet access there and can leave a small PC/notebook/tablet ... then you could build up a webpage and run a grabber from there like i do from my tree (still under maintenance). That would be ideal and it just feels good to see the own signal very clearly on a real RX in a short distance. You are then independent.
> >>
> >>
> >>   I currently have assembled an XO
> >> clocked DDS controlled by an arduino to do the initial tests but later
> >> when I decide to go QRSSSSSI can dig out and use the old rubidium
> >> clock as a reference for extra stability. For receiving I use a 24
> >> bit, 192 kHz USB sound card and spectrum lab (thanks Wolf!). The
> >> antenna I will use for receive is one of those monster ferrite rods.
> >> Amplification may not even be necessary, the signals I get when the
> >> antenna is tuned seem to be already quite good. Once I have a decent
> >> RX antenna I think I will start gifting these rods (I have a few) to
> >> interested amateurs in the region and help them get started with
> >> receiving on VLF. Make a small army of receivers, that would make life
> >> much easier when evaluating antennas!
> >>
> >>
> >> Oh yes! Fortunately there are a few arround here. These days this is (sorted by distance to my VLF loop): DK7FC, DF6NM, DL0AO, DL4YHF, IK1QFK, Paul Nicholson, SQ5BPF and RN3AUS. Oh and W1VD, K3SIW and Edgar J.T. This is about the complete VLF group worldwide, at least those who prooved to detect narrow band (sub mHz) signals close to the limits, in the last 3 years until now.
> >>
> >> Hey, you should document your experiments even if it is a summary of
> >> the activities and nothing more. The list is great but perhaps we are
> >> missing out on many other potentially interested people that may have
> >> not discovered the list.
> >>
> >> Yes, you are right. I had the same thought sometimes. Certainly there are many amateurs who would feel like having a new life when starting at VLF, It is an unknown spectrum for 99.9 % of the amateurs. Actually it is not even amateur radio because it is not a spectrum allocated to amateur radio. So everyone could operate there.
> >> But there is a risk, you know. There are those people who do not simply start to transmit/receive there and feel good. There are those who prefer to ask if this is legal at all. And then they ask here and there, as long as they find someone who triggers their fears and phobs, and then they do nothing at all! Beware of such people, they are contaminating your free mind. Concentrate on ideas and wishes, like for example detecting your own signal in Canberra. And then the question "Will this also work on lower frequencies", for example.
> >> When writing an article in a radio magazine, what will be the result? Will it actually lead to more active people on the band, who transmit and/or receive for a longer time, say at least 5 to 10 years? Or will it rise a short interest only, dominated by people telling it is not legal and so on... I'm not sure about that. It could be even better to stay in a smaller group who can do what it wants instead causing a decision / regulation by an 'authority'.
> >>
> >>   You are clearly not lazy having achieved so
> >> much on MF and below :-)
> >>
> >>
> >> Thanks but i'm lazy into a certain spectrum. On the other side, there are people who write many articles over the years but it is simply impossible for them to even imagine to wind a coil which has more than 100 turns. Maybe it is good that there is a variety of people, the article writers and the coil winders and something inbetween :-) Oh, and the programmers! Very important. Without Wolfgang and Paul and Markus we would do nothing at all!
> >> Oh BTW maybe i'll transmit on my loop again the next weekend. I can't await it, it is more than 2 weeks ago, a very long time!!
> >>
> >> I have played with ground loops before and had some good results in
> >> LF.
> >>
> >> On VLF it should work much better (relative to a vertical E field antenna). The idea is that the current runs back in a deep layer (skin depth), depending on the ground conductivity. So it should work better on poor conducting ground.
> >>
> >>   Once I establish a reference system, I can compare antennas
> >> including ground loops. Unlike Europe where you have plenty of people
> >> around you, I have to do both the TXing and the RXing and that
> >> requires effort and time. The latter is a very scarce resource!
> >>
> >> Anyway, looks like a nice day today to do some more outdoor work. We
> >> had lightning storms and plenty of rain the past few days, so I
> >> haven't made any progress.
> >>
> >>
> >> RR, good luck and fun with the new challenges.
> >> Looking forward to your next steps and reports.
> >>
> >> 73, Stefan
> >>
> >>
> >>
> >> 73, Dimitris VK2COW
> >>
> >>
> >>
> >>
> >>
> >
>


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Date: Fri, 8 Feb 2019 09:15:10 +1100
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 Content preview:  Hi Stefan, that's insane! What's the purpose of the DC offset
    of 7.5 kV? Is the antenna tuned (unlikley) or you are just applying the volts
    from a voltage amplifier? Hope the antenna is well insulated from people
   and nature as skin effect won't save your bacon (unlike the higher frequencies).
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Subject: Re: ELF: Carrier on 22.97 Hz
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Hi Stefan,

that's insane! What's the purpose of the DC offset of 7.5 kV?  Is the
antenna tuned (unlikley) or you are just applying the volts from a
voltage amplifier?

Hope the antenna is well insulated from people and nature as skin
effect won't save your bacon (unlike the higher frequencies).

73, Dimitris VK2COW

Στις Παρ, 8 Φεβ 2019 στις 3:10 π.μ., ο/η DK7FC <selberdenken@posteo.de> έγραψε:
>
> Hi ELF ;-)
>
> I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 ) for the first time ever.
>
> Here are the parameters:
>
> TX frequency: 22.970 Hz
> Wavelength of that frequency: 13060 km
> Antenna voltage: 4.8 kV rms (+ a DC component of 7.5 kV)
> Antenna current: 325 uA
> ERP: 600 aW, or 6E-16 W
>
> Call it QRP!
> The goal is to detect the signal on my 3.5 km distant tree grabber, whose E field is now working again. Since the E field probe is not to far above the tree, the effective height is not as much as it should ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can see the Schumann resonances and the 60 Hz power grid. So i hope it will work.
>
> A spectrogram which is centered on the frequency of interest in now shown at http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In a few minutes we'll see more :-) It takes about 40 minutes until a peak could have fully developed...
>
> 73, Stefan
>


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 Content preview:  Hi Dimitris, ELF, Well, The day has started here, the carrier
    is still there, the antenna current is stable, the tree has still enough
   solar energy, i have some coffee here, it looks a bit blue on the sky, so
   it is a g [...] 
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Hi Dimitris, ELF,

Well, The day has started here, the carrier is still there, the antenna 
current is stable, the tree has still enough solar energy, i have some 
coffee here, it looks a bit blue on the sky, so it is a good start into 
another good day on that planet :-) Good morning!

Well, the PA for this ELF project is quite different to normal RF 
amplifiers. You know, at this frequency (but also als SLF/ULF/VLF, even 
LF) the antenna acts as a pure capacitor. Mine has about 470 pF. At a 
given frequency and capacity you will get a certain antenna current from 
a certain voltage. Since the frequency is so low here, the antenna 
current is below 1 mA, despite the nearly 5 kV rms. So the TX power is 
very low, that's the first thing.

And how do you generate a sine of 5 kV at 23 Hz? You could use a mains 
transformer for 10 kV at 50 Hz and then just go down. But where do you 
get that from? There are some old voltage transformers on ebay, taken 
from 20 kV power grids.
Like this one: 
https://www.ebay.de/itm/MWB-REL20-24-50-2-125kV-90VA-SPANNUNGSWANDLER-POTENTIAL-TRANSFORMER-TRAFO/173246231511?hash=item285647b3d7:g:vqoAAOSwt21av7Vi:rk:1:pf:0
They are heavy and expensive and often do not even handle the required 
voltage. The one above is way to expensive and only handles 20 kV/sqrt3, 
and just at 50 Hz!
OK that would be fine for getting 6 kV at 23 Hz but if the experiment 
works well and i like to try e.g. 9.7 Hz, then the game is over with 
that transformer. It would be a large investment for just one experiment.
So i searched for another solution:

I'm using an old TV transformer (think they are called LOPT in english) 
to produce a high voltage of about 2 kV. The frequency is about 25 kHz. 
The output goes to a homemade Greinacher cascade 
(https://en.wikipedia.org/wiki/Voltage_doubler#Greinacher_circuit) to 
produce a higher DC voltage. In parallel to the output there is a 10 
MOhm HV resistor. This resistor is used to discharge the cascade and to 
build a voltage divider to measure the HV. The transformer is driven by 
a usual SG2535 switch mode regulator (and 2x IRFZ48Z MOSFETs). So i can 
regulate the output voltage (DC) of the cascade. The SG2535 has an 
'error amp' input which allows to control the output voltage by an input 
voltage. I then use a trim pot between the internal v-ref and gnd to set 
an offset in the middle of the regulation range. Then, decoupled by a 
4700 uF capacitor i can apply 23 Hz from the soundcard of my PC. This is 
decoupled by a 5 VA mains transformer, to avoid EMC problems and to rise 
the voltage level a bit.
So actually this is a DC HV supply whose output voltage is quickly 
changed, at 23 Hz. So i can tune from 0...15 kV. The DC offset doesn't 
matter and the AC component radiates a very very very very small signal, 
as we can see!
While trying to keep there series loss resistance as low as possible in 
a LF TX system, i switched 2x 10 kOhm in series to the antenna here! 
This builds a low pass filter (17 kHz corner frequency, i just see i 
could have used 100 kOhm in stead) for the switching frequency. At 325 
uA antenna current, it just 'costs' 0.65 V voltage drop! The transmitter 
consumes 12V*1.5A.
The parts you need to build such stuff is e.g. available at 
https://highvoltageshop.com/ There are very cheap HV diodes and 
capacitors. Very useful and rare!

So, the antenna is not tuned. For a tuned antenna i would need a coil 
which has 102 kH (kilo Henry) My lifetime is not long enough to wind 
such a coil :-)

73, Stefan



Am 07.02.2019 23:15, schrieb Dimitrios Tsifakis:
> Hi Stefan,
>
> that's insane! What's the purpose of the DC offset of 7.5 kV?  Is the
> antenna tuned (unlikley) or you are just applying the volts from a
> voltage amplifier?
>
> Hope the antenna is well insulated from people and nature as skin
> effect won't save your bacon (unlike the higher frequencies).
>
> 73, Dimitris VK2COW
>
> Στις Παρ, 8 Φεβ 2019 στις 3:10 π.μ., ο/η DK7FC<selberdenken@posteo.de>  έγραψε:
>    
>> Hi ELF ;-)
>>
>> I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 ) for the first time ever.
>>
>> Here are the parameters:
>>
>> TX frequency: 22.970 Hz
>> Wavelength of that frequency: 13060 km
>> Antenna voltage: 4.8 kV rms (+ a DC component of 7.5 kV)
>> Antenna current: 325 uA
>> ERP: 600 aW, or 6E-16 W
>>
>> Call it QRP!
>> The goal is to detect the signal on my 3.5 km distant tree grabber, whose E field is now working again. Since the E field probe is not to far above the tree, the effective height is not as much as it should ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can see the Schumann resonances and the 60 Hz power grid. So i hope it will work.
>>
>> A spectrogram which is centered on the frequency of interest in now shown at http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In a few minutes we'll see more :-) It takes about 40 minutes until a peak could have fully developed...
>>
>> 73, Stefan
>>
>>      
>    

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 Content preview:  LF EbNaut, I will run an LF EbNaut beacon this weekend from
    8 Feb - 10 Feb (3 days) as follows: QRG: 137479.000 Hz Code: 8K19A CRC: 16
    Symbol: 3 sec Char: 7 Duration: 30:24.0 (1824 sec) Start/Stop: 2100 UTC /
    1100 UTC (last) Repeat on the hour with carrier during idle. 1W EIRP. 10
   min CW ID (20 [...] 
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LF EbNaut,

I will run an LF EbNaut beacon this weekend from 8 Feb - 10 Feb (3 days) as follows:

QRG:  137479.000 Hz
Code:  8K19A
CRC: 16
Symbol:  3 sec
Char:  7
Duration:  30:24.0 (1824 sec)
Start/Stop:  2100 UTC / 1100 UTC (last)
Repeat on the hour with carrier during idle.  1W EIRP.  10 min CW ID (20 WPM) on modulated and unmodulated carrier.

73,
Rob - K3RWR
FM18qi


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 Content preview:  Hi Dimitris, Am 07.02.2019 22:59, schrieb Dimitrios Tsifakis:
    > You must have a much larger antenna than me as in my current 140 m^2, >
    3-turn loop, I can reach a bit over a 1 uW with a 1 kW input! On which freque
    [...] 
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Hi Dimitris,

Am 07.02.2019 22:59, schrieb Dimitrios Tsifakis:
> You must have a much larger antenna than me as in my current 140 m^2,
> 3-turn loop, I can reach a bit over a 1 uW with a 1 kW input!
On which frequency? Didn't you tell about a 120m x 3m single turn loop?
>   There
> are many physical limitation that cannot be exceeded that will never
> allow me 200 uW with this antenna. Of course, that's just the start,
> once I get some success, I will be looking for larger antennas (and I
> do have some ideas which extend past my fence).
One of the first steps could also be to place a receiver in the far 
field, a good receiver. You are working in Canberra, right? So you can 
place a RX there and make a webpage showing spectrograms?
Ah BTW are you skilled with Linux or do you arlready know that you'll 
never give it a try?

>   You know the
> addiction!
>    
Hehe, yes!
I already looked arround in your location. It is a QTH for dreamers! You 
know the history about the 'DREAMERS'? ;-)
What is that stuff in QF44OX02XI <http://k7fry.com/grid/?qth=QF44OX02XI> 
? Is it water? Or there in QF44OX01US 
<http://k7fry.com/grid/?qth=QF44OX01US> ? Water, that is water! Horray!! 
There you could throw some wire into, your aluminium wire.
Oh and here in QF44NW99XV <http://k7fry.com/grid/?qth=QF44NW99XV>  
That's excellent! There is just a little effort and you will be able to 
leave a trace on Edgars RX, TXing with 200 uW.
If you can lay a wire from here to there, see 
http://k7fry.com/grid/?qth=QF44OX01US&from=QF44NW99XV that's 1000m 
already and you can get a good conductivity. Try to find metallic 
plates, maybe 1 sqare metre. That could work fine. 1 km is not so much, 
you could even roll it up again after transmitting.
It would be interesting to see how much current you can get at DC or at 
various frequencies up to 30 kHz.

> Anyway, my plan is to start at 29.999 kHz (the entrance to VLF!)
> first. My antenna works a lot better on that frequency. I will them
> move down in frequency. For the legal limit of 7.5 uW, what distance
> would you expect a QRSS10 signal to cover at 29.99 kHz? We'll find out
> this weekend but I can start taking bets today! :-)
>    
If you have a well working RX, sensitive antenna, both H field, the 
right position and 'no' nearby QRM sources, it think you can make 10 km. 
That's my guess, without doing calculations.
If you run 50 uW on 17.47 kHz (Edgar is skilled on that frequency!) you 
will reach Edgar, if your loop points into his direction. If you can run 
just 500 mA into that 1 km long wire, on that frequency, you will be there!
Do you have enough wire for the weekend? :-) I use that cheap CCA 
loudspeaker cable which has 0.75 mm2. A 100m ring (i.e. 2x 100m) costs 
about 13 EUR here, quite affordable.

73, Stefan
> 73, Dimitris VK2COW
>

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Hi Dimitris,<br>
<br>
Am 07.02.2019 22:59, schrieb Dimitrios Tsifakis:
<blockquote
 cite="mid:CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com"
 type="cite">
  <pre wrap="">You must have a much larger antenna than me as in my current 140 m^2,
3-turn loop, I can reach a bit over a 1 uW with a 1 kW input!</pre>
</blockquote>
On which frequency? Didn't you tell about a 120m x 3m single turn loop?<br>
<blockquote
 cite="mid:CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com"
 type="cite">
  <pre wrap=""> There
are many physical limitation that cannot be exceeded that will never
allow me 200 uW with this antenna. Of course, that's just the start,
once I get some success, I will be looking for larger antennas (and I
do have some ideas which extend past my fence).</pre>
</blockquote>
One of the first steps could also be to place a receiver in the far
field, a good receiver. You are working in Canberra, right? So you can
place a RX there and make a webpage showing spectrograms?<br>
Ah BTW are you skilled with Linux or do you arlready know that you'll
never give it a try?<br>
<br>
<blockquote
 cite="mid:CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com"
 type="cite">
  <pre wrap=""> You know the
addiction!
  </pre>
</blockquote>
Hehe, yes! <br>
I already looked arround in your location. It is a QTH for dreamers!
You know the history about the 'DREAMERS'? ;-)<br>
What is that stuff in <a href="http://k7fry.com/grid/?qth=QF44OX02XI">QF44OX02XI</a>
? Is it water? Or there in <a
 href="http://k7fry.com/grid/?qth=QF44OX01US">QF44OX01US</a> ? Water,
that is water! Horray!! There you could throw some wire into, your
aluminium wire. <br>
Oh and here in <a href="http://k7fry.com/grid/?qth=QF44NW99XV">QF44NW99XV</a> 
That's excellent! There is just a little effort and you will be able to
leave a trace on Edgars RX, TXing with 200 uW.<br>
If you can lay a wire from here to there, see
<a class="moz-txt-link-freetext" href="http://k7fry.com/grid/?qth=QF44OX01US&amp;from=QF44NW99XV">http://k7fry.com/grid/?qth=QF44OX01US&amp;from=QF44NW99XV</a> that's 1000m
already and you can get a good conductivity. Try to find metallic
plates, maybe 1 sqare metre. That could work fine. 1 km is not so much,
you could even roll it up again after transmitting.<br>
It would be interesting to see how much current you can get at DC or at
various frequencies up to 30 kHz.<br>
<br>
<blockquote
 cite="mid:CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com"
 type="cite">
  <pre wrap="">Anyway, my plan is to start at 29.999 kHz (the entrance to VLF!)
first. My antenna works a lot better on that frequency. I will them
move down in frequency. For the legal limit of 7.5 uW, what distance
would you expect a QRSS10 signal to cover at 29.99 kHz? We'll find out
this weekend but I can start taking bets today! :-)
  </pre>
</blockquote>
If you have a well working RX, sensitive antenna, both H field, the
right position and 'no' nearby QRM sources, it think you can make 10
km. That's my guess, without doing calculations.<br>
If you run 50 uW on 17.47 kHz (Edgar is skilled on that frequency!) you
will reach Edgar, if your loop points into his direction. If you can
run just 500 mA into that 1 km long wire, on that frequency, you will
be there!<br>
Do you have enough wire for the weekend? :-) I use that cheap CCA
loudspeaker cable which has 0.75 mm2. A 100m ring (i.e. 2x 100m) costs
about 13 EUR here, quite affordable.<br>
<br>
73, Stefan<br>
<blockquote
 cite="mid:CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com"
 type="cite">
  <pre wrap="">
73, Dimitris VK2COW</pre>
  <br>
</blockquote>
</body>
</html>

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 Content preview:  Hi Tom, das kriegen wir noch hin dass Du auf 82 Hz bei DL0AO
    erscheinst...73 von Markus  ------ Originalnachricht------Von: DK7FCDatum:
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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Sat, 9 Feb 2019 09:01:47 +1100
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 Content preview:  Hi Stefan and VLF, well, I am now officially hooked! My signal
    on 29.5 kHz (VLF's edge) has been detected 22.3 km away in Canberra by Dale
    VK1DSH. Only casualty is the russian mica capacitors (K31-11-3) which got
    really [...] 
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Subject: Re: VLF: in VK?
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Hi Stefan and VLF,

well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)
has been detected 22.3 km away in Canberra by Dale VK1DSH. Only
casualty is the russian mica capacitors (K31-11-3) which got really
hot (I was focusing on the amplifier and neglected the poor caps). I
had 4 of them in parallel, each 4700 pF.  Maybe they will recover if I
let them cool down :-)

That's probably a first for Australia, I haven't heard anyone else
doing tests like this.

I now have to wait for properly sized caps that should be coming in
the mail.. Then we can continue the exploration of VLF :-)

73, Dimitris VK2COW


Στις Σάβ, 9 Φεβ 2019 στις 1:20 π.μ., ο/η DK7FC <selberdenken@posteo.de> έγραψε:
>
> Hi Dimitris,
>
> Am 07.02.2019 22:59, schrieb Dimitrios Tsifakis:
>
> You must have a much larger antenna than me as in my current 140 m^2,
> 3-turn loop, I can reach a bit over a 1 uW with a 1 kW input!
>
> On which frequency? Didn't you tell about a 120m x 3m single turn loop?
>
>  There
> are many physical limitation that cannot be exceeded that will never
> allow me 200 uW with this antenna. Of course, that's just the start,
> once I get some success, I will be looking for larger antennas (and I
> do have some ideas which extend past my fence).
>
> One of the first steps could also be to place a receiver in the far field, a good receiver. You are working in Canberra, right? So you can place a RX there and make a webpage showing spectrograms?
> Ah BTW are you skilled with Linux or do you arlready know that you'll never give it a try?
>
>  You know the
> addiction!
>
>
> Hehe, yes!
> I already looked arround in your location. It is a QTH for dreamers! You know the history about the 'DREAMERS'? ;-)
> What is that stuff in QF44OX02XI ? Is it water? Or there in QF44OX01US ? Water, that is water! Horray!! There you could throw some wire into, your aluminium wire.
> Oh and here in QF44NW99XV  That's excellent! There is just a little effort and you will be able to leave a trace on Edgars RX, TXing with 200 uW.
> If you can lay a wire from here to there, see http://k7fry.com/grid/?qth=QF44OX01US&from=QF44NW99XV that's 1000m already and you can get a good conductivity. Try to find metallic plates, maybe 1 sqare metre. That could work fine. 1 km is not so much, you could even roll it up again after transmitting.
> It would be interesting to see how much current you can get at DC or at various frequencies up to 30 kHz.
>
> Anyway, my plan is to start at 29.999 kHz (the entrance to VLF!)
> first. My antenna works a lot better on that frequency. I will them
> move down in frequency. For the legal limit of 7.5 uW, what distance
> would you expect a QRSS10 signal to cover at 29.99 kHz? We'll find out
> this weekend but I can start taking bets today! :-)
>
>
> If you have a well working RX, sensitive antenna, both H field, the right position and 'no' nearby QRM sources, it think you can make 10 km. That's my guess, without doing calculations.
> If you run 50 uW on 17.47 kHz (Edgar is skilled on that frequency!) you will reach Edgar, if your loop points into his direction. If you can run just 500 mA into that 1 km long wire, on that frequency, you will be there!
> Do you have enough wire for the weekend? :-) I use that cheap CCA loudspeaker cable which has 0.75 mm2. A 100m ring (i.e. 2x 100m) costs about 13 EUR here, quite affordable.
>
> 73, Stefan
>
> 73, Dimitris VK2COW
>
>


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 Content preview:  the BIA NDB at Rzesz�w Airport has been switched off a few
    months ago. now i know it's permanent. a VOR/DME is being installed to replace
    it. so no more signal on 473 kHz, 475 kHz and 474kHz. this has been a very
    useful beacon for testing equipment on 630m. 
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Subject: LF: BIA 474kHz is QRT
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the BIA NDB at Rzesz�w Airport has been switched off a few months ago. now 
i know it's permanent. a VOR/DME is being installed to replace it.

so no more signal on 473 kHz, 475 kHz and 474kHz. this has been a very 
useful beacon for testing equipment on 630m.

the upside is that now it's possible to have qsos in the cw segment 
without a narrow 300Hz filter.

antenna photo here:
https://klubnl.pl/wpr/en/index.php/2019/02/09/ndb-bia-qrt/

VY 73

Jacek / SQ5BPF

--17435139-1690595864-1549698346=:725--

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Message-ID: <5C5EC1CA.5000209@posteo.de>
Date: Sat, 09 Feb 2019 13:04:26 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hello Rob, I did not expect to receive you at all because
   my local ELF transmission is causing some QRM on the 20m distant LF RX antenna.
    Anyway! Even two decodes, at 4 UTC and 5 UTC. Best one in the attachment.
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                             [185.67.36.65 listed in list.dnswl.org]
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Subject: Re: LF: K3RWR LF EbNaut Beacon
Content-Type: multipart/mixed;
 boundary="------------080404080503020903000503"
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This is a multi-part message in MIME format.
--------------080404080503020903000503
Content-Type: text/plain; charset=ISO-8859-1; format=flowed
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Hello Rob,

I did not expect to receive you at all because my local ELF transmission 
is causing some QRM on the 20m distant LF RX antenna.
Anyway! Even two decodes, at 4 UTC and 5 UTC. Best one in the attachment.

73, Stefan



Am 08.02.2019 12:15, schrieb Rob Renoud:
> LF EbNaut,
>
> I will run an LF EbNaut beacon this weekend from 8 Feb - 10 Feb (3 days) as follows:
>
> QRG:  137479.000 Hz
> Code:  8K19A
> CRC: 16
> Symbol:  3 sec
> Char:  7
> Duration:  30:24.0 (1824 sec)
> Start/Stop:  2100 UTC / 1100 UTC (last)
> Repeat on the hour with carrier during idle.  1W EIRP.  10 min CW ID (20 WPM) on modulated and unmodulated carrier.
>
> 73,
> Rob - K3RWR
> FM18qi
>
>    

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 Content preview:  Hi Dimitris, My congrats! That is a good success and progress!
    Can you tell more details? How much power was used? How much antenna current?
    Was it the 3 turn loop? What type of receiver was used on the RX site? Is
    that site in a quiet location? Which bandwidth o [...] 
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Hi Dimitris,

My congrats! That is a good success and progress!

Can you tell more details?
How much power was used?
How much antenna current?
Was it the 3 turn loop?
What type of receiver was used on the RX site?
Is that site in a quiet location?
Which bandwidth or mode?
Was it actually QRSS-10 (Which i would watch in 122 mHz)?
What was the SNR?
Is there a screenshot for us to see?
What is your plan for today? :-)
Who is the next distant station?

This could be the beginning of a growing worldwide VLF activity, if you 
can 'mobilise' a team of stations who build up RX and TX systems arround 
VK.

73, Stefan


Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:
> Hi Stefan and VLF,
>
> well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)
> has been detected 22.3 km away in Canberra by Dale VK1DSH. Only
> casualty is the russian mica capacitors (K31-11-3) which got really
> hot (I was focusing on the amplifier and neglected the poor caps). I
> had 4 of them in parallel, each 4700 pF.  Maybe they will recover if I
> let them cool down :-)
>
> That's probably a first for Australia, I haven't heard anyone else
> doing tests like this.
>

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Sun, 10 Feb 2019 08:37:11 +1100
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Subject: Re: VLF: in VK?
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Hi Stefan,

> Can you tell more details?

Yes, see answers below!

> How much power was used?

The amplifier output power was about 50 W.

> How much antenna current?

Calculated current based on measured parameters about 2.2 A RMS

> Was it the 3 turn loop?

Yes!

> What type of receiver was used on the RX site?

E-field antenna (miniwhip) to an upconverter and HF receiver.

> Is that site in a quiet location?

Not particularly (it's in the suburbs) but VK1DSH reported it was a
relatively quiet morning.

> Which bandwidth or mode?
> Was it actually QRSS-10 (Which i would watch in 122 mHz)?

He was using spectran at QRSS30 setting,  0.042 Hz.

> What was the SNR?
> Is there a screenshot for us to see?

yes, see here: http://people.physics.anu.edu.au/~dxt103/pics/Dimitris_0004.jpg

Not stellar SNR but the radiated power I reported originally (7.5 uW)
is not correct. I think the capacitors have sustained some damage
because they seem to introduce a series R of about 6 ohm! After I
adjusted for that extra R, I now think that my radiated power was
closer to 2.3 uW. No wonder they got hot, poor things!! So if I fix
that problem I will gain another ~ 5dB for the same amplifier power.

> What is your plan for today? :-)
> Who is the next distant station?

The plan is to try to improve the SNR at the same location by using
better capacitors. Now that we are certain we are in the far field
(over 2 lambda), we can easily calculate how the signal will attenuate
over greater distances and eventually, when I am happy with the
stability of the system, I will get Edgar to do his magic!

> This could be the beginning of a growing worldwide VLF activity, if you
> can 'mobilise' a team of stations who build up RX and TX systems arround
> VK.

Yes, I have that in my mind. I am planning to donate a few of the
large ferrite bars to local hams that are interested in setting up a
VLF RX station. The relative immunity of the H-field antenna to noise
in the urban environment gives it a small advantage compared to the
E-field ones. I found that about 150 turns of wire on that ferrite
make a good general purpose untuned antenna which if desired can be
tuned to achieve better results.

What do you think of the plan? :-)

73, Dimitris VK2COW

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From: Rob Renoud <k3rwr@md.metrocast.net>
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 Content preview:  Stefan, Thanks for the report - I think TA signals are on
   the decline as we enter the winter/spring transition! K3SIW also reported
   multiple decodes over the much shorter North American path. Running again
   tonight with a new message. 
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Subject: Re: LF: K3RWR LF EbNaut Beacon
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Stefan,

Thanks for the report - I think TA signals are on the decline as we enter the winter/spring transition!  K3SIW also reported multiple decodes over the much shorter North American path.

Running again tonight with a new message.

Tnx & 73,
Rob - K3RWR



> On Feb 9, 2019, at 07:04, DK7FC <selberdenken@posteo.de> wrote:
> 
> Hello Rob,
> 
> I did not expect to receive you at all because my local ELF transmission is causing some QRM on the 20m distant LF RX antenna.
> Anyway! Even two decodes, at 4 UTC and 5 UTC. Best one in the attachment.
> 
> 73, Stefan
> 
> 
> 
> Am 08.02.2019 12:15, schrieb Rob Renoud:
>> LF EbNaut,
>> 
>> I will run an LF EbNaut beacon this weekend from 8 Feb - 10 Feb (3 days) as follows:
>> 
>> QRG:  137479.000 Hz
>> Code:  8K19A
>> CRC: 16
>> Symbol:  3 sec
>> Char:  7
>> Duration:  30:24.0 (1824 sec)
>> Start/Stop:  2100 UTC / 1100 UTC (last)
>> Repeat on the hour with carrier during idle.  1W EIRP.  10 min CW ID (20 WPM) on modulated and unmodulated carrier.
>> 
>> 73,
>> Rob - K3RWR
>> FM18qi
>> 
>>   
> <K3RWR.png>



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From: Michel Brunel <f5wk@mterrier.net>
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 Content preview:  Hi Rob, I guess you didn't receive the report (too big attachment
    ?) I sent you this morning. I got 8 easy decodes, one every hour starting
    from 0:00 TU please confirm your direct email. Michel - f5wk 
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Subject: Re: LF: K3RWR LF EbNaut Beacon
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------------09D050043250ADABC
Content-Type: text/plain; charset=windows-1252
Content-Transfer-Encoding: quoted-printable

Hi Rob,

I guess you didn't receive the report (too big attachment ?)  I sent you th=
is morning.
I got 8 easy decodes, one every hour starting from 0:00 TU=20
please confirm your direct email.

Michel - f5wk

Le samedi 9 f=E9vrier 2019 =E0 22:39:37, Rob =E9crivait :

> Stefan,

> Thanks for the report - I think TA signals are on the decline as we enter
> the winter/spring transition!  K3SIW also reported multiple decodes over
> the much shorter North American path.

> Running again tonight with a new message.

> Tnx & 73,
> Rob - K3RWR



>> On Feb 9, 2019, at 07:04, DK7FC <selberdenken@posteo.de> wrote:

>> Hello Rob,

>> I did not expect to receive you at all because my local ELF transmission=
 is causing some QRM on the 20m distant LF RX antenna.
>> Anyway! Even two decodes, at 4 UTC and 5 UTC. Best one in the attachment.

>> 73, Stefan



>> Am 08.02.2019 12:15, schrieb Rob Renoud:
>>> LF EbNaut,

>>> I will run an LF EbNaut beacon this weekend from 8 Feb - 10 Feb (3 days=
) as follows:

>>> QRG:  137479.000 Hz
>>> Code:  8K19A
>>> CRC: 16
>>> Symbol:  3 sec
>>> Char:  7
>>> Duration:  30:24.0 (1824 sec)
>>> Start/Stop:  2100 UTC / 1100 UTC (last)
>>> Repeat on the hour with carrier during idle.  1W EIRP.  10 min CW ID (2=
0 WPM) on modulated and unmodulated carrier.

>>> 73,
>>> Rob - K3RWR
>>> FM18qi

>>>  =20
>> <K3RWR.png>





-- 
------------09D050043250ADABC
Content-Type: text/html; charset=windows-1252
Content-Transfer-Encoding: quoted-printable

<html><head><title>Re: LF: K3RWR LF EbNaut Beacon</title>
</head>
<body>
<span style=3D" font-family:'Calibri'; font-size: 12pt;">Hi Rob,<br>
<br>
I guess you didn't receive the report (too big attachment ?) &nbsp;I sent y=
ou this morning.<br>
I got 8 easy decodes, one every hour starting from 0:00 TU <br>
please confirm your direct email.<br>
<br>
Michel - f5wk<br>
<br>
Le samedi 9 f&#233;vrier 2019 &#224; 22:39:37, Rob &#233;crivait :<br>
<br>
<span style=3D" font-family:'courier new'; font-size: 9pt; color: #800000;"=
><b>&gt; Stefan,<br>
<br>
&gt; Thanks for the report - I think TA signals are on the decline as we en=
ter<br>
&gt; the winter/spring transition! &nbsp;K3SIW also reported multiple decod=
es over<br>
&gt; the much shorter North American path.<br>
<br>
&gt; Running again tonight with a new message.<br>
<br>
&gt; Tnx &amp; 73,<br>
&gt; Rob - K3RWR<br>
<br>
<br>
<br>
<span style=3D" color: #800080;">&gt;&gt; On Feb 9, 2019, at 07:04, DK7FC &=
lt;</span></b></span></span><a style=3D" font-family:'courier new'; font-si=
ze: 9pt;" href=3D"mailto:selberdenken@posteo.de">selberdenken@posteo.de</a>=
<span style=3D" font-family:'courier new'; font-size: 9pt; color: #800080;"=
><b>&gt; wrote:<br>
<br>
&gt;&gt; Hello Rob,<br>
<br>
&gt;&gt; I did not expect to receive you at all because my local ELF transm=
ission is causing some QRM on the 20m distant LF RX antenna.<br>
&gt;&gt; Anyway! Even two decodes, at 4 UTC and 5 UTC. Best one in the atta=
chment.<br>
<br>
&gt;&gt; 73, Stefan<br>
<br>
<br>
<br>
&gt;&gt; Am 08.02.2019 12:15, schrieb Rob Renoud:<br>
<span style=3D" color: #800000;">&gt;&gt;&gt; LF EbNaut,<br>
<br>
&gt;&gt;&gt; I will run an LF EbNaut beacon this weekend from 8 Feb - 10 Fe=
b (3 days) as follows:<br>
<br>
&gt;&gt;&gt; QRG: &nbsp;137479.000 Hz<br>
&gt;&gt;&gt; Code: &nbsp;8K19A<br>
&gt;&gt;&gt; CRC: 16<br>
&gt;&gt;&gt; Symbol: &nbsp;3 sec<br>
&gt;&gt;&gt; Char: &nbsp;7<br>
&gt;&gt;&gt; Duration: &nbsp;30:24.0 (1824 sec)<br>
&gt;&gt;&gt; Start/Stop: &nbsp;2100 UTC / 1100 UTC (last)<br>
&gt;&gt;&gt; Repeat on the hour with carrier during idle. &nbsp;1W EIRP. &n=
bsp;10 min CW ID (20 WPM) on modulated and unmodulated carrier.<br>
<br>
&gt;&gt;&gt; 73,<br>
&gt;&gt;&gt; Rob - K3RWR<br>
&gt;&gt;&gt; FM18qi<br>
<br>
&gt;&gt;&gt; &nbsp; <br>
<span style=3D" color: #800080;">&gt;&gt; &lt;K3RWR.png&gt;<br>
<br>
<br>
<br>
<br>
<br>
</span></span></b><span style=3D" font-family:'arial'; font-size: 8pt; colo=
r: #c0c0c0;"><i>-- </body></html>
------------09D050043250ADABC--


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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Sun, 10 Feb 2019 09:58:49 +1100
Message-ID: <CAKvcm2dKftWUWFe0PagmCakDCgvRe-nuWDf0Qd4FquuoHJa12g@mail.gmail.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  > Not stellar SNR but the radiated power I reported originally
    (7.5 uW) > is not correct. I think the capacitors have sustained some damage
    > because they seem to introduce a series R of about 6 ohm! [...] 
 Content analysis details:   (0.0 points, 5.0 required)
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> Not stellar SNR but the radiated power I reported originally (7.5 uW)
> is not correct. I think the capacitors have sustained some damage
> because they seem to introduce a series R of about 6 ohm! After I
> adjusted for that extra R, I now think that my radiated power was
> closer to 2.3 uW. No wonder they got hot, poor things!! So if I fix
> that problem I will gain another ~ 5dB for the same amplifier power.

Well, what do you know! The unexpected losses are not just the
capacitors (their contribution is probably small). It is also the
coaxial cable that I used between the antenna feedpoint and the
amplifier. One of the cables uses copper plated steel as the inner
core (which of course has a plating depth appropriate for the expected
skin effect at the _intended_ frequency of operation), the other has
copper plated aluminium (I think!). Even the jumper leads I used have
losses and it all adds up. I now appreciate the problem of using a
very low impedance antenna! Perhaps I should install another
transmission line from the inside of the house to the antenna but not
like the others, I should get the thickest speaker cable I can find
and use that :-)

73, Dimitris VK2COW

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From: "marcocadeddu@tin.it" <marcocadeddu@tin.it>
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 Content preview:  Compliments for the new success you achieved Dimitris :-)))
    I'm not an expert of VLF thus my opinion could very wrong.. 1) if the caps
    exhibit a series resistance of 6 ohms at 2 Amperes (RF? it is almost DC hihi)
    they have to dissipate about 25W so they have a [...] 
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Subject: R: Re: VLF: in VK?
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Compliments for the new success you achieved Dimitris :-)))

I'm not an expert of VLF thus my opinion could very wrong..
1) if the caps exhibit a series resistance of 6 ohms at 2 Amperes (RF? it is almost DC hihi) they have to dissipate about 25W so they have all the rights to be warm! You should try to add more caps in parallel (if they are not tuning the antenna) or serie /parallel if they tune the antenna in order to reduce the resistance and improve the current capability.
2) how long is the coax from TX to antenna? it is probably a very small fraction of wavelenght so its mismatch should be negligible. Of course if there are problems in the connections or the material used for cable manifacture this is an ohmic matter as you pointed out ;-). Be careful low loss speaker cable are veeeeery expensive even when they are not really made of Litz wire ....
You coud do your own coax in BC style with standard power cord and spacers ;-)

73, Marco IK1HSS 



----Messaggio originale----
Da: dtsifakis@gmail.com
Data: 9-feb-2019 23.58
A: <rsgb_lf_group@blacksheep.org>
Ogg: Re: VLF: in VK?

> Not stellar SNR but the radiated power I reported originally (7.5 uW)
> is not correct. I think the capacitors have sustained some damage
> because they seem to introduce a series R of about 6 ohm! After I
> adjusted for that extra R, I now think that my radiated power was
> closer to 2.3 uW. No wonder they got hot, poor things!! So if I fix
> that problem I will gain another ~ 5dB for the same amplifier power.

Well, what do you know! The unexpected losses are not just the
capacitors (their contribution is probably small). It is also the
coaxial cable that I used between the antenna feedpoint and the
amplifier. One of the cables uses copper plated steel as the inner
core (which of course has a plating depth appropriate for the expected
skin effect at the _intended_ frequency of operation), the other has
copper plated aluminium (I think!). Even the jumper leads I used have
losses and it all adds up. I now appreciate the problem of using a
very low impedance antenna! Perhaps I should install another
transmission line from the inside of the house to the antenna but not
like the others, I should get the thickest speaker cable I can find
and use that :-)

73, Dimitris VK2COW





------=_Part_4925_5257539.1549788450174
Content-Type: text/html;charset="UTF-8"
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Compliments for the new success you achieved Dimitris :-)))<br><br>I'm not =
an expert of VLF thus my opinion could very wrong..<br>1) if the caps exhib=
it a series resistance of 6 ohms at 2 Amperes (RF? it is almost DC hihi) th=
ey have to dissipate about 25W so they have all the rights to be warm! You =
should try to add more caps in parallel (if they are not tuning the antenna=
) or serie /parallel if they tune the antenna in order to reduce the resist=
ance and improve the current capability.<br>2) how long is the coax from TX=
 to antenna? it is probably a very small fraction of wavelenght so its mism=
atch should be negligible. Of course if there are problems in the connectio=
ns or the material used for cable manifacture this is an ohmic matter as yo=
u pointed out ;-). Be careful low loss speaker cable are veeeeery expensive=
 even when they are not really made of Litz wire ....<br>You coud do your o=
wn coax in BC style with standard power cord and spacers ;-)<br><br>73, Mar=
co IK1HSS <br>
<br>
----Messaggio originale----<br>Da: dtsifakis@gmail.com<br>Data: 9-feb-2019 =
23.58<br>A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>Ogg: Re: VLF: in VK?<br=
><br>&gt; Not stellar SNR but the radiated power I reported originally (7.5=
 uW)<br>&gt; is not correct. I think the capacitors have sustained some dam=
age<br>&gt; because they seem to introduce a series R of about 6 ohm! After=
 I<br>&gt; adjusted for that extra R, I now think that my radiated power wa=
s<br>&gt; closer to 2.3 uW. No wonder they got hot, poor things!! So if I f=
ix<br>&gt; that problem I will gain another ~ 5dB for the same amplifier po=
wer.<br><br>Well, what do you know! The unexpected losses are not just the<=
br>capacitors (their contribution is probably small). It is also the<br>coa=
xial cable that I used between the antenna feedpoint and the<br>amplifier. =
One of the cables uses copper plated steel as the inner<br>core (which of c=
ourse has a plating depth appropriate for the expected<br>skin effect at th=
e _intended_ frequency of operation), the other has<br>copper plated alumin=
ium (I think!). Even the jumper leads I used have<br>losses and it all adds=
 up. I now appreciate the problem of using a<br>very low impedance antenna!=
 Perhaps I should install another<br>transmission line from the inside of t=
he house to the antenna but not<br>like the others, I should get the thicke=
st speaker cable I can find<br>and use that :-)<br><br>73, Dimitris VK2COW<=
br><br><br><br>

------=_Part_4925_5257539.1549788450174--


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 Content preview:  *Feb 9-10 Best QRB/reports OP32 / OPds :* 21:27 136 R7NT de
    EB8ARZ Op32 *5153* km -30 dB F:0% in Tenerife, Canary Island. 1541,0 Hz with
    200w + E.sLoop (9) 04:33 136 R7NT de G0LUJ Op32 *3009* km -35 d [...] 
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Subject: LF: Feb 9-10 Best QRB/reports
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--0000000000009d25050581869af8
Content-Type: text/plain; charset="UTF-8"

*Feb 9-10  Best QRB/reports OP32 / OPds :*
21:27    136 R7NT de EB8ARZ Op32 *5153* km -30 dB F:0% in Tenerife, Canary
Island. 1541,0 Hz with 200w + E.sLoop (9)
04:33    136 R7NT de G0LUJ Op32 *3009* km -35 dB F:8% in Lytham, England
1541.5 Hz with 200w + E.sLoop (4)
23:05    136 R7NT de PA0RDT Op32 *2574* km -34 dB F:1% in Middelburg,
Netherlands 1541,9 Hz with 200w + E.sLoop (11)
22:32    136 R7NT de PA0LSB Op32 *2482* km -28 dB F:8% in Waspik 1541,8 Hz
with 200w + E.sLoop (13)
02:55    136 R7NT de I55387FI Op32 *2259* km -37 dB F:3% in Riotorto (LI) -
ITALY - Antenna :Mini-Whip 1541,1 Hz with 200w + E. (15)
01:49    136 R7NT de SM2DJK Op32 *2178* km -30 dB F:2% in Umea 1541,0 Hz
with 200w + E.sLoop (20)
2019-02-10 02:55:03 R7NT    *2060* km 137540.998Hz  64mHz -28.3dBOp  89%
20.0dB DF6NM (26)
2019-02-10 02:55:06 R7NT    *2012* km 137541.018Hz 105mHz -25.0dBOp  87%
20.4dB DL0AO (25)
2019-02-09 20:54:25 R7NT    *1876* km 137540.998Hz  60mHz -28.1dBOp  73%
19.2dB IZ7SLZ (24)
2019-02-09 21:59:58 R7NT    *1811* km 137540.874Hz 104mHz -29.5dBOp  87%
19.8dB SV8RV (19)
21:27    136 R7NT de SV8RV Op32 *1809* km -30 dB F:10% in Zakynthos(Zante)
isl. GREECE 1540,9 Hz with 200w + E.sLoop (23)
2019-02-09 21:32:32 RK2Y    *1658* km 137533.680Hz   2mHz -42.4dBOp  89%
19.0dB DF6NM (1)
2019-02-09 21:32:35 RK2Y    *1612* km 137533.680Hz   3mHz -47.7dBOp  95%
17.0dB DL0AO (1)
21:32    136 RK2Y de SM2DJK Op32 *1430*  km -34 dB F:3% in Umea 1533,7 Hz
(1)
20:54    136 R7NT de SP5XSB Op32 *1400* km -27 dB F:1%_End in Raszyn nr
Warsaw (18)
02:55    136 R7NT de YO2NAA Op32 *1371* km -35 dB F:0% in Timisoara 1541.2
Hz with 200w + E.sLoop (8 )
2019-02-10 03:27:48 R7NT    *1152* km 137541.046Hz  67mHz -38.0dBOp  85%
18.9dB EW6X (4)
19:48    136 R7NT de EW6X Op32 -34 dB F:43% in KO45kl (*1151* km) Polotsk +
miniwhip 137541.1 Hz (11)
2019-02-09 21:32:32 RK2Y    *1147* km 137533.671Hz   2mHz -48.6dBOp 100%
16.7dB YO/4X1RF (1)
2019-02-10 00:43:53 R7NT    *1045* km 137540.992Hz 103mHz -27.4dBOp  82%
19.7dB YO/4X1RF (26)
02:22    136 R7NT de RA3-170-352 Op32 *968* km -29 dB F:2% in  1541,4 Hz
with 200w + E.sLoop (16)
2019-02-10 06:11:58 R7NT     *943* km 137540.871Hz  99mHz -39.3dBOp  88%
17.6dB RN3AUS (1)
06:44    136 R7NT de RN3AUS Op32 -39 dB F:46% in KO85fn (*942* km) nr
Moscow + MiniWhip 137539.8 Hz (2)
2019-02-09 21:32:30 RK2Y     *428* km 137533.706Hz   4mHz -34.5dBOp 100%
19.0dB EW6X (1)
21:32    136 RK2Y de EW6X Op32 -35 dB F:5% in KO45kl (*428*  km) Polotsk +
miniwhip 137533.7 Hz (1)
21:32    136 RK2Y de RA3-170-352 Op32 *359*  km -33 dB F:2% in  1534,1 Hz
(1)
*OP32 :* TX-2  RX-12 *OPds* RX-7
(n) - it's the total number of the reports - it's the best result of the
reports - it's the first result over time with the same levels
E.sLoop + 200W Output

--0000000000009d25050581869af8
Content-Type: text/html; charset="UTF-8"
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<div dir=3D"ltr"><font face=3D"arial, helvetica, sans-serif" style=3D"backg=
round-color:rgb(243,243,243)"><strong style=3D"color:rgb(0,0,0);font-size:1=
2.48px">Feb 9-10=C2=A0 Best QRB/reports=C2=A0<span class=3D"gmail-bbc_color=
" style=3D"color:red">OP32</span>=C2=A0/=C2=A0<span class=3D"gmail-bbc_colo=
r" style=3D"color:maroon">OPds</span>=C2=A0:</strong><br style=3D"color:rgb=
(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" style=3D"font-si=
ze:12.48px;color:red">21:27=C2=A0 =C2=A0 136 R7NT de EB8ARZ Op32=C2=A0<stro=
ng>5153</strong>=C2=A0km -30 dB F:0% in Tenerife, Canary Island. 1541,0 Hz =
with 200w + E.sLoop (9)</span><br style=3D"color:rgb(0,0,0);font-size:12.48=
px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:red">0=
4:33=C2=A0 =C2=A0 136 R7NT de G0LUJ Op32=C2=A0<strong>3009</strong>=C2=A0km=
 -35 dB F:8% in Lytham, England 1541.5 Hz with 200w + E.sLoop (4)</span><br=
 style=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_colo=
r" style=3D"font-size:12.48px;color:red">23:05=C2=A0 =C2=A0 136 R7NT de PA0=
RDT Op32=C2=A0<strong>2574</strong>=C2=A0km -34 dB F:1% in Middelburg, Neth=
erlands 1541,9 Hz with 200w + E.sLoop (11)</span><br style=3D"color:rgb(0,0=
,0);font-size:12.48px"><span class=3D"gmail-bbc_color" style=3D"font-size:1=
2.48px;color:red">22:32=C2=A0 =C2=A0 136 R7NT de PA0LSB Op32=C2=A0<strong>2=
482</strong>=C2=A0km -28 dB F:8% in Waspik 1541,8 Hz with 200w + E.sLoop (1=
3)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gm=
ail-bbc_color" style=3D"font-size:12.48px;color:red">02:55=C2=A0 =C2=A0 136=
 R7NT de I55387FI Op32=C2=A0<strong>2259</strong>=C2=A0km -37 dB F:3% in Ri=
otorto (LI) - ITALY - Antenna :Mini-Whip 1541,1 Hz with 200w + E. (15)</spa=
n><br style=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc=
_color" style=3D"font-size:12.48px;color:red">01:49=C2=A0 =C2=A0 136 R7NT d=
e SM2DJK Op32=C2=A0<strong>2178</strong>=C2=A0km -30 dB F:2% in Umea 1541,0=
 Hz with 200w + E.sLoop (20)</span><br style=3D"color:rgb(0,0,0);font-size:=
12.48px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:m=
aroon">2019-02-10 02:55:03 R7NT=C2=A0 =C2=A0=C2=A0<strong>2060</strong>=C2=
=A0km 137540.998Hz=C2=A0 64mHz -28.3dBOp=C2=A0 89% 20.0dB DF6NM (26)</span>=
<br style=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_c=
olor" style=3D"font-size:12.48px;color:maroon">2019-02-10 02:55:06 R7NT=C2=
=A0 =C2=A0=C2=A0<strong>2012</strong>=C2=A0km 137541.018Hz 105mHz -25.0dBOp=
=C2=A0 87% 20.4dB DL0AO (25)</span><br style=3D"color:rgb(0,0,0);font-size:=
12.48px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:m=
aroon">2019-02-09 20:54:25 R7NT=C2=A0 =C2=A0=C2=A0<strong>1876</strong>=C2=
=A0km 137540.998Hz=C2=A0 60mHz -28.1dBOp=C2=A0 73% 19.2dB IZ7SLZ (24)</span=
><br style=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_=
color" style=3D"font-size:12.48px;color:maroon">2019-02-09 21:59:58 R7NT=C2=
=A0 =C2=A0=C2=A0<strong>1811</strong>=C2=A0km 137540.874Hz 104mHz -29.5dBOp=
=C2=A0 87% 19.8dB SV8RV (19)</span><br style=3D"color:rgb(0,0,0);font-size:=
12.48px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:r=
ed">21:27=C2=A0 =C2=A0 136 R7NT de SV8RV Op32=C2=A0<strong>1809</strong>=C2=
=A0km -30 dB F:10% in Zakynthos(Zante) isl. GREECE 1540,9 Hz with 200w + E.=
sLoop (23)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px"><span cla=
ss=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:maroon">2019-02-09 =
21:32:32 RK2Y=C2=A0 =C2=A0=C2=A0<strong>1658</strong>=C2=A0km 137533.680Hz=
=C2=A0 =C2=A02mHz -42.4dBOp=C2=A0 89% 19.0dB DF6NM (1)</span><br style=3D"c=
olor:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" style=3D=
"font-size:12.48px;color:maroon">2019-02-09 21:32:35 RK2Y=C2=A0 =C2=A0=C2=
=A0<strong>1612</strong>=C2=A0km 137533.680Hz=C2=A0 =C2=A03mHz -47.7dBOp=C2=
=A0 95% 17.0dB DL0AO (1)</span><br style=3D"color:rgb(0,0,0);font-size:12.4=
8px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:red">=
21:32=C2=A0 =C2=A0 136 RK2Y de SM2DJK Op32=C2=A0<strong>1430</strong>=C2=A0=
 km -34 dB F:3% in Umea 1533,7 Hz (1)</span><br style=3D"color:rgb(0,0,0);f=
ont-size:12.48px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48p=
x;color:red">20:54=C2=A0 =C2=A0 136 R7NT de SP5XSB Op32=C2=A0<strong>1400</=
strong>=C2=A0km -27 dB F:1%_End in Raszyn nr Warsaw (18)</span><br style=3D=
"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" style=
=3D"font-size:12.48px;color:red">02:55=C2=A0 =C2=A0 136 R7NT de YO2NAA Op32=
=C2=A0<strong>1371</strong>=C2=A0km -35 dB F:0% in Timisoara 1541.2 Hz with=
 200w + E.sLoop (8 )</span><br style=3D"color:rgb(0,0,0);font-size:12.48px"=
><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:maroon">2=
019-02-10 03:27:48 R7NT=C2=A0 =C2=A0=C2=A0<strong>1152</strong>=C2=A0km 137=
541.046Hz=C2=A0 67mHz -38.0dBOp=C2=A0 85% 18.9dB EW6X (4)</span><br style=
=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" sty=
le=3D"font-size:12.48px;color:red">19:48=C2=A0 =C2=A0 136 R7NT de EW6X Op32=
 -34 dB F:43% in KO45kl (<strong>1151</strong>=C2=A0km) Polotsk + miniwhip =
137541.1 Hz (11)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px"><sp=
an class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:maroon">2019-=
02-09 21:32:32 RK2Y=C2=A0 =C2=A0=C2=A0<strong>1147</strong>=C2=A0km 137533.=
671Hz=C2=A0 =C2=A02mHz -48.6dBOp 100% 16.7dB YO/4X1RF (1)</span><br style=
=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" sty=
le=3D"font-size:12.48px;color:maroon">2019-02-10 00:43:53 R7NT=C2=A0 =C2=A0=
=C2=A0<strong>1045</strong>=C2=A0km 137540.992Hz 103mHz -27.4dBOp=C2=A0 82%=
 19.7dB YO/4X1RF (26)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px=
"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:red">02:=
22=C2=A0 =C2=A0 136 R7NT de RA3-170-352 Op32=C2=A0<strong>968</strong>=C2=
=A0km -29 dB F:2% in=C2=A0 1541,4 Hz with 200w + E.sLoop (16)</span><br sty=
le=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" s=
tyle=3D"font-size:12.48px;color:maroon">2019-02-10 06:11:58 R7NT=C2=A0 =C2=
=A0 =C2=A0<strong>943</strong>=C2=A0km 137540.871Hz=C2=A0 99mHz -39.3dBOp=
=C2=A0 88% 17.6dB RN3AUS (1)</span><br style=3D"color:rgb(0,0,0);font-size:=
12.48px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:r=
ed">06:44=C2=A0 =C2=A0 136 R7NT de RN3AUS Op32 -39 dB F:46% in KO85fn (<str=
ong>942</strong>=C2=A0km) nr Moscow + MiniWhip 137539.8 Hz (2)</span><br st=
yle=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" =
style=3D"font-size:12.48px;color:maroon">2019-02-09 21:32:30 RK2Y=C2=A0 =C2=
=A0 =C2=A0<strong>428</strong>=C2=A0km 137533.706Hz=C2=A0 =C2=A04mHz -34.5d=
BOp 100% 19.0dB EW6X (1)</span><br style=3D"color:rgb(0,0,0);font-size:12.4=
8px"><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;color:red">=
21:32=C2=A0 =C2=A0 136 RK2Y de EW6X Op32 -35 dB F:5% in KO45kl (<strong>428=
</strong>=C2=A0 km) Polotsk + miniwhip 137533.7 Hz (1)</span><br style=3D"c=
olor:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-bbc_color" style=3D=
"font-size:12.48px;color:red">21:32=C2=A0 =C2=A0 136 RK2Y de RA3-170-352 Op=
32=C2=A0<strong>359</strong>=C2=A0 km -33 dB F:2% in=C2=A0 1534,1 Hz (1)</s=
pan><br style=3D"color:rgb(0,0,0);font-size:12.48px"><span class=3D"gmail-b=
bc_color" style=3D"font-size:12.48px;color:red"><strong>OP32 :</strong>=C2=
=A0TX-2=C2=A0 RX-12=C2=A0</span><span style=3D"color:rgb(0,0,0);font-size:1=
2.48px"></span><span class=3D"gmail-bbc_color" style=3D"font-size:12.48px;c=
olor:maroon"><strong>OPds</strong>=C2=A0RX-7</span>=C2=A0</font><div style=
=3D"font-size:12.8px"><font face=3D"arial, helvetica, sans-serif" style=3D"=
background-color:rgb(243,243,243)"><span style=3D"color:rgb(0,0,0);font-siz=
e:12.48px;line-height:17.472px">(n) - it&#39;s the total number of the repo=
rts - it&#39;s the best result of the reports - it&#39;s the first result o=
ver time with the same levels</span><br></font></div><div style=3D"font-siz=
e:12.8px"><span style=3D"font-family:arial,helvetica,sans-serif;font-size:1=
2.48px;color:rgb(0,0,0)">E.sLoop + 200W Output</span><span style=3D"backgro=
und-color:rgb(243,243,243);font-family:arial,helvetica,sans-serif;font-size=
:small">=C2=A0</span><span style=3D"background-color:rgb(243,243,243);font-=
family:arial,helvetica,sans-serif;font-size:small">=C2=A0</span><br></div><=
/div>

--0000000000009d25050581869af8--

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References: <168c41b89f6.marcocadeddu@tin.it> <CAKvcm2eoZZOrjQ6zZ6Tx3zxHfahEL6eJ2jrcHELgsVdecfLA2g@mail.gmail.com> <5C5BE905.2010904@posteo.de> <CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com> <5C5D8F53.1080409@posteo.de> <CAKvcm2fbxX3Mx=bX3_pRVj2use52kdE6wNmrE6gmMApgNFK+gA@mail.gmail.com> <5C5EC5EB.7040209@posteo.de>
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 Content preview:  Hi all, last night I got exceptionally good decodes in WSPR.
    N1DAY,KC4SIT and AE2EA got no other spots in EU and only one station in UK
    (GM4OAS) spotted these. 73 Clemens DL4RAJ 
 Content analysis details:   (-0.7 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -0.7 RCVD_IN_DNSWL_LOW      RBL: Sender listed at http://www.dnswl.org/,
                             low trust
                             [212.227.17.20 listed in list.dnswl.org]
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                             provider (cpaul[at]gmx.net)
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Subject: LF: Very good conditions on MW last night
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Hi all,

last night I got exceptionally good decodes in WSPR.
N1DAY,KC4SIT and AE2EA  got no other spots in EU and 
only one station in UK (GM4OAS) spotted these.

73
Clemens
DL4RAJ 

   Timestamp	                Call	    MHz	SNR	Drift	  Grid	           Pwr	 Reporter	  RGrid	  km	 az

 2019-02-10 06:42 	 WA4SZE 	 0.475703 	 -21 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 06:32 	 WA4SZE 	 0.475703 	 -19 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 06:22 	 WA4SZE 	 0.475703 	 -9 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 06:12 	 WA4SZE 	 0.475703 	 -18 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 06:02 	 WA4SZE 	 0.475703 	 -22 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 05:52 	 WA4SZE 	 0.475703 	 -22 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 05:42 	 WA4SZE 	 0.475703 	 -22 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 05:32 	 WA4SZE 	 0.475703 	 -23 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 04:52 	 WA4SZE 	 0.475703 	 -26 	 0 	 EM65 	 0.2 	 DL4RAJ 	 JN68kj 	 7791 	 44 
 2019-02-10 06:14 	 N1DAY 	 0.475682 	 -27 	 0 	 EM85sg 	 5 	 DL4RAJ 	 JN68kj 	 7515 	 46 
 2019-02-10 06:16 	 KC4SIT 	 0.475612 	 -20 	 -1 	 EM85tg 	 1 	 DL4RAJ 	 JN68kj
7509 	 46 
 2019-02-10 06:08 	 KC4SIT 	 0.475612 	 -25 	 0 	 EM85tg 	 1 	 DL4RAJ 	 JN68kj
7509 	 46 
 2019-02-10 06:20 	 AE2EA 	 0.475725 	 -28 	 0 	 FN12fr 	 0.2 	 DL4RAJ 	 JN68kj 	 6644 	 50 
 2019-02-10 06:16 	 AE2EA 	 0.475724 	 -28 	 0 	 FN12fr 	 0.2 	 DL4RAJ 	 JN68kj 	 6644 	 50 
 2019-02-10 06:22 	 AA1A 	            0.475674 	 -29 	 0 	 FN42pb 	 1 	 DL4RAJ 	 JN68kj
6251 	 53 
 2019-02-10 06:08 	 AA1A 	            0.475674 	 -27 	 0 	 FN42pb 	 1 	 DL4RAJ 	 JN68kj
6251 	 53 
 2019-02-10 06:30 	 W1IR 	 0.475629 	 -29 	 0 	 FN34lp 	 5 	 DL4RAJ 	 JN68kj 	 6228 	 53 
 2019-02-10 06:24 	 W1IR 	 0.475629 	 -22 	 0 	 FN34lp 	 5 	 DL4RAJ 	 JN68kj 	 6228 	 53 
 2019-02-10 06:16 	 W1IR 	 0.475629 	 -14 	 0 	 FN34lp 	 5 	 DL4RAJ 	 JN68kj 	 6228 	 53 
 2019-02-10 06:12 	 W1IR 	 0.475629 	 -27 	 0 	 FN34lp 	 5 	 DL4RAJ 	 JN68kj 	 6228 	 53 
 2019-02-10 06:06 	 W1IR 	 0.475629 	 -22 	 0 	 FN34lp 	 5 	 DL4RAJ 	 JN68kj 	 6228 	 53 



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To: rsgb_lf_group@blacksheep.org
References: <168d6970d7b.marcocadeddu@tin.it>
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 Content preview:  Hi Dimitris, VLF, Am 10.02.2019 09:47, schrieb marcocadeddu@tin.it:
    > (RF? it is almost DC hihi) Ehm, no, it is almost LF! 29.5 kHz, you can't
    even hear that. The other (left) side of the audio spectrum that you can't
    [...] 
 Content analysis details:   (-2.3 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -2.3 RCVD_IN_DNSWL_MED      RBL: Sender listed at http://www.dnswl.org/,
                             medium trust
                             [185.67.36.65 listed in list.dnswl.org]
 -0.0 SPF_PASS               SPF: sender matches SPF record
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Subject: Re: R: Re: VLF: in VK?
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Hi Dimitris, VLF,

Am 10.02.2019 09:47, schrieb marcocadeddu@tin.it:
> (RF? it is almost DC hihi)
Ehm, no, it is almost LF! 29.5 kHz, you can't even hear that. The other 
(left) side of the audio spectrum that you can't hear too, maybe 
something below 30 Hz, that's close to DC :-)

Am 09.02.2019 23:58, schrieb Dimitrios Tsifakis:
> The unexpected losses are not just the
> capacitors (their contribution is probably small). It is also the
> coaxial cable that I used between the antenna feedpoint and the
> amplifier.
How long is that cable? And didn't you use a ferrite transformer to 
match the loop to the amplifier? If it is a normal audio amplifier that 
expects a 4 Ohm load, then maybe you don't need one, but then you should 
place the amp close to the loop, without the coax cable inbetween. If 
the loop is far from the house and you want to stay the amp into the 
shack, then use 2 ferrite transformers to transform up to 50 Ohm and 
then down to the antenna impedance again. I would place the amp in the 
shack and monitor voltage and current there using a scope. Then you see 
their ration (Impedance) and product = power (at resonance). I would 
first build a transformer that matches 4 Ohm to 50 Ohm for example, then 
use the cable, and then a transformer from 50 Ohm to the feedpoint 
impedance of the tuned loop.

In the end, such a closed loop will not perform as good as a ground 
loop. You will get much better results when connecting two of these 
little ponds beeing some hunderet meter distant. The current will be 
lower and so the capacitors will be less stressed.

BTW is your ground very dry? you could even try a dipole on the ground 
for the 630m band. A full size dipole. It would be able to carry much RF 
power :-)
And what about a vertical antenna?

Oh i see, i would spend several hours per day there building antennas!


73, Stefan


From owner-rsgb_lf_group@blacksheep.org  Sun Feb 10 11:17:33 2019
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 Content preview:  Thanks for the summary Alex! I also got several of your transmissions
    but since some time there are upload problems in Windows so i do it manually
    from time to time until i find the time/motivation to [...] 
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Thanks for the summary Alex!
I also got several of your transmissions but since some time there are 
upload problems in Windows so i do it manually from time to time until i 
find the time/motivation to solve the problem.

2019-02-10 05:06:12 R7NT    2234km 137541.014Hz 113mHz -38.9dBOp  98% 19.0dB
2019-02-10 04:33:24 R7NT    2234km 137540.998Hz   3mHz -45.2dBOp  87% 16.4dB
2019-02-10 03:27:50 R7NT    2234km 137541.018Hz 112mHz -38.0dBOp 100% 20.2dB
2019-02-10 02:55:05 R7NT    2234km 137540.998Hz   5mHz -45.5dBOp  82% 16.4dB
2019-02-10 02:22:17 R7NT    2234km 137540.997Hz   3mHz -45.3dBOp  86% 16.9dB
2019-02-10 01:49:29 R7NT    2234km 137540.997Hz   3mHz -44.5dBOp  99% 17.7dB
2019-02-10 01:16:43 R7NT    2234km 137540.998Hz   4mHz -43.2dBOp  99% 18.9dB
2019-02-10 00:43:55 R7NT    2234km 137540.996Hz   8mHz -45.0dBOp  91% 17.8dB
2019-02-10 00:11:09 R7NT    2234km 137540.997Hz   3mHz -43.1dBOp  94% 17.1dB
2019-02-09 23:38:21 R7NT    2234km 137540.998Hz  69mHz -37.9dBOp 100% 20.4dB
2019-02-09 23:05:35 R7NT    2234km 137541.015Hz 105mHz -37.5dBOp  96% 20.0dB
2019-02-09 22:32:47 R7NT    2234km 137540.997Hz   4mHz -43.4dBOp  87% 18.6dB
2019-02-09 21:59:59 R7NT    2234km 137541.017Hz  73mHz -38.8dBOp  97% 20.5dB
2019-02-09 21:27:13 R7NT    2234km 137540.996Hz   3mHz -44.3dBOp 100% 18.5dB
2019-02-09 20:54:26 R7NT    2234km 137540.998Hz  65mHz -36.7dBOp  84% 20.8dB
2019-02-09 20:21:40 R7NT    2234km 137540.996Hz   8mHz -42.3dBOp  92% 16.8dB
2019-02-09 19:48:52 R7NT    2234km 137540.997Hz  54mHz -34.3dBOp  76% 20.2dB
2019-02-09 19:16:06 R7NT    2234km 137540.996Hz   5mHz -42.5dBOp  98% 18.5dB
2019-02-09 18:43:18 R7NT    2234km 137540.997Hz   2mHz -47.6dBOp  89% 15.4dB
2019-02-09 18:10:32 R7NT    2234km 137540.998Hz  32mHz -41.8dBOp  81% 18.6dB
2019-02-09 17:37:44 R7NT    2234km 137540.997Hz   4mHz -43.8dBOp 100% 17.3dB

73, Stefan


Am 10.02.2019 10:13, schrieb Alex R7NT:
> *Feb 9-10  Best QRB/reports OP32 / OPds :*
> 21:27    136 R7NT de EB8ARZ Op32 *5153* km -30 dB F:0% in Tenerife, 
> Canary Island. 1541,0 Hz with 200w + E.sLoop (9)
> 04:33    136 R7NT de G0LUJ Op32 *3009* km -35 dB F:8% in Lytham, 
> England 1541.5 Hz with 200w + E.sLoop (4)
> 23:05    136 R7NT de PA0RDT Op32 *2574* km -34 dB F:1% in Middelburg, 
> Netherlands 1541,9 Hz with 200w + E.sLoop (11)
> 22:32    136 R7NT de PA0LSB Op32 *2482* km -28 dB F:8% in Waspik 
> 1541,8 Hz with 200w + E.sLoop (13)
> 02:55    136 R7NT de I55387FI Op32 *2259* km -37 dB F:3% in Riotorto 
> (LI) - ITALY - Antenna :Mini-Whip 1541,1 Hz with 200w + E. (15)
> 01:49    136 R7NT de SM2DJK Op32 *2178* km -30 dB F:2% in Umea 1541,0 
> Hz with 200w + E.sLoop (20)
> 2019-02-10 02:55:03 R7NT *2060* km 137540.998Hz  64mHz -28.3dBOp  89% 
> 20.0dB DF6NM (26)
> 2019-02-10 02:55:06 R7NT *2012* km 137541.018Hz 105mHz -25.0dBOp  87% 
> 20.4dB DL0AO (25)
> 2019-02-09 20:54:25 R7NT *1876* km 137540.998Hz  60mHz -28.1dBOp  73% 
> 19.2dB IZ7SLZ (24)
> 2019-02-09 21:59:58 R7NT *1811* km 137540.874Hz 104mHz -29.5dBOp  87% 
> 19.8dB SV8RV (19)
> 21:27    136 R7NT de SV8RV Op32 *1809* km -30 dB F:10% in 
> Zakynthos(Zante) isl. GREECE 1540,9 Hz with 200w + E.sLoop (23)
> 2019-02-09 21:32:32 RK2Y *1658* km 137533.680Hz   2mHz -42.4dBOp  89% 
> 19.0dB DF6NM (1)
> 2019-02-09 21:32:35 RK2Y *1612* km 137533.680Hz   3mHz -47.7dBOp  95% 
> 17.0dB DL0AO (1)
> 21:32    136 RK2Y de SM2DJK Op32 *1430*  km -34 dB F:3% in Umea 1533,7 
> Hz (1)
> 20:54    136 R7NT de SP5XSB Op32 *1400* km -27 dB F:1%_End in Raszyn 
> nr Warsaw (18)
> 02:55    136 R7NT de YO2NAA Op32 *1371* km -35 dB F:0% in Timisoara 
> 1541.2 Hz with 200w + E.sLoop (8 )
> 2019-02-10 03:27:48 R7NT *1152* km 137541.046Hz  67mHz -38.0dBOp  85% 
> 18.9dB EW6X (4)
> 19:48    136 R7NT de EW6X Op32 -34 dB F:43% in KO45kl (*1151* km) 
> Polotsk + miniwhip 137541.1 Hz (11)
> 2019-02-09 21:32:32 RK2Y *1147* km 137533.671Hz   2mHz -48.6dBOp 100% 
> 16.7dB YO/4X1RF (1)
> 2019-02-10 00:43:53 R7NT *1045* km 137540.992Hz 103mHz -27.4dBOp  82% 
> 19.7dB YO/4X1RF (26)
> 02:22    136 R7NT de RA3-170-352 Op32 *968* km -29 dB F:2% in  1541,4 
> Hz with 200w + E.sLoop (16)
> 2019-02-10 06:11:58 R7NT *943* km 137540.871Hz  99mHz -39.3dBOp  88% 
> 17.6dB RN3AUS (1)
> 06:44    136 R7NT de RN3AUS Op32 -39 dB F:46% in KO85fn (*942* km) nr 
> Moscow + MiniWhip 137539.8 Hz (2)
> 2019-02-09 21:32:30 RK2Y *428* km 137533.706Hz   4mHz -34.5dBOp 100% 
> 19.0dB EW6X (1)
> 21:32    136 RK2Y de EW6X Op32 -35 dB F:5% in KO45kl (*428*  km) 
> Polotsk + miniwhip 137533.7 Hz (1)
> 21:32    136 RK2Y de RA3-170-352 Op32 *359*  km -33 dB F:2% in  1534,1 
> Hz (1)
> *OP32 :* TX-2  RX-12 *OPds* RX-7
> (n) - it's the total number of the reports - it's the best result of 
> the reports - it's the first result over time with the same levels
> E.sLoop + 200W Output

--------------040907020903060208030605
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 8bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
Thanks for the summary Alex!<br>
I also got several of your transmissions but since some time there are
upload problems in Windows so i do it manually from time to time until
i find the time/motivation to solve the problem.<br>
<br>
2019-02-10 05:06:12 R7NT    2234km 137541.014Hz 113mHz -38.9dBOp  98%
19.0dB<br>
2019-02-10 04:33:24 R7NT    2234km 137540.998Hz   3mHz -45.2dBOp  87%
16.4dB<br>
2019-02-10 03:27:50 R7NT    2234km 137541.018Hz 112mHz -38.0dBOp 100%
20.2dB<br>
2019-02-10 02:55:05 R7NT    2234km 137540.998Hz   5mHz -45.5dBOp  82%
16.4dB<br>
2019-02-10 02:22:17 R7NT    2234km 137540.997Hz   3mHz -45.3dBOp  86%
16.9dB<br>
2019-02-10 01:49:29 R7NT    2234km 137540.997Hz   3mHz -44.5dBOp  99%
17.7dB<br>
2019-02-10 01:16:43 R7NT    2234km 137540.998Hz   4mHz -43.2dBOp  99%
18.9dB<br>
2019-02-10 00:43:55 R7NT    2234km 137540.996Hz   8mHz -45.0dBOp  91%
17.8dB<br>
2019-02-10 00:11:09 R7NT    2234km 137540.997Hz   3mHz -43.1dBOp  94%
17.1dB<br>
2019-02-09 23:38:21 R7NT    2234km 137540.998Hz  69mHz -37.9dBOp 100%
20.4dB<br>
2019-02-09 23:05:35 R7NT    2234km 137541.015Hz 105mHz -37.5dBOp  96%
20.0dB<br>
2019-02-09 22:32:47 R7NT    2234km 137540.997Hz   4mHz -43.4dBOp  87%
18.6dB<br>
2019-02-09 21:59:59 R7NT    2234km 137541.017Hz  73mHz -38.8dBOp  97%
20.5dB<br>
2019-02-09 21:27:13 R7NT    2234km 137540.996Hz   3mHz -44.3dBOp 100%
18.5dB<br>
2019-02-09 20:54:26 R7NT    2234km 137540.998Hz  65mHz -36.7dBOp  84%
20.8dB<br>
2019-02-09 20:21:40 R7NT    2234km 137540.996Hz   8mHz -42.3dBOp  92%
16.8dB<br>
2019-02-09 19:48:52 R7NT    2234km 137540.997Hz  54mHz -34.3dBOp  76%
20.2dB<br>
2019-02-09 19:16:06 R7NT    2234km 137540.996Hz   5mHz -42.5dBOp  98%
18.5dB<br>
2019-02-09 18:43:18 R7NT    2234km 137540.997Hz   2mHz -47.6dBOp  89%
15.4dB<br>
2019-02-09 18:10:32 R7NT    2234km 137540.998Hz  32mHz -41.8dBOp  81%
18.6dB<br>
2019-02-09 17:37:44 R7NT    2234km 137540.997Hz   4mHz -43.8dBOp 100%
17.3dB<br>
<br>
73, Stefan<br>
<br>
<br>
Am 10.02.2019 10:13, schrieb Alex R7NT:
<blockquote
 cite="mid:CAL-VeeNSzGwo2=AmnpunMpVgcLeSBqY9SHSt7C7zeSRqo_1fPQ@mail.gmail.com"
 type="cite">
  <div dir="ltr"><font style="background-color: rgb(243, 243, 243);"
 face="arial, helvetica, sans-serif"><strong
 style="color: rgb(0, 0, 0); font-size: 12.48px;">Feb 9-10  Best
QRB/reports <span class="gmail-bbc_color" style="color: red;">OP32</span> / <span
 class="gmail-bbc_color" style="color: maroon;">OPds</span> :</strong><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">21:27 
  136 R7NT de EB8ARZ Op32 <strong>5153</strong> km -30 dB F:0% in
Tenerife, Canary Island. 1541,0 Hz with 200w + E.sLoop (9)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">04:33 
  136 R7NT de G0LUJ Op32 <strong>3009</strong> km -35 dB F:8% in
Lytham, England 1541.5 Hz with 200w + E.sLoop (4)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">23:05 
  136 R7NT de PA0RDT Op32 <strong>2574</strong> km -34 dB F:1% in
Middelburg, Netherlands 1541,9 Hz with 200w + E.sLoop (11)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">22:32 
  136 R7NT de PA0LSB Op32 <strong>2482</strong> km -28 dB F:8% in
Waspik 1541,8 Hz with 200w + E.sLoop (13)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">02:55 
  136 R7NT de I55387FI Op32 <strong>2259</strong> km -37 dB F:3% in
Riotorto (LI) - ITALY - Antenna :Mini-Whip 1541,1 Hz with 200w + E. (15)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">01:49 
  136 R7NT de SM2DJK Op32 <strong>2178</strong> km -30 dB F:2% in Umea
1541,0 Hz with 200w + E.sLoop (20)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-10 02:55:03 R7NT    <strong>2060</strong> km
137540.998Hz  64mHz -28.3dBOp  89% 20.0dB DF6NM (26)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-10 02:55:06 R7NT    <strong>2012</strong> km
137541.018Hz 105mHz -25.0dBOp  87% 20.4dB DL0AO (25)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-09 20:54:25 R7NT    <strong>1876</strong> km
137540.998Hz  60mHz -28.1dBOp  73% 19.2dB IZ7SLZ (24)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-09 21:59:58 R7NT    <strong>1811</strong> km
137540.874Hz 104mHz -29.5dBOp  87% 19.8dB SV8RV (19)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">21:27 
  136 R7NT de SV8RV Op32 <strong>1809</strong> km -30 dB F:10% in
Zakynthos(Zante) isl. GREECE 1540,9 Hz with 200w + E.sLoop (23)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-09 21:32:32 RK2Y    <strong>1658</strong> km
137533.680Hz   2mHz -42.4dBOp  89% 19.0dB DF6NM (1)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-09 21:32:35 RK2Y    <strong>1612</strong> km
137533.680Hz   3mHz -47.7dBOp  95% 17.0dB DL0AO (1)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">21:32 
  136 RK2Y de SM2DJK Op32 <strong>1430</strong>  km -34 dB F:3% in Umea
1533,7 Hz (1)</span><br style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">20:54 
  136 R7NT de SP5XSB Op32 <strong>1400</strong> km -27 dB F:1%_End in
Raszyn nr Warsaw (18)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">02:55 
  136 R7NT de YO2NAA Op32 <strong>1371</strong> km -35 dB F:0% in
Timisoara 1541.2 Hz with 200w + E.sLoop (8 )</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-10 03:27:48 R7NT    <strong>1152</strong> km
137541.046Hz  67mHz -38.0dBOp  85% 18.9dB EW6X (4)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">19:48 
  136 R7NT de EW6X Op32 -34 dB F:43% in KO45kl (<strong>1151</strong> km)
Polotsk + miniwhip 137541.1 Hz (11)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-09 21:32:32 RK2Y    <strong>1147</strong> km
137533.671Hz   2mHz -48.6dBOp 100% 16.7dB YO/4X1RF (1)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-10 00:43:53 R7NT    <strong>1045</strong> km
137540.992Hz 103mHz -27.4dBOp  82% 19.7dB YO/4X1RF (26)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">02:22 
  136 R7NT de RA3-170-352 Op32 <strong>968</strong> km -29 dB F:2% in 
1541,4 Hz with 200w + E.sLoop (16)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-10 06:11:58 R7NT   
 <strong>943</strong> km 137540.871Hz  99mHz -39.3dBOp  88% 17.6dB
RN3AUS (1)</span><br style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">06:44 
  136 R7NT de RN3AUS Op32 -39 dB F:46% in KO85fn (<strong>942</strong> km)
nr Moscow + MiniWhip 137539.8 Hz (2)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color"
 style="font-size: 12.48px; color: maroon;">2019-02-09 21:32:30 RK2Y   
 <strong>428</strong> km 137533.706Hz   4mHz -34.5dBOp 100% 19.0dB EW6X
(1)</span><br style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">21:32 
  136 RK2Y de EW6X Op32 -35 dB F:5% in KO45kl (<strong>428</strong> 
km) Polotsk + miniwhip 137533.7 Hz (1)</span><br
 style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;">21:32 
  136 RK2Y de RA3-170-352 Op32 <strong>359</strong>  km -33 dB F:2% in 
1534,1 Hz (1)</span><br style="color: rgb(0, 0, 0); font-size: 12.48px;">
  <span class="gmail-bbc_color" style="font-size: 12.48px; color: red;"><strong>OP32
:</strong> TX-2  RX-12 </span><span
 style="color: rgb(0, 0, 0); font-size: 12.48px;"></span><span
 class="gmail-bbc_color" style="font-size: 12.48px; color: maroon;"><strong>OPds</strong> RX-7</span> </font>
  <div style="font-size: 12.8px;"><font
 style="background-color: rgb(243, 243, 243);"
 face="arial, helvetica, sans-serif"><span
 style="color: rgb(0, 0, 0); font-size: 12.48px; line-height: 17.472px;">(n)
- it's the total number of the reports - it's the best result of the
reports - it's the first result over time with the same levels</span><br>
  </font></div>
  <div style="font-size: 12.8px;"><span
 style="font-family: arial,helvetica,sans-serif; font-size: 12.48px; color: rgb(0, 0, 0);">E.sLoop
+ 200W Output</span><span
 style="background-color: rgb(243, 243, 243); font-family: arial,helvetica,sans-serif; font-size: small;"> </span><span
 style="background-color: rgb(243, 243, 243); font-family: arial,helvetica,sans-serif; font-size: small;"> </span><br>
  </div>
  </div>
</blockquote>
</body>
</html>

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 Content preview:  Stefan, TNX for the report! updated http://136.su/index.php/topic,18.msg23220.html#msg23220
    73! Alex R7NT 136.73.ru AWLF *136.73.ru/h_aw/ <http://136.73.ru/h_aw/>* вс,
    10 февр. 2019 г. в 13:16, DK7FC : 
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Stefan,
TNX for the report!
updated http://136.su/index.php/topic,18.msg23220.html#msg23220
73! Alex R7NT  136.73.ru    AWLF *136.73.ru/h_aw/ <http://136.73.ru/h_aw/>*


=D0=B2=D1=81, 10 =D1=84=D0=B5=D0=B2=D1=80. 2019 =D0=B3. =D0=B2 13:16, DK7FC=
 <selberdenken@posteo.de>:

> Thanks for the summary Alex!
> I also got several of your transmissions but since some time there are
> upload problems in Windows so i do it manually from time to time until i
> find the time/motivation to solve the problem.
>
> 2019-02-10 05:06:12 R7NT    2234km 137541.014Hz 113mHz -38.9dBOp  98%
> 19.0dB
> 2019-02-10 04:33:24 R7NT    2234km 137540.998Hz   3mHz -45.2dBOp  87%
> 16.4dB
> 2019-02-10 03:27:50 R7NT    2234km 137541.018Hz 112mHz -38.0dBOp 100%
> 20.2dB
> 2019-02-10 02:55:05 R7NT    2234km 137540.998Hz   5mHz -45.5dBOp  82%
> 16.4dB
> 2019-02-10 02:22:17 R7NT    2234km 137540.997Hz   3mHz -45.3dBOp  86%
> 16.9dB
> 2019-02-10 01:49:29 R7NT    2234km 137540.997Hz   3mHz -44.5dBOp  99%
> 17.7dB
> 2019-02-10 01:16:43 R7NT    2234km 137540.998Hz   4mHz -43.2dBOp  99%
> 18.9dB
> 2019-02-10 00:43:55 R7NT    2234km 137540.996Hz   8mHz -45.0dBOp  91%
> 17.8dB
> 2019-02-10 00:11:09 R7NT    2234km 137540.997Hz   3mHz -43.1dBOp  94%
> 17.1dB
> 2019-02-09 23:38:21 R7NT    2234km 137540.998Hz  69mHz -37.9dBOp 100%
> 20.4dB
> 2019-02-09 23:05:35 R7NT    2234km 137541.015Hz 105mHz -37.5dBOp  96%
> 20.0dB
> 2019-02-09 22:32:47 R7NT    2234km 137540.997Hz   4mHz -43.4dBOp  87%
> 18.6dB
> 2019-02-09 21:59:59 R7NT    2234km 137541.017Hz  73mHz -38.8dBOp  97%
> 20.5dB
> 2019-02-09 21:27:13 R7NT    2234km 137540.996Hz   3mHz -44.3dBOp 100%
> 18.5dB
> 2019-02-09 20:54:26 R7NT    2234km 137540.998Hz  65mHz -36.7dBOp  84%
> 20.8dB
> 2019-02-09 20:21:40 R7NT    2234km 137540.996Hz   8mHz -42.3dBOp  92%
> 16.8dB
> 2019-02-09 19:48:52 R7NT    2234km 137540.997Hz  54mHz -34.3dBOp  76%
> 20.2dB
> 2019-02-09 19:16:06 R7NT    2234km 137540.996Hz   5mHz -42.5dBOp  98%
> 18.5dB
> 2019-02-09 18:43:18 R7NT    2234km 137540.997Hz   2mHz -47.6dBOp  89%
> 15.4dB
> 2019-02-09 18:10:32 R7NT    2234km 137540.998Hz  32mHz -41.8dBOp  81%
> 18.6dB
> 2019-02-09 17:37:44 R7NT    2234km 137540.997Hz   4mHz -43.8dBOp 100%
> 17.3dB
>
> 73, Stefan
>
>
> Am 10.02.2019 10:13, schrieb Alex R7NT:
>
> *Feb 9-10  Best QRB/reports OP32 / OPds :*
> 21:27    136 R7NT de EB8ARZ Op32 *5153* km -30 dB F:0% in Tenerife,
> Canary Island. 1541,0 Hz with 200w + E.sLoop (9)
> 04:33    136 R7NT de G0LUJ Op32 *3009* km -35 dB F:8% in Lytham, England
> 1541.5 Hz with 200w + E.sLoop (4)
> 23:05    136 R7NT de PA0RDT Op32 *2574* km -34 dB F:1% in Middelburg,
> Netherlands 1541,9 Hz with 200w + E.sLoop (11)
> 22:32    136 R7NT de PA0LSB Op32 *2482* km -28 dB F:8% in Waspik 1541,8
> Hz with 200w + E.sLoop (13)
> 02:55    136 R7NT de I55387FI Op32 *2259* km -37 dB F:3% in Riotorto (LI)
> - ITALY - Antenna :Mini-Whip 1541,1 Hz with 200w + E. (15)
> 01:49    136 R7NT de SM2DJK Op32 *2178* km -30 dB F:2% in Umea 1541,0 Hz
> with 200w + E.sLoop (20)
> 2019-02-10 02:55:03 R7NT    *2060* km 137540.998Hz  64mHz -28.3dBOp  89%
> 20.0dB DF6NM (26)
> 2019-02-10 02:55:06 R7NT    *2012* km 137541.018Hz 105mHz -25.0dBOp  87%
> 20.4dB DL0AO (25)
> 2019-02-09 20:54:25 R7NT    *1876* km 137540.998Hz  60mHz -28.1dBOp  73%
> 19.2dB IZ7SLZ (24)
> 2019-02-09 21:59:58 R7NT    *1811* km 137540.874Hz 104mHz -29.5dBOp  87%
> 19.8dB SV8RV (19)
> 21:27    136 R7NT de SV8RV Op32 *1809* km -30 dB F:10% in
> Zakynthos(Zante) isl. GREECE 1540,9 Hz with 200w + E.sLoop (23)
> 2019-02-09 21:32:32 RK2Y    *1658* km 137533.680Hz   2mHz -42.4dBOp  89%
> 19.0dB DF6NM (1)
> 2019-02-09 21:32:35 RK2Y    *1612* km 137533.680Hz   3mHz -47.7dBOp  95%
> 17.0dB DL0AO (1)
> 21:32    136 RK2Y de SM2DJK Op32 *1430*  km -34 dB F:3% in Umea 1533,7 Hz
> (1)
> 20:54    136 R7NT de SP5XSB Op32 *1400* km -27 dB F:1%_End in Raszyn nr
> Warsaw (18)
> 02:55    136 R7NT de YO2NAA Op32 *1371* km -35 dB F:0% in Timisoara
> 1541.2 Hz with 200w + E.sLoop (8 )
> 2019-02-10 03:27:48 R7NT    *1152* km 137541.046Hz  67mHz -38.0dBOp  85%
> 18.9dB EW6X (4)
> 19:48    136 R7NT de EW6X Op32 -34 dB F:43% in KO45kl (*1151* km) Polotsk
> + miniwhip 137541.1 Hz (11)
> 2019-02-09 21:32:32 RK2Y    *1147* km 137533.671Hz   2mHz -48.6dBOp 100%
> 16.7dB YO/4X1RF (1)
> 2019-02-10 00:43:53 R7NT    *1045* km 137540.992Hz 103mHz -27.4dBOp  82%
> 19.7dB YO/4X1RF (26)
> 02:22    136 R7NT de RA3-170-352 Op32 *968* km -29 dB F:2% in  1541,4 Hz
> with 200w + E.sLoop (16)
> 2019-02-10 06:11:58 R7NT     *943* km 137540.871Hz  99mHz -39.3dBOp  88%
> 17.6dB RN3AUS (1)
> 06:44    136 R7NT de RN3AUS Op32 -39 dB F:46% in KO85fn (*942* km) nr
> Moscow + MiniWhip 137539.8 Hz (2)
> 2019-02-09 21:32:30 RK2Y     *428* km 137533.706Hz   4mHz -34.5dBOp 100%
> 19.0dB EW6X (1)
> 21:32    136 RK2Y de EW6X Op32 -35 dB F:5% in KO45kl (*428*  km) Polotsk
> + miniwhip 137533.7 Hz (1)
> 21:32    136 RK2Y de RA3-170-352 Op32 *359*  km -33 dB F:2% in  1534,1 Hz
> (1)
> *OP32 :* TX-2  RX-12 *OPds* RX-7
> (n) - it's the total number of the reports - it's the best result of the
> reports - it's the first result over time with the same levels
> E.sLoop + 200W Output
>
>

--0000000000007236a60581879e4e
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr">Stefan,<div>TNX for the report!</div><div=
>updated=C2=A0<a href=3D"http://136.su/index.php/topic,18.msg23220.html#msg=
23220">http://136.su/index.php/topic,18.msg23220.html#msg23220</a><br clear=
=3D"all"><div><div dir=3D"ltr" class=3D"gmail_signature"><div dir=3D"ltr"><=
div><div dir=3D"ltr"><div>73! Alex R7NT =C2=A0<a href=3D"http://136.73.ru" =
target=3D"_blank">136.73.ru</a>=C2=A0 =C2=A0 AWLF <font color=3D"#0000ee"><=
span style=3D"font-size:12.8px"><u><a href=3D"http://136.73.ru/h_aw/" targe=
t=3D"_blank">136.73.ru/h_aw/</a></u></span></font></div></div></div></div><=
/div></div><br></div></div></div><br><div class=3D"gmail_quote"><div dir=3D=
"ltr" class=3D"gmail_attr">=D0=B2=D1=81, 10 =D1=84=D0=B5=D0=B2=D1=80. 2019 =
=D0=B3. =D0=B2 13:16, DK7FC &lt;<a href=3D"mailto:selberdenken@posteo.de">s=
elberdenken@posteo.de</a>&gt;:<br></div><blockquote class=3D"gmail_quote" s=
tyle=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);pad=
ding-left:1ex"><u></u>


 =20

<div bgcolor=3D"#ffffff">
Thanks for the summary Alex!<br>
I also got several of your transmissions but since some time there are
upload problems in Windows so i do it manually from time to time until
i find the time/motivation to solve the problem.<br>
<br>
2019-02-10 05:06:12 R7NT=C2=A0=C2=A0=C2=A0 2234km 137541.014Hz 113mHz -38.9=
dBOp=C2=A0 98%
19.0dB<br>
2019-02-10 04:33:24 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.998Hz=C2=A0=C2=A0 =
3mHz -45.2dBOp=C2=A0 87%
16.4dB<br>
2019-02-10 03:27:50 R7NT=C2=A0=C2=A0=C2=A0 2234km 137541.018Hz 112mHz -38.0=
dBOp 100%
20.2dB<br>
2019-02-10 02:55:05 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.998Hz=C2=A0=C2=A0 =
5mHz -45.5dBOp=C2=A0 82%
16.4dB<br>
2019-02-10 02:22:17 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0=C2=A0 =
3mHz -45.3dBOp=C2=A0 86%
16.9dB<br>
2019-02-10 01:49:29 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0=C2=A0 =
3mHz -44.5dBOp=C2=A0 99%
17.7dB<br>
2019-02-10 01:16:43 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.998Hz=C2=A0=C2=A0 =
4mHz -43.2dBOp=C2=A0 99%
18.9dB<br>
2019-02-10 00:43:55 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.996Hz=C2=A0=C2=A0 =
8mHz -45.0dBOp=C2=A0 91%
17.8dB<br>
2019-02-10 00:11:09 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0=C2=A0 =
3mHz -43.1dBOp=C2=A0 94%
17.1dB<br>
2019-02-09 23:38:21 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.998Hz=C2=A0 69mHz =
-37.9dBOp 100%
20.4dB<br>
2019-02-09 23:05:35 R7NT=C2=A0=C2=A0=C2=A0 2234km 137541.015Hz 105mHz -37.5=
dBOp=C2=A0 96%
20.0dB<br>
2019-02-09 22:32:47 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0=C2=A0 =
4mHz -43.4dBOp=C2=A0 87%
18.6dB<br>
2019-02-09 21:59:59 R7NT=C2=A0=C2=A0=C2=A0 2234km 137541.017Hz=C2=A0 73mHz =
-38.8dBOp=C2=A0 97%
20.5dB<br>
2019-02-09 21:27:13 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.996Hz=C2=A0=C2=A0 =
3mHz -44.3dBOp 100%
18.5dB<br>
2019-02-09 20:54:26 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.998Hz=C2=A0 65mHz =
-36.7dBOp=C2=A0 84%
20.8dB<br>
2019-02-09 20:21:40 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.996Hz=C2=A0=C2=A0 =
8mHz -42.3dBOp=C2=A0 92%
16.8dB<br>
2019-02-09 19:48:52 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0 54mHz =
-34.3dBOp=C2=A0 76%
20.2dB<br>
2019-02-09 19:16:06 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.996Hz=C2=A0=C2=A0 =
5mHz -42.5dBOp=C2=A0 98%
18.5dB<br>
2019-02-09 18:43:18 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0=C2=A0 =
2mHz -47.6dBOp=C2=A0 89%
15.4dB<br>
2019-02-09 18:10:32 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.998Hz=C2=A0 32mHz =
-41.8dBOp=C2=A0 81%
18.6dB<br>
2019-02-09 17:37:44 R7NT=C2=A0=C2=A0=C2=A0 2234km 137540.997Hz=C2=A0=C2=A0 =
4mHz -43.8dBOp 100%
17.3dB<br>
<br>
73, Stefan<br>
<br>
<br>
Am 10.02.2019 10:13, schrieb Alex R7NT:
<blockquote type=3D"cite">
  <div dir=3D"ltr"><font style=3D"background-color:rgb(243,243,243)" face=
=3D"arial, helvetica, sans-serif"><strong style=3D"color:rgb(0,0,0);font-si=
ze:12.48px">Feb 9-10=C2=A0 Best
QRB/reports=C2=A0<span class=3D"gmail-m_-8520955909902486638gmail-bbc_color=
" style=3D"color:red">OP32</span>=C2=A0/=C2=A0<span class=3D"gmail-m_-85209=
55909902486638gmail-bbc_color" style=3D"color:maroon">OPds</span>=C2=A0:</s=
trong><br style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">21:27=C2=A0
=C2=A0 136 R7NT de EB8ARZ Op32=C2=A0<strong>5153</strong>=C2=A0km -30 dB F:=
0% in
Tenerife, Canary Island. 1541,0 Hz with 200w + E.sLoop (9)</span><br style=
=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">04:33=C2=A0
=C2=A0 136 R7NT de G0LUJ Op32=C2=A0<strong>3009</strong>=C2=A0km -35 dB F:8=
% in
Lytham, England 1541.5 Hz with 200w + E.sLoop (4)</span><br style=3D"color:=
rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">23:05=C2=A0
=C2=A0 136 R7NT de PA0RDT Op32=C2=A0<strong>2574</strong>=C2=A0km -34 dB F:=
1% in
Middelburg, Netherlands 1541,9 Hz with 200w + E.sLoop (11)</span><br style=
=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">22:32=C2=A0
=C2=A0 136 R7NT de PA0LSB Op32=C2=A0<strong>2482</strong>=C2=A0km -28 dB F:=
8% in
Waspik 1541,8 Hz with 200w + E.sLoop (13)</span><br style=3D"color:rgb(0,0,=
0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">02:55=C2=A0
=C2=A0 136 R7NT de I55387FI Op32=C2=A0<strong>2259</strong>=C2=A0km -37 dB =
F:3% in
Riotorto (LI) - ITALY - Antenna :Mini-Whip 1541,1 Hz with 200w + E. (15)</s=
pan><br style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">01:49=C2=A0
=C2=A0 136 R7NT de SM2DJK Op32=C2=A0<strong>2178</strong>=C2=A0km -30 dB F:=
2% in Umea
1541,0 Hz with 200w + E.sLoop (20)</span><br style=3D"color:rgb(0,0,0);font=
-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-10 02:55:03 R7NT=C2=A0 =C2=A0=C2=A0<str=
ong>2060</strong>=C2=A0km
137540.998Hz=C2=A0 64mHz -28.3dBOp=C2=A0 89% 20.0dB DF6NM (26)</span><br st=
yle=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-10 02:55:06 R7NT=C2=A0 =C2=A0=C2=A0<str=
ong>2012</strong>=C2=A0km
137541.018Hz 105mHz -25.0dBOp=C2=A0 87% 20.4dB DL0AO (25)</span><br style=
=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-09 20:54:25 R7NT=C2=A0 =C2=A0=C2=A0<str=
ong>1876</strong>=C2=A0km
137540.998Hz=C2=A0 60mHz -28.1dBOp=C2=A0 73% 19.2dB IZ7SLZ (24)</span><br s=
tyle=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-09 21:59:58 R7NT=C2=A0 =C2=A0=C2=A0<str=
ong>1811</strong>=C2=A0km
137540.874Hz 104mHz -29.5dBOp=C2=A0 87% 19.8dB SV8RV (19)</span><br style=
=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">21:27=C2=A0
=C2=A0 136 R7NT de SV8RV Op32=C2=A0<strong>1809</strong>=C2=A0km -30 dB F:1=
0% in
Zakynthos(Zante) isl. GREECE 1540,9 Hz with 200w + E.sLoop (23)</span><br s=
tyle=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-09 21:32:32 RK2Y=C2=A0 =C2=A0=C2=A0<str=
ong>1658</strong>=C2=A0km
137533.680Hz=C2=A0 =C2=A02mHz -42.4dBOp=C2=A0 89% 19.0dB DF6NM (1)</span><b=
r style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-09 21:32:35 RK2Y=C2=A0 =C2=A0=C2=A0<str=
ong>1612</strong>=C2=A0km
137533.680Hz=C2=A0 =C2=A03mHz -47.7dBOp=C2=A0 95% 17.0dB DL0AO (1)</span><b=
r style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">21:32=C2=A0
=C2=A0 136 RK2Y de SM2DJK Op32=C2=A0<strong>1430</strong>=C2=A0 km -34 dB F=
:3% in Umea
1533,7 Hz (1)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">20:54=C2=A0
=C2=A0 136 R7NT de SP5XSB Op32=C2=A0<strong>1400</strong>=C2=A0km -27 dB F:=
1%_End in
Raszyn nr Warsaw (18)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px=
">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">02:55=C2=A0
=C2=A0 136 R7NT de YO2NAA Op32=C2=A0<strong>1371</strong>=C2=A0km -35 dB F:=
0% in
Timisoara 1541.2 Hz with 200w + E.sLoop (8 )</span><br style=3D"color:rgb(0=
,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-10 03:27:48 R7NT=C2=A0 =C2=A0=C2=A0<str=
ong>1152</strong>=C2=A0km
137541.046Hz=C2=A0 67mHz -38.0dBOp=C2=A0 85% 18.9dB EW6X (4)</span><br styl=
e=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">19:48=C2=A0
=C2=A0 136 R7NT de EW6X Op32 -34 dB F:43% in KO45kl (<strong>1151</strong>=
=C2=A0km)
Polotsk + miniwhip 137541.1 Hz (11)</span><br style=3D"color:rgb(0,0,0);fon=
t-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-09 21:32:32 RK2Y=C2=A0 =C2=A0=C2=A0<str=
ong>1147</strong>=C2=A0km
137533.671Hz=C2=A0 =C2=A02mHz -48.6dBOp 100% 16.7dB YO/4X1RF (1)</span><br =
style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-10 00:43:53 R7NT=C2=A0 =C2=A0=C2=A0<str=
ong>1045</strong>=C2=A0km
137540.992Hz 103mHz -27.4dBOp=C2=A0 82% 19.7dB YO/4X1RF (26)</span><br styl=
e=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">02:22=C2=A0
=C2=A0 136 R7NT de RA3-170-352 Op32=C2=A0<strong>968</strong>=C2=A0km -29 d=
B F:2% in=C2=A0
1541,4 Hz with 200w + E.sLoop (16)</span><br style=3D"color:rgb(0,0,0);font=
-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-10 06:11:58 R7NT=C2=A0 =C2=A0
=C2=A0<strong>943</strong>=C2=A0km 137540.871Hz=C2=A0 99mHz -39.3dBOp=C2=A0=
 88% 17.6dB
RN3AUS (1)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">06:44=C2=A0
=C2=A0 136 R7NT de RN3AUS Op32 -39 dB F:46% in KO85fn (<strong>942</strong>=
=C2=A0km)
nr Moscow + MiniWhip 137539.8 Hz (2)</span><br style=3D"color:rgb(0,0,0);fo=
nt-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:maroon">2019-02-09 21:32:30 RK2Y=C2=A0 =C2=A0
=C2=A0<strong>428</strong>=C2=A0km 137533.706Hz=C2=A0 =C2=A04mHz -34.5dBOp =
100% 19.0dB EW6X
(1)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">21:32=C2=A0
=C2=A0 136 RK2Y de EW6X Op32 -35 dB F:5% in KO45kl (<strong>428</strong>=C2=
=A0
km) Polotsk + miniwhip 137533.7 Hz (1)</span><br style=3D"color:rgb(0,0,0);=
font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red">21:32=C2=A0
=C2=A0 136 RK2Y de RA3-170-352 Op32=C2=A0<strong>359</strong>=C2=A0 km -33 =
dB F:2% in=C2=A0
1534,1 Hz (1)</span><br style=3D"color:rgb(0,0,0);font-size:12.48px">
  <span class=3D"gmail-m_-8520955909902486638gmail-bbc_color" style=3D"font=
-size:12.48px;color:red"><strong>OP32
:</strong>=C2=A0TX-2=C2=A0 RX-12=C2=A0</span><span style=3D"color:rgb(0,0,0=
);font-size:12.48px"></span><span class=3D"gmail-m_-8520955909902486638gmai=
l-bbc_color" style=3D"font-size:12.48px;color:maroon"><strong>OPds</strong>=
=C2=A0RX-7</span>=C2=A0</font>
  <div style=3D"font-size:12.8px"><font style=3D"background-color:rgb(243,2=
43,243)" face=3D"arial, helvetica, sans-serif"><span style=3D"color:rgb(0,0=
,0);font-size:12.48px;line-height:17.472px">(n)
- it&#39;s the total number of the reports - it&#39;s the best result of th=
e
reports - it&#39;s the first result over time with the same levels</span><b=
r>
  </font></div>
  <div style=3D"font-size:12.8px"><span style=3D"font-family:arial,helvetic=
a,sans-serif;font-size:12.48px;color:rgb(0,0,0)">E.sLoop
+ 200W Output</span><span style=3D"background-color:rgb(243,243,243);font-f=
amily:arial,helvetica,sans-serif;font-size:small">=C2=A0</span><span style=
=3D"background-color:rgb(243,243,243);font-family:arial,helvetica,sans-seri=
f;font-size:small">=C2=A0</span><br>
  </div>
  </div>
</blockquote>
</div>

</blockquote></div>

--0000000000007236a60581879e4e--

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 Content preview:  Hi VLF Congratulations Dimitris :-) Anybody mentioned an activity
    rush in VLF ? I'm working on this right now 
 Content analysis details:   (0.9 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
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 Content preview:  uhh Luis.. are you minded to grow roses?? :-D ----Messaggio
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uhh Luis..

are you minded to grow roses?? :-D





----Messaggio originale----

Da: luis@vigilant.es

Data: 10-feb-2019 13.41

A: "rsgb_lf_group@blacksheep.org"<rsgb_lf_group@blacksheep.org>

Ogg: Re: VLF: in VK?







Hi VLF



Congratulations Dimitris :-)



Anybody mentioned an activity rush in VLF ? I'm working on this right now



https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=3D=
0





73 de Luis
EA5DOM






El 9 feb. 2019 1:26 p. m., DK7FC <selberdenken@posteo.de> escribi=C3=B3:


Hi Dimitris,



My congrats! That is a good success and progress!



Can you tell more details?

How much power was used?

How much antenna current?

Was it the 3 turn loop?

What type of receiver was used on the RX site?

Is that site in a quiet location?

Which bandwidth or mode?

Was it actually QRSS-10 (Which i would watch in 122 mHz)?

What was the SNR?

Is there a screenshot for us to see?

What is your plan for today? :-)

Who is the next distant station?



This could be the beginning of a growing worldwide VLF activity, if you=20

can 'mobilise' a team of stations who build up RX and TX systems arround=20

VK.



73, Stefan





Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:

> Hi Stefan and VLF,

>

> well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)

> has been detected 22.3 km away in Canberra by Dale VK1DSH. Only

> casualty is the russian mica capacitors (K31-11-3) which got really

> hot (I was focusing on the amplifier and neglected the poor caps). I

> had 4 of them in parallel, each 4700 pF.  Maybe they will recover if I

> let them cool down :-)

>

> That's probably a first for Australia, I haven't heard anyone else

> doing tests like this.

>



















------=_Part_43846_2469168.1549803549525
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uhh Luis..<br><br>are you minded to grow roses?? :-D<br><br><br>
<br>
----Messaggio originale----<br>
Da: luis@vigilant.es<br>
Data: 10-feb-2019 13.41<br>
A: "rsgb_lf_group@blacksheep.org"&lt;rsgb_lf_group@blacksheep.org&gt;<br>
Ogg: Re: VLF: in VK?<br>
<br>

<!--

-->

<div dir=3D"auto">
<div>Hi VLF
<div dir=3D"auto"><br>
</div>
<div dir=3D"auto">Congratulations Dimitris :-)</div>
<div dir=3D"auto"><br>
</div>
<div dir=3D"auto">Anybody mentioned an activity rush in VLF ? I'm working o=
n this right now</div>
<div dir=3D"auto"><br>
</div>
<div dir=3D"auto">https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_10=
4522_952.jpg?dl=3D0<br>
</div>
<div dir=3D"auto"><br>
</div>
73 de Luis</div>
<div dir=3D"auto">EA5DOM<br>
<div class=3D"gmail_extra" dir=3D"auto"><br>
</div>
<div class=3D"gmail_extra" dir=3D"auto"><br>
<div class=3D"gmail_quote">El 9 feb. 2019 1:26 p. m., DK7FC &lt;selberdenke=
n@posteo.de&gt; escribi=C3=B3:<br type=3D"attribution">
<blockquote class=3D"quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc=
 solid;padding-left:1ex">
<div><font size=3D"2"><span style=3D"font-size:10pt">
<div>Hi Dimitris,<br>
<br>
My congrats! That is a good success and progress!<br>
<br>
Can you tell more details?<br>
How much power was used?<br>
How much antenna current?<br>
Was it the 3 turn loop?<br>
What type of receiver was used on the RX site?<br>
Is that site in a quiet location?<br>
Which bandwidth or mode?<br>
Was it actually QRSS-10 (Which i would watch in 122 mHz)?<br>
What was the SNR?<br>
Is there a screenshot for us to see?<br>
What is your plan for today? :-)<br>
Who is the next distant station?<br>
<br>
This could be the beginning of a growing worldwide VLF activity, if you <br=
>
can 'mobilise' a team of stations who build up RX and TX systems arround <b=
r>
VK.<br>
<br>
73, Stefan<br>
<br>
<br>
Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:<br>
&gt; Hi Stefan and VLF,<br>
&gt;<br>
&gt; well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)<b=
r>
&gt; has been detected 22.3 km away in Canberra by Dale VK1DSH. Only<br>
&gt; casualty is the russian mica capacitors (K31-11-3) which got really<br=
>
&gt; hot (I was focusing on the amplifier and neglected the poor caps). I<b=
r>
&gt; had 4 of them in parallel, each 4700 pF.&nbsp; Maybe they will recover=
 if I<br>
&gt; let them cool down :-)<br>
&gt;<br>
&gt; That's probably a first for Australia, I haven't heard anyone else<br>
&gt; doing tests like this.<br>
&gt;<br>
<br>
</div>
</span></font></div>
</blockquote>
</div>
<br>
</div>
</div>
</div>


<br>
<br>

------=_Part_43846_2469168.1549803549525--


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Date: Sun, 10 Feb 2019 14:01:15 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hi Luis, Great! I somehow know that plastic pot :-) What is
    the wire diameter? Make sure to use double-sided bonding tape between the
    pot and the wire, otherwise the winding will move when becoming warm and
   co [...] 
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Subject: Re: VLF: in EA?
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--------------020907060006030509000905
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Hi Luis,

Great! I somehow know that plastic pot :-)
What is the wire diameter?
Make sure to use double-sided bonding tape between the pot and the wire, 
otherwise the winding will move when becoming warm and cold and warm and 
cold again. Also i would really recommend to use that Kapton tape, the 
cheap version from China is fully OK, for example: 
https://www.amazon.de/dp/B00CAMEB4W

Good luck :-)

73, Stefan

Am 10.02.2019 13:41, schrieb VIGILANT Luis Fernández:
> Hi VLF
>
> Congratulations Dimitris :-)
>
> Anybody mentioned an activity rush in VLF ? I'm working on this right now
>
> https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=0
>
> 73 de Luis
> EA5DOM
>
>
> El 9 feb. 2019 1:26 p. m., DK7FC <selberdenken@posteo.de> escribió:
>
>     Hi Dimitris,
>
>     My congrats! That is a good success and progress!
>
>     Can you tell more details?
>     How much power was used?
>     How much antenna current?
>     Was it the 3 turn loop?
>     What type of receiver was used on the RX site?
>     Is that site in a quiet location?
>     Which bandwidth or mode?
>     Was it actually QRSS-10 (Which i would watch in 122 mHz)?
>     What was the SNR?
>     Is there a screenshot for us to see?
>     What is your plan for today? :-)
>     Who is the next distant station?
>
>     This could be the beginning of a growing worldwide VLF activity,
>     if you
>     can 'mobilise' a team of stations who build up RX and TX systems
>     arround
>     VK.
>
>     73, Stefan
>
>
>     Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:
>     > Hi Stefan and VLF,
>     >
>     > well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)
>     > has been detected 22.3 km away in Canberra by Dale VK1DSH. Only
>     > casualty is the russian mica capacitors (K31-11-3) which got really
>     > hot (I was focusing on the amplifier and neglected the poor caps). I
>     > had 4 of them in parallel, each 4700 pF.  Maybe they will recover
>     if I
>     > let them cool down :-)
>     >
>     > That's probably a first for Australia, I haven't heard anyone else
>     > doing tests like this.
>     >
>
>

--------------020907060006030509000905
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 8bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
  <title></title>
</head>
<body bgcolor="#ffffff" text="#000000">
Hi Luis, <br>
<br>
Great! I somehow know that plastic pot :-)<br>
What is the wire diameter?<br>
Make sure to use double-sided bonding tape between the pot and the
wire, otherwise the winding will move when becoming warm and cold and
warm and cold again. Also i would really recommend to use that Kapton
tape, the cheap version from China is fully OK, for example:
<a class="moz-txt-link-freetext" href="https://www.amazon.de/dp/B00CAMEB4W">https://www.amazon.de/dp/B00CAMEB4W</a><br>
<br>
Good luck :-)<br>
<br>
73, Stefan<br>
<br>
Am 10.02.2019 13:41, schrieb VIGILANT Luis Fernández:
<blockquote
 cite="mid:1bd64d1b-12b3-4abc-b7f0-34a0076c2c9f@email.android.com"
 type="cite">
  <meta http-equiv="Content-Type" content="text/html; charset=UTF-8">
  <div dir="auto">
  <div>Hi VLF
  <div dir="auto"><br>
  </div>
  <div dir="auto">Congratulations Dimitris :-)</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">Anybody mentioned an activity rush in VLF ? I'm
working on this right now</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto"><a class="moz-txt-link-freetext" href="https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=0">https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=0</a><br>
  </div>
  <div dir="auto"><br>
  </div>
73 de Luis</div>
  <div dir="auto">EA5DOM<br>
  <div class="gmail_extra" dir="auto"><br>
  </div>
  <div class="gmail_extra" dir="auto"><br>
  <div class="gmail_quote">El 9 feb. 2019 1:26 p. m., DK7FC
<a class="moz-txt-link-rfc2396E" href="mailto:selberdenken@posteo.de">&lt;selberdenken@posteo.de&gt;</a> escribió:<br type="attribution">
  <blockquote class="quote"
 style="border-left: 1px solid rgb(204, 204, 204); margin: 0pt 0pt 0pt 0.8ex; padding-left: 1ex;">
    <div><font size="2"><span style="font-size: 10pt;">
    <div>Hi Dimitris,<br>
    <br>
My congrats! That is a good success and progress!<br>
    <br>
Can you tell more details?<br>
How much power was used?<br>
How much antenna current?<br>
Was it the 3 turn loop?<br>
What type of receiver was used on the RX site?<br>
Is that site in a quiet location?<br>
Which bandwidth or mode?<br>
Was it actually QRSS-10 (Which i would watch in 122 mHz)?<br>
What was the SNR?<br>
Is there a screenshot for us to see?<br>
What is your plan for today? :-)<br>
Who is the next distant station?<br>
    <br>
This could be the beginning of a growing worldwide VLF activity, if you
    <br>
can 'mobilise' a team of stations who build up RX and TX systems
arround <br>
VK.<br>
    <br>
73, Stefan<br>
    <br>
    <br>
Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:<br>
&gt; Hi Stefan and VLF,<br>
&gt;<br>
&gt; well, I am now officially hooked! My signal on 29.5 kHz (VLF's
edge)<br>
&gt; has been detected 22.3 km away in Canberra by Dale VK1DSH. Only<br>
&gt; casualty is the russian mica capacitors (K31-11-3) which got really<br>
&gt; hot (I was focusing on the amplifier and neglected the poor caps).
I<br>
&gt; had 4 of them in parallel, each 4700 pF.  Maybe they will recover
if I<br>
&gt; let them cool down :-)<br>
&gt;<br>
&gt; That's probably a first for Australia, I haven't heard anyone else<br>
&gt; doing tests like this.<br>
&gt;<br>
    <br>
    </div>
    </span></font></div>
  </blockquote>
  </div>
  <br>
  </div>
  </div>
  </div>
</blockquote>
</body>
</html>

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Date: Sun, 10 Feb 2019 13:27:24 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello VIGILANT, You are going to grow a sunflower and use
   it as an antenna? That's, errr, different :) A change from wet string! Sunday,
    February 10, 2019, 12:41:07 PM, you wrote: 
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Hello VIGILANT,

You  are  going  to grow a sunflower and use it as an antenna? That's,
errr, different :) A change from wet string!

Sunday, February 10, 2019, 12:41:07 PM, you wrote:

>   
>  
>  
> Hi VLF 

>   
> Congratulations Dimitris :-) 

>   
> Anybody mentioned an activity rush in VLF ? I'm working on this right now

>   
> https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=0
>   

>   73 de Luis 
> EA5DOM


-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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 Content preview:  I used a 2 x 2 m receiving loop for 136 kHz until a wild beast
    from the forest demolished it. John F5VLF > On 10 Feb 2019, at 14:27, Chris
    Wilson wrote: > > > > Hello VIGILANT, > > You are going to grow a sunflower
    and use it as an antenna? That's, > errr, different :) A change from wet
   string! > > Sun [...] 
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Subject: Re: VLF: in VK?
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I used a 2 x 2 m receiving loop for 136 kHz until a wild beast from the =
forest demolished it.

John F5VLF



> On 10 Feb 2019, at 14:27, Chris Wilson <dead.fets@gmail.com> wrote:
>=20
>=20
>=20
> Hello VIGILANT,
>=20
> You  are  going  to grow a sunflower and use it as an antenna? That's,
> errr, different :) A change from wet string!
>=20
> Sunday, February 10, 2019, 12:41:07 PM, you wrote:
>=20

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<html><head><meta http-equiv=3D"Content-Type" content=3D"text/html; =
charset=3Dus-ascii"></head><body style=3D"word-wrap: break-word; =
-webkit-nbsp-mode: space; line-break: after-white-space;" class=3D"">I =
used a 2 x 2 m receiving loop for 136 kHz until a wild beast from the =
forest demolished it.<div class=3D""><br class=3D""></div><div =
class=3D"">John F5VLF</div><div class=3D""><br class=3D""></div><div =
class=3D""><img apple-inline=3D"yes" =
id=3D"1C34AF6B-61A7-4A2F-98ED-06D94A098A54" =
src=3D"cid:AFE3411E-6BCA-449A-BF3D-645438CA20AD" class=3D""><br =
class=3D""><div><br class=3D""><blockquote type=3D"cite" class=3D""><div =
class=3D"">On 10 Feb 2019, at 14:27, Chris Wilson &lt;<a =
href=3D"mailto:dead.fets@gmail.com" class=3D"">dead.fets@gmail.com</a>&gt;=
 wrote:</div><br class=3D"Apple-interchange-newline"><div class=3D""><div =
class=3D""><br class=3D""><br class=3D"">Hello VIGILANT,<br class=3D""><br=
 class=3D"">You &nbsp;are &nbsp;going &nbsp;to grow a sunflower and use =
it as an antenna? That's,<br class=3D"">errr, different :) A change from =
wet string!<br class=3D""><br class=3D"">Sunday, February 10, 2019, =
12:41:07 PM, you wrote:<br class=3D""><br =
class=3D""></div></div></blockquote></div></div></body></html>=

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Date: Sun, 10 Feb 2019 10:38:34 -0500
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 Content preview:  Does anyone know if the NASA sponsored VLF INSPIRE program
    is still viable? The web site and Facebook page for INSPIRE haven't been
   updated in years. -- 73 Warren K2ORS WD2XGJ WD2XSH/23 WE2XEB/2 WE2XGR/1 
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Subject: LF: NASA VLF INSPIRE ?
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Does anyone know if the NASA sponsored VLF INSPIRE program is still viable?
The web site and Facebook page for INSPIRE haven't been updated in years.


-- 
73 Warren K2ORS
                WD2XGJ
                WD2XSH/23
                WE2XEB/2
                WE2XGR/1

--000000000000df076d05818bfc3c
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<div dir=3D"ltr">Does anyone know if the NASA sponsored VLF INSPIRE program=
 is still viable?<div>The web site and Facebook page for INSPIRE haven&#39;=
t been updated in years.</div><div><br clear=3D"all"><div><br></div>-- <br>=
<div dir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"gmail_signatur=
e">73 Warren K2ORS<br>=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=
=A0 WD2XGJ <br>=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 WD2X=
SH/23<br>=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 WE2XEB/2<b=
r>=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 WE2XGR/1<br><br>=
=C2=A0</div></div></div>

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 Content preview:  Hi VLF No gardening at all. Just following the way Stefan
   and others paved so clearly ;-) This is a motorized table to make winding
   an easier task. The pot is 50cm diameter but don't trust the quality and resistance
    to UV light. Will test a different model more rugged and about the same si
    [...] 
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Subject: Re: VLF: in EA?
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Hi VLF

No gardening at all. Just following the way Stefan and others paved so clea=
rly ;-)

This is a motorized table to make winding an easier task. The pot is 50cm d=
iameter but don't trust the
quality and resistance to UV light. Will test a different model more rugged=
 and about the same size
Another picture showing the details of this "tricotosa"
https://www.dropbox.com/s/05pgt96om2meqwb/IMG_20190210_104538_802.jpg?dl=3D=
0

Got a 7Kg x 0.20mm coil of wire from a company which used to wind their own=
 motors (time ago)

Yes Stefan, I plan to use the double side bonding tape and kapton. One ques=
tion about it:
Do you place kapton over the plastic as a base layer ? or just covering the=
 coil as end layer ?

73 de Luis
EA5DOM

________________________________
De: owner-rsgb_lf_group@blacksheep.org [owner-rsgb_lf_group@blacksheep.org]=
 en nombre de DK7FC [selberdenken@posteo.de]
Enviado: domingo, 10 de febrero de 2019 14:01
Para: rsgb_lf_group@blacksheep.org
Asunto: Re: VLF: in EA?

Hi Luis,

Great! I somehow know that plastic pot :-)
What is the wire diameter?
Make sure to use double-sided bonding tape between the pot and the wire, ot=
herwise the winding will move when becoming warm and cold and warm and cold=
 again. Also i would really recommend to use that Kapton tape, the cheap ve=
rsion from China is fully OK, for example: https://www.amazon.de/dp/B00CAME=
B4W

Good luck :-)

73, Stefan

Am 10.02.2019 13:41, schrieb VIGILANT Luis Fern=E1ndez:
Hi VLF

Congratulations Dimitris :-)

Anybody mentioned an activity rush in VLF ? I'm working on this right now

https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=3D=
0

73 de Luis
EA5DOM


El 9 feb. 2019 1:26 p. m., DK7FC <selberdenken@posteo.de><mailto:selberdenk=
en@posteo.de> escribi=F3:
Hi Dimitris,

My congrats! That is a good success and progress!

Can you tell more details?
How much power was used?
How much antenna current?
Was it the 3 turn loop?
What type of receiver was used on the RX site?
Is that site in a quiet location?
Which bandwidth or mode?
Was it actually QRSS-10 (Which i would watch in 122 mHz)?
What was the SNR?
Is there a screenshot for us to see?
What is your plan for today? :-)
Who is the next distant station?

This could be the beginning of a growing worldwide VLF activity, if you
can 'mobilise' a team of stations who build up RX and TX systems arround
VK.

73, Stefan


Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:
> Hi Stefan and VLF,
>
> well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)
> has been detected 22.3 km away in Canberra by Dale VK1DSH. Only
> casualty is the russian mica capacitors (K31-11-3) which got really
> hot (I was focusing on the amplifier and neglected the poor caps). I
> had 4 of them in parallel, each 4700 pF.  Maybe they will recover if I
> let them cool down :-)
>
> That's probably a first for Australia, I haven't heard anyone else
> doing tests like this.
>



--_000_6DB8451D7F3D3947A5918808A59621EA31522A7Dservigilantvigi_
Content-Type: text/html; charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<html dir=3D"ltr">
<head>
<meta http-equiv=3D"Content-Type" content=3D"text/html; charset=3Diso-8859-=
1">
<style type=3D"text/css" id=3D"owaParaStyle"></style>
</head>
<body bgcolor=3D"#ffffff" fpstyle=3D"1" ocsi=3D"0">
<div style=3D"direction: ltr;font-family: Tahoma;color: #000000;font-size: =
10pt;">Hi VLF
<div><br>
</div>
<div>No gardening at all. Just following the way Stefan and others paved so=
 clearly ;-)</div>
<div><br>
</div>
<div>This is a motorized table to make winding an easier task. The pot is 5=
0cm diameter but don't trust the</div>
<div>quality and resistance to UV light. Will test a different model more r=
ugged and about the same size</div>
<div>Another picture showing the details of this &quot;tricotosa&quot;</div=
>
<div>https://www.dropbox.com/s/05pgt96om2meqwb/IMG_20190210_104538_802.jpg?=
dl=3D0</div>
<div><br>
</div>
<div>Got a 7Kg x 0.20mm coil of wire from a company which used to wind thei=
r own motors (time ago)</div>
<div><br>
</div>
<div>Yes Stefan, I plan to use the double side bonding tape and kapton. One=
 question about it:</div>
<div>Do you place kapton over the plastic as a base layer ? or just coverin=
g the coil as end layer ?</div>
<div><br>
</div>
<div>73 de Luis</div>
<div>EA5DOM</div>
<div><br>
<div style=3D"font-family: Times New Roman; color: #000000; font-size: 16px=
">
<hr tabindex=3D"-1">
<div id=3D"divRpF527390" style=3D"direction: ltr;"><font face=3D"Tahoma" si=
ze=3D"2" color=3D"#000000"><b>De:</b> owner-rsgb_lf_group@blacksheep.org [o=
wner-rsgb_lf_group@blacksheep.org] en nombre de DK7FC [selberdenken@posteo.=
de]<br>
<b>Enviado:</b> domingo, 10 de febrero de 2019 14:01<br>
<b>Para:</b> rsgb_lf_group@blacksheep.org<br>
<b>Asunto:</b> Re: VLF: in EA?<br>
</font><br>
</div>
<div></div>
<div>Hi Luis, <br>
<br>
Great! I somehow know that plastic pot :-)<br>
What is the wire diameter?<br>
Make sure to use double-sided bonding tape between the pot and the wire, ot=
herwise the winding will move when becoming warm and cold and warm and cold=
 again. Also i would really recommend to use that Kapton tape, the cheap ve=
rsion from China is fully OK, for
 example: <a class=3D"moz-txt-link-freetext" href=3D"https://www.amazon.de/=
dp/B00CAMEB4W" target=3D"_blank">
https://www.amazon.de/dp/B00CAMEB4W</a><br>
<br>
Good luck :-)<br>
<br>
73, Stefan<br>
<br>
Am 10.02.2019 13:41, schrieb VIGILANT Luis Fern=E1ndez:
<blockquote type=3D"cite">
<div dir=3D"auto">
<div>Hi VLF
<div dir=3D"auto"><br>
</div>
<div dir=3D"auto">Congratulations Dimitris :-)</div>
<div dir=3D"auto"><br>
</div>
<div dir=3D"auto">Anybody mentioned an activity rush in VLF ? I'm working o=
n this right now</div>
<div dir=3D"auto"><br>
</div>
<div dir=3D"auto"><a class=3D"moz-txt-link-freetext" href=3D"https://www.dr=
opbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=3D0" target=3D"_=
blank">https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jp=
g?dl=3D0</a><br>
</div>
<div dir=3D"auto"><br>
</div>
73 de Luis</div>
<div dir=3D"auto">EA5DOM<br>
<div class=3D"gmail_extra" dir=3D"auto"><br>
</div>
<div class=3D"gmail_extra" dir=3D"auto"><br>
<div class=3D"gmail_quote">El 9 feb. 2019 1:26 p. m., DK7FC <a class=3D"moz=
-txt-link-rfc2396E" href=3D"mailto:selberdenken@posteo.de" target=3D"_blank=
">
&lt;selberdenken@posteo.de&gt;</a> escribi=F3:<br type=3D"attribution">
<blockquote class=3D"quote" style=3D"border-left:1px solid rgb(204,204,204)=
; margin:0pt 0pt 0pt 0.8ex; padding-left:1ex">
<div><font size=3D"2"><span style=3D"font-size:10pt">
<div>Hi Dimitris,<br>
<br>
My congrats! That is a good success and progress!<br>
<br>
Can you tell more details?<br>
How much power was used?<br>
How much antenna current?<br>
Was it the 3 turn loop?<br>
What type of receiver was used on the RX site?<br>
Is that site in a quiet location?<br>
Which bandwidth or mode?<br>
Was it actually QRSS-10 (Which i would watch in 122 mHz)?<br>
What was the SNR?<br>
Is there a screenshot for us to see?<br>
What is your plan for today? :-)<br>
Who is the next distant station?<br>
<br>
This could be the beginning of a growing worldwide VLF activity, if you <br=
>
can 'mobilise' a team of stations who build up RX and TX systems arround <b=
r>
VK.<br>
<br>
73, Stefan<br>
<br>
<br>
Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:<br>
&gt; Hi Stefan and VLF,<br>
&gt;<br>
&gt; well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)<b=
r>
&gt; has been detected 22.3 km away in Canberra by Dale VK1DSH. Only<br>
&gt; casualty is the russian mica capacitors (K31-11-3) which got really<br=
>
&gt; hot (I was focusing on the amplifier and neglected the poor caps). I<b=
r>
&gt; had 4 of them in parallel, each 4700 pF.&nbsp; Maybe they will recover=
 if I<br>
&gt; let them cool down :-)<br>
&gt;<br>
&gt; That's probably a first for Australia, I haven't heard anyone else<br>
&gt; doing tests like this.<br>
&gt;<br>
<br>
</div>
</span></font></div>
</blockquote>
</div>
<br>
</div>
</div>
</div>
</blockquote>
</div>
</div>
</div>
</div>
</body>
</html>

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 Content preview:  Hello Luis, Am 10.02.2019 19:42, schrieb VIGILANT Luis Fern�ndez:
    > > Got a 7Kg x 0.20mm coil of wire from a company which used to wind > their
    own motors (time ago) Oh that will be enough! 0.2 mm is almost a bit [...]
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Hello Luis,

Am 10.02.2019 19:42, schrieb VIGILANT Luis Fern�ndez:
>
> Got a 7Kg x 0.20mm coil of wire from a company which used to wind 
> their own motors (time ago)
Oh that will be enough! 0.2 mm is almost a bit thin but still ok. But it 
will not handle more than 250 mA i think, when using some forced 
cooling, otherwise it may hold 200 mA.

> Yes Stefan, I plan to use the double side bonding tape and kapton. One 
> question about it:
> Do you place kapton over the plastic as a base layer ? or just 
> covering the coil as end layer ?
I just covered the winding. As soon as the fresh wound coil allowed to 
add another layer of the Kapton tape i fixed it, i.e. it was wound 
arround the coil during the winding process. This gives a good 
mechanical stability from the first moment.
The pot is out of PVC so one has to take care not to cause an arcing 
track on the surface. Prevent it from humdity and sunlight. However due 
to the stacking of pots, which will be necessary, the voltage between 
two pots should not be higher than something arround 5 kV and therefore 
the field strength along the winding (or volts per turn) will be small, 
so it is not crtical to use PVC. All my recent wound coils are on PVC.

73, Stefan

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Hello Luis, <br>
<br>
Am 10.02.2019 19:42, schrieb VIGILANT Luis Fern&aacute;ndez:
<blockquote
 cite="mid:6DB8451D7F3D3947A5918808A59621EA31522A7D@servigilant.vigilant.local"
 type="cite">
  <meta http-equiv="Content-Type"
 content="text/html; charset=ISO-8859-1">
  <style type="text/css" id="owaParaStyle"></style>
  <div
 style="direction: ltr; font-family: Tahoma; color: rgb(0, 0, 0); font-size: 10pt;"><br>
  <div>Got a 7Kg x 0.20mm coil of wire from a company which used to
wind their own motors (time ago)</div>
  </div>
</blockquote>
Oh that will be enough! 0.2 mm is almost a bit thin but still ok. But
it will not handle more than 250 mA i think, when using some forced
cooling, otherwise it may hold 200 mA.<br>
<br>
<blockquote
 cite="mid:6DB8451D7F3D3947A5918808A59621EA31522A7D@servigilant.vigilant.local"
 type="cite">
  <div
 style="direction: ltr; font-family: Tahoma; color: rgb(0, 0, 0); font-size: 10pt;">
  <div>Yes Stefan, I plan to use the double side bonding tape and
kapton. One question about it:</div>
  <div>Do you place kapton over the plastic as a base layer ? or just
covering the coil as end layer ?</div>
  </div>
</blockquote>
I just covered the winding. As soon as the fresh wound coil allowed to
add another layer of the Kapton tape i fixed it, i.e. it was wound
arround the coil during the winding process. This gives a good
mechanical stability from the first moment.<br>
The pot is out of PVC so one has to take care not to cause an arcing
track on the surface. Prevent it from humdity and sunlight. However due
to the stacking of pots, which will be necessary, the voltage between
two pots should not be higher than something arround 5 kV and therefore
the field strength along the winding (or volts per turn) will be small,
so it is not crtical to use PVC. All my recent wound coils are on PVC.<br>
<br>
73, Stefan<br>
</body>
</html>

--------------060305070301020402080904--

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 Content preview:  LF EbNaut, I suspended the final day of transmissions (tonight)
    due to TX low pass filter overheating. Thanks for the reports from DK7FC,
    F5WK and K3SIW. 73, Rob - K3RWR 
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LF EbNaut,

I suspended the final day of transmissions (tonight) due to TX low pass filter  overheating.  Thanks for the reports from DK7FC, F5WK and K3SIW.

73,
Rob - K3RWR

> On Feb 8, 2019, at 06:15, Rob Renoud <k3rwr@md.metrocast.net> wrote:
> 
> LF EbNaut,
> 
> I will run an LF EbNaut beacon this weekend from 8 Feb - 10 Feb (3 days) as follows:
> 
> QRG:  137479.000 Hz
> Code:  8K19A
> CRC: 16
> Symbol:  3 sec
> Char:  7
> Duration:  30:24.0 (1824 sec)
> Start/Stop:  2100 UTC / 1100 UTC (last)
> Repeat on the hour with carrier during idle.  1W EIRP.  10 min CW ID (20 WPM) on modulated and unmodulated carrier.
> 
> 73,
> Rob - K3RWR
> FM18qi



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Date: Mon, 11 Feb 2019 11:09:48 +1100
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 Content preview:  Hi Luis, Looks good! My first large loading coil was my laundy
    basket. My wife wasn't terribly impressed but for a period, it served both
    as loading coil and a laundry basket :-) 73 and good luck with your experiments!
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Hi Luis,

Looks good! My first large loading coil was my laundy basket. My wife
wasn't terribly impressed but for a period, it served both as loading
coil and a laundry basket :-)

73 and good luck with your experiments!


Στις Κυρ, 10 Φεβ 2019 στις 11:46 μ.μ., ο/η VIGILANT Luis Fernández
<luis@vigilant.es> έγραψε:
>
> Hi VLF
>
> Congratulations Dimitris :-)
>
> Anybody mentioned an activity rush in VLF ? I'm working on this right now
>
> https://www.dropbox.com/s/1vkmlm8kn80688l/IMG_20190210_104522_952.jpg?dl=0
>
> 73 de Luis
> EA5DOM
>
>
> El 9 feb. 2019 1:26 p. m., DK7FC <selberdenken@posteo.de> escribió:
>
> Hi Dimitris,
>
> My congrats! That is a good success and progress!
>
> Can you tell more details?
> How much power was used?
> How much antenna current?
> Was it the 3 turn loop?
> What type of receiver was used on the RX site?
> Is that site in a quiet location?
> Which bandwidth or mode?
> Was it actually QRSS-10 (Which i would watch in 122 mHz)?
> What was the SNR?
> Is there a screenshot for us to see?
> What is your plan for today? :-)
> Who is the next distant station?
>
> This could be the beginning of a growing worldwide VLF activity, if you
> can 'mobilise' a team of stations who build up RX and TX systems arround
> VK.
>
> 73, Stefan
>
>
> Am 08.02.2019 23:01, schrieb Dimitrios Tsifakis:
> > Hi Stefan and VLF,
> >
> > well, I am now officially hooked! My signal on 29.5 kHz (VLF's edge)
> > has been detected 22.3 km away in Canberra by Dale VK1DSH. Only
> > casualty is the russian mica capacitors (K31-11-3) which got really
> > hot (I was focusing on the amplifier and neglected the poor caps). I
> > had 4 of them in parallel, each 4700 pF.  Maybe they will recover if I
> > let them cool down :-)
> >
> > That's probably a first for Australia, I haven't heard anyone else
> > doing tests like this.
> >
>
>


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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Mon, 11 Feb 2019 11:07:18 +1100
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 Content preview:  Hi Stefan, > > The unexpected losses are not just the > >
   capacitors (their contribution is probably small). It is also the > > coaxial
    cable that I used between the antenna feedpoint and the > > amplifier. >
   Ho [...] 
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Hi Stefan,

> > The unexpected losses are not just the
> > capacitors (their contribution is probably small). It is also the
> > coaxial cable that I used between the antenna feedpoint and the
> > amplifier.
> How long is that cable? And didn't you use a ferrite transformer to
> match the loop to the amplifier? If it is a normal audio amplifier that
> expects a 4 Ohm load, then maybe you don't need one, but then you should
> place the amp close to the loop, without the coax cable inbetween. If
> the loop is far from the house and you want to stay the amp into the
> shack, then use 2 ferrite transformers to transform up to 50 Ohm and
> then down to the antenna impedance again. I would place the amp in the
> shack and monitor voltage and current there using a scope. Then you see
> their ration (Impedance) and product = power (at resonance). I would
> first build a transformer that matches 4 Ohm to 50 Ohm for example, then
> use the cable, and then a transformer from 50 Ohm to the feedpoint
> impedance of the tuned loop.

Given the antenna has an impedance of about ~4 ohm and the amplifier
produces its maximum output on that impedance, it was tempting not to
do any impedance transformation and to stay at 4 ohm.

I have an idea about impedance transformation and that is to use high
power 70V/100V audio distribution transformers at both ends. I don't
have to go to 50 ohm as I don't use the coaxial cable as a
transmission line (it's only a tiny percentage of the wavelength!), so
I could use a 4 ohm to 400 ohm transformer or similar. I think in
general the impedance transformation ratio goes down as the power
rating goes up and we can live with that. THe audio transformer should
work fine on the higher frequency but that will have to be tested.
Perhaps something like this but not at that price!!

https://www.altronics.com.au/p/m1160-300w-100v-line-pa-transformer/

Another option is to get a PA amplifier of suitable power output that
has a 70V or 100V output. You only need one transformer at the antenna
end to get down to 4 ohm to reduce losses. I have a 50 W amp with such
output but that's not enough power.

> In the end, such a closed loop will not perform as good as a ground
> loop. You will get much better results when connecting two of these
> little ponds beeing some hunderet meter distant. The current will be
> lower and so the capacitors will be less stressed.

I can easily try the ground loop on the 120m long antenna as I do have
ground rods at both ends. It would be interesting to compare the
signal strength in both cases. THat's why I am building a network of
VLF stations by giving away the large ferrite rods to interested
amateurs! They can help doing comparisons like this.

> BTW is your ground very dry? you could even try a dipole on the ground
> for the 630m band. A full size dipole. It would be able to carry much RF
> power :-)

The ground is very rocky and there is almost no soil at the top.
Typical Australian native vegetation is the only thing that can
survive on it. I have thought about the dipole on the ground and I
have the perfect spot for it which is putting the feed point at the
top of the hill therefore making an inverted-V :-) Only concern with
that is the high voltage at the end of the dipole wires and the
possibility of a bush fire ignition. Definitely a project for winter!

> And what about a vertical antenna?

I have tried to tune my ~120 metre wire to VLF in the past with mixed
results. Worth revisiting this. The wire basically starts at my house
and follows the hill resulting in the top of the wire being maybe 20
metres higher than the bottom.

> Oh i see, i would spend several hours per day there building antennas!

;-) It was part of the motivation for buying this property!

73, Dimitris

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To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: LF: NASA VLF INSPIRE ?
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 Content preview:  Hi Warren - I got the last edition of the inspire mag a 9
   months back bit havent checked the site since then - Laurence > On Feb 10,
    2019, at 6:41 AM, Warren Ziegle wrote: > > Does anyone know if the NASA sponsored
    VLF INSPIRE program is still viable? > The web site and Facebook page for
    INSPIRE haven't been updated [...] 
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Hi Warren - I got the last edition of the inspire mag a 9 months back bit havent checked the site since then - 

Laurence

> On Feb 10, 2019, at 6:41 AM, Warren Ziegle <wd2xgj@gmail.com> wrote:
> 
> Does anyone know if the NASA sponsored VLF INSPIRE program is still viable?
> The web site and Facebook page for INSPIRE haven't been updated in years.
> 
> 
> -- 
> 73 Warren K2ORS
>                 WD2XGJ 
>                 WD2XSH/23
>                 WE2XEB/2
>                 WE2XGR/1
> 
>  


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See Attachment

73 de


See Attachment..

ANTENNA: MiniWhip


*Update: 11/02/2019*


*LOG -136.00 KHz*

*2019*

2E0ILY--wspr

DF6NM--wspr

DK7FC--wspr

DL7NN--wspr

EA5DOM--wspr

IK1HGI--Op.DS

IW4DXW--wspr

IZ7SLZ--wspr

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*2018*

2E0ILY--wspr

9A3KB--Op.32

DC0DX--wspr

EA5DOM--Op.32

IK1HSS--wspr

IW4DXW--wspr--Op.32

73 de Daniele
*I55387FI*
www.scientific-notes.blogspot.com

--000000000000b65b9205819bbcf0
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><pre class=3D"gmail-tw-data-text gmail-tw-ta gmail-tw-text=
-medium" id=3D"gmail-tw-target-text" dir=3D"ltr" style=3D"unicode-bidi:isol=
ate;border:none;padding:0px 0.14em 0px 0px;margin-top:0px;margin-bottom:0px=
;font-family:inherit;overflow:hidden;width:275px;white-space:pre-wrap;color=
:rgb(33,33,33);height:36px;font-size:29px;line-height:36px"><p style=3D"col=
or:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16px;font-v=
ariant-numeric:normal;font-variant-east-asian:normal;margin:0px;white-space=
:normal">See Attachment</p><p style=3D"color:rgb(0,0,0);font-family:&quot;T=
imes New Roman&quot;;font-size:16px;font-variant-numeric:normal;font-varian=
t-east-asian:normal;margin:0px;white-space:normal">73 de=C2=A0</p><p style=
=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16px=
;font-variant-numeric:normal;font-variant-east-asian:normal;margin:0px;whit=
e-space:normal"><br></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Time=
s New Roman&quot;;font-size:16px;font-variant-numeric:normal;font-variant-e=
ast-asian:normal;margin:0px;white-space:normal">See Attachment..</p><p styl=
e=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16p=
x;font-variant-numeric:normal;font-variant-east-asian:normal;margin:0px;whi=
te-space:normal">ANTENNA: MiniWhip</p><p style=3D"color:rgb(0,0,0);font-fam=
ily:&quot;Times New Roman&quot;;font-size:16px;font-variant-numeric:normal;=
font-variant-east-asian:normal;margin:0px;white-space:normal"><br></p><p st=
yle=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:1=
6px;font-variant-numeric:normal;font-variant-east-asian:normal;margin:0px;w=
hite-space:normal"><font color=3D"#00ff00"><b><i><u style=3D"background-col=
or:red">Update: 11/02/2019</u></i></b></font></p><p style=3D"color:rgb(0,0,=
0);font-family:&quot;Times New Roman&quot;;font-size:16px;font-variant-nume=
ric:normal;font-variant-east-asian:normal;margin:0px;white-space:normal"><b=
><i><u><font color=3D"#b02500" style=3D"background-color:red"></font></u></=
i></b><br></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Roma=
n&quot;;font-size:16px;font-variant-numeric:normal;font-variant-east-asian:=
normal;margin:0px;white-space:normal"><font color=3D"#00ff00" style=3D"back=
ground-color:red"><b>LOG -136.00 KHz</b></font></p><p style=3D"color:rgb(0,=
0,0);font-family:&quot;Times New Roman&quot;;font-size:16px;font-variant-nu=
meric:normal;font-variant-east-asian:normal;margin:0px;white-space:normal">=
<b><font color=3D"#ff0000">2019</font></b></p><p style=3D"color:rgb(0,0,0);=
font-family:&quot;Times New Roman&quot;;font-size:16px;font-variant-numeric=
:normal;font-variant-east-asian:normal;margin:0px;white-space:normal"><font=
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mal;font-variant-east-asian:normal;margin:0px;white-space:normal"><font col=
or=3D"#ffffff">DF6NM--wspr</font></p><p style=3D"color:rgb(0,0,0);font-fami=
ly:&quot;Times New Roman&quot;;font-size:16px;font-variant-numeric:normal;f=
ont-variant-east-asian:normal;margin:0px;white-space:normal"><font color=3D=
"#ffffff">DK7FC--wspr</font></p><p style=3D"color:rgb(0,0,0);font-family:&q=
uot;Times New Roman&quot;;font-size:16px;font-variant-numeric:normal;font-v=
ariant-east-asian:normal;margin:0px;white-space:normal"><font color=3D"#fff=
fff">DL7NN--wspr</font></p><p style=3D"color:rgb(0,0,0);font-family:&quot;T=
imes New Roman&quot;;font-size:16px;font-variant-numeric:normal;font-varian=
t-east-asian:normal;margin:0px;white-space:normal"><font color=3D"#ffffff">=
EA5DOM--wspr</font></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times=
 New Roman&quot;;font-size:16px;font-variant-numeric:normal;font-variant-ea=
st-asian:normal;margin:0px;white-space:normal"><font color=3D"#ffffff">IK1H=
GI--Op.DS</font></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times Ne=
w Roman&quot;;font-size:16px;font-variant-numeric:normal;font-variant-east-=
asian:normal;margin:0px;white-space:normal"><font color=3D"#ffffff">IW4DXW-=
-wspr</font></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Ro=
man&quot;;font-size:16px;font-variant-numeric:normal;font-variant-east-asia=
n:normal;margin:0px;white-space:normal"><font color=3D"#ffffff">IZ7SLZ--wsp=
r</font></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&=
quot;;font-size:16px;font-variant-numeric:normal;font-variant-east-asian:no=
rmal;margin:0px;white-space:normal"><font color=3D"#ffffff">M0DSZ--wspr</fo=
nt></p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;=
;font-size:16px;font-variant-numeric:normal;font-variant-east-asian:normal;=
margin:0px;white-space:normal"><font color=3D"#ffffff">R7NT--Op.32</font></=
p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font=
-size:16px;font-variant-numeric:normal;font-variant-east-asian:normal;margi=
n:0px;white-space:normal"><font color=3D"#ffffff">SV8CS--wspr--Op.32</font>=
</p><p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;fo=
nt-size:16px;font-variant-numeric:normal;font-variant-east-asian:normal;mar=
gin:0px;white-space:normal"><b><font color=3D"#ff0000">2018</font></b></p><=
p style=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-si=
ze:16px;font-variant-numeric:normal;font-variant-east-asian:normal;margin:0=
px;white-space:normal"><font color=3D"#ffffff">2E0ILY--wspr</font></p><p st=
yle=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:1=
6px;font-variant-numeric:normal;font-variant-east-asian:normal;margin:0px;w=
hite-space:normal"><font color=3D"#ffffff">9A3KB--Op.32</font></p><p style=
=3D"color:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16px=
;font-variant-numeric:normal;font-variant-east-asian:normal;margin:0px;whit=
e-space:normal"><font color=3D"#ffffff">DC0DX--wspr</font></p><p style=3D"c=
olor:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16px;font=
-variant-numeric:normal;font-variant-east-asian:normal;margin:0px;white-spa=
ce:normal"><font color=3D"#ffffff">EA5DOM--Op.32</font></p><p style=3D"colo=
r:rgb(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16px;font-va=
riant-numeric:normal;font-variant-east-asian:normal;margin:0px;white-space:=
normal"><font color=3D"#ffffff">IK1HSS--wspr</font></p><p style=3D"color:rg=
b(0,0,0);font-family:&quot;Times New Roman&quot;;font-size:16px;font-varian=
t-numeric:normal;font-variant-east-asian:normal;margin:0px;white-space:norm=
al"><font color=3D"#ffffff">IW4DXW--wspr--Op.32</font></p></pre><div><div d=
ir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"gmail_signature"><di=
v dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div dir=
=3D"ltr"><div><span style=3D"font-size:14px">73 de=C2=A0</span><span style=
=3D"font-size:14px">Daniele</span></div><div dir=3D"ltr"><font size=3D"4"><=
b>I55387FI</b></font><br><div><div><div><font color=3D"#0000ff" face=3D"Ver=
dana"><a href=3D"http://www.scientific-notes.blogspot.com" target=3D"_blank=
">www.scientific-notes.blogspot.com</a></font></div><div><font color=3D"#00=
00ff" face=3D"Verdana"><br></font></div><div><br></div></div></div></div></=
div></div></div></div></div></div></div></div>

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Date: Mon, 11 Feb 2019 11:59:29 +0000
From: Chris Wilson <dead.fets@gmail.com>
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To: Daniele Caccia <rsgb_lf_group@blacksheep.org>
CC: Daniele Caccia <daniele.caccia74@gmail.com>
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 Content preview:  Hello Daniele, Thanks for the reports Daniele, and may I say
    that you a nice web site there, very interesting! All the best from 2E0ILY
    Monday, February 11, 2019, 10:25:54 AM, you wrote: 
 Content analysis details:   (0.0 points, 5.0 required)
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Hello Daniele,

Thanks for the reports Daniele, and may I say that you a nice web site
there, very interesting! All the best from 2E0ILY

Monday, February 11, 2019, 10:25:54 AM, you wrote:

> See Attachment

> 73 de 




> See Attachment..

> ANTENNA: MiniWhip




> Update: 11/02/2019




> LOG -136.00 KHz

> 2019

> 2E0ILY--wspr

> DF6NM--wspr

> DK7FC--wspr

> DL7NN--wspr

> EA5DOM--wspr

> IK1HGI--Op.DS

> IW4DXW--wspr

> IZ7SLZ--wspr

> M0DSZ--wspr

> R7NT--Op.32

> SV8CS--wspr--Op.32

> 2018

> 2E0ILY--wspr

> 9A3KB--Op.32

> DC0DX--wspr

> EA5DOM--Op.32

> IK1HSS--wspr

> IW4DXW--wspr--Op.32


> 73 de Daniele
> I55387FI

> www.scientific-notes.blogspot.com






-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com



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 <Pine.LNX.4.64.1902071235480.9386@plato.ucs.mun.ca> <Pine.LNX.4.64.1902071306380.9507@plato.ucs.mun.ca>
In-Reply-To: <Pine.LNX.4.64.1902071306380.9507@plato.ucs.mun.ca>
From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Mon, 11 Feb 2019 12:56:17 +0100
Message-ID: <CANA3B6XJkgxPcktLkrYxNK6nVaTWs6Sp7Yux+-bMfohXfOT_oA@mail.gmail.com>
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 Content preview:  Joe, LF Very strong signal last night continuously from 2330z
    to 0530z. Best decode at 0300z, info attached. RX setup: inverted "L" TX
   antenna (slightly detuned, 6 dB attenuator inserted) and SDR. All the best,
 Content analysis details:   (0.3 points, 5.0 required)
  pts rule name              description
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 -0.0 RCVD_IN_DNSWL_NONE     RBL: Sender listed at http://www.dnswl.org/,
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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--000000000000cdcba005819cfd31
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--000000000000cdcb9d05819cfd2f
Content-Type: text/plain; charset="UTF-8"

Joe, LF

Very strong signal last night continuously from 2330z to 0530z.
Best decode at 0300z, info attached.
RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
inserted) and SDR.

All the best,

73 de Riccardo IW4DXW

Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca> ha scritto:

> Apologies: I misspelt Domenico and did not acknowledge Riccardo's
> autodetector.
> 73
> Joe
>
> On Thu, 7 Feb 2019, jcraig@mun.ca wrote:
>
> > Dominico,
> >
> > Thanks to you and Markus and Domenico for the autodecoder service.
> > I will check the modulator and try again tonight. Some antenna work
> > is planned as well when the wx improves so there should be some more
> > dB available soon.
> >
> > 73
> > Joe
> >
> > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
> >
> >> Joe, LF
> >> in my EbNaut log
> >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
> >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
> >> there are some decodes of your EbNaut of last nights (QRB=5426 km).
> Seems
> >> that since yesterday, only carrier is sent on usual qrg 137477 Hz.
> >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
> parameters:
> >>
> >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s
> >> T_OFFSET=0.0s F_OFFSET=0.000Hz
> >>
> >> 73, Domenico IZ7SLZ / JN80nu
> >>
> >
> >
>
>

--000000000000cdcb9d05819cfd2f
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><br><div>Joe, LF</div><div><br></div><div>Very strong sign=
al last night continuously from 2330z to 0530z.</div><div>Best decode at 03=
00z, info attached.</div><div>RX setup: inverted &quot;L&quot; TX antenna (=
slightly detuned, 6 dB attenuator inserted) and SDR.</div><div><br></div><d=
iv><span style=3D"line-height:1.5">All the best,</span><br></div><div><span=
 style=3D"line-height:1.5"><br></span></div><div>73 de Riccardo IW4DXW</div=
></div><br><div class=3D"gmail_quote"><div dir=3D"ltr" class=3D"gmail_attr"=
>Il giorno gio 7 feb 2019 alle ore 17:44 &lt;<a href=3D"mailto:jcraig@mun.c=
a">jcraig@mun.ca</a>&gt; ha scritto:<br></div><blockquote class=3D"gmail_qu=
ote" style=3D"margin:0px 0px 0px 0.8ex;border-left-width:1px;border-left-co=
lor:rgb(204,204,204);border-left-style:solid;padding-left:1ex">Apologies: I=
 misspelt Domenico and did not acknowledge Riccardo&#39;s <br>
autodetector.<br>
73<br>
Joe<br>
<br>
On Thu, 7 Feb 2019, <a href=3D"mailto:jcraig@mun.ca" target=3D"_blank">jcra=
ig@mun.ca</a> wrote:<br>
<br>
&gt; Dominico,<br>
&gt;<br>
&gt; Thanks to you and Markus and Domenico for the autodecoder service.<br>
&gt; I will check the modulator and try again tonight. Some antenna work<br=
>
&gt; is planned as well when the wx improves so there should be some more<b=
r>
&gt; dB available soon.<br>
&gt;<br>
&gt; 73<br>
&gt; Joe<br>
&gt;<br>
&gt; On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:<br>
&gt;<br>
&gt;&gt; Joe, LF<br>
&gt;&gt; in my EbNaut log<br>
&gt;&gt; *<a href=3D"https://qsl.net/iz7slz/EBNAUT/DECODED.TXT" rel=3D"nore=
ferrer" target=3D"_blank">https://qsl.net/iz7slz/EBNAUT/DECODED.TXT</a><br>
&gt;&gt; &lt;<a href=3D"https://qsl.net/iz7slz/EBNAUT/DECODED.TXT" rel=3D"n=
oreferrer" target=3D"_blank">https://qsl.net/iz7slz/EBNAUT/DECODED.TXT</a>&=
gt;*<br>
&gt;&gt; there are some decodes of your EbNaut of last nights (QRB=3D5426 k=
m). Seems<br>
&gt;&gt; that since yesterday, only carrier is sent on usual qrg 137477 Hz.=
<br>
&gt;&gt; Autodecoder here is now running, every XX:00 and XX:30 on Joe&#39;=
s parameters:<br>
&gt;&gt; <br>
&gt;&gt; 137477.000Hz N=3D7 T=3D3s 8K19A CRC=3D16 list=3D2000 sym=3D608 Dur=
ation=3D1824s<br>
&gt;&gt; T_OFFSET=3D0.0s F_OFFSET=3D0.000Hz<br>
&gt;&gt; <br>
&gt;&gt; 73, Domenico IZ7SLZ / JN80nu<br>
&gt;&gt; <br>
&gt;<br>
&gt;<br>
<br>
</blockquote></div>

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 Content preview:  Hello Riccardo, I like the precision of your RX frequency.
    I should add a few nulls to my file too :-) Good work regarding Joe's reception!
    73, Stefan 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Hello Riccardo,

I like the precision of your RX frequency. I should add a few nulls to 
my file too :-)
Good work regarding Joe's reception!

73, Stefan

Am 11.02.2019 12:56, schrieb Riccardo Zoli:
>
> Joe, LF
>
> Very strong signal last night continuously from 2330z to 0530z.
> Best decode at 0300z, info attached.
> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator 
> inserted) and SDR.
>
> All the best,
>
> 73 de Riccardo IW4DXW
>
> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca 
> <mailto:jcraig@mun.ca>> ha scritto:
>
>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
>     autodetector.
>     73
>     Joe
>
>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
>
>     > Dominico,
>     >
>     > Thanks to you and Markus and Domenico for the autodecoder service.
>     > I will check the modulator and try again tonight. Some antenna work
>     > is planned as well when the wx improves so there should be some more
>     > dB available soon.
>     >
>     > 73
>     > Joe
>     >
>     > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>     >
>     >> Joe, LF
>     >> in my EbNaut log
>     >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>     >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>     >> there are some decodes of your EbNaut of last nights (QRB=5426
>     km). Seems
>     >> that since yesterday, only carrier is sent on usual qrg 137477 Hz.
>     >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
>     parameters:
>     >>
>     >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s
>     >> T_OFFSET=0.0s F_OFFSET=0.000Hz
>     >>
>     >> 73, Domenico IZ7SLZ / JN80nu
>     >>
>     >
>     >
>

--------------060408080004090904080403
Content-Type: text/html; charset=UTF-8
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<html>
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</head>
<body bgcolor="#ffffff" text="#000000">
Hello Riccardo, <br>
<br>
I like the precision of your RX frequency. I should add a few nulls to
my file too :-)<br>
Good work regarding Joe's reception! <br>
<br>
73, Stefan<br>
<br>
Am 11.02.2019 12:56, schrieb Riccardo Zoli:
<blockquote
 cite="mid:CANA3B6XJkgxPcktLkrYxNK6nVaTWs6Sp7Yux+-bMfohXfOT_oA@mail.gmail.com"
 type="cite">
  <div dir="ltr"><br>
  <div>Joe, LF</div>
  <div><br>
  </div>
  <div>Very strong signal last night continuously from 2330z to 0530z.</div>
  <div>Best decode at 0300z, info attached.</div>
  <div>RX setup: inverted "L" TX antenna (slightly detuned, 6 dB
attenuator inserted) and SDR.</div>
  <div><br>
  </div>
  <div><span style="line-height: 1.5;">All the best,</span><br>
  </div>
  <div><span style="line-height: 1.5;"><br>
  </span></div>
  <div>73 de Riccardo IW4DXW</div>
  </div>
  <br>
  <div class="gmail_quote">
  <div dir="ltr" class="gmail_attr">Il giorno gio 7 feb 2019 alle ore
17:44 &lt;<a moz-do-not-send="true" href="mailto:jcraig@mun.ca">jcraig@mun.ca</a>&gt;
ha scritto:<br>
  </div>
  <blockquote class="gmail_quote"
 style="border-left: 1px solid rgb(204, 204, 204); margin: 0px 0px 0px 0.8ex; padding-left: 1ex;">Apologies:
I misspelt Domenico and did not acknowledge Riccardo's <br>
autodetector.<br>
73<br>
Joe<br>
    <br>
On Thu, 7 Feb 2019, <a moz-do-not-send="true"
 href="mailto:jcraig@mun.ca" target="_blank">jcraig@mun.ca</a> wrote:<br>
    <br>
&gt; Dominico,<br>
&gt;<br>
&gt; Thanks to you and Markus and Domenico for the autodecoder service.<br>
&gt; I will check the modulator and try again tonight. Some antenna work<br>
&gt; is planned as well when the wx improves so there should be some
more<br>
&gt; dB available soon.<br>
&gt;<br>
&gt; 73<br>
&gt; Joe<br>
&gt;<br>
&gt; On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:<br>
&gt;<br>
&gt;&gt; Joe, LF<br>
&gt;&gt; in my EbNaut log<br>
&gt;&gt; *<a moz-do-not-send="true"
 href="https://qsl.net/iz7slz/EBNAUT/DECODED.TXT" rel="noreferrer"
 target="_blank">https://qsl.net/iz7slz/EBNAUT/DECODED.TXT</a><br>
&gt;&gt; &lt;<a moz-do-not-send="true"
 href="https://qsl.net/iz7slz/EBNAUT/DECODED.TXT" rel="noreferrer"
 target="_blank">https://qsl.net/iz7slz/EBNAUT/DECODED.TXT</a>&gt;*<br>
&gt;&gt; there are some decodes of your EbNaut of last nights (QRB=5426
km). Seems<br>
&gt;&gt; that since yesterday, only carrier is sent on usual qrg 137477
Hz.<br>
&gt;&gt; Autodecoder here is now running, every XX:00 and XX:30 on
Joe's parameters:<br>
&gt;&gt; <br>
&gt;&gt; 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
Duration=1824s<br>
&gt;&gt; T_OFFSET=0.0s F_OFFSET=0.000Hz<br>
&gt;&gt; <br>
&gt;&gt; 73, Domenico IZ7SLZ / JN80nu<br>
&gt;&gt; <br>
&gt;<br>
&gt;<br>
    <br>
  </blockquote>
  </div>
</blockquote>
</body>
</html>

--------------060408080004090904080403--

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 Content preview:  Hi Dimitris, VLF, Am 11.02.2019 01:07, schrieb Dimitrios Tsifakis:
    > I have an idea about impedance transformation and that is to use high >
    power 70V/100V audio distribution transformers at both ends. I don't > have
    t [...] 
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Subject: Re: R: Re: VLF: in VK?
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Hi Dimitris, VLF,

Am 11.02.2019 01:07, schrieb Dimitrios Tsifakis:
> I have an idea about impedance transformation and that is to use high
> power 70V/100V audio distribution transformers at both ends. I don't
> have to go to 50 ohm as I don't use the coaxial cable as a
> transmission line (it's only a tiny percentage of the wavelength!), so
> I could use a 4 ohm to 400 ohm transformer or similar. I think in
> general the impedance transformation ratio goes down as the power
> rating goes up and we can live with that. THe audio transformer should
> work fine on the higher frequency but that will have to be tested.
> Perhaps something like this but not at that price!!
>
> https://www.altronics.com.au/p/m1160-300w-100v-line-pa-transformer/
>
> Another option is to get a PA amplifier of suitable power output that
> has a 70V or 100V output. You only need one transformer at the antenna
> end to get down to 4 ohm to reduce losses. I have a 50 W amp with such
> output but that's not enough power.
>    
These high power audio transformers are interesting. I wonder how well 
they work below 1 kHz. But they are to expensive, as you say. You don't 
need them. For any impedance transformation above 1 kHz i use ordinary 
N30 ferrite toroids. There may be slightly better core materials but i'm 
getting very good results and they are not expensive and you can find 
them at many distributors (min quantity = 1, not 
50000000000000000000000000). Especially at VLF they are well suitable 
and not expensive.
One of my preferred cores is that one: 
https://www.buerklin.com/en/ring-core-outer--x-inner--x-height--63-x-38-x-25-mm-n30/p/84d258
It works easily for a few hundret watts on all VLF frequencies.

Yes you don't need to match the cable impedance but the losses on your 
cable are caused by the current and resistance of the wire and so, if 
you transform from 4 Ohm to 50 Ohm, then your losses drop by 92 %, 
regardless if it is necessary to match the cable impedance.

> I can easily try the ground loop on the 120m long antenna as I do have
> ground rods at both ends. It would be interesting to compare the
> signal strength in both cases. THat's why I am building a network of
> VLF stations by giving away the large ferrite rods to interested
> amateurs! They can help doing comparisons like this.
>    
Yes, sure. Good luck in getting people motivated to build up a permanent 
VLF RX station. It would also be good to have someone building up a 
grabber site or maybe even providing a stream. Your activity can cause a 
world wide motivation for people who are principally interested in VLF 
reception and/or transmission, even if they won't be able to receive you 
from so far away.

> The ground is very rocky and there is almost no soil at the top.
> Typical Australian native vegetation is the only thing that can
> survive on it. I have thought about the dipole on the ground and I
> have the perfect spot for it which is putting the feed point at the
> top of the hill therefore making an inverted-V :-) Only concern with
> that is the high voltage at the end of the dipole wires and the
> possibility of a bush fire ignition. Definitely a project for winter!
> I have tried to tune my ~120 metre wire to VLF in the past with mixed
> results. Worth revisiting this. The wire basically starts at my house
> and follows the hill resulting in the top of the wire being maybe 20
> metres higher than the bottom.
>    
I'm taking part in your experiments by imagining that i would be in your 
position :-)
My latest thought is that a few (wooden?) poles of 10m height or so 
would be ideal. One is close to the house, and then two more in 100m 
distance from the house, e.g. here: 
http://k7fry.com/grid/?qth=QF44OX00PV&from=QF44OX00LN
The 2x 100m dipole could be connected using a good HF ladder line down 
to the shack.
Aluminium wire is light weight and cheap and the lower conductivity 
could be compensated by using a higher diameter, something like this, 
https://www.amazon.de/dp/B004UA7XT2
This antenna would have the advantage that you can use it from MF to DC 
and the kangaroos would not be able to destroy the antenna.
For VLF experiments, the ends of the wire can be grounded, just by 
adding another 100m of wire at the ends and let them slope down, maybe 
with another pole at 4m height.


73, Stefan

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Subject: RE: R: Re: VLF: in VK?
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 Content preview:  Hello Stefan! Today, the ferrite cores B64290L82X830 came
   to me. I'm building a transformer 1:1/1:4/1:9/1:16 and 1/25 on the VLF. I'll
    check if it works soon. 73! Marcin SQ2BXI 
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Hello Stefan!

Today, the ferrite cores B64290L82X830 came to me. I'm building a transformer 1:1/1:4/1:9/1:16 and 1/25 on the VLF. I'll check if it works soon.
73! Marcin SQ2BXI

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> On Behalf Of DK7FC
Sent: Monday, February 11, 2019 2:50 PM
To: rsgb_lf_group@blacksheep.org
Subject: Re: R: Re: VLF: in VK?

Hi Dimitris, VLF,

Am 11.02.2019 01:07, schrieb Dimitrios Tsifakis:
> I have an idea about impedance transformation and that is to use high 
> power 70V/100V audio distribution transformers at both ends. I don't 
> have to go to 50 ohm as I don't use the coaxial cable as a 
> transmission line (it's only a tiny percentage of the wavelength!), so 
> I could use a 4 ohm to 400 ohm transformer or similar. I think in 
> general the impedance transformation ratio goes down as the power 
> rating goes up and we can live with that. THe audio transformer should 
> work fine on the higher frequency but that will have to be tested.
> Perhaps something like this but not at that price!!
>
> https://www.altronics.com.au/p/m1160-300w-100v-line-pa-transformer/
>
> Another option is to get a PA amplifier of suitable power output that 
> has a 70V or 100V output. You only need one transformer at the antenna 
> end to get down to 4 ohm to reduce losses. I have a 50 W amp with such 
> output but that's not enough power.
>    
These high power audio transformers are interesting. I wonder how well they work below 1 kHz. But they are to expensive, as you say. You don't need them. For any impedance transformation above 1 kHz i use ordinary
N30 ferrite toroids. There may be slightly better core materials but i'm getting very good results and they are not expensive and you can find them at many distributors (min quantity = 1, not 50000000000000000000000000). Especially at VLF they are well suitable and not expensive.
One of my preferred cores is that one: 
https://www.buerklin.com/en/ring-core-outer--x-inner--x-height--63-x-38-x-25-mm-n30/p/84d258
It works easily for a few hundret watts on all VLF frequencies.

Yes you don't need to match the cable impedance but the losses on your cable are caused by the current and resistance of the wire and so, if you transform from 4 Ohm to 50 Ohm, then your losses drop by 92 %, regardless if it is necessary to match the cable impedance.

> I can easily try the ground loop on the 120m long antenna as I do have 
> ground rods at both ends. It would be interesting to compare the 
> signal strength in both cases. THat's why I am building a network of 
> VLF stations by giving away the large ferrite rods to interested 
> amateurs! They can help doing comparisons like this.
>    
Yes, sure. Good luck in getting people motivated to build up a permanent VLF RX station. It would also be good to have someone building up a grabber site or maybe even providing a stream. Your activity can cause a world wide motivation for people who are principally interested in VLF reception and/or transmission, even if they won't be able to receive you from so far away.

> The ground is very rocky and there is almost no soil at the top.
> Typical Australian native vegetation is the only thing that can 
> survive on it. I have thought about the dipole on the ground and I 
> have the perfect spot for it which is putting the feed point at the 
> top of the hill therefore making an inverted-V :-) Only concern with 
> that is the high voltage at the end of the dipole wires and the 
> possibility of a bush fire ignition. Definitely a project for winter!
> I have tried to tune my ~120 metre wire to VLF in the past with mixed 
> results. Worth revisiting this. The wire basically starts at my house 
> and follows the hill resulting in the top of the wire being maybe 20 
> metres higher than the bottom.
>    
I'm taking part in your experiments by imagining that i would be in your position :-) My latest thought is that a few (wooden?) poles of 10m height or so would be ideal. One is close to the house, and then two more in 100m distance from the house, e.g. here: 
http://k7fry.com/grid/?qth=QF44OX00PV&from=QF44OX00LN
The 2x 100m dipole could be connected using a good HF ladder line down to the shack.
Aluminium wire is light weight and cheap and the lower conductivity could be compensated by using a higher diameter, something like this,
https://www.amazon.de/dp/B004UA7XT2
This antenna would have the advantage that you can use it from MF to DC and the kangaroos would not be able to destroy the antenna.
For VLF experiments, the ends of the wire can be grounded, just by adding another 100m of wire at the ends and let them slope down, maybe with another pole at 4m height.


73, Stefan



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From: jcraig@mun.ca
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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 Content preview:  Hi Riccardo, Stefan, LF, Pleased to get your report of improved
    signal strength Riccardo. The R means "Rotated L" so it is in the sky again
    since yesterday. Today a cermaic feedthrough was installed on the PVC bucket
    that hou [...] 
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Hi Riccardo, Stefan, LF,

Pleased to get your report of improved signal strength Riccardo.
The R means "Rotated L" so it is in the sky again since yesterday.
Today a cermaic feedthrough was installed on the PVC bucket
that houses the coil. It was cold (-10 C) today but the work had
to be done; there was too much charring and arcing.  All seems OK
now and the TX is on (one Decca module) 2.2A RF

73
Joe VO1NA

On Mon, 11 Feb 2019, DK7FC wrote:

> Hello Riccardo,
>
> I like the precision of your RX frequency. I should add a few nulls to my 
> file too :-)
> Good work regarding Joe's reception!
>
> 73, Stefan
>
> Am 11.02.2019 12:56, schrieb Riccardo Zoli:
>> 
>> Joe, LF
>> 
>> Very strong signal last night continuously from 2330z to 0530z.
>> Best decode at 0300z, info attached.
>> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator 
>> inserted) and SDR.
>> 
>> All the best,
>> 
>> 73 de Riccardo IW4DXW
>> 
>> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca 
>> <mailto:jcraig@mun.ca>> ha scritto:
>>
>>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
>>     autodetector.
>>     73
>>     Joe
>>
>>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
>>
>>     > Dominico,
>>     >
>>     > Thanks to you and Markus and Domenico for the autodecoder service.
>>     > I will check the modulator and try again tonight. Some antenna work
>>     > is planned as well when the wx improves so there should be some more
>>     > dB available soon.
>>     >
>>     > 73
>>     > Joe
>>     >
>>     > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>>     >
>>     >> Joe, LF
>>     >> in my EbNaut log
>>     >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>>     >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>>     >> there are some decodes of your EbNaut of last nights (QRB=5426
>>     km). Seems
>>     >> that since yesterday, only carrier is sent on usual qrg 137477 Hz.
>>     >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
>>     parameters:
>>     >>
>>     >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s
>>     >> T_OFFSET=0.0s F_OFFSET=0.000Hz
>>     >>
>>     >> 73, Domenico IZ7SLZ / JN80nu
>>     >>
>>     >
>>     >
>> 
>

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Tue, 12 Feb 2019 08:44:50 +1100
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Subject: Re: R: Re: VLF: in VK?
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 Content preview:  Hi Stefan, > These high power audio transformers are interesting.
    I wonder how well > they work below 1 kHz. But they are to expensive, as
   you say. You don't > need them. For any impedance transformation above 1 [...]
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Hi Stefan,


> These high power audio transformers are interesting. I wonder how well
> they work below 1 kHz. But they are to expensive, as you say. You don't
> need them. For any impedance transformation above 1 kHz i use ordinary
> N30 ferrite toroids. There may be slightly better core materials but i'm
> getting very good results and they are not expensive and you can find
> them at many distributors (min quantity = 1, not
> 50000000000000000000000000). Especially at VLF they are well suitable
> and not expensive.
> One of my preferred cores is that one:
> https://www.buerklin.com/en/ring-core-outer--x-inner--x-height--63-x-38-x-25-mm-n30/p/84d258
> It works easily for a few hundret watts on all VLF frequencies.

I do have some ferrites that may be suitable for impedance
transformation at audio over a kHz, perhaps I should stop being lazy
and I should wind a transformer for testing. I keep forgetting that
audio transformers are large because they have to transform 3 orders
of magnitude in frequency - 20 Hz to 20 kHz. At this stage, I am only
interested in the top order of magnitude (2 kHz to 20 kHz) which
implies I can aim for a proportionally less winding inductance and
still have good results. The cores I have are N27 meterial E shape and
when you put to E's together you get a square of about 45 mm by 45 m.
N30 has better initial permeability by about a factor of two but has
worse losses (u" is higher). So I would probably require a few more
turns but I am generally on a higher frequency than you therefore it's
not a big deal :-)

> Yes you don't need to match the cable impedance but the losses on your
> cable are caused by the current and resistance of the wire and so, if
> you transform from 4 Ohm to 50 Ohm, then your losses drop by 92 %,
> regardless if it is necessary to match the cable impedance.

There is another solution to this problem which is more win-win :-) I
have another roll of 3-core cable I can put in parallel to the first
one, then my losses will go up by a factor of two but factoring that
in the calculations, so does the radiated power (for the same TX
power). Then my impedance is higher and as a percentage, the
transmission line loss has less effect. Only problem with this is that
it was a pain to get the wire up and I suspect it will be a 2^2 times
pain to put the second one in parallel :-)

> I'm taking part in your experiments by imagining that i would be in your
> position :-)

Your role as the motivator is quite important in getting anything done!

> My latest thought is that a few (wooden?) poles of 10m height or so
> would be ideal. One is close to the house, and then two more in 100m
> distance from the house, e.g. here:
> http://k7fry.com/grid/?qth=QF44OX00PV&from=QF44OX00LN
> The 2x 100m dipole could be connected using a good HF ladder line down
> to the shack.

The only difficulty with this is the 10 m wooden poles. It's not
something trivial to transport home and install. But I am always on
the lookout for supporting material! A few years ago, I went to a
large country fair and I was negotiating with a company that makes and
installs woden poles for mains power. They would be happy to come and
install a few around my place but the prices were absolutely
unrealistic for me. I also have to respect the wishes of my wife who
is a conservation ecologist and doesn't necessarily like huge
machinery drilling holes and making a mess in pristine native
Australian landscape :-) Wires on trees are fine though and I do have
a few eucalypts that potentially can be used for this.

> Aluminium wire is light weight and cheap and the lower conductivity
> could be compensated by using a higher diameter, something like this,
> https://www.amazon.de/dp/B004UA7XT2

Wow, I have never seen aluminium wire used for fencing, this must be a
really posh version. Also I am surprised to see fencing wire stating
its resistance (0.01 ohm/m) :-) How nice of them! Maybe it's for
electric fence but the resistance wouldn't be all that important in
that case I guess. May even be desirable for the poor animals :-)

> This antenna would have the advantage that you can use it from MF to DC
> and the kangaroos would not be able to destroy the antenna.
> For VLF experiments, the ends of the wire can be grounded, just by
> adding another 100m of wire at the ends and let them slope down, maybe
> with another pole at 4m height.

Fair enough! I think you have convinced me to try the grounded ends
experiment and I will start small with my 120 m loop. I'd be
interested to measure the impedance of that, my suspicion is that it
could be hundreds of ohms given the very rocky ground. I then have to
make appropriate impedance transformers. What sort of impedance range
have you observed with your ground antenna experiments on VLF? Also,
was the reactance part of the impedance positive (inductive) or
negative (capacitive)? I generally use my oscilloscope and signal
generator to measure these parameters using a home made bridge and my
capacitor box. This gets a bit tricky on the field. How do you do it?
Maybe we should start writing a 'techniques' manual for the beginner
VLF enthusiast? Perhaps I can start writing things down in my page and
you can contribute your trade secrets? ;-)

73, Dimitris

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To: <rsgb_lf_group@blacksheep.org>
References: <168d6970d7b.marcocadeddu@tin.it> <5C5FF6F8.7000007@posteo.de> <CAKvcm2dCPvyHjTEJ7=HuqHr1Pgi4Rd8iZBM4Tf=+hxjZ18BkDg@mail.gmail.com> <5C617D7A.8040105@posteo.de> <CAKvcm2cg9DQYPDwPjfZihcb30ZgaOh9jpwveYtqyejDGREf++g@mail.gmail.com>
In-Reply-To: <CAKvcm2cg9DQYPDwPjfZihcb30ZgaOh9jpwveYtqyejDGREf++g@mail.gmail.com>
Subject: LF: Re: in VK?
Date: Mon, 11 Feb 2019 16:14:37 -0800
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 Content preview:  >Maybe we should start writing a 'techniques' manual for the
    beginner VLF enthusiast? Yes ! WEB - "The VE7SL Radio Notebook": http://qsl.net/ve7sl/
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>Maybe we should start writing a 'techniques' manual for the beginner
VLF enthusiast?

Yes !



WEB - "The VE7SL Radio Notebook": http://qsl.net/ve7sl/

VE7SL BLOG - "Homebrewing and Operating Adventures From 2200m to Nanowaves": 
http://ve7sl.blogspot.ca/ 


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Message-ID: <5C62EBAD.9050904@posteo.de>
Date: Tue, 12 Feb 2019 16:52:13 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hi ELF, Yesterday, a 12 character EbNaut message was transferred
    over the 3.5 km (0.00027 wavelengths) path at 22.97 Hz. Higher noise levels
    caused some unsuccessful attempts but last night was quite good and [...]
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Subject: ELF: First EbNaut message transfer at ELF
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Hi ELF,

Yesterday, a 12 character EbNaut message was transferred over the 3.5 km 
(0.00027 wavelengths) path at 22.97 Hz.
Higher noise levels caused some unsuccessful attempts but last night was 
quite good and i increased the symbol length to 30 seconds. The message 
took 14:24 (hh:mm) to pass over to the tree.
Capture of the signal post-processing chain and message decode attached.

73, Stefan



Am 07.02.2019 17:05, schrieb DK7FC:
> Hi ELF ;-)
>
> I'm glad to announce that since 15:46 UTC i am transmitting on ELF 
> (the real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 
> <https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first 
> time ever.
>
> Here are the parameters:
>
> TX frequency: *22.970 Hz*
> Wavelength of that frequency: *13060 km*
> Antenna voltage: *4.8 kV rms* (+ a DC component of 7.5 kV)
> Antenna current: *325 uA*
> ERP: 600 aW, or *6E-16 W*
>
> Call it QRP!
> The goal is to detect the signal on my 3.5 km distant tree grabber, 
> whose E field is now working again. Since the E field probe is not to 
> far above the tree, the effective height is not as much as it should 
> ideally be, at this frequency, so the RX is somewhat deaf. Anyway i 
> can see the Schumann resonances and the 60 Hz power grid. So i hope it 
> will work.
>
> A spectrogram which is centered on the frequency of interest in now 
> shown at 
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html 
> (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! 
> In a few minutes we'll see more :-) It takes about 40 minutes until a 
> peak could have fully developed...
>
> 73, Stefan
>

--------------060909030801040602030504
Content-Type: text/html; charset=ISO-8859-15
Content-Transfer-Encoding: 7bit

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  <meta content="text/html; charset=ISO-8859-15"
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<body bgcolor="#ffffff" text="#000000">
Hi ELF, <br>
<br>
Yesterday, a 12 character EbNaut message was transferred over the 3.5
km (0.00027 wavelengths) path at 22.97 Hz.<br>
Higher noise levels caused some unsuccessful attempts but last night
was quite good and i increased the symbol length to 30 seconds. The
message took 14:24 (hh:mm) to pass over to the tree.<br>
Capture of the signal post-processing chain and message decode attached.<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 07.02.2019 17:05, schrieb DK7FC:
<blockquote cite="mid:5C5C5757.5080906@posteo.de" type="cite">
  <meta http-equiv="content-type"
 content="text/html; charset=ISO-8859-15">
Hi ELF ;-)<br>
  <br>
I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a moz-do-not-send="true"
 href="https://en.wikipedia.org/wiki/Radio_spectrum#ITU">ITU radio band
1</a> ) for the first time ever.<br>
  <br>
Here are the parameters: <br>
  <br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
  <br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
  <br>
A spectrogram which is centered on the frequency of interest in now
shown at
  <a moz-do-not-send="true" class="moz-txt-link-freetext"
 href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
  <br>
73, Stefan<br>
  <br>
</blockquote>
</body>
</html>

--------------060909030801040602030504--

--------------060602010102050409010501
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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Tue, 12 Feb 2019 16:42:14 +0000
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 Content preview:  What programme are you referring to ? Andy www.g4jnt.com On
    Tue, 12 Feb 2019 at 13:55, Chris Wilson wrote: 
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Subject: LF: Re: Simple Timer question
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What programme are you referring to ?

Andy
www.g4jnt.com



On Tue, 12 Feb 2019 at 13:55, Chris Wilson <dead.fets@gmail.com> wrote:

>
>
> Hello  Andy,
>
>   I  have  had  great  service from your Simple Timer programme, thank
>   you!  I  am  wondering how hard it would be to add a simple ON / OFF
>   command to it so I can turn my PSU on and off without entering times
>   for both? Thanks!  2E0ILY
>
> --
> Best regards,
>  Chris                          mailto:dead.fets@gmail.com
>
>

--000000000000b7a6050581b51e84
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">What programme are you referring to ?</div><div =
class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:sm=
all"><br></div><div><div dir=3D"ltr" class=3D"gmail_signature" data-smartma=
il=3D"gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=
=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=
=3D"font-size:12.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank">ww=
w.g4jnt.com</a></span><br></div><div><br></div></div></div></div></div></di=
v></div></div></div></div></div></div><br></div><br><div class=3D"gmail_quo=
te"><div dir=3D"ltr" class=3D"gmail_attr">On Tue, 12 Feb 2019 at 13:55, Chr=
is Wilson &lt;<a href=3D"mailto:dead.fets@gmail.com">dead.fets@gmail.com</a=
>&gt; wrote:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:0px=
 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><br=
>
<br>
Hello=C2=A0 Andy,<br>
<br>
=C2=A0 I=C2=A0 have=C2=A0 had=C2=A0 great=C2=A0 service from your Simple Ti=
mer programme, thank<br>
=C2=A0 you!=C2=A0 I=C2=A0 am=C2=A0 wondering how hard it would be to add a =
simple ON / OFF<br>
=C2=A0 command to it so I can turn my PSU on and off without entering times=
<br>
=C2=A0 for both? Thanks!=C2=A0 2E0ILY<br>
<br>
-- <br>
Best regards,<br>
=C2=A0Chris=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 mailto:<a href=3D"mailto:dead.fets@gmail.com" t=
arget=3D"_blank">dead.fets@gmail.com</a><br>
<br>
</blockquote></div>

--000000000000b7a6050581b51e84--

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 Content preview:  Hi Dimitris, Am 11.02.2019 22:44, schrieb Dimitrios Tsifakis:
    > [...] and I should wind a transformer for testing. Yes. First you only
   need the primary winding to see if it stays cool at the full volume level.
    You [...] 
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Hi Dimitris,

Am 11.02.2019 22:44, schrieb Dimitrios Tsifakis:
> [...] and I should wind a transformer for testing.
Yes. First you only need the primary winding to see if it stays cool at 
the full volume level. You know, saturation and so on. Only use as many 
turns as necessary for the frequency, that is ideal. But probably you 
know all that.
If you know the co
re material and the cross section area the the B max, then you can do a 
rough calculation as well...
Here it's a bit like sitting a pub, exchanging some ideas about VLF.

> The cores I have are N27 meterial E shape and
> when you put to E's together you get a square of about 45 mm by 45 m.
> N30 has better initial permeability by about a factor of two but has
> worse losses (u" is higher). So I would probably require a few more
> turns but I am generally on a higher frequency than you therefore it's
> not a big deal :-)
>    
It will work very good.

> I have another roll of 3-core cable I can put in parallel to the first
> one, then my losses will go up by a factor of two
Go up? I think you mean go down, or switch in series. Ah, yes, put in 
parallel but switch in series. Yes, then, twice the R, 4 times the L and 
so 1/4 of the Cs and only 70% of the current, at the same power level.
So you can switch the Cs in serial to get on resonance again. But this 
will be even a higher stress for them because the current is 40 % higher 
for each one then. So you need more of them and choose another 
configuration.

>   but factoring that
> in the calculations, so does the radiated power (for the same TX
> power). Then my impedance is higher and as a percentage, the
> transmission line loss has less effect. Only problem with this is that
> it was a pain to get the wire up and I suspect it will be a 2^2 times
> pain to put the second one in parallel :-)
>    
Yes. And just you are not the one with limited space, so it is better to 
use the wire in another arrangement...

> Your role as the motivator is quite important in getting anything done!
>    
Oh thanks.

> The only difficulty with this is the 10 m wooden poles. It's not
> something trivial to transport home and install. But I am always on
> the lookout for supporting material! A few years ago, I went to a
> large country fair and I was negotiating with a company that makes and
> installs woden poles for mains power. They would be happy to come and
> install a few around my place but the prices were absolutely
> unrealistic for me. I also have to respect the wishes of my wife who
> is a conservation ecologist and doesn't necessarily like huge
> machinery drilling holes and making a mess in pristine native
> Australian landscape :-) Wires on trees are fine though and I do have
> a few eucalypts that potentially can be used for this.
>    
How high are such trees? Can you climb them? Are there Koalas sitting on 
them? And are they dangerous? I've heared they are sleeping and eating 
all the time.

> Fair enough! I think you have convinced me to try the grounded ends
> experiment and I will start small with my 120 m loop. I'd be
> interested to measure the impedance of that, my suspicion is that it
> could be hundreds of ohms given the very rocky ground.
It all depends on the ground resistance you can get when using your 
ground rods or whatever at the end. The dry ground is ideal for getting 
a good radiation resistance but on the other sde you need a high antenna 
current and so you need a low loop resitance. It is a proadoxon.
I already asked about those small ponds arround the dry landscape. What 
is it? For what are they used?
It is no effort to walk arround and lay some cable on the ground and try 
see how much antenna current you will get, and then calculate the 
losses, or the serial resiatance. Make a DC measurement, that is very 
informative and quickly done. Then you have an impression how you have 
to wind the transformer. Use a higher DC voltage than 12 V, maybe 100V 
DC is a good idea, if you have a suitable power supply.
You will need to contact these small ponds to get the loop resistance 
down. They are ideal for the job, really ideal.
We also have to consider other conductive metallic structures below the 
ground. If there is a metally water pipe below the ground, it may bypass 
you antenna current, ie.e. it lowers the loop area! Also the electrical 
grounding of your house may be an issue. If you lay a 2000m wire close 
to the house of a neighbour, and your and his mains ground is conbnected 
together, then the efficiency will be poor.
Assuming a 1000 m distance between the wire ends, and using those small 
ponds (put a plate of 1m x 1m in there, for example and as a test at 
least), and assuming there is no bypass, i estimate you can come down to 
say 200 Ohm? At least it will be an interesting information and a next step.

> What sort of impedance range
> have you observed with your ground antenna experiments on VLF?
I am using guide rails near a street to ground my antenna. This is very 
comfortable and the resulting earth resistance is extremely low, lower 
than i ever expected! My cable has about 30 Ohm DC resistance, about 1 
km long. Before doing an experiment i usually measure the DC resistance 
by applying 1 A DC. I have a adjustable DC/DC converter that is gives 
0...150 V, homemade stuff. There is no electricity so i am transmitting 
from batteries. I bought a 120 Ah LiFePO4 battery that provides > 500 W 
for more than 2.5 hours, key down! In one of the last experiments i 
measured 64V at 1A, so i have 64 Ohm. And that means that both of the 
ground electrodes + the R of the ground is 34 Ohm. So one of the ground 
electrodes must have less than 17 Ohm! Unbelivable, isn't it?! At 500 W 
RF power i recently got nearly 3 A antenna current. I did a night 
transmission attempting to leave a trace near Moscow. There was no trace 
of my signal which confirmed that the antenna actually seems to radiate 
like a loop, at least in 2000 km distance this was clear. So it was not 
a negative result, it was information and confirmation of the theory (i 
don't care to much about theory, you know). BUT, Paul Nicholson detected 
the carrier and prooved that it was so strong that a 1350 character 
message could have been transferred in those 2 hours!
You know what that means? It means that we could do a QRP experiment: 
With just 5W TX power from one of my old 7 Ah lead acid gel batteries we 
could exchange a message, like callsign + locator or some funny stuff 
like 'I have a cat' (history). One day we have to try that, if he likes 
;-) And our distance is just as high as the distance between you and 
Edgar. OK, Paul will have a better RX system, but you have a mains 
connection and so you are not limited by time.
>   Also,
> was the reactance part of the impedance positive (inductive) or
> negative (capacitive)?
Inductive. So you need a series C to tune the antenna. I built a C 
network using WIMA FKP-1 capacitors and WIMA MKP-10 capacitors, each one 
in series with a switch. The smallest has 22 nF, the largest has 10 uF. 
With this network i can tune to frequencies lower than 1 kHz. At 8.27 
kHz the spectrum already looks quite good with that series C only. 
There, i need 169 nF (100+47+22) for the resonance. So the L seems to be 
about 2.2 mH.

>   I generally use my oscilloscope and signal
> generator to measure these parameters using a home made bridge and my
> capacitor box. This gets a bit tricky on the field. How do you do it?
>    
I have a very good scope that's also able to show a spectrum. I modified 
it that it can run on a 12 V battery and i take it to the feed point in 
my car each time. There there signal strengh of the fundamental 
frequency is maximised during the tuning process, using the FFT and auto 
measure function.
> Maybe we should start writing a 'techniques' manual for the beginner
> VLF enthusiast? Perhaps I can start writing things down in my page and
> you can contribute your trade secrets? ;-)
>    
That would be a very good idea and it is good to start at the beginning, 
your beginning.  It is also a bit like a diary, you can always look back 
what you've done a year ago.
Maybe, who knows, a few OM are following the discussion and will join 
the experiments, not only but hopefully in Australia.


73, Stefan


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Date: Tue, 12 Feb 2019 22:09:13 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello Andy, This one but it appears the directory has been
    removed subsequent to me downloading it a few months ago. Thanks. Try this
    http://www.g4jnt.com/DropF/simpletimer.zip 
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Hello Andy,

This  one  but it appears the directory has been removed subsequent to
me downloading it a few months ago. Thanks.

Try this
http://www.g4jnt.com/DropF/simpletimer.zip

It lets you abort the on time using the [esc] key

Source code is in there as well 

All in PowerBasic, command line compiler version
(By far the nicest way to programme simple things that don't need whizzy windows interfaces)

Andy



Tuesday, February 12, 2019, 4:42:14 PM, you wrote:

> What programme are you referring to ?




> Andy
> www.g4jnt.com




> On Tue, 12 Feb 2019 at 13:55, Chris Wilson <dead.fets@gmail.com> wrote:


>  
>  Hello  Andy,
>  
>    I  have  had  great  service from your Simple Timer programme, thank
>    you!  I  am  wondering how hard it would be to add a simple ON / OFF
>    command to it so I can turn my PSU on and off without entering times
>    for both? Thanks!  2E0ILY
>  
>  -- 
>  Best regards,
>   Chris                          mailto:dead.fets@gmail.com
>  
>  



-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com



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From: Andy Talbot <andy.g4jnt@gmail.com>
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 Content preview:  Oh yes, I vaguely remember writing it - in a slack few minutes
    one evening after someone (You ?) requested it. Found the original source
    code now What are you saying you actually want it to do? It's a simple text
    driven prog so difficult to write interactions and things. AN all singing
    all dancing prog with options and manual control would be better in a windows
    format. Are you saying you ju [...] 
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Subject: Re: LF: Re: Simple Timer question
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--0000000000006e6feb0581b9e83b
Content-Type: text/plain; charset="UTF-8"

Oh yes, I vaguely remember writing it  - in a slack few minutes one evening
after someone (You ?) requested it.  Found the original source code now
What are you saying you actually want it to do?

It's a simple text driven prog so difficult to write interactions and
things.   AN all singing all dancing prog with options and manual control
would be better in a windows format.  Are you saying you just want a simple
on / off control via that same COM port interface?   It seems  a rather
complicated way to go about things.  Wouldn't a toggle switch overriding
the COM port control be a simpler solution?

I clean out that DropF folder regulalrly - it is only for temporary file
transfers.   Permanent stuff goes elsewhere with fixed links

Andy
www.g4jnt.com



On Tue, 12 Feb 2019 at 22:18, Chris Wilson <dead.fets@gmail.com> wrote:

>
>
> Hello Andy,
>
> This  one  but it appears the directory has been removed subsequent to
> me downloading it a few months ago. Thanks.
>
> Try this
> http://www.g4jnt.com/DropF/simpletimer.zip
>
> It lets you abort the on time using the [esc] key
>
> Source code is in there as well
>
> All in PowerBasic, command line compiler version
> (By far the nicest way to programme simple things that don't need whizzy
> windows interfaces)
>
> Andy
>
>
>
> Tuesday, February 12, 2019, 4:42:14 PM, you wrote:
>
> > What programme are you referring to ?
>
>
>
>
> > Andy
> > www.g4jnt.com
>
>
>
>
> > On Tue, 12 Feb 2019 at 13:55, Chris Wilson <dead.fets@gmail.com> wrote:
>
>
> >
> >  Hello  Andy,
> >
> >    I  have  had  great  service from your Simple Timer programme, thank
> >    you!  I  am  wondering how hard it would be to add a simple ON / OFF
> >    command to it so I can turn my PSU on and off without entering times
> >    for both? Thanks!  2E0ILY
> >
> >  --
> >  Best regards,
> >   Chris                          mailto:dead.fets@gmail.com
> >
> >
>
>
>
> --
> Best regards,
>  Chris                            mailto:dead.fets@gmail.com
>
>
>

--0000000000006e6feb0581b9e83b
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div class=3D"gmail_default" style=3D"fon=
t-family:tahoma,sans-serif;font-size:small">Oh yes, I vaguely remember writ=
ing it=C2=A0 - in a slack few minutes one evening after someone (You ?) req=
uested it.=C2=A0 Found the original source code now</div><div class=3D"gmai=
l_default" style=3D"font-family:tahoma,sans-serif;font-size:small">What are=
 you saying you actually want it to do?</div><div class=3D"gmail_default" s=
tyle=3D"font-family:tahoma,sans-serif;font-size:small"><br></div><div class=
=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small">=
It&#39;s a simple text driven prog so difficult to write interactions and t=
hings.=C2=A0 =C2=A0AN all singing all dancing prog with options and manual =
control would be better in a windows format.=C2=A0 Are you saying you just =
want a simple on / off control via that same COM port interface?=C2=A0 =C2=
=A0It seems=C2=A0 a rather complicated way to go about things.=C2=A0 Wouldn=
&#39;t a toggle switch overriding the COM port control be a simpler solutio=
n?</div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small"><br></div><div class=3D"gmail_default" style=3D"font-fami=
ly:tahoma,sans-serif;font-size:small">I clean out that DropF folder regulal=
rly - it is only for temporary file transfers.=C2=A0 =C2=A0Permanent stuff =
goes elsewhere with fixed links</div><div class=3D"gmail_default" style=3D"=
font-family:tahoma,sans-serif;font-size:small"><br></div><div><div dir=3D"l=
tr" class=3D"gmail_signature" data-smartmail=3D"gmail_signature"><div dir=
=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr">=
<div><div dir=3D"ltr">Andy<div><span style=3D"font-size:12.8px"><a href=3D"=
http://www.g4jnt.com" target=3D"_blank">www.g4jnt.com</a></span><br></div><=
div><br></div></div></div></div></div></div></div></div></div></div></div><=
/div><br></div><br><div class=3D"gmail_quote"><div dir=3D"ltr" class=3D"gma=
il_attr">On Tue, 12 Feb 2019 at 22:18, Chris Wilson &lt;<a href=3D"mailto:d=
ead.fets@gmail.com">dead.fets@gmail.com</a>&gt; wrote:<br></div><blockquote=
 class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px so=
lid rgb(204,204,204);padding-left:1ex"><br>
<br>
Hello Andy,<br>
<br>
This=C2=A0 one=C2=A0 but it appears the directory has been removed subseque=
nt to<br>
me downloading it a few months ago. Thanks.<br>
<br>
Try this<br>
<a href=3D"http://www.g4jnt.com/DropF/simpletimer.zip" rel=3D"noreferrer" t=
arget=3D"_blank">http://www.g4jnt.com/DropF/simpletimer.zip</a><br>
<br>
It lets you abort the on time using the [esc] key<br>
<br>
Source code is in there as well <br>
<br>
All in PowerBasic, command line compiler version<br>
(By far the nicest way to programme simple things that don&#39;t need whizz=
y windows interfaces)<br>
<br>
Andy<br>
<br>
<br>
<br>
Tuesday, February 12, 2019, 4:42:14 PM, you wrote:<br>
<br>
&gt; What programme are you referring to ?<br>
<br>
<br>
<br>
<br>
&gt; Andy<br>
&gt; <a href=3D"http://www.g4jnt.com" rel=3D"noreferrer" target=3D"_blank">=
www.g4jnt.com</a><br>
<br>
<br>
<br>
<br>
&gt; On Tue, 12 Feb 2019 at 13:55, Chris Wilson &lt;<a href=3D"mailto:dead.=
fets@gmail.com" target=3D"_blank">dead.fets@gmail.com</a>&gt; wrote:<br>
<br>
<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 Hello=C2=A0 Andy,<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 =C2=A0 I=C2=A0 have=C2=A0 had=C2=A0 great=C2=A0 service from you=
r Simple Timer programme, thank<br>
&gt;=C2=A0 =C2=A0 you!=C2=A0 I=C2=A0 am=C2=A0 wondering how hard it would b=
e to add a simple ON / OFF<br>
&gt;=C2=A0 =C2=A0 command to it so I can turn my PSU on and off without ent=
ering times<br>
&gt;=C2=A0 =C2=A0 for both? Thanks!=C2=A0 2E0ILY<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 -- <br>
&gt;=C2=A0 Best regards,<br>
&gt;=C2=A0 =C2=A0Chris=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=
=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 mailto:<a href=3D"mailto:dead.fets@g=
mail.com" target=3D"_blank">dead.fets@gmail.com</a><br>
&gt;=C2=A0 <br>
&gt;=C2=A0 <br>
<br>
<br>
<br>
-- <br>
Best regards,<br>
=C2=A0Chris=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 mailto:<a href=3D"mailto:dead.fets@gmail=
.com" target=3D"_blank">dead.fets@gmail.com</a><br>
<br>
<br>
</blockquote></div></div>

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Thread-Topic: SlowJT9 update (v0.9.16.0)
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 Content preview:  Dear all, Beta-release v0.9.16.0 of SlowJT9 has been uploaded,
    see http://www.472khz.org/SlowJT9/. As mentioned earlier I was intrigued
   by one sentence in the mail from David, G0MRF, (17 Januari): 
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--_000_155001175480348795kuleuvenbe_
Content-Type: text/plain; charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Dear all,

Beta-release v0.9.16.0 of SlowJT9 has been uploaded, see http://www.472khz.=
org/SlowJT9/.

As mentioned earlier I was intrigued by one sentence in the mail from David=
, G0MRF,  (17 Januari):

"Interestingly Rik's SlowJT9 which was running in parallel, managed to deco=
de a couple of more transmissions than WSJT-X."

As SlowJT9 uses the JT9 decoder from the WSJT-X suite the performance of Sl=
owJT9 and WSJT-X should be identical. The only difference between both coul=
d be a small timing difference that made SlowJT9 to decode some extra trans=
missions (pure luck, it could have been the other way around as well).
So maybe the performance of SlowJT9 can be improved by running the recorded=
 audio several times through the decoder with each time a small (0.1 second=
 ?) time shift induced in the audio and then taking a "best off" all decode=
d signals?
A computer simulation showed an inprovement of 1-2 dB, see http://www.472kh=
z.org/SlowJT9/multidec.html.

So I decided to add a "Multiple decoding" option (Settings ? Mode ? check "=
Allow multiple decoding").
If "Multiple decoding" is enabled the received audio will first de decoded =
as it is and then shifted +/- 1 second in time steps of 0.2 seconds and dec=
oded again for each step.
Thus there will 11 decoding steps in total.
However decoding always will stopped at 1 second before the end of the cycl=
e at latest, so the next cycle will not be corrupted.
Decoding can also be stopped by clicking on the Band activity or RX frequen=
cy windows. After each decoding step the new (non-duplicate) decoded messag=
es are shown.
So even during the decoding process any already decoded message can be sele=
cted by triple-clicking on it (a single click for stopping the decoding fol=
lowed by a double click for selecting the message).

Be aware that for now all decodings are performed one after another and eac=
h one can take several seconds on a slow computer. In that case only a limi=
ted number of decoding steps will be performed.
But if multiple decoding also shows a significant improvement in the field =
I will have a look at parallel processing of the decodings.
In order to be able to evaluate multiple decoding the DT parameter now does=
 not show the time offset of the received signal but the time offset of the=
 decoded audio file. This means that any message with a DT value different =
from 0.0 is a decoded message that would have been missed before.

I will appreciate all feedback about the number of decoded messages with a =
DT diffeternt from 0.0.
Of course bug reports, remarks and suggestions are still welcome.

?73, Rik  ON7YD - OR7T

--_000_155001175480348795kuleuvenbe_
Content-Type: text/html; charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

<html>
<head>
<meta http-equiv=3D"Content-Type" content=3D"text/html; charset=3Diso-8859-=
1">
<style type=3D"text/css" style=3D"display:none"><!-- p { margin-top: 0px; m=
argin-bottom: 0px; }--></style>
</head>
<body dir=3D"ltr" style=3D"font-size:10pt;color:#000000;background-color:#F=
FFFFF;font-family:Tahoma,Geneva,sans-serif;">
<div dir=3D"ltr" style=3D"font-size:10pt; color:#000000; background-color:#=
FFFFFF; font-family:Tahoma,Geneva,sans-serif">
<div>Dear all,<br>
<br>
Beta-release v0.9.16.0 of SlowJT9 has been uploaded, see <a href=3D"http://=
www.472khz.org/SlowJT9/" target=3D"_blank">
http://www.472khz.org/SlowJT9/</a>.<br>
<br>
</div>
<div><span style=3D"font-family: Tahoma, Geneva, sans-serif; font-size: 13.=
3333px; background-color: rgb(255, 255, 255);">As mentioned earlier&nbsp;I =
was intrigued by one sentence in the&nbsp;mail from David, G0MRF,&nbsp; (17=
 Januari):</span>
<div style=3D"font-family: Tahoma, Geneva, sans-serif; font-size: 13.3333px=
; background-color: rgb(255, 255, 255);">
<br>
&quot;<em style=3D"color: rgb(0, 111, 201); text-decoration-style: solid; t=
ext-decoration-color: rgb(0, 111, 201);"><strong>Interestingly Rik's SlowJT=
9 which was running in parallel, managed to decode a couple of more transmi=
ssions than WSJT-X</strong>.</em>&quot;<br>
<br>
As SlowJT9&nbsp;uses the JT9 decoder from the WSJT-X suite the performance =
of SlowJT9 and WSJT-X should be identical. The only difference between both=
 could be a small timing difference that made SlowJT9 to decode some extra =
transmissions (pure luck, it could have
 been the other way around as well).&nbsp;</div>
<div style=3D"font-family: Tahoma, Geneva, sans-serif; font-size: 13.3333px=
; background-color: rgb(255, 255, 255);">
So maybe the performance of SlowJT9 can be improved by&nbsp;running the rec=
orded audio several times through the decoder with each time a small (0.1 s=
econd ?) time shift induced in the audio and then taking a &quot;best off&q=
uot; all decoded signals?<br>
</div>
<div style=3D"font-family: Tahoma, Geneva, sans-serif; font-size: 13.3333px=
; background-color: rgb(255, 255, 255);">
A computer simulation showed an inprovement of 1-2 dB, see&nbsp;<a href=3D"=
http://www.472khz.org/SlowJT9/multidec.html">http://www.472khz.org/SlowJT9/=
multidec.html</a>.<br>
</div>
<br>
</div>
<div><span style=3D"font-family: Tahoma, Geneva, sans-serif; font-size: 13.=
3333px; background-color: rgb(255, 255, 255);">So I decided to add a&nbsp;<=
/span><span style=3D"font-size: 10pt;">&quot;Multiple decoding&quot; option=
&nbsp;(Settings &#8594; Mode &#8594; check &quot;Allow multiple decoding&qu=
ot;).</span></div>
<div>If &quot;Multiple decoding&quot; is enabled the received audio will fi=
rst de decoded as it is and then shifted &#43;/- 1 second in time steps of =
0.2 seconds and decoded again for each step.<br>
Thus there will 11 decoding steps in total.<br>
However decoding always will stopped at 1 second before the end of the cycl=
e at latest, so the next cycle will not be corrupted.<br>
Decoding can also be stopped by clicking on the&nbsp;<em>Band activity</em>=
&nbsp;or&nbsp;<em>RX frequency</em>&nbsp;windows. After each decoding step =
the new (non-duplicate) decoded messages are&nbsp;shown.<br>
So even during the decoding process any already decoded message can be sele=
cted by&nbsp;<strong>triple-clicking</strong>&nbsp;on it (a single click fo=
r stopping the decoding followed by a double click for selecting the messag=
e).<br>
<br>
</div>
<div>Be aware that for now all&nbsp;decodings&nbsp;are performed one after =
another and&nbsp;each one can take several seconds on a slow computer.&nbsp=
;In that case only a limited number of decoding steps will be performed.</d=
iv>
<div>But if multiple decoding also&nbsp;shows a significant improvement in =
the field I will have a look at parallel processing of the decodings.</div>
<div>In order to be able to evaluate multiple decoding&nbsp;the DT paramete=
r now does not show the time offset of the received&nbsp;signal but the tim=
e offset of the decoded&nbsp;audio file.
<strong>This means that any message with a DT value different from 0.0 is a=
 decoded&nbsp;message that would have been missed before.</strong></div>
<div><br>
I will appreciate all feedback about the number of decoded messages with a =
DT diffeternt from 0.0.<br>
Of course bug reports, remarks and suggestions are still&nbsp;welcome.<br>
<br>
<div>
<div>&#8203;73, Rik&nbsp; ON7YD - OR7T<br>
</div>
</div>
</div>
</div>
</body>
</html>

--_000_155001175480348795kuleuvenbe_--

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Wed, 13 Feb 2019 10:35:54 +1100
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 Content preview:  Hi Stefan, > Yes. First you only need the primary winding
   to see if it stays cool at > the full volume level. You know, saturation and
    so on. Only use as many > turns as necessary for the frequency, that is idea
    [...] 
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Subject: Re: R: Re: VLF: in VK?
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Hi Stefan,

> Yes. First you only need the primary winding to see if it stays cool at
> the full volume level. You know, saturation and so on. Only use as many
> turns as necessary for the frequency, that is ideal. But probably you
> know all that.
> If you know the co
> re material and the cross section area the the B max, then you can do a
> rough calculation as well...
> Here it's a bit like sitting a pub, exchanging some ideas about VLF.

I'd love to participate in a pub outing with VLF gurus! There's
nothing like a good chat over a couple of beers!

I will do a proper test: an appropriate resistor (50 ohm if I decide
to do 50 ohm to 4 ohm transformer) at the output winding and the
amplifier at max power. The only thing that should get hot must be the
resistor!

I made long time ago a web calculator for this:

http://people.physics.anu.edu.au/~dxt103/calculators/toroid.php

Anyway, I should stop talking about it and just try it out.

> > I have another roll of 3-core cable I can put in parallel to the first
> > one, then my losses will go up by a factor of two
> Go up? I think you mean go down, or switch in series. Ah, yes, put in
> parallel but switch in series. Yes, then, twice the R, 4 times the L and
> so 1/4 of the Cs and only 70% of the current, at the same power level.
> So you can switch the Cs in serial to get on resonance again. But this
> will be even a higher stress for them because the current is 40 % higher
> for each one then. So you need more of them and choose another
> configuration.


Yes, I meant that I will physically put the two cables side by side
and then connect them in series.

> >   but factoring that
> > in the calculations, so does the radiated power (for the same TX
> > power). Then my impedance is higher and as a percentage, the
> > transmission line loss has less effect. Only problem with this is that
> > it was a pain to get the wire up and I suspect it will be a 2^2 times
> > pain to put the second one in parallel :-)
> >
> Yes. And just you are not the one with limited space, so it is better to
> use the wire in another arrangement...

Well, that's a compromise I choose to make in order to have all the
gear near the house and be able to use mains power. I have done field
operation on LF and MF before and it's tricky but not impossible. I
have a number of 12 V 65 Ah SLA batterries which are heavy but I can
transport them around with my car.


> > The only difficulty with this is the 10 m wooden poles. It's not
> > something trivial to transport home and install. But I am always on
> > the lookout for supporting material! A few years ago, I went to a
> > large country fair and I was negotiating with a company that makes and
> > installs woden poles for mains power. They would be happy to come and
> > install a few around my place but the prices were absolutely
> > unrealistic for me. I also have to respect the wishes of my wife who
> > is a conservation ecologist and doesn't necessarily like huge
> > machinery drilling holes and making a mess in pristine native
> > Australian landscape :-) Wires on trees are fine though and I do have
> > a few eucalypts that potentially can be used for this.
> >
> How high are such trees? Can you climb them? Are there Koalas sitting on
> them? And are they dangerous? I've heared they are sleeping and eating
> all the time.

Sadly there are no koalas here, they used to be here but not anymore.
Also sadly, Australian trees are not very good for climbing, they are
generally rather brittle. Not a problem though, I have developed other
techniques to get wires up!

> > Fair enough! I think you have convinced me to try the grounded ends
> > experiment and I will start small with my 120 m loop. I'd be
> > interested to measure the impedance of that, my suspicion is that it
> > could be hundreds of ohms given the very rocky ground.
> It all depends on the ground resistance you can get when using your
> ground rods or whatever at the end. The dry ground is ideal for getting
> a good radiation resistance but on the other sde you need a high antenna
> current and so you need a low loop resitance. It is a proadoxon.
> I already asked about those small ponds arround the dry landscape. What
> is it? For what are they used?

These are dams, people use the water in them for irrigation. The most
common crop here is grapes for making wine.

> It is no effort to walk arround and lay some cable on the ground and try
> see how much antenna current you will get, and then calculate the
> losses, or the serial resiatance. Make a DC measurement, that is very
> informative and quickly done. Then you have an impression how you have
> to wind the transformer. Use a higher DC voltage than 12 V, maybe 100V
> DC is a good idea, if you have a suitable power supply.
> You will need to contact these small ponds to get the loop resistance
> down. They are ideal for the job, really ideal.
> We also have to consider other conductive metallic structures below the
> ground. If there is a metally water pipe below the ground, it may bypass
> you antenna current, ie.e. it lowers the loop area! Also the electrical
> grounding of your house may be an issue. If you lay a 2000m wire close
> to the house of a neighbour, and your and his mains ground is conbnected
> together, then the efficiency will be poor.
> Assuming a 1000 m distance between the wire ends, and using those small
> ponds (put a plate of 1m x 1m in there, for example and as a test at
> least), and assuming there is no bypass, i estimate you can come down to
> say 200 Ohm? At least it will be an interesting information and a next step.

Hmm, my understanding is that a DC measurement won't be too useful as
it will suffer from polarisation problems. When you do a DC
measurement, try to reverse the polarity and let me know what happens
to the resistance you are measuring compared to the previous polarity.
I think the impedance should be measured with AC and in fact at the
same frequency you are planning to use. Anyway, there is enough space
here to avoid being close to other houses, which is good. I do have
the permission from the land owner north of me to put antennas on the
ground, but he runs cattle and they will probably interfere with the
wire. There are times though that the paddock is rested, and that's
when I should strike!


> >   I generally use my oscilloscope and signal
> > generator to measure these parameters using a home made bridge and my
> > capacitor box. This gets a bit tricky on the field. How do you do it?
> >
> I have a very good scope that's also able to show a spectrum. I modified
> it that it can run on a 12 V battery and i take it to the feed point in
> my car each time. There there signal strengh of the fundamental
> frequency is maximised during the tuning process, using the FFT and auto
> measure function.

Ok, I see. My CRO is an old digital Tek and I don't want to modify it
but it does run with a small 12V to 240VAC inverter.

> > Maybe we should start writing a 'techniques' manual for the beginner
> > VLF enthusiast? Perhaps I can start writing things down in my page and
> > you can contribute your trade secrets? ;-)
> >
> That would be a very good idea and it is good to start at the beginning,
> your beginning.  It is also a bit like a diary, you can always look back
> what you've done a year ago.
> Maybe, who knows, a few OM are following the discussion and will join
> the experiments, not only but hopefully in Australia.

I will start such a page and once it has enough material in it, I will
let the mailing list know. Then I will be open to contributions of
content :-)

73, Dimitris VK2COW/VK1SV

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Wed, 13 Feb 2019 16:17:49 +1100
Message-ID: <CAKvcm2eotJOvzSZGmn2Jy_GHM8RbAD=hHH0TWS2OpxqLtA-Akw@mail.gmail.com>
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 Content preview:  Hi VLF, > I will do a proper test: an appropriate resistor
    (50 ohm if I decide > to do 50 ohm to 4 ohm transformer) at the output winding
    and the > amplifier at max power. The only thing that should get hot m [...]
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Hi VLF,

> I will do a proper test: an appropriate resistor (50 ohm if I decide
> to do 50 ohm to 4 ohm transformer) at the output winding and the
> amplifier at max power. The only thing that should get hot must be the
> resistor!
>
> I made long time ago a web calculator for this:
>
> http://people.physics.anu.edu.au/~dxt103/calculators/toroid.php
>
> Anyway, I should stop talking about it and just try it out.

Just finished making a pair of impedance transformers. I used some
junk box large (OD=61.5mm, ID=37.5mm, L=12.8mm) ferrite toroids of
unknown material and I stacked two on each transformer. I then made an
autotransformer with a total of 52 turns tapped at 15 turns making
roughly a 4 ohm to 50 ohm transformer (48 ohm to 4 ohm to be pricese).
I wasn't aiming for 50 ohms it just happened to be the number of turns
that neatly fitted on the toroids!! A=3.2cm^2 and the calculated Bmax
for the expected power levels is less than 500 gauss so we are in
business.

I then did some tests with the amplifier, I connected the two 50 ohm
windings back to back and place the amplifier on one end and a 4 ohm
high wattage resistor at the other end. I was pleased to see that the
resistor got super hot and the transformers remained cool as a
cucumber. I was able to get on the resistor more than 100 watts from
f=3 kHz to 20 kHz, which reduced to 80 watts at 30 kHz. I can live
with that. The amplifier is nominally 100 W output per channel.

Fingers crossed now I will get a chance to fire it up on the antenna
this weekend!

73, Dimitris VK2COW/VK1SV

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Date: Wed, 13 Feb 2019 08:12:51 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hi ELF, Attached is the resulting spectrogram of the post-processing
    of the carrier transmission, using optimised filter and blanker parameters.
    The trace is something like 'O copy' in 212 uHz. It was the fir [...] 
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--------------070506020800080000020304
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Hi ELF,

Attached is the resulting spectrogram of the post-processing of the 
carrier transmission, using optimised filter and blanker parameters. The 
trace is something like 'O copy' in 212 uHz. It was the first goal of 
the transmissions on that frequency.
The time stamps are rubbish, the spectrogram covers 36 hours and scrolls 
at 20 min/pixel.

73, Stefan


Am 07.02.2019 17:05, schrieb DK7FC:
> Hi ELF ;-)
>
> I'm glad to announce that since 15:46 UTC i am transmitting on ELF 
> (the real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 
> <https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first 
> time ever.
>
> Here are the parameters:
>
> TX frequency: *22.970 Hz*
> Wavelength of that frequency: *13060 km*
> Antenna voltage: *4.8 kV rms* (+ a DC component of 7.5 kV)
> Antenna current: *325 uA*
> ERP: 600 aW, or *6E-16 W*
>
> Call it QRP!
> The goal is to detect the signal on my 3.5 km distant tree grabber, 
> whose E field is now working again. Since the E field probe is not to 
> far above the tree, the effective height is not as much as it should 
> ideally be, at this frequency, so the RX is somewhat deaf. Anyway i 
> can see the Schumann resonances and the 60 Hz power grid. So i hope it 
> will work.
>
> A spectrogram which is centered on the frequency of interest in now 
> shown at 
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html 
> (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! 
> In a few minutes we'll see more :-) It takes about 40 minutes until a 
> peak could have fully developed...
>
> 73, Stefan
>

--------------070506020800080000020304
Content-Type: text/html; charset=ISO-8859-15
Content-Transfer-Encoding: 7bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=ISO-8859-15"
 http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
Hi ELF, <br>
<br>
Attached is the resulting spectrogram of the post-processing of the
carrier transmission, using optimised filter and blanker parameters.
The trace is something like 'O copy' in 212 uHz. It was the first goal
of the transmissions on that frequency.<br>
The time stamps are rubbish, the spectrogram covers 36 hours and
scrolls at 20 min/pixel.<br>
<br>
73, Stefan<br>
<br>
<br>
Am 07.02.2019 17:05, schrieb DK7FC:
<blockquote cite="mid:5C5C5757.5080906@posteo.de" type="cite">
  <meta http-equiv="content-type"
 content="text/html; charset=ISO-8859-15">
Hi ELF ;-)<br>
  <br>
I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a moz-do-not-send="true"
 href="https://en.wikipedia.org/wiki/Radio_spectrum#ITU">ITU radio band
1</a> ) for the first time ever.<br>
  <br>
Here are the parameters: <br>
  <br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
  <br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
  <br>
A spectrogram which is centered on the frequency of interest in now
shown at
  <a moz-do-not-send="true" class="moz-txt-link-freetext"
 href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
  <br>
73, Stefan<br>
  <br>
</blockquote>
</body>
</html>

--------------070506020800080000020304--

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From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Wed, 13 Feb 2019 11:24:13 +0100
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 Content preview:  Joe, Stefan, LF Another night with a strong signal from you,
    Joe. Thanks again for your transmissions which provides good opportunities
    for RX equipment testing. Last night, in particular, I tried to listen your
    sign [...] 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Joe, Stefan, LF

Another night with a strong signal from you, Joe. Thanks again for your
transmissions which provides good opportunities for RX equipment testing.
Last night, in particular, I tried to listen your signal with my *SLMS
HP-3746A*, equipped with its high stability oscillator (OPT.014). I have
got good decodes with *NO GPS* *reference* connected to audio card or
instrument; I noticed only a slight phase rotation in a couple of cases.
I used my TX inv. "L" antenna (that was tuned this time) and a 6 dB
attenuator.
You can see here the results:

UTC   Eb/N0[dB] Carr.S/N[dB] Mess.
0030 7.1  32.14 *******
0100  8.0  32.20 VO1NA_R
0130 5.2  29.08 *******
0200 4.0  27.95 VO1NA_R
0230 5.7  29.01 *******
0300 3.3  27.79 VO1NA_R
0330 NIL    -              -
0400 9.0  32.46 VO1NA_R
0430 7.3  31.49 *******
0500 6.2  30.55 VO1NA_R
0530 6.1  29.86 *******
0600    -0.3  24.48 VO1NA_R


All the best


73 de Riccardo IW4DXW



Il giorno lun 11 feb 2019 alle ore 21:05 <jcraig@mun.ca> ha scritto:

> Hi Riccardo, Stefan, LF,
>
> Pleased to get your report of improved signal strength Riccardo.
> The R means "Rotated L" so it is in the sky again since yesterday.
> Today a cermaic feedthrough was installed on the PVC bucket
> that houses the coil. It was cold (-10 C) today but the work had
> to be done; there was too much charring and arcing.  All seems OK
> now and the TX is on (one Decca module) 2.2A RF
>
> 73
> Joe VO1NA
>
> On Mon, 11 Feb 2019, DK7FC wrote:
>
> > Hello Riccardo,
> >
> > I like the precision of your RX frequency. I should add a few nulls to
> my
> > file too :-)
> > Good work regarding Joe's reception!
> >
> > 73, Stefan
> >
> > Am 11.02.2019 12:56, schrieb Riccardo Zoli:
> >>
> >> Joe, LF
> >>
> >> Very strong signal last night continuously from 2330z to 0530z.
> >> Best decode at 0300z, info attached.
> >> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
> >> inserted) and SDR.
> >>
> >> All the best,
> >>
> >> 73 de Riccardo IW4DXW
> >>
> >> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca
> >> <mailto:jcraig@mun.ca>> ha scritto:
> >>
> >>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
> >>     autodetector.
> >>     73
> >>     Joe
> >>
> >>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
> >>
> >>     > Dominico,
> >>     >
> >>     > Thanks to you and Markus and Domenico for the autodecoder service.
> >>     > I will check the modulator and try again tonight. Some antenna
> work
> >>     > is planned as well when the wx improves so there should be some
> more
> >>     > dB available soon.
> >>     >
> >>     > 73
> >>     > Joe
> >>     >
> >>     > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
> >>     >
> >>     >> Joe, LF
> >>     >> in my EbNaut log
> >>     >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
> >>     >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
> >>     >> there are some decodes of your EbNaut of last nights (QRB=5426
> >>     km). Seems
> >>     >> that since yesterday, only carrier is sent on usual qrg 137477
> Hz.
> >>     >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
> >>     parameters:
> >>     >>
> >>     >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
> Duration=1824s
> >>     >> T_OFFSET=0.0s F_OFFSET=0.000Hz
> >>     >>
> >>     >> 73, Domenico IZ7SLZ / JN80nu
> >>     >>
> >>     >
> >>     >
> >>
> >
>
>

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Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><br><div>Joe, Stefan, LF</div><div><br></=
div><div>Another night with a strong signal from you, Joe. Thanks again for=
 your transmissions which provides good opportunities for RX equipment test=
ing.</div><div>Last night, in particular, I tried to listen your signal wit=
h my <b>SLMS HP-3746A</b>, equipped with its high stability oscillator (OPT=
.014). I have got good decodes with <b>NO GPS</b> <b>reference</b> connecte=
d to audio card or instrument; I noticed only a slight phase rotation in a =
couple of cases.</div><div>I used my TX inv. &quot;L&quot; antenna (that wa=
s tuned this time) and a 6 dB attenuator.</div><div>You can see here the re=
sults:</div><div><br></div><div><div>UTC =C2=A0 Eb/N0[dB] Carr.S/N[dB]<span=
 class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	</span>Mess.</di=
v><div>0030<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	=
    </span>7.1<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre=
">	</span> =C2=A032.14<span class=3D"gmail-Apple-tab-span" style=3D"white-s=
pace:pre">		</span>*******</div><div>0100<span style=3D"white-space:pre">=
=C2=A0    </span>8.0<span class=3D"gmail-Apple-tab-span" style=3D"white-spa=
ce:pre">	</span> =C2=A032.20<span class=3D"gmail-Apple-tab-span" style=3D"w=
hite-space:pre">		</span>VO1NA_R</div><div>0130<span class=3D"gmail-Apple-t=
ab-span" style=3D"white-space:pre">	    </span>5.2<span class=3D"gmail-Appl=
e-tab-span" style=3D"white-space:pre">	</span> =C2=A029.08<span class=3D"gm=
ail-Apple-tab-span" style=3D"white-space:pre">		</span>*******</div><div>02=
00<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	    </spa=
n>4.0<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	</span=
> =C2=A027.95<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre"=
>		</span>VO1NA_R</div><div>0230<span class=3D"gmail-Apple-tab-span" style=
=3D"white-space:pre">	    </span>5.7<span class=3D"gmail-Apple-tab-span" st=
yle=3D"white-space:pre">	</span> =C2=A029.01<span class=3D"gmail-Apple-tab-=
span" style=3D"white-space:pre">		</span>*******</div><div>0300<span class=
=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	    </span>3.3<span cl=
ass=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	</span> =C2=A027.79=
<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">		</span>VO1=
NA_R</div><div>0330<span class=3D"gmail-Apple-tab-span" style=3D"white-spac=
e:pre">	    </span>NIL<span class=3D"gmail-Apple-tab-span" style=3D"white-s=
pace:pre">	</span> =C2=A0 =C2=A0-<span class=3D"gmail-Apple-tab-span" style=
=3D"white-space:pre">		</span>=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=
=A0-</div><div>0400<span class=3D"gmail-Apple-tab-span" style=3D"white-spac=
e:pre">	    </span>9.0<span class=3D"gmail-Apple-tab-span" style=3D"white-s=
pace:pre">	</span> =C2=A032.46<span class=3D"gmail-Apple-tab-span" style=3D=
"white-space:pre">		</span>VO1NA_R</div><div>0430<span class=3D"gmail-Apple=
-tab-span" style=3D"white-space:pre">	    </span>7.3<span class=3D"gmail-Ap=
ple-tab-span" style=3D"white-space:pre">	</span> =C2=A031.49<span class=3D"=
gmail-Apple-tab-span" style=3D"white-space:pre">		</span>*******</div><div>=
0500<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	    </s=
pan>6.2<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pre">	</sp=
an> =C2=A030.55<span class=3D"gmail-Apple-tab-span" style=3D"white-space:pr=
e">		</span>VO1NA_R</div><div>0530<span class=3D"gmail-Apple-tab-span" styl=
e=3D"white-space:pre">	    </span>6.1<span class=3D"gmail-Apple-tab-span" s=
tyle=3D"white-space:pre">	</span> =C2=A029.86<span class=3D"gmail-Apple-tab=
-span" style=3D"white-space:pre">		</span>*******</div><div>0600 =C2=A0 =C2=
=A0<span style=3D"line-height:1.5">-0.3</span><span class=3D"gmail-Apple-ta=
b-span" style=3D"line-height:1.5;white-space:pre">	</span><span style=3D"li=
ne-height:1.5"> =C2=A024.48</span><span class=3D"gmail-Apple-tab-span" styl=
e=3D"line-height:1.5;white-space:pre">		</span><span style=3D"line-height:1=
.5">VO1NA_R</span><span class=3D"gmail-Apple-tab-span" style=3D"line-height=
:1.5;white-space:pre">	</span></div></div><div><br></div><div><br></div><di=
v>All the best</div><div><br></div><div><br></div><div>73 de Riccardo IW4DX=
W</div><div><br></div><div><br></div></div></div><br><div class=3D"gmail_qu=
ote"><div dir=3D"ltr" class=3D"gmail_attr">Il giorno lun 11 feb 2019 alle o=
re 21:05 &lt;<a href=3D"mailto:jcraig@mun.ca">jcraig@mun.ca</a>&gt; ha scri=
tto:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px=
 0.8ex;border-left-width:1px;border-left-color:rgb(204,204,204);border-left=
-style:solid;padding-left:1ex">Hi Riccardo, Stefan, LF,<br>
<br>
Pleased to get your report of improved signal strength Riccardo.<br>
The R means &quot;Rotated L&quot; so it is in the sky again since yesterday=
.<br>
Today a cermaic feedthrough was installed on the PVC bucket<br>
that houses the coil. It was cold (-10 C) today but the work had<br>
to be done; there was too much charring and arcing.=C2=A0 All seems OK<br>
now and the TX is on (one Decca module) 2.2A RF<br>
<br>
73<br>
Joe VO1NA<br>
<br>
On Mon, 11 Feb 2019, DK7FC wrote:<br>
<br>
&gt; Hello Riccardo,<br>
&gt;<br>
&gt; I like the precision of your RX frequency. I should add a few nulls to=
 my <br>
&gt; file too :-)<br>
&gt; Good work regarding Joe&#39;s reception!<br>
&gt;<br>
&gt; 73, Stefan<br>
&gt;<br>
&gt; Am 11.02.2019 12:56, schrieb Riccardo Zoli:<br>
&gt;&gt; <br>
&gt;&gt; Joe, LF<br>
&gt;&gt; <br>
&gt;&gt; Very strong signal last night continuously from 2330z to 0530z.<br=
>
&gt;&gt; Best decode at 0300z, info attached.<br>
&gt;&gt; RX setup: inverted &quot;L&quot; TX antenna (slightly detuned, 6 d=
B attenuator <br>
&gt;&gt; inserted) and SDR.<br>
&gt;&gt; <br>
&gt;&gt; All the best,<br>
&gt;&gt; <br>
&gt;&gt; 73 de Riccardo IW4DXW<br>
&gt;&gt; <br>
&gt;&gt; Il giorno gio 7 feb 2019 alle ore 17:44 &lt;<a href=3D"mailto:jcra=
ig@mun.ca" target=3D"_blank">jcraig@mun.ca</a> <br>
&gt;&gt; &lt;mailto:<a href=3D"mailto:jcraig@mun.ca" target=3D"_blank">jcra=
ig@mun.ca</a>&gt;&gt; ha scritto:<br>
&gt;&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0Apologies: I misspelt Domenico and did not ackn=
owledge Riccardo&#39;s<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0autodetector.<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A073<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0Joe<br>
&gt;&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0On Thu, 7 Feb 2019, <a href=3D"mailto:jcraig@mu=
n.ca" target=3D"_blank">jcraig@mun.ca</a> &lt;mailto:<a href=3D"mailto:jcra=
ig@mun.ca" target=3D"_blank">jcraig@mun.ca</a>&gt; wrote:<br>
&gt;&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; Dominico,<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; Thanks to you and Markus and Domenico for =
the autodecoder service.<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; I will check the modulator and try again t=
onight. Some antenna work<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; is planned as well when the wx improves so=
 there should be some more<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; dB available soon.<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; 73<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; Joe<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt; On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:=
<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; Joe, LF<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; in my EbNaut log<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; *<a href=3D"https://qsl.net/iz7slz/EBN=
AUT/DECODED.TXT" rel=3D"noreferrer" target=3D"_blank">https://qsl.net/iz7sl=
z/EBNAUT/DECODED.TXT</a><br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; &lt;<a href=3D"https://qsl.net/iz7slz/=
EBNAUT/DECODED.TXT" rel=3D"noreferrer" target=3D"_blank">https://qsl.net/iz=
7slz/EBNAUT/DECODED.TXT</a>&gt;*<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; there are some decodes of your EbNaut =
of last nights (QRB=3D5426<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0km). Seems<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; that since yesterday, only carrier is =
sent on usual qrg 137477 Hz.<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; Autodecoder here is now running, every=
 XX:00 and XX:30 on Joe&#39;s<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0parameters:<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; 137477.000Hz N=3D7 T=3D3s 8K19A CRC=3D=
16 list=3D2000 sym=3D608 Duration=3D1824s<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; T_OFFSET=3D0.0s F_OFFSET=3D0.000Hz<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt; 73, Domenico IZ7SLZ / JN80nu<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;<br>
&gt;&gt;=C2=A0 =C2=A0 =C2=A0&gt;<br>
&gt;&gt; <br>
&gt;<br>
<br>
</blockquote></div>

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Congratulation !
TOP!!!

*I55387FI*
*Daniele Caccia*


www.scientific-notes.blogspot.com
www.altamaremmacameratrapping.blogspot.com



Il giorno mer 13 feb 2019 alle ore 08:16 DK7FC <selberdenken@posteo.de> ha
scritto:

> Hi ELF,
>
> Attached is the resulting spectrogram of the post-processing of the
> carrier transmission, using optimised filter and blanker parameters. The
> trace is something like 'O copy' in 212 uHz. It was the first goal of the
> transmissions on that frequency.
> The time stamps are rubbish, the spectrogram covers 36 hours and scrolls
> at 20 min/pixel.
>
> 73, Stefan
>
>
> Am 07.02.2019 17:05, schrieb DK7FC:
>
> Hi ELF ;-)
>
> I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
> real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1
> <https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first time
> ever.
>
> Here are the parameters:
>
> TX frequency: *22.970 Hz*
> Wavelength of that frequency: *13060 km*
> Antenna voltage: *4.8 kV rms* (+ a DC component of 7.5 kV)
> Antenna current: *325 uA*
> ERP: 600 aW, or *6E-16 W*
>
> Call it QRP!
> The goal is to detect the signal on my 3.5 km distant tree grabber, whose
> E field is now working again. Since the E field probe is not to far above
> the tree, the effective height is not as much as it should ideally be, at
> this frequency, so the RX is somewhat deaf. Anyway i can see the Schumann
> resonances and the 60 Hz power grid. So i hope it will work.
>
> A spectrogram which is centered on the frequency of interest in now shown
> at http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html
> (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In a
> few minutes we'll see more :-) It takes about 40 minutes until a peak could
> have fully developed...
>
> 73, Stefan
>
>

--0000000000003359460581c4b774
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr">Congratulation !<div>TOP!!!</div><div><br></div><div><b><f=
ont size=3D"4">I55387FI</font></b><br clear=3D"all"><div><div dir=3D"ltr" c=
lass=3D"gmail_signature" data-smartmail=3D"gmail_signature"><div dir=3D"ltr=
"><div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div =
dir=3D"ltr"><b style=3D"font-size:14px">Daniele Caccia</b></div><div dir=3D=
"ltr"><div><br></div><div><div><br></div><div><font color=3D"#0000ff" face=
=3D"Verdana"><a href=3D"http://www.scientific-notes.blogspot.com" target=3D=
"_blank">www.scientific-notes.blogspot.com</a></font></div><div><font color=
=3D"#0000ff" face=3D"Verdana"><a href=3D"http://www.altamaremmacameratrappi=
ng.blogspot.com" target=3D"_blank">www.altamaremmacameratrapping.blogspot.c=
om</a>=C2=A0 <br></font></div><div><br></div></div></div></div></div></div>=
</div></div></div></div><br></div></div><br><div class=3D"gmail_quote"><div=
 dir=3D"ltr" class=3D"gmail_attr">Il giorno mer 13 feb 2019 alle ore 08:16 =
DK7FC &lt;<a href=3D"mailto:selberdenken@posteo.de">selberdenken@posteo.de<=
/a>&gt; ha scritto:<br></div><blockquote class=3D"gmail_quote" style=3D"mar=
gin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1=
ex"><u></u>


 =20

<div bgcolor=3D"#ffffff">
Hi ELF, <br>
<br>
Attached is the resulting spectrogram of the post-processing of the
carrier transmission, using optimised filter and blanker parameters.
The trace is something like &#39;O copy&#39; in 212 uHz. It was the first g=
oal
of the transmissions on that frequency.<br>
The time stamps are rubbish, the spectrogram covers 36 hours and
scrolls at 20 min/pixel.<br>
<br>
73, Stefan<br>
<br>
<br>
Am 07.02.2019 17:05, schrieb DK7FC:
<blockquote type=3D"cite">
 =20
Hi ELF ;-)<br>
  <br>
I&#39;m glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a href=3D"https://en.wikipedia=
.org/wiki/Radio_spectrum#ITU" target=3D"_blank">ITU radio band
1</a> ) for the first time ever.<br>
  <br>
Here are the parameters: <br>
  <br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
  <br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
  <br>
A spectrogram which is centered on the frequency of interest in now
shown at
  <a class=3D"gmail-m_7316536638829473026moz-txt-link-freetext" href=3D"htt=
p://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html" target=
=3D"_blank">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber=
2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we&#39;ll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
  <br>
73, Stefan<br>
  <br>
</blockquote>
</div>

</blockquote></div>

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Date: Wed, 13 Feb 2019 13:41:25 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello Andy, I use to remote power my amp power supply on and
    off from elsewhere in the house or remotely. It would be very handy if there
    were also a basic "Stay On" "Turn Off" function rather than having to type
    [...] 
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Hello Andy,

I use to remote power my amp power supply on and off from elsewhere in
the house or remotely. It would be very handy if there were also a
basic "Stay On" "Turn Off" function rather than having to type in
start and finish times. A minor thing, but if it were really easy to
implement.... :) Again thanks for this very useful app which has many
uses.

Tuesday, February 12, 2019, 10:25:31 PM, you wrote:

> Oh yes, I vaguely remember writing it  - in a slack few minutes one
> evening after someone (You ?) requested it.  Found the original source code now
> What are you saying you actually want it to do?


> It's a simple text driven prog so difficult to write interactions
> and things.   AN all singing all dancing prog with options and
> manual control would be better in a windows format.  Are you saying
> you just want a simple on / off control via that same COM port
> interface?   It seems  a rather complicated way to go about things. 
> Wouldn't a toggle switch overriding the COM port control be a simpler solution?


> I clean out that DropF folder regulalrly - it is only for temporary
> file transfers.   Permanent stuff goes elsewhere with fixed links


> Andy
> www.g4jnt.com





> On Tue, 12 Feb 2019 at 22:18, Chris Wilson <dead.fets@gmail.com> wrote:


>  
>  Hello Andy,
>  
>  This  one  but it appears the directory has been removed subsequent to
>  me downloading it a few months ago. Thanks.
>  
>  Try this
>  http://www.g4jnt.com/DropF/simpletimer.zip
>  
>  It lets you abort the on time using the [esc] key
>  
>  Source code is in there as well 
>  
>  All in PowerBasic, command line compiler version
>  (By far the nicest way to programme simple things that don't need whizzy windows interfaces)
>  
>  Andy



-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com



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 Content preview:  Having a clear out at work. There are some hefty studio grade
    audio amplifiers looking for a new home. I'm told they are MC^2 model MC1250,
    rated at (per channel) 1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W
    into 8 ohms. 
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Having a clear out at work.

There are some hefty studio grade audio amplifiers looking
for a new home.

I'm told they are MC^2  model MC1250, rated at (per channel)
1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into
8 ohms.

Weight: about 30kg

I believe there are about 50 of them to be disposed of.

If anyone is interested, they may be available for little more
than the shipping cost (which might be quite high considering
the weight).

Maybe they could be turned to VLF use?

--
Paul Nicholson
--


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To: rsgb_lf_group@blacksheep.org
References: <08e69bca-3228-d583-4c30-58c554b39a61@abelian.org>
From: Terry GW0EZY <GW0EZY@sky.com>
Message-ID: <83d7732c-816a-4972-b1c7-6178468f0220@sky.com>
Date: Wed, 13 Feb 2019 14:08:15 +0000
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 Content preview:  Hi Paul How do we make a request for these? I am interested
    and could fairly easily collect from Doncaster. The spec sheet is available
    with an easy Google "Audio Amplifier MC1250" and they look very good - response
    is quoted for 20 Hz - 20 kHz. 
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Subject: Re: LF: Surplus audio amplifiers
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Hi Paul

How do we make a request for these? I am interested and could fairly 
easily collect from Doncaster.

The spec sheet is available with an easy Google "Audio Amplifier MC1250" 
and they look very good - response is quoted for 20 Hz - 20 kHz.

73 Terry

On 13/02/2019 13:44, Paul Nicholson wrote:
>
> Having a clear out at work.
>
> There are some hefty studio grade audio amplifiers looking
> for a new home.
>
> I'm told they are MC^2  model MC1250, rated at (per channel)
> 1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into
> 8 ohms.
>
> Weight: about 30kg
>
> I believe there are about 50 of them to be disposed of.
>
> If anyone is interested, they may be available for little more
> than the shipping cost (which might be quite high considering
> the weight).
>
> Maybe they could be turned to VLF use?
>
> -- 
> Paul Nicholson
> -- 
>
>
>

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Date: Wed, 13 Feb 2019 14:09:28 +0000
From: Chris Wilson <dead.fets@gmail.com>
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To: Paul Nicholson <rsgb_lf_group@blacksheep.org>
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 Content preview:  Hello Paul, Where are they, maybe a collection would be possible,
    I am certainly interested, thank you. I am in north Shropshire, near the
   Cheshire, north Wales borders but travel about quite a bit. Wednesday, February
    13, 2019, 1:44:42 PM, you wrote: 
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Hello Paul,

Where  are  they, maybe a collection would be possible, I am certainly
interested,  thank  you.  I am in north Shropshire, near the Cheshire,
north Wales borders but travel about quite a bit.

Wednesday, February 13, 2019, 1:44:42 PM, you wrote:


> Having a clear out at work.

> There are some hefty studio grade audio amplifiers looking
> for a new home.

> I'm told they are MC^2  model MC1250, rated at (per channel)
> 1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into
> 8 ohms.

> Weight: about 30kg

> I believe there are about 50 of them to be disposed of.

> If anyone is interested, they may be available for little more
> than the shipping cost (which might be quite high considering
> the weight).

> Maybe they could be turned to VLF use?

> --
> Paul Nicholson
> --





-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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From: Paul Nicholson <vlf0403@abelian.org>
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 Content preview:  I'll arrange to have some transferred to my place of work
   at Stockport - that will secure them from the scrap man - at least until the
    next 5S red tagging exercise! They can probably be collected from [...] 
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I'll arrange to have some transferred to my place
of work at Stockport - that will secure them from
the scrap man - at least until the next 5S red tagging
exercise!  They can probably be collected from there,
or from Todmorden.

Will report back when available.

--
Paul Nicholson
--

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Date: Wed, 13 Feb 2019 15:02:53 +0000
From: Chris Wilson <dead.fets@gmail.com>
X-Priority: 3 (Normal)
Message-ID: <571631289.20190213150253@gmail.com>
To: Paul Nicholson <rsgb_lf_group@blacksheep.org>
In-Reply-To: <75410bf7-b442-0db5-6a97-42a0166ff64d@abelian.org>
References: <08e69bca-3228-d583-4c30-58c554b39a61@abelian.org> <2110578436.20190213140928@gmail.com> <75410bf7-b442-0db5-6a97-42a0166ff64d@abelian.org>
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 Content preview:  Hello Paul, Collection from Stockport would be perfect, I
   used to live in Gatley just up the road and go back a lot. if anyone wants
    one bringing to near Whitchurch in Shropshire I am happy to oblige. Price
    pleas [...] 
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  pts rule name              description
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Subject: Re: LF: Surplus audio amplifiers
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Hello Paul,

Collection  from  Stockport would be perfect, I used to live in Gatley
just  up  the  road and go back a lot. if anyone wants one bringing to
near  Whitchurch in Shropshire I am happy to oblige. Price please? Can
pay up front Paypal family and friends gift, bank transfer or the good
old readies :)

Wednesday, February 13, 2019, 2:52:15 PM, you wrote:


> I'll arrange to have some transferred to my place
> of work at Stockport - that will secure them from
> the scrap man - at least until the next 5S red tagging
> exercise!  They can probably be collected from there,
> or from Todmorden.

> Will report back when available.

> --
> Paul Nicholson
> --




-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


From owner-rsgb_lf_group@blacksheep.org  Wed Feb 13 18:15:58 2019
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To: rsgb_lf_group@blacksheep.org
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 Content preview:  Congrats, Genossen Funkamateurs LF/MF/VLF/ELF! Magic Power
    of Radio bless us! Truly Popov! 
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Congrats, Genossen Funkamateurs LF/MF/VLF/ELF!

Magic Power of Radio bless us!

Truly Popov!

-- 
73!
Roman, RW3ADB

From owner-rsgb_lf_group@blacksheep.org  Wed Feb 13 18:34:11 2019
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 Content preview:  Hello Paul, Would you send one to Germany? What would be the
    price? Datasheet: http://www.mc2-audio.co.uk/wp-content/uploads/mc1250_manual.pdf
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Subject: Re: LF: Surplus audio amplifiers
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Hello Paul,

Would you send one to Germany? What would be the price?

Datasheet: http://www.mc2-audio.co.uk/wp-content/uploads/mc1250_manual.pdf

73, Stefan



Am 13.02.2019 14:44, schrieb Paul Nicholson:
>
> Having a clear out at work.
>
> There are some hefty studio grade audio amplifiers looking
> for a new home.
>
> I'm told they are MC^2  model MC1250, rated at (per channel)
> 1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into
> 8 ohms.
>
> Weight: about 30kg
>
> I believe there are about 50 of them to be disposed of.
>
> If anyone is interested, they may be available for little more
> than the shipping cost (which might be quite high considering
> the weight).
>
> Maybe they could be turned to VLF use?
>
> -- 
> Paul Nicholson
> -- 
>
>

From owner-rsgb_lf_group@blacksheep.org  Wed Feb 13 18:52:26 2019
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From: "Greg Fismer" <DF2IC@DARC.de>
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 Content preview:  Hi Paul, I'm interested, and I'm willing to pay the costs
   for shipping to Germany and additionally for the costs of your efforts and
    the packing material. If that turns out to be too expensive or too much work
    [...] 
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Subject: LF: AW: Surplus audio amplifiers
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Hi Paul,

I'm interested, and I'm willing to pay the costs for shipping to Germany and additionally for the costs of your efforts and the packing material. If that turns out to be too expensive or too much work from your side, maybe shipping to my brother near Whitehaven (Cumbria) is possible? 

Greg DF2IC

-----Ursprüngliche Nachricht-----
Von: owner-rsgb_lf_group@blacksheep.org [mailto:owner-rsgb_lf_group@blacksheep.org] Im Auftrag von Paul Nicholson
Gesendet: Mittwoch, 13. Februar 2019 14:45
An: rsgb_lf_group@blacksheep.org
Betreff: LF: Surplus audio amplifiers


Having a clear out at work.

There are some hefty studio grade audio amplifiers looking for a new home.

I'm told they are MC^2  model MC1250, rated at (per channel) 1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into
8 ohms.

Weight: about 30kg

I believe there are about 50 of them to be disposed of.

If anyone is interested, they may be available for little more than the shipping cost (which might be quite high considering the weight).

Maybe they could be turned to VLF use?

--
Paul Nicholson
--




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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Wed, 13 Feb 2019 19:55:22 +0000
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 Content preview:  It was impractical to modify SimpleTimer, so I wrote another
    prog that just toggles the RTS/DTR lines under keyboard control, using the
    + key to turn on and teh - key to turn off You can find ComOnOff.exe as well
    as SimpleTimer.exe in https://groups.io/g/rsgb-lf-group/files/G4JNT 
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Subject: Re: LF: Re: Simple Timer question
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--000000000000bd588e0581cbecca
Content-Type: text/plain; charset="UTF-8"

It was impractical to modify SimpleTimer, so I wrote another prog that just
toggles the RTS/DTR lines under keyboard control, using the + key to turn
on and teh - key to turn off

You can find ComOnOff.exe  as well as SimpleTimer.exe in
https://groups.io/g/rsgb-lf-group/files/G4JNT


Andy
www.g4jnt.com



On Wed, 13 Feb 2019 at 13:50, Chris Wilson <dead.fets@gmail.com> wrote:

>
>
> Hello Andy,
>
> I use to remote power my amp power supply on and off from elsewhere in
> the house or remotely. It would be very handy if there were also a
> basic "Stay On" "Turn Off" function rather than having to type in
> start and finish times. A minor thing, but if it were really easy to
> implement.... :) Again thanks for this very useful app which has many
> uses.
>
> Tuesday, February 12, 2019, 10:25:31 PM, you wrote:
>
> > Oh yes, I vaguely remember writing it  - in a slack few minutes one
> > evening after someone (You ?) requested it.  Found the original source
> code now
> > What are you saying you actually want it to do?
>
>
> > It's a simple text driven prog so difficult to write interactions
> > and things.   AN all singing all dancing prog with options and
> > manual control would be better in a windows format.  Are you saying
> > you just want a simple on / off control via that same COM port
> > interface?   It seems  a rather complicated way to go about things.
> > Wouldn't a toggle switch overriding the COM port control be a simpler
> solution?
>
>
> > I clean out that DropF folder regulalrly - it is only for temporary
> > file transfers.   Permanent stuff goes elsewhere with fixed links
>
>
> > Andy
> > www.g4jnt.com
>
>
>
>
>
> > On Tue, 12 Feb 2019 at 22:18, Chris Wilson <dead.fets@gmail.com> wrote:
>
>
> >
> >  Hello Andy,
> >
> >  This  one  but it appears the directory has been removed subsequent to
> >  me downloading it a few months ago. Thanks.
> >
> >  Try this
> >  http://www.g4jnt.com/DropF/simpletimer.zip
> >
> >  It lets you abort the on time using the [esc] key
> >
> >  Source code is in there as well
> >
> >  All in PowerBasic, command line compiler version
> >  (By far the nicest way to programme simple things that don't need
> whizzy windows interfaces)
> >
> >  Andy
>
>
>
> --
> Best regards,
>  Chris                            mailto:dead.fets@gmail.com
>
>
>
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--000000000000bd588e0581cbecca
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div class=3D"gmail_defa=
ult" style=3D"font-family:tahoma,sans-serif;font-size:small">It was impract=
ical to modify SimpleTimer, so I wrote another prog that just toggles the R=
TS/DTR lines under keyboard control, using the=C2=A0+ key to turn on and te=
h - key to turn off</div><div class=3D"gmail_default" style=3D"font-family:=
tahoma,sans-serif;font-size:small"><br></div><div class=3D"gmail_default" s=
tyle=3D"font-family:tahoma,sans-serif;font-size:small">You can find ComOnOf=
f.exe=C2=A0 as well as SimpleTimer.exe in=C2=A0<a href=3D"https://groups.io=
/g/rsgb-lf-group/files/G4JNT">https://groups.io/g/rsgb-lf-group/files/G4JNT=
</a></div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-ser=
if;font-size:small"><br></div><div class=3D"gmail_default" style=3D"font-fa=
mily:tahoma,sans-serif;font-size:small"><br></div><div><div dir=3D"ltr" cla=
ss=3D"gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=
=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=
=3D"font-size:12.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank">ww=
w.g4jnt.com</a></span><br></div><div><br></div></div></div></div></div></di=
v></div></div></div></div></div></div><br></div></div><br><div class=3D"gma=
il_quote"><div dir=3D"ltr" class=3D"gmail_attr">On Wed, 13 Feb 2019 at 13:5=
0, Chris Wilson &lt;<a href=3D"mailto:dead.fets@gmail.com">dead.fets@gmail.=
com</a>&gt; wrote:<br></div><blockquote class=3D"gmail_quote" style=3D"marg=
in:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1e=
x"><br>
<br>
Hello Andy,<br>
<br>
I use to remote power my amp power supply on and off from elsewhere in<br>
the house or remotely. It would be very handy if there were also a<br>
basic &quot;Stay On&quot; &quot;Turn Off&quot; function rather than having =
to type in<br>
start and finish times. A minor thing, but if it were really easy to<br>
implement.... :) Again thanks for this very useful app which has many<br>
uses.<br>
<br>
Tuesday, February 12, 2019, 10:25:31 PM, you wrote:<br>
<br>
&gt; Oh yes, I vaguely remember writing it=C2=A0 - in a slack few minutes o=
ne<br>
&gt; evening after someone (You ?) requested it.=C2=A0 Found the original s=
ource code now<br>
&gt; What are you saying you actually want it to do?<br>
<br>
<br>
&gt; It&#39;s a simple text driven prog so difficult to write interactions<=
br>
&gt; and things.=C2=A0 =C2=A0AN all singing all dancing prog with options a=
nd<br>
&gt; manual control would be better in a windows format.=C2=A0 Are you sayi=
ng<br>
&gt; you just want a simple on / off control via that same COM port<br>
&gt; interface?=C2=A0 =C2=A0It seems=C2=A0 a rather complicated way to go a=
bout things.=C2=A0<br>
&gt; Wouldn&#39;t a toggle switch overriding the COM port control be a simp=
ler solution?<br>
<br>
<br>
&gt; I clean out that DropF folder regulalrly - it is only for temporary<br=
>
&gt; file transfers.=C2=A0 =C2=A0Permanent stuff goes elsewhere with fixed =
links<br>
<br>
<br>
&gt; Andy<br>
&gt; <a href=3D"http://www.g4jnt.com" rel=3D"noreferrer" target=3D"_blank">=
www.g4jnt.com</a><br>
<br>
<br>
<br>
<br>
<br>
&gt; On Tue, 12 Feb 2019 at 22:18, Chris Wilson &lt;<a href=3D"mailto:dead.=
fets@gmail.com" target=3D"_blank">dead.fets@gmail.com</a>&gt; wrote:<br>
<br>
<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 Hello Andy,<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 This=C2=A0 one=C2=A0 but it appears the directory has been remov=
ed subsequent to<br>
&gt;=C2=A0 me downloading it a few months ago. Thanks.<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 Try this<br>
&gt;=C2=A0 <a href=3D"http://www.g4jnt.com/DropF/simpletimer.zip" rel=3D"no=
referrer" target=3D"_blank">http://www.g4jnt.com/DropF/simpletimer.zip</a><=
br>
&gt;=C2=A0 <br>
&gt;=C2=A0 It lets you abort the on time using the [esc] key<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 Source code is in there as well <br>
&gt;=C2=A0 <br>
&gt;=C2=A0 All in PowerBasic, command line compiler version<br>
&gt;=C2=A0 (By far the nicest way to programme simple things that don&#39;t=
 need whizzy windows interfaces)<br>
&gt;=C2=A0 <br>
&gt;=C2=A0 Andy<br>
<br>
<br>
<br>
-- <br>
Best regards,<br>
=C2=A0Chris=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 mailto:<a href=3D"mailto:dead.fets@gmail=
.com" target=3D"_blank">dead.fets@gmail.com</a><br>
<br>
<br>
</blockquote></div></div><div id=3D"DAB4FAD8-2DD7-40BB-A1B8-4E2AA1F9FDF2"><=
br>
<table style=3D"border-top:1px solid #d3d4de">
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 Content preview:  Hi Riccardo, Group. Thanks for the details of your experiments
    and the signal reports. The set up here is an NEO7M to a Decca (one PA module)
    to a 100x20m RL aerial. Paul's Ebkey.c clocks the XOR. The RL has several
    dB o [...] 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Hi Riccardo, Group.

Thanks for the details of your experiments and the signal reports.
The set up here is an NEO7M to a Decca (one PA module) to a 100x20m
RL aerial. Paul's Ebkey.c clocks the XOR. The RL has several dB over
the monopole. Perhaps running a counterpoise under the top loading wire 
may yield another dB or 2.  Stefan's and Markus's grabbers are
very helpful too.

73
Joe VO1NA

On Wed, 13 Feb 2019, Riccardo Zoli wrote:

> Joe, Stefan, LF
>
> Another night with a strong signal from you, Joe. Thanks again for your
> transmissions which provides good opportunities for RX equipment testing.
> Last night, in particular, I tried to listen your signal with my *SLMS
> HP-3746A*, equipped with its high stability oscillator (OPT.014). I have
> got good decodes with *NO GPS* *reference* connected to audio card or
> instrument; I noticed only a slight phase rotation in a couple of cases.
> I used my TX inv. "L" antenna (that was tuned this time) and a 6 dB
> attenuator.
> You can see here the results:
>
> UTC   Eb/N0[dB] Carr.S/N[dB] Mess.
> 0030 7.1  32.14 *******
> 0100  8.0  32.20 VO1NA_R
> 0130 5.2  29.08 *******
> 0200 4.0  27.95 VO1NA_R
> 0230 5.7  29.01 *******
> 0300 3.3  27.79 VO1NA_R
> 0330 NIL    -              -
> 0400 9.0  32.46 VO1NA_R
> 0430 7.3  31.49 *******
> 0500 6.2  30.55 VO1NA_R
> 0530 6.1  29.86 *******
> 0600    -0.3  24.48 VO1NA_R
>
>
> All the best
>
>
> 73 de Riccardo IW4DXW
>
>
>
> Il giorno lun 11 feb 2019 alle ore 21:05 <jcraig@mun.ca> ha scritto:
>
>> Hi Riccardo, Stefan, LF,
>>
>> Pleased to get your report of improved signal strength Riccardo.
>> The R means "Rotated L" so it is in the sky again since yesterday.
>> Today a cermaic feedthrough was installed on the PVC bucket
>> that houses the coil. It was cold (-10 C) today but the work had
>> to be done; there was too much charring and arcing.  All seems OK
>> now and the TX is on (one Decca module) 2.2A RF
>>
>> 73
>> Joe VO1NA
>>
>> On Mon, 11 Feb 2019, DK7FC wrote:
>>
>>> Hello Riccardo,
>>>
>>> I like the precision of your RX frequency. I should add a few nulls to
>> my
>>> file too :-)
>>> Good work regarding Joe's reception!
>>>
>>> 73, Stefan
>>>
>>> Am 11.02.2019 12:56, schrieb Riccardo Zoli:
>>>>
>>>> Joe, LF
>>>>
>>>> Very strong signal last night continuously from 2330z to 0530z.
>>>> Best decode at 0300z, info attached.
>>>> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
>>>> inserted) and SDR.
>>>>
>>>> All the best,
>>>>
>>>> 73 de Riccardo IW4DXW
>>>>
>>>> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca
>>>> <mailto:jcraig@mun.ca>> ha scritto:
>>>>
>>>>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
>>>>     autodetector.
>>>>     73
>>>>     Joe
>>>>
>>>>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
>>>>
>>>>    > Dominico,
>>>>    >
>>>>    > Thanks to you and Markus and Domenico for the autodecoder service.
>>>>    > I will check the modulator and try again tonight. Some antenna
>> work
>>>>    > is planned as well when the wx improves so there should be some
>> more
>>>>    > dB available soon.
>>>>    >
>>>>    > 73
>>>>    > Joe
>>>>    >
>>>>    > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>>>>    >
>>>>    >> Joe, LF
>>>>    >> in my EbNaut log
>>>>    >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>>>>    >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>>>>    >> there are some decodes of your EbNaut of last nights (QRB=5426
>>>>     km). Seems
>>>>    >> that since yesterday, only carrier is sent on usual qrg 137477
>> Hz.
>>>>    >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
>>>>     parameters:
>>>>    >>
>>>>    >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
>> Duration=1824s
>>>>    >> T_OFFSET=0.0s F_OFFSET=0.000Hz
>>>>    >>
>>>>    >> 73, Domenico IZ7SLZ / JN80nu
>>>>    >>
>>>>    >
>>>>    >
>>>>
>>>
>>
>>
>

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 Content preview:  Hello Genossen LFers! May be may be you interesting NDB monitoring?
    The new programm in help to you! http://www.radioscanner.ru/forum/topic25179-126.html#msg1417487
 Content analysis details:   (-0.7 points, 5.0 required)
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Hello Genossen LFers!

May be may be you interesting NDB monitoring?
The new programm in help to you!

http://www.radioscanner.ru/forum/topic25179-126.html#msg1417487

Excuse - on russian language.
PSE Use a translator.

That programm analyze IQ files from SDR and use an autocorellation method to detect a very low signal NDB!
You can find in forum RX Bolivia and Cape Verde by Karapuz Vadim - he was beta tester - in south EU Russia nr Krasnodar city w/o beverages on LW 40m ant!
The author of that prog - wazzoo from Pskov city. 
Programm called 'Pskov NDB' in that.

-- 
73!
Roman, RW3ADB

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References: <CAC+C6w521S1Z2P59riMk3M3gxZ+Jj5MEwfCPBmA9Z6-CddugtA@mail.gmail.com> <Pine.LNX.4.64.1902071235480.9386@plato.ucs.mun.ca> <Pine.LNX.4.64.1902071306380.9507@plato.ucs.mun.ca> <CANA3B6XJkgxPcktLkrYxNK6nVaTWs6Sp7Yux+-bMfohXfOT_oA@mail.gmail.com> <5C616B8E.6000302@posteo.de> <Pine.LNX.4.64.1902111610030.4511@plato.ucs.mun.ca> <CANA3B6USAhFvdZoL7AcZoKn56nzYfNJPf7dzfE-u7Ca4vkgS2w@mail.gmail.com> <Pine.LNX.4.64.1902131632410.23275@plato.ucs.mun.ca>
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 Content preview:  Hello Joe, Your NEO7M emits 137 kHz directly? How do you tell
    it to do that? Ehm, did i ask you the same question some weeks ago or did
    i just thought that i should ask you. Ebkey, so your'e using a Raspi for
   th [...] 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Hello Joe,

Your NEO7M emits 137 kHz directly? How do you tell it to do that?
Ehm, did i ask you the same question some weeks ago or did i just 
thought that i should ask you.
Ebkey, so your'e using a Raspi for the job? I think so but maybe i 
remember wrong.
Would be interesting to know your rig in detail, the exciter stage.

73, Stefan

PS: Do you know, there are such forums, when you ask a question then 
someone answers "This question has been asked before. Did you run a 
search before?...". Terrible!

Am 13.02.2019 21:15, schrieb jcraig@mun.ca:
> Hi Riccardo, Group.
>
> Thanks for the details of your experiments and the signal reports.
> The set up here is an NEO7M to a Decca (one PA module) to a 100x20m
> RL aerial. Paul's Ebkey.c clocks the XOR. The RL has several dB over
> the monopole. Perhaps running a counterpoise under the top loading 
> wire may yield another dB or 2.  Stefan's and Markus's grabbers are
> very helpful too.
>
> 73
> Joe VO1NA
>
> On Wed, 13 Feb 2019, Riccardo Zoli wrote:
>
>> Joe, Stefan, LF
>>
>> Another night with a strong signal from you, Joe. Thanks again for your
>> transmissions which provides good opportunities for RX equipment 
>> testing.
>> Last night, in particular, I tried to listen your signal with my *SLMS
>> HP-3746A*, equipped with its high stability oscillator (OPT.014). I have
>> got good decodes with *NO GPS* *reference* connected to audio card or
>> instrument; I noticed only a slight phase rotation in a couple of cases.
>> I used my TX inv. "L" antenna (that was tuned this time) and a 6 dB
>> attenuator.
>> You can see here the results:
>>
>> UTC   Eb/N0[dB] Carr.S/N[dB] Mess.
>> 0030 7.1  32.14 *******
>> 0100  8.0  32.20 VO1NA_R
>> 0130 5.2  29.08 *******
>> 0200 4.0  27.95 VO1NA_R
>> 0230 5.7  29.01 *******
>> 0300 3.3  27.79 VO1NA_R
>> 0330 NIL    -              -
>> 0400 9.0  32.46 VO1NA_R
>> 0430 7.3  31.49 *******
>> 0500 6.2  30.55 VO1NA_R
>> 0530 6.1  29.86 *******
>> 0600    -0.3  24.48 VO1NA_R
>>
>>
>> All the best
>>
>>
>> 73 de Riccardo IW4DXW
>>
>>
>>
>> Il giorno lun 11 feb 2019 alle ore 21:05 <jcraig@mun.ca> ha scritto:
>>
>>> Hi Riccardo, Stefan, LF,
>>>
>>> Pleased to get your report of improved signal strength Riccardo.
>>> The R means "Rotated L" so it is in the sky again since yesterday.
>>> Today a cermaic feedthrough was installed on the PVC bucket
>>> that houses the coil. It was cold (-10 C) today but the work had
>>> to be done; there was too much charring and arcing.  All seems OK
>>> now and the TX is on (one Decca module) 2.2A RF
>>>
>>> 73
>>> Joe VO1NA
>>>
>>> On Mon, 11 Feb 2019, DK7FC wrote:
>>>
>>>> Hello Riccardo,
>>>>
>>>> I like the precision of your RX frequency. I should add a few nulls to
>>> my
>>>> file too :-)
>>>> Good work regarding Joe's reception!
>>>>
>>>> 73, Stefan
>>>>
>>>> Am 11.02.2019 12:56, schrieb Riccardo Zoli:
>>>>>
>>>>> Joe, LF
>>>>>
>>>>> Very strong signal last night continuously from 2330z to 0530z.
>>>>> Best decode at 0300z, info attached.
>>>>> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
>>>>> inserted) and SDR.
>>>>>
>>>>> All the best,
>>>>>
>>>>> 73 de Riccardo IW4DXW
>>>>>
>>>>> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca
>>>>> <mailto:jcraig@mun.ca>> ha scritto:
>>>>>
>>>>>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
>>>>>     autodetector.
>>>>>     73
>>>>>     Joe
>>>>>
>>>>>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
>>>>>
>>>>> > Dominico,
>>>>> >
>>>>> > Thanks to you and Markus and Domenico for the autodecoder service.
>>>>> > I will check the modulator and try again tonight. Some antenna
>>> work
>>>>> > is planned as well when the wx improves so there should be some
>>> more
>>>>> > dB available soon.
>>>>> >
>>>>> > 73
>>>>> > Joe
>>>>> >
>>>>> > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>>>>> >
>>>>> >> Joe, LF
>>>>> >> in my EbNaut log
>>>>> >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>>>>> >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>>>>> >> there are some decodes of your EbNaut of last nights (QRB=5426
>>>>>     km). Seems
>>>>> >> that since yesterday, only carrier is sent on usual qrg 137477
>>> Hz.
>>>>> >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
>>>>>     parameters:
>>>>> >>
>>>>> >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
>>> Duration=1824s
>>>>> >> T_OFFSET=0.0s F_OFFSET=0.000Hz
>>>>> >>
>>>>> >> 73, Domenico IZ7SLZ / JN80nu
>>>>> >>
>>>>> >
>>>>> >
>>>>>
>>>>
>>>
>>>
>>
>

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 Content preview:  Hi LF! The good programm Time Corrector from Alexander RN3AUS.
    Correct time on your comp via DCF-39/HGA-22 information. In new version WWV
    at 14996 khz also worked. Specially for field day and w/o internet positions
    needs! 
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Hi LF!

The good programm Time Corrector from Alexander RN3AUS.
Correct time on your comp via DCF-39/HGA-22 information.
In new version WWV at 14996 khz also worked.

Specially for field day and w/o internet positions needs!

http://136.su/index.php/topic,233.msg23262.html#msg23262



-- 
73!
Roman, RW3ADB

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 Content preview:  Hi Dimitris, Am 13.02.2019 00:35, schrieb Dimitrios Tsifakis:
    > > Sadly there are no koalas here, they used to be here but not anymore.
    > Also sadly, Australian trees are not very good for climbing, they are >
    gen [...] 
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Hi Dimitris,

Am 13.02.2019 00:35, schrieb Dimitrios Tsifakis:
>
> Sadly there are no koalas here, they used to be here but not anymore.
> Also sadly, Australian trees are not very good for climbing, they are
> generally rather brittle. Not a problem though, I have developed other
> techniques to get wires up!
>    
The voltages for such ground loop antennas are rather small, another 
advantage over the usual E field TX antennas. You will stay below 500 V, 
of course depending on the pwoer and loss resistance you will get.

> These are dams, people use the water in them for irrigation. The most
> common crop here is grapes for making wine.
>    
Ideal, just perfect. I wonder why you are the first one in Australia 
doing such experiments. I would...., ah you know...

> Hmm, my understanding is that a DC measurement won't be too useful as
> it will suffer from polarisation problems. When you do a DC
> measurement, try to reverse the polarity and let me know what happens
> to the resistance you are measuring compared to the previous polarity.
>    
I know about the effect of an extra voltage drop on the surface of an 
electrode into soil. Thus i recommend to use a larger voltage. Why do 
you expect a different DC resistance when changing the polarity?
I can do that test you suggested but i don't expect a difference. It 
could be interesting to rise the voltage from 0 to say 50V in small 
steps and note the current and then draw a graph. Then you would see the 
nonlinearity. I would expect that it is only visible below 10 V.

> I think the impedance should be measured with AC and in fact at the
> same frequency you are planning to use.
Yes, sure. It is interesting to measure the frequency response of the 
feed point impedance. That tells something about the loop. I didn't do 
it carefully enough so far.

> I will start such a page and once it has enough material in it, I will
> let the mailing list know. Then I will be open to contributions of
> content :-)
>    
Looking forward to that. Pictures are most interesting for many people. 
An important part of such a page. Looking forward to that.

> Just finished making a pair of impedance transformers. I used some
> junk box large (OD=61.5mm, ID=37.5mm, L=12.8mm) ferrite toroids of
> unknown material and I stacked two on each transformer. I then made an
> autotransformer with a total of 52 turns tapped at 15 turns making
> roughly a 4 ohm to 50 ohm transformer (48 ohm to 4 ohm to be pricese).
> I wasn't aiming for 50 ohms it just happened to be the number of turns
> that neatly fitted on the toroids!! A=3.2cm^2 and the calculated Bmax
> for the expected power levels is less than 500 gauss so we are in
> business.
>    
Nice.
I had to learn that 1 Gauss = 1E-4 Tesla. So then you have 50 mT, which 
is not much. I think that you can go 3x higher even.
In some cases, a separate primary and secondary winding is helpful, for 
example to avoid EMC issues, ground loops and so on. Also for safety 
considerations. And especially when the impedance ratio is very high, 
i.e. the currents are very different.

> I then did some tests with the amplifier, I connected the two 50 ohm
> windings back to back and place the amplifier on one end and a 4 ohm
> high wattage resistor at the other end. I was pleased to see that the
> resistor got super hot and the transformers remained cool as a
> cucumber. I was able to get on the resistor more than 100 watts from
> f=3 kHz to 20 kHz, which reduced to 80 watts at 30 kHz. I can live
> with that. The amplifier is nominally 100 W output per channel.
>    
Very well. Cucumber, a word i had to learn. Do you know how to bridge 
the PA to get another 3 dB of output power?

> Fingers crossed now I will get a chance to fire it up on the antenna
> this weekend!
>    
Good luck and fun.

73, Stefan


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Date: Thu, 14 Feb 2019 09:01:06 +0000 (UTC)
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 Content preview:  Paul would be interested in one please advise when you have
    more info. It would have to be sent so can this be done. Many thanks 
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Subject: Re: LF: Surplus audio amplifiers
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------=_Part_801617_2095756103.1550134866461
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Paul would be interested in one please advise when you have more info. It w=
ould have to be sent so can this be done. Many thanks
=20
=20
=20
-----Original Message-----
From: Paul Nicholson <vlf0403@abelian.org>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Sent: Wed, 13 Feb 2019 1:46 pm
Subject: LF: Surplus audio amplifiers


Having a clear out at work.

There are some hefty studio grade audio amplifiers looking
for a new home.

I'm told they are MC^2=C2=A0 model MC1250, rated at (per channel)
1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into
8 ohms.

Weight: about 30kg

I believe there are about 50 of them to be disposed of.

If anyone is interested, they may be available for little more
than the shipping cost (which might be quite high considering
the weight).

Maybe they could be turned to VLF use?

--
Paul Nicholson
--



------=_Part_801617_2095756103.1550134866461
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<font color='black' size='2' face='arial'>P<font size="2">aul would be interested in one please advise when you have more info. It would have to be sent so can this be done. Many thanks<br>
</font>
<div> <br>
</div>

<div> <br>
</div>

<div> <br>
</div>

<div style="font-family:arial,helvetica;font-size:10pt;color:black">-----Original Message-----<br>
From: Paul Nicholson &lt;vlf0403@abelian.org&gt;<br>
To: rsgb_lf_group@blacksheep.org &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Sent: Wed, 13 Feb 2019 1:46 pm<br>
Subject: LF: Surplus audio amplifiers<br>
<br>

<div dir="ltr"><br>
</div>

<div dir="ltr">Having a clear out at work.<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">There are some hefty studio grade audio amplifiers looking<br>
</div>

<div dir="ltr">for a new home.<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">I'm told they are MC^2&nbsp; model MC1250, rated at (per channel)<br>
</div>

<div dir="ltr">1.5kW continuous into 2 ohms, 1.3kW into 4 ohms, 575W into<br>
</div>

<div dir="ltr">8 ohms.<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">Weight: about 30kg<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">I believe there are about 50 of them to be disposed of.<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">If anyone is interested, they may be available for little more<br>
</div>

<div dir="ltr">than the shipping cost (which might be quite high considering<br>
</div>

<div dir="ltr">the weight).<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">Maybe they could be turned to VLF use?<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr">--<br>
</div>

<div dir="ltr">Paul Nicholson<br>
</div>

<div dir="ltr">--<br>
</div>

<div dir="ltr"><br>
</div>

<div dir="ltr"><br>
</div>
</div>
</font>
------=_Part_801617_2095756103.1550134866461--

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From: Daniele Caccia <daniele.caccia74@gmail.com>
Date: Thu, 14 Feb 2019 10:59:01 +0100
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 Content preview:  Hi Joe,LF last night your signal from JN52HX ! Rx: kenwood
    TS 450-S Antenna: Mini Whip I55387FI *Daniele Caccia* 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Hi Joe,LF
last night your signal from  JN52HX !

Rx: kenwood TS 450-S
Antenna: Mini Whip

I55387FI
*Daniele Caccia*





Il giorno mer 13 feb 2019 alle ore 22:34 DK7FC <selberdenken@posteo.de> ha
scritto:

> Hello Joe,
>
> Your NEO7M emits 137 kHz directly? How do you tell it to do that?
> Ehm, did i ask you the same question some weeks ago or did i just
> thought that i should ask you.
> Ebkey, so your'e using a Raspi for the job? I think so but maybe i
> remember wrong.
> Would be interesting to know your rig in detail, the exciter stage.
>
> 73, Stefan
>
> PS: Do you know, there are such forums, when you ask a question then
> someone answers "This question has been asked before. Did you run a
> search before?...". Terrible!
>
> Am 13.02.2019 21:15, schrieb jcraig@mun.ca:
> > Hi Riccardo, Group.
> >
> > Thanks for the details of your experiments and the signal reports.
> > The set up here is an NEO7M to a Decca (one PA module) to a 100x20m
> > RL aerial. Paul's Ebkey.c clocks the XOR. The RL has several dB over
> > the monopole. Perhaps running a counterpoise under the top loading
> > wire may yield another dB or 2.  Stefan's and Markus's grabbers are
> > very helpful too.
> >
> > 73
> > Joe VO1NA
> >
> > On Wed, 13 Feb 2019, Riccardo Zoli wrote:
> >
> >> Joe, Stefan, LF
> >>
> >> Another night with a strong signal from you, Joe. Thanks again for your
> >> transmissions which provides good opportunities for RX equipment
> >> testing.
> >> Last night, in particular, I tried to listen your signal with my *SLMS
> >> HP-3746A*, equipped with its high stability oscillator (OPT.014). I have
> >> got good decodes with *NO GPS* *reference* connected to audio card or
> >> instrument; I noticed only a slight phase rotation in a couple of cases.
> >> I used my TX inv. "L" antenna (that was tuned this time) and a 6 dB
> >> attenuator.
> >> You can see here the results:
> >>
> >> UTC   Eb/N0[dB] Carr.S/N[dB] Mess.
> >> 0030 7.1  32.14 *******
> >> 0100  8.0  32.20 VO1NA_R
> >> 0130 5.2  29.08 *******
> >> 0200 4.0  27.95 VO1NA_R
> >> 0230 5.7  29.01 *******
> >> 0300 3.3  27.79 VO1NA_R
> >> 0330 NIL    -              -
> >> 0400 9.0  32.46 VO1NA_R
> >> 0430 7.3  31.49 *******
> >> 0500 6.2  30.55 VO1NA_R
> >> 0530 6.1  29.86 *******
> >> 0600    -0.3  24.48 VO1NA_R
> >>
> >>
> >> All the best
> >>
> >>
> >> 73 de Riccardo IW4DXW
> >>
> >>
> >>
> >> Il giorno lun 11 feb 2019 alle ore 21:05 <jcraig@mun.ca> ha scritto:
> >>
> >>> Hi Riccardo, Stefan, LF,
> >>>
> >>> Pleased to get your report of improved signal strength Riccardo.
> >>> The R means "Rotated L" so it is in the sky again since yesterday.
> >>> Today a cermaic feedthrough was installed on the PVC bucket
> >>> that houses the coil. It was cold (-10 C) today but the work had
> >>> to be done; there was too much charring and arcing.  All seems OK
> >>> now and the TX is on (one Decca module) 2.2A RF
> >>>
> >>> 73
> >>> Joe VO1NA
> >>>
> >>> On Mon, 11 Feb 2019, DK7FC wrote:
> >>>
> >>>> Hello Riccardo,
> >>>>
> >>>> I like the precision of your RX frequency. I should add a few nulls to
> >>> my
> >>>> file too :-)
> >>>> Good work regarding Joe's reception!
> >>>>
> >>>> 73, Stefan
> >>>>
> >>>> Am 11.02.2019 12:56, schrieb Riccardo Zoli:
> >>>>>
> >>>>> Joe, LF
> >>>>>
> >>>>> Very strong signal last night continuously from 2330z to 0530z.
> >>>>> Best decode at 0300z, info attached.
> >>>>> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
> >>>>> inserted) and SDR.
> >>>>>
> >>>>> All the best,
> >>>>>
> >>>>> 73 de Riccardo IW4DXW
> >>>>>
> >>>>> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca
> >>>>> <mailto:jcraig@mun.ca>> ha scritto:
> >>>>>
> >>>>>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
> >>>>>     autodetector.
> >>>>>     73
> >>>>>     Joe
> >>>>>
> >>>>>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
> >>>>>
> >>>>> > Dominico,
> >>>>> >
> >>>>> > Thanks to you and Markus and Domenico for the autodecoder service.
> >>>>> > I will check the modulator and try again tonight. Some antenna
> >>> work
> >>>>> > is planned as well when the wx improves so there should be some
> >>> more
> >>>>> > dB available soon.
> >>>>> >
> >>>>> > 73
> >>>>> > Joe
> >>>>> >
> >>>>> > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
> >>>>> >
> >>>>> >> Joe, LF
> >>>>> >> in my EbNaut log
> >>>>> >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
> >>>>> >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
> >>>>> >> there are some decodes of your EbNaut of last nights (QRB=5426
> >>>>>     km). Seems
> >>>>> >> that since yesterday, only carrier is sent on usual qrg 137477
> >>> Hz.
> >>>>> >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
> >>>>>     parameters:
> >>>>> >>
> >>>>> >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
> >>> Duration=1824s
> >>>>> >> T_OFFSET=0.0s F_OFFSET=0.000Hz
> >>>>> >>
> >>>>> >> 73, Domenico IZ7SLZ / JN80nu
> >>>>> >>
> >>>>> >
> >>>>> >
> >>>>>
> >>>>
> >>>
> >>>
> >>
> >
>
>

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<div dir=3D"ltr"><div dir=3D"ltr"><div>Hi Joe,LF</div><div>last night your =
signal from=C2=A0 JN52HX !</div><div><br></div><div>Rx: kenwood TS 450-S</d=
iv><div>Antenna: Mini Whip</div><div><br></div>I55387FI<br clear=3D"all"><d=
iv><div dir=3D"ltr" class=3D"m_-8693634499532711970gmail_signature" data-sm=
artmail=3D"gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><di=
v dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div dir=3D"ltr">=
<b style=3D"font-size:14px">Daniele Caccia</b></div><div dir=3D"ltr"><br><d=
iv><font color=3D"#0000ff" face=3D"Verdana"><br></font></div><div><div><div=
><br></div></div></div></div></div></div></div></div></div></div></div></di=
v></div></div></div><br></div><br><div class=3D"gmail_quote"><div dir=3D"lt=
r" class=3D"gmail_attr">Il giorno mer 13 feb 2019 alle ore 22:34 DK7FC &lt;=
<a href=3D"mailto:selberdenken@posteo.de" target=3D"_blank">selberdenken@po=
steo.de</a>&gt; ha scritto:<br></div><blockquote class=3D"gmail_quote" styl=
e=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);paddin=
g-left:1ex">Hello Joe,<br>
<br>
Your NEO7M emits 137 kHz directly? How do you tell it to do that?<br>
Ehm, did i ask you the same question some weeks ago or did i just <br>
thought that i should ask you.<br>
Ebkey, so your&#39;e using a Raspi for the job? I think so but maybe i <br>
remember wrong.<br>
Would be interesting to know your rig in detail, the exciter stage.<br>
<br>
73, Stefan<br>
<br>
PS: Do you know, there are such forums, when you ask a question then <br>
someone answers &quot;This question has been asked before. Did you run a <b=
r>
search before?...&quot;. Terrible!<br>
<br>
Am 13.02.2019 21:15, schrieb <a href=3D"mailto:jcraig@mun.ca" target=3D"_bl=
ank">jcraig@mun.ca</a>:<br>
&gt; Hi Riccardo, Group.<br>
&gt;<br>
&gt; Thanks for the details of your experiments and the signal reports.<br>
&gt; The set up here is an NEO7M to a Decca (one PA module) to a 100x20m<br=
>
&gt; RL aerial. Paul&#39;s Ebkey.c clocks the XOR. The RL has several dB ov=
er<br>
&gt; the monopole. Perhaps running a counterpoise under the top loading <br=
>
&gt; wire may yield another dB or 2.=C2=A0 Stefan&#39;s and Markus&#39;s gr=
abbers are<br>
&gt; very helpful too.<br>
&gt;<br>
&gt; 73<br>
&gt; Joe VO1NA<br>
&gt;<br>
&gt; On Wed, 13 Feb 2019, Riccardo Zoli wrote:<br>
&gt;<br>
&gt;&gt; Joe, Stefan, LF<br>
&gt;&gt;<br>
&gt;&gt; Another night with a strong signal from you, Joe. Thanks again for=
 your<br>
&gt;&gt; transmissions which provides good opportunities for RX equipment <=
br>
&gt;&gt; testing.<br>
&gt;&gt; Last night, in particular, I tried to listen your signal with my *=
SLMS<br>
&gt;&gt; HP-3746A*, equipped with its high stability oscillator (OPT.014). =
I have<br>
&gt;&gt; got good decodes with *NO GPS* *reference* connected to audio card=
 or<br>
&gt;&gt; instrument; I noticed only a slight phase rotation in a couple of =
cases.<br>
&gt;&gt; I used my TX inv. &quot;L&quot; antenna (that was tuned this time)=
 and a 6 dB<br>
&gt;&gt; attenuator.<br>
&gt;&gt; You can see here the results:<br>
&gt;&gt;<br>
&gt;&gt; UTC=C2=A0 =C2=A0Eb/N0[dB] Carr.S/N[dB] Mess.<br>
&gt;&gt; 0030 7.1=C2=A0 32.14 *******<br>
&gt;&gt; 0100=C2=A0 8.0=C2=A0 32.20 VO1NA_R<br>
&gt;&gt; 0130 5.2=C2=A0 29.08 *******<br>
&gt;&gt; 0200 4.0=C2=A0 27.95 VO1NA_R<br>
&gt;&gt; 0230 5.7=C2=A0 29.01 *******<br>
&gt;&gt; 0300 3.3=C2=A0 27.79 VO1NA_R<br>
&gt;&gt; 0330 NIL=C2=A0 =C2=A0 -=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =
=C2=A0 -<br>
&gt;&gt; 0400 9.0=C2=A0 32.46 VO1NA_R<br>
&gt;&gt; 0430 7.3=C2=A0 31.49 *******<br>
&gt;&gt; 0500 6.2=C2=A0 30.55 VO1NA_R<br>
&gt;&gt; 0530 6.1=C2=A0 29.86 *******<br>
&gt;&gt; 0600=C2=A0 =C2=A0 -0.3=C2=A0 24.48 VO1NA_R<br>
&gt;&gt;<br>
&gt;&gt;<br>
&gt;&gt; All the best<br>
&gt;&gt;<br>
&gt;&gt;<br>
&gt;&gt; 73 de Riccardo IW4DXW<br>
&gt;&gt;<br>
&gt;&gt;<br>
&gt;&gt;<br>
&gt;&gt; Il giorno lun 11 feb 2019 alle ore 21:05 &lt;<a href=3D"mailto:jcr=
aig@mun.ca" target=3D"_blank">jcraig@mun.ca</a>&gt; ha scritto:<br>
&gt;&gt;<br>
&gt;&gt;&gt; Hi Riccardo, Stefan, LF,<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt; Pleased to get your report of improved signal strength Riccard=
o.<br>
&gt;&gt;&gt; The R means &quot;Rotated L&quot; so it is in the sky again si=
nce yesterday.<br>
&gt;&gt;&gt; Today a cermaic feedthrough was installed on the PVC bucket<br=
>
&gt;&gt;&gt; that houses the coil. It was cold (-10 C) today but the work h=
ad<br>
&gt;&gt;&gt; to be done; there was too much charring and arcing.=C2=A0 All =
seems OK<br>
&gt;&gt;&gt; now and the TX is on (one Decca module) 2.2A RF<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt; 73<br>
&gt;&gt;&gt; Joe VO1NA<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt; On Mon, 11 Feb 2019, DK7FC wrote:<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt; Hello Riccardo,<br>
&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt; I like the precision of your RX frequency. I should add a =
few nulls to<br>
&gt;&gt;&gt; my<br>
&gt;&gt;&gt;&gt; file too :-)<br>
&gt;&gt;&gt;&gt; Good work regarding Joe&#39;s reception!<br>
&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt; 73, Stefan<br>
&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt; Am 11.02.2019 12:56, schrieb Riccardo Zoli:<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; Joe, LF<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; Very strong signal last night continuously from 2330z =
to 0530z.<br>
&gt;&gt;&gt;&gt;&gt; Best decode at 0300z, info attached.<br>
&gt;&gt;&gt;&gt;&gt; RX setup: inverted &quot;L&quot; TX antenna (slightly =
detuned, 6 dB attenuator<br>
&gt;&gt;&gt;&gt;&gt; inserted) and SDR.<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; All the best,<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; 73 de Riccardo IW4DXW<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; Il giorno gio 7 feb 2019 alle ore 17:44 &lt;<a href=3D=
"mailto:jcraig@mun.ca" target=3D"_blank">jcraig@mun.ca</a><br>
&gt;&gt;&gt;&gt;&gt; &lt;mailto:<a href=3D"mailto:jcraig@mun.ca" target=3D"=
_blank">jcraig@mun.ca</a>&gt;&gt; ha scritto:<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A0Apologies: I misspelt Domenico and =
did not acknowledge Riccardo&#39;s<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A0autodetector.<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A073<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A0Joe<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A0On Thu, 7 Feb 2019, <a href=3D"mail=
to:jcraig@mun.ca" target=3D"_blank">jcraig@mun.ca</a> &lt;mailto:<a href=3D=
"mailto:jcraig@mun.ca" target=3D"_blank">jcraig@mun.ca</a>&gt; wrote:<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt; Dominico,<br>
&gt;&gt;&gt;&gt;&gt; &gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt; Thanks to you and Markus and Domenico for the aut=
odecoder service.<br>
&gt;&gt;&gt;&gt;&gt; &gt; I will check the modulator and try again tonight.=
 Some antenna<br>
&gt;&gt;&gt; work<br>
&gt;&gt;&gt;&gt;&gt; &gt; is planned as well when the wx improves so there =
should be some<br>
&gt;&gt;&gt; more<br>
&gt;&gt;&gt;&gt;&gt; &gt; dB available soon.<br>
&gt;&gt;&gt;&gt;&gt; &gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt; 73<br>
&gt;&gt;&gt;&gt;&gt; &gt; Joe<br>
&gt;&gt;&gt;&gt;&gt; &gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt; On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:<br>
&gt;&gt;&gt;&gt;&gt; &gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; Joe, LF<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; in my EbNaut log<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; *<a href=3D"https://qsl.net/iz7slz/EBNAUT/DEC=
ODED.TXT" rel=3D"noreferrer" target=3D"_blank">https://qsl.net/iz7slz/EBNAU=
T/DECODED.TXT</a><br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; &lt;<a href=3D"https://qsl.net/iz7slz/EBNAUT/=
DECODED.TXT" rel=3D"noreferrer" target=3D"_blank">https://qsl.net/iz7slz/EB=
NAUT/DECODED.TXT</a>&gt;*<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; there are some decodes of your EbNaut of last=
 nights (QRB=3D5426<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A0km). Seems<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; that since yesterday, only carrier is sent on=
 usual qrg 137477<br>
&gt;&gt;&gt; Hz.<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; Autodecoder here is now running, every XX:00 =
and XX:30 on Joe&#39;s<br>
&gt;&gt;&gt;&gt;&gt;=C2=A0 =C2=A0 =C2=A0parameters:<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; 137477.000Hz N=3D7 T=3D3s 8K19A CRC=3D16 list=
=3D2000 sym=3D608<br>
&gt;&gt;&gt; Duration=3D1824s<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; T_OFFSET=3D0.0s F_OFFSET=3D0.000Hz<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt; 73, Domenico IZ7SLZ / JN80nu<br>
&gt;&gt;&gt;&gt;&gt; &gt;&gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt;<br>
&gt;&gt;&gt;&gt;&gt; &gt;<br>
&gt;&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt;<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt;<br>
&gt;&gt;<br>
&gt;<br>
<br>
</blockquote></div></div>

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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Thu, 14 Feb 2019 11:15:05 +0000
Message-ID: <CAA8k23TcM_UMsOWFXX5nRLE65vt7+DepEL-eCURcH=uq-Hoh1Q@mail.gmail.com>
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 Content preview:  I wrote a couple of progs for someone that simply control
   RTS & DTR lines on a COM port, so remoted equipment could be turned on or
   off under PC control SimpleTimer.exe turns on at a specified time, then off
    again at another specified time. and that's it! 
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Subject: LF: Simple COM port on-off
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--000000000000e757a60581d8c5a2
Content-Type: text/plain; charset="UTF-8"

I wrote a couple of progs for someone that simply control RTS & DTR lines
on a COM port, so remoted equipment could be turned on or off under PC
control

SimpleTimer.exe  turns on at a specified time, then off again at another
specified time. and that's it!

ComOnOff.exe toggles the DTR & RTS lines using the + and - kets on the
keyboard.  Just a simple manual on-off.

Nothing complicated - but if you use COM port control for turning a Tx on
or off they may be usefiul.  Both progs can be found in the folder for the
groups.io LF files section
 https://groups.io/g/rsgb-lf-group/files/G4JNT


Andy
www.g4jnt.com


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<div dir=3D"ltr"><div dir=3D"ltr"><div class=3D"gmail_default" style=3D"fon=
t-family:tahoma,sans-serif;font-size:small">I wrote a couple of progs for s=
omeone that simply control RTS &amp; DTR lines on a COM port, so remoted eq=
uipment could be turned on or off under PC control</div><div class=3D"gmail=
_default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br></div=
><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-s=
ize:small">SimpleTimer.exe=C2=A0 turns on at a specified time, then off aga=
in at another specified time. and that&#39;s it!</div><div class=3D"gmail_d=
efault" style=3D"font-family:tahoma,sans-serif;font-size:small"><br></div><=
div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-siz=
e:small">ComOnOff.exe toggles the DTR &amp; RTS lines using the + and - ket=
s on the keyboard.=C2=A0 Just a simple manual on-off.</div><div class=3D"gm=
ail_default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br></=
div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;fon=
t-size:small">Nothing complicated - but if you use COM port control for tur=
ning a Tx on or off they may be usefiul.=C2=A0 Both progs can be found in t=
he folder for the <a href=3D"http://groups.io">groups.io</a> LF files secti=
on</div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small">=C2=A0<a href=3D"https://groups.io/g/rsgb-lf-group/files/=
G4JNT">https://groups.io/g/rsgb-lf-group/files/G4JNT</a></div><div class=3D=
"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br=
></div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;=
font-size:small">=C2=A0</div><div><div dir=3D"ltr" class=3D"gmail_signature=
"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div di=
r=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=3D"font-size:12.8px"><=
a href=3D"http://www.g4jnt.com" target=3D"_blank">www.g4jnt.com</a></span><=
br></div><div><br></div></div></div></div></div></div></div></div></div></d=
iv></div></div></div></div><div id=3D"DAB4FAD8-2DD7-40BB-A1B8-4E2AA1F9FDF2"=
><br>
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nt-family:Arial,Helvetica,sans-serif;line-height:18px">Virus-free. <a href=
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 Content preview:  Hi LF Group, soon I will have to buy a new kitchen and I wonder,
    if an induction cooker is the right choice (regarding QRM!). Does anyone
   have experience with QRM on MF, LF, VLF produced by an induction cooker? Wh
    [...] 
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Subject: LF: Question: QRM from induction cookers?
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Hi LF Group,

soon I will have to buy a new kitchen and I wonder, if an induction
cooker is the right choice (regarding QRM!). Does anyone have experience
with QRM on MF, LF, VLF produced by an induction cooker? Which brands
can be recommended?

I already heard, that there won't be problems on 80m, but what about
lower frequencies?

I'm not yet QRV on MF/LF, but maybe in the future..

Any comments and experiences will be helpful!

73,
de Steffi - dl8nsb


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From: Dexter McIntyre W4DEX <dexter.mc@gmail.com>
Date: Thu, 14 Feb 2019 08:37:58 -0500
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 Content preview:  No noise ever noticed on any frequencies from DC to daylight
    from our 35 years old GE induction cooktop. Some broadband noise can be detected
    within a few feet of the cooktop but seems to have never m [...] 
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Subject: Re: LF: Question: QRM from induction cookers?
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Content-Type: text/plain; charset="UTF-8"

No noise ever noticed on any frequencies from DC to daylight from our 35
years old GE induction cooktop.  Some broadband noise can be detected
within a few feet of the cooktop but seems to have never made it to any
outside antenna.  However GE appliances sure aren't' made like they use to
be.   Just like most well established companies that once had a good
reputation.  Actually GE appliances are now owned by Haier, a Chinese
company.   If our induction cooktop dies before I do I'll sure buy another
of some brand.

Dex

On Thu, Feb 14, 2019 at 8:21 AM Steffi <jota.s@gmx.de> wrote:

> Hi LF Group,
>
> soon I will have to buy a new kitchen and I wonder, if an induction
> cooker is the right choice (regarding QRM!). Does anyone have experience
> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
> can be recommended?
>
> I already heard, that there won't be problems on 80m, but what about
> lower frequencies?
>
> I'm not yet QRV on MF/LF, but maybe in the future..
>
> Any comments and experiences will be helpful!
>
> 73,
> de Steffi - dl8nsb
>
>
>

--000000000000e383b50581dac43a
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-size:small">No =
noise ever noticed on any frequencies from DC to daylight from our 35 years=
 old GE induction cooktop.=C2=A0 Some broadband noise can be detected withi=
n a few feet of the cooktop but seems to have never made it to any outside =
antenna.=C2=A0 However GE appliances sure aren&#39;t&#39; made like they us=
e to be.=C2=A0 =C2=A0Just like most well established companies that once ha=
d a good reputation.=C2=A0 Actually GE appliances are now owned by Haier, a=
 Chinese company.=C2=A0 =C2=A0If our induction cooktop dies before I do I&#=
39;ll sure buy another of some brand.</div><div class=3D"gmail_default" sty=
le=3D"font-size:small"><br></div><div class=3D"gmail_default" style=3D"font=
-size:small">Dex</div></div><br><div class=3D"gmail_quote"><div dir=3D"ltr"=
 class=3D"gmail_attr">On Thu, Feb 14, 2019 at 8:21 AM Steffi &lt;<a href=3D=
"mailto:jota.s@gmx.de">jota.s@gmx.de</a>&gt; wrote:<br></div><blockquote cl=
ass=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid=
 rgb(204,204,204);padding-left:1ex">Hi LF Group,<br>
<br>
soon I will have to buy a new kitchen and I wonder, if an induction<br>
cooker is the right choice (regarding QRM!). Does anyone have experience<br=
>
with QRM on MF, LF, VLF produced by an induction cooker? Which brands<br>
can be recommended?<br>
<br>
I already heard, that there won&#39;t be problems on 80m, but what about<br=
>
lower frequencies?<br>
<br>
I&#39;m not yet QRV on MF/LF, but maybe in the future..<br>
<br>
Any comments and experiences will be helpful!<br>
<br>
73,<br>
de Steffi - dl8nsb<br>
<br>
<br>
</blockquote></div>

--000000000000e383b50581dac43a--

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 Content preview:  I just added induction cooking and new refrigerator and led
    lights with dimmers. My RFI is off the chart. The bosh refrigerator creates
    crazy noise. On road this week but I am planning to flip circuit [...] 
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Subject: Re: LF: Question: QRM from induction cookers?
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From: Gaj Kumar <bsgkumar@gmail.com>
Date: Thu, 14 Feb 2019 20:22:28 +0530
Message-ID: <CANj9hPyCdbuPBO8Ft4OUEOA46Ji7GBiNrRr9AM+X6cr2gpXBKQ@mail.gmail.com>
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 Content preview:  dear Friends The GE's and RCA , Sonys of Yester years had
   EMI filters in their TV.s cookers etc , But nowadays s most of these have
   very neatly trimmed Tinned wires in place of the EMI filters , The s [...]
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Subject: Re: LF: Question: QRM from induction cookers?
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dear Friends
The GE's and RCA , Sonys of Yester years had EMI filters in their TV.s
cookers etc , But nowadays s most of these have very neatly trimmed Tinned
wires in place of the EMI filters , The same is the case with the Chargers
for phones to battery chargers .
solar chargers another wonderful source and have the panels help radiate
very well .
Is there any Inverter , UPS , solar charger which complies with FCC Rule 15
etc .
The ones manufactured by APC , Schneider etc have no filters installed in
the AC inputs or outputs .

it is getting worse each day

Best regards

Kumar
VU2BGS

On Thu, Feb 14, 2019 at 8:16 PM Musser, Elmer (HBO) <Elmer.Musser@hbo.com>
wrote:

> I just added induction cooking and new refrigerator and led lights with
> dimmers. My RFI is off the chart.  The bosh refrigerator creates crazy
> noise.
> On road this week but I am planning to flip circuit breakers and separate
> items one at a time. I have so much noise on 80 meters it=E2=80=99s usele=
ss.  My
> neighbors must have something going bad as well. Very few occasions I hav=
e
> quite(r) nites or hours.  But Saturday afternoon is nuts so adding TVs as
> sources. Newer UHD HDR lcd panels making tons of noise.
>
> I also have salty air living on water. Power line insulators are
> compromised and a little relief after a good rain storm.
>
> Moving to magnetic loop antennas to attempt noise reduction.
>
> Would love to go
> back to candles and wood stove.
>
> Elmer
> Sent from my iPhone
>
> On Feb 14, 2019, at 5:43 AM, Dexter McIntyre W4DEX <dexter.mc@gmail.com>
> wrote:
>
> **External Email received from: owner-rsgb_lf_group@blacksheep.org **
> No noise ever noticed on any frequencies from DC to daylight from our 35
> years old GE induction cooktop.  Some broadband noise can be detected
> within a few feet of the cooktop but seems to have never made it to any
> outside antenna.  However GE appliances sure aren't' made like they use t=
o
> be.   Just like most well established companies that once had a good
> reputation.  Actually GE appliances are now owned by Haier, a Chinese
> company.   If our induction cooktop dies before I do I'll sure buy anothe=
r
> of some brand.
>
> Dex
>
> On Thu, Feb 14, 2019 at 8:21 AM Steffi <jota.s@gmx.de> wrote:
>
>> Hi LF Group,
>>
>> soon I will have to buy a new kitchen and I wonder, if an induction
>> cooker is the right choice (regarding QRM!). Does anyone have experience
>> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
>> can be recommended?
>>
>> I already heard, that there won't be problems on 80m, but what about
>> lower frequencies?
>>
>> I'm not yet QRV on MF/LF, but maybe in the future..
>>
>> Any comments and experiences will be helpful!
>>
>> 73,
>> de Steffi - dl8nsb
>>
>>
>>

--0000000000005e4b800581dbcf5d
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div>dear Friends </div><div>The GE&#39;s and RCA , Sonys =
of Yester years had EMI filters in their TV.s cookers etc , But nowadays s =
most of these have very neatly trimmed Tinned wires in place of the EMI fil=
ters , The same is the case with the Chargers for phones to battery charger=
s . </div><div>solar chargers another wonderful source and have the panels =
help radiate very well .</div><div>Is there any Inverter , UPS , solar char=
ger which complies with FCC Rule 15 etc .</div><div>The ones manufactured b=
y APC , Schneider etc have no filters installed in the AC inputs or outputs=
 .</div><div><br></div><div>it is getting worse each day </div><div><br></d=
iv><div>Best regards </div><div><br></div><div>Kumar</div><div>VU2BGS=C2=A0=
<br></div></div><br><div class=3D"gmail_quote"><div class=3D"gmail_attr" di=
r=3D"ltr">On Thu, Feb 14, 2019 at 8:16 PM Musser, Elmer (HBO) &lt;<a href=
=3D"mailto:Elmer.Musser@hbo.com">Elmer.Musser@hbo.com</a>&gt; wrote:<br></d=
iv><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;padd=
ing-left:1ex;border-left-color:rgb(204,204,204);border-left-width:1px;borde=
r-left-style:solid">



<div dir=3D"auto">
I just added induction cooking and new refrigerator and led lights with dim=
mers. My RFI is off the chart.=C2=A0 The bosh refrigerator creates crazy no=
ise. =C2=A0
<div>On road this week but I am planning to flip circuit breakers and separ=
ate items one at a time. I have so much noise on 80 meters it=E2=80=99s use=
less.=C2=A0 My neighbors must have something going bad as well. Very few oc=
casions I have quite(r) nites or hours.=C2=A0 But
 Saturday afternoon is nuts so adding TVs as sources. Newer UHD HDR lcd pan=
els making tons of noise.=C2=A0<br>
<br>
I also have salty air living on water. Power line insulators are compromise=
d and a little relief after a good rain storm. =C2=A0</div>
<div><br>
</div>
<div>Moving to magnetic loop antennas to attempt noise reduction.=C2=A0</di=
v>
<div><br>
</div>
<div>Would love to go=C2=A0</div>
<div>back to candles and wood stove.=C2=A0</div>
<div><br>
</div>
<div>Elmer<br>
<div id=3D"gmail-m_-612114063999026911AppleMailSignature" dir=3D"ltr">Sent =
from my iPhone</div>
<div dir=3D"ltr"><br>
On Feb 14, 2019, at 5:43 AM, Dexter McIntyre W4DEX &lt;<a href=3D"mailto:de=
xter.mc@gmail.com" target=3D"_blank">dexter.mc@gmail.com</a>&gt; wrote:<br>
<br>
</div>
<blockquote type=3D"cite">
<div dir=3D"ltr">
<div>
<table>
<tbody>
<tr>
<td>**External Email received from: <a href=3D"mailto:owner-rsgb_lf_group@b=
lacksheep.org" target=3D"_blank">
owner-rsgb_lf_group@blacksheep.org</a> **</td>
</tr>
</tbody>
</table>
<br>
</div>
<div dir=3D"ltr">
<div class=3D"gmail_default" style=3D"font-size:small">No noise ever notice=
d on any frequencies from DC to daylight from our 35 years old GE induction=
 cooktop.=C2=A0 Some broadband noise can be detected within a few feet of t=
he cooktop but seems to have never made it
 to any outside antenna.=C2=A0 However GE appliances sure aren&#39;t&#39; m=
ade like they use to be.=C2=A0 =C2=A0Just like most well established compan=
ies that once had a good reputation.=C2=A0 Actually GE appliances are now o=
wned by Haier, a Chinese company.=C2=A0 =C2=A0If our induction cooktop
 dies before I do I&#39;ll sure buy another of some brand.</div>
<div class=3D"gmail_default" style=3D"font-size:small"><br>
</div>
<div class=3D"gmail_default" style=3D"font-size:small">Dex</div>
</div>
<br>
<div class=3D"gmail_quote">
<div class=3D"gmail_attr" dir=3D"ltr">On Thu, Feb 14, 2019 at 8:21 AM Steff=
i &lt;<a href=3D"mailto:jota.s@gmx.de" target=3D"_blank">jota.s@gmx.de</a>&=
gt; wrote:<br>
</div>
<blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;padding=
-left:1ex;border-left-color:rgb(204,204,204);border-left-width:1px;border-l=
eft-style:solid">
Hi LF Group,<br>
<br>
soon I will have to buy a new kitchen and I wonder, if an induction<br>
cooker is the right choice (regarding QRM!). Does anyone have experience<br=
>
with QRM on MF, LF, VLF produced by an induction cooker? Which brands<br>
can be recommended?<br>
<br>
I already heard, that there won&#39;t be problems on 80m, but what about<br=
>
lower frequencies?<br>
<br>
I&#39;m not yet QRV on MF/LF, but maybe in the future..<br>
<br>
Any comments and experiences will be helpful!<br>
<br>
73,<br>
de Steffi - dl8nsb<br>
<br>
<br>
</blockquote>
</div>
</div>
</blockquote>
</div>
</div>

</blockquote></div>

--0000000000005e4b800581dbcf5d--

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From: Gaj Kumar <bsgkumar@gmail.com>
Date: Thu, 14 Feb 2019 20:36:12 +0530
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 Content preview:  On Thu, Feb 14, 2019 at 8:22 PM Gaj Kumar wrote: > dear Friends
    > The GE's and RCA , Sonys of Yester years had EMI filters in their TV.s
   > cookers etc , But nowadays s most of these have very neatly trimmed Tinned
    > wires in place of the EMI filters [...] 
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Subject: Re: LF: Question: QRM from induction cookers?
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On Thu, Feb 14, 2019 at 8:22 PM Gaj Kumar <bsgkumar@gmail.com> wrote:

> dear Friends
> The GE's and RCA , Sonys of Yester years had EMI filters in their TV.s
> cookers etc , But nowadays s most of these have very neatly trimmed Tinne=
d
> wires in place of the EMI filters , The same is the case with the Charger=
s
> for phones to battery chargers .
> solar chargers another wonderful source and have the panels help radiate
> very well .
> Is there any Inverter , UPS , solar charger which complies with FCC Rule
> 15 etc .
> The ones manufactured by APC , Schneider etc have no filters installed in
> the AC inputs or outputs .
>
> it is getting worse each day
>
> Best regards
>
> Kumar
> VU2BGS
>
> On Thu, Feb 14, 2019 at 8:16 PM Musser, Elmer (HBO) <Elmer.Musser@hbo.com=
>
> wrote:
>
>> I just added induction cooking and new refrigerator and led lights with
>> dimmers. My RFI is off the chart.  The bosh refrigerator creates crazy
>> noise.
>> On road this week but I am planning to flip circuit breakers and separat=
e
>> items one at a time. I have so much noise on 80 meters it=E2=80=99s usel=
ess.  My
>> neighbors must have something going bad as well. Very few occasions I ha=
ve
>> quite(r) nites or hours.  But Saturday afternoon is nuts so adding TVs a=
s
>> sources. Newer UHD HDR lcd panels making tons of noise.
>>
>> I also have salty air living on water. Power line insulators are
>> compromised and a little relief after a good rain storm.
>>
>> Moving to magnetic loop antennas to attempt noise reduction.
>>
>> Would love to go
>> back to candles and wood stove.
>>
>> Elmer
>> Sent from my iPhone
>>
>> On Feb 14, 2019, at 5:43 AM, Dexter McIntyre W4DEX <dexter.mc@gmail.com>
>> wrote:
>>
>> **External Email received from: owner-rsgb_lf_group@blacksheep.org **
>> No noise ever noticed on any frequencies from DC to daylight from our 35
>> years old GE induction cooktop.  Some broadband noise can be detected
>> within a few feet of the cooktop but seems to have never made it to any
>> outside antenna.  However GE appliances sure aren't' made like they use =
to
>> be.   Just like most well established companies that once had a good
>> reputation.  Actually GE appliances are now owned by Haier, a Chinese
>> company.   If our induction cooktop dies before I do I'll sure buy anoth=
er
>> of some brand.
>>
>> Dex
>>
>> On Thu, Feb 14, 2019 at 8:21 AM Steffi <jota.s@gmx.de> wrote:
>>
>>> Hi LF Group,
>>>
>>> soon I will have to buy a new kitchen and I wonder, if an induction
>>> cooker is the right choice (regarding QRM!). Does anyone have experienc=
e
>>> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
>>> can be recommended?
>>>
>>> I already heard, that there won't be problems on 80m, but what about
>>> lower frequencies?
>>>
>>> I'm not yet QRV on MF/LF, but maybe in the future..
>>>
>>> Any comments and experiences will be helpful!
>>>
>>> 73,
>>> de Steffi - dl8nsb
>>>
>>>
>>>

--000000000000739b410581dc00ef
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><br></div><br><div class=3D"gmail_quote"><div class=3D"gma=
il_attr" dir=3D"ltr">On Thu, Feb 14, 2019 at 8:22 PM Gaj Kumar &lt;<a href=
=3D"mailto:bsgkumar@gmail.com">bsgkumar@gmail.com</a>&gt; wrote:<br></div><=
blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;padding-=
left:1ex;border-left-color:rgb(204,204,204);border-left-width:1px;border-le=
ft-style:solid"><div dir=3D"ltr"><div>dear Friends </div><div>The GE&#39;s =
and RCA , Sonys of Yester years had EMI filters in their TV.s cookers etc ,=
 But nowadays s most of these have very neatly trimmed Tinned wires in plac=
e of the EMI filters , The same is the case with the Chargers for phones to=
 battery chargers . </div><div>solar chargers another wonderful source and =
have the panels help radiate very well .</div><div>Is there any Inverter , =
UPS , solar charger which complies with FCC Rule 15 etc .</div><div>The one=
s manufactured by APC , Schneider etc have no filters installed in the AC i=
nputs or outputs .</div><div><br></div><div>it is getting worse each day </=
div><div><br></div><div>Best regards </div><div><br></div><div>Kumar</div><=
div>VU2BGS=C2=A0<br></div></div><br><div class=3D"gmail_quote"><div class=
=3D"gmail_attr" dir=3D"ltr">On Thu, Feb 14, 2019 at 8:16 PM Musser, Elmer (=
HBO) &lt;<a href=3D"mailto:Elmer.Musser@hbo.com" target=3D"_blank">Elmer.Mu=
sser@hbo.com</a>&gt; wrote:<br></div><blockquote class=3D"gmail_quote" styl=
e=3D"margin:0px 0px 0px 0.8ex;padding-left:1ex;border-left-color:rgb(204,20=
4,204);border-left-width:1px;border-left-style:solid">



<div dir=3D"auto">
I just added induction cooking and new refrigerator and led lights with dim=
mers. My RFI is off the chart.=C2=A0 The bosh refrigerator creates crazy no=
ise. =C2=A0
<div>On road this week but I am planning to flip circuit breakers and separ=
ate items one at a time. I have so much noise on 80 meters it=E2=80=99s use=
less.=C2=A0 My neighbors must have something going bad as well. Very few oc=
casions I have quite(r) nites or hours.=C2=A0 But
 Saturday afternoon is nuts so adding TVs as sources. Newer UHD HDR lcd pan=
els making tons of noise.=C2=A0<br>
<br>
I also have salty air living on water. Power line insulators are compromise=
d and a little relief after a good rain storm. =C2=A0</div>
<div><br>
</div>
<div>Moving to magnetic loop antennas to attempt noise reduction.=C2=A0</di=
v>
<div><br>
</div>
<div>Would love to go=C2=A0</div>
<div>back to candles and wood stove.=C2=A0</div>
<div><br>
</div>
<div>Elmer<br>
<div id=3D"gmail-m_41187858470325055gmail-m_-612114063999026911AppleMailSig=
nature" dir=3D"ltr">Sent from my iPhone</div>
<div dir=3D"ltr"><br>
On Feb 14, 2019, at 5:43 AM, Dexter McIntyre W4DEX &lt;<a href=3D"mailto:de=
xter.mc@gmail.com" target=3D"_blank">dexter.mc@gmail.com</a>&gt; wrote:<br>
<br>
</div>
<blockquote type=3D"cite">
<div dir=3D"ltr">
<div>
<table>
<tbody>
<tr>
<td>**External Email received from: <a href=3D"mailto:owner-rsgb_lf_group@b=
lacksheep.org" target=3D"_blank">
owner-rsgb_lf_group@blacksheep.org</a> **</td>
</tr>
</tbody>
</table>
<br>
</div>
<div dir=3D"ltr">
<div class=3D"gmail_default" style=3D"font-size:small">No noise ever notice=
d on any frequencies from DC to daylight from our 35 years old GE induction=
 cooktop.=C2=A0 Some broadband noise can be detected within a few feet of t=
he cooktop but seems to have never made it
 to any outside antenna.=C2=A0 However GE appliances sure aren&#39;t&#39; m=
ade like they use to be.=C2=A0 =C2=A0Just like most well established compan=
ies that once had a good reputation.=C2=A0 Actually GE appliances are now o=
wned by Haier, a Chinese company.=C2=A0 =C2=A0If our induction cooktop
 dies before I do I&#39;ll sure buy another of some brand.</div>
<div class=3D"gmail_default" style=3D"font-size:small"><br>
</div>
<div class=3D"gmail_default" style=3D"font-size:small">Dex</div>
</div>
<br>
<div class=3D"gmail_quote">
<div class=3D"gmail_attr" dir=3D"ltr">On Thu, Feb 14, 2019 at 8:21 AM Steff=
i &lt;<a href=3D"mailto:jota.s@gmx.de" target=3D"_blank">jota.s@gmx.de</a>&=
gt; wrote:<br>
</div>
<blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;padding=
-left:1ex;border-left-color:rgb(204,204,204);border-left-width:1px;border-l=
eft-style:solid">
Hi LF Group,<br>
<br>
soon I will have to buy a new kitchen and I wonder, if an induction<br>
cooker is the right choice (regarding QRM!). Does anyone have experience<br=
>
with QRM on MF, LF, VLF produced by an induction cooker? Which brands<br>
can be recommended?<br>
<br>
I already heard, that there won&#39;t be problems on 80m, but what about<br=
>
lower frequencies?<br>
<br>
I&#39;m not yet QRV on MF/LF, but maybe in the future..<br>
<br>
Any comments and experiences will be helpful!<br>
<br>
73,<br>
de Steffi - dl8nsb<br>
<br>
<br>
</blockquote>
</div>
</div>
</blockquote>
</div>
</div>

</blockquote></div>
</blockquote></div>

--000000000000739b410581dc00ef--

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 Content preview:  Hi Daniele, Listener reports have been quite rare. Thank-you
    for making the effort to receive the signals. I am please to report that
   the TX was acvive last night 500 watts 2.6 Amps and so confirm your reception.
    [...] 
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X-Scan-Signature: 87525734ac0bb319fb3f44295fe6963b
Subject: Re: LF: VO1NA Ebnaut recently decodes
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Hi Daniele,

Listener reports have been quite rare.  Thank-you for making the effort
to receive the signals. I am please to report that the TX was acvive last
night 500 watts 2.6 Amps and so confirm your reception. Congrats!

73
Joe VO1NA

On Thu, 14 Feb 2019, Daniele Caccia wrote:
q
> Hi Joe,LF
> last night your signal from  JN52HX !
>
> Rx: kenwood TS 450-S
> Antenna: Mini Whip
>
> I55387FI
> *Daniele Caccia*
>
>
>
>
>
> Il giorno mer 13 feb 2019 alle ore 22:34 DK7FC <selberdenken@posteo.de> ha
> scritto:
>
>> Hello Joe,
>>
>> Your NEO7M emits 137 kHz directly? How do you tell it to do that?
>> Ehm, did i ask you the same question some weeks ago or did i just
>> thought that i should ask you.
>> Ebkey, so your'e using a Raspi for the job? I think so but maybe i
>> remember wrong.
>> Would be interesting to know your rig in detail, the exciter stage.
>>
>> 73, Stefan
>>
>> PS: Do you know, there are such forums, when you ask a question then
>> someone answers "This question has been asked before. Did you run a
>> search before?...". Terrible!
>>
>> Am 13.02.2019 21:15, schrieb jcraig@mun.ca:
>>> Hi Riccardo, Group.
>>>
>>> Thanks for the details of your experiments and the signal reports.
>>> The set up here is an NEO7M to a Decca (one PA module) to a 100x20m
>>> RL aerial. Paul's Ebkey.c clocks the XOR. The RL has several dB over
>>> the monopole. Perhaps running a counterpoise under the top loading
>>> wire may yield another dB or 2.  Stefan's and Markus's grabbers are
>>> very helpful too.
>>>
>>> 73
>>> Joe VO1NA
>>>
>>> On Wed, 13 Feb 2019, Riccardo Zoli wrote:
>>>
>>>> Joe, Stefan, LF
>>>>
>>>> Another night with a strong signal from you, Joe. Thanks again for your
>>>> transmissions which provides good opportunities for RX equipment
>>>> testing.
>>>> Last night, in particular, I tried to listen your signal with my *SLMS
>>>> HP-3746A*, equipped with its high stability oscillator (OPT.014). I have
>>>> got good decodes with *NO GPS* *reference* connected to audio card or
>>>> instrument; I noticed only a slight phase rotation in a couple of cases.
>>>> I used my TX inv. "L" antenna (that was tuned this time) and a 6 dB
>>>> attenuator.
>>>> You can see here the results:
>>>>
>>>> UTC   Eb/N0[dB] Carr.S/N[dB] Mess.
>>>> 0030 7.1  32.14 *******
>>>> 0100  8.0  32.20 VO1NA_R
>>>> 0130 5.2  29.08 *******
>>>> 0200 4.0  27.95 VO1NA_R
>>>> 0230 5.7  29.01 *******
>>>> 0300 3.3  27.79 VO1NA_R
>>>> 0330 NIL    -              -
>>>> 0400 9.0  32.46 VO1NA_R
>>>> 0430 7.3  31.49 *******
>>>> 0500 6.2  30.55 VO1NA_R
>>>> 0530 6.1  29.86 *******
>>>> 0600    -0.3  24.48 VO1NA_R
>>>>
>>>>
>>>> All the best
>>>>
>>>>
>>>> 73 de Riccardo IW4DXW
>>>>
>>>>
>>>>
>>>> Il giorno lun 11 feb 2019 alle ore 21:05 <jcraig@mun.ca> ha scritto:
>>>>
>>>>> Hi Riccardo, Stefan, LF,
>>>>>
>>>>> Pleased to get your report of improved signal strength Riccardo.
>>>>> The R means "Rotated L" so it is in the sky again since yesterday.
>>>>> Today a cermaic feedthrough was installed on the PVC bucket
>>>>> that houses the coil. It was cold (-10 C) today but the work had
>>>>> to be done; there was too much charring and arcing.  All seems OK
>>>>> now and the TX is on (one Decca module) 2.2A RF
>>>>>
>>>>> 73
>>>>> Joe VO1NA
>>>>>
>>>>> On Mon, 11 Feb 2019, DK7FC wrote:
>>>>>
>>>>>> Hello Riccardo,
>>>>>>
>>>>>> I like the precision of your RX frequency. I should add a few nulls to
>>>>> my
>>>>>> file too :-)
>>>>>> Good work regarding Joe's reception!
>>>>>>
>>>>>> 73, Stefan
>>>>>>
>>>>>> Am 11.02.2019 12:56, schrieb Riccardo Zoli:
>>>>>>>
>>>>>>> Joe, LF
>>>>>>>
>>>>>>> Very strong signal last night continuously from 2330z to 0530z.
>>>>>>> Best decode at 0300z, info attached.
>>>>>>> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
>>>>>>> inserted) and SDR.
>>>>>>>
>>>>>>> All the best,
>>>>>>>
>>>>>>> 73 de Riccardo IW4DXW
>>>>>>>
>>>>>>> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca
>>>>>>> <mailto:jcraig@mun.ca>> ha scritto:
>>>>>>>
>>>>>>>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
>>>>>>>     autodetector.
>>>>>>>     73
>>>>>>>     Joe
>>>>>>>
>>>>>>>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
>>>>>>>
>>>>>>>> Dominico,
>>>>>>>>
>>>>>>>> Thanks to you and Markus and Domenico for the autodecoder service.
>>>>>>>> I will check the modulator and try again tonight. Some antenna
>>>>> work
>>>>>>>> is planned as well when the wx improves so there should be some
>>>>> more
>>>>>>>> dB available soon.
>>>>>>>>
>>>>>>>> 73
>>>>>>>> Joe
>>>>>>>>
>>>>>>>> On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>>>>>>>>
>>>>>>>>> Joe, LF
>>>>>>>>> in my EbNaut log
>>>>>>>>> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>>>>>>>>> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>>>>>>>>> there are some decodes of your EbNaut of last nights (QRB=5426
>>>>>>>     km). Seems
>>>>>>>>> that since yesterday, only carrier is sent on usual qrg 137477
>>>>> Hz.
>>>>>>>>> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
>>>>>>>     parameters:
>>>>>>>>>
>>>>>>>>> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
>>>>> Duration=1824s
>>>>>>>>> T_OFFSET=0.0s F_OFFSET=0.000Hz
>>>>>>>>>
>>>>>>>>> 73, Domenico IZ7SLZ / JN80nu
>>>>>>>>>
>>>>>>>>
>>>>>>>>
>>>>>>>
>>>>>>
>>>>>
>>>>>
>>>>
>>>
>>
>>
>

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 Content preview:  Hi Steffi, Their switching frequency is above the audible
   range but not to far of, to keep the switching losses low. But certainly a
    switched high power source which will have a load of harmonics. Avoid it
   of yo [...] 
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Subject: Re: LF: Question: QRM from induction cookers?
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Hi Steffi,

Their switching frequency is above the audible range but not to far of, 
to keep the switching losses low. But certainly a switched high power 
source which will have a load of harmonics.
Avoid it of you can, especially when you are a radio amateur!
If you qrz.com entry is correct you're living in N�rnberg. I know 
someone else on that reflector who's also living there and he is 
operating a VLF grabber which could then detect when you prepare a 
Schweinebraten. :-)

Another consideration is the life time. In our western throw-away and 
buy new society i would expect that the life time will be less tahn 5 
years maybe. The old models may behave different, because they are old!

And after all, for what do you need it at all? Is there any real 
advantace? I just see it is fancy and you might need to throw away your 
old pots and buy new ones, which is of course recommended.

If you look back in time, have you been unhappy with your old cooker? 
And do you think you will be more happy (not just in the first weeks) 
with the new one?


73, Stefan




Am 14.02.2019 14:18, schrieb Steffi:
> Hi LF Group,
>
> soon I will have to buy a new kitchen and I wonder, if an induction
> cooker is the right choice (regarding QRM!). Does anyone have experience
> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
> can be recommended?
>
> I already heard, that there won't be problems on 80m, but what about
> lower frequencies?
>
> I'm not yet QRV on MF/LF, but maybe in the future..
>
> Any comments and experiences will be helpful!
>
> 73,
> de Steffi - dl8nsb
>
>

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 Content preview:  Please find an article on some tests by the RSGB EMC Committee
    that may be interesting. This is available on https://rsgb.org/main/technical/emc/emc-publications-and-leaflets/
    Alan G3NYK ----- Original Message ----- From: "Steffi" <jota.s@gmx.de> To:
    <rsgb_lf_group@blacksheep.org> Sent: Thursday, February 14, 2019 1:18 PM
   Subject: LF: Question: QRM from induction cookers? 
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Please find  an article on some tests by the RSGB EMC Committee that may be 
interesting. This is available on
https://rsgb.org/main/technical/emc/emc-publications-and-leaflets/

Alan
G3NYK

----- Original Message ----- 
From: "Steffi" <jota.s@gmx.de>
To: <rsgb_lf_group@blacksheep.org>
Sent: Thursday, February 14, 2019 1:18 PM
Subject: LF: Question: QRM from induction cookers?


> Hi LF Group,
>
> soon I will have to buy a new kitchen and I wonder, if an induction
> cooker is the right choice (regarding QRM!). Does anyone have experience
> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
> can be recommended?
>
> I already heard, that there won't be problems on 80m, but what about
> lower frequencies?
>
> I'm not yet QRV on MF/LF, but maybe in the future..
>
> Any comments and experiences will be helpful!
>
> 73,
> de Steffi - dl8nsb
>
> 


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 Content preview:  Greetings Stefan and congrats on your remarkable work on ELF.
    I am still thinking about the guard rail for VLF. It is 10km+ from the shack
    so any operation will have to be mobile and of courss must ha [...] 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Greetings Stefan and congrats on your remarkable work on ELF.
I am still thinking about the guard rail for VLF.  It is 10km+ from the
shack so any operation will have to be mobile and of courss must
have the prior approval of Elmer the Safety Elephant. (hi hi)

EbNaut LF TX: 
The signal is taken from the time pulse output of the NEO7 board
which has a LED and dropping resistor across it. Paul has written
code to control the frequency, duty cycle etc with a Raspi.  Very handy.

This goes directly to a TTL XOR and then a TC4426 driver thence a
class E 100w TX or the Decca.  If you have any questions, I'll be happy
to help.  This system is very simple.

73
Joe VO1NA

On Wed, 13 Feb 2019, DK7FC wrote:

> Hello Joe,
>
> Your NEO7M emits 137 kHz directly? How do you tell it to do that?
> Ehm, did i ask you the same question some weeks ago or did i just thought 
> that i should ask you.
> Ebkey, so your'e using a Raspi for the job? I think so but maybe i remember 
> wrong.
> Would be interesting to know your rig in detail, the exciter stage.
>
> 73, Stefan
>
> PS: Do you know, there are such forums, when you ask a question then someone 
> answers "This question has been asked before. Did you run a search 
> before?...". Terrible!
>
> Am 13.02.2019 21:15, schrieb jcraig@mun.ca:
>> Hi Riccardo, Group.
>> 
>> Thanks for the details of your experiments and the signal reports.
>> The set up here is an NEO7M to a Decca (one PA module) to a 100x20m
>> RL aerial. Paul's Ebkey.c clocks the XOR. The RL has several dB over
>> the monopole. Perhaps running a counterpoise under the top loading wire may 
>> yield another dB or 2.  Stefan's and Markus's grabbers are
>> very helpful too.
>> 
>> 73
>> Joe VO1NA
>> 
>> On Wed, 13 Feb 2019, Riccardo Zoli wrote:
>> 
>>> Joe, Stefan, LF
>>> 
>>> Another night with a strong signal from you, Joe. Thanks again for your
>>> transmissions which provides good opportunities for RX equipment testing.
>>> Last night, in particular, I tried to listen your signal with my *SLMS
>>> HP-3746A*, equipped with its high stability oscillator (OPT.014). I have
>>> got good decodes with *NO GPS* *reference* connected to audio card or
>>> instrument; I noticed only a slight phase rotation in a couple of cases.
>>> I used my TX inv. "L" antenna (that was tuned this time) and a 6 dB
>>> attenuator.
>>> You can see here the results:
>>> 
>>> UTC   Eb/N0[dB] Carr.S/N[dB] Mess.
>>> 0030 7.1  32.14 *******
>>> 0100  8.0  32.20 VO1NA_R
>>> 0130 5.2  29.08 *******
>>> 0200 4.0  27.95 VO1NA_R
>>> 0230 5.7  29.01 *******
>>> 0300 3.3  27.79 VO1NA_R
>>> 0330 NIL    -              -
>>> 0400 9.0  32.46 VO1NA_R
>>> 0430 7.3  31.49 *******
>>> 0500 6.2  30.55 VO1NA_R
>>> 0530 6.1  29.86 *******
>>> 0600    -0.3  24.48 VO1NA_R
>>> 
>>> 
>>> All the best
>>> 
>>> 
>>> 73 de Riccardo IW4DXW
>>> 
>>> 
>>> 
>>> Il giorno lun 11 feb 2019 alle ore 21:05 <jcraig@mun.ca> ha scritto:
>>> 
>>>> Hi Riccardo, Stefan, LF,
>>>> 
>>>> Pleased to get your report of improved signal strength Riccardo.
>>>> The R means "Rotated L" so it is in the sky again since yesterday.
>>>> Today a cermaic feedthrough was installed on the PVC bucket
>>>> that houses the coil. It was cold (-10 C) today but the work had
>>>> to be done; there was too much charring and arcing.  All seems OK
>>>> now and the TX is on (one Decca module) 2.2A RF
>>>> 
>>>> 73
>>>> Joe VO1NA
>>>> 
>>>> On Mon, 11 Feb 2019, DK7FC wrote:
>>>> 
>>>>> Hello Riccardo,
>>>>> 
>>>>> I like the precision of your RX frequency. I should add a few nulls to
>>>> my
>>>>> file too :-)
>>>>> Good work regarding Joe's reception!
>>>>> 
>>>>> 73, Stefan
>>>>> 
>>>>> Am 11.02.2019 12:56, schrieb Riccardo Zoli:
>>>>>> 
>>>>>> Joe, LF
>>>>>> 
>>>>>> Very strong signal last night continuously from 2330z to 0530z.
>>>>>> Best decode at 0300z, info attached.
>>>>>> RX setup: inverted "L" TX antenna (slightly detuned, 6 dB attenuator
>>>>>> inserted) and SDR.
>>>>>> 
>>>>>> All the best,
>>>>>> 
>>>>>> 73 de Riccardo IW4DXW
>>>>>> 
>>>>>> Il giorno gio 7 feb 2019 alle ore 17:44 <jcraig@mun.ca
>>>>>> <mailto:jcraig@mun.ca>> ha scritto:
>>>>>>
>>>>>>     Apologies: I misspelt Domenico and did not acknowledge Riccardo's
>>>>>>     autodetector.
>>>>>>     73
>>>>>>     Joe
>>>>>>
>>>>>>     On Thu, 7 Feb 2019, jcraig@mun.ca <mailto:jcraig@mun.ca> wrote:
>>>>>> 
>>>>>> > Dominico,
>>>>>> >
>>>>>> > Thanks to you and Markus and Domenico for the autodecoder service.
>>>>>> > I will check the modulator and try again tonight. Some antenna
>>>> work
>>>>>> > is planned as well when the wx improves so there should be some
>>>> more
>>>>>> > dB available soon.
>>>>>> >
>>>>>> > 73
>>>>>> > Joe
>>>>>> >
>>>>>> > On Thu, 7 Feb 2019, Domenico IZ7SLZ wrote:
>>>>>> >
>>>>>> >> Joe, LF
>>>>>> >> in my EbNaut log
>>>>>> >> *https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>>>>>> >> <https://qsl.net/iz7slz/EBNAUT/DECODED.TXT>*
>>>>>> >> there are some decodes of your EbNaut of last nights (QRB=5426
>>>>>>     km). Seems
>>>>>> >> that since yesterday, only carrier is sent on usual qrg 137477
>>>> Hz.
>>>>>> >> Autodecoder here is now running, every XX:00 and XX:30 on Joe's
>>>>>>     parameters:
>>>>>> >>
>>>>>> >> 137477.000Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608
>>>> Duration=1824s
>>>>>> >> T_OFFSET=0.0s F_OFFSET=0.000Hz
>>>>>> >>
>>>>>> >> 73, Domenico IZ7SLZ / JN80nu
>>>>>> >>
>>>>>> >
>>>>>> >
>>>>>> 
>>>>> 
>>>> 
>>>> 
>>> 
>> 
>
>

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 Content preview:  Hallo Steffi http://dl3zid.darc.de/grabber/qrm.html nicht
   wirklich heftig, oberhalb 1MHz� nichts mehr 
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Subject: Re: LF: Question: QRM from induction cookers?
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--------------E727BC6D7A8E6D5D810C36FC
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Hallo Steffi

http://dl3zid.darc.de/grabber/qrm.html

nicht wirklich heftig, oberhalb 1MHz� nichts mehr

73�� de Eberhard�� DL3ZID

------------------------------------------------------------------------


Am 14.02.19 um 14:18 schrieb Steffi:
> Hi LF Group,
>
> soon I will have to buy a new kitchen and I wonder, if an induction
> cooker is the right choice (regarding QRM!). Does anyone have experience
> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
> can be recommended?
>
> I already heard, that there won't be problems on 80m, but what about
> lower frequencies?
>
> I'm not yet QRV on MF/LF, but maybe in the future..
>
> Any comments and experiences will be helpful!
>
> 73,
> de Steffi - dl8nsb
>
>
>

--------------E727BC6D7A8E6D5D810C36FC
Content-Type: text/html; charset=iso-8859-15
Content-Transfer-Encoding: 8bit

<html>
  <head>
    <meta http-equiv="Content-Type" content="text/html;
      charset=ISO-8859-15">
  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    <p>Hallo Steffi</p>
    <p><a class="moz-txt-link-freetext" href="http://dl3zid.darc.de/grabber/qrm.html">http://dl3zid.darc.de/grabber/qrm.html</a></p>
    <p>nicht wirklich heftig, oberhalb 1MHz� nichts mehr</p>
    <p>73�� de Eberhard�� DL3ZID</p>
    <hr width="100%" size="2">
    <p><br>
    </p>
    <div class="moz-cite-prefix">Am 14.02.19 um 14:18 schrieb Steffi:<br>
    </div>
    <blockquote type="cite" cite="mid:5C656A8F.70702@gmx.de">Hi LF
      Group,
      <br>
      <br>
      soon I will have to buy a new kitchen and I wonder, if an
      induction
      <br>
      cooker is the right choice (regarding QRM!). Does anyone have
      experience
      <br>
      with QRM on MF, LF, VLF produced by an induction cooker? Which
      brands
      <br>
      can be recommended?
      <br>
      <br>
      I already heard, that there won't be problems on 80m, but what
      about
      <br>
      lower frequencies?
      <br>
      <br>
      I'm not yet QRV on MF/LF, but maybe in the future..
      <br>
      <br>
      Any comments and experiences will be helpful!
      <br>
      <br>
      73,
      <br>
      de Steffi - dl8nsb
      <br>
      <br>
      <br>
      <br>
    </blockquote>
  </body>
</html>

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 Content preview:  Hello Joe, Am 14.02.2019 18:41, schrieb jcraig@mun.ca: > Greetings
    Stefan and congrats on your remarkable work on ELF. Thank you. A 100 character
    message is running since 12 UTC. It will take almost 4 days to pa [...] 
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Hello Joe,

Am 14.02.2019 18:41, schrieb jcraig@mun.ca:
> Greetings Stefan and congrats on your remarkable work on ELF.
Thank you. A 100 character message is running since 12 UTC. It will take 
almost 4 days to pass it over. The longest message (in hours, not in 
characters) ever sent in EbNaut, if i remember correctly :-)
> I am still thinking about the guard rail for VLF.  It is 10km+ from the
> shack so any operation will have to be mobile
Hm maybe you can send me the most accurate locator of your shack, like 
Dimitris did with his house? It would be interesting to see your 
location. Hay, we know each other since almost 10 years now but don't 
know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz at 
night, some years ago.

> EbNaut LF TX: The signal is taken from the time pulse output of the 
> NEO7 board
> which has a LED and dropping resistor across it. Paul has written
> code to control the frequency, duty cycle etc with a Raspi.  Very handy.
Yes, i'm using his tools too. Setting the time pulse works well but 
setting a frequency does not, somehow. Am i making a stupid mistake or 
does it have to do with the serial interface /dev/ttyAMA0 on a Raspi2B 
(unlikely) or is my module missing something. Oh no, i remember i 
successfully set a frequency output with the u-center software.
Need to try Markus' fresh developed tool for Windows, just to check if 
it works.

I would like to use a Raspi and Ebkey (using a XOR gate for the PSK) to 
run an EbNaut message from a Raspi. With just 5 W TX power (the 
classical QRP power level) i could pass a message over to Paul, when 
TXing at night, from a small battery. That would be a great test that 
could be done quite often and i don't need to have my car there and big 
batteries. What a fun!

> This goes directly to a TTL XOR and then a TC4426 driver thence a
> class E 100w TX or the Decca.  If you have any questions, I'll be happy
> to help.  This system is very simple.
Thanks Joe, I'll come back later to you. I'll try again and then pass 
the command lines into this email, just for your confirmation.
73, Stefan

From owner-rsgb_lf_group@blacksheep.org  Thu Feb 14 19:52:50 2019
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 Content preview:  Hello Eberhad, Interesting. BTW there is a QRM source that
    is there since years, almost every night, a drifting signal arround 474.3...474.5
    kHz. I saw it on your grabber as well, so i cannot be local! You can see
   i [...] 
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Hello Eberhad,

Interesting. BTW there is a QRM source that is there since years, almost 
every night, a drifting signal arround 474.3...474.5 kHz. I saw it on 
your grabber as well, so i cannot be local!
You can see it right now, e.g. at 
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html
It is only visible at night, at least here. So it seems to be > 300 km 
distant. If my colours are more or less accurate then it comes from the 
north.

Do you know what it is?

73, Stefan


Am 14.02.2019 18:49, schrieb eberhardvwedelstaedt:
>
> Hallo Steffi
>
> http://dl3zid.darc.de/grabber/qrm.html
>
> nicht wirklich heftig, oberhalb 1MHz  nichts mehr
>
> 73   de Eberhard   DL3ZID
>
> ------------------------------------------------------------------------
>
>
> Am 14.02.19 um 14:18 schrieb Steffi:
>> Hi LF Group,
>>
>> soon I will have to buy a new kitchen and I wonder, if an induction
>> cooker is the right choice (regarding QRM!). Does anyone have experience
>> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
>> can be recommended?
>>
>> I already heard, that there won't be problems on 80m, but what about
>> lower frequencies?
>>
>> I'm not yet QRV on MF/LF, but maybe in the future..
>>
>> Any comments and experiences will be helpful!
>>
>> 73,
>> de Steffi - dl8nsb
>>
>>
>>

--------------050007070606010405020601
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 http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
Hello Eberhad, <br>
<br>
Interesting. BTW there is a QRM source that is there since years,
almost every night, a drifting signal arround 474.3...474.5 kHz. I saw
it on your grabber as well, so i cannot be local!<br>
You can see it right now, e.g. at
<a class="moz-txt-link-freetext" href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html</a><br>
It is only visible at night, at least here. So it seems to be &gt; 300
km distant. If my colours are more or less accurate then it comes from
the north.<br>
<br>
Do you know what it is?<br>
<br>
73, Stefan<br>
<br>
<br>
Am 14.02.2019 18:49, schrieb eberhardvwedelstaedt:
<blockquote cite="mid:a592f294-4393-7ae0-4a35-0fb2c91c9620@mvnet.de"
 type="cite">
  <meta http-equiv="Content-Type"
 content="text/html; charset=ISO-8859-15">
  <p>Hallo Steffi</p>
  <p><a moz-do-not-send="true" class="moz-txt-link-freetext"
 href="http://dl3zid.darc.de/grabber/qrm.html">http://dl3zid.darc.de/grabber/qrm.html</a></p>
  <p>nicht wirklich heftig, oberhalb 1MHz� nichts mehr</p>
  <p>73�� de Eberhard�� DL3ZID</p>
  <hr width="100%" size="2">
  <p><br>
  </p>
  <div class="moz-cite-prefix">Am 14.02.19 um 14:18 schrieb Steffi:<br>
  </div>
  <blockquote type="cite" cite="mid:5C656A8F.70702@gmx.de">Hi LF Group,
    <br>
    <br>
soon I will have to buy a new kitchen and I wonder, if an induction <br>
cooker is the right choice (regarding QRM!). Does anyone have
experience <br>
with QRM on MF, LF, VLF produced by an induction cooker? Which brands <br>
can be recommended? <br>
    <br>
I already heard, that there won't be problems on 80m, but what about <br>
lower frequencies? <br>
    <br>
I'm not yet QRV on MF/LF, but maybe in the future.. <br>
    <br>
Any comments and experiences will be helpful! <br>
    <br>
73, <br>
de Steffi - dl8nsb <br>
    <br>
    <br>
    <br>
  </blockquote>
</blockquote>
</body>
</html>

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Fri, 15 Feb 2019 08:55:35 +1100
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 Content preview:  Hi Stefan, > > Hmm, my understanding is that a DC measurement
    won't be too useful as > > it will suffer from polarisation problems. When
    you do a DC > > measurement, try to reverse the polarity and let me know
   w [...] 
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Subject: Re: R: Re: VLF: in VK?
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Hi Stefan,

> > Hmm, my understanding is that a DC measurement won't be too useful as
> > it will suffer from polarisation problems. When you do a DC
> > measurement, try to reverse the polarity and let me know what happens
> > to the resistance you are measuring compared to the previous polarity.
> >
> I know about the effect of an extra voltage drop on the surface of an
> electrode into soil. Thus i recommend to use a larger voltage. Why do
> you expect a different DC resistance when changing the polarity?
> I can do that test you suggested but i don't expect a difference. It
> could be interesting to rise the voltage from 0 to say 50V in small
> steps and note the current and then draw a graph. Then you would see the
> nonlinearity. I would expect that it is only visible below 10 V.

What I was thinking is the induced polarization phenomenon in
geophysical ground measurements. It has to do with mobilization of
ions near the electrodes in the ground due to the constant electric
field which results in a measurement that changes with time. If the
time constant is low, perhaps that's not a problem but until you
check, you can't be sure. I think it's worth while doing that polarity
change next time you are doing measurement and report back on your
findings. Do that test you suggested, from 0 to 50 volts and then
repeat it using 0 to - 50 volts and plot them on the same chart..

> Very well. Cucumber, a word i had to learn. Do you know how to bridge
> the PA to get another 3 dB of output power?

Yes, it's quite simple however I will need one isolating transformer
as the output is given from the two non-grounded output terminals of
the two channels. That shouldn't be a problem. Alternatively, I can
ensure that no part of the loop is grounded, however that's more
difficult.

73, Dimitris VK2COW

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 Content preview:  What is worse Jim is there is no credible scientific study
    published on whether the work and how. For those with the ''right'' kinf
   of mind it can be an amusing exercise to take this up with the maker [...]
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Subject: LF: Re: QRM - Other
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This is a multi-part message in MIME format.

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What is worse Jim is there is no credible scientific study published on =
whether the work and how. For those with the ''right'' kinf of mind it =
can be an amusing exercise to take this up with the makers. Oh on the =
ones we looked at the chip (filed top) was a 555 or 556 timer. One maker =
quoted a University report. When chased it was not done by a science =
faculty and was never published. It gets boring when the best  =
justification is '' We've sold thousands so it must work''

Alan
G3NYK=20
  ----- Original Message -----=20
  From: hvanesce@comcast.net=20
  To: rsgb_lf_group@blacksheep.org=20
  Sent: Thursday, February 14, 2019 8:50 PM
  Subject: LF: QRM - Other


  =20

  This popular item doesn't seem particularly friendly for ULF-VLF; 40 =
to 76 turns wrapped around the home's water main pipe, ~ 2 amps out, =
sweeping 1 kHz to 20 kHz every 50 milliseconds.

  https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf

  =
https://www.scaleblaster.com/wp-content/uploads/docs/installation-max.pdf=


  which would seem to give roughly 40 fT at 100m at for the specified 70 =
turns on 4 cm water main, not counting eddy currents in the copper pipe.

  Not sure how current varies* with frequency in these devices, or how =
rectangular the current waveform is.

    * (guessing current varies as 1/f, which would mean roughly 30 fT at =
50m at 10 kHz)

  =20

  A commercial unit provides 10A-40A into a 200uH coil around the water =
main (less current into the nominal 1 mH coil):

  =
https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-4000-clm276.pd=
f

  =
https://www.scaleblaster.com/wp-content/uploads/2016/07/Sb1200-SB4000-Ins=
tall-Operations-Manual.pdf

  which would seem to give roughly 10 fT at 1 km for the specified 7 =
turns on 106 cm water main.

  =20

  - Jim AA5BW =20

------=_NextPart_000_001E_01D4C4B6.AC0E7E70
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<BODY lang=3DEN-US link=3Dblue bgColor=3D#ffffff vLink=3Dpurple>
<DIV><FONT size=3D2 face=3DArial>What is worse Jim is there is no =
credible=20
scientific study published on whether the work and how. For those with=20
the&nbsp;''right'' kinf of mind it can be an amusing exercise to take =
this up=20
with the makers. Oh on the ones we looked at the chip (filed top) was a =
555 or=20
556 timer. One maker quoted a University report. When chased it was not =
done by=20
a science faculty and was never published. It gets boring when the best=20
&nbsp;justification is '' We've sold thousands so&nbsp;it must=20
work''</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>Alan</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial>G3NYK</FONT>&nbsp;</DIV>
<BLOCKQUOTE=20
style=3D"BORDER-LEFT: #000000 2px solid; PADDING-LEFT: 5px; =
PADDING-RIGHT: 0px; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px"=20
dir=3Dltr>
  <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV=20
  style=3D"FONT: 10pt arial; BACKGROUND: #e4e4e4; font-color: =
black"><B>From:</B>=20
  <A title=3Dhvanesce@comcast.net=20
  href=3D"mailto:hvanesce@comcast.net">hvanesce@comcast.net</A> </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A =
title=3Drsgb_lf_group@blacksheep.org=20
  =
href=3D"mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org=
</A>=20
  </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Thursday, February 14, =
2019 8:50=20
  PM</DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> LF: QRM - Other</DIV>
  <DIV><BR></DIV>
  <DIV class=3DWordSection1>
  <P class=3DMsoNormal><o:p>&nbsp;</o:p></P>
  <P class=3DMsoNormal>This popular item doesn=92t seem particularly =
friendly for=20
  ULF-VLF; 40 to 76 turns wrapped around the home=92s water main pipe, ~ =
2 amps=20
  out, sweeping 1 kHz to 20 kHz every 50 milliseconds.<o:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf=
">https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf</A><o=
:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/docs/installation=
-max.pdf">https://www.scaleblaster.com/wp-content/uploads/docs/installati=
on-max.pdf</A><o:p></o:p></P>
  <P class=3DMsoNormal>which would seem to give roughly 40 fT at 100m at =
for the=20
  specified 70 turns on 4 cm water main, not counting eddy currents in =
the=20
  copper pipe.<o:p></o:p></P>
  <P class=3DMsoNormal>Not sure how current varies* with frequency in =
these=20
  devices, or how rectangular the current waveform is.<o:p></o:p></P>
  <P class=3DMsoNormal>&nbsp; * (guessing current varies as 1/f, which =
would mean=20
  roughly 30 fT at 50m at 10 kHz)<o:p></o:p></P>
  <P class=3DMsoNormal><o:p>&nbsp;</o:p></P>
  <P class=3DMsoNormal>A commercial unit provides 10A-40A into a 200uH =
coil around=20
  the water main (less current into the nominal 1 mH =
coil):<o:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-4000-c=
lm276.pdf">https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-400=
0-clm276.pdf</A><o:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/2016/07/Sb1200-SB=
4000-Install-Operations-Manual.pdf">https://www.scaleblaster.com/wp-conte=
nt/uploads/2016/07/Sb1200-SB4000-Install-Operations-Manual.pdf</A><o:p></=
o:p></P>
  <P class=3DMsoNormal>which would seem to give roughly 10 fT at 1 km =
for the=20
  specified 7 turns on 106 cm water main.<o:p></o:p></P>
  <P class=3DMsoNormal><o:p>&nbsp;</o:p></P>
  <P class=3DMsoNormal>- Jim AA5BW=20
&nbsp;<o:p></o:p></P></DIV></BLOCKQUOTE></BODY></HTML>

------=_NextPart_000_001E_01D4C4B6.AC0E7E70--


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 Content preview:  This popular item doesn't seem particularly friendly for ULF-VLF;
    40 to 76 turns wrapped around the home's water main pipe, ~ 2 amps out, sweeping
    1 kHz to 20 kHz every 50 milliseconds. https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf
 Content analysis details:   (-0.7 points, 5.0 required)
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This popular item doesn't seem particularly friendly for ULF-VLF; 40 to 76
turns wrapped around the home's water main pipe, ~ 2 amps out, sweeping 1
kHz to 20 kHz every 50 milliseconds.

https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf

https://www.scaleblaster.com/wp-content/uploads/docs/installation-max.pdf

which would seem to give roughly 40 fT at 100m at for the specified 70 turns
on 4 cm water main, not counting eddy currents in the copper pipe.

Not sure how current varies* with frequency in these devices, or how
rectangular the current waveform is.

  * (guessing current varies as 1/f, which would mean roughly 30 fT at 50m
at 10 kHz)

 

A commercial unit provides 10A-40A into a 200uH coil around the water main
(less current into the nominal 1 mH coil):

https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-4000-clm276.pdf

https://www.scaleblaster.com/wp-content/uploads/2016/07/Sb1200-SB4000-Instal
l-Operations-Manual.pdf

which would seem to give roughly 10 fT at 1 km for the specified 7 turns on
106 cm water main.

 

- Jim AA5BW  


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vlink=3Dpurple><div class=3DWordSection1><p =
class=3DMsoNormal><o:p>&nbsp;</o:p></p><p class=3DMsoNormal>This popular =
item doesn&#8217;t seem particularly friendly for ULF-VLF; 40 to 76 =
turns wrapped around the home&#8217;s water main pipe, ~ 2 amps out, =
sweeping 1 kHz to 20 kHz every 50 milliseconds.<o:p></o:p></p><p =
class=3DMsoNormal><a =
href=3D"https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf=
">https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf</a><o=
:p></o:p></p><p class=3DMsoNormal><a =
href=3D"https://www.scaleblaster.com/wp-content/uploads/docs/installation=
-max.pdf">https://www.scaleblaster.com/wp-content/uploads/docs/installati=
on-max.pdf</a><o:p></o:p></p><p class=3DMsoNormal>which would seem to =
give roughly 40 fT at 100m at for the specified 70 turns on 4 cm water =
main, not counting eddy currents in the copper pipe.<o:p></o:p></p><p =
class=3DMsoNormal>Not sure how current varies* with frequency in these =
devices, or how rectangular the current waveform is.<o:p></o:p></p><p =
class=3DMsoNormal>&nbsp; * (guessing current varies as 1/f, which would =
mean roughly 30 fT at 50m at 10 kHz)<o:p></o:p></p><p =
class=3DMsoNormal><o:p>&nbsp;</o:p></p><p class=3DMsoNormal>A commercial =
unit provides 10A-40A into a 200uH coil around the water main (less =
current into the nominal 1 mH coil):<o:p></o:p></p><p =
class=3DMsoNormal><a =
href=3D"https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-4000-c=
lm276.pdf">https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-400=
0-clm276.pdf</a><o:p></o:p></p><p class=3DMsoNormal><a =
href=3D"https://www.scaleblaster.com/wp-content/uploads/2016/07/Sb1200-SB=
4000-Install-Operations-Manual.pdf">https://www.scaleblaster.com/wp-conte=
nt/uploads/2016/07/Sb1200-SB4000-Install-Operations-Manual.pdf</a><o:p></=
o:p></p><p class=3DMsoNormal>which would seem to give roughly 10 fT at 1 =
km for the specified 7 turns on 106 cm water main.<o:p></o:p></p><p =
class=3DMsoNormal><o:p>&nbsp;</o:p></p><p class=3DMsoNormal>- Jim AA5BW =
&nbsp;<o:p></o:p></p></div></body></html>
------=_NextPart_000_028A_01D4C47D.0FBAE650--


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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Fri, 15 Feb 2019 11:22:48 +1100
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 Content preview:  Hi Steffi, I would ask the company that sells them for a demonstration
    and I would bring my pocket AM radio with me. These radios are pretty good
    at detecting this type of QRM. THese days I always do the AM pock [...] 
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Subject: Re: LF: Question: QRM from induction cookers?
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Hi Steffi,

I would ask the company that sells them for a demonstration and I
would bring my pocket AM radio with me. These radios are pretty good
at detecting this type of QRM. THese days I always do the AM pocket
radio test before buying any household appliances!

73, Dimitris VK2COW

Στις Παρ, 15 Φεβ 2019 στις 12:21 π.μ., ο/η Steffi <jota.s@gmx.de> έγραψε:
>
> Hi LF Group,
>
> soon I will have to buy a new kitchen and I wonder, if an induction
> cooker is the right choice (regarding QRM!). Does anyone have experience
> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
> can be recommended?
>
> I already heard, that there won't be problems on 80m, but what about
> lower frequencies?
>
> I'm not yet QRV on MF/LF, but maybe in the future..
>
> Any comments and experiences will be helpful!
>
> 73,
> de Steffi - dl8nsb
>
>


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From: Dexter McIntyre W4DEX <dexter.mc@gmail.com>
Date: Thu, 14 Feb 2019 19:46:48 -0500
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 Content preview:  On Thu, Feb 14, 2019 at 11:56 AM DK7FC wrote: > Is there any
    real > advantace? I just see it is fancy and you might need to throw away
    your > old pots and buy new ones, which is of course recommended. > 
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Subject: Re: LF: Question: QRM from induction cookers?
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On Thu, Feb 14, 2019 at 11:56 AM DK7FC <selberdenken@posteo.de> wrote:

> Is there any real
> advantace? I just see it is fancy and you might need to throw away your
> old pots and buy new ones, which is of course recommended.
>

Advantages I consider important:
(1) Safety, greatly reduced chance of starting a fire or being burned by a
flame or hot cooktop.
     No heat generated unless there is a pan on element.  Turns off
automatically when pan removed.
(2) Fast even heat (with proper cookware)
(3) Easy to clean.  The surface actually stays cooler than the pot or pan.

The only disadvantage is selecting the proper cookware.  Porcelain on steel
or cast iron is best.

Dex

>
>

--000000000000dc3e990581e41cb0
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Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div class=3D"gmail_default" style=3D"fon=
t-size:small"><br></div></div><br><div class=3D"gmail_quote"><div dir=3D"lt=
r" class=3D"gmail_attr">On Thu, Feb 14, 2019 at 11:56 AM DK7FC &lt;<a href=
=3D"mailto:selberdenken@posteo.de">selberdenken@posteo.de</a>&gt; wrote:<br=
></div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;=
border-left:1px solid rgb(204,204,204);padding-left:1ex">Is there any real =
<br>
advantace? I just see it is fancy and you might need to throw away your <br=
>
old pots and buy new ones, which is of course recommended.<br></blockquote>=
<div><br></div><div class=3D"gmail_default" style=3D"font-size:small">Advan=
tages I consider important:=C2=A0</div><div class=3D"gmail_default" style=
=3D"font-size:small">(1) Safety, greatly reduced chance of starting a fire =
or being burned by a flame or hot cooktop.</div><div class=3D"gmail_default=
" style=3D"font-size:small">=C2=A0 =C2=A0 =C2=A0No heat generated unless th=
ere is a pan on element.=C2=A0 Turns off automatically when pan removed.=C2=
=A0</div><div class=3D"gmail_default" style=3D"font-size:small">(2) Fast ev=
en heat (with proper cookware)</div><div class=3D"gmail_default" style=3D"f=
ont-size:small">(3) Easy to clean.=C2=A0 The surface actually stays cooler =
than the pot or pan.=C2=A0</div><div class=3D"gmail_default" style=3D"font-=
size:small"><br></div><div class=3D"gmail_default" style=3D"font-size:small=
">The only disadvantage is selecting the proper cookware.=C2=A0 Porcelain o=
n steel or cast iron is best.</div><div class=3D"gmail_default" style=3D"fo=
nt-size:small"><br></div><div class=3D"gmail_default" style=3D"font-size:sm=
all">Dex</div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px=
 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><br>
</blockquote></div></div>

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Fri, 15 Feb 2019 08:55:35 +1100
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 Content preview:  Hi Stefan, > > Hmm, my understanding is that a DC measurement
    won't be too useful as > > it will suffer from polarisation problems. When
    you do a DC > > measurement, try to reverse the polarity and let me know
   w [...] 
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Hi Stefan,

> > Hmm, my understanding is that a DC measurement won't be too useful as
> > it will suffer from polarisation problems. When you do a DC
> > measurement, try to reverse the polarity and let me know what happens
> > to the resistance you are measuring compared to the previous polarity.
> >
> I know about the effect of an extra voltage drop on the surface of an
> electrode into soil. Thus i recommend to use a larger voltage. Why do
> you expect a different DC resistance when changing the polarity?
> I can do that test you suggested but i don't expect a difference. It
> could be interesting to rise the voltage from 0 to say 50V in small
> steps and note the current and then draw a graph. Then you would see the
> nonlinearity. I would expect that it is only visible below 10 V.

What I was thinking is the induced polarization phenomenon in
geophysical ground measurements. It has to do with mobilization of
ions near the electrodes in the ground due to the constant electric
field which results in a measurement that changes with time. If the
time constant is low, perhaps that's not a problem but until you
check, you can't be sure. I think it's worth while doing that polarity
change next time you are doing measurement and report back on your
findings. Do that test you suggested, from 0 to 50 volts and then
repeat it using 0 to - 50 volts and plot them on the same chart..

> Very well. Cucumber, a word i had to learn. Do you know how to bridge
> the PA to get another 3 dB of output power?

Yes, it's quite simple however I will need one isolating transformer
as the output is given from the two non-grounded output terminals of
the two channels. That shouldn't be a problem. Alternatively, I can
ensure that no part of the loop is grounded, however that's more
difficult.

73, Dimitris VK2COW

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 Content preview:  What is worse Jim is there is no credible scientific study
    published on whether the work and how. For those with the ''right'' kinf
   of mind it can be an amusing exercise to take this up with the maker [...]
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Subject: LF: Re: QRM - Other
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What is worse Jim is there is no credible scientific study published on =
whether the work and how. For those with the ''right'' kinf of mind it =
can be an amusing exercise to take this up with the makers. Oh on the =
ones we looked at the chip (filed top) was a 555 or 556 timer. One maker =
quoted a University report. When chased it was not done by a science =
faculty and was never published. It gets boring when the best  =
justification is '' We've sold thousands so it must work''

Alan
G3NYK=20
  ----- Original Message -----=20
  From: hvanesce@comcast.net=20
  To: rsgb_lf_group@blacksheep.org=20
  Sent: Thursday, February 14, 2019 8:50 PM
  Subject: LF: QRM - Other


  =20

  This popular item doesn't seem particularly friendly for ULF-VLF; 40 =
to 76 turns wrapped around the home's water main pipe, ~ 2 amps out, =
sweeping 1 kHz to 20 kHz every 50 milliseconds.

  https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf

  =
https://www.scaleblaster.com/wp-content/uploads/docs/installation-max.pdf=


  which would seem to give roughly 40 fT at 100m at for the specified 70 =
turns on 4 cm water main, not counting eddy currents in the copper pipe.

  Not sure how current varies* with frequency in these devices, or how =
rectangular the current waveform is.

    * (guessing current varies as 1/f, which would mean roughly 30 fT at =
50m at 10 kHz)

  =20

  A commercial unit provides 10A-40A into a 200uH coil around the water =
main (less current into the nominal 1 mH coil):

  =
https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-4000-clm276.pd=
f

  =
https://www.scaleblaster.com/wp-content/uploads/2016/07/Sb1200-SB4000-Ins=
tall-Operations-Manual.pdf

  which would seem to give roughly 10 fT at 1 km for the specified 7 =
turns on 106 cm water main.

  =20

  - Jim AA5BW =20

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<BODY lang=3DEN-US link=3Dblue bgColor=3D#ffffff vLink=3Dpurple>
<DIV><FONT size=3D2 face=3DArial>What is worse Jim is there is no =
credible=20
scientific study published on whether the work and how. For those with=20
the&nbsp;''right'' kinf of mind it can be an amusing exercise to take =
this up=20
with the makers. Oh on the ones we looked at the chip (filed top) was a =
555 or=20
556 timer. One maker quoted a University report. When chased it was not =
done by=20
a science faculty and was never published. It gets boring when the best=20
&nbsp;justification is '' We've sold thousands so&nbsp;it must=20
work''</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT size=3D2 face=3DArial>Alan</FONT></DIV>
<DIV><FONT size=3D2 face=3DArial>G3NYK</FONT>&nbsp;</DIV>
<BLOCKQUOTE=20
style=3D"BORDER-LEFT: #000000 2px solid; PADDING-LEFT: 5px; =
PADDING-RIGHT: 0px; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px"=20
dir=3Dltr>
  <DIV style=3D"FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV=20
  style=3D"FONT: 10pt arial; BACKGROUND: #e4e4e4; font-color: =
black"><B>From:</B>=20
  <A title=3Dhvanesce@comcast.net=20
  href=3D"mailto:hvanesce@comcast.net">hvanesce@comcast.net</A> </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>To:</B> <A =
title=3Drsgb_lf_group@blacksheep.org=20
  =
href=3D"mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org=
</A>=20
  </DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Sent:</B> Thursday, February 14, =
2019 8:50=20
  PM</DIV>
  <DIV style=3D"FONT: 10pt arial"><B>Subject:</B> LF: QRM - Other</DIV>
  <DIV><BR></DIV>
  <DIV class=3DWordSection1>
  <P class=3DMsoNormal><o:p>&nbsp;</o:p></P>
  <P class=3DMsoNormal>This popular item doesn=92t seem particularly =
friendly for=20
  ULF-VLF; 40 to 76 turns wrapped around the home=92s water main pipe, ~ =
2 amps=20
  out, sweeping 1 kHz to 20 kHz every 50 milliseconds.<o:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf=
">https://www.scaleblaster.com/wp-content/uploads/docs/spec-max.pdf</A><o=
:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/docs/installation=
-max.pdf">https://www.scaleblaster.com/wp-content/uploads/docs/installati=
on-max.pdf</A><o:p></o:p></P>
  <P class=3DMsoNormal>which would seem to give roughly 40 fT at 100m at =
for the=20
  specified 70 turns on 4 cm water main, not counting eddy currents in =
the=20
  copper pipe.<o:p></o:p></P>
  <P class=3DMsoNormal>Not sure how current varies* with frequency in =
these=20
  devices, or how rectangular the current waveform is.<o:p></o:p></P>
  <P class=3DMsoNormal>&nbsp; * (guessing current varies as 1/f, which =
would mean=20
  roughly 30 fT at 50m at 10 kHz)<o:p></o:p></P>
  <P class=3DMsoNormal><o:p>&nbsp;</o:p></P>
  <P class=3DMsoNormal>A commercial unit provides 10A-40A into a 200uH =
coil around=20
  the water main (less current into the nominal 1 mH =
coil):<o:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-4000-c=
lm276.pdf">https://www.scaleblaster.com/wp-content/uploads/2016/08/SB-400=
0-clm276.pdf</A><o:p></o:p></P>
  <P class=3DMsoNormal><A=20
  =
href=3D"https://www.scaleblaster.com/wp-content/uploads/2016/07/Sb1200-SB=
4000-Install-Operations-Manual.pdf">https://www.scaleblaster.com/wp-conte=
nt/uploads/2016/07/Sb1200-SB4000-Install-Operations-Manual.pdf</A><o:p></=
o:p></P>
  <P class=3DMsoNormal>which would seem to give roughly 10 fT at 1 km =
for the=20
  specified 7 turns on 106 cm water main.<o:p></o:p></P>
  <P class=3DMsoNormal><o:p>&nbsp;</o:p></P>
  <P class=3DMsoNormal>- Jim AA5BW=20
&nbsp;<o:p></o:p></P></DIV></BLOCKQUOTE></BODY></HTML>

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From owner-rsgb_lf_group@blacksheep.org  Fri Feb 15 06:02:15 2019
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 Content preview:  Hello VLF! The primary coil of the transformer is ready. 10
    turns (diameter 2mm) give 9.62mH which gives about xl=500Ohms at 8.27kHz.
    It is a good idea! 73! Marcin SQ2BXI 
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Subject: RE: R: Re: VLF: in VK?
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Hello VLF!
The primary coil of the transformer is ready. 10 turns (diameter 2mm) =
give 9.62mH which gives about xl=3D500Ohms at 8.27kHz. It is a good =
idea!

73! Marcin SQ2BXI

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org =
<owner-rsgb_lf_group@blacksheep.org> On Behalf Of Marcin
Sent: Monday, February 11, 2019 4:55 PM
To: rsgb_lf_group@blacksheep.org
Subject: RE: R: Re: VLF: in VK?

Hello Stefan!

Today, the ferrite cores B64290L82X830 came to me. I'm building a =
transformer 1:1/1:4/1:9/1:16 and 1/25 on the VLF. I'll check if it works =
soon.
73! Marcin SQ2BXI

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org =
<owner-rsgb_lf_group@blacksheep.org> On Behalf Of DK7FC
Sent: Monday, February 11, 2019 2:50 PM
To: rsgb_lf_group@blacksheep.org
Subject: Re: R: Re: VLF: in VK?

Hi Dimitris, VLF,

Am 11.02.2019 01:07, schrieb Dimitrios Tsifakis:
> I have an idea about impedance transformation and that is to use high=20
> power 70V/100V audio distribution transformers at both ends. I don't=20
> have to go to 50 ohm as I don't use the coaxial cable as a=20
> transmission line (it's only a tiny percentage of the wavelength!), so =

> I could use a 4 ohm to 400 ohm transformer or similar. I think in=20
> general the impedance transformation ratio goes down as the power=20
> rating goes up and we can live with that. THe audio transformer should =

> work fine on the higher frequency but that will have to be tested.
> Perhaps something like this but not at that price!!
>
> https://www.altronics.com.au/p/m1160-300w-100v-line-pa-transformer/
>
> Another option is to get a PA amplifier of suitable power output that=20
> has a 70V or 100V output. You only need one transformer at the antenna =

> end to get down to 4 ohm to reduce losses. I have a 50 W amp with such =

> output but that's not enough power.
>   =20
These high power audio transformers are interesting. I wonder how well =
they work below 1 kHz. But they are to expensive, as you say. You don't =
need them. For any impedance transformation above 1 kHz i use ordinary
N30 ferrite toroids. There may be slightly better core materials but i'm =
getting very good results and they are not expensive and you can find =
them at many distributors (min quantity =3D 1, not =
50000000000000000000000000). Especially at VLF they are well suitable =
and not expensive.
One of my preferred cores is that one:=20
https://www.buerklin.com/en/ring-core-outer--x-inner--x-height--63-x-38-x=
-25-mm-n30/p/84d258
It works easily for a few hundret watts on all VLF frequencies.

Yes you don't need to match the cable impedance but the losses on your =
cable are caused by the current and resistance of the wire and so, if =
you transform from 4 Ohm to 50 Ohm, then your losses drop by 92 %, =
regardless if it is necessary to match the cable impedance.

> I can easily try the ground loop on the 120m long antenna as I do have =

> ground rods at both ends. It would be interesting to compare the=20
> signal strength in both cases. THat's why I am building a network of=20
> VLF stations by giving away the large ferrite rods to interested=20
> amateurs! They can help doing comparisons like this.
>   =20
Yes, sure. Good luck in getting people motivated to build up a permanent =
VLF RX station. It would also be good to have someone building up a =
grabber site or maybe even providing a stream. Your activity can cause a =
world wide motivation for people who are principally interested in VLF =
reception and/or transmission, even if they won't be able to receive you =
from so far away.

> The ground is very rocky and there is almost no soil at the top.
> Typical Australian native vegetation is the only thing that can=20
> survive on it. I have thought about the dipole on the ground and I=20
> have the perfect spot for it which is putting the feed point at the=20
> top of the hill therefore making an inverted-V :-) Only concern with=20
> that is the high voltage at the end of the dipole wires and the=20
> possibility of a bush fire ignition. Definitely a project for winter!
> I have tried to tune my ~120 metre wire to VLF in the past with mixed=20
> results. Worth revisiting this. The wire basically starts at my house=20
> and follows the hill resulting in the top of the wire being maybe 20=20
> metres higher than the bottom.
>   =20
I'm taking part in your experiments by imagining that i would be in your =
position :-) My latest thought is that a few (wooden?) poles of 10m =
height or so would be ideal. One is close to the house, and then two =
more in 100m distance from the house, e.g. here:=20
http://k7fry.com/grid/?qth=3DQF44OX00PV&from=3DQF44OX00LN
The 2x 100m dipole could be connected using a good HF ladder line down =
to the shack.
Aluminium wire is light weight and cheap and the lower conductivity =
could be compensated by using a higher diameter, something like this,
https://www.amazon.de/dp/B004UA7XT2
This antenna would have the advantage that you can use it from MF to DC =
and the kangaroos would not be able to destroy the antenna.
For VLF experiments, the ends of the wire can be grounded, just by =
adding another 100m of wire at the ends and let them slope down, maybe =
with another pole at 4m height.


73, Stefan


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------=_NextPart_000_0019_01D4C4F3.25E88740--


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 Content preview:  Hallo Stefan The drifting signal whith center at� 474,4kHz
    whith sidebands 50Hz ist since 4 or 5 Years permanent 365/7/24. I think it
    is a advertising plant or a neon sign in the geographical triangle hamburg
    kiel cuxhaven. we want to make it more accurate in the spring. 
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Subject: Re: LF: Question: QRM on 630m.
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Hallo Stefan

The drifting signal whith center at� 474,4kHz whith sidebands 50Hz ist 
since 4 or 5 Years permanent 365/7/24.

I think it is a advertising plant or a neon sign in the geographical 
triangle hamburg kiel cuxhaven. we want to make it more accurate in the 
spring.

73�� Eberhard�� DL3ZID

------------------------------------------------------------------------


Am 14.02.19 um 19:48 schrieb DK7FC:
> Hello Eberhad,
>
> Interesting. BTW there is a QRM source that is there since years, 
> almost every night, a drifting signal arround 474.3...474.5 kHz. I saw 
> it on your grabber as well, so i cannot be local!
> You can see it right now, e.g. at 
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html
> It is only visible at night, at least here. So it seems to be > 300 km 
> distant. If my colours are more or less accurate then it comes from 
> the north.
>
> Do you know what it is?
>
> 73, Stefan
>

--------------4397FBB61C98B5CFEF049B42
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Content-Transfer-Encoding: 8bit

<html>
  <head>
    <meta http-equiv="Content-Type" content="text/html;
      charset=ISO-8859-15">
  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    <p>Hallo Stefan</p>
    <p>The drifting signal whith center at� 474,4kHz whith sidebands
      50Hz ist since 4 or 5 Years permanent 365/7/24.</p>
    <p> <span class="tlid-translation translation"><span title="">I
          think it is a advertising plant or a neon sign in the
          geographical triangle hamburg kiel cuxhaven.</span> <span
          title="" class="">we want to make it more accurate in the
          spring.</span></span></p>
    <p><span class="tlid-translation translation"><span title=""
          class="">73�� Eberhard�� DL3ZID</span></span></p>
    <p><span class="tlid-translation translation"><span title=""
          class=""></span></span></p>
    <hr width="100%" size="2">
    <p><span class="tlid-translation translation"><span title=""
          class=""><br>
        </span></span></p>
    <div class="moz-cite-prefix">Am 14.02.19 um 19:48 schrieb DK7FC:<br>
    </div>
    <blockquote type="cite" cite="mid:5C65B7F5.6060608@posteo.de">
      <meta content="text/html; charset=ISO-8859-15"
        http-equiv="Content-Type">
      Hello Eberhad, <br>
      <br>
      Interesting. BTW there is a QRM source that is there since years,
      almost every night, a drifting signal arround 474.3...474.5 kHz. I
      saw
      it on your grabber as well, so i cannot be local!<br>
      You can see it right now, e.g. at
      <a class="moz-txt-link-freetext"
href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html"
        moz-do-not-send="true">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html</a><br>
      It is only visible at night, at least here. So it seems to be &gt;
      300
      km distant. If my colours are more or less accurate then it comes
      from
      the north.<br>
      <br>
      Do you know what it is?<br>
      <br>
      73, Stefan<br>
      <br>
    </blockquote>
  </body>
</html>

--------------4397FBB61C98B5CFEF049B42--

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Date: Fri, 15 Feb 2019 09:09:20 +0100
From: DK7FC <selberdenken@posteo.de>
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References: <5C656A8F.70702@gmx.de> <a592f294-4393-7ae0-4a35-0fb2c91c9620@mvnet.de> <5C65B7F5.6060608@posteo.de> <b68225a3-20a3-2c4f-ff0d-7eb19867a32b@mvnet.de>
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 Content preview:  Hello Eberhard, RR. And who is 'we'? Once you found the source
    you may also find someone living close to it. If the source makes QRM on
   other frequencies too, affecting broadcast reception, then he could tell it
    the [...] 
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Subject: Re: LF: Question: QRM on 630m.
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Hello Eberhard,

RR. And who is 'we'?
Once you found the source you may also find someone living close to it. 
If the source makes QRM on other frequencies too, affecting broadcast 
reception, then he could tell it the BNetzA. Probably they will ignore 
it if you say that it's disturbing the 630m band.
It must be something that is able to radiate a decent power at MF. It is 
barely audible here. So it can't be a compact structure.
Good luck.

73, Stefan



Am 15.02.2019 08:47, schrieb eberhardvwedelstaedt:
>
> Hallo Stefan
>
> The drifting signal whith center at  474,4kHz whith sidebands 50Hz ist 
> since 4 or 5 Years permanent 365/7/24.
>
> I think it is a advertising plant or a neon sign in the geographical 
> triangle hamburg kiel cuxhaven. we want to make it more accurate in 
> the spring.
>
> 73   Eberhard   DL3ZID
>
> ------------------------------------------------------------------------
>
>
> Am 14.02.19 um 19:48 schrieb DK7FC:
>> Hello Eberhad,
>>
>> Interesting. BTW there is a QRM source that is there since years, 
>> almost every night, a drifting signal arround 474.3...474.5 kHz. I 
>> saw it on your grabber as well, so i cannot be local!
>> You can see it right now, e.g. at 
>> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html
>> It is only visible at night, at least here. So it seems to be > 300 
>> km distant. If my colours are more or less accurate then it comes 
>> from the north.
>>
>> Do you know what it is?
>>
>> 73, Stefan
>>

--------------090104070809020807060602
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Hello Eberhard, <br>
<br>
RR. And who is 'we'?<br>
Once you found the source you may also find someone living close to it.
If the source makes QRM on other frequencies too, affecting broadcast
reception, then he could tell it the BNetzA. Probably they will ignore
it if you say that it's disturbing the 630m band.<br>
It must be something that is able to radiate a decent power at MF. It
is barely audible here. So it can't be a compact structure.<br>
Good luck.<br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 15.02.2019 08:47, schrieb eberhardvwedelstaedt:
<blockquote cite="mid:b68225a3-20a3-2c4f-ff0d-7eb19867a32b@mvnet.de"
 type="cite">
  <meta http-equiv="Content-Type"
 content="text/html; charset=ISO-8859-15">
  <p>Hallo Stefan</p>
  <p>The drifting signal whith center at� 474,4kHz whith sidebands 50Hz
ist since 4 or 5 Years permanent 365/7/24.</p>
  <p> <span class="tlid-translation translation"><span title="">I
think it is a advertising plant or a neon sign in the geographical
triangle hamburg kiel cuxhaven.</span> <span title="" class="">we want
to make it more accurate in the spring.</span></span></p>
  <p><span class="tlid-translation translation"><span title="" class="">73��
Eberhard�� DL3ZID</span></span></p>
  <p><span class="tlid-translation translation"><span title="" class=""></span></span></p>
  <hr width="100%" size="2">
  <p><span class="tlid-translation translation"><span title="" class=""><br>
  </span></span></p>
  <div class="moz-cite-prefix">Am 14.02.19 um 19:48 schrieb DK7FC:<br>
  </div>
  <blockquote type="cite" cite="mid:5C65B7F5.6060608@posteo.de">
    <meta content="text/html; charset=ISO-8859-15"
 http-equiv="Content-Type">
Hello Eberhad, <br>
    <br>
Interesting. BTW there is a QRM source that is there since years,
almost every night, a drifting signal arround 474.3...474.5 kHz. I saw
it on your grabber as well, so i cannot be local!<br>
You can see it right now, e.g. at <a class="moz-txt-link-freetext"
 href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html"
 moz-do-not-send="true">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html</a><br>
It is only visible at night, at least here. So it seems to be &gt; 300
km distant. If my colours are more or less accurate then it comes from
the north.<br>
    <br>
Do you know what it is?<br>
    <br>
73, Stefan<br>
    <br>
  </blockquote>
</blockquote>
</body>
</html>

--------------090104070809020807060602--

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 Content preview:  if it's drifting, then it might drift onto an NDB frequency.
    and that would be an aviation hazard. look for local NDB's near this frequency.
    if none is found, then maybe you could say that it might drift to NPR (488kHz,
    Airport at Tomaszow Mazowiecki). if BNetzA needs to have a reason to investigat
    [...] 
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Subject: Re: LF: Question: QRM on 630m.
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if it's drifting, then it might drift onto an NDB  frequency. and that 
would be an aviation hazard.

look for local NDB's near this frequency. if none is found, then maybe you 
could say that it might drift to NPR (488kHz, Airport at Tomaszow 
Mazowiecki). if BNetzA needs to have a reason to investigate, then maybe 
the possibility of interference to a foreign airport might be enough

VY 73

Jacek / SQ5BPF

On Fri, 15 Feb 2019, DK7FC wrote:

> Date: Fri, 15 Feb 2019 09:09:20 +0100
> From: DK7FC <selberdenken@posteo.de>
> Reply-To: rsgb_lf_group@blacksheep.org
> To: rsgb_lf_group@blacksheep.org
> Subject: Re: LF: Question: QRM on 630m.
> 
> Hello Eberhard,
> 
> RR. And who is 'we'?
> Once you found the source you may also find someone living close to it. If the source makes QRM on other frequencies
> too, affecting broadcast reception, then he could tell it the BNetzA. Probably they will ignore it if you say that
> it's disturbing the 630m band.
> It must be something that is able to radiate a decent power at MF. It is barely audible here. So it can't be a
> compact structure.
> Good luck.
> 
> 73, Stefan
> 
> 
> 
> Am 15.02.2019 08:47, schrieb eberhardvwedelstaedt:
>
>       Hallo Stefan
>
>       The drifting signal whith center at� 474,4kHz whith sidebands 50Hz ist since 4 or 5 Years permanent
>       365/7/24.
>
>       I think it is a advertising plant or a neon sign in the geographical triangle hamburg kiel cuxhaven. we
>       want to make it more accurate in the spring.
>
>       73�� Eberhard�� DL3ZID
> 
> ____________________________________________________________________________________________________________________
> 
>
>       Am 14.02.19 um 19:48 schrieb DK7FC:
>       Hello Eberhad,
>
>       Interesting. BTW there is a QRM source that is there since years, almost every night, a drifting
>       signal arround 474.3...474.5 kHz. I saw it on your grabber as well, so i cannot be local!
>       You can see it right now, e.g. at
>       http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_remote_RDF_Grabber.html
>       It is only visible at night, at least here. So it seems to be > 300 km distant. If my colours are
>       more or less accurate then it comes from the north.
>
>       Do you know what it is?
>
>       73, Stefan
> 
> 
>
--17435139-1304601374-1550225463=:22616--

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Message-ID: <C8C8E64CBC3249CB8B317DAEA6B13C8F@malcoHP>
From: "mal hamilton" <g3kevmal@talktalk.net>
To: <rsgb_lf_group@blacksheep.org>
References: <08e69bca-3228-d583-4c30-58c554b39a61@abelian.org> <2110578436.20190213140928@gmail.com> <75410bf7-b442-0db5-6a97-42a0166ff64d@abelian.org>
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 Content preview:  Hi Paul I am interested in one of your amplifiers for LF experiments.
    I will look into collection when available and cover any expense involved
    your end. 73 de MAL/G3KEV/Scarborough 
 Content analysis details:   (-0.0 points, 5.0 required)
  pts rule name              description
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Subject: LF: Re: Surplus audio amplifiers
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Hi Paul
I am interested in one of your amplifiers for LF experiments. I will look 
into collection when available and cover any expense involved your end.
73 de MAL/G3KEV/Scarborough


-----Original Message----- 
From: Paul Nicholson
Sent: Wednesday, February 13, 2019 2:52 PM
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Surplus audio amplifiers


I'll arrange to have some transferred to my place
of work at Stockport - that will secure them from
the scrap man - at least until the next 5S red tagging
exercise!  They can probably be collected from there,
or from Todmorden.

Will report back when available.

--
Paul Nicholson
-- 


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From: Alex R7NT <r7nt.73@gmail.com>
Date: Fri, 15 Feb 2019 13:24:48 +0300
Message-ID: <CAL-VeeO9abeTmMgzeZN42uB82jvmrr=HKLYuNmkqG2SUmgTUVw@mail.gmail.com>
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 Content preview:  David, you are very well made QSY to 137. The propagation
   was very good last night ! Forward to new successes (maybe TA 2way QSOs?)
   #669 QRB=6209,0 2019-02-09 K3RWR -> F5WK EbNaut #670 QRB=5671,6 2019-02-15
    G0MRF -> WA3U WSPR2 
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Subject: LF: G0MRF QSY to 137
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--000000000000f1ad2a0581ec2fdf
Content-Type: text/plain; charset="UTF-8"

David,
you are very well made QSY to 137.
The propagation was very good last night !
Forward to new successes (maybe TA 2way QSOs?)

#669  QRB=6209,0  2019-02-09  K3RWR    -> F5WK   EbNaut

#670  QRB=5671,6  2019-02-15  G0MRF    -> WA3U   WSPR2

#671  QRB=5543,5  2019-02-15  G0MRF    -> KD2OM  WSPR2

#672  QRB=5710,3  2019-02-15  K3RWR    -> 2E0ILY WSPR2

#673  QRB=5879,8  2019-02-15  G0MRF    -> WA3TTS WSPR2

#674  QRB=5816,6  2019-02-15  G0MRF    -> K3RWR  WSPR2

#675  QRB=7065,6  2019-02-15  G0MRF    -> K8RZ   WSPR2

#676  QRB=6242,7  2019-02-15  K3RWR    -> PA0LSB WSPR2

#677  QRB=5706,5  2019-02-15  G0MRF    -> K3MF   WSPR2

73! Alex R7NT  136.73.ru    AWLF *136.73.ru/h_aw <http://136.73.ru/h_aw/>*

--000000000000f1ad2a0581ec2fdf
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=C2=A0-&gt; K8RZ=C2=A0=C2=A0=C2=A0WSPR2</span></p><p class=3D"gmail-MsoNorm=
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rif"><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier =
New&quot;">#677=C2=A0=C2=A0QRB=3D5706,5=C2=A0=C2=A0</span><span lang=3D"EN-=
US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,=
0,204)">2019-02-15=C2=A0 G0MRF=C2=A0=C2=A0=C2=A0=C2=A0-&gt; K3MF=C2=A0=C2=
=A0=C2=A0WSPR2</span></p><div><div class=3D"gmail-m_3934635283863866133gmai=
l_signature_mailru_css_attribute_postfix" dir=3D"ltr"><div dir=3D"ltr"><div=
 dir=3D"ltr"><br>73! Alex R7NT =C2=A0<a href=3D"http://136.73.ru/" target=
=3D"_blank" rel=3D"noopener noreferrer" style=3D"text-decoration-line:none"=
>136.73.ru</a>=C2=A0 =C2=A0 AWLF=C2=A0<font color=3D"#0000ee"><span style=
=3D"font-size:12.8px"><u><a href=3D"http://136.73.ru/h_aw/" target=3D"_blan=
k" rel=3D"noopener noreferrer" style=3D"text-decoration-line:none">136.73.r=
u/h_aw</a></u></span></font></div></div></div></div></div>

--000000000000f1ad2a0581ec2fdf--

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From: eberhardvwedelstaedt <dl3zid-1@mvnet.de>
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Date: Fri, 15 Feb 2019 11:36:04 +0100
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 Content preview:  Hallo Jacek the nearest NDB is SA,� 474,5kHz the drift is�
    +-5Hz 
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Subject: Re: LF: Question: QRM on 630m.
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This is a multi-part message in MIME format.
--------------B50CE171AB704CEA7CEF0366
Content-Type: text/plain; charset=iso-8859-15; format=flowed
Content-Transfer-Encoding: 8bit

Hallo Jacek

the nearest NDB is SA,� 474,5kHz

the drift is� +-5Hz

 �ERP� valued to� 10..30mW

i think,� no hazard

It is not yet time for the BNetzA

73� Eberhard� DL3ZID

------------------------------------------------------------------------


Am 15.02.19 um 11:11 schrieb Jacek Lipkowski:
> if it's drifting, then it might drift onto an NDB� frequency. and that 
> would be an aviation hazard.
>
> look for local NDB's near this frequency. if none is found, then maybe 
> you could say that it might drift to NPR (488kHz, Airport at Tomaszow 
> Mazowiecki). if BNetzA needs to have a reason to investigate, then 
> maybe the possibility of interference to a foreign airport might be 
> enough
>
> VY 73
>
> Jacek / SQ5BPF
>
> On Fri, 15 Feb 2019, DK7FC wrote:
>

--------------B50CE171AB704CEA7CEF0366
Content-Type: text/html; charset=iso-8859-15
Content-Transfer-Encoding: 8bit

<html>
  <head>
    <meta http-equiv="Content-Type" content="text/html;
      charset=ISO-8859-15">
  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    <p>Hallo Jacek</p>
    <p>the nearest NDB is SA,� 474,5kHz� <br>
    </p>
    <p>the drift is� +-5Hz <br>
    </p>
    <p>�ERP� valued to� 10..30mW <br>
    </p>
    <p>i think,� no hazard <br>
    </p>
    <p><span class="tlid-translation translation"><span title=""
          class="">It is not yet time for the BNetzA</span></span></p>
    <p>73� Eberhard� DL3ZID</p>
    <hr width="100%" size="2">
    <p><br>
    </p>
    <div class="moz-cite-prefix">Am 15.02.19 um 11:11 schrieb Jacek
      Lipkowski:<br>
    </div>
    <blockquote type="cite"
      cite="mid:alpine.DEB.2.11.1902151102580.22616@mailn.lipkowski.org">if
      it's drifting, then it might drift onto an NDB� frequency. and
      that would be an aviation hazard.
      <br>
      <br>
      look for local NDB's near this frequency. if none is found, then
      maybe you could say that it might drift to NPR (488kHz, Airport at
      Tomaszow Mazowiecki). if BNetzA needs to have a reason to
      investigate, then maybe the possibility of interference to a
      foreign airport might be enough
      <br>
      <br>
      VY 73
      <br>
      <br>
      Jacek / SQ5BPF
      <br>
      <br>
      On Fri, 15 Feb 2019, DK7FC wrote:
      <br>
      <br>
    </blockquote>
  </body>
</html>

--------------B50CE171AB704CEA7CEF0366--

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From: Paul Nicholson <vlf0403@abelian.org>
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Date: Fri, 15 Feb 2019 17:38:43 +0000
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 Content preview:  Nine responses noted. I'll aim to secure at least a dozen.
    Have to tiptoe carefully through the corporate procedure minefield hoping
    that none of the company bean counters notice what these go for on [...] 
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Nine responses noted.  I'll aim to secure at least
a dozen.   Have to tiptoe carefully through the
corporate procedure minefield hoping that none of
the company bean counters notice what these go for
on Ebay!

Wonder if they can be made to work on LF?  Hard to
say.   Well, if nothing else its a nice big iron
power supply and rack and heat sink, needing only
the right bits of silicon and a coil or two.

--
Paul Nicholson
--

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From: Domenico IZ7SLZ <iz7slz.domenico@gmail.com>
Date: Sat, 16 Feb 2019 11:04:01 +0100
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 Content preview:  Hi Joe, LF Your EbNaut got one error free decode last night
    here in JN80nu using nominal values for time and frequency offsets: 2019-02-16_01:00:00
    137477.00Hz N=7 T=3s 8K19A CRC=16 list=2000 sym=608 Duration=1824s T_OFFSET=0.0s
    F_OFFSET [...] 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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--000000000000598b730582000579
Content-Type: text/plain; charset="UTF-8"

Hi Joe, LF

Your EbNaut got one error free decode last night here in JN80nu using
nominal values for time and frequency offsets:

------------------------------------------------------------------------------------------
2019-02-16_01:00:00 137477.00Hz N=7 T=3s 8K19A CRC=16 list=2000
sym=608 Duration=1824s
T_OFFSET=0.0s F_OFFSET=0.000Hz
initial reference phase -29.6 amplitude 1.424e+01
carrier phase: 1.5 deg
carrier Eb/N0: 22.6 dB
carrier Es/N0: 10.74 dB
carrier S/N: 38.58 dB in 548.2 uHz, 5.96 dB in 1Hz, -28.01 dB in 2.5kHz
found rank 0 ber 0.0000e+00 Eb/N0 71.8 M -3.575119629e+02 ph 1
180,180,180,180 [VO1NA:R]
------------------------------------------------------------------------------------------


Other auto-decodes are logged at
https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
There was a mains outage at the receiving site on Feb 14, so i have missed
unfortunatly LF transmissions of 14 and 15 february. Sorry.

Thank you for the signal Joe. Propagation peak for our path seems to be
around 01.00 UTC.
Maybe be you can be ready for receiving so we can attempt an exchange of
calls/report before the season ends ?

Vy 73 to all, Domenico IZ7SLZ

On Thu, 14 Feb 2019 at 19:44, DK7FC <selberdenken@posteo.de> wrote:

> Hello Joe,
>
> Am 14.02.2019 18:41, schrieb jcraig@mun.ca:
> > Greetings Stefan and congrats on your remarkable work on ELF.
> Thank you. A 100 character message is running since 12 UTC. It will take
> almost 4 days to pass it over. The longest message (in hours, not in
> characters) ever sent in EbNaut, if i remember correctly :-)
> > I am still thinking about the guard rail for VLF.  It is 10km+ from the
> > shack so any operation will have to be mobile
> Hm maybe you can send me the most accurate locator of your shack, like
> Dimitris did with his house? It would be interesting to see your
> location. Hay, we know each other since almost 10 years now but don't
> know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz at
> night, some years ago.
>
> > EbNaut LF TX: The signal is taken from the time pulse output of the
> > NEO7 board
> > which has a LED and dropping resistor across it. Paul has written
> > code to control the frequency, duty cycle etc with a Raspi.  Very handy.
> Yes, i'm using his tools too. Setting the time pulse works well but
> setting a frequency does not, somehow. Am i making a stupid mistake or
> does it have to do with the serial interface /dev/ttyAMA0 on a Raspi2B
> (unlikely) or is my module missing something. Oh no, i remember i
> successfully set a frequency output with the u-center software.
> Need to try Markus' fresh developed tool for Windows, just to check if
> it works.
>
> I would like to use a Raspi and Ebkey (using a XOR gate for the PSK) to
> run an EbNaut message from a Raspi. With just 5 W TX power (the
> classical QRP power level) i could pass a message over to Paul, when
> TXing at night, from a small battery. That would be a great test that
> could be done quite often and i don't need to have my car there and big
> batteries. What a fun!
>
> > This goes directly to a TTL XOR and then a TC4426 driver thence a
> > class E 100w TX or the Decca.  If you have any questions, I'll be happy
> > to help.  This system is very simple.
> Thanks Joe, I'll come back later to you. I'll try again and then pass
> the command lines into this email, just for your confirmation.
> 73, Stefan
>
>

--000000000000598b730582000579
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div>Hi Joe, LF</div><div><br></div><div>=
Your EbNaut got one error free decode last night here in JN80nu using nomin=
al values for time and frequency offsets:<br></div><div><br></div><div>
<pre>----------------------------------------------------------------------=
--------------------
2019-02-16_01:00:00 137477.00Hz N=3D7 T=3D3s 8K19A CRC=3D16 list=3D2000 sym=
=3D608 Duration=3D1824s
T_OFFSET=3D0.0s F_OFFSET=3D0.000Hz
initial reference phase -29.6 amplitude 1.424e+01
carrier phase: 1.5 deg
carrier Eb/N0: 22.6 dB
carrier Es/N0: 10.74 dB
carrier S/N: 38.58 dB in 548.2 uHz, 5.96 dB in 1Hz, -28.01 dB in 2.5kHz
found rank 0 ber 0.0000e+00 Eb/N0 71.8 M -3.575119629e+02 ph 1 180,180,180,=
180 [VO1NA:R]
---------------------------------------------------------------------------=
---------------</pre>

</div><div><br></div><div>Other auto-decodes are logged at <br></div><div><=
/div><div><a href=3D"https://qsl.net/iz7slz/EBNAUT/DECODED.TXT">https://qsl=
.net/iz7slz/EBNAUT/DECODED.TXT</a><br></div><div></div><div>There was a mai=
ns outage at the receiving site on Feb 14, so i have missed unfortunatly LF=
 transmissions of 14 and 15 february. Sorry.<br></div><div><br></div><div>T=
hank you for the signal Joe. Propagation peak for our path seems to be arou=
nd 01.00 UTC. <br></div><div>Maybe be you can be ready for receiving so we =
can attempt an exchange of calls/report before the season ends ?<br></div><=
div><br></div><div>Vy 73 to all, Domenico IZ7SLZ<br></div></div></div><br><=
div class=3D"gmail_quote"><div dir=3D"ltr" class=3D"gmail_attr">On Thu, 14 =
Feb 2019 at 19:44, DK7FC &lt;<a href=3D"mailto:selberdenken@posteo.de">selb=
erdenken@posteo.de</a>&gt; wrote:<br></div><blockquote class=3D"gmail_quote=
" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);=
padding-left:1ex">Hello Joe,<br>
<br>
Am 14.02.2019 18:41, schrieb <a href=3D"mailto:jcraig@mun.ca" target=3D"_bl=
ank">jcraig@mun.ca</a>:<br>
&gt; Greetings Stefan and congrats on your remarkable work on ELF.<br>
Thank you. A 100 character message is running since 12 UTC. It will take <b=
r>
almost 4 days to pass it over. The longest message (in hours, not in <br>
characters) ever sent in EbNaut, if i remember correctly :-)<br>
&gt; I am still thinking about the guard rail for VLF.=C2=A0 It is 10km+ fr=
om the<br>
&gt; shack so any operation will have to be mobile<br>
Hm maybe you can send me the most accurate locator of your shack, like <br>
Dimitris did with his house? It would be interesting to see your <br>
location. Hay, we know each other since almost 10 years now but don&#39;t <=
br>
know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz at <br>
night, some years ago.<br>
<br>
&gt; EbNaut LF TX: The signal is taken from the time pulse output of the <b=
r>
&gt; NEO7 board<br>
&gt; which has a LED and dropping resistor across it. Paul has written<br>
&gt; code to control the frequency, duty cycle etc with a Raspi.=C2=A0 Very=
 handy.<br>
Yes, i&#39;m using his tools too. Setting the time pulse works well but <br=
>
setting a frequency does not, somehow. Am i making a stupid mistake or <br>
does it have to do with the serial interface /dev/ttyAMA0 on a Raspi2B <br>
(unlikely) or is my module missing something. Oh no, i remember i <br>
successfully set a frequency output with the u-center software.<br>
Need to try Markus&#39; fresh developed tool for Windows, just to check if =
<br>
it works.<br>
<br>
I would like to use a Raspi and Ebkey (using a XOR gate for the PSK) to <br=
>
run an EbNaut message from a Raspi. With just 5 W TX power (the <br>
classical QRP power level) i could pass a message over to Paul, when <br>
TXing at night, from a small battery. That would be a great test that <br>
could be done quite often and i don&#39;t need to have my car there and big=
 <br>
batteries. What a fun!<br>
<br>
&gt; This goes directly to a TTL XOR and then a TC4426 driver thence a<br>
&gt; class E 100w TX or the Decca.=C2=A0 If you have any questions, I&#39;l=
l be happy<br>
&gt; to help.=C2=A0 This system is very simple.<br>
Thanks Joe, I&#39;ll come back later to you. I&#39;ll try again and then pa=
ss <br>
the command lines into this email, just for your confirmation.<br>
73, Stefan<br>
<br>
</blockquote></div>

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From: Alex R7NT <r7nt.73@gmail.com>
Date: Sat, 16 Feb 2019 22:52:01 +0300
Message-ID: <CAL-VeePw9yzYCiMpDw7_Wr9NX7EqdNn+t+-1yCw7-0Ga9V75Zw@mail.gmail.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  Dear LF enthusiasts, AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
    * 1. New database records have been added :* #669 QRB=6209,0 2019-02-09 K3RWR
    -> F5WK EbNaut #670 QRB=5671,6 2019-02-15 G0MRF -> WA3U WSPR2 
 Content analysis details:   (0.3 points, 5.0 required)
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Subject: LF: AWLF Updated 2019-02-16
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--0000000000006ae7540582083aa8
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Dear LF enthusiasts,
 AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
* 1. New database records have been added :*

#669  QRB=3D6209,0  2019-02-09  K3RWR    -> F5WK   EbNaut

#670  QRB=3D5671,6  2019-02-15  G0MRF    -> WA3U   WSPR2

#671  QRB=3D5543,5  2019-02-15  G0MRF    -> KD2OM  WSPR2

#672  QRB=3D5710,3  2019-02-15  K3RWR    -> 2E0ILY WSPR2

#673  QRB=3D5879,8  2019-02-15  G0MRF    -> WA3TTS WSPR2

#674  QRB=3D5816,6  2019-02-15  G0MRF    -> K3RWR  WSPR2

#675  QRB=3D7065,6  2019-02-15  G0MRF    -> K8RZ   WSPR2

#676  QRB=3D6242,7  2019-02-15  K3RWR    -> PA0LSB WSPR2

#677  QRB=3D5706,5  2019-02-15  G0MRF    -> K3MF   WSPR2

#678  QRB=3D5339,6  2019-02-16  G0MRF    -> W1VD   WSPR2



*2. Ratings have been updated :*
*W1VD    *AWLF 8 Rating 1 =E2=86=91 AWLF 8 Hall of Fame #6 =E2=86=91 AWLF 9=
 Rating 3
*K3RWR   *AWLF 4 Rating 2 =E2=86=91 AWLF 4 Hall of Fame #14 =E2=86=91 AWLF =
5 Rating 1
        AWLF 1 RX Rating 26 =E2=86=91 14

*2E0ILY  *AWLF 2 Rating 4 =E2=86=91 1
        AWLF 1 RX Rating 119 =E2=86=91 75

*F5WK    *AWLF 2 Rating 9 =E2=86=91 7
        AWLF 2 RX Rating 6 =E2=86=91 3

*K3MF    *AWLF 2 Rating 17 =E2=86=91 12
        AWLF 1 RX Rating 49 =E2=86=91 33

*WA3TTS  *AWLF 1 Rating 28 =E2=86=91 17
        AWLF 1 RX Rating 28 =E2=86=91 18

*KD2OM   *AWLF 1 Rating 32 =E2=86=91 22
        AWLF 1 RX Rating 34 =E2=86=91 22

*WA3U    *AWLF 1 Rating 96 =E2=86=91 69
        AWLF 1 RX Rating 101 =E2=86=91 69

*PA0LSB  *AWLF 1 Rating 131 =E2=86=91 74
        AWLF 1 RX Rating 131 =E2=86=91 73



*3. NEW ONE :*
*G0MRF   *0 =E2=86=91 AWLF 1 Hall of Fame #57 =E2=86=91 AWLF 2 Rating 26
        0 =E2=86=91 AWLF 1 Hall of Fame #33 =E2=86=91 AWLF 2 Rating 13

*K8RZ    *AWLF 1 Rating 96
        AWLF 1 RX Rating 99

*4. Some personal pdf files have been updated in "AWLF Data by Calls":*
*2E0ILY* *AWLF, **AWLF RX**   F5WK* *AWLF RX**   G0MRF* *AWLF TX**   K3MF*
*AWLF, **AWLF RX**   K3RWR* *AWLF, **AWLF RX**,* *AWLF TX**   K8RZ* *AWLF
RX**   KD2OM* *AWLF RX**   PA0LSB* *AWLF RX**   W1VD* *AWLF, **AWLF RX**
  WA3TTS* *AWLF RX**   WA3U* *AWLF RX*


*5. "Best QSOs" have been updated : *sorted in *QRB/Date* , *Chronological
order* , *Mode(Cat)/Date*
*http://136.73.ru/h_qso <http://136.73.ru/h_qso>*     (maybe refresh frame)

73! Alex R7NT  *http://136.73.ru <http://136.73.ru/>*

--0000000000006ae7540582083aa8
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;li=
ne-height:normal;background-image:initial;background-position:initial;backg=
round-size:initial;background-repeat:initial;background-origin:initial;back=
ground-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif">Dear LF e=
nthusiasts,<br>
=C2=A0AWLF=C2=A0</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-=
family:Arial,sans-serif;color:blue"><a href=3D"http://136.73.ru/h_aw" style=
=3D"color:blue">http://136.73.ru/h_aw</a></span></u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:Arial,sans-serif">=C2=A0=C2=A0</span><b><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;"><br>
<u>1. New database records have been added :</u></span></b><u><span lang=3D=
"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif"></span></u></p=
><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal=
;background-image:initial;background-position:initial;background-size:initi=
al;background-repeat:initial;background-origin:initial;background-clip:init=
ial;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" sty=
le=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#669=C2=A0=C2=A0QR=
B=3D6209,0=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fo=
nt-family:&quot;Courier New&quot;;color:rgb(0,102,0)">2019-02-09=C2=A0 K3RW=
R=C2=A0 =C2=A0=C2=A0-&gt; F5WK
=C2=A0=C2=A0EbNaut</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:rgb(23,59,211)"></span></p><p class=3D"=
MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;background-i=
mage:initial;background-position:initial;background-size:initial;background=
-repeat:initial;background-origin:initial;background-clip:initial;font-size=
:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D"font-si=
ze:9pt;font-family:&quot;Courier New&quot;">#670=C2=A0=C2=A0QRB=3D5671,6=C2=
=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&qu=
ot;Courier New&quot;;color:rgb(0,0,204)">2019-02-15=C2=A0 G0MRF=C2=A0=C2=A0=
=C2=A0 -&gt; WA3U=C2=A0 =C2=A0WSPR2</span><span lang=3D"EN-US" style=3D"fon=
t-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(23,59,211)"></span=
></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:no=
rmal;background-image:initial;background-position:initial;background-size:i=
nitial;background-repeat:initial;background-origin:initial;background-clip:=
initial;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US"=
 style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#671=C2=A0=C2=
=A0QRB=3D5543,5=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-15=C2=A0=
 G0MRF=C2=A0=C2=A0=C2=A0 -&gt; KD2OM
=C2=A0WSPR2</span></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001=
pt;line-height:normal;background-image:initial;background-position:initial;=
background-size:initial;background-repeat:initial;background-origin:initial=
;background-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><sp=
an lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot=
;">#672=C2=A0=C2=A0QRB=3D5710,3=C2=A0=C2=A0</span><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,0,204)">=
2019-02-15=C2=A0 K3RWR=C2=A0=C2=A0=C2=A0 -&gt; 2E0ILY=C2=A0WSPR2</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
"></span></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-h=
eight:normal;background-image:initial;background-position:initial;backgroun=
d-size:initial;background-repeat:initial;background-origin:initial;backgrou=
nd-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><span lang=
=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#673=
=C2=A0=C2=A0QRB=3D5879,8=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"fo=
nt-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02=
-15=C2=A0 G0MRF=C2=A0=C2=A0=C2=A0 -&gt; WA3TTS=C2=A0WSPR2</span></p><p clas=
s=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;backgro=
und-image:initial;background-position:initial;background-size:initial;backg=
round-repeat:initial;background-origin:initial;background-clip:initial;font=
-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D"fo=
nt-size:9pt;font-family:&quot;Courier New&quot;">#674=C2=A0=C2=A0QRB=3D5816=
,6=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-famil=
y:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-15=C2=A0 G0MRF=C2=A0=
=C2=A0=C2=A0 -&gt; K3RWR
=C2=A0WSPR2</span></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001=
pt;line-height:normal;background-image:initial;background-position:initial;=
background-size:initial;background-repeat:initial;background-origin:initial=
;background-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><sp=
an lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot=
;">#675=C2=A0=C2=A0QRB=3D7065,6=C2=A0=C2=A0</span><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,0,204)">=
2019-02-15=C2=A0 G0MRF=C2=A0=C2=A0=C2=A0 -&gt; K8RZ=C2=A0 =C2=A0WSPR2</span=
></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:no=
rmal;background-image:initial;background-position:initial;background-size:i=
nitial;background-repeat:initial;background-origin:initial;background-clip:=
initial;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US"=
 style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#676=C2=A0=C2=
=A0QRB=3D6242,7=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-15=C2=A0=
 K3RWR=C2=A0=C2=A0=C2=A0 -&gt; PA0LSB=C2=A0WSPR2</span><span lang=3D"EN-US"=
 style=3D"font-size:9pt;font-family:&quot;Courier New&quot;"></span></p><p =
class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;bac=
kground-image:initial;background-position:initial;background-size:initial;b=
ackground-repeat:initial;background-origin:initial;background-clip:initial;=
font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#677=C2=A0=C2=A0QRB=
=3D5706,5=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-15=C2=A0 G0MRF=
=C2=A0=C2=A0=C2=A0 -&gt; K3MF=C2=A0 =C2=A0WSPR2</span></p><p class=3D"MsoNo=
rmal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;background-image:=
initial;background-position:initial;background-size:initial;background-repe=
at:initial;background-origin:initial;background-clip:initial;font-size:11pt=
;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;">#678=C2=A0=C2=A0QRB=3D5339,6=C2=A0=
=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;=
Courier New&quot;;color:rgb(0,0,204)">2019-02-16=C2=A0 G0MRF=C2=A0=C2=A0=C2=
=A0 -&gt; W1VD=C2=A0 =C2=A0WSPR2</span><span lang=3D"EN-US" style=3D"font-s=
ize:9pt;font-family:&quot;Courier New&quot;"></span></p><p class=3D"MsoNorm=
al" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;background-image:in=
itial;background-position:initial;background-size:initial;background-repeat=
:initial;background-origin:initial;background-clip:initial;font-size:11pt;f=
ont-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D"font-size:9pt;=
font-family:&quot;Courier New&quot;">=C2=A0</span></p><p class=3D"MsoNormal=
" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;background-image:init=
ial;background-position:initial;background-size:initial;background-repeat:i=
nitial;background-origin:initial;background-clip:initial;font-size:11pt;fon=
t-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" style=3D"font-size:=
9pt;font-family:&quot;Courier New&quot;">2.=C2=A0Ratings have been
updated :</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"><br>
<b>W1VD =C2=A0=C2=A0=C2=A0</b>AWLF 8 Rating 1</span><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)=
">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span>=
<span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&q=
uot;;color:black">=C2=A0AWLF 8 Hall
of Fame #6</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&q=
uot;Courier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US"=
 style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;bac=
kground:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-=
size:9pt;font-family:&quot;Courier New&quot;;color:black">=C2=A0AWLF 9 Rati=
ng 3<br>
<b>K3RWR=C2=A0 =C2=A0</b>AWLF 4 Rating 2</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">=
=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;=
Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;;color:black">=C2=A0AWLF 4 Hall
of Fame #14</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;ba=
ckground:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font=
-size:9pt;font-family:&quot;Courier New&quot;;color:black">=C2=A0AWLF 5 Rat=
ing 1<br>
<b>=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0=C2=A0 </b></span><span lang=3D"EN-U=
S" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,1=
02,0)">AWLF 1 RX Rating
26</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A014</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">2=
E0ILY =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fam=
ily:&quot;Courier New&quot;;color:black">AWLF 2 Rating 4</span><span lang=
=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color=
:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=
=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;=
Courier New&quot;;color:black">=C2=A01<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
119</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A075</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">F=
5WK=C2=A0 =C2=A0=C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;;color:black">AWLF 2 Rating 9</span><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size=
:9pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,2=
11)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-famil=
y:&quot;Courier New&quot;;color:black">=C2=A07<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 2 RX Rating
6</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Couri=
er New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;background:r=
gb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;=
font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A03</span></p><=
p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;b=
ackground-image:initial;background-position:initial;background-size:initial=
;background-repeat:initial;background-origin:initial;background-clip:initia=
l;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">K3MF=
=C2=A0 =C2=A0=C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black">AWLF 2 Rating 17</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211=
)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black">=C2=A012<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
49</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A033</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">W=
A3TTS =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fam=
ily:&quot;Courier New&quot;;color:black">AWLF 1 Rating 28</span><span lang=
=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color=
:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=
=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;=
Courier New&quot;;color:black">=C2=A017<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
28</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A018</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">K=
D2OM=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:black">AWLF 1 Rating 32</span><span =
lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;c=
olor:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt=
;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)"=
>=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&q=
uot;Courier New&quot;;color:black">=C2=A022<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
34</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A022</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">W=
A3U=C2=A0=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;;color:black">AWLF 1 Rating 96</span><=
span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&qu=
ot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-siz=
e:9pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,=
211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-fami=
ly:&quot;Courier New&quot;;color:black">=C2=A069<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
101</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A069</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">P=
A0LSB =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fam=
ily:&quot;Courier New&quot;;color:black">AWLF 1 Rating 131</span><span lang=
=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color=
:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=
=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;=
Courier New&quot;;color:black">=C2=A074<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
131</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A073</span><=
/p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:norm=
al;background-image:initial;background-position:initial;background-size:ini=
tial;background-repeat:initial;background-origin:initial;background-clip:in=
itial;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">=
=C2=A0</span></b></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001p=
t;line-height:normal;background-image:initial;background-position:initial;b=
ackground-size:initial;background-repeat:initial;background-origin:initial;=
background-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><b><=
u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New=
&quot;">3.=C2=A0NEW ONE :</span></u></b><span lang=3D"EN-US" style=3D"font-=
size:9pt;font-family:&quot;Courier New&quot;;color:black"><br>
<b>G0MRF=C2=A0 =C2=A0</b>0</span><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">=C2=A0</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
;color:white;background:rgb(23,59,211)">=E2=86=91</span><b><span lang=3D"EN=
-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black=
"> </span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot=
;Courier New&quot;;color:black">AWLF 1 Hall of Fame #57</span><span lang=3D=
"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rg=
b(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=
=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">=C2=A0AWLF 2 Rating 26<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)"> =
0 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span><span =
lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;c=
olor:black">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:rgb(192,0,0)">AWLF 1 Hall of
Fame #33 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&qu=
ot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span=
><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&=
quot;;color:black">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt=
;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">AWLF 2 Rating 13</=
span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Couri=
er New&quot;;color:black"></span></b></p><p class=3D"MsoNormal" style=3D"ma=
rgin:0cm 0cm 12pt;line-height:normal;background-image:initial;background-po=
sition:initial;background-size:initial;background-repeat:initial;background=
-origin:initial;background-clip:initial;font-size:11pt;font-family:Calibri,=
sans-serif"><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;;color:black">K8RZ=C2=A0=C2=A0 =C2=A0</span></b><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;col=
or:black">AWLF 1 Rating 96<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
99</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)"></span></p><p class=3D"MsoNormal" style=
=3D"margin:0cm 0cm 12pt;line-height:normal;background-image:initial;backgro=
und-position:initial;background-size:initial;background-repeat:initial;back=
ground-origin:initial;background-clip:initial;font-size:11pt;font-family:Ca=
libri,sans-serif"><b><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black">4.=C2=A0Some personal pdf files h=
ave been updated in
&quot;AWLF Data by Calls&quot;:</span></u></b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;"><br>
</span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">2E0ILY</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0F5WK</span></b><b><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-fami=
ly:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><sp=
an lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot=
;;color:black"> =C2=A0=C2=A0G0MRF</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:rgb(192,0,0)">AWLF TX</span></i></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =C2=A0=
=C2=A0K3MF</span></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;"> </span></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:black">AWLF,=C2=
=A0</span></i></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-fa=
mily:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><=
span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&qu=
ot;;color:black">=C2=A0=C2=A0 K3RWR</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF RX</span></i></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font=
-family:&quot;Courier New&quot;;color:black">,</span></i></b><b><span lang=
=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color=
:black"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-=
family:&quot;Courier New&quot;;color:rgb(192,0,0)">AWLF TX</span></i></b><b=
><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&=
quot;;color:black"> =C2=A0=C2=A0K8RZ</span></b><b><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><=
span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&qu=
ot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =C2=A0=
=C2=A0KD2OM</span></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;"> </span></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0PA0LSB</span></b><b>=
<span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&q=
uot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-fa=
mily:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><=
span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&qu=
ot;;color:black"> =C2=A0=C2=A0W1VD</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0WA3TTS</span></b><b>=
<span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&q=
uot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-fa=
mily:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><=
span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&qu=
ot;;color:black"> =C2=A0=C2=A0WA3U</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =C2=A0=
=C2=A0</span></b></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;li=
ne-height:normal;background-image:initial;background-position:initial;backg=
round-size:initial;background-repeat:initial;background-origin:initial;back=
ground-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><b><u><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;">5. &quot;Best QSOs&quot; have been updated :<br>
</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">sorted in=C2=A0</span><b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">QRB/=
Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" style=3D"f=
ont-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">Chrono=
logical order</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0=
)">Mode(Cat)/Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:black"><br>
</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,san=
s-serif;color:blue"><a href=3D"http://136.73.ru/h_qso" style=3D"color:blue"=
>http://136.73.ru/h_qso</a></span></u><span lang=3D"EN-US" style=3D"font-si=
ze:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=A0(maybe refr=
esh frame)</span></p><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001p=
t;line-height:normal;background-image:initial;background-position:initial;b=
ackground-size:initial;background-repeat:initial;background-origin:initial;=
background-clip:initial;font-size:11pt;font-family:Calibri,sans-serif">

















































<span lang=3D"EN-US" style=3D"font-size:9pt;line-height:115%;font-family:Ar=
ial,sans-serif">73! Alex R7NT=C2=A0=C2=A0</span><u><span lang=3D"EN-US" sty=
le=3D"font-size:9pt;line-height:115%;font-family:Arial,sans-serif;color:blu=
e"><a href=3D"http://136.73.ru/" style=3D"color:blue">http://136.73.ru</a><=
/span></u>=C2=A0 =C2=A0=C2=A0<br></p></div>

--0000000000006ae7540582083aa8--

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 Content preview:  OK On the mains failure, Domenico. I have been reading on
   receiving EbNaut and hope to receive again soon. Thanks for the reports and
    the autodecoder. 73 Joe On Sat, 16 Feb 2019, Domenico IZ7SLZ wrote: 
 Content analysis details:   (0.0 points, 5.0 required)
  pts rule name              description
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X-Scan-Signature: 1bc6486c2865e7dc2ff7578e6d7fc226
Subject: Re: LF: VO1NA Ebnaut recently decodes
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OK On the mains failure, Domenico. I have been reading on receiving
EbNaut and hope to receive again soon.  Thanks for the reports and
the autodecoder.

73
Joe

On Sat, 16 Feb 2019, Domenico IZ7SLZ wrote:

> Hi Joe, LF
>
> Your EbNaut got one error free decode last night here in JN80nu using
> nominal values for time and frequency offsets:
>
> ------------------------------------------------------------------------------------------
> 2019-02-16_01:00:00 137477.00Hz N=7 T=3s 8K19A CRC=16 list=2000
> sym=608 Duration=1824s
> T_OFFSET=0.0s F_OFFSET=0.000Hz
> initial reference phase -29.6 amplitude 1.424e+01
> carrier phase: 1.5 deg
> carrier Eb/N0: 22.6 dB
> carrier Es/N0: 10.74 dB
> carrier S/N: 38.58 dB in 548.2 uHz, 5.96 dB in 1Hz, -28.01 dB in 2.5kHz
> found rank 0 ber 0.0000e+00 Eb/N0 71.8 M -3.575119629e+02 ph 1
> 180,180,180,180 [VO1NA:R]
> ------------------------------------------------------------------------------------------
>
>
> Other auto-decodes are logged at
> https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
> There was a mains outage at the receiving site on Feb 14, so i have missed
> unfortunatly LF transmissions of 14 and 15 february. Sorry.
>
> Thank you for the signal Joe. Propagation peak for our path seems to be
> around 01.00 UTC.
> Maybe be you can be ready for receiving so we can attempt an exchange of
> calls/report before the season ends ?
>
> Vy 73 to all, Domenico IZ7SLZ
>
> On Thu, 14 Feb 2019 at 19:44, DK7FC <selberdenken@posteo.de> wrote:
>
>> Hello Joe,
>>
>> Am 14.02.2019 18:41, schrieb jcraig@mun.ca:
>>> Greetings Stefan and congrats on your remarkable work on ELF.
>> Thank you. A 100 character message is running since 12 UTC. It will take
>> almost 4 days to pass it over. The longest message (in hours, not in
>> characters) ever sent in EbNaut, if i remember correctly :-)
>>> I am still thinking about the guard rail for VLF.  It is 10km+ from the
>>> shack so any operation will have to be mobile
>> Hm maybe you can send me the most accurate locator of your shack, like
>> Dimitris did with his house? It would be interesting to see your
>> location. Hay, we know each other since almost 10 years now but don't
>> know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz at
>> night, some years ago.
>>
>>> EbNaut LF TX: The signal is taken from the time pulse output of the
>>> NEO7 board
>>> which has a LED and dropping resistor across it. Paul has written
>>> code to control the frequency, duty cycle etc with a Raspi.  Very handy.
>> Yes, i'm using his tools too. Setting the time pulse works well but
>> setting a frequency does not, somehow. Am i making a stupid mistake or
>> does it have to do with the serial interface /dev/ttyAMA0 on a Raspi2B
>> (unlikely) or is my module missing something. Oh no, i remember i
>> successfully set a frequency output with the u-center software.
>> Need to try Markus' fresh developed tool for Windows, just to check if
>> it works.
>>
>> I would like to use a Raspi and Ebkey (using a XOR gate for the PSK) to
>> run an EbNaut message from a Raspi. With just 5 W TX power (the
>> classical QRP power level) i could pass a message over to Paul, when
>> TXing at night, from a small battery. That would be a great test that
>> could be done quite often and i don't need to have my car there and big
>> batteries. What a fun!
>>
>>> This goes directly to a TTL XOR and then a TC4426 driver thence a
>>> class E 100w TX or the Decca.  If you have any questions, I'll be happy
>>> to help.  This system is very simple.
>> Thanks Joe, I'll come back later to you. I'll try again and then pass
>> the command lines into this email, just for your confirmation.
>> 73, Stefan
>>
>>
>

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Message-ID: <5C697B5E.4070609@posteo.de>
Date: Sun, 17 Feb 2019 16:18:54 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hi VLF, Someone is transmitting on 8270.03 Hz it seems. Not
    me, not Markus, maybe it is Riccardo? It is a good signal on the local grabbers
    such as http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grab [...]
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Hi VLF,

Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus, 
maybe it is Riccardo? It is a good signal  on the local grabbers such as
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html or
https://vlf.u01.de/

Who is it ?

73, Stefan

From owner-rsgb_lf_group@blacksheep.org  Sun Feb 17 19:10:05 2019
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 <Pine.LNX.4.64.1902141357270.31354@plato.ucs.mun.ca> <5C65B65A.3080304@posteo.de>
 <CAC+C6w6gEV-rBU_Ur=4Zghy5CkGDaLE5TML+gfy+ZAprvM_WxA@mail.gmail.com> <Pine.LNX.4.64.1902161706160.18132@plato.ucs.mun.ca>
In-Reply-To: <Pine.LNX.4.64.1902161706160.18132@plato.ucs.mun.ca>
From: Daniele Caccia <daniele.caccia74@gmail.com>
Date: Sun, 17 Feb 2019 19:02:54 +0100
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 Content preview:  Hi Joe,Lf Last night your signal was really strong!!! *I55387FI*
    *Daniele Caccia* www.scientific-notes.blogspot.com 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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--000000000000c2dc3405821ad199
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--000000000000c2dc3005821ad197
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Hi Joe,Lf
Last night your signal was really strong!!!

*I55387FI*
*Daniele Caccia*



www.scientific-notes.blogspot.com




Il giorno sab 16 feb 2019 alle ore 21:42 <jcraig@mun.ca> ha scritto:

> OK On the mains failure, Domenico. I have been reading on receiving
> EbNaut and hope to receive again soon.  Thanks for the reports and
> the autodecoder.
>
> 73
> Joe
>
> On Sat, 16 Feb 2019, Domenico IZ7SLZ wrote:
>
> > Hi Joe, LF
> >
> > Your EbNaut got one error free decode last night here in JN80nu using
> > nominal values for time and frequency offsets:
> >
> >
> ------------------------------------------------------------------------------------------
> > 2019-02-16_01:00:00 137477.00Hz N=7 T=3s 8K19A CRC=16 list=2000
> > sym=608 Duration=1824s
> > T_OFFSET=0.0s F_OFFSET=0.000Hz
> > initial reference phase -29.6 amplitude 1.424e+01
> > carrier phase: 1.5 deg
> > carrier Eb/N0: 22.6 dB
> > carrier Es/N0: 10.74 dB
> > carrier S/N: 38.58 dB in 548.2 uHz, 5.96 dB in 1Hz, -28.01 dB in 2.5kHz
> > found rank 0 ber 0.0000e+00 Eb/N0 71.8 M -3.575119629e+02 ph 1
> > 180,180,180,180 [VO1NA:R]
> >
> ------------------------------------------------------------------------------------------
> >
> >
> > Other auto-decodes are logged at
> > https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
> > There was a mains outage at the receiving site on Feb 14, so i have
> missed
> > unfortunatly LF transmissions of 14 and 15 february. Sorry.
> >
> > Thank you for the signal Joe. Propagation peak for our path seems to be
> > around 01.00 UTC.
> > Maybe be you can be ready for receiving so we can attempt an exchange of
> > calls/report before the season ends ?
> >
> > Vy 73 to all, Domenico IZ7SLZ
> >
> > On Thu, 14 Feb 2019 at 19:44, DK7FC <selberdenken@posteo.de> wrote:
> >
> >> Hello Joe,
> >>
> >> Am 14.02.2019 18:41, schrieb jcraig@mun.ca:
> >>> Greetings Stefan and congrats on your remarkable work on ELF.
> >> Thank you. A 100 character message is running since 12 UTC. It will take
> >> almost 4 days to pass it over. The longest message (in hours, not in
> >> characters) ever sent in EbNaut, if i remember correctly :-)
> >>> I am still thinking about the guard rail for VLF.  It is 10km+ from the
> >>> shack so any operation will have to be mobile
> >> Hm maybe you can send me the most accurate locator of your shack, like
> >> Dimitris did with his house? It would be interesting to see your
> >> location. Hay, we know each other since almost 10 years now but don't
> >> know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz at
> >> night, some years ago.
> >>
> >>> EbNaut LF TX: The signal is taken from the time pulse output of the
> >>> NEO7 board
> >>> which has a LED and dropping resistor across it. Paul has written
> >>> code to control the frequency, duty cycle etc with a Raspi.  Very
> handy.
> >> Yes, i'm using his tools too. Setting the time pulse works well but
> >> setting a frequency does not, somehow. Am i making a stupid mistake or
> >> does it have to do with the serial interface /dev/ttyAMA0 on a Raspi2B
> >> (unlikely) or is my module missing something. Oh no, i remember i
> >> successfully set a frequency output with the u-center software.
> >> Need to try Markus' fresh developed tool for Windows, just to check if
> >> it works.
> >>
> >> I would like to use a Raspi and Ebkey (using a XOR gate for the PSK) to
> >> run an EbNaut message from a Raspi. With just 5 W TX power (the
> >> classical QRP power level) i could pass a message over to Paul, when
> >> TXing at night, from a small battery. That would be a great test that
> >> could be done quite often and i don't need to have my car there and big
> >> batteries. What a fun!
> >>
> >>> This goes directly to a TTL XOR and then a TC4426 driver thence a
> >>> class E 100w TX or the Decca.  If you have any questions, I'll be happy
> >>> to help.  This system is very simple.
> >> Thanks Joe, I'll come back later to you. I'll try again and then pass
> >> the command lines into this email, just for your confirmation.
> >> 73, Stefan
> >>
> >>
> >
>
>

--000000000000c2dc3005821ad197
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div>Hi Joe,Lf</div>Last night your signal was really stro=
ng!!!<div><br></div><div><b><font size=3D"4">I55387FI</font></b><br clear=
=3D"all"><div><div dir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"=
gmail_signature"><div dir=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><div di=
r=3D"ltr"><div dir=3D"ltr"><div dir=3D"ltr"><b style=3D"font-size:14px">Dan=
iele Caccia</b></div><div dir=3D"ltr"><br><div><font color=3D"#0000ff" face=
=3D"Verdana"><br></font></div><div><div><br></div><div><font color=3D"#0000=
ff" face=3D"Verdana"><a href=3D"http://www.scientific-notes.blogspot.com" t=
arget=3D"_blank">www.scientific-notes.blogspot.com</a></font></div><div><fo=
nt color=3D"#0000ff" face=3D"Verdana"><br></font></div><div><br></div></div=
></div></div></div></div></div></div></div></div><br></div></div><br><div c=
lass=3D"gmail_quote"><div dir=3D"ltr" class=3D"gmail_attr">Il giorno sab 16=
 feb 2019 alle ore 21:42 &lt;<a href=3D"mailto:jcraig@mun.ca">jcraig@mun.ca=
</a>&gt; ha scritto:<br></div><blockquote class=3D"gmail_quote" style=3D"ma=
rgin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:=
1ex">OK On the mains failure, Domenico. I have been reading on receiving<br=
>
EbNaut and hope to receive again soon.=C2=A0 Thanks for the reports and<br>
the autodecoder.<br>
<br>
73<br>
Joe<br>
<br>
On Sat, 16 Feb 2019, Domenico IZ7SLZ wrote:<br>
<br>
&gt; Hi Joe, LF<br>
&gt;<br>
&gt; Your EbNaut got one error free decode last night here in JN80nu using<=
br>
&gt; nominal values for time and frequency offsets:<br>
&gt;<br>
&gt; ----------------------------------------------------------------------=
--------------------<br>
&gt; 2019-02-16_01:00:00 137477.00Hz N=3D7 T=3D3s 8K19A CRC=3D16 list=3D200=
0<br>
&gt; sym=3D608 Duration=3D1824s<br>
&gt; T_OFFSET=3D0.0s F_OFFSET=3D0.000Hz<br>
&gt; initial reference phase -29.6 amplitude 1.424e+01<br>
&gt; carrier phase: 1.5 deg<br>
&gt; carrier Eb/N0: 22.6 dB<br>
&gt; carrier Es/N0: 10.74 dB<br>
&gt; carrier S/N: 38.58 dB in 548.2 uHz, 5.96 dB in 1Hz, -28.01 dB in 2.5kH=
z<br>
&gt; found rank 0 ber 0.0000e+00 Eb/N0 71.8 M -3.575119629e+02 ph 1<br>
&gt; 180,180,180,180 [VO1NA:R]<br>
&gt; ----------------------------------------------------------------------=
--------------------<br>
&gt;<br>
&gt;<br>
&gt; Other auto-decodes are logged at<br>
&gt; <a href=3D"https://qsl.net/iz7slz/EBNAUT/DECODED.TXT" rel=3D"noreferre=
r" target=3D"_blank">https://qsl.net/iz7slz/EBNAUT/DECODED.TXT</a><br>
&gt; There was a mains outage at the receiving site on Feb 14, so i have mi=
ssed<br>
&gt; unfortunatly LF transmissions of 14 and 15 february. Sorry.<br>
&gt;<br>
&gt; Thank you for the signal Joe. Propagation peak for our path seems to b=
e<br>
&gt; around 01.00 UTC.<br>
&gt; Maybe be you can be ready for receiving so we can attempt an exchange =
of<br>
&gt; calls/report before the season ends ?<br>
&gt;<br>
&gt; Vy 73 to all, Domenico IZ7SLZ<br>
&gt;<br>
&gt; On Thu, 14 Feb 2019 at 19:44, DK7FC &lt;<a href=3D"mailto:selberdenken=
@posteo.de" target=3D"_blank">selberdenken@posteo.de</a>&gt; wrote:<br>
&gt;<br>
&gt;&gt; Hello Joe,<br>
&gt;&gt;<br>
&gt;&gt; Am 14.02.2019 18:41, schrieb <a href=3D"mailto:jcraig@mun.ca" targ=
et=3D"_blank">jcraig@mun.ca</a>:<br>
&gt;&gt;&gt; Greetings Stefan and congrats on your remarkable work on ELF.<=
br>
&gt;&gt; Thank you. A 100 character message is running since 12 UTC. It wil=
l take<br>
&gt;&gt; almost 4 days to pass it over. The longest message (in hours, not =
in<br>
&gt;&gt; characters) ever sent in EbNaut, if i remember correctly :-)<br>
&gt;&gt;&gt; I am still thinking about the guard rail for VLF.=C2=A0 It is =
10km+ from the<br>
&gt;&gt;&gt; shack so any operation will have to be mobile<br>
&gt;&gt; Hm maybe you can send me the most accurate locator of your shack, =
like<br>
&gt;&gt; Dimitris did with his house? It would be interesting to see your<b=
r>
&gt;&gt; location. Hay, we know each other since almost 10 years now but do=
n&#39;t<br>
&gt;&gt; know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz=
 at<br>
&gt;&gt; night, some years ago.<br>
&gt;&gt;<br>
&gt;&gt;&gt; EbNaut LF TX: The signal is taken from the time pulse output o=
f the<br>
&gt;&gt;&gt; NEO7 board<br>
&gt;&gt;&gt; which has a LED and dropping resistor across it. Paul has writ=
ten<br>
&gt;&gt;&gt; code to control the frequency, duty cycle etc with a Raspi.=C2=
=A0 Very handy.<br>
&gt;&gt; Yes, i&#39;m using his tools too. Setting the time pulse works wel=
l but<br>
&gt;&gt; setting a frequency does not, somehow. Am i making a stupid mistak=
e or<br>
&gt;&gt; does it have to do with the serial interface /dev/ttyAMA0 on a Ras=
pi2B<br>
&gt;&gt; (unlikely) or is my module missing something. Oh no, i remember i<=
br>
&gt;&gt; successfully set a frequency output with the u-center software.<br=
>
&gt;&gt; Need to try Markus&#39; fresh developed tool for Windows, just to =
check if<br>
&gt;&gt; it works.<br>
&gt;&gt;<br>
&gt;&gt; I would like to use a Raspi and Ebkey (using a XOR gate for the PS=
K) to<br>
&gt;&gt; run an EbNaut message from a Raspi. With just 5 W TX power (the<br=
>
&gt;&gt; classical QRP power level) i could pass a message over to Paul, wh=
en<br>
&gt;&gt; TXing at night, from a small battery. That would be a great test t=
hat<br>
&gt;&gt; could be done quite often and i don&#39;t need to have my car ther=
e and big<br>
&gt;&gt; batteries. What a fun!<br>
&gt;&gt;<br>
&gt;&gt;&gt; This goes directly to a TTL XOR and then a TC4426 driver thenc=
e a<br>
&gt;&gt;&gt; class E 100w TX or the Decca.=C2=A0 If you have any questions,=
 I&#39;ll be happy<br>
&gt;&gt;&gt; to help.=C2=A0 This system is very simple.<br>
&gt;&gt; Thanks Joe, I&#39;ll come back later to you. I&#39;ll try again an=
d then pass<br>
&gt;&gt; the command lines into this email, just for your confirmation.<br>
&gt;&gt; 73, Stefan<br>
&gt;&gt;<br>
&gt;&gt;<br>
&gt;<br>
<br>
</blockquote></div>

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 Content preview:  Hi Daniele, Cnditions must be good. Thanks for the report.
    Pleased to confirm. 73 Joe 
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Subject: Re: LF: VO1NA Ebnaut recently decodes
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Hi Daniele,

Cnditions must be good.  Thanks for the report.
Pleased to confirm.

73
Joe

On Sun, 17 Feb 2019, Daniele Caccia wrote:

> Hi Joe,Lf
> Last night your signal was really strong!!!
>
> *I55387FI*
> *Daniele Caccia*
>
>
>
> www.scientific-notes.blogspot.com
>
>
>
>
> Il giorno sab 16 feb 2019 alle ore 21:42 <jcraig@mun.ca> ha scritto:
>
>> OK On the mains failure, Domenico. I have been reading on receiving
>> EbNaut and hope to receive again soon.  Thanks for the reports and
>> the autodecoder.
>>
>> 73
>> Joe
>>
>> On Sat, 16 Feb 2019, Domenico IZ7SLZ wrote:
>>
>>> Hi Joe, LF
>>>
>>> Your EbNaut got one error free decode last night here in JN80nu using
>>> nominal values for time and frequency offsets:
>>>
>>>
>> ------------------------------------------------------------------------------------------
>>> 2019-02-16_01:00:00 137477.00Hz N=7 T=3s 8K19A CRC=16 list=2000
>>> sym=608 Duration=1824s
>>> T_OFFSET=0.0s F_OFFSET=0.000Hz
>>> initial reference phase -29.6 amplitude 1.424e+01
>>> carrier phase: 1.5 deg
>>> carrier Eb/N0: 22.6 dB
>>> carrier Es/N0: 10.74 dB
>>> carrier S/N: 38.58 dB in 548.2 uHz, 5.96 dB in 1Hz, -28.01 dB in 2.5kHz
>>> found rank 0 ber 0.0000e+00 Eb/N0 71.8 M -3.575119629e+02 ph 1
>>> 180,180,180,180 [VO1NA:R]
>>>
>> ------------------------------------------------------------------------------------------
>>>
>>>
>>> Other auto-decodes are logged at
>>> https://qsl.net/iz7slz/EBNAUT/DECODED.TXT
>>> There was a mains outage at the receiving site on Feb 14, so i have
>> missed
>>> unfortunatly LF transmissions of 14 and 15 february. Sorry.
>>>
>>> Thank you for the signal Joe. Propagation peak for our path seems to be
>>> around 01.00 UTC.
>>> Maybe be you can be ready for receiving so we can attempt an exchange of
>>> calls/report before the season ends ?
>>>
>>> Vy 73 to all, Domenico IZ7SLZ
>>>
>>> On Thu, 14 Feb 2019 at 19:44, DK7FC <selberdenken@posteo.de> wrote:
>>>
>>>> Hello Joe,
>>>>
>>>> Am 14.02.2019 18:41, schrieb jcraig@mun.ca:
>>>>> Greetings Stefan and congrats on your remarkable work on ELF.
>>>> Thank you. A 100 character message is running since 12 UTC. It will take
>>>> almost 4 days to pass it over. The longest message (in hours, not in
>>>> characters) ever sent in EbNaut, if i remember correctly :-)
>>>>> I am still thinking about the guard rail for VLF.  It is 10km+ from the
>>>>> shack so any operation will have to be mobile
>>>> Hm maybe you can send me the most accurate locator of your shack, like
>>>> Dimitris did with his house? It would be interesting to see your
>>>> location. Hay, we know each other since almost 10 years now but don't
>>>> know very much actually ;-) I remember our DFCW-3 QSO on 137.7 kHz at
>>>> night, some years ago.
>>>>
>>>>> EbNaut LF TX: The signal is taken from the time pulse output of the
>>>>> NEO7 board
>>>>> which has a LED and dropping resistor across it. Paul has written
>>>>> code to control the frequency, duty cycle etc with a Raspi.  Very
>> handy.
>>>> Yes, i'm using his tools too. Setting the time pulse works well but
>>>> setting a frequency does not, somehow. Am i making a stupid mistake or
>>>> does it have to do with the serial interface /dev/ttyAMA0 on a Raspi2B
>>>> (unlikely) or is my module missing something. Oh no, i remember i
>>>> successfully set a frequency output with the u-center software.
>>>> Need to try Markus' fresh developed tool for Windows, just to check if
>>>> it works.
>>>>
>>>> I would like to use a Raspi and Ebkey (using a XOR gate for the PSK) to
>>>> run an EbNaut message from a Raspi. With just 5 W TX power (the
>>>> classical QRP power level) i could pass a message over to Paul, when
>>>> TXing at night, from a small battery. That would be a great test that
>>>> could be done quite often and i don't need to have my car there and big
>>>> batteries. What a fun!
>>>>
>>>>> This goes directly to a TTL XOR and then a TC4426 driver thence a
>>>>> class E 100w TX or the Decca.  If you have any questions, I'll be happy
>>>>> to help.  This system is very simple.
>>>> Thanks Joe, I'll come back later to you. I'll try again and then pass
>>>> the command lines into this email, just for your confirmation.
>>>> 73, Stefan
>>>>
>>>>
>>>
>>
>>
>

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 Content preview:  Not me ! Unfortunately :( Still windong coils 73 de Luis EA5DOM
    De: owner-rsgb_lf_group@blacksheep.org [owner-rsgb_lf_group@blacksheep.org]
    en nombre de DK7FC [selberdenken@posteo.de] Enviado: domingo, 17 [...] 
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  pts rule name              description
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                             low trust
                             [185.201.18.22 listed in list.dnswl.org]
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Subject: LF: Re: 8270
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Not me ! Unfortunately :(

Still windong coils 

73 de Luis
EA5DOM
________________________________________
De: owner-rsgb_lf_group@blacksheep.org [owner-rsgb_lf_group@blacksheep.org] en nombre de DK7FC [selberdenken@posteo.de]
Enviado: domingo, 17 de febrero de 2019 16:18
Para: rsgb_lf_group@blacksheep.org
Asunto: VLF: 8270

Hi VLF,

Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus,
maybe it is Riccardo? It is a good signal  on the local grabbers such as
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html or
https://vlf.u01.de/

Who is it ?

73, Stefan



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Thread-Topic: MF/LF chat over QA-100 Geostationary Satellite ? 
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Date: Sun, 17 Feb 2019 21:18:31 +0000
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 Content preview:  Hi All May be someone has the equipment and is in the footprint
    of Es'Hail-2, formely AMSAT QA-100 satellite? Nice place for chats working
    as an HF band permanently open and with outstanding sensibility 
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  pts rule name              description
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  1.5 RCVD_IN_SORBS_WEB      RBL: SORBS: sender is an abusable web server
                             [85.60.35.36 listed in dnsbl.sorbs.net]
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Subject: LF: MF/LF chat over QA-100 Geostationary Satellite ? 
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--_000_6DB8451D7F3D3947A5918808A59621EA31525CA4servigilantvigi_
Content-Type: text/plain; charset="iso-8859-1"
Content-Transfer-Encoding: quoted-printable

Hi All

May be someone has the equipment and is in the footprint of Es'Hail-2, form=
ely AMSAT QA-100 satellite?
Nice place for chats working as an HF band permanently open and with outsta=
nding sensibility

Anybody (appart from David, G0MRF) interested in joining an MF/LF/VLF chat =
?

You need just an SSB rig at 144 or 432, an upconverter to 2.4GHz and a WiFi=
 PA and antenna and you are in
For Rx you can even use the WebSDR at Goonhilly
https://eshail.batc.org.uk/nb/

Unfortunately the footprint of the satellite do not cover America (only the=
 extreme East of Brazil)
nor Australia (reaching up to thailand). But sites like Reunion are in the =
footprint

73 de Luis
EA5DOM

--_000_6DB8451D7F3D3947A5918808A59621EA31525CA4servigilantvigi_
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Content-Transfer-Encoding: quoted-printable

<html dir=3D"ltr">
<head>
<meta http-equiv=3D"Content-Type" content=3D"text/html; charset=3Diso-8859-=
1">
<style type=3D"text/css" id=3D"owaParaStyle"></style>
</head>
<body fpstyle=3D"1" ocsi=3D"0">
<div style=3D"direction: ltr;font-family: Tahoma;color: #000000;font-size: =
10pt;">Hi All
<div><br>
</div>
<div>May be someone has the equipment and is in the footprint of Es'Hail-2,=
 formely AMSAT QA-100 satellite?</div>
<div>Nice place for chats working as an HF band permanently open and with o=
utstanding sensibility</div>
<div><br>
</div>
<div>Anybody (appart from David, G0MRF) interested in joining an MF/LF/VLF =
chat ?</div>
<div><br>
</div>
<div>You need just an SSB rig at 144 or 432, an upconverter to 2.4GHz and a=
 WiFi PA and antenna and you are in</div>
<div>For Rx you can even use the WebSDR at Goonhilly</div>
<div><a href=3D"https://eshail.batc.org.uk/nb/" target=3D"_blank" style=3D"=
font-size: 10pt;">https://eshail.batc.org.uk/nb/</a></div>
<div><span style=3D"font-size: 10pt;"><br>
</span></div>
<div><span style=3D"font-size: 10pt;">Unfortunately the footprint of the sa=
tellite do not cover America (only the extreme East of Brazil)</span></div>
<div><span style=3D"font-size: 10pt;">nor Australia (reaching up to thailan=
d). But sites like Reunion are in the footprint</span></div>
<div><span style=3D"font-size: 10pt;"><br>
</span></div>
<div><span style=3D"font-size: 10pt;">73 de Luis</span></div>
<div><span style=3D"font-size: 10pt;">EA5DOM&nbsp;</span></div>
</div>
</body>
</html>

--_000_6DB8451D7F3D3947A5918808A59621EA31525CA4servigilantvigi_--

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 <5C5BE905.2010904@posteo.de> <CAKvcm2fZ6eWSMX+R9gGVR86kv=dEJHx+W1St=bD++q1m0obyQQ@mail.gmail.com>
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From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Sun, 17 Feb 2019 22:19:28 +0100
Message-ID: <CANA3B6XKR7JN-YeaGLcKPxtAEYcDSjWVg43VVqWr=-=3mPyocQ@mail.gmail.com>
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 Content preview:  Stefan, VLF, Yes, it's me! :-) I'm trying with a continuous
    carrier on 8270.003 Hz. Thanks for your report, Stefan: very good performance
    of your VLF grabber (that was offline during my last VLF transmission on
   la [...] 
 Content analysis details:   (0.3 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
 -0.0 RCVD_IN_DNSWL_NONE     RBL: Sender listed at http://www.dnswl.org/,
                             no trust
                             [2a00:1450:4864:20:0:0:0:52e listed in]
                             [list.dnswl.org]
 -0.0 SPF_PASS               SPF: sender matches SPF record
  0.0 FREEMAIL_FROM          Sender email is commonly abused enduser mail
                             provider (riccardozoli80[at]gmail.com)
  0.2 FREEMAIL_ENVFROM_END_DIGIT Envelope-from freemail username ends
                             in digit (riccardozoli80[at]gmail.com)
  0.0 HTML_MESSAGE           BODY: HTML included in message
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Subject: Re: VLF: 8270
Content-Type: multipart/alternative; boundary="000000000000f3d51505821d90b9"
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--000000000000f3d51505821d90b9
Content-Type: text/plain; charset="UTF-8"

Stefan, VLF,

Yes, it's me! :-) I'm trying with a continuous carrier on 8270.003 Hz.
Thanks for your report, Stefan: very good performance of your VLF grabber
(that was offline during my last VLF transmission on late december 2018).
Tomorrow I'll try to send a few characters if the noise will remain low.
Unfortunately at this moment the humidity is rising and I think I will go
QRT before midnight.


All the best


73 de Riccardo IW4DXW


P.S.: congrats for your latest (of a long series) fantastic results on the
ELF band. :-)



Il giorno Dom 17 Feb 2019, 16:25 DK7FC <selberdenken@posteo.de> ha scritto:

> Hi VLF,
>
> Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus,
> maybe it is Riccardo? It is a good signal  on the local grabbers such as
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html or
> https://vlf.u01.de/
>
> Who is it ?
>
> 73, Stefan
>
>

--000000000000f3d51505821d90b9
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"auto"><div dir=3D"auto"><br></div><div dir=3D"auto">Stefan, VLF=
,</div><div dir=3D"auto"><br></div><div dir=3D"auto">Yes, it&#39;s me! :-) =
I&#39;m trying with a continuous carrier on 8270.003 Hz.</div><div dir=3D"a=
uto">Thanks for your report, Stefan: very good performance of your VLF grab=
ber (that was offline during my last VLF transmission on late december 2018=
).</div><div dir=3D"auto">Tomorrow I&#39;ll try to send a few characters if=
 the noise will remain low.</div><div dir=3D"auto">Unfortunately at this mo=
ment the humidity is rising and I think I will go QRT before midnight.</div=
><div dir=3D"auto"><br></div><div dir=3D"auto"><br></div><div dir=3D"auto">=
All the best</div><div dir=3D"auto"><br></div><div dir=3D"auto"><br></div><=
div dir=3D"auto">73 de Riccardo IW4DXW</div><div dir=3D"auto"><br></div><di=
v dir=3D"auto"><br></div><div dir=3D"auto">P.S.: congrats for your latest (=
of a long series) fantastic results on the ELF band. :-)</div><div dir=3D"a=
uto"><br></div><br><br><div class=3D"gmail_quote" dir=3D"auto"><div dir=3D"=
ltr">Il giorno Dom 17 Feb 2019, 16:25 DK7FC &lt;<a href=3D"mailto:selberden=
ken@posteo.de" target=3D"_blank" rel=3D"noreferrer">selberdenken@posteo.de<=
/a>&gt; ha scritto:<br></div><blockquote class=3D"gmail_quote" style=3D"mar=
gin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex">Hi VLF,<br>
<br>
Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus, <br>
maybe it is Riccardo? It is a good signal=C2=A0 on the local grabbers such =
as<br>
<a href=3D"http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2=
.html" rel=3D"noreferrer noreferrer noreferrer" target=3D"_blank">http://ww=
w.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a> or<br>
<a href=3D"https://vlf.u01.de/" rel=3D"noreferrer noreferrer noreferrer" ta=
rget=3D"_blank">https://vlf.u01.de/</a><br>
<br>
Who is it ?<br>
<br>
73, Stefan<br>
<br>
</blockquote></div>
</div>

--000000000000f3d51505821d90b9--

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Date: Sun, 17 Feb 2019 22:25:48 +0100
From: Steffi <jota.s@gmx.de>
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 Content preview:  Hi again, thank you for so many answers! Special thanks to
    Eberhard, DL3ZID, for the detailed spectrum screenshots of different QRM
   sources and also to Alan, G3NYK, for the link to the excellent article about
    QRM from a NEFF induction hob. 
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Hi again,

thank you for so many answers!

Special thanks to Eberhard, DL3ZID, for the detailed spectrum 
screenshots of different QRM sources and also to Alan, G3NYK, for the 
link to the excellent article about QRM from a NEFF induction hob.

I see that there will sure be some QRM from an induction cooker. But 
mostly, it will be off >23 hours/day - and I can decide about it myself. 
Indeed, the advantages of an induction cooker mentioned by Dexter are 
important.
Maybe I will buy a little extra ceramic glass cooktop, to have a 
low-noise backup cooking solution :)

The answers also show, that in reality the major problem is QRM from 
other electronics which runs 24/7 and not only before lunch. So we must 
carefully chose a "quiet" solar (PV) inverter if we want to install 
solar panels on the roof, for example. Or we'll have to modify it with 
additional filters...

After all, it's even harder to prevent QRN = Neighbour-made-noise. 
Hopefully they don't use PLC or something like that!

And yes, Stefan, I live near N�rnberg and I know Markus and his VLF 
grabber. I will tell him to check the grabber for signals from my 
induction cooker, when it's active the first time. If he can prove the 
reception from MY(!) hob, I will send him a QSL card and invite him for 
lunch :) But it will be hard, it's more than 30 km.

73,
de Steffi - dl8nsb


Steffi schrieb:
> Hi LF Group,
> 
> soon I will have to buy a new kitchen and I wonder, if an induction
> cooker is the right choice (regarding QRM!). Does anyone have experience
> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
> can be recommended?
> 
> I already heard, that there won't be problems on 80m, but what about
> lower frequencies?
> 
> I'm not yet QRV on MF/LF, but maybe in the future..
> 
> Any comments and experiences will be helpful!
> 
> 73,
> de Steffi - dl8nsb
> 
> 
> 

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From: Dimitrios Tsifakis <dtsifakis@gmail.com>
Date: Mon, 18 Feb 2019 12:33:14 +1100
Message-ID: <CAKvcm2ect05e32rw0uykXWhEkiVCO9vHeunWGBAmteSLpLqLAA@mail.gmail.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  Hi Luis, > May be someone has the equipment and is in the
   footprint of Es'Hail-2, formely AMSAT QA-100 satellite? Isn't it ironic, using
    10 GHz to have a chat about the kHz bands :-) 
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Subject: Re: LF: MF/LF chat over QA-100 Geostationary Satellite ?
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Hi Luis,

> May be someone has the equipment and is in the footprint of Es'Hail-2, formely AMSAT QA-100 satellite?

Isn't it ironic, using 10 GHz to have a chat about the kHz bands :-)

Sadly, as you said, Australia isn't in the footprint. Hope one of the
geostationary sats in our view will have a amateur radio transponder
one day!

73, Dimitris VK2COW

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 Content preview:  It is one of those special nights on LF. I put a new exciter
    on this afternoon and was getting some early WSPR reports from across the
    Atlantic. During a failed QSO attempt with G0MRF, the class D amp blew my
    last set of FETs. I was discoura [...] 
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Subject: LF: LF magic
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It is one of those special nights on LF.

I put a new exciter on this afternoon and was getting some early
WSPR reports from across the Atlantic. During a failed QSO attempt
with G0MRF, the class D amp blew my last set of FETs. I was
discouraged but put the small class E amp back in so I could keep
playing with the new exciter.

Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
be heard. Surprise! We had an easy QSO with just one repeat sequence
required! Thank you Chris!

Now WSPR reports from Europe are getting even better. What else will
this night bring?

73,
Paul N1BUG

From owner-rsgb_lf_group@blacksheep.org  Mon Feb 18 08:53:00 2019
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Date: Mon, 18 Feb 2019 08:46:42 +0100
From: DK7FC <selberdenken@posteo.de>
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 Content preview:  Hello Luis, How does your bucket look now? Photo? 0.2 mm diameter
    is hard to wind. You need to be patient with yourselfe. But after some hours
    you will notice that your skills become better with each turn yo add [...]
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Subject: Re: LF: Re: 8270
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Hello Luis,

How does your bucket look now? Photo?
0.2 mm diameter is hard to wind. You need to be patient with yourselfe. 
But after some hours you will notice that your skills become better with 
each turn yo add :-)
It would be interesting to know the DC resistance and L of one bucket.

73, Stefan

Am 17.02.2019 22:06, schrieb VIGILANT Luis Fern�ndez:
> Not me ! Unfortunately :(
>
> Still windong coils
>
> 73 de Luis
> EA5DOM
> ________________________________________
> De: owner-rsgb_lf_group@blacksheep.org [owner-rsgb_lf_group@blacksheep.org] en nombre de DK7FC [selberdenken@posteo.de]
> Enviado: domingo, 17 de febrero de 2019 16:18
> Para: rsgb_lf_group@blacksheep.org
> Asunto: VLF: 8270
>
> Hi VLF,
>
> Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus,
> maybe it is Riccardo? It is a good signal  on the local grabbers such as
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html or
> https://vlf.u01.de/
>
> Who is it ?
>
> 73, Stefan
>
>
>    

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 Content preview:  Hi Riccardo, I'm ready on all frequencies for your message
    attempt. The conds are very good! At the night i completed my 83 hour long
    EbNaut message and did now QSY to 12.47 Hz, the 36km band is for you :-) 
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Subject: Re: VLF: 8270
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This is a multi-part message in MIME format.
--------------000506010605090903080109
Content-Type: text/plain; charset=UTF-8; format=flowed
Content-Transfer-Encoding: 7bit

Hi Riccardo,

I'm ready on all frequencies for your message attempt. The conds are 
very good! At the night i completed my 83 hour long EbNaut message and 
did now QSY to 12.47 Hz, the 36km band is for you :-)

What about your ground loop antenna? Didn't you say you want to build 
one near your house?

73, Stefan

Am 17.02.2019 22:19, schrieb Riccardo Zoli:
>
> Stefan, VLF,
>
> Yes, it's me! :-) I'm trying with a continuous carrier on 8270.003 Hz.
> Thanks for your report, Stefan: very good performance of your VLF 
> grabber (that was offline during my last VLF transmission on late 
> december 2018).
> Tomorrow I'll try to send a few characters if the noise will remain low.
> Unfortunately at this moment the humidity is rising and I think I will 
> go QRT before midnight.
>
>
> All the best
>
>
> 73 de Riccardo IW4DXW
>
>
> P.S.: congrats for your latest (of a long series) fantastic results on 
> the ELF band. :-)
>
>
>
> Il giorno Dom 17 Feb 2019, 16:25 DK7FC <selberdenken@posteo.de 
> <mailto:selberdenken@posteo.de>> ha scritto:
>
>     Hi VLF,
>
>     Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus,
>     maybe it is Riccardo? It is a good signal  on the local grabbers
>     such as
>     http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html
>     or
>     https://vlf.u01.de/
>
>     Who is it ?
>
>     73, Stefan
>

--------------000506010605090903080109
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 8bit

<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
</head>
<body bgcolor="#ffffff" text="#000000">
Hi Riccardo, <br>
<br>
I'm ready on all frequencies for your message attempt. The conds are
very good! At the night i completed my 83 hour long EbNaut message and
did now QSY to 12.47 Hz, the 36km band is for you :-)<br>
<br>
What about your ground loop antenna? Didn't you say you want to build
one near your house?<br>
<br>
73, Stefan<br>
<br>
Am 17.02.2019 22:19, schrieb Riccardo Zoli:
<blockquote
 cite="mid:CANA3B6XKR7JN-YeaGLcKPxtAEYcDSjWVg43VVqWr=-=3mPyocQ@mail.gmail.com"
 type="cite">
  <div dir="auto">
  <div dir="auto"><br>
  </div>
  <div dir="auto">Stefan, VLF,</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">Yes, it's me! :-) I'm trying with a continuous
carrier on 8270.003 Hz.</div>
  <div dir="auto">Thanks for your report, Stefan: very good performance
of your VLF grabber (that was offline during my last VLF transmission
on late december 2018).</div>
  <div dir="auto">Tomorrow I'll try to send a few characters if the
noise will remain low.</div>
  <div dir="auto">Unfortunately at this moment the humidity is rising
and I think I will go QRT before midnight.</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">All the best</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">73 de Riccardo IW4DXW</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">P.S.: congrats for your latest (of a long series)
fantastic results on the ELF band. :-)</div>
  <div dir="auto"><br>
  </div>
  <br>
  <br>
  <div class="gmail_quote" dir="auto">
  <div dir="ltr">Il giorno Dom 17 Feb 2019, 16:25 DK7FC &lt;<a
 moz-do-not-send="true" href="mailto:selberdenken@posteo.de"
 target="_blank" rel="noreferrer">selberdenken@posteo.de</a>&gt; ha
scritto:<br>
  </div>
  <blockquote class="gmail_quote"
 style="border-left: 1px solid rgb(204, 204, 204); margin: 0pt 0pt 0pt 0.8ex; padding-left: 1ex;">Hi
VLF,<br>
    <br>
Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus, <br>
maybe it is Riccardo? It is a good signal  on the local grabbers such as<br>
    <a moz-do-not-send="true"
 href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html"
 rel="noreferrer noreferrer noreferrer" target="_blank">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
or<br>
    <a moz-do-not-send="true" href="https://vlf.u01.de/"
 rel="noreferrer noreferrer noreferrer" target="_blank">https://vlf.u01.de/</a><br>
    <br>
Who is it ?<br>
    <br>
73, Stefan<br>
    <br>
  </blockquote>
  </div>
  </div>
</blockquote>
</body>
</html>

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 Content preview:  Hello Steffi, RR. Maybe you can ask for a cooker with a GPS
    input to stabilise the switching frequency. It also needs a PSK input, then
    you can send me a message. Hey, i also have a grabber, it is just 175 km
   dista [...] 
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Hello Steffi,

RR. Maybe you can ask for a cooker with a GPS input to stabilise the 
switching frequency. It also needs a PSK input, then you can send me a 
message. Hey, i also have a grabber, it is just 175 km distant. If you 
leave a trace here as well, you can invite me too ;-)

73, GL, Stefan

Am 17.02.2019 22:25, schrieb Steffi:
> Hi again,
>
> thank you for so many answers!
>
> Special thanks to Eberhard, DL3ZID, for the detailed spectrum 
> screenshots of different QRM sources and also to Alan, G3NYK, for the 
> link to the excellent article about QRM from a NEFF induction hob.
>
> I see that there will sure be some QRM from an induction cooker. But 
> mostly, it will be off >23 hours/day - and I can decide about it 
> myself. Indeed, the advantages of an induction cooker mentioned by 
> Dexter are important.
> Maybe I will buy a little extra ceramic glass cooktop, to have a 
> low-noise backup cooking solution :)
>
> The answers also show, that in reality the major problem is QRM from 
> other electronics which runs 24/7 and not only before lunch. So we 
> must carefully chose a "quiet" solar (PV) inverter if we want to 
> install solar panels on the roof, for example. Or we'll have to modify 
> it with additional filters...
>
> After all, it's even harder to prevent QRN = Neighbour-made-noise. 
> Hopefully they don't use PLC or something like that!
>
> And yes, Stefan, I live near N�rnberg and I know Markus and his VLF 
> grabber. I will tell him to check the grabber for signals from my 
> induction cooker, when it's active the first time. If he can prove the 
> reception from MY(!) hob, I will send him a QSL card and invite him 
> for lunch :) But it will be hard, it's more than 30 km.
>
> 73,
> de Steffi - dl8nsb
>
>
> Steffi schrieb:
>> Hi LF Group,
>>
>> soon I will have to buy a new kitchen and I wonder, if an induction
>> cooker is the right choice (regarding QRM!). Does anyone have experience
>> with QRM on MF, LF, VLF produced by an induction cooker? Which brands
>> can be recommended?
>>
>> I already heard, that there won't be problems on 80m, but what about
>> lower frequencies?
>>
>> I'm not yet QRV on MF/LF, but maybe in the future..
>>
>> Any comments and experiences will be helpful!
>>
>> 73,
>> de Steffi - dl8nsb
>>
>>
>>
>

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 Content preview:  Hi Stefan, VLF The "Tricotosa" works nicely. Added a pedal
    to activate the motor, which is very useful I think I used too much double
    side tape and need to get the kapton to be able to continue You are right,
    keeping the wire in place and avoiding overlapping in two layers is a tricky
    job. I'm thinking [...] 
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Hi Stefan, VLF

The "Tricotosa" works nicely. Added a pedal to activate the motor, which is very useful

I think I used too much double side tape and need to get the kapton to be able to continue
You are right, keeping the wire in place and avoiding overlapping in two layers is a tricky job. I'm thinking about adding
a vertical guide with a motorized threaded spindle. Adjustin the speed of the spindle will be possible to achieve a very nice
winding

Anyway, this is a picture of what I got manually https://www.dropbox.com/s/kh690bq353zzv0m/IMG_20190217_172317_478.jpg?dl=0

There is a lot of copper in this reel. I can start kniting copper head caps with personalized callsign for QRO operators
Do you need any ? ;-)

73 de Luis
EA5DOM

-----Mensaje original-----
De: owner-rsgb_lf_group@blacksheep.org [mailto:owner-rsgb_lf_group@blacksheep.org] En nombre de DK7FC
Enviado el: lunes, 18 de febrero de 2019 8:47
Para: rsgb_lf_group@blacksheep.org
Asunto: Re: LF: Re: 8270

Hello Luis,

How does your bucket look now? Photo?
0.2 mm diameter is hard to wind. You need to be patient with yourselfe. 
But after some hours you will notice that your skills become better with each turn yo add :-) It would be interesting to know the DC resistance and L of one bucket.

73, Stefan

Am 17.02.2019 22:06, schrieb VIGILANT Luis Fern�ndez:
> Not me ! Unfortunately :(
>
> Still windong coils
>
> 73 de Luis
> EA5DOM
> ________________________________________
> De: owner-rsgb_lf_group@blacksheep.org 
> [owner-rsgb_lf_group@blacksheep.org] en nombre de DK7FC 
> [selberdenken@posteo.de]
> Enviado: domingo, 17 de febrero de 2019 16:18
> Para: rsgb_lf_group@blacksheep.org
> Asunto: VLF: 8270
>
> Hi VLF,
>
> Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus, 
> maybe it is Riccardo? It is a good signal  on the local grabbers such 
> as 
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html 
> or https://vlf.u01.de/
>
> Who is it ?
>
> 73, Stefan
>
>
>    



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Hi ELF,

Last Friday, 15th i started a 100 character EbNaut message on 22.97 Hz. 
The message took almost 84 hours! I think it is the longest EbNaut 
message transmision (without stacking) so far. It was interesting to 
follow the SNR of the reproduced spectrum peak during the transmission. 
Inbetween it seemed to become quite critical for a decode but then the 
night periods were quiet and in the end i got an easy decode.
The Spectrum peak shows 28.78 dB in 3.3 uHz.
Screen capture including processing chain is in the attachment.

73, Stefan


> Am 07.02.2019 17:05, schrieb DK7FC:
>> Hi ELF ;-)
>>
>> I'm glad to announce that since 15:46 UTC i am transmitting on ELF 
>> (the real ELF, i.e. into the range of 3...30 Hz, ITU radio band 1 
>> <https://en.wikipedia.org/wiki/Radio_spectrum#ITU> ) for the first 
>> time ever.
>>
>> Here are the parameters:
>>
>> TX frequency: *22.970 Hz*
>> Wavelength of that frequency: *13060 km*
>> Antenna voltage: *4.8 kV rms* (+ a DC component of 7.5 kV)
>> Antenna current: *325 uA*
>> ERP: 600 aW, or *6E-16 W*
>>
>> Call it QRP!
>> The goal is to detect the signal on my 3.5 km distant tree grabber, 
>> whose E field is now working again. Since the E field probe is not to 
>> far above the tree, the effective height is not as much as it should 
>> ideally be, at this frequency, so the RX is somewhat deaf. Anyway i 
>> can see the Schumann resonances and the 60 Hz power grid. So i hope 
>> it will work.
>>
>> A spectrogram which is centered on the frequency of interest in now 
>> shown at 
>> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html 
>> (3rd window). But maybe 424 uHz FFT bin width is even to optimistic! 
>> In a few minutes we'll see more :-) It takes about 40 minutes until a 
>> peak could have fully developed...
>>
>> 73, Stefan
>>

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Hi ELF, <br>
<br>
Last Friday, 15th i started a 100 character EbNaut message on 22.97 Hz.
The message took almost 84 hours! I think it is the longest EbNaut
message transmision (without stacking) so far. It was interesting to
follow the SNR of the reproduced spectrum peak during the transmission.
Inbetween it seemed to become quite critical for a decode but then the
night periods were quiet and in the end i got an easy decode.<br>
The Spectrum peak shows 28.78 dB in 3.3 uHz.<br>
Screen capture including processing chain is in the attachment.<br>
<br>
73, Stefan<br>
<br>
<br>
<blockquote cite="mid:5C62EBAD.9050904@posteo.de" type="cite">Am
07.02.2019 17:05, schrieb DK7FC:
  <blockquote cite="mid:5C5C5757.5080906@posteo.de" type="cite">
    <meta http-equiv="content-type"
 content="text/html; charset=ISO-8859-15">
Hi ELF ;-)<br>
    <br>
I'm glad to announce that since 15:46 UTC i am transmitting on ELF (the
real ELF, i.e. into the range of 3...30 Hz, <a moz-do-not-send="true"
 href="https://en.wikipedia.org/wiki/Radio_spectrum#ITU">ITU radio band
1</a> ) for the first time ever.<br>
    <br>
Here are the parameters: <br>
    <br>
TX frequency: <b>22.970 Hz</b><br>
Wavelength of that frequency: <b>13060 km</b><br>
Antenna voltage: <b>4.8 kV rms</b> (+ a DC component of 7.5 kV)<br>
Antenna current: <b>325 uA</b> <br>
ERP: 600 aW, or <b>6E-16 W</b><br>
    <br>
Call it QRP!<br>
The goal is to detect the signal on my 3.5 km distant tree grabber,
whose E field is now working again. Since the E field probe is not to
far above the tree, the effective height is not as much as it should
ideally be, at this frequency, so the RX is somewhat deaf. Anyway i can
see the Schumann resonances and the 60 Hz power grid. So i hope it will
work.<br>
    <br>
A spectrogram which is centered on the frequency of interest in now
shown at <a moz-do-not-send="true" class="moz-txt-link-freetext"
 href="http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html</a>
(3rd window). But maybe 424 uHz FFT bin width is even to optimistic! In
a few minutes we'll see more :-) It takes about 40 minutes until a peak
could have fully developed...<br>
    <br>
73, Stefan<br>
    <br>
  </blockquote>
</blockquote>
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From: "Stan, W1LE" <stanw1le@verizon.net>
Message-ID: <2de2a5e1-850b-4c7e-f91e-7ddf618aa1f2@verizon.net>
Date: Mon, 18 Feb 2019 08:49:08 -0500
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 Content preview:  Hello Luis, Thanks for the update. I am in the midst of starting
    to think about winding a loading coil for the 50 foot vertical in the front
    yard. 
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Subject: LF: Tricotosa Rotory Table
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Hello Luis,

Thanks for the update. I am in the midst of starting to think about 
winding a loading

coil for the 50 foot vertical in the front yard.

What is the revolutions per minute of your rotary table ?

What speed are you most comfortable with ?

I am also thinking of a nested "bucket brigade" for a tunable loading coil.

My initial thought was to use a lathe and I built up a jig to 
horizontally hold the 5 gallon plastic bucket.

Unfortunately I could not get the speed low enough to allow me to 
comfortably wind the single layer coil.

The lathe has a DC motor and the DC drive board could not be adjusted 
low enough. I think I need about

0-20 RPM. 0.02mm solid wire is about a #32 AWG or a #36 British WG, 
rated at ~ 90 milliamperes.

My initial thought was to use a wide double sticky tape at about 4 
locations on the bucket, about 90 degrees apart.

I am also considering a tape over the entire coil after winding to hold 
everything in place.

Another thought is a clear UV proof epoxy over the entire coil, to hold 
in place.

My concern is the derating of the current due to the reduced dissipation 
of heat in the covered coil.

Back to the drawing board..... My coil winding will start with #22 AWG 
from a 4.4 Kg spool.


Stan, W1LE   Cape Cod   FN41sr




On 2/18/2019 7:20 AM, VIGILANT Luis Fernández wrote:
> Hi Stefan, VLF
>
> The "Tricotosa" works nicely. Added a pedal to activate the motor, which is very useful
>
>

--------------6B6B590E5871724CA0A589D5
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<html>
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  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    <p><font size="+2" face="Consolas">Hello Luis,</font></p>
    <p><font size="+2" face="Consolas">Thanks for the update. I am in
        the midst of starting to think about winding a loading <br>
      </font></p>
    <p><font size="+2" face="Consolas">coil for the 50 foot vertical in
        the front yard.</font></p>
    <p><font size="+2" face="Consolas">What is the revolutions per
        minute of your rotary table ? <br>
      </font></p>
    <p><font size="+2" face="Consolas">What speed are you most
        comfortable with ?</font></p>
    <p><font size="+2" face="Consolas">I am also thinking of a nested
        "bucket brigade" for a tunable loading coil.</font></p>
    <p><font size="+2" face="Consolas">My initial thought was to use a
        lathe and I built up a jig to horizontally hold the 5 gallon
        plastic bucket.</font></p>
    <p><font size="+2" face="Consolas">Unfortunately I could not get the
        speed low enough to allow me to comfortably wind the single
        layer coil.</font></p>
    <p><font size="+2" face="Consolas">The lathe has a DC motor and the
        DC drive board could not be adjusted low enough. I think I need
        about <br>
      </font></p>
    <p><font size="+2" face="Consolas">0-20 RPM. 0.02mm solid wire is
        about a #32 AWG or a #36 British WG, rated at ~ 90 milliamperes.</font></p>
    <p><font size="+2" face="Consolas">My initial thought was to use a
        wide double sticky tape at about 4 locations on the bucket,
        about 90 degrees apart.</font></p>
    <p><font size="+2" face="Consolas">I am also considering a tape over
        the entire coil after winding to hold everything in place. <br>
      </font></p>
    <p><font size="+2" face="Consolas">Another thought is a clear UV
        proof epoxy over the entire coil, to hold in place. <br>
      </font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"><font
            face="Consolas">My concern is the derating of the current
            due to the reduced dissipation of heat in the covered coil.</font></font></font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"><font
            face="Consolas">Back to the drawing board..... My coil
            winding will start with #22 AWG from a 4.4 Kg spool.<br>
          </font></font></font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"><font
            face="Consolas"><br>
          </font></font></font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"><font
            face="Consolas">Stan, W1LE   Cape Cod   FN41sr</font><br>
        </font></font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"><br>
        </font></font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"><br>
        </font></font></p>
    <p><font size="+2"><font face="Courier New, Courier, monospace"></font></font><br>
    </p>
    <div class="moz-cite-prefix">On 2/18/2019 7:20 AM, VIGILANT Luis
      Fernández wrote:<br>
    </div>
    <blockquote type="cite"
cite="mid:6DB8451D7F3D3947A5918808A59621EA3152609C@servigilant.vigilant.local">
      <pre class="moz-quote-pre" wrap="">Hi Stefan, VLF

The "Tricotosa" works nicely. Added a pedal to activate the motor, which is very useful


</pre>
    </blockquote>
  </body>
</html>

--------------6B6B590E5871724CA0A589D5--

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 Content preview:  Maybe i can contribute something here: Luis' wire is 0.2 mm
    diameter, not 0.02 mm. I would recommend to use a bigger wire if you have
    enough space. 0.4 mm is much more comfortable to wind and it holds [...] 
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Maybe i can contribute something here:
Luis' wire is 0.2 mm diameter, not 0.02 mm.
I would recommend to use a bigger wire if you have enough space. 0.4 mm 
is much more comfortable to wind and it holds a 500 mA in a stacked 
configuration.
If your motor is to fast, just try to switch a resistor in series. This 
has the advantage that the torque, or the force which pulls the wire is 
lower and you can manually regulate the motor speed by holding the wire 
a bit stronger/lighter.
This has worked very well here.

73, Stefan

Am 18.02.2019 14:49, schrieb Stan, W1LE:
>
> Hello Luis,
>
> Thanks for the update. I am in the midst of starting to think about 
> winding a loading
>
> coil for the 50 foot vertical in the front yard.
>
> What is the revolutions per minute of your rotary table ?
>
> What speed are you most comfortable with ?
>
> I am also thinking of a nested "bucket brigade" for a tunable loading 
> coil.
>
> My initial thought was to use a lathe and I built up a jig to 
> horizontally hold the 5 gallon plastic bucket.
>
> Unfortunately I could not get the speed low enough to allow me to 
> comfortably wind the single layer coil.
>
> The lathe has a DC motor and the DC drive board could not be adjusted 
> low enough. I think I need about
>
> 0-20 RPM. 0.02mm solid wire is about a #32 AWG or a #36 British WG, 
> rated at ~ 90 milliamperes.
>
> My initial thought was to use a wide double sticky tape at about 4 
> locations on the bucket, about 90 degrees apart.
>
> I am also considering a tape over the entire coil after winding to 
> hold everything in place.
>
> Another thought is a clear UV proof epoxy over the entire coil, to 
> hold in place.
>
> My concern is the derating of the current due to the reduced 
> dissipation of heat in the covered coil.
>
> Back to the drawing board..... My coil winding will start with #22 AWG 
> from a 4.4 Kg spool.
>
>
> Stan, W1LE   Cape Cod   FN41sr
>
>
>
>
> On 2/18/2019 7:20 AM, VIGILANT Luis Fernández wrote:
>> Hi Stefan, VLF
>>
>> The "Tricotosa" works nicely. Added a pedal to activate the motor, which is very useful
>>
>>
>>      

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Maybe i can contribute something here:<br>
Luis' wire is 0.2 mm diameter, not 0.02 mm.<br>
I would recommend to use a bigger wire if you have enough space. 0.4 mm
is much more comfortable to wind and it holds a 500 mA in a stacked
configuration.<br>
If your motor is to fast, just try to switch a resistor in series. This
has the advantage that the torque, or the force which pulls the wire is
lower and you can manually regulate the motor speed by holding the wire
a bit stronger/lighter. <br>
This has worked very well here.<br>
<br>
73, Stefan<br>
<br>
Am 18.02.2019 14:49, schrieb Stan, W1LE:
<blockquote cite="mid:2de2a5e1-850b-4c7e-f91e-7ddf618aa1f2@verizon.net"
 type="cite">
  <meta http-equiv="Content-Type" content="text/html; charset=UTF-8">
  <p><font face="Consolas" size="+2">Hello Luis,</font></p>
  <p><font face="Consolas" size="+2">Thanks for the update. I am in the
midst of starting to think about winding a loading <br>
  </font></p>
  <p><font face="Consolas" size="+2">coil for the 50 foot vertical in
the front yard.</font></p>
  <p><font face="Consolas" size="+2">What is the revolutions per minute
of your rotary table ? <br>
  </font></p>
  <p><font face="Consolas" size="+2">What speed are you most
comfortable with ?</font></p>
  <p><font face="Consolas" size="+2">I am also thinking of a nested
"bucket brigade" for a tunable loading coil.</font></p>
  <p><font face="Consolas" size="+2">My initial thought was to use a
lathe and I built up a jig to horizontally hold the 5 gallon plastic
bucket.</font></p>
  <p><font face="Consolas" size="+2">Unfortunately I could not get the
speed low enough to allow me to comfortably wind the single layer coil.</font></p>
  <p><font face="Consolas" size="+2">The lathe has a DC motor and the
DC drive board could not be adjusted low enough. I think I need about <br>
  </font></p>
  <p><font face="Consolas" size="+2">0-20 RPM. 0.02mm solid wire is
about a #32 AWG or a #36 British WG, rated at ~ 90 milliamperes.</font></p>
  <p><font face="Consolas" size="+2">My initial thought was to use a
wide double sticky tape at about 4 locations on the bucket, about 90
degrees apart.</font></p>
  <p><font face="Consolas" size="+2">I am also considering a tape over
the entire coil after winding to hold everything in place. <br>
  </font></p>
  <p><font face="Consolas" size="+2">Another thought is a clear UV
proof epoxy over the entire coil, to hold in place. <br>
  </font></p>
  <p><font size="+2"><font face="Courier New, Courier, monospace"><font
 face="Consolas">My concern is the derating of the current due to the
reduced dissipation of heat in the covered coil.</font></font></font></p>
  <p><font size="+2"><font face="Courier New, Courier, monospace"><font
 face="Consolas">Back to the drawing board..... My coil winding will
start with #22 AWG from a 4.4 Kg spool.<br>
  </font></font></font></p>
  <p><font size="+2"><font face="Courier New, Courier, monospace"><font
 face="Consolas"><br>
  </font></font></font></p>
  <p><font size="+2"><font face="Courier New, Courier, monospace"><font
 face="Consolas">Stan, W1LE   Cape Cod   FN41sr</font><br>
  </font></font></p>
  <p><font size="+2"><font face="Courier New, Courier, monospace"><br>
  </font></font></p>
  <p><font size="+2"><font face="Courier New, Courier, monospace"><br>
  </font></font></p>
  <p><br>
  </p>
  <div class="moz-cite-prefix">On 2/18/2019 7:20 AM, VIGILANT Luis
Fernández wrote:<br>
  </div>
  <blockquote type="cite"
 cite="mid:6DB8451D7F3D3947A5918808A59621EA3152609C@servigilant.vigilant.local">
    <pre class="moz-quote-pre" wrap="">Hi Stefan, VLF

The "Tricotosa" works nicely. Added a pedal to activate the motor, which is very useful


    </pre>
  </blockquote>
</blockquote>
</body>
</html>

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From: "Stan, W1LE" <stanw1le@verizon.net>
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 Content preview:  Hello Stefan,  My typo, thanks for correcting. I just looked
    at the lathe 1.5 HP DC motor and it has 2 wires, so I should be able to add
    a variable power resistor. Thanks for the tip. I also took another look at
    the drive gear train and no other gear ratio choices are available. All of
    the extra gears are for the lead screw 
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Hello Stefan,  My typo, thanks for correcting.


I just looked at the lathe 1.5 HP DC motor and it has 2 wires, so I 
should be able to add a variable power resistor. Thanks for the tip.

I also took another look at the drive gear train and no other gear ratio 
choices are available. All of the extra gears are for the lead screw

adjustments to cut different pitch threads.


Stan



On 2/18/2019 9:14 AM, DK7FC wrote:
> Maybe i can contribute something here:
> Luis' wire is 0.2 mm diameter, not 0.02 mm.
>

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    <p><font size="+1" face="Consolas">Hello Stefan,  My typo, thanks
        for correcting.</font></p>
    <p><font size="+1" face="Consolas"><br>
      </font></p>
    <p><font size="+1" face="Consolas">I just looked at the lathe 1.5 HP
        DC motor and it has 2 wires, so I should be able to add a
        variable power resistor. Thanks for the tip.</font></p>
    <p><font size="+1" face="Consolas">I also took another look at the
        drive gear train and no other gear ratio choices are available.
        All of the extra gears are for the lead screw <br>
      </font></p>
    <p><font size="+1" face="Consolas">adjustments to cut different
        pitch threads.</font></p>
    <p><font size="+1" face="Consolas"><br>
      </font></p>
    <p><font size="+1" face="Consolas">Stan</font></p>
    <p><font size="+1" face="Consolas"><br>
      </font></p>
    <p><font size="+1" face="Consolas"></font><br>
    </p>
    <div class="moz-cite-prefix">On 2/18/2019 9:14 AM, DK7FC wrote:<br>
    </div>
    <blockquote type="cite" cite="mid:5C6ABDB1.7010209@posteo.de">
      <meta content="text/html; charset=UTF-8" http-equiv="Content-Type">
      Maybe i can contribute something here:<br>
      Luis' wire is 0.2 mm diameter, not 0.02 mm.<br>
      <br>
    </blockquote>
  </body>
</html>

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 Content preview:  Hi Stan, Stefan, Tricotosa Yes, I’m using 0.2mm wire. Unfortunately
    this was the thicker wire I could get and the price was very nice. So I will
    test with this and see what can I get before looking for 0.4mm wire 
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eT4NCjwvaHRtbD4NCg==

--_000_6DB8451D7F3D3947A5918808A59621EA3152627Cservigilantvigi_--

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From: Alex R7NT <r7nt.73@gmail.com>
Date: Mon, 18 Feb 2019 21:09:56 +0300
Message-ID: <CAL-VeeOmXBbdMVzNRNu2SSKWz2GHSh0dHXcRP4YbBXfbF37MEw@mail.gmail.com>
To: rsgb_lf_group@blacksheep.org, Chris Wilson <chris@chriswilson.tv>,
        bernhard.wiesgickl@asamnet.net, g0mrf@aol.com, k3mf@aol.com,
        k3rwr@md.metrocast.net, paul@n1bug.com
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 the administrator of that system for details.
 Content preview:  Dear LF enthusiasts, AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
    * 1. New database records have been added :* #679 QRB=6673,0 2019-02-17 K3MF
    -> DL0AO WSPR2 #680 QRB=7184,3 2019-02-17 G0MRF -> N4WLO WSPR2 
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                             identical to background
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Subject: LF: AWLF Updated 2019-02-18
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--000000000000f3694105822f08d9
Content-Type: text/plain; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

Dear LF enthusiasts,
 AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
* 1. New database records have been added :*

#679  QRB=3D6673,0  2019-02-17  K3MF     -> DL0AO  WSPR2

#680  QRB=3D7184,3  2019-02-17  G0MRF    -> N4WLO  WSPR2

#681  QRB=3D5564,1  2019-02-17  2E0ILY   -> WA3U   WSPR2

#682  QRB=3D5816,6  2019-02-18  K3RWR    -> G0MRF  WSPR2

#683  QRB=3D6496,3  2019-02-18  G0MRF    -> N8OOU  WSPR2

#684  QRB=3D5404,8  2019-02-18  N1BUG    -> DC0DX  WSPR2

#685  QRB=3D5761,3  2019-02-18  G0MRF    -> WB3AVN WSPR2



*2. Ratings have been updated :*
*N1BUG   *AWLF 6 TX Rating 1 =E2=86=91 AWLF 6 TX Hall of Fame #5 =E2=86=91 =
AWLF 7 TX Rating
3

*2E0ILY  *AWLF 2 Rating 1 =E2=86=91 AWLF 2 Hall of Fame #28 =E2=86=91 AWLF =
3 TX Rating 7
        AWLF 2 TX Rating 2 =E2=86=91 1

*K3MF    *AWLF 2 Rating 12 =E2=86=91 9
        AWLF 1 TX Rating 4 =E2=86=91 AWLF 1 TX Hall of Fame #34 =E2=86=91 A=
WLF 2 TX Rating
15

*G0MRF   *AWLF 2 Rating 26 =E2=86=91 8
        AWLF 2 Rating 13 =E2=86=91 8

        AWLF 1 RX Rating 118

*DL0AO   *AWLF 1 Rating 16 =E2=86=91 6
        AWLF 1 RX Rating 17 =E2=86=91 4

*WA3U    *AWLF 1 Rating 69 =E2=86=91 52
        AWLF 1 RX Rating 69 =E2=86=91 53

*DC0DX   *AWLF 1 Rating 126 =E2=86=91 80
        AWLF 1 RX Rating 131



*3. NEW ONE :*
*N4WLO   *AWLF 1 Rating 96
        AWLF 1 RX Rating 98

*N8OOU   *AWLF 1 Rating 101

        AWLF 1 RX Rating 106

*WB3AVN  *AWLF 1 Rating 116
        AWLF 1 RX Rating 122



*4. Some personal pdf files have been updated in "AWLF Data by Calls":*
*2E0ILY* *AWLF, **AWLF TX**   DC0DX* *AWLF, **AWLF RX**   DL0AO* *AWLF RX**
  G0MRF* *AWLF, **AWLF RX**, **AWLF TX**   K3MF* *AWLF**, AWLF TX**   K3RWR=
*
*AWLF**, AWLF TX**   N1BUG* *AWLF, **AWLF TX**   N4WLO* *AWLF RX**
N8OOU* *AWLF
RX**   WA3U* *AWLF RX**   WB3AVN* *AWLF RX*


*5. "Best QSOs" have been updated : *sorted in *QRB/Date* , *Chronological
order* , *Mode(Cat)/Date*
*NEW ONE 2way QSO* have been added: QRB=3D4736,1  2019-02-18  *N1BUG <>
2E0ILY JT9-1*
*http://136.73.ru/h_qso <http://136.73.ru/h_qso>http://136.73.ru/h_qso
<http://136.73.ru/h_qso>*     (maybe refresh frame)

73! Alex R7NT  *http://136.73.ru <http://136.73.ru/>*

--000000000000f3694105822f08d9
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;li=
ne-height:normal;background-image:initial;background-position:initial;backg=
round-size:initial;background-repeat:initial;background-origin:initial;back=
ground-clip:initial;font-size:11pt;font-family:Calibri,sans-serif"><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif">Dear LF e=
nthusiasts,<br>
=C2=A0AWLF=C2=A0</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-=
family:Arial,sans-serif;color:blue"><a href=3D"http://136.73.ru/h_aw" style=
=3D"color:blue">http://136.73.ru/h_aw</a></span></u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:Arial,sans-serif">=C2=A0=C2=A0</span><b><s=
pan lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quo=
t;"><br>
<u>1. New database records have been added :</u></span></b><u><span lang=3D=
"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif"></span></u></p=
>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#679=C2=A0=C2=A0QRB=
=3D6673,0=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-17=C2=A0 K3MF =
=C2=A0=C2=A0=C2=A0=C2=A0-&gt; DL0AO
=C2=A0WSPR2</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(23,59,211)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#680=C2=A0=C2=A0QRB=
=3D7184,3=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-17=C2=A0 G0MRF=
=C2=A0=C2=A0=C2=A0 -&gt; N4WLO
=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#681=C2=A0=C2=A0QRB=
=3D5564,1=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-17=C2=A0 2E0IL=
Y=C2=A0=C2=A0 -&gt; WA3U=C2=A0 =C2=A0WSPR2</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#682=C2=A0=C2=A0QRB=
=3D5816,6=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-18=C2=A0 K3RWR=
=C2=A0=C2=A0=C2=A0 -&gt; G0MRF
=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#683=C2=A0=C2=A0QRB=
=3D6496,3=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-18=C2=A0 G0MRF=
=C2=A0=C2=A0=C2=A0 -&gt; N8OOU
=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#684=C2=A0=C2=A0QRB=
=3D5404,8=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-18=C2=A0 N1BUG=
=C2=A0=C2=A0=C2=A0 -&gt; DC0DX
=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#685=C2=A0=C2=A0QRB=
=3D5761,3=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-18=C2=A0 G0MRF=
=C2=A0=C2=A0=C2=A0 -&gt; WB3AVN=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">2.=C2=A0Ratin=
gs have been
updated :</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"><br>
<b>N1BUG=C2=A0 =C2=A0</b></span><span lang=3D"EN-US" style=3D"font-size:9pt=
;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">AWLF 6 TX Rating 1=
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"=
font-size:9pt;font-family:&quot;Courier New&quot;;color:white;background:rg=
b(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A0</span><span l=
ang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;co=
lor:rgb(192,0,0)">AWLF 6 TX Hall of Fame #5 </span><span lang=3D"EN-US" sty=
le=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgro=
und:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size=
:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)"> AWLF 7 TX Rat=
ing 3</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;C=
ourier New&quot;;color:rgb(0,102,0)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">2E0I=
LY =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;;color:black">AWLF 2 Rating 1</span><span lang=3D"E=
N-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(=
191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-fam=
ily:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=E2=86=
=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">=C2=A0</span><span lang=3D"EN-US" style=3D"font=
-size:9pt;font-family:&quot;Courier New&quot;;color:black">AWLF 2 Hall of F=
ame #28</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot=
;Courier New&quot;;color:rgb(192,0,0)"> </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)"> </span><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;col=
or:black">AWLF 3 TX Rating 7</span><span lang=3D"EN-US" style=3D"font-size:=
9pt;font-family:&quot;Courier New&quot;;color:black"><br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">A=
WLF 2 TX Rating
2</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Couri=
er New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;background:r=
gb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;=
font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A0</span><span =
lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;c=
olor:rgb(192,0,0)">1</span><span lang=3D"EN-US" style=3D"font-size:9pt;font=
-family:&quot;Courier New&quot;;color:rgb(0,102,0)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">K3MF=
=C2=A0=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black">AWLF 2 Rating 12</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211=
)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black">=C2=A09<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">A=
WLF 1 TX Rating
4</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Couri=
er New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;background:r=
gb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;=
font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A0</span><span =
lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;c=
olor:rgb(192,0,0)">AWLF 1 TX Hall of Fame #34 </span><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backg=
round:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-si=
ze:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)"> AWLF 2 TX R=
ating 15</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;;color:rgb(0,102,0)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">G0MR=
F=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:black">AWLF 2 Rating 26 </span><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;col=
or:white;background:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)=
">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;;color:black">8</span><span lang=3D"EN-US" style=3D"font=
-size:9pt;font-family:&quot;Courier New&quot;;color:black"><br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">A=
WLF 2 Rating 13
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;col=
or:rgb(192,0,0)">=C2=A08</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=
=A0 =C2=A0 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(0,102,0)">AWLF 1 RX Rating 118</span><span=
 lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;=
color:rgb(192,0,0)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">DL0A=
O=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:black">AWLF 1 Rating 16</span><span lan=
g=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;colo=
r:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fo=
nt-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=
=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&qu=
ot;Courier New&quot;;color:black">=C2=A06<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
17</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A04</span></=
p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">WA3U=
=C2=A0=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black">AWLF 1 Rating 69</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211=
)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black">=C2=A052<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
69</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A053</span><=
/p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">DC0D=
X=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:black">AWLF 1 Rating 126</span><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;col=
or:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)">=
=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&qu=
ot;Courier New&quot;;color:black">=C2=A080<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
131</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">=C2=
=A0</span></b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">3.=C2=A0NEW O=
NE :</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black"><br>
<b>N4WLO=C2=A0 =C2=A0</b>AWLF 1 Rating 96<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
98</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">N8OO=
U=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:black">AWLF 1 Rating 101</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=
=A0 =C2=A0 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(0,102,0)">AWLF 1 RX Rating 106</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">WB3A=
VN =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family=
:&quot;Courier New&quot;;color:black">AWLF 1 Rating 116<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
122</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">=
=C2=A0</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">4.=C2=
=A0Some personal pdf files have been updated in
&quot;AWLF Data by Calls&quot;:</span></u></b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;"><br>
</span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">2E0ILY</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">A=
WLF TX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0DC0DX</span></b><b><=
span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&qu=
ot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-fam=
ily:&quot;Courier New&quot;;color:black">AWLF, </span></i></b><b><i><span l=
ang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;co=
lor:rgb(0,102,0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"fo=
nt-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0D=
L0AO</span></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"fon=
t-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX<=
/span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&q=
uot;Courier New&quot;;color:black"> =C2=A0=C2=A0G0MRF</span></b><b><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> <=
/span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&qu=
ot;Courier New&quot;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lan=
g=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;colo=
r:rgb(0,102,0)">AWLF RX</span></i></b><b><i><span lang=3D"EN-US" style=3D"f=
ont-size:8pt;font-family:&quot;Courier New&quot;;color:black">, </span></i>=
</b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Cou=
rier New&quot;;color:rgb(192,0,0)">AWLF TX</span></i></b><b><span lang=3D"E=
N-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:blac=
k"> =C2=A0=C2=A0K3MF</span></b><b><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><span lang=3D"EN-=
US" style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:black"=
>AWLF</span></i></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-=
family:&quot;Courier New&quot;;color:rgb(192,0,0)">,=C2=A0AWLF TX</span></i=
></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Couri=
er New&quot;;color:black">=C2=A0=C2=A0 K3RWR</span></b><b><span lang=3D"EN-=
US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b=
><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courie=
r New&quot;;color:black">AWLF</span></i></b><b><i><span lang=3D"EN-US" styl=
e=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">=
,=C2=A0AWLF TX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt=
;font-family:&quot;Courier New&quot;;color:black">=C2=A0=C2=A0 N1BUG</span>=
</b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;=
font-family:&quot;Courier New&quot;;color:black">AWLF,=C2=A0</span></i></b>=
<b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier=
 New&quot;;color:rgb(192,0,0)">AWLF TX</span></i></b><b><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =
=C2=A0=C2=A0N4WLO</span></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;=
font-family:&quot;Courier New&quot;"> </span></b><b><i><span lang=3D"EN-US"=
 style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102=
,0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0N8OOU</span></=
b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier =
New&quot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;fo=
nt-family:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b=
><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier N=
ew&quot;;color:black"> =C2=A0=C2=A0WA3U</span></b><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><=
i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New=
&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black"> =C2=
=A0=C2=A0WB3AVN</span></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;fo=
nt-family:&quot;Courier New&quot;"> </span></b><b><i><span lang=3D"EN-US" s=
tyle=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0=
)">AWLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0</span></b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;">5. &quot;Best QSO=
s&quot; have been updated :<br>
</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">sorted in=C2=A0</span><b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">QRB/=
Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" style=3D"f=
ont-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">Chrono=
logical order</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0=
)">Mode(Cat)/Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:black"><br>
</span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;">NEW ONE 2way QSO</span></b><span lang=3D"EN-US" style=3D"fo=
nt-size:9pt;font-family:&quot;Courier New&quot;"> have been added: QRB=3D47=
36,1=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-fam=
ily:&quot;Courier New&quot;;color:black">2019-02-18</span><span lang=3D"EN-=
US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,=
0,204)">=C2=A0 </span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;">N1BUG &lt;&gt; 2E0ILY JT9-1</span></b><span =
lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;c=
olor:black"><br>
</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,san=
s-serif;color:blue"><a href=3D"http://136.73.ru/h_qso" style=3D"color:blue"=
>http://136.73.ru/h_qso</a><a href=3D"http://136.73.ru/h_qso" style=3D"colo=
r:blue">http://136.73.ru/h_qso</a></span></u><span lang=3D"EN-US" style=3D"=
font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=A0(may=
be refresh frame)</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:Arial,sans-serif">73! Alex R7NT=C2=A0=C2=A0</spa=
n><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-ser=
if;color:blue"><a href=3D"http://136.73.ru/" style=3D"color:blue">http://13=
6.73.ru</a></span></u><span lang=3D"EN-US" style=3D"font-size:9pt;font-fami=
ly:Arial,sans-serif"></span></p></div>

--000000000000f3694105822f08d9--

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 Content preview:  Paul and Chris, 2200M propagation last night was indeed quite
    good. Well done on the JT9 TA QSO! 73, Rob - K3RWR 
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Paul and Chris,

2200M propagation last night was indeed quite good.  Well done on the JT9 TA QSO!

73,
Rob - K3RWR

> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
> 
> It is one of those special nights on LF.
> 
> I put a new exciter on this afternoon and was getting some early
> WSPR reports from across the Atlantic. During a failed QSO attempt
> with G0MRF, the class D amp blew my last set of FETs. I was
> discouraged but put the small class E amp back in so I could keep
> playing with the new exciter.
> 
> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
> be heard. Surprise! We had an easy QSO with just one repeat sequence
> required! Thank you Chris!
> 
> Now WSPR reports from Europe are getting even better. What else will
> this night bring?
> 
> 73,
> Paul N1BUG
> 



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From: Chris Wilson <dead.fets@gmail.com>
Date: Mon, 18 Feb 2019 19:34:29 +0000
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 Content preview:  Yes, the band is still full of surprises, I thank the dog
   for waking me up and me looking at the pc 😀 Best Regards Chris Wilson On
    Mon, 18 Feb 2019, 19:14 Rob Renoud 
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Subject: Re: LF: LF magic
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--00000000000058324d05823037a9
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Yes, the band is still full of surprises, I thank the dog for waking me up
and me looking at the pc =F0=9F=98=80

Best Regards
Chris Wilson

On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:

> Paul and Chris,
>
> 2200M propagation last night was indeed quite good.  Well done on the JT9
> TA QSO!
>
> 73,
> Rob - K3RWR
>
> > On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
> >
> > It is one of those special nights on LF.
> >
> > I put a new exciter on this afternoon and was getting some early
> > WSPR reports from across the Atlantic. During a failed QSO attempt
> > with G0MRF, the class D amp blew my last set of FETs. I was
> > discouraged but put the small class E amp back in so I could keep
> > playing with the new exciter.
> >
> > Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
> > be heard. Surprise! We had an easy QSO with just one repeat sequence
> > required! Thank you Chris!
> >
> > Now WSPR reports from Europe are getting even better. What else will
> > this night bring?
> >
> > 73,
> > Paul N1BUG
> >
>
>
>

--00000000000058324d05823037a9
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"auto">Yes, the band is still full of surprises, I thank the dog=
 for waking me up and me looking at the pc =F0=9F=98=80<br><br><div data-sm=
artmail=3D"gmail_signature">Best Regards<br>Chris Wilson</div></div><br><di=
v class=3D"gmail_quote"><div dir=3D"ltr">On Mon, 18 Feb 2019, 19:14 Rob Ren=
oud &lt;<a href=3D"mailto:k3rwr@md.metrocast.net">k3rwr@md.metrocast.net</a=
> wrote:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:0 0 0 .=
8ex;border-left:1px #ccc solid;padding-left:1ex">Paul and Chris,<br>
<br>
2200M propagation last night was indeed quite good.=C2=A0 Well done on the =
JT9 TA QSO!<br>
<br>
73,<br>
Rob - K3RWR<br>
<br>
&gt; On Feb 17, 2019, at 21:19, N1BUG &lt;<a href=3D"mailto:paul@n1bug.com"=
 target=3D"_blank" rel=3D"noreferrer">paul@n1bug.com</a>&gt; wrote:<br>
&gt; <br>
&gt; It is one of those special nights on LF.<br>
&gt; <br>
&gt; I put a new exciter on this afternoon and was getting some early<br>
&gt; WSPR reports from across the Atlantic. During a failed QSO attempt<br>
&gt; with G0MRF, the class D amp blew my last set of FETs. I was<br>
&gt; discouraged but put the small class E amp back in so I could keep<br>
&gt; playing with the new exciter.<br>
&gt; <br>
&gt; Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to<br=
>
&gt; be heard. Surprise! We had an easy QSO with just one repeat sequence<b=
r>
&gt; required! Thank you Chris!<br>
&gt; <br>
&gt; Now WSPR reports from Europe are getting even better. What else will<b=
r>
&gt; this night bring?<br>
&gt; <br>
&gt; 73,<br>
&gt; Paul N1BUG<br>
&gt; <br>
<br>
<br>
</blockquote></div>

--00000000000058324d05823037a9--

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 Content preview:  Give that dog my thanks too! Email on the way later, I've
   been busy making final adjustments and tests on the new exciter today. New
    exciter, exciting QSO. :-) Paul On 2/18/19 2:34 PM, Chris Wilson wrote: >
    Yes, the band is still full of surprises, I thank the dog for waking me up
    > and me looking at the pc 😀 > > Best Regards > Chris Wilson > > On Mon,
    18 Feb [...] 
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Give that dog my thanks too! Email on the way later, I've been busy
making final adjustments and tests on the new exciter today. New
exciter, exciting QSO. :-)

Paul


On 2/18/19 2:34 PM, Chris Wilson wrote:
> Yes, the band is still full of surprises, I thank the dog for waking me up
> and me looking at the pc 😀
> 
> Best Regards
> Chris Wilson
> 
> On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:
> 
>> Paul and Chris,
>>
>> 2200M propagation last night was indeed quite good.  Well done on the JT9
>> TA QSO!
>>
>> 73,
>> Rob - K3RWR
>>
>>> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
>>>
>>> It is one of those special nights on LF.
>>>
>>> I put a new exciter on this afternoon and was getting some early
>>> WSPR reports from across the Atlantic. During a failed QSO attempt
>>> with G0MRF, the class D amp blew my last set of FETs. I was
>>> discouraged but put the small class E amp back in so I could keep
>>> playing with the new exciter.
>>>
>>> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
>>> be heard. Surprise! We had an easy QSO with just one repeat sequence
>>> required! Thank you Chris!
>>>
>>> Now WSPR reports from Europe are getting even better. What else will
>>> this night bring?
>>>
>>> 73,
>>> Paul N1BUG

From owner-rsgb_lf_group@blacksheep.org  Tue Feb 19 16:47:57 2019
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From: Rik Strobbe <rik.strobbe@kuleuven.be>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: LF: LF magic
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 Content preview:  Hello Chris, so you trained the dog to watch the screen all
    night and wake you up when a DX call appears? I want such a dog too, what
    breed is it? 73, Rik ON7YD - OR7T 
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Subject: Re: LF: LF magic
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Hello Chris,

so you trained the dog to watch the screen all night and wake you up when a DX call appears?
I want such a dog too, what breed is it?

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens N1BUG <paul@n1bug.com>
Verzonden: maandag 18 februari 2019 21:17
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: Re: LF: LF magic

Give that dog my thanks too! Email on the way later, I've been busy
making final adjustments and tests on the new exciter today. New
exciter, exciting QSO. :-)

Paul


On 2/18/19 2:34 PM, Chris Wilson wrote:
> Yes, the band is still full of surprises, I thank the dog for waking me up
> and me looking at the pc 😀
>
> Best Regards
> Chris Wilson
>
> On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:
>
>> Paul and Chris,
>>
>> 2200M propagation last night was indeed quite good.  Well done on the JT9
>> TA QSO!
>>
>> 73,
>> Rob - K3RWR
>>
>>> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
>>>
>>> It is one of those special nights on LF.
>>>
>>> I put a new exciter on this afternoon and was getting some early
>>> WSPR reports from across the Atlantic. During a failed QSO attempt
>>> with G0MRF, the class D amp blew my last set of FETs. I was
>>> discouraged but put the small class E amp back in so I could keep
>>> playing with the new exciter.
>>>
>>> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
>>> be heard. Surprise! We had an easy QSO with just one repeat sequence
>>> required! Thank you Chris!
>>>
>>> Now WSPR reports from Europe are getting even better. What else will
>>> this night bring?
>>>
>>> 73,
>>> Paul N1BUG


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From: John Andrews <w1tag@charter.net>
Message-ID: <feace26c-574d-b968-f5f8-906870a47c57@charter.net>
Date: Tue, 19 Feb 2019 11:13:06 -0500
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 Content preview:  Rik, It depends on the mode. We use to use WOLFhounds, for
    example. John, W1TAG 
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Subject: Re: LF: LF magic
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Rik,

It depends on the mode. We use to use WOLFhounds, for example.

John, W1TAG

On 2/19/2019 10:36 AM, Rik Strobbe wrote:
> Hello Chris,
> 
> so you trained the dog to watch the screen all night and wake you up when a DX call appears?
> I want such a dog too, what breed is it?
> 
> 73, Rik  ON7YD - OR7T
> 
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens N1BUG <paul@n1bug.com>
> Verzonden: maandag 18 februari 2019 21:17
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: LF magic
> 
> Give that dog my thanks too! Email on the way later, I've been busy
> making final adjustments and tests on the new exciter today. New
> exciter, exciting QSO. :-)
> 
> Paul
> 
> 
> On 2/18/19 2:34 PM, Chris Wilson wrote:
>> Yes, the band is still full of surprises, I thank the dog for waking me up
>> and me looking at the pc 😀
>>
>> Best Regards
>> Chris Wilson
>>
>> On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:
>>
>>> Paul and Chris,
>>>
>>> 2200M propagation last night was indeed quite good.  Well done on the JT9
>>> TA QSO!
>>>
>>> 73,
>>> Rob - K3RWR
>>>
>>>> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
>>>>
>>>> It is one of those special nights on LF.
>>>>
>>>> I put a new exciter on this afternoon and was getting some early
>>>> WSPR reports from across the Atlantic. During a failed QSO attempt
>>>> with G0MRF, the class D amp blew my last set of FETs. I was
>>>> discouraged but put the small class E amp back in so I could keep
>>>> playing with the new exciter.
>>>>
>>>> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
>>>> be heard. Surprise! We had an easy QSO with just one repeat sequence
>>>> required! Thank you Chris!
>>>>
>>>> Now WSPR reports from Europe are getting even better. What else will
>>>> this night bring?
>>>>
>>>> 73,
>>>> Paul N1BUG
> 

From owner-rsgb_lf_group@blacksheep.org  Tue Feb 19 19:32:06 2019
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From: Rik Strobbe <rik.strobbe@kuleuven.be>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: LF: LF magic
Thread-Index: AQHUx74k0uPfNPYZw0GpI9eEigpBdqXl4a2AgAAMHoCAAVQVpv//+d4AgAA1Arw=
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 Content preview:  Aha, I got it. So I should be looking for a Japanese Terrier,
    I just hope I won't need 9 of them ... 73, Rik ON7YD - OR7T Van: owner-rsgb_lf_group@blacksheep.org
    <owner-rsgb_lf_group@blacksheep.org> namens John Andrews <w1tag@charter.net>
    Verzonden: dinsdag 19 februari 2019 17:13 [...] 
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Aha, I got it.
So I should be looking for a Japanese Terrier, I just hope I won't need 9 of them ...

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens John Andrews <w1tag@charter.net>
Verzonden: dinsdag 19 februari 2019 17:13
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: Re: LF: LF magic

Rik,

It depends on the mode. We use to use WOLFhounds, for example.

John, W1TAG

On 2/19/2019 10:36 AM, Rik Strobbe wrote:
> Hello Chris,
>
> so you trained the dog to watch the screen all night and wake you up when a DX call appears?
> I want such a dog too, what breed is it?
>
> 73, Rik  ON7YD - OR7T
>
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens N1BUG <paul@n1bug.com>
> Verzonden: maandag 18 februari 2019 21:17
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: LF magic
>
> Give that dog my thanks too! Email on the way later, I've been busy
> making final adjustments and tests on the new exciter today. New
> exciter, exciting QSO. :-)
>
> Paul
>
>
> On 2/18/19 2:34 PM, Chris Wilson wrote:
>> Yes, the band is still full of surprises, I thank the dog for waking me up
>> and me looking at the pc 😀
>>
>> Best Regards
>> Chris Wilson
>>
>> On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:
>>
>>> Paul and Chris,
>>>
>>> 2200M propagation last night was indeed quite good.  Well done on the JT9
>>> TA QSO!
>>>
>>> 73,
>>> Rob - K3RWR
>>>
>>>> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
>>>>
>>>> It is one of those special nights on LF.
>>>>
>>>> I put a new exciter on this afternoon and was getting some early
>>>> WSPR reports from across the Atlantic. During a failed QSO attempt
>>>> with G0MRF, the class D amp blew my last set of FETs. I was
>>>> discouraged but put the small class E amp back in so I could keep
>>>> playing with the new exciter.
>>>>
>>>> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
>>>> be heard. Surprise! We had an easy QSO with just one repeat sequence
>>>> required! Thank you Chris!
>>>>
>>>> Now WSPR reports from Europe are getting even better. What else will
>>>> this night bring?
>>>>
>>>> 73,
>>>> Paul N1BUG
>


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 Content preview:  John & All:  How about a Schrödinger's cat---if you can
    get it to come out of the box alive.... Mike wa3tts 
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John & All:=C2=A0 How about a=C2=A0Schr=C3=B6dinger's cat---if you can get =
it to come out of the box alive....
Mike wa3tts

-----Original Message-----
From: John Andrews <w1tag@charter.net>
To: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Sent: Tue, Feb 19, 2019 11:16 am
Subject: Re: LF: LF magic

Rik,

It depends on the mode. We use to use WOLFhounds, for example.

John, W1TAG

On 2/19/2019 10:36 AM, Rik Strobbe wrote:
> Hello Chris,
>=20
> so you trained the dog to watch the screen all night and wake you up when=
 a DX call appears?
> I want such a dog too, what breed is it?
>=20
> 73, Rik=C2=A0 ON7YD - OR7T
>=20
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.o=
rg> namens N1BUG <paul@n1bug.com>
> Verzonden: maandag 18 februari 2019 21:17
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: LF magic
>=20
> Give that dog my thanks too! Email on the way later, I've been busy
> making final adjustments and tests on the new exciter today. New
> exciter, exciting QSO. :-)
>=20
> Paul
>=20
>=20
> On 2/18/19 2:34 PM, Chris Wilson wrote:
>> Yes, the band is still full of surprises, I thank the dog for waking me =
up
>> and me looking at the pc =F0=9F=98=80
>>
>> Best Regards
>> Chris Wilson
>>
>> On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:
>>
>>> Paul and Chris,
>>>
>>> 2200M propagation last night was indeed quite good.=C2=A0 Well done on =
the JT9
>>> TA QSO!
>>>
>>> 73,
>>> Rob - K3RWR
>>>
>>>> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
>>>>
>>>> It is one of those special nights on LF.
>>>>
>>>> I put a new exciter on this afternoon and was getting some early
>>>> WSPR reports from across the Atlantic. During a failed QSO attempt
>>>> with G0MRF, the class D amp blew my last set of FETs. I was
>>>> discouraged but put the small class E amp back in so I could keep
>>>> playing with the new exciter.
>>>>
>>>> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to
>>>> be heard. Surprise! We had an easy QSO with just one repeat sequence
>>>> required! Thank you Chris!
>>>>
>>>> Now WSPR reports from Europe are getting even better. What else will
>>>> this night bring?
>>>>
>>>> 73,
>>>> Paul N1BUG
>=20


------=_Part_2051775_1305758086.1550632681877
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:12pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"font-family:arial,helvetica,sans-serif;font-size:10pt;=
color:black;"><br></div><div style=3D"font-family:arial,helvetica,sans-seri=
f;font-size:10pt;color:black;">John &amp; All:&nbsp; How about a&nbsp;<span=
 style=3D"font-weight: bold; color: rgb(106, 106, 106); font-family: Roboto=
, arial, sans-serif; font-size: small;">Schr=C3=B6dinger's cat---if you can=
 get it to come out of the box alive....</span></div><div style=3D""><font =
color=3D"#6a6a6a" face=3D"Roboto, arial, sans-serif" size=3D"2"><b><br></b>=
</font></div><div style=3D""><font color=3D"#6a6a6a" face=3D"Roboto, arial,=
 sans-serif" size=3D"2">Mike wa3tts</font><br><br><span style=3D"font-size:=
 10pt;">-----Original Message-----</span><br><span style=3D"font-size: 10pt=
;">From: John Andrews &lt;w1tag@charter.net&gt;</span><br><span style=3D"fo=
nt-size: 10pt;">To: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;</spa=
n><br><span style=3D"font-size: 10pt;">Sent: Tue, Feb 19, 2019 11:16 am</sp=
an><br><span style=3D"font-size: 10pt;">Subject: Re: LF: LF magic</span><br=
><br></div><div dir=3D"ltr">Rik,<br clear=3D"none"><br clear=3D"none">It de=
pends on the mode. We use to use WOLFhounds, for example.<br clear=3D"none"=
><br clear=3D"none">John, W1TAG<br clear=3D"none"><div class=3D"yqt33545190=
75" id=3D"yqtfd43069"><br clear=3D"none">On 2/19/2019 10:36 AM, Rik Strobbe=
 wrote:<br clear=3D"none">&gt; Hello Chris,<br clear=3D"none">&gt; <br clea=
r=3D"none">&gt; so you trained the dog to watch the screen all night and wa=
ke you up when a DX call appears?<br clear=3D"none">&gt; I want such a dog =
too, what breed is it?<br clear=3D"none">&gt; <br clear=3D"none">&gt; 73, R=
ik&nbsp; ON7YD - OR7T<br clear=3D"none">&gt; <br clear=3D"none">&gt; ______=
__________________________________<br clear=3D"none">&gt; Van: <a shape=3D"=
rect" ymailto=3D"mailto:owner-rsgb_lf_group@blacksheep.org" rel=3D"noopener=
 noreferrer" href=3D"mailto:owner-rsgb_lf_group@blacksheep.org">owner-rsgb_=
lf_group@blacksheep.org</a> &lt;<a shape=3D"rect" ymailto=3D"mailto:owner-r=
sgb_lf_group@blacksheep.org" rel=3D"noopener noreferrer" href=3D"mailto:own=
er-rsgb_lf_group@blacksheep.org">owner-rsgb_lf_group@blacksheep.org</a>&gt;=
 namens N1BUG &lt;<a shape=3D"rect" ymailto=3D"mailto:paul@n1bug.com" rel=
=3D"noopener noreferrer" href=3D"mailto:paul@n1bug.com">paul@n1bug.com</a>&=
gt;<br clear=3D"none">&gt; Verzonden: maandag 18 februari 2019 21:17<br cle=
ar=3D"none">&gt; Aan: <a shape=3D"rect" ymailto=3D"mailto:rsgb_lf_group@bla=
cksheep.org" rel=3D"noopener noreferrer" href=3D"mailto:rsgb_lf_group@black=
sheep.org">rsgb_lf_group@blacksheep.org</a><br clear=3D"none">&gt; Onderwer=
p: Re: LF: LF magic<br clear=3D"none">&gt; <br clear=3D"none">&gt; Give tha=
t dog my thanks too! Email on the way later, I've been busy<br clear=3D"non=
e">&gt; making final adjustments and tests on the new exciter today. New<br=
 clear=3D"none">&gt; exciter, exciting QSO. :-)<br clear=3D"none">&gt; <br =
clear=3D"none">&gt; Paul<br clear=3D"none">&gt; <br clear=3D"none">&gt; <br=
 clear=3D"none">&gt; On 2/18/19 2:34 PM, Chris Wilson wrote:<br clear=3D"no=
ne">&gt;&gt; Yes, the band is still full of surprises, I thank the dog for =
waking me up<br clear=3D"none">&gt;&gt; and me looking at the pc =F0=9F=98=
=80<br clear=3D"none">&gt;&gt;<br clear=3D"none">&gt;&gt; Best Regards<br c=
lear=3D"none">&gt;&gt; Chris Wilson<br clear=3D"none">&gt;&gt;<br clear=3D"=
none">&gt;&gt; On Mon, 18 Feb 2019, 19:14 Rob Renoud &lt;<a shape=3D"rect" =
ymailto=3D"mailto:k3rwr@md.metrocast.net" rel=3D"noopener noreferrer" href=
=3D"mailto:k3rwr@md.metrocast.net">k3rwr@md.metrocast.net</a> wrote:<br cle=
ar=3D"none">&gt;&gt;<br clear=3D"none">&gt;&gt;&gt; Paul and Chris,<br clea=
r=3D"none">&gt;&gt;&gt;<br clear=3D"none">&gt;&gt;&gt; 2200M propagation la=
st night was indeed quite good.&nbsp; Well done on the JT9<br clear=3D"none=
">&gt;&gt;&gt; TA QSO!<br clear=3D"none">&gt;&gt;&gt;<br clear=3D"none">&gt=
;&gt;&gt; 73,<br clear=3D"none">&gt;&gt;&gt; Rob - K3RWR<br clear=3D"none">=
&gt;&gt;&gt;<br clear=3D"none">&gt;&gt;&gt;&gt; On Feb 17, 2019, at 21:19, =
N1BUG &lt;<a shape=3D"rect" ymailto=3D"mailto:paul@n1bug.com" rel=3D"noopen=
er noreferrer" href=3D"mailto:paul@n1bug.com">paul@n1bug.com</a>&gt; wrote:=
<br clear=3D"none">&gt;&gt;&gt;&gt;<br clear=3D"none">&gt;&gt;&gt;&gt; It i=
s one of those special nights on LF.<br clear=3D"none">&gt;&gt;&gt;&gt;<br =
clear=3D"none">&gt;&gt;&gt;&gt; I put a new exciter on this afternoon and w=
as getting some early<br clear=3D"none">&gt;&gt;&gt;&gt; WSPR reports from =
across the Atlantic. During a failed QSO attempt<br clear=3D"none">&gt;&gt;=
&gt;&gt; with G0MRF, the class D amp blew my last set of FETs. I was<br cle=
ar=3D"none">&gt;&gt;&gt;&gt; discouraged but put the small class E amp back=
 in so I could keep<br clear=3D"none">&gt;&gt;&gt;&gt; playing with the new=
 exciter.<br clear=3D"none">&gt;&gt;&gt;&gt;<br clear=3D"none">&gt;&gt;&gt;=
&gt; Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to<br=
 clear=3D"none">&gt;&gt;&gt;&gt; be heard. Surprise! We had an easy QSO wit=
h just one repeat sequence<br clear=3D"none">&gt;&gt;&gt;&gt; required! Tha=
nk you Chris!<br clear=3D"none">&gt;&gt;&gt;&gt;<br clear=3D"none">&gt;&gt;=
&gt;&gt; Now WSPR reports from Europe are getting even better. What else wi=
ll<br clear=3D"none">&gt;&gt;&gt;&gt; this night bring?<br clear=3D"none">&=
gt;&gt;&gt;&gt;<br clear=3D"none">&gt;&gt;&gt;&gt; 73,<br clear=3D"none">&g=
t;&gt;&gt;&gt; Paul N1BUG<br clear=3D"none">&gt; <br clear=3D"none"><br cle=
ar=3D"none"></div></div></div>
------=_Part_2051775_1305758086.1550632681877--

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 Content preview:  An Ape would definetly be the right choice But I'm afraid
   you would find him using FT8 sooner or later ! ;-) 73 de Luis EA5DOM 
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Subject: RE: LF: LF magic
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An Ape would definetly be the right choice

But I'm afraid you would find him using FT8 sooner or later ! ;-)

73 de Luis
EA5DOM

-----Mensaje original-----
De: owner-rsgb_lf_group@blacksheep.org [mailto:owner-rsgb_lf_group@blacksheep.org] En nombre de Rik Strobbe
Enviado el: martes, 19 de febrero de 2019 19:26
Para: rsgb_lf_group@blacksheep.org
Asunto: Re: LF: LF magic

Aha, I got it.
So I should be looking for a Japanese Terrier, I just hope I won't need 9 of them ...

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens John Andrews <w1tag@charter.net>
Verzonden: dinsdag 19 februari 2019 17:13
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: Re: LF: LF magic

Rik,

It depends on the mode. We use to use WOLFhounds, for example.

John, W1TAG

On 2/19/2019 10:36 AM, Rik Strobbe wrote:
> Hello Chris,
>
> so you trained the dog to watch the screen all night and wake you up when a DX call appears?
> I want such a dog too, what breed is it?
>
> 73, Rik  ON7YD - OR7T
>
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org 
> <owner-rsgb_lf_group@blacksheep.org> namens N1BUG <paul@n1bug.com>
> Verzonden: maandag 18 februari 2019 21:17
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: LF magic
>
> Give that dog my thanks too! Email on the way later, I've been busy 
> making final adjustments and tests on the new exciter today. New 
> exciter, exciting QSO. :-)
>
> Paul
>
>
> On 2/18/19 2:34 PM, Chris Wilson wrote:
>> Yes, the band is still full of surprises, I thank the dog for waking 
>> me up and me looking at the pc 😀
>>
>> Best Regards
>> Chris Wilson
>>
>> On Mon, 18 Feb 2019, 19:14 Rob Renoud <k3rwr@md.metrocast.net wrote:
>>
>>> Paul and Chris,
>>>
>>> 2200M propagation last night was indeed quite good.  Well done on 
>>> the JT9 TA QSO!
>>>
>>> 73,
>>> Rob - K3RWR
>>>
>>>> On Feb 17, 2019, at 21:19, N1BUG <paul@n1bug.com> wrote:
>>>>
>>>> It is one of those special nights on LF.
>>>>
>>>> I put a new exciter on this afternoon and was getting some early 
>>>> WSPR reports from across the Atlantic. During a failed QSO attempt 
>>>> with G0MRF, the class D amp blew my last set of FETs. I was 
>>>> discouraged but put the small class E amp back in so I could keep 
>>>> playing with the new exciter.
>>>>
>>>> Then I saw 2E0ILY calling CQ on JT9-1. I answered, not expecting to 
>>>> be heard. Surprise! We had an easy QSO with just one repeat 
>>>> sequence required! Thank you Chris!
>>>>
>>>> Now WSPR reports from Europe are getting even better. What else 
>>>> will this night bring?
>>>>
>>>> 73,
>>>> Paul N1BUG
>


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 Content preview:  Hi All Transformer is ready. https://klubnl.pl/wpr/en/index.php/artykuly/uniwersalny-nadawczy-autotransformator-antenowy-na-pasma-827khz-136khz-i-472khz/
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Hi All
Transformer is ready.
https://klubnl.pl/wpr/en/index.php/artykuly/uniwersalny-nadawczy-autotransformator-antenowy-na-pasma-827khz-136khz-i-472khz/
73! Marcin SQ2BXI

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> On Behalf Of Marcin
Sent: Friday, February 15, 2019 5:56 AM
To: rsgb_lf_group@blacksheep.org
Subject: RE: R: Re: VLF: in VK?

Hello VLF!
The primary coil of the transformer is ready. 10 turns (diameter 2mm) give 9.62mH which gives about xl=500Ohms at 8.27kHz. It is a good idea!

73! Marcin SQ2BXI

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> On Behalf Of Marcin
Sent: Monday, February 11, 2019 4:55 PM
To: rsgb_lf_group@blacksheep.org
Subject: RE: R: Re: VLF: in VK?

Hello Stefan!

Today, the ferrite cores B64290L82X830 came to me. I'm building a transformer 1:1/1:4/1:9/1:16 and 1/25 on the VLF. I'll check if it works soon.
73! Marcin SQ2BXI

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> On Behalf Of DK7FC
Sent: Monday, February 11, 2019 2:50 PM
To: rsgb_lf_group@blacksheep.org
Subject: Re: R: Re: VLF: in VK?

Hi Dimitris, VLF,

Am 11.02.2019 01:07, schrieb Dimitrios Tsifakis:
> I have an idea about impedance transformation and that is to use high 
> power 70V/100V audio distribution transformers at both ends. I don't 
> have to go to 50 ohm as I don't use the coaxial cable as a 
> transmission line (it's only a tiny percentage of the wavelength!), so 
> I could use a 4 ohm to 400 ohm transformer or similar. I think in 
> general the impedance transformation ratio goes down as the power 
> rating goes up and we can live with that. THe audio transformer should 
> work fine on the higher frequency but that will have to be tested.
> Perhaps something like this but not at that price!!
>
> https://www.altronics.com.au/p/m1160-300w-100v-line-pa-transformer/
>
> Another option is to get a PA amplifier of suitable power output that 
> has a 70V or 100V output. You only need one transformer at the antenna 
> end to get down to 4 ohm to reduce losses. I have a 50 W amp with such 
> output but that's not enough power.
>    
These high power audio transformers are interesting. I wonder how well they work below 1 kHz. But they are to expensive, as you say. You don't need them. For any impedance transformation above 1 kHz i use ordinary
N30 ferrite toroids. There may be slightly better core materials but i'm getting very good results and they are not expensive and you can find them at many distributors (min quantity = 1, not 50000000000000000000000000). Especially at VLF they are well suitable and not expensive.
One of my preferred cores is that one: 
https://www.buerklin.com/en/ring-core-outer--x-inner--x-height--63-x-38-x-25-mm-n30/p/84d258
It works easily for a few hundret watts on all VLF frequencies.

Yes you don't need to match the cable impedance but the losses on your cable are caused by the current and resistance of the wire and so, if you transform from 4 Ohm to 50 Ohm, then your losses drop by 92 %, regardless if it is necessary to match the cable impedance.

> I can easily try the ground loop on the 120m long antenna as I do have 
> ground rods at both ends. It would be interesting to compare the 
> signal strength in both cases. THat's why I am building a network of 
> VLF stations by giving away the large ferrite rods to interested 
> amateurs! They can help doing comparisons like this.
>    
Yes, sure. Good luck in getting people motivated to build up a permanent VLF RX station. It would also be good to have someone building up a grabber site or maybe even providing a stream. Your activity can cause a world wide motivation for people who are principally interested in VLF reception and/or transmission, even if they won't be able to receive you from so far away.

> The ground is very rocky and there is almost no soil at the top.
> Typical Australian native vegetation is the only thing that can 
> survive on it. I have thought about the dipole on the ground and I 
> have the perfect spot for it which is putting the feed point at the 
> top of the hill therefore making an inverted-V :-) Only concern with 
> that is the high voltage at the end of the dipole wires and the 
> possibility of a bush fire ignition. Definitely a project for winter!
> I have tried to tune my ~120 metre wire to VLF in the past with mixed 
> results. Worth revisiting this. The wire basically starts at my house 
> and follows the hill resulting in the top of the wire being maybe 20 
> metres higher than the bottom.
>    
I'm taking part in your experiments by imagining that i would be in your position :-) My latest thought is that a few (wooden?) poles of 10m height or so would be ideal. One is close to the house, and then two more in 100m distance from the house, e.g. here: 
http://k7fry.com/grid/?qth=QF44OX00PV&from=QF44OX00LN
The 2x 100m dipole could be connected using a good HF ladder line down to the shack.
Aluminium wire is light weight and cheap and the lower conductivity could be compensated by using a higher diameter, something like this,
https://www.amazon.de/dp/B004UA7XT2
This antenna would have the advantage that you can use it from MF to DC and the kangaroos would not be able to destroy the antenna.
For VLF experiments, the ends of the wire can be grounded, just by adding another 100m of wire at the ends and let them slope down, maybe with another pole at 4m height.


73, Stefan




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Date: Fri, 22 Feb 2019 11:27:04 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  This week the EbNaut autodecoders at DL0AO and DF6NM have
    been refurbished, producing more compact output with one line for each successful
    decode. My current script and required utilities are here [...] 
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Subject: Re: LF: VO1NA 137477 Hz
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------=_Part_3467999_1522011633.1550834824124
Content-Type: text/plain; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

This week=C2=A0the EbNaut autodecoders at DL0AO and DF6NM have been refurbi=
shed, producing more compact output with one line for each successful decod=
e. My current=C2=A0script=C2=A0and required utilities are here:
http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip

Our autodecoders are currently observing 137477 Hz. Until yesterday, VO1NA =
has been making strong and consistent decodes every night. Today I'm doing =
a few of low-power daytime tests on his QRG, with the LEA-6T barefoot to th=
e antenna.

Best 73,
Markus (DF6NM)


-----Urspr=C3=BCngliche Mitteilung-----
Von: Markus Vester <markusvester@aol.com>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Sa, 22. Dez 2018 14:55
Betreff: LF: VO1NA 137477 Hz

Hi Joe,=20

the carrier on your frequency is nicely visible night and day.=C2=A0When th=
e signal is strong, some=C2=A0symmetrical sidebands become visible, are you=
=C2=A0still modulating with 7 char EbNaut messages every other half hour?=
=C2=A0

I've placed=C2=A0my=C2=A0current autodecoder scripts here
but note that=C2=A0this setup is driven by=C2=A0opds and sort of specific t=
o my LF grabber. For Linux, you may want to start from the scripts which Do=
menico has recently posted.

Best 73,
Markus=C2=A0(DF6NM)



-----Urspr=C3=BCngliche Mitteilung-----
Von: jcraig <jcraig@mun.ca>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Mo, 17. Dez 2018 22:53
Betreff: Re: LF: EbNaut 137.542 kHz

Hi Markus, Stefan EbNauters,

Thanks for the reports and autodetectors.=C2=A0 The TX carrier is on
continuously at 50 watts with the excitation XOR phase inverted
by Paul's Ebkey.c on a raspi3.

There have been some daytime decodes recently.

Is the autodetect easy to set up?=C2=A0 If not perhaps I'd best
review the advice from you and Stefan again.

73
Joe

------=_Part_3467999_1522011633.1550834824124
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"299">This week&nbsp;the EbNaut autodecoders at DL=
0AO and DF6NM have been refurbished, producing more compact output with one=
 line for each successful decode. My current&nbsp;script&nbsp;and required =
utilities are here:<br>http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autode=
code_scripts.zip<br abp=3D"319"><br>Our autodecoders are currently observin=
g 137477 Hz. Until yesterday, VO1NA has been making strong and consistent d=
ecodes every night. Today I'm doing a few of low-power daytime tests on his=
 QRG, with the LEA-6T barefoot to the antenna.<br><br>Best 73,<br>Markus (D=
F6NM)<br><br><br abp=3D"302">-----Urspr=C3=BCngliche Mitteilung-----<br abp=
=3D"303">Von: Markus Vester &lt;markusvester@aol.com&gt;<br abp=3D"304">An:=
 rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br abp=3D"305">Verschic=
kt: Sa, 22. Dez 2018 14:55<br abp=3D"306">Betreff: LF: VO1NA 137477 Hz<br a=
bp=3D"307"><br abp=3D"308"></div><div id=3D"yiv1297951877" abp=3D"309"><div=
 style=3D"color: black; font-family: arial, helvetica, sans-serif; font-siz=
e: 10pt;" abp=3D"310"><div id=3D"yiv1297951877" abp=3D"311"><div style=3D"c=
olor: black; font-family: arial, helvetica, sans-serif; font-size: 10pt;" a=
bp=3D"312"><div style=3D"color: black; font-family: arial, helvetica, sans-=
serif; font-size: 10pt;" abp=3D"313">Hi Joe, <br abp=3D"314"><br abp=3D"315=
">the carrier on your frequency is nicely visible night and day.&nbsp;When =
the signal is strong, some&nbsp;symmetrical sidebands become visible, are y=
ou&nbsp;still modulating with 7 char EbNaut messages every other half hour?=
&nbsp;<br abp=3D"316"><br abp=3D"317">I've placed&nbsp;my&nbsp;current auto=
decoder scripts here<br abp=3D"318">but note that&nbsp;this setup is driven=
 by&nbsp;opds and sort of specific to my LF grabber. For Linux, you may wan=
t to start from the scripts which Domenico has recently posted.<br abp=3D"3=
20"><br abp=3D"321">Best 73,<br abp=3D"322">Markus&nbsp;(DF6NM)<br abp=3D"3=
23"><br abp=3D"324"><br abp=3D"325"><br abp=3D"326">-----Urspr=C3=BCngliche=
 Mitteilung-----<br abp=3D"327">Von: jcraig &lt;jcraig@mun.ca&gt;<br abp=3D=
"328">An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br abp=3D"329"=
>Verschickt: Mo, 17. Dez 2018 22:53<br abp=3D"330">Betreff: Re: LF: EbNaut =
137.542 kHz<br abp=3D"331"><br abp=3D"332"></div><div dir=3D"ltr" abp=3D"33=
3">Hi Markus, Stefan EbNauters,<br clear=3D"none" abp=3D"334"><br clear=3D"=
none" abp=3D"335">Thanks for the reports and autodetectors.&nbsp; The TX ca=
rrier is on<br clear=3D"none" abp=3D"336">continuously at 50 watts with the=
 excitation XOR phase inverted<br clear=3D"none" abp=3D"337">by Paul's Ebke=
y.c on a raspi3.<br clear=3D"none" abp=3D"338"><br clear=3D"none" abp=3D"33=
9">There have been some daytime decodes recently.<br clear=3D"none" abp=3D"=
340"><br clear=3D"none" abp=3D"341">Is the autodetect easy to set up?&nbsp;=
 If not perhaps I'd best<br clear=3D"none" abp=3D"342">review the advice fr=
om you and Stefan again.<br clear=3D"none" abp=3D"343"><br clear=3D"none" a=
bp=3D"344">73<br clear=3D"none" abp=3D"345">Joe<br clear=3D"none" abp=3D"34=
6"></div></div></div></div></div></div>
------=_Part_3467999_1522011633.1550834824124--

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 Content preview:  Markus, group, Thank-you for the insipiring anecdotes and
   signal reports. I am sad to report that my dad G3LMD/ VO1FB became a silent
    key yeserday morning. 73 Joe VO1NA 
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Subject: Re: LF: VO1NA 137477 Hz
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Markus, group,

Thank-you for the insipiring anecdotes and signal reports.
I am sad to report that my dad  G3LMD/ VO1FB became a silent key
yeserday morning.

73
Joe VO1NA

On Fri, 22 Feb 2019, Markus Vester wrote:

> This week=C2=A0the EbNaut autodecoders at DL0AO and DF6NM have been refur=
bished, producing more compact output with one line for each successful dec=
ode. My current=C2=A0script=C2=A0and required utilities are here:
> http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip
>
> Our autodecoders are currently observing 137477 Hz. Until yesterday, VO1N=
A has been making strong and consistent decodes every night. Today I'm doin=
g a few of low-power daytime tests on his QRG, with the LEA-6T barefoot to =
the antenna.
>
> Best 73,
> Markus (DF6NM)
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: Markus Vester <markusvester@aol.com>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Sa, 22. Dez 2018 14:55
> Betreff: LF: VO1NA 137477 Hz
>
> Hi Joe,
>
> the carrier on your frequency is nicely visible night and day.=C2=A0When =
the signal is strong, some=C2=A0symmetrical sidebands become visible, are y=
ou=C2=A0still modulating with 7 char EbNaut messages every other half hour?=
=C2=A0
>
> I've placed=C2=A0my=C2=A0current autodecoder scripts here
> but note that=C2=A0this setup is driven by=C2=A0opds and sort of specific=
 to my LF grabber. For Linux, you may want to start from the scripts which =
Domenico has recently posted.
>
> Best 73,
> Markus=C2=A0(DF6NM)
>
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: jcraig <jcraig@mun.ca>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Mo, 17. Dez 2018 22:53
> Betreff: Re: LF: EbNaut 137.542 kHz
>
> Hi Markus, Stefan EbNauters,
>
> Thanks for the reports and autodetectors.=C2=A0 The TX carrier is on
> continuously at 50 watts with the excitation XOR phase inverted
> by Paul's Ebkey.c on a raspi3.
>
> There have been some daytime decodes recently.
>
> Is the autodetect easy to set up?=C2=A0 If not perhaps I'd best
> review the advice from you and Stefan again.
>
> 73
> Joe
>
---1719232024-173815503-1550839829=:23134--

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Date: Fri, 22 Feb 2019 12:58:03 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
Message-ID: <1671197972.3501357.1550840283306@mail.yahoo.com>
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 Content preview:  Joe, I'm sorry to read that. May he rest in peace! All the
    best to you and yours, Markus 
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Subject: Re: LF: VO1NA 137477 Hz
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Joe, I'm sorry to read that. May he rest in peace!

All the best to you and yours,

Markus


-----Urspr=C3=BCngliche Mitteilung-----
Von: jcraig <jcraig@mun.ca>
An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Verschickt: Fr, 22. Feb. 2019 13:53
Betreff: Re: LF: VO1NA 137477 Hz

Markus, group,

Thank-you for the insipiring anecdotes and signal reports.
I am sad to report that my dad=C2=A0 G3LMD/ VO1FB became a silent key
yeserday morning.

73
Joe VO1NA

On Fri, 22 Feb 2019, Markus Vester wrote:

> This week=C2=A0the EbNaut autodecoders at DL0AO and DF6NM have been refur=
bished, producing more compact output with one line for each successful dec=
ode. My current=C2=A0script=C2=A0and required utilities are here:
> http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip
>
> Our autodecoders are currently observing 137477 Hz. Until yesterday, VO1N=
A has been making strong and consistent decodes every night. Today I'm doin=
g a few of low-power daytime tests on his QRG, with the LEA-6T barefoot to =
the antenna.
>
> Best 73,
> Markus (DF6NM)
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: Markus Vester <markusvester@aol.com>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Sa, 22. Dez 2018 14:55
> Betreff: LF: VO1NA 137477 Hz
>
> Hi Joe,
>
> the carrier on your frequency is nicely visible night and day.=C2=A0When =
the signal is strong, some=C2=A0symmetrical sidebands become visible, are y=
ou=C2=A0still modulating with 7 char EbNaut messages every other half hour?=
=C2=A0
>
> I've placed=C2=A0my=C2=A0current autodecoder scripts here
> but note that=C2=A0this setup is driven by=C2=A0opds and sort of specific=
 to my LF grabber. For Linux, you may want to start from the scripts which =
Domenico has recently posted.
>
> Best 73,
> Markus=C2=A0(DF6NM)
>
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: jcraig <jcraig@mun.ca>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Mo, 17. Dez 2018 22:53
> Betreff: Re: LF: EbNaut 137.542 kHz
>
> Hi Markus, Stefan EbNauters,
>
> Thanks for the reports and autodetectors.=C2=A0 The TX carrier is on
> continuously at 50 watts with the excitation XOR phase inverted
> by Paul's Ebkey.c on a raspi3.
>
> There have been some daytime decodes recently.
>
> Is the autodetect easy to set up?=C2=A0 If not perhaps I'd best
> review the advice from you and Stefan again.
>
> 73
> Joe
>
------=_Part_3501356_506240969.1550840283304
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"675">Joe, I'm sorry to read that. May he rest in =
peace!<br><br>All the best to you and yours,<br><br>Markus<br abp=3D"676"><=
br abp=3D"677"><br abp=3D"678">-----Urspr=C3=BCngliche Mitteilung-----<br a=
bp=3D"679">Von: jcraig &lt;jcraig@mun.ca&gt;<br abp=3D"680">An: rsgb_lf_gro=
up &lt;rsgb_lf_group@blacksheep.org&gt;<br abp=3D"681">Verschickt: Fr, 22. =
Feb. 2019 13:53<br abp=3D"682">Betreff: Re: LF: VO1NA 137477 Hz<br abp=3D"6=
83"><br abp=3D"684"></div><div dir=3D"ltr" abp=3D"685">Markus, group,<br cl=
ear=3D"none" abp=3D"686"><br clear=3D"none" abp=3D"687">Thank-you for the i=
nsipiring anecdotes and signal reports.<br clear=3D"none" abp=3D"688">I am =
sad to report that my dad&nbsp; G3LMD/ VO1FB became a silent key<br clear=
=3D"none" abp=3D"689">yeserday morning.<br clear=3D"none" abp=3D"690"><br c=
lear=3D"none" abp=3D"691">73<br clear=3D"none" abp=3D"692">Joe VO1NA<br cle=
ar=3D"none" abp=3D"693"><div class=3D"yqt6286295739" id=3D"yqtfd76526" abp=
=3D"694"><br clear=3D"none" abp=3D"695">On Fri, 22 Feb 2019, Markus Vester =
wrote:<br clear=3D"none" abp=3D"696"><br clear=3D"none" abp=3D"697">&gt; Th=
is week&nbsp;the EbNaut autodecoders at DL0AO and DF6NM have been refurbish=
ed, producing more compact output with one line for each successful decode.=
 My current&nbsp;script&nbsp;and required utilities are here:<br clear=3D"n=
one" abp=3D"698">&gt; <a href=3D"http://df6nm.bplaced.net/VLF/fec_tests/ebn=
aut_autodecode_scripts.zip" target=3D"_blank" rel=3D"noopener noreferrer" s=
hape=3D"rect" abp=3D"699">http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_aut=
odecode_scripts.zip</a><br clear=3D"none" abp=3D"700">&gt;<br clear=3D"none=
" abp=3D"701">&gt; Our autodecoders are currently observing 137477 Hz. Unti=
l yesterday, VO1NA has been making strong and consistent decodes every nigh=
t. Today I'm doing a few of low-power daytime tests on his QRG, with the LE=
A-6T barefoot to the antenna.<br clear=3D"none" abp=3D"702">&gt;<br clear=
=3D"none" abp=3D"703">&gt; Best 73,<br clear=3D"none" abp=3D"704">&gt; Mark=
us (DF6NM)<br clear=3D"none" abp=3D"705">&gt;<br clear=3D"none" abp=3D"706"=
>&gt;<br clear=3D"none" abp=3D"707">&gt; -----Urspr=C3=BCngliche Mitteilung=
-----<br clear=3D"none" abp=3D"708">&gt; Von: Markus Vester &lt;<a href=3D"=
mailto:markusvester@aol.com" rel=3D"noopener noreferrer" shape=3D"rect" abp=
=3D"709" ymailto=3D"mailto:markusvester@aol.com">markusvester@aol.com</a>&g=
t;<br clear=3D"none" abp=3D"710">&gt; An: rsgb_lf_group &lt;<a href=3D"mail=
to:rsgb_lf_group@blacksheep.org" rel=3D"noopener noreferrer" shape=3D"rect"=
 abp=3D"711" ymailto=3D"mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@=
blacksheep.org</a>&gt;<br clear=3D"none" abp=3D"712">&gt; Verschickt: Sa, 2=
2. Dez 2018 14:55<br clear=3D"none" abp=3D"713">&gt; Betreff: LF: VO1NA 137=
477 Hz<br clear=3D"none" abp=3D"714">&gt;<br clear=3D"none" abp=3D"715">&gt=
; Hi Joe,<br clear=3D"none" abp=3D"716">&gt;<br clear=3D"none" abp=3D"717">=
&gt; the carrier on your frequency is nicely visible night and day.&nbsp;Wh=
en the signal is strong, some&nbsp;symmetrical sidebands become visible, ar=
e you&nbsp;still modulating with 7 char EbNaut messages every other half ho=
ur?&nbsp;<br clear=3D"none" abp=3D"718">&gt;<br clear=3D"none" abp=3D"719">=
&gt; I've placed&nbsp;my&nbsp;current autodecoder scripts here<br clear=3D"=
none" abp=3D"720">&gt; but note that&nbsp;this setup is driven by&nbsp;opds=
 and sort of specific to my LF grabber. For Linux, you may want to start fr=
om the scripts which Domenico has recently posted.<br clear=3D"none" abp=3D=
"721">&gt;<br clear=3D"none" abp=3D"722">&gt; Best 73,<br clear=3D"none" ab=
p=3D"723">&gt; Markus&nbsp;(DF6NM)<br clear=3D"none" abp=3D"724">&gt;<br cl=
ear=3D"none" abp=3D"725">&gt;<br clear=3D"none" abp=3D"726">&gt;<br clear=
=3D"none" abp=3D"727">&gt; -----Urspr=C3=BCngliche Mitteilung-----<br clear=
=3D"none" abp=3D"728">&gt; Von: jcraig &lt;<a href=3D"mailto:jcraig@mun.ca"=
 rel=3D"noopener noreferrer" shape=3D"rect" abp=3D"729" ymailto=3D"mailto:j=
craig@mun.ca">jcraig@mun.ca</a>&gt;<br clear=3D"none" abp=3D"730">&gt; An: =
rsgb_lf_group &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" rel=3D"no=
opener noreferrer" shape=3D"rect" abp=3D"731" ymailto=3D"mailto:rsgb_lf_gro=
up@blacksheep.org">rsgb_lf_group@blacksheep.org</a>&gt;<br clear=3D"none" a=
bp=3D"732">&gt; Verschickt: Mo, 17. Dez 2018 22:53<br clear=3D"none" abp=3D=
"733">&gt; Betreff: Re: LF: EbNaut 137.542 kHz<br clear=3D"none" abp=3D"734=
">&gt;<br clear=3D"none" abp=3D"735">&gt; Hi Markus, Stefan EbNauters,<br c=
lear=3D"none" abp=3D"736">&gt;<br clear=3D"none" abp=3D"737">&gt; Thanks fo=
r the reports and autodetectors.&nbsp; The TX carrier is on<br clear=3D"non=
e" abp=3D"738">&gt; continuously at 50 watts with the excitation XOR phase =
inverted<br clear=3D"none" abp=3D"739">&gt; by Paul's Ebkey.c on a raspi3.<=
br clear=3D"none" abp=3D"740">&gt;<br clear=3D"none" abp=3D"741">&gt; There=
 have been some daytime decodes recently.<br clear=3D"none" abp=3D"742">&gt=
;<br clear=3D"none" abp=3D"743">&gt; Is the autodetect easy to set up?&nbsp=
; If not perhaps I'd best<br clear=3D"none" abp=3D"744">&gt; review the adv=
ice from you and Stefan again.<br clear=3D"none" abp=3D"745">&gt;<br clear=
=3D"none" abp=3D"746">&gt; 73<br clear=3D"none" abp=3D"747">&gt; Joe<br cle=
ar=3D"none" abp=3D"748">&gt;</div></div></div>
------=_Part_3501356_506240969.1550840283304--

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Date: Fri, 22 Feb 2019 15:10:01 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello Joe, I did not know your father was an amateur operator
    too. My condolences to you and your family, when did he last operate? It's
    great to see you carrying on in his fashion though, he must of [...] 
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Hello Joe, I did not know your father was an amateur operator too. My
condolences to you and your family, when did he last operate? It's
great to see you carrying on in his fashion though, he must of been
proud of your achievements! All the best, I am sorry to read of your
loss.

Friday, February 22, 2019, 12:50:29 PM, you wrote:

> Markus, group,

> Thank-you for the insipiring anecdotes and signal reports.
> I am sad to report that my dad  G3LMD/ VO1FB became a silent key
> yeserday morning.

> 73
> Joe VO1NA



-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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Subject: R: Re: LF: VO1NA 137477 Hz
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Joe,

sad to read that.. I'm close to you

Marco, IK1HSS



----Messaggio originale----
Da: jcraig@mun.ca
Data: 22-feb-2019 13.50
A: <rsgb_lf_group@blacksheep.org>
Ogg: Re: LF: VO1NA 137477 Hz

Markus, group,

Thank-you for the insipiring anecdotes and signal reports.
I am sad to report that my dad  G3LMD/ VO1FB became a silent key
yeserday morning.

73
Joe VO1NA

On Fri, 22 Feb 2019, Markus Vester wrote:

> This week the EbNaut autodecoders at DL0AO and DF6NM have been refurbishe=
d, producing more compact output with one line for each successful decode. =
My current script and required utilities are here:
> http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip
>
> Our autodecoders are currently observing 137477 Hz. Until yesterday, VO1N=
A has been making strong and consistent decodes every night. Today I'm doin=
g a few of low-power daytime tests on his QRG, with the LEA-6T barefoot to =
the antenna.
>
> Best 73,
> Markus (DF6NM)
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: Markus Vester <markusvester@aol.com>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Sa, 22. Dez 2018 14:55
> Betreff: LF: VO1NA 137477 Hz
>
> Hi Joe,
>
> the carrier on your frequency is nicely visible night and day. When the s=
ignal is strong, some symmetrical sidebands become visible, are you still m=
odulating with 7 char EbNaut messages every other half hour?=20
>
> I've placed my current autodecoder scripts here
> but note that this setup is driven by opds and sort of specific to my LF =
grabber. For Linux, you may want to start from the scripts which Domenico h=
as recently posted.
>
> Best 73,
> Markus (DF6NM)
>
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: jcraig <jcraig@mun.ca>
> An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> Verschickt: Mo, 17. Dez 2018 22:53
> Betreff: Re: LF: EbNaut 137.542 kHz
>
> Hi Markus, Stefan EbNauters,
>
> Thanks for the reports and autodetectors.  The TX carrier is on
> continuously at 50 watts with the excitation XOR phase inverted
> by Paul's Ebkey.c on a raspi3.
>
> There have been some daytime decodes recently.
>
> Is the autodetect easy to set up?  If not perhaps I'd best
> review the advice from you and Stefan again.
>
> 73
> Joe
>



------=_Part_3357_13758049.1550908257783
Content-Type: text/html;charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

Joe,<br><br>sad to read that.. I'm close to you<br><br>Marco, IK1HSS<br>
<br>
----Messaggio originale----<br>Da: jcraig@mun.ca<br>Data: 22-feb-2019 13.50=
<br>A: &lt;rsgb_lf_group@blacksheep.org&gt;<br>Ogg: Re: LF: VO1NA 137477 Hz=
<br><br>Markus, group,<br><br>Thank-you for the insipiring anecdotes and si=
gnal reports.<br>I am sad to report that my dad&nbsp; G3LMD/ VO1FB became a=
 silent key<br>yeserday morning.<br><br>73<br>Joe VO1NA<br><br>On Fri, 22 F=
eb 2019, Markus Vester wrote:<br><br>&gt; This week&nbsp;the EbNaut autodec=
oders at DL0AO and DF6NM have been refurbished, producing more compact outp=
ut with one line for each successful decode. My current&nbsp;script&nbsp;an=
d required utilities are here:<br>&gt; http://df6nm.bplaced.net/VLF/fec_tes=
ts/ebnaut_autodecode_scripts.zip<br>&gt;<br>&gt; Our autodecoders are curre=
ntly observing 137477 Hz. Until yesterday, VO1NA has been making strong and=
 consistent decodes every night. Today I'm doing a few of low-power daytime=
 tests on his QRG, with the LEA-6T barefoot to the antenna.<br>&gt;<br>&gt;=
 Best 73,<br>&gt; Markus (DF6NM)<br>&gt;<br>&gt;<br>&gt; -----Urspr=C3=BCng=
liche Mitteilung-----<br>&gt; Von: Markus Vester &lt;markusvester@aol.com&g=
t;<br>&gt; An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br>&gt; V=
erschickt: Sa, 22. Dez 2018 14:55<br>&gt; Betreff: LF: VO1NA 137477 Hz<br>&=
gt;<br>&gt; Hi Joe,<br>&gt;<br>&gt; the carrier on your frequency is nicely=
 visible night and day.&nbsp;When the signal is strong, some&nbsp;symmetric=
al sidebands become visible, are you&nbsp;still modulating with 7 char EbNa=
ut messages every other half hour?&nbsp;<br>&gt;<br>&gt; I've placed&nbsp;m=
y&nbsp;current autodecoder scripts here<br>&gt; but note that&nbsp;this set=
up is driven by&nbsp;opds and sort of specific to my LF grabber. For Linux,=
 you may want to start from the scripts which Domenico has recently posted.=
<br>&gt;<br>&gt; Best 73,<br>&gt; Markus&nbsp;(DF6NM)<br>&gt;<br>&gt;<br>&g=
t;<br>&gt; -----Urspr=C3=BCngliche Mitteilung-----<br>&gt; Von: jcraig &lt;=
jcraig@mun.ca&gt;<br>&gt; An: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.or=
g&gt;<br>&gt; Verschickt: Mo, 17. Dez 2018 22:53<br>&gt; Betreff: Re: LF: E=
bNaut 137.542 kHz<br>&gt;<br>&gt; Hi Markus, Stefan EbNauters,<br>&gt;<br>&=
gt; Thanks for the reports and autodetectors.&nbsp; The TX carrier is on<br=
>&gt; continuously at 50 watts with the excitation XOR phase inverted<br>&g=
t; by Paul's Ebkey.c on a raspi3.<br>&gt;<br>&gt; There have been some dayt=
ime decodes recently.<br>&gt;<br>&gt; Is the autodetect easy to set up?&nbs=
p; If not perhaps I'd best<br>&gt; review the advice from you and Stefan ag=
ain.<br>&gt;<br>&gt; 73<br>&gt; Joe<br>&gt;<br><br>

------=_Part_3357_13758049.1550908257783--


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 Content preview:  I am sorry for your loss Joe. May he RIP. 73, Paul On 2/22/19
    7:50 AM, jcraig@mun.ca wrote: > Markus, group, > > Thank-you for the insipiring
    anecdotes and signal reports. > I am sad to report that my dad G3LMD/ VO1FB
    became a silent key > yeserday mo [...] 
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I am sorry for your loss Joe. May he RIP.

73,
Paul


On 2/22/19 7:50 AM, jcraig@mun.ca wrote:
> Markus, group,
> 
> Thank-you for the insipiring anecdotes and signal reports.
> I am sad to report that my dad  G3LMD/ VO1FB became a silent key
> yeserday morning.
> 
> 73
> Joe VO1NA

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 <1341300776.3468000.1550834824126@mail.yahoo.com> <Pine.LNX.4.64.1902220917000.23134@plato.ucs.mun.ca>
In-Reply-To: <Pine.LNX.4.64.1902220917000.23134@plato.ucs.mun.ca>
From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Sat, 23 Feb 2019 19:47:24 +0100
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 Content preview:  Dear Joe, I am sorry to read about the loss of your father:
    I'm close to you. Riccardo IW4DXW 
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Subject: Re: LF: VO1NA 137477 Hz
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--0000000000001f25fe0582942469
Content-Type: text/plain; charset="UTF-8"
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Dear Joe,

I am sorry to read about the loss of your father: I'm close to you.


Riccardo IW4DXW




Il giorno Ven 22 Feb 2019, 13:55 <jcraig@mun.ca> ha scritto:

> Markus, group,
>
> Thank-you for the insipiring anecdotes and signal reports.
> I am sad to report that my dad  G3LMD/ VO1FB became a silent key
> yeserday morning.
>
> 73
> Joe VO1NA
>
> On Fri, 22 Feb 2019, Markus Vester wrote:
>
> > This week the EbNaut autodecoders at DL0AO and DF6NM have been
> refurbished, producing more compact output with one line for each
> successful decode. My current script and required utilities are here:
> > http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip
> >
> > Our autodecoders are currently observing 137477 Hz. Until yesterday,
> VO1NA has been making strong and consistent decodes every night. Today I'=
m
> doing a few of low-power daytime tests on his QRG, with the LEA-6T barefo=
ot
> to the antenna.
> >
> > Best 73,
> > Markus (DF6NM)
> >
> >
> > -----Urspr=C3=BCngliche Mitteilung-----
> > Von: Markus Vester <markusvester@aol.com>
> > An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> > Verschickt: Sa, 22. Dez 2018 14:55
> > Betreff: LF: VO1NA 137477 Hz
> >
> > Hi Joe,
> >
> > the carrier on your frequency is nicely visible night and day. When the
> signal is strong, some symmetrical sidebands become visible, are you stil=
l
> modulating with 7 char EbNaut messages every other half hour?
> >
> > I've placed my current autodecoder scripts here
> > but note that this setup is driven by opds and sort of specific to my L=
F
> grabber. For Linux, you may want to start from the scripts which Domenico
> has recently posted.
> >
> > Best 73,
> > Markus (DF6NM)
> >
> >
> >
> > -----Urspr=C3=BCngliche Mitteilung-----
> > Von: jcraig <jcraig@mun.ca>
> > An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
> > Verschickt: Mo, 17. Dez 2018 22:53
> > Betreff: Re: LF: EbNaut 137.542 kHz
> >
> > Hi Markus, Stefan EbNauters,
> >
> > Thanks for the reports and autodetectors.  The TX carrier is on
> > continuously at 50 watts with the excitation XOR phase inverted
> > by Paul's Ebkey.c on a raspi3.
> >
> > There have been some daytime decodes recently.
> >
> > Is the autodetect easy to set up?  If not perhaps I'd best
> > review the advice from you and Stefan again.
> >
> > 73
> > Joe
> >

--0000000000001f25fe0582942469
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"auto"><div dir=3D"auto"><br></div><div dir=3D"auto">Dear Joe,=
=C2=A0</div><div dir=3D"auto"><br></div><div dir=3D"auto">I am sorry to rea=
d about the loss of your father: I&#39;m close to you.<br></div><div dir=3D=
"auto"><br></div><div dir=3D"auto"><br></div><div dir=3D"auto">Riccardo IW4=
DXW</div><div dir=3D"auto"><br></div><div dir=3D"auto"><br></div><div><br><=
br><div class=3D"gmail_quote"><div dir=3D"ltr">Il giorno Ven 22 Feb 2019, 1=
3:55  &lt;<a href=3D"mailto:jcraig@mun.ca" rel=3D"noreferrer noreferrer" ta=
rget=3D"_blank">jcraig@mun.ca</a>&gt; ha scritto:<br></div><blockquote clas=
s=3D"gmail_quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc solid;pad=
ding-left:1ex">Markus, group,<br>
<br>
Thank-you for the insipiring anecdotes and signal reports.<br>
I am sad to report that my dad=C2=A0 G3LMD/ VO1FB became a silent key<br>
yeserday morning.<br>
<br>
73<br>
Joe VO1NA<br>
<br>
On Fri, 22 Feb 2019, Markus Vester wrote:<br>
<br>
&gt; This week=C2=A0the EbNaut autodecoders at DL0AO and DF6NM have been re=
furbished, producing more compact output with one line for each successful =
decode. My current=C2=A0script=C2=A0and required utilities are here:<br>
&gt; <a href=3D"http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_sc=
ripts.zip" rel=3D"noreferrer noreferrer noreferrer noreferrer" target=3D"_b=
lank">http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip<=
/a><br>
&gt;<br>
&gt; Our autodecoders are currently observing 137477 Hz. Until yesterday, V=
O1NA has been making strong and consistent decodes every night. Today I&#39=
;m doing a few of low-power daytime tests on his QRG, with the LEA-6T baref=
oot to the antenna.<br>
&gt;<br>
&gt; Best 73,<br>
&gt; Markus (DF6NM)<br>
&gt;<br>
&gt;<br>
&gt; -----Urspr=C3=BCngliche Mitteilung-----<br>
&gt; Von: Markus Vester &lt;<a href=3D"mailto:markusvester@aol.com" rel=3D"=
noreferrer noreferrer noreferrer" target=3D"_blank">markusvester@aol.com</a=
>&gt;<br>
&gt; An: rsgb_lf_group &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" =
rel=3D"noreferrer noreferrer noreferrer" target=3D"_blank">rsgb_lf_group@bl=
acksheep.org</a>&gt;<br>
&gt; Verschickt: Sa, 22. Dez 2018 14:55<br>
&gt; Betreff: LF: VO1NA 137477 Hz<br>
&gt;<br>
&gt; Hi Joe,<br>
&gt;<br>
&gt; the carrier on your frequency is nicely visible night and day.=C2=A0Wh=
en the signal is strong, some=C2=A0symmetrical sidebands become visible, ar=
e you=C2=A0still modulating with 7 char EbNaut messages every other half ho=
ur?=C2=A0<br>
&gt;<br>
&gt; I&#39;ve placed=C2=A0my=C2=A0current autodecoder scripts here<br>
&gt; but note that=C2=A0this setup is driven by=C2=A0opds and sort of speci=
fic to my LF grabber. For Linux, you may want to start from the scripts whi=
ch Domenico has recently posted.<br>
&gt;<br>
&gt; Best 73,<br>
&gt; Markus=C2=A0(DF6NM)<br>
&gt;<br>
&gt;<br>
&gt;<br>
&gt; -----Urspr=C3=BCngliche Mitteilung-----<br>
&gt; Von: jcraig &lt;<a href=3D"mailto:jcraig@mun.ca" rel=3D"noreferrer nor=
eferrer noreferrer" target=3D"_blank">jcraig@mun.ca</a>&gt;<br>
&gt; An: rsgb_lf_group &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" =
rel=3D"noreferrer noreferrer noreferrer" target=3D"_blank">rsgb_lf_group@bl=
acksheep.org</a>&gt;<br>
&gt; Verschickt: Mo, 17. Dez 2018 22:53<br>
&gt; Betreff: Re: LF: EbNaut 137.542 kHz<br>
&gt;<br>
&gt; Hi Markus, Stefan EbNauters,<br>
&gt;<br>
&gt; Thanks for the reports and autodetectors.=C2=A0 The TX carrier is on<b=
r>
&gt; continuously at 50 watts with the excitation XOR phase inverted<br>
&gt; by Paul&#39;s Ebkey.c on a raspi3.<br>
&gt;<br>
&gt; There have been some daytime decodes recently.<br>
&gt;<br>
&gt; Is the autodetect easy to set up?=C2=A0 If not perhaps I&#39;d best<br=
>
&gt; review the advice from you and Stefan again.<br>
&gt;<br>
&gt; 73<br>
&gt; Joe<br>
&gt;</blockquote></div></div></div>

--0000000000001f25fe0582942469--

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From: Roger Lapthorn <rogerlapthorn@gmail.com>
Date: Sun, 24 Feb 2019 11:30:30 +0000
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 Content preview:  Joe, Please accept my condolences. 73s Roger G3XBM 
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Subject: Re: LF: VO1NA 137477 Hz
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--0000000000008aea010582a2274b
Content-Type: text/plain; charset="UTF-8"
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Joe,

Please accept my condolences.

73s
Roger G3XBM

On Sat, 23 Feb 2019 at 18:55, Riccardo Zoli <riccardozoli80@gmail.com>
wrote:

>
> Dear Joe,
>
> I am sorry to read about the loss of your father: I'm close to you.
>
>
> Riccardo IW4DXW
>
>
>
>
> Il giorno Ven 22 Feb 2019, 13:55 <jcraig@mun.ca> ha scritto:
>
>> Markus, group,
>>
>> Thank-you for the insipiring anecdotes and signal reports.
>> I am sad to report that my dad  G3LMD/ VO1FB became a silent key
>> yeserday morning.
>>
>> 73
>> Joe VO1NA
>>
>> On Fri, 22 Feb 2019, Markus Vester wrote:
>>
>> > This week the EbNaut autodecoders at DL0AO and DF6NM have been
>> refurbished, producing more compact output with one line for each
>> successful decode. My current script and required utilities are here:
>> > http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip
>> >
>> > Our autodecoders are currently observing 137477 Hz. Until yesterday,
>> VO1NA has been making strong and consistent decodes every night. Today I=
'm
>> doing a few of low-power daytime tests on his QRG, with the LEA-6T baref=
oot
>> to the antenna.
>> >
>> > Best 73,
>> > Markus (DF6NM)
>> >
>> >
>> > -----Urspr=C3=BCngliche Mitteilung-----
>> > Von: Markus Vester <markusvester@aol.com>
>> > An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
>> > Verschickt: Sa, 22. Dez 2018 14:55
>> > Betreff: LF: VO1NA 137477 Hz
>> >
>> > Hi Joe,
>> >
>> > the carrier on your frequency is nicely visible night and day. When th=
e
>> signal is strong, some symmetrical sidebands become visible, are you sti=
ll
>> modulating with 7 char EbNaut messages every other half hour?
>> >
>> > I've placed my current autodecoder scripts here
>> > but note that this setup is driven by opds and sort of specific to my
>> LF grabber. For Linux, you may want to start from the scripts which
>> Domenico has recently posted.
>> >
>> > Best 73,
>> > Markus (DF6NM)
>> >
>> >
>> >
>> > -----Urspr=C3=BCngliche Mitteilung-----
>> > Von: jcraig <jcraig@mun.ca>
>> > An: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
>> > Verschickt: Mo, 17. Dez 2018 22:53
>> > Betreff: Re: LF: EbNaut 137.542 kHz
>> >
>> > Hi Markus, Stefan EbNauters,
>> >
>> > Thanks for the reports and autodetectors.  The TX carrier is on
>> > continuously at 50 watts with the excitation XOR phase inverted
>> > by Paul's Ebkey.c on a raspi3.
>> >
>> > There have been some daytime decodes recently.
>> >
>> > Is the autodetect easy to set up?  If not perhaps I'd best
>> > review the advice from you and Stefan again.
>> >
>> > 73
>> > Joe
>> >
>
>

--0000000000008aea010582a2274b
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div>Joe,</div><div><br></div><div>Please accept my condol=
ences.=C2=A0</div><div><br></div><div>73s</div><div>Roger G3XBM</div></div>=
<br><div class=3D"gmail_quote"><div class=3D"gmail_attr" dir=3D"ltr">On Sat=
, 23 Feb 2019 at 18:55, Riccardo Zoli &lt;<a href=3D"mailto:riccardozoli80@=
gmail.com">riccardozoli80@gmail.com</a>&gt; wrote:<br></div><blockquote cla=
ss=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;padding-left:1ex;borde=
r-left-color:rgb(204,204,204);border-left-width:1px;border-left-style:solid=
"><div dir=3D"auto"><div dir=3D"auto"><br></div><div dir=3D"auto">Dear Joe,=
=C2=A0</div><div dir=3D"auto"><br></div><div dir=3D"auto">I am sorry to rea=
d about the loss of your father: I&#39;m close to you.<br></div><div dir=3D=
"auto"><br></div><div dir=3D"auto"><br></div><div dir=3D"auto">Riccardo IW4=
DXW</div><div dir=3D"auto"><br></div><div dir=3D"auto"><br></div><div><br><=
br><div class=3D"gmail_quote"><div dir=3D"ltr">Il giorno Ven 22 Feb 2019, 1=
3:55  &lt;<a href=3D"mailto:jcraig@mun.ca" target=3D"_blank" rel=3D"norefer=
rer noreferrer">jcraig@mun.ca</a>&gt; ha scritto:<br></div><blockquote clas=
s=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;padding-left:1ex;border=
-left-color:rgb(204,204,204);border-left-width:1px;border-left-style:solid"=
>Markus, group,<br>
<br>
Thank-you for the insipiring anecdotes and signal reports.<br>
I am sad to report that my dad=C2=A0 G3LMD/ VO1FB became a silent key<br>
yeserday morning.<br>
<br>
73<br>
Joe VO1NA<br>
<br>
On Fri, 22 Feb 2019, Markus Vester wrote:<br>
<br>
&gt; This week=C2=A0the EbNaut autodecoders at DL0AO and DF6NM have been re=
furbished, producing more compact output with one line for each successful =
decode. My current=C2=A0script=C2=A0and required utilities are here:<br>
&gt; <a href=3D"http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_sc=
ripts.zip" target=3D"_blank" rel=3D"noreferrer noreferrer noreferrer norefe=
rrer">http://df6nm.bplaced.net/VLF/fec_tests/ebnaut_autodecode_scripts.zip<=
/a><br>
&gt;<br>
&gt; Our autodecoders are currently observing 137477 Hz. Until yesterday, V=
O1NA has been making strong and consistent decodes every night. Today I&#39=
;m doing a few of low-power daytime tests on his QRG, with the LEA-6T baref=
oot to the antenna.<br>
&gt;<br>
&gt; Best 73,<br>
&gt; Markus (DF6NM)<br>
&gt;<br>
&gt;<br>
&gt; -----Urspr=C3=BCngliche Mitteilung-----<br>
&gt; Von: Markus Vester &lt;<a href=3D"mailto:markusvester@aol.com" target=
=3D"_blank" rel=3D"noreferrer noreferrer noreferrer">markusvester@aol.com</=
a>&gt;<br>
&gt; An: rsgb_lf_group &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" =
target=3D"_blank" rel=3D"noreferrer noreferrer noreferrer">rsgb_lf_group@bl=
acksheep.org</a>&gt;<br>
&gt; Verschickt: Sa, 22. Dez 2018 14:55<br>
&gt; Betreff: LF: VO1NA 137477 Hz<br>
&gt;<br>
&gt; Hi Joe,<br>
&gt;<br>
&gt; the carrier on your frequency is nicely visible night and day.=C2=A0Wh=
en the signal is strong, some=C2=A0symmetrical sidebands become visible, ar=
e you=C2=A0still modulating with 7 char EbNaut messages every other half ho=
ur?=C2=A0<br>
&gt;<br>
&gt; I&#39;ve placed=C2=A0my=C2=A0current autodecoder scripts here<br>
&gt; but note that=C2=A0this setup is driven by=C2=A0opds and sort of speci=
fic to my LF grabber. For Linux, you may want to start from the scripts whi=
ch Domenico has recently posted.<br>
&gt;<br>
&gt; Best 73,<br>
&gt; Markus=C2=A0(DF6NM)<br>
&gt;<br>
&gt;<br>
&gt;<br>
&gt; -----Urspr=C3=BCngliche Mitteilung-----<br>
&gt; Von: jcraig &lt;<a href=3D"mailto:jcraig@mun.ca" target=3D"_blank" rel=
=3D"noreferrer noreferrer noreferrer">jcraig@mun.ca</a>&gt;<br>
&gt; An: rsgb_lf_group &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" =
target=3D"_blank" rel=3D"noreferrer noreferrer noreferrer">rsgb_lf_group@bl=
acksheep.org</a>&gt;<br>
&gt; Verschickt: Mo, 17. Dez 2018 22:53<br>
&gt; Betreff: Re: LF: EbNaut 137.542 kHz<br>
&gt;<br>
&gt; Hi Markus, Stefan EbNauters,<br>
&gt;<br>
&gt; Thanks for the reports and autodetectors.=C2=A0 The TX carrier is on<b=
r>
&gt; continuously at 50 watts with the excitation XOR phase inverted<br>
&gt; by Paul&#39;s Ebkey.c on a raspi3.<br>
&gt;<br>
&gt; There have been some daytime decodes recently.<br>
&gt;<br>
&gt; Is the autodetect easy to set up?=C2=A0 If not perhaps I&#39;d best<br=
>
&gt; review the advice from you and Stefan again.<br>
&gt;<br>
&gt; 73<br>
&gt; Joe<br>
&gt;</blockquote></div></div></div>
</blockquote></div>

--0000000000008aea010582a2274b--

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To: rsgb_lf_group@blacksheep.org
From: Eric NO3M <no3m@no3m.net>
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 Content preview:  I recently got a current mode (outp xfmr center tap not bypassed)
    Class D amp going on 136khz, basically modeled after the W1VD / G0MRF circuits. 
    FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t [...] 
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I recently got a current mode (outp xfmr center tap not bypassed) Class 
D amp going on 136khz, basically modeled after the W1VD / G0MRF 
circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90 
42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on the 
power supply in use:

30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out

I am also using the G0MRF keying circuit, ie. P-channel MOSFET (IRF9540) 
in the driver (MCP1404) supply line.

If the driver is left active (key down), the beginning and end of the 
input RF envelope produces a "clicking" noise... assume this is from 
current spikes being developed and sunk by the FET body diodes?  If the 
driver is keyed with input RF already applied, thereby interrupting the 
drive to the FETs, there is no such behavior.  The keying is shaped, 
resulting in a ramping of the driver supply voltage and resultant gate 
waveforms to the FETs.

These current spikes do not bother my 30V linear power supply, however, 
when I attempt to use a 48V switching supply (rated at 17.7A), it seems 
to be OK with the current spike generated on the beginning of the RF 
envelope, but not the spike at the end of the envelope and goes into 
fault mode.  If the driver is keyed with continuous RF applied, it's 
happy and does not trip out.  But keying the driver doesn't seem 
practical for digi modes without some exotic circuitry or engaging 
computer generated signaling to key down *after* RF drive is applied and 
key up *before* RF drive is removed.... again, this phenomena only 
happens at the beginning and end of the input RF envelope.

Is there way to mitigate these current spikes, especially the one 
generated when RF is removed?

73 Eric NO3M


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To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: Class D current spikes
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 Content preview:  Hello Eric, I had a similar problem: at "key up" one of the
    driver outputs will remain low and the other high. As a result the gate of
    one of the power MOSFETs is kept high for a time much longer that half a
   peri [...] 
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Hello Eric,

I had a similar problem:
at "key up" one of the driver outputs will remain low and the other high. As a result the gate of one of the power MOSFETs is kept high for a time much longer that half a period. During that time this MOSFET is in ON-state (conducting) and thus drawing excessive current.
I solved the problem by adding monostable multivibrators that disable the MOSFET driver when one of the driver outputs stays high longer than 3 microseconds.

Assuming that you refer to the W1VD "500W RF-deck" (http://www.w1vd.com/137-500-500WTX.pdf): it is actually a voltage mode design (thus having current spikes).
A current mode class D amp has a choke between the supply voltgae and the output transformer center tap, limiting the current (and causing voltage spikes).

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens Eric NO3M <no3m@no3m.net>
Verzonden: zondag 24 februari 2019 13:08
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: LF: Class D current spikes

I recently got a current mode (outp xfmr center tap not bypassed) Class
D amp going on 136khz, basically modeled after the W1VD / G0MRF
circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on the
power supply in use:

30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out

I am also using the G0MRF keying circuit, ie. P-channel MOSFET (IRF9540)
in the driver (MCP1404) supply line.

If the driver is left active (key down), the beginning and end of the
input RF envelope produces a "clicking" noise... assume this is from
current spikes being developed and sunk by the FET body diodes?  If the
driver is keyed with input RF already applied, thereby interrupting the
drive to the FETs, there is no such behavior.  The keying is shaped,
resulting in a ramping of the driver supply voltage and resultant gate
waveforms to the FETs.

These current spikes do not bother my 30V linear power supply, however,
when I attempt to use a 48V switching supply (rated at 17.7A), it seems
to be OK with the current spike generated on the beginning of the RF
envelope, but not the spike at the end of the envelope and goes into
fault mode.  If the driver is keyed with continuous RF applied, it's
happy and does not trip out.  But keying the driver doesn't seem
practical for digi modes without some exotic circuitry or engaging
computer generated signaling to key down *after* RF drive is applied and
key up *before* RF drive is removed.... again, this phenomena only
happens at the beginning and end of the input RF envelope.

Is there way to mitigate these current spikes, especially the one
generated when RF is removed?

73 Eric NO3M




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To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: Class D current spikes
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 Content preview:  Addendum: 3 microseconds is for 472kHz, for a 136kHz PA it
    should be 10 microseconds. 73, Rik ON7YD - OR7T Van: owner-rsgb_lf_group@blacksheep.org
    <owner-rsgb_lf_group@blacksheep.org> namens Rik Strobbe <rik.strobbe@kuleuven.be>
    Verzonden: zondag 24 februari 2019 13 [...] 
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Subject: LF: Re: Class D current spikes
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Addendum: 3 microseconds is for 472kHz, for a 136kHz PA it should be 10 microseconds.

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens Rik Strobbe <rik.strobbe@kuleuven.be>
Verzonden: zondag 24 februari 2019 13:38
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: LF: Re: Class D current spikes

Hello Eric,

I had a similar problem:
at "key up" one of the driver outputs will remain low and the other high. As a result the gate of one of the power MOSFETs is kept high for a time much longer that half a period. During that time this MOSFET is in ON-state (conducting) and thus drawing excessive current.
I solved the problem by adding monostable multivibrators that disable the MOSFET driver when one of the driver outputs stays high longer than 3 microseconds.

Assuming that you refer to the W1VD "500W RF-deck" (http://www.w1vd.com/137-500-500WTX.pdf): it is actually a voltage mode design (thus having current spikes).
A current mode class D amp has a choke between the supply voltgae and the output transformer center tap, limiting the current (and causing voltage spikes).

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens Eric NO3M <no3m@no3m.net>
Verzonden: zondag 24 februari 2019 13:08
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: LF: Class D current spikes

I recently got a current mode (outp xfmr center tap not bypassed) Class
D amp going on 136khz, basically modeled after the W1VD / G0MRF
circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on the
power supply in use:

30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out

I am also using the G0MRF keying circuit, ie. P-channel MOSFET (IRF9540)
in the driver (MCP1404) supply line.

If the driver is left active (key down), the beginning and end of the
input RF envelope produces a "clicking" noise... assume this is from
current spikes being developed and sunk by the FET body diodes?  If the
driver is keyed with input RF already applied, thereby interrupting the
drive to the FETs, there is no such behavior.  The keying is shaped,
resulting in a ramping of the driver supply voltage and resultant gate
waveforms to the FETs.

These current spikes do not bother my 30V linear power supply, however,
when I attempt to use a 48V switching supply (rated at 17.7A), it seems
to be OK with the current spike generated on the beginning of the RF
envelope, but not the spike at the end of the envelope and goes into
fault mode.  If the driver is keyed with continuous RF applied, it's
happy and does not trip out.  But keying the driver doesn't seem
practical for digi modes without some exotic circuitry or engaging
computer generated signaling to key down *after* RF drive is applied and
key up *before* RF drive is removed.... again, this phenomena only
happens at the beginning and end of the input RF envelope.

Is there way to mitigate these current spikes, especially the one
generated when RF is removed?

73 Eric NO3M





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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Sun, 24 Feb 2019 13:29:35 +0000
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 Content preview:  Why not AC couple your gates. That removes all possibility
    of latching 100nF in series, reverse biassed diode to ground shunted by 10k
    or so for DC restoration Or transformer couple Andy www.g4jnt.com 
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Subject: Re: LF: Re: Class D current spikes
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--000000000000cce6a40582a3d17f
Content-Type: text/plain; charset="UTF-8"

Why not AC couple your gates.  That removes all possibility of latching
100nF in series, reverse biassed diode to ground shunted by 10k or so for
DC restoration
Or transformer couple

Andy
www.g4jnt.com



On Sun, 24 Feb 2019 at 13:24, Rik Strobbe <rik.strobbe@kuleuven.be> wrote:

> Addendum: 3 microseconds is for 472kHz, for a 136kHz PA it should be 10
> microseconds.
>
> 73, Rik  ON7YD - OR7T
>
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org <
> owner-rsgb_lf_group@blacksheep.org> namens Rik Strobbe <
> rik.strobbe@kuleuven.be>
> Verzonden: zondag 24 februari 2019 13:38
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: LF: Re: Class D current spikes
>
> Hello Eric,
>
> I had a similar problem:
> at "key up" one of the driver outputs will remain low and the other high.
> As a result the gate of one of the power MOSFETs is kept high for a time
> much longer that half a period. During that time this MOSFET is in ON-state
> (conducting) and thus drawing excessive current.
> I solved the problem by adding monostable multivibrators that disable the
> MOSFET driver when one of the driver outputs stays high longer than 3
> microseconds.
>
> Assuming that you refer to the W1VD "500W RF-deck" (
> http://www.w1vd.com/137-500-500WTX.pdf): it is actually a voltage mode
> design (thus having current spikes).
> A current mode class D amp has a choke between the supply voltgae and the
> output transformer center tap, limiting the current (and causing voltage
> spikes).
>
> 73, Rik  ON7YD - OR7T
>
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org <
> owner-rsgb_lf_group@blacksheep.org> namens Eric NO3M <no3m@no3m.net>
> Verzonden: zondag 24 februari 2019 13:08
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: LF: Class D current spikes
>
> I recently got a current mode (outp xfmr center tap not bypassed) Class
> D amp going on 136khz, basically modeled after the W1VD / G0MRF
> circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
> 42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on the
> power supply in use:
>
> 30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
> 48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out
>
> I am also using the G0MRF keying circuit, ie. P-channel MOSFET (IRF9540)
> in the driver (MCP1404) supply line.
>
> If the driver is left active (key down), the beginning and end of the
> input RF envelope produces a "clicking" noise... assume this is from
> current spikes being developed and sunk by the FET body diodes?  If the
> driver is keyed with input RF already applied, thereby interrupting the
> drive to the FETs, there is no such behavior.  The keying is shaped,
> resulting in a ramping of the driver supply voltage and resultant gate
> waveforms to the FETs.
>
> These current spikes do not bother my 30V linear power supply, however,
> when I attempt to use a 48V switching supply (rated at 17.7A), it seems
> to be OK with the current spike generated on the beginning of the RF
> envelope, but not the spike at the end of the envelope and goes into
> fault mode.  If the driver is keyed with continuous RF applied, it's
> happy and does not trip out.  But keying the driver doesn't seem
> practical for digi modes without some exotic circuitry or engaging
> computer generated signaling to key down *after* RF drive is applied and
> key up *before* RF drive is removed.... again, this phenomena only
> happens at the beginning and end of the input RF envelope.
>
> Is there way to mitigate these current spikes, especially the one
> generated when RF is removed?
>
> 73 Eric NO3M
>
>
>
>
>

--000000000000cce6a40582a3d17f
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<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">Why not AC couple your gates.=C2=A0 That removes=
 all possibility of latching</div><div class=3D"gmail_default" style=3D"fon=
t-family:tahoma,sans-serif;font-size:small">100nF in series, reverse biasse=
d diode to ground shunted by 10k or so for DC restoration</div><div class=
=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small">=
Or transformer couple</div><div class=3D"gmail_default" style=3D"font-famil=
y:tahoma,sans-serif;font-size:small"><br></div><div><div dir=3D"ltr" class=
=3D"gmail_signature" data-smartmail=3D"gmail_signature"><div dir=3D"ltr"><d=
iv><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div d=
ir=3D"ltr">Andy<div><span style=3D"font-size:12.8px"><a href=3D"http://www.=
g4jnt.com" target=3D"_blank">www.g4jnt.com</a></span><br></div><div><br></d=
iv></div></div></div></div></div></div></div></div></div></div></div><br></=
div><br><div class=3D"gmail_quote"><div dir=3D"ltr" class=3D"gmail_attr">On=
 Sun, 24 Feb 2019 at 13:24, Rik Strobbe &lt;<a href=3D"mailto:rik.strobbe@k=
uleuven.be">rik.strobbe@kuleuven.be</a>&gt; wrote:<br></div><blockquote cla=
ss=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid =
rgb(204,204,204);padding-left:1ex">Addendum: 3 microseconds is for 472kHz, =
for a 136kHz PA it should be 10 microseconds.<br>
<br>
73, Rik=C2=A0 ON7YD - OR7T<br>
<br>
________________________________________<br>
Van: <a href=3D"mailto:owner-rsgb_lf_group@blacksheep.org" target=3D"_blank=
">owner-rsgb_lf_group@blacksheep.org</a> &lt;<a href=3D"mailto:owner-rsgb_l=
f_group@blacksheep.org" target=3D"_blank">owner-rsgb_lf_group@blacksheep.or=
g</a>&gt; namens Rik Strobbe &lt;<a href=3D"mailto:rik.strobbe@kuleuven.be"=
 target=3D"_blank">rik.strobbe@kuleuven.be</a>&gt;<br>
Verzonden: zondag 24 februari 2019 13:38<br>
Aan: <a href=3D"mailto:rsgb_lf_group@blacksheep.org" target=3D"_blank">rsgb=
_lf_group@blacksheep.org</a><br>
Onderwerp: LF: Re: Class D current spikes<br>
<br>
Hello Eric,<br>
<br>
I had a similar problem:<br>
at &quot;key up&quot; one of the driver outputs will remain low and the oth=
er high. As a result the gate of one of the power MOSFETs is kept high for =
a time much longer that half a period. During that time this MOSFET is in O=
N-state (conducting) and thus drawing excessive current.<br>
I solved the problem by adding monostable multivibrators that disable the M=
OSFET driver when one of the driver outputs stays high longer than 3 micros=
econds.<br>
<br>
Assuming that you refer to the W1VD &quot;500W RF-deck&quot; (<a href=3D"ht=
tp://www.w1vd.com/137-500-500WTX.pdf" rel=3D"noreferrer" target=3D"_blank">=
http://www.w1vd.com/137-500-500WTX.pdf</a>): it is actually a voltage mode =
design (thus having current spikes).<br>
A current mode class D amp has a choke between the supply voltgae and the o=
utput transformer center tap, limiting the current (and causing voltage spi=
kes).<br>
<br>
73, Rik=C2=A0 ON7YD - OR7T<br>
<br>
________________________________________<br>
Van: <a href=3D"mailto:owner-rsgb_lf_group@blacksheep.org" target=3D"_blank=
">owner-rsgb_lf_group@blacksheep.org</a> &lt;<a href=3D"mailto:owner-rsgb_l=
f_group@blacksheep.org" target=3D"_blank">owner-rsgb_lf_group@blacksheep.or=
g</a>&gt; namens Eric NO3M &lt;<a href=3D"mailto:no3m@no3m.net" target=3D"_=
blank">no3m@no3m.net</a>&gt;<br>
Verzonden: zondag 24 februari 2019 13:08<br>
Aan: <a href=3D"mailto:rsgb_lf_group@blacksheep.org" target=3D"_blank">rsgb=
_lf_group@blacksheep.org</a><br>
Onderwerp: LF: Class D current spikes<br>
<br>
I recently got a current mode (outp xfmr center tap not bypassed) Class<br>
D amp going on 136khz, basically modeled after the W1VD / G0MRF<br>
circuits.=C2=A0 FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90<b=
r>
42mm output xfmr, 62uH (25t T157-26) choke.=C2=A0 Output xfmr depends on th=
e<br>
power supply in use:<br>
<br>
30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out<br>
48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out<br>
<br>
I am also using the G0MRF keying circuit, ie. P-channel MOSFET (IRF9540)<br=
>
in the driver (MCP1404) supply line.<br>
<br>
If the driver is left active (key down), the beginning and end of the<br>
input RF envelope produces a &quot;clicking&quot; noise... assume this is f=
rom<br>
current spikes being developed and sunk by the FET body diodes?=C2=A0 If th=
e<br>
driver is keyed with input RF already applied, thereby interrupting the<br>
drive to the FETs, there is no such behavior.=C2=A0 The keying is shaped,<b=
r>
resulting in a ramping of the driver supply voltage and resultant gate<br>
waveforms to the FETs.<br>
<br>
These current spikes do not bother my 30V linear power supply, however,<br>
when I attempt to use a 48V switching supply (rated at 17.7A), it seems<br>
to be OK with the current spike generated on the beginning of the RF<br>
envelope, but not the spike at the end of the envelope and goes into<br>
fault mode.=C2=A0 If the driver is keyed with continuous RF applied, it&#39=
;s<br>
happy and does not trip out.=C2=A0 But keying the driver doesn&#39;t seem<b=
r>
practical for digi modes without some exotic circuitry or engaging<br>
computer generated signaling to key down *after* RF drive is applied and<br=
>
key up *before* RF drive is removed.... again, this phenomena only<br>
happens at the beginning and end of the input RF envelope.<br>
<br>
Is there way to mitigate these current spikes, especially the one<br>
generated when RF is removed?<br>
<br>
73 Eric NO3M<br>
<br>
<br>
<br>
<br>
</blockquote></div>

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From: Eric NO3M <no3m@no3m.net>
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 Content preview:  Rik Thanks for the reply.  This particular build is current
    mode (choke off center tap)... so I guess I'm dealing with voltage spikes. 
    I didn't notice voltage spikes while monitoring the envelopes when [...] 
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Rik

Thanks for the reply.  This particular build is current mode (choke off 
center tap)... so I guess I'm dealing with voltage spikes.  I didn't 
notice voltage spikes while monitoring the envelopes when sending dits 
from the exciter, but may not have had the scope adjusted to best 
visualize them.

The driver outputs are AC coupled to the FETs using a 0.22u coupling 
cap, shunt schottky (SB560), series 10 ohm, and shunt 4.7k.  Should the 
same behavior with extended ON time be present?


On 2/24/19 7:38 AM, Rik Strobbe wrote:
> Hello Eric,
>
> I had a similar problem:
> at "key up" one of the driver outputs will remain low and the other high. As a result the gate of one of the power MOSFETs is kept high for a time much longer that half a period. During that time this MOSFET is in ON-state (conducting) and thus drawing excessive current.
> I solved the problem by adding monostable multivibrators that disable the MOSFET driver when one of the driver outputs stays high longer than 3 microseconds.
>
> Assuming that you refer to the W1VD "500W RF-deck" (http://www.w1vd.com/137-500-500WTX.pdf): it is actually a voltage mode design (thus having current spikes).
> A current mode class D amp has a choke between the supply voltgae and the output transformer center tap, limiting the current (and causing voltage spikes).
>
> 73, Rik  ON7YD - OR7T
>
>


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From: Eric NO3M <no3m@no3m.net>
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 Content preview:  The driver and FET gates in mine are AC coupled (0.22u, SB560
    schottky shunt, 10 ohm series, 4.7k shunt) and the problem still exists. 
    Apparently same thing Paul N1BUG was having problems with. The [...] 
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The driver and FET gates in mine are AC coupled (0.22u, SB560 schottky 
shunt, 10 ohm series, 4.7k shunt) and the problem still exists.  
Apparently same thing Paul N1BUG was having problems with. The spike on 
the end of the RF envelope is what seems most ominous and results in my 
48v switcher going into fault mode.


On 2/24/19 8:29 AM, Andy Talbot wrote:
> Why not AC couple your gates.  That removes all possibility of latching
> 100nF in series, reverse biassed diode to ground shunted by 10k or so 
> for DC restoration
> Or transformer couple
>
> Andy
> www.g4jnt.com <http://www.g4jnt.com>
>
>
>


--------------CD7C842621A5F5B7E81AC796
Content-Type: text/html; charset=utf-8
Content-Transfer-Encoding: 8bit

<html>
  <head>
    <meta http-equiv="Content-Type" content="text/html; charset=UTF-8">
  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    The driver and FET gates in mine are AC coupled (0.22u, SB560
    schottky shunt, 10 ohm series, 4.7k shunt) and the problem still
    exists.  Apparently same thing Paul N1BUG was having problems with. 
    The spike on the end of the RF envelope is what seems most ominous
    and results in my 48v switcher going into fault mode.<br>
    <br>
    <br>
    <div class="moz-cite-prefix">On 2/24/19 8:29 AM, Andy Talbot wrote:<br>
    </div>
    <blockquote type="cite"
cite="mid:CAA8k23Qt3k4B8CNanY3F3s3NYw5EpbJmKop8iKXyMZeH_bKd1Q@mail.gmail.com">
      <meta http-equiv="content-type" content="text/html; charset=UTF-8">
      <div dir="ltr">
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small">Why not
          AC couple your gates.  That removes all possibility of
          latching</div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small">100nF in
          series, reverse biassed diode to ground shunted by 10k or so
          for DC restoration</div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small">Or
          transformer couple</div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small"><br>
        </div>
        <div>
          <div dir="ltr" class="gmail_signature"
            data-smartmail="gmail_signature">
            <div dir="ltr">
              <div>
                <div dir="ltr">
                  <div>
                    <div dir="ltr">
                      <div>
                        <div dir="ltr">
                          <div>
                            <div dir="ltr">Andy
                              <div><span style="font-size:12.8px"><a
                                    href="http://www.g4jnt.com"
                                    target="_blank"
                                    moz-do-not-send="true">www.g4jnt.com</a></span><br>
                              </div>
                              <div><br>
                              </div>
                            </div>
                          </div>
                        </div>
                      </div>
                    </div>
                  </div>
                </div>
              </div>
            </div>
          </div>
        </div>
        <br>
      </div>
      <br>
    </blockquote>
    <br>
  </body>
</html>

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 Content preview:  I will be watching this discussion closely. Mine is a W1VD
    kilowatt deck: http://w1vd.com/137-500-KWRev3.0.pdf It has blown FETs several
    times. The problem always occurs at the end of the RF envelope. To further
    confuse this issue, I have lost only one FET while running with my U3S exciter
    in hundreds of hours [...] 
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Subject: Re: LF: Re: Class D current spikes
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I will be watching this discussion closely. Mine is a W1VD kilowatt
deck:

http://w1vd.com/137-500-KWRev3.0.pdf

It has blown FETs several times. The problem always occurs at the
end of the RF envelope. To further confuse this issue, I have lost
only one FET while running with my U3S exciter in hundreds of hours
of operation. I have lost many FETs when driving it with HF
transceiver and down converter. I have also lost FETs driving it
with a phasing exciter. It seems using it with either of the latter
exciters almost guarantees one or more dead FETs within a few
minutes. I was running at about 300 watts output during all of these
failures.

73,
Paul


On 2/24/19 8:42 AM, Eric NO3M wrote:
> The driver and FET gates in mine are AC coupled (0.22u, SB560
> schottky shunt, 10 ohm series, 4.7k shunt) and the problem still
> exists.  Apparently same thing Paul N1BUG was having problems with. 
> The spike on the end of the RF envelope is what seems most ominous
> and results in my 48v switcher going into fault mode.

From owner-rsgb_lf_group@blacksheep.org  Sun Feb 24 15:27:19 2019
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From: Rik Strobbe <rik.strobbe@kuleuven.be>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: LF: Re: Class D current spikes
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Date: Sun, 24 Feb 2019 14:23:12 +0000
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 Content preview:  Hello Paul, Eric, Andy, AC coupling with a large C will not
    solve the problem. At "key up" one of the driver outputs will remain high
    thus the gate of theFET connected to that output will remain high (and the
    FET conducting) [...] 
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Subject: Re: LF: Re: Class D current spikes
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Hello Paul, Eric, Andy,

AC coupling with a large C will not solve the problem.
At "key up" one of the driver outputs will remain high thus the gate of theFET connected to that output will remain high (and the FET conducting) during a time depending on  RC constant of the driver / gate network. For 0.22uF and 4.7kOhm the RC constant is 1 millisecond. So for a driver running on 12V iit will take about that time for the gate voltage to drop below the treshold. During that 1ms the FET is more or less shortcircuiting the powersupply. One of them will die sooner ot later ;-)

73, Rik  ON7YD - OR7T
________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens N1BUG <paul@n1bug.com>
Verzonden: zondag 24 februari 2019 15:03
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: Re: LF: Re: Class D current spikes

I will be watching this discussion closely. Mine is a W1VD kilowatt
deck:

http://w1vd.com/137-500-KWRev3.0.pdf

It has blown FETs several times. The problem always occurs at the
end of the RF envelope. To further confuse this issue, I have lost
only one FET while running with my U3S exciter in hundreds of hours
of operation. I have lost many FETs when driving it with HF
transceiver and down converter. I have also lost FETs driving it
with a phasing exciter. It seems using it with either of the latter
exciters almost guarantees one or more dead FETs within a few
minutes. I was running at about 300 watts output during all of these
failures.

73,
Paul


On 2/24/19 8:42 AM, Eric NO3M wrote:
> The driver and FET gates in mine are AC coupled (0.22u, SB560
> schottky shunt, 10 ohm series, 4.7k shunt) and the problem still
> exists.  Apparently same thing Paul N1BUG was having problems with.
> The spike on the end of the RF envelope is what seems most ominous
> and results in my 48v switcher going into fault mode.



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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Sun, 24 Feb 2019 14:41:57 +0000
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 Content preview:  For on-off keying of a switch mode PA you really should be
    using supply line control. Switching the drive then trying to reduce rise
    /fall times for keyclick elimination by controlling drive amplitude [...]
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Subject: Re: LF: Re: Class D current spikes
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For on-off keying of a switch mode PA you really should be using supply
line control.  Switching the drive then trying to reduce rise /fall times
for keyclick elimination by controlling drive amplitude(something that
seems to be done in some designs) is really asking for trouble.  Even
hard-switching drive gives its problems , as we see here repeatedly

Instead, why not a simple emitter follower in the positive supply, then you
can apply waveform shaping  to the base drive at low current, where you've
got full control.   Even a 20A supply could be controlled this way with a
suitably rated transistor.  Quite likely have to be a Darlington.   There
will be a slight fixed drop across it, say 1V at saturation / full power,
so a few watts of dissipation, but it's only operating non saturated for a
short period during the rise / fall times.

A power FET could be used, but you'd need a drive voltage Vgs higher than
the supply, albeit only a few mA capability; nothing a small switcher
module couldn't manage.

Andy
www.g4jnt.com



On Sun, 24 Feb 2019 at 14:26, Rik Strobbe <rik.strobbe@kuleuven.be> wrote:

> Hello Paul, Eric, Andy,
>
> AC coupling with a large C will not solve the problem.
> At "key up" one of the driver outputs will remain high thus the gate of
> theFET connected to that output will remain high (and the FET conducting)
> during a time depending on  RC constant of the driver / gate network. For
> 0.22uF and 4.7kOhm the RC constant is 1 millisecond. So for a driver
> running on 12V iit will take about that time for the gate voltage to drop
> below the treshold. During that 1ms the FET is more or less shortcircuiting
> the powersupply. One of them will die sooner ot later ;-)
>
> 73, Rik  ON7YD - OR7T
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org <
> owner-rsgb_lf_group@blacksheep.org> namens N1BUG <paul@n1bug.com>
> Verzonden: zondag 24 februari 2019 15:03
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: Re: Class D current spikes
>
> I will be watching this discussion closely. Mine is a W1VD kilowatt
> deck:
>
> http://w1vd.com/137-500-KWRev3.0.pdf
>
> It has blown FETs several times. The problem always occurs at the
> end of the RF envelope. To further confuse this issue, I have lost
> only one FET while running with my U3S exciter in hundreds of hours
> of operation. I have lost many FETs when driving it with HF
> transceiver and down converter. I have also lost FETs driving it
> with a phasing exciter. It seems using it with either of the latter
> exciters almost guarantees one or more dead FETs within a few
> minutes. I was running at about 300 watts output during all of these
> failures.
>
> 73,
> Paul
>
>
> On 2/24/19 8:42 AM, Eric NO3M wrote:
> > The driver and FET gates in mine are AC coupled (0.22u, SB560
> > schottky shunt, 10 ohm series, 4.7k shunt) and the problem still
> > exists.  Apparently same thing Paul N1BUG was having problems with.
> > The spike on the end of the RF envelope is what seems most ominous
> > and results in my 48v switcher going into fault mode.
>
>
>

--000000000000a854990582a4d4a4
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">For on-off keying of a switch mode PA you really=
 should be using supply line control.=C2=A0 Switching the drive then trying=
 to reduce rise /fall times for keyclick elimination by controlling drive a=
mplitude(something that seems to be done in some designs) is really asking =
for trouble.=C2=A0 Even hard-switching drive gives its problems , as we see=
 here repeatedly</div><div class=3D"gmail_default" style=3D"font-family:tah=
oma,sans-serif;font-size:small"><br></div><div class=3D"gmail_default" styl=
e=3D"font-family:tahoma,sans-serif;font-size:small">Instead, why not a simp=
le emitter follower in the positive supply, then you can apply waveform sha=
ping=C2=A0 to the base drive at low current, where you&#39;ve got full cont=
rol.=C2=A0 =C2=A0Even a 20A supply could be controlled this way with a suit=
ably rated transistor.=C2=A0 Quite likely have to be a Darlington.=C2=A0 =
=C2=A0There will be a slight fixed drop across it, say 1V at saturation / f=
ull power, so a few watts of dissipation, but it&#39;s only operating non s=
aturated for a short period during the rise / fall times.</div><div class=
=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small">=
<br></div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-ser=
if;font-size:small">A power FET could be used, but you&#39;d need a drive v=
oltage Vgs higher than the supply, albeit only a few mA capability; nothing=
 a small switcher module couldn&#39;t manage.</div><div class=3D"gmail_defa=
ult" style=3D"font-family:tahoma,sans-serif;font-size:small">=C2=A0<br></di=
v><div><div dir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"gmail_s=
ignature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div=
><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=3D"font-size:1=
2.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank">www.g4jnt.com</a>=
</span><br></div><div><br></div></div></div></div></div></div></div></div><=
/div></div></div></div><br></div><br><div class=3D"gmail_quote"><div dir=3D=
"ltr" class=3D"gmail_attr">On Sun, 24 Feb 2019 at 14:26, Rik Strobbe &lt;<a=
 href=3D"mailto:rik.strobbe@kuleuven.be">rik.strobbe@kuleuven.be</a>&gt; wr=
ote:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px=
 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex">Hello Paul,=
 Eric, Andy,<br>
<br>
AC coupling with a large C will not solve the problem.<br>
At &quot;key up&quot; one of the driver outputs will remain high thus the g=
ate of theFET connected to that output will remain high (and the FET conduc=
ting) during a time depending on=C2=A0 RC constant of the driver / gate net=
work. For 0.22uF and 4.7kOhm the RC constant is 1 millisecond. So for a dri=
ver running on 12V iit will take about that time for the gate voltage to dr=
op below the treshold. During that 1ms the FET is more or less shortcircuit=
ing the powersupply. One of them will die sooner ot later ;-)<br>
<br>
73, Rik=C2=A0 ON7YD - OR7T<br>
________________________________________<br>
Van: <a href=3D"mailto:owner-rsgb_lf_group@blacksheep.org" target=3D"_blank=
">owner-rsgb_lf_group@blacksheep.org</a> &lt;<a href=3D"mailto:owner-rsgb_l=
f_group@blacksheep.org" target=3D"_blank">owner-rsgb_lf_group@blacksheep.or=
g</a>&gt; namens N1BUG &lt;<a href=3D"mailto:paul@n1bug.com" target=3D"_bla=
nk">paul@n1bug.com</a>&gt;<br>
Verzonden: zondag 24 februari 2019 15:03<br>
Aan: <a href=3D"mailto:rsgb_lf_group@blacksheep.org" target=3D"_blank">rsgb=
_lf_group@blacksheep.org</a><br>
Onderwerp: Re: LF: Re: Class D current spikes<br>
<br>
I will be watching this discussion closely. Mine is a W1VD kilowatt<br>
deck:<br>
<br>
<a href=3D"http://w1vd.com/137-500-KWRev3.0.pdf" rel=3D"noreferrer" target=
=3D"_blank">http://w1vd.com/137-500-KWRev3.0.pdf</a><br>
<br>
It has blown FETs several times. The problem always occurs at the<br>
end of the RF envelope. To further confuse this issue, I have lost<br>
only one FET while running with my U3S exciter in hundreds of hours<br>
of operation. I have lost many FETs when driving it with HF<br>
transceiver and down converter. I have also lost FETs driving it<br>
with a phasing exciter. It seems using it with either of the latter<br>
exciters almost guarantees one or more dead FETs within a few<br>
minutes. I was running at about 300 watts output during all of these<br>
failures.<br>
<br>
73,<br>
Paul<br>
<br>
<br>
On 2/24/19 8:42 AM, Eric NO3M wrote:<br>
&gt; The driver and FET gates in mine are AC coupled (0.22u, SB560<br>
&gt; schottky shunt, 10 ohm series, 4.7k shunt) and the problem still<br>
&gt; exists.=C2=A0 Apparently same thing Paul N1BUG was having problems wit=
h.<br>
&gt; The spike on the end of the RF envelope is what seems most ominous<br>
&gt; and results in my 48v switcher going into fault mode.<br>
<br>
<br>
</blockquote></div>

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 Content preview:  Dear LF enthusiasts, AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
    * 1. New database records have been added :* #686 QRB=5238,8 2019-02-22 K3MF
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Dear LF enthusiasts,
 AWLF *http://136.73.ru/h_aw <http://136.73.ru/h_aw>*
* 1. New database records have been added :*

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#687  QRB=3D5312,9  2019-02-22  NO3M     -> EI0CF  WSPR2

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#689  QRB=3D5685,7  2019-02-22  NO3M     -> 2E0ILY WSPR2

#690  QRB=3D5706,5  2019-02-23  K3FM     -> G0MRF  WSPR2


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*2E0ILY  *AWLF 3 Rating 7 =E2=86=91 6
        AWLF 1 RX Rating 75 =E2=86=91 55

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        AWLF 2 TX Rating 15 =E2=86=91 11

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        AWLF 1 RX Rating 118 =E2=86=91 74

*G0LUJ   *AWLF 1 Rating 18 =E2=86=91 10

        AWLF 1 RX Rating 19 =E2=86=91 10

*NO3M    *AWLF 1 Rating 49 =E2=86=91 12
        AWLF 1 TX Rating 27 =E2=86=91 6


*3. NEW ONE :*
*EI0CF   *AWLF 1 Rating 83
        AWLF 1 RX Rating 84


*4. Some personal pdf files have been updated in "AWLF Data by Calls":*
*2E0ILY* *AWLF, **AWLF RX**   EI0CF* *AWLF RX**   G0LUJ* *AWLF RX**   G0MRF=
*
*AWLF,** AWLF RX**   K3MF* *AWLF**, AWLF TX**   NO3M* *AWLF**, AWLF TX*


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order* , *Mode(Cat)/Date*
*http://136.73.ru/h_qso <http://136.73.ru/h_qso>http://136.73.ru/h_qso
<http://136.73.ru/h_qso>*     (maybe refresh frame)

73! Alex R7NT  *http://136.73.ru <http://136.73.ru/>*

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ng=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif">Dear LF e=
nthusiasts,<br>
=C2=A0AWLF=C2=A0</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-=
family:Arial,sans-serif;color:blue"><a href=3D"http://136.73.ru/h_aw" style=
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yle=3D"font-size:9pt;font-family:Arial,sans-serif">=C2=A0=C2=A0</span><b><s=
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t;"><br>
<u>1. New database records have been added :</u></span></b><u><span lang=3D=
"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-serif"></span></u></p=
>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#686=C2=A0=C2=A0QRB=
=3D5238,8=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-22=C2=A0 K3MF =
=C2=A0=C2=A0=C2=A0=C2=A0-&gt; EI0CF
=C2=A0WSPR2</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(23,59,211)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
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e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#687=C2=A0=C2=A0QRB=
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=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
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t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-22=C2=A0 NO3M=
=C2=A0=C2=A0=C2=A0=C2=A0 -&gt; G0LUJ
=C2=A0WSPR2</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#689=C2=A0=C2=A0QRB=
=3D5685,7=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-22=C2=A0 NO3M=
=C2=A0=C2=A0=C2=A0=C2=A0 -&gt; 2E0ILY=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">#690=C2=A0=C2=A0QRB=
=3D5706,5=C2=A0=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:rgb(0,0,204)">2019-02-23=C2=A0 K3FM=
=C2=A0=C2=A0=C2=A0=C2=A0 -&gt; G0MRF
=C2=A0WSPR2</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><br></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">2.=C2=A0Ratin=
gs have been
updated :</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"><br>
<b>2E0ILY =C2=A0</b>AWLF 3 Rating 7</span><span lang=3D"EN-US" style=3D"fon=
t-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">=C2=A0</=
span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier =
New&quot;;color:white;background:rgb(23,59,211)">=E2=86=91</span><span lang=
=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color=
:black">=C2=A06<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
75</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A055</span><=
/p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">K3MF=
=C2=A0=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black">AWLF 2 Rating 9</span><span=
 lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;=
color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)=
">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:black">=C2=A02<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">A=
WLF 2 TX Rating
15</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A0</span><sp=
an lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot=
;;color:rgb(192,0,0)">11</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">G0MR=
F=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:black">AWLF 2 Rating 8 </span><span lan=
g=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;colo=
r:white;background:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" sty=
le=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)"=
>=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot=
;Courier New&quot;;color:black">6</span><span lang=3D"EN-US" style=3D"font-=
size:9pt;font-family:&quot;Courier New&quot;;color:black"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=
=A0 =C2=A0 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(0,102,0)">AWLF 1 RX Rating 118</span><span=
 lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;=
color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)=
">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A074</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">G0LU=
J=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-f=
amily:&quot;Courier New&quot;;color:black">AWLF 1 Rating 18 </span><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;col=
or:white;background:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)=
">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;;color:black">10</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" styl=
e=3D"font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=
=A0 =C2=A0 </span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&=
quot;Courier New&quot;;color:rgb(0,102,0)">AWLF 1 RX Rating 19</span><span =
lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;c=
olor:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9pt=
;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211)"=
>=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&q=
uot;Courier New&quot;;color:rgb(0,102,0)">=C2=A010</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">NO3M=
=C2=A0=C2=A0 =C2=A0</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:black">AWLF 1 Rating 49</span><spa=
n lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;=
;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:white;background:rgb(23,59,211=
)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black">=C2=A012<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)">A=
WLF 1 TX Rating
27</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cour=
ier New&quot;;color:rgb(191,0,0)">=C2=A0</span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:white;backgroun=
d:rgb(23,59,211)">=E2=86=91</span><span lang=3D"EN-US" style=3D"font-size:9=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">=C2=A0</span><sp=
an lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot=
;;color:rgb(192,0,0)">6</span><span lang=3D"EN-US" style=3D"font-size:9pt;f=
ont-family:&quot;Courier New&quot;;color:rgb(0,102,0)"></span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><br></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US=
" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;">3.=C2=A0NEW O=
NE :</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:=
&quot;Courier New&quot;;color:black"><br>
<b>EI0CF=C2=A0 =C2=A0</b>AWLF 1 Rating 83<br>
</span><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;">=C2=A0 =C2=A0 =C2=A0 =C2=A0 </span><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF 1 RX Rating
84</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 0.0001pt;line-height:normal;=
background-image:initial;background-position:initial;background-size:initia=
l;background-repeat:initial;background-origin:initial;background-clip:initi=
al;font-size:11pt;font-family:Calibri,sans-serif"><br></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:black">4.=C2=
=A0Some personal pdf files have been updated in
&quot;AWLF Data by Calls&quot;:</span></u></b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;"><br>
</span><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black">2E0ILY</span></b><b><span lang=3D"EN-US" style=
=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><s=
pan lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quo=
t;;color:black">AWLF,=C2=A0</span></i></b><b><i><span lang=3D"EN-US" style=
=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">A=
WLF RX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;;color:black"> =C2=A0=C2=A0EI0CF</span></b><b><=
i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New=
&quot;;color:black"> </span></i></b><b><i><span lang=3D"EN-US" style=3D"fon=
t-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX<=
/span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&q=
uot;Courier New&quot;;color:black"> =C2=A0=C2=A0G0LUJ</span></b><b><span la=
ng=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> <=
/span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&qu=
ot;Courier New&quot;;color:rgb(0,102,0)">AWLF RX</span></i></b><b><span lan=
g=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;;colo=
r:black"> =C2=A0=C2=A0G0MRF</span></b><b><span lang=3D"EN-US" style=3D"font=
-size:9pt;font-family:&quot;Courier New&quot;"> </span></b><b><i><span lang=
=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color=
:black">AWLF,</span></i></b><b><i><span lang=3D"EN-US" style=3D"font-size:8=
pt;font-family:&quot;Courier New&quot;;color:rgb(0,102,0)"> AWLF RX</span><=
/i></b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Cou=
rier New&quot;;color:black"> =C2=A0=C2=A0K3MF</span></b><b><span lang=3D"EN=
-US" style=3D"font-size:9pt;font-family:&quot;Courier New&quot;"> </span></=
b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Couri=
er New&quot;;color:black">AWLF</span></i></b><b><i><span lang=3D"EN-US" sty=
le=3D"font-size:8pt;font-family:&quot;Courier New&quot;;color:rgb(192,0,0)"=
>,=C2=A0AWLF TX</span></i></b><b><span lang=3D"EN-US" style=3D"font-size:9p=
t;font-family:&quot;Courier New&quot;;color:black">=C2=A0 =C2=A0NO3M</span>=
</b><b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quot;Courie=
r New&quot;"> </span></b><b><i><span lang=3D"EN-US" style=3D"font-size:8pt;=
font-family:&quot;Courier New&quot;;color:black">AWLF</span></i></b><b><i><=
span lang=3D"EN-US" style=3D"font-size:8pt;font-family:&quot;Courier New&qu=
ot;;color:rgb(192,0,0)">,=C2=A0AWLF TX</span></i></b></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><b><u><span lang=3D"EN-US" st=
yle=3D"font-size:9pt;font-family:&quot;Courier New&quot;">5. &quot;Best QSO=
s&quot; have been updated :<br>
</span></u></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">sorted in=C2=A0</span><b><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">QRB/=
Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:&quo=
t;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" style=3D"f=
ont-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0)">Chrono=
logical order</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;font-fa=
mily:&quot;Courier New&quot;">=C2=A0,=C2=A0</span><b><span lang=3D"EN-US" s=
tyle=3D"font-size:9pt;font-family:&quot;Courier New&quot;;color:rgb(191,0,0=
)">Mode(Cat)/Date</span></b><span lang=3D"EN-US" style=3D"font-size:9pt;fon=
t-family:&quot;Courier New&quot;;color:black"><br>
</span><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,san=
s-serif;color:blue"><a href=3D"http://136.73.ru/h_qso" style=3D"color:blue"=
>http://136.73.ru/h_qso</a><a href=3D"http://136.73.ru/h_qso" style=3D"colo=
r:blue">http://136.73.ru/h_qso</a></span></u><span lang=3D"EN-US" style=3D"=
font-size:9pt;font-family:&quot;Courier New&quot;">=C2=A0 =C2=A0 =C2=A0(may=
be refresh frame)</span></p>

<p class=3D"MsoNormal" style=3D"margin:0cm 0cm 12pt;line-height:normal;back=
ground-image:initial;background-position:initial;background-size:initial;ba=
ckground-repeat:initial;background-origin:initial;background-clip:initial;f=
ont-size:11pt;font-family:Calibri,sans-serif"><span lang=3D"EN-US" style=3D=
"font-size:9pt;font-family:Arial,sans-serif">73! Alex R7NT=C2=A0=C2=A0</spa=
n><u><span lang=3D"EN-US" style=3D"font-size:9pt;font-family:Arial,sans-ser=
if;color:blue"><a href=3D"http://136.73.ru/" style=3D"color:blue">http://13=
6.73.ru</a></span></u><span lang=3D"EN-US" style=3D"font-size:9pt;font-fami=
ly:Arial,sans-serif"></span></p></div>

--000000000000fe9ec70582a5ecec--

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Date: Sun, 24 Feb 2019 16:19:03 +0000 (UTC)
From: Markus Vester <markusvester@aol.com>
To: rsgb_lf_group@blacksheep.org
Message-ID: <752184680.4363593.1551025143826@mail.yahoo.com>
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 Content preview:  Looks like Riccardo is sending a carrier on 8269.997 today.
    Good luck, Markus  -----Ursprüngliche Mitteilung----- Von: Riccardo Zoli
    An: LF Group Verschickt: So, 17. Feb. 2019 22:21 Betreff: Re: VLF: 8270 
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Subject: VLF: 8269.997 Hz
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------=_Part_4363592_1965755368.1551025143824
Content-Type: text/plain; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

Looks like Riccardo is sending a=C2=A0carrier on 8269.997 today.

Good luck,
Markus=C2=A0


-----Urspr=C3=BCngliche Mitteilung-----
Von: Riccardo Zoli <riccardozoli80@gmail.com>
An: LF Group <rsgb_lf_group@blacksheep.org>
Verschickt: So, 17. Feb. 2019 22:21
Betreff: Re: VLF: 8270

Stefan, VLF,
Yes, it's me! :-) I'm trying with a continuous carrier on 8270.003 Hz.Thank=
s for your report, Stefan: very good performance of your VLF grabber (that =
was offline during my last VLF transmission on late december 2018).Tomorrow=
 I'll try to send a few characters if the noise will remain low.Unfortunate=
ly at this moment the humidity is rising and I think I will go QRT before m=
idnight.
=C2=A0All the best

73 de Riccardo IW4DXW

P.S.: congrats for your latest (of a long series) fantastic results on the =
ELF band. :-)


Il giorno Dom 17 Feb 2019, 16:25 DK7FC <selberdenken@posteo.de> ha scritto:

Hi VLF,

Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus,=20
maybe it is Riccardo? It is a good signal=C2=A0 on the local grabbers such =
as
http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html or
https://vlf.u01.de/

Who is it ?

73, Stefan



------=_Part_4363592_1965755368.1551025143824
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: quoted-printable

<div style=3D"font-size:10pt;font-family:arial,helvetica,sans-serif;color:b=
lack;"><div style=3D"color: black; font-family: arial,helvetica,sans-serif;=
 font-size: 10pt;" abp=3D"300">Looks like Riccardo is sending a&nbsp;carrie=
r on 8269.997 today.<br><br>Good luck,<br>Markus&nbsp;<br abp=3D"301"><br a=
bp=3D"302"><br abp=3D"303">-----Urspr=C3=BCngliche Mitteilung-----<br abp=
=3D"304">Von: Riccardo Zoli &lt;riccardozoli80@gmail.com&gt;<br abp=3D"305"=
>An: LF Group &lt;rsgb_lf_group@blacksheep.org&gt;<br abp=3D"306">Verschick=
t: So, 17. Feb. 2019 22:21<br abp=3D"307">Betreff: Re: VLF: 8270<br abp=3D"=
308"><br clear=3D"none" abp=3D"314"></div><div id=3D"yiv6367657040" abp=3D"=
310"><div abp=3D"311"><div abp=3D"312"><div abp=3D"315">Stefan, VLF,</div><=
div abp=3D"316"><br clear=3D"none" abp=3D"317"></div><div abp=3D"318">Yes, =
it's me! :-) I'm trying with a continuous carrier on 8270.003 Hz.</div><div=
 abp=3D"319">Thanks for your report, Stefan: very good performance of your =
VLF grabber (that was offline during my last VLF transmission on late decem=
ber 2018).</div><div abp=3D"320">Tomorrow I'll try to send a few characters=
 if the noise will remain low.</div><div abp=3D"321">Unfortunately at this =
moment the humidity is rising and I think I will go QRT before midnight.</d=
iv><div abp=3D"322"><br clear=3D"none" abp=3D"325">&nbsp;</div><div abp=3D"=
326">All the best</div><div abp=3D"327"><br clear=3D"none" abp=3D"328"></di=
v><div abp=3D"329"><br clear=3D"none" abp=3D"330"></div><div abp=3D"331">73=
 de Riccardo IW4DXW</div><div abp=3D"332"><br clear=3D"none" abp=3D"333"></=
div><div abp=3D"334"><br clear=3D"none" abp=3D"335"></div><div abp=3D"336">=
P.S.: congrats for your latest (of a long series) fantastic results on the =
ELF band. :-)</div><div abp=3D"337"><br clear=3D"none" abp=3D"338"></div><b=
r clear=3D"none" abp=3D"339"><br clear=3D"none" abp=3D"340"><div class=3D"y=
iv6367657040yqt6161655750" id=3D"yiv6367657040yqt09507" abp=3D"341"><div cl=
ass=3D"yiv6367657040gmail_quote" abp=3D"342"><div dir=3D"ltr" abp=3D"343">I=
l giorno Dom 17 Feb 2019, 16:25 DK7FC &lt;<a href=3D"mailto:selberdenken@po=
steo.de" target=3D"_blank" rel=3D"noopener noreferrer" shape=3D"rect" abp=
=3D"344" ymailto=3D"mailto:selberdenken@posteo.de">selberdenken@posteo.de</=
a>&gt; ha scritto:<br clear=3D"none" abp=3D"345"></div><blockquote class=3D=
"yiv6367657040gmail_quote" style=3D"margin: 0px 0px 0px 0.8ex; padding-left=
: 1ex; border-left-color: rgb(204, 204, 204); border-left-width: 1px; borde=
r-left-style: solid;" abp=3D"346">Hi VLF,<br clear=3D"none" abp=3D"347">
<br clear=3D"none" abp=3D"348">
Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus, <br cle=
ar=3D"none" abp=3D"349">
maybe it is Riccardo? It is a good signal&nbsp; on the local grabbers such =
as<br clear=3D"none" abp=3D"350">
<a href=3D"http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2=
.html" target=3D"_blank" rel=3D"noopener noreferrer" shape=3D"rect" abp=3D"=
351">http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html<=
/a> or<br clear=3D"none" abp=3D"352">
<a href=3D"https://vlf.u01.de/" target=3D"_blank" rel=3D"noopener noreferre=
r" shape=3D"rect" abp=3D"353">https://vlf.u01.de/</a><br clear=3D"none" abp=
=3D"354">
<br clear=3D"none" abp=3D"355">
Who is it ?<br clear=3D"none" abp=3D"356">
<br clear=3D"none" abp=3D"357">
73, Stefan<br clear=3D"none" abp=3D"358">
<br clear=3D"none" abp=3D"359">
</blockquote></div></div>
</div></div></div></div>
------=_Part_4363592_1965755368.1551025143824--

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From: Eric NO3M <no3m@no3m.net>
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 Content preview:  Andy This recommendation is all well and good, but seems applicable
    to only CW where either the operator is manually keying or using computer
    controlled keying with a constant carrier input. With digi modes (WSPR, JT9,
    etc.) that do not present a constant RF input, the traditional PTT signaling
    is of no use as it keys active prior to the RF envelope start and goes inactive
    after the RF en [...] 
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Subject: Re: LF: Re: Class D current spikes
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--------------FD2AB5AB36422392F9BEC655
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Andy

This recommendation is all well and good, but seems applicable to only 
CW where either the operator is manually keying or using computer 
controlled keying with a constant carrier input.

With digi modes (WSPR, JT9, etc.) that do not present a constant RF 
input, the traditional PTT signaling is of no use as it keys active 
prior to the RF envelope start and goes inactive after the RF envelope 
ends.  The spikes would still be present and problematic.

Other than Rik's suggestion of killing the lingering active high driver 
output, it seems that only using a supply control scheme (whether driver 
or FET drain supply) would require sampling the original RF input to 
detect the end of the envelope and apply the key up (inactive) signal.  
Prior to reaching the driver subsystem, the input RF would need to be 
delayed by some amount.

73 Eric NO3M


On 2/24/19 9:41 AM, Andy Talbot wrote:
> For on-off keying of a switch mode PA you really should be using 
> supply line control.  Switching the drive then trying to reduce rise 
> /fall times for keyclick elimination by controlling drive 
> amplitude(something that seems to be done in some designs) is really 
> asking for trouble.  Even hard-switching drive gives its problems , as 
> we see here repeatedly
>
> Instead, why not a simple emitter follower in the positive supply, 
> then you can apply waveform shaping  to the base drive at low current, 
> where you've got full control.   Even a 20A supply could be controlled 
> this way with a suitably rated transistor.  Quite likely have to be a 
> Darlington.   There will be a slight fixed drop across it, say 1V at 
> saturation / full power, so a few watts of dissipation, but it's only 
> operating non saturated for a short period during the rise / fall times.
>
> A power FET could be used, but you'd need a drive voltage Vgs higher 
> than the supply, albeit only a few mA capability; nothing a small 
> switcher module couldn't manage.
>
> Andy
> www.g4jnt.com <http://www.g4jnt.com>
>
>
>


--------------FD2AB5AB36422392F9BEC655
Content-Type: text/html; charset=utf-8
Content-Transfer-Encoding: 8bit

<html>
  <head>
    <meta http-equiv="Content-Type" content="text/html; charset=UTF-8">
  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    Andy<br>
    <br>
    This recommendation is all well and good, but seems applicable to
    only CW where either the operator is manually keying or using
    computer controlled keying with a constant carrier input.<br>
    <br>
    With digi modes (WSPR, JT9, etc.) that do not present a constant RF
    input, the traditional PTT signaling is of no use as it keys active
    prior to the RF envelope start and goes inactive after the RF
    envelope ends.  The spikes would still be present and problematic. <br>
    <br>
    Other than Rik's suggestion of killing the lingering active high
    driver output, it seems that only using a supply control scheme
    (whether driver or FET drain supply) would require sampling the
    original RF input to detect the end of the envelope and apply the
    key up (inactive) signal.  Prior to reaching the driver subsystem,
    the input RF would need to be delayed by some amount.<br>
    <br>
    73 Eric NO3M<br>
    <br>
    <br>
    <div class="moz-cite-prefix">On 2/24/19 9:41 AM, Andy Talbot wrote:<br>
    </div>
    <blockquote type="cite"
cite="mid:CAA8k23Ta-zh3Kvnpe79qt3ame-H_mQdZuJXyzxg8L2tWRiZ0Dg@mail.gmail.com">
      <meta http-equiv="content-type" content="text/html; charset=UTF-8">
      <div dir="ltr">
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small">For
          on-off keying of a switch mode PA you really should be using
          supply line control.  Switching the drive then trying to
          reduce rise /fall times for keyclick elimination by
          controlling drive amplitude(something that seems to be done in
          some designs) is really asking for trouble.  Even
          hard-switching drive gives its problems , as we see here
          repeatedly</div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small"><br>
        </div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small">Instead,
          why not a simple emitter follower in the positive supply, then
          you can apply waveform shaping  to the base drive at low
          current, where you've got full control.   Even a 20A supply
          could be controlled this way with a suitably rated
          transistor.  Quite likely have to be a Darlington.   There
          will be a slight fixed drop across it, say 1V at saturation /
          full power, so a few watts of dissipation, but it's only
          operating non saturated for a short period during the rise /
          fall times.</div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small"><br>
        </div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small">A power
          FET could be used, but you'd need a drive voltage Vgs higher
          than the supply, albeit only a few mA capability; nothing a
          small switcher module couldn't manage.</div>
        <div class="gmail_default"
          style="font-family:tahoma,sans-serif;font-size:small"> <br>
        </div>
        <div>
          <div dir="ltr" class="gmail_signature"
            data-smartmail="gmail_signature">
            <div dir="ltr">
              <div>
                <div dir="ltr">
                  <div>
                    <div dir="ltr">
                      <div>
                        <div dir="ltr">
                          <div>
                            <div dir="ltr">Andy
                              <div><span style="font-size:12.8px"><a
                                    href="http://www.g4jnt.com"
                                    target="_blank"
                                    moz-do-not-send="true">www.g4jnt.com</a></span><br>
                              </div>
                              <div><br>
                              </div>
                            </div>
                          </div>
                        </div>
                      </div>
                    </div>
                  </div>
                </div>
              </div>
            </div>
          </div>
        </div>
        <br>
      </div>
      <br>
    </blockquote>
    <br>
  </body>
</html>

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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Sun, 24 Feb 2019 18:20:02 +0000
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To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
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 Content preview:  IN that case some sort of protection needs to be incorporated
    - and few have come up with really properly designed and foolproof circuitry.
    I use the technique adopted in the hold Decca transmitters, [...] 
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Subject: Re: LF: Re: Class D current spikes
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Content-Type: text/plain; charset="UTF-8"

IN that case some sort of protection needs to be incorporated - and few
have come up with really properly designed and foolproof circuitry.
I use the technique adopted in the hold Decca transmitters, detailed here
http://g4jnt.com/137tx.pdf  but it assumes a tank circuit is in use.    For
transformer and traditional PI/Tee LPF arrangements it's not applicable

I don't know of anyone who has used this technique outside designs based
around that article that I've been told about- which seems amazing
considering how absolutely robust and foolproof it is.   Complete overload
protection against any mismatch.

I've seen all sorts of overload protection circuitry in use, current
monitors and trips, Hall sensors etc etc  But if there is going to be a
current spike then it has to be designed-out in the first place.   Choke
fed PAs could perhaps have a bigger choke that can absorb a few 100us .
 Put voltage clamps in if overvoltage is the problem.  Just Schottky diodes
up and down to the rails.

Andy
www.g4jnt.com



On Sun, 24 Feb 2019 at 18:08, Eric NO3M <no3m@no3m.net> wrote:

> Andy
>
> This recommendation is all well and good, but seems applicable to only CW
> where either the operator is manually keying or using computer controlled
> keying with a constant carrier input.
>
> With digi modes (WSPR, JT9, etc.) that do not present a constant RF input,
> the traditional PTT signaling is of no use as it keys active prior to the
> RF envelope start and goes inactive after the RF envelope ends.  The spikes
> would still be present and problematic.
>
> Other than Rik's suggestion of killing the lingering active high driver
> output, it seems that only using a supply control scheme (whether driver or
> FET drain supply) would require sampling the original RF input to detect
> the end of the envelope and apply the key up (inactive) signal.  Prior to
> reaching the driver subsystem, the input RF would need to be delayed by
> some amount.
>
> 73 Eric NO3M
>
>
> On 2/24/19 9:41 AM, Andy Talbot wrote:
>
> For on-off keying of a switch mode PA you really should be using supply
> line control.  Switching the drive then trying to reduce rise /fall times
> for keyclick elimination by controlling drive amplitude(something that
> seems to be done in some designs) is really asking for trouble.  Even
> hard-switching drive gives its problems , as we see here repeatedly
>
> Instead, why not a simple emitter follower in the positive supply, then
> you can apply waveform shaping  to the base drive at low current, where
> you've got full control.   Even a 20A supply could be controlled this way
> with a suitably rated transistor.  Quite likely have to be a Darlington.
>  There will be a slight fixed drop across it, say 1V at saturation / full
> power, so a few watts of dissipation, but it's only operating non saturated
> for a short period during the rise / fall times.
>
> A power FET could be used, but you'd need a drive voltage Vgs higher than
> the supply, albeit only a few mA capability; nothing a small switcher
> module couldn't manage.
>
> Andy
> www.g4jnt.com
>
>
>
>
>

--0000000000009131960582a7e009
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div dir=3D"ltr"><div class=3D"gmail_default" style=3D"fon=
t-family:tahoma,sans-serif;font-size:small">IN that case some sort of prote=
ction needs to be incorporated - and few have come up with really properly =
designed and foolproof circuitry.</div><div class=3D"gmail_default" style=
=3D"font-family:tahoma,sans-serif;font-size:small">I use the technique adop=
ted in the hold Decca transmitters, detailed here=C2=A0<a href=3D"http://g4=
jnt.com/137tx.pdf">http://g4jnt.com/137tx.pdf</a>=C2=A0 but it assumes a ta=
nk circuit is in use.=C2=A0 =C2=A0 For transformer and traditional PI/Tee L=
PF arrangements it&#39;s not applicable</div><div class=3D"gmail_default" s=
tyle=3D"font-family:tahoma,sans-serif;font-size:small"><br></div><div class=
=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small">=
I don&#39;t know of anyone who has used this technique outside designs base=
d around that article that I&#39;ve been told about- which seems amazing co=
nsidering how absolutely robust and foolproof it is.=C2=A0 =C2=A0Complete o=
verload protection against any mismatch.=C2=A0 =C2=A0</div><div class=3D"gm=
ail_default" style=3D"font-family:tahoma,sans-serif;font-size:small"><br></=
div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;fon=
t-size:small">I&#39;ve seen all sorts of overload protection circuitry in u=
se, current monitors and trips, Hall sensors etc etc=C2=A0 But if there is =
going to be a current spike then it has to be designed-out in the first pla=
ce.=C2=A0 =C2=A0Choke fed PAs could perhaps have a bigger choke that can ab=
sorb a few 100us .=C2=A0 =C2=A0Put voltage clamps in if overvoltage is the =
problem.=C2=A0 Just Schottky diodes up and down to the rails.</div><div cla=
ss=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small=
"><br></div><div><div dir=3D"ltr" class=3D"gmail_signature"><div dir=3D"ltr=
"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr"><div><d=
iv dir=3D"ltr">Andy<div><span style=3D"font-size:12.8px"><a href=3D"http://=
www.g4jnt.com" target=3D"_blank">www.g4jnt.com</a></span><br></div><div><br=
></div></div></div></div></div></div></div></div></div></div></div></div><b=
r></div></div><br><div class=3D"gmail_quote"><div dir=3D"ltr" class=3D"gmai=
l_attr">On Sun, 24 Feb 2019 at 18:08, Eric NO3M &lt;<a href=3D"mailto:no3m@=
no3m.net">no3m@no3m.net</a>&gt; wrote:<br></div><blockquote class=3D"gmail_=
quote" style=3D"margin:0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,=
204);padding-left:1ex">
 =20
   =20
 =20
  <div bgcolor=3D"#FFFFFF">
    Andy<br>
    <br>
    This recommendation is all well and good, but seems applicable to
    only CW where either the operator is manually keying or using
    computer controlled keying with a constant carrier input.<br>
    <br>
    With digi modes (WSPR, JT9, etc.) that do not present a constant RF
    input, the traditional PTT signaling is of no use as it keys active
    prior to the RF envelope start and goes inactive after the RF
    envelope ends.=C2=A0 The spikes would still be present and problematic.=
 <br>
    <br>
    Other than Rik&#39;s suggestion of killing the lingering active high
    driver output, it seems that only using a supply control scheme
    (whether driver or FET drain supply) would require sampling the
    original RF input to detect the end of the envelope and apply the
    key up (inactive) signal.=C2=A0 Prior to reaching the driver subsystem,
    the input RF would need to be delayed by some amount.<br>
    <br>
    73 Eric NO3M<br>
    <br>
    <br>
    <div class=3D"gmail-m_3222824818606889367moz-cite-prefix">On 2/24/19 9:=
41 AM, Andy Talbot wrote:<br>
    </div>
    <blockquote type=3D"cite">
     =20
      <div dir=3D"ltr">
        <div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small">For
          on-off keying of a switch mode PA you really should be using
          supply line control.=C2=A0 Switching the drive then trying to
          reduce rise /fall times for keyclick elimination by
          controlling drive amplitude(something that seems to be done in
          some designs) is really asking for trouble.=C2=A0 Even
          hard-switching drive gives its problems , as we see here
          repeatedly</div>
        <div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small"><br>
        </div>
        <div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small">Instead,
          why not a simple emitter follower in the positive supply, then
          you can apply waveform shaping=C2=A0 to the base drive at low
          current, where you&#39;ve got full control.=C2=A0 =C2=A0Even a 20=
A supply
          could be controlled this way with a suitably rated
          transistor.=C2=A0 Quite likely have to be a Darlington.=C2=A0 =C2=
=A0There
          will be a slight fixed drop across it, say 1V at saturation /
          full power, so a few watts of dissipation, but it&#39;s only
          operating non saturated for a short period during the rise /
          fall times.</div>
        <div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small"><br>
        </div>
        <div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small">A power
          FET could be used, but you&#39;d need a drive voltage Vgs higher
          than the supply, albeit only a few mA capability; nothing a
          small switcher module couldn&#39;t manage.</div>
        <div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif=
;font-size:small">=C2=A0<br>
        </div>
        <div>
          <div dir=3D"ltr" class=3D"gmail-m_3222824818606889367gmail_signat=
ure">
            <div dir=3D"ltr">
              <div>
                <div dir=3D"ltr">
                  <div>
                    <div dir=3D"ltr">
                      <div>
                        <div dir=3D"ltr">
                          <div>
                            <div dir=3D"ltr">Andy
                              <div><span style=3D"font-size:12.8px"><a href=
=3D"http://www.g4jnt.com" target=3D"_blank">www.g4jnt.com</a></span><br>
                              </div>
                              <div><br>
                              </div>
                            </div>
                          </div>
                        </div>
                      </div>
                    </div>
                  </div>
                </div>
              </div>
            </div>
          </div>
        </div>
        <br>
      </div>
      <br>
    </blockquote>
    <br>
  </div>

</blockquote></div>

--0000000000009131960582a7e009--

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Subject: Re: LF: Re: Class D current spikes
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Eric

One or two FETs per phase?

Jay W1VD





----- Original Message -----
From: Eric NO3M <no3m@no3m.net>
Reply-To: <rsgb_lf_group@blacksheep.org>
To: <rsgb_lf_group@blacksheep.org>
Sent: 2/24/2019 1:04:52 PM
Subject: Re: LF: Re: Class D current spikes


Andy

This recommendation is all well and good, but seems applicable to only=
 CW where=20
either the operator is manually keying or using computer controlled ke=
ying with=20
a constant carrier input.

With digi modes (WSPR, JT9, etc.) that do not present a constant RF in=
put, the=20
traditional PTT signaling is of no use as it keys active prior to the =
RF=20
envelope start and goes inactive after the RF envelope ends.  The spik=
es would=20
still be present and problematic.=20

Other than=20
Rik's suggestion of killing the lingering active high driver output, i=
t seems that only using a supply control scheme (whether driver or FET=
 drain supply) would require sampling the original RF input to detect =
the end of the envelope and apply the key up (inactive) signal.  Prior=
 to reaching the driver subsystem, the input RF would need to be delay=
ed by some amount.

73 Eric NO3M



On 2/24/19 9:41 AM, Andy Talbot wrote:

For on-off keying of a switch mode PA you really should be using suppl=
y line control.  Switching the drive then trying to reduce rise /fall =
times for keyclick elimination by controlling drive amplitude(somethin=
g that seems to be done in some designs) is really asking for trouble.=
  Even hard-switching drive gives its problems , as we see here repeat=
edly


Instead, why not a simple emitter follower in the positive supply, the=
n you can apply waveform shaping  to the base drive at low current, wh=
ere you've=20
got full control.   Even a 20A supply could be controlled this way wit=
h a=20
suitably rated transistor.  Quite likely have to be a Darlington.   Th=
ere will=20
be a slight fixed drop across it, say 1V at saturation / full power, s=
o a few=20
watts of dissipation, but=20
it's only operating non saturated for a short period during the rise /=
 fall times.


A power FET could be used, but you'd=20
need a drive voltage Vgs higher than the supply, albeit only a few mA=20=

capability; nothing a small switcher module couldn't manage.


Andy=20
www.g4jnt.com

--EUHVcWIkh9sX0kiM=_tO6LDTMlqrnXJBRa
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<HTML><HEAD>
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CFntDef div { font-family:Arial,"Segoe UI",Tahoma,Verdana,Helvetica,sa=
ns-serif;font-size:10pt; }</STYLE>

<META name=3DGENERATOR content=3D"MSHTML 11.00.9600.18450"></HEAD>
<BODY spellcheck=3Dtrue class=3DOECFntDef>
<DIV>Eric</DIV>
<DIV>&nbsp;</DIV>
<DIV>One&nbsp;or two FETs per phase?</DIV>
<DIV>&nbsp;</DIV>
<DIV>Jay W1VD</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE style=3D"PADDING-BOTTOM: 0px; PADDING-TOP: 0px; PADDING-LE=
FT: 0.5em; MARGIN: 0px 0px 0px 0.5em; BORDER-LEFT: #c7e5ff 1px solid; =
PADDING-RIGHT: 0px">
<DIV><B>----- Original Message -----</B></DIV>
<DIV><B>From:</B> Eric NO3M &lt;<A href=3D"mailto:no3m@no3m.net">no3m@=
no3m.net</A>&gt;</DIV>
<DIV><B>Reply-To:</B> &lt;<A href=3D"mailto:rsgb_lf_group@blacksheep.o=
rg">rsgb_lf_group@blacksheep.org</A>&gt;</DIV>
<DIV><B>To:</B> &lt;<A href=3D"mailto:rsgb_lf_group@blacksheep.org">rs=
gb_lf_group@blacksheep.org</A>&gt;</DIV>
<DIV><B>Sent:</B> 2/24/2019 1:04:52 PM</DIV>
<DIV><B>Subject:</B> Re: LF: Re: Class D current spikes</DIV>
<HR style=3D"BORDER-TOP: medium none; HEIGHT: 1px; BORDER-RIGHT: mediu=
m none; BORDER-BOTTOM: medium none; COLOR: #ccc; BORDER-LEFT: medium n=
one; BACKGROUND-COLOR: #ccc">
Andy<BR><BR>This recommendation is all well and good, but seems applic=
able to only CW where either the operator is manually keying or using =
computer controlled keying with a constant carrier input.<BR><BR>With =
digi modes (WSPR, JT9, etc.) that do not present a constant RF input, =
the traditional PTT signaling is of no use as it keys active prior to =
the RF envelope start and goes inactive after the RF envelope ends.&nb=
sp; The spikes would still be present and problematic. <BR><BR>Other t=
han Rik's suggestion of killing the lingering active high driver outpu=
t, it seems that only using a supply control scheme (whether driver or=
 FET drain supply) would require sampling the original RF input to det=
ect the end of the envelope and apply the key up (inactive) signal.&nb=
sp; Prior to reaching the driver subsystem, the input RF would need to=
 be delayed by some amount.<BR><BR>73 Eric NO3M<BR><BR><BR>
<DIV class=3Dmoz-cite-prefix>On 2/24/19 9:41 AM, Andy Talbot wrote:<BR=
></DIV>
<BLOCKQUOTE cite=3Dmid:CAA8k23Ta-zh3Kvnpe79qt3ame-H_mQdZuJXyzxg8L2tWRi=
Z0Dg@mail.gmail.com type=3D"cite">
<DIV dir=3Dltr>
<DIV class=3Dgmail_default style=3D"FONT-SIZE: small; FONT-FAMILY: tah=
oma,sans-serif">For on-off keying of a switch mode PA you really shoul=
d be using supply line control.&nbsp; Switching the drive then trying =
to reduce rise /fall times for keyclick elimination by controlling dri=
ve amplitude(something that seems to be done in some designs) is reall=
y asking for trouble.&nbsp; Even hard-switching drive gives its proble=
ms , as we see here repeatedly</DIV>
<DIV class=3Dgmail_default style=3D"FONT-SIZE: small; FONT-FAMILY: tah=
oma,sans-serif"><BR></DIV>
<DIV class=3Dgmail_default style=3D"FONT-SIZE: small; FONT-FAMILY: tah=
oma,sans-serif">Instead, why not a simple emitter follower in the posi=
tive supply, then you can apply waveform shaping&nbsp; to the base dri=
ve at low current, where you've got full control.&nbsp; &nbsp;Even a 2=
0A supply could be controlled this way with a suitably rated transisto=
r.&nbsp; Quite likely have to be a Darlington.&nbsp; &nbsp;There will =
be a slight fixed drop across it, say 1V at saturation / full power, s=
o a few watts of dissipation, but it's only operating non saturated fo=
r a short period during the rise / fall times.</DIV>
<DIV class=3Dgmail_default style=3D"FONT-SIZE: small; FONT-FAMILY: tah=
oma,sans-serif"><BR></DIV>
<DIV class=3Dgmail_default style=3D"FONT-SIZE: small; FONT-FAMILY: tah=
oma,sans-serif">A power FET could be used, but you'd need a drive volt=
age Vgs higher than the supply, albeit only a few mA capability; nothi=
ng a small switcher module couldn't manage.</DIV>
<DIV class=3Dgmail_default style=3D"FONT-SIZE: small; FONT-FAMILY: tah=
oma,sans-serif"><BR>&nbsp;</DIV>
<DIV>
<DIV class=3Dgmail_signature dir=3Dltr data-smartmail=3D"gmail_signatu=
re">
<DIV dir=3Dltr>
<DIV>
<DIV dir=3Dltr>
<DIV>
<DIV dir=3Dltr>
<DIV>
<DIV dir=3Dltr>
<DIV>
<DIV dir=3Dltr>Andy=20
<DIV><SPAN style=3D"FONT-SIZE: 12px"><A href=3D"http://www.g4jnt.com/"=
 target=3D_blank moz-do-not-send=3D"true">www.g4jnt.com</A></SPAN><BR>=
</DIV>
<DIV><BR></DIV></DIV></DIV></DIV></DIV></DIV></DIV></DIV></DIV></DIV><=
/DIV></DIV><BR></DIV><BR></BLOCKQUOTE><BR></BLOCKQUOTE></BODY></HTML>

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From: Eric NO3M <no3m@no3m.net>
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 Content preview:  Jay Just one FET (59N25) on each side. On 2/24/19 3:26 PM,
    jrusgrove@comcast.net wrote: > Eric > One or two FETs per phase? > Jay W1VD
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Subject: Re: LF: Re: Class D current spikes
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Jay

Just one FET (59N25) on each side.



On 2/24/19 3:26 PM, jrusgrove@comcast.net wrote:
> Eric
> One or two FETs per phase?
> Jay W1VD

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    Jay<br>
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    Just one FET (59N25) on each side.<br>
    <br>
    <br>
    <br>
    <div class="moz-cite-prefix">On 2/24/19 3:26 PM,
      <a class="moz-txt-link-abbreviated" href="mailto:jrusgrove@comcast.net">jrusgrove@comcast.net</a> wrote:<br>
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      <div>One or two FETs per phase?</div>
      <div> </div>
      <div>Jay W1VD</div>
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 Content preview:  Try using a synchronous keying circuit, only uses a few ics
    and is reliable. I have used it on a modified Decca 5501 on 136 and a similar
    tx on 475 with no blown fets even to a short circuit, guard ci [...] 
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Subject: Re: LF: Re: Class D current spikes
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Try using a synchronous keying circuit, only uses a few ics and is reliable=
. I have used it on a modified Decca 5501 on 136 and a similar tx on 475 wi=
th no blown fets even to a short circuit, guard circuit used as in the decc=
a design.73 Dave
=20
=20
=20
-----Original Message-----
From: Eric NO3M <no3m@no3m.net>
To: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Sent: Sun, 24 Feb 2019 18:07
Subject: Re: LF: Re: Class D current spikes

 Andy
=20
 This recommendation is all well and good, but seems applicable to only CW =
where either the operator is manually keying or using computer controlled k=
eying with a constant carrier input.
=20
 With digi modes (WSPR, JT9, etc.) that do not present a constant RF input,=
 the traditional PTT signaling is of no use as it keys active prior to the =
RF envelope start and goes inactive after the RF envelope ends.=C2=A0 The s=
pikes would still be present and problematic.=20
=20
 Other than Rik's suggestion of killing the lingering active high driver ou=
tput, it seems that only using a supply control scheme (whether driver or F=
ET drain supply) would require sampling the original RF input to detect the=
 end of the envelope and apply the key up (inactive) signal.=C2=A0 Prior to=
 reaching the driver subsystem, the input RF would need to be delayed by so=
me amount.
=20
 73 Eric NO3M
=20
=20
 On 2/24/19 9:41 AM, Andy Talbot wrote:
 =20
=20
 For on-off keying of a switch mode PA you really should be using supply li=
ne control.=C2=A0 Switching the drive then trying to reduce rise /fall time=
s for keyclick elimination by controlling drive amplitude(something that se=
ems to be done in  some designs) is really asking for trouble.=C2=A0 Even h=
ard-switching drive gives its problems , as we see here repeatedly=20
  Instead, why not a simple emitter follower in the positive supply, then y=
ou can apply waveform shaping=C2=A0 to the base drive at low current, where=
 you've got full control.=C2=A0 =C2=A0Even a 20A supply could be controlled=
 this way with a suitably rated transistor.=C2=A0 Quite likely have to be a=
 Darlington.=C2=A0 =C2=A0There will be a slight fixed drop across it, say 1=
V at saturation / full power, so a few watts of dissipation, but it's only =
operating non saturated for a short period during the rise / fall times.=20
  A power FET could be used, but you'd need a drive voltage Vgs higher than=
 the supply, albeit only a few mA capability; nothing a small switcher modu=
le couldn't manage. =C2=A0
            Andy www.g4jnt.com
 =20
            =20
 =20
=20
=20
------=_Part_4685788_492961906.1551085336679
Content-Type: text/html; charset=UTF-8
Content-Transfer-Encoding: 7bit

<font color='black' size='2' face='arial'>
<div>Try<font size="2"> using a synchronous keying circuit, only uses a few ics and is reliable. I have used it on a modified Decca 5501 on 136 and a similar tx on 475 with no blown fets even to a short circuit, guard circuit used as in the decca design.</font></div>

<div><font size="2">73 Dave<br>
</font></div>

<div> <br>
</div>

<div> <br>
</div>

<div> <br>
</div>

<div style="font-family:arial,helvetica;font-size:10pt;color:black">-----Original Message-----<br>
From: Eric NO3M &lt;no3m@no3m.net&gt;<br>
To: rsgb_lf_group &lt;rsgb_lf_group@blacksheep.org&gt;<br>
Sent: Sun, 24 Feb 2019 18:07<br>
Subject: Re: LF: Re: Class D current spikes<br>
<br>

<div id="yiv1826142172">
<div>
    Andy<br clear="none">
    <br clear="none">
    This recommendation is all well and good, but seems applicable to
    only CW where either the operator is manually keying or using
    computer controlled keying with a constant carrier input.<br clear="none">
    <br clear="none">
    With digi modes (WSPR, JT9, etc.) that do not present a constant RF
    input, the traditional PTT signaling is of no use as it keys active
    prior to the RF envelope start and goes inactive after the RF
    envelope ends.&nbsp; The spikes would still be present and problematic. <br clear="none">
    <br clear="none">
    Other than Rik's suggestion of killing the lingering active high
    driver output, it seems that only using a supply control scheme
    (whether driver or FET drain supply) would require sampling the
    original RF input to detect the end of the envelope and apply the
    key up (inactive) signal.&nbsp; Prior to reaching the driver subsystem,
    the input RF would need to be delayed by some amount.<br clear="none">
    <br clear="none">
    73 Eric NO3M<br clear="none">
    <br clear="none">
    <br clear="none">
    
<div class="yiv1826142172yqt1949966360" id="yiv1826142172yqtfd25958">
<div class="yiv1826142172moz-cite-prefix">On 2/24/19 9:41 AM, Andy Talbot wrote:<br clear="none">
    </div>

    <blockquote type="cite">
      </blockquote></div>
</div>

<div class="yiv1826142172yqt1949966360" id="yiv1826142172yqtfd00351">
<div>
<div dir="ltr">
        
<div class="yiv1826142172gmail_default" style="font-family:tahoma, sans-serif;font-size:small;">For
          on-off keying of a switch mode PA you really should be using
          supply line control.&nbsp; Switching the drive then trying to
          reduce rise /fall times for keyclick elimination by
          controlling drive amplitude(something that seems to be done in
          some designs) is really asking for trouble.&nbsp; Even
          hard-switching drive gives its problems , as we see here
          repeatedly</div>

        
<div class="yiv1826142172gmail_default" style="font-family:tahoma, sans-serif;font-size:small;"><br clear="none">
        </div>

        
<div class="yiv1826142172gmail_default" style="font-family:tahoma, sans-serif;font-size:small;">Instead,
          why not a simple emitter follower in the positive supply, then
          you can apply waveform shaping&nbsp; to the base drive at low
          current, where you've got full control.&nbsp; &nbsp;Even a 20A supply
          could be controlled this way with a suitably rated
          transistor.&nbsp; Quite likely have to be a Darlington.&nbsp; &nbsp;There
          will be a slight fixed drop across it, say 1V at saturation /
          full power, so a few watts of dissipation, but it's only
          operating non saturated for a short period during the rise /
          fall times.</div>

        
<div class="yiv1826142172gmail_default" style="font-family:tahoma, sans-serif;font-size:small;"><br clear="none">
        </div>

        
<div class="yiv1826142172gmail_default" style="font-family:tahoma, sans-serif;font-size:small;">A power
          FET could be used, but you'd need a drive voltage Vgs higher
          than the supply, albeit only a few mA capability; nothing a
          small switcher module couldn't manage.</div>

        
<div class="yiv1826142172gmail_default" style="font-family:tahoma, sans-serif;font-size:small;">&nbsp;<br clear="none">
        </div>

        
<div>
          
<div class="yiv1826142172gmail_signature" dir="ltr">
            
<div dir="ltr">
              
<div>
                
<div dir="ltr">
                  
<div>
                    
<div dir="ltr">
                      
<div>
                        
<div dir="ltr">
                          
<div>
                            
<div dir="ltr">Andy
                              
<div><span style="font-size:12.8px;"><a rel="noopener noreferrer" shape="rect" target="_blank" href="http://www.g4jnt.com">www.g4jnt.com</a></span><br clear="none">
                              </div>

                              
<div><br clear="none">
                              </div>

                            </div>

                          </div>

                        </div>

                      </div>

                    </div>

                  </div>

                </div>

              </div>

            </div>

          </div>

        </div>

        <br clear="none">
      </div>

      <br clear="none">
    
    <br clear="none">
  </div>
</div>
</div>
</div>
</font>
------=_Part_4685788_492961906.1551085336679--

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From: Riccardo Zoli <riccardozoli80@gmail.com>
Date: Mon, 25 Feb 2019 14:10:43 +0100
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 Content preview:  Markus, VLF Yes, indeed: with DL0AO and Stefan's RDF there
    are no doubt :-) Yesterday the carrier was produced feeding my antenna with
    about 650mA but I think the noise was too high to attempt an EbNaut transmiss
    [...] 
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Subject: Re: VLF: 8269.997 Hz
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--000000000000b406330582b7abf9
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Markus, VLF

Yes, indeed: with DL0AO and Stefan's RDF there are no doubt :-)
Yesterday the carrier was produced feeding my antenna with about 650mA but
I think the noise was too high to attempt an EbNaut transmission.


All the best

73 de Riccardo IW4DXW



Il giorno Dom 24 Feb 2019, 17:21 Markus Vester <markusvester@aol.com> ha
scritto:

> Looks like Riccardo is sending a carrier on 8269.997 today.
>
> Good luck,
> Markus
>
>
> -----Urspr=C3=BCngliche Mitteilung-----
> Von: Riccardo Zoli <riccardozoli80@gmail.com>
> An: LF Group <rsgb_lf_group@blacksheep.org>
> Verschickt: So, 17. Feb. 2019 22:21
> Betreff: Re: VLF: 8270
>
> Stefan, VLF,
>
> Yes, it's me! :-) I'm trying with a continuous carrier on 8270.003 Hz.
> Thanks for your report, Stefan: very good performance of your VLF grabber
> (that was offline during my last VLF transmission on late december 2018).
> Tomorrow I'll try to send a few characters if the noise will remain low.
> Unfortunately at this moment the humidity is rising and I think I will go
> QRT before midnight.
>
>
> All the best
>
>
> 73 de Riccardo IW4DXW
>
>
> P.S.: congrats for your latest (of a long series) fantastic results on th=
e
> ELF band. :-)
>
>
>
> Il giorno Dom 17 Feb 2019, 16:25 DK7FC <selberdenken@posteo.de> ha
> scritto:
>
> Hi VLF,
>
> Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus,
> maybe it is Riccardo? It is a good signal  on the local grabbers such as
> http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2.html or
> https://vlf.u01.de/
>
> Who is it ?
>
> 73, Stefan
>
>
>

--000000000000b406330582b7abf9
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"auto"><div dir=3D"auto"><br></div><div dir=3D"auto">Markus, VLF=
</div><div dir=3D"auto"><br></div><div dir=3D"auto">Yes, indeed: with DL0AO=
 and Stefan&#39;s RDF there are no doubt :-)</div><div dir=3D"auto">Yesterd=
ay the carrier was produced feeding my antenna with about 650mA but I think=
 the noise was too high to attempt an EbNaut transmission.</div><div dir=3D=
"auto"><br></div><div dir=3D"auto"><br></div><div dir=3D"auto">All the best=
</div><div dir=3D"auto"><br></div><div dir=3D"auto">73 de Riccardo IW4DXW</=
div><div dir=3D"auto"><br></div><br><br><div class=3D"gmail_quote" dir=3D"a=
uto"><div dir=3D"ltr">Il giorno Dom 24 Feb 2019, 17:21 Markus Vester &lt;<a=
 href=3D"mailto:markusvester@aol.com" rel=3D"noreferrer noreferrer" target=
=3D"_blank">markusvester@aol.com</a>&gt; ha scritto:<br></div><blockquote c=
lass=3D"gmail_quote" style=3D"margin:0 0 0 .8ex;border-left:1px #ccc solid;=
padding-left:1ex"><div style=3D"font-size:10pt;font-family:arial,helvetica,=
sans-serif;color:black"><div style=3D"color:black;font-family:arial,helveti=
ca,sans-serif;font-size:10pt">Looks like Riccardo is sending a=C2=A0carrier=
 on 8269.997 today.<br><br>Good luck,<br>Markus=C2=A0<br><br><br>-----Urspr=
=C3=BCngliche Mitteilung-----<br>Von: Riccardo Zoli &lt;<a href=3D"mailto:r=
iccardozoli80@gmail.com" rel=3D"noreferrer noreferrer noreferrer" target=3D=
"_blank">riccardozoli80@gmail.com</a>&gt;<br>An: LF Group &lt;<a href=3D"ma=
ilto:rsgb_lf_group@blacksheep.org" rel=3D"noreferrer noreferrer noreferrer"=
 target=3D"_blank">rsgb_lf_group@blacksheep.org</a>&gt;<br>Verschickt: So, =
17. Feb. 2019 22:21<br>Betreff: Re: VLF: 8270<br><br clear=3D"none"></div><=
div id=3D"m_4699517367090353591m_350527375242899668m_-2783172161452174212yi=
v6367657040"><div><div><div>Stefan, VLF,</div><div><br clear=3D"none"></div=
><div>Yes, it&#39;s me! :-) I&#39;m trying with a continuous carrier on 827=
0.003 Hz.</div><div>Thanks for your report, Stefan: very good performance o=
f your VLF grabber (that was offline during my last VLF transmission on lat=
e december 2018).</div><div>Tomorrow I&#39;ll try to send a few characters =
if the noise will remain low.</div><div>Unfortunately at this moment the hu=
midity is rising and I think I will go QRT before midnight.</div><div><br c=
lear=3D"none">=C2=A0</div><div>All the best</div><div><br clear=3D"none"></=
div><div><br clear=3D"none"></div><div>73 de Riccardo IW4DXW</div><div><br =
clear=3D"none"></div><div><br clear=3D"none"></div><div>P.S.: congrats for =
your latest (of a long series) fantastic results on the ELF band. :-)</div>=
<div><br clear=3D"none"></div><br clear=3D"none"><br clear=3D"none"><div cl=
ass=3D"m_4699517367090353591m_350527375242899668m_-2783172161452174212yiv63=
67657040yqt6161655750" id=3D"m_4699517367090353591m_350527375242899668m_-27=
83172161452174212yiv6367657040yqt09507"><div class=3D"m_4699517367090353591=
m_350527375242899668m_-2783172161452174212yiv6367657040gmail_quote"><div di=
r=3D"ltr">Il giorno Dom 17 Feb 2019, 16:25 DK7FC &lt;<a href=3D"mailto:selb=
erdenken@posteo.de" rel=3D"noopener noreferrer noreferrer noreferrer norefe=
rrer" shape=3D"rect" target=3D"_blank">selberdenken@posteo.de</a>&gt; ha sc=
ritto:<br clear=3D"none"></div><blockquote class=3D"m_4699517367090353591m_=
350527375242899668m_-2783172161452174212yiv6367657040gmail_quote" style=3D"=
margin:0px 0px 0px 0.8ex;padding-left:1ex;border-left-color:rgb(204,204,204=
);border-left-width:1px;border-left-style:solid">Hi VLF,<br clear=3D"none">
<br clear=3D"none">
Someone is transmitting on 8270.03 Hz it seems. Not me, not Markus, <br cle=
ar=3D"none">
maybe it is Riccardo? It is a good signal=C2=A0 on the local grabbers such =
as<br clear=3D"none">
<a href=3D"http://www.iup.uni-heidelberg.de/schaefer_vlf/DK7FC_VLF_Grabber2=
.html" rel=3D"noopener noreferrer noreferrer noreferrer noreferrer" shape=
=3D"rect" target=3D"_blank">http://www.iup.uni-heidelberg.de/schaefer_vlf/D=
K7FC_VLF_Grabber2.html</a> or<br clear=3D"none">
<a href=3D"https://vlf.u01.de/" rel=3D"noopener noreferrer noreferrer noref=
errer noreferrer" shape=3D"rect" target=3D"_blank">https://vlf.u01.de/</a><=
br clear=3D"none">
<br clear=3D"none">
Who is it ?<br clear=3D"none">
<br clear=3D"none">
73, Stefan<br clear=3D"none">
<br><br clear=3D"none">
</blockquote></div></div>
</div></div></div></div></blockquote></div>
</div>

--000000000000b406330582b7abf9--

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 Content preview:  Hi Eric, What happens to the supply behaviour if you just
   switch some Cs parallel to the output, say 4x 4700 uF (low ESR) rated at 63V
    ? Maybe it solves the problem of the supply going into fault mode, althoug
    [...] 
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Subject: Re: LF: Class D current spikes
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Hi Eric,

What happens to the supply behaviour if you just switch some Cs parallel 
to the output, say 4x 4700 uF (low ESR) rated at 63V ?
Maybe it solves the problem of the supply going into fault mode, 
although it is no the perfect solution.

73, Stefan

Am 24.02.2019 13:08, schrieb Eric NO3M:
> I recently got a current mode (outp xfmr center tap not bypassed) 
> Class D amp going on 136khz, basically modeled after the W1VD / G0MRF 
> circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90 
> 42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on 
> the power supply in use:
>
> 30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
> 48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out
>
> I am also using the G0MRF keying circuit, ie. P-channel MOSFET 
> (IRF9540) in the driver (MCP1404) supply line.
>
> If the driver is left active (key down), the beginning and end of the 
> input RF envelope produces a "clicking" noise... assume this is from 
> current spikes being developed and sunk by the FET body diodes?  If 
> the driver is keyed with input RF already applied, thereby 
> interrupting the drive to the FETs, there is no such behavior.  The 
> keying is shaped, resulting in a ramping of the driver supply voltage 
> and resultant gate waveforms to the FETs.
>
> These current spikes do not bother my 30V linear power supply, 
> however, when I attempt to use a 48V switching supply (rated at 
> 17.7A), it seems to be OK with the current spike generated on the 
> beginning of the RF envelope, but not the spike at the end of the 
> envelope and goes into fault mode.  If the driver is keyed with 
> continuous RF applied, it's happy and does not trip out.  But keying 
> the driver doesn't seem practical for digi modes without some exotic 
> circuitry or engaging computer generated signaling to key down *after* 
> RF drive is applied and key up *before* RF drive is removed.... again, 
> this phenomena only happens at the beginning and end of the input RF 
> envelope.
>
> Is there way to mitigate these current spikes, especially the one 
> generated when RF is removed?
>
> 73 Eric NO3M
>
>

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From: Rik Strobbe <rik.strobbe@kuleuven.be>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Thread-Topic: LF: Class D current spikes
Thread-Index: AQHUzDqCt8U6/kU7w0aNBM6ZXdfQC6Xwf8yAgAAfQf0=
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 Content preview:  Hi Stefan, Eric, this might solve the PS tripping problem,
    but on the other hand it might also provide the MOSFET the draincurrent it
    needs to die ;-) 73, Rik ON7YD - OR7T 
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Subject: Re: LF: Class D current spikes
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Hi Stefan, Eric,

this might solve the PS tripping problem, but on the other hand it might also provide the MOSFET the draincurrent it needs to die ;-)

73, Rik  ON7YD - OR7T

________________________________________
Van: owner-rsgb_lf_group@blacksheep.org <owner-rsgb_lf_group@blacksheep.org> namens DK7FC <selberdenken@posteo.de>
Verzonden: maandag 25 februari 2019 15:15
Aan: rsgb_lf_group@blacksheep.org
Onderwerp: Re: LF: Class D current spikes

Hi Eric,

What happens to the supply behaviour if you just switch some Cs parallel
to the output, say 4x 4700 uF (low ESR) rated at 63V ?
Maybe it solves the problem of the supply going into fault mode,
although it is no the perfect solution.

73, Stefan

Am 24.02.2019 13:08, schrieb Eric NO3M:
> I recently got a current mode (outp xfmr center tap not bypassed)
> Class D amp going on 136khz, basically modeled after the W1VD / G0MRF
> circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
> 42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on
> the power supply in use:
>
> 30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
> 48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out
>
> I am also using the G0MRF keying circuit, ie. P-channel MOSFET
> (IRF9540) in the driver (MCP1404) supply line.
>
> If the driver is left active (key down), the beginning and end of the
> input RF envelope produces a "clicking" noise... assume this is from
> current spikes being developed and sunk by the FET body diodes?  If
> the driver is keyed with input RF already applied, thereby
> interrupting the drive to the FETs, there is no such behavior.  The
> keying is shaped, resulting in a ramping of the driver supply voltage
> and resultant gate waveforms to the FETs.
>
> These current spikes do not bother my 30V linear power supply,
> however, when I attempt to use a 48V switching supply (rated at
> 17.7A), it seems to be OK with the current spike generated on the
> beginning of the RF envelope, but not the spike at the end of the
> envelope and goes into fault mode.  If the driver is keyed with
> continuous RF applied, it's happy and does not trip out.  But keying
> the driver doesn't seem practical for digi modes without some exotic
> circuitry or engaging computer generated signaling to key down *after*
> RF drive is applied and key up *before* RF drive is removed.... again,
> this phenomena only happens at the beginning and end of the input RF
> envelope.
>
> Is there way to mitigate these current spikes, especially the one
> generated when RF is removed?
>
> 73 Eric NO3M
>
>



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 Content preview:  ...yes, might. But also it might not, especially when the
   critical event happens only once per minute. 73, Stefan Am 25.02.2019 16:09,
    schrieb Rik Strobbe: > Hi Stefan, Eric, > > this might solve the PS tripping
    problem, but on the other hand it might also provide the MOSFET the draincurrent
    it needs to die ;-) > [...] 
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Subject: Re: LF: Class D current spikes
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...yes, might.
But also it might not, especially when the critical event happens only 
once per minute.

73, Stefan

Am 25.02.2019 16:09, schrieb Rik Strobbe:
> Hi Stefan, Eric,
>
> this might solve the PS tripping problem, but on the other hand it might also provide the MOSFET the draincurrent it needs to die ;-)
>
> 73, Rik  ON7YD - OR7T
>
> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org<owner-rsgb_lf_group@blacksheep.org>  namens DK7FC<selberdenken@posteo.de>
> Verzonden: maandag 25 februari 2019 15:15
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: Class D current spikes
>
> Hi Eric,
>
> What happens to the supply behaviour if you just switch some Cs parallel
> to the output, say 4x 4700 uF (low ESR) rated at 63V ?
> Maybe it solves the problem of the supply going into fault mode,
> although it is no the perfect solution.
>
> 73, Stefan
>
> Am 24.02.2019 13:08, schrieb Eric NO3M:
>    
>> I recently got a current mode (outp xfmr center tap not bypassed)
>> Class D amp going on 136khz, basically modeled after the W1VD / G0MRF
>> circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
>> 42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on
>> the power supply in use:
>>
>> 30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
>> 48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out
>>
>> I am also using the G0MRF keying circuit, ie. P-channel MOSFET
>> (IRF9540) in the driver (MCP1404) supply line.
>>
>> If the driver is left active (key down), the beginning and end of the
>> input RF envelope produces a "clicking" noise... assume this is from
>> current spikes being developed and sunk by the FET body diodes?  If
>> the driver is keyed with input RF already applied, thereby
>> interrupting the drive to the FETs, there is no such behavior.  The
>> keying is shaped, resulting in a ramping of the driver supply voltage
>> and resultant gate waveforms to the FETs.
>>
>> These current spikes do not bother my 30V linear power supply,
>> however, when I attempt to use a 48V switching supply (rated at
>> 17.7A), it seems to be OK with the current spike generated on the
>> beginning of the RF envelope, but not the spike at the end of the
>> envelope and goes into fault mode.  If the driver is keyed with
>> continuous RF applied, it's happy and does not trip out.  But keying
>> the driver doesn't seem practical for digi modes without some exotic
>> circuitry or engaging computer generated signaling to key down *after*
>> RF drive is applied and key up *before* RF drive is removed.... again,
>> this phenomena only happens at the beginning and end of the input RF
>> envelope.
>>
>> Is there way to mitigate these current spikes, especially the one
>> generated when RF is removed?
>>
>> 73 Eric NO3M
>>
>>
>>      
>
>    

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From: DK7FC <selberdenken@posteo.de>
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 Content preview:  PS: In a current mode call-D PA i would rather expect an overvoltage
    issue rather than an overcurrent issue (at the power supply). Maybe the sudden
    stop of the current consumption (100% to 0%) is to f [...] 
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PS: In a current mode call-D PA i would rather expect an overvoltage 
issue rather than an overcurrent issue (at the power supply). Maybe the 
sudden stop of the current consumption (100% to 0%) is to fast for the 
regulator of the SMPS, so it does not regulate the duty cycle fast 
enough and produces its own overvoltage. Or, a voltage peak across the 
terminals due to the high di/dt across the L of the cable between SMPS 
and PA.
Such problems could be minimised easily by some additional C near the 
SMPS...

73, Stefan

Am 25.02.2019 16:19, schrieb DK7FC:
> ...yes, might.
> But also it might not, especially when the critical event happens only 
> once per minute.
>
> 73, Stefan
>
> Am 25.02.2019 16:09, schrieb Rik Strobbe:
>> Hi Stefan, Eric,
>>
>> this might solve the PS tripping problem, but on the other hand it 
>> might also provide the MOSFET the draincurrent it needs to die ;-)
>>
>> 73, Rik  ON7YD - OR7T
>>
>> ________________________________________
>> Van: 
>> owner-rsgb_lf_group@blacksheep.org<owner-rsgb_lf_group@blacksheep.org>  
>> namens DK7FC<selberdenken@posteo.de>
>> Verzonden: maandag 25 februari 2019 15:15
>> Aan: rsgb_lf_group@blacksheep.org
>> Onderwerp: Re: LF: Class D current spikes
>>
>> Hi Eric,
>>
>> What happens to the supply behaviour if you just switch some Cs parallel
>> to the output, say 4x 4700 uF (low ESR) rated at 63V ?
>> Maybe it solves the problem of the supply going into fault mode,
>> although it is no the perfect solution.
>>
>> 73, Stefan
>>
>> Am 24.02.2019 13:08, schrieb Eric NO3M:
>>> I recently got a current mode (outp xfmr center tap not bypassed)
>>> Class D amp going on 136khz, basically modeled after the W1VD / G0MRF
>>> circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
>>> 42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on
>>> the power supply in use:
>>>
>>> 30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
>>> 48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out
>>>
>>> I am also using the G0MRF keying circuit, ie. P-channel MOSFET
>>> (IRF9540) in the driver (MCP1404) supply line.
>>>
>>> If the driver is left active (key down), the beginning and end of the
>>> input RF envelope produces a "clicking" noise... assume this is from
>>> current spikes being developed and sunk by the FET body diodes?  If
>>> the driver is keyed with input RF already applied, thereby
>>> interrupting the drive to the FETs, there is no such behavior.  The
>>> keying is shaped, resulting in a ramping of the driver supply voltage
>>> and resultant gate waveforms to the FETs.
>>>
>>> These current spikes do not bother my 30V linear power supply,
>>> however, when I attempt to use a 48V switching supply (rated at
>>> 17.7A), it seems to be OK with the current spike generated on the
>>> beginning of the RF envelope, but not the spike at the end of the
>>> envelope and goes into fault mode.  If the driver is keyed with
>>> continuous RF applied, it's happy and does not trip out.  But keying
>>> the driver doesn't seem practical for digi modes without some exotic
>>> circuitry or engaging computer generated signaling to key down *after*
>>> RF drive is applied and key up *before* RF drive is removed.... again,
>>> this phenomena only happens at the beginning and end of the input RF
>>> envelope.
>>>
>>> Is there way to mitigate these current spikes, especially the one
>>> generated when RF is removed?
>>>
>>> 73 Eric NO3M
>>>
>>>
>>

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Date: Mon, 25 Feb 2019 15:48:08 +0000
From: Chris Wilson <dead.fets@gmail.com>
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To: Rik Strobbe <rsgb_lf_group@blacksheep.org>
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 Content preview:  Hello Rik, Monday, February 25, 2019, 3:09:18 PM, you wrote:
    > Hi Stefan, Eric, 
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Subject: Re: LF: Class D current spikes
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Hello Rik,

Monday, February 25, 2019, 3:09:18 PM, you wrote:

> Hi Stefan, Eric,

> this might solve the PS tripping problem, but on the other hand it
> might also provide the MOSFET the draincurrent it needs to die ;-)

> 73, Rik  ON7YD - OR7T

> ________________________________________
> Van: owner-rsgb_lf_group@blacksheep.org
> <owner-rsgb_lf_group@blacksheep.org> namens DK7FC <selberdenken@posteo.de>
> Verzonden: maandag 25 februari 2019 15:15
> Aan: rsgb_lf_group@blacksheep.org
> Onderwerp: Re: LF: Class D current spikes

> Hi Eric,

> What happens to the supply behaviour if you just switch some Cs parallel
> to the output, say 4x 4700 uF (low ESR) rated at 63V ?
> Maybe it solves the problem of the supply going into fault mode,
> although it is no the perfect solution.

> 73, Stefan

> Am 24.02.2019 13:08, schrieb Eric NO3M:
>> I recently got a current mode (outp xfmr center tap not bypassed)
>> Class D amp going on 136khz, basically modeled after the W1VD / G0MRF
>> circuits.  FETs are 59N25s, 4820p / 10ohm snubbers, 5t+5t / 21t 3C90
>> 42mm output xfmr, 62uH (25t T157-26) choke.  Output xfmr depends on
>> the power supply in use:
>>
>> 30V linear supply: 5t+5t / 21t 3C90 42mm, 300W out
>> 48V switching supply: 5t + 5t / 16t 3C90 51mm, 500W out
>>
>> I am also using the G0MRF keying circuit, ie. P-channel MOSFET
>> (IRF9540) in the driver (MCP1404) supply line.
>>
>> If the driver is left active (key down), the beginning and end of the
>> input RF envelope produces a "clicking" noise... assume this is from
>> current spikes being developed and sunk by the FET body diodes?  If
>> the driver is keyed with input RF already applied, thereby
>> interrupting the drive to the FETs, there is no such behavior.  The
>> keying is shaped, resulting in a ramping of the driver supply voltage
>> and resultant gate waveforms to the FETs.
>>
>> These current spikes do not bother my 30V linear power supply,
>> however, when I attempt to use a 48V switching supply (rated at
>> 17.7A), it seems to be OK with the current spike generated on the
>> beginning of the RF envelope, but not the spike at the end of the
>> envelope and goes into fault mode.  If the driver is keyed with
>> continuous RF applied, it's happy and does not trip out.  But keying
>> the driver doesn't seem practical for digi modes without some exotic
>> circuitry or engaging computer generated signaling to key down *after*
>> RF drive is applied and key up *before* RF drive is removed.... again,
>> this phenomena only happens at the beginning and end of the input RF
>> envelope.
>>
>> Is there way to mitigate these current spikes, especially the one
>> generated when RF is removed?
>>
>> 73 Eric NO3M
>>
>>



I have a series of scope captures from my W1VD amp showing huge
voltage spikes on the FET drains at the end of WSPR and especially
OPERA TX sequences. I suspected inductance was the cause. In fact I
try not use OPERA at high power as i am pretty sure to kill a FET
after a few sessions... Oddly (although I hope msomeone more
knowlegeable has the answer), using WSPR from my U3S direct from CLK0
of  th  Si535a  or  whatever it is never causes these spikes...  Or at
least they are well contained. 

-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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 Content preview:  Chris, et.al. N1BUG relayed the same information regarding
    the U3S and class-D amp behavior, so your observation is not a one off...
    > > I have a series of scope captures from my W1VD amp showing huge > voltage
    spikes on the FET drains at the end of WSPR and especially > OPERA TX sequences.
    I suspected inductance was the cause. In [...] 
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Chris, et.al.

N1BUG relayed the same information regarding the U3S and class-D amp 
behavior, so your observation is not a one off...



>
> I have a series of scope captures from my W1VD amp showing huge
> voltage spikes on the FET drains at the end of WSPR and especially
> OPERA TX sequences. I suspected inductance was the cause. In fact I
> try not use OPERA at high power as i am pretty sure to kill a FET
> after a few sessions... Oddly (although I hope msomeone more
> knowlegeable has the answer), using WSPR from my U3S direct from CLK0
> of  th  Si535a  or  whatever it is never causes these spikes...  Or at
> least they are well contained.
>


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Date: Mon, 25 Feb 2019 17:20:52 +0100
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 Content preview:  Hi ULF friends, Last Friday i run another carrier transmission
    on my 900m long ground loop antenna. It was the second experiment at *470.1
    Hz*. The last experiment failed because just a few 1/10 dB were missed to
    rea [...] 
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Subject: ULF: 470.1 Hz detected in 57.6 km distance
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Hi ULF friends,

Last Friday i run another carrier transmission on my 900m long ground 
loop antenna. It was the second experiment at *470.1 Hz*. The last 
experiment failed because just a few 1/10 dB were missed to reach the 14 
dB SNR level which is the criterium for a valid detection.
During the last week i managed to reduce the background QRM on the E 
field significantly (at least 10 dB) in that frequency range by changing 
the ground connection on the RX system, so it was an EMC issue.

In the recent experiment the DC measurement showed 1 A at 58 V, so the 
loop loss was just 58 Ohm, which is one of the best values so far.

Conecting the PA to the LiFePo4 accu produced 620 W RF power and 3 A 
antenna current (!) in the first moment. But the DC/DC converter became 
a bit to warm and i (thought) had enough time so i reduced the input 
voltage. The power dropped to *460 W* and so the *antenna current during 
the experiment was 2.75 A*. The carrier started at 14:50 UTC and was on 
the air for 2.5 hours!

It was a quiet day and so i decided spontaneously to do the experiment. 
But i've been at work in the morning and so i was late, a bit to late 
actually, since the band already opened and the QRN increased during the 
experiment. Who knows what happened to the phase over that path. The 
only RX station detecting the signal was my own tree in *57.6 km 
distance*.  Due to the rising QRN the last 30 minutes did not help to 
rise the SNR of the postprocessed spectrum peak. But 2 hours were fine 
to get a clear copy!

Usually i have to ways to determine the final SNR: One is to read the 
output of the EbNaut decoder decoding a '*' message. The ouput, if using 
the -f15 -f16 -M'*****' options, then shows the carrier S/N directly.
The other method is a script that calculates the SNR dB value based on 
the spectrum peak and 0 dB noise level. This 0 dB noise level 
calculation is done according to the description in SpectumLab's help 
sites. Here is the quote:
"*The definition of noise levels is not easy. Here is the basic 
algorithm of the 'noise' function: *

   1. * An array of amplitudes (usually dB values) from the last FFT
      calculation is sorted into order of increasing amplitude. *
   2. * The amplitude of the lower quartile value (for example bin
      number 256 in a sorted set of 1024 points) PLUS 3dB is then
      returned as an estimate of the mean noise level. *

* This technique automatically throws away very high values (strong 
signals) that would otherwise affect the result.*"

This technique is used in my script. I find the result adequate, the 0 
dB level is visually in the center of the noise. But sometimes the SNR 
statements are a bit different between my script and the result of the 
EbNaut program. Maybe it is due to the fact that i am calculating the 
mean level based on just 1000 bins arround the spectrum peak, and EbNaut 
watches a higher bandwidth, which may contain more QRM peaks that rise 
the mean noise baseline?
That may explain why my script whows an* SNR of 18.2 dB* whereas the 
EbNaut decoder says it is an *SNR of 16.17 dB*. Anyway, well above 14 dB.

The signal was strong enough, it could have carried a *6 character 
EbNaut message*.

Attached is a 424 uHz spectrogram showing a short carrier trace just 
before the high QRN sets in. Also attached, a single spectrum peak 
detection and the result for an EbNaut message (showing the carrier S/N).


So, it is the first amateur radio signal on the *638 km band* detected 
over such a distance i think.


73, Stefan

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Hi ULF friends, <br>
<br>
Last Friday i run another carrier transmission on my 900m long ground
loop antenna. It was the second experiment at <b>470.1 Hz</b>. The
last experiment failed because just a few 1/10 dB were missed to reach
the 14 dB SNR level which is the criterium for a valid detection.<br>
During the last week i managed to reduce the background QRM on the E
field significantly (at least 10 dB) in that frequency range by
changing the ground connection on the RX system, so it was an EMC issue.<br>
<br>
In the recent experiment the DC measurement showed 1 A at 58 V, so the
loop loss was just 58 Ohm, which is one of the best values so far.<br>
<br>
Conecting the PA to the LiFePo4 accu produced 620 W RF power and 3 A
antenna current (!) in the first moment. But the DC/DC converter became
a bit to warm and i (thought) had enough time so i reduced the input
voltage. The power dropped to <b>460 W</b> and so the <b>antenna
current during the experiment was 2.75 A</b>. The carrier started at
14:50 UTC and was on the air for 2.5 hours!<br>
<br>
It was a quiet day and so i decided spontaneously to do the experiment.
But i've been at work in the morning and so i was late, a bit to late
actually, since the band already opened and the QRN increased during
the experiment. Who knows what happened to the phase over that path.
The only RX station detecting the signal was my own tree in <b>57.6 km
distance</b>.  Due to the rising QRN the last 30 minutes did not help
to rise the SNR of the postprocessed spectrum peak. But 2 hours were
fine to get a clear copy!<br>
<br>
Usually i have to ways to determine the final SNR: One is to read the
output of the EbNaut decoder decoding a '*' message. The ouput, if
using the -f15 -f16 -M'*****' options, then shows the carrier S/N
directly.<br>
The other method is a script that calculates the SNR dB value based on
the spectrum peak and 0 dB noise level. This 0 dB noise level
calculation is done according to the description in SpectumLab's help
sites. Here is the quote:<br>
"<b>The definition of noise levels is not easy. Here is the basic
algorithm of the 'noise' function: </b>
<ol>
  <li><b> An array of amplitudes (usually dB values) from the last FFT
calculation is sorted into order of increasing amplitude. </b></li>
  <li><b> The amplitude of the lower quartile value (for example bin
number 256 in a sorted set of 1024 points) PLUS 3dB is then returned as
an estimate of the mean noise level. </b></li>
</ol>
<p><b> This technique automatically throws away very high values
(strong signals) that would otherwise affect the result.</b>"</p>
This technique is used in my script. I find the result adequate, the 0
dB level is visually in the center of the noise. But sometimes the SNR
statements are a bit different between my script and the result of the
EbNaut program. Maybe it is due to the fact that i am calculating the
mean level based on just 1000 bins arround the spectrum peak, and
EbNaut watches a higher bandwidth, which may contain more QRM peaks
that rise the mean noise baseline?<br>
That may explain why my script whows an<b> SNR of 18.2 dB</b> whereas
the EbNaut decoder says it is an <b>SNR of 16.17 dB</b>. Anyway, well
above 14 dB.<br>
<br>
The signal was strong enough, it could have carried a <b>6 character
EbNaut message</b>.<br>
<br>
Attached is a 424 uHz spectrogram showing a short carrier trace just
before the high QRN sets in. Also attached, a single spectrum peak
detection and the result for an EbNaut message (showing the carrier
S/N).<br>
<br>
<br>
So, it is the first amateur radio signal on the <b>638 km band</b>
detected over such a distance i think.<br>
<br>
<br>
73, Stefan<br>
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 Content preview:  Chris, LF, Yes, although I run mine differently. I use the
    full output of the U3S into a doubler. I have run WSPR, JT9, and DFCW from
    the U3S without having any problems. I have also extensively used CW ID with
    [...] 
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Subject: Re: LF: Class D current spikes
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Chris, LF,

Yes, although I run mine differently. I use the full output of the
U3S into a doubler. I have run WSPR, JT9, and DFCW from the U3S
without having any problems. I have also extensively used CW ID with
the U3S and amp without problems. Yet both other exciters blow FETs
at the instant RF stops.

Chris, I know you are busy but if you get a chance I would like to
see those scope captures. I thought I had it figured out that this
is a voltage mode amp and should be seeing current spikes, but maybe
I still have that wrong! If they are voltage spikes that may be
easier to control.

One thing I would like to learn more about is why do the drivers
leave one phase high for a longer period than a half cycle when RF
stops. What causes this? Is this only with specific FET drivers or
are all of them prone to this?

73,
Paul


On 2/25/19 11:13 AM, Eric NO3M wrote:
> Chris, et.al.
> 
> N1BUG relayed the same information regarding the U3S and class-D amp 
> behavior, so your observation is not a one off...
> 
> 
> 
>>
>> I have a series of scope captures from my W1VD amp showing huge
>> voltage spikes on the FET drains at the end of WSPR and especially
>> OPERA TX sequences. I suspected inductance was the cause. In fact I
>> try not use OPERA at high power as i am pretty sure to kill a FET
>> after a few sessions... Oddly (although I hope msomeone more
>> knowlegeable has the answer), using WSPR from my U3S direct from CLK0
>> of  th  Si535a  or  whatever it is never causes these spikes...  Or at
>> least they are well contained.

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 Content preview:  Stefan, Congratulations on this latest milestone. 57.6 km
   at 470 Hz at an SNR that would have supported 6 bits of information with 90%
    of battery energy unused is impressive; nice work. Using r^2.5 extinction
    it seems like another 13 dB would reach the far field. 
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Subject: LF: RE: 470.1 Hz detected in 57.6 km distance
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Stefan,

=20

Congratulations on this latest milestone. 57.6 km at 470 Hz at an SNR =
that would have supported 6 bits of information with 90% of battery =
energy unused is impressive; nice work.

=20

Using r^2.5 extinction it seems like another 13 dB would reach the far =
field.

=20

I wonder if some fine-tuning of distance could be helpful in that case. =
I=E2=80=99m not sure how to easily calculate modal null separation =
distances at wavelengths greater than ionospheric height, but by =
extrapolation from 3 kHz it would seem that at 470 Hz, ten nulls (from =
modes 1 through 5) might be fairly closely spaced near a 110 km target =
location, such that a small increase or decrease in receiver distance =
from transmitter could move the receiver toward a peak in the =
interference pattern.

=20

I=E2=80=99m not sure how you changed receiver locations in the past so =
perhaps in this case you can=E2=80=99t easily move the receiver.

=20

Your 2-hour spectral plot is a welcome sight.

=20

73,

=20

Jim AA5BW

=20

=20

=20

From: owner-rsgb_lf_group@blacksheep.org =
[mailto:owner-rsgb_lf_group@blacksheep.org] On Behalf Of DK7FC
Sent: Monday, February 25, 2019 11:21 AM
To: rsgb_lf_group@blacksheep.org
Subject: ULF: 470.1 Hz detected in 57.6 km distance

=20

Hi ULF friends,=20

Last Friday i run another carrier transmission on my 900m long ground =
loop antenna. It was the second experiment at 470.1 Hz. The last =
experiment failed because just a few 1/10 dB were missed to reach the 14 =
dB SNR level which is the criterium for a valid detection.
During the last week i managed to reduce the background QRM on the E =
field significantly (at least 10 dB) in that frequency range by changing =
the ground connection on the RX system, so it was an EMC issue.

In the recent experiment the DC measurement showed 1 A at 58 V, so the =
loop loss was just 58 Ohm, which is one of the best values so far.

Conecting the PA to the LiFePo4 accu produced 620 W RF power and 3 A =
antenna current (!) in the first moment. But the DC/DC converter became =
a bit to warm and i (thought) had enough time so i reduced the input =
voltage. The power dropped to 460 W and so the antenna current during =
the experiment was 2.75 A. The carrier started at 14:50 UTC and was on =
the air for 2.5 hours!

It was a quiet day and so i decided spontaneously to do the experiment. =
But i've been at work in the morning and so i was late, a bit to late =
actually, since the band already opened and the QRN increased during the =
experiment. Who knows what happened to the phase over that path. The =
only RX station detecting the signal was my own tree in 57.6 km =
distance.  Due to the rising QRN the last 30 minutes did not help to =
rise the SNR of the postprocessed spectrum peak. But 2 hours were fine =
to get a clear copy!

Usually i have to ways to determine the final SNR: One is to read the =
output of the EbNaut decoder decoding a '*' message. The ouput, if using =
the -f15 -f16 -M'*****' options, then shows the carrier S/N directly.
The other method is a script that calculates the SNR dB value based on =
the spectrum peak and 0 dB noise level. This 0 dB noise level =
calculation is done according to the description in SpectumLab's help =
sites. Here is the quote:
"The definition of noise levels is not easy. Here is the basic algorithm =
of the 'noise' function:=20

1.	An array of amplitudes (usually dB values) from the last FFT =
calculation is sorted into order of increasing amplitude.=20
2.	The amplitude of the lower quartile value (for example bin number 256 =
in a sorted set of 1024 points) PLUS 3dB is then returned as an estimate =
of the mean noise level.=20

This technique automatically throws away very high values (strong =
signals) that would otherwise affect the result."

This technique is used in my script. I find the result adequate, the 0 =
dB level is visually in the center of the noise. But sometimes the SNR =
statements are a bit different between my script and the result of the =
EbNaut program. Maybe it is due to the fact that i am calculating the =
mean level based on just 1000 bins arround the spectrum peak, and EbNaut =
watches a higher bandwidth, which may contain more QRM peaks that rise =
the mean noise baseline?
That may explain why my script whows an SNR of 18.2 dB whereas the =
EbNaut decoder says it is an SNR of 16.17 dB. Anyway, well above 14 dB.

The signal was strong enough, it could have carried a 6 character EbNaut =
message.

Attached is a 424 uHz spectrogram showing a short carrier trace just =
before the high QRN sets in. Also attached, a single spectrum peak =
detection and the result for an EbNaut message (showing the carrier =
S/N).


So, it is the first amateur radio signal on the 638 km band detected =
over such a distance i think.


73, Stefan


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class=3DMsoNormal><span =
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style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Congratulations on this latest milestone. 57.6 km at 470 Hz at an SNR =
that would have supported 6 bits of information with 90% of battery =
energy unused is impressive; nice work.<o:p></o:p></span></p><p =
class=3DMsoNormal><span =
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D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Using r^2.5 extinction it seems like another 13 dB would reach the =
far field.<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>I wonder if some fine-tuning of distance could be helpful in that =
case. I=E2=80=99m not sure how to easily calculate modal null separation =
distances at wavelengths greater than ionospheric height, but by =
extrapolation from 3 kHz it would seem that at 470 Hz, ten nulls (from =
modes 1 through 5) might be fairly closely spaced near a 110 km target =
location, such that a small increase or decrease in receiver distance =
from transmitter could move the receiver toward a peak in the =
interference pattern.<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
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style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>I=E2=80=99m not sure how you changed receiver locations in the past =
so perhaps in this case you can=E2=80=99t easily move the =
receiver.<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Your 2-hour spectral plot is a welcome sight.<o:p></o:p></span></p><p =
class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>73,<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'>Jim AA5BW<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'> =C2=A0<o:p></o:p></span></p><p class=3DMsoNormal><span =
style=3D'font-size:11.0pt;font-family:"Calibri","sans-serif";color:#1F497=
D'><o:p>&nbsp;</o:p></span></p><div><div =
style=3D'border:none;border-top:solid #B5C4DF 1.0pt;padding:3.0pt 0in =
0in 0in'><p class=3DMsoNormal><b><span =
style=3D'font-size:10.0pt;font-family:"Tahoma","sans-serif";color:windowt=
ext'>From:</span></b><span =
style=3D'font-size:10.0pt;font-family:"Tahoma","sans-serif";color:windowt=
ext'> owner-rsgb_lf_group@blacksheep.org =
[mailto:owner-rsgb_lf_group@blacksheep.org] <b>On Behalf Of =
</b>DK7FC<br><b>Sent:</b> Monday, February 25, 2019 11:21 =
AM<br><b>To:</b> rsgb_lf_group@blacksheep.org<br><b>Subject:</b> ULF: =
470.1 Hz detected in 57.6 km =
distance<o:p></o:p></span></p></div></div><p =
class=3DMsoNormal><o:p>&nbsp;</o:p></p><p class=3DMsoNormal>Hi ULF =
friends, <br><br>Last Friday i run another carrier transmission on my =
900m long ground loop antenna. It was the second experiment at <b>470.1 =
Hz</b>. The last experiment failed because just a few 1/10 dB were =
missed to reach the 14 dB SNR level which is the criterium for a valid =
detection.<br>During the last week i managed to reduce the background =
QRM on the E field significantly (at least 10 dB) in that frequency =
range by changing the ground connection on the RX system, so it was an =
EMC issue.<br><br>In the recent experiment the DC measurement showed 1 A =
at 58 V, so the loop loss was just 58 Ohm, which is one of the best =
values so far.<br><br>Conecting the PA to the LiFePo4 accu produced 620 =
W RF power and 3 A antenna current (!) in the first moment. But the =
DC/DC converter became a bit to warm and i (thought) had enough time so =
i reduced the input voltage. The power dropped to <b>460 W</b> and so =
the <b>antenna current during the experiment was 2.75 A</b>. The carrier =
started at 14:50 UTC and was on the air for 2.5 hours!<br><br>It was a =
quiet day and so i decided spontaneously to do the experiment. But i've =
been at work in the morning and so i was late, a bit to late actually, =
since the band already opened and the QRN increased during the =
experiment. Who knows what happened to the phase over that path. The =
only RX station detecting the signal was my own tree in <b>57.6 km =
distance</b>.&nbsp; Due to the rising QRN the last 30 minutes did not =
help to rise the SNR of the postprocessed spectrum peak. But 2 hours =
were fine to get a clear copy!<br><br>Usually i have to ways to =
determine the final SNR: One is to read the output of the EbNaut decoder =
decoding a '*' message. The ouput, if using the -f15 -f16 -M'*****' =
options, then shows the carrier S/N directly.<br>The other method is a =
script that calculates the SNR dB value based on the spectrum peak and 0 =
dB noise level. This 0 dB noise level calculation is done according to =
the description in SpectumLab's help sites. Here is the =
quote:<br>&quot;<b>The definition of noise levels is not easy. Here is =
the basic algorithm of the 'noise' function: </b><o:p></o:p></p><ol =
start=3D1 type=3D1><li class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto;mso-list:l0 =
level1 lfo1'><b>An array of amplitudes (usually dB values) from the last =
FFT calculation is sorted into order of increasing amplitude. =
</b><o:p></o:p></li><li class=3DMsoNormal =
style=3D'mso-margin-top-alt:auto;mso-margin-bottom-alt:auto;mso-list:l0 =
level1 lfo1'><b>The amplitude of the lower quartile value (for example =
bin number 256 in a sorted set of 1024 points) PLUS 3dB is then returned =
as an estimate of the mean noise level. =
</b><o:p></o:p></li></ol><p><b>This technique automatically throws away =
very high values (strong signals) that would otherwise affect the =
result.</b>&quot;<o:p></o:p></p><p class=3DMsoNormal>This technique is =
used in my script. I find the result adequate, the 0 dB level is =
visually in the center of the noise. But sometimes the SNR statements =
are a bit different between my script and the result of the EbNaut =
program. Maybe it is due to the fact that i am calculating the mean =
level based on just 1000 bins arround the spectrum peak, and EbNaut =
watches a higher bandwidth, which may contain more QRM peaks that rise =
the mean noise baseline?<br>That may explain why my script whows an<b> =
SNR of 18.2 dB</b> whereas the EbNaut decoder says it is an <b>SNR of =
16.17 dB</b>. Anyway, well above 14 dB.<br><br>The signal was strong =
enough, it could have carried a <b>6 character EbNaut =
message</b>.<br><br>Attached is a 424 uHz spectrogram showing a short =
carrier trace just before the high QRN sets in. Also attached, a single =
spectrum peak detection and the result for an EbNaut message (showing =
the carrier S/N).<br><br><br>So, it is the first amateur radio signal on =
the <b>638 km band</b> detected over such a distance i =
think.<br><br><br>73, Stefan<o:p></o:p></p></div></body></html>
------=_NextPart_000_0092_01D4CD21.04B199F0--


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Date: Mon, 25 Feb 2019 22:02:54 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello Paul. everyone A series of overlapping scope captures
    at end of WSPR sequence with expensive high voltage / current Wolfspeed FET's
    that usually survived, into the antenna and into a 10kW dummy load, taken
    after the [...] 
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Subject: Re: LF: Class D current spikes
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Hello  Paul. everyone

A  series  of  overlapping  scope  captures  at end of WSPR
sequence  with  expensive  high  voltage  /  current  Wolfspeed  FET's
that usually survived, into the antenna and into a 10kW dummy load, taken
after  the choke and also at the drains of the W1VD amp. Driver TS-590
/  W1VD  doubler,  and W1VD amp ( end part of another circuit). U3S does
not show anything like this oscillating end to a TX sequence.:

http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip

http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip

Green trace drain, yellow after the choke.



Monday, February 25, 2019, 4:34:05 PM, you wrote:

> Chris, LF,

> Yes, although I run mine differently. I use the full output of the
> U3S into a doubler. I have run WSPR, JT9, and DFCW from the U3S
> without having any problems. I have also extensively used CW ID with
> the U3S and amp without problems. Yet both other exciters blow FETs
> at the instant RF stops.

> Chris, I know you are busy but if you get a chance I would like to
> see those scope captures. I thought I had it figured out that this
> is a voltage mode amp and should be seeing current spikes, but maybe
> I still have that wrong! If they are voltage spikes that may be
> easier to control.

> One thing I would like to learn more about is why do the drivers
> leave one phase high for a longer period than a half cycle when RF
> stops. What causes this? Is this only with specific FET drivers or
> are all of them prone to this?

> 73,
> Paul


> On 2/25/19 11:13 AM, Eric NO3M wrote:
>> Chris, et.al.
>> 
>> N1BUG relayed the same information regarding the U3S and class-D amp 
>> behavior, so your observation is not a one off...
>> 
>> 
>> 
>>>
>>> I have a series of scope captures from my W1VD amp showing huge
>>> voltage spikes on the FET drains at the end of WSPR and especially
>>> OPERA TX sequences. I suspected inductance was the cause. In fact I
>>> try not use OPERA at high power as i am pretty sure to kill a FET
>>> after a few sessions... Oddly (although I hope msomeone more
>>> knowlegeable has the answer), using WSPR from my U3S direct from CLK0
>>> of  th  Si535a  or  whatever it is never causes these spikes...  Or at
>>> least they are well contained.




-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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 Content preview:  Hello Riccardo, Thank you for the transmission in daylight.
    It was interesting to compare the different antennas. I analysed just two
    hours centered at 12 UTC and looked on all 3 antennas separately. 
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Subject: Re: VLF: 8269.997 Hz
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--------------090408080009050101090409
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Hello Riccardo,

Thank you for the transmission in daylight. It was interesting to 
compare the different antennas. I analysed just two hours centered at 12 
UTC and looked on all 3 antennas separately.

E field: 15.16 dB SNR (in 138.9 uHz)
NE loop: 17.61 dB
NW loop:  -0.2 dB

mixing both H field antennas:
NE+0.2*NW: 18.58 dB

Adding the E field:
NE+0.2*NW+0.4*E(rotated by -30 deg): *19.10 dB in 138.9 uHz*

Then, 4 hours centered at 12 UTC gives *22.09 dB in 69.4 uHz*.
And 8 hours centered at 12 UTC gives *24.99 dB in 34.7 uHz*

Between 8 and 16 UTC you could have transferred a 50 character EbNaut 
message over to my RX!

73, Stefan



Am 25.02.2019 14:10, schrieb Riccardo Zoli:
>
> Markus, VLF
>
> Yes, indeed: with DL0AO and Stefan's RDF there are no doubt :-)
> Yesterday the carrier was produced feeding my antenna with about 650mA 
> but I think the noise was too high to attempt an EbNaut transmission.
>
>
> All the best
>
> 73 de Riccardo IW4DXW
>
>
>
> Il giorno Dom 24 Feb 2019, 17:21 Markus Vester <markusvester@aol.com 
> <mailto:markusvester@aol.com>> ha scritto:
>
>     Looks like Riccardo is sending a carrier on 8269.997 today.
>
>     Good luck,
>     Markus
>

--------------090408080009050101090409
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
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Hello Riccardo, <br>
<br>
Thank you for the transmission in daylight. It was interesting to
compare the different antennas. I analysed just two hours centered at
12 UTC and looked on all 3 antennas separately.<br>
<br>
E field: 15.16 dB SNR (in 138.9 uHz)<br>
NE loop: 17.61 dB<br>
NW loop:  -0.2 dB<br>
<br>
mixing both H field antennas:<br>
NE+0.2*NW: 18.58 dB<br>
<br>
Adding the E field:<br>
NE+0.2*NW+0.4*E(rotated by -30 deg): <b>19.10 dB in 138.9 uHz</b><br>
<br>
Then, 4 hours centered at 12 UTC gives <b>22.09 dB in 69.4 uHz</b>.<br>
And 8 hours centered at 12 UTC gives <b>24.99 dB in 34.7 uHz</b><br>
<br>
Between 8 and 16 UTC you could have transferred a 50 character EbNaut
message over to my RX! <br>
<br>
73, Stefan<br>
<br>
<br>
<br>
Am 25.02.2019 14:10, schrieb Riccardo Zoli:
<blockquote
 cite="mid:CANA3B6W7F_fHGLCELkGZrhwgu8tpvAmyOFRgDPRKBwgpCbHvWw@mail.gmail.com"
 type="cite">
  <div dir="auto">
  <div dir="auto"><br>
  </div>
  <div dir="auto">Markus, VLF</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">Yes, indeed: with DL0AO and Stefan's RDF there are no
doubt :-)</div>
  <div dir="auto">Yesterday the carrier was produced feeding my antenna
with about 650mA but I think the noise was too high to attempt an
EbNaut transmission.</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">All the best</div>
  <div dir="auto"><br>
  </div>
  <div dir="auto">73 de Riccardo IW4DXW</div>
  <div dir="auto"><br>
  </div>
  <br>
  <br>
  <div class="gmail_quote" dir="auto">
  <div dir="ltr">Il giorno Dom 24 Feb 2019, 17:21 Markus Vester &lt;<a
 moz-do-not-send="true" href="mailto:markusvester@aol.com"
 rel="noreferrer noreferrer" target="_blank">markusvester@aol.com</a>&gt;
ha scritto:<br>
  </div>
  <blockquote class="gmail_quote"
 style="border-left: 1px solid rgb(204, 204, 204); margin: 0pt 0pt 0pt 0.8ex; padding-left: 1ex;">
    <div
 style="font-size: 10pt; font-family: arial,helvetica,sans-serif; color: black;">
    <div
 style="color: black; font-family: arial,helvetica,sans-serif; font-size: 10pt;">Looks
like Riccardo is sending a carrier on 8269.997 today.<br>
    <br>
Good luck,<br>
Markus <br>
    </div>
    </div>
  </blockquote>
  </div>
  </div>
</blockquote>
</body>
</html>

--------------090408080009050101090409--

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 Content preview:  Thanks Chris. After seeing those I wish I had a storage scope.
    There is much which could be done to get to the bottom of what is going on
    with these things. If I had the proper equipment I would do several things
    a [...] 
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Thanks Chris.

After seeing those I wish I had a storage scope. There is much which
could be done to get to the bottom of what is going on with these
things. If I had the proper equipment I would do several things and
document the results:

1. Look at FET drains on both phases at the same time

2. Try that using every exciter at my disposal both into the dummy
load and antenna

3. Look at traces earlier in the system (FET gates, driver chip
inputs, doubler, exciter.

Those with more technical knowledge probably have additional ideas.

Clearly the amp is not handling end of RF envelope well but the fact
id does better with the U3S than other exciters seems to suggest
this problem starts earlier in the chain.

73,
Paul


On 2/25/19 5:02 PM, Chris Wilson wrote:
> 
> 
> Hello  Paul. everyone
> 
> A  series  of  overlapping  scope  captures  at end of WSPR
> sequence  with  expensive  high  voltage  /  current  Wolfspeed  FET's
> that usually survived, into the antenna and into a 10kW dummy load, taken
> after  the choke and also at the drains of the W1VD amp. Driver TS-590
> /  W1VD  doubler,  and W1VD amp ( end part of another circuit). U3S does
> not show anything like this oscillating end to a TX sequence.:
> 
> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
> 
> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
> 
> Green trace drain, yellow after the choke.
> 
> 
> 
> Monday, February 25, 2019, 4:34:05 PM, you wrote:
> 
>> Chris, LF,
> 
>> Yes, although I run mine differently. I use the full output of the
>> U3S into a doubler. I have run WSPR, JT9, and DFCW from the U3S
>> without having any problems. I have also extensively used CW ID with
>> the U3S and amp without problems. Yet both other exciters blow FETs
>> at the instant RF stops.
> 
>> Chris, I know you are busy but if you get a chance I would like to
>> see those scope captures. I thought I had it figured out that this
>> is a voltage mode amp and should be seeing current spikes, but maybe
>> I still have that wrong! If they are voltage spikes that may be
>> easier to control.
> 
>> One thing I would like to learn more about is why do the drivers
>> leave one phase high for a longer period than a half cycle when RF
>> stops. What causes this? Is this only with specific FET drivers or
>> are all of them prone to this?
> 
>> 73,
>> Paul
> 
> 
>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>> Chris, et.al.
>>>
>>> N1BUG relayed the same information regarding the U3S and class-D amp 
>>> behavior, so your observation is not a one off...
>>>
>>>
>>>
>>>>
>>>> I have a series of scope captures from my W1VD amp showing huge
>>>> voltage spikes on the FET drains at the end of WSPR and especially
>>>> OPERA TX sequences. I suspected inductance was the cause. In fact I
>>>> try not use OPERA at high power as i am pretty sure to kill a FET
>>>> after a few sessions... Oddly (although I hope msomeone more
>>>> knowlegeable has the answer), using WSPR from my U3S direct from CLK0
>>>> of  th  Si535a  or  whatever it is never causes these spikes...  Or at
>>>> least they are well contained.

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 Content preview:  Chris Thanks for the waveforms ... very informative. Sure
   looks like something is triggering the input of the amplifier and thus causing
    the problem. Since the problem doesn't exist with U3S's (which generates
   the various modes internally) driving the amplifier (either directly or through
    a frequency doubler) one has to wonder what the difference i [...] 
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Subject: Re: LF: Class D current spikes
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Chris

Thanks for the waveforms ... very informative. Sure looks like something is triggering the input of the amplifier and thus causing the problem. 

Since the problem doesn't exist with U3S's (which generates the various modes internally) driving the amplifier (either directly or through a frequency doubler) one has to wonder what the difference is between the U3S and the other exciter setups that cause the problem. The fact that the U3S / amplifier combination works correctly would argue that the 'problem' is likely not the amplifier.

The one thing that the non U3S setups have in common is that the modes are generated by software / computer / sound card. Think the first step in tracking down the problem would be to see if there are any unexpected outputs from the soundcard that are causing the problem. When you get a chance maybe you can capture waveforms of the sound card output up to and after the end of a transmission.

Assume that you have disabled all 'computer sounds' on the machines that are supplying audio for the various modes?

Jay W1VD    

       



----- Original Message ----- 
From: "Chris Wilson" <dead.fets@gmail.com>
To: "N1BUG" <rsgb_lf_group@blacksheep.org>
Sent: Monday, February 25, 2019 5:02 PM
Subject: Re: LF: Class D current spikes


> 
> 
> Hello  Paul. everyone
> 
> A  series  of  overlapping  scope  captures  at end of WSPR
> sequence  with  expensive  high  voltage  /  current  Wolfspeed  FET's
> that usually survived, into the antenna and into a 10kW dummy load, taken
> after  the choke and also at the drains of the W1VD amp. Driver TS-590
> /  W1VD  doubler,  and W1VD amp ( end part of another circuit). U3S does
> not show anything like this oscillating end to a TX sequence.:
> 
> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
> 
> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
> 
> Green trace drain, yellow after the choke.
> 
> 
> 
> Monday, February 25, 2019, 4:34:05 PM, you wrote:
> 
>> Chris, LF,
> 
>> Yes, although I run mine differently. I use the full output of the
>> U3S into a doubler. I have run WSPR, JT9, and DFCW from the U3S
>> without having any problems. I have also extensively used CW ID with
>> the U3S and amp without problems. Yet both other exciters blow FETs
>> at the instant RF stops.
> 
>> Chris, I know you are busy but if you get a chance I would like to
>> see those scope captures. I thought I had it figured out that this
>> is a voltage mode amp and should be seeing current spikes, but maybe
>> I still have that wrong! If they are voltage spikes that may be
>> easier to control.
> 
>> One thing I would like to learn more about is why do the drivers
>> leave one phase high for a longer period than a half cycle when RF
>> stops. What causes this? Is this only with specific FET drivers or
>> are all of them prone to this?
> 
>> 73,
>> Paul
> 
> 
>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>> Chris, et.al.
>>> 
>>> N1BUG relayed the same information regarding the U3S and class-D amp 
>>> behavior, so your observation is not a one off...
>>> 
>>> 
>>> 
>>>>
>>>> I have a series of scope captures from my W1VD amp showing huge
>>>> voltage spikes on the FET drains at the end of WSPR and especially
>>>> OPERA TX sequences. I suspected inductance was the cause. In fact I
>>>> try not use OPERA at high power as i am pretty sure to kill a FET
>>>> after a few sessions... Oddly (although I hope msomeone more
>>>> knowlegeable has the answer), using WSPR from my U3S direct from CLK0
>>>> of  th  Si535a  or  whatever it is never causes these spikes...  Or at
>>>> least they are well contained.
> 
> 
> 
> 
> -- 
> Best regards,
> Chris                            mailto:dead.fets@gmail.com
> 
>


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 Content preview:  Jay, Good idea, but it isn't just the sound card. I can guarantee
    one or more destroyed FETs after sending two or three characters of CW where
    computer and sound card are not involved at all. I can also co [...] 
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Subject: Re: LF: Class D current spikes
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Jay,

Good idea, but it isn't just the sound card. I can guarantee one or
more destroyed FETs after sending two or three characters of CW
where computer and sound card are not involved at all. I can also
confirm that with CW the FETs are still blowing at the end of RF
envelope. I can hear the fuse when it opens. I tried some very slow
CW to confirm exactly when it was happening.

73,
Paul


On 2/25/19 7:30 PM, jrusgrove@comcast.net wrote:
> Chris
> 
> Thanks for the waveforms ... very informative. Sure looks like
> something is triggering the input of the amplifier and thus
> causing the problem.
> 
> Since the problem doesn't exist with U3S's (which generates the
> various modes internally) driving the amplifier (either directly
> or through a frequency doubler) one has to wonder what the
> difference is between the U3S and the other exciter setups that
> cause the problem. The fact that the U3S / amplifier combination
> works correctly would argue that the 'problem' is likely not the
> amplifier.
> 
> The one thing that the non U3S setups have in common is that the
> modes are generated by software / computer / sound card. Think
> the first step in tracking down the problem would be to see if
> there are any unexpected outputs from the soundcard that are
> causing the problem. When you get a chance maybe you can capture
> waveforms of the sound card output up to and after the end of a
> transmission.
> 
> Assume that you have disabled all 'computer sounds' on the
> machines that are supplying audio for the various modes?
> 
> Jay W1VD
> 
> 
> 
> 
> 
> ----- Original Message ----- From: "Chris Wilson"
> <dead.fets@gmail.com> To: "N1BUG" <rsgb_lf_group@blacksheep.org> 
> Sent: Monday, February 25, 2019 5:02 PM Subject: Re: LF: Class D
> current spikes
> 
> 
>> 
>> 
>> Hello  Paul. everyone
>> 
>> A  series  of  overlapping  scope  captures  at end of WSPR 
>> sequence  with  expensive  high  voltage  /  current  Wolfspeed
>> FET's that usually survived, into the antenna and into a 10kW
>> dummy load, taken after  the choke and also at the drains of
>> the W1VD amp. Driver TS-590 /  W1VD  doubler,  and W1VD amp (
>> end part of another circuit). U3S does not show anything like
>> this oscillating end to a TX sequence.:
>> 
>> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
>>
>>
>> 
http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
>> 
>> Green trace drain, yellow after the choke.
>> 
>> 
>> 
>> Monday, February 25, 2019, 4:34:05 PM, you wrote:
>> 
>>> Chris, LF,
>> 
>>> Yes, although I run mine differently. I use the full output
>>> of the U3S into a doubler. I have run WSPR, JT9, and DFCW
>>> from the U3S without having any problems. I have also
>>> extensively used CW ID with the U3S and amp without problems.
>>> Yet both other exciters blow FETs at the instant RF stops.
>> 
>>> Chris, I know you are busy but if you get a chance I would
>>> like to see those scope captures. I thought I had it figured
>>> out that this is a voltage mode amp and should be seeing
>>> current spikes, but maybe I still have that wrong! If they
>>> are voltage spikes that may be easier to control.
>> 
>>> One thing I would like to learn more about is why do the
>>> drivers leave one phase high for a longer period than a half
>>> cycle when RF stops. What causes this? Is this only with
>>> specific FET drivers or are all of them prone to this?
>> 
>>> 73, Paul
>> 
>> 
>>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>>> Chris, et.al.
>>>> 
>>>> N1BUG relayed the same information regarding the U3S and
>>>> class-D amp behavior, so your observation is not a one
>>>> off...
>>>> 
>>>> 
>>>> 
>>>>> 
>>>>> I have a series of scope captures from my W1VD amp
>>>>> showing huge voltage spikes on the FET drains at the end
>>>>> of WSPR and especially OPERA TX sequences. I suspected
>>>>> inductance was the cause. In fact I try not use OPERA at
>>>>> high power as i am pretty sure to kill a FET after a few
>>>>> sessions... Oddly (although I hope msomeone more 
>>>>> knowlegeable has the answer), using WSPR from my U3S
>>>>> direct from CLK0 of  th  Si535a  or  whatever it is never
>>>>> causes these spikes...  Or at least they are well
>>>>> contained.

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From: "jrusgrove@comcast.net" <jrusgrove@comcast.net>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
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Date: Mon, 25 Feb 2019 20:57:48 -0500
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 Content preview:  Paul Was this with a continuous frequency source at the input
    (HP3325A maybe?) and using a keyer plugged into the amplifier key jack? Jay
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Subject: Re: LF: Class D current spikes
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Paul

Was this with a continuous frequency source at the input (HP3325A maybe?) and using a keyer plugged into the amplifier key jack?

Jay
 




----- Original Message -----
From: N1BUG <paul@n1bug.com>
Reply-To: <rsgb_lf_group@blacksheep.org>
To: <rsgb_lf_group@blacksheep.org>
Sent: 2/25/2019 7:50:17 PM
Subject: Re: LF: Class D current spikes
________________________________________________________________________________

Jay,

Good idea, but it isn't just the sound card. I can guarantee one or
more destroyed FETs after sending two or three characters of CW
where computer and sound card are not involved at all. I can also
confirm that with CW the FETs are still blowing at the end of RF
envelope. I can hear the fuse when it opens. I tried some very slow
CW to confirm exactly when it was happening.

73,
Paul


On 2/25/19 7:30 PM, jrusgrove@comcast.net wrote:
> Chris
> 
> Thanks for the waveforms ... very informative. Sure looks like
> something is triggering the input of the amplifier and thus
> causing the problem.
> 
> Since the problem doesn't exist with U3S's (which generates the
> various modes internally) driving the amplifier (either directly
> or through a frequency doubler) one has to wonder what the
> difference is between the U3S and the other exciter setups that
> cause the problem. The fact that the U3S / amplifier combination
> works correctly would argue that the 'problem' is likely not the
> amplifier.
> 
> The one thing that the non U3S setups have in common is that the
> modes are generated by software / computer / sound card. Think
> the first step in tracking down the problem would be to see if
> there are any unexpected outputs from the soundcard that are
> causing the problem. When you get a chance maybe you can capture
> waveforms of the sound card output up to and after the end of a
> transmission.
> 
> Assume that you have disabled all 'computer sounds' on the
> machines that are supplying audio for the various modes?
> 
> Jay W1VD
> 
> 
> 
> 
> 
> ----- Original Message ----- From: "Chris Wilson"
> <dead.fets@gmail.com> To: "N1BUG" <rsgb_lf_group@blacksheep.org> 
> Sent: Monday, February 25, 2019 5:02 PM Subject: Re: LF: Class D
> current spikes
> 
> 
>> 
>> 
>> Hello  Paul. everyone
>> 
>> A  series  of  overlapping  scope  captures  at end of WSPR 
>> sequence  with  expensive  high  voltage  /  current  Wolfspeed
>> FET's that usually survived, into the antenna and into a 10kW
>> dummy load, taken after  the choke and also at the drains of
>> the W1VD amp. Driver TS-590 /  W1VD  doubler,  and W1VD amp (
>> end part of another circuit). U3S does not show anything like
>> this oscillating end to a TX sequence.:
>> 
>> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
>>
>>
>> 
http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
>> 
>> Green trace drain, yellow after the choke.
>> 
>> 
>> 
>> Monday, February 25, 2019, 4:34:05 PM, you wrote:
>> 
>>> Chris, LF,
>> 
>>> Yes, although I run mine differently. I use the full output
>>> of the U3S into a doubler. I have run WSPR, JT9, and DFCW
>>> from the U3S without having any problems. I have also
>>> extensively used CW ID with the U3S and amp without problems.
>>> Yet both other exciters blow FETs at the instant RF stops.
>> 
>>> Chris, I know you are busy but if you get a chance I would
>>> like to see those scope captures. I thought I had it figured
>>> out that this is a voltage mode amp and should be seeing
>>> current spikes, but maybe I still have that wrong! If they
>>> are voltage spikes that may be easier to control.
>> 
>>> One thing I would like to learn more about is why do the
>>> drivers leave one phase high for a longer period than a half
>>> cycle when RF stops. What causes this? Is this only with
>>> specific FET drivers or are all of them prone to this?
>> 
>>> 73, Paul
>> 
>> 
>>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>>> Chris, et.al.
>>>> 
>>>> N1BUG relayed the same information regarding the U3S and
>>>> class-D amp behavior, so your observation is not a one
>>>> off...
>>>> 
>>>> 
>>>> 
>>>>> 
>>>>> I have a series of scope captures from my W1VD amp
>>>>> showing huge voltage spikes on the FET drains at the end
>>>>> of WSPR and especially OPERA TX sequences. I suspected
>>>>> inductance was the cause. In fact I try not use OPERA at
>>>>> high power as i am pretty sure to kill a FET after a few
>>>>> sessions... Oddly (although I hope msomeone more 
>>>>> knowlegeable has the answer), using WSPR from my U3S
>>>>> direct from CLK0 of  th  Si535a  or  whatever it is never
>>>>> causes these spikes...  Or at least they are well
>>>>> contained.


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 Content preview:  Has anyone used an existing Versatower or similar as a vertical
    radiator for LF or MF? I know some use them on topband, running an insulated
    wire on the outside up to the top and feeding as a folded m [...] 
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--00000000000097dcd60582c781c4
Content-Type: text/plain; charset="UTF-8"

Has anyone used an existing Versatower or similar as a vertical radiator
for LF or MF?    I know some use them on topband, running an insulated wire
on the outside up to the top and feeding as a folded monopole.

Only asking as a local amateur who has a tower and beam cannot justify
extra wire in his garden for lower frequencies (Serious XYL-i problems,
apparently :-)

Andy
www.g4jnt.com


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serif">Has anyone used an existing Versatower or similar as a vertical radi=
ator for LF or MF?=C2=A0 =C2=A0 I know some use them on topband, running an=
 insulated wire on the outside up to the top and feeding as a folded monopo=
le.</span></div><div class=3D"gmail_default" style=3D"font-family:tahoma,sa=
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 Content preview:  Jay, I was using an HF transceiver in CW mode through a down
    converter. Other FETs were lost at end of envelope while running JT9 with
    the transceiver in USB being fed audio from a sound card. The latest was
   with audio from a different sound card into the new phasing exci [...] 
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Subject: Re: LF: Class D current spikes
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Jay,

I was using an HF transceiver in CW mode through a down converter.

Other FETs were lost at end of envelope while running JT9 with the
transceiver in USB being fed audio from a sound card. The latest was
with audio from a different sound card into the new phasing exciter.

I have never lost a FET while running with the U3S.

73,
Paul


On 2/25/19 8:57 PM, jrusgrove@comcast.net wrote:
> Paul
> 
> Was this with a continuous frequency source at the input (HP3325A
> maybe?) and using a keyer plugged into the amplifier key jack?
> 
> Jay
> 
> 
> 
> 
> 
> ----- Original Message ----- From: N1BUG <paul@n1bug.com> 
> Reply-To: <rsgb_lf_group@blacksheep.org> To:
> <rsgb_lf_group@blacksheep.org> Sent: 2/25/2019 7:50:17 PM 
> Subject: Re: LF: Class D current spikes 
> ________________________________________________________________________________
>
>  Jay,
> 
> Good idea, but it isn't just the sound card. I can guarantee one
> or more destroyed FETs after sending two or three characters of
> CW where computer and sound card are not involved at all. I can
> also confirm that with CW the FETs are still blowing at the end
> of RF envelope. I can hear the fuse when it opens. I tried some
> very slow CW to confirm exactly when it was happening.
> 
> 73, Paul
> 
> 
> On 2/25/19 7:30 PM, jrusgrove@comcast.net wrote:
>> Chris
>> 
>> Thanks for the waveforms ... very informative. Sure looks like 
>> something is triggering the input of the amplifier and thus 
>> causing the problem.
>> 
>> Since the problem doesn't exist with U3S's (which generates
>> the various modes internally) driving the amplifier (either
>> directly or through a frequency doubler) one has to wonder what
>> the difference is between the U3S and the other exciter setups
>> that cause the problem. The fact that the U3S / amplifier
>> combination works correctly would argue that the 'problem' is
>> likely not the amplifier.
>> 
>> The one thing that the non U3S setups have in common is that
>> the modes are generated by software / computer / sound card.
>> Think the first step in tracking down the problem would be to
>> see if there are any unexpected outputs from the soundcard that
>> are causing the problem. When you get a chance maybe you can
>> capture waveforms of the sound card output up to and after the
>> end of a transmission.
>> 
>> Assume that you have disabled all 'computer sounds' on the 
>> machines that are supplying audio for the various modes?
>> 
>> Jay W1VD
>> 
>> 
>> 
>> 
>> 
>> ----- Original Message ----- From: "Chris Wilson" 
>> <dead.fets@gmail.com> To: "N1BUG"
>> <rsgb_lf_group@blacksheep.org> Sent: Monday, February 25, 2019
>> 5:02 PM Subject: Re: LF: Class D current spikes
>> 
>> 
>>> 
>>> 
>>> Hello  Paul. everyone
>>> 
>>> A  series  of  overlapping  scope  captures  at end of WSPR 
>>> sequence  with  expensive  high  voltage  /  current
>>> Wolfspeed FET's that usually survived, into the antenna and
>>> into a 10kW dummy load, taken after  the choke and also at
>>> the drains of the W1VD amp. Driver TS-590 /  W1VD  doubler,
>>> and W1VD amp ( end part of another circuit). U3S does not
>>> show anything like this oscillating end to a TX sequence.:
>>> 
>>> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
>>>
>>>
>>>
>
>>> 
http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
>>> 
>>> Green trace drain, yellow after the choke.
>>> 
>>> 
>>> 
>>> Monday, February 25, 2019, 4:34:05 PM, you wrote:
>>> 
>>>> Chris, LF,
>>> 
>>>> Yes, although I run mine differently. I use the full
>>>> output of the U3S into a doubler. I have run WSPR, JT9, and
>>>> DFCW from the U3S without having any problems. I have also 
>>>> extensively used CW ID with the U3S and amp without
>>>> problems. Yet both other exciters blow FETs at the instant
>>>> RF stops.
>>> 
>>>> Chris, I know you are busy but if you get a chance I would 
>>>> like to see those scope captures. I thought I had it
>>>> figured out that this is a voltage mode amp and should be
>>>> seeing current spikes, but maybe I still have that wrong!
>>>> If they are voltage spikes that may be easier to control.
>>> 
>>>> One thing I would like to learn more about is why do the 
>>>> drivers leave one phase high for a longer period than a
>>>> half cycle when RF stops. What causes this? Is this only
>>>> with specific FET drivers or are all of them prone to
>>>> this?
>>> 
>>>> 73, Paul
>>> 
>>> 
>>>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>>>> Chris, et.al.
>>>>> 
>>>>> N1BUG relayed the same information regarding the U3S and 
>>>>> class-D amp behavior, so your observation is not a one 
>>>>> off...
>>>>> 
>>>>> 
>>>>> 
>>>>>> 
>>>>>> I have a series of scope captures from my W1VD amp 
>>>>>> showing huge voltage spikes on the FET drains at the
>>>>>> end of WSPR and especially OPERA TX sequences. I
>>>>>> suspected inductance was the cause. In fact I try not
>>>>>> use OPERA at high power as i am pretty sure to kill a
>>>>>> FET after a few sessions... Oddly (although I hope
>>>>>> msomeone more knowlegeable has the answer), using WSPR
>>>>>> from my U3S direct from CLK0 of  th  Si535a  or
>>>>>> whatever it is never causes these spikes...  Or at
>>>>>> least they are well contained.
> 
> 


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Date: Tue, 26 Feb 2019 11:18:36 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello N1BUG, Just to add things were MUCH worst using a X2
    multiplier circuit (Jay's). I now use an exciter frequency of X2 direct both
    from the U3S, and as of late X2 from the TS-590 into a simple squarer and
    use [...] 
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Hello N1BUG,

Just to add things were MUCH worst using a X2 multiplier circuit
(Jay's). I now use an exciter frequency of X2 direct both from the
U3S, and as of late X2 from the TS-590 into a simple squarer and use
WSPR in the "Advanced" X2 mode to correct the WSPR tones. No issues at
all with either. OPERA is a no no as of this time, it is a FET killer
:)  Don't  know  why though. It would be great to get to the bottom of
all this!

Tuesday, February 26, 2019, 11:05:15 AM, you wrote:

> Jay,

> I was using an HF transceiver in CW mode through a down converter.

> Other FETs were lost at end of envelope while running JT9 with the
> transceiver in USB being fed audio from a sound card. The latest was
> with audio from a different sound card into the new phasing exciter.

> I have never lost a FET while running with the U3S.

> 73,
> Paul




-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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 Content preview:  Paul Have you run cw from the U3S? I have never run cw from
    a transceiver through the amplifier ... instead I always attach a continuous
    source of RF (GPS referenced HP3325A for example) to the amplifier input
   and use a keyer to key th [...] 
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Subject: Re: LF: Class D current spikes
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Paul

Have you run cw from the U3S?

I have never run cw from a transceiver through the amplifier ... instead I always attach a continuous source of RF (GPS referenced HP3325A for example) to the amplifier input and use a keyer to key the amplifier. There has never been a problem in thousands of hours of operation. 

CW from a transceiver is not the same ... it's an amplitude varying signal when you consider the rise and fall times of the shaped waveform. Rise and fall times of 5 milliseconds used to be the 'standard' ...  which is an eternity at 137 or 500 kHz. The amplifier, as designed, is not expecting an amplitude varying waveform at it's input. 

Jay W1VD   

p.s. in addition to looking at the sound card output for clues, I'd also look at the output of the transceiver as well


----- Original Message -----
From: N1BUG <paul@n1bug.com>
Reply-To: <rsgb_lf_group@blacksheep.org>
To: <rsgb_lf_group@blacksheep.org>
Sent: 2/26/2019 6:05:15 AM
Subject: Re: LF: Class D current spikes
________________________________________________________________________________

Jay,

I was using an HF transceiver in CW mode through a down converter.

Other FETs were lost at end of envelope while running JT9 with the
transceiver in USB being fed audio from a sound card. The latest was
with audio from a different sound card into the new phasing exciter.

I have never lost a FET while running with the U3S.

73,
Paul


On 2/25/19 8:57 PM, jrusgrove@comcast.net wrote:
> Paul
> 
> Was this with a continuous frequency source at the input (HP3325A
> maybe?) and using a keyer plugged into the amplifier key jack?
> 
> Jay
> 
> 
> 
> 
> 
> ----- Original Message ----- From: N1BUG <paul@n1bug.com> 
> Reply-To: <rsgb_lf_group@blacksheep.org> To:
> <rsgb_lf_group@blacksheep.org> Sent: 2/25/2019 7:50:17 PM 
> Subject: Re: LF: Class D current spikes 
> ________________________________________________________________________________
>
>  Jay,
> 
> Good idea, but it isn't just the sound card. I can guarantee one
> or more destroyed FETs after sending two or three characters of
> CW where computer and sound card are not involved at all. I can
> also confirm that with CW the FETs are still blowing at the end
> of RF envelope. I can hear the fuse when it opens. I tried some
> very slow CW to confirm exactly when it was happening.
> 
> 73, Paul
> 
> 
> On 2/25/19 7:30 PM, jrusgrove@comcast.net wrote:
>> Chris
>> 
>> Thanks for the waveforms ... very informative. Sure looks like 
>> something is triggering the input of the amplifier and thus 
>> causing the problem.
>> 
>> Since the problem doesn't exist with U3S's (which generates
>> the various modes internally) driving the amplifier (either
>> directly or through a frequency doubler) one has to wonder what
>> the difference is between the U3S and the other exciter setups
>> that cause the problem. The fact that the U3S / amplifier
>> combination works correctly would argue that the 'problem' is
>> likely not the amplifier.
>> 
>> The one thing that the non U3S setups have in common is that
>> the modes are generated by software / computer / sound card.
>> Think the first step in tracking down the problem would be to
>> see if there are any unexpected outputs from the soundcard that
>> are causing the problem. When you get a chance maybe you can
>> capture waveforms of the sound card output up to and after the
>> end of a transmission.
>> 
>> Assume that you have disabled all 'computer sounds' on the 
>> machines that are supplying audio for the various modes?
>> 
>> Jay W1VD
>> 
>> 
>> 
>> 
>> 
>> ----- Original Message ----- From: "Chris Wilson" 
>> <dead.fets@gmail.com> To: "N1BUG"
>> <rsgb_lf_group@blacksheep.org> Sent: Monday, February 25, 2019
>> 5:02 PM Subject: Re: LF: Class D current spikes
>> 
>> 
>>> 
>>> 
>>> Hello  Paul. everyone
>>> 
>>> A  series  of  overlapping  scope  captures  at end of WSPR 
>>> sequence  with  expensive  high  voltage  /  current
>>> Wolfspeed FET's that usually survived, into the antenna and
>>> into a 10kW dummy load, taken after  the choke and also at
>>> the drains of the W1VD amp. Driver TS-590 /  W1VD  doubler,
>>> and W1VD amp ( end part of another circuit). U3S does not
>>> show anything like this oscillating end to a TX sequence.:
>>> 
>>> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
>>>
>>>
>>>
>
>>> 
http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
>>> 
>>> Green trace drain, yellow after the choke.
>>> 
>>> 
>>> 
>>> Monday, February 25, 2019, 4:34:05 PM, you wrote:
>>> 
>>>> Chris, LF,
>>> 
>>>> Yes, although I run mine differently. I use the full
>>>> output of the U3S into a doubler. I have run WSPR, JT9, and
>>>> DFCW from the U3S without having any problems. I have also 
>>>> extensively used CW ID with the U3S and amp without
>>>> problems. Yet both other exciters blow FETs at the instant
>>>> RF stops.
>>> 
>>>> Chris, I know you are busy but if you get a chance I would 
>>>> like to see those scope captures. I thought I had it
>>>> figured out that this is a voltage mode amp and should be
>>>> seeing current spikes, but maybe I still have that wrong!
>>>> If they are voltage spikes that may be easier to control.
>>> 
>>>> One thing I would like to learn more about is why do the 
>>>> drivers leave one phase high for a longer period than a
>>>> half cycle when RF stops. What causes this? Is this only
>>>> with specific FET drivers or are all of them prone to
>>>> this?
>>> 
>>>> 73, Paul
>>> 
>>> 
>>>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>>>> Chris, et.al.
>>>>> 
>>>>> N1BUG relayed the same information regarding the U3S and 
>>>>> class-D amp behavior, so your observation is not a one 
>>>>> off...
>>>>> 
>>>>> 
>>>>> 
>>>>>> 
>>>>>> I have a series of scope captures from my W1VD amp 
>>>>>> showing huge voltage spikes on the FET drains at the
>>>>>> end of WSPR and especially OPERA TX sequences. I
>>>>>> suspected inductance was the cause. In fact I try not
>>>>>> use OPERA at high power as i am pretty sure to kill a
>>>>>> FET after a few sessions... Oddly (although I hope
>>>>>> msomeone more knowlegeable has the answer), using WSPR
>>>>>> from my U3S direct from CLK0 of  th  Si535a  or
>>>>>> whatever it is never causes these spikes...  Or at
>>>>>> least they are well contained.
> 
> 


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Date: Tue, 26 Feb 2019 06:39:34 -0500
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 Content preview:  Chris When running Opera here I used the same setup as on
   cw. A continuous source of RF attached to the input of the amplifier with
   the Opera signal keying the amplifier directly. There was never a problem
   [...] 
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Subject: Re: LF: Class D current spikes
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Chris

When running Opera here I used the same setup as on cw. A continuous source of RF attached to the input of the amplifier with the Opera signal keying the amplifier directly. There was never a problem in many hours of operation. Are the leading and falling edges of your Opera signal shaped similar to a cw signal?

Jay W1VD 



----- Original Message -----
From: Chris Wilson <dead.fets@gmail.com>
Reply-To: <rsgb_lf_group@blacksheep.org>
To: N1BUG <rsgb_lf_group@blacksheep.org>
Sent: 2/26/2019 6:18:36 AM
Subject: Re: LF: Class D current spikes
________________________________________________________________________________



Hello N1BUG,

Just to add things were MUCH worst using a X2 multiplier circuit
(Jay's). I now use an exciter frequency of X2 direct both from the
U3S, and as of late X2 from the TS-590 into a simple squarer and use
WSPR in the "Advanced" X2 mode to correct the WSPR tones. No issues at
all with either. OPERA is a no no as of this time, it is a FET killer
:)  Don't  know  why though. It would be great to get to the bottom of
all this!

Tuesday, February 26, 2019, 11:05:15 AM, you wrote:

> Jay,

> I was using an HF transceiver in CW mode through a down converter.

> Other FETs were lost at end of envelope while running JT9 with the
> transceiver in USB being fed audio from a sound card. The latest was
> with audio from a different sound card into the new phasing exciter.

> I have never lost a FET while running with the U3S.

> 73,
> Paul




-- 
Best regards,
Chris                            mailto:dead.fets@gmail.com


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 Content preview:  I have investigated waveforms at every stage using all three
    exciters here: exciter output, doubler output, IR2110 input, FET gates, FET
    drains. I see no difference at any of these points between exci [...] 
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Subject: Re: LF: Class D current spikes
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I have investigated waveforms at every stage using all three
exciters here: exciter output, doubler output, IR2110 input, FET
gates, FET drains. I see no difference at any of these points
between exciters. However I cannot capture brief events that may
happen at the start or end of the RF envelope. I believe that is the
key.

I do find things don't look at good using the doubler was when I
made earlier tests using the HP 3325B without the doubler. I am
still rejecting the idea of running 2Fo drive from exciters as I do
not want to get locked into that requirement.

Undoubtedly I was trying to use the amp in ways Jay never intended
so I can't blame the design. Mine is now retired as I am unable to
get to the bottom of this issue with the limited test equipment at
my disposal.

73,
Paul



On 2/26/19 6:18 AM, Chris Wilson wrote:
> 
> 
> Hello N1BUG,
> 
> Just to add things were MUCH worst using a X2 multiplier circuit
> (Jay's). I now use an exciter frequency of X2 direct both from the
> U3S, and as of late X2 from the TS-590 into a simple squarer and use
> WSPR in the "Advanced" X2 mode to correct the WSPR tones. No issues at
> all with either. OPERA is a no no as of this time, it is a FET killer
> :)  Don't  know  why though. It would be great to get to the bottom of
> all this!
> 
> Tuesday, February 26, 2019, 11:05:15 AM, you wrote:
> 
>> Jay,
> 
>> I was using an HF transceiver in CW mode through a down converter.
> 
>> Other FETs were lost at end of envelope while running JT9 with the
>> transceiver in USB being fed audio from a sound card. The latest was
>> with audio from a different sound card into the new phasing exciter.
> 
>> I have never lost a FET while running with the U3S.
> 
>> 73,
>> Paul

From owner-rsgb_lf_group@blacksheep.org  Tue Feb 26 13:09:20 2019
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To: rsgb_lf_group@blacksheep.org
References: <942860C848184BA2A0A9103E0EE56DF7@DELL4>
 <1UTEEgOcyQ.DAejAuRZtn9@optiplex980-pc>
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From: Eric NO3M <no3m@no3m.net>
Message-ID: <c7ee7c98-78c6-3d45-92a0-5a2c4e700d60@no3m.net>
Date: Tue, 26 Feb 2019 07:04:43 -0500
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 Content preview:  Don't have a U3S to test with here, but the normal drive chain
    is: K3 (10.137 khz out) xvtr (137 khz out) 137 khz LPF Doubler (trifilar
   xfmr, BAT41 schottky diodes) Tuned filter (parallel coil + cap between signal
    and ground) LM311P squarer (80-90mV level detect) 401 [...] 
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Subject: Re: LF: Class D current spikes
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Don't have a U3S to test with here, but the normal drive chain is:

K3 (10.137 khz out)
xvtr (137 khz out)
137 khz LPF
Doubler (trifilar xfmr, BAT41 schottky diodes)
Tuned filter (parallel coil + cap between signal and ground)
LM311P squarer (80-90mV level detect)
4013 flip-flop
MCP1404 driver (4.5A) with ability to key supply line (per G0MRF circuit)

I'm primarily interested in CW, WSPR, JT9...

CW not a problem with a constant carrier and keying the driver. Don't 
intend to run Opera but understand Jay's method of doing so.

So running the exciter at 2x excitation and WSJTx at 2x tone spacing 
works flawlessly?  Guess that's an option...

But, going back to what Rik was eluding to... a hanging driver output.  
Can anyone capture the end of the RF envelope from a U3S when running 
WSPR?  Just a thought, perhaps the RF is ending exactly at a zero 
crossing, whereas a typical PC/soundcard + exciter may not be and that 
is causing this issue.  I can't imagine anything else that would be 
different; after all the filtering and processing, my driver outputs to 
the FET gates are very clean.

73 Eric NO3M


On 2/26/19 6:18 AM, Chris Wilson wrote:
>
> Hello N1BUG,
>
> Just to add things were MUCH worst using a X2 multiplier circuit
> (Jay's). I now use an exciter frequency of X2 direct both from the
> U3S, and as of late X2 from the TS-590 into a simple squarer and use
> WSPR in the "Advanced" X2 mode to correct the WSPR tones. No issues at
> all with either. OPERA is a no no as of this time, it is a FET killer
> :)  Don't  know  why though. It would be great to get to the bottom of
> all this!
>
>


From owner-rsgb_lf_group@blacksheep.org  Tue Feb 26 13:17:43 2019
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From: Eric NO3M <no3m@no3m.net>
To: rsgb_lf_group@blacksheep.org
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 Content preview:  Or in the case of a U3S with a square wave output at CLK0
   (I assume it's square)... a complete positive half cycle without any further
    "noise", etc. On 2/26/19 7:04 AM, Eric NO3M wrote: > Just a thought, perhaps
    the RF is ending exactly at a zero crossing, > whereas a typical PC/soundcard
    + exciter may not be and that is > causing this issue. 
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Subject: Re: LF: Class D current spikes
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Or in the case of a U3S with a square wave output at CLK0 (I assume it's 
square)... a complete positive half cycle without any further "noise", etc.

On 2/26/19 7:04 AM, Eric NO3M wrote:
> Just a thought, perhaps the RF is ending exactly at a zero crossing, 
> whereas a typical PC/soundcard + exciter may not be and that is 
> causing this issue.


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Date: Tue, 26 Feb 2019 07:12:23 -0500
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 Content preview:  Jay, I have used CW ID from the U3S extensively with never
    a problem. I understand your comments about the shaped waveform and have
   already suspected that as an issue. I am not sure what happens at the end
   of the waveform using the transceiver in USB mode driven by audi [...] 
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Subject: Re: LF: Class D current spikes
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Jay,

I have used CW ID from the U3S extensively with never a problem.

I understand your comments about the shaped waveform and have
already suspected that as an issue. I am not sure what happens at
the end of the waveform using the transceiver in USB mode driven by
audio or the phasing exciter. Based on circumstantial evidence I
suspect those are also shaped or terminate in some way the amp
cannot handle.

The bottom line is I was trying to use the amp in ways you never
intended and it wasn't working.

As a matter of curiosity it would be very interesting to investigate
and find the real cause but I must leave that to those with the
proper test equipment. If the amp could be protected from the drive
conditions which cause this issue I would resume using it. It is
more efficient than my other alternative.

73,
Paul




On 2/26/19 6:32 AM, jrusgrove@comcast.net wrote:
> Paul
> 
> Have you run cw from the U3S?
> 
> I have never run cw from a transceiver through the amplifier ...
> instead I always attach a continuous source of RF (GPS referenced
> HP3325A for example) to the amplifier input and use a keyer to
> key the amplifier. There has never been a problem in thousands of
> hours of operation.
> 
> CW from a transceiver is not the same ... it's an amplitude
> varying signal when you consider the rise and fall times of the
> shaped waveform. Rise and fall times of 5 milliseconds used to be
> the 'standard' ...  which is an eternity at 137 or 500 kHz. The
> amplifier, as designed, is not expecting an amplitude varying
> waveform at it's input.
> 
> Jay W1VD
> 
> p.s. in addition to looking at the sound card output for clues,
> I'd also look at the output of the transceiver as well
> 
> 
> ----- Original Message ----- From: N1BUG <paul@n1bug.com> 
> Reply-To: <rsgb_lf_group@blacksheep.org> To:
> <rsgb_lf_group@blacksheep.org> Sent: 2/26/2019 6:05:15 AM 
> Subject: Re: LF: Class D current spikes 
> ________________________________________________________________________________
>
>  Jay,
> 
> I was using an HF transceiver in CW mode through a down
> converter.
> 
> Other FETs were lost at end of envelope while running JT9 with
> the transceiver in USB being fed audio from a sound card. The
> latest was with audio from a different sound card into the new
> phasing exciter.
> 
> I have never lost a FET while running with the U3S.
> 
> 73, Paul
> 
> 
> On 2/25/19 8:57 PM, jrusgrove@comcast.net wrote:
>> Paul
>> 
>> Was this with a continuous frequency source at the input
>> (HP3325A maybe?) and using a keyer plugged into the amplifier
>> key jack?
>> 
>> Jay
>> 
>> 
>> 
>> 
>> 
>> ----- Original Message ----- From: N1BUG <paul@n1bug.com> 
>> Reply-To: <rsgb_lf_group@blacksheep.org> To: 
>> <rsgb_lf_group@blacksheep.org> Sent: 2/25/2019 7:50:17 PM 
>> Subject: Re: LF: Class D current spikes 
>> ________________________________________________________________________________
>>
>>
>> 
Jay,
>> 
>> Good idea, but it isn't just the sound card. I can guarantee
>> one or more destroyed FETs after sending two or three
>> characters of CW where computer and sound card are not involved
>> at all. I can also confirm that with CW the FETs are still
>> blowing at the end of RF envelope. I can hear the fuse when it
>> opens. I tried some very slow CW to confirm exactly when it was
>> happening.
>> 
>> 73, Paul
>> 
>> 
>> On 2/25/19 7:30 PM, jrusgrove@comcast.net wrote:
>>> Chris
>>> 
>>> Thanks for the waveforms ... very informative. Sure looks
>>> like something is triggering the input of the amplifier and
>>> thus causing the problem.
>>> 
>>> Since the problem doesn't exist with U3S's (which generates 
>>> the various modes internally) driving the amplifier (either 
>>> directly or through a frequency doubler) one has to wonder
>>> what the difference is between the U3S and the other exciter
>>> setups that cause the problem. The fact that the U3S /
>>> amplifier combination works correctly would argue that the
>>> 'problem' is likely not the amplifier.
>>> 
>>> The one thing that the non U3S setups have in common is that 
>>> the modes are generated by software / computer / sound card. 
>>> Think the first step in tracking down the problem would be
>>> to see if there are any unexpected outputs from the soundcard
>>> that are causing the problem. When you get a chance maybe you
>>> can capture waveforms of the sound card output up to and
>>> after the end of a transmission.
>>> 
>>> Assume that you have disabled all 'computer sounds' on the 
>>> machines that are supplying audio for the various modes?
>>> 
>>> Jay W1VD
>>> 
>>> 
>>> 
>>> 
>>> 
>>> ----- Original Message ----- From: "Chris Wilson" 
>>> <dead.fets@gmail.com> To: "N1BUG" 
>>> <rsgb_lf_group@blacksheep.org> Sent: Monday, February 25,
>>> 2019 5:02 PM Subject: Re: LF: Class D current spikes
>>> 
>>> 
>>>> 
>>>> 
>>>> Hello  Paul. everyone
>>>> 
>>>> A  series  of  overlapping  scope  captures  at end of WSPR
>>>>  sequence  with  expensive  high  voltage  /  current 
>>>> Wolfspeed FET's that usually survived, into the antenna
>>>> and into a 10kW dummy load, taken after  the choke and also
>>>> at the drains of the W1VD amp. Driver TS-590 /  W1VD
>>>> doubler, and W1VD amp ( end part of another circuit). U3S
>>>> does not show anything like this oscillating end to a TX
>>>> sequence.:
>>>> 
>>>> http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-antenna.zip
>>>>
>>>>
>>>>
>>
>>>>
>
>>>> 
http://www.chriswilson.tv/wolfspeed-choke-and-drain-50v-smps-dummy-load.zip
>>>> 
>>>> Green trace drain, yellow after the choke.
>>>> 
>>>> 
>>>> 
>>>> Monday, February 25, 2019, 4:34:05 PM, you wrote:
>>>> 
>>>>> Chris, LF,
>>>> 
>>>>> Yes, although I run mine differently. I use the full 
>>>>> output of the U3S into a doubler. I have run WSPR, JT9,
>>>>> and DFCW from the U3S without having any problems. I have
>>>>> also extensively used CW ID with the U3S and amp without 
>>>>> problems. Yet both other exciters blow FETs at the
>>>>> instant RF stops.
>>>> 
>>>>> Chris, I know you are busy but if you get a chance I
>>>>> would like to see those scope captures. I thought I had
>>>>> it figured out that this is a voltage mode amp and should
>>>>> be seeing current spikes, but maybe I still have that
>>>>> wrong! If they are voltage spikes that may be easier to
>>>>> control.
>>>> 
>>>>> One thing I would like to learn more about is why do the
>>>>>  drivers leave one phase high for a longer period than a 
>>>>> half cycle when RF stops. What causes this? Is this only 
>>>>> with specific FET drivers or are all of them prone to 
>>>>> this?
>>>> 
>>>>> 73, Paul
>>>> 
>>>> 
>>>>> On 2/25/19 11:13 AM, Eric NO3M wrote:
>>>>>> Chris, et.al.
>>>>>> 
>>>>>> N1BUG relayed the same information regarding the U3S
>>>>>> and class-D amp behavior, so your observation is not a
>>>>>> one off...
>>>>>> 
>>>>>> 
>>>>>> 
>>>>>>> 
>>>>>>> I have a series of scope captures from my W1VD amp 
>>>>>>> showing huge voltage spikes on the FET drains at the 
>>>>>>> end of WSPR and especially OPERA TX sequences. I 
>>>>>>> suspected inductance was the cause. In fact I try
>>>>>>> not use OPERA at high power as i am pretty sure to
>>>>>>> kill a FET after a few sessions... Oddly (although I
>>>>>>> hope msomeone more knowlegeable has the answer),
>>>>>>> using WSPR from my U3S direct from CLK0 of  th
>>>>>>> Si535a  or whatever it is never causes these
>>>>>>> spikes...  Or at least they are well contained.

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Date: Tue, 26 Feb 2019 16:09:50 +0000
From: Chris Wilson <dead.fets@gmail.com>
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To: Eric NO3M <rsgb_lf_group@blacksheep.org>
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 Content preview:  Hello Eric, Yes, the output is a square wave when I use the
    U3S I take the output direct from CLK0 at 2X frequency (set in the U3S menu)
    via a co-ax to the input of the W1VD amp to Pin 3 of 74F74 with no 50 Ohm
    l [...] 
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Subject: Re: LF: Class D current spikes
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Hello Eric,

Yes, the output is a square wave when I use the U3S I take the output
direct from CLK0 at 2X frequency (set in the U3S menu) via a co-ax to
the input of the W1VD amp to Pin 3 of 74F74 with no 50 Ohm load
resistor. It works perfectly. It makes me think other exciters are
doing something different at the end of the TX cycle. I know not what
though...

The amp is powered all the time, the output solely depends on the
presence or not of an input signal.

Same with the TS-590S, output from the DRV socket at under 0dBm sine
wave at 2X frequency from the 590 into a squarer. Squarer drives the
W1VD amp the same, (no 50 ohm resistor) direct to Pin 3 of the 74F74.
no issues. Run the 590 at 136kHz into a W1VD doubler and a pre amp and
the FETS's life is always short. Death always seemingly occurs at the
end of a WSPR or OPERA cycle. Again the amp stays powered all the time
from either a huge linear supply or an HP SMPS 50V supply from a
server.

I have noted that running the over current limiter on the linear on
the cusp of triggering helps. The SMPS is ruthless in the doubler
scenario and FET life is *always* on the edge. The gate waveforms seem
OK, it's the drain waveform that shows the spikes as the oscillations
decay away. I would love to get to the bottom of this as I have too
many different set ups to remember :) I assumed it was some sort of
feedback from the antenna perhaps, but I am a novice and once I found
what saved me from spending loads at Farnell I gave up chasing the
cause.

Tuesday, February 26, 2019, 12:12:08 PM, you wrote:

> Or in the case of a U3S with a square wave output at CLK0 (I assume it's
> square)... a complete positive half cycle without any further "noise", etc.

> On 2/26/19 7:04 AM, Eric NO3M wrote:
>> Just a thought, perhaps the RF is ending exactly at a zero crossing, 
>> whereas a typical PC/soundcard + exciter may not be and that is 
>> causing this issue.





-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Tue, 26 Feb 2019 16:38:15 +0000
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 Content preview:  AH - HA !!!!!!!!!!!! Therein may lie your problem. If you
   take your input direct to the 74F74 clock and don't hit that with anything
    other than a square wave you are bound to have problems. TTL device [...]
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Subject: Re: LF: Class D current spikes
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--000000000000642a150582ceb086
Content-Type: text/plain; charset="UTF-8"

AH - HA !!!!!!!!!!!!
Therein may lie your problem.   If you take your input direct to the 74F74
clock and don't hit that with anything other than a square wave you are
bound to have problems.   TTL devices (and F series really IS real TTL) get
very unhappy with slow edges and can oscillate or show instability at the
edges

Even if you precede that with the classic inverter and linearising
resistor, at low frequencies you will often see instability.   That
fed-back gate design usually works fine at tens of MHz and up, even MHz,
but expect instability at kHz frequencies.   Look at the output on a scope,
and don't be surprised to see ringing on the edges , especially at low
drive levels, and low drive levels are just what you get when the input
waveform is keyed on / off

At these frequencies, linear to logic conversion really MUST be done with a
Schmitt trigger.   74xCT14 or similar.   Use the ACT or HCT families as
opposed to the HC or AC ones as they have a smaller hysteresis between
Vin(HI) and Vin(lo), allowing for lower amplitude drive.  They also need
different centre biassing for AC coupled signals.  Assuming a 5V rail, Use
2.5V  for HC and AC families,  1.8V for ACT and  HCT devices.

Or an RS422 / RS485  line receiver works well; that has even lower
hysteresis and hence lower permitted drive level.

Andy
www.g4jnt.com



On Tue, 26 Feb 2019 at 16:14, Chris Wilson <dead.fets@gmail.com> wrote:

>
>
> Hello Eric,
>
> Yes, the output is a square wave when I use the U3S I take the output
> direct from CLK0 at 2X frequency (set in the U3S menu) via a co-ax to
> the input of the W1VD amp to Pin 3 of 74F74 with no 50 Ohm load
> resistor. It works perfectly. It makes me think other exciters are
> doing something different at the end of the TX cycle. I know not what
> though...
>
> The amp is powered all the time, the output solely depends on the
> presence or not of an input signal.
>
> Same with the TS-590S, output from the DRV socket at under 0dBm sine
> wave at 2X frequency from the 590 into a squarer. Squarer drives the
> W1VD amp the same, (no 50 ohm resistor) direct to Pin 3 of the 74F74.
> no issues. Run the 590 at 136kHz into a W1VD doubler and a pre amp and
> the FETS's life is always short. Death always seemingly occurs at the
> end of a WSPR or OPERA cycle. Again the amp stays powered all the time
> from either a huge linear supply or an HP SMPS 50V supply from a
> server.
>
> I have noted that running the over current limiter on the linear on
> the cusp of triggering helps. The SMPS is ruthless in the doubler
> scenario and FET life is *always* on the edge. The gate waveforms seem
> OK, it's the drain waveform that shows the spikes as the oscillations
> decay away. I would love to get to the bottom of this as I have too
> many different set ups to remember :) I assumed it was some sort of
> feedback from the antenna perhaps, but I am a novice and once I found
> what saved me from spending loads at Farnell I gave up chasing the
> cause.
>
> Tuesday, February 26, 2019, 12:12:08 PM, you wrote:
>
> > Or in the case of a U3S with a square wave output at CLK0 (I assume it's
> > square)... a complete positive half cycle without any further "noise",
> etc.
>
> > On 2/26/19 7:04 AM, Eric NO3M wrote:
> >> Just a thought, perhaps the RF is ending exactly at a zero crossing,
> >> whereas a typical PC/soundcard + exciter may not be and that is
> >> causing this issue.
>
>
>
>
>
> --
> Best regards,
>  Chris                            mailto:dead.fets@gmail.com
>
>
>

--000000000000642a150582ceb086
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">AH - HA !!!!!!!!!!!!</div><div class=3D"gmail_de=
fault" style=3D"font-family:tahoma,sans-serif;font-size:small">Therein may =
lie your problem.=C2=A0 =C2=A0If you take your input direct to the 74F74 cl=
ock and don&#39;t hit that with anything other than a square wave you are b=
ound to have problems.=C2=A0 =C2=A0TTL devices (and F series really IS real=
 TTL) get very unhappy with slow edges and can oscillate or show instabilit=
y at the edges</div><div class=3D"gmail_default" style=3D"font-family:tahom=
a,sans-serif;font-size:small"><br></div><div class=3D"gmail_default" style=
=3D"font-family:tahoma,sans-serif;font-size:small">Even if you precede that=
 with the classic inverter and linearising resistor, at low frequencies you=
 will often see instability.=C2=A0 =C2=A0That fed-back gate design usually =
works fine at tens of MHz and up, even MHz, but expect instability at kHz f=
requencies.=C2=A0 =C2=A0Look at the output on a scope, and don&#39;t be sur=
prised to see ringing on the edges , especially at low drive levels, and lo=
w drive levels are just what you get when the input waveform is keyed on / =
off</div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-seri=
f;font-size:small"><br></div><div class=3D"gmail_default" style=3D"font-fam=
ily:tahoma,sans-serif;font-size:small">At these frequencies, linear to logi=
c conversion really MUST be done with a Schmitt trigger.=C2=A0 =C2=A074xCT1=
4 or similar.=C2=A0 =C2=A0Use the ACT or HCT families as opposed to the HC =
or AC ones as they have a smaller hysteresis between Vin(HI) and Vin(lo), a=
llowing for lower amplitude drive.=C2=A0 They also need different centre bi=
assing for AC coupled signals.=C2=A0 Assuming a 5V rail, Use 2.5V=C2=A0 for=
 HC and AC families,=C2=A0 1.8V for ACT and=C2=A0 HCT devices.</div><div cl=
ass=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:smal=
l"><br></div><div class=3D"gmail_default" style=3D"font-family:tahoma,sans-=
serif;font-size:small">Or an RS422 / RS485=C2=A0 line receiver works well; =
that has even lower hysteresis and hence lower permitted drive level.</div>=
<div class=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-si=
ze:small"><br></div><div><div dir=3D"ltr" class=3D"gmail_signature" data-sm=
artmail=3D"gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><di=
v dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span st=
yle=3D"font-size:12.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank"=
>www.g4jnt.com</a></span><br></div><div><br></div></div></div></div></div><=
/div></div></div></div></div></div></div><br></div><br><div class=3D"gmail_=
quote"><div dir=3D"ltr" class=3D"gmail_attr">On Tue, 26 Feb 2019 at 16:14, =
Chris Wilson &lt;<a href=3D"mailto:dead.fets@gmail.com">dead.fets@gmail.com=
</a>&gt; wrote:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:=
0px 0px 0px 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex">=
<br>
<br>
Hello Eric,<br>
<br>
Yes, the output is a square wave when I use the U3S I take the output<br>
direct from CLK0 at 2X frequency (set in the U3S menu) via a co-ax to<br>
the input of the W1VD amp to Pin 3 of 74F74 with no 50 Ohm load<br>
resistor. It works perfectly. It makes me think other exciters are<br>
doing something different at the end of the TX cycle. I know not what<br>
though...<br>
<br>
The amp is powered all the time, the output solely depends on the<br>
presence or not of an input signal.<br>
<br>
Same with the TS-590S, output from the DRV socket at under 0dBm sine<br>
wave at 2X frequency from the 590 into a squarer. Squarer drives the<br>
W1VD amp the same, (no 50 ohm resistor) direct to Pin 3 of the 74F74.<br>
no issues. Run the 590 at 136kHz into a W1VD doubler and a pre amp and<br>
the FETS&#39;s life is always short. Death always seemingly occurs at the<b=
r>
end of a WSPR or OPERA cycle. Again the amp stays powered all the time<br>
from either a huge linear supply or an HP SMPS 50V supply from a<br>
server.<br>
<br>
I have noted that running the over current limiter on the linear on<br>
the cusp of triggering helps. The SMPS is ruthless in the doubler<br>
scenario and FET life is *always* on the edge. The gate waveforms seem<br>
OK, it&#39;s the drain waveform that shows the spikes as the oscillations<b=
r>
decay away. I would love to get to the bottom of this as I have too<br>
many different set ups to remember :) I assumed it was some sort of<br>
feedback from the antenna perhaps, but I am a novice and once I found<br>
what saved me from spending loads at Farnell I gave up chasing the<br>
cause.<br>
<br>
Tuesday, February 26, 2019, 12:12:08 PM, you wrote:<br>
<br>
&gt; Or in the case of a U3S with a square wave output at CLK0 (I assume it=
&#39;s<br>
&gt; square)... a complete positive half cycle without any further &quot;no=
ise&quot;, etc.<br>
<br>
&gt; On 2/26/19 7:04 AM, Eric NO3M wrote:<br>
&gt;&gt; Just a thought, perhaps the RF is ending exactly at a zero crossin=
g, <br>
&gt;&gt; whereas a typical PC/soundcard + exciter may not be and that is <b=
r>
&gt;&gt; causing this issue.<br>
<br>
<br>
<br>
<br>
<br>
-- <br>
Best regards,<br>
=C2=A0Chris=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 mailto:<a href=3D"mailto:dead.fets@gmail=
.com" target=3D"_blank">dead.fets@gmail.com</a><br>
<br>
<br>
</blockquote></div>

--000000000000642a150582ceb086--

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Date: Tue, 26 Feb 2019 17:07:57 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello Andy, Thanks for that! Bearing in mind i am not the
   sharpest knife in this drawer, would that perhaps explain why the U3S Si5351a
    output drives more reliably at 3.3V than say the output of a doubler / pre
    a [...] 
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Hello Andy,

Thanks for that! Bearing in mind i am not the sharpest knife in this
drawer,  would  that  perhaps explain  why the U3S Si5351a output drives more
reliably at 3.3V  than  say the output of a doubler / pre amp (and I was never
happy  about  the  pre amp output level being correct...), and perhaps
the  output  from the squarer also being more "reliable"? Would you be
able to sketch an interface design to try please? Thanks again, are we
getting somewhere? ;)

Tuesday, February 26, 2019, 4:38:15 PM, you wrote:

> AH - HA !!!!!!!!!!!!
> Therein may lie your problem.   If you take your input direct to
> the 74F74 clock and don't hit that with anything other than a square
> wave you are bound to have problems.   TTL devices (and F series
> really IS real TTL) get very unhappy with slow edges and can
> oscillate or show instability at the edges


> Even if you precede that with the classic inverter and linearising
> resistor, at low frequencies you will often see instability.   That
> fed-back gate design usually works fine at tens of MHz and up, even
> MHz, but expect instability at kHz frequencies.   Look at the output
> on a scope, and don't be surprised to see ringing on the edges ,
> especially at low drive levels, and low drive levels are just what
> you get when the input waveform is keyed on / off


> At these frequencies, linear to logic conversion really MUST be
> done with a Schmitt trigger.   74xCT14 or similar.   Use the ACT or
> HCT families as opposed to the HC or AC ones as they have a smaller
> hysteresis between Vin(HI) and Vin(lo), allowing for lower amplitude
> drive.  They also need different centre biassing for AC coupled
> signals.  Assuming a 5V rail, Use 2.5V  for HC and AC families,  1.8V for ACT and  HCT devices.


> Or an RS422 / RS485  line receiver works well; that has even lower
> hysteresis and hence lower permitted drive level.


> Andy
> www.g4jnt.com




-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com



From owner-rsgb_lf_group@blacksheep.org  Tue Feb 26 18:41:35 2019
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References: <942860C848184BA2A0A9103E0EE56DF7@DELL4>
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From: Eric NO3M <no3m@no3m.net>
Message-ID: <57e33c0d-6904-9010-a1c8-69b80f474068@no3m.net>
Date: Tue, 26 Feb 2019 12:35:10 -0500
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 Content preview:  Just to clarify... did you say previously that the U3S also
    worked fine running at 1x and feeding a doubler, squarer, etc. also? On 2/26/19
    11:09 AM, Chris Wilson wrote: > > Hello Eric, > > Yes, the output is a square
    wave when I use the U3S I take the output > direct from CLK0 at 2X frequency
    (set in the U3S menu) via a co-ax [...] 
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Just to clarify... did you say previously that the U3S also worked fine 
running at 1x and feeding a doubler, squarer, etc. also?



On 2/26/19 11:09 AM, Chris Wilson wrote:
>
> Hello Eric,
>
> Yes, the output is a square wave when I use the U3S I take the output
> direct from CLK0 at 2X frequency (set in the U3S menu) via a co-ax to
> the input of the W1VD amp to Pin 3 of 74F74 with no 50 Ohm load
> resistor. It works perfectly. It makes me think other exciters are
> doing something different at the end of the TX cycle. I know not what
> though...
>
> The amp is powered all the time, the output solely depends on the
> presence or not of an input signal.
>
> Same with the TS-590S, output from the DRV socket at under 0dBm sine
> wave at 2X frequency from the 590 into a squarer. Squarer drives the
> W1VD amp the same, (no 50 ohm resistor) direct to Pin 3 of the 74F74.
> no issues. Run the 590 at 136kHz into a W1VD doubler and a pre amp and
> the FETS's life is always short. Death always seemingly occurs at the
> end of a WSPR or OPERA cycle. Again the amp stays powered all the time
> from either a huge linear supply or an HP SMPS 50V supply from a
> server.
>
> I have noted that running the over current limiter on the linear on
> the cusp of triggering helps. The SMPS is ruthless in the doubler
> scenario and FET life is *always* on the edge. The gate waveforms seem
> OK, it's the drain waveform that shows the spikes as the oscillations
> decay away. I would love to get to the bottom of this as I have too
> many different set ups to remember :) I assumed it was some sort of
> feedback from the antenna perhaps, but I am a novice and once I found
> what saved me from spending loads at Farnell I gave up chasing the
> cause.
>
> Tuesday, February 26, 2019, 12:12:08 PM, you wrote:
>
>> Or in the case of a U3S with a square wave output at CLK0 (I assume it's
>> square)... a complete positive half cycle without any further "noise", etc.
>> On 2/26/19 7:04 AM, Eric NO3M wrote:
>>> Just a thought, perhaps the RF is ending exactly at a zero crossing,
>>> whereas a typical PC/soundcard + exciter may not be and that is
>>> causing this issue.
>
>
>
>


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Date: Tue, 26 Feb 2019 17:52:07 +0000
From: Chris Wilson <dead.fets@gmail.com>
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 Content preview:  Hello Eric, No, I have always run the U3S in X2 mode as far
    as I can remember. No doubler, no squarer, just straight out of CLK0 to Pin
    3 of the 74F74. And no issues at all. Thanks. BTW, I really admire your old
    [...] 
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Hello Eric,

No,  I have always run the U3S in X2 mode as far as I can remember. No
doubler,  no squarer, just straight out of CLK0 to Pin 3 of the 74F74.
And  no  issues  at all. Thanks. BTW, I really admire your old gear on
your web site, awesome build standards and so nice to look at!

Tuesday, February 26, 2019, 5:35:10 PM, you wrote:

> Just to clarify... did you say previously that the U3S also worked fine
> running at 1x and feeding a doubler, squarer, etc. also?







-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


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From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Tue, 26 Feb 2019 18:10:47 +0000
Message-ID: <CAA8k23S3fMCbY+ku3si2+xnNV=f8cetCi8jOngi7x2a1sD6fNg@mail.gmail.com>
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 Content preview:  I'll put it in the groups.io folder under my callsign [image:
    LF_IFACE.gif] Andy www.g4jnt.com On Tue, 26 Feb 2019 at 17:12, Chris Wilson
    wrote: > > > Hello Andy, > > Thanks for that! Bearing in mind i am not the
    sharpest knife in this > drawer, would that perhaps explain why the U3S Si5351a
    output drives > more > reliably at 3.3V than say the [...] 
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Subject: Re: LF: Class D current spikes
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I'll put it in the groups.io folder under my callsign
[image: LF_IFACE.gif]
Andy
www.g4jnt.com



On Tue, 26 Feb 2019 at 17:12, Chris Wilson <dead.fets@gmail.com> wrote:

>
>
> Hello Andy,
>
> Thanks for that! Bearing in mind i am not the sharpest knife in this
> drawer,  would  that  perhaps explain  why the U3S Si5351a output drives
> more
> reliably at 3.3V  than  say the output of a doubler / pre amp (and I was
> never
> happy  about  the  pre amp output level being correct...), and perhaps
> the  output  from the squarer also being more "reliable"? Would you be
> able to sketch an interface design to try please? Thanks again, are we
> getting somewhere? ;)
>
> Tuesday, February 26, 2019, 4:38:15 PM, you wrote:
>
> > AH - HA !!!!!!!!!!!!
> > Therein may lie your problem.   If you take your input direct to
> > the 74F74 clock and don't hit that with anything other than a square
> > wave you are bound to have problems.   TTL devices (and F series
> > really IS real TTL) get very unhappy with slow edges and can
> > oscillate or show instability at the edges
>
>
> > Even if you precede that with the classic inverter and linearising
> > resistor, at low frequencies you will often see instability.   That
> > fed-back gate design usually works fine at tens of MHz and up, even
> > MHz, but expect instability at kHz frequencies.   Look at the output
> > on a scope, and don't be surprised to see ringing on the edges ,
> > especially at low drive levels, and low drive levels are just what
> > you get when the input waveform is keyed on / off
>
>
> > At these frequencies, linear to logic conversion really MUST be
> > done with a Schmitt trigger.   74xCT14 or similar.   Use the ACT or
> > HCT families as opposed to the HC or AC ones as they have a smaller
> > hysteresis between Vin(HI) and Vin(lo), allowing for lower amplitude
> > drive.  They also need different centre biassing for AC coupled
> > signals.  Assuming a 5V rail, Use 2.5V  for HC and AC families,  1.8V
> for ACT and  HCT devices.
>
>
> > Or an RS422 / RS485  line receiver works well; that has even lower
> > hysteresis and hence lower permitted drive level.
>
>
> > Andy
> > www.g4jnt.com
>
>
>
>
> --
> Best regards,
>  Chris                            mailto:dead.fets@gmail.com
>
>
>

--0000000000004e04a60582cffb28
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<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">I&#39;ll put it in the <a href=3D"http://groups.=
io">groups.io</a> folder under my callsign</div><div class=3D"gmail_default=
" style=3D"font-family:tahoma,sans-serif;font-size:small"><div><img src=3D"=
cid:ii_jsm36n370" alt=3D"LF_IFACE.gif" width=3D"472" height=3D"327"><br></d=
iv></div><div><div dir=3D"ltr" class=3D"gmail_signature" data-smartmail=3D"=
gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"lt=
r"><div><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=3D"font=
-size:12.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank">www.g4jnt.=
com</a></span><br></div><div><br></div></div></div></div></div></div></div>=
</div></div></div></div></div><br></div><br><div class=3D"gmail_quote"><div=
 dir=3D"ltr" class=3D"gmail_attr">On Tue, 26 Feb 2019 at 17:12, Chris Wilso=
n &lt;<a href=3D"mailto:dead.fets@gmail.com">dead.fets@gmail.com</a>&gt; wr=
ote:<br></div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px=
 0.8ex;border-left:1px solid rgb(204,204,204);padding-left:1ex"><br>
<br>
Hello Andy,<br>
<br>
Thanks for that! Bearing in mind i am not the sharpest knife in this<br>
drawer,=C2=A0 would=C2=A0 that=C2=A0 perhaps explain=C2=A0 why the U3S Si53=
51a output drives more<br>
reliably at 3.3V=C2=A0 than=C2=A0 say the output of a doubler / pre amp (an=
d I was never<br>
happy=C2=A0 about=C2=A0 the=C2=A0 pre amp output level being correct...), a=
nd perhaps<br>
the=C2=A0 output=C2=A0 from the squarer also being more &quot;reliable&quot=
;? Would you be<br>
able to sketch an interface design to try please? Thanks again, are we<br>
getting somewhere? ;)<br>
<br>
Tuesday, February 26, 2019, 4:38:15 PM, you wrote:<br>
<br>
&gt; AH - HA !!!!!!!!!!!!<br>
&gt; Therein may lie your problem.=C2=A0 =C2=A0If you take your input direc=
t to<br>
&gt; the 74F74 clock and don&#39;t hit that with anything other than a squa=
re<br>
&gt; wave you are bound to have problems.=C2=A0 =C2=A0TTL devices (and F se=
ries<br>
&gt; really IS real TTL) get very unhappy with slow edges and can<br>
&gt; oscillate or show instability at the edges<br>
<br>
<br>
&gt; Even if you precede that with the classic inverter and linearising<br>
&gt; resistor, at low frequencies you will often see instability.=C2=A0 =C2=
=A0That<br>
&gt; fed-back gate design usually works fine at tens of MHz and up, even<br=
>
&gt; MHz, but expect instability at kHz frequencies.=C2=A0 =C2=A0Look at th=
e output<br>
&gt; on a scope, and don&#39;t be surprised to see ringing on the edges ,<b=
r>
&gt; especially at low drive levels, and low drive levels are just what<br>
&gt; you get when the input waveform is keyed on / off<br>
<br>
<br>
&gt; At these frequencies, linear to logic conversion really MUST be<br>
&gt; done with a Schmitt trigger.=C2=A0 =C2=A074xCT14 or similar.=C2=A0 =C2=
=A0Use the ACT or<br>
&gt; HCT families as opposed to the HC or AC ones as they have a smaller<br=
>
&gt; hysteresis between Vin(HI) and Vin(lo), allowing for lower amplitude<b=
r>
&gt; drive.=C2=A0 They also need different centre biassing for AC coupled<b=
r>
&gt; signals.=C2=A0 Assuming a 5V rail, Use 2.5V=C2=A0 for HC and AC famili=
es,=C2=A0 1.8V for ACT and=C2=A0 HCT devices.<br>
<br>
<br>
&gt; Or an RS422 / RS485=C2=A0 line receiver works well; that has even lowe=
r<br>
&gt; hysteresis and hence lower permitted drive level.<br>
<br>
<br>
&gt; Andy<br>
&gt; <a href=3D"http://www.g4jnt.com" rel=3D"noreferrer" target=3D"_blank">=
www.g4jnt.com</a><br>
<br>
<br>
<br>
<br>
-- <br>
Best regards,<br>
=C2=A0Chris=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 =
=C2=A0 =C2=A0 =C2=A0 =C2=A0 =C2=A0 mailto:<a href=3D"mailto:dead.fets@gmail=
.com" target=3D"_blank">dead.fets@gmail.com</a><br>
<br>
<br>
</blockquote></div>

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 Content preview:  Eric, I I have always run my U3S through the W1VD doubler.
    Never had any problems with blown FETs with that setup, even when I tested
    at 1 kW under Part 5 license. There is apparently something different ab
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Subject: Re: LF: Class D current spikes
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Eric,

I I have always run my U3S through the W1VD doubler. Never had any
problems with blown FETs with that setup, even when I tested at 1 kW
under Part 5 license. There is apparently something different about
the U3S at end of RF envelope.

73,
Paul


On 2/26/19 12:52 PM, Chris Wilson wrote:
> 
> 
> Hello Eric,
> 
> No,  I have always run the U3S in X2 mode as far as I can remember. No
> doubler,  no squarer, just straight out of CLK0 to Pin 3 of the 74F74.
> And  no  issues  at all. Thanks. BTW, I really admire your old gear on
> your web site, awesome build standards and so nice to look at!
> 
> Tuesday, February 26, 2019, 5:35:10 PM, you wrote:
> 
>> Just to clarify... did you say previously that the U3S also worked fine
>> running at 1x and feeding a doubler, squarer, etc. also?

From owner-rsgb_lf_group@blacksheep.org  Tue Feb 26 20:16:59 2019
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 Content preview:  Anyone have a U3S schematic handy? Link to same? Jay W1VD
   ----- Original Message ----- From: "N1BUG" To: Sent: Tuesday, February 26,
    2019 2:01 PM Subject: Re: LF: Class D current spikes 
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Subject: Re: LF: Class D current spikes
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Anyone have a U3S schematic handy? Link to same?

Jay W1VD

----- Original Message ----- 
From: "N1BUG" <paul@n1bug.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, February 26, 2019 2:01 PM
Subject: Re: LF: Class D current spikes


> Eric,
> 
> I I have always run my U3S through the W1VD doubler. Never had any
> problems with blown FETs with that setup, even when I tested at 1 kW
> under Part 5 license. There is apparently something different about
> the U3S at end of RF envelope.
> 
> 73,
> Paul
> 
> 
> On 2/26/19 12:52 PM, Chris Wilson wrote:
>> 
>> 
>> Hello Eric,
>> 
>> No,  I have always run the U3S in X2 mode as far as I can remember. No
>> doubler,  no squarer, just straight out of CLK0 to Pin 3 of the 74F74.
>> And  no  issues  at all. Thanks. BTW, I really admire your old gear on
>> your web site, awesome build standards and so nice to look at!
>> 
>> Tuesday, February 26, 2019, 5:35:10 PM, you wrote:
>> 
>>> Just to clarify... did you say previously that the U3S also worked fine
>>> running at 1x and feeding a doubler, squarer, etc. also?
>

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 Content preview:  Jay, The U3S schematic is in the assembly manual: http://qrp-labs.com/images/ultimate3s/assembly_u3s_r3_lt.pdf
 Content analysis details:   (-0.0 points, 5.0 required)
  pts rule name              description
 ---- ---------------------- --------------------------------------------------
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                             no trust
                             [74.208.4.194 listed in list.dnswl.org]
 -0.0 SPF_HELO_PASS          SPF: HELO matches SPF record
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Subject: Re: LF: Class D current spikes
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Jay,

The U3S schematic is in the assembly manual:

http://qrp-labs.com/images/ultimate3s/assembly_u3s_r3_lt.pdf

73,
Paul


On 2/26/19 2:12 PM, jrusgrove@comcast.net wrote:
> Anyone have a U3S schematic handy? Link to same?
> 
> Jay W1VD
> 
> ----- Original Message ----- 
> From: "N1BUG" <paul@n1bug.com>
> To: <rsgb_lf_group@blacksheep.org>
> Sent: Tuesday, February 26, 2019 2:01 PM
> Subject: Re: LF: Class D current spikes
> 
> 
>> Eric,
>>
>> I I have always run my U3S through the W1VD doubler. Never had any
>> problems with blown FETs with that setup, even when I tested at 1 kW
>> under Part 5 license. There is apparently something different about
>> the U3S at end of RF envelope.
>>
>> 73,
>> Paul
>>
>>
>> On 2/26/19 12:52 PM, Chris Wilson wrote:
>>>
>>>
>>> Hello Eric,
>>>
>>> No,  I have always run the U3S in X2 mode as far as I can remember. No
>>> doubler,  no squarer, just straight out of CLK0 to Pin 3 of the 74F74.
>>> And  no  issues  at all. Thanks. BTW, I really admire your old gear on
>>> your web site, awesome build standards and so nice to look at!
>>>
>>> Tuesday, February 26, 2019, 5:35:10 PM, you wrote:
>>>
>>>> Just to clarify... did you say previously that the U3S also worked fine
>>>> running at 1x and feeding a doubler, squarer, etc. also?

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References: <942860C848184BA2A0A9103E0EE56DF7@DELL4> <1UTEEgOcyQ.DAejAuRZtn9@optiplex980-pc>
 <92784b07-a799-fb4e-9080-e1e8bb167b75@n1bug.com> <1UTEEhG1Ft.EdI1dlVbFOZ@optiplex980-pc>
 <3062ef19-bb69-3187-e8db-6a6bf5050739@n1bug.com> <234098919.20190226111836@gmail.com>
 <c7ee7c98-78c6-3d45-92a0-5a2c4e700d60@no3m.net> <0a79de5c-3274-caae-c000-d5f49bb44540@no3m.net>
 <21240445.20190226160950@gmail.com> <57e33c0d-6904-9010-a1c8-69b80f474068@no3m.net>
 <1191469216.20190226175207@gmail.com> <edd9cdbe-494a-da9a-f15c-b0d63fe0040c@n1bug.com>
 <823BBA7099F84CE9924D2D9E7E379C05@DELL4> <1677ed22-9174-82d9-e7aa-f08d1c42f130@n1bug.com>
In-Reply-To: <1677ed22-9174-82d9-e7aa-f08d1c42f130@n1bug.com>
From: Andy Talbot <andy.g4jnt@gmail.com>
Date: Tue, 26 Feb 2019 19:25:58 +0000
Message-ID: <CAA8k23SVFQR3fCTTsRLuVdLCcP-rhrGAHFL1PPsmxRt2i2c7Dg@mail.gmail.com>
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
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 Content preview:  So if used with no LPF (as it should be in this situation)
    the RF output may well have quite sharp edges. Just what's wanted. But for
    driving a divider, a direct connection to CLK0 is ideal and preferred. 
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Subject: Re: LF: Class D current spikes
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--000000000000225c730582d108bd
Content-Type: text/plain; charset="UTF-8"

So if used with no LPF (as it should be in this situation) the RF output
may well have quite sharp edges.
Just what's wanted.

But for driving a divider, a direct connection to CLK0 is ideal and
preferred.

Andy
www.g4jnt.com



On Tue, 26 Feb 2019 at 19:23, N1BUG <paul@n1bug.com> wrote:

> Jay,
>
> The U3S schematic is in the assembly manual:
>
> http://qrp-labs.com/images/ultimate3s/assembly_u3s_r3_lt.pdf
>
> 73,
> Paul
>
>
> On 2/26/19 2:12 PM, jrusgrove@comcast.net wrote:
> > Anyone have a U3S schematic handy? Link to same?
> >
> > Jay W1VD
> >
> > ----- Original Message -----
> > From: "N1BUG" <paul@n1bug.com>
> > To: <rsgb_lf_group@blacksheep.org>
> > Sent: Tuesday, February 26, 2019 2:01 PM
> > Subject: Re: LF: Class D current spikes
> >
> >
> >> Eric,
> >>
> >> I I have always run my U3S through the W1VD doubler. Never had any
> >> problems with blown FETs with that setup, even when I tested at 1 kW
> >> under Part 5 license. There is apparently something different about
> >> the U3S at end of RF envelope.
> >>
> >> 73,
> >> Paul
> >>
> >>
> >> On 2/26/19 12:52 PM, Chris Wilson wrote:
> >>>
> >>>
> >>> Hello Eric,
> >>>
> >>> No,  I have always run the U3S in X2 mode as far as I can remember. No
> >>> doubler,  no squarer, just straight out of CLK0 to Pin 3 of the 74F74.
> >>> And  no  issues  at all. Thanks. BTW, I really admire your old gear on
> >>> your web site, awesome build standards and so nice to look at!
> >>>
> >>> Tuesday, February 26, 2019, 5:35:10 PM, you wrote:
> >>>
> >>>> Just to clarify... did you say previously that the U3S also worked
> fine
> >>>> running at 1x and feeding a doubler, squarer, etc. also?
>
>

--000000000000225c730582d108bd
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div dir=3D"ltr"><div class=3D"gmail_default" style=3D"font-family:tahoma,s=
ans-serif;font-size:small">So if used with no LPF (as it should be in this =
situation) the RF output may well have quite sharp edges.</div><div class=
=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:small">=
Just what&#39;s wanted.</div><div class=3D"gmail_default" style=3D"font-fam=
ily:tahoma,sans-serif;font-size:small"><br></div><div class=3D"gmail_defaul=
t" style=3D"font-family:tahoma,sans-serif;font-size:small">But for driving =
a divider, a direct connection to CLK0 is ideal and preferred.</div><div cl=
ass=3D"gmail_default" style=3D"font-family:tahoma,sans-serif;font-size:smal=
l"><br></div><div><div dir=3D"ltr" class=3D"gmail_signature" data-smartmail=
=3D"gmail_signature"><div dir=3D"ltr"><div><div dir=3D"ltr"><div><div dir=
=3D"ltr"><div><div dir=3D"ltr"><div><div dir=3D"ltr">Andy<div><span style=
=3D"font-size:12.8px"><a href=3D"http://www.g4jnt.com" target=3D"_blank">ww=
w.g4jnt.com</a></span><br></div><div><br></div></div></div></div></div></di=
v></div></div></div></div></div></div><br></div><br><div class=3D"gmail_quo=
te"><div dir=3D"ltr" class=3D"gmail_attr">On Tue, 26 Feb 2019 at 19:23, N1B=
UG &lt;<a href=3D"mailto:paul@n1bug.com">paul@n1bug.com</a>&gt; wrote:<br><=
/div><blockquote class=3D"gmail_quote" style=3D"margin:0px 0px 0px 0.8ex;bo=
rder-left:1px solid rgb(204,204,204);padding-left:1ex">Jay,<br>
<br>
The U3S schematic is in the assembly manual:<br>
<br>
<a href=3D"http://qrp-labs.com/images/ultimate3s/assembly_u3s_r3_lt.pdf" re=
l=3D"noreferrer" target=3D"_blank">http://qrp-labs.com/images/ultimate3s/as=
sembly_u3s_r3_lt.pdf</a><br>
<br>
73,<br>
Paul<br>
<br>
<br>
On 2/26/19 2:12 PM, <a href=3D"mailto:jrusgrove@comcast.net" target=3D"_bla=
nk">jrusgrove@comcast.net</a> wrote:<br>
&gt; Anyone have a U3S schematic handy? Link to same?<br>
&gt; <br>
&gt; Jay W1VD<br>
&gt; <br>
&gt; ----- Original Message ----- <br>
&gt; From: &quot;N1BUG&quot; &lt;<a href=3D"mailto:paul@n1bug.com" target=
=3D"_blank">paul@n1bug.com</a>&gt;<br>
&gt; To: &lt;<a href=3D"mailto:rsgb_lf_group@blacksheep.org" target=3D"_bla=
nk">rsgb_lf_group@blacksheep.org</a>&gt;<br>
&gt; Sent: Tuesday, February 26, 2019 2:01 PM<br>
&gt; Subject: Re: LF: Class D current spikes<br>
&gt; <br>
&gt; <br>
&gt;&gt; Eric,<br>
&gt;&gt;<br>
&gt;&gt; I I have always run my U3S through the W1VD doubler. Never had any=
<br>
&gt;&gt; problems with blown FETs with that setup, even when I tested at 1 =
kW<br>
&gt;&gt; under Part 5 license. There is apparently something different abou=
t<br>
&gt;&gt; the U3S at end of RF envelope.<br>
&gt;&gt;<br>
&gt;&gt; 73,<br>
&gt;&gt; Paul<br>
&gt;&gt;<br>
&gt;&gt;<br>
&gt;&gt; On 2/26/19 12:52 PM, Chris Wilson wrote:<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt; Hello Eric,<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt; No,=C2=A0 I have always run the U3S in X2 mode as far as I can=
 remember. No<br>
&gt;&gt;&gt; doubler,=C2=A0 no squarer, just straight out of CLK0 to Pin 3 =
of the 74F74.<br>
&gt;&gt;&gt; And=C2=A0 no=C2=A0 issues=C2=A0 at all. Thanks. BTW, I really =
admire your old gear on<br>
&gt;&gt;&gt; your web site, awesome build standards and so nice to look at!=
<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt; Tuesday, February 26, 2019, 5:35:10 PM, you wrote:<br>
&gt;&gt;&gt;<br>
&gt;&gt;&gt;&gt; Just to clarify... did you say previously that the U3S als=
o worked fine<br>
&gt;&gt;&gt;&gt; running at 1x and feeding a doubler, squarer, etc. also?<b=
r>
<br>
</blockquote></div>

--000000000000225c730582d108bd--

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References: <942860C848184BA2A0A9103E0EE56DF7@DELL4>
 <1UTEEgOcyQ.DAejAuRZtn9@optiplex980-pc>
 <92784b07-a799-fb4e-9080-e1e8bb167b75@n1bug.com>
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 <3062ef19-bb69-3187-e8db-6a6bf5050739@n1bug.com>
 <234098919.20190226111836@gmail.com>
 <c7ee7c98-78c6-3d45-92a0-5a2c4e700d60@no3m.net>
 <0a79de5c-3274-caae-c000-d5f49bb44540@no3m.net>
 <21240445.20190226160950@gmail.com>
 <57e33c0d-6904-9010-a1c8-69b80f474068@no3m.net>
 <1191469216.20190226175207@gmail.com>
 <edd9cdbe-494a-da9a-f15c-b0d63fe0040c@n1bug.com>
 <823BBA7099F84CE9924D2D9E7E379C05@DELL4>
From: N1BUG <paul@n1bug.com>
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Update:

U3S schematic

http://qrp-labs.com/images/ultimate3s/assembly_u3s_r3_lt.pdf

U3S Synthesizer module schematic

http://qrp-labs.com/images/synth/synth_assembly4.pdf

My U3S has the low pass filter installed, so it is CLK0 of he
Si5351A > BS170 FET > LPF > W1VD doubler, amplifier.

Paul


On 2/26/19 2:12 PM, jrusgrove@comcast.net wrote:
> Anyone have a U3S schematic handy? Link to same?
> 
> Jay W1VD
> 
> ----- Original Message ----- 
> From: "N1BUG" <paul@n1bug.com>
> To: <rsgb_lf_group@blacksheep.org>
> Sent: Tuesday, February 26, 2019 2:01 PM
> Subject: Re: LF: Class D current spikes
> 
> 
>> Eric,
>>
>> I I have always run my U3S through the W1VD doubler. Never had any
>> problems with blown FETs with that setup, even when I tested at 1 kW
>> under Part 5 license. There is apparently something different about
>> the U3S at end of RF envelope.
>>
>> 73,
>> Paul
>>
>>
>> On 2/26/19 12:52 PM, Chris Wilson wrote:
>>>
>>>
>>> Hello Eric,
>>>
>>> No,  I have always run the U3S in X2 mode as far as I can remember. No
>>> doubler,  no squarer, just straight out of CLK0 to Pin 3 of the 74F74.
>>> And  no  issues  at all. Thanks. BTW, I really admire your old gear on
>>> your web site, awesome build standards and so nice to look at!
>>>
>>> Tuesday, February 26, 2019, 5:35:10 PM, you wrote:
>>>
>>>> Just to clarify... did you say previously that the U3S also worked fine
>>>> running at 1x and feeding a doubler, squarer, etc. also?
>>
> 
> 

-- 
Paul
N1BUG  2200m-2m        DXCC Honor Roll
FN55mf      ME      Piscataquis County
http://www.n1bug.com
http://www.aurorasentry.com

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Date: Wed, 27 Feb 2019 01:16:16 +0100
Message-ID: <CAC+C6w4vGhOm8tu6TmMsR4WEwRQO+ffHVccQcXV9pL-R2Ska-g@mail.gmail.com>
Subject: LF: 6th april 2019 : gps week rollover
To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
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 Content preview:  The GPS Week Number parameter is a ten-bit value in the range
    0-1023, repeating every 1024 weeks. Every gps converts the week number in
    UTC date. Week 0 started at 00:00:00 UTC on Sunday, 6th January [...] 
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--000000000000c7adc40582d51506
Content-Type: text/plain; charset="UTF-8"

The GPS Week Number parameter is a ten-bit value in the range 0-1023,
repeating every 1024 weeks. Every gps converts the week number in UTC date.
Week 0 started at 00:00:00 UTC on Sunday, 6th January 1980, so the week
number 'rolled over' from 1023 to 0 at 23:59:47 UTC on Saturday, 21st
August 1999.
This week number rollover will occur again now on the 6th April 2019.
For sure, many of the old gps models, after the reset, will report a wrong
date.
BTW 1pps or 10 kHz references should be accurate as usual.

A new neo8 gps has been already ordered to replace the ancient Jupiter gps
wich actually synchronize my EbNaut linux pc clock by means of its 'binary
protocol' strings and 1pps via the programs 'gpsd' and 'chrony'.

In the industrial world, this rollover will cause certainly many issues. My
jupiter, for istance, comes from a old ship's AIS (automatic identification
system). This mandatory transponder is a safety equipment onboard that
communicates, via a VHF link, the own ship position and receives the
position of the other ships in the range. Many of old transponders equipped
with the same Jupiter gps , are still operational onboard, so for these
installations there will be a problem at least in showing the correct date
of the reports, but more serious failures could be observed.

73, Domenico IZ7SLZ

--000000000000c7adc40582d51506
Content-Type: text/html; charset="UTF-8"
Content-Transfer-Encoding: quoted-printable

<div style=3D"white-space:pre-wrap"><br>=C2=A0<br>=C2=A0<br>The GPS Week Nu=
mber parameter is a ten-bit value in the range 0-1023, repeating every 1024=
 weeks. Every gps converts the week number in UTC date. Week 0 started at 0=
0:00:00 UTC on Sunday, 6th January 1980, so the week number &#39;rolled ove=
r&#39; from 1023 to 0 at 23:59:47 UTC on Saturday, 21st August 1999. <br>Th=
is week number rollover will occur again now on the 6th April 2019.<br>For =
sure, many of the old gps models,  after the reset,  will report a wrong da=
te.<br>BTW  1pps or 10 kHz references should be accurate as usual.<br><br>A=
 new neo8 gps has been already ordered to replace the ancient Jupiter gps w=
ich  actually synchronize my EbNaut linux pc clock by means of its &#39;bin=
ary protocol&#39; strings and 1pps via the programs &#39;gpsd&#39; and &#39=
;chrony&#39;.<br><br>In the industrial world,  this rollover will cause cer=
tainly many issues. My  jupiter, for istance, comes from a old ship&#39;s A=
IS (automatic identification system). This mandatory transponder is a safet=
y equipment onboard  that communicates, via a VHF link,  the own ship posit=
ion and receives the position of the other ships in the range. Many of old =
transponders equipped with the same Jupiter gps , are still operational onb=
oard, so for these installations there will be a problem at least in showin=
g the correct date of the reports, but more serious failures could be obser=
ved.<br><br>73, Domenico IZ7SLZ<br><br><br><br><br><br><br></div>

--000000000000c7adc40582d51506--

From owner-rsgb_lf_group@blacksheep.org  Wed Feb 27 22:58:27 2019
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 Content preview:  Thanks to the the archives kindly donated by Dave G3YXM and
    Markus DF6NM we now have an archive of 20 years of radioamateur longwave
   history at the klubnl.pl site: https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/
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Subject: Re: LF: LF Reflector archive
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Thanks to the the archives kindly donated by Dave G3YXM and Markus DF6NM 
we now have an archive of 20 years of radioamateur longwave history at the 
klubnl.pl site:

https://klubnl.pl/rsgb_lf_group-archives/html/rsgb_lf_group/

Article about it here:
https://klubnl.pl/wpr/en/index.php/2019/02/27/rsgb_lf_group-complete-archive/

VY 73

Jacek / SQ5BPF


On Sun, 3 Feb 2019, DAVE PICK wrote:

> Date: Sun, 3 Feb 2019 18:06:41 +0000 (GMT)
> From: DAVE PICK <daveyxm@virginmedia.com>
> Reply-To: rsgb_lf_group@blacksheep.org
> To: rsgb_lf_group@blacksheep.org, Jacek Lipkowski <sq5bpf@lipkowski.org>
> Subject: LF: LF Reflector archive
> 
> 
> Jacek
> 
> 
> I have an archive of the LF reflector from 1999 to early 2006. It's in a Thunderbird
> archive folder which is readable by Thunderbird if you have it. I don't know how to
> convert the emails into the format you asked for in bulk and I'm certainly not going to
> do them one by one! If it's any use I'll send you a link to it. It's about 126MB.
> 
> I may find some more if I keep looking!
> 
> 73
> 
> Dave G3YXM
> 
> 
> 
>

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Date: Wed, 27 Feb 2019 23:11:06 +0000
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 Content preview:  Hello Jacek, Well done all, a VERY useful archive indeed,
   thank you! -- Best regards, Chris mailto:dead.fets@gmail.com 
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Hello Jacek,

Well done all, a VERY useful archive indeed, thank you!



-- 
Best regards,
 Chris                            mailto:dead.fets@gmail.com


From owner-rsgb_lf_group@blacksheep.org  Thu Feb 28 22:08:40 2019
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Date: Thu, 28 Feb 2019 21:42:55 +0100
From: DK7FC <selberdenken@posteo.de>
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To: "rsgb_lf_group@blacksheep.org" <rsgb_lf_group@blacksheep.org>
Subject: VLF: DJ8WX (?)
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 Content preview:  Looks like there was a good trace of DJ8WX today on 8269.996
    Hz today. A purple trace on my RDF spectrogram. Nice to see some continuous
    activity there. The signal would be good enough for some EbNaut [...] 
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Looks like there was a good trace of DJ8WX today on 8269.996 Hz today. A 
purple trace on my RDF spectrogram.
Nice to see some continuous activity there. The signal would be good 
enough for some EbNaut as well.

73, Stefan