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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
Return-Path: <owner-rsgb_lf_group@blacksheep.org>
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From: "cesare tagliabue" <cestag@dada.it>
To: rsgb_lf_group@blacksheep.org
References: <000c01c2a79b$175dfc00$53e4fc3e@l8p8y6> <002f01c2a7a2$18434ec0$28676ec3@cestag> <000b01c2c93b$6d8ce980$0bc828c3@erica>
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        Hello Peter
        Obviously you can use my web page as source of informations about my
antennas, I'll search in my PC for any possible further useful pictures or
schematics, may be there are some high resolution images, I'll send what I
find as soon as possible. Best 73 for now  Cesare

Cesare Tagliabue   I 5 TGC
WW-Loc  JN53PS
e-mail: cestag@dada.it
url: http://dai5tgc.dadacasa.supereva.it

-----Messaggio Originale-----
Da: "g3ldo" <g3ldo@ukonline.co.uk>
A: <rsgb_lf_group@blacksheep.org>
Data invio: venerdì 31 gennaio 2003 16.11
Oggetto: LF: Re: R: I5TGC


> Hello Cesare
>
> I write a column each month for the RSGB magazine, RadCom, called
> 'Antennas'.  I often get letters from readers who ask 'what is the best
> commercial antenna to use if you have only a small garden or no garden at
> all and talk about the impossability of operating on the lower frequency
> bands from such a QTH.
> I would like to describe your lower frequency antennas as an example of
what
> can be done to overcome these difficulties.
> I would like to use the description from your web page (or any other
> information that you might have). Do you have some higher resolution
images
> that could be used. In general a .JPG image needs to be over 100k in size
to
> be reproduced in a magazine.
>
> Many thanks
>
>
> Peter, G3LDO
>
> e-mail <g3ldo@ukonline.co.uk>
>
> Web <http://web.ukonline.co.uk/g3ldo>
>
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "dj9dw" <dj9dw@t-online.de>
To: rsgb_lf_group@blacksheep.org
Date: Fri, 31 Jan 2003 20:12:38 +0100
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	charset="Windows-1252"
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Hello LF-Group,
is there any formula to calculate a basket weave coil ( to load my =
marconi in spe) ?
Suppose 3 mH will be handy.
73, dj9dw, Peter.


------=_NextPart_000_000F_01C2C965.1A3F6F80
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	charset="Windows-1252"
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=3DContent-Type content=3D"text/html; =
charset=3Dwindows-1252">
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=3D#ffffff>
<DIV><FONT face=3DArial size=3D2>Hello LF-Group,</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>is there any formula to calculate a =
basket weave=20
coil&nbsp;( to load my marconi in spe) ?</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>Suppose 3 mH will be =
handy.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2>73, dj9dw, Peter.</FONT></DIV>
<DIV><FONT face=3DArial size=3D2></FONT>&nbsp;</DIV></BODY></HTML>

------=_NextPart_000_000F_01C2C965.1A3F6F80--





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <002101c2c94e$8efe7cb0$1b00a8c0@dellboy>
From: "Dave Pick" <g3yxm@wireless.org.uk>
To: rsgb_lf_group@blacksheep.org
References: <2D280BB697C7EE4C979C5C89925418EFB05AB6@TNS-FBU-2E-003.corp.telenor.no>
Date: Fri, 31 Jan 2003 17:31:13 -0000
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gifs are smaller for areas of solid colour, like diagrams. Jpegs are smaller
for photos.

Dave G3YXM
----- Original Message -----
From: <jan-martin.noding@telenor.com>
To: <rsgb_lf_group@blacksheep.org>
Cc: <la8ak@online.no>
Sent: Friday, January 31, 2003 4:30 PM
Subject: LF: RE: Re: R: I5TGC


well,

gif type files are smaller, don't really understand why it should be jpg?

73,
Jan-Martin
---
J M Nøding, Kristiansand



-----Original Message-----
From: g3ldo [mailto:g3ldo@ukonline.co.uk]
Sent: 31. januar 2003 16:11
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: R: I5TGC


Hello Cesare

I write a column each month for the RSGB magazine, RadCom, called
'Antennas'.  I often get letters from readers who ask 'what is the best
commercial antenna to use if you have only a small garden or no garden at
all and talk about the impossability of operating on the lower frequency
bands from such a QTH.
I would like to describe your lower frequency antennas as an example of what
can be done to overcome these difficulties.
I would like to use the description from your web page (or any other
information that you might have). Do you have some higher resolution images
that could be used. In general a .JPG image needs to be over 100k in size to
be reproduced in a magazine.

Many thanks


Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: jan-martin.noding@telenor.com
To: rsgb_lf_group@blacksheep.org
Cc: la8ak@online.no
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Subject: LF: RE: Re: R: I5TGC
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This is a multi-part message in MIME format.
--------------060203000909060509070307
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well, 

gif type files are smaller, don't really understand why it should be jpg?

73,
Jan-Martin
---
J M Nøding, Kristiansand



-----Original Message-----
From: g3ldo [mailto:g3ldo@ukonline.co.uk]
Sent: 31. januar 2003 16:11
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: R: I5TGC


Hello Cesare

I write a column each month for the RSGB magazine, RadCom, called
'Antennas'.  I often get letters from readers who ask 'what is the best
commercial antenna to use if you have only a small garden or no garden at
all and talk about the impossability of operating on the lower frequency
bands from such a QTH.
I would like to describe your lower frequency antennas as an example of what
can be done to overcome these difficulties.
I would like to use the description from your web page (or any other
information that you might have). Do you have some higher resolution images
that could be used. In general a .JPG image needs to be over 100k in size to
be reproduced in a magazine.

Many thanks


Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 31 Jan 2003 16:18:38 +0100
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
From: "Dick Rollema" <d.w.rollema@freeler.nl>
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Subject: LF: Magazine articles on LF
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<html>
<b>To All from PA0SE<br><br>
<i>Practical Wireless</i> of January 2003 contains the following
article:<br><br>
&quot;Rugby Radio - Serving Britain For 75 Years&quot;, by Stan Brown,
G4LU.<br><br>
In <i>RadCom </i>of February 2003 you will find:<br><br>
&quot;A Class-D Transmitter for 136kHz&quot;; The concluding part of the
300W design by David Bowman, G0MRF.<br><br>
73, Dick, PA0SE <br><br>
</b></html>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <000c01c2a79b$175dfc00$53e4fc3e@l8p8y6> <002f01c2a7a2$18434ec0$28676ec3@cestag>
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Hello Cesare

I write a column each month for the RSGB magazine, RadCom, called
'Antennas'.  I often get letters from readers who ask 'what is the best
commercial antenna to use if you have only a small garden or no garden at
all and talk about the impossability of operating on the lower frequency
bands from such a QTH.
I would like to describe your lower frequency antennas as an example of what
can be done to overcome these difficulties.
I would like to use the description from your web page (or any other
information that you might have). Do you have some higher resolution images
that could be used. In general a .JPG image needs to be over 100k in size to
be reproduced in a magazine.

Many thanks


Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John W Gould" <g3wkl@btinternet.com>
To: rsgb_lf_group@blacksheep.org
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Subject: LF: RE: Re: IARU Region 1 position on 500kHz
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Arnie, nice to hear from you again and your comments on 500kHz are welcome.
I think that we all recognise that it's not yet quite the time to expect to
get an allocation at this part of the spectrum, however, that shouldn't
cause us not to prepare and see if there are some small areas where we might
gain some sort of agreement to undertake some experiments. I think we all
agree that it would prove an interesting frequency between 1.8MHz and
136kHz.

Re. you interest in trying to secure a 136kHz allocation prior to WRC03.  I
should be in the position to help you with information of which Region 1
countries have implemented CEPT/ERC Recommendation 62-01 E (Mainz 1997),
however, I don't have a complete list. I have posted this reply to the
reflector in the hope that someone on the reflector can help us by providing
a list or pointing to a URL.  The other point that I would stress is that
the IARU Region 1 discussion on 500kHz made it quite clear that they would
not want to press for anything at 500kHz prior or at WRC03; the IARU will
only consider the 500kHz Working Group's recommendations after WRC03.

I have note your interest in receiving status/updates of the Working Group's
activity, which I am sure will not be a problem.

73 John, G3WKL



> -----Original Message-----
> From: owner-rsgb_lf_group@blacksheep.org
> [mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of Prof. Arnaldo
> Coro Antich
> Sent: Wednesday, January 29, 2003 13:27
> To: rsgb_lf_group@blacksheep.org
> Cc: John W Gould
> Subject: LF: Re: IARU Region 1 position on 500kHz
>
>
> Dear John:
> We have heard about similar interests related to an allocation around 500
> kHz. But I must advise that many Third World nations are still using that
> segment of the spectrum for maritime communications.
> Recent efforts to try to obtain a 600 meters band assignment by
> amateurs in
> neighboring countries came to a standstill when their telecommunications
> administrations replied that this was not possible because the segment was
> still in use for maritime communications.
> It would be very interesting and useful to have access to any
> documentation
> that Region I and Region III IARU coordinators may have, in order to
> approach our telecommunications administration regarding the preparations
> for the upcoming WARC 2003 to take place in Geneva later this year.
> I believe that one solid argument backing the request would be
> the succesful
> use of the 136 kiloHertz band by amateurs in many different countries, and
> along that line, I would like to request information regarding
> the number of
> countries in Region I already authorized to operate on 136
> kiloHertz at this
> moment.
> We Cuban amateurs are trying to obtain our 136 kiloHertz band before WARC
> 2003 takes place, and would like to have the 600 meters assignment too !!!
> My personal experience participating at ITU conferences is that
> this efforts
> require great coordination and to be worked well in advance of the actual
> WARC 2003....
> 73 and DX
> YOur friend in Havana
> CO2KK
>
> ----- Original Message -----
> From: "John W Gould" <g3wkl@btinternet.com>
> To: "Rsgb_Lf_Group@Blacksheep.Org" <rsgb_lf_group@blacksheep.org>
> Cc: "HF. Chairman List Member" <Colin.Thomas@rsgb.org.uk>; "Vk4du@Gmdss.
> Com. Au" <vk4du@gmdss.com.au>
> Sent: Wednesday, January 29, 2003 3:24 AM
> Subject: LF: IARU Region 1 position on 500kHz
>
>
> > My apologies for not bringing to this group's attention before
> the outcome
> > of a discussion of the RSGB paper on 500kHz, at the San Marino Region 1
> > Conference.  AMRAD have usefully summarised the position with the
> following
> > in their Jan-Feb 2003 Newsletter, which I quote with their agreement:
> >
> > "G3PSM chaired a working group of ON7ZV, PA0SHY, PA0AWN, ZL2AMJ
> and G4OUT.
> > The result was the adoption of Recommendation REC/02/SMC4.11,
> as follows:
> >
> > A Working Group would be formed to investigate the possibility of a
> > frequency allocation of approximately 10kHz between 470-490kHz to
> > investigate propagation and the use of new communication
> technologies.  A
> > progress report should be circulated to the secretaries of Region 2 and
> > Region 3 for information."
> >
> > I would add to that statement a comment to me from Colin, G3PSM on his
> > return that we should be looking in a post-WRC2003 timeframe to
> come back
> > with proposals in relation to this part of the spectrum, thus this is a
> > long-term issue.
> >
> > As IARU Region 1 LF Coordinator I have assumed some responsibility for
> > forming a "500kHz Working Group" and have approached a few
> people to lead
> > such a group.  This has been without success, so I put the
> question to the
> > LF Group - Can I have volunteers please to work in a group, using e-mail
> and
> > a dedicated website, to carry out the task detailed by the above IARU
> Region
> > 1 recommendation. Once a group has been formed it can choose its
> > chairperson. I would like to see an international membership of
> the Group,
> > hence the need to conduct business over the Internet.  Meeting together
> > would be expensive and probably difficult to arrange. Volunteers should
> > e-mail me directly rather than post to the reflector.
> >
> > This e-mail has been copied to Colin, G3PSM and also Glenn, VK4DU (for
> > Region 3).
> >
> > 73 John, G3WKL
> > g3wkl@btinternet.com
> >
> >
> >
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Prof. Arnaldo Coro Antich" <inforhc@ip.etecsa.cu>
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Cc: "John W Gould" <g3wkl@btinternet.com>
References: <LOBBIDNOENMNHIBGDCKBCEKBDGAA.g3wkl@btinternet.com>
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Dear John:
We have heard about similar interests related to an allocation around 500
kHz. But I must advise that many Third World nations are still using that
segment of the spectrum for maritime communications.
Recent efforts to try to obtain a 600 meters band assignment by amateurs in
neighboring countries came to a standstill when their telecommunications
administrations replied that this was not possible because the segment was
still in use for maritime communications.
It would be very interesting and useful to have access to any documentation
that Region I and Region III IARU coordinators may have, in order to
approach our telecommunications administration regarding the preparations
for the upcoming WARC 2003 to take place in Geneva later this year.
I believe that one solid argument backing the request would be the succesful
use of the 136 kiloHertz band by amateurs in many different countries, and
along that line, I would like to request information regarding the number of
countries in Region I already authorized to operate on 136 kiloHertz at this
moment.
We Cuban amateurs are trying to obtain our 136 kiloHertz band before WARC
2003 takes place, and would like to have the 600 meters assignment too !!!
My personal experience participating at ITU conferences is that this efforts
require great coordination and to be worked well in advance of the actual
WARC 2003....
73 and DX
YOur friend in Havana
CO2KK

----- Original Message -----
From: "John W Gould" <g3wkl@btinternet.com>
To: "Rsgb_Lf_Group@Blacksheep.Org" <rsgb_lf_group@blacksheep.org>
Cc: "HF. Chairman List Member" <Colin.Thomas@rsgb.org.uk>; "Vk4du@Gmdss.
Com. Au" <vk4du@gmdss.com.au>
Sent: Wednesday, January 29, 2003 3:24 AM
Subject: LF: IARU Region 1 position on 500kHz


> My apologies for not bringing to this group's attention before the outcome
> of a discussion of the RSGB paper on 500kHz, at the San Marino Region 1
> Conference.  AMRAD have usefully summarised the position with the
following
> in their Jan-Feb 2003 Newsletter, which I quote with their agreement:
>
> "G3PSM chaired a working group of ON7ZV, PA0SHY, PA0AWN, ZL2AMJ and G4OUT.
> The result was the adoption of Recommendation REC/02/SMC4.11, as follows:
>
> A Working Group would be formed to investigate the possibility of a
> frequency allocation of approximately 10kHz between 470-490kHz to
> investigate propagation and the use of new communication technologies.  A
> progress report should be circulated to the secretaries of Region 2 and
> Region 3 for information."
>
> I would add to that statement a comment to me from Colin, G3PSM on his
> return that we should be looking in a post-WRC2003 timeframe to come back
> with proposals in relation to this part of the spectrum, thus this is a
> long-term issue.
>
> As IARU Region 1 LF Coordinator I have assumed some responsibility for
> forming a "500kHz Working Group" and have approached a few people to lead
> such a group.  This has been without success, so I put the question to the
> LF Group - Can I have volunteers please to work in a group, using e-mail
and
> a dedicated website, to carry out the task detailed by the above IARU
Region
> 1 recommendation. Once a group has been formed it can choose its
> chairperson. I would like to see an international membership of the Group,
> hence the need to conduct business over the Internet.  Meeting together
> would be expensive and probably difficult to arrange. Volunteers should
> e-mail me directly rather than post to the reflector.
>
> This e-mail has been copied to Colin, G3PSM and also Glenn, VK4DU (for
> Region 3).
>
> 73 John, G3WKL
> g3wkl@btinternet.com
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John W Gould" <g3wkl@btinternet.com>
To: "Rsgb_Lf_Group@Blacksheep.Org" <rsgb_lf_group@blacksheep.org>
Cc: "HF. Chairman List Member" <Colin.Thomas@rsgb.org.uk>, 
 "Vk4du@Gmdss. Com. Au" <vk4du@gmdss.com.au>
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My apologies for not bringing to this group's attention before the outcome
of a discussion of the RSGB paper on 500kHz, at the San Marino Region 1
Conference.  AMRAD have usefully summarised the position with the following
in their Jan-Feb 2003 Newsletter, which I quote with their agreement:

"G3PSM chaired a working group of ON7ZV, PA0SHY, PA0AWN, ZL2AMJ and G4OUT.
The result was the adoption of Recommendation REC/02/SMC4.11, as follows:

A Working Group would be formed to investigate the possibility of a
frequency allocation of approximately 10kHz between 470-490kHz to
investigate propagation and the use of new communication technologies.  A
progress report should be circulated to the secretaries of Region 2 and
Region 3 for information."

I would add to that statement a comment to me from Colin, G3PSM on his
return that we should be looking in a post-WRC2003 timeframe to come back
with proposals in relation to this part of the spectrum, thus this is a
long-term issue.

As IARU Region 1 LF Coordinator I have assumed some responsibility for
forming a "500kHz Working Group" and have approached a few people to lead
such a group.  This has been without success, so I put the question to the
LF Group - Can I have volunteers please to work in a group, using e-mail and
a dedicated website, to carry out the task detailed by the above IARU Region
1 recommendation. Once a group has been formed it can choose its
chairperson. I would like to see an international membership of the Group,
hence the need to conduct business over the Internet.  Meeting together
would be expensive and probably difficult to arrange. Volunteers should
e-mail me directly rather than post to the reflector.

This e-mail has been copied to Colin, G3PSM and also Glenn, VK4DU (for
Region 3).

73 John, G3WKL
g3wkl@btinternet.com




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Thread-Topic: Siemens D2006
Thread-Index: AcLG94yaFO4I7TLOSQ+gfMIb1DYnkgAG+mLQ
From: jan-martin.noding@telenor.com
To: rsgb_lf_group@blacksheep.org
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Hi 'LF-Group'!

Could scan some pages if you know what you are after, but have so much demand for 
copies of Racal and other receivers that I can't overcome. For the DIN-socket it not
much to find, only an overview which tells the colour of the wire from one board to the
SKT.

Think it is a problem with manuals because too often people request copies, and later
throw it in the bin and sell the equipment, but tell the next person where they believe
they could get the manual from, so I would like better to pass the material to 
somebody like K4XL Kenneth who runs a site for manuals, in this case it is for boatanchors...

73
Jan-Martin

PS. never really understand why somebody don't require the handbooks for their equipment
---
J M Noeding LA8AK, Kristiansand *** mailto:la8ak@online.no ***


-----Opprinnelig melding-----
Fra: James Moritz [mailto:j.r.moritz@herts.ac.uk]
Sendt: 28. januar 2003 18:48
Til: rsgb_lf_group@blacksheep.org
Emne: LF: Siemens D2006


Dear LF Group,

I recently acquired a Siemens D2006 selective voltmeter, with the 
accompanying W2006 generator. Does anybody have manuals or circuit diagrams 
for these units that I could borrow/copy etc? Naturally, I would be happy 
to cover any costs involved.

Cheers, Jim Moritz
73 de M0BMU





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Dear LF Group,

I recently acquired a Siemens D2006 selective voltmeter, with the 
accompanying W2006 generator. Does anybody have manuals or circuit diagrams 
for these units that I could borrow/copy etc? Naturally, I would be happy 
to cover any costs involved.

Cheers, Jim Moritz
73 de M0BMU




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Group,
Like many just starting out with LF, I'm using an audio amplifier to
transmit with.
I had a bit of a surprise when tinkering about with it.
I had connected a loudspeaker to the output and put a 1kHz signal through as
a confidence check, that the amp was working ok.

Afterwards I reconnected the antenna, before removing the loudspeaker. As I
did so there was a horrible hum - well buzz really, since I have reduced the
size of coupling capacitors to give it less gain at low frequencies.

It didn't take long to realise that there was a big earth loop. The signal
source is referenced to mains earth, and when I connected the aerial (and
earth) the amplifier was also connected to RF earth.
I have cured the problem by introducing a transformer between the signal
source and the amplifier, but I wouldn't have realised that the amplifier
was trying to amplify both 136kHz and huge amounts of 50Hz at the same time.
If I had a (working) oscilloscope, I would probably have spotted the problem
earlier, but it's not something that I expected.

I did make me wonder whether hum had a bearing on the mysterious FET and
fuse blowing problems with the BK amplifiers - but I expect large amounts of
hum would have been quickly noticed when the problem was investigated.

73
Hugh M0WYE







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Seems TEA6200 is an interesting device for making the field strength meter, 
somewhat different from PAøSE Dick's, but I believe it could be easy. 
Hope to get some samples for test. TEA6200 has a highlevel mixer and 
intended to upconvert the VLF signal, a simple xtal filter could easily be 
made on 3.58, 4.43361875, 8.667, or other frequencies for cheap xtals

73 
Jan-Martin
LA8AK
----- Original Message ----- 
From: "VLAD" <kb9olm@yahoo.com>
To: "J M Noeding" <la8ak@online.no>
Sent: Friday, June 28, 2002 4:47 PM
Subject: TEA6200


> Hi JM,
> 
> Have you used this IC: TEA6200 from Philips?
> 
> http://www-us9.semiconductors.com/acrobat/datasheets/TEA6200_CNV_2.pdf
> 
> Looks good for ham Rx.
> 
> vlad
> kb9olm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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I think that most of you know that I have to fold my antenna mast over
during the day because of planning restrictions. This means that I get to
transmit on LF a good deal less than I would like to. However I do listen on
136 using my loop. Today I heard OK1DTN tuning up with a big signal and then
calling CQ a few times. I couldn't resist the temptation to raise the mast
and give him a call. If you heard some strange CW coming from G3LDO this
morning the reeason is because when I came to plug in the electronic keyer I
found that its battery was flat so I used the QRSS system on 0.1 second
dots, a very cumbersom CW operating procedure. Nevertheless we did have a
QSO.
Worked G3XIZ and F6CNI late this afternoon.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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Dear Werner, LF Group,


At 19:52 25/01/2003 +0100, you wrote:
>At first sight it work FB
>Loop perimeter is 85 meters and 12 meters above ground
>Series coil is 1.5 mH series cap is home made butterfly 280 pf
>plate space is 20mm, current in the circuit is 3.5 Amp
>Cap and coil are in the shack , and two wires are going
>out through the wall widely spaced from the wall, and so
>straight to the loop .
>In the shack it smells like ozone Hi

You didn't say exactly how the tuning components and TX are connected to 
the loop - but it seems to me that if there is a significant voltage 
between the loop wire and ground, the antenna could actually be operating 
as a vertical tuned against ground. Obviously the antenna radiates quite 
well, but it is not clear that it is actually radiating in a horizontal 
loop mode - 3.5A seems a low current for a loop antenna to radiate much 
signal. The highest possible radiation resistance would occur if the loop 
were circular - in that case the area would be 575m^2, giving Rrad of 
0.44milliohms, and a very optimistic estimate of  ERP of maybe 10mW, 
assuming none is dissipated in the ground or environment.

I expect the loop will have an inductance between 100 - 200uH; If both the 
1.5mH coil and 280p capacitor are connected in series with one terminal of 
the loop, and the other terminal is near ground potential, the loop wire 
will be at a low potential (with 3.5A , some 100's of volts maximum), and 
there will be little radiation in "vertical" mode. But if this is the case, 
with total L of 1.7mH, and C of 280p, resonant frequency will be about 
230kHz or slightly more. If, on the other hand, the inductor is connected 
to one terminal of the loop, and the capacitor to the other, the whole loop 
wire will be at high potential, and there will be a large "displacement 
current" flowing to ground through the antenna capacitance, so one would 
expect the antenna to be operating primarily as a vertical. In this 
condition, the capacitance to ground of the loop wire would effectively be 
in parallel with the 280p tuning capacitance. Estimating this to be 6pF/m, 
85m of wire gives 510pF, so 790pF total capacitance. With 1.5mH 
inductance,  this gives a resonant frequency of 146kHz, much nearer 
reality! There will be additional capacitance due to the connections to the 
shack, which would bring the resonant frequency to 136k. In this condition, 
the voltage on the loop wire would be roughly 4.5kV, and the antenna would 
be predominantly acting as a vertical, giving roughly 300mW ERP, again 
assuming no environmental losses.

Cheers, Jim Moritz
73 de M0BMU





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From: "DE BONDT WERNER" <w.bondt@belgacom.net>
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META content="text/html; charset=iso-8859-1" http-equiv=Content-Type>
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<DIV><FONT face=Arial size=2>Hi all</FONT></DIV>
<DIV><FONT face=Arial size=2>Thanks for the reply on my loop.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>But wait to build a loop antenna Hi</FONT></DIV>
<DIV><FONT face=Arial size=2>Since I was not sure about my loop was a real 
loop.</FONT></DIV>
<DIV><FONT face=Arial size=2>Because de junction&nbsp; 
coil-capacitor&nbsp;&nbsp; was still grounded .</FONT></DIV>
<DIV><FONT face=Arial size=2>I made averting floating, and coupled the TX by a 
link.</FONT></DIV>
<DIV><FONT face=Arial size=2>So averting was disconnected from the ground 
now.</FONT></DIV>
<DIV><FONT face=Arial size=2>The configuration is now.</FONT></DIV>
<DIV><FONT face=Arial size=2>One end from the loop to the coil--from the coil to 
capacitor</FONT></DIV>
<DIV><FONT face=Arial size=2>than via the Amp meter to other end of the loop, 
and power in the</FONT></DIV>
<DIV><FONT face=Arial size=2>coil via the link.</FONT></DIV>
<DIV><FONT face=Arial size=2>Now I could only drive with abt 75 Watts, because 
of arcing in the cap</FONT></DIV>
<DIV><FONT face=Arial size=2>but still 3,5 Amp in the circuit .</FONT></DIV>
<DIV><FONT face=Arial size=2>Now big flames all over but no QSO&nbsp;. So Loops 
still on the side .</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Close but no cigar , keep on trying</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 Werner ON6ND</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>To day I hear many times a test carrier more ore 
less strong ,</FONT></DIV>
<DIV><FONT face=Arial size=2>pleas attach a 
call-singe</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Regarding ON4ND's horizontal loop Alan G3NYK said:

> . My estimation is that he was about 2 S points
> down on the strength I normally hear him. Thus 559 against his usual 579
on
> the vertical. This report seems to be confirmed by Dave G3YXMs comments.

The EZNEC model gave it about -40dBi in free space. Above ground it was
worse at -50dBi, - so bad that I suspected the model.
80m of wire 12m high is a lot of wire in the air. If configured as a Marconi
we get -30dBi even with poor ground.

> To Peter
> A take off at 45 degrees is not actually too clever, as it then puts the
> signal back down again just 100kms further on !! (Check the geometry with
a
> 50km reflecting D-Layer.) In fact it is likely to give fading in the 300
to
> 400kms region. The fact that there was no sign (as far as I could tell) of
> fading on Werner suggests that the high angle radiation was just totally
> lost in absorption in the D-layer. To use "skywave" effectively one has to
> "aim" at the horizon. (see the Simple Geometry page on my web site) as
only
> grazing incidence waves are returned in daytime.

Yes Alan, you are right. In fact the marconi antenna over poor ground has a
maximum gain elevation angle of 15 degrees. Over good ground it is 12
degrees with the above antenna having a gain of -24dBi. These figures do not
take into account electromagnetic obstructions or other enviomental
absorbsion.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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Is this an inductively loaded DDRR antenna? 

Mike, G3XDV
http://www.lf.thersgb.net
=================


-----------------------------------
Just made a test with a horizontal loop antenna
and made QSO with F6BWO--F6CNI--DL3FDO
At first sight it work FB
Loop perimeter is 85 meters and 12 meters above ground
Series coil is 1.5 mH series cap is home made butterfly 280 pf
plate space is 20mm, current in the circuit is 3.5 Amp
Cap and coil are in the shack , and two wires are going 
out through the wall widely spaced from the wall, and so
straight to the loop .
73 Werner ON6ND





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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi all, I have already replied direct to Werner. I heard his transmissions
today and as he is a regular and almost a "local" to me was able to give at
least an "audible" report. My estimation is that he was about 2 S points
down on the strength I normally hear him. Thus 559 against his usual 579 on
the vertical. This report seems to be confirmed by Dave G3YXMs comments.

To Peter
A take off at 45 degrees is not actually too clever, as it then puts the
signal back down again just 100kms further on !! (Check the geometry with a
50km reflecting D-Layer.) In fact it is likely to give fading in the 300 to
400kms region. The fact that there was no sign (as far as I could tell) of
fading on Werner suggests that the high angle radiation was just totally
lost in absorption in the D-layer. To use "skywave" effectively one has to
"aim" at the horizon. (see the Simple Geometry page on my web site) as only
grazing incidence waves are returned in daytime.

Still it nice to see someone has had the energy and bottle to try it!! Well
done Werner.
How about rotating it vertical next....and give us a warning so we can be
sure to be listening. It seemed very quiet today only 6 callsigns on my pad.
I think it is possible that LA1TN is listening this weekend so the is every
possibility of a report from Norway
(Trondheim I think).....but not if you dont transmit !!

Cheers de Alan G3NYK
alan.melia@btinternet.com





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Werner ON6ND said

----------------------------------------------
Just made a test with a horizontal loop antenna
and made QSO with F6BWO--F6CNI--DL3FDO
At first sight it work FB
Loop perimeter is 85 meters and 12 meters above ground
Series coil is 1.5 mH series cap is home made butterfly 280 pf
plate space is 20mm, current in the circuit is 3.5 Amp
Cap and coil are in the shack , and two wires are going
out through the wall widely spaced from the wall, and so
straight to the loop .
In the shack it smells like ozone Hi
---------------------------------------------
Interesting! Most loops tried in the past have been vertical because then
you only need two supporting masts. If this antenna is square or a rectangle
then you will need four.
I tried making an EZNEC model of this antenna but the results are not
reliable for two reasons: the antenna is an electrically small loop and it
is electrically very close to the ground. Even a free space model seemed
quite lossy (-40+dBi). For what its worth changing the quality of ground
material had little effect on a ground model; unlike a Marconi. The other
characteristic is that the greatest gain was at 45 degrees - good sky wave.
Not the sort of antenna a commercial station would use but it might be good
for amateur sky-wave DX.
Have the USA Lowfers tried this one out?

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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Dexter W4DEX said:

> I am now plotting DCF39's signal as received here in North Carolina.
> The plots are uploaded at ten minuets intervals.

Interesting to compare the signal strengths received by W4DEX with W3EEE.

Both plots are similar with signal dips around 0200z and 0400z although the
signal build up was later and the fade out earlier at W4DEX, as you might
expect. Well done the USA 'team' - will give us valuable LF propagation
data.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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Werner.

I heard your CQ, about 559. Sorry I was not able to transmit. I will look
out for you tomorrow.

73
Dave G3YXM.

----------------

Just made a test with a horizontal loop antenna
and made QSO with F6BWO--F6CNI--DL3FDO
At first sight it work FB





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<DIV><FONT face=Arial size=2>COOL!!!!!</FONT></DIV>
<BLOCKQUOTE dir=ltr 
style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV 
  style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
  <A title=w.bondt@belgacom.net href="mailto:w.bondt@belgacom.net">DE BONDT 
  WERNER</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A title=rsgb_lf_group@blacksheep.org 
  href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org</A> 
  </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Saturday, January 25, 2003 1:52 
  PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: TX with LOOP</DIV>
  <DIV><BR></DIV>
  <DIV><FONT face=Arial size=2>Hello All</FONT></DIV>
  <DIV>&nbsp;</DIV>
  <DIV><FONT face=Arial size=2>Just made a test with a horizontal loop 
  antenna</FONT></DIV>
  <DIV><FONT face=Arial size=2>and made QSO with 
  F6BWO--F6CNI--DL3FDO</FONT></DIV>
  <DIV><FONT face=Arial size=2>At first sight it work FB</FONT></DIV>
  <DIV><FONT face=Arial size=2>Loop perimeter is 85 meters and 12 meters above 
  ground</FONT></DIV>
  <DIV><FONT face=Arial size=2>Series coil is 1.5 mH series cap is home made 
  butterfly 280 pf</FONT></DIV>
  <DIV><FONT face=Arial size=2>plate space is 20mm, current in the circuit is 
  3.5 Amp</FONT></DIV>
  <DIV><FONT face=Arial size=2>Cap and coil are in the shack , and two wires are 
  going </FONT></DIV>
  <DIV><FONT face=Arial size=2>out through the wall widely spaced from the wall, 
  and so</FONT></DIV>
  <DIV><FONT face=Arial size=2>straight to the loop .</FONT></DIV>
  <DIV><FONT face=Arial size=2>In the shack it smells like ozone Hi</FONT></DIV>
  <DIV>&nbsp;</DIV>
  <DIV><FONT face=Arial size=2>More test later</FONT></DIV>
  <DIV><FONT face=Arial size=2>73 Werner 
ON6ND</FONT></DIV></BLOCKQUOTE></BODY></HTML>

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<DIV><FONT face=Arial size=2>Hello All</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Just made a test with a horizontal loop 
antenna</FONT></DIV>
<DIV><FONT face=Arial size=2>and made QSO with F6BWO--F6CNI--DL3FDO</FONT></DIV>
<DIV><FONT face=Arial size=2>At first sight it work FB</FONT></DIV>
<DIV><FONT face=Arial size=2>Loop perimeter is 85 meters and 12 meters above 
ground</FONT></DIV>
<DIV><FONT face=Arial size=2>Series coil is 1.5 mH series cap is home made 
butterfly 280 pf</FONT></DIV>
<DIV><FONT face=Arial size=2>plate space is 20mm, current in the circuit is 3.5 
Amp</FONT></DIV>
<DIV><FONT face=Arial size=2>Cap and coil are in the shack , and two wires are 
going </FONT></DIV>
<DIV><FONT face=Arial size=2>out through the wall widely spaced from the wall, 
and so</FONT></DIV>
<DIV><FONT face=Arial size=2>straight to the loop .</FONT></DIV>
<DIV><FONT face=Arial size=2>In the shack it smells like ozone Hi</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>More test later</FONT></DIV>
<DIV><FONT face=Arial size=2>73 Werner ON6ND</FONT></DIV></BODY></HTML>

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Subject: Re: LF: DCF39 protocol
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Alberto di Bene schrieb:
>   Good afternoon all,
>
>   may be this is old hat for some of you, but if you are interested in the
> protocol DCF39 uses for its signalling, go here :
> http://longwave.bei.t-online.de/Efr.pdf
>
> 73  Alberto  I2PHD
>
>
Hi Alberto,

tks for the hint. Klaus makes a good job of listing and describing 
lf stations, doesn`t he.

regards
Uwe/dj8wx





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Date: Fri, 24 Jan 2003 20:33:56 +0000
From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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Subject: LF: Plotting DCF39 in NC
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I am now plotting DCF39's signal as received here in North Carolina. 
The plots are uploaded at ten minuets intervals.  The latest plot can be
accessed from my main web page at:

http://www.w4dex.com/ 

Or go directly to the plot at:

http://www.w4dex.com/plot/dcf39/dcf39.gif

The daily plots will be stored in the directory:

http://www.w4dex.com/plot/dcf39/

These plots are in .gif format as suggested by Steve, W3EEE.  Looks good
to me and saves a little bandwidth.

Dexter



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Subject: Re: LF: AW: VFO for VLF receiver? Digital type pre-mixer, any  ideas?
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Dear Jan-Martin, LF group

At 11:37 24/01/2003 +0100, you wrote:
>Suppose I could use an FF, preferably CD4013 for the mixer.
>
>But I can't find any reference to similar constructions, only have a vague
>memory that it has been mentioned in TT some time in the last 35 years

A D-type flip-flop  does work something like a mixer. If you feed 1MHz into 
the clock input, and 1.001MHz square wave into the D input, the output will 
approximately be a 1kHz square wave. The interesting thing is that you will 
also get the 1kHz square wave if the D input is 0.001, 0.999, 1.999, 2.001, 
2.999, 3.001... nMHZ +/-1kHz. The D-type flip-flop effectively "samples" 
the logic level at the D input the moment the clock transition occurs - it 
works like a sample-and-hold with a square wave input, and no anti-aliasing 
filter (this analogue scheme is used in things like sampling scopes, 
modulation meters, vector voltmeters, etc., or optically with a 
stroboscope). The trouble is that, since it is effectively mixing the 
square wave input with a train of impulses at the clock frequency, and low 
pass filtering the result, the output spectrum contains many harmonic and 
non-harmonic components as well as the desired output. These are easy to 
filter out if the difference frequency is much smaller than either input 
frequency, but if you try to use the sum frequency output, or the output 
frequency is comparable to the input frequency, the output waveform is 
roughly a square wave but with substantial pulse-width modulation, which 
would be difficult to filter to get a clean VFO  signal. So for your 
mixer-VFO, a conventional mixer would work better.

Cheers, Jim Moritz
73 de M0BMU




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          Good afternoon all,<br>
 <br>
 &nbsp; may be this is old hat for some of you, but if you are interested in the<br>
 protocol DCF39 uses for its signalling, go here :<br>
 <a class="moz-txt-link-freetext"
 href="http://longwave.bei.t-online.de/Efr.pdf">http://longwave.bei.t-online.de/Efr.pdf</a><br>
 <br>
 73 &nbsp;Alberto &nbsp;I2PHD<br>
 <br>
 
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: AW: VFO for VLF receiver? Digital type pre-mixer, any ideas?
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Hi 

yes, any ideas, please look at www.mvnet.de/priv/vw/index~1.htm

I will write any schematics and programs thes evening and on the weekend
01.Feb  to the homepage

73 
Eberhard

-----Ursprüngliche Nachricht-----
Von: jan-martin.noding@telenor.com
[mailto:jan-martin.noding@telenor.com]
Gesendet: Mittwoch, 22. Januar 2003 18:03
An: rsgb_lf_group@blacksheep.org
Betreff: LF: VFO for VLF receiver? Digital type pre-mixer, any ideas?


Hi

planning to build a VFO for a boatanchor VLF receiver covering 50-140KHz, 
first IF is 169kHz and it was originally using xtal control. The VFO must
cover 220-310kHz.

The variation needs to 85kHz, and it seems easier to make a VFO above 1MHz, 
possibly Clapp oscillator (my favourite since everybody else disregard it!),
might also try the Seiler.

I thought of using a 2457.6MHz xtal and mix with VFO (ca 2MHz), and divide
the output
by two or more. Suppose I could use an FF, preferably CD4013 for the mixer.

But I can't find any reference to similar constructions, only have a vague
memory that it has been mentioned in TT some time in the last 35 years

Wonder if somebody else have some experience in this, and will the mixer
divide
or just mix?

960kHz resonators are also readily available, but they won't pull much.

73
Jan-Martin

---
J M Nøding, Datakvalitet, TTS, Kristiansand
Telefon 0047-380-52660, 9077-7126 (QTH: 0047-380-87178)



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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<DIV><FONT face=Arial size=2>Hello Mal:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Do you think to transmit on QRSS3 for european 
QSO´s?</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE dir=ltr 
style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV 
  style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
  <A title=g3kev.ham@virgin.net href="mailto:g3kev.ham@virgin.net">hamilton 
  mal</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A title=rsgb_lf_group@blacksheep.org 
  href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org</A> 
  </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Monday, January 20, 2003 7:26 
  PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: DXPEDITION</DIV>
  <DIV><BR></DIV>
  <DIV><FONT face=Arial size=2>I will be transmitting QRS during late 
  evening/early morning for&nbsp;Transatlantic xband QSO'S. TX 135.922 and 
  RX&nbsp;on HF 7030 Khz. I will not have email facilities so 
  therefore&nbsp;please reply on HF, or tel nr 0774 808 8937.</FONT></DIV>
  <DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
  <DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV></BLOCKQUOTE></BODY></HTML>

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Thread-Topic: Remote operated active antenna for 10kHz-40MHz
Thread-Index: AcLCZhDTp2MWp5lXRkGphYIvbCU4ZwAY7L6A
From: jan-martin.noding@telenor.com
To: rsgb_lf_group@blacksheep.org
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Subject: LF: Remote operated active antenna for 10kHz-40MHz (J310)
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This is the recommended design for a broad-band amplifier, 
LA7MI has a very strong signal on 96MHz, so he added an RFC at the 
input to form a lowpassfilter. I do have very strong signal on CEPT TV Ch2 (48.25MHz) 
and followed LA7MI's recommendations, but also used a more lowfrequent core. 
Never tested the frequency range since I am only interested in 10-400kHz range.

the JFET/PNP-type amplifier is NOT recommended for 
antenna amplifier, but of course useful for many other purposes, this J310 type was 
mentioned in Radcom some time in the autumn 2002

Used it earlier for frame antenna with a remote switch, too, but later discovered 
that it was no need for an amplifier (two cables; one for varactor tuning and one for
power and signal). Now I have two cables, one for either antennas

TIY050 is a transistor I don't know anything more than it is epoxy pnp and free.

73,
Jan_Martin
LA8AK (in JO38XC)  
N4623-Kristiansand (tel.: +47-380-87178 Home)(38052660 Work 90777126 Mobile)
http://www.laud.no/la6nca/LA8AK/ 

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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi Steve and LF-Group,<BR>
<BR>
thanks for inserting the 10dB-attenuation at W3EEE: last night's plot definitely proved it's value and allowed an evaluation of the path budget from Central Eu into the USA. During the&nbsp; -7dB-peak between 0630 and 0700, the noise curves apparently replicated the signal, supporting Steve's point that displayed SNR is actually limited (to about 30dB) by the modulation sidebands.<BR>
<BR>
An extrapolation of the noise during the nearest troughs (about -43dB) would have given 36dB SNR at the peak. Gaining 16dB by going from 0.4Hz to 10mHz and allowing some 3dB for the&nbsp; peak-maximum-type noise evaluation, SNR from DCF's 40kW EMRP was 55dB. A 1W E(D)RP amateur station would have produced 48.5dB less signal or 6.5dB SNR, good enough for an "M" report. But, as Alan has said, a UK-to-East-Coast path could have been significantly stronger.<BR>
<BR>
A detailed look on the sideband-spectrum during many FSK telegrams (see image) revealed a number of gaps where its intensity is another 30dB less than close to space frequency; good channels for noise measurements would be near 138563, 138634, 138765 or 138966Hz. Another approach might be to take a little advantage of the relatively short telegram duration by using true-rms averaging rather than peak-hold in the noise channels, although I'm not quite sure how to tell SpecLab to do just that.<BR>
<BR>
73 de Markus, DF6NM<BR>
</FONT></HTML>
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hi Larry,
<BR>
<BR>Spectrum Lab has been tested with the Audigy 2, the 96kHz sampling rate seems to work but the amplitudes are lower than expected (maybe some fiddling with 24-bit samples required). The "old" Audigy does not support 96kHz though the chip's specification says something different. So beware, if you want to process signals up to 48 kHz get the Audigy 2 and not the older Audigy.
<BR>All lower sampling rates (8000, 11025, 22050, 44100, 48000 Hz) work nicely. Other DSP programs surely will have no problems with these cards because none of the Windoze progs does direct hardware access these days.
<BR>
<BR>
<BR>Regards,
<BR> Wolf DL4YHF.</FONT></HTML>

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From: jan-martin.noding@telenor.com
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Subject: LF: VFO for VLF receiver? Digital type pre-mixer, any ideas?
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Hi

planning to build a VFO for a boatanchor VLF receiver covering 50-140KHz, 
first IF is 169kHz and it was originally using xtal control. The VFO must
cover 220-310kHz.

The variation needs to 85kHz, and it seems easier to make a VFO above 1MHz, 
possibly Clapp oscillator (my favourite since everybody else disregard it!),
might also try the Seiler.

I thought of using a 2457.6MHz xtal and mix with VFO (ca 2MHz), and divide the output
by two or more. Suppose I could use an FF, preferably CD4013 for the mixer.

But I can't find any reference to similar constructions, only have a vague
memory that it has been mentioned in TT some time in the last 35 years

Wonder if somebody else have some experience in this, and will the mixer divide
or just mix?

960kHz resonators are also readily available, but they won't pull much.

73
Jan-Martin

---
J M Nøding, Datakvalitet, TTS, Kristiansand
Telefon 0047-380-52660, 9077-7126 (QTH: 0047-380-87178)



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Subject: Re: LF: Video Card, ATI Radeon 7500
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Larry Kayser wrote:

> Greetings again....
>
> Does anyone in the LF community have any experience in using the ATI 
> Radeon 7500 Video Card, especially with the DSP processing programs?
>
> This card allows me to spread the Microsoft Desktop over two CRT's.
>
> Larry
> VA3LK

I have on my PC the Radeon 9000 128 Mb card, not exactly the same as 
yours, but rather similar.
No problems whatsoever with any (DSP or not) programs. This with both 
Windows 98SE and
Windows XP Pro.  Not tested with Linux. I have the RedHat V8  CDs, but I 
haven't found the time
so far to install it.

73  Alberto  I2PHD
P.S. Though the card allows for two monitors, I have used it with just one.





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi all. Last nights plot from Steve was very interesting. Despite his
reduction of the "gain" by some 10dB, DCF39 showed the highest recorded
levels so far around 0600z.
This is despite an small increase in the Kp recently. I think this probably
indicates that the geomagnetic disturbance only produced the same effect as
would be seen normally many days after a major storm. We have had a very
quiet period through late December and into January. I believe that under
these conditions a small increase in the ionisation in the D-layer due to a
small number of precipated electrons from the minor disturbance has lead
some multipath propagation, and some constructive interference. ( Of course
I could be totally wrong !! ) I did suggest that the rise in the Kp to 4
would manifest itself by Tues/Wed , but I suggested increased absorption and
deep troughs. There is little evidence of absorption but there are some
sharp fading troughs, which would be expected when the different path phases
are opposed.

This is a  "good omen"  for the coming solar minimum !! It indicates to me
that with a quiet sun, a small geomagnetic disturbance can be beneficial to
long distance propagation. I believe that some coronal hole activity will
continue through the quiet years whilst there may be few sunspots and
flares. (I do need to try and check on this).

It will be interesting to see the results from tonight (22/23rd) and
tomorrow night as the Kp rose to 5 just after midnight on the 20th, and has
had some further periods at 4.

Good DXing
Cheers de Alan G3NYK
alan.melia@btinternet.com





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Greetings again....

Does anyone in the LF community have any experience in using the ATI Radeon 
7500 Video Card, especially with the DSP processing programs?

This card allows me to spread the Microsoft Desktop over two CRT's.

Larry
VA3LK





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Greetings:

Does anyone in the LF community have any experience in using the Sound 
Blaster Card Audigy with any of the DSP programs?

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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During this very wet spell I noticed that the total antenna resistance has
gone up - probably due to environmental losses. The daily cycling of antenna
resistance does not seem so bad on 136kHz as on 73kHz or should I say that
it is different. I have found no external effect such as tide or weather
that correlate with these antenna current variations.
When the area around the antenna is very wet, and I leave the transmitter on
for testing, the antenna current starts very low then creeps up over a
period of about 5 minutes or more by up to 100%. So much so that I have to
readjust the matching transformer to avoid overloading the transmitter. This
implies that the total antenna resistance has fallen.
When we had a fall of snow a couple of weeks ago this caused a change in the
resonant point although not the total resistance of the antenna. No wonder
the Decca stations had this elaborate auto tuning and matching arrangement.

Just over a week ago (when it was cold and relatively dry) I was using the
transmitter at night and was alarmed by fire and sparks coming from one of
the insulated wires that goes to the top of the mast. In the beam of my
torch I could see a twig that had obviously got caught up with the wire when
the antenna was tilted over during the day. I turned of the transmitter and
hooked the twig down and found it was steaming and nearly too hot to touch.
It shows how lossy wet trees and shrubs are if located close to the
transmitting antenna.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Subject: Re: LF: Re: Re: Notch for DCF39/Spectrograms/Luxembourg effect
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Dear Jan-Martin, LF group,

At 14:10 21/01/2003 +0100, you wrote:
>A source follower has incredible low gain - even when driving high impedance,
>that's the reason I discard such constructions, but using a PNP instead of 
>NPN
>you may achieve over unity gain. A BJT emitter follower has in the region of
>0.8-0.95x voltage gain.
>You set the feedback to adjust the gain, and add some postive feedback to
>the input and achieve very high input impedance.
A source follower has unity gain only with infinite load impedance. But 
most source followers have a built-in load in the form of the source bias 
resistor, which will normally be a few hundred ohms. A FET with 
transconductance of a few mS has a source follower output impedance of a 
few hundred ohms, so the bias resistor substantially loads the output, 
resulting in gain well below unity. This can be avoided by increasing the 
load impedance in different ways, eg. by connecting a high impedance choke 
in series with the source resistor. In the compound follower circuit, the 
low potential end of the 100R resistor is bootstrapped by the output of the 
emitter follower, making its effective impedance much higher. The bipolar 
follower has much higher transconductance, giving an output impedance of a 
couple of ohms, and so can achieve nearly unity gain even with a 50 ohm 
load. The actual gain of the complete circuit was about 0.9 - 0.95, 
depending on the transistors used.

With a high impedance source, the thermal noise will be high also - eg. for 
10k Rs, about 0.2uV in 300Hz. Most reasonable receivers have lower noise 
floor than this, so increasing gain is not very useful.  If you do need 
higher gain, a circuit like LA8AK suggests is a good way to go.

The circuit I experimented with is not the best high impedance buffer money 
can buy, but it is simple, requires no adjustment, and delivers nearly 
unity gain with adequately low noise and low distortion for many purposes.

Cheers, Jim Moritz
73 de M0BMU




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Thread-Topic: Jan-Martin's Preamp circuit
Thread-Index: AcLBWGTa58y2IkWYTLGMVPSMFV1hdgAAoJEQ
From: jan-martin.noding@telenor.com
To: rsgb_lf_group@blacksheep.org
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TNX
This was constructed in times where we listened to BBC2 and no lower frequencies, so the capacitors are probably small.
Perhaps a resistor in series with the 10nF capacitor to adjust the positive feedback... hi
73
Jan-Martin
---
J M Nøding, Datakvalitet, TTS, Kristiansand
Telefon 0047-9077-7126



-----Opprinnelig melding-----
Fra: Hugh M0WYE [mailto:m0wye@thersgb.net]
Sendt: 21. januar 2003 15:11
Til: rsgb_lf_group@blacksheep.org
Emne: LF: Jan-Martin's Preamp circuit


Hi Jan-Martin and LF group,
I was going to ask if your preamp could be posted on the Reflector ...
Being the "some-other" Here it is ...
73
Hugh M0WYE

----- Original Message -----
From: <jan-martin.noding@telenor.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, January 21, 2003 1:10 PM
Subject: LF: Re: Re: Notch for DCF39/Spectrograms/Luxembourg effect


> Hi,
> I don't see the point in using NPN devices (PNP are better for this
purpose),
> you would probably not have more than 0.5x voltage gain
> A source follower has incredible low gain - even when driving high
impedance,
> that's the reason I discard such constructions, but using a PNP instead of
NPN
> you may achieve over unity gain. A BJT emitter follower has in the region
of
> 0.8-0.95x voltage gain.
> You set the feedback to adjust the gain, and add some postive feedback to
> the input and achieve very high input impedance.
>
> Unfortunately I forgot to forward the circuit from home, but sent it to
Alan
> and some other. Too high gain is of course a problem and may cause some
IMD,
> will try to remember to pass the circuit later (I am in Stavanger at the
moment).
>
> Passed the spectrogram as a separate mail
>
> 73 Jan-Martin
> LA8AK
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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--------------080003080701020502000000
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Hi Jan-Martin and LF group,
I was going to ask if your preamp could be posted on the Reflector ...
Being the "some-other" Here it is ...
73
Hugh M0WYE

----- Original Message -----
From: <jan-martin.noding@telenor.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, January 21, 2003 1:10 PM
Subject: LF: Re: Re: Notch for DCF39/Spectrograms/Luxembourg effect


> Hi,
> I don't see the point in using NPN devices (PNP are better for this
purpose),
> you would probably not have more than 0.5x voltage gain
> A source follower has incredible low gain - even when driving high
impedance,
> that's the reason I discard such constructions, but using a PNP instead of
NPN
> you may achieve over unity gain. A BJT emitter follower has in the region
of
> 0.8-0.95x voltage gain.
> You set the feedback to adjust the gain, and add some postive feedback to
> the input and achieve very high input impedance.
>
> Unfortunately I forgot to forward the circuit from home, but sent it to
Alan
> and some other. Too high gain is of course a problem and may cause some
IMD,
> will try to remember to pass the circuit later (I am in Stavanger at the
moment).
>
> Passed the spectrogram as a separate mail
>
> 73 Jan-Martin
> LA8AK
>


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Thread-Topic: Re: Notch for DCF39/Spectrograms/Luxembourg effect
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From: jan-martin.noding@telenor.com
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Subject: LF: Re: Re: Notch for DCF39/Spectrograms/Luxembourg effect
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Hi,
I don't see the point in using NPN devices (PNP are better for this purpose), 
you would probably not have more than 0.5x voltage gain
A source follower has incredible low gain - even when driving high impedance, 
that's the reason I discard such constructions, but using a PNP instead of NPN 
you may achieve over unity gain. A BJT emitter follower has in the region of 
0.8-0.95x voltage gain.
You set the feedback to adjust the gain, and add some postive feedback to 
the input and achieve very high input impedance.

Unfortunately I forgot to forward the circuit from home, but sent it to Alan 
and some other. Too high gain is of course a problem and may cause some IMD, 
will try to remember to pass the circuit later (I am in Stavanger at the moment).

Passed the spectrogram as a separate mail

73 Jan-Martin
LA8AK

-----Opprinnelig melding-----
Fra: James Moritz [mailto:j.r.moritz@herts.ac.uk]
Sendt: 18. januar 2003 13:42
Til: rsgb_lf_group@blacksheep.org
Emne: LF: Re: Notch for DCF39/Spectrograms/Luxembourg effect


At 12:09 17/01/2003 -0500, you wrote:

><< This is the wrong way to achieve high impedance (and good IMD),
>  it is no need to keep the "source current low" {etc} >>
>
>I do not see anything in the Web page that suggests keeping the source
>current low.  It only says "reasonable amount," which I took to mean "be sure
>to use enough" to keep IMD low.

Dear LF Group,

The output impedance of a follower is roughly the inverse of it's 
transconductance, ie. 1/gm. A J310 JFET has a gm of about 10 - 20 mS, so 
the output impedance is roughly 50 - 100 ohms. To get low distortion, and 
gain close to unity with such a follower requires that the load it is 
driving should be much greater than the output impedance of the follower. 
So a J310 source follower would be fine if driving several hundred ohms or 
greater, but not for a 50 or 75 ohms system.

To get around this, one could use a special FET like the CP640 device used 
in the AMRAD active antenna circuit, with much higher gm. A small power 
MOSFET would give a low output impedance, but rather high input 
capacitance. Bipolar transistors have much higher gm (roughly Ic/25mV), but 
would have relatively low input impedance, in the kilohm range, and be 
relatively noisy with a high source impedance. Various high speed op-amps 
and IC buffers can be used, but they tend to be quite noisy.

A cheap and easy alternative is to use a compound follower, with JFET and 
bipolar followers cascaded. I tried the one shown in the attachment - Zin 
is basically 500k in parallel with the FET capacitance, the gain with 50ohm 
load is about 0.95. The noise at 136kHz with the input shorted was about 
0.05uV in 400Hz BW. About 1V RMS can be applied to the input before there 
is much distortion whilst driving 50ohms, so it ought to be OK with most 
antennas, and is probably better than most receivers. The FET was a J310, 
but other devices with Idss > about 8mA should be OK. A lower gm device 
with lower Idss could be used if the 100R resistor were increased in value, 
but would be noisier. The output BJT used was a 2N3053, but can be a wide 
range of small power transistors with Hfe > 50 when biased to 30mA or so 
and fT in the 10s of MHz - eg. BD131, BFY50, ZTX650 etc. Zout is a few ohms 
- If driving a capacitive load, a resistor in series with the output of 10 
- 20 ohms will prevent oscillation. Extra decoupling will be required if 
the 12V supply is noisy.

Using spectrogram software to monitor the band for signals works very well 
- it allows you to see CW signals that are inaudible, which you can then 
try to "zoom in" using a narrow filter. Although you can't copy the morse 
from the screen display, you can detect the presence of signals that are 
too weak to hear even in the narrowest filter, whilst monitoring the whole 
band segment at once. Some of the spectrogram programs have DSP audio 
filters built in, too.

The broadcast station noises M0WYE is hearing may well be "Luxembourg 
effect", where cross-modulation of the DCF39 carrier by the BC signals 
occurs in the ionosphere, and is often quite strong at my QTH. Usually I 
can here the audio of at least two stations at once.

Hope this is helpful,

Cheers, Jim Moritz
73 de M0BMU



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Subject: LF: DCF39 Frequency shift
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<DIV><FONT color=#0000ff face=Arial size=2><SPAN class=409525112-21012003>Using 
the sigview program LA1TN has shown that the shift is 330Hz, the highest peak is 
138.8kHz, see attached file</SPAN></FONT></DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=409525112-21012003></SPAN></FONT>&nbsp;</DIV>
<DIV>73,<BR>Jan_Martin<BR>LA8AK (in JO38XC)&nbsp; <BR>N4623-Kristiansand (tel.: 
+47-380-87178 Home)(38052660 Work 90777126 Mobile)<BR><A 
href="http://www.laud.no/la6nca/LA8AK/">http://www.laud.no/la6nca/LA8AK/</A> 
</DIV></BODY></HTML>

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--------------030209090500050304090604--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Dear Hugh, LF Group,

At 22:57 19/01/2003 +0000, you wrote:

>I notice the sounds and patterning on the screen are only there during the
>hours of darkness, does that prove that it is the ionosphere and not the
>radio ?
>Does the ionosphere cause non-linear mixing of higher frequencies or just LF
>?

I believe it's called the Luxembourg effect because it was first observed 
on MF signals from Radio Luxembourg in the 20s or 30s. I don't know much 
about the field, but any frequency that is absorbed by the ionosphere will 
cause "heating", which modulates it's reflecting properties. There are 
number of  research facilities which transmit megawatts of HF straight up 
in order to investigate ionospheric physics - searching the web under 
"ionospheric heater", "HAARP" or "EISCAT" will give you lots of hits, 
including the conspiracy theorists, who of course will tell you what the 
real purpose of these experiments is!
The fact that the noises disappear during daytime, also that any amount of 
preselector filtering does not remove them, is quite convincing that these 
signals originate outside the receiver.

>Have you tried out your buffer circuit - or is it just a "circuit idea" I
>wonder ?

Yes, it is a real circuit - I have not tried it with the notch filter, but 
I did test it as a high impedance antenna preamp, as well as the bench 
measurements I mentioned - it seems to do the job quite well, and since 
there are 4 medium wave broadcast stations within 1km of my QTH, it 
demonstrates the linearity must be OK!

Cheers, Jim Moritz
73 de M0BMU




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
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The files I posted this morning at:
> http://webpages.charter.net/w1tag/136/
may not have been readable due to my early morning foggy brain. If you
couldn't make sense of them, please try again -- the problem has been fixed.

John Andrews, W1TAG





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi all, The Kp index rose to 5 just after midnight 20th, so I am expecting
some increase in absorption by about Wed/Thurs 22/23rd night. This should
reduce levels of night-time signals for a few days. NOAA is forecasting
unsettled geomagnetic conditions by the 22nd due a geoeffective (aiming at
us !) coronal hole. If this "burps" it means the depressed period could be
prolonged somewhat.

We need to keep an eye on Steve's log to see how bad it gets.

I think Laurie is right that closer behind a disturbance we can often ride
in on a enhancement "wave" due to constructive interference between the
different radio paths and get signals at 3 sec dot easily displayed. This Kp
increase could be a chance but I suspect it will only be a "beginers wave"
unless the Kp rises further.

We need to be careful about interpreting Steve's plots regarding UK paths.
DCF is 700 or more kms east and Steve is nearly 1000kms west of John. This
will influence the timing of the peaks and troughs he sees, and sometimes
the maximum levels. In general I believe in a relatively quiet period like
we have just had there may be little difference. When we run into a period
of more serious multi-path fading Steve's results may diverge from those
achieved by John ,Dex and Lloyd. It will be interesting to see by how much.

Cheers de Alan G3NYK
alan.melia@btinternet.com




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 20 Jan 2003 16:49:24 -0500
From: "Steve Dove" <dsp@hifidelity.com>
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Greetings insomniacs,

Header says it all.  In order to provide a bit more headroom to display
possibly bigger propagation peaks, the sensitivity of the DCF-39
monitoring system has been dropped 10dB.

http://www.w3eee.com

        73,

                Steve







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From: "PY2PLL" <py2pll@py.qsl.br>
To: rsgb_lf_group@blacksheep.org
References: <23.2aadfb3f.2b5c5522@aol.com> <5.1.0.14.0.20030120171137.00b158e0@gemini.herts.ac.uk>
Date: Mon, 20 Jan 2003 18:12:49 -0300
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Hi James . . .

> It seems to me this is quite a large loop, and will generate a large
output:

Yes, it´s large ... at least the bigest one I ever did. And it´s a
prototype. I´m using PVC covered wire ... not soft enough to have evenly
"nice" turns spacing.

>
> For your loop, and a f/s of 1uV/m, this gives 0.21uV @ 400k, 0.85uV @
1600k.,
> With a Q of 200, the voltage at resonance will be increased to 42uV @
400k,
> 170uV @ 1600k

I think I´ll built a smaller one, just to make some "real" FSM and then
generate a table with the levels obtained with the bigger one. I have an SLM
from G&W which have a balanced 6K / unbalanced 75ohm input Z.

> The loop noise depends on the RX bandwidth, but in 10kHz BW it will be
> roughly 6uV @ 400k, 12uV @ 1600k. So for 1uV/m, SNR would be 17dB @ 400k,
> 23dB @ 1600k.

The thermal noise in my tables are simply the "coil" thermal noise @ 250Hz
BW. I used the article formula´s.

> The tuning is a problem - 4:1 tuning range needs 16:1 capacitance
> variation, including the stray capacitance of the loop. If L is about
446uH
> from the table, this means 350p - 22p. The stray capacitance of the loop
> may be greater than 22p, so you may not get the full tuning range. Using a
> varicap diode, it is unlikely the minimum- to maximum capacitance ratio
> will be high enough. it may be necessary to reduce the number of turns and
> use a larger tuning capacitor.

The loop turns are spaced by 5mm. I used G4FGQ´s software to estimate stray
C ...

> The other problem is that local stations will give very large signals -
eg.
> 10mV/m from an 1MHz MF broadcast station will result in about 1V across
the
> loop at resonance, which will probably lead to severe intermods from both
> the preamp and the varicap.

Ooopps ... this is true ... air-insulated C is winning ...

> You could connect the preamp across only 1 turn
> instead of all 9 - this would still give several uV out for 1uV/m f/s,
more
> than enough for a decent receiver.

I already did this way. I couldn´t resist to test it with an air-variable C
and no pre-amp so I added a 1 turn loop inside the main one, about 3 inches
between coils.

> In fact, since the loop output is so
> large, you could probably eliminate the preamp by using a single turn
> coupling loop to a 50ohm RX input. The air-variable tuning capacitor would
> also be a good idea for this reason, unless you live a very long way from
> any broadcast stations!

I guess I´ll keep this 1 turn solution ... the local BCs - nearest is about
5Km away - are pushing Kachina´s S Meter from 9+40 to 9+70 with internal
pre-amp off.

I´ll start the 136KHz prototype and compare it´s performance using 153KHz BC
and DCF39 as signal sources.

Thanks on the comments;

73
Marcus
PY3CRX/PY2PLL
http://py.qsl.br
Active from "DC" to Laser ...








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Hugh" <m0wye@thersgb.net>
To: rsgb_lf_group@blacksheep.org
References: <5.1.0.14.0.20030117183432.00af50f0@gemini.herts.ac.uk>
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Hi Jim,
Thankyou for your contribution on the notch filter.
Also for the idea about the "Luxemborg effect".
I notice the sounds and patterning on the screen are only there during the
hours of darkness, does that prove that it is the ionosphere and not the
radio ?
Does the ionosphere cause non-linear mixing of higher frequencies or just LF
?
Have you tried out your buffer circuit - or is it just a "circuit idea" I
wonder ?
73
Hugh M0WYE




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Hugh" <m0wye@thersgb.net>
To: rsgb_lf_group@blacksheep.org
References: <000401c2bf5f$2864fae0$ea00a8c0@f3a3a2>
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Hi PA0BWL
I don't know if you monitor this reflector, but if you do
you were an excellent signal here at Wye, Near Ashford. JO01LE.
I answered your QRSS CQ call just before 13:00, but I don't think you can
have heard me.
Your signals were audible in the loudspeaker.
73
Hugh M0WYE







From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Dear Marcus, LF Group,

It seems to me this is quite a large loop, and will generate a large output:

I think across an untuned loop V = 2.1e-8.f.N.A.E

where N = turns, f is frequency in Hz, A is area in m^2, E is f/s in V/m

For your loop, and a f/s of 1uV/m, this gives 0.21uV @ 400k, 0.85uV @ 1600k.,
With a Q of 200, the voltage at resonance will be increased to 42uV @ 400k, 
170uV @ 1600k

The loop noise depends on the RX bandwidth, but in 10kHz BW it will be 
roughly 6uV @ 400k, 12uV @ 1600k. So for 1uV/m, SNR would be 17dB @ 400k, 
23dB @ 1600k. The JFET noise will be negligible. I think most of the time 
the atmospheric noise level in 10k BW at MF will be well above 1uV/m, so it 
should be more than sensitive enough. Reducing the Q to 100 due to 
resistors or varicap will make the output voltage decrease by 6dB and loop 
noise decrease by 3dB - still probably OK. Reducing the RX bandwidth will 
improve the SNR, of course.

The tuning is a problem - 4:1 tuning range needs 16:1 capacitance 
variation, including the stray capacitance of the loop. If L is about 446uH 
from the table, this means 350p - 22p. The stray capacitance of the loop 
may be greater than 22p, so you may not get the full tuning range. Using a 
varicap diode, it is unlikely the minimum- to maximum capacitance ratio 
will be high enough. it may be necessary to reduce the number of turns and 
use a larger tuning capacitor.

The other problem is that local stations will give very large signals - eg. 
10mV/m from an 1MHz MF broadcast station will result in about 1V across the 
loop at resonance, which will probably lead to severe intermods from both 
the preamp and the varicap. You could connect the preamp across only 1 turn 
instead of all 9 - this would still give several uV out for 1uV/m f/s, more 
than enough for a decent receiver. In fact, since the loop output is so 
large, you could probably eliminate the preamp by using a single turn 
coupling loop to a 50ohm RX input. The air-variable tuning capacitor would 
also be a good idea for this reason, unless you live a very long way from 
any broadcast stations!

Hope this is helpful,
Cheers, Jim Moritz
73 de M0BMU



At 13:35 20/01/2003 -0300, you wrote:
>Hi ...
>
>After read an article last year (Wireless World) about loop antennas X DCF39
>calibration, I constructed a octogonal RX loop, #16 awg wire, to cover from
>400KHz to 1.6MHz.
>
>There´s 9 turns, 5mm spacing, 1.9 meter diameter. About 55 meter of wire.
>
>This is the first version. Later I´ll build another one to 136KHz.
>
>Acording with this article, I should expect a Q=200 ... 220 from such loop.
>
>I considered the NTE618 to tune it and a push-pull pre-amp (J310) with gates
>conected to the loop ends. No resistors there. The article consider that for
>such loop at this frequency will have something like .20uV of thermal noise.
>The resistors will add some extra noise there so I removed them.
>
>But the Q=210 ... and the NTE618 Q is 200.
>
>Is there any gain If I use a dual-gang air variable driven by a step motor +
>reduction in place of the NTE618?



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "hamilton mal" <g3kev.ham@virgin.net>
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<DIV><FONT face=Arial size=2>Hi All</FONT></DIV>
<DIV><FONT face=Arial size=2>I intend to be in Tyrone/Ireland</FONT><FONT 
face=Arial size=2>&nbsp;operating GI3KEV from about&nbsp;the 27th January for 
two weeks approximately. I will be active on 136.5&nbsp;khz&nbsp;normal CW and 
QRS around 135.922 khz plus/minus to avoid other activity.&nbsp;Frequencies can 
vary to avoid qrm. I have VFO control.&nbsp;I will be active&nbsp;during 
weekdays&nbsp;and weekends, daytime as well as night time.&nbsp;</FONT></DIV>
<DIV><FONT face=Arial size=2>I will be transmitting QRS during late 
evening/early morning for&nbsp;Transatlantic xband QSO'S. TX 135.922 and 
RX&nbsp;on HF 7030 Khz. I will not have email facilities so 
therefore&nbsp;please reply on HF, or tel nr 0774 808 8937.</FONT></DIV>
<DIV><FONT face=Arial size=2>Antenna consists of a 120 feet tower with 3 x inv L 
antennas each with&nbsp;a horizontal&nbsp; top section of 300 feet 
approx.</FONT></DIV>
<DIV>&nbsp;<FONT face=Arial size=2>TX H/Built mosfet, power approx 1W erp. HF 
antenna doublet for all bands 1.8 - 50 mhz up at 80 feet.</FONT></DIV>
<DIV><FONT face=Arial size=2>73 de Mal/G3KEV</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
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Hi Jim and the LF group,
Last nights experiment was useful,it certainly seems that early morning is a
good time,however I am sure that the situation we have had recently is
"average".When the earlier crossings on 136 and my 73kHz  crossings were
made,conditions were above average.I am sure that this requires a period of
decay 14-20 days after a disturbance CME etc. As we are moving into a less
active solar situation (2006 is predicted as the minimum) perhaps we should
make the most of the present situation.
Anyway thanks for all the reports. 73 Laurie.



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Hi Lloyd,
I tried to send a mail to your address but it was rejected twice.So I hope
the group will excuse me sending it via the reflector.I simply want to say
thanks for the capture,
it looks like early morning(here) is a good time as Jim predicted.Looking
foreward to recieving you chaps when the time comes.
73 Laurie.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "PY2PLL" <py2pll@py.qsl.br>
To: lowfer@mailman.qth.net,  rsgb_lf_group@blacksheep.org
References: <23.2aadfb3f.2b5c5522@aol.com>
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Subject: LF: Loops x Q
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Hi ...

After read an article last year (Wireless World) about loop antennas X DCF39
calibration, I constructed a octogonal RX loop, #16 awg wire, to cover from
400KHz to 1.6MHz.

There´s 9 turns, 5mm spacing, 1.9 meter diameter. About 55 meter of wire.

This is the first version. Later I´ll build another one to 136KHz.

Acording with this article, I should expect a Q=200 ... 220 from such loop.

I considered the NTE618 to tune it and a push-pull pre-amp (J310) with gates
conected to the loop ends. No resistors there. The article consider that for
such loop at this frequency will have something like .20uV of thermal noise.
The resistors will add some extra noise there so I removed them.

But the Q=210 ... and the NTE618 Q is 200.

Is there any gain If I use a dual-gang air variable driven by a step motor +
reduction in place of the NTE618?

P.S.: I put two tables, considering standard loop areas, both for 136 and BC
band at:

http://py.qsl.br/loop136e.gif and
http://py.qsl.br/loop-om-e.gif

73
Marcus
PY3CRX/PY2PLL
http://py.qsl.br
Active from "DC" to Laser ...







From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Dear LF Group,

Thanks to all for the T/A reports. The interesting thing is that, allthough 
from the DCF39 plots last night was quite good by recent standards, the 
signal strength was not a long way above the threshold required for copy of 
QRSS60, and the signals fade in and out. For example, in W1TAG's "20 Jan-4" 
image, the M of my callsign is visible, most of the 0 has dissapeared, and 
the BMU is again visible. Since this same path has previously supported 
signals with shorter element lengths (eg, Jason during December with it's 
12 sec "dots"), it is clear that signal levels can improve substantially 
over last night - perhaps by 10dB or more. I would like to see what the 
DCF39 plot looks like then!

Cheers, Jim Moritz
73 de M0BMU



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Date: Mon, 20 Jan 2003 13:53:26 +0000
From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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Subject: Re: LF: Early morning tests?
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Looks like my best capture of Laurie's and Jim's signal occurred around
0630.  Comparing John's captures with mine it's obvious it takes a
little better conditions or a little more power to get another 1130 km. 
The difference certainly can't be due to skill and equipment :) 

Best screen is:

http://www.w4dex.com/argo/20jan03/0630.jpg

All overnight captures with any trace of signal can be seen from the
directory:

http://www.w4dex.com/argo/20jan03/

Lloyd's 0730 capture from Maryland shows good copy of both signals while
Laurie's signal has vanished here.  Was still seeing some of Jim's
signal though.  

Lloyds capture:

http://www.geocities.com/lacwman/135jan20.jpg

Dex





John Andrews wrote:
> 
> Jim's and Laurie's excellent morning signals may be seen in the "20Jan"
> files at:
> http://webpages.charter.net/w1tag/136/
> 
> "M0BMU" sure didn't fit on one screen!
> 
> John Andrews, W1TAG


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Date: Mon, 20 Jan 2003 13:32:07 -0000
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Hi Lloyd there is a clear QRSS trace of "BMU" at 922 Congratulations.

Cheers de Alan G3NYK
alan.melia@btinternet.com





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From: "John Andrews" <w1tag@charter.net>
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Jim's and Laurie's excellent morning signals may be seen in the "20Jan"
files at:
http://webpages.charter.net/w1tag/136/

"M0BMU" sure didn't fit on one screen!

John Andrews, W1TAG




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From: "lloyd chastant" <chastant@smart.net>
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Subject: LF: 135.922 capture in Maryland
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Here is a capture of AQC at about 0739z hr in Maryland

 www.geocities.com/lacwman/135jan20.jpg

may have been traces of others?/
de Lloyd W3NF FM19MH


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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi John, Dexter, Jim and Laurie,<BR>
<BR>
 congrats for the ufb results of the early morning T/A session: Jim and Laurie were continuously visible with O-signals on John's screenshots from before 05:00 until QRT around 7:30 and 8:20 respectively. Also, both callsigns are very clear on Dexters 07:10 capture. No trace though of the third party in the middle (myself) ;-(.<BR>
<BR>
Compared to Sat/Sun, DCF39 plots from W3EEE showed a later start of the opening, with strong saturated levels after 02:00 and a continuous flat peak from 04:00 right through to the short interruption at 07:30.<BR>
<BR>
Tnx for watching and posting captures, 73 es best wishes<BR>
<BR>
Markus, DF6NM<BR>
</FONT></HTML>

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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Dear LF Group,

Transmitted "M0BMU" repeated from about 0400 - 0730 utc this morning using 
QRSS60 on 139.9225kHz, and something around 1W ERP. I also saw DFCW signals 
from G3AQC and DF6NM. The signal levels on W3EEE's DCF39 chart look good 
for that period, up near the "clipping" level - anybody see anything?

Cheers, Jim Moritz
73 de M0BMU



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This is a multi-part message in MIME format.
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<html>
At 00:27 18/01/03 +0100, EA1PX wrote:<br><br>
<blockquote type=cite class=cite cite><font face="arial" size=2>Hi
Group:</font><br>
&nbsp;<br>
<font face="arial" size=2>I copy transmissions on 132.930 and 133.230
kHz.</font><br>
<font face="arial" size=2>Can anyone to confirm me if they are of the
Datatrak System and where are the TX located?</font><br>
&nbsp;<br>
<font face="arial" size=2>73 de José, EA1PX</font></blockquote><br><br>
Hello Jose,<br><br>
They are Datatrak but there are no stations in Iberia so it must be
skywave from the UK, Dutch or Austrian transmitters. Difficult to tell
which because they are interleaved. <br><br>
73 de Walter, G3JKV<br>
</html>


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
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Hi All,
Further to Jims tests,I made the following transmissions last night/this
morning.
0900 - 0000       AQC repeated
0500                   AQC once 20 mins.
0600                   AQC once 20 mins
0700 - 0830        AQC repeated

Hope this helps.  73 Laurie.



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From: "John Andrews" <w1tag@charter.net>
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Just received a good AQC on 135.9209/135.921. No other signals thus far. I
should be getting a Loran line on 135.92092 later on, so I may have trouble
with that frequency.

John Andrews, W1TAG





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From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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I'm up and running on 135 kHz as of 23:00 hrs.  Screen captures will be
posted at the usual location:

http://www.w4dex.com/argo/135khz.jpg

Will leave system running overnight in auto mode.  

Dex

MarkusVester@aol.com wrote:
> 
> Dear John and LF Group,
> 
> now Sunday 21:30, I have signed on using 135922.2 /.3Hz DFCW
> (60s/20s), which is 1.28Hz above Laurie's AQC. Will try to keep going
> for at least a couple of hours now and then come back in the morning
> around 06:00. Wx here is humid and no frost, EDRP abt 0.2W, some 4dB
> less than a week ago.
> 
> 73 de Markus, DF6NM



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi All, nothing much has changed on the solar front. The day has been quiet
with no flares and a background X-ray flux of about B5. The Kp index did go
up to 4 again for 3 perios, and is expected to stay in the 2 to 4 range over
the next few days. I dont expect that increase to have a great effect on
conditions at 136kHz. There is just the possibility that it may start to
increase absorption a little from Tuesday, though these low levels (4) in
the past have not produced noticable effects. The first signs of trouble
will probably be deep troughs on Steve's plots.

Good Luck to those trying the early morning "watch".

Cheers de Alan G3NYK
alan.melia@btinternet.com





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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Dear John and LF Group,<BR>
<BR>
now Sunday 21:30, I have signed on using 135922.2 /.3Hz DFCW (60s/20s), which is 1.28Hz above Laurie's AQC. Will try to keep going for at least a couple of hours now and then come back in the morning around 06:00. Wx here is humid and no frost, EDRP abt 0.2W, some 4dB less than a week ago.<BR>
<BR>
73 de Markus, DF6NM<BR>
</FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "G4WGT" <g4wgt@talkgas.net>
To: "Rsgb_Lf_Group" <rsgb_lf_group@blacksheep.org>
Date: Sun, 19 Jan 2003 20:40:53 -0000
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Hi to you all  at LF,

For about 3 or four days or so I have been receiving a cw type signal on
about 137.280 Khz continually sending what is like a letter N without breaks
or spaces, something like "dah dit   dah dit   dah dit   dah dit"
continuously.

It has only recently appeared it is audible but weak & visually the
characters are perfectly repetitive (always the same space, dot & dash
length).

Can anyone else hear/see it or could it be something local to me or a mix
product ?

Would appreciate any explanation.

Thanks

73

Gary   G4WGT
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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<DIV><FONT face=Arial size=2>I have just worked VK3IO /Ron in&nbsp;Cockatoo Aus 
on 160 metres. This is a good omen for tonight for those adventuring to cross 
the Atlantic on 136 khz. In the past when 160 prop is good likewise LF is good 
for long haul. </FONT></DIV>
<DIV><FONT face=Arial size=2>Good Luck de Mal.G3KEV</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Ian Kyle" <ian.gi8ayz@virgin.net>
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To whom it may concern,

for various reasons there will be no radio activity from MI0AYZ for a few
weeks, although I shall still be watching the reflector.
Anyone wanting a 73KHz QSO will I hope get one before the season closes.

73,

Ian GI8AYZ/MI0AYZ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
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I will run the screen captures again tonight (Sunday --> Monday) on 135.922
kHz, starting at 2100 and ending at 1200 on Monday. This should take care of
any who don't have to go to work tomorrow, as well as those who can't wait
to get there. Jim's suggestion is an excellent one. I've had my best results
here in the U.S. during the immediate pre-dawn hours.

Captures will be posted at:
http://webpages.charter.net/w1tag/136-1.jpg

John Andrews, W1TAG





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
References: <001d01c2bf62$233a03a0$597e6051@oemcomputer> <00b001c2bf63$ce652d80$0500a8c0@charter.net> <000801c2bfbe$526c0ea0$597e6051@oemcomputer>
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Mike,

> I think you are right. I took a couple of screen dumps from your site and
> cannot see anything I could positively identify as my sigs. Do you have an
> archive of the night's captures?

I have posted four captures from the most productive part of the night at:
http://webpages.charter.net/w1tag/136/

The Newfoundland line shouldn't have affected my ability to see you, but
perhaps you could go a little "north" of that.

John Andrews, W1TAG





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Dear LF Group,

Looking at W3EEE's very useful graphs of DCF39 over the last week or so, it 
looks like the best conditions are quite consistently in the few hours 
before 0600 - it's just unfortunate that normal humans like to be tucked up 
in bed at that time!

So in an attempt to find out if T/A propagation really is better then, I 
propose to do some tests tomorrow morning, starting before or at 0400 and 
carrying on until 0700 or so - so if US listeners would like to leave their 
gear running until then, hopefully something will be seen. I will try 
QRSS60 on  135.9225kHz, unless someone is already there, in which case I 
will re-tune a few tenths of a Hz. Any reports will be very welcome.

Cheers, Jim Moritz
73 de M0BMU




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
References: <001d01c2bf62$233a03a0$597e6051@oemcomputer> <00b001c2bf63$ce652d80$0500a8c0@charter.net>
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> I believe the signal you see is a Loran line from Newfoundland on
135921.60.
> I can't see any sign of your signal in the captures, but please do go
> through them!
> John Andrews, W1TAG

I think you are right. I took a couple of screen dumps from your site and
cannot see anything I could positively identify as my sigs. Do you have an
archive of the night's captures?

Looks like I need to improve the signal to get as far as the USA. The W3EEE
plot of DCF39 suggested that the band was open for several hours, so perhaps
a QRSS120 transmission would be worthwhile. In the meantime, I will use a
frequency a little higher to avoid that Loran line.

Mike, G3XDV
http://www.lf.thersgb.net
=================




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Mike,

> There is one other
> signal present which is within 0.1Hz of my frequency and has some of the
> characteristics of my signal (dots and dashes made from 30s elements with
> gaps in between), but not sure. Will do a comparison in the morning
between
> my local Argo monitoring and the W1TAG Argo.

I believe the signal you see is a Loran line from Newfoundland on 135921.60.
I can't see any sign of your signal in the captures, but please do go
through them!

I will leave the capture running overnight in case there are any early
risers who may want to try the morning path.

John Andrews, W1TAG





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Nice sigs from Laurie and Dave on the W1TAG screen. There is one other
signal present which is within 0.1Hz of my frequency and has some of the
characteristics of my signal (dots and dashes made from 30s elements with
gaps in between), but not sure. Will do a comparison in the morning between
my local Argo monitoring and the W1TAG Argo.

Going to bed now at 0225. I will pay for this late night with a migraine!
The things we do for ham radio.

Mike, G3XDV
http://www.lf.thersgb.net
==================




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Gotta get some sleep now,thanks for the captures. Best of luck 
GN all. Laurie.




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From: "Dave Pick" <g3yxm@wireless.org.uk>
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Thanks everyone.

I'm off to bed. Last message was "GN" in case it's not too clear!
I had a bit of tripping due to heavy rain which delayed the last "M" of the
callsign at 01:10ish.

Good Night.
Dave 'YXM.





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References: <000901c2bf26$d4e90a60$597e6051@oemcomputer> <005001c2bf28$561355e0$1700a8c0@home> <008701c2bf52$73ba2e00$0500a8c0@charter.net> <002c01c2bf55$1202e460$1700a8c0@home>
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Dave,

Was that a GN from you? If so, GN!

John A.




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----- Original Message ----- 
From: "John Andrews" <w1tag@charter.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, January 19, 2003 12:33 AM
Subject: LF: Re: Re: T/A tonight


> Dave - your DFCW is coming in well right now.
> 
> Good signal from what I think is Laurie on 921.3.
> 
> John A.
> 
> Yes I confirm 921.3, nothing yet on Dex's capture.
going to DFCW now. Cheers Laurie. 




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Got a complete YXM. Both Dave and Laurie are doing very well right now. No
sign of other sigs, though.

John Andrews





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From: "Dave Pick" <g3yxm@wireless.org.uk>
To: rsgb_lf_group@blacksheep.org
References: <000901c2bf26$d4e90a60$597e6051@oemcomputer> <005001c2bf28$561355e0$1700a8c0@home> <008701c2bf52$73ba2e00$0500a8c0@charter.net>
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John.

Yes I can see one complete "YXM" on the latest screen and Laurie is very
strong. Interesting that our two signals came out of the noise at different
times earlier. I am about 120 miles north and about 50 west of Laurie.

Dave 'YXM.
----- Original Message -----
From: "John Andrews" <w1tag@charter.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, January 19, 2003 12:33 AM
Subject: LF: Re: Re: T/A tonight


> Dave - your DFCW is coming in well right now.
>
> Good signal from what I think is Laurie on 921.3.
>
> John A.
>
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Dave - your DFCW is coming in well right now.

Good signal from what I think is Laurie on 921.3.

John A.




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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
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<DIV><FONT face=Arial size=2>Just a hint of signals on John's latest 
scan.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Dave 'YXM</FONT></DIV></BODY></HTML>

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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
References: <74S2VLF93VUXSTQGSM09USTSNL3YJF.3e29837a@Charlie_Drake> <004201c2bf46$e6e24680$0de486d4@erica>
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Is anyone transmitting on 135921.3?

John Andrews



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From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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Subject: Re: LF: Re: T/A tonight
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Noise here in NC is about as low as it gets.  It isn't often I can run
Argo in manual gain mode.  This probably won't last long after dark. 
Screen captures will be available at:

http://www.w4dex.com/argo/135khz.jpg

Dex

John Andrews wrote:
> 
> I am running the "capture machine" again tonight. Shots will appear every 15
> minutes at:
> http://webpages.charter.net/w1tag/136-1.jpg
> 
> The window is from 135920.5 to 135923.5. Avoid 921.05 and 920.92 because of
> Loran lines. The screen is set for 60 seconds, normal speed.
> 
> Dave: I had a strong line on 921.8 all day yesterday, ending sometime during
> the early morning over here. I don't see it right now, but will advise if it
> reappears.
> 
> John Andrews, W1TAG



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
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Hi Steve
13/1/03

> Having just returned from a week long business trip to find that
> w3eee.com was still working(!) I'm also gratified to see that it is
> of use . . .

This is really a very useful site and I have contributed somewhat to
w3eee.com hits.
I guess this is an extension of the service that Alan provided when he
monitored the station in Newfoundland but gives us a good idea of the
propagation from a North American perspective. The ability of the display to
monitor adjacent channels for electronic environment (squirglies) so that
we get a fuller picture is very well thought out. The fact that it is in
near real time is a real bonus and enables us to keep our powder dry until
we have something to shoot at.

>.... also amazed by the great propagation it captured last night.

Yes, this seems nearly as good as the 'Scorcher' early this month.
Acting on the information from KL1X in his e-mail of the 13/1/03, and from
the strength of DFC39 on the w3eee site, I transmitted from 0600 until 0900
on 137769kHz. I will have to wait until 3rd Feb to know if this was
successful. (The 'Scorcher' at w3eee coincided with large
strength EU B/C station signal strengths in Alaska).
I don't think I will be transmitting tonight. Gale force winds and driving
rain make putting up the antenna just a tad too exciting!
(new pictures of G3LDO LF station and antenna on web site, see below)
>
>
> As Alan has noted,  some traces show suspicious signs of the
> measuring system clipping, or 'topping out';  this can be seen at
> about the -8dB level on the !' trace, and at 0700z+ on
> the present trace.

Yes, the 'top' sensitivity are probably more important than the bottom when
trying to correlate DFC39 or other commercial stations with amateur stations
in propagation studies.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: =?iso-8859-1?Q?Jos=E9_Manuel?= <jpradoes@telefonica.net>
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References: <001d01c2bee7$4baf55e0$96e9fc3e@l8p8y6>
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META http-equiv=Content-Type content="text/html; charset=iso-8859-1">
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<DIV><FONT face=Arial size=2>Thanks for nice report Mal.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX</FONT></DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE dir=ltr 
style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV 
  style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
  <A title=g3kev.ham@virgin.net href="mailto:g3kev.ham@virgin.net">hamilton 
  mal</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A title=rsgb_lf_group@blacksheep.org 
  href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org</A> 
  </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Saturday, January 18, 2003 12:15 
  PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: EA1PX</DIV>
  <DIV><BR></DIV>
  <DIV><FONT face=Arial size=2>I saw your signal a couple of nights ago at OOO 
  copy. You were calling cq around 137.7 khz. F6BWO was also on at the same time 
  with a very strong signal.</FONT></DIV>
  <DIV><FONT face=Arial size=2>73 de Mal/G3KEV IO94SH</FONT></DIV>
  <DIV>&nbsp;</DIV></BLOCKQUOTE></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
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I am running the "capture machine" again tonight. Shots will appear every 15
minutes at:
http://webpages.charter.net/w1tag/136-1.jpg

The window is from 135920.5 to 135923.5. Avoid 921.05 and 920.92 because of
Loran lines. The screen is set for 60 seconds, normal speed.

Dave: I had a strong line on 921.8 all day yesterday, ending sometime during
the early morning over here. I don't see it right now, but will advise if it
reappears.

John Andrews, W1TAG





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From: "Mike Dennison" <mike.dennison@ntlworld.com>
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> If anyone is prepared to post grabs I'll join in too, 60sec DFCW on
> 135.9228/9 until I fall asleep, probably about 0100.
> Dave G3YXM.

Mine will be QRSS60, too. My mistake.

Mike, G3XDV
http://www.lf.thersgb.net
====================




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If anyone is prepared to post grabs I'll join in too, 60sec DFCW on
135.9228/9 until I fall asleep, probably about 0100.

Dave G3YXM.

----- Original Message -----
From: "Mike Dennison" <mike.dennison@ntlworld.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Saturday, January 18, 2003 7:21 PM
Subject: LF: T/A tonight


> I missed last night's message, but would be happy to transmit tonight
> (Sat/Sun) using QRSS120 on 135.92175kHz for as long as I can.
>
> Mike, G3XDV
> http://www.lf.thersgb.net
> ====================
>
>
>
>
>





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From: "Mike Dennison" <mike.dennison@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Date: Sat, 18 Jan 2003 19:21:39 -0000
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I missed last night's message, but would be happy to transmit tonight
(Sat/Sun) using QRSS120 on 135.92175kHz for as long as I can.

Mike, G3XDV
http://www.lf.thersgb.net
====================





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Pick" <g3yxm@wireless.org.uk>
To: rsgb_lf_group@blacksheep.org
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Steve.

Yes it's excellent. laurie and I did try some T/A tests last night but were
diappointed by the results around 0000utc and went off. It looks from your
latest graph that we should have persevered! The sig/noise at 0600 looks
very good. You need to couple that s/n figure to a big bell in our bedrooms!

Cheers.
Dave Pick
G3YXM.
----- Original Message -----
From: "Steve Dove" <dsp@hifidelity.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Saturday, January 18, 2003 4:40 PM
Subject: Re: LF: LF T/A


> Greetings, fellow static-heads,
>
> Having just returned from a week long business trip to find that
> w3eee.com was still working(!) I'm also gratified to see that it is
> of use . . .   also amazed by the great propagation it captured
> last night.
>
> (1)  Daytime noises
>
> As Peter queried and Alan correctly answered, the daytime
> noises evident are switch-mode 'squirglies' and the odd electric
> drill from construction down the road.  When I'm here (w3eee.com
> is in my downstairs office) I'm able to 'police' the house for known
> grotties that have otherwise not been fixed, 'retired' or 'broken'.
> These are the ones that require 'social engineering' to keep under
> control.  There is a bad one from an adjacent property (300' away)
> about which nothing much can be done.
>
> That said, it is fairly clear if the 'squirglies' are causing false
readings;
> that is the purpose of the 'control' traces from adjacent frequencies.
> And since the 'squirglies' really only affect measurements when no-one
> in their right mind is going to be attempting transatlantic QSOs, for
> the immediate purpose they really don't matter;  obviously for the
> science aspect, they have to go.  This is going to involve a new
> antenna, further away from houses  -  since we're still armpit deep
> in snow, and the weather-man's favourite utterance of late is
> "single digits!" (of degrees Fahrenheit) this isn't going to happen
> any time soon . . .
>
> Incidentally, the signal strength 'bloom' centered around 1400z
> on today's graph is real, and not a 'squirgly'  -  note that the
> noises are well below the DCF trace.
>
> (2)  Data clipping
>
> As Alan has noted,  some traces show suspicious signs of the
> measuring system clipping, or 'topping out';  this can be seen at
> about the -8dB level on the 'Scorcher!' trace, and at 0700z+ on
> the present trace. The actual data figures behind these traces
> still show signs of wiggle, so, I'm really not sure.  However, since
> there is 'plenty of room' at the low-level end of the graph, at the
> next reasonable opportunity (i.e. when the 'puter falls over next)
> I might spend the time to recalibrate it down 10dB, as per Alan's
> suggestion.
>
> Don't worry.  I'll let you know if it happens, just so that people
> won't assume the band's over for the season!
>
>         Cheers,
>
>                 Steve
>
>
>
>
>
>
>
>





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Steve Dove" <dsp@hifidelity.com>
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Greetings, fellow static-heads,

Having just returned from a week long business trip to find that
w3eee.com was still working(!) I'm also gratified to see that it is
of use . . .   also amazed by the great propagation it captured
last night.

(1)  Daytime noises

As Peter queried and Alan correctly answered, the daytime 
noises evident are switch-mode 'squirglies' and the odd electric
drill from construction down the road.  When I'm here (w3eee.com
is in my downstairs office) I'm able to 'police' the house for known
grotties that have otherwise not been fixed, 'retired' or 'broken'.
These are the ones that require 'social engineering' to keep under
control.  There is a bad one from an adjacent property (300' away)
about which nothing much can be done.

That said, it is fairly clear if the 'squirglies' are causing false readings;
that is the purpose of the 'control' traces from adjacent frequencies.
And since the 'squirglies' really only affect measurements when no-one
in their right mind is going to be attempting transatlantic QSOs, for
the immediate purpose they really don't matter;  obviously for the
science aspect, they have to go.  This is going to involve a new
antenna, further away from houses  -  since we're still armpit deep
in snow, and the weather-man's favourite utterance of late is
"single digits!" (of degrees Fahrenheit) this isn't going to happen
any time soon . . . 

Incidentally, the signal strength 'bloom' centered around 1400z
on today's graph is real, and not a 'squirgly'  -  note that the
noises are well below the DCF trace.

(2)  Data clipping

As Alan has noted,  some traces show suspicious signs of the 
measuring system clipping, or 'topping out';  this can be seen at
about the -8dB level on the 'Scorcher!' trace, and at 0700z+ on 
the present trace. The actual data figures behind these traces
still show signs of wiggle, so, I'm really not sure.  However, since
there is 'plenty of room' at the low-level end of the graph, at the
next reasonable opportunity (i.e. when the 'puter falls over next)
I might spend the time to recalibrate it down 10dB, as per Alan's 
suggestion.  

Don't worry.  I'll let you know if it happens, just so that people
won't assume the band's over for the season!

        Cheers,

                Steve








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "James Moritz" <j.r.moritz@herts.ac.uk>
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At 12:09 17/01/2003 -0500, you wrote:

><< This is the wrong way to achieve high impedance (and good IMD),
>  it is no need to keep the "source current low" {etc} >>
>
>I do not see anything in the Web page that suggests keeping the source
>current low.  It only says "reasonable amount," which I took to mean "be sure
>to use enough" to keep IMD low.

Dear LF Group,

The output impedance of a follower is roughly the inverse of it's 
transconductance, ie. 1/gm. A J310 JFET has a gm of about 10 - 20 mS, so 
the output impedance is roughly 50 - 100 ohms. To get low distortion, and 
gain close to unity with such a follower requires that the load it is 
driving should be much greater than the output impedance of the follower. 
So a J310 source follower would be fine if driving several hundred ohms or 
greater, but not for a 50 or 75 ohms system.

To get around this, one could use a special FET like the CP640 device used 
in the AMRAD active antenna circuit, with much higher gm. A small power 
MOSFET would give a low output impedance, but rather high input 
capacitance. Bipolar transistors have much higher gm (roughly Ic/25mV), but 
would have relatively low input impedance, in the kilohm range, and be 
relatively noisy with a high source impedance. Various high speed op-amps 
and IC buffers can be used, but they tend to be quite noisy.

A cheap and easy alternative is to use a compound follower, with JFET and 
bipolar followers cascaded. I tried the one shown in the attachment - Zin 
is basically 500k in parallel with the FET capacitance, the gain with 50ohm 
load is about 0.95. The noise at 136kHz with the input shorted was about 
0.05uV in 400Hz BW. About 1V RMS can be applied to the input before there 
is much distortion whilst driving 50ohms, so it ought to be OK with most 
antennas, and is probably better than most receivers. The FET was a J310, 
but other devices with Idss > about 8mA should be OK. A lower gm device 
with lower Idss could be used if the 100R resistor were increased in value, 
but would be noisier. The output BJT used was a 2N3053, but can be a wide 
range of small power transistors with Hfe > 50 when biased to 30mA or so 
and fT in the 10s of MHz - eg. BD131, BFY50, ZTX650 etc. Zout is a few ohms 
- If driving a capacitive load, a resistor in series with the output of 10 
- 20 ohms will prevent oscillation. Extra decoupling will be required if 
the 12V supply is noisy.

Using spectrogram software to monitor the band for signals works very well 
- it allows you to see CW signals that are inaudible, which you can then 
try to "zoom in" using a narrow filter. Although you can't copy the morse 
from the screen display, you can detect the presence of signals that are 
too weak to hear even in the narrowest filter, whilst monitoring the whole 
band segment at once. Some of the spectrogram programs have DSP audio 
filters built in, too.

The broadcast station noises M0WYE is hearing may well be "Luxembourg 
effect", where cross-modulation of the DCF39 carrier by the BC signals 
occurs in the ionosphere, and is often quite strong at my QTH. Usually I 
can here the audio of at least two stations at once.

Hope this is helpful,

Cheers, Jim Moritz
73 de M0BMU
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<DIV><FONT face=Arial size=2>I have been watching the discussion about Filters 
on here with interest. With DCF39 you have two modes to cope with, the carrier 
and the data bursts. A notch filter does not handle this condition very well, 
because of the sudden bandwidth extension when the data burst occurs. If you 
cater for this then you also desense/attenuate adjacent frequencies of interest 
around 137.7 khz a&nbsp;popular frequency for QRS. </FONT></DIV>
<DIV><FONT face=Arial size=2>The preferred approach would be a 
tight&nbsp;Bandpass filter at the front end of the RX and good IF selectivity as 
narrow as you&nbsp; can manage. This way you will be able to hear/see even the 
weakest of signals. Some of the&nbsp; weaker signals on the band at my qth 
are&nbsp;perfectly readable but only in a very narrow bandwidth, giving a good 
signal over noise. These same signals are barely detectable with&nbsp;a wide 
bandwidth, either aural or visual.&nbsp;To&nbsp;ensure that nothing of interest 
is missed on 73 or 136 khz it is preferable to&nbsp;tune&nbsp;the band 
slowly&nbsp;with very narrow selectivity.&nbsp;</FONT></DIV>
<DIV><FONT face=Arial size=2>To try and monitor the whole band visually with the 
appropriate bandwidth selected does not work for weak signal reception, these 
weak signals would be buried in the noise and not detectable.</FONT></DIV>
<DIV><FONT face=Arial size=2>Most LF operators suffer 
from&nbsp;poor&nbsp;reception on LF because of environmental noise pickup and 
the last thing needed is to attenuate signals even more with 
unnecessary&nbsp;notch filters.&nbsp;The&nbsp;best approach is to use a good 
sensitive RX with good IF selectivity&nbsp;plus a DSP audio filter (or 
IF)&nbsp;and if necessary a well designed tight bandpass filter (tuned would be 
an advantage)&nbsp;at&nbsp;the front end of the RX.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de 
Mal/G3KEV&nbsp;&nbsp;&nbsp;</FONT></DIV></BODY></HTML>

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<DIV><FONT face=Arial size=2>I saw your signal a couple of nights ago at OOO 
copy. You were calling cq around 137.7 khz. F6BWO was also on at the same time 
with a very strong signal.</FONT></DIV>
<DIV><FONT face=Arial size=2>73 de Mal/G3KEV IO94SH</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
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It is 0730.
The W3EEE continues to show an excellent CFH39 signal (-6 or -7 dB) so I
will keep up the 137.769+ transmissions.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




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John Andrews said
>
> A very nice "Q" toward the end! (from Laurie). The other signal is a line
that's been there
> all day. I'm not sure of the source.
>
The W3EEE page showed CFH39 to be not so good at the time
At the moment 0645Z it is very good so I am transmitting on 1377695 for a
possible capture by KL1X

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




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From: "John Andrews" <w1tag@charter.net>
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Laurie,

> Hi John,
> I transmitted on 135,921.25 from 2330 until 0030.
> Saw some traces on my freq. and a stronger signal above me, who ?   Closed
> down since prop. obviously not too good.

A very nice "Q" toward the end! The other signal is a line that's been there
all day. I'm not sure of the source.

John Andrews



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From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
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Hi John,
I transmitted on 135,921.25 from 2330 until 0030.
Saw some traces on my freq. and a stronger signal above me, who ?   Closed
down since prop. obviously not too good. Thanks for the captures. 73 Laurie.




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<DIV><FONT face=Arial size=2>John W1TAG.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I tried some test transmissions on 135.923 DFCW but 
nothing seen up to 2400. Laurie or Peter (don't know which) is on 135.921 and is 
just visible on your 23.57 capture.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73.</FONT></DIV>
<DIV><FONT face=Arial size=2>Dave G3YXM.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Hugh" <m0wye@thersgb.net>
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Hi Alan, LF Group,
I found out why the pot setting was so critical. I measued the value for
best notch and it was about 330 ohms ! I have replaced the 25k with a 1k pot
and it is much better behaved. I have also added a dual gang 500pF airspaced
tuning cap in parallel with the existing caps (22n and 4n7) and that now
brings it down onto DCF39 nicely.

I set up the antenna this afternoon and have been experimenting with "real"
signals.
I can now reduce DCF39 from -54dBm without the filter in circuit, to -112
dBm with the filter. When a burst of modulation occurs the level rises by
10dB suggesting the frequency shift is fairly small compared to the size of
the notch.

I have continued to use the filter with the 12 : 1 toroidal transformer to
achieve matching, so I still have an overall reduction in signal from the
antenna due to the turns ratio. I generated some signals that could be
picked up by the antenna, and found that a signal at 136.562 kHz is reduced
by 23dB and one at 137.700 kHz is reduced by 27dB.

But the main thing is the filter does the job. I can set the SLM to 3.1kHz
band width and not be totally swamped by DCF39. So now I can leave Argo
running and see what is happening right across the band. For example I was
able to receive DJ9IE sending ordinary morse on 136.590 by spotting the line
appearing on the screen. And someone's sending some QRSS40 (?) on 137.800
and just now (23:15)I've got some more long dots or dashes around 137.800.
This is good. Before I had to tune around the band with the 80Hz filter to
find things and probably missed lots of stuff.

However getting rid of the worst interfering station does mean that one can
hear other flaws in the set-up. I can now hear a broadcast station very
faintly, and I guess it must be resonsible for some patterning on the
screen.

73
Hugh M0WYE




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From: =?iso-8859-1?Q?Jos=E9_Manuel?= <jpradoes@telefonica.net>
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<DIV><FONT face=Arial size=2>Hi Group:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I copy transmissions&nbsp;on 132.930 and 133.230 
kHz.</FONT></DIV>
<DIV><FONT face=Arial size=2>Can anyone to&nbsp;confirm me&nbsp;if they are of 
the Datatrak System and where are the TX located?</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX</FONT></DIV></BODY></HTML>

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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
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I'll be away from home until 0300 or so, but I left the receiver on 135.922
this morning, with the auto-capture running. Shots are being posted every 15
minutes to:

http://webpages.charter.net/w1tag/136-1.jpg

Given that I was listening to the EU AM BC stations on 183 and 162 kHz at 10
AM local time this morning, conditions can't be too bad. Anyone who wants to
give it a try is welcome.

John Andrews, W1TAG




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From: "Vernall" <vernall@xtra.co.nz>
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Alan G3NYK,

OK on the notch filter design, but for a high impedance load.

I have often wanted to try a notch filter in a low impedance feeder, for
such purposes as reducing a TV line oscillator harmonic or other carrier
type of unwanted signal that is a few kHz from the wanted signal, as the
unwanted carrier can paralyse a noise blanker from working effectively (the
bandwidth of the noise blanker is necessarily relatively wide).

On searching for information on notch filters I found a very good series of
articles in Wireless World.  Part 2 of the series in September 1979 deals
with low impedance notch filters.  The circuit used in "example 4" is a
variant of what you used, with L and C in the leg to ground.

If you can locate old copies of WW you could try modelling a low impedance
notch filter.

73, Bob ZL2CA




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In a message dated 1/17/03 11:52:04 AM Eastern Standard Time, 
jan-martin.noding@telenor.com writes:

<< This is the wrong way to achieve high impedance (and good IMD),
 it is no need to keep the "source current low" {etc} >>

I do not see anything in the Web page that suggests keeping the source 
current low.  It only says "reasonable amount," which I took to mean "be sure 
to use enough" to keep IMD low.

73
John




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From: jan-martin.noding@telenor.com
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Hi,

noticed something I'd wish to comment further, ref. quoted text 
from http://www.alan.melia.btinternet.co.uk/BR-t-Notch.htm

>As far as I can see at the moment the only problem is that the 
>output of the filter must not be loaded too heavily, so a FET 
>source follower is probably called for ( J310 running reasonable 
>amount of source current to keep the IMDs down ??). 

This is the wrong way to achieve high impedance (and good IMD),
it is no need to keep the "source current low" or whatever,
don't understand where one could get such assumptions from,

A simple source follower has also very low gain, probably around 0.2-0.4x 
voltage gain, but this is easily improved using an extra PNP device running
with 10-30mA, so it may even have higher gain than unity, and to improve 
the input impedance you add some positive feedback to the gate.

A more complicated solution using J310 fet was shown in Radcom some time ago,
described for my frame antenna, but I use it for my active antenna on the roof

73
Jan_Martin
LA8AK (in JO38XC)  [mailto:LA8AK@Online.no]
N4623-Kristiansand (tel.: +47-380-87178 Home)(38052660 Work 90777126 Mobile)
http://www.laud.no/la6nca/LA8AK/ 

----- Original Message ----- 
From: Alan Melia [mailto:Alan.Melia@btinternet.com]
Send: 17. januar 2003 10:45


Hi all, a belated Chrismas present to the Group. As a result of a discussion
with Hugh M0WYE,  I calculated, and simulated a Bridged-T Notch Filter for
136kHz, which should reduce the level of DCF39 by about 30dB which only
giving about 2 or 3 dB loss at the top of the band. Hugh has made up the
filter and from workbench tests it seems promising. It occurs to me that
this may be of interest to those living closer to Burg that we do.

Details on http://www.alan.melia.btinternet.co.uk/BR-t-Notch.htm

We would be interested if anyone finds it useful.

Cheers de Alan G3NYK
alan.melia@btinternet.com
http://www.alan.melia.btinternet.co.uk






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From: jan-martin.noding@telenor.com
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Hi all,

It is a problem that you have to attenuate 138.8 and the lower shift frequency, which is active 
every tenth seconds or so. So I agree to the solution Hans-Joachim suggest using bandpassfilter.

A tuned two stage filter is fairly simple, but it is also an idea to use high Q frame antennas,
my frame antennas attenuate 138.9 by 26dB when listening to 136.0kHz

73,
Jan-Martin, LA8AK
---
J M Nøding, Datakvalitet, TTS, Kristiansand
Telefon 0047-380-52660, 9077-7126 (QTH: 0047-380-87178)



-----Opprinnelig melding-----
Fra: Hans-Joachim Brandt [mailto:hajo.brandt.dj1zb@t-online.de]
Sendt: 17. januar 2003 13:35
Til: rsgb_lf_group@blacksheep.org
Emne: Re: LF: Notch for DCF39


Hi all,

as I had to design a group-delay controlled band-pass filter once, needing two pole circuits at both sides of the pass-band I have also been designing such a filter for the amateur LF band using the ARRL Radio Designer, but have not completed it, because I am living in the southeast of Germany (JN68GN) and do not need it. But concerning the LF activity in eastern Germany I have also thought that DCF39 at Burg, close to Magdeburg, would severely hinder such activity.

When DL2HRE, Edgar, located at Bernburg, half way between Magdeburg and Halle, appeared on the LF band, I have asked him how he has managed to listen on LF. He is using an rx input filter consisting of seven resonant circuits employing pot cores, capacitively top-coupled, centered at 136.4 kHz. I also feel that this should not be the optimum solution; a filter with poles (one for DCF39 and perhaps another for SVX) would be better, but so far Edgar does not seem to look for a filter employing poles. 

Anyway, his rx sensitivity on the LF band using his 250 meters long antenna seems to be very good. He has become the utmost station in the northeast of Germany which I can contact reliably on LF in normal CW. So far I have not found a comparable station in the northwest of Germany. DL2HRE has also told me of another east German LF station at Plauen (the callsign I have not noted, sri) but so far I have not heard it. 

DL2HRE has no internet connection.

73 Ha-Jo, DJ1ZB 


"Alan Melia" <Alan.Melia@btinternet.com> schrieb:
>Hi all, a belated Chrismas present to the Group. As a result of a discussion
>with Hugh M0WYE,  I calculated, and simulated a Bridged-T Notch Filter for
>136kHz, which should reduce the level of DCF39 by about 30dB which only
>giving about 2 or 3 dB loss at the top of the band. Hugh has made up the
>filter and from workbench tests it seems promising. It occurs to me that
>this may be of interest to those living closer to Burg that we do.
>
>Details on http://www.alan.melia.btinternet.co.uk/BR-t-Notch.htm
>
>We would be interested if anyone finds it useful.
>
>Cheers de Alan G3NYK
>alan.melia@btinternet.com
>http://www.alan.melia.btinternet.co.uk
>
>
>
>






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Hi all,

as I had to design a group-delay controlled band-pass filter once, needing two pole circuits at both sides of the pass-band I have also been designing such a filter for the amateur LF band using the ARRL Radio Designer, but have not completed it, because I am living in the southeast of Germany (JN68GN) and do not need it. But concerning the LF activity in eastern Germany I have also thought that DCF39 at Burg, close to Magdeburg, would severely hinder such activity.

When DL2HRE, Edgar, located at Bernburg, half way between Magdeburg and Halle, appeared on the LF band, I have asked him how he has managed to listen on LF. He is using an rx input filter consisting of seven resonant circuits employing pot cores, capacitively top-coupled, centered at 136.4 kHz. I also feel that this should not be the optimum solution; a filter with poles (one for DCF39 and perhaps another for SVX) would be better, but so far Edgar does not seem to look for a filter employing poles. 

Anyway, his rx sensitivity on the LF band using his 250 meters long antenna seems to be very good. He has become the utmost station in the northeast of Germany which I can contact reliably on LF in normal CW. So far I have not found a comparable station in the northwest of Germany. DL2HRE has also told me of another east German LF station at Plauen (the callsign I have not noted, sri) but so far I have not heard it. 

DL2HRE has no internet connection.

73 Ha-Jo, DJ1ZB 


"Alan Melia" <Alan.Melia@btinternet.com> schrieb:
>Hi all, a belated Chrismas present to the Group. As a result of a discussion
>with Hugh M0WYE,  I calculated, and simulated a Bridged-T Notch Filter for
>136kHz, which should reduce the level of DCF39 by about 30dB which only
>giving about 2 or 3 dB loss at the top of the band. Hugh has made up the
>filter and from workbench tests it seems promising. It occurs to me that
>this may be of interest to those living closer to Burg that we do.
>
>Details on http://www.alan.melia.btinternet.co.uk/BR-t-Notch.htm
>
>We would be interested if anyone finds it useful.
>
>Cheers de Alan G3NYK
>alan.melia@btinternet.com
>http://www.alan.melia.btinternet.co.uk
>
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hello all,
Alan wrote:
> Hugh has made up the filter and from workbench tests it seems promising.

Yes it does what it says on the tin ... I got a notch depth of 47dB.
I used a Panasonic ELC08D101E coil available from RS Components part no.
233-5213.
I unwound it and found it had 50 turns. Rewinding with 36 turns and tapping
at 18 gives the correct 50uH.
I think a multiturn pot (or a fixed value resistor in series with a pot)
might be best as it is a very sharp adjustment with a single turn type. I
used polycarbonate film type capacitors (hen's teeth now Bayer don't make
the film any more)
Alan and I are presently discussing impedance matching, as it is 100 ohms
in, 10k out.
73
Hugh M0WYE
http://www.m0wye.thersgb.net/lf.htm

>
> Details on http://www.alan.melia.btinternet.co.uk/BR-t-Notch.htm
>





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Hi Gary,

many thanks for the report and the capture. It's always nice to see what
ones signal looks like.

73 de,

Ian GI8AYZ/MI0AYZ



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<html>
Mal,<br><br>
Meanwhile I collected all I need to contruct the loop. But unfortunately
I have to work for a living and I also want to spend some time with my
wife and daughter so hobby time was rather limited over the last
months.<br>
But the plan is still alive and the loop will be contructed one day
...<br><br>
73, Rik&nbsp; ON7YD<br><br>
At 09:59 17/01/2003 +0000, you wrote:<br>
<blockquote type=cite class=cite cite><font face="arial" size=2>I wonder
how Rik/ON7YD is getting on with the proposed big loop that was discussed
some time back. </font><br>
<font face="arial" size=2>73 de Mal/G3KEV</font><br>
&nbsp;</blockquote></html>

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From: "hamilton mal" <g3kev.ham@virgin.net>
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<DIV><FONT face=Arial size=2>I wonder how Rik/ON7YD is getting on with the 
proposed big loop that was discussed some time back. </FONT></DIV>
<DIV><FONT face=Arial size=2>73 de Mal/G3KEV</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi all, a belated Chrismas present to the Group. As a result of a discussion
with Hugh M0WYE,  I calculated, and simulated a Bridged-T Notch Filter for
136kHz, which should reduce the level of DCF39 by about 30dB which only
giving about 2 or 3 dB loss at the top of the band. Hugh has made up the
filter and from workbench tests it seems promising. It occurs to me that
this may be of interest to those living closer to Burg that we do.

Details on http://www.alan.melia.btinternet.co.uk/BR-t-Notch.htm

We would be interested if anyone finds it useful.

Cheers de Alan G3NYK
alan.melia@btinternet.com
http://www.alan.melia.btinternet.co.uk




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: rsgb_lf_group@blacksheep.org
References: <006601c2ba97$9ac00a20$6507a8c0@Main> <000401c2bc1d$9af64720$c6e086d4@erica> <000601c2bdc1$c4577940$d1e486d4@erica>
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Hi Peter, Steve often gets these daytime bursts. He is not sure what they
are often drifty TVs we suspect but also DIY noises. The night-time signal
was actually quite good again last night between 0300 and about 0730z. It
did not go into limiting but there were few deep troughs. I am trying to see
whether it is possible to get a "datum" line on the plot with some idea of
"average conditions" so far no ideas.

Cheers de Alan G3NYK
alan.melia@btinternet.com

----- Original Message -----
From: "g3ldo" <g3ldo@ukonline.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: 17 January 2003 00:45
Subject: LF: T/A prop


>
>
>  The W3EEE site shows a large burst of noise late afternoon followed by
> suppressed conditions
> What happened?
>
> Regards,
> Peter, G3LDO
>
> e-mail <g3ldo@ukonline.co.uk>
>
> Web <http://web.ukonline.co.uk/g3ldo>
>
>
>
>
>




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From: "g3ldo" <g3ldo@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <006601c2ba97$9ac00a20$6507a8c0@Main> <000401c2bc1d$9af64720$c6e086d4@erica>
Date: Fri, 17 Jan 2003 00:45:41 -0000
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 The W3EEE site shows a large burst of noise late afternoon followed by
suppressed conditions
What happened?

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>







From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "G4WGT" <g4wgt@talkgas.net>
To: rsgb_lf_group@blacksheep.org
Date: Thu, 16 Jan 2003 19:11:53 -0000
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Subject: LF: RE: Re:136 Mon.
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Hi Ian & LF,

I wrote :-

If of any interest here is a screen shot of your QRSS on Monday night from
across the water in Lancashire, IO87QP.

Locator should be IO83QP.

73

Gary    G4WGT

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of Ian Kyle
Sent: 14 January 2003 20:21
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re:136 Mon.


Thanks to Jim M0BMU for my first  two-way 136MHz QSO last night but nothing
heard or seen of anybody else.

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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "G4WGT" <g4wgt@talkgas.net>
To: rsgb_lf_group@blacksheep.org
Date: Thu, 16 Jan 2003 18:37:41 -0000
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Subject: LF: RE: Re:136 Mon.
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Ian & LF,

If of any interest here is a screen shot of your QRSS on Monday night from
across the water in Lancashire, IO87QP.

73

Gary  G4WGT.

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of Ian Kyle
Sent: 14 January 2003 20:21
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re:136 Mon.


Thanks to Jim M0BMU for my first  two-way 136MHz QSO last night but nothing
heard or seen of anybody else.
Obviously the system works sort of,  and the much-put-upon BK actually
manages to get up to 125 w out on that band but there are marked anomalies
in the inductance settings required - at maximum antenna current (1+A)  the
reqired L is far too high and replacing the antenna with an equivalent
circuit produces resonance at around 95KHz.
There's summat cockeyed somewhere, so more work is needed to ascertain
whether it's the mathematics or the hardware.
Howsomever,  if anyone feels that way inclined I am willing to try a sked or
two.

73 de,

Ian  GI8AYZ/MI0AYZ

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--------------040309070006010706010208--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: =?iso-8859-1?Q?Jos=E9_Manuel?= <jpradoes@telefonica.net>
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<DIV><FONT face=Arial size=2>Hi Group:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I´ve changed some e-mails with Marcelo (LW2ETU) and 
Daniel (LU8EDR) about the beginning of LF activity in Argentina, and they told 
me about their inmediate projects. I think they will be here soon in the 
reflector. I told them about the interest in Europe to make TA test with South 
America. They will&nbsp;try to&nbsp;receive &nbsp;DCF39 
transmissions.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Perhaps Alan can make any comment about the 
possibilities of this 11000 km path.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Only indirectly related but the North East/South West trans Atlantic paths
between Uk and Antarctica  (6734S 6808W) in Northern Hem winter times
1979/80  (same sort of flux as now?) produced near nightly reception of
Capital (ol?) Radio from London on 1.548MHz .... Good enough to pipe thru
to our small bar at Rothera Base, Adelaide Island. around our local
midnight 0300-0500Z - around 16,000 Km most sea path.



Laurence KL1X (VP8SB)
Presently  onroute to C America



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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At 20:21 14/01/2003 +0000, you wrote:
>Thanks to Jim M0BMU for my first  two-way 136MHz QSO last night but nothing
>heard or seen of anybody else.

Dear Ian, LF Group,

Very pleased to be your 1st 136kHz QSO - and also to have a first LF QSO 
with Hugh, M0WYE. MI0AYZ was just audible here in Hatfield, so getting out 
quite well with 1 amp. I guess a normal CW contact would be possible under 
quiet band conditions, but would have been difficult on Monday night due to 
the strong "Luxembourg effect" splatter I was experiencing.

M0WYE was quite a weak QRSS3 signal here, but no problem with copy. With 
0.1A into a fairly small antenna, this is quite good going too! Hugh was 
also able to see some of Ian's signal, but apparently not the other way round.

Cheers, Jim Moritz
73 de M0BMU



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Andrews" <w1tag@charter.net>
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Peter,

No complete ID's, but a lot better results than we had Sunday night. I note
that the Loran line on 921.6 from Newfoundland was quite visible tonight, as
it has been on other good evenings. I will pay closer attention to it in the
future.

John Andrews, W1TAG





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> Captures of 135.922 kHz are being posted every 15 minutes at:
>
> http://webpages.charter.net/w1tag/cap-1.jpg
>

John has captured some fragments of my wobbly signal, which appears to be
cycling in frequency by about 0.1Hz. I'm not sure of the reason for this.
The temperature in the transmitter shed seem stable but there is a strong
wind blowing. I will have to put the DDS in a draught proof box! The longer
term strategy to have it in the inside shack with a divide by 10 unit to
give a 0.1Hz resolution and improved stability.
DCF39 has taken a nose dive but there again it often does after midnight our
time - and then picks up again.
I will transmit until around 0100Z and then ZZZZZZZZZ.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>






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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
References: <11a.1ceb118c.2b534ef7@aol.com> <18Y3Jz-24310KC@fwd10.sul.t-online.com>
Date: Tue, 14 Jan 2003 23:40:21 -0000
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Captures of 135.922 kHz are being posted every 15 minutes at:

http://webpages.charter.net/w1tag/cap-1.jpg

John Andrews, W1TAG



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Date: Tue, 14 Jan 2003 23:01:11 +0000
From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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Subject: Re: LF: Re: T/A prop
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Push hard, I'm looking.  Posting to:

http://www.w4dex.com/argo/135khz.jpg

Dex


g3ldo wrote:
> 
> a quick look at Steve's site shows that the DCF39 level is -12dB relative
> level at 2230.
> I will put out a test transmission on 1359... whatever it was I used last
> time. QRSS60 I guess unless DCF39 goes through the roof.
> 
> Regards,
> Peter, G3LDO
> 
> e-mail <g3ldo@ukonline.co.uk>
> 
> Web <http://web.ukonline.co.uk/g3ldo>


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a quick look at Steve's site shows that the DCF39 level is -12dB relative
level at 2230.
I will put out a test transmission on 1359... whatever it was I used last
time. QRSS60 I guess unless DCF39 goes through the roof.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




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From: "Ian Kyle" <ian.gi8ayz@virgin.net>
To: rsgb_lf_group@blacksheep.org
References: <LEEGIKOMHIEKBPDOHLOIIECECCAA.we0h@gentekcom.com> <003801c2b9e6$7a85c940$0500a8c0@charter.net> <5.1.0.14.0.20030113182353.00af0e30@gemini.herts.ac.uk>
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Thanks to Jim M0BMU for my first  two-way 136MHz QSO last night but nothing
heard or seen of anybody else.
Obviously the system works sort of,  and the much-put-upon BK actually
manages to get up to 125 w out on that band but there are marked anomalies
in the inductance settings required - at maximum antenna current (1+A)  the
reqired L is far too high and replacing the antenna with an equivalent
circuit produces resonance at around 95KHz.
There's summat cockeyed somewhere, so more work is needed to ascertain
whether it's the mathematics or the hardware.
Howsomever,  if anyone feels that way inclined I am willing to try a sked or
two.

73 de,

Ian  GI8AYZ/MI0AYZ



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Rik Strobbe schrieb:
> Hello Uwe,
>
.........
> How did you measure this phase shift ? In the past I have noticed that 
> measuring waveforms at the gate of a FET with the drain open can give very 
> strange results ...
>
> 73, Rik  ON7YD
>
>

Dear Rik, Alberto, Jim es all,

tks for the responses. 

yes Rik, the drains were open. the PSU was not finished. 

but today I connected in a first step 50V operating voltage to the PA.

I can`t belief it: the phase shift has diminished to abt 2dgr.

I know from my other PA, a two channel N-/P-MOSFET equipment, that the 
scope is ok. but I didn`t measure without the PA operating voltage 
connected.

yes, the Cgs of the IRFP450/451 is vy high. that is the reason I use in 
the other PA many of the weaker MOSFETs IRF620 for the one channel 
and IRF9622 for the other. you don`t need the high input power.

tks Alberto es Jim that you do not blame on me or my (in)ability doing the 
things right but suspecting the scope.

regards
Uwe/dj8wx




 



 

 



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Hello Uwe,

power-FETs do have rather large gate-source capacitances that can differ 
from FET to FET. For the popular IRF450 Cgs is about 2nF, variations 
between FET's can easily be a few 100pF. If the FETs are driven from a 
rather high-Z source the variations in Cgs might cause a phase shift, 
although 10 degrees look very much to me.
How did you measure this phase shift ? In the past I have noticed that 
measuring waveforms at the gate of a FET with the drain open can give very 
strange results ...

73, Rik  ON7YD


>Hi all,
>
>guess many of you built the G0MRF-Quarter-Kilowatt-Amplifier.
>I did. the PSU is not finished yet.
>
>got some trouble with the phase of the 137kHz sines
>(es triangular and rectangular) measured at the gates of the MOSFETs.
>there is a diff btwn the two channels of estimated 10degr.
>that means parasitic oscillation if operating the PA, doesn`t it.



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From: "hamilton mal" <g3kev.ham@virgin.net>
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Date: Tue, 14 Jan 2003 09:38:10 -0000
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
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<DIV><FONT face=Arial size=2>Last night might have been better for&nbsp; LF TA 
dx because 160 metres was very good. I worked VK6HD at 579 each way and heard 
DU9 and a few UA9 stns active, plus a lot of Eu acty.</FONT></DIV>
<DIV><FONT face=Arial size=2>Did'nt stay around late to look for North American 
acty. </FONT></DIV>
<DIV><FONT face=Arial size=2>73 de Mal/G3KEV</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

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Subject: Re: LF: push/pull
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James Moritz wrote:

> [...]
> Another possibility is that the circuit is OK, but the scope is not 
> triggering correctly - this sometimes happens if the scope is set to 
> "mixed" trigger, if it has this setting.
> [...]


Tek scopes have the 'Alternate' and 'Chopped' settings on the vertical 
amplifier
plug-in, usually. Don't use 'Alternate' for phase comparisons, results 
are meaningless.
Only 'Chopped' is reliable in this case.

73  Alberto  I2PHD




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Dear Hugh, LF group,

Will aim to be QRV tonight about 2000. After the last few nights of 3am, 
think I'll have an early night though!

Cheers, Jim Moritz
73 de M0BMU



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At 22:42 12/01/2003 +0100, you wrote:
>Hi all,
>
>guess many of you built the G0MRF-Quarter-Kilowatt-Amplifier.
>I did. the PSU is not finished yet.
>
>got some trouble with the phase of the 137kHz sines
>(es triangular and rectangular) measured at the gates of the MOSFETs.
>there is a diff btwn the two channels of estimated 10degr.
>that means parasitic oscillation if operating the PA, doesn`t it.

Dear Uwe,

Assuming this is G0MRF's linear PA, the circuit is completely symmetrical. 
So if there is any phase shift in the drive circuit, the drive waveforms 
will be phase shifted by the same amount by the time they reach the gates 
of each MOSFETs. So the drive waveforms should always be 180degrees out of 
phase unless one of the components on one side of the circuit is different 
from it's counterpart on the other side. I would start by checking that all 
components on the input side of the circuit are correct.

Another possibility is that the circuit is OK, but the scope is not 
triggering correctly - this sometimes happens if the scope is set to 
"mixed" trigger, if it has this setting.

Cheers, Jim Moritz
73 de M0BMU



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Thankyou, Ian,
I'll start around 20:00 and carry on 'til after 21:00.
I shall use QRSS3, I don't think the signal source is stable enough for
anything more.
(I'm still waiting for Farnell to deliver the Atmel part to build a DDS
source)
73
Hugh


----- Original Message -----
From: "Ian Kyle" <ian.gi8ayz@virgin.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Monday, January 13, 2003 3:51 PM
Subject: LF: Re: QRSS transmission tonight


> HI there Hugh,
> Will look for you tonight but not available until about 2045z.
> What mode - QRSS3 or QRSS10?
>
> Radiating a return sgnal will be difficult but I shall try. Like you, 1A
> antenna current is about as much as my setup can manage.
>
> Will check the reflector again about 1800z
>
> 73 de,
>
> Ian  MI0AYZ
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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<DIV><FONT face=Arial size=2>Generally when 160 metres propogation&nbsp;is good 
the lower freqs are also good. This past couple of nights were not good for dx 
propagation although I did hear a UA0 and JA7NI at 559 last night, but the usual 
crowd of&nbsp;UA9,&nbsp;UA0 bar one&nbsp;to the East&nbsp;were not audible. I 
did not hear any W/VE either to the West, a bad sign for&nbsp;the lower 
LF&nbsp;freqs transatlantic. There could be exceptions but this is generally the 
rule from this QTH.</FONT></DIV>
<DIV><FONT face=Arial size=2>At this time of year&nbsp;on occassions during my 
late evening&nbsp;I have worked at least 20 JA stns in succession plus&nbsp;any 
amount of&nbsp;&nbsp;mainly East Coast USA&nbsp;and Canadian stations. Early 
morning is best for me to the West&nbsp;Coast W6, W7 and VE7&nbsp;and KL7 
Alaska</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de Mal/G3KEV</FONT></DIV>
<DIV><FONT face=Arial size=2>&nbsp;&nbsp;&nbsp;</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Ian and all:

I´ll try to copy to both of you.
I´d like to make my fifth country, I never copied any GI station on 137.

73 de José, EA1PX


> Will look for you tonight but not available until about 2045z.
> What mode - QRSS3 or QRSS10?








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HI there Hugh,
Will look for you tonight but not available until about 2045z.
What mode - QRSS3 or QRSS10?

Radiating a return sgnal will be difficult but I shall try. Like you, 1A
antenna current is about as much as my setup can manage.

Will check the reflector again about 1800z

73 de,

Ian  MI0AYZ



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To: rsgb_lf_group@blacksheep.org
X-Mailer: Lotus Notes Release 5.0.8  June 18, 2001
Message-ID: <OFB3B40B00.D4BB1694-ON89256CAD.0054075C@ppco.com>
From: "Laurence J Howell" <L.Howell@conocophillips.com>
Date: Mon, 13 Jan 2003 06:24:24 -0900
X-MIMETrack: Serialize by Router on BVLNOTES07/CIT/Phillips Petroleum/us(Release 5.0.7 |March 21, 2001) at 01/13/2003 09:24:26 AM
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Subject: LF: Alaska monitoring 24 hours until 3rd Feb
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Im on route to Costa Rica but the receive system is on (TS 870 and Cap top,
bottom loaded resonated vertical at 90ft)  and capture  will remain on
until my return to Alaska on 3rd Feb. Ill have a few Jpegs to look
thru....cant export jpegs  to the net in real time but that will come.


Pray for :
No Stratwarm
No Thunderstorms
Low A/Ks
Low Flux
Anything that makes the Au belt or H proton number increase etc etc etc!

Using QRSS 60  centered on 137.7700 +-1.5 Hz.

Avoid 137.7700 Loran line.

Laurence  KL1X    BP41XD Anchorage.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <3E22C9F9.54D7F50F@diolog.de>
Date: Mon, 13 Jan 2003 14:15:22 +0000
From: "Fabian Kurz" <fk@diolog.de>
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References: <11a.1ceb118c.2b534ef7@aol.com> <18Y3Jz-24310KC@fwd10.sul.t-online.com>
Subject: Re: LF: TA Test
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This is a multi-part message in MIME format.
--------------010005000302060806010802
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Yet another screenshot from JO32QG ...

73, Fabian DJ1YFK


jannsen schrieb:

> DL4YHF@aol.com schrieb:
> > Hello group,
> >
> > received this colorful image under adverse conditions: Random wire plugged
> > into a TS850, tuned to 135.92 in "CW" (usb), pitch = 650 Hz, so 650Hz on
> > screenshot is near 135.920 kHz . The decibel scale is not calibrated against
> > anything, so just a relative measure.
> >
> > The different power levels received here in JO42FD are quite strange, but see
> > for yourself.
> >
> > Must go to bed, work starts early. I would appreciate a similar test from
> > saturday to sunday, better for the "working class" (and especially to those
> > not QRV from home). Good luck to everyone.
> >
> > Cheers,
> >  Wolf  DL4YHF (not at DF0WD)
> >
> >
>
> Hi all,
>
> an other checkered midnights painting (SpecLab shot). see attachment.
>
> regards
>
> Uwe/dj8wx/jo43sv
>
>   ------------------------------------------------------------------------
>  [Image]

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Date: Mon, 13 Jan 2003 13:47:46 +0000
From: "Dexter McIntyre" <dmcintyre@att.net>
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To: "RSGB LF" <rsgb_lf_group@blacksheep.org>, 
 "lowfer" <lowfer@mailman.qth.net>
Subject: LF: [Fwd: AW: HBG 75 kHz transmitter]
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On several occasions the HBG plot showed an almost instant drop and
return of the signal received here in NC.  These drops didn't look like
propagation events so I emailed the HBG engineer to see if perhaps these
events were transmitter related.  Below is the response I received.

Dex 


Gregor.Dudle@metas.admin.ch wrote:
> 
> Sir
> 
> Thank you very much for your message. It is a nice to hear that our signals
> can be received in North Carolina.
> 
> As for the signal drops, I confirm that our transmitter was down for a short
> time on both occasions you mention in your mail. Both events were due to bad
> weather conditions (strong winds) in the antenna area.
> 
> Jan 7   05:57 to 06:22 (UTC) (I'm recording a measurement every 5 minute,
> therefore the real downtime might be slightly longer)
> Jan 11  06:43 to 07:18 (UTC)
> 
> To complete your records: the transmitter was also down at least 2 times for
> shorter laps (on Jan 6 around 18:00 UTC and 20:37 UTC (I think they these
> failures are also visible on your graph
> http://www.w4dex.com/75khz/hbg07jan03.jpg)
> 
> Do not hesitate to contact me again if you need further information
> 
> Best regards
> 
> Gregor Dudle
> 
> > -----Ursprüngliche Nachricht-----
> > Von:  Dexter McIntyre [SMTP:dmcintyre@att.net]
> > Gesendet am:  11 January 2003 15:47
> > An:   gregor.dudle@metas.admin.ch
> > Betreff:      HBG 75 kHz transmitter
> >
> > Sir,
> >
> > For the past month I have been monitoring and plotting the signal
> > strength of your 75 kHz transmission for LF propagation studies.  I am
> > located in North Carolina, USA.  Today, 11 January and on 7 January, I
> > saw a sudden drop in signal strength of approximately 15 dB.  Both times
> > the signal was down for about half an hour then came back to normal
> > level.  I am trying to determine if these were actually propagation
> > events or if perhaps there was transmitter maintenance being performed
> > during these times.
> >
> > If you are interested in seeing my plots the current one is available
> > at:
> >
> > http://www.w4dex.com/75khz/hbg.jpg
> >
> > The dip at approximately 0640 to 0720 on the 11th of January:
> >
> > http://www.w4dex.com/75khz/hbg11jan03.jpg
> >
> > The dip at approximately 0550 to 0620 on the 7th of January:
> >
> > http://www.w4dex.com/75khz/hbg07jan03.jpg
> >
> > Also a directory of all plots is at:
> >
> > http://www.w4dex.com/75khz/
> >
> > Thank you,
> > Dexter McIntyre
> > Stanfield, NC USA
> > http://www.w4dex.com/



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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DL4YHF@aol.com schrieb:
> Hello group,
>
> received this colorful image under adverse conditions: Random wire plugged 
> into a TS850, tuned to 135.92 in "CW" (usb), pitch = 650 Hz, so 650Hz on 
> screenshot is near 135.920 kHz . The decibel scale is not calibrated against 
> anything, so just a relative measure.
>
> The different power levels received here in JO42FD are quite strange, but see 
> for yourself.
>
> Must go to bed, work starts early. I would appreciate a similar test from 
> saturday to sunday, better for the "working class" (and especially to those 
> not QRV from home). Good luck to everyone. 
>
> Cheers,
>  Wolf  DL4YHF (not at DF0WD)
>
>

Hi all,

an other checkered midnights painting (SpecLab shot). see attachment.

regards

Uwe/dj8wx/jo43sv
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--------------070603090400050503090102--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Hugh M0WYE" <m0wye@thersgb.net>
To: rsgb_lf_group@blacksheep.org
References: <002701c2bafb$34a0b460$6507a8c0@Main>
Date: Mon, 13 Jan 2003 12:32:59 -0000
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Subject: LF: QRSS transmission tonight
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Hi All,
I did some test transmissions over the weekend, and I seem to be able to
radiate some sort of signal now.
I will send some CQs in the QRSS part of the band around 20:00 tonight, and
will of course monitor for replies using Argo.
Any signal reports would be most welcome.
They won't be big signals as I only have about 0.1A of antenna current, but
maybe some of the more local stations might pick something up. (if anybody
is still awake after last night !)
73
Hugh M0WYE
E-mail: m0wye@thersgb.net
Description of antenna, TX, etc. here ...
http://www.m0wye.thersgb.net/lf.htm





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Date: Mon, 13 Jan 2003 11:59:12 -0000
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Subject: LF: T/A Prop last night
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Hi all, well done last night. A quick look at Steve's site this morning
shows that the early levels (before 0300z) were about 10dB down on the later
levels, between 0400 and 0600z. I am not sure how the country wide
conditions would relate to this "spot" measurement. My experience is that
most would get a better result in the second half of the night though the
individual timing of the good conditions (peaks) would differ at different
locations. The levels seen by Steve in the 0000 to 0300z period could be
considered as borderline because some elements were received by John from
Laurie. Did anyone send or capture in the later period ??

I am not putting great store by it, but it is just interesting to note that
Steve's highest recorded levels were just about 16 days after the Kp=5 minor
storm on the 19/20th Dec. This sort of period has shown up in some of
Laurie's previous successes. It does tend to suggest that totally benign,
quiet solar conditions are not quite adequate for us to make the trip. This
may become more obvious as slide down the solar activity curve, over the
next few years.

I did a quick and dirty test on my rx system here some time back and I find
only 3-4dB between a T copy and a full O on QRSS, when receiving against
local band noise.

There seems to be no doubt that crossings are never going to be telphone
style "plug-in" contacts at our power levels, we are going to have to work
for them.

Cheers de Alan G3NYK
alan.melia@btinternet.com







From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Ian Kyle" <ian.gi8ayz@virgin.net>
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Last night I was witness to what can only be described as a cavalry charge
at the low end of the band.
Cuirassiers  identified were, reading from the top of the screen:- Dave;
Marcus; Peter; Mike, and Laurie as 'left marker'.
There were at least two other intermittent and unidenifiable signals there
in the middle so who did I miss?
Identification difficult due to signal strengths being such that heavy
'dog-boning' made the screen look  like a snowball fight for much of the
time.
Amazing!

73 to all,

Ian GI8AYZ/MI0AYZ



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> Nil. Captures discontinued at 0230. Tnx to all.
> John Andrews, W1TAG

Thanks for taking the trouble to listen (watch?), John and Dex. There were
five or six stations active here. I am sure another test soon would be
welcome. The captures on the web are very helpful, though auto-refresh (see
Alan's page) would be useful. Thanks also to those in Eu who sent pictures
of everyone. It is good to see how signals compare (though not so nice to
see that I am the weakest!).

Mike, G3XDV
http://www.lf.thersgb.net
====================



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Nil. Captures discontinued at 0230. Tnx to all.

John Andrews, W1TAG




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These are my best captures from tonites test hr in Maryland FM19Mh

www.geocities.com/lacwman/135.922.jpg

www.geociyies.com/lacwman/135.922a.jpg

www.geocities.com/lacwman/135.922b.jpg

de Lloyd W3NF


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Hi Alan and Group:

The Laurie´s signal peaked slightly before Steve´s register, peak was clear
between 23.08 and 23.24, perhaps the last of the night?







> possible that UK stations will peak before DCF39 being nearly 1000km
nearer





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Other than a little signal from Laurie earlier, I haven't seen anything to
justify lost sleep tonight. Anyone transmitting on 135.922 who wants to drop
out will not be missed at this end! I will keep the capture running until
0300, anyway.

Maybe by next weekend, things will be better.

John Andrews




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I believe the jet stream is in your favor Alberto.  Thanks for posting
that shot.  Nice to see what we are looking for.

Dex

Alberto di Bene wrote:
> 
> If our friends over the pond are curious to see how the T/A slot
> of spectrum looks like here in Italy  JN45SL  , they can go to
> check how crowded it is here :
> http://www.qsl.net/i2phd/13jan00000.jpg
> 
> 73  Alberto  I2PHD



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Hi all, a quick look at Steve's site suggests that the DCF39 level is still
climbing and didn't peak last night until about 0100z It is about 10dB below
that level at the moment. Of course John and Dex and anyone else listening
(watching !!) will not see the same fading pattern as Steve registers. It
will be very dependent on the actual path length and position. It is also
possible that UK stations will peak before DCF39 being nearly 1000km nearer
to N.A.. The climb shown on Steve's site is slower tonight and there are no
big troughs. This might mean that the peaks will not be quite as high as
last night, but the conditions will last longer. Solar conditions are still
quiet and have been for some time now. This might be described as
"undisturbed conditions", and as such may not be as good as the dying stages
of a "disturbance event" The last really good days were the 5/6th of Jan.
which were probably about 6dB higher than last night. However Steve's system
"topped out" on the 5th limiting the graph peak. Even last nights levels are
some 12 dB above the average since 29th Dec.

Good Luck all
Cheers de Alan G3NYK
alan.melia@btinternet.com




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<DIV><FONT face=Arial size=2>Hi Group:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Congratulations. Signals from Laurie can be seen in 
the John´s &nbsp;capture.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José,EA1PX</FONT></DIV></BODY></HTML>

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From: "Dave Pick" <g3yxm@wireless.org.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
Date: Sun, 12 Jan 2003 22:50:03 -0000
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<DIV><FONT face=Arial size=2>Dex / John etc.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Everyone is blasting away as promised, things don't 
look too good yet though.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Dave</FONT></DIV>
<DIV><FONT face=Arial size=2>G3YXM.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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If our friends over the pond are curious to see how the T/A slot
of spectrum looks like here in Italy  JN45SL  , they can go to
check how crowded it is here :
http://www.qsl.net/i2phd/13jan00000.jpg

73  Alberto  I2PHD





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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hello group,
<BR>
<BR>received this colorful image under adverse conditions: Random wire plugged into a TS850, tuned to 135.92 in "CW" (usb), pitch = 650 Hz, so 650Hz on screenshot is near 135.920 kHz . The decibel scale is not calibrated against anything, so just a relative measure.
<BR>
<BR>The different power levels received here in JO42FD are quite strange, but see for yourself.
<BR>
<BR>Must go to bed, work starts early. I would appreciate a similar test from saturday to sunday, better for the "working class" (and especially to those not QRV from home). Good luck to everyone. 
<BR>
<BR>Cheers,
<BR> Wolf &nbsp;DL4YHF (not at DF0WD)
<BR></FONT></HTML>

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Subject: Re: LF: Re: QRSS Monitoring 12-13 Jan
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My Argo window for tonight's run can be seen at:

http://www.w4dex.com/argo/135khz.jpg

Noise level is low right now.  Just hearing an occasional static crash.

Dex

John Andrews wrote:
> 
> Captures 0f 136.922 from W1TAG will be posted every 15 minutes at:
> http://webpages.charter.net/w1tag/cap-1.jpg
> 
> John Andrews, W1TAG


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Hi all,

guess many of you built the G0MRF-Quarter-Kilowatt-Amplifier.
I did. the PSU is not finished yet.

got some trouble with the phase of the 137kHz sines 
(es triangular and rectangular) measured at the gates of the MOSFETs.
there is a diff btwn the two channels of estimated 10degr.
that means parasitic oscillation if operating the PA, doesn`t it.

for hours I try to set the diff to zero by changing the windings of the 
input coils (T1)and by changing the MOSFETs. no success. 
abt 10degr is the min. the ampludes are ok.

see attachment.

any hint ?

regards
Uwe/dj8wx





   
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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Subject: Re: LF: Jason Beacon signals
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Dear LF Group,

Thanks again for the reports on the Jason beacon signal last night - there 
was less QRN, but I guess propagation across the pond is still down. It was 
the same story in previous years; not a squeak for weeks on end, then 
suddenly wonderful conditions for a few days.

I was QRV using QRSS earlier today, and was quite amazed by DF6NM's "SSTV" 
- see the attachment. Luckily, SpecLab was already set up just right to 
catch it, although I hope Markus isn't really that colour!

I monitored the antenna resistance while transmitting the Jason signal last 
night - there was a hard frost, and by the end of the night, the loss 
resistance had fallen to 26 ohms, compared to 45 ohms during the rain a 
week or so ago. Unfortunately, the ice seems to have thawed now, requiring 
me to use more kWh to radiate the same signal.

I will run the Jason beacon again tonight, in the hope that propagation 
must improve sometime. If you find that the QRSS60 stations are coming in 
at good strengths, then try taking a look at 137.5025kHz - as usual, any 
reports very welcome.

Cheers, Jim Moritz
73 de M0BMU
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--------------060701080509030408030908--

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From: "John Andrews" <w1tag@charter.net>
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Captures 0f 136.922 from W1TAG will be posted every 15 minutes at:
http://webpages.charter.net/w1tag/cap-1.jpg

John Andrews, W1TAG



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Sorry to disappoint a lot of people who rang and emailed about the books; 
both gone I'm afraid. However, since there seems to be a demand I will try 
to find some more. Watch this space! Let me try a few more while I'm on a 
winning streak:

1955 ed of "Electrical Measurements and Measuring Instruments"  B. W. Golding
(the standard BSc(Eng) and City and Guilds textbook - remember?)

1941 ed of "The Practical Wireless Encyclopedia" by (guess who?) F. J. Camm

1942 ed of "Newnes Short-Wave Manual" by (yes, him again) F. J. Camm

All in good nick.

Alan - I've got several of the MIT series including Vol 4 Loran but not for 
sale. Can send you extracts if you know what you want. Presume it was Loran 
you meant and not really Vol 5 which is "Pulse Generators" (Oh, I don't 
know though!!)

While talking books I strongly recommend Robert Buderi's book "The 
Invention that changed the world - the story of radar from war to 
peace".  One of the best researched books on the subject I've read (and 
I've read a lot); technically and historically accurate. Waterstone's can 
supply if asked.

Walter G3JKV.
  

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Hello José!

Sunday, January 12, 2003, 8:06:39 PM, you wrote:

JM> I saw yesterday , in the popup, the news about Argentina. I e-mailed to
JM> Marcelo (LW2ETU) and Daniel (LU8EDR)
JM> but I haven´t got any answer yet, do you know if they are in the reflector?

E-mail from Marcelo lw2etu@hotmail.com  Jan 10 1750z to me :

My tx is a single mosfet IRF840 in E class. Pw 50w, Ant long
wire 100m. Tx in cw mode.
In same days pw 100w, and tx in qrss to. I am work to make better the
station.
I am contruction a 2,2m loop for rx.

73! Ed  RU6LA  ed@dx.ru



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Hi dave and all:

I saw yesterday , in the popup, the news about Argentina. I e-mailed to
Marcelo (LW2ETU) and Daniel (LU8EDR)
but I haven´t got any answer yet, do you know if they are in the reflector?
I mentioned them the tonight´s TA test also.

I´ll monitor the tonnight´s pile-up.

73 de José,  EA1PX



----- Original Message -----
From: "Dave Pick" <g3yxm@wireless.org.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, January 12, 2003 5:06 PM
Subject: LF: Re: Re: QRSS Monitoring 12-13 Jan


> John et al.
>
>
> > I'll slot myself in amongst the lines somewhere...
> >
> Having checked the gear, I will try to be on 135.9228/9 using DFCW (60
sec).
> If my DFCW generator breaks I'll use QRSS in that slot.
>
> Cheers.
> Dave. G3YXM.
>
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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John et al.


> I'll slot myself in amongst the lines somewhere...
>
Having checked the gear, I will try to be on 135.9228/9 using DFCW (60 sec).
If my DFCW generator breaks I'll use QRSS in that slot.

Cheers.
Dave. G3YXM.




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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I'll slot myself in amongst the lines somewhere...

Dave G3YXM.
----- Original Message -----
From: "John Andrews" <w1tag@charter.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, January 12, 2003 2:58 AM
Subject: LF: QRSS Monitoring 12-13 Jan


> In an effort to drum up some activity, W4DEX and I will be watching the
> 135.922 kHz region on Sunday night/ Monday morning, starting at 2200 UTC
on
> Sunday. Notes:
>
> Using ARGO 60 second normal-speed screen.
> Upper Freq = 135923.5
> Lower Freq = 135920.5
> Avoid: 135921.05 and 135920.92 (Loran lines)
>
> We will both post captures to the Web, and will post the URL's before the
> start.
>
> Anyone who wishes to participate (sending or receiving) is welcome.
>
> John Andrews, W1TAG
>
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi all, just as a comparison, I browsed my little 2nd hand bookstore in
Felixstowe just before Christmas and he has several copies of the Ad.
Handbook Part I 1938 (later impressions abt 1942) and one copy of the the
Part II. He wanted £20 for the part II !! The copy of Terman's Radio
Engineering I bought from him, was more of a bargain.

Anyone got a spare copy of Vol 5 (Loran) of the Radiation Lab Series ??

Cheers de Alan G3NYK
alan.melia@btinternet.com




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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi group,<BR>
<BR>
 the band is fairly quiet this sunday, and had most enjoyable QSO's with DF8ZR, EA1PX and M0BMU using QRSS, DFCW and Hell modes.<BR>
<BR>
At 13:15, I tried a small survey of spectral lines I can see between 137744 and 137753Hz on Argo-60. Noise was around -34 dBµV/m in 10mHz RBW.<BR>
<BR>
&nbsp;&nbsp; f/Hz&nbsp;&nbsp;&nbsp;&nbsp; FS/dBµV/m<BR>
-137700&nbsp;&nbsp; (approx.)<BR>
<BR>
752.99&nbsp; -22<BR>
751.70&nbsp; -21<BR>
750.70&nbsp; -28<BR>
750.42&nbsp; -18<BR>
750.22&nbsp;&nbsp; ? (seen last night, now gone)<BR>
748.42&nbsp; -30<BR>
748.31&nbsp; -28<BR>
746.97&nbsp; -18<BR>
745.04&nbsp; -23<BR>
744.53&nbsp; -18 (also seen by EA1PX)<BR>
<BR>
I assume that most of these lines are from LORAN. The three strongest ones appear to be coming in from WNW, so an origin in Western France seems reasonable. Hope this may help...<BR>
<BR>
73 es have a nice sunday<BR>
<BR>
Markus,<BR>
DF6NM in Nuernberg, JN59NK<BR>
</FONT></HTML>

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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Dear John,<BR>
<BR>
listen to the drums ... ;-)<BR>
<BR>
I will try to get on my usual DFCW frequency pair 135922.3 / 922.4 Hz, 60s/20s on/off.<BR>
<BR>
73 <BR>
Markus, DF6NM<BR>
</FONT></HTML>

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Subject: Re: LF: Books
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Walter Blanchard wrote:
> Have a spare copy of Termans' 1943 "Radio Engineers' Handbook" if anyone 
> wants it.
> Also Vol II, 1938 ed.  "Admiralty Handbook of Wireless Telegraphy" - the
> one with all the gen on loops and LF antennas.
> 
> Walter G3JKV
> 

Hello Walter,
I would like to give a new home to your Admiralty book.
Let's discuss the modalities (payment, shipment) off this reflector.
73
André N4ICK



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From: "hamilton mal" <g3kev.ham@virgin.net>
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----- Original Message ----- 
From: "merv" <nc1k@thecia.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, December 29, 2002 11:15 PM
Subject: LF: autoresponder...


> My apologies to all:  my site-hosting company changed servers and
> activated the autoresponder by mistake. It has now been turned off again.

Hi Merv
Did you get my message sent recently.
de Mal/G3KEV

> 
>  73's
> 
>    NC1K.
> 
> 




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From: "hamilton mal" <g3kev.ham@virgin.net>
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----- Original Message -----
From: "WE0H" <we0h@gentekcom.com>
To: "Rsgb_Lf_Group" <rsgb_lf_group@blacksheep.org>
Sent: Sunday, January 12, 2003 1:18 AM
Subject: LF: FW: [Lowfer] WC2XSR/13 New Frequency


>
>
>
> -----Original Message-----
> From: lowfer-admin@mailman.qth.net [mailto:lowfer-admin@mailman.qth.net]
On
> Behalf Of Ralph Hartwell
> Sent: Saturday, January 11, 2003 6:18 PM
> To: Lowfer
> Subject: [Lowfer] WC2XSR/13 New Frequency
>
> WC2XSR/13 went back on the at 1739 CST.
>
> The modulation is QRSS30, repeating "XSR" one time, followed by CD ID at
> 10 WPM. Transmitter power output to the antenna is 400 watts.
>
> The frequency has been changed to 164.500 KC to facilitate possible
> reception by several stations who have reported interference on 166.500
> KC.

This freq is completely swamped at my QTH by a French Broadcast Stn S9 plus
a hundred db over. You probably know already the freq range 190 khz - 400
khz is allocated to the European broadcasting service and there are some
very loud stations active. I am surprised you do not hear some of these
stations across the ocean blue.
Mal/G3KEV

>
> 73,
>
> Ralph   W5JGV / WC2XSR / 13
>
> The current On-The-Air status of WC2XSR/13 is available at:
> http://home.att.net/~shmrg/wc2xsr-13_log.htm
>
> My 600 Meter Research Group files are at:
> http://home.att.net/~shmrg
>
> My Home Page is at:
> http://home.att.net/~ralph.hartwell
> Home of the Rife Biomedical Research Web Ring
>
> _______________________________________________
> >From the Lowfer mailing list
> Send messages to: Lowfer@mailman.qth.net
> To sub/unsub visit: http://mailman.qth.net/mailman/listinfo/lowfer
>
>
>



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From: "hamilton mal" <g3kev.ham@virgin.net>
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<DIV><FONT face=Arial size=2>Nice signal from DL6NM on hell a few mins 
ago&nbsp;&nbsp;&nbsp; </FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>R BMU TU 73 DE DF6NM CUL SK</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>de G3KEV</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

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References: <5.1.0.14.0.20030110103024.00a96cd0@gemini.herts.ac.uk>	 <16594.030111@pyrotherm.co.yu> <5.1.0.14.0.20030111142631.00a970f8@gemini.herts.ac.uk> <3E20DFBC.2A9B9198@otenet.gr>
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Failrly good copy of Jim's transmission in JN45SL, especially <br>
considering I am without an LF antenna.<br>
<br>
73  Alberto  I2PHD<br>
<br>
<img src="cid:part1.08030708.04080101@usa.net" alt="" width="589"
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--------------000106040801020804040806--

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From: "g3ldo" <g3ldo@ukonline.co.uk>
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Hi John,

Sounds like a good idea. I will allocate myself 135922 transmitting 'LDO'
QRSS60

> In an effort to drum up some activity, W4DEX and I will be watching the
> 135.922 kHz region on Sunday night/ Monday morning, starting at 2200 UTC
on
> Sunday. Notes:
>
> Using ARGO 60 second normal-speed screen.
> Upper Freq = 135923.5
> Lower Freq = 135920.5
> Avoid: 135921.05 and 135920.92 (Loran lines)
>
> We will both post captures to the Web, and will post the URL's before the
> start.
>
> Anyone who wishes to participate (sending or receiving) is welcome.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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From: "Matti Niemela" <mattis.niemela@kolumbus.fi>
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Hi Walter,

I am interested in Termans Handbook. Still left? Price?

73 Matti OH2ZT
----- Original Message -----
From: "Walter Blanchard" <blanch@pncl.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, January 12, 2003 2:25 PM
Subject: LF: Books


> Have a spare copy of Termans' 1943 "Radio Engineers' Handbook" if anyone
> wants it.
> Also Vol II, 1938 ed.  "Admiralty Handbook of Wireless Telegraphy" - the
> one with all the gen on loops and LF antennas.
>
> Walter G3JKV
>


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Have a spare copy of Termans' 1943 "Radio Engineers' Handbook" if anyone 
wants it.
Also Vol II, 1938 ed.  "Admiralty Handbook of Wireless Telegraphy" - the
one with all the gen on loops and LF antennas.

Walter G3JKV

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> In an effort to drum up some activity, W4DEX and I will be watching the
> 135.922 kHz region on Sunday night/ Monday morning, starting at 2200 UTC
on
> Sunday. Notes:
> John Andrews, W1TAG

I will be active on 135.92175kHz.

Mike, G3XDV
http://www.lf.thersgb.net
====================




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Date: Sun, 12 Jan 2003 05:23:40 +0200
From: "Alex Deligiannis" <sv8qg@otenet.gr>
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References: <5.1.0.14.0.20030110103024.00a96cd0@gemini.herts.ac.uk> <16594.030111@pyrotherm.co.yu> <5.1.0.14.0.20030111142631.00a970f8@gemini.herts.ac.uk>
Subject: Re: LF: Jason Beacon signals
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Dear James,
                   The last part of your JASON transmission ended at 03.05z
received at KM39GC
73 Alex SV8QG

James Moritz wrote:

> Dear LF Group,
>
> The Jason beacon signals were transmitted as planned last night - many
> thanks to YU7AR for my first report from YU. I think this is the first
> report I have had from YU in any mode on LF
>
> The QRN was also very strong here last night - it was still strong earlier
> this afternoon. Looking at the lightning activity maps, there seems to be
> thunderstorms in the Mediterranean just off the southern tip of Italy -
> perhaps this is where the noise is coming from.
>
> When I started transmitting last night, the temperature was about +2C, but
> as time passed the temperature dropped below freezing, causing the antenna
> loss resistance to drop by about 20% by 0300. It is surprising to have this
> much effect, because things were only frozen on the surface, as I found out
> splashing around in the mud when I took the antenna mast down afterwards!
>
> I will run the beacon again tonight,  from 2200 - 0300utc on 137.5025kHz as
> before. Any reports will be very welcome.
>
> Cheers, Jim Moritz
> 73 de M0BMU






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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
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In an effort to drum up some activity, W4DEX and I will be watching the
135.922 kHz region on Sunday night/ Monday morning, starting at 2200 UTC on
Sunday. Notes:

Using ARGO 60 second normal-speed screen.
Upper Freq = 135923.5
Lower Freq = 135920.5
Avoid: 135921.05 and 135920.92 (Loran lines)

We will both post captures to the Web, and will post the URL's before the
start.

Anyone who wishes to participate (sending or receiving) is welcome.

John Andrews, W1TAG




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From: "WE0H" <we0h@gentekcom.com>
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Subject: LF: FW: [Lowfer] WC2XSR/13 New Frequency
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-----Original Message-----
From: lowfer-admin@mailman.qth.net [mailto:lowfer-admin@mailman.qth.net] On
Behalf Of Ralph Hartwell
Sent: Saturday, January 11, 2003 6:18 PM
To: Lowfer
Subject: [Lowfer] WC2XSR/13 New Frequency

WC2XSR/13 went back on the at 1739 CST.

The modulation is QRSS30, repeating "XSR" one time, followed by CD ID at
10 WPM. Transmitter power output to the antenna is 400 watts.

The frequency has been changed to 164.500 KC to facilitate possible
reception by several stations who have reported interference on 166.500
KC.

73,

Ralph   W5JGV / WC2XSR / 13

The current On-The-Air status of WC2XSR/13 is available at:
http://home.att.net/~shmrg/wc2xsr-13_log.htm

My 600 Meter Research Group files are at:
http://home.att.net/~shmrg

My Home Page is at:
http://home.att.net/~ralph.hartwell
Home of the Rife Biomedical Research Web Ring

_______________________________________________
>>From the Lowfer mailing list
Send messages to: Lowfer@mailman.qth.net
To sub/unsub visit: http://mailman.qth.net/mailman/listinfo/lowfer




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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="0">Steve,<BR>
<BR>
I don't see the S/N ratios that you do with your 100 ft loop, but I can copy DCF-39 clearly by ear on skywave using my Wellbrook LFL-1010 here at FN20WW.<BR>
<BR>
Ray, W2RS</FONT></HTML>

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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: rsgb_lf_group@blacksheep.org
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What do you mean neighbours, he couldn't let them find that big crock-clip
on the bottom of their 600foot mast could he !!
(If in doubt check about that the postal address)
Cheers de Alan G3NYK
----- Original Message -----
From: "G4WGT" <g4wgt@talkgas.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: 11 January 2003 19:32
Subject: RE: LF: Jason Beacon signals


> Hi to Jim & LF,
>
> You wrote -
>
>  as I found out splashing around in the mud when I took the antenna mast
> down afterwards!
>
> ************
>
> Is the antenna that big you dare not let the neighbours see it in
daylight,
> HI HI.
>
> Received your JASON Tx 100% but not surprising, your sig is S5 on my
> reciever.
>
> Regards
>
> Gary  G4WGT.
>
>
>
>
> ---
> Outgoing mail is certified Virus Free.
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>



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From: "G4WGT" <g4wgt@talkgas.net>
To: rsgb_lf_group@blacksheep.org
Date: Sat, 11 Jan 2003 19:32:39 -0000
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Subject: RE: LF: Jason Beacon signals
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Hi to Jim & LF,

You wrote -

 as I found out splashing around in the mud when I took the antenna mast
down afterwards!

************

Is the antenna that big you dare not let the neighbours see it in daylight,
HI HI.

Received your JASON Tx 100% but not surprising, your sig is S5 on my
reciever.

Regards

Gary  G4WGT.




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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "WE0H" <we0h@gentekcom.com>
To: rsgb_lf_group@blacksheep.org
Date: Sat, 11 Jan 2003 10:23:18 -0600
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That is where I bought my '43 Terman. Excellent service and fast shipping.

Mike>WE0H
http://www.we0h.us/lf

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of Andre Kesteloot
Sent: Saturday, January 11, 2003 10:07 AM
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re: Off topic: buying used books via Internet

Holger 'Geri', DK8KW wrote:
 > Thanks, Dick,
 >
 >  >I gave this hint also to a Dutch amateur who was looking
 >  >for Terman's Radio Engineer's Handbook and he bought
 >  >a used copy also at ALIBRIS.
 >
 >
 > that was an excellent hint, just ordered my copy of that book  :-)
 >
 > Best 73
 >
 > Geri, DK8KW (W1KW)
 > Still without LF-antenna ...

Another excellent and reliable address is
http://www.abebooks.com

73
André N4ICK






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Holger 'Geri', DK8KW wrote:
 > Thanks, Dick,
 >
 >  >I gave this hint also to a Dutch amateur who was looking
 >  >for Terman's Radio Engineer's Handbook and he bought
 >  >a used copy also at ALIBRIS.
 >
 >
 > that was an excellent hint, just ordered my copy of that book  :-)
 >
 > Best 73
 >
 > Geri, DK8KW (W1KW)
 > Still without LF-antenna ...

Another excellent and reliable address is
http://www.abebooks.com

73
André N4ICK




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Holger 'Geri', DK8KW" <holger.kinzel@qru.de>
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<DIV><FONT face=Arial>Thanks, Dick,</FONT></DIV>
<DIV><FONT size=3><BR>&gt;I gave this hint also to a Dutch amateur who was 
looking </DIV>
<DIV>&gt;for Terman's <I>Radio Engineer's Handbook</I> and he bought </DIV>
<DIV>&gt;a used copy also at ALIBRIS.</DIV>
<DIV><BR>&nbsp;</DIV>
<DIV><FONT face=Arial>that was an excellent hint, just ordered my copy of that 
book&nbsp; :-)</FONT></DIV>
<DIV><FONT face=Arial></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial>Best 73</FONT></DIV>
<DIV><FONT face=Arial></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial>Geri, DK8KW (W1KW)</FONT></DIV>
<DIV><FONT face=Arial>Still without LF-antenna ...</FONT></DIV>
<DIV><STRONG></STRONG>&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><STRONG><BR></STRONG></DIV></FONT></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Dear LF Group,

The Jason beacon signals were transmitted as planned last night - many 
thanks to YU7AR for my first report from YU. I think this is the first 
report I have had from YU in any mode on LF

The QRN was also very strong here last night - it was still strong earlier 
this afternoon. Looking at the lightning activity maps, there seems to be 
thunderstorms in the Mediterranean just off the southern tip of Italy - 
perhaps this is where the noise is coming from.

When I started transmitting last night, the temperature was about +2C, but 
as time passed the temperature dropped below freezing, causing the antenna 
loss resistance to drop by about 20% by 0300. It is surprising to have this 
much effect, because things were only frozen on the surface, as I found out 
splashing around in the mud when I took the antenna mast down afterwards!

I will run the beacon again tonight,  from 2200 - 0300utc on 137.5025kHz as 
before. Any reports will be very welcome.

Cheers, Jim Moritz
73 de M0BMU




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: rsgb_lf_group@blacksheep.org
References: <000901c2b909$66f0da60$6507a8c0@Main> <000401c2b94e$63fe6800$18c828c3@erica> <000601c2b956$32a81f00$d3e086d4@erica> <003d01c2b96e$c4113b80$d5c863d5@BI57429bankinter>
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Subject: LF: Re: Re: Re:  French lines
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Hi Jose, it is just that Peter, Mike and I ( and a few others) have often
discussed these lines in the past and speculated on their origin. They seem
to peak up southerly to us, which might put them somewhere in
France.....hence they get called "the  French Lines"....if anyone knows
better we would all be interested.

Cheers de Alan G3NYK   JO02PB
alan.melia@btinternet.com

----- Original Message -----
From: "José Manuel" <jpradoes@telefonica.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: 11 January 2003 12:41
Subject: LF: Re: Re: French lines


> Hi Peter and Group:
>
> I copy a very weak line now , I need QRSS60, on 137744.54 Hz,  but what
is
> it? why French line?
>
> 73 de José, EA1PX
>
>
>
> > > Most of the time I only get one line and it is quite strong - audible
at
> > > around S5.
> > > On my receive system it is 137.7465kHz
>
>
>
>
>
>
>
>
>
>
>
>
>



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Hi Peter and Group:

I copy a very weak line now , I need QRSS60, on 137744.54 Hz,  but what  is
it? why French line?

73 de José, EA1PX



> > Most of the time I only get one line and it is quite strong - audible at
> > around S5.
> > On my receive system it is 137.7465kHz














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Date: Sat, 11 Jan 2003 13:35:09 +0000
From: "Dexter McIntyre" <dmcintyre@att.net>
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Subject: Re: LF: Jason Beacon signals
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No copy in NC last night.  Propagation looked fair but S/N was poor. 
Lots of QRN form somewhere.  QRN wasn't local so LF propagation to it's
source was also good.

Dex


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Date: Sat, 11 Jan 2003 14:16:44 +0100
From: "YU7AR" <yu7ar@pyrotherm.co.yu>
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Subject: Re: LF: Jason Beacon signals
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Hello James,

Friday, January 10, 2003, 12:10:40 PM, you wrote:

JM> Dear LF Group,

JM> I am planning to run the Jason beacon again tonight and during the weekend. 
JM> I aim to start tonight around 2200 utc and carry on until about 0300. 
JM> Frequency will be centered on 137.5025kHz, in an attempt to dodge some of 
JM> the Loran spectral lines present across the pond. I am hoping for some 
JM> further transatlantic signal reports, but of course any other signal 
JM> reports will also be very welcome.

JM> Cheers, Jim Moritz
JM> 73 de M0BMU


Hi Jim,
Here is your last night JASON95 sigs. KN05BW 1621km

73 Teo  YU7AR

-- 
Best regards,
 YU7AR                            mailto:yu7ar@pyrotherm.co.yu

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<html>
<font size=3 color="#FF0000"><b>Correction: The URL should be
<a href="http://www.alibris.com/" eudora="autourl">http://www.alibris.com/</a>).<br><br>
</font><font size=3>To All from PA0SE<br><br>
A useful internet site for used books is ALIBRIS
(<a href="http://alibris.com/" eudora="autourl">http://alibris.com/</a>).<br><br>
I looked for a book on radar by Buderi:<i> The Invention that changed the
world.<br><br>
</i>The list price at the Internet bookshop AMAZON was $39.98 but is was
out of print.<br><br>
At ALIBRIS I bought it for $5.47 (plus $9.95 shipping cost :-(&nbsp;
)<br><br>
It is a bound, used copy but I can see no difference with a new
book.<br><br>
I gave this hint also to a Dutch amateur who was looking for Terman's
<i>Radio Engineer's Handbook</i> and he bought a used copy also at
ALIBRIS.<br><br>
73</b>, <b>Dick, PA0SE</font></b></html>

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<html>
<font size=3><b>To All from PA0SE<br><br>
A useful internet site for used books is ALIBRIS 
(<a href="http://alibris.com/" eudora="autourl">http://alibris.com/</a>).<br><br>
I looked for a book on radar by Buderi:<i> The Invention that changed the
world.<br><br>
</i>The list price at the Internet bookshop AMAZON was $39.98 but is was
out of print.<br><br>
At ALIBRIS I bought it for $5.47 (plus $9.95 shipping cost :-(&nbsp;
)<br><br>
It is a bound, used copy but I can see no difference with a new
book.<br><br>
I gave this hint also to a Dutch amateur who was looking for Terman's
<i>Radio Engineer's Handbook</i> and he bought a used copy also at
ALIBRIS.<br><br>
73</b>, <b>Dick, PA0SE</font></b></html>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
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> Hi Peter, I am not really in calibration at the moment and I have a limit
of
> +/- 0.1Hz. But for what its worth I make the lines 137.7446 and 137.7528.
I
> doubt whether Markus can hear(see) them at his location. I will try again
> tomorrow when its a bit quieter, as they do make a useful marker at this
end
> of the band.
> Cheers de Alan G3NYK

I agree with these measurements. I use Argo calibrated against 60kHz. The
IC-706 Mk1 seems to re-set to within a fraction of 1Hz after 10 minutes warm
up, and stays better than 0.1Hz after that.

Mike, G3XDV
http://www.lf.thersgb.net
=================





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From: "g3ldo" <g3ldo@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
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>
> Most of the time I only get one line and it is quite strong - audible at
> around S5.
> On my receive system it is 137.7465kHz
> On the other hand DFC39 is on 138.8305.
> If I assume DFC is on 138.830kHz then I can apply a correction of -.5Hz to
> make the line that I am receiving 137.747kHz


Correction
 make the line that I am receiving 137.746kHz

G3LDO




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
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Hi Alan

> Hi Peter, I am not really in calibration at the moment and I have a limit
of
> +/- 0.1Hz. But for what its worth I make the lines 137.7446 and 137.7528.
I
> doubt whether Markus can hear(see) them at his location. I will try again
> tomorrow when its a bit quieter, as they do make a useful marker at this
end
> of the band.

Most of the time I only get one line and it is quite strong - audible at
around S5.
On my receive system it is 137.7465kHz
On the other hand DFC39 is on 138.8305.
If I assume DFC is on 138.830kHz then I can apply a correction of -.5Hz to
make the line that I am receiving 137.747kHz

That W3EEE site is good is it not? During the period when the T/A was
exceptional Laurence was receiving most of the LF broadcast stations in EU
much stronger than usual.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
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Alan G3NYK said

> Hi all, the Trans-Atlantic path seems to be peaking about 10dB above
average
> tonight. It is still 5/6dB below the peaks on the best nights (5 & 6 Jan)
> according to Steve's realtime plot. You may find the plot on my web-site
in
> place of the old CFH plot useful. It gives the plots for the 5th and 6th
and
> an average line for all the data between 19th Dec to 6th Jan. This is a
> useful benchmark to put against the realtime plot. Geomag conditions have
> been fairly quiet since about 19th Dec with the Kp not exceeding 4 since
> then.

I am currently transmitting on 137.7695kHz QRS60

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




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From: "Thomas Giella KN4LF" <kn4lf@tampabay.rr.com>
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KN4LF 7 Day HF/MF Radio Propagation Outlook #2003-03 Published 11:00 PM EST
03/01/10 For 03/01/11-03/01/16.

PROPAGATION OUTLOOK-

Global HF Propagation Conditions:

Low Latitude: Good
Mid Latitude: Good
Hi Latitude: Fair To Good

Global MF Propagation Conditions:

Expect fair to good domestic propagation conditions on east-west paths and
fair on north south paths in the northern hemisphere out to approximately
1050 miles.

Expect fair domestic propagation conditions on east-west paths and poor to
fair on north south paths in the southern hemisphere out to approximately
1050 miles.


"High latitude" northern hemispheric (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be fair.

"High latitude" southern hemispheric (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be poor to fair.


"Mid latitude" northern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be fair to good.

"Mid latitude" southern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be fair.


"Low latitude" northern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
propagation conditions in excess of approximately 3000 miles should be good.

"Low latitude" southern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
propagation conditions in excess of approximately 3000 miles should be fair.


QRN OUTLOOK-

During the outlook period there will be "high" lightning induced QRN levels
in low latitude areas of the northern hemisphere due to proximity of the
Inter Tropical Convergence Zone (ITCZ).

Northern hemisphere mid latitude regions can expect "moderate to
occasionally high" lightning induced QRN tied to cold season thunderstorms,
cold/warm/occluded fronts and associated extra-tropical cold core low
pressure systems. These weather systems are currently being enhanced by the
moderate level El Nino ocean water temperature anomaly.

Northern hemisphere high latitude regions can expect "low to occasionally
moderate" lightning induced QRN tied to cold season thunderstorms,
cold/warm/occluded fronts and associated extra-tropical cold core low
pressure systems. These weather systems are currently being enhanced by the
moderate level El Nino ocean water temperature anomaly.


During the outlook period there will be "high" lightning induced QRN levels
in low latitude areas of the southern hemisphere tied to warm season
thunderstorms and tropical systems.

Southern hemisphere mid latitude regions can expect "moderate to high"
lightning induced QRN, tied to warm season thunderstorms and tropical
systems.

Southern hemisphere high latitude regions can expect "moderate" lightning
induced QRN, tied to warm season thunderstorms and tropical systems.


Here are some general guidelines concerning correlation of space weather and
propagation indices to actual expected HF/MF propagation conditions.

1.) Dropping indices numbers are better.

2.) Solar flux under 150 okay, under 100 better, 70 is best for E layer
multi hop.

2a.) For high frequencies (HF) solar flux of 100 is okay, 150 better, above
200 best.

3.) Solar flux of at least 100 for E valley-F layer ducting mechanism.

4.) Previous 24 hour Ap index under 10, under 7 for several days
consecutively is best.

5.) Previous 3 hour Kp index under 3 for mid latitude paths, under 2 for
high latitude paths, 0-1 for several days consecutively is best.

6.) Energetic protons no greater then 10 MeV (10+0) for 160/120 meters and
no greater then (10-1) on MF broadcast band.

7.) Background x-ray flux levels less than C2 for several days consecutively
for 160/120 meters and less then C1 for MF broadcast band.

8.) No current STRATWARM alert.

9.) IMF Bz with a negative sign, indicates a better chance of high latitude
path auroral absorption/unpredictable refraction or scattering of MF RF
signals, when the Kp is above 3.


SPACE WEATHER INDICES DURING THE PAST 7 DAY PERIOD, SPACE WEATHER INDICES
EXPECTED DURING THE 7 DAY OUTLOOK PERIOD AND EXPLANATIONS OF THEIR IMPACT ON
ANTICIPATED PROPAGATION CONDITIONS.


ENERGETIC PROTON FLUX-

During the previous 7 day period no elevated energetic proton flux events of
>10 MeV (10+0) occurred.

During the 7 day outlook period the probability of an elevated energetic
proton flux event >10 MeV (10+0) is placed at 30%.


An elevated energetic proton flux level greater then (10+0) on 160 meters
and greater then (10-1) on the medium frequency broadcast band creates
noticeably increased winter time day and year round night time D layer
absorption of medium wave frequencies, especially on high latitude
propagation paths but it can also negatively impact mid latitudes, depending
on the intensity of the event.

Elevated energetic proton events too small to be categorized as a Polar Cap
Absorption event (PCA) can still impact high and mid level medium frequency
propagation paths in the form of excessive D layer absorption. This fact is
still stubbornly opposed by some otherwise very knowledgeable space weather
physicists over dependent on high latitude threshold Riometer readings.

((((Note, high latitude medium frequency radio propagation paths can still
be disturbed for days and up to weeks, following the end of an official >10
MeV (10+0) proton event.))))


SOLAR FLUX-

During the previous 7 day period the daily solar flux level ranged between
186 and 114.

During the outlook period the daily solar flux values should range between
approximately 200 and 165.

During the previous 7 day period the daily "average" Background X-Ray Flux
level ranged between B4.4 and C1.1.


Elevated background X-ray flux levels can impact propagation of medium
frequency signals in a negative manner. Background X-ray flux levels of C1
or greater creates increased D-layer absorption of 160 and 120 meter signals
and B9 or greater creates increased D-layer absorption of AM broadcast band
signals.

Remember though that there are daily extremes of the Background X-ray flux
level. So even though the daily average might have been good at say B2.2,
the daily "extreme" maximum could have been C1.5, which would have been bad
and have cause a short period of increased D layer absorption.

High solar flux values are generally considered to be detrimental to
propagation of medium frequency signals both domestic and Trans Atlantic
(TA) & Trans Pacific (TP), as more absorption can be present via the
transmitted signals' two trips through the D layer at the takeoff and
arrival points.

Most "strong" longer haul medium frequency DX signals in excess of 3000
miles is via the E Valley-F layer ducting and/or Chordal Hop propagation
modes. Therefore high solar flux values can aid in long haul medium
frequency propagation paths in excess of 3000 miles, as a high solar flux
value ensures a strong F layer part of the E Valley-F layer duct or Chordal
Hop propagation mechanism.

However high solar activity in the form of increased ionization created by
Ultraviolet and X-Ray radiation can fill in the E Valley region and
interfere with the E Valley-F layer ducting mechanism. In a sense the E
Valley-F layer duct is closed on one or both ends of a propagation path and
the transmitted MF RF signal only propagates between the E layer and
land/ocean surface, with a higher angle and more loss.


SOLAR FLARES & SUNSPOT GROUP REGIONS-

During the previous 7 day period three M class solar flares occurred. The
largest was an M4.6 class solar flare that occured on 03/01/07-08 between
2329-0009 UTC and was released from #10251.

Sunspot group #10251 located at S13E58 contains a beta-gamma-delta magnetic
structure that harbors energy for huge X class solar flares. It is not in
geo-effective position at this time.

Sunspot group #10242 located at S08W34 contains a beta-gamma magnetic
structure that harbors energy for large M class solar flares. It is in
geo-effective position at this time.

Solar flare forecast during the outlook period.

C- 100%

M- 80%

X- 40%


A C4 or higher class solar flare "can" elevate the proton flux above 10 MeV
(10+0) and initiate large scale high and mid latitude propagation path
absorption on the AM broadcast band, 160 and 120 meters, both stateside and
DX, as a transfer of increased density and RF signal absorption from the day
side D layer to night side of the ionosphere occurs through high level
neutral winds. Unfortunately even smaller C3 solar flares can create hour to
hour and night to night variations in signal strength on medium frequencies.

High and mid latitude Trans Atlantic (TA) and Trans Pacific (TP) propagation
paths tend to open up after a significant period of time passes without an
elevated energetic proton event of >10 MeV (10+0). This fact is still
stubbornly opposed by some otherwise very knowledgeable space weather
physicists over dependent on high latitude threshold Riometer readings.

Openings also occur when the solar background x-ray level falls back to
below C2 for 160 and 120 meters and below C1 for the AM broadcast band.


CORONAL MASS EJECTIONS/IONOSPHERIC STORMS/VISIBLE AURORA-

During the previous 7 day period no geo-effective (Earth facing) Coronal
Mass Ejections occurred. During the outlook period the probability of a
geo-effective (Earth facing) Coronal Mass Ejection (CME) is placed at 30%.



During the previous 7 day period a small Coronal Hole was in a geo-effective
(Earth facing) position. It's related Solar Wind Stream impacted the (IMF)
on 03/01/03-04, with a peak of 4 (Active), then with a Kp index of 3
(Unsettled) for the rest of the period.

During the outlook period no recurring Coronal Holes will rotate into
geo-effective (Earth facing) position and impact the (IMF).

The following related geomagnetic conditions will occur:

During the outlook period the probability of unsettled (Kp-3) geomagnetic
conditions is placed at 100%.

During the outlook period the probability of active (Kp-4) geomagnetic
conditions is placed at 40%.

During the outlook period the probability of at least a minor ionospheric
storm (Kp-5)(G1) is placed at 20%.

During the outlook period the probability of at least a moderate ionospheric
storm (Kp-6)(G2) is placed at 10%.

During the outlook period the probability of at least a strong ionospheric
storm (Kp-7+)(G3+) is placed at 0%.

G5 = Extreme - Kp = 9
G4 = Severe - Kp = 8
G3 = Strong - Kp = 7
G2 = Moderate - Kp = 6
G1 = Minor - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

During the outlook period the probability of a visible high latitude Aurora
display is placed at 100%, mid latitude 30%.

The Aurora Index at 0031 UTC 03/01/11 is a 7.

The NOAA POES historical database that was used to construct statistical
patterns of auroral power flux for each of the 10 levels of auroral activity
as defined by total power dissipation as illustrated in the following table.

Total Power Dissipation in Gigawatts/Activity Index Kp Index/Aurora Index

04-06/3/1+
10-16/5/2+
24-39/7/3+
61-96/9/5-


At 0218 UTC On 03/01/11 the Bz was 2.8 nt south.

The Wang-Sheeley Interplanetary Magnetic Field (IMF) Model which predicts
the Sun's IMF polarity, forecasts a negative (-) polarity between
03/01/11-03/01/16.


When the polarity of the IMF is negative a visible mid latitude Aurora
display is likely when a CME strikes the Earth's magnetic field. When the
polarity of the IMF is positive a visible mid latitude Aurora display is
unlikely as a CME strikes the Earth's magnetic field.

A Geomagnetic or Ionospheric Storm is a worldwide disturbance of the earth's
magnestosphere induced by the Sun's interplanetary magnetic field (IMF),
distinct from regular diurnal variations.

A Coronal Mass Ejection is the name given to an ejection of a large amount
of matter from the Sun's outer atmosphere or corona. These ejections
typically comprise millions of tons of material in the form of charged
particles, and can be seen because the material reflects sunlight. When one
of these ejections is directed towards the Earth (or conversely, directly
away from the Earth), it looks like a roughly circular "halo" surrounding
the Sun.

The "Halo CME's" then are those CME's which are more likely to impact the
Earth than those which are shot out at right angles to the Earth-Sun line.
Energetic protons emitted during CME's play a major role in increased day
time and night-time D-layer absorption of mediumwave frequencies.

Coronal Mass Ejections were once thought to be completely initiated by solar
flares. However it is now known that many (CME's) are not associated with
Solar Flares. If a (CME) collides with the Earth, it can excite a
Geomagnetic Storm if the polarity of the IMF has a negative sign. We must be
vigilant in watching for geoeffective (CME's), in order to not be caught by
surprise with a seemingly sudden and unexpected Geomagnetic Storm.

As the Kp index reaches 3-4, the aurora oval begins expanding equatorward in
magnetic latitude and generally begins having a negative impact on high
latitude medium frequency propagation paths. A Kp index of 5 or higher
begins to have a negative impact on high latitude high frequency shortwave
propagation paths. However at times skewed path propagation conditions can
compensate for high latitude propagation path auroral absorption.


STRATOSPHERIC WARMING-

During the past 7 day outlook period Stratospheric Warming did occur. During
the outlook period increased winter like day and year round night time D
layer absorption of medium frequency signals, tied to Stratospheric Warming
in the northern hemisphere is "probable".


As the SEC explains it:

Stratwarm: STRATWARM ALERT / SUNDAY / STRATWARM EXISTS INTENSE WARMING
CONTINUES IN THE UPPER STRATOSPHERE. WITHIN THE NEXT THREE DAYS: EASILY
WINDS AT 60N IN 1 HPA; REVERSED TEMPERATURE GRADIENT BETWEEN THE NORTH POLE
AND 60N FROM 10 TO 1 HPA; AN ELONGATION OF THE COLD POLAR VORTEX INTO TWO
CENTERS IN THE LOWER AND MID-STRATOSPHERE.

This occurrence is tied to intense warming in the Stratosphere due to the
cold Circumpolar Vortex splitting and shifting in it's Arctic position.

A little related Meteorology:

Interrelated with the splitting and shifting of the Arctic Circumpolar
Vortex, is a Tropospheric level negative North Atlantic Oscillation (NAO)
and Pacific-North America Anomaly (PNA), mid and upper air height anomaly
pattern. This equates to a large high pressure ridge in Western North
America extending northward all the way into the Yukon region of Canada and
a deep trough in the Eastern North America, from the eastern U.S. extending
down into the Yucatan region of Mexico, with a second ridge in the western
North Atlantic Ocean. This pattern is also called a dual blocking ridge and
taps Siberian Arctic air, sending it across the North Pole into the eastern
2/3's of Canada and the U.S.,providing for very cold surface temperatures.

As the stratosphere lies below the ionosphere, which is at mesosphere and
thermosphere height, you would not expect to see stratospheric warming
effect medium frequency propagation in any way BUT medium frequency signals
do propagate off of temperature inversions and moisture discontinuities and
a temperature inversion is involved with stratospheric warming. So it's
probable that a medium frequency signal could do any number of things when
scattering off of a temperature inversion, at any height. Unfortunately
though some otherwise very knowledgeable Physicists stubbornly resist this
concept.

Also stratospheric warming (STRATWARM) has a negative effect on medium
frequency propagation, due to increasing medium frequency radio wave
absorption by the D layer, via upward propagating Internal Gravity Waves
(IGW).

This phenomenon also occurs in southern hemisphere winter but seems to be
less pronounced.

73,
Thomas Giella, KN4LF
EL87WX
Plant City, FL, USA

KN4LF 160 Meter Amateur Radio Resources And More:
http://www.kn4lf.com

KN4LF Daily Solar Space Weather Geomagnetic Data Plus
MF Propagation Outlook:
http://www.kn4lf.com/kn4lf5.htm






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000901c2b909$66f0da60$6507a8c0@Main>
From: "Alan Melia" <Alan.Melia@btinternet.com>
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Hi Peter, I am not really in calibration at the moment and I have a limit of
+/- 0.1Hz. But for what its worth I make the lines 137.7446 and 137.7528. I
doubt whether Markus can hear(see) them at his location. I will try again
tomorrow when its a bit quieter, as they do make a useful marker at this end
of the band.

Cheers de Alan G3NYK
alan.melia@btinternet.com





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Hi all, the Trans-Atlantic path seems to be peaking about 10dB above average
tonight. It is still 5/6dB below the peaks on the best nights (5 & 6 Jan)
according to Steve's realtime plot. You may find the plot on my web-site in
place of the old CFH plot useful. It gives the plots for the 5th and 6th and
an average line for all the data between 19th Dec to 6th Jan. This is a
useful benchmark to put against the realtime plot. Geomag conditions have
been fairly quiet since about 19th Dec with the Kp not exceeding 4 since
then.

Steve's real time plot at www.w3eee.com

Cheers de Alan G3NYK
alan.melia@btinternet.com
http://www.alan.melia.btinternet.co.uk/latest.htm  for prop data.




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James Moritz wrote:

> Maybe that is a job for some future piece of software - but if you 
> have a few PCs lying around in the shack, there is nothing to stop you 
> doing it now - connect them all to the RX audio output , set one up 
> with a waterfall display to identify signals of interest, then set up 
> the rest running Jason decoders (or other modes, for that matter), so 
> that as soon as a signal is identified, one of the other  PCs can be 
> assigned to decode that signal
> [...]
> . 

And, if you have an AC97-compliant sound card, you can have multiple 
Jason and Argo and Spectran  etc. sessions all running
at the same time on the same PC. This is how I initially tested Jason : 
two copies on the same PC, one transmitting and the other
receiving. Hardly classifiable as a DX, but handy for testing.

73  Alberto  I2PHD




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From: "g3ldo" <g3ldo@ukonline.co.uk>
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Hi Markus


>saw both your nighttime and morning emissions, ufb signal up to
>10dBµV/m with QSB, drifting very slightly from 137769.93 to 769.96Hz.

>Last night, I joined in for a while:
>  23:16...23:52 on 137698.5 QRSS30 and
> 00:01...01:57 on 137699.95 / 700.05 DFCW(60+20).

Thank you for your report. Your  measurement put my frequency higher than I
thought it was.
I use Argo for frequency measurement. I make a calibration on 60kHz Rugby by
setting the receiver frequency dial to 59kHz USB. Rugby comes up at 1000Hz.
I then put the cursor over the signal and switch to narrow band mode 60s
dots. In my case the signal registers .2Hz high.
I have repeated the test with DFC39 and that is .5Hz high and the BBC on
198kHz is .6Hz high
Does anyone have an accurate measurement of the 'French' signal near 137750?


>With the green absorbers well frozen, aerial efficiency has gone up by 2dB
>to 0.135%, ie almost 0.5W E(D)RP from 200W TX power,
>including a few sparkling corona lights.

Your signal is much stronger than it used to be although I have not actually
measured it. A good antenna to put out such a good signal with only 200w.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>











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From: "Steve Dove" <dsp@hifidelity.com>
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Greetings,

Since there is talk of possible transatlantic tests again on 136kHz,  it may
be of interest that for some little while I've been running a near-real-time
signal-vs-time graph of DCF-39 as measured here in Pennsylvania.  The
site is still very much a work-in-progress, but should be useful as is:

http://www.w3eee.com

It operates on much the same principal as Dex, W4DEX's measurement
of HBG at 75kHz at:

http://www.gostanly.com/w4dex/index.html

(On the face of it, there seems to be NO correlation between 73kHz and 
136kHz, other than they both happen at night!).

Of course, for comparison with a shorter, intra-EU path, there is Brian,
CT1DRP's measurement of DCF at:

http://ct1drp.home.sapo.pt/index.htm

        73 all,

                Steve








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<html>
just to tease Alberto :<br>
shouldn't it be possible to decode multiple JASON signals within a
certain frequency window ? Main obstacle may be an algoritm that detects
signals from noise. And of course sufficient &quot;calculation
power&quot; would be needed, maybe we'll have to wait for the 10GHz
Pentium 7 processor ...<br><br>
73, Rik&nbsp; ON7YD<br>
&nbsp;<br>
At 11:28 10/01/2003 -0500, you wrote:<br>
<blockquote type=cite class=cite cite><font size=2>Dear Jim and
group,<br><br>
no criticism intended, but in my opinion machine-decoded modes like Jason
or WOLF have one disadvantage for long-haul propagation experiments: They
are exclusive, in the sense that potential receivers on the far side can
only see one signal at a time, whereas visual modes like QRSS or DFCW
allow several stations transmitting side by side.<br><br>
73 es best of luck<br>
Markus, DF6NM</font></blockquote></html>

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From: "hamilton mal" <g3kev.ham@virgin.net>
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<DIV><FONT face=Arial size=2>Reference recent info from Alaska. I have worked 
KL7 quite a number of times on 160 metres with very good sig reports each way, 
especially early in the morning here, could check the log for exact&nbsp; times 
if necessary, around 0600z/0700z at this time&nbsp;of year. Also worked W6 and 
W7 and VE7 at these times. </FONT></DIV>
<DIV><FONT face=Arial size=2>LF 136 khz could be a possibility, given a good 
antenna system at each end plus plenty of RF.</FONT></DIV>
<DIV><FONT face=Arial size=2>To be in with a chance a good high&nbsp;100 ft 
plus&nbsp;vertical resonated antenna&nbsp;at each end would be a start.&nbsp;At 
this distance and path forget about small loops and&nbsp;1 metre walking sticks. 
</FONT></DIV>
<DIV><FONT face=Arial size=2>73 de Mal/G3KEV IO94SH</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

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At 11:28 10/01/2003 -0500, you wrote:
>Dear Jim and group,
>
>no criticism intended, but in my opinion machine-decoded modes like Jason 
>or WOLF have one disadvantage for long-haul propagation experiments: They 
>are exclusive, in the sense that potential receivers on the far side can 
>only see one signal at a time, whereas visual modes like QRSS or DFCW 
>allow several stations transmitting side by side.
>
>73 es best of luck
>Markus, DF6NM

Dear Markus, LF group,

This is certainly a drawback of current digital modes - but not necessarily 
so with a "slow" mode like Jason, where the operator can read the received 
information at a much faster rate than the data is transmitted. In 
principle at least , you could do this: Digitise a relatively large 
bandwidth as a .wav file or similar, and store , for the sake of argument, 
30 minutes worth of data in memory. Then generate a waterfall display from 
this data , so that the operator could see the signals present. Then the 
operator could specify the frequency of a signal of interest, and the 
demodulation/ decoding DSP algorithm could decode the signal, again using 
the same data in memory. Having done that, the operator could repeat the 
procedure with another signal, and so on.  Since Jason et al transmit data 
slowly, and DSP algorithms can run quite fast, it should be possible to 
receive, store and process several signals simultaneously, and display them 
sequentially.

Maybe that is a job for some future piece of software - but if you have a 
few PCs lying around in the shack, there is nothing to stop you doing it 
now - connect them all to the RX audio output , set one up with a waterfall 
display to identify signals of interest, then set up the rest running Jason 
decoders (or other modes, for that matter), so that as soon as a signal is 
identified, one of the other  PCs can be assigned to decode that signal . 
At the moment, since there is no more than 1 Jason signal most of the time, 
this would only require 2 PCs, one to monitor the Jason frequency, and one 
to monitor the QRSS frequencies. The problem would be that the RX bandwidth 
would have to be wide enough to include 135.9xx kHz, as well as 137.5kHz., 
so the RX would probably be overloaded if anyone local was QRV in the CW 
band segment . But that might not be a problem in the USA. An easy solution 
would be If I  transmitted the Jason beacon closer to the "transatlantic" 
segment, so that all the signals would fit through a CW filter. If anyone 
would care to try this, and would care to nominate a suitable frequency 
near 135.9kHz, I could do that now.....

Cheers, Jim Moritz
73 de M0BMU




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From: "John Andrews" <w1tag@charter.net>
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Markus,

Two thoughts regarding your comments on the machine-decoded modes:

1. Jason and WOLF (especially if it ever moves into real time) have the
ability to move enough information in a reasonable amount of time, to permit
2-way contacts. It seems proper to be testing that approach. The band seems
wide enough to accomodate the operation.

2. Please do beat the drum to get more QRSS fellows to beacon in clusters.
There's been fairly little of that operation this year. And unless we're
notified over here in Western Pond-Land, there won't be anyone looking.
Since I'm out a lot in the evening, I will probably miss messages sent at
2300 that someone is going to beacon for a few hours. A little advance
warning would be a help.

John Andrews, W1TAG



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From: "Dave Pick" <g3yxm@wireless.org.uk>
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<DIV><FONT face=Arial size=2>That's a good point Markus.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I thought of joining the beacon test but there 
would be no point as only one signal can be in the window at once.</FONT></DIV>
<DIV><FONT face=Arial size=2>We could do a timed window idea with different 
stations at different times on the same frequency I suppose?</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Dave</FONT></DIV>
<DIV><FONT face=Arial size=2>G3YXM.</FONT></DIV>
<BLOCKQUOTE 
style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV 
  style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
  <A title=MarkusVester@aol.com 
  href="mailto:MarkusVester@aol.com">MarkusVester@aol.com</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A title=rsgb_lf_group@blacksheep.org 
  href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org</A> 
  </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Friday, January 10, 2003 4:28 
  PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> Re: LF: Jason Beacon 
  signals</DIV>
  <DIV><BR></DIV><FONT face=arial,helvetica><FONT lang=2 face=Arial size=2 
  FAMILY="SANSSERIF">Dear Jim and group,<BR><BR>no criticism intended, but in my 
  opinion machine-decoded modes like Jason or WOLF have one disadvantage for 
  long-haul propagation experiments: They are exclusive, in the sense that 
  potential receivers on the far side can only see one signal at a time, whereas 
  visual modes like QRSS or DFCW allow several stations transmitting side by 
  side.<BR><BR>73 es best of luck<BR>Markus, 
DF6NM</BLOCKQUOTE></FONT></FONT></BODY></HTML>

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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Dear Jim and group,<BR>
<BR>
 no criticism intended, but in my opinion machine-decoded modes like Jason or WOLF have one disadvantage for long-haul propagation experiments: They are exclusive, in the sense that potential receivers on the far side can only see one signal at a time, whereas visual modes like QRSS or DFCW allow several stations transmitting side by side.<BR>
<BR>
73 es best of luck<BR>
Markus, DF6NM<BR>
</FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Dear LF Group,

I am planning to run the Jason beacon again tonight and during the weekend. 
I aim to start tonight around 2200 utc and carry on until about 0300. 
Frequency will be centered on 137.5025kHz, in an attempt to dodge some of 
the Loran spectral lines present across the pond. I am hoping for some 
further transatlantic signal reports, but of course any other signal 
reports will also be very welcome.

Cheers, Jim Moritz
73 de M0BMU



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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Peter,<BR>
<BR>
oops, correction... that should have been "137768.93 to 768.96Hz". Yes, there is a built-in error-checking function here - it's automagically activated by hitting the "send" button ;-(<BR>
<BR>
Markus, DF6NM<BR>
<BR>
<BLOCKQUOTE TYPE=CITE style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px">saw both your nighttime and morning emissions, ufb signal up to 10dBµV/m with QSB, drifting very slightly from 137769.93 to 769.96Hz.</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"></BLOCKQUOTE><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi Peter,<BR>
<BR>
saw both your nighttime and morning emissions, ufb signal up to 10dBµV/m with QSB, drifting very slightly from 137769.93 to 769.96Hz.<BR>
<BR>
Last night, I joined in for a while:<BR>
&nbsp; 23:16...23:52 on 137698.5 QRSS30 and<BR>
&nbsp; 00:01...01:57 on 137699.95 / 700.05 DFCW(60+20).<BR>
<BR>
With the green absorbers well frozen, aerial efficiency has gone up by 2dB to 0.135%, ie almost 0.5W E(D)RP from 200W TX power, including a few sparkling corona lights.<BR>
<BR>
73 de Markus, DF6NM<BR>
<BR>
<BR>
<BLOCKQUOTE TYPE=CITE style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px">0630Z<BR>
<BR>
I am making a test transmission in the hope that it may be received by<BR>
KL1X - frequency 137.7695kHz QRSS60<BR>
If anyone sees it I would appreciate a frequency check.<BR>
<BR>
Regards,<BR>
Peter, G3LDO<BR>
</BLOCKQUOTE><BR>
<BR>
</FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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0630Z

 I am making a test transmission in the hope that it may be received by
KL1X - frequency 137.7695kHz QRSS60
If anyone sees it I would appreciate a frequency check.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>





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Dex...will you be QRSSing tomorrow night & Saturday night with the loopers?
If condx hold up I would like to have another crack at the six- pack...or is
it seven ?

Steve / VE7SL



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Hi Dave

"Anyone" might be able to receive NDBs over a reasonable distance but like
any other area of listening there are some who manage to hear things that
most others don't.
Perhaps you'd better give some of the Canadian and South American NDBs a try
if they're so easy to receive? :-)

73s Tracey

> That bloke seems to really like Wellbrook stuff....
> Has anyone ever tried one as a 136 receiving antenna? How does it cope
with
> being under a TX antenna on power?
> Anyone can receive beacons and broadcast stations! ;-)




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A small horizontal loop cannot generate vertical polarisation though, so 
presumably it just radiates vertically upwards, in which case what does the 
polarisation come down as after reflection ?  Will it be arbitrary ?

Andy  G4JNT

-----Original Message-----
From:	Laurie Mayhead [SMTP:laurie@g3aqc.freeserve.co.uk]
Sent:	2003/01/09 13:23
To:	rsgb_lf_group@blacksheep.org
Subject:	LF: Re. LF noise

Hi Walter,
Perhaps the reason why "noise"is vertically polarised is that noise sources
are close to ground,even at HF.
Hence ground losses inhibit the establishment of horizontal
polarisation.This is more so the lower the frequency, at LF it is impossible
to generate Horiz. polarisation using reasonable heights.I know of no LF
antenna that can produce horiz. polarisation.Perhaps the story is different
at VHF/UHF.
73 Laurie G3AQC




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Hi Walter,
Perhaps the reason why "noise"is vertically polarised is that noise sources
are close to ground,even at HF.
Hence ground losses inhibit the establishment of horizontal
polarisation.This is more so the lower the frequency, at LF it is impossible
to generate Horiz. polarisation using reasonable heights.I know of no LF
antenna that can produce horiz. polarisation.Perhaps the story is different
at VHF/UHF.
73 Laurie G3AQC




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>Apart from that, can anyone tell me why local noise IS a 
>vertically-polarised E-field problem? I can intuitively (I think) 
>understand that it would be E-field since it is primarily a high-impedance 
>phenomenon; but why VERTICALLY-polarised? If it's radiated from local 
>house wiring etc surely it should be randomly-polarised and just as 
>evident on horizontally-polarised antennas? I have a 30 m vertical I 
>occasionally use on 80m and a horizontal dipole for 80m near it. VERY 
>often there is so much noise on the vertical I can't even hear my local 
>net; on the horizontal at the same time there is only the faintest trace 
>of noise and everyone is easily audible.  Same on 160m. All the texbooks 
>agree local noise is vertically-polarised but not one of them explains why.

Hello Walter,

Maybe "local noise" is vertically polarized because it is generated 
"against ground" : the wiring in the house acts as antenna, the ground as 
counterweight. As far as I got it any "against ground" fed antenna is 
vertically polarized, a nice example is the DDRR antenna that is a 
completely horizontal construction and yet a vertical polarized antenna.
But there might be another reason for the high noise levels on your vertical :
Years ago I contructed a full-sized Marconi antenna for 7MHz. In an attempt 
to be smart I connected just a few short radials and used the "house 
grounding stake" as counterweight. That worked fine on TX (antenna 
resistance was very close to 36 Ohm) but I had a tremendous noiselevel on 
RX. Disconnecting the "house grounding stake" solved the noise problem, but 
I had to add more and longer radials to get the antenna impedance back to 
36 Ohm.

73, Rik  ON7YD



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Dear Tracey, LF group,

At 16:50 08/01/2003 +0000, you wrote:
>John Wilson did a comparison test in the Nov 2001 Short Wave Magazine
>between the RF Systems 520 and the Wellbrook Communications LFL1010 VLF loop
>antenna and the 520 was well beaten by the 1010 .
>
>http://www.wellbrook.uk.com/LFL1010.html
>
>The SWM review of the 520/1010 and John's savage comments about the 520 can
>be found here! :-)
>
>http://www.wellbrook.uk.com/reviews/SWM2001Nov.html

Looking at this review, it does not actually contain the information you 
really want to know for a receiving antenna, ie.is the antenna noise floor 
below the band noise level?. Unless that is true, it would not be much use 
for weak signal reception. However, the reviewer does compare the SNR when 
receiving what appears to be DCF29 (DBF29?) on 128.93kHz (see fig 3 and the 
paragraph above), and on the LFL1010 (the better of the two), gets an SNR 
of 33dB. I usually find this signal is 50 - 60dB over the band noise (in 
300Hz BW - the bandwidth used in the test also does not seem to be stated), 
so it looks like this antenna has rather poor sensitivity, even though the 
reviewer likes it. The tests seem to have taken place near Exmoor, so 
somewhat further from DL than me, but I would not think far enough to 
reduce the signal level by 20dB. I suppose it is possible the transmitter 
was running lower power that day, but "Caveat Emptor", as Mr Wilson says!

Incidentally, the stuff about having to mount an E-field antenna on a 
grounded metal pole is a bit peculiar - so long as the feeder is grounded 
somewhere, it should be happy. Also the idea that local noise is 
predominantly E-field is certainly not universally true, and at LF, in my 
opinion, probably a myth.

Cheers, Jim Moritz
73 de M0BMU




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Re the 520/1010 discussion.  Wilsons' main objection to the 520 appears to 
be that it suffers from a great deal of local noise pickup, which actually 
would be expected from ANY vertically-polarised E-field antenna. An H-field 
antenna; e.g. a loop, does not so suffer but this is a fundamental physical 
fact and should not be attributed to the 520 as if it were something wrong 
with that antenna itself. These little active verticals are very handy for 
restricted spaces; e.g. on boats, where there simply isn't the space to put 
up a loop; but mounting them on a grounded metal mast is ESSENTIAL - if 
they're put up on a fibreglass pole they will have far less pickup.  I had 
one on my boat top of the mast and it could pick up 10w 300 kHz DGPS 
stations 800 kms away in daylight  - no local noise there, of course (at 
least, when the engine was off!).

Apart from that, can anyone tell me why local noise IS a 
vertically-polarised E-field problem? I can intuitively (I think) 
understand that it would be E-field since it is primarily a high-impedance 
phenomenon; but why VERTICALLY-polarised? If it's radiated from local house 
wiring etc surely it should be randomly-polarised and just as evident on 
horizontally-polarised antennas? I have a 30 m vertical I occasionally use 
on 80m and a horizontal dipole for 80m near it. VERY often there is so much 
noise on the vertical I can't even hear my local net; on the horizontal at 
the same time there is only the faintest trace of noise and everyone is 
easily audible.  Same on 160m. All the texbooks agree local noise is 
vertically-polarised but not one of them explains why.

Incidentally for 80m reception my horizontal dipole out-performs not only 
the vertical but also a 1m dia loop quite easily both in terms of s/n ratio 
and absolute pickup. I suspect the same would be true of 136 kHz if anyone 
ever had the space to put up a 136 kHz horizontal dipole at a reasonable 
height!  Now THERE's a challenge for G3KEV.

And a Happy New Year to all!!!

Walter G3JKV.


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From: "Thomas Giella" <kn4lf@tampabay.rr.com>
To: "a HCDX E-List" <hard-core-dx@hard-core-dx.com>, 
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Please pardon my test.

73,
Thomas Giella, KN4LF
EL87WX
Plant City, FL, USA

KN4LF Daily Solar Space Weather Geomagnetic Data Plus 
MF Propagation Outlook:
http://www.kn4lf.com/kn4lf5.htm

KN4LF 160 Meter Amateur Radio Resources And More:
http://www.kn4lf.com


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Pick" <g3yxm@wireless.org.uk>
To: rsgb_lf_group@blacksheep.org
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That bloke seems to really like Wellbrook stuff....
Has anyone ever tried one as a 136 receiving antenna? How does it cope with
being under a TX antenna on power?
Anyone can receive beacons and broadcast stations! ;-)

Dave
G3YXM

> John Wilson did a comparison test in the Nov 2001 Short Wave Magazine
> between the RF Systems 520 and the Wellbrook Communications LFL1010 VLF
loop
> antenna and the 520 was well beaten by the 1010 .
>
> http://www.wellbrook.uk.com/LFL1010.html
>
> The SWM review of the 520/1010 and John's savage comments about the 520
can
> be found here! :-)
>
> http://www.wellbrook.uk.com/reviews/SWM2001Nov.html
>
> 73s Tracey
>
>
> >
> > Anybody have experiences with receiving antenna LFA 520 from RF SYSTEMS
?
> >
> > Rich OM2TW
> >
>
>
>




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Hi Rich

John Wilson did a comparison test in the Nov 2001 Short Wave Magazine
between the RF Systems 520 and the Wellbrook Communications LFL1010 VLF loop
antenna and the 520 was well beaten by the 1010 .

http://www.wellbrook.uk.com/LFL1010.html

The SWM review of the 520/1010 and John's savage comments about the 520 can
be found here! :-)

http://www.wellbrook.uk.com/reviews/SWM2001Nov.html

73s Tracey


>
> Anybody have experiences with receiving antenna LFA 520 from RF SYSTEMS ?
>
> Rich OM2TW
>



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From: "James Moritz" <j.r.moritz@herts.ac.uk>
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Dear Lawrence, LF Group,

At 11:45 30/12/2002 -0900, you wrote:

> From Laurence aka Flo AL1V (G4DMA) BP41xd 10Kms SW Anchorage Alaska.
>
>Hi Im now QRV on Rx on this band using Argo 131
>
>The 138.8Khz Eu beacon signal is audible to S9+ in the mornings before 
>2030Z and from 2300Z. (It is very variable on a minute to min basis)
>
>Long wave stations are even audible thru my winter dayliight hours with 
>France Inter on 162 and others on 153 sometimes HI quality. BBC R4 is 
>never strong and is very close to the local US NDB's
>
>If we take this as a good indicator of band conditions,Id be interested to 
>know how strong this beacon is being received on the Eastern states at the 
>time that Eu stations are audible...there may be a chance..we are about 
>6000Kms from the UK.


Nice to have another part of the world to aim at....
DCF39 on 138.83k has about 40kW ERP, so will be roughly 50dB up on most 
amateur signals of somewhat less than 1W ERP. So if DCF39 gives about 
20-30dB SNR in a few hundred Hz CW bandwidth, it should be possible to copy 
European signals using QRSS signals with small fractions of a Hz bandwidth. 
Of course, what that translates to on the S meter depends very much on that 
particular meter! W4DEX has received several European signals over a 
similar distance, but a somewhat different path, so I guess Alaska should 
be quite feasible

>The path to Europe tends to cross a large cross section of the Au Oval but 
>whether this is going to make a large difference to prop unless under 
>extreme proton events I dont know.

It would certainly be interesting to see what the difference is in 
propagation to Alaska compared to other parts of the USA - As well as that, 
I would expect you will get considerably less thunderstorm QRN than in the 
more southern states, which would certainly help reception.

Wishing you good luck on LF,

Cheers, Jim Moritz
73 de M0BMU





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From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
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Hi Teo and all,
Many thanks Teo for the report yesterday, looks like a good signal. I will
transmit again this afternoon from 1530 on 71.8kHz.
 I will be using DFCW 15sec elements, 1Hz shift (use 10s ARGO),each CQ call
will take 10mins.I will be looking on 137.650kHz  for 3sec.QRSS replies.
73 Laurie.




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Hi LF-ers...

Anybody have experiences with receiving antenna LFA 520 from RF SYSTEMS ?

Rich OM2TW


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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi Peter,<BR>
<BR>
welcome to the LF reflector !<BR>
My transmission started at Jan 7th, 23:30 and ended today Jan 8th, 01:07 UT.<BR>
<BR>
Good luck<BR>
Markus<BR>
<BR>
<BLOCKQUOTE TYPE=CITE style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px">Hi Markus,</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">currently means all day long the 8-th of january?&nbsp; </FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">73 </FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Peter, dj9dw - experimenting with the "GAMAL-Loop"</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2"></BLOCKQUOTE><BR>
<BLOCKQUOTE TYPE=CITE style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px"><BLOCKQUOTE TYPE=CITE style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px"><BR>
I am currently transmitting on 137770+-0.05Hz DFCW, 60s on / 20s off, until about 0:30 UT.<BR>
<BR>
73<BR>
Markus, DF6NM</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"></BLOCKQUOTE><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2"></BLOCKQUOTE><BR>
<BR>
</FONT></HTML>

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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi group,<BR>
<BR>
since the beginning of Dec. 2002, the daytime 153kHz BC emissions were again accompanied by the infamous spurious sidebands centered around 136kHz up to -57dBc, and a number of amateur stations in South Germany have reported increased noise levels in QSOs. After another telephone call, the system engineers in Donebach could apparently fix the spurious sidebands yesterday, and it has been relatively quiet since 13:27 UT. <BR>
<BR>
The problem seems to be a design flaw in the 250kW AEG PANTEL transmitters, as it is present in both of their two units. It is caused by an unidentified parasitic oscillation in the 54-kHz swich-mode modulator drive circuitry. It was found empirically that chilling a certain CD4011 IC largely suppressed the sidebands, and the ad-hoc solution is opening up the modulator compartment and placing the affected circuit board on an extender board. - On the other hand, this condition is not very well reproducible, and the problem tends to reappear especially at high room temperatures in summer.<BR>
<BR>
73 de Markus, DF6NM<BR>
</FONT></HTML>

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<DIV><FONT face=Arial size=2>Hi Markus,</FONT></DIV>
<DIV><FONT face=Arial size=2>currently means all day long the 8-th of 
january?&nbsp; </FONT></DIV>
<DIV><FONT face=Arial size=2>73 </FONT></DIV>
<DIV><FONT face=Arial size=2>Peter, dj9dw - experimenting with the 
"GAMAL-Loop"</FONT></DIV>
<BLOCKQUOTE 
style="PADDING-RIGHT: 0px; PADDING-LEFT: 5px; MARGIN-LEFT: 5px; BORDER-LEFT: #000000 2px solid; MARGIN-RIGHT: 0px">
  <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV 
  style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
  <A title=MarkusVester@aol.com 
  href="mailto:MarkusVester@aol.com">MarkusVester@aol.com</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A title=rsgb_lf_group@blacksheep.org 
  href="mailto:rsgb_lf_group@blacksheep.org">rsgb_lf_group@blacksheep.org</A> 
  </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Wednesday, January 08, 2003 12:53 
  AM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: Re: Strange Signal</DIV>
  <DIV><BR></DIV><FONT face=arial,helvetica><FONT lang=2 face=Arial size=2 
  FAMILY="SANSSERIF">Hi group,<BR><BR>I am currently transmitting on 
  137770+-0.05Hz DFCW, 60s on / 20s off, until about 0:30 
  UT.<BR><BR>73<BR>Markus, DF6NM<BR></BLOCKQUOTE></FONT></FONT></BODY></HTML>

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Date: Tue, 07 Jan 2003 20:10:31 -0500
From: "Andre Kesteloot" <andre.kesteloot@verizon.net>
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Subject: LF: Off subject  :-)
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A "nostalgia" site for (some of) the readers of this reflector...
73
André

http://www.militaryradio.com/spyradio



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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Hi group,<BR>
<BR>
 I am currently transmitting on 137770+-0.05Hz DFCW, 60s on / 20s off, until about 0:30 UT.<BR>
<BR>
73<BR>
Markus, DF6NM<BR>
</FONT></HTML>

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From: "Alberto di Bene" <dibene@usa.net>
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References: <3E19A930.8010706@usa.net> <154365002515.20030106211845@dx.ru> <3E1AE882.500@usa.net> <000901c2b667$9f7002c0$33c828c3@erica> <008001c2b673$ada71de0$b7bdfea9@nnn0hus>
Subject: Re: LF: Argo V1 build 132
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Thomas Giella KN4LF wrote:

>Can we get the Argo V1 build 132 software to balance my check book and fix
>my XP O/S
>when it crashes?
>
>  
>
I'm working on that.  When you won't hear anymore of me, and suddenly I 
disappear
from the Internet community, then maybe you will be right in guessing 
that I succeeded
in programming Argo to positively interact with my bank account.
And when I say "positively", I mean it in the algebraic acception of the 
word..... :-)

73  Alberto  I2PHD
 



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From: "WE0H" <we0h@gentekcom.com>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 7 Jan 2003 16:42:27 -0600
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
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<p class=MsoNormal><span class=EmailStyle15><font size=2 color=navy face=Arial><span
style='font-size:10.0pt;mso-bidi-font-size:12.0pt;font-family:Arial'>If they
write it, I&#8217;ll read it. If I don&#8217;t like it, I&#8217;ll hit the delete key.<o:p></o:p></span></font></span></p>

<p class=MsoNormal><span class=EmailStyle15><font size=2 color=navy face=Arial><span
style='font-size:10.0pt;mso-bidi-font-size:12.0pt;font-family:Arial'><![if !supportEmptyParas]>&nbsp;<![endif]><o:p></o:p></span></font></span></p>

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12.0pt;font-family:Arial'><span style='mso-element:field-begin'></span><span 
style="mso-spacerun: yes">&nbsp;</span>AUTOTEXTLIST \s &quot;E-mail 
Signature&quot; <span style='mso-element:field-separator'></span></span></font></span><![endif]--><font
color=navy><span style='color:navy'>Mike&gt;WE0H</span></font><font color=navy><span
style='color:navy;mso-color-alt:windowtext'><o:p></o:p></span></font></p>

<p class=MsoAutoSig><font size=3 color=navy face="Times New Roman"><span
style='font-size:12.0pt;color:navy'><a href="http://www.we0h.us/lf">http://www.we0h.us/lf</a></span></font><font
color=navy><span style='color:navy;mso-color-alt:windowtext'><o:p></o:p></span></font></p>

<p class=MsoNormal><!--[if supportFields]><span class=EmailStyle15><font 
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class=EmailStyle15><font size=2 color=navy face=Arial><span style='font-size:
10.0pt;mso-bidi-font-size:12.0pt;font-family:Arial'><![if !supportEmptyParas]>&nbsp;<![endif]><o:p></o:p></span></font></span></p>

<p class=MsoNormal style='margin-left:.5in'><font size=2 color=black
face=Tahoma><span style='font-size:10.0pt;font-family:Tahoma;color:black'>-----Original
Message-----<br>
<b><span style='font-weight:bold'>From:</span></b>
owner-rsgb_lf_group@blacksheep.org [mailto:owner-rsgb_lf_group@blacksheep.org]<b><span
style='font-weight:bold'>On Behalf Of </span></b>hamilton mal<br>
<b><span style='font-weight:bold'>Sent:</span></b> Tuesday, January 07, 2003
11:57 AM<br>
<b><span style='font-weight:bold'>To:</span></b> rsgb_lf_group@blacksheep.org<br>
<b><span style='font-weight:bold'>Subject:</span></b> LF: Argo</span></font></p>

<p class=MsoNormal style='margin-left:.5in'><font size=3 face="Times New Roman"><span
style='font-size:12.0pt'><![if !supportEmptyParas]>&nbsp;<![endif]><o:p></o:p></span></font></p>

<p class=MsoNormal style='margin-left:.5in'><font size=2 color=black
face=Arial><span style='font-size:10.0pt;font-family:Arial;color:black'>Has
ARGO taken over the LF reflector, never seen so much trivial comment. Try some
private email to the writer. Does it matter what format the date happens to be
presented, plus other comments like well done, poor etc. Genuine comments like
compatibility observations&nbsp;by some about the type of computer&nbsp;used
are ignored. </span></font><font color=black><span style='color:black;
mso-color-alt:windowtext'><o:p></o:p></span></font></p>

<p class=MsoNormal style='margin-left:.5in'><font size=2 color=black
face=Arial><span style='font-size:10.0pt;font-family:Arial;color:black'>G3KEV</span></font><font
color=black><span style='color:black;mso-color-alt:windowtext'><o:p></o:p></span></font></p>

<p class=MsoNormal style='margin-left:.5in'><font size=3 color=black
face="Times New Roman"><span style='font-size:12.0pt;color:black'>&nbsp;</span></font><font
color=black><span style='color:black;mso-color-alt:windowtext'><o:p></o:p></span></font></p>

<p class=MsoNormal style='margin-left:.5in'><font size=3 color=black
face="Times New Roman"><span style='font-size:12.0pt;color:black'>&nbsp;</span></font><font
color=black><span style='color:black;mso-color-alt:windowtext'><o:p></o:p></span></font></p>

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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dexter McIntyre" <dmcintyre@att.net>
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To: "RSGB LF" <rsgb_lf_group@blacksheep.org>, 
 "lowfer" <lowfer@mailman.qth.net>
Subject: LF: 15db drop in HBG today, 2003-01-07-0600
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There was a sudden 15 dB drop in the 75 kHz HBG signal received here in
NC at just before 0600 UT.  Looks like it was down for about half and
hour then suddenly came back up to normal.  The noise floor, which
usually fluctuates with propagation changes, remained constant during
this time.  Transmitter maintenance maybe?

Plot can be seen at:

http://www.w4dex.com/75khz/hbg07dec02.jpg

Near real time plot can be seen at:

http://www.w4dex.com/75khz/hbg.jpg

Dex


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From: "Thomas Giella KN4LF" <kn4lf@gbronline.com>
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Date: Tue, 7 Jan 2003 15:55:30 -0500
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Can we get the Argo V1 build 132 software to balance my check book and fix
my XP O/S when it crashes?

Hope no one was offended by my dry sense of humor when I posted the above.
Seeing that I'm still new to LF, all posts here have been very helpful to
me. Not
many are interested in LF yet on this side of the big pond but I think that
will change
when we get our 2200 meter allocation.

73,
Thomas Giella, KN4LF
EL87WX
Plant City, FL, USA

kn4lf@gbronline.com
kn4lf@tampabay.rr.com

KN4LF 160 Meter Amateur Radio Resources And More:
http://www.kn4lf.com

KN4LF Daily Solar Space Weather Geomagnetic Data Plus
MF Propagation Outlook:
http://www.kn4lf.com/kn4lf5.htm




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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "Bob Eldridge " <r.c.eldridge@ieee.org>
Message-ID: <E18Vynv-0001ZC-00@twiddle.look.ca>
Date: Tue, 07 Jan 2003 13:50:24 -0500
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Subject: LF: Date format
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>Isn't the most logical one YYYY/MM/dd  ? 
>Does anyone use this format routinely ?
>Andy  G4JNT>

This has been the international standard for at least 25 years, intended to
avoid the confusion between the U.S. and the rest of the world. I adopted it
for everything in the days of Comm 64, as the computer automatically sorted
dates as if they were numbers, and hours and minutes could be added as well
for logging. The Year 2K mess should have converted everyone!


Bob VE7BS



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Staubach" <walter.staubach@fen-net.de>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 7 Jan 2003 18:50:38 +0100
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Subject: LF: Re: 73kHz JASON
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Hallo Laurie,
      see your signal with good strength, but due to local qrm bad
reception. I think the signal would be good for QRSS or DFCW.
73  Walter DJ2LF

-----Ursprüngliche Nachricht-----
Von: Laurie Mayhead <laurie@g3aqc.freeserve.co.uk>
An: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Datum: Dienstag, 7. Januar 2003 16:53
Betreff: LF: 73kHz JASON


>Hi All,
>Having sorted that one out, my apologies to all, I will have another go at
>JASON on 71.8kHz USB over the twilight period here ,1630 to 1730 UTC.
>Reports welcome.
>73 Laurie.
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 7 Jan 2003 19:21:18 +0100
From: "YU7AR" <yu7ar@pyrotherm.co.yu>
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To: "Laurie Mayhead" <rsgb_lf_group@blacksheep.org>
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Subject: Re: LF: 73kHz JASON
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--------------050104010803030209000603
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Hello Laurie,

Your signals is very good in KN05BW ,see the screen capture.

 73 Teo
-- 
Best regards,
 YU7AR                            mailto:yu7ar@pyrotherm.co.yu

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From: "hamilton mal" <g3kev.ham@virgin.net>
To: rsgb_lf_group@blacksheep.org
References: <3E19A930.8010706@usa.net> <154365002515.20030106211845@dx.ru> <3E1AE882.500@usa.net> <000901c2b667$9f7002c0$33c828c3@erica>
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----- Original Message -----
From: "g3ldo" <g3ldo@ukonline.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, January 07, 2003 4:11 PM
Subject: Re: LF: Argo V1 build 132


>
> Hi Alberto
>
> > Boys, that screen is becoming fast crowded... but maybe that callsign
> > could just automagically
> > show only in the captured images, without cluttering the normal
> viewing....
>
> What Alberto has produces is an effective yet simple and easy to piece of
> software. You don't have to know about technical things like 'FFTs, 'bins'
> and 'sampling times' to set it up and use it. I have worked in software
> development places where there always seems to be a "wouldn't it be nice
if"
> section who want to add things until the whole SW package becomes unwieldy
> and difficult to use.
> I propose that ARGO is left much as it is unless any new bugs are found or
> some new way of processing the signals is found.

Agree. It works perfectly well for what was intended. If you need more as I
do sometimes use something else like Spectran or Speclab
> For the more technical there is Spectran and SpectrumLab.
> It is easy to add cSpectran and Speclab.

allsigns to images using any package that handles .JPG
> files.
>
> Regards,
> Peter, G3LDO
>
> e-mail <g3ldo@ukonline.co.uk>
>
> Web <http://web.ukonline.co.uk/g3ldo>
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "hamilton mal" <g3kev.ham@virgin.net>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 7 Jan 2003 17:57:20 -0000
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<DIV><FONT face=Arial size=2>Has ARGO taken over the LF reflector, never seen so 
much trivial comment. Try some private email to the writer. Does it matter what 
format the date happens to be presented, plus other comments like well done, 
poor etc. Genuine comments like compatibility observations&nbsp;by some about 
the type of computer&nbsp;used are ignored. </FONT></DIV>
<DIV><FONT face=Arial size=2>G3KEV</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "hamilton mal" <g3kev.ham@virgin.net>
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----- Original Message ----- 
From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, January 07, 2003 1:29 PM
Subject: LF: 73kHz ARGO


> Actually I don't know how to transmit ARGO !
> so many messages about it that my brain flipped.
Exactly my observations, never seen so much gibberish.
> I did in fact transmit JASON from 0830 until about 1015 this morning. 73s
> Laurie.
> 
> 
> 



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Thomas Giella KN4LF" <kn4lf@gbronline.com>
To: rsgb_lf_group@blacksheep.org
References: <3E19A930.8010706@usa.net> <154365002515.20030106211845@dx.ru> <3E1AE882.500@usa.net> <000901c2b667$9f7002c0$33c828c3@erica>
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Can we get the Argo V1 build 132 software to balance my check book and fix
my XP O/S
when it crashes?

73,
Thomas Giella, KN4LF
EL87WX
Plant City, FL, USA

kn4lf@gbronline.com
kn4lf@tampabay.rr.com

KN4LF 160 Meter Amateur Radio Resources And More:
http://www.kn4lf.com

KN4LF Daily Solar Space Weather Geomagnetic Data Plus
MF Propagation Outlook:
http://www.kn4lf.com/kn4lf5.htm



----- Original Message -----
From: "g3ldo" <g3ldo@ukonline.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, January 07, 2003 11:11 AM
Subject: Re: LF: Argo V1 build 132


>
> Hi Alberto
>
> > Boys, that screen is becoming fast crowded... but maybe that callsign
> > could just automagically
> > show only in the captured images, without cluttering the normal
> viewing....
>
> What Alberto has produces is an effective yet simple and easy to piece of
> software. You don't have to know about technical things like 'FFTs, 'bins'
> and 'sampling times' to set it up and use it. I have worked in software
> development places where there always seems to be a "wouldn't it be nice
if"
> section who want to add things until the whole SW package becomes unwieldy
> and difficult to use.
> I propose that ARGO is left much as it is unless any new bugs are found or
> some new way of processing the signals is found.
> For the more technical there is Spectran and SpectrumLab.
> It is easy to add callsigns to images using any package that handles .JPG
> files.
>
> Regards,
> Peter, G3LDO
>
> e-mail <g3ldo@ukonline.co.uk>
>
> Web <http://web.ukonline.co.uk/g3ldo>
>
>
>
>


---
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Johan Bodin" <sm6lkm.jbeab@swipnet.se>
To: rsgb_lf_group@blacksheep.org
References: <3E19A930.8010706@usa.net> <3E19BF5D.3D63E21A@att.net> <002501c2b5ca$b31defa0$12c5e150@RSGB613192> <00b901c2b620$e8e18e20$bc33f7c2@a7j7r2>
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Yes, we use the YMD format in Sweden, falling digit significance
from left to right. We use this strange format for normal numbers too ;-)

CU on 713 Hkz

73
Johan SM6LKM


----- Ursprungligt meddelande ----- 
Från: "John Rabson" <word.factory@zetnet.co.uk>
Till: <rsgb_lf_group@blacksheep.org>
Skickat: den 7 januari 2003 08:39
Ämne: Re: LF: Argo V1 build 132


> The Swedes?
> John Rabson G3PAI
> 
> ----- Original Message ----- 
> From: "Andy Talbot" <G4JNT@THERSGB.NET>
> To: <rsgb_lf_group@blacksheep.org>
> Sent: Monday, January 06, 2003 9:29 PM
> Subject: Re: LF: Argo V1 build 132
> 
> 
> > Isn't the most logical one YYYY/MM/dd  ? 
> > Does anyone use this format routinely ?
> > Andy  G4JNT
> > 
> > 
> > ----- Original Message ----- 
> > From: Dexter McIntyre <dmcintyre@att.net>
> > To: <rsgb_lf_group@blacksheep.org>
> > Cc: <lowfer@mailman.qth.net>
> > Sent: Monday, January 06, 2003 5:39 PM
> > Subject: Re: LF: Argo V1 build 132
> > 
> > 
> > > Looks great Alberto!  
> > > 
> > > >>Alberto di Bene wrote:
> > > >> I used this format :  MMM, dd, yyyy
> > > 
> > > I thought sure you would be the logical dd,MMM,yy type :)
> > > 
> > > W4DEX
> > > 
> > > 
> > 
> > 
> > 
> 
> 
> 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
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Hi Alberto

> Boys, that screen is becoming fast crowded... but maybe that callsign
> could just automagically
> show only in the captured images, without cluttering the normal
viewing....

What Alberto has produces is an effective yet simple and easy to piece of
software. You don't have to know about technical things like 'FFTs, 'bins'
and 'sampling times' to set it up and use it. I have worked in software
development places where there always seems to be a "wouldn't it be nice if"
section who want to add things until the whole SW package becomes unwieldy
and difficult to use.
I propose that ARGO is left much as it is unless any new bugs are found or
some new way of processing the signals is found.
For the more technical there is Spectran and SpectrumLab.
It is easy to add callsigns to images using any package that handles .JPG
files.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 7 Jan 2003 15:59:54 -0000
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Hi All,
Having sorted that one out, my apologies to all, I will have another go at
JASON on 71.8kHz USB over the twilight period here ,1630 to 1730 UTC.
Reports welcome.
73 Laurie.




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Ed Lesnichy wrote:

>Can then and callsign that who accepts it?
>or callsing + QTH-loc? hi! ....
>
>Callsign  to  establish  in  Setup.  Conveniently  for  captured  down
>files... Who accepted it at once is seen in the files, sent by others..
>
>  
>
Ed,
      not sure I fully understand your request.
Do you mean that you would like to have the callsign of the station that 
is running Argo displayed
somewhere on the screen ?
Boys, that screen is becoming fast crowded... but maybe that callsign 
could just automagically
show only in the captured images, without cluttering the normal viewing....

73  Alberto  I2PHD
 




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Subject: Re: LF: Argo 132
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Hugh M0WYE wrote:

>I like the date too. (which comes out as day, month, year ... even though
>"MMM,DD,YY" appears on the screen moments before the real date appears)
>  
>
That's a just a place holder, which is briefly shown when the  program 
starts, before it has the
first chance to update that field.

>I hope you get some time to operate radio in between the software writing !
>  
>
Yes, almost every evening I partecipate in a local round table on 2m, 
mainly dealing with technical
topics and projects. The hot subject of the moment is a precision LC 
meter I am building around
an Atmel AVR AT90S4433 microcontroller, inspired to the AADE unit, but 
with some improvements.
If/when it will be ready, I will publish it on my site. The software 
will be free, of course.

And when there are announced transmissions on LF, I try to receive 
something, sometimes with
success.  At present I am lacking a decent LF antenna.

73  Alberto  I2PHD





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From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
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Actually I don't know how to transmit ARGO !
so many messages about it that my brain flipped.
I did in fact transmit JASON from 0830 until about 1015 this morning. 73s
Laurie.



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From: "Hugh M0WYE" <m0wye@thersgb.net>
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References: <LEEGIKOMHIEKBPDOHLOIGEMBCBAA.we0h@gentekcom.com> <3E18C3D3.1030808@usa.net> <000401c2b517$3dc6a8e0$0500a8c0@charter.net> <3E196AE8.3060104@usa.net>
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Hello Alberto,
The explorer style dialogue works well.
Thankyou for fixing it so quickly.
I like the date too. (which comes out as day, month, year ... even though
"MMM,DD,YY" appears on the screen moments before the real date appears)

I hope you get some time to operate radio in between the software writing !

73
Hugh M0WYE




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From: "John Rabson" <word.factory@zetnet.co.uk>
To: rsgb_lf_group@blacksheep.org
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The Swedes?
John Rabson G3PAI

----- Original Message ----- 
From: "Andy Talbot" <G4JNT@THERSGB.NET>
To: <rsgb_lf_group@blacksheep.org>
Sent: Monday, January 06, 2003 9:29 PM
Subject: Re: LF: Argo V1 build 132


> Isn't the most logical one YYYY/MM/dd  ? 
> Does anyone use this format routinely ?
> Andy  G4JNT
> 
> 
> ----- Original Message ----- 
> From: Dexter McIntyre <dmcintyre@att.net>
> To: <rsgb_lf_group@blacksheep.org>
> Cc: <lowfer@mailman.qth.net>
> Sent: Monday, January 06, 2003 5:39 PM
> Subject: Re: LF: Argo V1 build 132
> 
> 
> > Looks great Alberto!  
> > 
> > >>Alberto di Bene wrote:
> > >> I used this format :  MMM, dd, yyyy
> > 
> > I thought sure you would be the logical dd,MMM,yy type :)
> > 
> > W4DEX
> > 
> > 
> 
> 
> 



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From: "Mike Dennison" <mike.dennison@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
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> A continious carrier on 137.7708kHz, with an occasional burs of
modulation,
> has been on most of the evening. Anyone know what it is? Quite strong - S7
> on the meter.
> Peter, G3LDO

I was on that frequency from 1755 to 1914 sending 'XDV' in QRSS120. The
dashes and dots were made from 30s elements which is the longest my memory
keyer will produce. This produces slight 'blips' on the signal. Anything
after 1914 was not me.

Mike, G3XDV
http://www.lf.thersgb.net
====================



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "WE0H" <we0h@gentekcom.com>
To: rsgb_lf_group@blacksheep.org
Date: Mon, 6 Jan 2003 21:31:02 -0600
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Thank you.

Mike>WE0H
http://www.we0h.us/lf

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of Alberto di Bene
Sent: Monday, January 06, 2003 9:28 AM
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Argo 1.31 bug report

g6tmk wrote:

>Hi Alberto,
>What about having a "browse" button next to the "file prefix" box on the
>capture setup dialogue, which brings up an Explorer style thing to select
or
>add the right directory (sorry ... folder). ?
>
>
>
Hi Hugh,

   already done.... i have just finished modifying and compiling build
132 of Argo,
which now behaves just as you say. You cannot anymore modify the prefix name
directly in the edit box, but you have to choose it in an explorer-like
tree, where
you can also create a new directory, if you so need.

I am just now modifying the home page, but if you are impatient, you can
already
download it from this URL :  http://www.weaksignals.com/bin/argopak1_132.exe

73  Alberto  I2PHD







From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "WE0H" <we0h@gentekcom.com>
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Date: Mon, 6 Jan 2003 21:28:32 -0600
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That would be a very nice feature. Can we have it Alberto???

Mike>WE0H
http://www.we0h.us/lf

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of g6tmk
Sent: Monday, January 06, 2003 6:52 AM
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Re: Argo 1.31 bug report

Hi Alberto,
What about having a "browse" button next to the "file prefix" box on the
capture setup dialogue, which brings up an Explorer style thing to select or
add the right directory (sorry ... folder). ?

I guess all the code to do these interfaces must be in Windows somewhere -
after all that's the point of using such a gigantic operating system ...

I bet it's not that simple !

73
Hugh M0WYE








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From: "Andy Talbot" <G4JNT@THERSGB.NET>
To: rsgb_lf_group@blacksheep.org
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Subject: Re: LF: Argo V1 build 132
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Isn't the most logical one YYYY/MM/dd  ? 
Does anyone use this format routinely ?
Andy  G4JNT


----- Original Message ----- 
From: Dexter McIntyre <dmcintyre@att.net>
To: <rsgb_lf_group@blacksheep.org>
Cc: <lowfer@mailman.qth.net>
Sent: Monday, January 06, 2003 5:39 PM
Subject: Re: LF: Argo V1 build 132


> Looks great Alberto!  
> 
> >>Alberto di Bene wrote:
> >> I used this format :  MMM, dd, yyyy
> 
> I thought sure you would be the logical dd,MMM,yy type :)
> 
> W4DEX
> 
> 




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 06 Jan 2003 23:00:37 +0100
From: "Alberto di Bene" <dibene@usa.net>
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Subject: Re: LF: Argo V1 build 132
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Andy Talbot wrote:

>Isn't the most logical one YYYY/MM/dd  ? 
>Does anyone use this format routinely ?
>Andy  G4JNT
>
>  
>
That's why I made the format customizable by simply modifying
the Regional Settings in the Control Panel.
You can choose whatever format most pleases you.
Mine was just an example,  not a must.

73  Alberto  I2PHD




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From: "g3ldo" <g3ldo@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
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Subject: LF: Strange Signal
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This is a multi-part message in MIME format.
--------------010404010808010505020901
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A continious carrier on 137.7708kHz, with an occasional burs of modulation,
has been on most of the evening. Anyone know what it is? Quite strong - S7
on the meter.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>


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--------------010404010808010505020901--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <001001c2b5ca$49dc70c0$ea00a8c0@f3a3a2>
From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Date: Mon, 6 Jan 2003 21:23:52 -0000
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Subject: LF: 73kHz ARGO
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Should anyone be interested I am transmitting ARGO tonight on 71.8kHz ,until
2200 utc.
I will be on again in the morning from 0830 utc for about   one hour.
73s Laurie.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 6 Jan 2003 21:18:45 +0300
From: "Ed Lesnichy" <ed@dx.ru>
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To: "Alberto di Bene" <rsgb_lf_group@blacksheep.org>
In-reply-to: <3E19A930.8010706@usa.net>
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Alberto,

Monday, January 6, 2003, you wrote:

AdB> There are just a couple of mods :
AdB> - On the main panel now also the date is shown, in addition to the time

Can then and callsign that who accepts it?
or callsing + QTH-loc? hi! ....

Callsign  to  establish  in  Setup.  Conveniently  for  captured  down
files... Who accepted it at once is seen in the files, sent by others..

TNXs for the excellent program !

73! Ed  RU6LA  ed@dx.ru



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Argo V1 build 132
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Looks great Alberto!  

>>Alberto di Bene wrote:
>> I used this format :  MMM, dd, yyyy

I thought sure you would be the logical dd,MMM,yy type :)

W4DEX



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Subject: LF: Argo V1 build 132
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I have just uploaded Argo V1 build 132 to the weaksignals site.

There are just a couple of mods :

- On the main panel now also the date is shown, in addition to the time

- An error has been corrected, where strange things happened if you
  specified an inexistent path for the capture file. This dialog has been
  rewritten.

Just one note : the date format used is what is set on your PC, in the
Regional Settings panel. Open the Windows Control Panel, then select
Regional Settings, then the tab Date (should be the last one).
Here set the  Short Date Style as you please. I used this format :  MMM 
dd, yyyy
(cut and paste that directly into the edit field).
If you choose a too long format, then the date display could corrupt the
peak display on the panel of Argo.

URL for downloading :  http://www.weaksignals.com

Enjoy and report any errors,  thanks.

73  Alberto  I2PHD




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Subject: LF: Re:  Argo 1.31 bug report
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g6tmk wrote:

>Hi Alberto,
>What about having a "browse" button next to the "file prefix" box on the
>capture setup dialogue, which brings up an Explorer style thing to select or
>add the right directory (sorry ... folder). ?
>
>  
>
Hi Hugh,

   already done.... i have just finished modifying and compiling build 
132 of Argo,
which now behaves just as you say. You cannot anymore modify the prefix name
directly in the edit box, but you have to choose it in an explorer-like 
tree, where
you can also create a new directory, if you so need.

I am just now modifying the home page, but if you are impatient, you can 
already
download it from this URL :  http://www.weaksignals.com/bin/argopak1_132.exe

73  Alberto  I2PHD





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Hi Alberto,
What about having a "browse" button next to the "file prefix" box on the
capture setup dialogue, which brings up an Explorer style thing to select or
add the right directory (sorry ... folder). ?

I guess all the code to do these interfaces must be in Windows somewhere -
after all that's the point of using such a gigantic operating system ...

I bet it's not that simple !

73
Hugh M0WYE






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Subject: LF: Re:  Argo 1.31 bug report
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John Andrews wrote:

>>OK, due to the gentle but firm way my arm has been bent, I will
>>spontaneously honor
>>this request  :-)
>>    
>>
>
>It hopefully won't be too difficult to type with your arm in that condition.
><g>
>Tnx.
>  
>

Oh, when I was an ape, in a previous life, I learnt how to type with the 
feet.... I will use
the remaining arm to hold a cup of strong Italian coffe, it helps to not 
fall asleep
between two C++ rows....

73  Alberto  I2PHD




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Thread-Topic: LF: Loops again
Thread-Index: AcKqvVSHFNvwmRzOQFG9IshGWthZawKrzoHw
From: jan-martin.noding@telenor.com
To: rsgb_lf_group@blacksheep.org
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Subject: Measuring antenna performance, was "Re: LF: Loops again"
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Happy New Year.
What is important for those receiving aerials is the actual S/N in the receiver. 
One aerial may have higher signal, but also higher noise. So the actual performance 
may not have been improved at all.

Once did some comparisons between different aerials at P.O. Laboratories at Bearley, near Stratford on Avon,
but I couldn't verify that the log.meter worked as it should. So I've had some interest to build a better 
equipment later.

One possibility is to use two SPM-3 (Pegelmesser's) - one set for 138.8 kHz, and the other for reference on
quiet spot of the band.
The other is to measure S/N directly from the signal output from SPM-3 or D2006.

Does somebody know some circuits I could build for reasonable accuracy?

73,
Jan-Martin

N4623-Kristiansand (tel.: +47-380-87178 Home)(38052660 Work 90777126 Mobile)
http://www.laud.no/la6nca/LA8AK/ 

-----Opprinnelig melding-----
Fra: James Moritz [mailto:j.r.moritz@herts.ac.uk]
Sendt: 23. desember 2002 20:49
Til: rsgb_lf_group@blacksheep.org
Emne: Re: LF: Loops again


At 16:55 23/12/2002 +0000, you wrote:
>With all the loop talk that has been going on since before time began has 
>anyone found a design for a near perfect small loop, suppose its like how 
>long is a piece of string, obviously the bigger the better but then there 
>is the diminishing returns senario, it there much noticeable difference 
>between a 2 meter side square loop and a 4meter.

How much signal power a loop can deliver to the receiver depends on 2 
factors - the area, and the Q (or losses). How much you need  depends on 
the overall system design; how good or bad the RX is, whether you want to 
trade off sensitivity against bandwidth, have a wide tuning range, etc., so 
yes, it is a "how long is a piece of string" question. But as a rough 
guide, a 1m^2 tuned loop with a sensibly designed preamp, or with good 
matching to a low noise receiver will give a noise floor well below the 
band noise. The signal to noise ratio of the loop is good, but the absolute 
signal level is much smaller than with a vertical, so the performance of 
the receiver is much more important. If you double the size to 4m^2, the 
design becomes a lot less critical because you are picking up 12dB more 
signal to start with. With very large loops, almost anything will deliver 
more than adequate signal levels, but then you lose the advantages of a 
small loop - being able to rotate it for optimum peaking or nulling, and 
being able to move it to find a location with low noise levels.

>Which is better a single turn loop, several turns in series, several turns 
>in parallel and the best method of feed and matching at the loop.

It is largely a matter of convenience of design - Several alternatives have 
been mentioned; they all work if done properly.

>I have a lot of information about all of these loops little and large but 
>never used a very small loop and might try but there is a lot of 
>conflicting info about the various configurations and I do not want to re 
>invent the wheel so if someone has had good practical results it would be 
>useful.

Maybe it would be a good idea not to keep saying how they are all rubbish 
before you have actually tried them...

>I have been watching QRS activity lately while in the shack doing other 
>things and notice a lot of CQ'S from various amateurs around the UK and 
>Europe and sometimes all going at once, the screen is getting cluttered, 
>but only a few result in QSO'S so it would appear obvious to me that the 
>majority are not seeing each other, and that would indicate poor receiving 
>capabilities.

...Or that they worked each other a couple of days ago.

>I appear to be receiving all of the activity but my 90 meter perimiter 
>loop is reasonably large and is doing well on receive but not as good as 
>my vertical, however I would like to try a very small loop and compare 
>results, but I dont want to build several small loops varying in design, 
>if someone has already done this and knows which ones to forget about.
>I know location is also important, good ground, reasonable and poor ground 
>etc under the loop and some use loops to null out qrm but I am not 
>concerned about qrm, this location is rural and as qrm free as one can 
>get, this is why my vertical is also good on receive.
>Please dont tell me to read the Comic, I need todays technology.
>73 de Mal/G3KEV
>

If you have no QRM, and adequate sensitivity already, you can't expect to 
gain much from other types of antennas. Perhaps you need to install more of 
today's technology - light dimmers, home entertainment systems, compact 
florescent bulbs, computers etc. etc. so you can really put things to the test!

Cheers, Jim Moritz
73 de M0BMU






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From: jan-martin.noding@telenor.com
To: rsgb_lf_group@blacksheep.org
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Interesting to know, 
but I bought mine around 2000-2001, so I am surprised that I didn't get the latest version. hi.
Not sure whether I bought it from RSGB or DARC

73 Jan-Martin, LA8AK

-----Opprinnelig melding-----
Fra: g3ldo [mailto:g3ldo@ukonline.co.uk]
Sendt: 24. desember 2002 02:30
Til: rsgb_lf_group@blacksheep.org
Emne: LF: Re: LF Handbook





> I think what Jan-Martin has is the old LF Experimenters Sourcebook which
is
> a comb bound compilation with a blue cover, of copies of articles
published
> before 1995. In fact I think there were two editions of the "Sourcebook".
> The book Dick is refering to is a later glossy bound printed book (pub
2001)
> which is much more up to date with current projects., including Dave's
Amp.
> LF is moving so fast that we will be needing an update of that book soon
!!
>
> Cheers de Alan G3NYK

Yes, Alan is right. The original LF Experimenters Sourcebook was produced in
1996 in response to a requirement for information for the then new 73kHz
allocation in the UK. Information for this book came from such sources as
'LF Scene' (by ZL1CA & ZL2BBJ), a column from the New Zealand ham radio mag
'Break In' and 'The Lowdown', the magazine of the Longwave Club of America;
these guys were the only ones with experiance in LF at the time. It was
produced comb bound with a blue cover.
A second edition was produced in 1998. By this time we had some experiance
of our own to include and we also had the new 136kHz band. This publication
also was produced comb bound with a blue cover.
These publications were produced rather hurredly to meet a need and the
pages were photocopies of paste-ups. A higher quality publication was
required and this was met with 'The Low Frequency Experimenter's Handbook',
which was published in 2000.
I have included an Addendum and Erratta to this book on my website, shown
below. Work on this site is a bit behind shedule but it will be updated very
shortly. I have a mass of stuff that has been edited from hundreds of
e-mails on the LF reflector and this also will be included.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>







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From: "John Andrews" <w1tag@charter.net>
To: rsgb_lf_group@blacksheep.org
References: <LEEGIKOMHIEKBPDOHLOIGEMBCBAA.we0h@gentekcom.com> <3E18C3D3.1030808@usa.net>
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> OK, due to the gentle but firm way my arm has been bent, I will
> spontaneously honor
> this request  :-)

It hopefully won't be too difficult to type with your arm in that condition.
<g>
Tnx.

John Andrews




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From: "WE0H" <we0h@gentekcom.com>
To: rsgb_lf_group@blacksheep.org
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All right, you're the man Alberto. Thank you.

Mike>WE0H
http://www.we0h.us/lf

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of Alberto di Bene
Sent: Sunday, January 05, 2003 5:46 PM
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Argo 1.31 bug report


> While you're playing with the code, how about adding the date next to the
> time? <g>

> What a good idea.
>
> 73


>Most definitely. It is hard to tell what day the captures are from without
a
>date. Please add it if it isn't too awful of a job.
>
>

OK, due to the gentle but firm way my arm has been bent, I will
spontaneously honor
this request  :-)

73  Alberto  I2PHD






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> While you're playing with the code, how about adding the date next to the
> time? <g>

> What a good idea.
>
> 73


>Most definitely. It is hard to tell what day the captures are from without a
>date. Please add it if it isn't too awful of a job.
>  
>

OK, due to the gentle but firm way my arm has been bent, I will 
spontaneously honor
this request  :-)

73  Alberto  I2PHD





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But be aware that the generated JPG file will show the date/time under
Windoz Explorer when
it is created. 

Use this as a patch until the next update

Bob  K3DJC
 

On Sun, 5 Jan 2003 10:03:52 -0600 "WE0H" <we0h@gentekcom.com> writes:
>Most definitely. It is hard to tell what day the captures are from 
>without a
>date. Please add it if it isn't too awful of a job.
>Thanks,
>Mike>WE0H
>
>Mike
>
>-----Original Message-----
>From: owner-rsgb_lf_group@blacksheep.org
>[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of John Andrews
>Sent: Sunday, January 05, 2003 9:55 AM
>To: rsgb_lf_group@blacksheep.org
>Subject: Re: LF: Argo 1.31 bug report
>
>Alberto,
>
>> Expect soon build 132.
>
>While you're playing with the code, how about adding the date next to 
>the
>time? <g>
>
>John Andrews
>
>
>
>
>



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From: "Laurence J Howell" <L.Howell@conocophillips.com>
Date: Sun, 5 Jan 2003 13:17:28 -0900
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>From : Laurence KL1X, BP 41 XD, 10 Kms W Anchorage.(was AL1V till
yesterday)

Using a number of sources including the German data txm on 138.8XKhz,
conditions to EU long haul continue to be depressed and estimated  max 40+
dB down on signals at the same time of day, pre the recent disturbance of
elevated K/Au etc. The data signal at times peaked S9+25 on a quiet
background, save Loran spurs; its averaging S5 at the moment.

Even with the present poor conditions I can still hear some Eu LF broadcast
stations +24 hours including the very strong Norwegian signal on 153Khz

All paths to Europe (and Africa)from here run into/across/within the
Auroral Oval, both sides, and dependant on them nasty Protons and other
factors, LF signals are depressed as much as HF is. Its going to be a
challenge!

The receiver sits most of the time  centered on 137.770 plus or minus 1.5Hz
using QRSS60. Im capturing most of the day and night.

Regards

Laurence (Flo)
Please note the new email address
L.HOWELL@CONOCOPHILLIPS.COM



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From: "G4WGT" <g4wgt@talkgas.net>
To: rsgb_lf_group@blacksheep.org
Date: Sun, 5 Jan 2003 19:15:46 -0000
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What a good idea.

73

Gary  G4WGT

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of John Andrews
Sent: 05 January 2003 15:55
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Argo 1.31 bug report

Alberto,

> Expect soon build 132.

While you're playing with the code, how about adding the date next to the
time? <g>

John Andrews
---

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Subject: RE: LF: Argo 1.31 bug report
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Most definitely. It is hard to tell what day the captures are from without a
date. Please add it if it isn't too awful of a job.
Thanks,
Mike>WE0H

Mike

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of John Andrews
Sent: Sunday, January 05, 2003 9:55 AM
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Argo 1.31 bug report

Alberto,

> Expect soon build 132.

While you're playing with the code, how about adding the date next to the
time? <g>

John Andrews





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<DIV><FONT face=Arial size=2>Hi Group:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Splendid "O" signal from DF0WD calling at 11.37 
UTC,</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Gary and Group:

Thanks a lot for your report.
I hope to contact you soon on LF.

73 de José, EA1PX


> Saw your CQ calls on Sunday morning at 0947, 0957, 1026 all at M sigs & at
> 1118 at T sigs, did not see any resulting QSO from the calls. My location
> north west UK, Loc IO83QP.






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Alberto,

> Expect soon build 132.

While you're playing with the code, how about adding the date next to the
time? <g>

John Andrews



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hugh wrote:

>Hi Alberto et al,
>Forgive me if this has already been reported.
>On the capture menu, if you enter setup, and enter a file prefix, which
>includes a path which is not valid, then the program accepts it ... until
>you click "capture now" and then it says it can't create the file.
>After that it removes "Capture" from the menu at the top and won't let you
>correct the mistake  !  You have to restart the program.
>[...]
>  
>
Hi Hugh and Jay,
      bug reproduced and confirmed.  Sorry, my mistake.
Expect soon build 132.   Thanks for reporting.

73  Alberto  I2PHD





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From: "G4WGT" <g4wgt@talkgas.net>
To: "Rsgb_Lf_Group" <rsgb_lf_group@blacksheep.org>
Date: Sun, 5 Jan 2003 12:08:22 -0000
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Hi Jose & LF,

Saw your CQ calls on Sunday morning at 0947, 0957, 1026 all at M sigs & at
1118 at T sigs, did not see any resulting QSO from the calls. My location
north west UK, Loc IO83QP.

Screen capture showing your CQ call approx 0957.

Was not able to monitor from 1030 to 1112 due to a sked on 40 Mtrs & rig in
use there.

73

Gary  G4WGT.
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--------------060903020204060303020301--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hugh & Alberto

Ditto - noticed the same thing on my system.

Jay Rusgrove, W1VD

Hugh wrote:

> Hi Alberto et al,
> Forgive me if this has already been reported.
> On the capture menu, if you enter setup, and enter a file prefix, which
> includes a path which is not valid, then the program accepts it ... until
> you click "capture now" and then it says it can't create the file.
> After that it removes "Capture" from the menu at the top and won't let you
> correct the mistake  !  You have to restart the program.
>
> I'm using build 131 on a Win 98SE machine. (Pentium III, 700MHz,
> Soundblaster 1024)
>
> Nice QRSS signals received from G3LDO and G3XDV this morning, about 09:30.
> So it doesn't stop me using some very excellent software.
> Thanks Alberto.
>
> 73
> Hugh M0WYE
>
> ----- Original Message -----
> From: Alberto di Bene <dibene@usa.net>
> To: <rsgb_lf_group@blacksheep.org>
> Sent: Tuesday, December 24, 2002 6:37 PM
> Subject: Re: LF: Spectran DSP Audio Problem
>
> > Thomas Giella, KN4LF wrote:
> >
> > >I'm experiencing the same problem as others have mentioned. The DSP
> filters
> > >in Spectran
> > >do not alter the audio.
> > >
> > >
> > >
> > Thomas,
> >     what you hear with most probability is the audio going directly from
> > the line input
> > to the speakers.  See the very good  explanation given by Jim Moritz on
> > this subject,
> > and his suggestions on how to proceed.
> >
> > 73  Alberto  I2PHD
> >
> >
> >
> >



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From: "Hugh" <g6tmk@thersgb.net>
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Hi Alberto et al,
Forgive me if this has already been reported.
On the capture menu, if you enter setup, and enter a file prefix, which
includes a path which is not valid, then the program accepts it ... until
you click "capture now" and then it says it can't create the file.
After that it removes "Capture" from the menu at the top and won't let you
correct the mistake  !  You have to restart the program.

I'm using build 131 on a Win 98SE machine. (Pentium III, 700MHz,
Soundblaster 1024)

Nice QRSS signals received from G3LDO and G3XDV this morning, about 09:30.
So it doesn't stop me using some very excellent software.
Thanks Alberto.

73
Hugh M0WYE








----- Original Message -----
From: Alberto di Bene <dibene@usa.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, December 24, 2002 6:37 PM
Subject: Re: LF: Spectran DSP Audio Problem


> Thomas Giella, KN4LF wrote:
>
> >I'm experiencing the same problem as others have mentioned. The DSP
filters
> >in Spectran
> >do not alter the audio.
> >
> >
> >
> Thomas,
>     what you hear with most probability is the audio going directly from
> the line input
> to the speakers.  See the very good  explanation given by Jim Moritz on
> this subject,
> and his suggestions on how to proceed.
>
> 73  Alberto  I2PHD
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "g3ldo" <g3ldo@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
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Andy  G4JNT said:

>I have a suite of programmes that calculate distance bearing, as well as a
height database of the UK for plotting terrain maps and microwave paths,
plus a database of most of the decent highspot. /P locations in the UK and a
few other worldwide plotting utilities   The progs operate together so it
isn't possible to supply just the one that converts NGR/Latlong/UTM and
calculates distance and bearings.   The whole suite is 1.4Meg zipped up and
I'll send you a copy direct, and to anyone else wanting it.

-------------------------------------------------------------

I have been using Andy's Distance Calculator and Slow Morse program for some
years now. It is installed on a cheap laptop dedicated to LF and radio
calculation DOS programs - and they work fine.
Why should a distance calculator be 'off topic'? I only started using it
when I got into LF.

Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dr. Tom Gruis", "=?iso-8859-1?B?S9hIVEY=?=" <donnatom@netins.net>
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Subject: Re: LF: Distance calculator  (off topic)
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<!DOCTYPE html PUBLIC "-//W3C//DTD HTML 4.01 Transitional//EN">
<html>
<head>
  <meta http-equiv="Content-Type" content="text/html;charset=ISO-8859-1">
  <title></title>
</head>
<body>
Hi from Iowa, USA!<br>
<br>
&nbsp;&nbsp;&nbsp; Please shhot me an E-copy of your distance calculating program!<br>
<br>
Many thanx &amp; 73,<br>
<br>
Doc.<br>
<br>
Walter Blanchard wrote:<br>
<blockquote type="cite"
 cite="mid5.1.0.14.2.20030104180813.00a0e1a0@mail.pncl.co.uk"> At 07:32 04/01/03
G0MRF wrote:<br>
  <br>
 
  <blockquote type="cite" class="cite" cite=""><font face="arial"
 size="2">Hello Group.&nbsp;&nbsp;&nbsp; Happy New Year. <br>
    <br>
 Does anyone know of, or have, any windows software that can calculate distances
based on the UK National Grid Reference system?&nbsp; (e.g.&nbsp; TQ147951 ) <br>
    <br>
 I have one for the Maidenhead system (if anyone would like it just ask) but
not for calculating distance between two NGR's. <br>
    <br>
 Many Thanks <br>
    <br>
 73 <br>
    <br>
 David</font><font face="arial"> </font></blockquote>
  <font face="arial"><br>
  <br>
 I wrote a little program 15 yrs ago to do this, available free to anyone 
who wants it.<br>
 Also converts&nbsp; NGR to/from lat/lon at about the 10m level.<br>
 Will not pass this reflector as an attachment. Sent one to David direct.<br>
  <br>
 NGR distances are easy to do in a spreadsheet . Unlike&nbsp; Maidenhead and Lat/Lon&nbsp;
  <br>
 NG is a true rectilinear grid so if you know how to translate NGR's<br>
 given as e.g. TQ 169483&nbsp; into actual Eastings and Northings in terms of
metres<br>
 all you have to do is a root sum of squares equation.&nbsp; Done this way <br>
 distances will be correct but bearings will be in terms of Grid North - about<br>
 2 degs different&nbsp; from True North in Central England. My program corrects
for this<br>
 and gives bearings as degs True. <br>
  <br>
 If you really want to go to town get onto Ordnance Survey's&nbsp; GPS website
-<br>
 <a href="http://www.gps.gov.uk/" eudora="autourl">www.gps.gov.uk</a> , get
a password and log in and you can get, free, a <br>
 massive 10 Mb program that converts everything to everything at millimetre
  <br>
 accuracy (GridInquest). Or it lets you do conversions on-line.<br>
  <br>
 Walter G3JKV.<br>
 &nbsp;</font>
  <pre wrap="">
<hr width="90%" size="4">

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  </pre>
</blockquote>
<br>
</body>
</html>

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From: "Thomas Giella KN4LF" <kn4lf@gbronline.com>
To: "a Greyline Prop E-List" <greyline@yahoogroups.co.uk>, 
 "a RSGB LF E-List" <rsgb_lf_group@blacksheep.org>,
 "a PSC E-List" <PSC.Committee@rsgb.org.uk>, 
 "a HCDX Prop Channel" <propagation@hard-core-dx.com>
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KN4LF 7 Day Medium Frequency Radio Propagation Outlook

#2003-02 Published 11:00 PM EST 03/01/03 For 03/01/04-03/01/10.


PROPAGATION OUTLOOK-

Expect fair to good domestic propagation conditions on east-west paths and
poor to fair on north south paths in the northern hemisphere out to
approximately 1050 miles.

Expect fair domestic propagation conditions on east-west paths and poor on
north south paths in the southern hemisphere out to approximately 1050
miles.


"High latitude" northern hemispheric (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be poor to fair.

"High latitude" southern hemispheric (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be poor.


"Mid latitude" northern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be fair to good.

"Mid latitude" southern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
and cross equatorial propagation conditions in excess of approximately 3000
miles should be fair.


"Low latitude" northern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
propagation conditions in excess of approximately 3000 miles should be good.

"Low latitude" southern hemisphere (TA) Trans Atlantic, (TP) Trans Pacific
propagation conditions in excess of approximately 3000 miles should be fair.


QRN OUTLOOK-

During the outlook period there will be "high" lightning induced QRN levels
in low latitude areas of the northern hemisphere due to proximity of the
Inter Tropical Convergence Zone (ITCZ).

Northern hemisphere mid latitude regions can expect "moderate to
occasionally high" lightning induced QRN tied to cold season thunderstorms,
cold/warm/occluded fronts and associated extra-tropical cold core low
pressure systems. These weather systems are currently being enhanced by the
moderate level El Nino ocean water temperature anomaly.

Northern hemisphere high latitude regions can expect "low to occasionally
moderate" lightning induced QRN tied to cold season thunderstorms,
cold/warm/occluded fronts and associated extra-tropical cold core low
pressure systems. These weather systems are currently being enhanced by the
moderate level El Nino ocean water temperature anomaly.


During the outlook period there will be "high" lightning induced QRN levels
in low latitude areas of the southern hemisphere tied to warm season
thunderstorms and tropical systems.

Southern hemisphere mid latitude regions can expect "moderate to high"
lightning induced QRN, tied to warm season thunderstorms and tropical
systems.

Southern hemisphere high latitude regions can expect "moderate" lightning
induced QRN, tied to warm season thunderstorms and tropical systems.


Here are some general guidelines concerning correlation of space weather and
propagation indices to actual expected HF/MF propagation conditions.

1.) Dropping indices numbers are better.

2.) Solar flux under 150 okay, under 100 better, 70 is best for E layer
multi hop.

2a.) For high frequencies (HF) solar flux of 100 is okay, 150 better, above
200 best.

3.) Solar flux of at least 100 for E valley-F layer ducting mechanism.

4.) Previous 24 hour Ap index under 10, under 7 for several days
consecutively is best.

5.) Previous 3 hour Kp index under 3 for mid latitude paths, under 2 for
high latitude paths, 0-1 for several days consecutively is best.

6.) Energetic protons no greater then 10 MeV (10+0) for 160/120 meters and
no greater then (10-1) on MF broadcast band.

7.) Background x-ray flux levels less than C2 for several days consecutively
for 160/120 meters and less then C1 for MF broadcast band.

8.) No current STRATWARM alert.

9.) IMF Bz with a negative sign, indicates a better chance of high latitude
path auroral absorption/unpredictable refraction or scattering of MF RF
signals, when the Kp is above 3.


SPACE WEATHER INDICES DURING THE PAST 7 DAY PERIOD, SPACE WEATHER INDICES
EXPECTED DURING THE 7 DAY OUTLOOK PERIOD AND EXPLANATIONS OF THEIR IMPACT ON
ANTICIPATED PROPAGATION CONDITIONS.


ENERGETIC PROTON FLUX-

During the previous 7 day period no elevated energetic proton flux events of
>10 MeV (10+0) occurred.

During the 7 day outlook period the probability of an elevated energetic
proton flux event >10 MeV (10+0) is placed at 20%.


An elevated energetic proton flux level greater then (10+0) on 160 meters
and greater then (10-1) on the medium frequency broadcast band creates
noticeably increased winter time day and year round night time D layer
absorption of medium wave frequencies, especially on high latitude
propagation paths but it can also negatively impact mid latitudes, depending
on the intensity of the event.

Elevated energetic proton events too small to be categorized as a Polar Cap
Absorption event (PCA) can still impact high and mid level medium frequency
propagation paths in the form of excessive D layer absorption. This fact is
still stubbornly opposed by some otherwise very knowledgeable space weather
physicists over dependent on high latitude threshold Riometer readings.

((((Note, high latitude medium frequency radio propagation paths can still
be disturbed for days and up to weeks, following the end of an official >10
MeV (10+0) proton event.))))


SOLAR FLUX-

During the previous 7 day period the daily solar flux level ranged between
145 and 111. The 111 is the lowest daily solar flux value to occur since
January 1999!

During December 2002 the daily solar flux ranged between 245 and 111. During
2002 the daily solar flux ranged between 275 and 111. As a comparison, in
2001 it ranged between 294 and 123.

During the outlook period the daily solar flux values should range between
approximately 185 and 135.

During the previous 7 day period the daily "average" Background X-Ray Flux
level ranged between B2.6 and B1.7.


Elevated background X-ray flux levels can impact propagation of medium
frequency signals in a negative manner. Background X-ray flux levels of C1
or greater creates increased D-layer absorption of 160 and 120 meter signals
and B9 or greater creates increased D-layer absorption of AM broadcast band
signals.

Remember though that there are daily extremes of the Background X-ray flux
level. So even though the daily average might have been good at say B2.2,
the daily "extreme" maximum could have been C1.5, which would have been bad
and have cause a short period of increased D layer absorption.

High solar flux values are generally considered to be detrimental to
propagation of medium frequency signals both domestic and Trans Atlantic
(TA) & Trans Pacific (TP), as more absorption can be present via the
transmitted signals' two trips through the D layer at the takeoff and
arrival points.

Most "strong" longer haul medium frequency DX signals in excess of 3000
miles is via the E Valley-F layer ducting and/or Chordal Hop propagation
modes. Therefore high solar flux values can aid in long haul medium
frequency propagation paths in excess of 3000 miles, as a high solar flux
value ensures a strong F layer part of the E Valley-F layer duct or Chordal
Hop propagation mechanism.

However high solar activity in the form of increased ionization created by
Ultraviolet and X-Ray radiation can fill in the E Valley region and
interfere with the E Valley-F layer ducting mechanism. In a sense the E
Valley-F layer duct is closed on one or both ends of a propagation path and
the transmitted MF RF signal only propagates between the E layer and
land/ocean surface, with a higher angle and more loss.


SOLAR FLARES & SUNSPOT GROUP REGIONS-

During the previous 7 day period only no M class solar flares occurred.

Amazingly for the second week in a row, no sunspot group regions currently
harbor even beta-gamma class magnetic signatures that would harbor energy
for large M class solar flares. Only isolated M class solar flares are
possible.

However sunspot group #'s 10224 and 10226 are due to rotate around the sun's
eastern limb by 03/01/08 and may be a source of renewed large M class solar
flare activity. Solar flare forecast during the outlook period.

C- 100%

M- 50%

X- 10%


A C4 or higher class solar flare "can" elevate the proton flux above 10 MeV
(10+0) and initiate large scale high and mid latitude propagation path
absorption on the AM broadcast band, 160 and 120 meters, both stateside and
DX, as a transfer of increased density and RF signal absorption from the day
side D layer to night side of the ionosphere occurs through high level
neutral winds. Unfortunately even smaller C3 solar flares can create hour to
hour and night to night variations in signal strength on medium frequencies.

High and mid latitude Trans Atlantic (TA) and Trans Pacific (TP) propagation
paths tend to open up after a significant period of time passes without an
elevated energetic proton event of >10 MeV (10+0). This fact is still
stubbornly opposed by some otherwise very knowledgeable space weather
physicists over dependent on high latitude threshold Riometer readings.

Openings also occur when the solar background x-ray level falls back to
below C2 for 160 and 120 meters and below C1 for the AM broadcast band.


CORONAL MASS EJECTIONS/IONOSPHERIC STORMS/VISIBLE AURORA-

During the previous 7 day period no geo-effective (Earth facing) Coronal
Mass Ejections occurred. During the outlook period the probability of a
geo-effective (Earth facing) Coronal Mass Ejection (CME) is placed at 20%.



During the previous 7 day period a small Coronal Hole was in a geo-effective
(Earth facing) position. It's related Solar Wind Stream impacted the (IMF)
for a three day period of time, with a Kp index of 4 (Active) to 5 (Minor
Storm).

During the outlook period a recurring Coronal Hole will rotate into
geo-effective (Earth facing) position and it's related Solar Wind Stream
will begin impacting the (IMF) on 03/01/06-07.

The following related geomagnetic conditions will occur:

During the outlook period the probability of unsettled (Kp-3) geomagnetic
conditions is placed at 100%.

During the outlook period the probability of active (Kp-4) geomagnetic
conditions is placed at 90%.

During the outlook period the probability of at least a minor ionospheric
storm (Kp-5)(G1) is placed at 50%.

During the outlook period the probability of at least a moderate ionospheric
storm (Kp-6)(G2) is placed at 30%.

During the outlook period the probability of at least a strong ionospheric
storm (Kp-7+)(G3+) is placed at 20%.

G5 = Extreme - Kp = 9
G4 = Severe - Kp = 8
G3 = Strong - Kp = 7
G2 = Moderate - Kp = 6
G1 = Minor - Kp = 5
Active - Kp = 4
Unsettled - Kp = 3

During the outlook period the probability of a visible high latitude Aurora
display is placed at 100%, mid latitude 60%.

The Aurora Index at 2028 UTC 03/01/03 is a 7.

The NOAA POES historical database that was used to construct statistical
patterns of auroral power flux for each of the 10 levels of auroral activity
as defined by total power dissipation as illustrated in the following table.

Total Power Dissipation in Gigawatts/Activity Index Kp Index/Aurora Index

04-06/3/1+
10-16/5/2+
24-39/7/3+
61-96/9/5-


On 03/01/03 at 2206 UTC the Bz was 2.4 nt north.

The Wang-Sheeley Interplanetary Magnetic Field (IMF) Model which predicts
the Sun's IMF polarity, forecasts a negative (-) polarity between
03/01/04-03/01/10.


When the polarity of the IMF is negative a visible mid latitude Aurora
display is likely when a CME strikes the Earth's magnetic field. When the
polarity of the IMF is positive a visible mid latitude Aurora display is
unlikely as a CME strikes the Earth's magnetic field.

A Geomagnetic or Ionospheric Storm is a worldwide disturbance of the earth's
magnestosphere induced by the Sun's interplanetary magnetic field (IMF),
distinct from regular diurnal variations.

A Coronal Mass Ejection is the name given to an ejection of a large amount
of matter from the Sun's outer atmosphere or corona. These ejections
typically comprise millions of tons of material in the form of charged
particles, and can be seen because the material reflects sunlight. When one
of these ejections is directed towards the Earth (or conversely, directly
away from the Earth), it looks like a roughly circular "halo" surrounding
the Sun.

The "Halo CME's" then are those CME's which are more likely to impact the
Earth than those which are shot out at right angles to the Earth-Sun line.
Energetic protons emitted during CME's play a major role in increased day
time and night-time D-layer absorption of mediumwave frequencies.

Coronal Mass Ejections were once thought to be completely initiated by solar
flares. However it is now known that many (CME's) are not associated with
Solar Flares. If a (CME) collides with the Earth, it can excite a
Geomagnetic Storm if the polarity of the IMF has a negative sign. We must be
vigilant in watching for geoeffective (CME's), in order to not be caught by
surprise with a seemingly sudden and unexpected Geomagnetic Storm.

As the Kp index reaches 3-4, the aurora oval begins expanding equatorward in
magnetic latitude and generally begins having a negative impact on high
latitude medium frequency propagation paths. A Kp index of 5 or higher
begins to have a negative impact on high latitude high frequency shortwave
propagation paths. However at times skewed path propagation conditions can
compensate for high latitude propagation path auroral absorption.


STRATOSPHERIC WARMING-

During the past 7 day outlook period Stratospheric Warming did occur. During
the outlook period increased winter like day and year round night time D
layer absorption of medium frequency signals, tied to Stratospheric Warming
in the northern hemisphere is "probable".


As the SEC explains it:

Stratwarm: STRATWARM ALERT / SUNDAY / STRATWARM EXISTS INTENSE WARMING
COMTINUES IN THE UPPER STRATOSPHERE. WITHIN THE NEXT THREE DAYS: EASILY
WINDS AT 60N IN 1 HPA; REVERSED TEMPERATURE GRADIENT BETWEEN THE NORTH POLE
AND 60N FROM 10 TO 1 HPA; AN ELONGATION OF THE COLD POLAR VORTEX INTO TWO
CENTRES IN THE LOWER AND MID-STRATOSPHERE.

This occurence is tied to intense warming in the Stratosphere due to the
cold Circumpolar Vortex splitting and shifting in it's Arctic position.

A little related Meteorology:

Interrelated with the splitting and shifting of the Arctic Circumpolar
Vortex, is a Tropospheric level negative North Atlantic Oscillation (NAO)
and Pacific-North America Anomaly (PNA), mid and upper air height anomaly
pattern. This equates to a large high pressure ridge in Western North
America extending northward all the way into the Yukon region of Canada and
a deep trough in the Eastern North America, from the eastern U.S. extending
down into the Yucatan region of Mexico, with a second ridge in the western
North Atlantic Ocean. This pattern is also called a dual blocking ridge and
taps Siberian Arctic air, sending it across the North Pole into the eastern
2/3's of Canada and the U.S.,providing for very cold surface temperatures.

As the stratosphere lies below the ionosphere, which is at mesosphere and
thermosphere height, you would not expect to see stratospheric warming
effect medium frequency propagation in any way BUT medium frequency signals
do propagate off of temperature inversions and moisture discontinuities and
a temperature inversion is involved with stratospheric warming. So it's
probable that a medium frequency signal could do any number of things when
scattering off of a temperature inversion, at any height. Unfortunately
though some otherwise very knowledgeable Physicists stubbornly resist this
concept.

Also stratospheric warming (STRATWARM) has a negative effect on medium
frequency propagation, due to increasing medium frequency radio wave
absorption by the D layer, via upward propagating Internal Gravity Waves
(IGW).

This phenomenon also occurs in southern hemisphere winter but seems to be
less pronounced.

73,
Thomas Giella,
KN4LF
Plant City, FL, USA

KN4LF 160 Meter Amateur Radio Resources And More:
http://www.kn4lf.com

KN4LF Daily Solar Space Weather Geomagnetic Data Plus
MF Propagation Outlook:
http://www.kn4lf.com/kn4lf5.htm

FL Meteorological & Climatic Institute:
http://www.kn4lf.com/sub/fmci.htm

FMCI 2002 Florida Daily Weather Discussion:
http://www.kn4lf.com/sub/fmci17.htm



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Date: Sat, 4 Jan 2003 14:07:07 -0500
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Subject: Re: LF: Re: Distance calculator  (off topic)
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<DIV>Hi Andy:</DIV>
<DIV>&nbsp;</DIV>
<DIV>If you have a suite of programs zipped, and, they will function when 
using</DIV>
<DIV>USA parameters, I would appreciate you e-mailing the zipped file.&nbsp; 
Use</DIV>
<DIV><A 
href="mailto:rlau@wcnet.org.&nbsp;&nbsp;">mailto:rlau@wcnet.org.&nbsp;&nbsp;</A></DIV>
<DIV>&nbsp;</DIV>
<DIV>Many thanks and best wished for 2003,</DIV>
<DIV>&nbsp;</DIV>
<DIV>Tom N8TL</DIV>
<DIV>&nbsp;</DIV>
<DIV>On Sat, 4 Jan 2003 16:12:55 -0000 "Andy talbot" &lt;<A 
href="mailto:G4JNT@THERSGB.NET">G4JNT@THERSGB.NET</A>&gt; writes:</DIV>
<BLOCKQUOTE 
style="BORDER-LEFT: #000000 2px solid; MARGIN-LEFT: 10px; PADDING-LEFT: 10px">
  <DIV><FONT face=Arial size=2>I have a suite of programmes that calculate 
  distance bearing, as well as a height database of the UK for plotting terrain 
  maps and microwave paths, plus&nbsp;a database of most of the decent highspot. 
  /P locations in the UK and a few other worldwide plotting 
  utilities&nbsp;&nbsp; The progs operate together so it isn't possible to 
  supply just the one&nbsp;that converts NGR/Latlong/UTM and calculates distance 
  and bearings.&nbsp;&nbsp; The whole suite is 1.4Meg zipped up and I'll send 
  you a copy direct, and to anyone else wanting it.</FONT></DIV>
  <DIV>&nbsp;</DIV>
  <DIV><FONT face=Arial size=2>Andy&nbsp; G4JNT</FONT></DIV>
  <DIV>&nbsp;</DIV>
  <BLOCKQUOTE 
  style="BORDER-LEFT: #000000 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px; PADDING-RIGHT: 0px">
    <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
    <DIV 
    style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
    <A href="mailto:G0MRF@aol.com" title=G0MRF@aol.com>G0MRF@aol.com</A> </DIV>
    <DIV style="FONT: 10pt arial"><B>To:</B> <A 
    href="mailto:rsgb_lf_group@blacksheep.org" 
    title=rsgb_lf_group@blacksheep.org>rsgb_lf_group@blacksheep.org</A> </DIV>
    <DIV style="FONT: 10pt arial"><B>Sent:</B> Saturday, January 04, 2003 12:32 
    PM</DIV>
    <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: Distance calculator (off 
    topic)</DIV>
    <DIV><BR></DIV><FONT face=arial,helvetica><FONT size=2>Hello Group. 
    &nbsp;&nbsp;&nbsp;Happy New Year. <BR><BR>Does anyone know of, or have, any 
    windows software that can calculate distances based on the UK National Grid 
    Reference system? &nbsp;(e.g. &nbsp;TQ147951 ) <BR><BR>I have one for the 
    Maidenhead system (if anyone would like it just ask) but not for calculating 
    distance between two NGR's. <BR><BR>Many Thanks <BR><BR>73 
    <BR><BR>David</FONT> </FONT></BLOCKQUOTE>
  <DIV>&nbsp;</DIV></BLOCKQUOTE></BODY></HTML>

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<html>
At 07:32 04/01/03 G0MRF wrote:<br><br>
<blockquote type=cite class=cite cite><font face="arial" size=2>Hello
Group.&nbsp;&nbsp;&nbsp; Happy New Year. <br><br>
Does anyone know of, or have, any windows software that can calculate
distances based on the UK National Grid Reference system?&nbsp;
(e.g.&nbsp; TQ147951 ) <br><br>
I have one for the Maidenhead system (if anyone would like it just ask)
but not for calculating distance between two NGR's. <br><br>
Many Thanks <br><br>
73 <br><br>
David</font><font face="arial"> </blockquote><br><br>
I wrote a little program 15 yrs ago to do this, available free to anyone
who wants it.<br>
Also converts&nbsp; NGR to/from lat/lon at about the 10m level.<br>
Will not pass this reflector as an attachment. Sent one to David
direct.<br><br>
NGR distances are easy to do in a spreadsheet . Unlike&nbsp; Maidenhead
and Lat/Lon&nbsp; <br>
NG is a true rectilinear grid so if you know how to translate NGR's<br>
given as e.g. TQ 169483&nbsp; into actual Eastings and Northings in terms
of metres<br>
all you have to do is a root sum of squares equation.&nbsp; Done this way
<br>
distances will be correct but bearings will be in terms of Grid North -
about<br>
2 degs different&nbsp; from True North in Central England. My program
corrects for this<br>
and gives bearings as degs True. <br><br>
If you really want to go to town get onto Ordnance Survey's&nbsp; GPS
website -<br>
<a href="http://www.gps.gov.uk/" eudora="autourl">www.gps.gov.uk</a> ,
get a password and log in and you can get, free, a <br>
massive 10 Mb program that converts everything to everything at
millimetre <br>
accuracy (GridInquest). Or it lets you do conversions on-line.<br><br>
Walter G3JKV.<br>
&nbsp;</font></html>


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From: "Dave Pick" <g3yxm@wireless.org.uk>
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Subject: LF: QSOs
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<DIV><FONT face=Arial size=2>Dear all.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I just saw on the DX cluster that S57A has worked 
OK1DTN for the first S5/OK contact.</FONT></DIV>
<DIV><FONT face=Arial size=2>Also, following EA1PX's mail about his QSO with 
Hube, I called him on QRSS and we had a QSO. Thanks José. I make the distance 
1120km.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73</FONT></DIV>
<DIV><FONT face=Arial size=2>Dave</FONT></DIV>
<DIV><FONT face=Arial size=2>G3YXM, IO92BK</FONT></DIV></BODY></HTML>

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From: "Andy talbot" <G4JNT@THERSGB.NET>
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<DIV><FONT face=Arial size=2>I have a suite of programmes that calculate 
distance bearing, as well as a height database of the UK for plotting terrain 
maps and microwave paths, plus&nbsp;a database of most of the decent highspot. 
/P locations in the UK and a few other worldwide plotting utilities&nbsp;&nbsp; 
The progs operate together so it isn't possible to supply just the one&nbsp;that 
converts NGR/Latlong/UTM and calculates distance and bearings.&nbsp;&nbsp; The 
whole suite is 1.4Meg zipped up and I'll send you a copy direct, and to anyone 
else wanting it.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Andy&nbsp; G4JNT</FONT></DIV>
<DIV>&nbsp;</DIV>
<BLOCKQUOTE 
style="BORDER-LEFT: #000000 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px; PADDING-RIGHT: 0px">
  <DIV style="FONT: 10pt arial">----- Original Message ----- </DIV>
  <DIV 
  style="BACKGROUND: #e4e4e4; FONT: 10pt arial; font-color: black"><B>From:</B> 
  <A href="mailto:G0MRF@aol.com" title=G0MRF@aol.com>G0MRF@aol.com</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A 
  href="mailto:rsgb_lf_group@blacksheep.org" 
  title=rsgb_lf_group@blacksheep.org>rsgb_lf_group@blacksheep.org</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Saturday, January 04, 2003 12:32 
  PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: Distance calculator (off 
  topic)</DIV>
  <DIV><BR></DIV><FONT face=arial,helvetica><FONT size=2>Hello Group. 
  &nbsp;&nbsp;&nbsp;Happy New Year. <BR><BR>Does anyone know of, or have, any 
  windows software that can calculate distances based on the UK National Grid 
  Reference system? &nbsp;(e.g. &nbsp;TQ147951 ) <BR><BR>I have one for the 
  Maidenhead system (if anyone would like it just ask) but not for calculating 
  distance between two NGR's. <BR><BR>Many Thanks <BR><BR>73 
  <BR><BR>David</FONT> </FONT></BLOCKQUOTE></BODY></HTML>

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From: =?iso-8859-1?Q?Jos=E9_Manuel?= <jpradoes@telefonica.net>
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<DIV><FONT face=Arial size=2>Hi all:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Last night, at 21 UTC, I had first QSO with Hubert, 
F6CWA ( 1086 Km ), on 137704 Hz-QRSS3&nbsp;with "O" signals both ways, actually 
Hubert´s signals were audible.&nbsp;We&nbsp;had QSO again this 
morning&nbsp;after the QSO with Mike, G3XDV.&nbsp;</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Some minutes ago I copied "M" signals from DF0WD in 
QSO with F6CWA; I called him but I had no reply.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX loc 
IN53TI</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@ntlworld.com>
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G0MRF wrote:
> Does anyone know of, or have, any windows software that can calculate
> distances based on the UK National Grid Reference system?  (e.g.
 TQ147951 )
>
> I have one for the Maidenhead system (if anyone would like it just ask)
but
> not for calculating distance between two NGR's.

David,

Not a perfect solution, but go to
http://www.aber.ac.uk/cgi-bin/user/auj/locate.pl which is a utility to
convert NGR or Lat/Long into a Locator, then use your favourite Loc-Loc
program (I use the one by OH3NJC).

Mike, G3XDV
http://www.lf.thersgb.net
=================




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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hello Group. &nbsp;&nbsp;&nbsp;Happy New Year.
<BR>
<BR>Does anyone know of, or have, any windows software that can calculate distances based on the UK National Grid Reference system? &nbsp;(e.g. &nbsp;TQ147951 )
<BR>
<BR>I have one for the Maidenhead system (if anyone would like it just ask) but not for calculating distance between two NGR's.
<BR>
<BR>Many Thanks
<BR>
<BR>73
<BR>
<BR>David</FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@ntlworld.com>
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Just had a nice QRSS3 contact with Jose, EA1PX at 1152km. This is country
no:20 for me and my 89th different station on 136kHz. [full list at
http://www.lf.thersgb.net/136calls.htm]

Jose was not strong, but clearly readable, so he should have many QSOs
across Europe.

Mike, G3XDV
http://www.lf.thersgb.net
==================



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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Subject: LF: Well Done Jose
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Hi all, congratulations to Jose for struggling with difficult conditions. He
was a good signal in the UK at near local midnight, and even on my "small"
aerial would have been close to audible without the noise from TVs and
external Christmas lights. He should be good copy on QRSS3 most evenings in
the UK, as the majority is a sea-water path.

Cheers de Alan G3NYK
alan.melia@btinternet.com




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<DIV><FONT face=Arial size=2>Hi all:</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Yesterday,&nbsp;Thursday, from 0.06 to 0.56 UTC, 
took place a QSO between DF6NM and me, on 137704 Hz-QRSS3. Markus´ &nbsp;signals 
were "O" , and he copied me with "M".</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Thanks a lot to Markus for the first DL-EA QSO and 
for the hard work and skills deployed to read all my characters.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Thanks to Brian for his DCF39´s registers, that 
helped me to make the call in the appropiated time.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Thanks to Alan for his report as well.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 de José, EA1PX, loc 
IN53TI</FONT></DIV></BODY></HTML>

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Subject: Re: LF: Re: Re: Yagi (off subject)
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It will be in the IEE library Savoy Place, and the Patent Library
in London, and the Science Museam Library at Imperial College.

Stewart



g3ldo wrote:
> Hi Igor,
> Many thanks for the information
> 
> 
>>Peter: It was reprinted at Proc. IRE, #5, Vol. 72, 1984.
>>
>>
>>>I apologise for this off subject question but I am not sure where else
>>
> to
> 
>>>look.
>>>I am trying to find a detailed description of the original experiments
>>
>>done
>>
>>>by Prof Uda on the parasitic element antenna now known as the Yagi. I
>>
> have
> 
>>>one reference Proc. IRE, 16 715-740 June 1928 but don't know how to get
>>
> at
> 
>>>it. Do you know of any other sources?
>>>
>>
> Regards,
> Peter, G3LDO
> 
> e-mail <g3ldo@ukonline.co.uk>
> 
> Web <http://web.ukonline.co.uk/g3ldo>
> 
> 
> 
> 




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "G4WGT" <g4wgt@talkgas.net>
To: rsgb_lf_group@blacksheep.org
Date: Thu, 2 Jan 2003 21:33:25 -0000
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Hi Ed & LF,

Thank you for the detailed reply regarding your antenna & the licence
conditions in Russia.

I am still working on my station including a 300 watt transmitter &
improvements to the antenna system for receive & an antenna for transmit, I
only have a small garden behind my house but I am going to give 136 my best
shot !

Thanks again Ed.

73

Gary  G4WGT

-----Original Message-----

In Russia there are following limitations on 136 kHz:.................etc.

73! Ed  RU6LA  ed@dx.ru
---

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Hi Igor,
Many thanks for the information

>
> Peter: It was reprinted at Proc. IRE, #5, Vol. 72, 1984.
>
> > I apologise for this off subject question but I am not sure where else
to
> > look.
> > I am trying to find a detailed description of the original experiments
> done
> > by Prof Uda on the parasitic element antenna now known as the Yagi. I
have
> > one reference Proc. IRE, 16 715-740 June 1928 but don't know how to get
at
> > it. Do you know of any other sources?
> >
Regards,
Peter, G3LDO

e-mail <g3ldo@ukonline.co.uk>

Web <http://web.ukonline.co.uk/g3ldo>




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From: "Johan Bodin" <sm6lkm.jbeab@swipnet.se>
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The DFCW beacon on 40m is now QRT but I am planning
to try milliwatt DFCW or QRSS on 160m soon.

73
Johan SM6LKM

----- Ursprungligt meddelande ----- 
Från: "Alberto di Bene" <dibene@usa.net>
Till: <rsgb_lf_group@blacksheep.org>
Skickat: den 2 januari 2003 14:33
Ämne: Re: LF: OT: DFCW on HF


> Johan Bodin wrote:
> 
> >Hi
> >
> >There is a DFCW beacon on 40 meters.
> >
> >Frequency: 7022.381 kHz (dot), 7022.383 kHz (dash).
> >[...]
> >  
> >
> Nothing received here Johan, sorry... but will keep trying.
> 
> 73  Alberto  I2PHD




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Johan Bodin wrote:

>Hi
>
>There is a DFCW beacon on 40 meters.
>
>Frequency: 7022.381 kHz (dot), 7022.383 kHz (dash).
>[...]
>  
>
Nothing received here Johan, sorry... but will keep trying.

73  Alberto  I2PHD





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<!doctype html public "-//w3c//dtd html 4.0 transitional//en">
<html>
<body bgcolor="#FFFFFF">
Hello Dave,
<p>thanks for your efforts - wonderful ooo-signal on a wonderful noise-free
1st of January (everyone was tired or even worse ...). QSL is already posted
to G3YXM. Fine to get country no. 13 on LF!
<p>Happy New Year to you es everyone on the reflector.
<br>Vy 73 es hpe to cuagn
<p>Tom, DK1IS
<br>JN59WK
<p>Pick schrieb:
<blockquote TYPE=CITE><style></style>
<font face="Arial"><font size=-1>Thanks
to F6CWA, F6BWO and DK1IS for good QRSS QSOs from the GM QTH (IO75WC).</font></font><font face="Arial"><font size=-1>I
also had an excellent copy of DF6NM's Hell transmission to I5TGC this afternoon.</font></font>&nbsp;<font face="Arial"><font size=-1>Happy
New Year to all!</font></font>&nbsp;<font face="Arial"><font size=-1>Dave
G(M)3YXM.</font></font></blockquote>

</body>
</html>



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Subject: Re: LF: hell
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Dear Mal, Dave and LF-Group,<BR>
<BR>
... ah, lower sideband reception of "GL - TGC NM SK .." - one may have to use a mirror ;-) <BR>
<BR>
Mni tnx to you and Dave for the reports. I wonder if you might have seen traces of Cesare's HELL as well, he had a very nice signal here today.<BR>
<BR>
Wishing all of you a wonderful year 2003 and lotsa fun,<BR>
<BR>
73 de Markus, DF6NM<BR>
<BR>
<BR>
g3kev.ham@virgin.net:<BR>
<BR>
<BLOCKQUOTE TYPE=CITE style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px">Who was transmitting Hell a short time ago on 137.7 khz</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">I just noticed the end of the transmission something like </FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">Cr - LCC NH ZX - -</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">73&nbsp;</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"> <BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2">de G3KEV</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=3 FAMILY="SANSSERIF" FACE="Arial" LANG="2"></BLOCKQUOTE><BR>
</FONT><FONT  COLOR="#000000" style="BACKGROUND-COLOR: #ffffff" SIZE=2 FAMILY="SANSSERIF" FACE="Arial" LANG="2"><BR>
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<DIV><FONT face=Arial size=2>Who was transmitting Hell a short time ago on 137.7 
khz</FONT></DIV>
<DIV><FONT face=Arial size=2>I just noticed the end of the transmission 
something like </FONT></DIV>
<DIV><FONT face=Arial size=2>Cr - LCC NH ZX&nbsp;- -</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 </FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>de G3KEV</FONT></DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

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From: "Pick" <us@picks.f9.co.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
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Subject: LF: Hell copy
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<DIV><FONT face=Arial size=2>Thanks to F6CWA, F6BWO and DK1IS for good QRSS QSOs 
from the GM QTH (IO75WC).</FONT></DIV>
<DIV><FONT face=Arial size=2>I also had an excellent copy of DF6NM's Hell 
transmission to I5TGC this afternoon.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Happy New Year to all!</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Dave G(M)3YXM.</FONT></DIV></BODY></HTML>

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Subject: LF: UA Limitations
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Hello LF_Group!

Tuesday, December 31, 2002, G4WGT wrote:

G> The ERP stated here seems very high in respect of my limited experience with
G> LF power levels & antenna efficiency limitations. If these levels are
G> correct I will be interested to know how they are being achieved & what
G> restrictions are imposed by the licencing authorities in that area.

In Russia there are following limitations on 136 kHz:

29 jun 1998  radio amateurs of Russia have permission for
135.7-137.8 kHz A1A with power (Output - not ERP!):
100w  1 kategory
50w   2/3 kat
10w   4 kat
I.e. not CEPT's limitations in pwr

I use Big Vertical (see attach) on high (135m) tower
H effective ~90m
As fairly has noticed Dave G3YXM (RadCom July 2002):
"These  restrictions  mean  that  only those who have access to really
efficient aerials (like Ed's) are going to be heard in the UK"

I remind, that distance up to England from mine QTH abt 3000km!
I believe that such restrictions detain development 136 in Russia.

I use 100w TX and it allows me to achieve abt 20w ERP.
But at me is 3? thermo-current-meter in ANT and I usually support a current
in the aerial < 3A   i.e. abt 10w ERP at ~40w Output

My LF-correspondents are in the best conditions on reception than I ;-))
Seldom at whom from them is even 1w ERP ;-((

In 2002 I have made 5 weekends LF-activites and I have abt 40 QSOs with
11 countries DXCC (136/136 QRSS and CW)

73! Ed  RU6LA  ed@dx.ru
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From: "WE0H" <we0h@gentekcom.com>
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Date: Tue, 31 Dec 2002 20:22:23 -0600
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Subject: LF: RE: RE: Dec 27-28 UA6-activity
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BIG amplifier & BIG antenna.

Mike>WE0H
http://www.we0h.us/lf

-----Original Message-----
From: owner-rsgb_lf_group@blacksheep.org
[mailto:owner-rsgb_lf_group@blacksheep.org]On Behalf Of G4WGT
Sent: Tuesday, December 31, 2002 12:14 PM
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Dec 27-28 UA6-activity

Hi Ed & all at LF.

On 27/12/2002  Ed  RU6LA  ed@dx.ru wrote :-

DEC 28:
0000 - 0530  QRSS60 10w ERP Beacon test ("RU6LA") 135.922
0530 - 1000  QRSS3/CW 1w ERP Beacon test ("RU6LA 1W") 137.7
1000 - abt 1500 QRSS60 20w ERP Beacon test ("RU6LA") 137.7


The ERP stated here seems very high in respect of my limited experience with
LF power levels & antenna efficiency limitations. If these levels are
correct I will be interested to know how they are being achieved & what
restrictions are imposed by the licencing authorities in that area.

May I also take this opportunity to wish everyone on LF seasons greetings &
a Happy New year 2003.

73

Gary  G4WGT







