From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 31 Mar 2001 20:10:27 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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Subject: LF: lf xatlantic
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Hi has anyone been transmitting?  I have seen nil here, but condx have
been poor

   73 de John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: rsgb_lf_group@blacksheep.org
References: <14gpKS-1kYC0WC@fwd04.sul.t-online.com> <14h8HU-0thmHAC@fwd06.sul.t-online.com> <14i0Fh-1gkX5sC@fwd06.sul.t-online.com> <004901c0b897$a06dd960$a047073e@j1r9b7> <14j7sz-25SSYaC@fwd02.sul.t-online.com>
Subject: LF: Re: PVC tks
Date: Sat, 31 Mar 2001 09:40:58 +0200
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Uwe and All,

PVC is certainly good enough at LF. When you want to be sure put a piece of
pipe in the microwave oven (together with a glass of water as dummy load).
When it survives that test you know there will be no problems at lower
frequencies.

73, Dick, PA0SE

----- Oorspronkelijk bericht -----
Van: jannsen <0482183881-0001@t-online.de>
Aan: <rsgb_lf_group@blacksheep.org>
Verzonden: zaterdag 31 maart 2001 1:00
Onderwerp: LF: PVC tks


> Hi Derek, Dick and Robin
> tks fer the infos abt the PVC dielectric constant.
> I found in my garden some PVC-tubes of usefull diameter for new antenna
matching
> coils wondering if that material is right for lf. the d-c cld  be ok. I
will
> prove the loss by comparing the PVC-coil with an air-coil of same
structure.
> Regards
> Uwe/dj8wx
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: PVC tks
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Hi Derek, Dick and Robin
tks fer the infos abt the PVC dielectric constant. 
I found in my garden some PVC-tubes of usefull diameter for new antenna matching 
coils wondering if that material is right for lf. the d-c cld  be ok. I will 
prove the loss by comparing the PVC-coil with an air-coil of same structure.
Regards
Uwe/dj8wx




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000301c0b96b$923ec3c0$462b073e@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Solar Events
Date: Fri, 30 Mar 2001 23:47:44 +0100
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Hi all, for those of you that are interested in propagation, sunspots, solar
X-ray flares and aurora (not to mention Coronal holes and CMEs ) there is an
interesting article in the April 2001 issue of the Scientific American
Journal. It does not have anything to say about disruption to radio
propagation but it does have a lot of 'new' information about CMEs and the
production of the shock-front.
(It may be available on their web site, I haven't looked)

It describes the injection and ejection of particles from the
'plasma-sphere' by the collision with the magnetic field of the CME. ( I
think the 'plasma-sphere' they refer to is what is often called the Van
Allen belts.) I believe this 'dynamo' effect could also inject energetic
particles into the ionosphere, at the poles. These would be much 'hotter'
than photo-dissociated ions, and so would take quite a long time to
recombine (decay)....maybe as much as 10 days.

The most interesting thing for me is that it 'decouples' the CME events from
the X-ray flares. The older references were not able to do this not having
access to data from the Geos and SOHO satellites. CMEs it seems can be
caused by the same mechanism that releases an X-ray flare, but they can
occur by other means without the release of X-rays.  This accounts for some
'bad nights' on the CFH plots that did not seem to correlate with previous
flares.

SXV seems to be showing some signs of the effects of the recent CMEs as it
has become very weak in daytime today.

If the D-layer is heavily ionised by now it will be interesting to see if
there is enhanced range from some of the weaker eastern European stations
this weekend, due to daytime 'skywave'.

Cheers de Alan G3NYK   JO02PB
Alan.Melia@btinternet.com




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 30 Mar 2001 15:43:15 -0500
From: "Rye Gewalt" <ryeg@sitestar.net>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: <Tech> BPSK PLL, wheels
References: <8d.4763591.27f50ca5@aol.com>
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I couldn't agree with you more regarding re-inventing things.  I think that there
are a lot of roads that were investigated and abandon as dead ends years ago  ---
and with today's technology they can be very fruitful and interesting.  In some
respects this LF activity is like that.   But I still like my wheel idea.
Sometimes my sense of humor gets me into trouble -- I apologize but hope a few
got a chuckle or two out of it....

Rye

MarkusVester@aol.com wrote:

> Hi Rik, Jim, Rye and all,
>
> >  The error between input and
> >  output phases could be corrected either by increasing the VCO
> >  frequency until the output phase "catches up" with the input, or
> >  decreasing it until it "slows down" to match the input. The output
> >  phase could shift in either direction, although the end result would
> >  always be to match the input phase.
>
> Like in real life, it's sometimes a sad thing to have to decide one way or
> another. If that PLL could take both routes simultaneously, the result would
> be perfect soft BPSK again :-) . In the 30's, there was a scheme called
> "Chireix modulation" which added the power outputs of two phase-modulated
> class-C transmitters to achieve AM in an efficient way.
>
> > I am working on this round thing that can be used to reduce friction rather
> > than simply dragging things across the ground.....
>
> Me too, apparently... I hardly dare say it in public, but in my opinion,
> re-inventing basic stuff is not so stupid at all. Don't we learn a lot more
> by own thinking and fiddling than by just believing in the solutions the
> experts have come up with for us? Trying to catch a glimpse of tiny dots
> encircling Jupiter in a homemade cardbord-roll telescope may be more exciting
> and instructive than a great show of colourful deep-sky HST images on the
> web. Which of course is not bad, either...
>
> 73 de Markus, DF6NM



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <25649.200103301702@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org
Date: Fri, 30 Mar 2001 18:07:11 +0000
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Subject: LF: Argo -simplicity, sig strength etc.
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Dear LF group,

I don't think it is possible for any one piece of software to be all 
things to all people - for the person who is trying to copy a QRSS 
signal, Argo is very well "tuned", but the trade-off for this 
specialisation and being simple to use is that it is less versatile. If 
you want to examine the spectrum of a different type of signal, it is 
better to use a program like Spectrum Lab or Spectran, where you 
have greater control over the parameters of the FFT and display. 

Having said that, I still think a signal level/SNR measurement 
function would be a valuable addition to Argo, even if you are only 
using it for QRSS. It is important to be able to get a meaningful 
measurement of signal strength - eg. 3dB down on yesterday, 
10dB above the noise level, rather than just calling it T,M or O.

Cheers, Jim Moritz
73 de M0BMU



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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References: <65AECDF1F89AD411900400508BFC869F9C0413@pdw-mail-1.dera.gov.uk> <002301c0b900$ec54e8a0$a3e086d4@ericadodd>
Subject: LF: Re: Re: Dumbing down
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> The implied criticism of Alberto's work is inappropriate. 
> Keep up the good work Alberto.
> 
> Regards,
> Peter, G3LDO
> 

Well said!!



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: <8d.4763591.27f50ca5@aol.com>
Subject: Re: LF: <Tech> BPSK PLL, wheels
Date: Fri, 30 Mar 2001 14:31:47 +0100
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> > I am working on this round thing that can be used to reduce friction
rather
> > than simply dragging things across the ground.....
>
> Me too, apparently... I hardly dare say it in public, but in my opinion,
> re-inventing basic stuff is not so stupid at all. Don't we learn a lot
more
> by own thinking and fiddling than by just believing in the solutions the
> experts have come up with for us? .........>
> 73 de Markus, DF6NM

Isn't that exactly what makes amateur radio fun? This is the 'self-training'
that is part of the international definition of AR.

Mike, G3XDV



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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Re: Dumbing down
Date: Fri, 30 Mar 2001 12:16:38 +0100
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I'm not criticising the S/W, just saying that in life generally there is
a strong tendency to make things excessively simple for everyone to
understand, to the detriment of those who really do want to know.
Rather than telling them everything and allowing those who don't know to
find out.  If they are not told, people don't know what they don't know.
Have you watched 'Tomorrows World' recently - it's cringing.  Or even
when something even remotely scientific comes up on the TV News - the
newscasters actually apologise for using a technical word !

Andy


> -----Original Message-----
> From: g3ldo [mailto:g3ldo@ukonline.co.uk]
> Sent: 2001-03-30 11:02
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: Dumbing down
> 
> 
> 
> Andy said:
> 
> > What we call "Dumbing Down" in the UK (and the US ?).   It 
> happens a lot
> > with science programmes on television, and a lot more with science
> > education in schools and universites   :-(    :-((
> 
> >
> > > If you noticed, terms like 'sampling rate',  'FFT size', etc.
> > > are totally absent from
> > > Argo, which uses a terminology, like sec/dot, taken from the
> > > intended usage of
> > > the program, and not from its implementation technicalities.
> >
> 
> The implied criticism of Alberto's work is inappropriate. To 
> say that use of
> these techniques should not be pursued unless you fully 
> understand what
> 'sampling rate' 'FFT size' etc is like saying you should not 
> be playing with
> RF circuits and antennas unless you have a full grasp of 
> electromagnetic
> theory and Maxwell's equations.
> 
> To me this amateur radio stuff is a hobby. While I appreciate 
> the value of
> the work done by the technically advanced members of the group I also
> appreciate the value of the work done by those who have made 
> such techniques
> accessible to those like myself.
> 
> Keep up the good work Alberto.
> 
> Regards,
> Peter, G3LDO
> 
> e-mail <g3ldo@ukonline.co.uk>
> 
> Web <http://web.ukonline.co.uk/g3ldo>
> 
> 
> 
> 
> 
> 


-- 
The Information contained in this E-Mail and any subsequent correspondence
is private and is intended solely for the intended recipient(s).
For those other than the recipient any disclosure, copying, distribution, 
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <003501c0b90a$6200b940$2873073e@dave>
From: "Dave Sergeant" <dsergeant@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
References: <000d01c0b894$135b6040$a047073e@j1r9b7>
Subject: LF: Re: Proposed LF Forum at the Crawley Club
Date: Fri, 30 Mar 2001 12:12:12 +0100
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>From Dave G3YMC

G3GRO wrote:
>Regretfully therefore the Club committee have to withdraw the offer to host
>the event for this year.

That is sad, yet another victim of the crisis.  There is unlikely to be HF
or VHF field days this year.  Mr Blair, the countryside is not open!

Let us hope possibly another venue can be found.

73s Dave G3YMC
dsergeant@btinternet.com
dsergeant@iee.org
http://www.btinternet.com/~dsergeant







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: <65AECDF1F89AD411900400508BFC869F9C0413@pdw-mail-1.dera.gov.uk>
Subject: LF: Re: Dumbing down
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Andy said:

> What we call "Dumbing Down" in the UK (and the US ?).   It happens a lot
> with science programmes on television, and a lot more with science
> education in schools and universites   :-(    :-((

>
> > If you noticed, terms like 'sampling rate',  'FFT size', etc.
> > are totally absent from
> > Argo, which uses a terminology, like sec/dot, taken from the
> > intended usage of
> > the program, and not from its implementation technicalities.
>

The implied criticism of Alberto's work is inappropriate. To say that use of
these techniques should not be pursued unless you fully understand what
'sampling rate' 'FFT size' etc is like saying you should not be playing with
RF circuits and antennas unless you have a full grasp of electromagnetic
theory and Maxwell's equations.

To me this amateur radio stuff is a hobby. While I appreciate the value of
the work done by the technically advanced members of the group I also
appreciate the value of the work done by those who have made such techniques
accessible to those like myself.

Keep up the good work Alberto.

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: "Petr Maly" <p.maly@gmc.net>
To: rsgb_lf_group@blacksheep.org
References: <4c.12d909d6.27f521e5@aol.com>
Subject: Re: LF: PRUVODKA: PROTECTION 3.14.02 RELEASE
Date: Fri, 30 Mar 2001 09:47:34 +0200
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Hi David

This message comes really from my office, it is a message that is
automatically sent by an utility on some event. I am sorry it was sent to
the reflector too, at the moment it looks as a failure of Outlook because
the e-mail address if set fixly in an INI file and there is no chance to do
this by mistake.
I made already some measurements and I hope it will not happen again. Sorry.

73 Petr OK1FiG

----- Original Message -----
From: <G0MRF@aol.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Friday, March 30, 2001 1:40 AM
Subject: Re: LF: PRUVODKA: PROTECTION 3.14.02 RELEASE


> In a message dated 3/29/01 4:09:59 PM GMT Daylight Time, p.maly@gmc.net
> writes:
>
> << Subj:     LF: PRUVODKA: PROTECTION 3.14.02 RELEASE
>  Date:  3/29/01 4:09:59 PM GMT Daylight Time
>  From:  p.maly@gmc.net (Petr Maly)
>  Sender:    majordom@post.thorcom.com
>  Reply-to:  rsgb_lf_group@blacksheep.org
>  To:    rsgb_lf_group@blacksheep.org (136 group)
>
>  Pruvodka at:
>
> file://N:\Income\Protection 3.14.02\info.gmc
>   >>
>
>
> Is this anything to do with LF?   If not, please don't send it. If so,
please
> include brief explanation.
>
> Thanks
>
> David
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: G0MRF@aol.com
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Date: Thu, 29 Mar 2001 18:40:21 EST
Subject: Re: LF: PRUVODKA: PROTECTION 3.14.02 RELEASE
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In a message dated 3/29/01 4:09:59 PM GMT Daylight Time, p.maly@gmc.net 
writes:

<< Subj:     LF: PRUVODKA: PROTECTION 3.14.02 RELEASE
 Date:  3/29/01 4:09:59 PM GMT Daylight Time
 From:  p.maly@gmc.net (Petr Maly)
 Sender:    majordom@post.thorcom.com
 Reply-to:  rsgb_lf_group@blacksheep.org
 To:    rsgb_lf_group@blacksheep.org (136 group)
 
 Pruvodka at:
 
file://N:\Income\Protection 3.14.02\info.gmc
  >>


Is this anything to do with LF?   If not, please don't send it. If so, please 
include brief explanation.

Thanks

David


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: MarkusVester@aol.com
Message-ID: <8d.4763591.27f50ca5@aol.com>
Date: Thu, 29 Mar 2001 17:09:41 EST
Subject: Re: LF: <Tech> BPSK PLL, wheels
To: rsgb_lf_group@blacksheep.org
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Hi Rik, Jim, Rye and all,

>  The error between input and 
>  output phases could be corrected either by increasing the VCO 
>  frequency until the output phase "catches up" with the input, or 
>  decreasing it until it "slows down" to match the input. The output 
>  phase could shift in either direction, although the end result would 
>  always be to match the input phase.

Like in real life, it's sometimes a sad thing to have to decide one way or 
another. If that PLL could take both routes simultaneously, the result would 
be perfect soft BPSK again :-) . In the 30's, there was a scheme called 
"Chireix modulation" which added the power outputs of two phase-modulated 
class-C transmitters to achieve AM in an efficient way.

> I am working on this round thing that can be used to reduce friction rather
> than simply dragging things across the ground.....

Me too, apparently... I hardly dare say it in public, but in my opinion, 
re-inventing basic stuff is not so stupid at all. Don't we learn a lot more 
by own thinking and fiddling than by just believing in the solutions the 
experts have come up with for us? Trying to catch a glimpse of tiny dots 
encircling Jupiter in a homemade cardbord-roll telescope may be more exciting 
and instructive than a great show of colourful deep-sky HST images on the 
web. Which of course is not bad, either...

73 de Markus, DF6NM


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Derek Atter" <Datter@btinternet.com>
To: rsgb_lf_group@blacksheep.org
References: <14gpKS-1kYC0WC@fwd04.sul.t-online.com> <14h8HU-0thmHAC@fwd06.sul.t-online.com> <14i0Fh-1gkX5sC@fwd06.sul.t-online.com>
Subject: LF: Re: PVC
Date: Thu, 29 Mar 2001 22:30:57 +0100
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Uwe,

According to my reference book the dielectric constant (permittivity) of PVC
varies slightly with frequency.  At 1khz the value is given as 3.1 and at
1Mhz as 2.88.

I hope this helps !         73,  de Derek G3GRO

----- Original Message -----
From: "jannsen" <0482183881-0001@t-online.de>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 27, 2001 9:39 PM
Subject: LF: PVC


> Hi group,
>
> is there any who knows or can look up the  - ah I do`nt know the correct
word -
> elecric property constant (dielektrizitätskonstante in the german
language)
> for PVC ? ok, glass has  2 -12, air 1, ceramic 100 -10000. PVC is not on
my
> list.
> tks for the answer in advance
> Uwe/dj8wx
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
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Date: Thu, 29 Mar 2001 16:06:44 EST
Subject: Re: LF: Re: PLL filter for BPSK
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Rye Gewalt writes:
<< I always thought that was a standard method of demodulating phase 
information....>>
  (and)
vernall@xtra.co.nz writes:
<< This approach may have applicability to detection of weak BPSK signals on
 LF, but I suspect that a single PLL with free running VCO would be rather
 useless for noise to signal scenarios. >>

I'm not sure we're all talking about the same thing here.  Rik, Jim, and I 
were discussing whether it would be feasible to use a PLL for filtering out 
abrupt phase transitions in the transmit exciter.  I don't see any way of 
using one for detection at the receive end, for the very reason Bob mentions.

73,
John


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Derek Atter" <Datter@btinternet.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Proposed LF Forum at the Crawley Club
Date: Thu, 29 Mar 2001 22:05:21 +0100
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>From Derek Atter

After the very successful LF Forum at the RSGB Windsor HF Convention in the
UK last October, it was suggested that there may be support for a similar
follow-up session in about 6 months time - i.e. about mid-way between HF
Conventions. The Crawley Amateur Radio Club volunteered to host such a
meeting at their clubhouse in Tilgate Forest and a provisional date of 13th
May 2001 was suggested at the time
   We were about to post a general invitation on the reflector but
unfortunately owing to the current problem with foot and mouth disease in
some areas of the UK, Tilgate Forest has just been closed to the general
public as a precaution in order to protect the children's zoo and the wild
deer which roam free in the forest. Since the CARC clubhouse is located
right on the edge of the forest and we have been instructed to keep access
the club premises to a minimum for the time being. Regretfully therefore the
Club committee have to withdraw the offer to host the event for this year.

                             73,  de  Derek Atter G3GRO on behalf of Crawley
Amateur Radio Club




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Petr Maly" <p.maly@gmc.net>
To: "136 group" <rsgb_lf_group@blacksheep.org>
Subject: LF: PRUVODKA: PROTECTION 3.14.02 RELEASE
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Pruvodka at:

file://N:\Income\Protection 3.14.02\info.gmc

----------


HW and SW improvements


Programmer:

HW security:  caching information red from HW key (dongle). Useful on 

network.

SW security:

- added more detailed error messages.

- added checking of PMLOGS directory whether user has rights to modify this 

directory.

- DLL now use date only to determine number of days to run in demo mode. It 

should avoid problems on network.

- usage of both PS VIPP and PS BTF in demo mode may cause problems with 

old 

license files and this new DLL. In such case download updated license files 

from 

FTP.


Support:

SPATNE CISLO VERZE V PROPERTIES






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: <Tech> A Question
Date: Thu, 29 Mar 2001 14:45:17 +0100
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What we call "Dumbing Down" in the UK (and the US ?).   It happens a lot
with science programmes on television, and a lot more with science
education in schools and universites   :-(    :-((


Andy  G4JNT



> If you noticed, terms like 'sampling rate',  'FFT size', etc. 
> are totally absent from
> Argo, which uses a terminology, like sec/dot, taken from the 
> intended usage of
> the program, and not from its implementation technicalities.


-- 
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 29 Mar 2001 14:40:40 +0200
From: "Alberto di Bene" <dibene@usa.net>
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Subject: LF: Re: <Tech> A Question
References: <21660.200103271337@gemini> <000c01c0b826$599244c0$f2c928c3@ericadodd>
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>  Might I suggest that
> Alberto does development work, such as amplitude measurement, on Spectran,
> which already has this uncalibrated facility. Having said that I find that
> the improvements so far made to Argo have not compromised simplicity.
>

Peter, Laurie and others,

     we are in full agreement on this. The main reason for developing Argo when
Spectran did already exist was to have a program very simple to use.
If you noticed, terms like 'sampling rate',  'FFT size', etc. are totally absent
from
Argo, which uses a terminology, like sec/dot, taken from the intended usage of
the program, and not from its implementation technicalities.
And this simplicity will always be of upmost priority.

73  Alberto  I2PHD




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
Subject: LF: Re. (TECH) A Question.
Date: Thu, 29 Mar 2001 10:59:18 +0100
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<DIV><FONT face=Arial size=2>Alberto, I fully support Peters comments about the 
operational simplicity of ARGO. I am sure recent T/A successes were due to 
this.73s Laurie.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: [TECH] A question
Date: Thu, 29 Mar 2001 11:01:56 +0100
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Alberto,

This facility exists on Spectrgram. Perhaps you can e-mail Richard Horne and
see what he did.

Mike, G3XDV
==========


> I am implementing both in Argo and Spectran a function that will
> display the relative level (in dB) of the spectral lines when you hover
the
> mouse cursor over them. So far so good.
> What I am uncertain about, is that word, 'relative'. Relative to what ?
>




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: <21660.200103271337@gemini>
Subject: LF: Re: <Tech>Re: A Question
Date: Wed, 28 Mar 2001 23:44:27 +0100
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> Adding an amplitude measurement capability to Argo/Spectran
> sounds like an excellent idea - it would enable a meaningful
> measurement of relative signal strengths to be made.

> DL4YHF's Spectrum Lab has such a facility -


Spectrogram also had this facility with a calibrated scale. I use it
sometimes for measuring the relative levels of signals.

Alberto, Wolf and others have done a great job in providing us with FFT S/W
and I would just like to make a comment.

One of the main virtues of Argo (as well as its effectiveness) is its
simplicity. This is of utmost importance in an operational situation.
Ensuring that the receiver is set up correctly, that the transmitter
operating correctly, while at the same time (under certain conditions)
operating an HF link can take a lot of effort. To have software that is so
easy to use is a big help in these situations.
However, there is always improvements that can be made. Might I suggest that
Alberto does development work, such as amplitude measurement, on Spectran,
which already has this uncalibrated facility. Having said that I find that
the improvements so far made to Argo have not compromised simplicity.


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: "Vernall" <vernall@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <000b01c0b7d3$630617a0$1de57ad5@default>
Subject: LF: Re: PLL filter for BPSK
Date: Thu, 29 Mar 2001 15:45:34 +1200
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Hi all,

While PLL systems are in service for systems having quite good signal to
noise ratio (such as telephone modems) it is quite another thing to try and
decode the wanted signal when it is a noise to signal situation.

For other than LF applications I have been looking at "dejitter"
countermeasures for accurate clock recovery from signals passing through
digital links (the sampling causes phase jitter in the original signals),
and it seems that a dual PLL setup is an answer.  PLL#1 to recover what
clock signal can be readily found, then PLL#2 to clean up the jitter from
PLL#1.  PLL#2 could need to have a high performance oven oscillator VCO, to
hold centre frequency for long periods, so it is not without complication.
This approach may have applicability to detection of weak BPSK signals on
LF, but I suspect that a single PLL with free running VCO would be rather
useless for noise to signal scenarios.

73, Bob ZL2CA



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Message-ID: <000b01c0b7d3$630617a0$1de57ad5@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: PLL filter for BPSK
Date: Wed, 28 Mar 2001 20:13:49 +0100
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Hi all, well there are several simulators for PLL systems that will allow
you to play with loop gain, and filter characteristics whilst tracking the
transient response. So it should be quite easy to see whether this one will
run.
As an example I believe there is a simulator for the 4046 on the Philips
site. I certainly have Pascal source code from one of the Journals of a few
years ago. You can tell how long ago because I ran it under Turbo Pascal III
!!

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: Wed, 28 Mar 2001 17:08:59 -0500
From: "Rye Gewalt" <ryeg@sitestar.net>
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Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
References: <97.132e3372.27f3537e@aol.com>
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I always thought that was a standard method of demodulating phase
information.....

I am working on this round thing that can be used to reduce friction rather
than simply dragging things across the ground.....

Rye

WarmSpgs@aol.com wrote:

> In a message dated 3/28/01 2:58:35 AM Eastern Standard Time,
> rik.strobbe@fys.kuleuven.ac.be writes:
>
> << What happens if you send a BPSK (instant phase switching) as reference
>  signal to a PLL ? >>
>
> An interesting thought.  T



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: DL4YHF@aol.com
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Date: Wed, 28 Mar 2001 15:14:21 EST
Subject: RE: LF: <Tech>Re: A Question
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hi Alberto, Jim, and LF group,
<BR>
<BR>As Jim already wrote, the amplitude measuring facility of Spectrum Lab uses a 
<BR>more or less arbitrarily chosen scale which is 0 dB for the lowest possible 
<BR>signal which can be detected (with a 16 bit ADC). However, I am not very 
<BR>happy with that choice myself. There is also the possibility of using Andy's 
<BR>CFAR noise detection algorithm (it is hidden somewhere in the spectrum alert 
<BR>function, works perfect except for the case when there is no input signal at 
<BR>all ;-).
<BR>
<BR>Someone (was it Alberto ?) has already written about the problem that some 
<BR>soundcards seem to use a kind of AGC (no matter what the mixer settings say), 
<BR>&nbsp;making absolute measurements inaccurate in the presence of static crashes 
<BR>etc.
<BR>
<BR>IMO, a good solution is to display the difference (in dB) from the 'cursor 
<BR>position' to a definable 'reference area' where either the noise level or the 
<BR>amlitude of a reference generator can be measured. An optional "smoothing" 
<BR>(or averaging) of the displayed dB value can also help.
<BR>
<BR>Alberto, if you find a good solution for this I would like to know how it 
<BR>works. Thanks...
<BR>
<BR>Good luck for now,
<BR>73s Wolf (DL4YHF).
<BR></FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <003e01c0b7ba$708665b0$0a00a8c0@ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010328085558.2f57efaa@mail.cc.kuleuven.ac.be>
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
Date: Wed, 28 Mar 2001 09:04:11 -0500
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Greetings All:

From: "Rik Strobbe"

> That is 100% correct, my aim is to find a trade-off between simplicity and
> bandwidth. This is standard practice for any CW transmitter where
> key-clicks are surpressed to an acceptable level.

Oh my, the "acceptable level" issue around hard keying again.  I thought
this discussion was only undertaken in the high speed CW community - at 50
WPM on CW I use hard keying, very hard keying, as an aid to making the CW
copyable as the speed increases.  Some operators in the CW community find
the hard keying hard to take, but I also find the "bell" like keying of some
signals so very objectionable - to each his own.

The issue of BPSK keying should in my opinion focus around determining the
losses in signal recovery when the phase reversal is "softened".  If the
loss is measurable in the receive system performance then it should not be
done.  Pushing the envelope of LF propagation with BPSK must not be degraded
by "softening" the keying, if it does in a measurable way, say .1 dB or more
then I for one just wont use such a system here at all.

This position might sound a tad hard for some of you on this reflector but I
have only to look at the Loran signal garbage to tell me what good
engineering practice allows.  We need do nothing better than that service is
achieving.

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <15264.200103281753@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
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Subject: LF: <Tech>BPSK modulation - PLL
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Dear Rick, LF group,

Suppose the PLL is phase locked to the input signal, and suddenly 
a 180degrees phase transition occurs at the input. There would 
then be an error signal in the loop, which would force the relative 
phase of the output to change until it matched the input signal 
again. The phase would have to change in a continuous fashion 
since the loop filter would prevent the VCO tuning voltage from 
changing discontinuously - presumably, you could control the rate 
at which the phase changed by altering the loop filter time 
constants. 

But I can see a problem - what will the PLL do at the instant the 
phase changes? as far as the phase detector is concerned, a 
sudden 180degree phase change could mean either a lead of 180 
degrees or a lag of 180degrees. The error between input and 
output phases could be corrected either by increasing the VCO 
frequency until the output phase "catches up" with the input, or 
decreasing it until it "slows down" to match the input. The output 
phase could shift in either direction, although the end result would 
always be to match the input phase. The PLL texts call the period 
that the circuit is achieving the phase-locked condition the "capture 
transient", and each capture transient is an individual, depending 
on the type of phase detector, the timing of the input transient 
relative to the VCO output phase, residual phase errors and noise 
in the loop, etc, etc. The output phase can go through a much more 
complicated trajectory than the input.

Therefore, each output phase transition would be different as well 
as gradual; presumably, this would add a noise-like element to the 
sidebands of the signal. Hopefully, there would be an equal number 
of "up" transitions as "down" transitions, otherwise the mean 
frequency of the output would be different to that of the input. What 
effect all this would have on the bandwidth, and communications 
efficiency of the signal, I don't know, but for a simple circuit, 
behaviour would be quite complex.

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
Message-ID: <53.44a5545.27f3564d@aol.com>
Date: Wed, 28 Mar 2001 09:59:25 EST
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
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In a message dated 3/28/01 2:58:35 AM Eastern Standard Time, 
rik.strobbe@fys.kuleuven.ac.be writes:

<< What happens if you send a BPSK (instant phase switching) as reference
 signal to a PLL ? >>

An interesting thought.  (Apologies to everyone for the previous message 
which ended at this point.  I was typing merrily along, when AOL abruptly 
announced: "your mail has been sent.")

The PLL would certainly perform filtering action, but I suspect some 
attention would need to be paid to the loop filter.  There will be a tradeoff 
to be determined between settling speed and overshoot, but apart from that 
I'd think it would be physically simpler to implement than the high-Q 
filtering and limiting.  An abrupt 180 degree transition is a bit ambiguous 
for some phase detectors to handle, so a single stage of L-C pre-filtering 
may still be desirable.  Overall, though, this seems as if it should be 
practical to try.

73,
John


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: rsgb_lf_group@blacksheep.org
References: <14gpKS-1kYC0WC@fwd04.sul.t-online.com> <14h8HU-0thmHAC@fwd06.sul.t-online.com> <14i0Fh-1gkX5sC@fwd06.sul.t-online.com>
Subject: LF: Re: PVC
Date: Wed, 28 Mar 2001 13:29:37 +0200
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According to one of my books the dielectric constant of PVC is 3.5.

73, Dick, PA0SE

----- Oorspronkelijk bericht -----
Van: jannsen <0482183881-0001@t-online.de>
Aan: <rsgb_lf_group@blacksheep.org>
Verzonden: dinsdag 27 maart 2001 22:39
Onderwerp: LF: PVC


> Hi group,
>
> is there any who knows or can look up the  - ah I do`nt know the correct
word -
> elecric property constant (dielektrizitätskonstante in the german
language)
> for PVC ? ok, glass has  2 -12, air 1, ceramic 100 -10000. PVC is not on
my
> list.
> tks for the answer in advance
> Uwe/dj8wx
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <3AC1AFA8.894F6591@usa.net>
Date: Wed, 28 Mar 2001 11:32:24 +0200
From: "Alberto di Bene" <dibene@usa.net>
Organization: Undisclosed
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Subject: LF: Re: [TECH] A question
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Andy,
          thanks for your suggestion. As a matter of fact I am already using
your algorithm ! I use it to compute the brightness levels for the spectrogram,
but only when AGC is on. So, with AGC on, the brightness is a (non-linear)
function of the ratio between the magnitude and the base noise level
computed with the CFAR method. I learnt it from your previous post of many
months ago, I liked it, and I put it into immediate use.
I will use it when implementing the S/N display, together with the choice of
selecting first a frequency range, whose mean level will be the noise reference
level for the computation.
For the present problem, displaying a relative strenght level, I think I will
allow the choice between the two main methods that have been suggested,
i.e. referring it either to the saturation value of the ADC, or to a previously
choosen reference level.

73  Alberto  I2PHD

Talbot Andrew wrote:

> One method for determining S/N ration in an environment where signals
> and noise are constantly changing  - used a lot in Radar and Other
> techniques - is an algorithm called Constant False Alarm Rate.   I
> covered this in detail in postings to this reflector several months ago,
> but basically the technique is as follows :
>
> 1)      Perform an FFT on a block of data
> 2)      Sort all the bins into increasing order of amplitude.
> 3)      Take the amplitude of the lower quartile bin.
> 4)      Add 3dB to this figure and this gives a very good approximation
> to the noise level
> 5)      For new signal alarm and signal detection add a threshold - 10dB
> is a good starting point
> 6)      Check for successive hits above this threshold N out of M times
> before indicating valid.
>
> You will only be interested in satges 1) to 4).  This assumes the real
> noise level is flat across the FFT width, which I hope is true for all
> narrowband work, but not necesssarily so for full SSB bandwidth
> sampling.
>
> Andy  G4JNT
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 28 Mar 2001 08:55:58
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
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>However, I believe the object of Rik's proposal was to decrease bandwidth 
>while retaining as much simplicity in the system as possible.  If one can 
>abide the slower phase transitions of the filtered signal, and the modest 
>increase in bandwidth from not having dragged out the transitions even 
>further, the technique should work at moderate power levels.  It's a 
>collection of trade-offs, as is anything in engineering.

Hello John and group,

That is 100% correct, my aim is to find a trade-off between simplicity and
bandwidth. This is standard practice for any CW transmitter where
key-clicks are surpressed to an acceptable level. If one would want a CW
transmission with absolute minimal key-clicks the same kind of envelloping
as used with PSK would be needed, the soft keying we use is a compromise.
The main reason why 'rude BPSK' has a relative large bandwidth (compared to
CW) is because :
- the 180 degrees phase jumps are the equivalent of an extreme hard keying
- the BPSK sidebands are 6dB stronger than CW sidebands (this is directly
related to the 1/-1 switching versus 1/0 switching that gives BPSK a 6dB
advantage over CW).
My goal is to make the phase transition 'less hard' in order to reduce the
bandwidth of a (10BPS) BPSK transmission to that of a normal keyed (12WPM)
CW transmission.

BTW,  another idea : 
What happens if you send a BPSK (instant phase switching) as reference
signal to a PLL ? 
The reaction time of the PLL would depend on the feedback circuitery, maybe
this could also be used to get 'soft phase transistions'. 
At 136kHz the whole PLL could be incorporated in a single CMOS4046, just 1
cheap IC and half a dozen resistors/capacitors might do the job.

73, Rik  ON7YD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: [TECH] A question
Date: Wed, 28 Mar 2001 08:48:26 +0100
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One method for determining S/N ration in an environment where signals
and noise are constantly changing  - used a lot in Radar and Other
techniques - is an algorithm called Constant False Alarm Rate.   I
covered this in detail in postings to this reflector several months ago,
but basically the technique is as follows :

1)	Perform an FFT on a block of data 
2)	Sort all the bins into increasing order of amplitude.
3)	Take the amplitude of the lower quartile bin.
4)	Add 3dB to this figure and this gives a very good approximation
to the noise level
5)	For new signal alarm and signal detection add a threshold - 10dB
is a good starting point
6)	Check for successive hits above this threshold N out of M times
before indicating valid.

You will only be interested in satges 1) to 4).  This assumes the real
noise level is flat across the FFT width, which I hope is true for all
narrowband work, but not necesssarily so for full SSB bandwidth
sampling.

Andy  G4JNT


> -----Original Message-----
> From: Alberto di Bene [mailto:dibene@usa.net]
> Sent: 2001-03-27 13:33
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: [TECH] A question
> 
> 
> I have a question for you all.
> 
> I am implementing both in Argo and Spectran a function that will
> display the relative level (in dB) of the spectral lines when 
> you hover the
> mouse cursor over them. So far so good.
> What I am uncertain about, is that word, 'relative'. Relative 
> to what ?
> 
> One possibility is to first click on a given point of the 
> display, take this
> bin amplitude as a reference, and the values subsequently 
> displayed will
> be relative to this reference level.  But frankly I don't 
> like this solution
> very much, even if this will be perhaps the correct way to measure
> the S/N ratio, but this is another topic.
> 
> Another solution which has been suggested is to take as reference
> level the saturation level of the ADC. This is quite valid is case of
> a single signal, but on a real case what will happen with this method
> is that the measured level will vary depending on the total 
> input to the
> ADC, even if the signal being measured is constant in amplitude.
> 
> I gave a thought about using the Parseval equation, but 
> before pursuing
> this further, I decided to ask the question here, as perhaps 
> this problem
> has been already encountered and solved by others.
> I am open to any suggestions and advices.   Thanks.
> 
> 73   Alberto   I2PHD
> 
> 
> 
> 
> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Robin T. Greenwood" <robin@g3lba.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <14gpKS-1kYC0WC@fwd04.sul.t-online.com> <14h8HU-0thmHAC@fwd06.sul.t-online.com> <14i0Fh-1gkX5sC@fwd06.sul.t-online.com>
Subject: LF: Re: PVC
Date: Tue, 27 Mar 2001 21:11:05 +0100
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Dielectric constant is 4 and loss tangent is 600x10*4
Robin
----- Original Message -----
From: "jannsen" <0482183881-0001@t-online.de>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 27, 2001 9:39 PM
Subject: LF: PVC


> Hi group,
>
> is there any who knows or can look up the  - ah I do`nt know the correct
word -
> elecric property constant (dielektrizitätskonstante in the german
language)
> for PVC ? ok, glass has  2 -12, air 1, ceramic 100 -10000. PVC is not on
my
> list.
> tks for the answer in advance
> Uwe/dj8wx
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: PVC
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Hi group,

is there any who knows or can look up the  - ah I do`nt know the correct word -
elecric property constant (dielektrizitätskonstante in the german language)
for PVC ? ok, glass has  2 -12, air 1, ceramic 100 -10000. PVC is not on my 
list. 
tks for the answer in advance
Uwe/dj8wx



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
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Date: Tue, 27 Mar 2001 11:32:24 EST
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
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In a message dated 3/26/01 12:06:05 PM Eastern Standard Time, 
j.r.moritz@herts.ac.uk writes:

<< But  unfortunately, any clipping or AGC will distort the amplitude 
 envelope, which in turn will re-introduce unwanted sidebands.  >>

This may be a matter of semantics, but clipping won't actually "re-introduce" 
sidebands.  While AGC would indeed distort the amplitude envelope and worsen 
sidebands, hard RF clipping eliminates envelope variations entirely.  The 
consequence of clipping is that we no longer have the envelope to help us 
further suppress the phase-modulation sidebands.  The sidebands themselves 
remain just as they would for any continuous-shift PSK signal--less energetic 
than for brute-force instantaneous PSK, but broader than if we retained the 
amplitude variations that accompany appropriate filtering.

The ideal case would be to generate a waveform based on root-raised-cosine 
filtering in the exciter, use envelope-elimination-and-recovery to amplify 
the signal at maximum efficiency, and use a corresponding filter at the 
receive end.

However, I believe the object of Rik's proposal was to decrease bandwidth 
while retaining as much simplicity in the system as possible.  If one can 
abide the slower phase transitions of the filtered signal, and the modest 
increase in bandwidth from not having dragged out the transitions even 
further, the technique should work at moderate power levels.  It's a 
collection of trade-offs, as is anything in engineering.

73,
John


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 27 Mar 2001 17:48:38 +0200
From: "Alberto di Bene" <dibene@usa.net>
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>
> I don't understand why the measured level will vary with the total
> input - surely provided the A/D converter is not overloaded, the
> signal component being displayed should only be proportional to
> the amplitude of that component of the input signal?
>

Thanks to all who answered so far (I am still open to suggestions !).
Jim, yes, I used the wrong phrasing to express what I had in mind.
What I meant is that I cannot use the instantaneous level in the time
domain as a parameter of the equation that computes the dB value
of the bin, as the same input level can be obtained by summing
different frequency components.

Would the following method be acceptable :
I compute (using the Parseval equation) what the single bin magnitude
would be if I feed to the ADC only a pure sinusoid such that the ADC is
just at the saturation point (i.e. a level of 32767 for a 16-bit card).
Then I use the computed magnitude as a reference value to display
the dB values of the various bins, which would of course be all
negative with this method.
What do you all think of this ?  Thanks for feedbacks.

73  Alberto  I2PHD





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 27 Mar 2001 14:48:52
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF:(TECH) A question.
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Hello Alberto,

I agree with Laurie for measuring the strength of a signal. 
Another usefull 'option' might be to give the SNR of any signal you put the
cursor on, so in that case the reference has to be the 'background noise'.

73, Rik  ON7YD

At 13:22 27/03/01 +0100, you wrote:
>Alberto,I am not an expert here, but if I wanted to compare signals over a
period of time, I would think it necessesary to establish a reference level
say from a signal generator.This would include all the elements in the
chain including the reciever.So if a ref. level is established in this way,
clicking on this first and then on the unknown signal would determine the
difference in db as you suggest. For what its worth! 73s Laurie.
>
>Attachment Converted: "C:\EUDORA\ATTACH\LF(TECH).htm"
>


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 Alberto, LF group,

Adding an amplitude measurement capability to Argo/Spectran 
sounds like an excellent idea - it would enable a meaningful 
measurement of relative signal strengths to be made.

DL4YHF's Spectrum Lab has such a facility - I don't know how 
Wolf has implemented this, but the amplitude scale seems to be 
fixed relative to the input full scale or minumum resolution. I think 
this is as good a method as any - there are many different ways 
one might want to specify the amplitude or SNR.

I don't understand why the measured level will vary with the total 
input - surely provided the A/D converter is not overloaded, the 
signal component being displayed should only be proportional to 
the amplitude of that component of the input signal?

Cheers, Jim Moritz
73 de M0BMU


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
Subject: LF:(TECH) A question.
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<DIV><FONT face=Arial size=2>Alberto,I am not an expert here, but if I wanted to 
compare signals over a period of time, I would think it necessesary to establish 
a reference level say from a signal generator.This would include all the 
elements in the chain including the reciever.So if a ref. level is established 
in this way, clicking on this first and then on the unknown signal would 
determine the difference in db as you suggest. For what its worth! 73s 
Laurie.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alberto di Bene" <dibene@usa.net>
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To: rsgb_lf_group@blacksheep.org
Subject: LF: [TECH] A question
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I have a question for you all.

I am implementing both in Argo and Spectran a function that will
display the relative level (in dB) of the spectral lines when you hover the
mouse cursor over them. So far so good.
What I am uncertain about, is that word, 'relative'. Relative to what ?

One possibility is to first click on a given point of the display, take this
bin amplitude as a reference, and the values subsequently displayed will
be relative to this reference level.  But frankly I don't like this solution
very much, even if this will be perhaps the correct way to measure
the S/N ratio, but this is another topic.

Another solution which has been suggested is to take as reference
level the saturation level of the ADC. This is quite valid is case of
a single signal, but on a real case what will happen with this method
is that the measured level will vary depending on the total input to the
ADC, even if the signal being measured is constant in amplitude.

I gave a thought about using the Parseval equation, but before pursuing
this further, I decided to ask the question here, as perhaps this problem
has been already encountered and solved by others.
I am open to any suggestions and advices.   Thanks.

73   Alberto   I2PHD






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Petr Maly" <p.maly@gmc.net>
To: rsgb_lf_group@blacksheep.org
References: <000201c0b622$de4b6440$36ea7ad5@default> <01ad01c0b68f$896d63c0$1601a8c0@maly.gmccz.cz.gmc.net> <000d01c0b6a3$38c912c0$5f6e883e@g3aqc>
Subject: LF: Re: Re: Re: DX Cluster spots for 24/25th Mar at GB7DXM
Date: Tue, 27 Mar 2001 13:24:14 +0200
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That's right. I was surprised how fast the signal dropped down. From the
beginning it looked for "armchair copy" QSO but at the end it was pretty
hard for me to get RST at least. It was either short positive peak in the
conditions or vice versa sharp drop down during QSO.

73 Petr OK1FiG

----- Original Message -----
From: Laurie Mayhead <laurie@g3aqc.freeserve.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 27, 2001 11:48 AM
Subject: LF: Re: Re: DX Cluster spots for 24/25th Mar at GB7DXM


> Hi Petr, your signal dropped from Q5 to Q4 or less during our QSO. Perhaps
> we were seeing the arrival of disturbed condx due to CMEs. 73s Laurie.
> ----- Original Message -----
> From: "Petr Maly" <p.maly@gmc.net>
> To: <rsgb_lf_group@blacksheep.org>
> Sent: Tuesday, March 27, 2001 8:28 AM
> Subject: LF: Re: DX Cluster spots for 24/25th Mar at GB7DXM
>
>
> > Hi all
> > I was on air again this weekend. On Saturday there was a lot of stations
> and
> > conditions were good. On Sunday the band was totally empty and deaf
> (except
> > a QSO with G3AQC). Is there any explanation for this?
> >
> > 73 Petr OK1FiG
> >
> >
> > ----- Original Message -----
> > From: Alan Melia <Alan.Melia@BTINTERNET.COM>
> > To: LF-Group <rsgb_lf_group@blacksheep.org>
> > Sent: Monday, March 26, 2001 5:15 PM
> > Subject: LF: DX Cluster spots for 24/25th Mar at GB7DXM
> >
> >
> > > Hi all, not a lot of spots this week, and whilst I did not do a lot of
> > > listening, when I was within range of the radio it seemed fairly
quiet.
> > >
> > >    136.7  OK1FIG      25-Mar-2001 1130Z  cq cq ...
> > > <DK8KW>
> > >    136.8  ON6NL       24-Mar-2001 1410Z  in QSO with dl/om2tw . 519
> > > <DJ1YFK>
> > >    136.8  DL/OM2TW    24-Mar-2001 1408Z  519in jo32qg,he in jo52bd
> > > <DJ1YFK>
> > >    136.7  DL/OM2TW    24-Mar-2001 1400Z  559 cq
> > > <DL1SAN>
> > >    137.1  OK1FIG      24-Mar-2001 1355Z  559 cq
> > > <DL1SAN>
> > >    136.5  PA3CPM      22-Mar-2001 1901Z  calling cq UK
> > > <PA3CNX>
> > >    136.5  DJ6FU       21-Mar-2001 1719Z  cq cq
> > > <DL3FDO>
> > >    137.7  OM2YL       18-Mar-2001 1557Z  CQ on QRSS
> > > <OM2TW>
> > >    137.2  OM2TW       18-Mar-2001 1546Z  CQ  599...
> > > <OM2KM>
> > >    137.2  OK1DTN      18-Mar-2001 1235Z  CQ
> > > <OM2TW>
> > > G3NYK de GB7MRS 26-Mar-2001 1500Z >
> > >
> > > Cheers de Alan G3NYK  JO02PB
> > > Alan.Melia@btinternet.com
> > >
> > >
> > >
> > >
> >
> >
> >
>
>
>



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
References: <000201c0b622$de4b6440$36ea7ad5@default> <01ad01c0b68f$896d63c0$1601a8c0@maly.gmccz.cz.gmc.net>
Subject: LF: Re: Re: DX Cluster spots for 24/25th Mar at GB7DXM
Date: Tue, 27 Mar 2001 10:48:53 +0100
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Hi Petr, your signal dropped from Q5 to Q4 or less during our QSO. Perhaps
we were seeing the arrival of disturbed condx due to CMEs. 73s Laurie.
----- Original Message -----
From: "Petr Maly" <p.maly@gmc.net>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 27, 2001 8:28 AM
Subject: LF: Re: DX Cluster spots for 24/25th Mar at GB7DXM


> Hi all
> I was on air again this weekend. On Saturday there was a lot of stations
and
> conditions were good. On Sunday the band was totally empty and deaf
(except
> a QSO with G3AQC). Is there any explanation for this?
>
> 73 Petr OK1FiG
>
>
> ----- Original Message -----
> From: Alan Melia <Alan.Melia@BTINTERNET.COM>
> To: LF-Group <rsgb_lf_group@blacksheep.org>
> Sent: Monday, March 26, 2001 5:15 PM
> Subject: LF: DX Cluster spots for 24/25th Mar at GB7DXM
>
>
> > Hi all, not a lot of spots this week, and whilst I did not do a lot of
> > listening, when I was within range of the radio it seemed fairly quiet.
> >
> >    136.7  OK1FIG      25-Mar-2001 1130Z  cq cq ...
> > <DK8KW>
> >    136.8  ON6NL       24-Mar-2001 1410Z  in QSO with dl/om2tw . 519
> > <DJ1YFK>
> >    136.8  DL/OM2TW    24-Mar-2001 1408Z  519in jo32qg,he in jo52bd
> > <DJ1YFK>
> >    136.7  DL/OM2TW    24-Mar-2001 1400Z  559 cq
> > <DL1SAN>
> >    137.1  OK1FIG      24-Mar-2001 1355Z  559 cq
> > <DL1SAN>
> >    136.5  PA3CPM      22-Mar-2001 1901Z  calling cq UK
> > <PA3CNX>
> >    136.5  DJ6FU       21-Mar-2001 1719Z  cq cq
> > <DL3FDO>
> >    137.7  OM2YL       18-Mar-2001 1557Z  CQ on QRSS
> > <OM2TW>
> >    137.2  OM2TW       18-Mar-2001 1546Z  CQ  599...
> > <OM2KM>
> >    137.2  OK1DTN      18-Mar-2001 1235Z  CQ
> > <OM2TW>
> > G3NYK de GB7MRS 26-Mar-2001 1500Z >
> >
> > Cheers de Alan G3NYK  JO02PB
> > Alan.Melia@btinternet.com
> >
> >
> >
> >
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000c01c0b6a3$9c2d1aa0$ba9e01d5@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: solar alert
Date: Tue, 27 Mar 2001 10:50:36 +0100
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The attached was received from NASA this morning, the sun has become very
active suddenly within the last few days, so expect a prolonged period of
disturbed conditions.
------------------------------
SOLAR ACTIVITY: In recent days the Boulder sunspot number has rocketed to
339, its highest level since July 2000.  At least one large sunspot group
has a complex magnetic field that could harbor energy for powerful solar
flares.  Forecasters estimate a 20% chance of an X-class eruption during
the next 24 hours.

AURORA WATCH: An interplanetary shock wave buffeted Earth's magnetosphere
Tuesday morning and another may be following close behind. A coronal mass
ejection that left the Sun on March 25th will arrive late Tuesday or
Wednesday and possibly trigger additional geomagnetic disturbances. In
recent days Alaskan sky watchers have enjoyed some of the best auroras of
the current solar cycle.  Check out our gallery of aurora photos for the
latest images.
----------------------

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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References: <000201c0b622$de4b6440$36ea7ad5@default>
Subject: LF: Re: DX Cluster spots for 24/25th Mar at GB7DXM
Date: Tue, 27 Mar 2001 09:28:36 +0200
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Hi all
I was on air again this weekend. On Saturday there was a lot of stations and
conditions were good. On Sunday the band was totally empty and deaf (except
a QSO with G3AQC). Is there any explanation for this?

73 Petr OK1FiG


----- Original Message -----
From: Alan Melia <Alan.Melia@BTINTERNET.COM>
To: LF-Group <rsgb_lf_group@blacksheep.org>
Sent: Monday, March 26, 2001 5:15 PM
Subject: LF: DX Cluster spots for 24/25th Mar at GB7DXM


> Hi all, not a lot of spots this week, and whilst I did not do a lot of
> listening, when I was within range of the radio it seemed fairly quiet.
>
>    136.7  OK1FIG      25-Mar-2001 1130Z  cq cq ...
> <DK8KW>
>    136.8  ON6NL       24-Mar-2001 1410Z  in QSO with dl/om2tw . 519
> <DJ1YFK>
>    136.8  DL/OM2TW    24-Mar-2001 1408Z  519in jo32qg,he in jo52bd
> <DJ1YFK>
>    136.7  DL/OM2TW    24-Mar-2001 1400Z  559 cq
> <DL1SAN>
>    137.1  OK1FIG      24-Mar-2001 1355Z  559 cq
> <DL1SAN>
>    136.5  PA3CPM      22-Mar-2001 1901Z  calling cq UK
> <PA3CNX>
>    136.5  DJ6FU       21-Mar-2001 1719Z  cq cq
> <DL3FDO>
>    137.7  OM2YL       18-Mar-2001 1557Z  CQ on QRSS
> <OM2TW>
>    137.2  OM2TW       18-Mar-2001 1546Z  CQ  599...
> <OM2KM>
>    137.2  OK1DTN      18-Mar-2001 1235Z  CQ
> <OM2TW>
> G3NYK de GB7MRS 26-Mar-2001 1500Z >
>
> Cheers de Alan G3NYK  JO02PB
> Alan.Melia@btinternet.com
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 27 Mar 2001 08:29:41
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
In-reply-to: <25798.200103261700@gemini>
References: <3.0.1.16.20010326144713.21b765b2@mail.cc.kuleuven.ac.be> <65AECDF1F89AD411900400508BFC869F9C03FA@pdw-mail-1.dera.gov .uk>
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Hello Jim & LF group,

That is indeed another way to have a look at it. But I would't try to make
a perfect envelloped BPSK signal (that would take a filter with a Q of many
1000) but a signal that has a bandwidth that is approximately the same as
that of a normal CW signal.
The same way as the key clicks are surpressed by soft keying (avoiding
steep slopes) I would try to avoid the 'steep' phase jumps and spread the
180 degrees phase change over a few milliseconds.

73, Rik  ON7YD

At 18:05 26/03/01 +0000, you wrote:
>Dear Rik, LF Group,
>
>Another way of looking at this modulation method is that the high Q 
>tuned circuit acts as a narrow filter which removes the unwanted 
>sidebands of your "rude" BPSK - the signal will certainly be 
>amplitude modulated at the output of the tuned circuit; in fact it will 
>look very similar to the "ideal" envelope-modulated BPSK signal. 
>This is effectively another way of generating the BPSK signal, 
>analagous to generating SSB by the filter method. But 
>unfortunately, any clipping or AGC will distort the amplitude 
>envelope, which in turn will re-introduce unwanted sidebands. 
>
>Of course, if the filter was placed at the transmitter output, this 
>criticism would not apply. But although it is probably possible, 
>producing an antenna tuning network with a loaded Q of 700 would 
>be quite difficult.
>
>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: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: DX Cluster spots for 24/25th Mar at GB7DXM
Date: Mon, 26 Mar 2001 16:15:12 +0100
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Hi all, not a lot of spots this week, and whilst I did not do a lot of
listening, when I was within range of the radio it seemed fairly quiet.

   136.7  OK1FIG      25-Mar-2001 1130Z  cq cq ...
<DK8KW>
   136.8  ON6NL       24-Mar-2001 1410Z  in QSO with dl/om2tw . 519
<DJ1YFK>
   136.8  DL/OM2TW    24-Mar-2001 1408Z  519in jo32qg,he in jo52bd
<DJ1YFK>
   136.7  DL/OM2TW    24-Mar-2001 1400Z  559 cq
<DL1SAN>
   137.1  OK1FIG      24-Mar-2001 1355Z  559 cq
<DL1SAN>
   136.5  PA3CPM      22-Mar-2001 1901Z  calling cq UK
<PA3CNX>
   136.5  DJ6FU       21-Mar-2001 1719Z  cq cq
<DL3FDO>
   137.7  OM2YL       18-Mar-2001 1557Z  CQ on QRSS
<OM2TW>
   137.2  OM2TW       18-Mar-2001 1546Z  CQ  599...
<OM2KM>
   137.2  OK1DTN      18-Mar-2001 1235Z  CQ
<OM2TW>
G3NYK de GB7MRS 26-Mar-2001 1500Z >

Cheers de Alan G3NYK  JO02PB
Alan.Melia@btinternet.com




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>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org,  lowfer@qth.net
Date: Mon, 26 Mar 2001 18:38:24 +0000
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Subject: LF: M0BMU Wolf Beacon
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Dear LF Group and Lowfers,

Unfortunately, I was not able to transmit beacon signals last night 
due to a local power cut.

However, I hope to be on tonight, between 0000 and 0200, on 
137.500kHz again.

Cheers, Jim Moritz
73 de M0BMU


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>
Organization: University of Hertfordshire
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Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
In-reply-to: <3.0.1.16.20010326144713.21b765b2@mail.cc.kuleuven.ac.be>
References: <65AECDF1F89AD411900400508BFC869F9C03FA@pdw-mail-1.dera.gov .uk>
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Dear Rik, LF Group,

Another way of looking at this modulation method is that the high Q 
tuned circuit acts as a narrow filter which removes the unwanted 
sidebands of your "rude" BPSK - the signal will certainly be 
amplitude modulated at the output of the tuned circuit; in fact it will 
look very similar to the "ideal" envelope-modulated BPSK signal. 
This is effectively another way of generating the BPSK signal, 
analagous to generating SSB by the filter method. But 
unfortunately, any clipping or AGC will distort the amplitude 
envelope, which in turn will re-introduce unwanted sidebands. 

Of course, if the filter was placed at the transmitter output, this 
criticism would not apply. But although it is probably possible, 
producing an antenna tuning network with a loaded Q of 700 would 
be quite difficult.

Cheers, Jim Moritz
73 de M0BMU




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
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Date: Mon, 26 Mar 2001 10:12:34 EST
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
To: rsgb_lf_group@blacksheep.org
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In a message dated 3/26/01 8:49:52 AM Eastern Standard Time, 
rik.strobbe@fys.kuleuven.ac.be writes:

<< So if one would send a 'rude BPSK' signal (as is  created with an XOR 
gate) through a resonant LC-circuit you will get continuous phase shift at 
the output. The phase shift time will depend on  the Q of the LC-circuit.... 
(snip)....  A side effect will be that there is also some AM created, but 
this can be  'corrected' by an AGC amplifier (or just hard clipping, but this 
might  increase bandwidth too much). >>

Hard clipping will not increase bandwidth if one has indeed made the phase 
shift continuous by that point in the circuit.  In fact, it will be a 
necessity.  AGC could not be made fast enough to remove the amplitude 
variations, and if they are not removed, a practical power amplifier 
following the high-Q circuitry would tend to reintroduce extraneous sidebands.

73,
John

 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 26 Mar 2001 14:47:13
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
In-reply-to: <65AECDF1F89AD411900400508BFC869F9C03FA@pdw-mail-1.dera.gov .uk>
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Over the weekend I had a closer look at the possibilities of reducing the
bandwidth of a BPSk signal by continuous phase modulation.
Simple simulations show that the bandwidth of the signal is reduced when
continuous phase modulation is applied. When 5% of the bit-time (= 5ms) is
allowed the continuous phase shift the bandwidth of the BPSK signal should
be less than that of a normal keyed CW transmission at 12WPM.
Next question was how to implement the continuous phase shift?
One way would be to implement this digital, but this would require a rather
high reference oscillator (in the 30-100MHz range, depending on how 'soft'
the signal should be).
But there might be an alternative and much simpler way :
If you send an RF signal through a (resonant) LC-circuit this circuit will
act as a kind of 'freewheel' where any change of amplitude ... and phase
will be 'softened'. So if one would send a 'rude BPSK' signal (as is
created with an XOR gate) through a resonant LC-circuit you will get
continuous phase shift at the output. The phase shift time will depend on
the Q of the LC-circuit, for our purposes (+/- 5ms phase shift time) we
would need a Q of about 700. At 136kHz it should not be impossible to
achieve such a Q, especially if we not use a simple passive LC circuit but
a LC-circuit with feedback amplifier.
A side effect will be that there is also some AM created, but this can be
'corrected' by an AGC amplifier (or just hard clipping, but this might
increase bandwidth too much).
A main advantage would be that the whole BPSK modulation circuitery can be
inserted between VFO and PA.

73, Rik  ON7YD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: "LF Group \(E-mail\)" <rsgb_lf_group@blacksheep.org>
Subject: LF: LF Propagation Monitoring using LORAN
Date: Mon, 26 Mar 2001 11:43:47 +0100
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A couple of weeks ago there was discussion on this reflector about using
LORAN as a source of LF propagation information.  I forwarded these on
to Perter, G3PLX, who looked at LOARN for this purpose some time ago.
Here are the two responses received from him :

Andy  G4JNT
------------------------------------------------------------------------
------------------
Thanks for the LORAN information. I had, as you will remember in the
days I was active on LF, done the LORAN software and was seeing most
of the phenomena quoted. If you remember, I was able to integrate the
energy received over the 136 kHz band and show that ALL the LORAN
transmitters audible on 100kHz were also emitting crap on 136kHz. I
must have another look, especially for the dx signals, about which I
had no chain GRI data. Looking for individual spectral lines is not
at all a good way to detect distant LORAN, since the amount of power
in one spectral line is a very small proportion of the total signal
power. It's rather better to receive the full bandwidth coherently at
100kHz, integrating the I and Q signals in an array of "time bins" at
the group repetition rate, and watch the narrow sqrt(sqr(I)+sqr(Q)
pulses creep out of the noise as time goes by.
---------------------------------------------------------------------

-----Original Message-----
From: Peter Martinez [mailto:Peter.Martinez@btinternet.com]
Sent: 2001-03-25 20:09
To: Talbot Andrew
Subject: Re: LF Propagation Monitoring 

Andy:

I dug out the LORAN software and had another play with it, and also
visited the Megapulse site to get a copy of the table mentioned by
one of your correspondents. As a result I have been able to identify
all the signals he was hearing, including some of the Newfoundland
sites, the West Russian one and the Saudi chain. I am doing this by
listening in a 3 kHz band straddling 100kHz and coherently
demodulating and integrating I/Q over several minutes at the chosen
group repetition rate.

I have also started writing a program to streamline this activity. It
isn't finsihed yet but will be able to derive frequency and time
references from one transmitter (for example Lessay) and use this to
attempt to coherently demodulate and synchronously detect other
signals, although I probably won't use the fascinating fact that all
LORAN transmitters emitted their first pulses at midnight on
01/01/1958 to get the timing absolute. Such a program could be
written for a soundcard/PC combination and would just need a
receiver, preferably the full LORAN bandwidth, tuned to make 100kHz
appear in the centre of the sampled audio band. At the moment I am
running it on my old DSP card and I don't think I could make it run
on the EVM because the front-end processing requires rather more data
fed to the PC than I can squeeze down the serial port.

73
Peter


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sun, 25 Mar 2001 15:53:24 -0500
From: "boffin1" <boffin1@compuserve.com>
Subject: Re: LF: Old Radcoms and PWs
To: rsgb_lf_group@blacksheep.org
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I still have one or two from pre-war days but in those days it had the
magnificent title "T and R  Bulletin"  !
Roger, G2AJV.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sun, 25 Mar 2001 19:30:45 +0100
From: "gii3kev" <gii3kev@netscapeonline.co.uk>
Organization: Netscape Online member
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To: "rsgb rsgb" <rsgb_lf_group@blacksheep.org>
Subject: LF: G3IPL/73
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Hello All
G3IPL/Don died suddenly last week. He was issued with one of the
original 73 khz permits.
He was licensed in his early teens and was only 66 years old.
73 de Mal/G3KEV


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "bernd grupe" <Bernd.Grupe@t-online.de>
To: rsgb_lf_group@blacksheep.org
References: <14gpKS-1kYC0WC@fwd04.sul.t-online.com> <14h8HU-0thmHAC@fwd06.sul.t-online.com>
Subject: Re: LF: TECH> new applet
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> Hallo Bernd,
> ich habe mir deine downloads mal angeschaut. rfc1.zip und rcode.zip lassen
>  sich 
> downloaden. vy dks dafür, Bernd.
> spule.-, loop.- und resonanz.zip kann ich nicht herunterladen. seite nicht 
> vorhaden, heißt es. sri.
> vy 73
> Uwe/dj8wx
>
>
Hallo Uwe,
danke für die Rückmeldung. Habe jetzt die fehlenden files alle mehrfach 
hochgeladen. mein Browser IE5.5 spinnt manchmal. Er behält die Seiteninformation 
während einer Sitzung gespeichert und reagiert nicht auf Aktualisieren. Daher 
kann ich oft nicht prüfen, ob eine seite wirklich verfügbar ist, wenn 
vorhergehend ein Fehler aufgetreten war. Nun aber habe ich den download geprüft, 
es geht! Viel spass mit den Programmen. Ich arbeite gerade an einem zusätzliche 
Applet. Es wird eine dB-Umrechnung machen und hat eine Vielfachskala für dBuV , 
Ueff/50 Ohm, S VHF und S HF usw.
73 Bernd,DF8ZR



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: PBRS176562@aol.com
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Date: Sun, 25 Mar 2001 11:07:53 EST
Subject: Re: LF: Old Radcoms and PWs
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=3 FAMILY="SANSSERIF" FACE="Verdana" LANG="0">hi
<BR>well the rsgb has gone all modern offering radcom's on cd-rom however at a 
<BR>price sure the cd rom take up less room.
<BR>but I still prefer the old paper copies and my collection of radcom takes up 
<BR>two book cases and i have the complete sets &nbsp;from 1950-2000 back then it was 
<BR>called radio communication. One day I hope to have the complete paper set.
<BR>
<BR>73 Paul RS176562
<BR></FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: TECH> new applet
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bernd grupe schrieb:
> Hello group,
>
> There has born an new applet on my homepage:
>
> http://go.to/df8zr
>
> choose: Applets --> name: RFC1
>
>  It's  programmed like a calculator and written in JAVA. You can run it
>  online 
> or download the zip-file as well. Hope it will be a useful tool for you. But 
> before scratching the assignments i would please you to proof the right
>  English 
> terms. Any suggestions for improvements are welcome.Thanks in advance..
> vy 73 bernd, DF8ZR
>
>
Hallo Bernd,
ich habe mir deine downloads mal angeschaut. rfc1.zip und rcode.zip lassen sich 
downloaden. vy dks dafür, Bernd.
spule.-, loop.- und resonanz.zip kann ich nicht herunterladen. seite nicht 
vorhaden, heißt es. sri.
vy 73
Uwe/dj8wx



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 24 Mar 2001 16:59:35 -0600
To: rsgb_lf_group@blacksheep.org,  rsgb_lf_group@blacksheep.org
From: "Les Rayburn" <les@highnoonfilm.com>
Subject: Re: LF: Re: wolf and inputpwr
Cc: lowfer@qth.net
In-reply-to: <000901c0b4a4$cc589ed0$687a37c0@w2ksn>
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At 12:55 PM 3/24/01 -0800, Stewart Nelson wrote:
>Hi Uwe and all,
>
>The present implementation of WOLF, unfortunately, has very poor
>dynamic range.  The BPSK signal must be between -20 dB and -50 dB,
>relative to full scale.
>
>If you are receiving your own transmission, or one from a nearby
>station, you may need to reduce the record level by 20 dB to prevent
>internal overload when it starts averaging.
>
>If you are trying to receive a signal buried in noise, you should
>set the record level so that frequent peaks reach -6 dB or higher,
>even if it means that occasional static crashes overload.
>This will ensure that the -50 dB minimum is not a limiting factor.
>
>If your Rx output is dominated by a strong interfering carrier, it may
>not be possible to set the record level high enough.  In this case,
>try to reduce the interference with a narrower IF filter, with a notch
>filter, or by preprocessing the recording through an audio editor
>with filtering features.
>
>Although 8-bit recordings normally degrade the effective S/N only
>slightly, recording in 16 bits can be a big help if the signal is
>mostly QRM, rather than noise.
>
>You will have to live with the dynamic range limitations for quite
>a while, because my priorities are for improving usability and weak
>signal performance.  Sorry for the trouble it has caused.
>
>73,
>
>Stewart KK7KA
>


I think we'd all agree that no apologies are necessary. This software is 
remarkable, and the first
practical application of something that developers have "talked" about for 
years. You are to be
congratulated. Many have mentioned features they would like to see, 
including GUI interface,
real time processing, etc...but I think your priority for development 
should rightly be
weak signal performance.

Thank you again for your efforts that have benefited all of us!

Les Rayburn, N1LF





Les Rayburn, N1LF
4919 Cox Cove
Helena, AL 35080
XMGR 184.8988khz WOLF Mode
1LF 187.300khz

Looking for a challenge? Try the ultimate weak signal mode, on 1750 Meters!
Visit the Noise Floor!
http://www.highnoonfilm.com/xmgr






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Stewart Nelson" <sn@scgroup.com>
To: rsgb_lf_group@blacksheep.org
References: <3.0.5.32.20010322142117.0083bc10@pop3.esoterica.pt> <14gsjv-0BYKP2C@fwd07.sul.t-online.com>
Subject: LF: Re: wolf and inputpwr
Date: Sat, 24 Mar 2001 12:55:45 -0800
Organization: SC Group
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Hi Uwe and all,

The present implementation of WOLF, unfortunately, has very poor
dynamic range.  The BPSK signal must be between -20 dB and -50 dB,
relative to full scale.

If you are receiving your own transmission, or one from a nearby
station, you may need to reduce the record level by 20 dB to prevent
internal overload when it starts averaging.

If you are trying to receive a signal buried in noise, you should
set the record level so that frequent peaks reach -6 dB or higher,
even if it means that occasional static crashes overload.
This will ensure that the -50 dB minimum is not a limiting factor.

If your Rx output is dominated by a strong interfering carrier, it may
not be possible to set the record level high enough.  In this case,
try to reduce the interference with a narrower IF filter, with a notch
filter, or by preprocessing the recording through an audio editor
with filtering features.

Although 8-bit recordings normally degrade the effective S/N only
slightly, recording in 16 bits can be a big help if the signal is
mostly QRM, rather than noise.

You will have to live with the dynamic range limitations for quite
a while, because my priorities are for improving usability and weak
signal performance.  Sorry for the trouble it has caused.

73,

Stewart KK7KA

----- Original Message -----
From: "jannsen" <0482183881-0001@t-online.de>
To: <rsgb_lf_group@blacksheep.org>
Sent: Saturday, March 24, 2001 10:26 AM
Subject: LF: wolf and inputpwr


> Hi all WOLFers,
> I am in the believe WOLF decodes vy weak signals. but with my equipment it
> decodes only if dp: is higher than abt 32. seems Brians line (down on the
page)
> proves that for true.
> what is wrong with my believe ?
>
> WOLF version 0.52
> t:  24 f:-0.646 a: 0.5 dp: -4.9 ci: 0 cj:302 ??????????????? -
> t:  48 f: 0.356 a: 0.4 dp: -9.0 ci: 0 cj:302 ??????????????? -
>
> t:  24 f: 0.356 a: 0.4 dp: -5.0 ci: 7 cj:384 ??????????????? -
> t:  48 f: 0.355 a: 0.5 dp: -9.2 ci: 7 cj:277 ??????????????? -
>
> t:  24 f:-0.646 a: 0.5 dp: -5.2 ci: 0 cj:302 ??????????????? -
> t:  48 f: 0.351 a: 0.8 dp:-10.3 ci: 6 cj:297 ??????????????? -
>
> t:  24 f:-0.001 a: 0.5 dp: 20.4 ci:13 cj:136 ????????????/O* -
> t:  48 f:-0.001 a: 0.5 dp: 19.6 ci: 6 cj: 91 Q94???????????? ?
>
> t:  24 f: 0.000 a:-0.6 dp: 31.7 ci:12 cj: 63 31O3Z4053???3OW ?
> t:  48 f: 0.001 a:-0.7 dp: 26.0 ci:12 cj: 63 3TNU1O053???3OW ?
>
> t:  24 f: 0.000 a:-0.0 dp: 33.4 ci:14 cj:104 RFJ*TV8*K/1KRH* ?
> t:  48 f: 0.000 a:-0.0 dp: 29.3 ci:11 cj:145 G.4YPJQIFDV*2.W ?
>
> a line from Brian:
> t:  24 f: 0.001 a:-1.2 dp: 79.9 ci: 9 cj: 44 CQ M0BMU M0BMU  -
>
> t:  24 f: 0.000 a: 1.4 dp:139.3 ci: 0 cj:373 531531531531531 -
> t:  48 f: 0.000 a: 1.4 dp:135.2 ci:10 cj:427 K*4/USY0JZLB9P/ ?
>
> regards
> Uwe/dj8wx




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "jannsen" <0482183881-0001@t-online.de>
To: rsgb_lf_group@blacksheep.org
References: <3.0.5.32.20010322142117.0083bc10@pop3.esoterica.pt>
Subject: LF: wolf and inputpwr
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Hi all WOLFers,
I am in the believe WOLF decodes vy weak signals. but with my equipment it 
decodes only if dp: is higher than abt 32. seems Brians line (down on the page)
proves that for true.
what is wrong with my believe ?
 
WOLF version 0.52
t:  24 f:-0.646 a: 0.5 dp: -4.9 ci: 0 cj:302 ??????????????? -
t:  48 f: 0.356 a: 0.4 dp: -9.0 ci: 0 cj:302 ??????????????? -

t:  24 f: 0.356 a: 0.4 dp: -5.0 ci: 7 cj:384 ??????????????? -
t:  48 f: 0.355 a: 0.5 dp: -9.2 ci: 7 cj:277 ??????????????? -

t:  24 f:-0.646 a: 0.5 dp: -5.2 ci: 0 cj:302 ??????????????? -
t:  48 f: 0.351 a: 0.8 dp:-10.3 ci: 6 cj:297 ??????????????? -

t:  24 f:-0.001 a: 0.5 dp: 20.4 ci:13 cj:136 ????????????/O* -
t:  48 f:-0.001 a: 0.5 dp: 19.6 ci: 6 cj: 91 Q94???????????? ?

t:  24 f: 0.000 a:-0.6 dp: 31.7 ci:12 cj: 63 31O3Z4053???3OW ?
t:  48 f: 0.001 a:-0.7 dp: 26.0 ci:12 cj: 63 3TNU1O053???3OW ?

t:  24 f: 0.000 a:-0.0 dp: 33.4 ci:14 cj:104 RFJ*TV8*K/1KRH* ?
t:  48 f: 0.000 a:-0.0 dp: 29.3 ci:11 cj:145 G.4YPJQIFDV*2.W ?

a line from Brian:
t:  24 f: 0.001 a:-1.2 dp: 79.9 ci: 9 cj: 44 CQ M0BMU M0BMU  -

t:  24 f: 0.000 a: 1.4 dp:139.3 ci: 0 cj:373 531531531531531 -
t:  48 f: 0.000 a: 1.4 dp:135.2 ci:10 cj:427 K*4/USY0JZLB9P/ ?

regards
Uwe/dj8wx









From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "bernd grupe" <Bernd.Grupe@t-online.de>
To: rsgb_lf_group@blacksheep.org
Subject: LF: TECH> new applet
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Hello group,

There has born an new applet on my homepage:

http://go.to/df8zr

choose: Applets --> name: RFC1

 It's  programmed like a calculator and written in JAVA. You can run it online 
or download the zip-file as well. Hope it will be a useful tool for you. But 
before scratching the assignments i would please you to proof the right English 
terms. Any suggestions for improvements are welcome.Thanks in advance..
vy 73 bernd, DF8ZR



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Nick" <maad65@dial.pipex.com>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: The EF50
Date: Sat, 24 Mar 2001 13:20:29 +0000
Message-ID: <47nobt4669lvk7goshag8sgcgoqr7uijhn@4ax.com>
References: <5.0.2.1.2.20010320102742.00aa05a0@mail.pncl.co.uk>
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On Wed, 21 Mar 2001 09:11:06 +0000, you wrote:

>Although off-subject there seems to be a lot of interest in the EF50.
>Attached is a text-only version of a recent article written by
>Keith Thrower, an ex-Director of Racal and an electronics historian.
>It comes from the journal of the "Centre for the History of Defence 
>Electronics"
>at Bournemouth University -  http://chide.bournemouth.a.c.uk


The URL should be 

http://chide.bournemouth.ac.uk

Nick


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>
Organization: University of Hertfordshire
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Subject: LF: M0BMU Wolf Beacon
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Dear Lowfers/LF Group,

I operated the Wolf BPSK beacon on 137.500kHz last night from 
0000 until 0400. Due to other commitments, I will not be QRV 
tonight, but the beacon will be operating again on Sunday night.

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
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Date: Sat, 24 Mar 2001 00:41:03 EST
Subject: Re: LF: <Tech> BPSK and bandwidth
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In a message dated 3/23/01 12:11:23 PM Eastern Standard Time, 
mike.dennison@rsgb.org.uk writes:

<< We must not be trapped into thinking that bandwidths close to those used 
for 
 QRSS are essential. >>

An interesting thought.  Spectrum usage depends on more than just the 
bandwidth of a signal, after all.  It's also related to the amount of time 
required to complete a transfer of information, and sometimes also ergonomic 
issues.

A couple of years ago, I witnessed a curious thing on 160m.  A couple of 
stations using AM phone had a half-hour QSO on 1995kHz, reminiscing about the 
good old days of amplitude modulation, occupying a total of about 10kHz.  
During and after that conversation, in the course of checking the band, I 
encountered some SSB operators a little lower on the dial, discoursing 
mightily about what a terrible waste of spectrum AM is, and how it shouldn't 
be allowed on the air.  Through continual misuse of incremental tuning, their 
QSO was occupying about 4kHz, and it went on for two hours.  So, the AM QSO 
used 5kHz-hours while the SSB QSO used 8kHz-hours of spectrum.

Now, obviously, this isn't a comparison based on technical issues only.  But 
it does illustrate that occupied bandwidth is not the whole story of spectrum 
utilization.    If one technique uses sub-Hertz bandwidths but requires 
multiple nights to complete a rudimentary QSO, while another technique needs 
tens of Hertz but can complete the same QSO in half an hour, there is no 
necessary reason to exclude the broader method from a band plan.

73,
John


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000c01c0b3e1$7c0fd600$468d883e@g3aqc>
From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. Beacon
Date: Fri, 23 Mar 2001 21:36:58 -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>In view of the disturbed conditions,I will not run 
the beacon tonight. Could do with an early night Hi. 73s 
Laurie.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Stewart Nelson" <sn@scgroup.com>
To: rsgb_lf_group@blacksheep.org
References: <65AECDF1F89AD411900400508BFC869F9C03FE@pdw-mail-1.dera.gov.uk>
Subject: LF: Re: Re: WOLF - Transmit
Date: Fri, 23 Mar 2001 11:06:56 -0800
Organization: SC Group
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Hi Andy and all,

In my implementation, the code which uses pnpat is intertwined
with modulation, etc., so I didn't include it.  Sorry.

The output of enccnv is an array 480 long, as is pnpat.
You transmit the first enccnv output, then the first bit of
pnpat, then the second enccnv output, etc.

If the message is all blanks, the result of enccnv is all
zeros.  In this case, the final transmit data stream would begin
with 00000101010101000100010001010000.

73,

Stewart KK7KA

----- Original Message ----- 
From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Friday, March 23, 2001 3:56 AM
Subject: LF: Re: WOLF - Transmit 


> Where is the array   pnpat[]  used ?  It is declared at the end of the
> listing you sent, but not referenced anywhere else.
> Not being a C programmer, it will take a bit ot time to translate the
> code  ;-|
>  Andy  G4JNT




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>
Organization: University of Hertfordshire
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Date: Fri, 23 Mar 2001 18:43:13 +0000
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Dear LF Group,

Will be running the WOLF beacon again tonight from 0000utc 
onwards, on 137.500kHz. If anyone would like to try some tests 
over the weekend, please let me know.

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@rsgb.org.uk>
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Date: Fri, 23 Mar 2001 16:55:00 -0000
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Subject: Re: LF: Old Radcoms and PWs
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>......... I wondered if anyone would be interested in piles of old
> Radcom and Practical Wireless from 1972 and thereabouts. Goodness knows why
> I kept them but they've got to go!
> Dave G3YXM, Birmingham.

Dave,

[commercial break] Can I interest you in the CD versions of these RadComs? 
They use up far less space. [end commercial break]



Mike Dennison, G3XDV
Publications Manager

* RadCom * GB2RS News *
* RSGB Books and CDs *
* RSGB Online Web Site *

Radio Society of Great Britain
Lambda House, Cranborne Road
Potters Bar, Herts UK, EN6 3JE
Tel: +44 (0) 1707 659015; Fax: +44 (0) 1707 645105
www.rsgb.org
RSGB - UK AMATEUR RADIO



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Date: Fri, 23 Mar 2001 16:51:59 -0000
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Subject: Re: LF: <Tech> BPSK and bandwidth
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Jim posed some possible flaws in alternative ways of generating BPSK in 
terms of bandwidth.

I think we must work out what is an acceptable bandwidth for LF 
transcontinental working (or indeed any other distance or path).

We must not be trapped into thinking that bandwidths close to those used for 
QRSS are essential. They may be convenient - even efficient - but if there is 
room on the band for people to use CW for intra-Europe working, why be 
forced into anything less for inter-continental? This means 30dB bandwidths in 
the region of 100Hz and 60dB bandwidths of, say 500Hz. In practice, there 
are very few people close enough to each other for a signal 60dB down to be 
audible at all.

Plainly there must be enough space to accommodate a group of people trying 
to work across the Atlantic, but this is a bandplanning issue not a technical 
one.

In short, if it is acceptable for me to use CW to work VE, it should be 
acceptable for BPSK to have the same practical bandwidth.

I bet that will start a battle!!!

Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Sergeant" <dsergeant@btinternet.com>
To: rsgb_lf_group@blacksheep.org
References: <28702.200103221619@gemini>
Subject: LF: Re: Key clicks
Date: Fri, 23 Mar 2001 16:52:21 -0000
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>From Dave G3YMC
>Actually, key clicks are never likely to be a huge issue on LF; when
>compared to HF standards, even a full 1W ERP is a sub-QRP
>signal, and the higher noise level will tend to swamp clicks from all
>but the most local stations anyway.

I am not sure this generalisation is really true.  I receive quite a few
stations who are up to s9 + 20dB and they are hardly 'most local'.  Local
noise level varies considerably between stations, and with many of us the
limiting factor is loran - I was in the shack a week ago when Lessay went
off air for around 10 seconds - I saw first hand what my noise level was
without it, and how strong it really was.  Although I am not aware of any
stations with key clicks, I am pretty sure I would be able to copy the
clicks if they were there on the stronger stations I hear, even with loran.

By the way, I just happened to spot this remark in the 'sea' of wolf
messages yesterday.  Most of course get deleted before I read them..

Cheers Dave G3YMC
dsergeant@btinternet.com
dsergeant@iee.org
http://www.btinternet.com/~dsergeant






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "G3YXM" <g3yxm@wireless.org.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Old Radcoms and PWs
Date: Fri, 23 Mar 2001 14:29:29 -0000
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Dear all.

As there seems to be a fondness for nostalgia on here (yes I do know and
love the EF50!) I wondered if anyone would be interested in piles of old
Radcom and Practical Wireless from 1972 and thereabouts. Goodness knows why
I kept them but they've got to go!
Free but transport needs paying for....

Dave G3YXM, Birmingham.

dave@wireless.org.uk




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>
Organization: University of Hertfordshire
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Date: Fri, 23 Mar 2001 16:07:48 +0000
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Subject: LF: <Tech> BPSK Modulation Variants
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Dear LF group,

ON7YD's comment that BPSK "gives away" 3dB is only true for the 
limiting case of phase-keying data input consisting of alternating 1s 
and 0s, and therefore a phase transition for every bit. For real 
data, I reckon there is on average around 1 transition for every 2 
bits, so the "loss" in mean TX power is more like 1.3dB. I suppose 
the real question is if this "missing" power were present, would it 
do anything useful at the RX end? This would depend on the type 
of modulation and demodulation used.

As far as continuously varying phase modulation goes, my 
undergraduate text book makes the point that phase modulation is 
essentially equivalent to frequency modulation. Saying that the 
phase of a signal is varying relative to some reference phase is 
the same thing as saying the instantaneous frequency is different 
from the carrier frequency, since instantaneous frequency is the 
time derrivative of phase. What Rik is proposing is a kind of FSK - 
varying the phase linearly with time is the same as shifting the 
frequency. In the limiting case, with a 101010... bit sequence at 
10bits per second being a 5Hz square wave, for the phase to 
change by +/-180degrees (pi radians) within  a 1/10 second 
period, the frequency shift would need to be at least +/-10pi 
radians/sec, or  +/-5Hz. I have not tried to analyse this in the 
frequency domain, but it must have a spectrum with sidebands at 
5Hz intervals with a sinx/x component, not unlike that of the original 
un-shaped BPSK, but probably smaller.

With Andy's proposed scheme, in the 101010.. limiting case, and 
with the raised-cosine phase modulating slope, this would be 
equivalent to phase modulating with a 5Hz sine wave to a deviation 
of +/-pi/2 radians, mf = pi/2. Inspecting the functions of FM and PM 
modulated waves, this would be equivalent to FM with a modulating 
frequency of 5Hz (and without the DC offset), and deviation of 
7.8Hz. Looking at the Bessel function tables for mf = 1.5, this 
means the sidebands at +/- 5Hz would be up 0.7dB on the carrier, 
those at +/- 10Hz  -6.9, at +/- 15Hz -18.5dB and so on.

For the 10101010... limiting case, and ideal sine - envelope 
shaping, the BPSK signal is equivalent to a double sideband, 
supressed carrier signal modulated with a 5Hz sine wave, with two 
sidebands at +/- 5Hz only (see the article on PSK31 in the LF 
handbook). I checked this when I was building my modulator, and it 
was pretty close to what I actually got.  

I realise that these are rather crude analyses of the 3 types of 
modulation, and because the modulation is not in reality a uniform 
101010.. string of data, other spectrum components will also be 
present, and the spectrum will be continuous rather than discrete 
sidebands.  Also , the relative phase of the spectrum components 
is not considered. However, the other 2 methods seem to be a) 
different from the "ideal" BPSK, and b)apparently have more 
sidebands. Perhaps someone could provide a more accurate 
analysis, that would show whether either of these methods would 
be as effective for communications, would produce a satisfactory 
spectrum, or would require a different approach to demodulation.

Cheers, Jim Moritz
73 de M0BMU





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Date: Fri, 23 Mar 2001 15:10:53
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: LF: QRS beta version (external timing)
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Hello group,

Recently there have been some requests to be able to let an external (and
accurate) timing source control the PC clock while running QRS.
I had a look at it and a basic 'external time control' was rather easy to
implement.
In version 3.06 beta 1 it is possible to connect a accurate timing source
to  COM port CTS pin (on a D9 connector : pin 8, on a D25 : pin 5). At this
moment it must be a 1 minute clock source (maybe more posibilies later).

You can download this version from : 
http://www.qsl.net/on7yd/QRS/qrs306b1.zip

In SETUP you can click on TIME to get to the external clock menue. There
you have 3 possibilies :
- DISABLE : no external clocking
- ABSOLUTE : the PC clock will increment 1 minute for every pulse at CTS
(compared to time at the previous pulse).
- ADJUSTING : a pulse at CTS will adjust the PC clock to the closest minute

May sound complicated, therefore an example :

1. Before starting QRS you have to set the PC clock as accurate as you can
(by hand using the default windows device for setting the clock or using
software that sets the PC clock based on DCF77 or similar).

2A. If you select ABSOLUTE then QRS will take a 'reference time' at the
first pulse on CTS and from then on will increase time by 1 minute for
every pulse. In the time between the pulses the PC clock will run at its
own pace.
eg. Assume 14:25:36 is taken as reference time. At the next CTS pulse the
clock will be set to 14:26:36, then to 14:27:36 etc ...

2B. If you select ADJUSTING then QRS will also take a 'reference time' at
the first CTS pulse but from then on will only adjust the clock on every
CTS pulse.
eg. Assume 14:25:36 is taken as reference time. At the next CTS pulse QRS
reads the PC clock, let's say 14:26:35 -> this will be adjusted to 14:26:36.

The difference between the 2 options is that if (for whatever reason) there
is a CTS pulse missed that in the ABSOLUTE mode the PC clock will be 1
minute wrong while in the ADJUSTING mode the clock will be set correct as
long as the in the time between 2 CTS pulses it hasn't gone wrong more than
30 seconds in its own pace. 

One could use an atomic clock or GPS to generate the 60 second timing, but
for the mere mortals a simple Xtal oscillator + divider train will do (keep
the error less than a second over a period of several days).
Keep in mind that the pulses must exactly come in a 60 second interval, but
that there is no need that the pulse comes just on a full minute.
Finaly : the pulse applied to CTS must be positive and have a width between
10us and 10ms.

If there is sufficient feedback I am willing to continue and make more
flexible external timing possibilies.

73, Rik  ON7YD






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: RE: WOLF (BPSK) modulation continuous phase modulation.
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At 09:52 23/03/01 -0000, you wrote:
>Other tasks got in the way so never perused this much further, but the major 
>task putting me off was to work out a way of continuously phase modulating a 
>transmitter over a full 360 degree range.   This looked at first sight even 
>more difficult than amplitude modulating -  had already made a PWM modulator,
>although not big enough for the Decca transmitters, published in the lastest
>LF Experimenters book.

Hello Andy & group,

What I had in mind was a kind of digital 'smooth' phase-shifting.
The 'rude' way to perform BPSK is just to send the RF (square wave) through
an XOR gate, what will cause an instant 180 degrees phase shift.
Let us (for simplicity) assume that we would modulate BPSK on 100kHz square
wave. Further assume that the phase shift occurs exactly on the rising edge
of the 100kHz signal. 
If there is no phase shift we have a nice 100kHz square wave (5us high /
5us low). At the moment of a phase shift you will have 1 cycle with 10us
high and 5us low, we have an 'extra' 5us high level (or otherwise seen :
the frequency is down to 66.7kHz for 1 cycle = 15us). A 180 degrees phase
jump (at 100kHz) could be seen as a 5us 'time jump'.
If we want a more smooth phase transition we can spread this 5u 'time jump'
over several cycles, instead of a single 15us cycle we could have 5 cycles
of each 11us (otherwise seen : the frequency would be down to 90.9kHz for
55us).
If this is still too 'bumpy' we could have 50 cycles of 10.1us (frequency
down to 99.01kHz for 505us) or even 500 cycles of 10.01us (frequency down
to 99.9kHz for 5005us).
How smooth you can make the phase transition would depend on 2 things :
1. the transition time must be relatively short compared to the duration of
a bit (I believe that 5 to 10% of the time would be acceptable)
2. the smoother the transistion, the higher the reference frequency you need
To explain this last :
The 'base frequency' (in this example 100kHz) and the 'transition
frequency' (in this case 90.9kHz or 99.01kHz ... depending on how smooth
you want it to be) must be directly derived from the same source. So if you
take a rather fast transition (eg. the 5 cycles of 90.9kHz) you need a
source of 1MHz (divided by 10 = 100kHz, divided by 11 = 90.9kHz). But if
you want a slow transition (eg. 500 cycles of 99.9kHz) you will need a
source of 100MHz (divided by 1000 = 100kHz, divided by 1001 = 99.9kHz).
I believe that the 2. limitation will be more stringent.

Now back to 137.5kHz : A stable signal source (PLL or DDS) to to 40 or
50MHz is rather easy to make. This would give us a practical ratio of 256
(35.2MHz source for a 137.5kHz 'base frequency' and a 2 millisecond
transition time.

I am aware that this method will require substancial hardware, but it will
be at the 'low power' end (reducing the firework) and once you have it, it
can be used with any PA. And maybe there are more intelligent methods to
achieve this smooth phase shifting, I wonder if we cannot put most of it
into a PIC or similar ?

73, Rik  ON7YD



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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: WOLF - Transmit
Date: Fri, 23 Mar 2001 11:56:21 -0000
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 Where is the array   pnpat[]  used ?  It is declared at the end of the
listing you sent, but not referenced anywhere else.
Not being a C programmer, it will take a bit ot time to translate the
code  ;-|
 Andy  G4JNT
 
 
 > -----Original Message-----
 > From: Stewart Nelson [mailto:sn@scgroup.com]
 > Sent: 2001-03-22 17:24
 > To: rsgb_lf_group@blacksheep.org
 > Subject: LF: Re: RE: Re: WOLF - Transmit?
 > 
 > 
 > Hi Andy and all,
 > 
 > Sorry that I don't have a good document on the format, but
 > here is the code used to generate it; I hope that it is
 > enough info for you to build something compatible with WOLF.
 > > 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Litz wire
Date: Fri, 23 Mar 2001 09:40:05 +0100
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<HTML><HEAD>
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<DIV><STRONG>To All from PA0SE</STRONG></DIV>
<DIV>&nbsp;</DIV>
<DIV><STRONG>Radio station Kootwijk in The Netherlands is being dismantled (that 
is were the "PA0SE aerial insulators" came from; I still have some). 
</STRONG></DIV>
<DIV><STRONG></STRONG>&nbsp;</DIV>
<DIV><STRONG>At the point of being scrapped now is a spool with about 188 metres 
silk covered litz wire with a diameter of about 8 or 9 
millimetres.</STRONG></DIV>
<DIV><STRONG>It came&nbsp;from a former LW transmitter on 1875 m.</STRONG></DIV>
<DIV><STRONG>The litz wire&nbsp;can be collected free but you have to organise 
transport to your place yourself.</STRONG></DIV>
<DIV>&nbsp;</DIV>
<DIV><STRONG>If you are interested please let me know as soon as possible 
because the Kootwijk station manager wants to get rid of it on very short 
notice.</STRONG></DIV>
<DIV>&nbsp;</DIV>
<DIV><STRONG>73, Dick, PA0SE</STRONG></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: WOLF (BPSK) modulation continuous ph	ase modulation.
Date: Fri, 23 Mar 2001 09:52:11 -0000
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I modelled this, generating ET2 Coherent waveforms with gradual phase
transitions and stored as .WAV files, then played back into the Coherent
decoder.  With a Raised Cosine phase transition slope and the ability to
adjust the amount of this from practically no slope to a full envelopes
worth of phase transition,  decoding results looked quite encouraging -
the bandwidth was reduced considerably and decoding of good signals
worked 100%.  Never got the opportunity to test in QRM apart from some
simple tests adding to off air received noise.   Other tasks got in the
way so never perused this much further, but the major task putting me
off was to work out a way of continuously phase modulating a transmitter
over a full 360 degree range.   This looked at first sight even more
difficult than amplitude modulating -  had already made a PWM modulator,
although not big enough for the Decca transmitters, published in the
lastest LF Experimenters book.

Andy  G4JNT

> -----Original Message-----
> From: Rik Strobbe [mailto:rik.strobbe@fys.kuleuven.ac.be]
> Sent: 2001-03-23 09:55
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: WOLF (BPSK) modulation
> 
> 
> Hello Mike & group,
> 
> With Mike's suggestion to cut the signal for a short time 
> during the phase
> tranisitions the cure might be worse than the illness :
> WOLF is (currently) used at 10BPS, so you would need to cut the signal
> (worst case) 10 times a second for a short time (few 
> milliseconds). This
> will create a lot of sidebands, the signal might be worse 
> than with 'rude
> BPSK'.
> 
> Jim's signal is remarkable clean, as could be expected from a PSK-like
> signal. The 2 'disadvantages' (in my opinion) are :
> - 'high power' electronics involved
> - giving away 3dB (by the envelope AM), versus 'rude BPSK'
> 
> An alternative way to get a 'clean' signal might be to have a 
> smooth phase
> transition. Instead of a 180 degrees instant phase jump one 
> could have a
> gradual phase change, let's say over 10 milliseconds. At 
> 10BPS this would
> leave the signal for 90% of the time in the 'correct phase'.
> Advantages would be :
> - additional electronics would be at the 'low power end'
> - any PA (wether linear or not) could be used without any changes
> - signals would be only 0.54dB down versus 'rude BPSK'
> 
> Depending on the amount of sidebands that is acceptable the transision
> period could be changed. A shorter transisition period would 
> give a better
> SNR, but more sidebands while a longer transistion period would give a
> cleaner signal but less SNR.
> 
> There would be different ways to implement the smooth phase 
> shifting, going
> from the classic phase modulator to digital techniques.
> 
> But before I start any project in that direction I would like 
> the opinion
> of the experts, maybe I have just overseen some facts that 
> make my whole
> suggestion worthless ...
> 
> 73, Rik  ON7YD
> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 23 Mar 2001 09:54:54
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: LF: WOLF (BPSK) modulation
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Hello Mike & group,

With Mike's suggestion to cut the signal for a short time during the phase
tranisitions the cure might be worse than the illness :
WOLF is (currently) used at 10BPS, so you would need to cut the signal
(worst case) 10 times a second for a short time (few milliseconds). This
will create a lot of sidebands, the signal might be worse than with 'rude
BPSK'.

Jim's signal is remarkable clean, as could be expected from a PSK-like
signal. The 2 'disadvantages' (in my opinion) are :
- 'high power' electronics involved
- giving away 3dB (by the envelope AM), versus 'rude BPSK'

An alternative way to get a 'clean' signal might be to have a smooth phase
transition. Instead of a 180 degrees instant phase jump one could have a
gradual phase change, let's say over 10 milliseconds. At 10BPS this would
leave the signal for 90% of the time in the 'correct phase'.
Advantages would be :
- additional electronics would be at the 'low power end'
- any PA (wether linear or not) could be used without any changes
- signals would be only 0.54dB down versus 'rude BPSK'

Depending on the amount of sidebands that is acceptable the transision
period could be changed. A shorter transisition period would give a better
SNR, but more sidebands while a longer transistion period would give a
cleaner signal but less SNR.

There would be different ways to implement the smooth phase shifting, going
from the classic phase modulator to digital techniques.

But before I start any project in that direction I would like the opinion
of the experts, maybe I have just overseen some facts that make my whole
suggestion worthless ...

73, Rik  ON7YD


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: <200103171435.f2HEZMq11665@smtp.wanadoo.nl>
Subject: LF: Re. Mad Hatters Tea Party
Date: Thu, 22 Mar 2001 23:49:30 -0000
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There was an exchange of e-mails between Ko and Laurie a few days ago.
> >Hi Ko.
> >Your pictures are indeed very busy, do you have un-invited guests at your
party?  I see a lot of Loran. 73s Laurie.
>
> Hi Laurie.
> I am not sure, but are the lines really there or are they created in the
L202 preamp i am trying?
> The L202 does not have a bandpass filter like the other one i use.
> Watched 01:00 this morning and the lines were even worse but none was
> transmitting inside of them, though the lines were very close.

I felt that the pictures on Ko's website were rather noisy and that they
could be improved. Most of the time there are no amateur signals in the band
so there should only be background noise and Loran sidebands in the
displays.
I have now included some pictures, which show what the 136kHz band looks
like from this QTH. Click on 'Receiving LF Signals' on the home page of the
site shown below. I feel that a bandpass filter would help a lot
particularly with the strong EU broadcast stations just up the band.

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: "C Andersson" <sm6pxj@swipnet.se>
To: "RSGB LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Auroral propagation
Date: Thu, 22 Mar 2001 20:48:28 +0100
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As already has been mentioned on this reflector I had a nice QSO with Ron G6RO on Monday evening.
Heard his CQ call  with "local" strength and could not resist to answer, even though I don't normally transmit during TV-time. I have some TVI on my own TV set and I'm not sure about my neighbour's. I'm suspicios that my TX signal is nicely distributed to the neighbours via the mains earth, which is a part of my earthing system.
There are 3 houses between me and the ground connection for the mains system.

>perhaps we were seeing an auroral path from SM.

Maybe. I have put together some information here:
http://home5.swipnet.se/~w-54761/aurora.htm

73
Christer
sm6pxj




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>
Organization: University of Hertfordshire
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Date: Thu, 22 Mar 2001 18:11:33 +0000
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Dear Brian, LF Group,

Many thanks to Brian for the report, glad to see you are getting 
some positive results from the test signals. I am a little puzzled by 
the 0.15Hz frequency offset; to get this much error in my TX 
frequency would require an actual fault in the synthesiser. In 
addition, my frequency counter would have to be reading wrong 
too. These things are not very likely, but not impossible, so I will 
check. I don't know if this could be some sort of artefact of the 
decoding process -I did get peculiar frequency readings when the 
signal level was too high.

If you run Wolf without the -l option, and the timing is all correct, 
the value in the pm: column will increase from one row of results to 
the next.

I will take a break from sending the beacon sigs tonight, to catch up 
on a bit of sleep. I will start again on Friday night. No doubt this will 
be the cue for superb transatlantic propagation conditions, lasting 
one night only.

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Stewart Nelson" <sn@scgroup.com>
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References: <65AECDF1F89AD411900400508BFC869F9C03F4@pdw-mail-1.dera.gov.uk>
Subject: LF: Re: RE: Re: WOLF - Transmit?
Date: Thu, 22 Mar 2001 09:23:41 -0800
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Hi Andy and all,

Sorry that I don't have a good document on the format, but
here is the code used to generate it; I hope that it is
enough info for you to build something compatible with WOLF.

You can run WOLF in the "EEPROM" mode to see if a given
message encoding matches your software.  If you have trouble,
let me know and I'll try to help.

Transmission involves radix-40 encode, convolutional encode,
interleave, and reference bit insertion.

#define MSGLEN 15  /* source message len in chars */
#define MSGLENW 5  /* radix 40 message len in 16-bit words */
#define WLEN 16   /* bits in 3-character coded group */
#define MSGLENB 80  /* message length in bits */
#define RRATE 6   /* reciprocal of code rate */

/* Radix-40 encoder */
/* Future versions may use codes >=64000 for
   control functions, CRC, etc. */
/* in: ASCII string, up to 15 chars
   out: array of 16 bit words, radix-40 encoded */
void encr40(char *in, ushort out[])
{
  int ch, fill, val, i;
  fill = 0;
  val = 0;
  for (i = 0; i < MSGLEN; ++i) {
    if (fill)
      ch = 0;
    else if (!(ch = *in++))
      fill = 1;
    else if (ch >= 'A' && ch <= 'Z')
      ch = ch - 'A' + 1;
    else if (ch >= 'a' && ch <= 'z')
      ch = ch - 'a' + 1;
    else if (ch >= '0' && ch <= '9')
      ch = ch - '0' + 27;
    else if (ch == ' ')
      ch = 0;
    else if (ch == '.')
      ch = 37;
    else if (ch == '/')
      ch = 38;
    else
      ch = 39;
    val = val * 40 + ch;
    if (i % 3 == 2) {
      *out++ = val;
      val = 0;
    }
  }
}

/* These values are bit-reversed from those in the NASA paper
   because the register shifts left */

int cnvcod[] = {042631, 047245, 073363, 056507, 077267, 064537};

/* tail-biting encoder
   in: array of radix-40 encoded 16 bit words
   out: baseband signal in xmit order, array of chars */
void enccnv(ushort in[], char out[])
{
  int sr, i, j, k, b, t;
  sr = in[MSGLENW-1];  /* init sr to last 15 bits */
  for (i = 0; i < MSGLENW; ++i) {
    for (j = 0; j < WLEN; ++j) {
      sr = (sr << 1) | (in[i] >> (15-j)) & 1;
      for (k = 0; k < RRATE; ++k) {
        b = 0;
        for (t = sr & cnvcod[k]; t; t &= t-1)
          b ^= 1;
        /* store */
#if INTLV
        out[k*MSGLENB + (j&7)*10 + ((j&8)>>3) + i*2] = b;
#else
        out[k*MSGLENB + j + i*WLEN] = b;
#endif
      }
    }
  }
}

char pnpat[] = {
0,0,1,1,1,1,1,0,1,0,1,0,1,1,0,0,0,0,1,1,0,1,0,1,1,0,0,1,0,1,0,0,1,0,0,0,1,0,0,1,
1,0,1,0,0,0,0,0,1,1,1,0,1,0,1,0,1,1,1,0,0,0,1,0,1,1,0,0,0,1,0,1,1,1,1,0,1,0,1,1,
1,1,0,0,1,0,0,0,1,0,0,1,1,1,0,1,0,1,0,0,0,1,0,1,1,0,0,0,1,0,1,0,1,1,0,1,1,0,1,0,
1,0,1,1,0,0,0,0,0,1,0,1,1,0,1,1,0,1,0,0,0,1,0,1,1,1,0,0,0,1,1,1,1,0,1,1,1,0,0,1,
1,0,1,1,0,1,0,0,1,1,1,0,1,0,0,1,1,0,1,0,1,0,0,1,0,0,0,1,1,1,0,1,0,0,1,0,0,0,1,1,
0,0,1,0,1,0,1,1,1,1,0,1,0,1,0,0,0,0,0,0,0,0,0,0,1,0,1,1,1,1,1,1,0,1,1,0,0,1,1,1,
1,1,0,1,0,0,1,0,1,0,1,0,1,1,0,1,0,0,1,0,1,0,0,0,1,0,1,0,1,1,0,0,0,0,0,0,0,0,0,0,
1,1,1,1,1,1,0,1,0,1,1,0,0,1,0,0,1,1,0,1,0,1,1,0,1,1,1,0,0,1,0,1,0,1,0,1,1,1,1,0,
1,1,0,0,1,0,0,0,0,0,0,1,1,1,1,1,0,0,1,1,0,0,0,1,1,1,1,1,0,1,0,0,0,0,0,0,1,0,0,1,
0,1,0,0,0,1,1,0,0,1,0,1,0,1,0,0,1,1,0,1,1,1,0,0,1,1,1,0,0,1,1,1,1,1,0,1,1,0,1,0,
1,0,0,1,1,1,0,0,0,0,0,1,0,0,1,0,1,0,0,0,0,1,1,0,0,0,0,1,1,0,1,0,1,1,1,0,1,0,1,1,
1,0,0,0,1,1,1,1,1,0,0,0,1,1,0,1,0,0,1,1,1,1,1,1,0,1,0,0,1,0,0,1,0,1,0,0,0,1,1,1,
};

Notes:  The interleave function is far from optimum but a lot better than
nothing.  The PN pattern was chosen literally at random, selecting for low
autocorrelation and for low autocorrelation with short substrings, but is
also far from optimum.  I would greatly appreciate it if you find a good
replacement pattern.

Hope this is useful.

73,

Stewart KK7KA


----- Original Message -----
From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Thursday, March 22, 2001 7:02 AM
Subject: LF: RE: Re: WOLF - Transmit?


> I would like add Wolf coding to my PIC based BPSK generator.
> Stuart, can you reveal the exact coding details, I can't find them in
> any of the documentation on the Web.   Just a comment that the mesage
> data is interleaved (?) with a PN Sequence to assist clock recovery and
> timing.
>
> Andy  G4JNT




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>
Organization: University of Hertfordshire
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Subject: LF: <Tech>WOLF Transmit
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Dear Mike, LF Group,

Mine is certainly not the only way of generating a BPSK signal, and 
it is certainly true from experience that little trouble results from key 
clicks on 136k, in spite of the fact that a lot of TXs on the band 
have less than ideal keying. But in my own position, being in an 
area relatively densely populated with LF stations, having a high 
ERP compared to most, and transmitting beacon signals over 
extended periods means I feel obliged to try and produce as clean 
a signal as possible.

Actually, key clicks are never likely to be a huge issue on LF; when 
compared to HF standards, even a full 1W ERP is a sub-QRP 
signal, and the higher noise level will tend to swamp clicks from all 
but the most local stations anyway.

Both "WOLF" and (usually) "Coherent" BPSK use a 10 bits/second 
rate; so the number of phase transitions per second will be similar 
to the number of on-off transitions of a 12wpm CW signal. Cutting 
the drive before a phase transition would eliminate the click due to 
the phase change, but would add 2 more, when the drive was 
switched off and then back on again, so little would be gained.

Having "redundant" envelope modulation when no phase transition 
occurs would actually increase the sideband levels - the 
explanation I gave was something of an over-simplification. It 
would still be neccessary to synchronise the amplitude modulation 
with the phase modulation somehow, so little saving in complexity 
would be acheived.

A perfectly good way of generating BPSK would be to first low-
pass filter the logic level signal, and then mix it with the carrier in a 
linear balanced mixer (rather than an ex-or gate). A linear PA would 
be required. This would be a good option if you do have a linear, 
but do not have an SSB exciter that will give output on 136k.

To put the complexity into perspective, my prototype modulator is 
built on 2 100 x 160mm prototyping boards, plus a heatsink 
assembly carrying the MOSFETs. Implementing the waveform 
generator part on a PIC - type microcontroller would roughly halve 
the number of components and interconnections. If a PCB were 
designed, the small-signal parts of the circuit would be no more 
difficult to build than, say, a fairly elaborate audio filter kit. The 
MOSFET pass element obviously needs to be quite big to handle 
the power. The Heatsink assembly could be simplified by using a 
really big MOSFET power module instead of 8 small ones, but I 
doubt if this would be cost-effective. 

cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Re: WOLF - Transmit?
Date: Thu, 22 Mar 2001 15:02:19 -0000
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I would like add Wolf coding to my PIC based BPSK generator.   
Stuart, can you reveal the exact coding details, I can't find them in
any of the documentation on the Web.   Just a comment that the mesage
data is interleaved (?) with a PN Sequence to assist clock recovery and
timing.

Andy  G4JNT



> -----Original Message-----
> From: Stewart Nelson [mailto:sn@scgroup.com]
> Sent: 2001-03-22 07:51
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: WOLF - Transmit?
> 
> 
> Hi Mike and all,
> 
> Bill de Carle VE2IQ has added WOLF mode to his KEYER package.
> Can upload to keyer or provide data for an EPROM, etc.
> Download from Bill's web page at
> http://cafe.rapidus.net/bill1/bbs.htm .
> 
> 73,> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 22 Mar 2001 14:21:17 +0000
To: rsgb_lf_group@blacksheep.org
From: "Brian Rogerson" <brian@esoterica.pt>
Subject: LF: Wolf at the door or I am still missing something
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Gentlemen,

After careful calibration of the sampling rate using HP
signal generator and WWV on 5MHz AM which gave the
same value, also checking the stability and absolute frequency
accuracy of the receiver using 60 and 198KHz with 800Hz
offset, (the calibration files are available), nothing but
gibberish was seen on trial wolf decodes.

Eventually as a last deperate effort I copied the first part of
the high power transmission after 2400 yesterday into the
wolf directory and using the verbose mode I found I still had
to change the -f parameter.  Below is the result.

C:\Wolf>wolf -q wolfr5a.wav -f 800.146 -t .2 -r 8018.543 -l
WOLF version 0.52
t:  24 f: 0.001 a:-1.2 dp: 79.9 ci: 9 cj: 44 CQ M0BMU M0BMU  -
t:  48 f: 0.012 a: 1.2 dp: 85.7 ci:13 cj: 62 80B97/C1HQS7XEL ?
t:  96 f: 0.181 a: 1.3 dp: 87.4 ci: 8 cj: 33 R26WLGILX*MUWQ9 -
t: 192 f: 0.000 pm:  91 jm:872               CQ M0BMU M0BMU  -
t: 288 f: 0.000 pm: 128 jm:872               CQ M0BMU M0BMU  -
t: 384 f: 0.000 pm: 123 jm:872               CQ M0BMU M0BMU  -
t: 480 f: 0.000 pm: 135 jm:872               CQ M0BMU M0BMU  -
t: 576 f: 0.000 pm: 126 jm:872               CQ M0BMU M0BMU  -
t: 672 f: 0.000 pm: 130 jm:872               CQ M0BMU M0BMU  -
t: 768 f: 0.000 pm: 138 jm:872               CQ M0BMU M0BMU  -
t: 864 f: 0.000 pm: 158 jm:872               CQ M0BMU M0BMU  -
t: 960 f: 0.000 pm: 146 jm:872               CQ M0BMU M0BMU  -
t:1056 f: 0.000 pm: 177 jm:872               CQ M0BMU M0BMU  -
t:1152 f: 0.000 pm: 150 jm:872               CQ M0BMU M0BMU  -
t:1248 f: 0.000 pm: 134 jm:872               CQ M0BMU M0BMU  -
t:1344 f: 0.000 pm: 158 jm:872               CQ M0BMU M0BMU  -
t:1440 f: 0.000 pm: 126 jm:872               CQ M0BMU M0BMU  -
t:1536 f: 0.010 pm:  27 jm:872               CQ M0BMU M0BMU  -
t:1632 f: 0.000 pm: 160 jm:872               CQ M0BMU M0BMU  -

But there is still something missing.  My intuition alarm bells are
jangling.  How this could have crossed the Atlantic site unseen is
totally beyond me.   I have also broken the law.

Thank you to Jim, and to all the programme writers who have made
this possible.

73, Brian
73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
http://homepage.esoterica.pt/~brian



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Subject: LF: WOLF - transmit
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Thanks, Jim, for the useful description of your transmit system for WOLF.

Being a very lazy constructor, I am trying to find a simpler solution.

Am I right in saying that my Decca Tx does not cause you a problem when I 
key it with normal CW? If that is the case - I certainly don't get any clicks 
from you - and bearing in mind that I key the 'VFO' output, why not simply cut 
the drive during the critical transition period?

Alternatively, why go to the trouble of only reducing the PSU volts only when 
there is a transition? Why not reduce it every time there =could= be a 
transition, ie once every second (I think I am right in saying the bit rate is one 
bps?). This would mean that the whole thing could be driven by an oscillator. 
Of course it would need to be synched to the keyer, but isn't that easier than 
what you are using?

And what about using a linear amplifier, eg BK Electronics, and simply putting 
an LPF on the output of the XOR gate modulator used by the Lowfers? This 
would be a really easy answer, at least up to a few hundred watts, wouldn't it?

I mean no criticism of your circuitry - it's just that I don't fancy building 
something that complex. Have I missed something terribly important?

I remain fascinated but still rather baffled, and would appreciate your 
thoughts, and those of anyone else.

Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Stewart Nelson" <sn@scgroup.com>
To: rsgb_lf_group@blacksheep.org
References: <3AB89EE8.130.AB12B1@localhost>
Subject: LF: Re: WOLF - Transmit?
Date: Wed, 21 Mar 2001 23:50:35 -0800
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Hi Mike and all,

Bill de Carle VE2IQ has added WOLF mode to his KEYER package.
Can upload to keyer or provide data for an EPROM, etc.
Download from Bill's web page at
http://cafe.rapidus.net/bill1/bbs.htm .

73,

Stewart KK7KA

----- Original Message -----
From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Wednesday, March 21, 2001 4:30 AM
Subject: LF: WOLF - Transmit?


> Ok, so having cracked the receive side, how do I transmit WOLF?
>
> As I understand it there are three methods:
>
> 1 - Audio from the soundcard is fed into a 136kHz SSB transmitter, including
> of course an HF SSB Tx with a transverter. Presumably the transmission is
> independent of which sideband is selected.
>
> 2 - Audio from the soundcard can be combined with the 'VFO' in an XOR gate
> and fed into an amplifier - presumably linear. This looks useful to me as I
have
> a 200W linear amp.
>
> 3 - The M0BMU method that allows the use of a non-linear Class D Tx. How
> and why does this work?
>
> All three methods are potentially simple, but are made complex by the need for
> very careful bandwidth tailoring to keep the transmission to about 20Hz wide.
>
> Have I got any of this wrong? Is there anything published on the subject?
> What is in use?
>
> I understand that some Lowfers have used WOLF, but I suspect that
> bandwidth has not been an issue because of the total width of the allocation
> and the low ERP. I believe that Larry, VA3LK, has transmitted WOLF, but
> again perhaps the bandwidth was not a problem. Jim, will you publish your
> circuits? Or perhaps they are rig specific?
>
> It appears relatively easy to get going on receive but practical transmit has
an
> information black hole.
>
> Advice, please.
>
>
>
> Mike, G3XDV (IO91VT)
> http://www.lf.thersgb.net
>
>



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: <5186.200103191301@gemini>
Subject: LF: Sound card sample rate cal for WOLF
Date: Wed, 21 Mar 2001 17:05:55 -0500
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In a quick experiment this morning, I recorded 15 minutes of LORAN-C with my
receiver in AM mode. The recording was done with my normal WOLF setup, 8000
Hz sampling, 16 bit. My "local" LORAN-C station has a 9960 microsecond
repetition rate, which is 100.4016 Hz. I then set WOLF to measure the 8th
harmonic of that rate, as follows:
wolf -f 803.21285 -q (filename.wav) -m 60

WOLF then nicely gave me a list of frequency offsets measured every 60
seconds. In my case, the offset was -0.197 Hz, which yielded 8001.96 Hz for
the sampling rate. This agrees very closely with measurements made with an
accurate 1 kHz tone. The calculation has been described earlier on this
list:
8000(803.21285 / (803.21285 - 0.197)) = 8001.96

This method relieves the need for an accurate tone source. It also uses your
normal WOLF recording and crunching software and sampling rate. You do need
to know a repetition rate for a LORAN-C signal in your receiver's output.

John Andrews, W1TAG



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
Subject: LF: Re. LF Tests
Date: Wed, 21 Mar 2001 21:11:29 -0000
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<DIV><FONT face=Arial size=2>Hi John,</FONT></DIV>
<DIV><FONT face=Arial size=2>Yes I was on last night but NASA said that there 
was a geomagnetic storm on monday and that a CME is expected on 22/23 March. So 
I guess conditions will be very disturbed for a while. I will transmit again 
tonight from about 2230utc and will revert to&nbsp;30sec dots to see if this 
helps. 73s Laurie.&nbsp;</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi all , I had bad 60 Hz noise. early on .  I thought G3AQC was visible
at 2130Z.  Noise cleared up aruond 0330 but never saw any  signals .
Laurie ,  were you transmitting? I will look again tonight.
   73 de John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: exact audio reference
Date: Thu, 22 Mar 2001 07:55:12 +1200
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Rik and other readers,

> For those who want to calibrate the soundcard there is also a simple
> hardware solution :
> Take a CMOS4060 (14-stage divider with internal oscillator) and let it run
> with a xtal in the 8-12MHz range. At the end of the divider chain (pin 3)
> you will get the xtal frequency divided by 16384 (will be in the 500-700Hz
> range).

I have had such an accessory for a few years, delivering an output of 1000
Hz.  The squarewave output has much harmonic content, but it can be
filtered.  I also have a distortion measuring instrument that shows that
most audio oscillators have "rude" harmonic content, but my home brew unit
with suitable filtering gives about 70 dB of purity to the 1000 Hz
fundamental.  So it is very good for both frequency accuracy, and purity.

The 1000 Hz tone, to millihertz accuracy, is very handy for checking the
dial accuracy of amateur transceivers, in SSB mode.  With a frequency
counter on the output, the sideband should be either +1000 Hz for USB,
or -1000 Hz for LSB, and any error is in the transceiver RF department.
1000 Hz is the best frequency for least mental arithmetic by the operator
;o)

I have more recently made considerable use of the accessory for calibrating
PC sound cards.

72, Bob ZL2CA



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>
Organization: University of Hertfordshire
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Dear LF group, 

Will run some more WOLF signals tonight at the 30mW ERP level 
on 137.5000kHz, starting around 2000utc. Also will be running 1W 
ERP around 0000 onwards. 

Cheers, Jim Moritz
73 de M0BMU


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From: "jannsen" <0482183881-0001@t-online.de>
To: rsgb_lf_group@blacksheep.org
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Subject: Re: LF: Wolf Tests
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James Moritz schrieb:

>
> The obvious problem is how to determine the soundcard error, if 
> you don't have a accurate audio frequency source. I used the 
> reference output of my synthesiser divided doown to 1kHz (and 
> filtered; a fairly clean sine wave seemed to be neccessary to avoid 
> aliasing problems with the soundcard). You could use the RX audio 
> out, but only if you knew what the RX frequency error was to within 
> a small fraction of a Hz. 

> Cheers, Jim Moritz
> 73 de M0BMU

Hi Jim and all,
audio qrg source out of ur old PC does it too. take Rik`s QRS-progr, switch 
setup/sound/dfcw/enable/fill in the qrg u want in both dash- and dot-window the 
same qrg. 
hardware: take the speaker output (kill the speaker as Rik suggested), form the 
needle-waves into sinus-waves (I took out of my junk-box a pot-core 330mH, 
1,8mikroF and 100nF for c1 and c2 of a Pi-Filter for transforming 10ohm to abt 
6kohm)and measure the qrg. Taking 1000Hz  out of my junk-pc (486/66Mhz with the 
motherboard crystal tempcompensated)in the above described manner the counter 
shows 1000.0706Hz to 1000.1804Hz  constance over 4 hours.
regards
Uwe/dj8wx



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Subject: Re: LF: DFCW
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DL4YHF@aol.com schrieb:

> I once implemented such "time marker lines" in Spectrum Lab (configurable 
> from 1 sec per line to several minutes) but that feature seems to be hidden 
> too deep in the configuration dialog hi. 
.................
> 73's Wolf.

Hi Wolf,
the Spectrum Lab here has the time marker lines once and for all
switched on, 
hi.
rgds
Uwe/dj8wx 



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BOB RIESE schrieb:
> What the heck is a mudball/
>  John VE1ZJ
>
>
> That would be the 3rd rock 
> from the sun
>
> Bob  
There are mudbloods es muggles on that rock (harry potter)
Uwe/dj8wx



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From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
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Subject: LF: <TECH>BPSK Modulator details
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<?color><?param 0100,0100,0100>Dear Mike, LF group,<br><br>I am in the process of putting together some info about my BPSK  modulator for the Decca class D PA - it will take a little time to  collate all the details from my meticulously cross-referenced  notebook (ahem..), but here is some general information about the  method I am using.<br><br>The BPSK signal can be generated by exclusive-ORing an  AF or  RF carrier with the binary keying data. this produces an output  whose phase is unchanged when the data value is zero, but shifted  by 180 degrees (ie. inverted) when the data is 1. This signal can  be amplified by any linear or non-linear amplifier, and is a perfectly  OK signal as far as demodulating goes, but it also generates  sidebands analogous to key-clicks from a CW TX. In fact, for the  same transmit PEP, the clicks generated by BPSK will be 6dB  stronger than an on-off CW signal. So obviously, if you are trying  to generate 1W ERP it isn't really on, although you
 can get away  with it for a QRP transmitter.<br><br>The remedy is similar to that used for CW: the output is gently  reduced to zero before the phase change occurs, then gently  increased to it's full value again after, in other words amplitude  modulation is applied to the BPSK signal, as well as phase  modulation. It turns out the ideal amplitude envelope is like a full- wave rectified sine wave - see the description of PSK31 in the LF  handbook, which is basically the same.<br><br>There are two main ways of generating this signal in practice -  the  most popular is to synthesise the waveform directly using a DSP  algorithm and a digital to analogue converter, eg. soundcard plus  software. However, most DSP DACs are limited to audio frequency  outputs, so the signal must be mixed up to RF, and also amplified in  a linear PA so the modulation envelope does not get distorted.  However, If you have an HF rig with LF output, and a QRO linear  PA, this is the easiest route to a
 BPSK capability.<br><br>I didn't have, so... <br><br>The other method is to apply the phase modulated signal direct to  the PA, and simultaneously amplitude modulate the PA to get the  required envelope. A class D PA is well suited to this due to the  linear relation between supply voltage and RF output amplitude -  what is required is to replace the normal DC supply with the full- wave rectified sine waveform which follows the phase transitions.<br><br>The advantages of this are:<br>-Efficiency can be relatively high compared to a linear<br>-No frequency conversion means few spurious outputs, and  minimal frequency errors.<br>-Simplified digital system required.<br><br>In my present system, the 136kHz carrier is generated by a  synthesiser, and phase keyed using a simple ex-or gate. The  envelope modulating waveform is generated from the phase keying  signal. <?/color>The envelope-shaping part is built using 4000 series logic  and some analogue bits. It is a prime candidate
 for implementation  using a PIC with a D/A, but I haven't got a programmer, hence the  hard wired circuit. It is synchronously clocked at 256 x the bit rate  by a 555 timer. The incoming phase signal is appied to a transition  detector. When a transition occurs, an 8-bit counter is reset, which  clocks through all it's states and then stops. The 4 MSBs are used  as the addresses for a 16 input analogue MUX. The MUX inputs  are connected to taps on a sine weighted potential divider fed with  a DC reference voltage, producing a stepped approximation to the  modulation envelope, which is low pass filtered to smooth it out.  This then goes to the power stage of the modulator. The "middle"  count of the counter is decoded and used to clock the phase data  through a D flip-flop to get a delayed phase output, which is what is  actually fed into the ex-or phase modulator, to keep it in step with  the modulation envelope. The reference voltage can also be keyed  through another LPF t
o get a nice textbook CW keying waveform.<br><br>The high power modulator part is physically the biggest bit. <?color><?param 0100,0100,0100><?bigger><br><?/color><?smaller>I started off wanting to build a PWM modulator, but it ended up <br>being linear - this sounds like a thoroughly bad idea, massive  heatsinks and so on, but the power dissipation did not turn out as  bad as you might think. It evolved like this:<br><br>With a PWM, the output tends to be quite spiky due to non - ideal <br>filter components, and the amount of filtering you can apply is  limited - very big filter capacitors limit the slew rate of the output in  the troughs of the modulation, multi-section filters introduce other  problems, especially if you want to use feedback to improve  regulation, reduce mains ripple etc. The spikes will produce IM  products in the PA  output, which Murphy's law dictates will be at  the right frequency to cause maximum trouble. One way round this  would be to clock the PW
M at the carrier frequency (or better, 2x),   but then you end up with something quite big and complex due to  the high frequency, with higher switching losses to boot, which  defeats the object. <br><br>So I looked again at using a linear circuit. If you keep the input-<br>output voltage differential to a minimum while transmitting a  continuous carrier, the power dissipation is minimised. Since you  don't really need a perfectly constant output provided it is  reasonably ripple free and so on, the modulator output can be  made to track variations of the input voltage, and maintain a  roughly constant, small, differential.  I did this by using a filtered  sample of the raw input DC as the reference voltage for the  envelope waveform circuit described above.<br><br>When sending CW at full power, the output to the Decca PA is 60V  max, 21.4A, and the differential 5V. Power dissipation is 107W.  During the phase transitions of BPSK, power dissipation is higher,  but in fact wit
h a sinusoidal envelope, average dissipation works  out to 243W for phase transitions on every bit, or 175W for a  phase transition every two bits, which I reckon is about average.  The power dissipated is therefore similar to a 300 - 400W linear,  which is quite managable. I think the overall TX efficiency DC input - &gt; TX out is near 75 - 80% still, so not too bad. With a PWM  modulator, there would still be some dissipation and you would be  lucky to get 90% overall efficiency, so overall there is not a huge  difference between the two approaches - less than 1dB in signal  terms. The pass element uses 8 x STW34NB20 Mosfets, which is  a bit oversized, but was done in case I felt like increasing output in  the future. 5 or 6 would do. The linear design makes it very easy to  include foldback current limiting and so on. Each MOSFET is driven  by a seperate op-amp to ensure even current sharing, and  individual current limiting for each device. Overall, the circuit  maintain
s a fraction of the output voltage equal to the  instantaneous amplitude of modulation waveform - in other words,  it is a big feedback amplifier. This also serves the function of  removing mains ripple from the PA supply<br><br>The phase keying signal can be any logic level signal - for  "Coherent", it uses the signal on one pin on the PC RS232 port  provided for the purpose. For WOLF, I built a dedicated EPROM  keyer, very similar to the Lowfer designs. This enables me to use  the reference output of the synthesiser, divided down to 10Hz, to  provide very accurate timing for the BPSK signal. The synthesiser  uses a Racal 9442 OCXO reference, stable to within 1 part in  10^7, which it seems to manage easily. So you just dial in the  frequency, and  there is no messing around with frequency  calibration for soundcards, HF rigs etc., thank goodness!<br><br>The complete system is fully working with CW, QRSS and BPSK,  but not yet finished. It is compatible with existing softwar
e for these  modes. It should be flexible enough to use with other modulation  methods, should these look promising. I think the results so far  show that superior results can be acheived compared to a  soundcard/SSB exciter/linear PA TX, althought there is obviously a  lot more work involved. The same techniques could be applied to  any class D TX. One thing I will do when I get the chance and the  bits is to replace the current PSU with a variac/transformer/rectifier  arrangement. I will get some legible circuit diagrams together when  I get time; I am a bit pressed at the moment.<br><br>Cheers, Jim Moritz<br>73 de M0BMU<br><br><br><br>

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From: "Gasparik Richard" <Richard.Gasparik@sbs.sk>
To: "Rsgb_Lf_Group \(E-mail\)" <rsgb_lf_group@blacksheep.org>
Subject: LF: DL/OM2TW QRV...
Date: Wed, 21 Mar 2001 18:40:37 +0100
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Hi LF-ers...

	I have a trip to the CeBit in Hannover for next 5 days. Saturday
morning I'll be with Geri DK8KW in his QTH and I'll be probably QRV on
136kHz (DL/OM2TW). Hope to see you on LF. Best regards to all...

73 de Rich OM2TW 


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From: "Andre' Kesteloot" <andre.kesteloot@ieee.org>
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Is this reflector still working?
Andre' N4ICK





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Date: Wed, 21 Mar 2001 13:59:06 +0100
From: "Alberto di Bene" <dibene@usa.net>
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References: <3.0.1.16.20010321131726.312fb70e@mail.cc.kuleuven.ac.be>
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Rik Strobbe wrote:

> To avoid panic amongst QRS users : the next version will compensate for the
> changing value of light speed when calculating the length of a dot ;-)
>
> Rik
>

You come second, Rik... Argo has already a builtin function that takes into
consideration
the age of the universe, the local mass distribution (to cope with General
Relativity induced
effects) and the recent Superstring theory, to adjust the sampling rate
correction when you
do a Calibrate...  :-)

73  Alberto  I2PHD




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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Re. Lf DFCW
Date: Wed, 21 Mar 2001 12:41:22 -0000
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<DIV><FONT color=#0000ff face=Arial size=2><SPAN class=241113512-21032001>I 
doubt if 1s pulses could be extracted from those.&nbsp;&nbsp;The reason they are 
so cheap is that all the electronics is on one custom chip driving the LCD, with 
no extra connections accessible.&nbsp;&nbsp; </SPAN></FONT></DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001></SPAN></FONT>&nbsp;</DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001>Exactly the same argument applies to some handheld GPS 
receivers, the 1pps output is availalbe from the more expensive OEM modules such 
as the GPS25, but not from the £60 hand held devices.</SPAN></FONT></DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001></SPAN></FONT>&nbsp;</DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001>However, MSF clock receiver kits used to be availabe 
from some of the kit suppliers.&nbsp; That would be a better route to getting 
UTC pulses.&nbsp; They will only be accurate to a few milliseconds though as the 
delay through tuned circuits and IF filters, as well as the flight time from 
Rugby, cannot be taken into account in the same way as GPS 
can.</SPAN></FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN class=241113512-21032001>Also, 
if you have a decent ovenned crystal oscillator&nbsp;capable of even 0.1ppm, 
that will give a quite accurate clock, good for a about 3 seconds per 
year.&nbsp;&nbsp; Most TCXOs can probably manage that sort of accuracy if kept 
indoors at a reasonably constant temperature.</SPAN></FONT></DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001></SPAN></FONT>&nbsp;</DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001>Andy&nbsp; G4JNT</SPAN></FONT></DIV>
<DIV><FONT color=#0000ff face=Arial size=2><SPAN 
class=241113512-21032001></SPAN></FONT>&nbsp;</DIV>
<BLOCKQUOTE 
style="BORDER-LEFT: #0000ff 2px solid; MARGIN-LEFT: 5px; MARGIN-RIGHT: 0px; PADDING-LEFT: 5px">
  <DIV align=left class=OutlookMessageHeader dir=ltr><FONT face=Tahoma 
  size=2>-----Original Message-----<BR><B>From:</B> Laurie Mayhead 
  [mailto:laurie@g3aqc.freeserve.co.uk]<BR><B>Sent:</B> 2001-03-21 
  11:51<BR><B>To:</B> rsgb_lf_group@blacksheep.org<BR><B>Subject:</B> LF: Re. Lf 
  DFCW<BR><BR></DIV></FONT>
  <DIV><FONT face=Arial size=2>Hello All,</FONT></DIV>
  <DIV><FONT face=Arial size=2>Rik in a recent posting mentioned the timing 
  inaccuracies of PC clock cards.Now I may be getting out of my depth here!but 
  MSF Rugby puts out a time signal accurate to 1pt in a million,with long term 
  correction to take care of drift.Surely other countries have similar 
  systems(WWV for example.So why cant we use a cheap clock module £20 in the UK 
  extract 1sec pulses&nbsp;to sync our QRSS and ARGO systems? Is this too 
  naive?. I would like eventually to be able to use the equivalent of 10secs 
  dots in order to make DX contacts a more realistic possibility. 73s 
  Laurie.</FONT></DIV></BLOCKQUOTE><CODE><FONT SIZE=3><BR>
<BR>
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Date: Wed, 21 Mar 2001 12:30:32 -0000
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Subject: LF: WOLF - Transmit?
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Ok, so having cracked the receive side, how do I transmit WOLF?

As I understand it there are three methods:

1 - Audio from the soundcard is fed into a 136kHz SSB transmitter, including 
of course an HF SSB Tx with a transverter. Presumably the transmission is 
independent of which sideband is selected.

2 - Audio from the soundcard can be combined with the 'VFO' in an XOR gate 
and fed into an amplifier - presumably linear. This looks useful to me as I have 
a 200W linear amp.

3 - The M0BMU method that allows the use of a non-linear Class D Tx. How 
and why does this work?

All three methods are potentially simple, but are made complex by the need for 
very careful bandwidth tailoring to keep the transmission to about 20Hz wide. 

Have I got any of this wrong? Is there anything published on the subject? 
What is in use? 

I understand that some Lowfers have used WOLF, but I suspect that 
bandwidth has not been an issue because of the total width of the allocation 
and the low ERP. I believe that Larry, VA3LK, has transmitted WOLF, but 
again perhaps the bandwidth was not a problem. Jim, will you publish your 
circuits? Or perhaps they are rig specific?

It appears relatively easy to get going on receive but practical transmit has an 
information black hole.

Advice, please.



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



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>
Organization: University of Hertfordshire
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Date: Wed, 21 Mar 2001 12:31:44 +0000
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Subject: LF: <Tech> Soundcard calibration
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Dear LF group,

Rik's method of producing an accurate audio tone for calibrating 
the soundcard is very similar to what I am doing, and I can confirm 
this gives an accurate and unambiguous result. I did have some 
problems, however - the logic level square wave (in my case 1kHz) 
contains many harmonics, and I found that my soundcard did not 
have a very good anti-aliasing filter. The result of this was that 
many spurious frequency components were present in the output 
data, which could confuse the calibration program. I overcame this 
by adding a simple filter - 10k in series with the divider logic output, 
connected to a parallel - tuned circuit consisting of a 100mH 
inductance in parallel with 220n + 22n capacitors. This made the 
output a fairly clean sine wave. You may have to fiddle with the 
capacitors to peak up the output, or for different audio frequencies.

If you don't want to build a calibrator, there are a couple of ways of 
using a receiver as a calibrated audio source. If the reference 
oscillator output in the RX is reasonably accessible, it can be 
coupled with a capacitive probe wire to the RX input. If the RX is 
tuned to the reference frequency, the audio output will then be the 
nominal value within the tolerance of the reference; errors in RX 
tuning due to the reference will cancel out. This should work well 
with an RX like the RA1792, where it is easy to get at the 
reference output.

If the reference is not available, the frequency offset can be 
eliminated by a differential method; Tune the RX to a stable carrier, 
so as to produce a fairly high frequency audio output - I used 
1.3kHz. Record several minutes at 8k samples/sec, and measure 
the exact frequency using the Wolf -m option. Re-tune the RX on 
the same carrier to produce a low frequency audio output - I used 
300Hz. Repeat the frequency calibration using Wolf -m. Calculate 
the difference between the two RX frequency settings, and the 
difference between the frequencies as measured by Wolf. The 
soundcard sample rate is then:

8000 x (difference in RX tuning setting) / (difference in measured 
audio frequency)

This gave me almost the same results as calibrating with an 
accurate audio frequency. Both methods assume the receiver 
reference oscillator is accurate, but it's accuracy will normally be 
pretty good compared to the soundcard. Note, however, that both 
methods may be defeated by receivers using DDS synthesisers, 
which tune in odd-frequency steps, but display the output to the 
nearest Hz.

Note also that the soundcard sampling rate error depends on the 
actual rate selected - for example, measuring 800Hz using 
Spectrum Lab with 8k sample rate gave me a frequency error of 
about +4.5Hz, but with the 11k rate, the error was about -1.6Hz. 
The errors are different with different types of soundcard. So using 
other software to measure frequency offsets will not be helpful, 
unless it also uses an 8k sample rate. I think Argo uses the 11k 
rate. I don't know about the PSK31 software. Oh joy.....

Hope this is helpful,

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
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To avoid panic amongst QRS users : the next version will compensate for the
changing value of light speed when calculating the length of a dot ;-)

Rik

At 11:10 21/03/01 -0000, you wrote:
>According to the latest theories, time may be slowing down.   By
>acccepting that the speed of light has been continuously reducing from
>the point at which the universe was formed, they've worked out that the
>uncertainty as to whether the Universe is continuously expanding, or
>going to collapse again in a Big Crunch goes away.   Apparently, the
>Hubble Space Telescope is just beginning to show some evidence for this
>theory of a reducing value for c.
>
>So, in about 4000 000 000 years 137kHz may have become 73kHz.  Or
>Topband, or 10GHz, who knows.  Not sure what the implication of a
>variable value for c really means.   Antennas will have to change in
>length - or will they, perhaps wavelength will stay constant and
>frequency change.  Will my Caesium standard still be accurate ? 
>
>Its all very worrying :-(
>
>Andy  G4JNT



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Andy,  interesting, but please don't scare me like that
73 de John VE1ZJ

Talbot Andrew wrote:

> According to the latest theories, time may be slowing down.   By
> acccepting that the speed of light has been continuously reducing from
> the point at which the universe was formed, they've worked out that the
> uncertainty as to whether the Universe is continuously expanding, or
> going to collapse again in a Big Crunch goes away.   Apparently, the
> Hubble Space Telescope is just beginning to show some evidence for this
> theory of a reducing value for c.
>
> So, in about 4000 000 000 years 137kHz may have become 73kHz.  Or
> Topband, or 10GHz, who knows.  Not sure what the implication of a
> variable value for c really means.   Antennas will have to change in
> length - or will they, perhaps wavelength will stay constant and
> frequency change.  Will my Caesium standard still be accurate ?
>
> Its all very worrying :-(
>
> Andy  G4JNT
>
> > a DAC is needed... TNX for clarifying.
> >
> > Time is continous... this was a great debate in the
> > Theoretical Physics field
> > many, many years ago. But now I have lost contact with that ambient
> > and don't know what the present theories say. But this is
> > totally off-topic...
> >
> > 73  Alberto   I2PHD
> >
> >
> >
>
> --
> The Information contained in this E-Mail and any subsequent correspondence
> is private and is intended solely for the intended recipient(s).
> For those other than the recipient any disclosure, copying, distribution,
> or any action taken or omitted to be taken in reliance on such information is
> prohibited and may be unlawful.



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
Subject: LF: Re. Lf DFCW
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<DIV><FONT face=Arial size=2>Hello All,</FONT></DIV>
<DIV><FONT face=Arial size=2>Rik in a recent posting mentioned the timing 
inaccuracies of PC clock cards.Now I may be getting out of my depth here!but MSF 
Rugby puts out a time signal accurate to 1pt in a million,with long term 
correction to take care of drift.Surely other countries have similar systems(WWV 
for example.So why cant we use a cheap clock module £20 in the UK extract 1sec 
pulses&nbsp;to sync our QRSS and ARGO systems? Is this too naive?. I would like 
eventually to be able to use the equivalent of 10secs dots in order to make DX 
contacts a more realistic possibility. 73s Laurie.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: exact audio reference
Date: Wed, 21 Mar 2001 11:26:22 -0000
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Another solution is to run G3PLX's  PSK31 SB software.   There is a
setup routine in the software that allows the Soundcard sampling rate to
be calibrated. The procedure is given in the Help file, accessible from
the menu bar.   Again, an accurate audio frequency source will be
necessary.

The vectorscope in that software allows fine tuning accuracy to an
arbitrary audio tone, and frequency resolution of less than 1Hz is
clearly seen.   So it becomes a useful tool for measuring carrier
frequencies even if you don't actually want to use the PSK31 data mode.

Andy  G4JNT
> 
> For those who want to calibrate the soundcard there is also a simple
> hardware solution :
> Take a CMOS4060 (14-stage divider with internal oscillator) 
> and let it run
> with a xtal in the 8-12MHz range. At the end of the divider 
> chain (pin 3)
> 


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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE PICs and DDS etc.
Date: Wed, 21 Mar 2001 11:10:53 -0000
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According to the latest theories, time may be slowing down.   By
acccepting that the speed of light has been continuously reducing from
the point at which the universe was formed, they've worked out that the
uncertainty as to whether the Universe is continuously expanding, or
going to collapse again in a Big Crunch goes away.   Apparently, the
Hubble Space Telescope is just beginning to show some evidence for this
theory of a reducing value for c.

So, in about 4000 000 000 years 137kHz may have become 73kHz.  Or
Topband, or 10GHz, who knows.  Not sure what the implication of a
variable value for c really means.   Antennas will have to change in
length - or will they, perhaps wavelength will stay constant and
frequency change.  Will my Caesium standard still be accurate ? 

Its all very worrying :-(

Andy  G4JNT



> a DAC is needed... TNX for clarifying.
> 
> Time is continous... this was a great debate in the 
> Theoretical Physics field
> many, many years ago. But now I have lost contact with that ambient
> and don't know what the present theories say. But this is 
> totally off-topic...
> 
> 73  Alberto   I2PHD
> 
> 
> 


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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: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: LF: exact audio reference
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For those who want to calibrate the soundcard there is also a simple
hardware solution :
Take a CMOS4060 (14-stage divider with internal oscillator) and let it run
with a xtal in the 8-12MHz range. At the end of the divider chain (pin 3)
you will get the xtal frequency divided by 16384 (will be in the 500-700Hz
range).
If you can measure the oscillator frequency (available at pin 9) with a
100Hz accuracy you will know the audio frequency with 0.006Hz accuracy. You
get 100Hz accuracy with almost any frequency counter or by tuning into the
signal with a HF receiver. 
With a better counter or a good RF receiver you can measure the oscillator
signal even up to 10Hz accurate (= 0.0006Hz for the audio signal).
Finaly, 'freaks' can take a 10MHz xtal and tune it zero beat against
Boulder or so. That will give a 1Hz accuracy on the xtal or 0.00006Hz on
the audio signal.

For those who want to try it but don't have acces to a CMOS databook I can
e-mail the circuit diagram.

73, Rik  ON7YD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alberto di Bene" <dibene@usa.net>
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Klaus von der Heide wrote:

> [snip]
> The problem is the discrete time the DDS uses. The high order bit
> only changes at the clock edges. The result is a square wave with
> heavy phase jitter.  For example, draw a sine wave (3 waves),
> sample it at about 8/3 of its frequency in your sketch, and generate
> the square wave from these sample values (all on the paper).
> The one-periods and the zero-periods then are one or two clock cycles
> long. That's what Andy in other words already said.
> If a DAC is used then time is continuous and a clean square wave can
> be obtained.

Hi Klaus,
                 yes, that makes a lot of sense. It seems that, after all,
a DAC is needed... TNX for clarifying.

Time is continous... this was a great debate in the Theoretical Physics field
many, many years ago. But now I have lost contact with that ambient
and don't know what the present theories say. But this is totally off-topic...

73  Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: LF: Loran
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Markus et al,

There is a data transmission superimposed on Sylt (and now on the other EU 
Loran tx). which may explain your unknown lines. This extract from a paper 
given by TU Delft at the US PLANS 98 conference explains it a bit  (I have 
full tech data if you really want it but it's too long to put on here)

Quote:

LORAN-C DATA TRANSMISSION

As Loran-C is a navigation system in itself, its navigation requirements 
and parameters
restricts the use of the signals for transmission of information. The 
additional data modulation
onto the Loran-C signal shall not influence normal Loran-C operation. 
Therefore, the
following restrictions are imposed on the use of the Eurofix datalink:

-    The blinking service must be preserved, which excludes the first two 
pulses of each
Loran-C group from Eurofix  modulation.
-    The modulation is not allowed to induce tracking biases, which 
requires a balanced
type of modulation.
-    The modulation index must be kept small in order to prevent an 
undesirable loss in
tracking signal power.

Based on these requirements, a pulse position modulation with a 1 uS 
modulation index is
chosen. Only 6 out of 8 pulses per group will be modulated and the 
modulation is always
balanced on a per GRI basis. The application of 3-level modulation (a 1 uS 
advance, a prompt,
or a 1 uS delay) leaves a possible 7 bit of information per GRI. With 
Loran-C GRI's varying
between 40 ms and 100 ms, the raw bit rate available for data transmission 
ranges from 175 to
70 bps.

Normal Loran-C users only experience a slight signal loss of 0.79 dB. 
Future Loran-C
receivers, which have knowledge of the Eurofix modulation, can easily 
compensate for the
applied modulation, once the pulses are demodulated. This will cancel the 
signal loss
completely. Note that the influences of Cross-Rate interference and 
blanking, phenomena
inherent to the choice of the Loran-C signal structure, cause larger signal 
degradation.

DGNSS message format

The differential information is sent to the user in an asynchronous message 
format. The use of
standard RTCM type-1 messages requires too much time to transmit a complete 
set of
corrections. To keep data latency within acceptable limits, a minimum RTCM 
type-9
compatible message of 56 bits is applied, Table 1. Unfortunately, the 
simple parity schemes
used in the RTCM messages do not suffice in the Loran-C signal environment 
of Cross-Rate
interference and high ambient noise levels. Therefore. a different error 
correcting strategy is
chosen. However, as standard and commercially available DGNSS receivers must be
facilitated, the received Eurofix data is converted into a standard RTCM 
type-9 message.

Forward Error Correction

To ensure reliable broadcast data communication through Loran-C. Forward 
Error Correcting
codes are applied. These codes provide an effective means to correct 
occasional errors
(improved datalink availability) and validate the decoded data (integrity) 
at the cost of an
increased message overhead. Figure 1 shows the modulation and encoding 
currently used to
transmit data via Loran-C. In Eurofix a Reed-Solomon code ensures datalink 
availability for
stations up to 1,000 km. Each 56-bit message (8 GRI's of 7 bits) is 
protected by additional
Reed-Solomon parity GRI's. In recent experiments messages contained in 20 
and 30 GRI's
have been tested. Depending on the Group Repetition Interval (40-100 ms) of 
the Loran-C
station the effective datarate of these schemes will be 70-28 bps and 47-19 
bps, respectively.

Message integrity is protected in three steps:
1.   Before demodulation a received pulse is first compared with a stored 
reference pulse,
built up by integration of the first 2 unmodulated pulses (Receiver 
Autonomous Signal
Integrity Monitoring, RASIM). This way, the quality of the demodulated 
pulses is preserved
[6].
2.   The Reed-Solomon code inherently adds integrity to the messages. The 
Probability of
Undetected Error. Pue for a 10-error correcting Reed-Solomon code (30-GRI 
Eurofix
message) is 1/10! = 2.7*10-7.
3.   As a final safety net a 14-bit Cyclic Redundancy Check (CRC) ensures a 
lower bound
on the Pue of better than 2(-14)=6.1*10-5.

The final message integrity will be a combination (probably product) of the 
above three
mechanisms. This level of message integrity outperforms the level of the 
standard RTCM
messages without further integrity improvements.

IMPLEMENTATION OF DGPS SERVICE AT THE SYLT LORAN-C STATION

On February 5th, 1997, Delft University installed a DGPS reference station 
at the Sylt
Loran-C transmitter site (Germany) on an experimental basis. From that date 
on differential
corrections have been broadcast throughout Europe on the Sylt Secondary 
rate 8940.
Corrections for all satellites in view are broadcast in RTCM type-9 
compatible messages with
one satellite correction per message. The update rate for a 30-GRI message 
at the Sylt's GRI
is once every 2.7 seconds per satellite (30*89.40 ms). Since September 
23"', 1997, Sylt
operates as a Secondary in the new French chain 6731. The slightly lower 
GRI number
increased the update rate to once every 2.0 seconds. When also the Master 
rate of Sylt (7499)
will be used for data transmission the correction update rate will be even 
further improved.

End quote.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Date: Wed, 21 Mar 2001 09:53:34 -0000
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> If you're still having trouble with Jim's WOLF signal, please
> email me a one minute .wav file, and I try to diagnose the
> problem.  You can convert it to 8-bit samples to save some
> space, if you like.  My mail server will accept attachments of
> up to about 7 MB.
> Stewart KK7KA

Stewart,

Many thanks for the offer but I have now fixed the problem by using the -r 
parameter to compensate for sound card sample rate.

I tried the method suggested by JIm - the use of the -m command - but got a 
totally inaccurate result that fooled me for an hour.

I recorded M0BMU's test transmission (thanks, Jim - this is a really useful 
service) last night at a lower level than previously but still had no copy. I then 
fiddled about with the parameters until suddenly it all worked. I had to set -r to 
anything between 8090 and 8110. Inside this range it was perfect, outside no 
copy at all. 

Plainly a really good way of being able to set this parameter would be useful. 

I think this makes me the first G station to receive another amateur using 
WOLF. This is hardly an achievement, though as Jim is less than 10km from 
me and he has already been read in the USA.

Is there a web page that details the significance of the figures you see on 
screen before the text? I have found some info but not much that says "this 
should be in the region of . . .", or "if this is below xxx, adjust yyy".

Thanks for the software. 


Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Re: lf tests
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G3YMC wrote:
> While the rest of you were playing with exotic modes on Monday evening I
> was listening to Christer SM6PXJ in QSO with Ron G6RO - around 2030-2100z 
> 
> During the QSO Christer remarked that he might have been causing tvi, and as
> such couldn't stay to work Uli DJ9IE who called him afterwards. 
> ...................... - is this the first reported case of TVI on
> lf??

More likely the Aurora was causing the TVI and Christer was being blamed!


Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Petr Maly" <p.maly@gmc.net>
To: "136 group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Skeds please
Date: Wed, 21 Mar 2001 10:32:12 +0100
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Hi LowFers
I plan to be QRV again after a long time this weekend, from Friday evening
to Sunday noon. Any skeds welcome, mainly from EI, EA, CT, F,  GW. Both CW
and Visual-CW.

73 Petr OK1FIG





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From: "Stewart Nelson" <sn@scgroup.com>
To: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Cc: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010321095813.2c2f637a@mail.cc.kuleuven.ac.be>
Subject: LF: Re: WOLF
Date: Wed, 21 Mar 2001 01:25:06 -0800
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Hi Rik and all,

I think that this bug has been fixed, but I failed
to post to the LF group.  My apologies.  If 0.52 doesn't
fix the problem for you, please tell me what program
you are using to record, or email me a failing sample.

----- Original Message ----- 
From: "Stewart Nelson" <sn@scgroup.com>
To: "LowFER reflector" <lowfer@qth.net>
Sent: Monday, March 19, 2001 9:21 PM
Subject: Re: [Lowfer] RecAll help (new WOLF release)

Hi all,

The bug in WOLF which caused only partial processing
of .wav files written by programs such as RecAll has,
I hope, been fixed.

The '-v' (verbose) option will now also display the
resolution and sample count of the file being read.

The new version is 0.52 and can be downloaded at
http://www.scgroup.com/ham/wolf.html .

Sorry for all the hassle this bug has caused.

Please let me know of any further problems.

73,

Stewart KK7KA


----- Original Message ----- 
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
To: "Stewart Nelson" <sn@scgroup.com>
Sent: Wednesday, March 21, 2001 9:58 AM
Subject: WOLF


> Hello Stewart,
> 
> While testing WOLF on M0BMU's transmissions I came across a problem :
> I have about a dozen recordings (different in length) of Jim's
> transmissions. WOLF accepts all of them, but with some the program
> terminates just after one 'cycle' (so I get the 24 sec. result and the WOLF
> terminates). All recordings are at least 1 minute long, so there should be
> at least 2 full cycles.
> Any idea what is going wrong ?
> 
> thanks,
> 
> 73, Rik  ON7YD
> 



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: LF: The EF50
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--------------020606040603060009050803
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Although off-subject there seems to be a lot of interest in the EF50.
Attached is a text-only version of a recent article written by
Keith Thrower, an ex-Director of Racal and an electronics historian.
It comes from the journal of the "Centre for the History of Defence 
Electronics"
at Bournemouth University -  http://chide.bournemouth.a.c.uk

Walter G3JKV.
   
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The following article was published in the December 2000 issue of "Transmission Lines", the
journal of the "Centre for the History of Defence Electronics", based at Bournemouth
University.

Illustrations have been omitted in this text-only copy to save space. 
If you'd like to see the full article ask CHiDE for a copy of their journal  - 
chide@bournemouth.ac.uk.


The Famous EF50 Valve of WWII

by Keith Thrower OBE

By the early 1930s screen grid and pentode valves were available for RF amplification for
frequencies up to about 30MHz, which was adequate for both broadcast and commercial
purposes at the time, when radio usage had not extended into the UHF band. At frequencies
above 30MHz the gain available from valves fell very sharply; there were two principal
problems: the first was caused by the inductance and capacitance of the internal leads that
connected the valve electrodes to the terminating pins; the second was due to the finite transit
time that the electrons took to travel between the valve electrodes.

The first problem arose through the valve design and manufacturing techniques which had
evolved from those used in the electric lamp industry. One particular constructional feature of
the valve, copied directly from the lamp industry, was the use of an internal glass stem and
pinch that held the support wires to the electrode assembly, and also provided a vacuum seal
for the lead-out wires. The problem that arose from this method of construction was that the
total length of the connections from the electrodes to their terminating pins was quite long,
resulting in significant self-inductance of the wires as well as excessive self-capacitance
between them. At frequencies below 30MHz, these parasitic inductive and capacitive
components did not seriously affect the performance of the valve, but their effects became
increasingly more serious at frequencies above this.

The second problem - the finite transit time for the electrons to move between the electrodes -
was very serious for valve circuits operating at frequencies above 30MHz. For a typical RF
valve of conventional construction, the transit time for the electrons to move between the
cathode and control grid was about one nanosecond (one thousand-millionth of a second). At
frequencies of a few megahertz, this transit time was insignificant compared with the time for
one cycle of the signal frequency. At 100MHz, however, the time was about 10% of one cycle
and this was very significant. The phase lag caused by this time delay resulted in a low input
resistance at high frequencies, which significantly reduced the amplification available.

A great deal of experimental research work was carried out at the RCA laboratories during the
early 1930s to investigate the behaviour of radio frequency amplifier valves, where it was
found that improved circuit performance could be achieved if the valve dimensions were
reduced. With a linear reduction, the mutual conductance and other valve parameters remained
almost unchanged, but the lead inductance, interelectrode capacitance and electron transit time
all fell in direct proportion to the reduction of dimensions. In fact, such a linear reduction was
not practical; however, the tiny 'Acorn' valves that resulted from this work were capable of
providing amplification at frequencies up to about 400MHz.

The first of these valves to go into production was the type 955 triode which was introduced
in 1934. This was followed by the 954 pentode in 1935 and a variable-mu pentode, the type
956, in 1936 (see Figure 1). They all had indirectly heated cathodes, operating at 6.3V, 0.l5A.
The diameter of the heater-cathode assembly was comparable with that of a common
household pin and the overall length was less than one half. The capacitance between the
control grid and anode for both the triode and pentode was about half that of conventional
valves, and all other internal capacitances were also significantly reduced.

Before long, acorn valves, based on the RCA design, were introduced in Britain by Mazda,
Marconi-Osram and Mullard. Initially, all the British acorn valves had 4V heaters, but 6.3V
versions were introduced in 1940.
Figure 2 shows how the input resistance of a valve is affected by transit time, where a
comparison is made between an acorn pentode and an equivalent, conventional pentode. At
30MHz, the conventional pentode (B) has an input resistance of 17k which falls to only 1.5k
at 100MHz. The equivalent figures for the acorn pentode (A) are 220k at 30MHz and 20k at
100MHz. This fall of input resistance, which has a critical effect on the amplification that the
valve can provide is inversely proportional to the square of the frequency: if the frequency is
doubled, the resistance falls by a factor of four and a ten-fold increase in frequency results in a
hundred-fold decrease of input resistance. It is not difficult to see, therefore, that conventional
valves were unsuitable for operation in the UHF band, whereas the acorn or similar miniature
valves were better suited.

British companies, such as MOV and Mullard, found the acorn valves very difficult to
manufacture because of the highly skilled labour required. As a result, considerable quantities
of the valves were imported from the US for use in military radar equipment during World
War 2. Because of the manufacturing problems and the eventual availability of alternative
valves, the acorn types were blacklisted by the Inter-Service Technical Valve Committee in
June 1941.

With the commencement of high definition television in 1936 there was a need for a new type
of valve capable of providing wideband RF amplification. The frequencies required for the
Alexandra Palace transmission were 41.5MHz for the sound channel and 45MHz for the vision
channel, the latter requiring a bandwidth of 3MHz in order to accommodate the full picture
information. In order to achieve satisfactory amplification of the video signal, valves were
required with a high value of mutual conductance, and if this amplification was to be achieved
at RF the valves must have low values of internal capacitance and self-inductance, in addition
to a short electron transit time. The early valves produced for this role were far from
satisfactory.

By the mid-1930s top-secret work was in progress at Bawdsey Manor in Essex on radio
direction finding (RDF)later to be re-named radar. For this, once again, valves capable of
providing wideband UHF amplification were required. At this time Tom Goldup, a senior
director of the Mullard Valve Company, was liaising with the British government and was
made aware of this requirement. Mullard was wholly owned by the Dutch Philips Company
and all the valve R&D work was carried out at the Philips Eindhoven plant. Goldup
approached Philips asking if there was a valve with the required specification. (Because RDF
could not be mentioned I suspect he referred to television applications.) He was told that a
suitable valve was being developed for the Dutch government; samples, therefore, could not
be supplied to Mullard. It would appear that the UK government approached the Dutch
government and samples were then supplied. The valve in question was the EF50, which
became available for television use in 1939. At this time all the valves were being
manufactured in Holland.

The construction of the Mullard FF50 is of interest because it marked a significant departure
from the conventional types used in Britain at the time. The usual Bakelite base and internal
glass pinch were replaced by an all-glass base. Elimination of the stem and pinch resulted in a
considerable reduction in length of the internal wires. The valve had nine chromium-iron pins,
which were sealed into the glass base and arranged uniformly around a central metallic spigot,
which was keyed in order to facilitate insertion into the valveholder. The spigot was joined to
an external metal screen that covered the whole base, with small holes to allow the pins
through. Because of the screening provided, it was possible to bring all the connections out to
the base, avoiding the need for a top cap connection.
With the outbreak of war it was realized that the supply of EF50 valves would dry up and
Mullard did not have the capability of manufacturing the special glass base with sealed-in pins.
Consequently, just before Germany invaded Holland, a truck came from Holland with one
million of these glass bases. Later, huge numbers of the valves were manufactured by Sylvania
in the US.

Figure 4 shows a selection of EF50 valves from various suppliers available during the War.
The original Air Force type number was VR91, the Army type ARP35 and the CV number
1091. From left to right these are:

(i) and (ii) Sylvania manufactured VR91, front and back view.
(iii) Silver UK version of VR91 for RAF use. 
(iv) Silver UK version ARP35 for Army use.
(v) Mullard EF50 red. 
(vi) Mullard EF50 silver
(vii) Cossor 63SPT
(viii) Osram Z90.

A typical use of the EF5O was in the Pye 45MHz IF strip - Receiving Unit Type 153 - which
was used universally in British radar equipment during the war. A picture of this can be seen in
Figure 5. It had six EF50s (VR91s) and one EA50 (VR92) miniature signal diode.

A variant of the EF50 was the RL7 (VR136). This had aligned grids to reduce partition noise,
and the cathode was connected by leads to two separate pins to reduce still further the
selfinductance. The valve was capable of proving RF amplification at 200MHz and could thus
displace the acorn valve. In post war years it was re-designated as EF54.

Acknowledgements

I am grateful to Dr Graham Winbolt who provided the photographs of the EF5O valves in
Figure 4 and the Receiving Unit Type 153 in Figure 5. The information on the RL7 was
obtained from Brian Callick's excellent book Metres to Microwaves (published by Peter
Peregrinus Ltd and obtainable from the IEE).
For more information on early British valves see History of the British Radio Valve to 1940 by
K Thrower and published by Speedwell.


--------------020606040603060009050803--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 21 Mar 2001 10:04:59
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: lf tests
In-reply-to: <000001c0b1d2$13f44d00$34a401d5@dave>
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>but Christer was a steady 589, not much weaker than Ron, and the
>strongest I have ever heard him.  They had an excellent chat and exchanged
>589 reports and I think they were each surprised at how good signals were.
>Whether this is related to the auroral conditions I don't know.

Hi Dave,

I'm sure it has. I noticed enhanced propagation toward OH1TN at 'auroral
days' ever since I'm active on LF. It wasn't unusual for Reino's signal to
be 10-15dB stronger at such occasions. I have the impression that this
effect is more effective on a north-south path than on an east-west path.

73, Rik  ON7YD


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: DFCW
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Hello Wolf,

>The problem is, PC clocks (though called 'Real Time Clocks') can be quite 
>bad, much worse than the cheapest wristwatch you can buy in a coffee-store. 
>So setting the clock for an accuracy of 0.1 sec or better only lasts for a 
>few MINUTES (!) on some nasty PCs (like the one I have to use sometimes). 

When I was thinking of implementing 'time synchronisation' in QRS I did
some tests with 5 different PC's : I set the clock to DCF77, let them run
for 16 hours and checked the difference between the PC clock and DCF77.
The differences turned out to be between +10 and -8 seconds, so a 'drift'
of about 0.6 seconds/hour.
Taking into account that 5% error in the 'time synchronisation' equals a
0.2dB loss (seems acceptable to me) would mean that for 30 sec./dot a 1.5
second timing error is acceptable. Taking worst case (PC clocks drifting in
different directions) this would mean that the time for a QSO is about 70
minutes.
If there is some real interest in this 'time synchronized' stuff I will
have a closer look a the drift of the PC clock, if it tends to be a (more
or less) linear drift it could even be compensated in QRS.

>What really helps would be a GPS (costly, only works if satellites visible) 
>or a cheap DCF receiver connected to the serial port (if not already
occupied 
>by mouse, modem, PIC, TRX control, DSP board etc etc).
>You have to readjust the clock continously, if you want 'reliable' second 
>markers for recording intervals of an hour or so. A possible workaround
would 
>be using the soundcards "calibrated" sample rate as a timebase.

Using the soundcard may be more 'user friendly' that using a GPS. A good idea.


73, Rik  ON7YD



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To: rsgb_lf_group@blacksheep.org
Cc: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
References: <57.132cfa73.27e951ff@aol.com>
Subject: LF: Re: Loran DX
Date: Wed, 21 Mar 2001 00:19:41 -0800
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Hi Markus and all,

I'm quite interested in this idea; perhaps we can work together
to develop the code.  We might call it the LAMP (Loran Analysis
for Monitoring Propagation), but other suggestions are welcome.

I haven't written any real code yet, but processed some .wav files
with a simple perl script and plotted the results with Excel.
You can see a sample at http://www.scgroup.com/ham/h9610.gif .
I used a one-minute recording made by Dexter W4DEX in Stanfield,
North Carolina.  The horizontal scale is samples from the beginning
of the recording, modulo the GRI "tuned", 9610 in this case.  The
vertical scale is arbitrary voltage units.  The four colors show
correlation with master and secondary codes, with both A/B sequences.
Layout of the 9610 chain can be found at
http://www.megapulse.com/pix/chain/9610.gif .  The magenta peak at
1592 is the master in Boise City, Oklahoma.  The big yellow peaks
at 307 and 641 are Raymondville, TX and Grangeville, LA, respectively.
Cyan peaks at 2069 and 2618 are Gillette, WY, and Searchlight, NV.
This last one is 3115 km from W4DEX.  You can't see Las Cruces
because of a bug related to wraparound.

My best DX is Ejde, 5760 km from W4DEX.  It was just slightly above
the highest noise peak for the 9007 chain.  Unfortunately, I couldn't
positively identify stations such as Sylt or Lessay.

To make this system really useful, we need IMO about 10 dB more S/N.
I have some ideas on how to get it, and I'd very much like to hear
yours.  For starters, we can integrate for more than one minute.
Unfortunately, this must be partly noncoherent, because I think
that the skywave path is generally not phase stable for longer than
a couple of minutes.  We could use a filter properly matched to
the receiver's impulse response.  My script has only a crude two
point equalizer.  For dual-rated stations, we could coherently
combine pulses from both GRI's (see below).  And, most complex,
we could use an adaptive equalizer to cancel most of the local
QRM.  W4DEX is only 261 km from the Carolina Beach station;
the present script simply goes deaf during those pulses.  The
perl code is at http://www.scgroup.com/ham/loran1f.txt .
You can see that it is pretty crude - I used Cool Edit to convert
the .wav to 32000 Hz samples and to text, and determined the true
sample rate and BFO frequency manually.  Sorry that there are
no comments.

Not only do LORAN transmitters use atomic clocks, but they are
monitored and kept within 200 nanoseconds of UTC.  The long term
frequency error is zero!  Also, every LORAN master conceptually
emitted a pulse on January 1, 1958 at 00:00:00 UTC.  So if you
know the time within 1 GRI, you can tell the exact time.  Better,
by looking at the timing from a dual-rated station, you only need
know the time within a few seconds.  With two dual-rated stations,
within several hours, and with three, within about a year.  So,
by carefully examining the recording, I determined that the first
recorded master pulse from the 9960 chain was the one emitted from
Seneca on March 12, 2001 at 01:28:31.0544 UTC.  I then used this
information to predict exactly where pulses should appear from
stations in various other chains.  If within ground wave range,
the match was always within 20 microseconds, so any additional
sky wave delay could be judged quite accurately.  Also, the
amplitude of the signal from the closest station is probably
consistent within 0.1 dB, so the system could continuously
self-calibrate and give accurate field strength readings, too.

How should we proceed from here?

73,

Stewart KK7KA

----- Original Message -----
From: <MarkusVester@aol.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 20, 2001 4:38 PM
Subject: LF: Loran DX


> Hi Wolf and all,
>
> triggered by John VE1ZJ's recent remarks on Loran as a skywave propagation
> monitor, a couple of weeks ago I took a deeper look at what could be
> received. John's "www.G4CNN.f2s.com/Loran_lines.htm" pointed me to the list
> at "www.megapulse.com/table.html". With this at hand I tried to identify the
> lines I could see on Argo around 100.0 kHz.
>
> The key to their frequencies is the "GRI" (group repetition interval), which
> is the number of 10us carrier periods between two repetitions of the
> modulating pulse groups. Each group consists of 9 or 8 pulses, 1 ms apart.
> Some of these pulses have an alternating phase, so that the periodicity of
> the pattern is actually two times the GRI:
>    Master       Secondary
>  ++--+-+- +     +++++--+
>  +--+++++ -     +-+-++--
> Thus the frequency spacing of the lines is Df = 100kHz/(2*GRI), eg.
> 100kHz/(2*7499) = 6.6676 Hz for the Sylt chain. The Loran-C carrier frequency
> is generated by atomic clocks and claimed to be accurate on the order of
> 10^-13.
>
> The chains I could clearly observe here were
>
> GRI     Df      Chain  (Wolf's AM line)
> /10us  /Hz
> 5930  8.4317  Canadian East Coast
> 6731  7.4283  Lessay
> 7001  7.1418  Bo  (140*Df = 999.8572 Hz)
> 7030  7.1124  Saudi Arabia S
> 7270  6.8776  Newfoundland East Coast
> 7499  6.6676  Sylt  (150*Df = 1000.1334 Hz)
> 8000  6.2500  Western Russia  (160*Df = 1000.000 Hz)
> 8830  5.6625  Saudi Arabia N
> 9007  5.5512  Eide
>
> Then there were additional weak lines which were too close to 100 kHz, at
> offsets of 1.52, 3.04 and 4.56 Hz. Their explanation is a little more subtle:
> Many loran stations are "dual-rated", they transmit in two chains with
> different GRI's. In case of a collision between two pulses that would have to
> be sent simultaneously, one of the pulses is simply left out. These dropped
> pulses occur at the beat frequency between the two GRI's. For the Sylt
> station, these "intermodulation" lines are multiples of
> (100kHz/6731-100kHz/7499) = 1.5215Hz.
>
> There were even more lines I could not identify, eg. on 5.14, 5.90, 7.24,
> 8.18, 8.95 Hz. This made me wonder if the table is really complete, as stated
> by megapulse. Also, I can't explain Wolf's observed 999.96 Hz.
>
> The fun got even more interesting when I went to time domain. Using a
> programmable divider clocked by 100 kHz, I generated 2*GRI trigger signals
> for a digital oscilloscope in 128-averaging mode, and viewed the SSB output
> tuned to 100.0 kHz zero beat  (thus allowing phase-sensitive averaging). With
> this setup I could see the individual pulse groups of distant chains grow out
> of the noise, identify their stations and measure the time-differences. These
> matched calculated great-circle distances with a surprising accuracy of less
> than 100us, and it even worked fine for all five of the Saudi-Arabian
> stations, up to 4642 km from here.
>
> Thus I think that Loran-C can be used not only as a precise frequency and
> time standard, but also as a powerful instrument for worldwide LF propagation
> monitoring, aided by its ability to resolve propagation delays.
>
> 73s and happy experimenting
> de Markus, DF6NM
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 21 Mar 2001 07:44:24 +0000
To: rsgb_lf_group@blacksheep.org
From: "Tom Boucher" <tom@telemetry.demon.co.uk>
Subject: Re: LF: Re: lf tests
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Dave

I was also eavesdropping on Ron & Christer's QSO while working in the
shack and Christer was no stronger than usual here in the South-West.
However....I worked him one night a few months ago and exchanged 599
both ways. On that occasion signals were very definitely enhanced for
some reason or other.

73, Tom G3OLB


In message <000001c0b1d2$13f44d00$34a401d5@dave>, Dave Sergeant
<dsergeant@btinternet.com> writes
>>From Dave G3YMC
>
>John Currie wrote:
>>The K index was a 4 at 0000z last nite and a 6 at 0900z .  We had
>>widespread Au propagation on 144 mHz in both Eu es NA.  I had visible
>>Aurora at 0833Z here
>
>While the rest of you were playing with exotic modes on Monday evening I
>was listening to Christer SM6PXJ in QSO with Ron G6RO - around 2030-2100z if
>I remember right. Not only was it nice to here Ron after his sad news last
>week, but Christer was a steady 589, not much weaker than Ron, and the
>strongest I have ever heard him.  They had an excellent chat and exchanged
>589 reports and I think they were each surprised at how good signals were.
>Whether this is related to the auroral conditions I don't know.
>
>During the QSO Christer remarked that he might have been causing tvi, and as
>such couldn't stay to work Uli DJ9IE who called him afterwards. Uli was
>weaker than Christer, and I noticed that both he and F6BWO were their normal
>signals, so perhaps we were seeing an auroral path from SM.  Perhaps
>Christer would like to comment - is this the first reported case of TVI on
>lf??
>
>
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000001c0b1d2$13f44d00$34a401d5@dave>
From: "Dave Sergeant" <dsergeant@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
References: <3AB79746.7E947458@ns.sympatico.ca>
Subject: LF: Re: lf tests
Date: Tue, 20 Mar 2001 18:45:06 -0000
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>From Dave G3YMC

John Currie wrote:
>The K index was a 4 at 0000z last nite and a 6 at 0900z .  We had
>widespread Au propagation on 144 mHz in both Eu es NA.  I had visible
>Aurora at 0833Z here

While the rest of you were playing with exotic modes on Monday evening I
was listening to Christer SM6PXJ in QSO with Ron G6RO - around 2030-2100z if
I remember right. Not only was it nice to here Ron after his sad news last
week, but Christer was a steady 589, not much weaker than Ron, and the
strongest I have ever heard him.  They had an excellent chat and exchanged
589 reports and I think they were each surprised at how good signals were.
Whether this is related to the auroral conditions I don't know.

During the QSO Christer remarked that he might have been causing tvi, and as
such couldn't stay to work Uli DJ9IE who called him afterwards. Uli was
weaker than Christer, and I noticed that both he and F6BWO were their normal
signals, so perhaps we were seeing an auroral path from SM.  Perhaps
Christer would like to comment - is this the first reported case of TVI on
lf??

73s Dave
dsergeant@btinternet.com
dsergeant@iee.org
http://www.btinternet.com/~dsergeant








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 20 Mar 2001 21:17:41 -0500
Subject: Re: LF: Re: Re: DFCW
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What the heck is a mudball/
 John VE1ZJ


That would be the 3rd rock 
from the sun

Bob  


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Stewart Nelson" <sn@scgroup.com>
To: rsgb_lf_group@blacksheep.org
References: <4736.200103191732@gemini> <000201c0b0c8$76567820$6fe086d4@ericadodd> <006e01c0b0e6$d26adfc0$687a37c0@w2ksn> <000e01c0b12a$78868b00$1cce28c3@ericadodd>
Subject: LF: Re: Re: WOLF BPSK
Date: Tue, 20 Mar 2001 17:08:25 -0800
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Hi Peter,

It appears that Rik solved this problem, but if you're still
having trouble, please let me know and I'll try to help.

73,

Stewart KK7KA




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: Success and failure
Date: Tue, 20 Mar 2001 17:06:23 -0800
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Hi Mike,

If you're still having trouble with Jim's WOLF signal, please
email me a one minute .wav file, and I try to diagnose the
problem.  You can convert it to 8-bit samples to save some
space, if you like.  My mail server will accept attachments of
up to about 7 MB.

73,

Stewart KK7KA

----- Original Message -----
From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 20, 2001 2:24 AM
Subject: WOLF: Success and failure


> I tried out WOLF for the first time last night with total success.
>
> Jim was sending GY(^%? JGGF, followed by H(*^RCKO KKl, followed by . . . .
>
> OK, so it wasn't quite as successful as I would have liked.
>
> My first problem was finding the Command Prompt (pseudo DOS) on
> Windows ME. After 20 minutes, I located it under Programs, Accessories!!
>
> I then successfully generated a test signal (WAV file) and 'received' it 100%
> as per the instructions. So WOLF is easy after all.
>
> Now for the big test - real RF. Jim came up with his test transmission and I
> recorded it using Spectrogram but this didn't work. The problem seems to be
> that WOLF needs a sample rate of 8kb, and Spectrogram doesn't do this rate.
> An hour later, I used Cool Edit (a nice program) to generate a usable WAV
> file of Jim's signal.
>
> Several hours later I gave up, having failed to read anything at all from Jim.
>
> Possible causes: Jim's signal is very strong so possible sound card level
> problem. Also I may have been a long way off frequency (see below). Will test
> further tonight.
>
> Getting the correct audio frequency proved difficult and I only fixed it this
> morning after breakfast. I can use BBC 198kHz to calibrate Argo to measure
> a 136kHz signal to much better than 1Hz, but could not find an easy way of
> measuring 800Hz!! First I believed the Argo readout at 800Hz, but later tests
> showed this to be a long way out (this is not a complaint against Argo). I
> finally listened to DBF38 on AM and beat my DDS against it, then used the
> resultant 800Hz beat note to calibrate Argo. Later I found the offset facility
on
> my IC-706. This sets the audio frequency for comfortable CW reception -
> normally about 400Hz. Setting this to 800Hz gave me 800Hz audio to within
> half a Hertz with the RF dial set to the correct frequency. Now why didn't I
> think of that in the first place?
>
> Some thoughts on WOLF:
>
> It looks very useful and I think it may well be the mode for the 2001/2002 DX
> season (though I will still run CW and QRSS).
>
> The command line is hard work and needs a lot of interpretation. I am sure
> there are programmers out there who could provide an easy display with
> 'switches' and 'dials', and some automation of the variables to optimise
> reception.
>
> Transmit is a bigger problem if you cannot generate high power SSB at
> 136kHz. Jim has cracked the problem with his Decca (Class D), and I look
> forward to him publishing his modulator circuit. His signal is VERY clean with
> me only a few km away.
>
> We will need to devise a protocol for QSOs.
>
> We will also need to find a way of having 'random' QSOs. At present the
> frequency must be known accurately in advance and monitored for a very
> long time. This is not viable if you don't know there is someone transmitting.
>
> I find WOLF fascinating and challenging, whilst - at least on receive - not
> needing huge amounts of work to get going.
>
> I hope Jim will continue his test transmissions to get more people set up.
>
>
>
> Mike, G3XDV (IO91VT)
> http://www.lf.thersgb.net
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: MarkusVester@aol.com
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Date: Tue, 20 Mar 2001 19:38:23 EST
Subject: LF: Loran DX
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Hi Wolf and all,

triggered by John VE1ZJ's recent remarks on Loran as a skywave propagation 
monitor, a couple of weeks ago I took a deeper look at what could be 
received. John's "www.G4CNN.f2s.com/Loran_lines.htm" pointed me to the list 
at "www.megapulse.com/table.html". With this at hand I tried to identify the 
lines I could see on Argo around 100.0 kHz.

The key to their frequencies is the "GRI" (group repetition interval), which 
is the number of 10us carrier periods between two repetitions of the 
modulating pulse groups. Each group consists of 9 or 8 pulses, 1 ms apart. 
Some of these pulses have an alternating phase, so that the periodicity of 
the pattern is actually two times the GRI:
   Master       Secondary 
 ++--+-+- +     +++++--+ 
 +--+++++ -     +-+-++--
Thus the frequency spacing of the lines is Df = 100kHz/(2*GRI), eg. 
100kHz/(2*7499) = 6.6676 Hz for the Sylt chain. The Loran-C carrier frequency 
is generated by atomic clocks and claimed to be accurate on the order of 
10^-13.

The chains I could clearly observe here were

GRI     Df      Chain  (Wolf's AM line)
/10us  /Hz 
5930  8.4317  Canadian East Coast
6731  7.4283  Lessay   
7001  7.1418  Bo  (140*Df = 999.8572 Hz)
7030  7.1124  Saudi Arabia S
7270  6.8776  Newfoundland East Coast
7499  6.6676  Sylt  (150*Df = 1000.1334 Hz)
8000  6.2500  Western Russia  (160*Df = 1000.000 Hz)
8830  5.6625  Saudi Arabia N
9007  5.5512  Eide

Then there were additional weak lines which were too close to 100 kHz, at 
offsets of 1.52, 3.04 and 4.56 Hz. Their explanation is a little more subtle: 
Many loran stations are "dual-rated", they transmit in two chains with 
different GRI's. In case of a collision between two pulses that would have to 
be sent simultaneously, one of the pulses is simply left out. These dropped 
pulses occur at the beat frequency between the two GRI's. For the Sylt 
station, these "intermodulation" lines are multiples of 
(100kHz/6731-100kHz/7499) = 1.5215Hz.

There were even more lines I could not identify, eg. on 5.14, 5.90, 7.24, 
8.18, 8.95 Hz. This made me wonder if the table is really complete, as stated 
by megapulse. Also, I can't explain Wolf's observed 999.96 Hz.

The fun got even more interesting when I went to time domain. Using a 
programmable divider clocked by 100 kHz, I generated 2*GRI trigger signals 
for a digital oscilloscope in 128-averaging mode, and viewed the SSB output 
tuned to 100.0 kHz zero beat  (thus allowing phase-sensitive averaging). With 
this setup I could see the individual pulse groups of distant chains grow out 
of the noise, identify their stations and measure the time-differences. These 
matched calculated great-circle distances with a surprising accuracy of less 
than 100us, and it even worked fine for all five of the Saudi-Arabian 
stations, up to 4642 km from here.

Thus I think that Loran-C can be used not only as a precise frequency and 
time standard, but also as a powerful instrument for worldwide LF propagation 
monitoring, aided by its ability to resolve propagation delays. 

73s and happy experimenting
de Markus, DF6NM


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <00b401c0b18b$a189b160$0301a8c0@steve>
From: "Steve Olney" <ollaneg@zeta.org.au>
To: rsgb_lf_group@blacksheep.org
References: <e8.121dea87.27e920b6@aol.com>
Subject: LF: Re: TECH: Loran signals received in AM as audio reference ?
Date: Wed, 21 Mar 2001 09:17:57 +1100
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<DIV><FONT face=Arial size=2>G'day Wolf,</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I have been using this technique for some time now 
with no problems.&nbsp;&nbsp; The difference is I having been using the 1000Hz 
time pips from a local time and frequency station (VNG - 2.5MHz).</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>As long as you stick to the "standard" sample rates 
of 11025Hz, 22050Hz and 44100Hz then the sample rate will be pretty much as 
accurate as normal xtal oscillator (usually +/-100ppm).&nbsp;&nbsp;&nbsp; This 
means there is no ambiguity (trying to decide which peak is the correct one) as 
+/-100ppm is +/-0.1Hz @ 1000Hz.&nbsp;&nbsp;&nbsp; There is more than one peak 
because the pips vary from a 50mS burst to a 500mS burst producing varying 
relative amplitudes of the 1 second sidebands.&nbsp;&nbsp;&nbsp; The result is a 
peak at 1000Hz, 1001Hz, 1002Hz....&nbsp; (and going down 999Hz. 998Hz, 
997Hz...).&nbsp;&nbsp;&nbsp; But as long as your card is within +/-500ppm then 
you just pick the nearest one to 1000Hz.&nbsp;&nbsp;&nbsp; I have found that on 
many signals the "biggest" one may not be the correct one, so be careful with 
trying to sort out the correct one using Loran lines as they appear to be spaced 
by 0.1Hz.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Doesn't WWV or other time frequency stations have 
pips (maybe not 1000Hz).&nbsp;&nbsp; </FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>8000Hz is a "semi-standard" frequency so it may 
follow the same behaviour.</FONT></DIV>
<DIV><FONT face=Arial size=2></FONT>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>BTW, for those doing programming, avoid any 
"non-standard" sampling frequencies (I can't say one way or another about 8000Hz 
- simply that the error on my laptop at 11025Hz is +53ppm, while the error at 
8000Hz is +300ppm) as I have found that, for example, using 5500Hz can be a 
disaster for anything other than a 100.000% soundblaster soundcard.&nbsp;&nbsp; 
On my VFSKCW program I have had reports ranging from mild inaccuracies to a 
factor of 6 !!!! in output frequency.&nbsp;&nbsp;&nbsp; It seems to be fairly 
common on laptops because they don't have soundblaster cards.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>You might be interested in some measurements I did 
using this technique a couple of years back.&nbsp;&nbsp; They are still relevant 
to me as I still have the same gear :-)</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Go to: -</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2><A 
href="http://www.qsl.net/vk2zto/ExpModes/freqaccstab.htm">http://www.qsl.net/vk2zto/ExpModes/freqaccstab.htm</A></FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2><BR>73s Steve Olney (VK2ZTO/AXSO - QF56IK : Lat -33 
34 07, Long +150 44 
40)<BR>=============================================<BR>HomePage URLs:<BR><A 
href="http://www.qsl.net/vk2zto">http://www.qsl.net/vk2zto</A><BR><A 
href="http://www.zeta.org.au/~ollaneg">http://www.zeta.org.au/~ollaneg</A></FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Containing:-<BR>ULF, ELF, VLF &amp; LF 
Experimentation<BR>InfraSonic Experimentation<BR>Laser Comms DX<BR>Amateur Radio 
Astronomy<BR>=============================================</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Rabson" <word.factory@zetnet.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <7677381.985113404895.JavaMail.imail@zero.excite.com>
Subject: Re: LF: Re: WOLF  - am I missing something ?
Date: Tue, 20 Mar 2001 22:02:40 -0000
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----- Original Message -----
From: john sexton <computernetworks@excite.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, March 20, 2001 6:36 PM
Subject: Re: LF: Re: WOLF - am I missing something ?


>
> Hi Guys,
> I have been rather quiet lately due to work pressure. The job that I have
> been asked to do has required me to get up to speed on the latest 32-bit
> Windows SDK and DDKs.
> You would not believe how complicated it has now become! I have piles and
> piles of CDs from Microsoft.
> For Amateurs (i.e. non-paid professionals, who cannot afford the degree of
> investment required) I would recommend steering away from Windows (perhaps
> to Linux?). I have a distinct feeling that Microsoft is a latter-day Pied
> Piper.
> We were taught to apply a principle known as KISS. The latest Windows
looks
> more like the kiss of death for software productivity.
> 73, John, G4CNN
It was suggested recently that, instead of Microsoft being dismembered they
should be required to fix the bugs in their current product range. (but
doesn't the US constitution forbid cruel and unusual punishment?)

73 de
John Rabson G3PAI




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
Subject: RE: LF: Transatlantic Challenge: the Canadian / Europe contacts
Date: Tue, 20 Mar 2001 22:12:23 -0000
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I guess I've been working too much ......

John
G3WKL

-----Original Message-----
From: majordom@post.thorcom.com [mailto:majordom@post.thorcom.com]On
Behalf Of Walter Blanchard
Sent: Thursday, March 15, 2001 08:13
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Transatlantic Challenge: the Canadian / Europe contacts


At 21:43 14/03/01 Wednesday, John Gould wrote:
>............................(once and if the FAA agree to licence the band
>for amateur usage in the USA).

Apart from congratulating all concerned,
I hope you meant the FCC. The
Federal Aviation Authority might take a
very long time dealing with a ham radio
matter!!

Walter G3JKV






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From: DL4YHF@aol.com
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Date: Tue, 20 Mar 2001 16:08:06 EST
Subject: LF: TECH: Loran signals received in AM as audio reference ?
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hello group,
<BR>
<BR>I just thought about an audio frequency reference for all who don't have an 
<BR>accurate audio reference but a longwave receiver (like myself..)
<BR>In one of his recent postings Jim 'BMU explained why such a reference is 
<BR>required for the WOLF experiments. There MAY (!) be an easy solution to this, 
<BR>maybe the experts can help to verify the following.
<BR>
<BR>Here is what to do:
<BR>1.) Tune the LF RX to 100.00 kHz and set the receiver to AM (not SSB !)
<BR> &nbsp;&nbsp;&nbsp;&nbsp;You should hear Loran's sharp "clicketiclick" sound in the receiver.
<BR> &nbsp;&nbsp;&nbsp;&nbsp;The "clicketiclick" is a mixture of a lot of many audio frequencies,
<BR> &nbsp;&nbsp;&nbsp;&nbsp;and because we are using an AM RX the frequencies do NOT depend
<BR> &nbsp;&nbsp;&nbsp;&nbsp;on the accuracy of the VFO in the receiver (crude explanation...)
<BR>2.) Record a spectrogram with ARGO, SpecLab or whatever you use.
<BR> &nbsp;&nbsp;&nbsp;&nbsp;Use a &nbsp;high resolution, at least 0.01 Hz &nbsp;(the attached screenshot,
<BR> &nbsp;&nbsp;&nbsp;&nbsp;LORAN_AM.JPG, has 0.002 Hz resolution and took 6 minutes).
<BR>3.) Look at the audio frequencies close to 1kHz. There are lines visible at
<BR> &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;999.85 Hz
<BR> &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;999.96 Hz
<BR> &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;1000.00 Hz
<BR> &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;1000.13 Hz &nbsp;(the strongest in the range 999 - 1001 Hz)
<BR>Note: The spectrum has been recorded in the midwestern part of DL (JO42FD), 
<BR>and the amplitude of the spectra may be different in other parts of Europe 
<BR>but the lines should be detectable everywhere.
<BR>
<BR>I think this could be a way to verify the accuracy of ANY audio recording 
<BR>tool (for the last fractions of a Hertz), no matter if a soundcard, DSP, 
<BR>PIC-based converter or whatever is used.
<BR>
<BR>There has been a list of Loran frequencies on this reflector a few months ago 
<BR>(sh.., I didn't save it). Maybe one of the experts can calculate the accurate 
<BR>frequencies contained in an AM-received Loran signal on 100kHz, or one of the 
<BR>lucky fellows with a high-precision audio source can repeat the experiment 
<BR>described above to check the results.
<BR>
<BR>Thanks,
<BR> &nbsp;&nbsp;73 from Wolf (DL4YHF).
<BR>
<BR>
<BR>
<BR>
<BR> &nbsp;&nbsp;&nbsp;
<BR></FONT></HTML>

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bzTTeb9qvFJPONNk5Hp196U/DiYgD7TdgD/qGyf412tFafX8Tdvm38l/kLkRwP8Awq2b7X9o
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2T/Gll+G08kDRC7uxkEZ/s2T/Gu3oqvr2Itbm/BByo83f4QzOoH9o3g9T/ZUnP61qj4dzBQP
tN2cf9Q2T/GuzoqKWKrUW3B2v6DcU9zh5vhpNLGVF3eLkEZ/s2T/ABp1v8N5oFAN1dtjv/Zs
g/rXbUVax2IU+dS19F/kLlRxMvw3llYk3N2M/wDUNk/xpkfwyeMEC5u+Tn/kGSf413NFDx2I
cuZy19F/kHKjH8I+GZvDdsLTNzOpllmaWS0eIKDCVxzx1A7962KKK5G7u7KP/9k=
--------------040100070809080003050406--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Vernall" <vernall@xtra.co.nz>
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References: <3.0.1.16.20010320161213.2b1f2852@mail.cc.kuleuven.ac.be> <3AB77A23.971D3F4E@usa.net>
Subject: LF: Re: Re: WOLF  - am I missing something ?
Date: Wed, 21 Mar 2001 07:56:47 +1200
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> > Unfortunately the Windows designers decided that they were next in line
> > after God and that the simple guys writing software had no longer the
right
> > to access all these 'goodies' ...
>
> Your knowledge of the mind attitude of the Windows designers is very
approximate.
> They never thought, never for a while, that God was before them....

Windows inevitabley involves several panes.

73, Bob



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Klaus von der Heide" <v.d.heide@on-line.de>
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Subject: Re: LF: Re: RE PICs and DDS etc.
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Hello Alberto, hello all,

> I thought again and, yes, the high order bit of the phase accumulator is not
> the squared up version of the sine output, but, after the phase accumulator,
> a DDS has a sine lookup ROM. What I really meant was the high order
> bit of the output of this ROM. Using this bit, I feel confident to state again
> that you don't need a DAC to generate a square wave of the wanted frequency.
> 
> With the AD9850 you have to use the comparator, as you do not have external
> access to the output of the sine ROM.
> You are right saying that a PIC probably doesn't have enough horse power
> for this task. Maybe some chips  of the Scenic family ???

The problem is the discrete time the DDS uses. The high order bit 
only changes at the clock edges. The result is a square wave with 
heavy phase jitter.  For example, draw a sine wave (3 waves), 
sample it at about 8/3 of its frequency in your sketch, and generate 
the square wave from these sample values (all on the paper). 
The one-periods and the zero-periods then are one or two clock cycles 
long. That's what Andy in other words already said.
If a DAC is used then time is continuous and a clean square wave can 
be obtained. 

73 de Klaus, DJ5HG





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>
Organization: University of Hertfordshire
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Subject: LF: <Tech> DOS/Windows and PC clocks
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Dear LF Group,

Although it may be possible to access the PC's internal clocks one 
way or another, I can't see it would be much help for timing 
accuracy - after all, it's all derrived from a very ordinary, un-
trimmed crystal on the motherboard somewhere.

I did some work at U of H a while ago with Dave Lauder, G0SNO, 
investigating PC clocks. In fact, a lot of PCs (and other things) are 
now using 'dithered clocks', where the clock is frequency 
modulated to a deviation of a fraction of a percent, by a spiky 
looking triangle wave. The reason for doing this is to spread 
radiated noise emissions from the PC over a wider range of 
frequencies, which in turn reduces the noise power seen by a 
narrow band EMC receiver when noise emissions testing is being 
performed. This slightly perverse idea is basically a fiddle to allow 
PC's to generate more RF noise, while still passing the EMC 
regulations. It saves the manufacturers some money on screening 
and filter components. I'm sure it does not do much for timing 
accuracy, though!

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 sexton" <computernetworks@excite.com>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re: WOLF  - am I missing something ?
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Hi Guys,
I have been rather quiet lately due to work pressure. The job that I have
been asked to do has required me to get up to speed on the latest 32-bit
Windows SDK and DDKs.
You would not believe how complicated it has now become! I have piles and
piles of CDs from Microsoft.
For Amateurs (i.e. non-paid professionals, who cannot afford the degree of
investment required) I would recommend steering away from Windows (perhaps
to Linux?). I have a distinct feeling that Microsoft is a latter-day Pied
Piper.
We were taught to apply a principle known as KISS. The latest Windows looks
more like the kiss of death for software productivity.
73, John, G4CNN





_______________________________________________________
Send a cool gift with your E-Card
http://www.bluemountain.com/giftcenter/




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: DL4YHF@aol.com
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Date: Tue, 20 Mar 2001 13:06:01 EST
Subject: Re: LF: DFCW
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hello Rik and others,
<BR>
<BR>Rik wrote
<BR>&gt; 1. Using DCF77 (or similar) and the appropriate software (such as provided
<BR>&gt; by DL4YHF) one can set the PC clock with a 1/10 second accuracy. 
<BR>&gt; Even by
<BR>&gt; setting the PC clock by hand an accuracy of better than 1 second can be
<BR>&gt; achieved. So the PC's at both sides (TX and RX) can have their clock
<BR>&gt; 'synchronized' at 1 second or better.
<BR>
<BR>Well, the DCF77 decoder was a nice experiment, but not too much more than 
<BR>that.
<BR>The problem is, PC clocks (though called 'Real Time Clocks') can be quite 
<BR>bad, much worse than the cheapest wristwatch you can buy in a coffee-store. 
<BR>So setting the clock for an accuracy of 0.1 sec or better only lasts for a 
<BR>few MINUTES (!) on some nasty PCs (like the one I have to use sometimes). 
<BR>What really helps would be a GPS (costly, only works if satellites visible) 
<BR>or a cheap DCF receiver connected to the serial port (if not already occupied 
<BR>by mouse, modem, PIC, TRX control, DSP board etc etc).
<BR>You have to readjust the clock continously, if you want 'reliable' second 
<BR>markers for recording intervals of an hour or so. A possible workaround would 
<BR>be using the soundcards "calibrated" sample rate as a timebase.
<BR>
<BR>I once implemented such "time marker lines" in Spectrum Lab (configurable 
<BR>from 1 sec per line to several minutes) but that feature seems to be hidden 
<BR>too deep in the configuration dialog hi. Anyway, you may try it to check how 
<BR>fast the PC clock 'runs away' from the DCF-signal observed with a fast 
<BR>scrolling waterfall (by the way, a nice experiment comparing the clock pulses 
<BR>from DCF and MSF).
<BR>
<BR>Sorry abt my latest posting - it has a redundancy of exactly 100 percent !
<BR>
<BR>73's Wolf.
<BR>
<BR>
<BR>
<BR>
<BR></FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alberto di Bene" <dibene@usa.net>
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> NO Think again, the high order bit of a DDS output is very definitely
> not a squared up version of the fundamental !  Used on its own it would
> have a spectrum not totally unlike noise.

I thought again and, yes, the high order bit of the phase accumulator is not
the squared up version of the sine output, but, after the phase accumulator,
a DDS has a sine lookup ROM. What I really meant was the high order
bit of the output of this ROM. Using this bit, I feel confident to state again
that you don't need a DAC to generate a square wave of the wanted frequency.

With the AD9850 you have to use the comparator, as you do not have external
access to the output of the sine ROM.
You are right saying that a PIC probably doesn't have enough horse power
for this task. Maybe some chips  of the Scenic family ???

And, while the AD983x may be inexpensive, they are nevertheless SMD devices,
not particularly easy to solder (what an understatement...!)

73  Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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References: <3.0.1.16.20010320155747.2b1f164c@mail.cc.kuleuven.ac.be> <3AB7787E.B8F6AD37@usa.net> <003501c0b157$80775830$0a00a8c0@ThreeLakes.ca>
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What the heck is a mudball/
 John VE1ZJ

Larry Kayser wrote:

> Greetings All:
>
> > > 3. If Alberto could adapt ARGO and let the 'time markers' also appear on
> > > exact multiples of 30 seconds (or 1 minute etc..) and eventually replace
> > > the 'time ticks' at the bottom by thin vertical lines (over the entire
> > > window) then the RX would also have the required 'time synchronisation'
> :
> > > 'key up' or 'key down' of the TX would be at the same time when a 'time
> > > marker' appears on the ARGO screen.
>
> Well if your going this far why not ad real time as an optional alternative?
> Connect the INVERTED 1 PPS output from a GPS receiver to the RI line in
> RS232 and use the RI interrupt to make the timing coherent to a rather
> excellent and free standard available everywhere on this mudball.
>
> RI (Ring Indicate) is available on dB-25 Pin 22, and DB-9 Pin 9.
>
> Larry
> VA3LK



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From: DL4YHF@aol.com
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Date: Tue, 20 Mar 2001 12:26:10 EST
Subject: TECH: Re^2: LF: WOLF - am I missing something ?
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hi &nbsp;Andy, &nbsp;Rik, and others,
<BR>
<BR>A kind of "microtimer" is still there, no matter if you write your programs 
<BR>in Delphi, C++Builder or any of Microstuff's Visual something. 
<BR>The routine is called "QueryPerformanceCounter", it returns a 32 bit integer 
<BR>value of a 'hardware timer' which ticks with a certain frequency ("ticks per 
<BR>second"). The frequency of this timer can be detected by calling 
<BR>"QueryPerformanceFrequency", it returns a value 1193180 which may sound 
<BR>familiar to many DOS freaks. In fact, this timer seems to be clocked by the 
<BR>1.193 MHz counter which was already present in the very first IBM PC.
<BR>
<BR>Apart from that, I totally agree with your comments about DOS vs Windows. 
<BR>Most of the REAL goodies are not acessable, or only with extreme 'red tape' 
<BR>(thinking about soundards, interrupts, I/O-ports &nbsp;- sigh !)
<BR>
<BR>73, Wolf DL4YHF.
<BR>
<BR>
<BR>
<BR>
<BR></FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: Re: DFCW
In-reply-to: <003501c0b157$80775830$0a00a8c0@ThreeLakes.ca>
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Hi Larry,

That would be good to use 'time synchronized' DFCW (or QRSS) at higher
speeds (well ... 'high' means 3 sec./dot or so). But for 30 sec./dot the
internal PC clock (if set correct) will do the job.

But if there is any interest to use a GPS receiver (or any other timer
source) for synchronisation I am willing to see if I can adapt QRS.

73, Rik ON7YD

At 11:04 20/03/01 -0500, you wrote:
>Greetings All:
>
>> > 3. If Alberto could adapt ARGO and let the 'time markers' also appear on
>> > exact multiples of 30 seconds (or 1 minute etc..) and eventually replace
>> > the 'time ticks' at the bottom by thin vertical lines (over the entire
>> > window) then the RX would also have the required 'time synchronisation'
>:
>> > 'key up' or 'key down' of the TX would be at the same time when a 'time
>> > marker' appears on the ARGO screen.
>
>Well if your going this far why not ad real time as an optional alternative?
>Connect the INVERTED 1 PPS output from a GPS receiver to the RI line in
>RS232 and use the RI interrupt to make the timing coherent to a rather
>excellent and free standard available everywhere on this mudball.
>
>RI (Ring Indicate) is available on dB-25 Pin 22, and DB-9 Pin 9.
>
>Larry
>VA3LK
>
>
>
>
>


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 20 Mar 2001 17:12:36
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: WOLF  - am I missing something ?
In-reply-to: <3AB77304.B462970E@usa.net>
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Alberto,

I do some PIC programming, if you give me some more details about what you
want to be done I will can give it a try.
About direct output on 137kHz, a PIC can run up to 0.2us clock (5MHz), so
whatever you want do do, you have only abt. 35 clock cycles. Fortunately
PIC works with RISC commands so most commands take only 1 cycle ('jumps'
take 2 cycles.

73, Rik  ON7YD

At 16:11 20/03/01 +0100, you wrote:
>>  Then I abandonned software
>> timing by using an external interface (a PIC) on the serial port and
>> ended up with something very similar to the VE2IQ I/F.
>>
>
>A few days ago I was thinking on how to generate a programmable
>frequency for an MFSK scheme (I did post a message on this reflector),
>and the DDS was one the possibilities. Thinking again at it, after all we
just
>need the high order bit of the phase accumulator, as the TX is driven with a
>square wave. This makes the DAC completely unnecessary.
>Would it be possible then to implement a 32-bit phase accumulator with
>a PIC, to generate a frequency on the 137 kHz band ?
>My knowledge of PICs is quite limited, any PIC guru with an answer ?
>If positive, then it would be possible to make a really inexpensive outboard
>generator for such an MFSK modulation scheme.
>
>73  Alberto   I2PHD
>
>
>
>


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE PICs and DDS etc.
Date: Tue, 20 Mar 2001 16:07:36 -0000
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NO Think again, the high order bit of a DDS output is very definitely
not a squared up version of the fundamental !  Used on its own it would
have a spectrum not totally unlike noise.

Before the DDS output anti-allias filter, for a given output frequency
all terms of   Fclock +/- Fout are present, as sampled sinewaves with a
SIN(X) / X amplitude roll-off.   Also present is what effectively is
quantising noise (Nq) .   The level of this  Nq is given approximately
by  6.N dBc, so for a 12 Bit D/A in the DDS (as in the AD9850),   Nq can
only be 72 dB down at most.   In fact the manufacturers clain about
65dBc to play safe.   Just using the MSB gives 1 bit quantisation so
spurious products will be at 0 - 6dBc.    To generate a square wave, you
have to generate a proper sinewaveform, low pass filter and feed back
into a high speed comparator.  The AD9850 has such a comparator built in
and all you have to supply is a Clock, command word and output filter.

I once looked at using a PIC plus external D/A for a low speed DDS, and
for audio freqs it could be done, but again with spurious limitiations.
Assuming 8 bit arithmetic - any more would slow it down considerably and
you do need a sine look up table with this resolution as well - the
output could only manage around -40dB spurious and determining timing
would be a horrendous programming job.  A 32 bit accumulator with the
attendant maths all within a critical timing loop.

For MFSK, why not just use a DDS chip / module and send it commands to
set the frequency.   Some of the the now obsolete DDS chips such as
AD9831 and AD9832 can cost not much more than a PIC .

Andy  G4JNT


> -----Original Message-----
> From: Alberto di Bene [mailto:dibene@usa.net]
> Sent: 2001-03-20 15:11
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: WOLF - am I missing something ?
> 
> 
> >  Then I abandonned software
> > timing by using an external interface (a PIC) on the serial port and
> > ended up with something very similar to the VE2IQ I/F.
> >
> 
> A few days ago I was thinking on how to generate a programmable
> frequency for an MFSK scheme (I did post a message on this reflector),
> and the DDS was one the possibilities. Thinking again at it, 
> after all we just
> need the high order bit of the phase accumulator, as the TX 
> is driven with a
> square wave. This makes the DAC completely unnecessary.
> Would it be possible then to implement a 32-bit phase accumulator with
> a PIC, to generate a frequency on the 137 kHz band ?
> My knowledge of PICs is quite limited, any PIC guru with an answer ?
> If positive, then it would be possible to make a really 
> inexpensive outboard
> generator for such an MFSK modulation scheme.
> 
> 73  Alberto   I2PHD
> 
> 
> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <003501c0b157$80775830$0a00a8c0@ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010320155747.2b1f164c@mail.cc.kuleuven.ac.be> <3AB7787E.B8F6AD37@usa.net>
Subject: LF: Re: Re: DFCW
Date: Tue, 20 Mar 2001 11:04:48 -0500
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Greetings All:

> > 3. If Alberto could adapt ARGO and let the 'time markers' also appear on
> > exact multiples of 30 seconds (or 1 minute etc..) and eventually replace
> > the 'time ticks' at the bottom by thin vertical lines (over the entire
> > window) then the RX would also have the required 'time synchronisation'
:
> > 'key up' or 'key down' of the TX would be at the same time when a 'time
> > marker' appears on the ARGO screen.

Well if your going this far why not ad real time as an optional alternative?
Connect the INVERTED 1 PPS output from a GPS receiver to the RI line in
RS232 and use the RI interrupt to make the timing coherent to a rather
excellent and free standard available everywhere on this mudball.

RI (Ring Indicate) is available on dB-25 Pin 22, and DB-9 Pin 9.

Larry
VA3LK





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>
Organization: University of Hertfordshire
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Subject: LF: Wolf Tests
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Dear LF Group,

Thanks for the reports and comments. Some pointers to receiving 
WOLF mode BPSK-

The receive audio must be recorded at 8000 samples/sec., mono. 
DL4YHF's Spectrum Lab can do this, and generate a spectrogram 
at the same time. WOLF can operate on up to about 25mins of 
sampled data; at about 1 megabyte per minute, the files are quite 
large. With a good SNR, only a few minutes recording is required, 
but more data is needed for low SNR.

In order to decode successfully, 3 parameters need to be set up 
correctly:

-The level: The signal must be about 20-40dB down on the full 
scale level of the soundcard- WOLF simply does not work properly 
with a strong signal. If everything else is OK, what you see is that 
the first 3 lines of output are correct, but the rest is gibberish. The 
low level can be achieved by reducing the RX gain, or post-editing 
with sound recorder software. If the signal is down in the noise, 
KK7KA says you should set the level so that the noise peaks are 
6dB below full scale.

- The soundcard sampling rate correction (-r switch); The 
frequency error due to the soundcard is often the biggest 
frequency error in the whole system (about 4.5Hz in my case). It 
varies with the particular soundcard, and the particular sample rate 
it is set to. It also upsets the timing of the decoding process. One 
way to determine the actual sample rate is to inject an accurately 
known audio frequency into the sound card, and measure the 
apparent frequency using the Wolf -m option; the sample rate is 
then (8000 x real frequency)/apparent frequency. Once 
determined, the correction seems to be stable. KK7KA describes 
the neccessary accuracy as being in the parts per million range for 
optimum performance, ie you are aiming for better than 0.1 
samples/second accuracy.

-The frequency offset (-f switch): This corrects for frequency errors 
in TX and/or RX tuning; it can be determined by receiving a signal 
of known frequency, and measuring the received audio frequency 
using the Wolf -m option again. This is perhaps less critical than 
the soundcard sampling rate error; about 0.1Hz or so is tolerable.

The obvious problem is how to determine the soundcard error, if 
you don't have a accurate audio frequency source. I used the 
reference output of my synthesiser divided doown to 1kHz (and 
filtered; a fairly clean sine wave seemed to be neccessary to avoid 
aliasing problems with the soundcard). You could use the RX audio 
out, but only if you knew what the RX frequency error was to within 
a small fraction of a Hz. The effect of having the wrong sampling 
rate is that the first few lines of decoding work OK, but after that 
you get gobbledygook, so trial and error is a possible, if time 
consuming method. I think a technique where you measure the 
difference between two audio output frequencies might work OK, 
but this needs some further work to check it out. 

All this is a bit of a pain, but once completed, Wolf seems to work 
straight away all the time.

I'm not sure about the effects of QRM on this signal - obviously, it 
has been designed to work with low SNR, but does it's 
performance with gaussian noise also apply to QRM such as 
carriers, or pulsed waveforms like mains noise and Loran?

I intend to run some more tests this evening, starting about 
2000utc, at about the 30mW ERP level for an hour or so. Later , I 
will be running the full 1W ERP for possible transatlantic reception, 
between at least 0000 - 0200utc. As before frequency will be 
137.500kHz. If anyone would like a different frequency, power 
level, time etc. please let me know.

Cheers, Jim Moritz
73 de M0BMU




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From: "Alberto di Bene" <dibene@usa.net>
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Subject: LF: Re: WOLF  - am I missing something ?
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> Unfortunately the Windows designers decided that they were next in line
> after God and that the simple guys writing software had no longer the right
> to access all these 'goodies' ...

Your knowledge of the mind attitude of the Windows designers is very approximate.
They never thought, never for a while, that God was before them....

73  Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alberto di Bene" <dibene@usa.net>
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Rik Strobbe wrote:

> [snip]
> 3. If Alberto could adapt ARGO and let the 'time markers' also appear on
> exact multiples of 30 seconds (or 1 minute etc..) and eventually replace
> the 'time ticks' at the bottom by thin vertical lines (over the entire
> window) then the RX would also have the required 'time synchronisation' :
> 'key up' or 'key down' of the TX would be at the same time when a 'time
> marker' appears on the ARGO screen.
> [snip]

I can make this a customizable option. I have build 127 in the works and will add

this requirement.

73   Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 20 Mar 2001 16:12:13
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: RE: Re: WOLF  - am I missing something ?
In-reply-to: <65AECDF1F89AD411900400508BFC869F9C03E6@pdw-mail-1.dera.gov .uk>
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Hi Andy,

In the 'dark ages' of DOS it was possible to 'reprogram' the DOS Hartbeat
interrupt to much shorter times (you had to take care of the timekeeping
yourself). This timer was very accurate and with a 40MHz 386 it was
possible to have an accurate timer at 20us intervals or so ...
Also direct acces of interrupts, serial and parallel ports etc... was
'peanuts' once you figured it out.

Unfortunately the Windows designers decided that they were next in line
after God and that the simple guys writing software had no longer the right
to access all these 'goodies' ...

(Break down the fences and we don't need Gates ...)

73, Rik

At 14:20 20/03/01 -0000, you wrote:
>PowerBasic (the language I use) does incorporate a "microtimer"
>instruction for measuring time to 1us so something has always been
>available in the underlying hardware in the PC,   via the same timer
>chip that generates sounds from the PC speaker.  
>
>However, it becomes inaccurate for intervals > 55ms as the timing
>function get messed up by the DOS Heartbeat interrupt at 18.2Hz.  Also
>(at least in PBasic) it cannot be used to set a delay, only for
>measuring an interval.    Back in the Dark Ages, I used  a FOR / NEXT
>loop with a fixed count, accurately timed this using the microtimer,
>then generated a calibration factor for subsequently using in the loop
>to generate software timings.   Once again this was upset every 55ms,
>but did work satisfactorily with a Pico Products 8 bit A/D on the
>printer port for first forays into DSP.  Then I abandonned software
>timing by using an external interface (a PIC) on the serial port and
>ended up with something very similar to the VE2IQ I/F.
>
>Andy  G4JNT
>
>
>> -----Original Message-----
>> From: Alberto di Bene [mailto:dibene@usa.net]
>> Sent: 2001-03-20 13:36
>> To: rsgb_lf_group@blacksheep.org
>> Subject: LF: Re: WOLF - am I missing something ?
>> 
>> 
>> > We all have to accept that doing any sort of accurate 
>> timing operation
>> > on a PC is futile - whether Soundacard, serial port or, 
>> even worse, by
>> > software timing.   Therefore some sort of external interface really
>> > should be used to resynchronise Tx and Rx data samples        .
>> 
>> Hmm, perhaps not all is lost. The Pentium II class CPUs and 
>> the Athlons
>> do have the so-called Performance Timer, an hardware timer
>> that can be queried through Windoze APIs, with resolution 
>> around 1 usec.
>> 
>> This however would rule out old Pentiums, 486 and the AMD K6, which do
>> not have that counter.
>> 
>> 73   Alberto   I2PHD
>> 
>> 
>> 
>
>
>-- 
>The Information contained in this E-Mail and any subsequent correspondence
>is private and is intended solely for the intended recipient(s).
>For those other than the recipient any disclosure, copying, distribution, 
>or any action taken or omitted to be taken in reliance on such information is
>prohibited and may be unlawful.
>
>


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 20 Mar 2001 16:11:00 +0100
From: "Alberto di Bene" <dibene@usa.net>
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>  Then I abandonned software
> timing by using an external interface (a PIC) on the serial port and
> ended up with something very similar to the VE2IQ I/F.
>

A few days ago I was thinking on how to generate a programmable
frequency for an MFSK scheme (I did post a message on this reflector),
and the DDS was one the possibilities. Thinking again at it, after all we just
need the high order bit of the phase accumulator, as the TX is driven with a
square wave. This makes the DAC completely unnecessary.
Would it be possible then to implement a 32-bit phase accumulator with
a PIC, to generate a frequency on the 137 kHz band ?
My knowledge of PICs is quite limited, any PIC guru with an answer ?
If positive, then it would be possible to make a really inexpensive outboard
generator for such an MFSK modulation scheme.

73  Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 20 Mar 2001 15:57:47
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: LF: DFCW
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At 14:03 20/03/01 -0000, G3AQC wrote:
>I experimented last night with slightly shorter dots- 25secs rather than my 
>usual 30. This reduced my total message time (for three repeats of G3AQC)
from 
>56mins to44mins,including CW ident. I want to get shorter times without 
>reducing readability and both Rik and Alberto are helping with this. I think 
>DFCW is the most effective of the simpler techniques and well worth 
>developing. Last nights results are very encouraging.

Hello group,

Laurie had been busy in 'time optimizing' DFCW, mainly by reducing the
'idle' gaps. At the very slow speeds used these days for TA tests one can
indeed win a fair ammount of time by avoiding idle times. 
The main function of the DFCW gaps is to improve the readability of DFCW in
case of a series of dashes or dots. Or otherwise said, it is some kind of
'time synchronisation'.

This 'time synchonisation' has proven to be usefull, mainly for the reason
that at the RX side you otherwise had to guess when a dot or dash started
and stopped. If the RX would know at what times the TX was keying this gaps
wouldn't be nessecary ...

At the dot lengths used in recent TA tests (30 to 120 seconds) it shouldn't
be so difficult to get sufficient 'time synchronisation' between TX and RX :

1. Using DCF77 (or similar) and the appropriate software (such as provided
by DL4YHF) one can set the PC clock with a 1/10 second accuracy. Even by
setting the PC clock by hand an accuracy of better than 1 second can be
achieved. So the PC's at both sides (TX and RX) can have their clock
'synchronized' at 1 second or better.

2. QRS (v3.05) allows you start keying on exact multiples of 30 seconds (or
1 minute, 2 minutes, 5 minutes etc...). Of course this only makes sense if
you set the dotlength also at 30 seconds (or 1 minute etc..). 
So the TX can be 'time synchronized'.

3. If Alberto could adapt ARGO and let the 'time markers' also appear on
exact multiples of 30 seconds (or 1 minute etc..) and eventually replace
the 'time ticks' at the bottom by thin vertical lines (over the entire
window) then the RX would also have the required 'time synchronisation' :
'key up' or 'key down' of the TX would be at the same time when a 'time
marker' appears on the ARGO screen.

Result : no more need for time gaps (what should be a 20-25% time saving).

73, Rik  ON7YD



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: <4736.200103191732@gemini> <3.0.1.16.20010320095838.2dbff988@mail.cc.kuleuven.ac.be>
Subject: LF: WOLF
Date: Tue, 20 Mar 2001 11:02:42 -0000
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Hi Rik


> >I downloaded Wolf but it would not run on any of the systems I have (DOS,
> >Win 3.11 and Win98). So unable to progress.

> I run WOLF under Win98. Try to open an MS-DOS window and start WOLF from
> there.

Thanks. Yes that did the trick. I must get the .wav file and see how it
goes.

Regards,
Peter, G3LDO

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

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




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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Re: WOLF  - am I missing something ?
Date: Tue, 20 Mar 2001 14:20:40 -0000
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PowerBasic (the language I use) does incorporate a "microtimer"
instruction for measuring time to 1us so something has always been
available in the underlying hardware in the PC,   via the same timer
chip that generates sounds from the PC speaker.  

However, it becomes inaccurate for intervals > 55ms as the timing
function get messed up by the DOS Heartbeat interrupt at 18.2Hz.  Also
(at least in PBasic) it cannot be used to set a delay, only for
measuring an interval.    Back in the Dark Ages, I used  a FOR / NEXT
loop with a fixed count, accurately timed this using the microtimer,
then generated a calibration factor for subsequently using in the loop
to generate software timings.   Once again this was upset every 55ms,
but did work satisfactorily with a Pico Products 8 bit A/D on the
printer port for first forays into DSP.  Then I abandonned software
timing by using an external interface (a PIC) on the serial port and
ended up with something very similar to the VE2IQ I/F.

Andy  G4JNT


> -----Original Message-----
> From: Alberto di Bene [mailto:dibene@usa.net]
> Sent: 2001-03-20 13:36
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: WOLF - am I missing something ?
> 
> 
> > We all have to accept that doing any sort of accurate 
> timing operation
> > on a PC is futile - whether Soundacard, serial port or, 
> even worse, by
> > software timing.   Therefore some sort of external interface really
> > should be used to resynchronise Tx and Rx data samples        .
> 
> Hmm, perhaps not all is lost. The Pentium II class CPUs and 
> the Athlons
> do have the so-called Performance Timer, an hardware timer
> that can be queried through Windoze APIs, with resolution 
> around 1 usec.
> 
> This however would rule out old Pentiums, 486 and the AMD K6, which do
> not have that counter.
> 
> 73   Alberto   I2PHD
> 
> 
> 


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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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Subject: LF: Re. LF Tests
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<DIV><FONT face=Arial size=2>Hi John,</FONT></DIV>
<DIV><FONT face=Arial size=2>Many thanks for your report. I was transmitting 
continuously from2130 until 0630utc.</FONT></DIV>
<DIV><FONT face=Arial size=2>I experimented last night with slightly shorter 
dots- 25secs</FONT></DIV>
<DIV><FONT face=Arial size=2>rather than my usual 30. This reduced my total 
message time (for three repeats of G3AQC) 
from&nbsp;56mins&nbsp;to44mins,including&nbsp;CW ident.&nbsp;I want to get 
shorter times without reducing readability and both Rik and Alberto are helping 
with this.I think DFCW is the most effective of the simpler techniques and well 
worth developing.Last nights results are very encouraging.&nbsp;I will be there 
again tonight from </FONT></DIV>
<DIV><FONT face=Arial size=2>2130. 73s Laurie.</FONT></DIV></BODY></HTML>

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> We all have to accept that doing any sort of accurate timing operation
> on a PC is futile - whether Soundacard, serial port or, even worse, by
> software timing.   Therefore some sort of external interface really
> should be used to resynchronise Tx and Rx data samples        .

Hmm, perhaps not all is lost. The Pentium II class CPUs and the Athlons
do have the so-called Performance Timer, an hardware timer
that can be queried through Windoze APIs, with resolution around 1 usec.

This however would rule out old Pentiums, 486 and the AMD K6, which do
not have that counter.

73   Alberto   I2PHD




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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: "LF Group \(E-mail\)" <rsgb_lf_group@blacksheep.org>
Subject: LF: WOLF  - am I missing something ?
Date: Tue, 20 Mar 2001 12:56:16 -0000
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<DIV><FONT face=Arial size=2><SPAN class=678124412-20032001>I've just been 
reading throught the documentation for Wolf and it all seems rather over 
complicated for an enhanced BPSK system - having to loop-play .WAV files through 
some kind of audio-RF interface.&nbsp; I</SPAN></FONT><FONT face=Arial 
size=2><SPAN class=678124412-20032001>sn't there a way of using the VE2IQ 
interface(s) for Wolf ?&nbsp;&nbsp;At one stroke this would remove all need for 
Soundcard and serial port data rates to be measured and calibration 
procedures.&nbsp;&nbsp;&nbsp; </SPAN></FONT></DIV>
<DIV><FONT face=Arial size=2><SPAN 
class=678124412-20032001></SPAN></FONT>&nbsp;</DIV>
<DIV><SPAN class=678124412-20032001>
<DIV><FONT face=Arial size=2><SPAN class=678124412-20032001>Reading the 
description it&nbsp;appears to be&nbsp;a 10b/s BPSK&nbsp;convolutionally encoded 
bitstream with FEC added.&nbsp;&nbsp; This surely lends itself to soft descision 
decoding which&nbsp;presumably is how the software works.&nbsp; But that is all 
software, the samples are in exactly&nbsp;the same form as used by Bill's system 
?</SPAN></FONT></DIV>
<DIV><SPAN class=678124412-20032001></SPAN>&nbsp;</DIV>
<DIV><FONT face=Arial size=2><SPAN class=678124412-20032001>We all have to 
accept that doing any sort of accurate timing operation on a PC is futile - 
whether Soundacard, serial port or, even worse, by software timing.&nbsp;&nbsp; 
Therefore some sort of external interface really should be used to resynchronise 
Tx and Rx data samples.</SPAN></FONT></DIV>
<DIV><SPAN class=678124412-20032001></SPAN>&nbsp;</DIV>
<DIV><FONT face=Arial size=2><SPAN class=678124412-20032001>Andy&nbsp; 
G4JNT</SPAN></FONT></DIV>
<DIV><SPAN class=678124412-20032001></SPAN>&nbsp;</DIV>
<DIV><SPAN 
class=678124412-20032001></SPAN>&nbsp;</DIV></SPAN></DIV><CODE><FONT SIZE=3><BR>
<BR>
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Subject: LF: WOLF again
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G3LDO wrote:
 
>  When I run WOLF under Win 98 for a split
> second I get a small black window (similar to running DOS) but it
> disappeared so fast I wasn't able to read it. By repeated running I found
> that I hadn't included the .wav file (looking through the documentation,
> belatedly!, I see this is necessary).

Peter, the program is accessed via the "DOS" window, though it isn't a DOS 
application (confused? wait till you try to run the program!). This window tends 
to be hidden these days but try all the options from the START button until you 
find Command Prompt.

> I also understand that only off-line processing on receive is available.
> >From this I guess that what I should have done was to make a .wav file of
> Jim's signal and process it later. In the presence of QSB this could make a
> QSO a bit tricky.

At present only a pre-recorded file can be analysed - but this is an advantage 
in these early stages because you can keep readjusting the numerous 
parameters and re-checking the same signal until you have it optimised. I 
would hope that eventually all of this will be automated so that the computer 
can do all of the tedious work for you.

As for QSB, the whole point of WOLF is that it is better than QRSS in the 
presence of QSB. QRSS stretches the message over an hour or so which is 
fine so long as the signal stays up for long enough. WOLF, as I understand it, 
sends a fairly short message over and over again until it is received 
satisfactorily - in other words the integration is done in parallel, not in series 
{experts, please tell me if I have it wrong}. So you could take advantage of a 
10 minute peak in conditions to pass the message rapidly (whereas QRSS 
would still be sending slowly), or conversely you can ignore deep QSB 
because the receiver will find the signal again later.

> >From what I have read about WOLF it does appear to be a good system for
> extracting data from weak signals buried in the noise and if the claims are
> to be believed it has some dB improvement on QRSS systems.

I am still skeptical, but Jim's reception in the USA at only his first attempt 
indicates that there are real possibilities when everything is optimised.

> However, in my case very narrow band QRSS has the great advantage of being
> able to work between the very strong Loran lines received here.  QRSS and
> Argo now has given us a system of the utmost simplicity, which encourages
> lots of users. In addition it enables us to know what is going on around us
> and the ability to read several stations at a time in a very narrow
> bandwidth (a valuable asset in propagation studies).

Loran is listed as one of the potential problems. However, it is suggested that a 
software comb filter can be produced, and that the Loran lines can even be 
used to maintain frequency accuracy.

I agree that computer-only modes - as distinct from modes where the 
computer displays something the brain can interpret - leave the operator with 
a feeling of remoteness. I have already identified the problem that random 
QSOs will be almost impossible with WOLF. What would be useful would be to 
incorporate a spectrogram into any front-end software for WOLF. Thus you 
would be able to see what was going on, and perhaps someone looking for a 
WOLF QSO would send a string of 10s dashes (or Ws in QRSS?) before his 
transmission so that he could be identified and tuned to.

The important thing, I feel, is to spend some time this summer evaluating and 
refining this software, and operating practices, so that it is useful next winter.

For me, the ideal solution would be to have real-time WOLF, with an easy 
front-end, combined with the means to transmit and receive 
CW/QRSS/DFCW, all in one piece of software/hardware. This would avoid 
fragmenting the activity. It would also allow the best mode to be used for each 
set of circumstances.

Thanks to all concerned in developing WOLF. I am sure it will become a more 
friendly application. I still remember the first QRSS reception using 
Spectrogram when you needed a stopwatch to time the dots and dashes as 
the display was only a few seconds wide. I'll bet the first HF SSB QSO was 
hard work, too.



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi all I think last night the results from observing G3AQC 's signals
were significant. Firstly the condx were terrible. At times DCF39 was as
low as S-1. Typically it was S-2 toS-3.  128.9  had a max of S-4
typically S-3
       The K index was a 4 at 0000z last nite and a 6 at 0900z .  We had
widespread Au propagation on 144 mHz in both Eu es NA.  I had visible
Aurora at 0833Z here.
       G3AQC was "M" or "O" copy for most of the time between 2222Z and
0300z
      There was nil from Laurie at 0330, butI thought I could see G3AQC
at 0420"T" copy.  I am not sure of the last statement Please tell me
when you were transmitting last night Laurie.
      I wish we had had more experience with DFCW and 30 sec dots
during the trials with Jack.
     This shows rhat even with very adverse condx less than 1/2 w erp
can get across, a sign of great reliability.
     One strange thing. Last night , and on other occaisions when aurora
was visible, I have listened to 128.9 and DCF39. The flutter heard on
160 and 80 and 40 has never been observed on LF

73 de John VE1ZJ



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Subject: LF: Re: WOLF BPSK
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Hi Stewart

> I don't have Win98 myself, but several users have run WOLF under
> Win98 with no trouble.  Please send me the failing console output,
> or tell me what OS error message you are getting, and I'll try to
> diagnose the problem.

Thanks for the offer of help. When I run WOLF under Win 98 for a split
second I get a small black window (similar to running DOS) but it
disappeared so fast I wasn't able to read it. By repeated running I found
that I hadn't included the .wav file (looking through the documentation,
belatedly!, I see this is necessary).

I also understand that only off-line processing on receive is available.
>From this I guess that what I should have done was to make a .wav file of
Jim's signal and process it later. In the presence of QSB this could make a
QSO a bit tricky.

>From what I have read about WOLF it does appear to be a good system for
extracting data from weak signals buried in the noise and if the claims are
to be believed it has some dB improvement on QRSS systems.

However, in my case very narrow band QRSS has the great advantage of being
able to work between the very strong Loran lines received here.  QRSS and
Argo now has given us a system of the utmost simplicity, which encourages
lots of users. In addition it enables us to know what is going on around us
and the ability to read several stations at a time in a very narrow
bandwidth (a valuable asset 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: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 20 Mar 2001 10:24:11 -0000
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Subject: WOLF: Success and failure
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I tried out WOLF for the first time last night with total success.

Jim was sending GY(^%? JGGF, followed by H(*^RCKO KKl, followed by . . . . 

OK, so it wasn't quite as successful as I would have liked.

My first problem was finding the Command Prompt (pseudo DOS) on 
Windows ME. After 20 minutes, I located it under Programs, Accessories!!

I then successfully generated a test signal (WAV file) and 'received' it 100% 
as per the instructions. So WOLF is easy after all.

Now for the big test - real RF. Jim came up with his test transmission and I 
recorded it using Spectrogram but this didn't work. The problem seems to be 
that WOLF needs a sample rate of 8kb, and Spectrogram doesn't do this rate. 
An hour later, I used Cool Edit (a nice program) to generate a usable WAV 
file of Jim's signal. 

Several hours later I gave up, having failed to read anything at all from Jim.

Possible causes: Jim's signal is very strong so possible sound card level 
problem. Also I may have been a long way off frequency (see below). Will test 
further tonight.

Getting the correct audio frequency proved difficult and I only fixed it this 
morning after breakfast. I can use BBC 198kHz to calibrate Argo to measure 
a 136kHz signal to much better than 1Hz, but could not find an easy way of 
measuring 800Hz!! First I believed the Argo readout at 800Hz, but later tests 
showed this to be a long way out (this is not a complaint against Argo). I 
finally listened to DBF38 on AM and beat my DDS against it, then used the 
resultant 800Hz beat note to calibrate Argo. Later I found the offset facility on 
my IC-706. This sets the audio frequency for comfortable CW reception - 
normally about 400Hz. Setting this to 800Hz gave me 800Hz audio to within 
half a Hertz with the RF dial set to the correct frequency. Now why didn't I 
think of that in the first place?

Some thoughts on WOLF:

It looks very useful and I think it may well be the mode for the 2001/2002 DX 
season (though I will still run CW and QRSS).

The command line is hard work and needs a lot of interpretation. I am sure 
there are programmers out there who could provide an easy display with 
'switches' and 'dials', and some automation of the variables to optimise 
reception.

Transmit is a bigger problem if you cannot generate high power SSB at 
136kHz. Jim has cracked the problem with his Decca (Class D), and I look 
forward to him publishing his modulator circuit. His signal is VERY clean with 
me only a few km away.

We will need to devise a protocol for QSOs.

We will also need to find a way of having 'random' QSOs. At present the 
frequency must be known accurately in advance and monitored for a very 
long time. This is not viable if you don't know there is someone transmitting.

I find WOLF fascinating and challenging, whilst - at least on receive - not 
needing huge amounts of work to get going.

I hope Jim will continue his test transmissions to get more people set up.



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: rsgb_lf_group@blacksheep.org
Date: Tue, 20 Mar 2001 09:47:54 -0000
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Subject: Re: LF: lf transatlantic
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>  My belief is that we will be able to get through even during
> most of the summer.  i would like to continue testing throughout
> summer.  I do not think we need to have continuous beaconing.   Perhaps
> 20 minutes at top of hour from Eu and 20 min at bottom of hour from NA .
>          My sunset now is around 2200Z  so I don't start seeing Eu
> stations til 2130Z So no point in starting before 2130Z.   My sunset at
> summer solstice will be around 2345z So starting time then of 2315Z
> would be good .  Is anybody interested in continuing through summer?
>         73 all de John VE1ZJ

I am happy to continue testing during the summer, but to save effort/electricity 
would it be useful to reduce all-night sessions to, say, one night a week? 
Whilst this would obviously reduce the scope for hitting optimum conditions, it 
would concentrate activity so that both sides could assume that someone was 
transmitting/listening. 



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 20 Mar 2001 09:58:38
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: WOLF BPSK tests tonight
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>I downloaded Wolf but it would not run on any of the systems I have (DOS,
>Win 3.11 and Win98). So unable to progress.
>
>Regards,
>Peter Dodd

Hi Peter,

I run WOLF under Win98. Try to open an MS-DOS window and start WOLF from
there.

73, Rik  ON7YD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: WOLF BPSK tests tonight
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Hi Jim,

Sorry, I couldn't be QRV last night. 
Regarding power levels :
On a second thought it is OK for me if you run high power for the TA test.
I can reduce your SRN by receiving on a short piece of wire. If I keep the
wire indoor the household electronics will provide sufficient noise.
At a later stage it might be interesting to have a test sequence with
reduced power level for inter-EU testing, eventually during daytime (weekend).
Meanwhile it might be to know whe, beside Wolf end me, is equiped (and
interested) in WOLF tests (in Europe).

73, Rik  ON7YD


At 17:37 19/03/01 +0000, you wrote:
>Dear Wolf, Rik, LF Group,
>
>I will try some lower power WOLF BPSK tests tonight, starting 
>about 2000utc. Because different stations are experiencing widely 
>different signal levels, and since with weak signals the WOLF 
>software requires quite a long run of signal to successfully decode, 
>I will start off with big steps in power level every 20mins or so, so 
>we can determine roughly what levels will be interesting for future 
>tests. 
>
>I will start at the 300mW ERP level, and reduce power in 10dB 
>steps - say 30mW, 3mW, 300uW. At each step change I will 
>transmit the CW station ID and the ERP level for the next period, 
>followed by 3 minutes of carrier for frequency checking, all 
>transmitted at full power. Then I will reduce the TX power level and 
>start sending BPSK, until the next station ID. The frequency will be 
>137.500kHz again. I will listen on the frequency afterwards if 
>anybody wants to call in CW about the tests. At some time 
>between 2300 and 0000, I will start up again with the full 1W ERP 
>for the benefit of North American stations.
>
>I hope this is OK - let me know if you would prefer something 
>different!
>
>Cheers, Jim Moritz
>73 de M0BMU
>
>


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
Subject: LF: Re. lf Transatlantic.
Date: Tue, 20 Mar 2001 07:05:46 -0000
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<DIV><FONT face=Arial size=2>Hi John,</FONT></DIV>
<DIV><FONT face=Arial size=2>I didn't see your message last night, another lost 
opportunity!</FONT></DIV>
<DIV><FONT face=Arial size=2>I will have a look for Jack tonight. 73s 
Laurie.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Stewart Nelson" <sn@scgroup.com>
To: rsgb_lf_group@blacksheep.org
References: <4736.200103191732@gemini> <000201c0b0c8$76567820$6fe086d4@ericadodd>
Subject: LF: Re: Re: WOLF BPSK tests tonight
Date: Mon, 19 Mar 2001 18:37:59 -0800
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Hi Peter,

I don't have Win98 myself, but several users have run WOLF under
Win98 with no trouble.  Please send me the failing console output,
or tell me what OS error message you are getting, and I'll try to
diagnose the problem.

73,

Stewart KK7KA

----- Original Message ----- 
From: "g3ldo" <g3ldo@ukonline.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Monday, March 19, 2001 1:21 PM
Subject: LF: Re: WOLF BPSK tests tonight


> 
> Jim said
> > I will try some lower power WOLF BPSK tests tonight, starting
> > about 2000utc. .................
> 
> A really good signal here as might be expected at 2100
> 
> I downloaded Wolf but it would not run on any of the systems I have (DOS,
> Win 3.11 and Win98). So unable to progress.
> 
> Regards,
> Peter Dodd
> 
> 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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Subject: LF: Re: WOLF BPSK tests tonight
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Jim said
> I will try some lower power WOLF BPSK tests tonight, starting
> about 2000utc. .................

A really good signal here as might be expected at 2100

I downloaded Wolf but it would not run on any of the systems I have (DOS,
Win 3.11 and Win98). So unable to progress.

Regards,
Peter Dodd

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

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



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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re. lf Transatlantic.
References: <001401c0b0b3$73b8cf60$3414883e@g3aqc>
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Hi Laurie,&nbsp; I'm sure you could have QSO with VE1ZZ in about an hour
with you
<br>on DFCW as you transmit now es Jack on 3 sec dot QRSS
<br>&nbsp;&nbsp; 73 de John VE1ZJ
<p>Laurie Mayhead wrote:
<blockquote TYPE=CITE><style></style>
<font face="Arial"><font size=-1>John
I certainly will be around during the summer. Not every night but from
time to time. I want to keep on with DFCW possibly trying a bit shorter
dots,to see where the limit is.So reports will always be welcome. I am
sure a QSO is possible in one night,but it would mean staying up all night,something
which I find very difficult at my age Hi.</font></font></blockquote>

</body>
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Mar 2001 21:58:39 -0500
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Hi all the K index is a 4 .  I hope many will be transmitting tonight so
we can see how we do with disturbed condx 73 de John VE1ZJ



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
Subject: LF: Re. lf Transatlantic.
Date: Mon, 19 Mar 2001 20:29:56 -0000
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<DIV><FONT face=Arial size=2>John I certainly will be around during the summer. 
Not every night but from time to time. I want to keep on with DFCW possibly 
trying a bit shorter dots,to see where the limit is.So reports will always be 
welcome. I am sure a QSO is&nbsp;possible in one night,but it would mean staying 
up all night,something which I find very difficult at my age 
Hi.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Mar 2001 20:19:37 +0000
To: rsgb_lf_group@blacksheep.org
From: "Brian Rogerson" <brian@esoterica.pt>
Subject: LF: Jim's Frequency
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What is it please?

73, Brian
73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
http://homepage.esoterica.pt/~brian



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: <001601c0b0a6$034cd300$2c45893e@g3aqc>
Subject: LF: Re: Re. WOLF across the pond.
Date: Mon, 19 Mar 2001 15:09:58 -0500
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I'm enjoying the comments about WOLF.  Here are my own:

This is very much a work-in-progress. Stewart Nelson has kindly provided
workable software, a number of improvements, and much tech support to those
of us who have been playing with it. I have spent a LOT of time playing with
the receiving end, and have enjoyed it. Hopefully, in another year we'll be
chuckling about the old days of the command line interface, etc.

The goal, I believe, is to work on methods of completing 2-way QSOs in short
enough time to compete with changing band conditions. WOLF is one approach.
It is certainly not the most spectrum-efficient, and may not be the best way
of receiving down-in-the-mud signals. But it may, in a later version, be a
good approach to the 2-way problem.

Personally, I'm an old CW guy, and prefer that mode. The various flavors of
slow speed CW have been quite effective, and I've enjoyed chasing them. I'm
quite taken with Laurie's DFCW transmissions - they are quite easy to ID and
read.

So for now, I'm content to try to add to the common stock of knowledge, and
help those doing things like transmitting and software development to
improve their stuff.  And I've learned a lot in the process, which is never
a bad idea!

John Andrews, W1TAG



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Mar 2001 19:39:25 -0800
From: "John Currie" <john.currie@ns.sympatico.ca>
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Hi all ,  Just some thoughts.  I only have anecdotal evidence for what I
am about to write but anyway here are some feelings.   Since we went to
30 second dots I cant remember a night when I didn't see a UK station
here except when either
         1.  Nobody was transmitting   or
         2   I had severe 60 HZ pickup
                In other words the path between US es Nova Scotia  is
available to stations with erp of the order of Laurie's 0.3 watt or
better most of the time.  I have seen M0BMU or G3AQC  when 129.9 or
DCF39 were as weak as S-4.  Normally the 2 german stations are S-5 to
S-7  .  Last night at around  0400  128.9 was S-8 but G3AQC was weaker
than usual.  On at least one occaision M0BMU was received well even
though the K index was a 3.
            I feel the path is therefore quite reliable and QRSS with 30
second dots will produce QSOs more than half the winter nights.  Some
nights such as when I visited Jack'S house condx can be bad and even
Jack's signals are not reliable.  But even that night  we saw MM0ALM for
1/2 hour and I believe Jack would have been  at least "M" copy if he
were using 30 second dots rather than 3 sec dots.
           QRN doesn't seem to have much effect.  I have seen EU stns
through static crashes during snow storms that were 10 db over S-9 on
peaks.  During precipitation static caused by charged snowflakes all
sigs were wiped out.
          My belief is that we will be able to get through even during
most of the summer.  i would like to continue testing throughout
summer.  I do not think we need to have continuous beaconing.   Perhaps
20 minutes at top of hour from Eu and 20 min at bottom of hour from NA .

         My sunset now is around 2200Z  so I don't start seeing Eu
stations til 2130Z So no point in starting before 2130Z.   My sunset at
summer solstice will be around 2345z So starting time then of 2315Z
would be good .  Is anybody interested in continuing through summer?
        Last night had 60 Hz trouble only saw G3AQC
        73 all de John VE1ZJ



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
Subject: LF: Re. WOLF across the pond.
Date: Mon, 19 Mar 2001 18:53:28 -0000
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<DIV><FONT face=Arial size=2>Congratulations Jim another first! just wish I knew 
how it works.</FONT></DIV>
<DIV><FONT face=Arial size=2>For those intrested in old fashioned modes I will 
transmit again tonight DFCW. 73s All. Laurie.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Congratulations to John and Jim.  This is a fine achievement.  I would
like to point out ,however that 40 stations could transmit
simultaneously with QRSS and 30 second dots.

   73 de John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Wolf BPSK across pond
References: <5186.200103191301@gemini> <3.0.1.16.20010319183255.77e7b476@mail.cc.kuleuven.ac.be>
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Hi Rik I was pleased to see your email you will see that I have just sent one
with a proposal for testing throughout summer
73 de john VE1ZJ
Rik Strobbe wrote:

> >Congrats to John and Jim on this accomplishment. I'd like to also point out
> >that this successful reception took place on what, the first or second
> night of
> >transmissions ?
> >And in the middle of March!!
>
> Congrats are in order, but things have to be seen in perspective :
> - Jim has one of the strongest signals in Europe and his QRSS signals have
> been copied in the USA / Canada on an almost daily base.
> - transatlantic propagation has been excellent for the last week(s). CFH is
> booming in day and night (here in Belgium abt. 10dB stronger than in
> Octover/November) and modest stations (such as G3XDV) have made it across.
>
> Keeping in mind that the first succesfull transatlantic test was mid
> september, it might turn out that midwinter has not nessecarily the best
> propagation. I suggest to continue the transatlantic test until signals are
> gone.
>
> 73, Rik  ON7YD



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Date: Mon, 19 Mar 2001 18:32:55
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Wolf BPSK across pond
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>Congrats to John and Jim on this accomplishment. I'd like to also point out 
>that this successful reception took place on what, the first or second
night of 
>transmissions ? 
>And in the middle of March!!

Congrats are in order, but things have to be seen in perspective :
- Jim has one of the strongest signals in Europe and his QRSS signals have
been copied in the USA / Canada on an almost daily base.
- transatlantic propagation has been excellent for the last week(s). CFH is
booming in day and night (here in Belgium abt. 10dB stronger than in
Octover/November) and modest stations (such as G3XDV) have made it across.

Keeping in mind that the first succesfull transatlantic test was mid
september, it might turn out that midwinter has not nessecarily the best
propagation. I suggest to continue the transatlantic test until signals are
gone.

73, Rik  ON7YD




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>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org
Date: Mon, 19 Mar 2001 17:37:47 +0000
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Subject: LF: WOLF BPSK tests tonight
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Dear Wolf, Rik, LF Group,

I will try some lower power WOLF BPSK tests tonight, starting 
about 2000utc. Because different stations are experiencing widely 
different signal levels, and since with weak signals the WOLF 
software requires quite a long run of signal to successfully decode, 
I will start off with big steps in power level every 20mins or so, so 
we can determine roughly what levels will be interesting for future 
tests. 

I will start at the 300mW ERP level, and reduce power in 10dB 
steps - say 30mW, 3mW, 300uW. At each step change I will 
transmit the CW station ID and the ERP level for the next period, 
followed by 3 minutes of carrier for frequency checking, all 
transmitted at full power. Then I will reduce the TX power level and 
start sending BPSK, until the next station ID. The frequency will be 
137.500kHz again. I will listen on the frequency afterwards if 
anybody wants to call in CW about the tests. At some time 
between 2300 and 0000, I will start up again with the full 1W ERP 
for the benefit of North American stations.

I hope this is OK - let me know if you would prefer something 
different!

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Mar 2001 11:08:34 -0600
To: rsgb_lf_group@blacksheep.org,  rsgb_lf_group@blacksheep.org
From: "Les Rayburn" <les@highnoonfilm.com>
Subject: Re: LF: Wolf BPSK across pond
Cc: lowfer@qth.net
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At 01:06 PM 3/19/01 +0000, James Moritz wrote:
>Dear LF Group,
>
>I arrived at work this morning to find that:
>
> > Well, WOLF has successfully crossed the pond. Got two lines of clean
> > copy between 0135 and 0200 Z tonight (3/19 Z). Frequency was about 0.13
> > Hz below 137.5 kHz. Had to do some tweaking to get the copy. Those
> > command line switches do come in handy.
> >
> > John Andrews, W1TAG
> >
>
>Many thanks to John for this report, and his perseverance. Also to 
>Stewart, KK7KA for developing the mode in the first place. I believe this 
>is the first time a mode other than QRSS or DFCW has benn successfully 
>copied across the pond.
>
>I will run some more tests this evening; details to follow.
>
>Cheers, Jim Moritz
>73 de M0BMU



Congrats to John and Jim on this accomplishment. I'd like to also point out 
that this successful
reception took place on what, the first or second night of transmissions? 
And in the middle
of March!!

While you don't want to make too much out of a single test, this reception 
has well as many
receptions at great distances in the US make it clear that WOLF must be 
taken very
seriously has the mode for next season. I encourage all "lowfers" on both sides
of the Atlantic to strongly consider adding the WOLF mode to both your 
transmission
and reception capabilities.

And, yes, hats off to Stewart, KK7KA for developing this mode...and really 
also to Lyle
Koehler, K0LR who once again led the charge in doing on air testing of this 
new mode.

Congrats to all again.




Les Rayburn, N1LF
4919 Cox Cove
Helena, AL 35080
XMGR 184.8988khz WOLF Mode
1LF 187.300khz

Looking for a challenge? Try the ultimate weak signal mode, on 1750 Meters!
Visit the Noise Floor!
http://www.highnoonfilm.com/xmgr






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: M0BMU "Wolfed" in the U.S.
Date: Mon, 19 Mar 2001 16:32:16 -0000
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Congrats both.  That is impressive, and bears out the value of spread
spectrum communications - which is what this mode really amounts to.

Andy  G4JNT


> -----Original Message-----
> From: John Andrews [mailto:w1tag@charter.net]
> Sent: 2001-03-19 12:29
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: M0BMU "Wolfed" in the U.S.
> 
> 
> In my haste to get to bed last night, I neglected to post here that I
> successfully copied M0BMU's WOLF transmission in a 25 minute 
> recording made
> from 0135 - 0200 UTC (19 Mar). There are two lines of clear 
> copy at this
> point. I say that, because I'm not done tweaking the various 
> command line
> parameters yet. As Jim has pointed out, you should enter the correct
> sampling rate for your sound card, and this appears to be 
> more important
> with weak signals. Also, I find that adding short delays in 
> increments of
> 1/20 second (-s 400, -s 800...) may transform partial lines 
> into complete
> ones.
> 
> I'm located in central Massachusetts, about 80 km west of 
> Boston. This is a
> fairly noisy residential area, and I'm stuck with a loud 
> carrier just above
> 137 kHz that does deafen my receiver somewhat. Hardly an 
> ideal location. I
> believe that my neighbor nearest the loop antenna turned 
> their light dimmer
> off around 0145 last night, thereby helping my situation greatly!
> 
> John Andrews, W1TAG
> 
> 


-- 
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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>
Subject: LF: DX Cluster spots for 17/18 Mar at GB7DXM
Date: Mon, 19 Mar 2001 16:08:07 -0000
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Hi all, not many G stations spotted again....maybe there weren't any on ! I
cannot believe conditions were that bad as I heard DJ9IE regularly during
the week and a good signal from Christer SM6PXJ.

CFH has been on fairly reliably during the week and is often visible in
daytime. This seems to be the result of some disturbance and there are signs
of what I think is multipath fading during the night. These lead to
stupendous levels over Sunday/Monday with peak levels on my plots of 46dBu.
These have all been posted to Rik for inclusion on his site.
http://www.qsl.net/on7yd

Cluster spots follow:-

   137.7  OM2YL       18-Mar-2001 1557Z  CQ on QRSS
<OM2TW>
   137.2  OM2TW       18-Mar-2001 1546Z  CQ  599...
<OM2KM>
   137.2  OK1DTN      18-Mar-2001 1235Z  CQ
<OM2TW>
   137.7  DJ2LF       18-Mar-2001 1131Z  CQ
<OM2TW>
   136.5  DF0WD       18-Mar-2001 1027Z  559 cq
<DL1SAN>
   136.8  F6BWO       18-Mar-2001 1022Z  539 qso with dj7rd 599
<DL1SAN>
   136.8  DK5PT       18-Mar-2001 1008Z  559 qso with on7zo 239
<DL1SAN>
   137.7  HB9ASB      18-Mar-2001 0809Z
<OM2TW>
   137.5  M0BMU       17-Mar-2001 2047Z  perfect copy in WOLF BPSK
<DF0WD>
   137.7  OM2TW       17-Mar-2001 1725Z  cq qrss
<OM5CW>
   137.7  OM2TW       17-Mar-2001 1716Z  slow CQ & any QRN...
<HA6PC>
   137.7  OM2TW       17-Mar-2001 1333Z  QRSS 599 + 20 dB hr
<OM5CW>
   137.7  DK8KW       17-Mar-2001 1238Z  DFCW CQ
<OM2TW>

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, 19 Mar 2001 17:25:48
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: DX Cluster spots for 17/18 Mar at GB7DXM
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>CFH has been on fairly reliably during the week and is often visible in
>daytime. This seems to be the result of some disturbance and there are signs
>of what I think is multipath fading during the night. These lead to
>stupendous levels over Sunday/Monday with peak levels on my plots of 46dBu.
>These have all been posted to Rik for inclusion on his site.
>http://www.qsl.net/on7yd
>

For those who want to take a 'shortcut', the CFH plots are at :

http://www.qsl.net/on7yd/136cfbh.htm

more general LF info is via :

http://www.qsl.net/on7yd/136khz.htm


73, Rik  ON7YD


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>
Organization: University of Hertfordshire
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Date: Mon, 19 Mar 2001 13:06:39 +0000
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Subject: LF: Wolf BPSK across pond
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<?color><?param 0100,0100,0100>Dear LF Group,<br><br>I arrived at work this morning to find that:<br><br><?color><?param 7F00,0000,0000>&gt; Well, WOLF has successfully crossed the pond. Got two lines of  clean<br>&gt; copy between 0135 and 0200 Z tonight (3/19 Z). Frequency was  about 0.13<br>&gt; Hz below 137.5 kHz. Had to do some tweaking to get the copy.  Those<br>&gt; command line switches do come in handy.<br>&gt; <br>&gt; John Andrews, W1TAG<br>&gt; <br><br><?/color>Many thanks to John for this report, and his perseverance. Also to  Stewart, KK7KA for developing the mode in the first place. I  believe this is the first time a mode other than QRSS or DFCW has  benn successfully copied across the pond.<br><br>I will run some more tests this evening; details to follow.<br><br>Cheers, Jim Moritz<br>73 de M0BMU<br><br>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Date: Mon, 19 Mar 2001 12:26:26 -0000
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Subject: LF: Transatlantic: CFH good
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Being a great believer in the saying "There's no point in losing sleep over 
insomnia", I was up at 0040 and noticed that CFH was a massive S9+10dB. 
As a guide to how good that was, there are only three amateur stations I hear 
at this strength (G3GRO, G3YXM and G3XTZ) and only one that is stronger 
(M0BMU 10km away)!

I transmitted my callsign with 60s dots and 120s dashes until sleep finally 
overcame me at 0300. By this time CFH was down to S9.

Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



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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Subject: LF: M0BMU "Wolfed" in the U.S.
Date: Mon, 19 Mar 2001 07:28:55 -0500
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In my haste to get to bed last night, I neglected to post here that I
successfully copied M0BMU's WOLF transmission in a 25 minute recording made
from 0135 - 0200 UTC (19 Mar). There are two lines of clear copy at this
point. I say that, because I'm not done tweaking the various command line
parameters yet. As Jim has pointed out, you should enter the correct
sampling rate for your sound card, and this appears to be more important
with weak signals. Also, I find that adding short delays in increments of
1/20 second (-s 400, -s 800...) may transform partial lines into complete
ones.

I'm located in central Massachusetts, about 80 km west of Boston. This is a
fairly noisy residential area, and I'm stuck with a loud carrier just above
137 kHz that does deafen my receiver somewhat. Hardly an ideal location. I
believe that my neighbor nearest the loop antenna turned their light dimmer
off around 0145 last night, thereby helping my situation greatly!

John Andrews, W1TAG



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Mar 2001 10:48:02
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: LF: Jim's BPSK
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I wasn't aware of Jim's BPSK tests on saturday, but as I heard a
'suspicious signal' in the digtal mode segment I decided to record a 1
minute WAV file and let WOLF have a try on it.
Result : a 100% copy at the firsqt attempt. But Jim's signal is about 25dB
over noise here, so it wasn't a real challenge.
Using DL4YHF's software as spectrum analyzer I noticed that the bandwidth
was about 20Hz, so one should stay out of the QRSS segment (above 137600)
with BPSK.
I would like to do some more tests with weaker signals, if WOLF  is as good
as told (100% copy at -40dB SNR) than Jim could reduce his power by about
65dB.
Jim, is it possible for you to reduce power in steps, let's say -6dB every
10 minutes. I believe you could start at a level that is 20dB down on the
power you were running on saturday (at least for me).

73, Rik  ON7YD


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Mar 2001 10:25:41
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From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: QRS v3.05
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Hello Mike,

So far I didn't get any similar error reports of 'mixing up' characters.
Any chance that you selected DFCW mode instead of QRSS ? If you select DFCW
and transmit without applying a frequency shift an 'L' will appear as an 'H'.
Just a 'wild guess' ...

73, Rik  ON7YD

At 23:01 18/03/01 +1200, you wrote:
>Rik
>
>I have possibly a small problem with QRS305. Yesterday I was sending a text
>"LLLLLL" with 120 second dots. From reception reports (2000 km) it appeared
>that H's were being sent instead of L's. I confirmed this by setting the
>speed to 1 second dots and indeed it was H's. I typed in a second text
>"HHHHHH" and this worked normally. I then selected the first text (the L's)
>again and it worked perfectly sending L's. Testing again today there is no
>problem. Do you have any suggestions?
>
>Mike ZL4OL
>
>
>


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: MarkusVester@aol.com
Message-ID: <94.119ce742.27e6b961@aol.com>
Date: Sun, 18 Mar 2001 20:22:41 EST
Subject: Re: LF: DF6NM/G3AQC
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Hi Uwe, hi all,

thanks a lot for your image, that is exactly the kind of fast and precise 
feedback I always wished to have while transmitting.

Transatlantic condx appear to be excellent tonight, CFH consistently at 
+35dBuV/m is the strongest I have seen so far. Or have they upgraded their 
tx? (hopefully _not_ ;-)

Another station has come up on 922.50 , as far as I can see "between the 
lines", slightly weaker than Laurie.

73 de Markus, DF6NM


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: MarkusVester@aol.com
Message-ID: <33.122e4757.27e6af93@aol.com>
Date: Sun, 18 Mar 2001 19:40:51 EST
Subject: LF: Transatlantic with QRP ?
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Hi John, Andy and group,

>  How about stations in the 40mW range,   even less than Mike ?
>  We do have the advantage of absolute frequency accuracy.
>  Andy
>  
>  > Hi all, I haven't said I have quit transatlantic testing.  In 
>  > fact I would like to continue looking for stations in the 0.1 to 0.5 
watt 
>  > erp range. 

Well, maybe things are not completely hopeless for us  "single-yagi" boys?

CFH's carrier was above 30dBuV/m for several hours during last week's nights. 
Without helium, I can radiate about 30mW, some 55dB below CFH's 10kW or 
-25dBuV/m in VE. This would be a T to M signal here on a very quiet day with 
3s dots in 0.34Hz. Noise is certainly higher at night, but 30s dots will make 
up 10dB.

Right now CFH is coming up again, 32 dBuV/m at 23:40 !  Time to fire up the 
tx and put out a call sign on 135922.19Hz (0.2 Hz above Laurie's upper 
frequency).

73s de Markus, DF6NM


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: MarkusVester@aol.com
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Date: Sun, 18 Mar 2001 19:40:50 EST
Subject: Re: LF: Transatlantic Challenge: the Canadian / Europe contacts
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Hi friends,

a late comment, after a few days away from the net: 

That sure is good news! Since I first read about the original and ingenious 
ways to achieve these contacts, I had hoped for a decision like that. 
Congratulations to all of you!

Markus, DF6NM

John wrote:
>  In these unexpected circumstances, and taking into consideration the intent
>  behind setting up the Challenge that was to commemorate Peter Bobek's
>  practical and fun approach to amateur radio, we have unanimously decided to
>  award both contacts with special plaques to commemorate their achievements,
>  that is the contact between VA3LK, G3AQC, and the contact between VE1ZZ,
>  VE1ZJ and G3LDO.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: DF6NM/G3AQC
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This is a multi-part message in MIME format.
--------------030605000002030003050504
Content-Type: text/plain; charset=windows-1252; format=flowed
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Hi all,
captured DF6NM es G3AQC (30s dots, agc off)on 18.03.01 at 23.38utc. 
have a look at the enclosed pic, pse.
regards
Uwe/dj8wx

--------------030605000002030003050504
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Content-Transfer-Encoding: base64
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/9j/4AAQSkZJRgABAQEBLAEsAAD/2wBDAAgGBgcGBQgHBwcJCQgKDBQNDAsLDBkSEw8UHRof
Hh0aHBwgJC4nICIsIxwcKDcpLDAxNDQ0Hyc5PTgyPC4zNDL/2wBDAQkJCQwLDBgNDRgyIRwh
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CAEdAjUDASIAAhEBAxEB/8QAHwAAAQUBAQEBAQEAAAAAAAAAAAECAwQFBgcICQoL/8QAtRAA
AgEDAwIEAwUFBAQAAAF9AQIDAAQRBRIhMUEGE1FhByJxFDKBkaEII0KxwRVS0fAkM2JyggkK
FhcYGRolJicoKSo0NTY3ODk6Q0RFRkdISUpTVFVWV1hZWmNkZWZnaGlqc3R1dnd4eXqDhIWG
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NOEl8RcYGRomJygpKjU2Nzg5OkNERUZHSElKU1RVVldYWVpjZGVmZ2hpanN0dXZ3eHl6goOE
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--------------030605000002030003050504--

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From: "g3ldo" <g3ldo@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: LF book update
Date: Sun, 18 Mar 2001 21:50:54 -0000
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I have now included the programs used to produce the LF antenna impedance
signature shown in Fig 6.17 of the LF Experimenters HB. Just click on to
'AEGextra' from the home page. The site is given below.

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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Hi All I will start looking tonight at 2030. Last night saw G3AQC from
2130Z .  Also unintelligeable sigs just above G3AQC.

   Freq used by IK5ZPV bad Here .  I have spur from CFH exactly where
you were transmitting .  Please move up 1/4 or 1/2 or 1 Hertz higher
    73 de John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Staubach" <walter.staubach@fen.baynet.de>
To: "Reflektor" <rsgb_lf_group@blacksheep.org>
Subject: LF: Test
Date: Sun, 18 Mar 2001 20:51:11 +0100
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Thanks Brian for the test. We both saw you "O" and answered, but sri no QSO.
Better antennas and more power will be necessary here.
73 Walter

---------------------------------------------
Walter.Staubach@fen-net.de



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Staubach" <walter.staubach@fen.baynet.de>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: DJ2LF  unknown attachment
Date: Sun, 18 Mar 2001 16:41:46 +0100
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Hallo David,
   Brian sent e-mail with images from the EF50`s via reflektor. I answered
to him just by "reply" and asked for sked. Today he answered again and we
(Markus and me) will try to make QSO with him. Please let me know what was
wrong.
73 Walter

-----Urspr|ngliche Nachricht-----
Von: G0MRF@aol.com <G0MRF@aol.com>
An: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Datum: Sonntag, 18. Mdrz 2001 12:11
Betreff: LF: DJ2LF unknown attachment


>Walter.
>Your private e-mail to Brian arrived here with an attachment marked
"UNKNOWN"
>
>What is this please?
>
>David
>
>
>
>In a message dated 3/16/01 3:26:49 PM GMT Standard Time,
>walter.staubach@fen.baynet.de writes:
>
><< Subj:     LF: EF50
> Date:  3/16/01 3:26:49 PM GMT Standard Time
> From:  walter.staubach@fen.baynet.de (Walter Staubach)
> Sender:    majordom@post.thorcom.com
> Reply-to:  rsgb_lf_group@blacksheep.org
> To:    rsgb_lf_group@blacksheep.org (Reflektor)
>
> File:  Unknown (862 bytes)
> DL Time (32000 bps): < 1 minute
>
>
>
> --------------------
> Thanks, Brian, for the pictures. Yes, that they are.
> But about modern times: How about a QRSS-test on - lets say 137.695 this
>night (fri/sat) or next (sat/sun) at 23utc? I think Markus, DF6NM, would
like
>to join.
> He already saw you days ago.
> 73 Walter DJ2LF
>  >>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Staubach" <walter.staubach@fen.baynet.de>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: EF50
Date: Sun, 18 Mar 2001 16:23:52 +0100
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Dear Brian, thanks for info. Markus, DF6NM, and me will try to contact you,
beginning today at 1700utc and ending 2000utc. At first we will take 3s/dot,
later on if necessery 10s/dot. QRG 137.695 +-3.
73 Walter DJ2LF


-----Urspr|ngliche Nachricht-----
Von: Brian Rogerson <brian@esoterica.pt>
An: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Datum: Samstag, 17. Mdrz 2001 21:06
Betreff: Re: LF: EF50


>Walter
>
>I will be very pleased to have a qso but I am afraid that I "crash out"
>about 2100utc.  I do wake early if that is any use but otherwise during
>the day.  Let me know a time, 137.695 seems ok and 3sec dot and I
>will go to 10 sec if I am not receiving well.  73, Brian
>
>At 16:14 16/03/01 +0100, you wrote:
>>    Thanks, Brian, for the pictures. Yes, that they  are. But about modern
>>times: How about a QRSS-test on - lets say  137.695 this night (fri/sat)
or
>>next (sat/sun) at 23utc? I think Markus, DF6NM,  would like to join. He
>>already saw you days ago. 73 Walter DJ2LF    Attachment Converted:
>>"C:\Eudora\Attach\LF EF50.gif"
>
>
>73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
>http://homepage.esoterica.pt/~brian
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <10671.200103181251@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org
Date: Sun, 18 Mar 2001 12:56:22 +0000
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Subject: LF: <WOLF>Tests last night
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Dear LF group,

I transmitted "Wolf" mode signals from 2000 until 0330 utc last 
night on 137.5kHz. Thanks to DL4YHF for the reception report; I 
recorded several "random samples" of my signal off-air, which I 
was also able to decode without problems.

If anyone would like further tests, different power levels etc, please 
let me know. I will be transmitting again tonight for a few hours 
around midnight, at least covering 0000 - 0200 utc in case anyone 
in North America would like to try.

Cheers, Jim Moritz
73 de M0BMU 


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
Subject: LF: SV: Transatlantic-mystery
Date: Sun, 18 Mar 2001 13:26:40 +0100
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Hi Uwe

>first line: lf-meteorites ?

Yes, probably, or perhaps parts of MIR, hihi...

To me, it looks like a QRSS station sending "DDK"... with severe QRH/QRI.

73
Johan Bodin SM6LKM





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sun, 18 Mar 2001 07:12:49 -0500
From: "'Geri' Kinzel, DK8KW" <DK8KW@compuserve.com>
Subject: LF: Transatlantic-mystery
To: rsgb_lf_group@blacksheep.org
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Hello Uwe and LF-group,

>Hi all,
>during night ARGO/30s-dots/AGC-off captured on 18.03.01 at 0116utc the
enclosed
>pic.
>first line: lf-meteorites ?
>second line: IK5ZPV
>third line: DK8KW ?
>4th line: G3AQC<

>Uwe/dj8wx jo43sv 

... looking at these pictures, I believe that this was my signal! At least
easy to identify ... hope I didn't cause too much trouble ... I used my
Hagenug EX-1001 SSB esxciter on 134.000 kHz (suppressed) carrier frequency
and mixed 1923.70 Hz to it ... from a relatively stabil AF source. What I
did not think about is that the Exciter is PLL-driven and obviously needs
some time to reach its oroginal frequency ... thats the "trails" you cyn
see on Uwe's pictures. Next time I need to keep both frequency sources
running, and key only the buffer and PA!

Thanks for your observation, Uwe, best 73

Geri, DK8KW (W1KW) 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
References: <200103170559_MC2-C91E-9394@compuserve.com>
Subject: LF: Transatlantic-mystery
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This is a multi-part message in MIME format.
--------------050502090200040401020603
Content-Type: text/plain; charset=windows-1252; format=flowed
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Hi all,
during night ARGO/30s-dots/AGC-off captured on 18.03.01 at 0116utc the enclosed
pic.
first line: lf-meteorites ?
second line: IK5ZPV
third line: DK8KW ?
4th line: G3AQC

the pics 30min before and 60 min afterwards: no mysteries shown.
(during capture 18db es bandpath-filter switched btwn ant an rx).
regards
Uwe/dj8wx jo43sv 
--------------050502090200040401020603
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--------------050502090200040401020603--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "mcalevey" <mcalevey@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010309105514.22079226@mail.cc.kuleuven.ac.be>
Subject: LF: Re: QRS v3.05
Date: Sun, 18 Mar 2001 23:01:09 +1200
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Rik

I have possibly a small problem with QRS305. Yesterday I was sending a text
"LLLLLL" with 120 second dots. From reception reports (2000 km) it appeared
that H's were being sent instead of L's. I confirmed this by setting the
speed to 1 second dots and indeed it was H's. I typed in a second text
"HHHHHH" and this worked normally. I then selected the first text (the L's)
again and it worked perfectly sending L's. Testing again today there is no
problem. Do you have any suggestions?

Mike ZL4OL



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: G0MRF@aol.com
Message-ID: <c4.114c175b.27e5e8eb@aol.com>
Date: Sun, 18 Mar 2001 05:33:15 EST
Subject: LF: DJ2LF  unknown attachment
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Walter.
Your private e-mail to Brian arrived here with an attachment marked "UNKNOWN"

What is this please?

David



In a message dated 3/16/01 3:26:49 PM GMT Standard Time, 
walter.staubach@fen.baynet.de writes:

<< Subj:     LF: EF50
 Date:  3/16/01 3:26:49 PM GMT Standard Time
 From:  walter.staubach@fen.baynet.de (Walter Staubach)
 Sender:    majordom@post.thorcom.com
 Reply-to:  rsgb_lf_group@blacksheep.org
 To:    rsgb_lf_group@blacksheep.org (Reflektor)
 
 File:  Unknown (862 bytes)
 DL Time (32000 bps): < 1 minute
 
 
 
 --------------------
 Thanks, Brian, for the pictures. Yes, that they are.
 But about modern times: How about a QRSS-test on - lets say 137.695 this 
night (fri/sat) or next (sat/sun) at 23utc? I think Markus, DF6NM, would like 
to join.
 He already saw you days ago.
 73 Walter DJ2LF
  >>


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: DL4YHF@aol.com
Message-ID: <45.3be7bc9.27e55adc@aol.com>
Date: Sat, 17 Mar 2001 19:27:08 EST
Subject: LF: Jim's WOLF Tests on Saturday evening - FB !
To: rsgb_lf_group@blacksheep.org
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hello group,
<BR>
<BR>there was nice signal from Jim M0BMU in the new promising WOLF BPSK mode on 
<BR>saturday evening (just got home from the club station with 30 megabytes of 
<BR>recorded audio..)
<BR>
<BR>I had 100% error free copy right from the start, even though there was heavy 
<BR>QRN (static crashes) and a lousy drifting receiver (about 0.5Hz in 30 
<BR>minutes) on this side, so a lot has to be improved here before I will be able 
<BR>to transmit a useful signal from DF0WD (sri). 
<BR>
<BR>Jim transmitted an unmodulated carrier of some minutes at the beginning of 
<BR>every TX interval, which allowed a kind of 'calibration' of the RX frequency. 
<BR>It also helped very much to find the center frequency, which must be passed 
<BR>to &nbsp;&nbsp;the decoding software as a command line argument.
<BR>
<BR>May I suggest a dramatically reduced power for the next test transmissions, 
<BR>so that also the EU stations can dig in the noise for a weak signal (let's 
<BR>say 1mW instead of 300mW), because with Jim's powerful signal was much higher 
<BR>than &nbsp;the noise floor on saturday. 
<BR>
<BR>So thanks again to Stewart (KK7KA) for the invention of WOLF and to Jim for 
<BR>his test transmissions.
<BR>
<BR>
<BR>73's from Wolf (DL4YHF).
<BR></FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 17 Mar 2001 19:53:17 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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Subject: LF: lf tonight
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I will be looking for Eu stations from 2000Z til 0030z and again from
0400Z to 0600
   73 es gl John VE1ZJ



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<DIV><FONT face=Arial size=2>I tried to send this message direct but it got 
rejected.</FONT></DIV>
<DIV><FONT face=Arial size=2>Hi Ko,</FONT></DIV>
<DIV><FONT face=Arial size=2>Well its very difficult to tell from here what are 
real lines and what may be spurious The broad bands are very like the modulation 
patterns fron stations such as SXV on 135.7 to 135.85. You will have to 
frequency calibrate the system and try to idintify the lines.Lists of LORAN 
lines from various atations were published on the reflector some time ago. 
Vertical lines on horiz traces are usually noise (static) but yours are too 
regular.You should be able to see the UK stations around 135.925. I will be on 
later on 135.922. I do think a filter is neccesary to prevent overload of the 
pre-amp. Best of luck sorting things out.&nbsp; 73s 
Laurie.</FONT></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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<DIV><FONT face=Arial size=2>Hi All,</FONT></DIV>
<DIV><FONT face=Arial size=2>Johns report on my signal "best from 
about&nbsp;0100 to about 0215</FONT></DIV>
<DIV><FONT face=Arial size=2>corresponds with Alans plot for CFH which shows a 
similar peak to above 40db for just the same time period. This would indicate 
that&nbsp;the propagation is bi-directional. To be expected of course but nice 
to have confirmed.&nbsp;I will be on again tonight from about 2300utc.&nbsp; 73s 
Laurie.</FONT>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Brian Rogerson" <brian@esoterica.pt>
Subject: Re: LF: EF50
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Walter

I will be very pleased to have a qso but I am afraid that I "crash out"
about 2100utc.  I do wake early if that is any use but otherwise during
the day.  Let me know a time, 137.695 seems ok and 3sec dot and I
will go to 10 sec if I am not receiving well.  73, Brian

At 16:14 16/03/01 +0100, you wrote:
>    Thanks, Brian, for the pictures. Yes, that they  are. But about modern
>times: How about a QRSS-test on - lets say  137.695 this night (fri/sat) or
>next (sat/sun) at 23utc? I think Markus, DF6NM,  would like to join. He
>already saw you days ago. 73 Walter DJ2LF    Attachment Converted:
>"C:\Eudora\Attach\LF EF50.gif" 


73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
http://homepage.esoterica.pt/~brian



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi all saw 3 stations last night.  SM6PXJ,  from 0030 til 0130.   G3AQC
for most of night til  qrt 0530.  Very strong es readable from both AQC
somewhat stronger.Don't know when Christer went QRT but lost him at
0130.
     Strongest sigs were from CT1DRP  but his dots es dashes were longer
so perhaps just more integration.
    Frequencies posted b4 look ok wl look for xyz aqc zpv kw .  Best if
all use 30 second dots
   wl send pix later
73 de John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 17 Mar 2001 15:35:39 +0100
From: "Ko Versteeg" <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re. Mad Hatters Tea Party
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At 3/17/01 13:54:00, you wrote:
>Hi Ko.
>Your pictures are indeed very busy, do you have un-invited guests at your party?  I see a lot of Loran. 73s Laurie.
>

Hi Laurie.
I am not sure, but are the lines really there or are they created in the L202 preamp i am trying?
The L202 does not have a bandpass filter like the other one i use.

Watched 01:00 this morning and the lines were even worse but noone was
transmitting inside of them, though the lines were very close.

73 de Ko, NL9222.




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re. Mad Hatters Tea Party
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<DIV><FONT face=Arial size=2>Hi Ko.</FONT></DIV>
<DIV><FONT face=Arial size=2>Your pictures are indeed very busy, do you have 
un-invited guests at your party?&nbsp; I see a lot of Loran. 73s 
Laurie.</FONT></DIV></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>
Organization: University of Hertfordshire
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Subject: LF: <WOLF>Test signals
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Dear LF Group, 

Thanks for the interest in the "Wolf" BPSK trials. To make a start, I 
intend to transmit a test signal this evening, in order to make 
available a real signal for people to record and experiment with. Mr. 
Murphy has intervened as usual, and I have to fix a problem with 
my synthesiser, but I hope to be QRV around 2000utc. The format 
of the signal will be:

Frequency: 137.5000kHz. If occupied, I will QSY up or down by 
50Hz.

Power: about 300mW ERP

ID: Normal CW at 6wpm, approximately on every hour and half 
hour, followed by a few minutes of carrier for frequency 
measurement purposes. 

The rest of the time, the signal will be BPSK in the Wolf format. 
This is 10 bits/second, and consists of 96 second frames that 
repeat continuously. The Wolf program can operate on a signal of 
length up to about 25 minutes, so if you record from 5 minutes past 
the hour/half hour, for 25 minutes, you will have a full set of data. 
However, if the signal is reasonably strong at your QTH, only a few 
minutes of recording is required.

The web pages contain a fair amount of info, but here are some 
hints from my experience.

The signal must be recorded at 8000 samples/sec - I used 
DL4YHF's Spectrum Laboratory to do this; it also produces a 
spectrogram at the same time. Most sound editing software seems 
to offer a choice of sample rate too.

The program expects a nominal audio frequency of 800Hz. It does 
not work well with a very strong signal; I found that with a local 
signal it was neccessary to reduce signal level to 20 or 30dB 
below the sound card's overload point to get good results. KK7KA 
says that signal level should be -20 to -50dB below full scale. The 
noise level should be at least -6dB on full scale. You can alter this 
on a recorded signal using sound editing software if neccessary.

It is neccessary to calibrate the soundcard sample rate accurately. 
This can be done by feeding an audio signal with accurately known 
frequency into the soundcard, recording a few minutes, and then 
running Wolf in the -m (frequency measure) mode; the true sample 
rate is then (true f / measured f) x nominal sample rate. In my case, 
this worked out to 7954.801 samples/sec. It is essential to do this 
on receive, although the web page info could be interpreted to 
suggest it isn't

You can do a similar thing to determine the frequency error in the 
receiver; receive an accurately known frequency, run it through 
Wolf in measure mode, which gives you the frequency offset. 
Using the Spectrum Lab spectrogram to measure the apparent 
audio frequency gave very similar results, but with less resolution 
than the Wolf software.

If it does not work first time, you can use the same recorded signal 
as many times as you like, until the settings are right. Once I had 
level, sampling rate, and frequency offset correctly set, I got 
perfect decoding straight away. 

Hope this is some help - please let me know if you have queries, 
suggestions for improvements, flames, etc.

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 17 Mar 2001 14:18:36 +0100
From: "Ko Versteeg" <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re: Mad hatter's tea party
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At 3/17/01 11:29:00, you wrote:
>
> Steve, GW4ALG, said:
>
>>I know that many CW ops were
>> hoping that the use of continuous beacons just below 136.0 would
>> be stopping soon - especially with the return of CFH.
>
>The reason for transatlantic QRSS operation below 136kHz is because of CFH,
>which is located close to VE1ZJ and VE1ZZ.
>
>Most of this operation takes place through the night. I have often seen the
>136kHz spectrum viewed via Argo, with several QRSS stations a few Hz apart
>(below 136) while there are no signals at all in the  wide open spaces above
>136kHz.
>Reminiscent of the Mad Hatter's Tea Party from Alice in Wonderland.
>
>Regards,
>Peter, G3LDO
>
>e-mail <g3ldo@ukonline.co.uk>
>
>Web <http://web.ukonline.co.uk/g3ldo>
-----
Peter,   and others wishing to compare spectrograms.
I am not sure if i see "too much" but overhere it's crowded.
Night's are even worse!

Have a look at the first third part of this image
wich shows the lower part of 136Khz received 1 hour ago.
http://home.wanadoo.nl/nl9222/pix/136l202.jpg    (29Kb)

Or watch all the images at: 
http://home.wanadoo.nl/nl9222/136pics.htm
73 de Ko Versteeg, NL9222



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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References: <5337.200103161327@gemini> <005701c0ae34$b88796c0$f29201d5@dave> <3AB29557.49556C59@alg.demon.co.uk>
Subject: LF: Re: Mad hatter's tea party
Date: Sat, 17 Mar 2001 11:29:27 -0000
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 Steve, GW4ALG, said:

>I know that many CW ops were
> hoping that the use of continuous beacons just below 136.0 would
> be stopping soon - especially with the return of CFH.

The reason for transatlantic QRSS operation below 136kHz is because of CFH,
which is located close to VE1ZJ and VE1ZZ.

Most of this operation takes place through the night. I have often seen the
136kHz spectrum viewed via Argo, with several QRSS stations a few Hz apart
(below 136) while there are no signals at all in the  wide open spaces above
136kHz.
Reminiscent of the Mad Hatter's Tea Party from Alice in Wonderland.

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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I wish to thank all those who responded, both directly and through the
reflector, to my query about zipping 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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Date: Sat, 17 Mar 2001 05:59:31 -0500
From: "'Geri' Kinzel, DK8KW" <DK8KW@compuserve.com>
Subject: LF: Transatlantic
To: rsgb_lf_group@blacksheep.org
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Hello John (and whoever observes LF on the other side of the Atlantic)

>I wish to try this nigth on 135.923 kHz with 30 sec. dotlength  from
>00.00  to 1:00 UTC and from 4.00 to 5.00 UTC.
>
>'73 Valerio (IK5ZPV)

I would like to join in and give it a try, too. Would 135.9237 kHz be a
suitable frequency for 30 seconds or is anybody else using it? If so, I
would use it during the same time slot as Valerio (and try to keep it as
stabil as possible, trying not to interfere with IK5ZPV).

Thanks, best 73 

Geri, DK8KW (W1KW)

 



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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References: <3AB0D6A9.19741.7C3874@localhost> <3AB2A000.4A183F4E@ns.sympatico.ca>
Subject: Re: LF: Bad propagation or QRT ?
Date: Sat, 17 Mar 2001 10:34:01 -0000
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> Mike have you posted those pics yet. Were they OK?
> 73 de John VE1ZJ


John,

The pics were very useful, thanks. The first set showed my 10s dot CW but
only the dashes appeared because of the integration time, but it is
certainly possible to see the dashes in the right place. The next set were
magnificent and I was very pleased to see them. I made a composite pic so
that the whole of 'XDV' is displayed.

I haven't posted them on the site yet as I keep forgetting to e-mail myself
from work where I made the composite pic. I am going in to work today (via a
pub that is celebrating St Patrick's Day with cheap Guinness!) and will pick
up the file then.

Check the site this evening (Sat).

Sorry if I gave anyone the impression that you were stopping the listening
tests. I stopped this end because I did not want to put you to any further
trouble after many nights of monioring. If there are more tests to do I will
be there. Certainly some summer tests would be excellent (you may remember
that W1BB did some summer 160m tests years ago) but the limitting facor is
going to be QRN - though QRS is nowhere near as badly affected by QRN as
audible Morse is.

CUL.

de Mike, G3XDV




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 17 Mar 2001 11:04:12 +0100
From: "valerio gabbani" <valerio@mailsrv.dii.unisi.it>
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Hello John and all

I wish to try this nigth on 135.923 kHz with 30 sec. dotlength  from
00.00  to 1:00 UTC and from 4.00 to 5.00 UTC.

'73 Valerio (IK5ZPV)



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: DL4YHF@aol.com
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Subject: LF: "Wolf" BPSK tests anyone?
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<HTML><FONT FACE=arial,helvetica><FONT  SIZE=2>Hello Jim and others,
<BR>
<BR>I also like to do some RX-Tests with WOLF, because that seems to be a very 
<BR>interesting mode (not only because of its nice name hi).
<BR>Because I always have to drive up to the club station DF0WD and take my PC 
<BR>with me, it would be nice if you can give us some 'time schedule' when your 
<BR>transmissions will take place. 
<BR>With your planned ERP, you can leave the TX running for a few hours.
<BR>I hope the frequency stability of my RX will be good enough this time to get 
<BR>a first impression of how WOLF works 'on air'.
<BR>
<BR>Btw: Programmer's Info:
<BR>There is something going on with WOLF (the communication mode), Stewart 
<BR>(KK7KA) will try to put the WOLF code into a DLL which can be called by other 
<BR>programs (like XYZ.exe) to give it some real time capability. But that is 
<BR>something **planned** for the future because Stewart is a little short of 
<BR>time.
<BR>
<BR>
<BR>So, thanks Jim for the test transmission in advance, &nbsp;&nbsp;see you later,
<BR>
<BR>
<BR>73's from the 'living' Wolf (DL4YHF, who is not the inventor of WOLF)
<BR>
<BR>
<BR></FONT></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "C Andersson" <sm6pxj@swipnet.se>
To: rsgb_lf_group@blacksheep.org
Subject: SV: SV: LF: Transatlantic QRSS
Date: Sat, 17 Mar 2001 05:11:13 +0100
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W4DEX wrote:
> I have seen several faint lines on Argo at 135.92456. 
>Can anyone confirm SM6PXJ's exact frequency?

I think I started on 135.9246 and slowly drifted towards 135.9245 during 1,5 hours.
Sorry for not beeing "spot on".


>John Currie wrote:
>> 
>> Hi chris congratulations.  your sigs are O"O copy  first seen around
>> 0030
>> 73 de john VE1ZJ.


That's good news... Thanks

73
Christer
sm6pxj





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 21:03:44 -0500
From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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QRN here in North Carolina isn't as bad tonight as it has been the last
several weeks.  I have seen several faint lines on Argo at 135.92456. 
Can anyone confirm SM6PXJ's exact frequency?  I'm also carefully
watching for Laurie's DFCW on 135.922.

Dexter

John Currie wrote:
> 
> Hi chris congratulations.  your sigs are O"O copy  first seen around
> 0030
> 73 de john VE1ZJ.
> 
> C Andersson wrote:
> 
> > Hello John and the group,
> >
> > I'll be on 135.9245 between 00-01 and between 04-05 UTC tonight.
> > 30 sec dots.
> > I hope this fq is not already in use by anyone.
> >
> > /sm6pxj


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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Subject: LF: G3AQC DFCW
Date: Fri, 16 Mar 2001 21:01:34 -0500
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Very nice copy of G3AQC dfcw on 135.922 kHz, 0115 - 0200 here in Central
Massachusetts. Lots of static crashes, but a good signal.

John Andrews, W1TAG



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Date: Sat, 17 Mar 2001 01:15:31 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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Subject: Re: SV: LF: Transatlantic QRSS
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Hi chris congratulations.  your sigs are O"O copy  first seen around
0030
73 de john VE1ZJ.

C Andersson wrote:

> Hello John and the group,
>
> I'll be on 135.9245 between 00-01 and between 04-05 UTC tonight.
> 30 sec dots.
> I hope this fq is not already in use by anyone.
>
> /sm6pxj



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 23:29:42 +0000
From: "Steve Rawlings" <steve@alg.demon.co.uk>
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Subject: Re: LF: Activity from G6RO
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Dear All,

I received some very sad news today.

Last week, I wrote:
> Ron has written to say that Doris is very poorly and is spending
> some time in hospital.  The hospital visiting schedule, among
> other things, means that Ron will be less active than usual.

Earlier this evening, Bob G8RW telephoned me to say that Doris,
the wife of Ron G6RO, died on Thursday 8th March.  They had been
married for 61 years.

I later had a long telephone conversation with Ron, and we talked
about many things.  It is clear to me that Ron is looking forward
to meeting his LF friends again on 136 kHz, just as soon as
circumstances allow.

Regards to all,
Steve GW4ALG



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Steve Rawlings" <steve@alg.demon.co.uk>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re: "Wolf" BPSK tests anyone?
References: <5337.200103161327@gemini> <005701c0ae34$b88796c0$f29201d5@dave>
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Dave G3YMC wrote:

> May I politely remind us all that the agreed band plan is for data to be in
> the 137.4-137.6 range.  Use of slow CW below 136.0 (band plan beacon
> section) has seemed to have become common for transatlantic qsos, but there
> is no reason to continue this practice for local tests.

Thanks for the reminder, Dave.  I know that many CW ops were
hoping that the use of continuous beacons just below 136.0 would
be stopping soon - especially with the return of CFH.

To shift the QRSS/data modes back up to the top end of the band
would be a significant help to those experimenters using
receivers with only 'average' IF filters.

Regards to all,
Steve GW4ALG




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From: "C Andersson" <sm6pxj@swipnet.se>
To: rsgb_lf_group@blacksheep.org
Subject: SV: LF: Transatlantic QRSS
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Hello John and the group,

I'll be on 135.9245 between 00-01 and between 04-05 UTC tonight.
30 sec dots.
I hope this fq is not already in use by anyone.

/sm6pxj





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <3AB2D1B5.67429069@ns.sympatico.ca>
Date: Fri, 16 Mar 2001 18:53:42 -0800
From: "John Currie" <john.currie@ns.sympatico.ca>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Transatlantic QRSS
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Hi Jim ,  Yes i agree.  I believe I have seen "T" copy from DF6NM. would
like to try again.  Also would like to look for SM6PXJ again es IK5ZPV
73 de John VE1ZJ
James Moritz wrote:

> Dear LF Group,
>
> Congratulations to VE1ZJ, VE1ZZ, G3LDO, VA3LK and G3AQC on
> their awards - Also to G3XDV on finally getting across with his
> "QRP" signal.
>
> For possible further transatlantic QRSS activity, how about some
> signals from mainland Europe and Scandinavia?  As far as I can
> remember, the only non-G stations seen on the other side of the
> pond so far have been OK1FIG (with the aid of a huge commercial
> antenna), and CT1DRP. I have a personal motive too; it would
> make an interesting change from 'XDV's signal trying to melt it's
> way through my preselector!
>
> Cheers, Jim Moritz
> 73 de M0BMU



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <3AB2D09A.3887155B@ns.sympatico.ca>
Date: Fri, 16 Mar 2001 18:49:01 -0800
From: "John Currie" <john.currie@ns.sympatico.ca>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: RE:"Wolf" BPSK tests anyone?
References: <65AECDF1F89AD411900400508BFC869F9C03D8@pdw-mail-1.dera.gov.uk>
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Hi Andy I'm willing to try .  Currently only have ARGO with 30 sec dots, but
could download later version es try at 60 or 90sec dots
      73 de John VE1ZJ

Talbot Andrew wrote:

> How about stations in the 40mW range,   even less than Mike ?
>
> We do have the advantage of absolute frequency accuracy.
>
> Andy
>
> > Hi all, I haven't said I have quit transatlantic testing.  In
> > fact I would
> > like to continue looking for stations in the 0.1 to 0.5 watt
> > erp range. I
> >
>
> --
> The Information contained in this E-Mail and any subsequent correspondence
> is private and is intended solely for the intended recipient(s).
> For those other than the recipient any disclosure, copying, distribution,
> or any action taken or omitted to be taken in reliance on such information is
> prohibited and may be unlawful.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <001001c0ae45$1ed7a7c0$46bd883e@g3aqc>
From: "Laurie Mayhead" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. Testing
Date: Fri, 16 Mar 2001 18:15:01 -0000
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<DIV><FONT face=Arial size=2>John Currie wrote "I will be looking for DFCW or 
QRSS 30sec dots..."</FONT></DIV>
<DIV><FONT face=Arial size=2>In that case I will run my 350mW beacon tonight 
from 0000utc</FONT></DIV>
<DIV><FONT face=Arial size=2>on 135.922. DFCW 30sec. Anyone care to join 
me?&nbsp;&nbsp;I am interested in exploiting this mode for faster DX QSOs,we 
still hav'nt exhausted the possibilities. 73s 
Laurie.&nbsp;&nbsp;</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <25392.200103161701@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
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Date: Fri, 16 Mar 2001 17:06:19 +0000
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Subject: LF: Transatlantic QRSS
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Dear LF Group,

Congratulations to VE1ZJ, VE1ZZ, G3LDO, VA3LK and G3AQC on 
their awards - Also to G3XDV on finally getting across with his 
"QRP" signal.

For possible further transatlantic QRSS activity, how about some 
signals from mainland Europe and Scandinavia?  As far as I can 
remember, the only non-G stations seen on the other side of the 
pond so far have been OK1FIG (with the aid of a huge commercial 
antenna), and CT1DRP. I have a personal motive too; it would 
make an interesting change from 'XDV's signal trying to melt it's 
way through my preselector!

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <005701c0ae34$b88796c0$f29201d5@dave>
From: "Dave Sergeant" <dsergeant@btinternet.com>
To: rsgb_lf_group@blacksheep.org
References: <5337.200103161327@gemini>
Subject: LF: Re: "Wolf" BPSK tests anyone?
Date: Fri, 16 Mar 2001 15:53:41 -0000
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>From Dave G3YMC

James Moritz wrote:
>The most important thing seems to be which frequency to  use; from this
end,
>the obvious choice seems to be either in the
>135.9 - 136.0kHz, or 137.4 - 137.6kHz ranges

May I politely remind us all that the agreed band plan is for data to be in
the 137.4-137.6 range.  Use of slow CW below 136.0 (band plan beacon
section) has seemed to have become common for transatlantic qsos, but there
is no reason to continue this practice for local tests.

73s Dave G3YMC
dsergeant@btinternet.com
dsergeant@iee.org
http://www.btinternet.com/~dsergeant




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Date: Fri, 16 Mar 2001 16:54:23
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: "Wolf" BPSK tests anyone?
In-reply-to: <5337.200103161327@gemini>
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Hello Jim,

I just downloaded the WOLF software. I'll try to get it running during the
weekend, I will let you know when I can receive WOLF.
You're 599+ with 1 Watt ERP so I'd prefer something in the mW range.

73, Rik  ON7YD

At 13:31 16/03/01 +0000, you wrote:
>Dear LF Group,
>
>Since transatlantic QRSS activity seems to have ceased for the 
>time being, I thought I would give KK7KA's "Wolf" a try. This is 
>essentially BPSK, but the encoding and decoding scheme is 
>designed so that a weak signal can be effectively integrated over a 
>long period. The current version of the software operates with a 
>fixed-length 15 character message; with good SNR, this will 
>decode in 24 seconds, but with a weak signal, the software will 
>operate on up to about 25 minutes of received signal, hopefully 
>leading to a significant improvement in performance. The US 
>Lowfers seem to have been doing quite well with it. There is quite 
>a bit of info on http://www.scgroup.com/ham/wolf.html, and also 
>http://www.highnoonfilm.com/xmgr/updates/wolf.htm .
>
>I have now tested my Decca TX with a specially built BPSK keyer 
>which has the accurate timing required by Wolf. I am able to 
>receive my own signals, and decode them successfully, so I know 
>it works! Both the carrier frequency, and the timing of the data 
>should be within 1 part in 10^7, which seems to be more than 
>adequate.
>
>The requirements for receiving this mode are basically just 
>receiver plus soundcard/PC, but great care is needed in initially 
>calibrating both the system frequency offsets, and the errors in the 
>soundcard sampling rate, in order to successfully decode weak 
>signals. This is critical for successful operation. The software 
>includes some utilities to help do this. The signal processing is "off 
>line"; first you record a period of received signal at 8k samples/sec 
>using the software of you choice (I used DL4YHF's Spectrum Lab, 
>which conveniently allows you to display a spectrogram at the 
>same time). Then, you run the recorded .wav file through the Wolf 
>program, together with the appropriate calibration factors. The 
>program prints the decoded message. This can be repeated if 
>neccessary, until you are happy with the results.
>
>I gather VA3LK is also nearly ready to start trials using this mode, 
>so if anyone is interested in trying some tests, I would be happy to 
>oblige. The most important thing seems to be which frequency to 
>use; from this end, the obvious choice seems to be either in the 
>135.9 - 136.0kHz, or 137.4 - 137.6kHz ranges. I can vary ERP 
>from about 1W down to 1mW, or less if you like, and set frequency 
>in 0.1Hz steps.  Let me know what signal would best suit your 
>needs. I should be able to be QRV most evenings over the next 
>couple of weeks. 
>
>Cheers, Jim Moritz
>73 de M0BMU
>
>


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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE:"Wolf" BPSK tests anyone?
Date: Fri, 16 Mar 2001 15:45:04 -0000
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How about stations in the 40mW range,   even less than Mike ?

We do have the advantage of absolute frequency accuracy.

Andy


> Hi all, I haven't said I have quit transatlantic testing.  In 
> fact I would
> like to continue looking for stations in the 0.1 to 0.5 watt 
> erp range. I
> 


-- 
The Information contained in this E-Mail and any subsequent correspondence
is private and is intended solely for the intended recipient(s).
For those other than the recipient any disclosure, copying, distribution, 
or any action taken or omitted to be taken in reliance on such information is
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Staubach" <walter.staubach@fen.baynet.de>
To: "Reflektor" <rsgb_lf_group@blacksheep.org>
Subject: LF: EF50
Date: Fri, 16 Mar 2001 16:14:02 +0100
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This is a multi-part message in MIME format.
--------------040605070309090809040205
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD W3 HTML//EN">
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<DIV><FONT size=2>Thanks, Brian, for the pictures. Yes, that they 
are.</FONT></DIV>
<DIV><FONT size=2>But about modern times: How about a QRSS-test on - lets say 
137.695 this night (fri/sat) or next (sat/sun) at 23utc? I think Markus, DF6NM, 
would like to join.</FONT></DIV>
<DIV><FONT size=2>He already saw you days ago.</FONT></DIV>
<DIV><FONT size=2>73 Walter DJ2LF</FONT></DIV>
<DIV><FONT size=2></FONT>&nbsp;</DIV></BODY></HTML>

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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Mike have you posted those pics yet. Were they OK?
73 de John VE1ZJ

Mike Dennison wrote:

> > Since a few evenings I don't hear nor see anymore the Greek
> > Rtty station. It's just the bad propagation, or did they QRT ?
> > TNX.
>
> I have not heard it for several days. The last time it went off, it came back
> several kHz from where it was before. Will it return on the same frequency?
>
> Mike, G3XDV (IO91VT)
> http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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In a message dated 3/16/01 9:18:40 AM Eastern Standard Time, 
stewart.bryant@virgin.net writes:

<< There is
 also the danger of accidental execution in the browser. >>

I always suspected I might expire while waiting for graphics-intensive pages 
to load, but this could represent a whole new danger.  :-)

73,
John




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi all, I haven't said I have quit transatlantic testing.  In fact I would
like to continue looking for stations in the 0.1 to 0.5 watt erp range. I
consider the reception of G3XDV at "O" copy this week to be an
encouragement to continue.  If anyone wants to continue please let me know
by E-mail
    Also I will be setting up an antenna for transmitting at summer QTH in
may if anyone wants to try for summer QSO. I will be looking for dfcw or
qrss 30 second dots
    73 de John VE1ZJ

James Moritz wrote:

> Dear LF Group,
>
> Since transatlantic QRSS activity seems to have ceased for the
> time being, I thought I would give KK7KA's "Wolf" a try. This is
> essentially BPSK, but the encoding and decoding scheme is
> designed so that a weak signal can be effectively integrated over a
> long period. The current version of the software operates with a
> fixed-length 15 character message; with good SNR, this will
> decode in 24 seconds, but with a weak signal, the software will
> operate on up to about 25 minutes of received signal, hopefully
> leading to a significant improvement in performance. The US
> Lowfers seem to have been doing quite well with it. There is quite
> a bit of info on http://www.scgroup.com/ham/wolf.html, and also
> http://www.highnoonfilm.com/xmgr/updates/wolf.htm .
>
> I have now tested my Decca TX with a specially built BPSK keyer
> which has the accurate timing required by Wolf. I am able to
> receive my own signals, and decode them successfully, so I know
> it works! Both the carrier frequency, and the timing of the data
> should be within 1 part in 10^7, which seems to be more than
> adequate.
>
> The requirements for receiving this mode are basically just
> receiver plus soundcard/PC, but great care is needed in initially
> calibrating both the system frequency offsets, and the errors in the
> soundcard sampling rate, in order to successfully decode weak
> signals. This is critical for successful operation. The software
> includes some utilities to help do this. The signal processing is "off
> line"; first you record a period of received signal at 8k samples/sec
> using the software of you choice (I used DL4YHF's Spectrum Lab,
> which conveniently allows you to display a spectrogram at the
> same time). Then, you run the recorded .wav file through the Wolf
> program, together with the appropriate calibration factors. The
> program prints the decoded message. This can be repeated if
> neccessary, until you are happy with the results.
>
> I gather VA3LK is also nearly ready to start trials using this mode,
> so if anyone is interested in trying some tests, I would be happy to
> oblige. The most important thing seems to be which frequency to
> use; from this end, the obvious choice seems to be either in the
> 135.9 - 136.0kHz, or 137.4 - 137.6kHz ranges. I can vary ERP
> from about 1W down to 1mW, or less if you like, and set frequency
> in 0.1Hz steps.  Let me know what signal would best suit your
> needs. I should be able to be QRV most evenings over the next
> couple of weeks.
>
> Cheers, Jim Moritz
> 73 de M0BMU



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 16:01:58 +0200
To: rsgb_lf_group@blacksheep.org
From: "Costas Krallis" <sv1xv@eexi.gr>
Subject: LF: Re: EF50
In-reply-to: <65AECDF1F89AD411900400508BFC869F9C03D2@pdw-mail-1.dera.gov .uk>
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At 08:37 16/03/2001 -0000, you wrote:

> Amongst the mine of nostalgia out there, I there anyone who understands
> valve circuit topology and can tell us if the circuit I described really
> can be considered as a cascode but using just a single pentode.    

According to ye olde electronics textbooks, the cascode circuit
is  electrically equivalent to a pentode, having the advantage
of the lower noise of the triode valve/tube.

Costas



 +------------------------------------------------------------+
 | Costas Krallis SV1XV      *   LOC KM18UA                   |
 | P.O.Box 3066              *   E-Mail: sv1xv@eexi.gr        |
 | GR-10210 Athens           *   PGP key: 0x3BDBBC34          |
 | GREECE                    *   http://www.qsl.net/sv1xv/    |
 |                           *   http://w4u.eexi.gr/~sv1xv/   |
 +------------------------------------------------------------+



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 14:12:43 +0000
From: "Stewart Bryant" <stewart.bryant@virgin.net>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Zip files
References: <000901c0ae0a$789af0e0$32ca28c3@ericadodd>
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Peter

Since most people have the capability for unzipping, it is perhaps better
to use the .zip format rather than the .exe format. You always
know what you are getting with a .zip and have complete control over
the operation. With a .exe you have to trust the site and trust that it has
not been hacked and a substitute program put in its place. There is
also the danger of accidental execution in the browser.

Just mp 2d

73

Stewart G3YSX

g3ldo wrote:

> I have a group of small DOS .exe files, plus some .txt data files
> (associated with measuring antenna feed impedance) that I would like to put
> on to my web site for the benefit of LF experimenters.
> I have PKZIP and UNZIP, which I know how to use but these are DOS programs
> and are probably not appropriate.
> I could use WINZIP but I have never used this before.
> The one I like best is the .exe file that, when run, explodes all the zipped
> files automatically.
> Can anyone advise me?
>
> 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: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org
Date: Fri, 16 Mar 2001 13:31:53 +0000
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Subject: LF: "Wolf" BPSK tests anyone?
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Dear LF Group,

Since transatlantic QRSS activity seems to have ceased for the 
time being, I thought I would give KK7KA's "Wolf" a try. This is 
essentially BPSK, but the encoding and decoding scheme is 
designed so that a weak signal can be effectively integrated over a 
long period. The current version of the software operates with a 
fixed-length 15 character message; with good SNR, this will 
decode in 24 seconds, but with a weak signal, the software will 
operate on up to about 25 minutes of received signal, hopefully 
leading to a significant improvement in performance. The US 
Lowfers seem to have been doing quite well with it. There is quite 
a bit of info on http://www.scgroup.com/ham/wolf.html, and also 
http://www.highnoonfilm.com/xmgr/updates/wolf.htm .

I have now tested my Decca TX with a specially built BPSK keyer 
which has the accurate timing required by Wolf. I am able to 
receive my own signals, and decode them successfully, so I know 
it works! Both the carrier frequency, and the timing of the data 
should be within 1 part in 10^7, which seems to be more than 
adequate.

The requirements for receiving this mode are basically just 
receiver plus soundcard/PC, but great care is needed in initially 
calibrating both the system frequency offsets, and the errors in the 
soundcard sampling rate, in order to successfully decode weak 
signals. This is critical for successful operation. The software 
includes some utilities to help do this. The signal processing is "off 
line"; first you record a period of received signal at 8k samples/sec 
using the software of you choice (I used DL4YHF's Spectrum Lab, 
which conveniently allows you to display a spectrogram at the 
same time). Then, you run the recorded .wav file through the Wolf 
program, together with the appropriate calibration factors. The 
program prints the decoded message. This can be repeated if 
neccessary, until you are happy with the results.

I gather VA3LK is also nearly ready to start trials using this mode, 
so if anyone is interested in trying some tests, I would be happy to 
oblige. The most important thing seems to be which frequency to 
use; from this end, the obvious choice seems to be either in the 
135.9 - 136.0kHz, or 137.4 - 137.6kHz ranges. I can vary ERP 
from about 1W down to 1mW, or less if you like, and set frequency 
in 0.1Hz steps.  Let me know what signal would best suit your 
needs. I should be able to be QRV most evenings over the next 
couple of weeks. 

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Zip files
Date: Fri, 16 Mar 2001 12:00:00 -0000
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Winzip is only an envelope for PKZIP and UNZIP so these two progs are
still perfectly valid.  Packaged with these should be a utility called
ZIP2EXE.    Just type    ZIP2EXE XXXXXX    where XXXXXX is your ZIP file
produced under PKZIP

Andy  G4JNT


> -----Original Message-----
> From: g3ldo [mailto:g3ldo@ukonline.co.uk]
> Sent: 2001-03-16 11:15
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Zip files
> 
> 
> I have a group of small DOS .exe files, plus some .txt data files
> (associated with measuring antenna feed impedance) that I 
> would like to put
> on to my web site for the benefit of LF experimenters.
> I have PKZIP and UNZIP, which I know how to use but these are 
> DOS programs
> and are probably not appropriate.
> I could use WINZIP but I have never used this before.
> The one I like best is the .exe file that, when run, explodes 
> all the zipped
> files automatically.
> Can anyone advise me?
> 
> 
> Regards,
> Peter, G3LDO
> 
> e-mail <g3ldo@ukonline.co.uk>
> 
> Web <http://web.ukonline.co.uk/g3ldo>
> 
> 
> 


-- 
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is private and is intended solely for the intended recipient(s).
For those other than the recipient any disclosure, copying, distribution, 
or any action taken or omitted to be taken in reliance on such information is
prohibited and may be unlawful.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Petr Maly" <p.maly@gmc.net>
To: rsgb_lf_group@blacksheep.org
References: <000901c0ae0a$789af0e0$32ca28c3@ericadodd>
Subject: LF: Re: Zip files
Date: Fri, 16 Mar 2001 12:55:54 +0100
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For example, you can get PK250DOS.EXE from
http://www.pkware.com/shareware/download/pk250dos.html

this package contains also ZIP2EXE with which you can convert ZIP file to
self-extract ZIP.
All in your favourite DOS.

73 Petr OK1FIG



----- Original Message -----
From: g3ldo <g3ldo@ukonline.co.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Friday, March 16, 2001 12:15 PM
Subject: LF: Zip files


> I have a group of small DOS .exe files, plus some .txt data files
> (associated with measuring antenna feed impedance) that I would like to
put
> on to my web site for the benefit of LF experimenters.
> I have PKZIP and UNZIP, which I know how to use but these are DOS programs
> and are probably not appropriate.
> I could use WINZIP but I have never used this before.
> The one I like best is the .exe file that, when run, explodes all the
zipped
> files automatically.
> Can anyone advise me?
>
>
> 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: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: rsgb_lf_group@blacksheep.org
Date: Fri, 16 Mar 2001 11:25:53 -0000
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Subject: Re: LF: who is ufo?
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> BTW. what stn is transmitting a carrier on 137.052,0 kHz at night vy strong, at 
> day vy weak.
> regards
> Uwe/dj8wx jo43sv

This is CFH, a Canadian maritime station. It is not on all the time but is a very 
good guide to DX propagation levels. Note that a good signal during the day 
usually means a poor one at night - which is not what you might expect.

73



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re:  EF50
Date: Fri, 16 Mar 2001 11:24:59 -0000
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In the early 1980s the VMP4 was going to answer both  our VHF power
amplifier and wide dynamic range receiver problems, so I scrounged some
freebies;  couldn't afford to buy any, they were too expensive.  But it
never happened, there were plenty of other devices to do the job and the
VMP4 never really went anywhere.   

Nowadays we have a huge range of power MOSFETS for switching (very
cheap) and others for RF, (expensive) and a plethora of components for
building very good receivers - which are usually quite cheap.   Its all
down to mass production and who wants what components.

Now who's showing the nostalgia syndrome :-(

Andy  G4JNT

> -----Original Message-----
> From: Alberto di Bene [mailto:dibene@usa.net]
> Sent: 2001-03-16 10:44
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: EF50
> 
> 
> Rik Strobbe wrote:
> 
> > >A pity, I threw away some old VMP4 devices only a few 
> weeks ago in a
> 
> Oh, no ! I have been in search of VMP4 for years .....without 
> luck, and you
> throw them away...:-(  There is no justice in this world ... :-)
> 
> 73  Alberto   I2PHD
> 
> 
> 


-- 
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is private and is intended solely for the intended recipient(s).
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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
Subject: LF: Zip files
Date: Fri, 16 Mar 2001 11:15:09 -0000
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I have a group of small DOS .exe files, plus some .txt data files
(associated with measuring antenna feed impedance) that I would like to put
on to my web site for the benefit of LF experimenters.
I have PKZIP and UNZIP, which I know how to use but these are DOS programs
and are probably not appropriate.
I could use WINZIP but I have never used this before.
The one I like best is the .exe file that, when run, explodes all the zipped
files automatically.
Can anyone advise me?


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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Date: Fri, 16 Mar 2001 11:44:00 +0100
From: "Alberto di Bene" <dibene@usa.net>
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Subject: LF: Re:  EF50
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Rik Strobbe wrote:

> >A pity, I threw away some old VMP4 devices only a few weeks ago in a

Oh, no ! I have been in search of VMP4 for years .....without luck, and you
throw them away...:-(  There is no justice in this world ... :-)

73  Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 02:00:49 -0800 (PST)
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Ceramic insulators (AD)
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Hi,
Put me down for a pack please Alan.
I will put a cheque in the post as soon as you confirm that I am not too
late.
Sorry to hear you have been ill. Nothing serious I hope.
Graham and Steve are due here on Sunday with a catapult. So hopefully my
signal should improve soon.
Best 73, John
 & keep up the good work.





_______________________________________________________
Send a cool gift with your E-Card
http://www.bluemountain.com/giftcenter/




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 10:31:31
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: RE: EF50
In-reply-to: <65AECDF1F89AD411900400508BFC869F9C03D2@pdw-mail-1.dera.gov .uk>
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Hi Andy,

>A pity, I threw away some old VMP4 devices only a few weeks ago in a
>clear out of ancient and obsolete semiconductors as part of teh shack
>rebuild,  they would have been quite good for an active antenna.

It is a variant on Murphy's law : you will not need a component until you
have thrown (given) it away.

Due to the same law :
- when you drop anything heavy (hammer, screwdriver) it will always land on
something fragile or when you drop a sandwich it will alway come with the
'buttered' side down (law of selective gravity)
- when you need x components to built a project you will always find x-1
components available (law of selective statistics)
- any expensive component protected by a fuse will protect the fuse by
'melting' first
- the chance that a component gets defective is proportional to its value
and so on ...

73, Rik  ON7YD

PS : 
Sespite all semiconductor theories we were told the truth is that any
transistor or IC just works on some smoke that is kept inside.
Proof : put in an IC / transistor the wrong way or increase voltage /
current above the allowed level and wait until the smoke comes out. The
device will not work anymore afterwards.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: EF50
Date: Fri, 16 Mar 2001 08:37:36 -0000
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Could that be because the Navy used E55F  (presumably = EF55).  The
active antenna whose description started this thread does use three of
these devices.

Amongst the mine of nostalgia out there, I there anyone who understands
valve circuit topology and can tell us if the circuit I described really
can be considered as a cascode but using just a single pentode.    

The dual gate mosfet can be considered to operate in this way  - ie.
cascode operation available from a single device with one current
carrying path - but to my knowledge no equivalent has ever been produced
for power FETs.

A pity, I threw away some old VMP4 devices only a few weeks ago in a
clear out of ancient and obsolete semiconductors as part of teh shack
rebuild,  they would have been quite good for an active antenna.   But I
guess one of the modern RF packaged MOSFETs designed for HF - UHF
transmitters (which still cost quite a lot) will probably do a better
job.  Probably have a spare MRF150 somewhere.

Wish I'd never mentioned the Naval active antenna in the first place !

Andy  G4JNT

> Sorry abt the mine of mis-information. Army EF50 was ARP35  (also
CV1091,
> CV1578). Still can't find a navy version......
> 


-- 
The Information contained in this E-Mail and any subsequent correspondence
is private and is intended solely for the intended recipient(s).
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 16 Mar 2001 09:27:16
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: who is ufo?
In-reply-to: <14di8t-2HNKyGC@fwd00.sul.t-online.com>
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Hello Uwe,

It could have been OH5UFO, an 'alias' callsign of Reino (OH1TN).

73, Rik  ON7YD

At 01:30 16/03/01 +0100, you wrote:
>Hi all, 
>back from night-committee finding on screen "UFO" on 135,898.1 kHz at
0024utc vy 
>strong. who is "UFO" ? he (she?) did not react on  my resp.
>BTW. what stn is transmitting a carrier on 137.052,0 kHz at night vy
strong, at 
>day vy weak.
>regards
>Uwe/dj8wx jo43sv



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
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Subject: LF: Re: Re: Re: Transatlantic Challenge: the Canadian / Europe contacts
Date: Thu, 15 Mar 2001 21:54:23 -0800
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----- Original Message -----
From: Larry Kayser <kayser@sympatico.ca>
To: <rsgb_lf_group@blacksheep.org>
Sent: Thursday, March 15, 2001 9:16 PM
Subject: LF: Re: Re: Transatlantic Challenge: the Canadian / Europe contacts


> Dave:
>
> > Now for the Pacific eh Larry?
>
> Yes, starting as soon as I can get a new antenna pulled  up and into
place.
>
> Larry
> VA3LK
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: Re: Transatlantic Challenge: the Canadian / Europe contacts
Date: Fri, 16 Mar 2001 00:16:21 -0500
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Dave:

> Now for the Pacific eh Larry?

Yes, starting as soon as I can get a new antenna pulled  up and into place.

Larry
VA3LK





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Message-ID: <009501c0add8$cfec3980$0a00a8c0@ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
References: <3AB09A04.24872.3479A7@localhost>
Subject: LF: Re: Transatlantic tests this season
Date: Fri, 16 Mar 2001 00:05:30 -0500
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Mike:

> Unless anyone else is looking for Eu signals (Larry?),

I lost the big LF antenna due to Ice/freezing rain late on Tuesday - I am
completely out of business until I haul up a whole new antenna.  I am also
not hearing anything from Europe for some days - maybe the season is over
for the North Atlantic.

I had just started transmitting WOLF data over the weekend but that is over
till I get a new antenna pulled up into place and tuned.

It has been a great season but it seems to be ending on a very harsh note
for me anyways hi.

73 es GL to u Mike

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "jannsen" <0482183881-0001@t-online.de>
To: rsgb_lf_group@blacksheep.org
References: <65AECDF1F89AD411900400508BFC869F9C03A7@pdw-mail-1.dera.gov.uk> <3AB0BE6A.DCDE2F88@usa.net>
Subject: LF: who is ufo?
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Hi all, 
back from night-committee finding on screen "UFO" on 135,898.1 kHz at 0024utc vy 
strong. who is "UFO" ? he (she?) did not react on  my resp.
BTW. what stn is transmitting a carrier on 137.052,0 kHz at night vy strong, at 
day vy weak.
regards
Uwe/dj8wx jo43sv




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 19:15:16 +0000
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Tube EF50
References: <004901c0ad60$39936300$1fd725c3@194.95.193.10.fen.baynet.de> <3.0.5.32.20010315161208.0082a100@pop3.esoterica.pt>
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In message <3.0.5.32.20010315161208.0082a100@pop3.esoterica.pt>, Brian
Rogerson <brian@esoterica.pt> writes
>I'm sorry, I could not resist.  73, Brian
>
>At 15:55 15/03/01 +0100, you wrote:
>>With nostalgic smile I read the many mails about EF50 and other tubes that I
>>used in the "tube-times" of my ham-life.
>>Here some electrical data of it:
>>(source: Röhren-Taschen-Tabelle Franzis-Verlag München 1964)
>>
>>The tube was used for HF- and wideband-amplification up to 50MHz. The
>>amplification could be regulated by varying the negative voltage at grid 3 -
>>says the book. This seems a little unbelievable to me, because mostly a
>>variable voltage at grid1 was used.

That's the normal method, but when used in the H2S equipment, after the
Tx pulse the Rx was used in high gain mode, with a few plus volts on the
g3 to catch the first ground return.

Mike
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Paul" <slowpoke@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: EF50
Date: Thu, 15 Mar 2001 22:04:49 -0000
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Hi all,

Sorry abt the mine of mis-information. Army EF50 was ARP35 (also CV1091,
CV1578). Still can't find a navy version......

Regards de Paul G4MD

E-mail Paul :- slowpoke@ntlworld.com



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "G3YXM" <g3yxm@wireless.org.uk>
To: rsgb_lf_group@blacksheep.org
References: <LOBBIDNOENMNHIBGDCKBGELFCGAA.g3wkl@btinternet.com>
Subject: LF: Re: Transatlantic Challenge: the Canadian / Europe contacts
Date: Thu, 15 Mar 2001 21:38:10 -0000
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Hearty congratulations to all.

It's been an all-consuming goal for most of the participants, sleepless
nights, skinned knuckles, melted insulators and blown fets.

Well done Jack, John, Larry, Laurie and Peter.

Amateur radio history is made.

Now for the Pacific eh Larry?

73. Dave G3YXM.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 21:14:38 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Ceramic insulators (AD)
References: <004901c0ad80$fe56e2a0$58c47ad5@default>
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Hi Alan I would like a package of the insulators, i hope to transmit from summer
place
73 de john VE1ZJ

Alan Melia wrote:

> Hi all I have just managed to wrench those remaining insulators from my
> local trader. After satisfying the original demand (Larry , Brian, Mike
> Probert, & Alan Lowe)  I have 24 left which I think best  makes 3 packs of
> 8.
> The cost will be £2-00 for the insulators (0.25p ea) and £1-30 postage
> (Inland UK)
> First reflector orders, come first
>
> Copy of my original 'advert'
> -----------------------------------------
> At a recent Rally I came across a local trader with some brand new
> brown-glazed ceramic 'rod' insulators for wire aerials at 25p each. (I
> bought 8)  They are about 10.5cms long and 1.7cms diameter, with a leakage
> path of about 6.5cms (between the holes). Possibly a little small for the
> Kilowatters, but at least they wont catch fire.
> ----------------------------------------
> There may be some more available later when he clears his garage out! But at
> least it means he will remember me if anything else in that field comes
> along. He threw some marine 500k stuff in a skip last year because he didn't
> have room in his car (sob sob!). I have put him under orders to ring me for
> emergency transport if it happens again.
>
> 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: WarmSpgs@aol.com
Message-ID: <61.c41b838.27e26c02@aol.com>
Date: Thu, 15 Mar 2001 14:03:30 EST
Subject: Re: LF: Transatlantic Challenge: the Canadian / Europe contacts
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In a message dated 3/15/01 3:18:32 AM Eastern Standard Time, 
blanch@pncl.co.uk writes:

<< Apart from congratulating all concerned,
 I hope you meant the FCC. The
 Federal Aviation Authority might take a
 very long time dealing with a ham radio
 matter!! >>

Oh, I don't know.  The FAA consider themselves qualified to regulate VHF FM 
broadcast allocations and the type of RF emission filters used on digital TV 
transmitters, so perhaps we shouldn't be surprised to see them making a move 
to take over ham regulation as well.  [grin]




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Splendid news, and a fine decision.  Congratulations to all concerned!

John,  KD4IDY




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <004901c0ad80$fe56e2a0$58c47ad5@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Ceramic insulators (AD)
Date: Thu, 15 Mar 2001 15:07:12 -0000
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Hi all I have just managed to wrench those remaining insulators from my
local trader. After satisfying the original demand (Larry , Brian, Mike
Probert, & Alan Lowe)  I have 24 left which I think best  makes 3 packs of
8.
The cost will be £2-00 for the insulators (0.25p ea) and £1-30 postage
(Inland UK)
First reflector orders, come first

Copy of my original 'advert'
-----------------------------------------
At a recent Rally I came across a local trader with some brand new
brown-glazed ceramic 'rod' insulators for wire aerials at 25p each. (I
bought 8)  They are about 10.5cms long and 1.7cms diameter, with a leakage
path of about 6.5cms (between the holes). Possibly a little small for the
Kilowatters, but at least they wont catch fire.
----------------------------------------
There may be some more available later when he clears his garage out! But at
least it means he will remember me if anything else in that field comes
along. He threw some marine 500k stuff in a skip last year because he didn't
have room in his car (sob sob!). I have put him under orders to ring me for
emergency transport if it happens again.

Cheers de Alan G3NYK
Alan.Melia@btinternet.com





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Date: Thu, 15 Mar 2001 16:12:08 +0000
To: rsgb_lf_group@blacksheep.org
From: "Brian Rogerson" <brian@esoterica.pt>
Subject: Re: LF: Tube EF50
In-reply-to: <004901c0ad60$39936300$1fd725c3@194.95.193.10.fen.baynet.de >
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I'm sorry, I could not resist.  73, Brian

At 15:55 15/03/01 +0100, you wrote:
>With nostalgic smile I read the many mails about EF50 and other tubes that I
>used in the "tube-times" of my ham-life.
>Here some electrical data of it:
>(source: Röhren-Taschen-Tabelle Franzis-Verlag München 1964)
>
>The tube was used for HF- and wideband-amplification up to 50MHz. The
>amplification could be regulated by varying the negative voltage at grid 3 -
>says the book. This seems a little unbelievable to me, because mostly a
>variable voltage at grid1 was used.
>
>heater     6.3V - 0.3A / anode 250V  10mA / grid3  0..-54V / grid2   250V
>3mA / grid1   -2V / resistor at cathode 600ohms.
>socket loctal, comparable type EF53.
>73 Walter DJ2LF
>
>
>
>
>---------------------------------------------
>Walter.Staubach@fen-net.de
>
>
>
>
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73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
http://homepage.esoterica.pt/~brian

--------------040505010706000809030904--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: rsgb_lf_group@blacksheep.org
Date: Thu, 15 Mar 2001 14:50:17 -0000
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Subject: Re: LF: Bad propagation or QRT ?
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> Since a few evenings I don't hear nor see anymore the Greek
> Rtty station. It's just the bad propagation, or did they QRT ?
> TNX.

I have not heard it for several days. The last time it went off, it came back 
several kHz from where it was before. Will it return on the same frequency?


Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Walter Staubach" <walter.staubach@fen.baynet.de>
To: "Reflektor" <rsgb_lf_group@blacksheep.org>
Subject: LF: Tube EF50
Date: Thu, 15 Mar 2001 15:55:22 +0100
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With nostalgic smile I read the many mails about EF50 and other tubes that I
used in the "tube-times" of my ham-life.
Here some electrical data of it:
(source: Röhren-Taschen-Tabelle Franzis-Verlag München 1964)

The tube was used for HF- and wideband-amplification up to 50MHz. The
amplification could be regulated by varying the negative voltage at grid 3 -
says the book. This seems a little unbelievable to me, because mostly a
variable voltage at grid1 was used.

heater     6.3V - 0.3A / anode 250V  10mA / grid3  0..-54V / grid2   250V
3mA / grid1   -2V / resistor at cathode 600ohms.
socket loctal, comparable type EF53.
73 Walter DJ2LF




---------------------------------------------
Walter.Staubach@fen-net.de



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Bad propagation or QRT ?
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Hi Alberto,   Judging by the european amateur stations I have seen here
in Canada  propagation has been good this week
73 de John VE1ZJ
Alberto di Bene wrote:

> Since a few evenings I don't hear nor see anymore the Greek
> Rtty station. It's just the bad propagation, or did they QRT ?
> TNX.
>
> 73   Alberto   I2PHD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 14:45:34
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: "O" copy
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At 02:44 15/03/01 -0500, you wrote:
>Hi all tonight G3XDV was "O" copy here .  I believe his signals are the
>most weakly challanged that I have received across pond.  I have sent
>pics to Mike.
>     73 de    John VE1ZJ

Well done Mike & John,

It gives hope to the other 'modest' stations to cross the pond one day.

Mike, remember our first QRSS QSO in may 1998 (probably the first 2-way
QRSS QSO ever) ? Quite an evolution in a period of less than 3 years ...


73, Rik  ON7YD


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: <3AB072D4.C43770A4@ns.sympatico.ca>
Subject: LF: Re: "O" copy
Date: Thu, 15 Mar 2001 10:07:03 -0000
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John, VE1ZJ said:

> Tonight G3XDV was "O" copy here .  I believe his signals are the
> most weakly challanged that I have received across pond.  I have sent
> pics to Mike.

Congratulations to Mike and John. You only have to see just how small Mike's
garden is to realise what an achievement this is. Well done.

While in a discussion with a radio Ham friend (not an LFer) about the Peter
Bobek award and the final outcome, he remarked that DARC, AMRAD and the RSGB
HF Committee had shown a good deal of collective wisdom - I think that says
it all!

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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Message-ID: <3AB0BE6A.DCDE2F88@usa.net>
Date: Thu, 15 Mar 2001 14:06:50 +0100
From: "Alberto di Bene" <dibene@usa.net>
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To: rsgb_lf_group@blacksheep.org
Subject: LF: Bad propagation or QRT ?
References: <65AECDF1F89AD411900400508BFC869F9C03A7@pdw-mail-1.dera.gov.uk>
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Since a few evenings I don't hear nor see anymore the Greek
Rtty station. It's just the bad propagation, or did they QRT ?
TNX.

73   Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <15208.200103151208@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org
Date: Thu, 15 Mar 2001 12:12:53 +0000
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Subject: Re: LF: VR136 = EF50?
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Dear Dick, LF Group,

Not much to do with LF I know, but the very interesting book 
"Metres to Microwaves" by E.B. Callick has a lot of info on British 
valve development in the WWII period, including many detailed 
drawings and tables. Obviously, it is mainly about the VHF - 
microwave spectrum.

The EF50 gets a mention; it was used a lot as an IF amp. The RL7 
was a development of the EF50 with aligned grids to reduce 
partition noise, and was developed for use in VHF radar RX front 
ends, where it was used as an improved replacement for the 
difficult-to-manufacture "acorn" valves. Later, it was re-designated 
the EF54.

The EF50 was, in spite of it's external metal can, one of the first 
"all glass" valves, in which the base was an integral part of the 
envelope. This meant the electrodes could be mounted directly on 
the base pins, which greatly reduced parasitic inductance 
compared to valves with a pinch seal for the lead-out wires. It also 
had relatively high transconductance. These features greatly 
improved high frequency and wide band performance. By the end 
of the war, minature B7G all-glass valves of american origin, such 
as the 6AK5, were making the much bigger EF50 obsolete.  

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "cesare tagliabue" <cestag@dada.it>
To: "LF group" <rsgb_lf_group@blacksheep.org>
Subject: LF: web fault
Date: Thu, 15 Mar 2001 11:39:33 +0100
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<HTML>
<HEAD>

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<DIV><FONT color=#000000 size=2>&nbsp;&nbsp;&nbsp; <FONT color=#000000>Hi 
all</FONT></FONT></DIV>
<DIV><FONT color=#000000 size=2><FONT color=#000000></FONT>&nbsp;&nbsp;&nbsp; 
Since my provider is updating the server, my web pages are temporarily confused 
and unusable.</FONT></DIV>
<DIV><FONT color=#000000 size=2></FONT><FONT size=2>&nbsp;&nbsp;&nbsp;&nbsp; 
73&nbsp;&nbsp; Cesare</FONT></DIV>
<DIV><FONT size=2></FONT>&nbsp;</DIV>
<DIV><FONT color=#000000 size=2>Cesare Tagliabue&nbsp;&nbsp; I 5 
TGC<BR>WW-Loc&nbsp; JN53PS<BR>e-mail: <A 
href="mailto:cestag@dada.it">cestag@dada.it</A><BR>url: <A 
href="http://www.dadacasa.com/i5tgc">http://www.dadacasa.com/i5tgc</A><BR></FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: rsgb_lf_group@blacksheep.org
References: <16005567.984503931546.JavaMail.imail@chilly.excite.com> <004601c0ac7d$58993920$32d41ad4@w8k3f0> <000501c0acad$b595ffc0$2d2f883e@robing>
Subject: LF: VR136 = EF50?
Date: Thu, 15 Mar 2001 10:51:15 +0100
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To All from PA0SE

Robin T. Greenwood wrote:

> I think it was known as an EF54?

You are right!

In a list of equivalent valves I found VR136 = RL7

And then in another list RL7 = EF54.

Thanks Robin!

73, Dick, PA0SE

> ----- Original Message -----
> From: "Dick Rollema" <d.w.rollema@freeler.nl>
> To: <rsgb_lf_group@blacksheep.org>
> Sent: Wednesday, March 14, 2001 11:52 AM
> Subject: Re: LF: Re. E88cc in parallel
>
>
> > To All from PA0SE
> >
> > John, G4CNN wrote:
> >
> > That's my memory too - i.e. the red or aluminium cans were EF50s. Why
some
> > were red I don't think I ever knew.
> > _______________________________________________________
> >
> > Is it not so that the red EF50 was the original one, developed by
Philips
> at
> > Eindhoven for television treceivers? Just before Germany occupied The
> > Netherlands on May 10th, 1940, info on the production of the EF50 was
> passed
> > to on Mullard.
> >
> > The aluminium military equivalent of the EF50 was the VR136, which was
> used
> > in for instance tuning units of the Gee set; one as RF amplifier, one as
> > a mixer and a VR137 triode as oscillator.
> >
> > 73, Dick, PA0SE
> >
> >
> >
> >
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Subject: LF: Transatlantic: Thanks John
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> Hi all tonight G3XDV was "O" copy here .  I believe his signals are the
> most weakly challanged that I have received across pond.  I have sent
> pics to Mike.
>      73 de    John VE1ZJ

John,

Many thanks for the pics and for your perseverance in looking for my weak 
signals night after night. My previous Atlantic crossing was to your holiday site 
(much better for receiving Eu) and was only a fragment of a callsign, so small 
that you missed it, and it was only because you published a picture that I was 
able to spot my strange Morse. This one is much more satisfactory and a 
greater distance.

Unless anyone else is looking for Eu signals (Larry?), I will finish 
transmissions for the season, except when I see CFH at S9, and save on my 
electricity bill.

I am sure I speak for all Eu LF DXers when I thank all those in VE and W for 
their patience in monitoring over the last few months. The results this year 
have been much better than we could have hoped for.

What would be useful now are complete logs of when conditions permitted DX 
reception and when they did not. This could be correlated with the work that 
Alan is doing on CFH, and with the solar data. The key to even better 
successes (eg normal CW) is being able to predict the really big openings.

John's pictures will be on my web site tonight.

Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



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
Subject: LF: Re. Transatlantic Challenge the Canadian/European contacts.
Date: Thu, 15 Mar 2001 09:28:15 -0000
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<DIV><FONT face=Arial size=2>Many thanks to David, and all who have sent their 
congratulations. </FONT></DIV>
<DIV><FONT face=Arial size=2>Thanks also to John and his colleagues for a wise 
and unifying decision.</FONT></DIV>
<DIV><FONT face=Arial size=2>Roll on next season and even greater 
achievements,its been fun.&nbsp;&nbsp;&nbsp;&nbsp; 73s Laurie 
G3AQC.</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 08:13:13 +0000
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From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: Re: LF: Transatlantic Challenge: the Canadian / Europe contacts
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At 21:43 14/03/01 Wednesday, John Gould wrote:
>............................(once and if the FAA agree to licence the band
>for amateur usage in the USA).

Apart from congratulating all concerned,
I hope you meant the FCC. The
Federal Aviation Authority might take a
very long time dealing with a ham radio
matter!!

Walter G3JKV



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 02:18:26 -0500
From: "Holger 'Geri' Kinzel, DK8KW" <DK8KW@compuserve.com>
Subject: LF: Transatlantic Challenge: the Canadian / Europe contacts
To: rsgb_lf_group@blacksheep.org
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Hello LF Group,

>In these unexpected circumstances, and taking into consideration the
intent
>behind setting up the Challenge that was to commemorate Peter Bobek's
>practical and fun approach to amateur radio, we have unanimously decided
to
>award both contacts with special plaques to commemorate their
achievements,
>that is the contact between VA3LK, G3AQC, and the contact between VE1ZZ,
>VE1ZJ and G3LDO.

excellent decision!

73

Geri, DK8KW (W1KW)


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000901c0acfc$43143df0$0a00a8c0@ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
References: <c0.1127b027.27e17c83@aol.com>
Subject: LF: Re: Transatlantic Challenge: the Canadian / Europe contacts
Date: Wed, 14 Mar 2001 22:01:39 -0500
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David:

> Since the original announcement of the challenge all five of you have
devoted
> an enormous amount of time effort and dedication to the task. Yours has
been
> a fine achievement and one which I'm sure Peter Bobek would have
> wholeheartedly approved.

Thank You, I do hope I get to buy you a good cup of coffee this year on this
side of the Atlantic, it would be great to see you at Dayton.

There sure has been a pile of water under the bridge this past year since we
met in Niagara Falls. Pun intended.

Larry
VA3LK






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 02:44:20 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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Subject: LF: "O" copy
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Hi all tonight G3XDV was "O" copy here .  I believe his signals are the
most weakly challanged that I have received across pond.  I have sent
pics to Mike.
     73 de    John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Mar 2001 02:47:13 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Transatlantic Challenge: the Canadian / Europe contacts
References: <LOBBIDNOENMNHIBGDCKBGELFCGAA.g3wkl@btinternet.com>
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Hi John I think you have made a wise choice. Thank you all from myself and Jack
73 de john VE1ZJ
John W Gould wrote:

> The three sponsors of the Transatlantic Challenge have considered the two
> recent transatlantic contacts.  We were impressed by the dedication, skill
> and perseverance that was shown in each case.   The contacts were so
> incredible that we had not anticipate the ways in which they were achieved
> when we devised the rules!
>
> In these unexpected circumstances, and taking into consideration the intent
> behind setting up the Challenge that was to commemorate Peter Bobek's
> practical and fun approach to amateur radio, we have unanimously decided to
> award both contacts with special plaques to commemorate their achievements,
> that is the contact between VA3LK, G3AQC, and the contact between VE1ZZ,
> VE1ZJ and G3LDO.
>
> In these circumstances we will not make a further award for a Canadian and
> European QSO. Further, we have clarified the rules for the case of the
> outstanding USA to Europe QSO (once and if the FAA agree to licence the band
> for amateur usage in the USA).
>
> I hope that all involved in this LF aspect of our hobby will accept this
> outcome and continue the excellent work that is being done to improve and
> innovate reception, transmission, and aerial technology.
>
> On behalf of my colleagues and their committees our appreciation goes out to
> the work of those who we will be awarding plaques.  But we would also like
> to extend our appreciation to the work carried out by many others who have
> made experimentation on this amateur allocation such an interesting and
> absorbing hobby.
>
> Best 73
>
> John Gould
> G3WKL
> RSGB HF Committee
>
> On behalf of DARC, AMRAD and RSGB



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: G0MRF@aol.com
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Date: Wed, 14 Mar 2001 21:01:39 EST
Subject: LF: Transatlantic Challenge: the Canadian / Europe contacts
To: rsgb_lf_group@blacksheep.org
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In a message dated 3/14/01 9:48:07 PM GMT Standard Time, g3wkl@btinternet.com 
writes:

<< we have unanimously decided to
 award both contacts with special plaques to commemorate their achievements,
 that is the contact between VA3LK, G3AQC, and the contact between VE1ZZ,
 VE1ZJ and G3LDO.
  >>

Well done RSGB AMRAD and DARC on making a unanimous and unifying decision, 
and of course, my sincere congratulations to Larry, Laurie, Jack, John and 
Peter for bringing some lateral thinking to the inspiring Transatlantic 
Challenge.
Since the original announcement of the challenge all five of you have devoted 
an enormous amount of time effort and dedication to the task. Yours has been 
a fine achievement and one which I'm sure Peter Bobek would have 
wholeheartedly approved.

Great work.  -  David  G0MRF


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>
Subject: LF: Transatlantic Challenge: the Canadian / Europe contacts
Date: Wed, 14 Mar 2001 21:43:41 -0000
Message-ID: <LOBBIDNOENMNHIBGDCKBGELFCGAA.g3wkl@btinternet.com>
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The three sponsors of the Transatlantic Challenge have considered the two
recent transatlantic contacts.  We were impressed by the dedication, skill
and perseverance that was shown in each case.   The contacts were so
incredible that we had not anticipate the ways in which they were achieved
when we devised the rules!

In these unexpected circumstances, and taking into consideration the intent
behind setting up the Challenge that was to commemorate Peter Bobek's
practical and fun approach to amateur radio, we have unanimously decided to
award both contacts with special plaques to commemorate their achievements,
that is the contact between VA3LK, G3AQC, and the contact between VE1ZZ,
VE1ZJ and G3LDO.

In these circumstances we will not make a further award for a Canadian and
European QSO. Further, we have clarified the rules for the case of the
outstanding USA to Europe QSO (once and if the FAA agree to licence the band
for amateur usage in the USA).

I hope that all involved in this LF aspect of our hobby will accept this
outcome and continue the excellent work that is being done to improve and
innovate reception, transmission, and aerial technology.

On behalf of my colleagues and their committees our appreciation goes out to
the work of those who we will be awarding plaques.  But we would also like
to extend our appreciation to the work carried out by many others who have
made experimentation on this amateur allocation such an interesting and
absorbing hobby.

Best 73

John Gould
G3WKL
RSGB HF Committee

On behalf of DARC, AMRAD and RSGB



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 14 Mar 2001 19:36:46 +0100
From: "Ko Versteeg" <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org
Subject: Re: Re: LF: Lf Engineering A Hoax?
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>LF Engineering makes excellent products for the Lowfer community and is 
>co-owned
>by Sal DeFransico, who once operated a beacon himself. I have purchased several
>products from them in recent months, but do find them very slow to respond to
>e-mail...often two or three weeks would pass. Quicker response will come via
>snail mail.

------------
Hi Les..
(Glad i am not the only one BUYING)
Just came home and found a note there was a small packet from USA
perhaps it finally arrived, will check the post office tomorrow.

Right,there has never been any response for this order neither snail or email.
But as a bonus i got another ticket from the Dutch Customs,
amazing how they keep remembering me ;-)

Thanks for the info Les.
73 de Ko, NL9222.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Robin T. Greenwood" <robin@g3lba.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <16005567.984503931546.JavaMail.imail@chilly.excite.com> <004601c0ac7d$58993920$32d41ad4@w8k3f0>
Subject: Re: LF: Re. E88cc in parallel
Date: Wed, 14 Mar 2001 17:39:01 -0000
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I think it was known as an EF54?
----- Original Message -----
From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: <rsgb_lf_group@blacksheep.org>
Sent: Wednesday, March 14, 2001 11:52 AM
Subject: Re: LF: Re. E88cc in parallel


> To All from PA0SE
>
> John, G4CNN wrote:
>
> That's my memory too - i.e. the red or aluminium cans were EF50s. Why some
> were red I don't think I ever knew.
> _______________________________________________________
>
> Is it not so that the red EF50 was the original one, developed by Philips
at
> Eindhoven for television treceivers? Just before Germany occupied The
> Netherlands on May 10th, 1940, info on the production of the EF50 was
passed
> to on Mullard.
>
> The aluminium military equivalent of the EF50 was the VR136, which was
used
> in for instance tuning units of the Gee set; one as RF amplifier, one as
> a mixer and a VR137 triode as oscillator.
>
> 73, Dick, PA0SE
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: rsgb_lf_group@blacksheep.org
References: <16005567.984503931546.JavaMail.imail@chilly.excite.com>
Subject: Re: LF: Re. E88cc in parallel
Date: Wed, 14 Mar 2001 12:52:26 +0100
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To All from PA0SE

John, G4CNN wrote:

That's my memory too - i.e. the red or aluminium cans were EF50s. Why some
were red I don't think I ever knew.
_______________________________________________________

Is it not so that the red EF50 was the original one, developed by Philips at
Eindhoven for television treceivers? Just before Germany occupied The
Netherlands on May 10th, 1940, info on the production of the EF50 was passed
to on Mullard.

The aluminium military equivalent of the EF50 was the VR136, which was used
in for instance tuning units of the Gee set; one as RF amplifier, one as
a mixer and a VR137 triode as oscillator.

73, Dick, PA0SE




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: <005201c0abf2$2e992e40$3025ff3e@oemcomputer>
Subject: LF: Re: Valves
Date: Wed, 14 Mar 2001 08:45:31 -0000
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Paul, G4MD, said

> Subject thread is heading back towards my territory!

Same here - showing my age!
>
> The silver EF50's were service issue valves - VR91 for the RAF, ARP12 for
> the army. I suppose the navy must have had them as well, but I don't
recall
> the designation....Red ones were the civilian issue.
> I'm sure I recall my late father saying the H2S set had over 100 of them,
> and it was unknown for them all to be working simultaneously!

I worked on H2S Radar when I was in the RAF but I can't remember there being
100 VR91s used. The equipment had a wide band 45MHz IF strip with about 8 or
9 red VR91s. Much sought after from the ex-govnt radio stores as home-brew
TV
receivers for receiving Alexander Palace.
H2S Mk 3G and H2S Mk4A were quite reliable considering their complexity. The
greatest cause of faults was the Pye plugs used for coaxial cable inter unit
connections.

The ARP12 is a directly heated pentode used in battery operated Army pack
sets.

The E88CC is a double triode frame grid valve that was used in UHF TV
tuners, designed to overcome the space charge effect at these frequencies.
They were used until superior solid state devices came along.

At the Amberley Museum we have 1000s of these valves!


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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Date: Tue, 13 Mar 2001 23:14:39 -0600
To: rsgb_lf_group@blacksheep.org,  rsgb_lf_group@blacksheep.org
From: "Les Rayburn" <les@highnoonfilm.com>
Subject: Re: LF: Lf Engineering A Hoax?
In-reply-to: <200103101351.OAA11349@smtp.wanadoo.nl>
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At 02:51 PM 3/10/01 +0100, Ko Versteeg wrote:
>Group..
>
>Has anyone ever tried products from Lf Engineering USA?
>Found at: http://www.lfengineering.com/
>Reason for this is they have not been answering my
>messages for 2 weeks... One year ago they DID answer.
>
>Do they still excist or is it an abandoned website
>that's left, just like many other sites ?
>
>73 de Ko, NL9222


LF Engineering makes excellent products for the Lowfer community and is 
co-owned
by Sal DeFransico, who once operated a beacon himself. I have purchased several
products from them in recent months, but do find them very slow to respond to
e-mail...often two or three weeks would pass. Quicker response will come via
snail mail.




Les Rayburn, N1LF
4919 Cox Cove
Helena, AL 35080
XMGR 184.900khz
1LF 187.300khz





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 14 Mar 2001 06:42:35 +0200
To: rsgb_lf_group@blacksheep.org
From: "Costas Krallis" <sv1xv@eexi.gr>
Subject: Re: LF: E88cc in parallel
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Could someone please post a schematic or two of these
valve/tube antenna amplifiers?

Regards,

Costas SV1XV





 +------------------------------------------------------------+
 | Costas Krallis SV1XV      *   LOC KM18UA                   |
 | P.O.Box 3066              *   E-Mail: sv1xv@eexi.gr        |
 | GR-10210 Athens           *   PGP key: 0x3BDBBC34          |
 | GREECE                    *   http://www.qsl.net/sv1xv/    |
 |                           *   http://w4u.eexi.gr/~sv1xv/   |
 +------------------------------------------------------------+



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 13 Mar 2001 20:24:10 +0000
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Valves
References: <005201c0abf2$2e992e40$3025ff3e@oemcomputer>
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In message <005201c0abf2$2e992e40$3025ff3e@oemcomputer>, Paul
<slowpoke@ntlworld.com> writes
>Hi all,
>
>Subject thread is heading back towards my territory!
>
>The silver EF50's were service issue valves - VR91 for the RAF, ARP12 for
>the army. I suppose the navy must have had them as well, but I don't recall
>the designation....Red ones were the civilian issue.
>
>The EF50 has been described as "the valve that won the war" so ubiquitous
>was it and so advanced in performance compared to other valves of the time.
>I'm sure I recall my late father saying the H2S set had over 100 of them,
>and it was unknown for them all to be working simultaneously!
>
>Might go and dig some out and try a new LF preamp. (need all my 807's for
>the PA.....)

I made an RF pre-amp using one in about 1948, tuned to Ally Pally TV
sound. With a dipole mounted on a broomstick poking out of my bedroom
window I received the London TV sound channel loud and clear in south
Wales!

Mike
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 13 Mar 2001 20:56:50 +0000
To: rsgb_lf_group@blacksheep.org
From: "Tom Boucher" <tom@telemetry.demon.co.uk>
Subject: Re: LF: Re. E88cc in parallel
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....Red ones were made by Sylvania weren't they?

> red or aluminium cans were EF50s. 
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Paul" <slowpoke@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Valves
Date: Tue, 13 Mar 2001 19:16:41 -0000
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Hi all,

Subject thread is heading back towards my territory!

The silver EF50's were service issue valves - VR91 for the RAF, ARP12 for
the army. I suppose the navy must have had them as well, but I don't recall
the designation....Red ones were the civilian issue.

The EF50 has been described as "the valve that won the war" so ubiquitous
was it and so advanced in performance compared to other valves of the time.
I'm sure I recall my late father saying the H2S set had over 100 of them,
and it was unknown for them all to be working simultaneously!

Might go and dig some out and try a new LF preamp. (need all my 807's for
the PA.....)

Regards to all

Paul G4MD
E-mail Paul :- slowpoke@ntlworld.com



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 13 Mar 2001 15:08:35 +0000
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Re. E88cc in parallel
References: <000101c0aba4$4b4d0960$b383883e@lvm> <3AADF9C0.E15D68E7@virgin.net>
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In message <3AADF9C0.E15D68E7@virgin.net>, Stewart Bryant
<stewart.bryant@virgin.net> writes
>
>
>LAWRENCE MAYHEAD wrote:
>
>> Alan is right,when I was at Hanslope I saw the 807 distribution amps and
>> also some using EF80s the red metal case valve . Those Rhombic ants were
>> enormous so I guess the signals were pretty large. 73s Laurie.
>
>Weren't the red cased valves Mullard EF50s? (also available in silver)

Yes, and the taller ones were EF55 IIRC. I once won a small prize for
guessing that the X-ray photograph of the inside of a valve was an EF50!

Mike
-- 
M.J.Powell


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Date: Tue, 13 Mar 2001 09:18:36 -0800 (PST)
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Subject: Re: LF: Re. E88cc in parallel
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Hi All,
That's my memory too - i.e. the red or aluminium cans were EF50s. Why some
were red I don't think I ever knew. They were popular for RF and IF strips.
You could walk away with big boxes full of them for a £1 in Lyle Street.
Those were the days.
73, John, G4CNN






_______________________________________________________
Send a cool gift with your E-Card
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
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References: <000101c0aba4$4b4d0960$b383883e@lvm>
Subject: LF: Re: Re. E88cc in parallel
Date: Tue, 13 Mar 2001 17:16:47 +0100
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To All from PA0SE

The red metal valve must have been an EF50.

73, Dick, PA0SE



> Alan is right,when I was at Hanslope I saw the 807 distribution amps and
> also some using EF80s the red metal case valve . Those Rhombic ants were
> enormous so I guess the signals were pretty large. 73s Laurie.
> 
> 
> 



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Re. E88cc in parallel
Date: Tue, 13 Mar 2001 12:56:53 -0000
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Sorry your dead right put it down to anno domini 73s Laurie.
-----Original Message-----
From: Stewart Bryant <stewart.bryant@virgin.net>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 13 March 2001 11:14
Subject: Re: LF: Re. E88cc in parallel


>
>
>LAWRENCE MAYHEAD wrote:
>
>> Alan is right,when I was at Hanslope I saw the 807 distribution amps and
>> also some using EF80s the red metal case valve . Those Rhombic ants were
>> enormous so I guess the signals were pretty large. 73s Laurie.
>
>Weren't the red cased valves Mullard EF50s? (also available in silver)
>
>Stewart G3YSX
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 13 Mar 2001 11:09:41 +0000
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: LF: RE: Active antennas at LF.Wrong valve sp ecified 1
References: <65AECDF1F89AD411900400508BFC869F9C03BF@pdw-mail-1.dera.gov.uk>
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In message <65AECDF1F89AD411900400508BFC869F9C03BF@pdw-mail-
1.dera.gov.uk>, Talbot Andrew <ACTALBOT@dera.gov.uk> writes
>Sorry, I confused you all and remembered the wrong device.  The valves
>are E55L Pentodes.   (E88CC is a doube triode, sort of ECC88 then they
>ran out of numbers! )

IIRC The E88CC was a reliable form of the ECC88, gold-plated everything.
Quite common in TV B/C in the 60s.

Mike
-- 
M.J.Powell


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LAWRENCE MAYHEAD wrote:

> Alan is right,when I was at Hanslope I saw the 807 distribution amps and
> also some using EF80s the red metal case valve . Those Rhombic ants were
> enormous so I guess the signals were pretty large. 73s Laurie.

Weren't the red cased valves Mullard EF50s? (also available in silver)

Stewart G3YSX



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Paul Keinanen" <keinanen@sci.fi>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Active antennas at LF.Wrong valve sp ecified 1
Date: Tue, 13 Mar 2001 12:04:41 +0200
Message-ID: <s9qrat4u17s1h36dq63pg9r8jjfhu4armi@4ax.com>
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On Tue, 13 Mar 2001 08:59:25 -0000, Talbot Andrew
<ACTALBOT@dera.gov.uk> wrote:

>Sorry, I confused you all and remembered the wrong device.  The valves
>are E55L Pentodes.   (E88CC is a doube triode, sort of ECC88 then they
>ran out of numbers! )

I don't think running out of numbers is the reason for these strange
codes. 

At least the Siemens Taschenbuch 1964 lists the ordinary xxnn
(x=letter, n=digit) types as "standard receiving and amplification
tubes", while the xnnx and xnnxx style tubes were listed under
"special tubes", some of which were assosiated with the Reliability,
Long life, Tight tolerance, Vibration and shock proofed and/or Cathode
free from interface attributes.

The first digit usually defined the base, thus 3n, 3nn were Octal, 8n,
8nn, 8nnn were Noval and 9n, 9nn Miniatur. However, 13n, 23n could
also be Octal and 18n, 28n could also be Noval.
 
So I do not think the reason for going to xnnxx format is simply due
to running out of xxnn, xxnnn numbers.
 
>FETs are much easier to understand - wonder if a solid state version has
>been produced yet ?

Are you referring to Fetrons, which appeared around 1972 and had the
same base connection as the tube counterpart and you  could just swap
the corresponding tube with this high voltage FET ?

Paul OH3LWR



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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: "rsgb lf group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Re. E88cc in parallel
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Alan is right,when I was at Hanslope I saw the 807 distribution amps and
also some using EF80s the red metal case valve . Those Rhombic ants were
enormous so I guess the signals were pretty large. 73s Laurie.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alberto di Bene" <dibene@usa.net>
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Subject: LF: Re: Active antennas at LF.Wrong valve specified
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> Sorry, I confused you all and remembered the wrong device.  The valves
> are E55L Pentodes.   (E88CC is a doube triode, sort of ECC88 then they
> ran out of numbers! )
>

The E88CC was a professional (military?) version of the ECC88. More tightly
controlled specs, more ruggedized, etc.  All the professional versions had that
reversal between the last two groups of letters and digits.

73  Alberto  I2PHD




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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Active antennas at LF.Wrong valve sp	ecified 1
Date: Tue, 13 Mar 2001 08:59:25 -0000
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Sorry, I confused you all and remembered the wrong device.  The valves
are E55L Pentodes.   (E88CC is a doube triode, sort of ECC88 then they
ran out of numbers! )

The E55L  presumably belongs to the EL55 family, 6.3V heaters, power
pentode Octal base - Its all coming back to me now,  the only time I
ever used valves was back in teen years in the early 1970s

Circuit is :
Grid2 connected to anode and decoupled to ground.
Input to each Grid1 from antenna connection via a 270 ohms stopper on
each valve.
Grid3 connected direct to cathode, 100 ohms from each valve to common
output point, DC choke to gnd so the 100R acts as both cathode load and
RF stopper / attenuator.
Three of these blocks in parallel.  250V supply, positive grid bias
applied to all 3 valves at comon input point adjustable 0 - 2V.

This was described to me as a sort of cascode circuit but all internal
to the one pentode structure - looks more like normal pentode operation
to me.

FETs are much easier to understand - wonder if a solid state version has
been produced yet ?

Andy  

> -----Original Message-----
> From: Walter Blanchard [mailto:blanch@pncl.co.uk]
> Sent: 2001-03-12 21:27
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Active antennas at LF.
> 
> 
> In the 1960's I had an active aerial using an 807 as the 
> front-end - with 
> 600v on it too!
> Later modified to use an E186F instead. Why are they using 
> double triode 
> E88CC?
> Can't possibly have the slope and overload characteristics of 
> an E186F.
> 
> Walter G3JKV.
> 
>   
> 
> 


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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>
Subject: LF: E88CCs in parallel
Date: Tue, 13 Mar 2001 00:10:26 -0000
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Hi Andy and Andre' it sounds a bit more like....MMMmm we have rather a lot
of those left in the stores....I wonder what we can use 'em for! I have a
feeling that the 'frame-grid' valves ( 'tubes'  for Andre's benefit) were
fairly susceptible to grid overvolts. At least a lot more so than the
standard grid structures. That is based on Oceanic submerged repeater
experience, where they see a 15kV pulse when your friendy trawlerman decides
not to wait for the compensation for his snagged nets, and puts his axe
through the cable!. Still I suppose they are still a bit better than
'3-legged fuses'.

I have seen suggestions of transistors like VMP-1s and VMP-4s (a bit old now
but VMOS VHF power devices) for good big signal handling capability at HF,
but you would certainly need static protection on those, which does tend to
defeat the object.

Wasn't the 807 (like Walter's) running about 20-30mA praised up for its
performance as an aerial distribution amp, at Hanslope Park and Bletchly
Park.
Despite the use of many HROs which can put a considerable number of mVs of
local oscillator signal out of the aerial socket. (I have even seen TVI on
Band I from an HRO)

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: "Andre' Kesteloot" <andre.kesteloot@ieee.org>
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Subject: Re: LF: Active antennas at LF.
References: <65AECDF1F89AD411900400508BFC869F9C03BE@pdw-mail-1.dera.gov.uk> <5.0.2.1.2.20010312211617.00a8e050@mail.pncl.co.uk>
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Walter Blanchard wrote:

>  Why are they using double triode
> E88CC?

a cascode circuit, no doubt, as was used in TV tuners of yesteryear...
And connect several in parallel for reliability.
73
Andre' N4ICK




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andre' Kesteloot" <andre.kesteloot@ieee.org>
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Talbot Andrew wrote:

> Incidently, returning to an earlier topic, the current Naval standard HF
> receiving antenna on board ships is an active whip, made from a 2m
> length of 50mm diameter Al pole.   The amp is made from three E88CC
> valves in parallel, operating in a cascode / common collector circuit.

Indeed, in case of EMP, a valve preamplifier would have better chances
of
surviving. 
Andre' N4ICK




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <002101c0ab3e$61b444e0$ecde043e@mh70i>
From: "DE BONDT WERNER" <w.bondt@belgacom.net>
To: rsgb_lf_group@blacksheep.org
References: <000201c0aa55$65fa04c0$45df043e@mh70i> <3AACCF46.7D9A19B9@mailsrv.dii.unisi.it>
Subject: Re: LF: sin
Date: Mon, 12 Mar 2001 22:49:56 +0100
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Nice to hear from you Valerio . Sin s forgiven .
Hope to hear you soon on the band 73 .

Abt the sin of Dave I am not sure the involve LF  hi .
73 Werner ON6ND

----- Original Message ----- 
From: valerio gabbani <valerio@firewall.dii.unisi.it>
To: <rsgb_lf_group@blacksheep.org>
Sent: Monday, March 12, 2001 2:29 PM
Subject: Re: LF: sin


> DE BONDT WERNER wrote:
> 
> > Nice sig from IK5ZPV  at 17-50  rst 5-4-9But He was listening in
> > visual CW !Its a sin . Best 73 to all Werner  ON6ND
> 
> Hello Werner,
> i was listening by ear also,signal to noise ratio was too low for my not
> well trained ears but high enaugh for spectrogram.
> Werner thank you for report , hope to meet you again  with better cndx.
> '73, Valerio (IK5ZPV)
> 
> 
> 



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: LF: Active antennas at LF.
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In the 1960's I had an active aerial using an 807 as the front-end - with 
600v on it too!
Later modified to use an E186F instead. Why are they using double triode 
E88CC?
Can't possibly have the slope and overload characteristics of an E186F.

Walter G3JKV.

  



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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hi Mike I'll be looking.   Yes looked like short stuff last night
73 de john VE1ZJ
PS Jack very happy    as am I
"mike.dennison" wrote:

> > No AQC  Beacon tonight. Will resume if requested. 73s Laurie
>
> I will beacon tonight on 135.9230kHz, 60s dots.
>
> Mike, G3XDV



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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> No AQC  Beacon tonight. Will resume if requested. 73s Laurie

I will beacon tonight on 135.9230kHz, 60s dots.

Mike, G3XDV



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: "rsgb lf group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Re. Beacon
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No AQC  Beacon tonight. Will resume if requested. 73s Laurie



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Rabson" <word.factory@zetnet.co.uk>
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References: <65AECDF1F89AD411900400508BFC869F9C03BE@pdw-mail-1.dera.gov.uk>
Subject: LF: Re: Active antennas at LF.
Date: Mon, 12 Mar 2001 18:28:10 -0000
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Now that's a thought. I have some E88CCs somewhere...

----- Original Message ----- 
From: Talbot Andrew <ACTALBOT@dera.gov.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Monday, March 12, 2001 4:32 PM
Subject: LF: RE: Manual and active antennas at LF.


> Incidently, returning to an earlier topic, the current Naval standard HF
> receiving antenna on board ships is an active whip, made from a 2m
> length of 50mm diameter Al pole.   The amp is made from three E88CC
> valves in parallel, operating in a cascode / common collector circuit.

73 de
John Rabson G3PAI




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>
Organization: University of Hertfordshire
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Date: Mon, 12 Mar 2001 18:25:29 +0000
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Subject: LF: Re: Active antennas at LF.
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<?color><?param 0100,0100,0100>Dear Andy, LF Group,<br><br>&gt;<?/color>The amp is specified as having a 50dBm third order intercept  &gt;point and by my reckoning could function as a power amp  &gt;delivering over 10W.   That's linear !!! Frequency response is  &gt;10kHz to 60MHz.   <?color><?param 0100,0100,0100><br><br>Sounds like the kind of thing I could do with - living near Brookmans  Park gives me MF field strengths of the order of 10V/m RMS, and  much higher than that on the peaks. I abandoned attempts to make  a wideband whip when I observed about 40v pk-pk RF on a 1m  antenna connected to a scope probe... <?/color> A tuned input certainly  makes life easier sometimes!<?color><?param 0100,0100,0100><br><br>I read somewhere that pre-WW2 naval receiving systems, using  basically long-wire antennas, were designed to operate with "up to  100V" unwanted signal on the antenna, with frequency separation  of 10% or more. This was achieved using passive preselectors.  The ob
jective was to allow simultaneous multi - transmitter  operation. When the war broke out, it was not found to be a big  issue, because radio transmission from ships was kept to an  absolute minimum to avoid direction-finding. <br><br>Cheers, Jim Moritz<br>73 de M0BMU<br><br>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Nick" <maad65@dial.pipex.com>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: RE: Manual and active antennas at LF.
Date: Mon, 12 Mar 2001 18:10:47 +0000
Message-ID: <464qat0hlkdbs78001jnt1mm93oedqvqik@4ax.com>
References: <65AECDF1F89AD411900400508BFC869F9C03BE@pdw-mail-1.dera.gov.uk>
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On Mon, 12 Mar 2001 16:32:03 -0000, you wrote:

>
>Ships do have the advantage of a near perfect groundplane

Not the fibre glass ones :-(

Nick
G4WHO


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "tracey.gardner" <tracey.gardner@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: 1792 coupling caps
Date: Mon, 12 Mar 2001 17:53:15 -0000
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In my manual all the RF coupling capacitors, C1, C4 & C11, in
the 1792
front end are shown/listed as 1uF.

The manual is Issue 8.5.85-350 and is for the RA1792
(83000,82129 and 85830)
apparently these model numbers relate to different
synthesisers.

The guy that I bought the manual from wanted to know the
serial number etc
before he supplied a copy to me.

The manual quotes the frequency range as being 150kHz - 30MHz.

Brian's 50v rated capacitor went short circuit and proceeded
to put the 15v
supply to earth via an 18 ohm resistor needless to say it
cooked very quickly!
Perhaps that's why they changed to 100v rating in later
models?


73s Tracey





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Manual and active antennas at LF.
Date: Mon, 12 Mar 2001 16:32:03 -0000
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I think you have later versions of the 1792.  My one only tunes in 10Hz
steps and I know others mentioned on this reflector have 1Hz tuning.
Wonder if the later version is specified down to a lower frequency.

Incidently, returning to an earlier topic, the current Naval standard HF
receiving antenna on board ships is an active whip, made from a 2m
length of 50mm diameter Al pole.   The amp is made from three E88CC
valves in parallel, operating in a cascode / common collector circuit.
A company somewhere is working on a solid state replacement based around
power FETs, but don't know the progress on that.   The amp is specified
as having a 50dBm third order intercept point and by my reckoning could
function as a power amp delivering over 10W.   That's linear !!!
Frequency response is 10kHz to 60MHz.   

Ships do have the advantage of a near perfect groundplane so presumably
they can get away with this sort of antenna to lower freqs than normal.

Andy  'JNT


> C1,4,11 are all marked as 1 not 0u1 on both the cd and the components
> list.  The only difference is that 1 is a polyester 100v 
> whereas 4 and 11 are
> ceramics 50v.  Unfortunately nowhere on the five sheets sent 
> to me by the
> vendor is there an issue or date reference.  Still, with the 
> components
> I had to hand, it now works, if out of spec.
> 
> Thanks to all who took the trouble to send information, it is much
> appreciated.
> 
> 73, Brian
> > >is private and is intended solely for the intended recipient(s).
> >For those other than the recipient any disclosure, copying, 
> distribution, 
> >or any action taken or omitted to be taken in reliance on 
> such information is
> >prohibited and may be unlawful.
> >
> >
> >
> 73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
> http://homepage.esoterica.pt/~brian
> 
> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Mar 2001 15:45:41 +0000
To: rsgb_lf_group@blacksheep.org
From: "Brian Rogerson" <brian@esoterica.pt>
Subject: Re: LF: RE: Manual
In-reply-to: <65AECDF1F89AD411900400508BFC869F9C03BC@pdw-mail-1.dera.gov .uk>
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Andy and Tracey, possibly others,

C1,4,11 are all marked as 1 not 0u1 on both the cd and the components
list.  The only difference is that 1 is a polyester 100v whereas 4 and 11 are
ceramics 50v.  Unfortunately nowhere on the five sheets sent to me by the
vendor is there an issue or date reference.  Still, with the components
I had to hand, it now works, if out of spec.

Thanks to all who took the trouble to send information, it is much
appreciated.

73, Brian


At 14:47 12/03/01 -0000, you wrote:
>Well, my manual shows it in the parts list as 1uF 50V but since the
>highest voltage in the RA1792 anywhere is 28V, and only 15V on the RF
>AMP then I would have thought 25V would do.
>
>However,  the circuit diagram shows it as 0.1uF.  As this coupling cap
>is in a 50 ohm part of the circuit and the RA1792 is specified down to
>150kHz (Yes, we all know it goes a lot lower !), 0.1uF gives a break
>point at 32kHz so I guess 0.1uF is the correct value and the parts list
>is wrong.  C4, doing a similar function before the amp, is 0.1uF
>
>Andy  G4JNT
>
>
>
>> -----Original Message-----
>> From: tracey.gardner [mailto:tracey.gardner@ntlworld.com]
>> Sent: 2001-03-12 13:56
>> To: rsgb_lf_group@blacksheep.org
>> Subject: LF: Re: RE: Manual
>> 
>> 
>> Hi Andy
>> 
>> My 1792 manual shows C11 on the RF amp board to be 1uF 100v
>> whereas Brian's manual shows it to be 50v.
>> 
>> 73s Tracey
>> 
>> 
>> 
>> > I have access to a RA1792 manual, is there any particualr
>> area / info
>> >you need ?
>> >Farnell do a radial 1uF ceramic capacitor - part no. 287-064.
>> >
>> > Andy  G4JNT
>> >
>> 
>> 
>> 
>
>
>-- 
>The Information contained in this E-Mail and any subsequent correspondence
>is private and is intended solely for the intended recipient(s).
>For those other than the recipient any disclosure, copying, distribution, 
>or any action taken or omitted to be taken in reliance on such information is
>prohibited and may be unlawful.
>
>
>
73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
http://homepage.esoterica.pt/~brian



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Manual
Date: Mon, 12 Mar 2001 14:47:09 -0000
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Well, my manual shows it in the parts list as 1uF 50V but since the
highest voltage in the RA1792 anywhere is 28V, and only 15V on the RF
AMP then I would have thought 25V would do.

However,  the circuit diagram shows it as 0.1uF.  As this coupling cap
is in a 50 ohm part of the circuit and the RA1792 is specified down to
150kHz (Yes, we all know it goes a lot lower !), 0.1uF gives a break
point at 32kHz so I guess 0.1uF is the correct value and the parts list
is wrong.  C4, doing a similar function before the amp, is 0.1uF

Andy  G4JNT



> -----Original Message-----
> From: tracey.gardner [mailto:tracey.gardner@ntlworld.com]
> Sent: 2001-03-12 13:56
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: RE: Manual
> 
> 
> Hi Andy
> 
> My 1792 manual shows C11 on the RF amp board to be 1uF 100v
> whereas Brian's manual shows it to be 50v.
> 
> 73s Tracey
> 
> 
> 
> > I have access to a RA1792 manual, is there any particualr
> area / info
> >you need ?
> >Farnell do a radial 1uF ceramic capacitor - part no. 287-064.
> >
> > Andy  G4JNT
> >
> 
> 
> 


-- 
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is private and is intended solely for the intended recipient(s).
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "tracey.gardner" <tracey.gardner@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: RE: Manual
Date: Mon, 12 Mar 2001 13:56:10 -0000
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Hi Andy

My 1792 manual shows C11 on the RF amp board to be 1uF 100v
whereas Brian's manual shows it to be 50v.

73s Tracey



> I have access to a RA1792 manual, is there any particualr
area / info
>you need ?
>Farnell do a radial 1uF ceramic capacitor - part no. 287-064.
>
> Andy  G4JNT
>




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Date: Mon, 12 Mar 2001 14:29:42 +0100
From: "valerio gabbani" <valerio@mailsrv.dii.unisi.it>
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Subject: Re: LF: sin
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DE BONDT WERNER wrote:

> Nice sig from IK5ZPV  at 17-50  rst 5-4-9But He was listening in
> visual CW !Its a sin . Best 73 to all Werner  ON6ND

Hello Werner,
i was listening by ear also,signal to noise ratio was too low for my not
well trained ears but high enaugh for spectrogram.
Werner thank you for report , hope to meet you again  with better cndx.
'73, Valerio (IK5ZPV)



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Manual
Date: Mon, 12 Mar 2001 08:41:55 -0000
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 I have access to a RA1792 manual, is there any particualr area / info
you need ?
Farnell do a radial 1uF ceramic capacitor - part no. 287-064.

 Andy  G4JNT
 
 > -----Original Message-----
 > From: Brian Rogerson [mailto:brian@esoterica.pt]
 > Sent: 2001-03-10 15:16
 > To: rsgb_lf_group@blacksheep.org
 > Subject: LF: Manual
 > 
 > 
 > Gentlemen,
 > 
 > Can anyone point me in the direction of a RA1792 tech manual/circuit
 > diagrams and more specifically a 1uF 50v ceramic capacitor, radial
 > leads about 0.3in spacing.
 > 
 > 73, Brian
 > 73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
 > http://homepage.esoterica.pt/~brian
 > 
 > 


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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>
Subject: LF: DX Cluster spots for 10/11Mar at GB7DXM
Date: Sun, 11 Mar 2001 21:26:10 -0000
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Hi all, no G spots but quite a bit of activity reported to the east .
Despite hearing that Jack had got a new computer I have not seen any cluster
activity from him on 160m, which is where he usually posts his LF activity
shedule (1800.0) as well as his normal Top-Band activity. I believe there
was a lot of snow early in the month, and some ice-storms.

CFH returned on Friday evening for a run overnight and went off again at
about 1900z on Saturday. It came on again this afternoon (Sun) and is still
active at 2100z so there could well be another chance of a full overnight
plot. It is still running just a 'carrier'. This is about 45Hz low of the
nominal center frequency.  Usually when it is visible in daytime it suggests
high levels of ionisation in the D-layer and it does not augur well for
nightime conditions. The Friday/Saturday plot showed the characteristics of
a quiet or undisturbed ionosphere, with no signs of high absorbtion of deep
fading, despite daytime visibility of the signal.

Cluster spots follow :-
   137.5  DF6NM       11-Mar-2001 1531Z  psk31
<DL6SN>
   137.7  DJ2LF       11-Mar-2001 1512Z  qrss- vy weak now
<DL6SN>
   137.7  I5TGC       11-Mar-2001 1458Z  29Hz above DJ2LF, CQ
<OM2TW>
   137.7  DJ2LF       11-Mar-2001 1457Z  CQ QRSS
<OM2TW>
   137.7  I5TGC       11-Mar-2001 1448Z  cq qrss
<DL6SN>
   136.6  DL3FDO      11-Mar-2001 1418Z  cq
<DL6SN>
   136.7  DK6NI       11-Mar-2001 1418Z  cq
<DL6SN>
   137.7  OM2TW       11-Mar-2001 1230Z  cq qrss
<DL6SN>
   136.5  DJ9IE       11-Mar-2001 1059Z  in qso with dj2lf
<DL6SN>
   137.0  DL3FDO      11-Mar-2001 1035Z  559
<DL1SAN>
   137.7  IK5ZPV      11-Mar-2001 0957Z  cq qrss
<DL6SN>
   136.4  PA0BWL      11-Mar-2001 0945Z  cq
<DL6SN>
   136.8  DL1SAN      11-Mar-2001 0942Z
<DL6SN>
   136.8  DJ2LF       11-Mar-2001 0940Z
<DL6SN>
   136.7  DJ2LF       11-Mar-2001 0938Z  579 cq - vy strong today
<DL1SAN>
   137.7  DL7YA       11-Mar-2001 0938Z  cq dfcw
<DL6SN>
   137.7  DJ2LF       10-Mar-2001 1520Z  qrss cq
<DL6SN>
   136.6  DJ9IE       10-Mar-2001 1039Z  cq
<DL6SN>
   137.7  OM2TW       10-Mar-2001 1015Z  cq qrss
<DL6SN>
   136.5  OM5CW       10-Mar-2001 0749Z  QRSS
<OM2TW>
   136.5  OK1DKJ       7-Mar-2001 1242Z  cq test
<OK1RP>
G3NYK de GB7MRS 11-Mar-2001 2105Z >

Cheers de Alan  G3NYK   JO02PB
Alan.Melia@btinternet.com




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Pick" <pick@sniffout.com>
To: rsgb_lf_group@blacksheep.org
References: <000201c0aa55$65fa04c0$45df043e@mh70i>
Subject: LF: Re: sin
Date: Sun, 11 Mar 2001 20:59:44 -0000
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<DIV><FONT face=Arial size=2>I like a bit of sin every now and 
then!</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Dave G3YXM</FONT></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:w.bondt@belgacom.net" title=w.bondt@belgacom.net>DE BONDT 
  WERNER</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> Sunday, March 11, 2001 6:00 
PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: sin</DIV>
  <DIV><BR></DIV>
  <DIV><FONT face=Arial size=2>Nice sig from IK5ZPV&nbsp; at 17-50&nbsp; rst 
  5-4-9</FONT></DIV>
  <DIV><FONT face=Arial size=2>But He was listening in visual CW !</FONT></DIV>
  <DIV><FONT face=Arial size=2>Its a sin .</FONT></DIV>
  <DIV>&nbsp;</DIV>
  <DIV><FONT face=Arial size=2>Best 73 to all Werner&nbsp; 
ON6ND</FONT></DIV></BLOCKQUOTE></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "DE BONDT WERNER" <w.bondt@belgacom.net>
To: rsgb_lf_group@blacksheep.org
Subject: LF: sin
Date: Sun, 11 Mar 2001 19:00:45 +0100
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<DIV><FONT face=Arial size=2>Nice sig from IK5ZPV&nbsp; at 17-50&nbsp; rst 
5-4-9</FONT></DIV>
<DIV><FONT face=Arial size=2>But He was listening in visual CW !</FONT></DIV>
<DIV><FONT face=Arial size=2>Its a sin .</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>Best 73 to all Werner&nbsp; 
ON6ND</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: friday night
Date: Sat, 10 Mar 2001 23:35:00 -0000
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Fine John just the info I needed. I will revert to the wider spacing. 73s
Laurie.
-----Original Message-----
From: John Currie <john.currie@ns.sympatico.ca>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 10 March 2001 20:48
Subject: LF: friday night


>M0BMU and G3AQC were visible for hours last night
>    Laurie I prefer the earlier spacing  .  The last 2 nights sigs were
>harder to read when only "M" copy during QSB
>              73 de John VE1ZJ
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 10 Mar 2001 17:01:56 EST
Subject: Re: LF: QRS v3.05
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Thanks, Rik, for another splendid piece of software!  It will be available 
from the lwca.org site this weekend.

73,
John


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Date: Sat, 10 Mar 2001 20:42:39 -0500
From: "John Currie" <john.currie@ns.sympatico.ca>
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M0BMU and G3AQC were visible for hours last night
    Laurie I prefer the earlier spacing  .  The last 2 nights sigs were
harder to read when only "M" copy during QSB
              73 de John VE1ZJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Claudio" <cla.po@tiscalinet.it>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: <TECH>Transatlantic modes - what next?
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Hello LF group,

I agree with Rik arguments about BPSK and I add some more considerations.
 
On 07-Mar-01 Rik Strobbe wrote:
> Hello Jim & group,
> 
> Excellent paper from Jim, it seems a good starting point for an open
> discussion.
> 
> SNIP

> 
> An additional difference occurs at the RX side. QRSS/DFCW are received
> 'wideband', this means you can observe a rather big part of the spectrum
> for DFCW/QRSS signals. This has the advantage that, even at signal
> bandwidths of 0.01Hz, there is nor problem to 'hit' the transmitted signal.
> One can even 'decode' more that one signal at the same time. Opposite to
> this all receiving software for BPSK / WOLF is 'narrowband'. This means
> that you have to 'hit' the transmitted signal very accurate and you can
> receive only 1 signal at a time.
> 
> SNIP
> So far my contribution,
> 
> 73, Rik  ON7YD

BPSK modulation is very sensitive to carrier frequency shift or difference
between transmitter and receiver. The receiver must be frequency locked to the
carrier, if the difference between TX and RX frequency is more that one tenth
of the bit rate you must add some circuit to scan the RX frequency and lock the
receiver local oscillator (do it in hardware or software, doesn't matter) to
the carrier (kiked oscillator ;-) ). After the carrier is locked, the receiver
does lock the data bit clock, this require a training sequence (some data bits
that doesn't carry useful informations) and synchronize the RX side data rate
clock with the transmit side. Those bits are lost and add some time to QSO time.
In general BPSK is easy to implement for hight bit rate

I think that you can ask more to some OSCAR satellite guru about the BPSK
modulation.

73 de Claudio, ik2pii

----------------------------------------------------------------------
Claudio Pozzi       http://www.qsl.net/ik2pii       happy Linux user
E-Mail: Claudio <cla.po@tiscalinet.it> <ik2pii@amsat.org>
Date: 10-Mar-01   Time: 16:26:23
This message was sent by XFMail
----------------------------------------------------------------------


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Brian Rogerson" <brian@esoterica.pt>
Subject: LF: Manual
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Gentlemen,

Can anyone point me in the direction of a RA1792 tech manual/circuit
diagrams and more specifically a 1uF 50v ceramic capacitor, radial
leads about 0.3in spacing.

73, Brian
73 Brian     CT1DRP     IN51QD     41 09 58N  08 39 11W
http://homepage.esoterica.pt/~brian



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 10 Mar 2001 14:51:16 +0100
From: "Ko Versteeg" <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Lf Engineering A Hoax?
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Group..

Has anyone ever tried products from Lf Engineering USA?
Found at: http://www.lfengineering.com/
Reason for this is they have not been answering my 
messages for 2 weeks... One year ago they DID answer.

Do they still excist or is it an abandoned website 
that's left, just like many other sites ?

73 de Ko, NL9222



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
Subject: LF: Test
Date: Fri, 9 Mar 2001 22:57:10 -0000
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=#ffffff>
<DIV>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 9 Mar 2001 20:15:47 +0100
From: "Ko Versteeg" <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: QRS v3.05
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At 3/9/01 10:55:00, you wrote:
>Hello all,
>
>I got a new version of QRS (v3.05) ready for release. It is sent to LCWA,
>G3YXM and NL9222, so should be downloadable via these websites soon.
>For the impatient I will have it on my website temporarily (just over the
>weekend) for downloading :
>
>http://www.qsl.net/on7yd/QRS/qrs305.zip
>
>I want to thank everybody who gave me 'feedback', especially Laurie
>(G3AQC), Jim (M0BMU) and Mike (ZL4OL) for the testing and bug reporting of
>the trail versions and also John (KD4IDY), Dave (G3YXM) and Ko (NL9222) for
>making it available through their websites.
>
>73, Rik  ON7YD
>
>
>
>

Rik and all.
Just uploaded the new Qrs and the pages, look for the "new" image
or just follow the alphabet :-) 

A good weekend all and 73
Ko Versteeg, NL9222.

Oh it can be found via:
http://home.wanadoo.nl/nl9222/index.htm
http://leden.tref.nl/~nl9222tv/default.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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<!doctype html public "-//w3c//dtd html 4.0 transitional//en">
<html>
<body bgcolor="#FFFFFF">
Hi Laurie saw you"M" from 2305 til fade oput 2346 Lwft house 0015 back
0400 0400 you were ")" copy
<p>LAWRENCE MAYHEAD wrote:
<blockquote TYPE=CITE><style></style>
<font face="Arial"><font size=-1>I
wont be able to start until 22:00utc tonight. Slightly different format,
DFCW, shift now 0.15Hz centered on 135.922. Also slightly shorter inter-element
spacing (15secs was 20 secs)</font></font><font face="Arial"><font size=-1>saving
2mins on each call at the expense of readability? Hope for some propagation,
reports welcome.&nbsp; 73s Laurie.</font></font></blockquote>

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Subject: LF: Tonight-G3XDV/G3AQC
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LAWRENCE MAYHEAD schrieb:
> I wont be able to start until 22:00utc tonight. Slightly different format,
>  DFCW, shift now 0.15Hz centered on 135.922. Also slightly shorter
>  inter-element spacing (15secs was 20 secs)
> saving 2mins on each call at the expense of readability? Hope for some
>  propagation, reports welcome.  73s Laurie. 
>
=Hi Laurie
Hi Mike
got an other pic (see enclosure).
relat. rx-input-voltage and QRG meassured over ten minutes at 2210utc on 
08.03.2001:
G3AQC 51 - 53 db, 135,922.14 - .09 / 135,921.98 - .93 kHz (if G3XDV was exactly
on his ann. QRG.)
G3XDV 41 - 46 db, 135.922.98 - 923.00 kHz
noise 11 - 29 db
regards
Uwe/dj8wx - jo43sv - dds-contr.rx - QRG calibr. with PeakTech 2840 -  
inv.Vee340/400mlws.ant #

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--------------000906080902080109050205--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000401c0a871$bd91e580$1ad01bd4@OK1FIG>
From: "Petr Maly" <ok1fig@volny.cz>
To: rsgb_lf_group@blacksheep.org
References: <001301c0a4ea$a0799900$cd666ec3@cestag>
Subject: LF: Re: new station
Date: Mon, 5 Mar 2001 21:19:28 -0000
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<DIV><FONT face=Arial size=2>Ruda lives in the same city as me. Actually it was 
me who "infected" him to go on for LF. He uses LW 80 meters (slopping) and 
listens on IC-756.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>73 Petr OK1FIG</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:cestag@dada.it" title=cestag@dada.it>cesare tagliabue</A> 
  </DIV>
  <DIV style="FONT: 10pt arial"><B>To:</B> <A 
  href="mailto:rsgb_lf_group@blacksheep.org" 
  title=rsgb_lf_group@blacksheep.org>LF group</A> </DIV>
  <DIV style="FONT: 10pt arial"><B>Sent:</B> Sunday, March 04, 2001 8:35 
PM</DIV>
  <DIV style="FONT: 10pt arial"><B>Subject:</B> LF: new station</DIV>
  <DIV><BR></DIV>
  <DIV><FONT color=#000000 size=2>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 
  <FONT color=#000000>Hi all</FONT></FONT></DIV>
  <DIV><FONT color=#000000 size=2><FONT 
  color=#000000></FONT>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; This afternoon 
  Sun 4 March, around 14.15 UTC I've heard the new OK station OK1DTN calling CQ, 
  the signal was very strong, 579 here in Florence; this station seems to be 
  well equipped.</FONT></DIV>
  <DIV><FONT color=#000000 size=2></FONT><FONT size=2>&nbsp; 73&nbsp; 
  Cesare</FONT></DIV>
  <DIV><FONT size=2></FONT>&nbsp;</DIV>
  <DIV><FONT color=#000000 size=2>Cesare Tagliabue&nbsp;&nbsp; I 5 
  TGC<BR>WW-Loc&nbsp; JN53PS<BR>e-mail: <A 
  href="mailto:cestag@dada.it">cestag@dada.it</A><BR>url: <A 
  href="http://www.dadacasa.com/i5tgc">http://www.dadacasa.com/i5tgc</A><BR></FONT></DIV></BLOCKQUOTE></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 09 Mar 2001 06:53:58 +0000
From: "Steve Rawlings" <steve@alg.demon.co.uk>
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Subject: LF: Activity from G6RO
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Hi All,

Many will know that Ron G6RO, for several years, has been a full
time carer for his wife, Doris.  They are both 88 years old.

Ron has written to say that Doris is very poorly and is spending
some time in hospital.  The hospital visiting schedule, among
other things, means that Ron will be less active than usual. 
(His busy caring schedule has always meant that finding time to
operate on any band has been, to say the least, 'difficult'.)

Nevertheless, Ron will be snatching the odd few minutes to check
136, so if you do happen to hear Ron calling 'CQ', please give
him a call. 

Regards to all,
Steve GW4ALG


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
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Date: Thu, 8 Mar 2001 21:31:58 EST
Subject: Re: LF: Re: <TECH>Re: Transcontinental modes - what next?
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Vernall" <vernall@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <3715.200103081328@gemini>
Subject: LF: Re: <TECH>Re: Transcontinental modes - what next?
Date: Fri, 9 Mar 2001 14:43:58 +1300
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Dear James and LF Group,

Your perception of being limited to some 100 Hz of overall bandwidth for
transcontinental LF work is unlikely to be the case in other continents.
Down here we have 165 - 190 kHz, and can even have LF SSB nets, and they
work fine.  Limitation on emission bandwidth is probably the SWR bandwidth
of a typical backyard antenna, and nobody here who has tried SSB has had a
problem.

For digital modes, Shannon's Law is not limited to slow symbol rate, even if
the net recovered data is slow rate.

I still do not believe there needs to be an arbitrary cap of 10 Hz on
digital mode emission bandwidth.  If someone can come up with a cunning
scheme that uses say 50 Hz bandwidth, then it why not use it?

Cheers,

Bob ZL2CA



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. Tonight
Date: Thu, 8 Mar 2001 18:12:27 -0000
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<DIV><FONT face=Arial size=2>I wont be able to start until 22:00utc tonight. 
Slightly different format, DFCW, shift now 0.15Hz centered on 135.922. Also 
slightly shorter inter-element spacing (15secs was 20 secs)</FONT></DIV>
<DIV><FONT face=Arial size=2>saving 2mins on each call at the expense of 
readability? Hope for some propagation, reports welcome.&nbsp; 73s 
Laurie.&nbsp;</FONT></DIV></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>
Organization: University of Hertfordshire
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Subject: LF: <TECH>Re: Transcontinental modes - what next?
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Dear Bob, LF group

> Jim,
> 
> Your statement
> 
> > All this means that the spectrum available for 
> > a group of transmitting stations participating in "transatlantic tests"
> > is probably only 100Hz. 
> 
> assumes that the EU band plan can not adapt to demand.
> 
> 73, Bob ZL2CA

Some aspects of band use are not within the power of amateurs to 
do much adapting to - for example CFH and SXV can transmit 
where and when they like in the band, as can the intermods that 
plague some parts of Europe.

The other thing is that the long distance/exotic modes activity is a 
minority interest among LF amateurs - it is not really reasonable to 
fill a large portion of the available band with signals that most of the 
band users cannot make use of. There has already been more than 
enough debate as to whether this is good or bad, but there it is.

So I think operating in small bandwidths is an inevitable part of the 
challenge of LF; it has certainly proved useful with the current crop 
of QRSS type modes, where virtually all the beacon activity has 
fitted easily into a bandwidth as wide as a single CW signal. 

Cheers, Jim Moritz
73 de M0BMU
 




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. QRS 2300 z etc.
Date: Thu, 8 Mar 2001 12:46:26 -0000
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<DIV><FONT face=Arial size=2>Thanks John for the report. Very encouraging to see 
that 30sec dots are coming through even in indifferent conditions,and my power 
still 350mW!.</FONT></DIV>
<DIV><FONT face=Arial size=2>I am sure DFCW is the answer at least for now,until 
something better is thought of, Its not difficult to implement. &nbsp;I use a 
Xtal oscillator with a relay switched capacitor (two bits of wire 
twisted</FONT></DIV>
<DIV><FONT face=Arial size=2>together Hi, so I can always alter the F.Shift 
).</FONT></DIV>
<DIV><FONT face=Arial size=2>I will shorten the dots sometime although 10 sec is 
rather a big jump..</FONT></DIV>
<DIV><FONT face=Arial size=2>Now that Rik has implemented half element spacing, 
we are really shortening the time scale. So as you say even the lower power 
stations have a chance.&nbsp; 73s Laurie..</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Laken, W.H.P.A. van der \(Wil\)" <w.laken@organon.oss.akzonobel.nl>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Hamradio Ralley in Rosmalen
Date: Thu, 8 Mar 2001 12:20:19 +0100
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Saturday 10 March is the (big) Hamradio Ralley in Rosmalen - Holland. 
 
I suggest that lf enthousiasts visiting the ralley can meet and shake hands
at 11:30 at the info-booth.
 
 
73 Wil - PA0BWL
  



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Re. QRS 2300z Mar 7th
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<body bgcolor="#FFFFFF">
Hi Laurie,&nbsp; It seems that 30 second dots is so superior to 3 sec dots
it comes through despite cmes .&nbsp; I thought I saw M0BMU at 2315. I
had "O" copy on G3AQC&nbsp; and M0BMU at 0212.
<br>&nbsp;&nbsp;&nbsp;&nbsp; The German station at 128.9 was S-3 up until
i saw it at S-5 at 0230.&nbsp; By 0246 QRM from 60 Hz wiped me out
<br>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; It is obvious that dfcw is far superior
when it comes to speed of information transfer. I will be sending picture
later
<br>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; There&nbsp; appears to be a third station
just below G3AQC.&nbsp; He is&nbsp; lower by about 1.5 times the difference
between Laurie's dots and dashes
<br>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; I'll be looking from 2100 thru 0000Z
tonight and agn for short period at 0400
<br>&nbsp;&nbsp;&nbsp;&nbsp; I figure 30 sec dots is 10 db better than
3sec dots and from a reliability standpoint&nbsp; this also seems to be
true.&nbsp; Condx like last night would never Have produced readable sigs
with 3 sec dots.&nbsp; I reckon With good condx 100 to 200 milliwatt stations
could get across .&nbsp; The reception of G3XDV proves this
<br>&nbsp;&nbsp; 73 de John VE1ZJ
<p>LAWRENCE MAYHEAD wrote:
<blockquote TYPE=CITE><style></style>
<font face="Arial"><font size=-1>Hi
all.</font></font><font face="Arial"><font size=-1>I was transmitting 30sec
dot DFCW from 20:00 until 07:00 last night, on 135,922 +/-. I saw G3XDV
above me on 135.923,but have no idea where the interleaving signal comes
from.</font></font><font face="Arial"><font size=-1>Looks like propagation
still in trouble from CMEs, will try again tonight. 73s Laurie.</font></font></blockquote>

</body>
</html>

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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. QRS 2300z Mar 7th
Date: Thu, 8 Mar 2001 09:32:20 -0000
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<DIV><FONT face=Arial size=2>Hi all.</FONT></DIV>
<DIV><FONT face=Arial size=2>I was transmitting 30sec dot DFCW from 20:00 until 
07:00 last night, on 135,922 +/-. I saw G3XDV above me on 135.923,but have no 
idea where the interleaving signal comes from.</FONT></DIV>
<DIV><FONT face=Arial size=2>Looks like propagation still in trouble from CMEs, 
will try again tonight. 73s Laurie.</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@rsgb.org.uk>
To: rsgb_lf_group@blacksheep.org
Date: Thu, 8 Mar 2001 09:13:50 -0000
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Subject: LF: Transatlantic tests
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> Many thanks John for the report, I will have another go tonight.
> Same time same format. 73s  Laurie.
> 

I was on last night with 120s dashes, 60s dots, sending "G3XDV" on 
135.923kHz.

I will be on again tonight using those parameters unless anyone wants 
anything different.

73 and thanks for listening.




Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Transcontinental modes - what next?
Date: Thu, 8 Mar 2001 08:35:00 -0000
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www.hf-inst.co.uk has all the documentation and can supply the modules.
It was also written up in the RSGB's Dec 2000 Radio Communication.  

With a 5MHz clock source, it will allow steps as low as 1.1mHz.  WIth
the maximum 120MHz clock, frequency steps will be 0.028Hz.

Andy  G4JNT


> -----Original Message-----
> From: Alberto di Bene [mailto:dibene@usa.net]
> Sent: 2001-03-07 17:27
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: Re: Transcontinental modes - what next?
> > Any URL for this ? Is the interfacing described somewhere on 
> the Internet ?
> Would that board be adequate for steps of  0.16 Hz ?   TNX.
> 
> 73  Alberto   I2PHD
> 
> 
> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Haiko Hebig" <h.hebig@fs.mb.uni-dortmund.de>
Subject: Re: LF: 7S6SAJ antenna demolition
To: rsgb_lf_group@blacksheep.org
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Always sad to see antennas being broken down (but what a
luck for 7S6SAJ being allowed to use it!). I forwarded this
message to the Germany A-DX mailing list (general Shortwave
mailing list). Sadly, I do not understand the Swedish
language - perhaps can give me someone an idea what was said
in the TV coverage?

73, Haiko 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Vernall" <vernall@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <18142.200103071719@gemini>
Subject: LF: Re: <TECH>Re: Transcontinental modes - what next?
Date: Thu, 8 Mar 2001 08:57:41 +1300
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Jim,

Your statement
 
> All this means that the spectrum available for 
> a group of transmitting stations participating in "transatlantic tests" 
> is probably only 100Hz. 

assumes that the EU band plan can not adapt to demand.

73, Bob ZL2CA



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Subject: LF: Re: RE: Transcontinental modes - what next?
Date: Thu, 8 Mar 2001 08:32:29 +1300
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Alberto

> Hi all,
>           which would you all prefer as a way to frequency-shift your TX ?
> With frequency shift I mean many steps, separated by a fraction of an
Hertz.
> The first two possibilities that come to my mind are an audio output from
the
> sound card (requiring then a mixer to bring the tone to the wanted freq.),
> or a binary value output from, say, the parallel port, which then would
require
> a small external board with a DDS or a microcontroller to drive the TX.
>
> No linearity requirements will be needed. I need your input to not start
in a
> false direction.    TNX for any advices.

My preference is to transceive via a PC sound card, and use the likes of an
SSB transceiver, i.e. very little different to practices for HF digital
modes, except much longer message times.  When fine tuning is available on a
sound card, it is a very convenient way to arrange for quite accurate LF
carriers.

73, Bob ZL2CA



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From: "cesare tagliabue" <cestag@dada.it>
To: "LF group" <rsgb_lf_group@blacksheep.org>
Subject: LF: qso ik5zpv/ct1drp
Date: Wed, 7 Mar 2001 19:28:37 +0100
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<DIV><FONT color=#000000 size=2>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; <FONT 
color=#000000>Hi Brian and all</FONT></FONT></DIV>
<DIV><FONT color=#000000 size=2><FONT color=#000000></FONT>&nbsp;&nbsp;&nbsp; 
Yesterday evening, around 20.30 UTC I saw part of your QSO with IK5ZPV, the 
signal from Portugal was very good here in Florence, attached a little 
screenshot.</FONT></DIV>
<DIV><FONT color=#000000 size=2></FONT><FONT size=2>&nbsp;&nbsp;&nbsp; 
73&nbsp;&nbsp; Cesare</FONT></DIV>
<DIV><FONT size=2></FONT>&nbsp;</DIV>
<DIV><FONT color=#000000 size=2>Cesare Tagliabue&nbsp;&nbsp; I 5 
TGC<BR>WW-Loc&nbsp; JN53PS<BR>e-mail: <A 
href="mailto:cestag@dada.it">cestag@dada.it</A><BR>url: <A 
href="http://www.dadacasa.com/i5tgc">http://www.dadacasa.com/i5tgc</A><BR></FONT></DIV></BODY></HTML>

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--------------030001030903080902050105--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "C Andersson" <sm6pxj@swipnet.se>
To: "RSGB LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: 7S6SAJ antenna demolition
Date: Wed, 7 Mar 2001 19:22:14 +0100
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Here's some pictures from the demolition of the longwave antenna in Kraak, Karlsborg which took place yesterday, 06 March.

http://home5.swipnet.se/~w-54761/krk/7s6saj_the_end.htm

And this is what the antenna looked like before:
http://home5.swipnet.se/~w-54761/7s6saj.JPG

The 7S6SAJ operation on 136 kHz (in Feb 2000) became the last time this antenna was in use.

/sm6pxj

(some better pictures may appear later on)




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 07 Mar 2001 18:27:17 +0100
From: "Alberto di Bene" <dibene@usa.net>
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To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Transcontinental modes - what next?
References: <65AECDF1F89AD411900400508BFC869F9C03A2@pdw-mail-1.dera.gov.uk>
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>
> The best route of course is just to use the serial port to control a DDS
> - and HF-Instruments has now supplied around 100 suitable DDS modules.
>

Any URL for this ? Is the interfacing described somewhere on the Internet ?
Would that board be adequate for steps of  0.16 Hz ?   TNX.

73  Alberto   I2PHD




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>
Organization: University of Hertfordshire
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Subject: LF: <TECH>Re: Transcontinental modes - what next?
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Dear LF Group,

Some useful points raised on the subject of Transcontinental 
modes - here are some responses:

The simplest way to improve the capabilities of existing methods is 
undoubtedly what G3LDO suggests - tailoring the QRSS dot length 
to the prevailing conditions. As W4DEX observes, there are often 
times when faster keying could be used to advantage. But to do 
this requires feedback  from receiving to transmitting station so 
that dot lengths at both ends can be adjusted, to acheive any 
benefit. There is no point in the receiving station reducing 
bandwidth without the transmitting station increasing dot length, 
and vice versa. This could be done with the aid of a phone call, HF 
talkback, etc, but to me this is missing the point a bit - it's much 
more impressive if an LF contact can take place without any 
"external assistance". One way to do it might be to change the 
signal reporting system from the TMO good, bad or indifferent, to a 
single letter system where the letters represent "OK for 3s dots", 
"OK for 10s dots" etc. That way, both stations could start with long 
dot lengths, and adjust speed accordingly as the contact 
progressed. If this could be made to work efficiently, I think it would 
be a great help.

I used  the figure of 1 hour for a QSO because in my experience, 
this is a typical duration for a propagation "lift". Occasionally, I 
have seen good signals for up to 2 hours continuously. I don't think 
I have ever seen a 4 hour lift as reported by CT1DRP - maybe 
propagation is different at his more southerly QTH?

I set a bandwidth of 10Hz based on the experience of the last few 
months. The total LF band is 2.1kHz, but a large chunk of this is the 
long standing "CW Only" band segment, and various other parts of 
the band are not really usable at any particular QTH because of 
various types of QRM; CFH for example. As I recall, the use of 
135.9 - 136 was a sort of consensus amongst North American 
stations as to what were usable receiving frequencies for weak 
signals. There are big practical advantages in having 2 segments 
with some separation in frequency. Weak DX stations can then be 
received without the RX being de-sensitised by the local stations 
transmitting to them. All this means that the spectrum available for 
a group of transmitting stations participating in "transatlantic tests" 
is probably only 100Hz. This segment is likely to include assorted 
other narrow-band modes, so there would only be room for one or 
at most 2 MS100, 40Hz bandwidth BPSK signals. In the short term 
this is not a big problem, but with increased activity on this mode it 
would soon become one. Unless a high bit rate proves absolutely 
neccessary, it would seem to make sense in the long term to 
design systems that only require small bandwidths, so that several 
stations can transmit for extended periods without mutual 
interference. For general  QSO use with reasonable signal 
strengths, a wider bandwidth would be perfectly reasonable in the 
digi-modes band segment, with the advantage of quicker QSOs.

 As far as frequency stability requirements go, the recent use of 
very slow QRSS has seen the sudden improvement of amateur LF 
frequency control to within small fractions of 1Hz. It could be made 
better still fairly easily.

For operation of the Decca TX at 1200W PEP in BPSK mode, 
amplitude modulation of the PA DC supply was essential to get 
reasonable sideband levels. It will work quite happily with no 
amplitude control, but the sidebands go on for ever... The 
modulator circuit is quite big of course, but not unreasonably so. 
The unwanted sidebands are 40dB or more down on the main lobe 
of the signal. The overall efficiency is about 75 - 80%, so still much 
better than a linear amplifier. The modulator circuit only needs the 
logic level phase keying signal and the 136kHz carrier as input. At 
the moment, it is hard wired CMOS logic and analogue bits, but 
much of it could be put on a PIC or similar. This eliminates the 
need for a soundcard and it's attendant wrinkles, so excellent 
frequency accuracy and stability are easily achieved. For receive, 
I am using G4JNT's very simple PIC implementation of the VE2IQ 
interface - it is also easy to set up the frequency very accurately 
with this.

To the software developers, I would say that soundcards are 
probably best avoided for BPSK or similar modes. They work fine 
for QRSS, but this mode is relatively not fussy about frequency 
accuracy. I suppose the benefit of a sound card is that it provides 
a ready made A/D, D/A converter module that can be plugged into 
the MIC input of a ready made HF tranceiver to generate an RF 
output. But an HF rig does not make a very good LF transmitter by 
itself, and the combined frequency errors of rig and soundcard, 
plus the "compatability"  issues that come with soundcards, have 
already caused plenty of hair loss, both for software writers and 
the people using them. A transmitter that generates the BPSK 
waveform directly at the RF frequency is simpler overall, and 
probably capable of better performance and efficiency. Any LF 
transmitter requires quite a lot of home construction, and dedicated 
interfaces can be quite simple, so I would suggest that this is the 
better way. The VE2IQ/G4JNT interface already exists for receive, 
and only requires a serial port on the computer, so I guess it  would 
be easier to program too.

It was funny that the postings about the "WOLF" mode crossed 
mine - I have not looked at it thoroughly yet, but I would certainly 
be interested to try some tests.

Cheers, Jim Moritz
73 de M0BMU






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. LF
Date: Wed, 7 Mar 2001 16:53:51 -0000
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<DIV><FONT face=Arial size=2>Many thanks John for the report, I will have 
another go tonight.</FONT></DIV>
<DIV><FONT face=Arial size=2>Same time same format. 73s&nbsp; 
Laurie.</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@rsgb.org.uk>
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Date: Wed, 7 Mar 2001 16:37:24 -0000
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Subject: LF: Chat Room
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> 73 de John VE1ZJ   PS how does one get on the DJ8WL chat line?

John,

This should be the DK8KW chat room. DJ8WL is the late Peter Bobeck (alias 
DA0LF) and I am very much afraid that I gave his call to you in error. 

The chat room is at: http://www.qru.de/chat.htm



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 07 Mar 2001 16:12:01 -0800
From: "John Currie" <john.currie@ns.sympatico.ca>
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Hi all, Condx were quite poor last night, but G3AQC was readable  from
2300 hours for a couple of hours.  He was only "M" copy .  Most of the
time I did not have the 60 Hz QRM

73 de John VE1ZJ   PS how does one get on the DJ8WL chat line?



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Sergeant" <dsergeant@btinternet.com>
To: rsgb_lf_group@blacksheep.org
References: <14313.200103061746@gemini>
Subject: LF: Re: <TECH>Transatlantic modes - what next?
Date: Wed, 7 Mar 2001 14:47:05 -0000
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>From Dave G3YMC
>3)Occupy a bandwidth of less than 10Hz - this is neccesary
>because of the very limited spectrum available, and the fact that
>several stations will be operating simultaneously.

Although this is a clear requirement for QRSS qsos in order that everyone
can have a fair chance within defined segments for QRSS operation, if the
discussed other data modes allow much faster qso times then it should not be
a requirement for them.  If the qso time can be reduced to 15 minutes or
less (as I sure these modes will allow) then operators can time share and
all have qsos in sequence.  In any case, unless qso times are reduced to
these lengths qsos will remain rare as they will be unable to take advantage
of relatively short openings.

73s Dave G3YMC
dsergeant@btinternet.com
dsergeant@iee.org
http://www.btinternet.com/~dsergeant






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <001d01c0a70e$7691a0d0$0a00a8c0@ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010307120313.08b7191a@mail.cc.kuleuven.ac.be>
Subject: LF: <TECH>Intercontinental modes - what next?
Date: Wed, 7 Mar 2001 08:56:47 -0500
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Jim and the others who have commented - Wonderful, a great start to a
discussion that is needed at this time of year.

I offer that there are two, as I see it, distinct directions we are moving
to, the first is the use of DFT processes for detecting power in smaller and
smaller buckets (read as longer and longer information bits) and secondly
those who are into using information coding to decrease the time for the
transfer of information at the expense of needing a higher level of signal.
The later is what I consider to be the more tranditional mode of amateur
radio operating.

Jim's three step "wish list" is an excellent documentation of the second
mode, a more traditional orientation, of item two above.  I wish those who
wish to focus on what I call the second mode well, and good luck going down
that road - I however will not be with you in that area of focus for next
year.

For the rest of the 2001 spring season I am available to run long duration
90 second per bit QSO attempts or to have a special session of transmitting
WOLF data if there is any interest in Europe in having such a test session.

WOLF is extremely difficult for me to send, the I/O implementation choosen
by Stewart when mixed with my situation here makes if very difficult - but
if there is interest I am available to run a couple of overnight tests
before the end of this season.  I have loaded 18 hours of WOLF in one file,
in 25 minute segments, thank goodness for 30 gigabyte hard drives!   I will
have to build up some hardware and do a fair amount of software to make WOLF
work from here - if the interest is present I will do it.  The operative
words here are to set a time period and a reasonable level of participation
from Europe.

My work going forward from here will focus on extream weak signal detection
which continues with the goals I set here when I came to the LF community
some 18 months ago.  My focus will now shift to Time and Frequency coherency
to not worse than a part or two in 10-11th.  I now have GPS controlled
systems at both my home and the remote site, they are not yet complete but
they exist and will be completly functional by the fall.

The status of LF operation from Canada remains tenuous.  The TransAtlantic
II project that was the basis of Canadian participation on LF has been
eclipsed from bordering on believability and achievability a year ago to
common practice in so short a time as to place in question much of the
"common wisdom" of the day.  A plan for an LF allocation in Canada is before
our regulatory authority, the issue is - will enough time and resources be
available to do the work of authorizing general use of the LF band be
available in the near future?

The next issue is how many amateurs will build the systems and learn the
tricks to have an active LF community - there will be at least a year of
growth needed.  With just three transmitting stations in Canada now we have
seen the limits of LF paticipation, aural only operation only by Jack,
VE1ZZ, and severly hampered (foliage challenged)  LF operation by Mitch,
VE3OT and my own setup here in eastern Ontario.  The situation of an LF
allocation in the United States is certainly not understood by myself - but
it can be said there is a community waiting for the opportunity to make use
of an LF allocation, but at the moment there is no certainty of
participation and this community will need growth time as well.

This being said, there is also some opportunity in the information coding
area.  WOLF uses an internal synchronization process, very costly in
information bits.  There are opportunities in Time Coherency as well as the
Turbo Product Codes that are achieving very high levels of performance
approaching the Shannon limit.  (By the way Dr. Shannon passed away only a
month ago I learned in yesterday's newspaper).  I personally want very much
to understand these coding processes and demodulation/modulation methods
enough to write my own code and experiment with them on the air, this is the
only way I will return to the information coding area of operation that I
mentioned above.

The current operational status from here is that I continue to see many
trace level weak signals from Europe almost every night.  Many of them are
using bit rates that result is complete smearing here and are not readable
at all.

I have tested the 7 level FSK coding on 160M and as well on 20 Meters
(hiding in amongst the DX Beacons on 14100 kHz - they are spread out over
about 150 Hz - terrible waste of spectrum Hi).  I do not recommend this work
go further, there is far greater value in the information coding mentioned
above and it is important to focus our efforts in order to make meaningful
progress.

I have no idea why but I have still not seen a single recognizable DFCW
signal on this side of the Atlantic.

The two different directions that I mentioned at the start of this memo, DFT
with longer and longer bits, and the use of information coding to increase
the signalling rate are I suggest critical to the evolution of LF.  I ask
each of you to consider and comment on this segmentation and what you see as
your participation in the "speaking slowly" mode of operation.  I am keen to
find others to work with in this area of extremely weak signal
communications.  I encourage others who might wish to focus on really really
weak signal work to contact me directly.

Larry
VA3LK





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To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: <TECH>Transatlantic modes - what next?
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Hello Jim & group,

Excellent paper from Jim, it seems a good starting point for an open
discussion.


One of the point that Jim mentions is the duration of a QSO.
While making the recent changes on QRS I have been doing some thinking how
we 'speed up' things.

I started with analyzing some typical QRSS (or DFCW) QSO's and came,
similar to Jim, to the conclusion that it takes about 50 characters to
complete a QSO.
The main if that is exchanged are callsigns (or parts of it), what means
that there is a rather random distribution of letters. So the 'smart
coding' of CW won't be of much use as 'E' and 'Y' will have the same
occurance.

Digging a bit further into the 'typical QSO' shows that the 50 characters
can be divided in :
- 32 letters (almost random)
- 18 figures (almost random)
- 10 spaces

Next I started comparing the modes, starting with the existing ones :
- in CW (QRSS) the average letter has a length of 11.2 dots, the average
figure is 17.0 dots long and a space is 6.0 dots long (inter character
spacing included).
- in DFCW the average letter is 4.1 dots long, the average figure is 5.0
dots long and the a space is 2.0 dots long
That means that the typical QRSS QSO will take 724 dotlengths while a
typical DFCW QSO will take 211 dotlengths, a time saving factor of 3.43.
So at 3 sec/dot it will take 36'12" in QRSS and 10'33" in DFCW. At 10
sec/dit it will take 2 hours in QRSS and 35 minutes in DFCW. And at 60
sec/dot it will take 12 hours in QRSS and 3.5 hours in DFCW.
Or the other way arround, if you want a complete QSO in 1 hour then you can
use 5 sec/dot in QRSS and 17 sec/dot in DFCW.

As mentioned by Jim, DFCW is a bit more difficult to implement, as you need
to FSK the transmitter. So the main advantage of QRSS is its simplicity.
The efficiency of QRSS can be improved by :
- reducing the dash/dot ratio from 3 to 2
- reducing the inter character spacing from 3 dotlengths to 2 dotlengths
- reducing the space length from 6 dots to 4 dots
As a result the average letter will be 8.8 dots long, the average figure
will be 13.5 dots long and a space will be 4 dots long. A typical (50
character) QSO will now be 565 dots long, a time saving factor of 1.28.
This means a 8 minute saving on a 3sec/dot QSO, a 26 minute saving on a 10
sec/dot QSO and a 2h40m saving on a 60 sec/dot QSO. This is not nearly as
good as DFCW, but it can be achieved without any changes to the equipement.

If we want more time efficient coding then we have to go to 'multiple
frequency modes'. A possibility is a 7 tone mode that will give us the
possibility to transmit 49 characters (enough for our purpose) at a typical
length of 3 dots/char (or 2 dots/char without inter character spacing).
At 3 dots/char a typical QSO will be 150 dots long, a time saving factor of
1.41 compared to DFCW.
At 2 dots/char a typical QSO will be 100 dots long, a time saving factor of
2.11 compared to DFCW. But at 2 dot/char this system has 2 disadvantages:
1. We loose synchronisation (so the RX has to know the start time of the TX)
2. We loose the reference frequency, so any offset between TX and RX will
cause problems (at 3 dots/char we can use the inter character spacing to
transmit a reference frequency).
Technical implementation of multi tone modes more difficult than DFCW. So
to be honest, taking into account that only very few stations (abt. 4-5 in
Europe) have set the step from QRSS to DFCW I'm afraid that the technical
implementation of a multi tone more will be a real burden.

Finally there were some suggestions for double tone modes, where 2 tones
wil be sent parallel. First of all you will need a linear PA, with reduced
efficiency, more stabilty problems and more difficult to built. But is
there really an advantage ?
If you transmit 2 tones, each tone will be 3dB down compared to a single
tone mode  (if you take the reduced efficiency into account it will be even
4dB or more). So what is the difference in transmitting 2 tones parallel
during 20 seconds or 2 tones sequential during each 10 seconds ? SNR will
be the same.


Another 'branch' are the modes as BPSK and WOLF (what is in fact BPSK with
some added 'intelligence'). First of all BPSK has an advantage of 6dB over
traditional 'on-off keying', at the same dotlength (while on-off keying is
a kind of 1 to 0 switching BPSK is a kind of 1 to -1 switching).
Further these modes have a different approach of improving SNR. Instead of
transmitting the characters very slow (as QRSS/DFCW does) they transmit the
characters rather fast and improve SNR by repeating them over and over and
doing some smart error correction.

An additional difference occurs at the RX side. QRSS/DFCW are received
'wideband', this means you can observe a rather big part of the spectrum
for DFCW/QRSS signals. This has the advantage that, even at signal
bandwidths of 0.01Hz, there is nor problem to 'hit' the transmitted signal.
One can even 'decode' more that one signal at the same time. Opposite to
this all receiving software for BPSK / WOLF is 'narrowband'. This means
that you have to 'hit' the transmitted signal very accurate and you can
receive only 1 signal at a time.

BPSK modulation is not so difficult, in theory you just need an XOR gate in
the drver circuit. But if you modulate you TX 'rude' the bandwidth of the
signal will be rather wide. In PSK this is solved by 'enveloping' the
signal (so you have zero amplitude at phase switching) but this requires a
linear PA and is not very power efficient.
Lowfers tend to use the 'rude' BPSK, but they have a 30kHz wide band and
are limited to 1 Watt input (few mW ERP) while we hams can run up to 1W ERP
(1kW input or more) and have only a 2.1kHz wide (or narrow) band.

Recents tests of the WOLF system have shown that it has some possibilities.
In my opinion the best way to check what WOLF is worth transatlantic is to
have a strong WOLF beacon in VE/W and as many as possible stations
monitoring this beacon in Europe. When good software becomes available it
will be no problem to get a few dozen receving sites all over Europe, the
WOLF system just invites for unattended (overnight) recepetion. That way we
would also avoid inter-EU QRM during this test phase.
So, we would need someone who is willing (and able) to write a good piece
of WOLF receiving software (using the soundcard, running under windows) and
who someone (at the other side of the pond) who can setup a 24h beacon.


So far my contribution,

73, Rik  ON7YD


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: : Transcontinental modes - what next?
Date: Wed, 7 Mar 2001 10:17:20 -0000
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I was thinking of this aspect as well, for SMT Hell modesl.   Most
stations do not transvert, so soundcard output gives a problem.   
The parallel port is difficult, though not impossible, to utilise in
this way through Windoze so I cam to the conclusion that the serial port
is once again the optimum route.   It may mean constructing a bit of
hardware, but this need only be along the lines of a shift register/
latch and possibly a D/A converter to drive a varicap across a crystal.

Alternatively, one of the many serial D/A converters around now could
probably be driven directly from the serial port if this has its lines
toggled in a non-standard way to match the serial format needed by the
D/A - this may give Windoze software authors a headache but it can be
done.

The best route of course is just to use the serial port to control a DDS
- and HF-Instruments has now supplied around 100 suitable DDS modules.

Andy  G4JNT


> -----Original Message-----
> From: Alberto di Bene [mailto:dibene@usa.net]
> Sent: 2001-03-07 09:40
> To: rsgb_lf_group@blacksheep.org
> Subject: LF: RE: Transcontinental modes - what next?
> 
> 
> Hi all,
>           which would you all prefer as a way to 
> frequency-shift your TX ?
> With frequency shift I mean many steps, separated by a 
> fraction of an Hertz.
> The first two possibilities that come to my mind are an audio 
> output from the
> sound card (requiring then a mixer to bring the tone to the 
> wanted freq.),
> or a binary value output from, say, the parallel port, which 
> then would require
> a small external board with a DDS or a microcontroller to 
> drive the TX.
> 
> No linearity requirements will be needed. I need your input 
> to not start in a
> false direction.    TNX for any advices.
> 
> 73  Alberto   I2PHD
> 
> 
> 


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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: <14313.200103061746@gemini>
Subject: LF: Re: Transatlantic modes - what next?
Date: Wed, 7 Mar 2001 09:55:31 -0000
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Jim said:

> The QRSS modes easily meet 2 and 3; in order to meet 1, a dot
> length of about 7 seconds maximum would be required. With the
> best possible conditions, I guess several stations might manage
> transatlantic QSOs with these dot lengths. However, it would
> probably not be enough to reach the more inland parts of Canada,
> or the USA and further afield.

With the existing technology, as Jim says, two way transatlantic contacts
have been shown to be possible with relatively short dot periods. The secret
is to monitor LF conditions and then choose appropriate dot periods. With
the VE1ZZ/VE1ZJ/G3LDO QSO, VE1ZZ used 3 second dots because he was using a
relatively high erp, while I allocated myself (in the first instance) 10
second dots. In the event this worked so there was no need for me to
increase the dot period.
This method of optimum dot period selection can be used to optimise the QSO
time so that it can be contained within a peak of good LF conditions. I
think we got it right because our QSO lasted around 50 minutes.
However, even with the 20w erp or so that VE1ZZ is using we had to wait for
a couple of days before we could make our reverse crossband 136/80m contact
on the 21/2. This goes to show that LF conditions are everything and that
close liaison between the operators taking part in any tests is essential.

I acknowledge that the QRSS coding is primitive but it has the advantage of
simplicity and has shown itself to be successful. It will be interesting to
see how things change now that the WOLF is at the door.


Regards,
Peter, G3LDO

<g3ldo@ukonline.co.uk>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alberto di Bene" <dibene@usa.net>
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Subject: LF: RE: Transcontinental modes - what next?
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Hi all,
          which would you all prefer as a way to frequency-shift your TX ?
With frequency shift I mean many steps, separated by a fraction of an Hertz.
The first two possibilities that come to my mind are an audio output from the
sound card (requiring then a mixer to bring the tone to the wanted freq.),
or a binary value output from, say, the parallel port, which then would require
a small external board with a DDS or a microcontroller to drive the TX.

No linearity requirements will be needed. I need your input to not start in a
false direction.    TNX for any advices.

73  Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Subject: Re: LF: Transatlantic.G3XDV/G3AQC
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> Hi Laurie
> Hi Mike
[cut]
> the diff rx-input-voltage between ur signs is 10db +/-2db.
> 
> Uwe/dj8wx jo43sv ant: inv.Ve with 340m and 400m lws 

Uwe, 

Many thanks for the picture again. It is interesting that Laurie is 8-12dB 
stronger than me as his ERP is only twice mine. It could be the take-off as 
Laurie is very close to the coast, or perhaps our antennas show some 
directivity. Also it is possible that the sky-wave and ground-wave combined in 
different phases.

73



Mike



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Vernall" <vernall@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
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Subject: LF: Re: <TECH>Transcontinental modes - what next?
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Dear LF Group,

Thanks to Jim M0BMU for generating a good discussion paper.  I have a few
comments:

I've taken the liberty of changing a word in the title from transatlantic to
transcontinental.

I'm don't see why the occupied bandwidth should be arbitrarily restricted to
10 Hz.  There could be something to gain from multicarriers, frequency
diversity or "spread spectrum".  Something like 50 Hz bandwidth may be a
better arbitrary upper cap to nominate for occupied bandwidth.

> One way to use longer dot lengths without increasing overall QSO
> time is to use multiple frequencies - for example, DFCW, VA3LK's
> 7-tone scheme, and VK2ZTO's one-tone-per character VFSKCW.

VFSKCW uses a sound card but otherwise is very similar to DFCW.  VK2ZTO's
other scheme is frequency difference keying (FDK) which would appear to
greatly reduce the need for high stability frequencies for transmitters,
receivers or sound cards.  I'm testing both VFSKCW and beta FDK.

I'm still in discovery mode with WOLF, and that certainly looks interesting.

73, Bob ZL2CA



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LAWRENCE MAYHEAD schrieb:
> Hi John and All,
> Glad to hear that there is still some TA propagation. I will run DFCW tonight
>  using 30 sec dots. Dot freq. 135,921.5 dash freq.
> 135.922. I am very intrested to see wether this mode gets through, and would
>  appreciate any reports Start time 20:00utc
> 73s Laurie. G3AQC. 
>
Hi Laurie
Hi Mike


I made a 30 dots ARGO-screenshot at 2319utc 06.03.01 (enclosed). 
for better reading I 
took the ARGO sensitivity down and got 12db  between the antenna and the first 
mixer of the receiver. the loads of the beginnings and endings of the dashes and 
dots seen in the pic enclosed in my todays first e-mail - so far not from 
FFT-processing - vanished. now ur line, Mike, is vy good readable.

the diff rx-input-voltage between ur signs is 10db +/-2db.

it is visible that the emission of Laurie has a "noise curtain" (as we do term 
it in the german language) up to +/- 100 Hz.

Regards
Uwe/dj8wx jo43sv ant: inv.Ve with 340m and 400m lws 

    
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--------------020504020802080203010500--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 17:39:55 -0500
From: "Dexter McIntyre W4DEX" <dmcintyre@att.net>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: <TECH>Transatlantic modes - what next?
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James Moritz wrote:
> 

> The QRSS modes easily meet 2 and 3; in order to meet 1, a dot
> length of about 7 seconds maximum would be required. With the
> best possible conditions, I guess several stations might manage
> transatlantic QSOs with these dot lengths. However, it would
> probably not be enough to reach the more inland parts of Canada,
> or the USA and further afield. 

Jim,

Several times your signal was strong enough here in North Carolina that
I could have copied 7 second dots, maybe less.  When I copied Laurie's
complete call his signal was also strong enough for much shorter
elements.  Most of the nights that I could copy G3AQC, CT1DRP and your
signal the best propagation lasted about one hour.  For QRSS I think 10
to 20 second element DFCW would work well.

Dexter


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 13:18:18 -0600
To: rsgb_lf_group@blacksheep.org
From: "Les Rayburn" <les@highnoonfilm.com>
Subject: Re: LF: <TECH>Transatlantic modes WOLF
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I would have to second Bill de Carle's remarks about the future of long
distance LF communication being made via WOLF mode. While WOLF
is a form of BPSK, it offers significant advantages. And while frequency
stability is more of an issue than when using QRSS mode, we have
had remarkable results in our on-air testing using frequency standards
that should be easy for any amateur to maintain.

For the latest news on WOLF operations in the states, and links
to resources to get you started, please visit the Noise Floor Web
Site:

http://www.highnoonfilm.com/xmgr/updates/wolf.htm

Les Rayburn, N1LF





Les Rayburn, director
High Noon Film & Interactive
100 Centerview Drive
Suite 111
Birmingham, AL 35216
(205) 824-8930
(205) 824-8960 FAX



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Transatlantic: on now
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Hi Rik Das mittler signal war M0BMU
73 von John VE1ZJ
Rik Strobbe wrote:

> Hallo Uli,
>
> Das obere Signal ist Mike (DV = Ende seines Rufzeichens)
> Das mittlere Signal ist mir unbekant, aber es schaut recht stark aus
> Das untere Signal ist DF6NM
>
> 73, Rik  ON7YD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 13:42:53 -0500
To: rsgb_lf_group@blacksheep.org
From: "Bill de Carle" <bill1@cgocable.ca>
Subject: Re: LF: <TECH>Transatlantic modes - what next?
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At 05:50 PM 3/6/01 +0000, Jim Moritz wrote:
[..]
>What is required for a practical 2 way LF DX mode, capable of 
>operating at the extremes of distance and SNR? A while ago, 
>G4JNT posted an estimate of what might be theoretically possible 
>using different techniques; another way is to look at what is 
>needed to serve our purposes. I would suggest the following "wish 
>list":
>
>1)Be able to complete a minimal QSO (about 50 characters) in one 
>hour. This would give the lowest rate of signalling capable of using 
>the propagation lifts to complete a QSO "in one sitting".
>
>2)Be able to transmit/receive all alphanumeric characters and 
>essential punctuation/procedure signs, in order to be generally 
>usable by any station without special arrangements.
>
>3)Occupy a bandwidth of less than 10Hz - this is neccesary 
>because of the very limited spectrum available, and the fact that 
>several stations will be operating simultaneously. 
>
>The QRSS modes easily meet 2 and 3; in order to meet 1, a dot 
>length of about 7 seconds maximum would be required. With the 
>best possible conditions, I guess several stations might manage 
>transatlantic QSOs with these dot lengths. However, it would 
>probably not be enough to reach the more inland parts of Canada, 
>or the USA and further afield. By the way, I reckon about 6dB SNR 
>is needed to see a QRSS signal on a spectrogram under 
>favourable conditions; if there is much QRN, 10dB is probably 
>required. It is possible to see a trace of signal with 0dB or less 
>SNR. All this is fairly subjective, however.
[..]
>Then there are the "digital" modes, specifically BPSK. Currently, 
>most effort has been expended on the MS100, 10 bits per second 
>variety of BPSK. This easily meets conditions 1 and 2. However, 
>for the same signal levels, QRSS seems to do better with 
>acceptable, if much slower, speed. Also, the bandwidth occupied is 
>roughly 40Hz, too wide for condition 3. But with the 16 bits per 
>character coding scheme normally used for BPSK, 2250 
>characters per hour can be transmitted, far higher than is actually 
>required. So the bit rate could be greatly reduced, and/or the 
>coding altered to a greatly increased number of bits per character, 
>hopefully improving the readability of the signal. Reducing the 
>overall speed by a factor as much as 45 would still meet condition 
>1. To fit into a 10Hz bandwidth, the bit rate would have to be 2.5 
>bits/sec (MS400) or less, so you could encode each character with 
>up to 180 bits if you wanted to. Or, sticking with 16 bit codes, 0.22 
>bits/second (MS4500) would still be OK. What we want is the best 
>trade off between bit rate and encoding for very poor signal to 
>noise ratio. I don't know a great deal about this subject, but I 
>expect some readers of this reflector already know the answer. 

Apart from the bandwidth, I believe Stewart Nelson's WOLF system
is the best approach that most closely meets all the requirements.
It shouldn't be difficult to slow down WOLF's 100 msec keying rate
if you really have to reduce the bandwidth.  Of course Tx, Rx frequency
stability and accuracy will become increasingly important as with
any slow BPSK mode.

>So any suggestions/comments would be welcome -     well, almost 
>any! By the way, I now have BPSK at up to 1200W PEP from my 
>Decca TX, if anyone would like a sked/tests, etc.

If you'd care to run a test using WOLF, I'd be happy to send you the
results.

For more information on WOLF, see:

www.scgroup.com/ham/wolf.html

Bill VE2IQ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <14313.200103061746@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
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Subject: LF: <TECH>Transatlantic modes - what next?
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Dear LF Group,

The winter has seen a fair amount of success in the transatlantic 
tests, and now that the "season" is probably near to an end, it is 
worth thinking about what the next steps could be, in good time for 
next winter. The following ramblings were the result of thinking what 
I could do next, in the way of technical development of my LF 
station, in particular regarding what would be the best mode to 
work on:
-------------------------------------------------------------------------------------
So far, all reported trans-atlantic signals have used some type of 
QRSS. The variable parameter is the dot length - longer dots mean 
better signal-to-noise ratio, with the penalty of slower message 
transmission. Recognisable callsigns have been produced with 60s 
dots or longer, which requires more than an hour to transmit one 
callsign. ON7YD's DFCW roughly halves the time required, at the 
expense of doubling the bandwidth occupied by the transmitted 
signal and being slightly more complex to implement, which seems 
to be a good trade-off. 

The maximum radiated power available to several stations has 
reached the 1W ERP level in Europe, and somewhat more than 
this for the stations active in Canada. The ERP that is feasible 
depends mostly on how big an antenna can be put up, but in any 
case is limited by regulation to 1W in Europe, which eliminates 
further improvements. ERPs of a few 100 milliwatts have been 
sufficient to cross the Atlantic on several occasions.

Under optimum conditions, with favorably sited and equipped 
stations, 3s per dot QRSS signals have been passed both ways 
across the Atlantic, but this is the exception rather than the rule. 
The problem with longer duration dots is that any kind of 2-way 
contact takes an excessively long time, running into several hours. 
This problem is compounded by the fact that propagation "lifts" on 
LF only last an hour or so. So it would seem we are reaching the 
practical limits with QRSS.

What is required for a practical 2 way LF DX mode, capable of 
operating at the extremes of distance and SNR? A while ago, 
G4JNT posted an estimate of what might be theoretically possible 
using different techniques; another way is to look at what is 
needed to serve our purposes. I would suggest the following "wish 
list":

1)Be able to complete a minimal QSO (about 50 characters) in one 
hour. This would give the lowest rate of signalling capable of using 
the propagation lifts to complete a QSO "in one sitting".

2)Be able to transmit/receive all alphanumeric characters and 
essential punctuation/procedure signs, in order to be generally 
usable by any station without special arrangements.

3)Occupy a bandwidth of less than 10Hz - this is neccesary 
because of the very limited spectrum available, and the fact that 
several stations will be operating simultaneously. 

The QRSS modes easily meet 2 and 3; in order to meet 1, a dot 
length of about 7 seconds maximum would be required. With the 
best possible conditions, I guess several stations might manage 
transatlantic QSOs with these dot lengths. However, it would 
probably not be enough to reach the more inland parts of Canada, 
or the USA and further afield. By the way, I reckon about 6dB SNR 
is needed to see a QRSS signal on a spectrogram under 
favourable conditions; if there is much QRN, 10dB is probably 
required. It is possible to see a trace of signal with 0dB or less 
SNR. All this is fairly subjective, however.

One way to use longer dot lengths without increasing overall QSO 
time is to use multiple frequencies - for example, DFCW, VA3LK's 
7-tone scheme, and VK2ZTO's one-tone-per character VFSKCW. 
Taking this to it's logical extreme, it would be possible to assign 
different frequencies to all possible combinations of callsigns and 
signal reports, so each over of a QSO would just consist of a 
single tone. However, it would then be difficult to meet condition 2. 
I guess there must be an optimum trade off between number of 
tones, difficulty of encoding and decoding, redundancy and so on. I 
suspect it might be 2 tone DFCW, but I don't know.

Then there are the "digital" modes, specifically BPSK. Currently, 
most effort has been expended on the MS100, 10 bits per second 
variety of BPSK. This easily meets conditions 1 and 2. However, 
for the same signal levels, QRSS seems to do better with 
acceptable, if much slower, speed. Also, the bandwidth occupied is 
roughly 40Hz, too wide for condition 3. But with the 16 bits per 
character coding scheme normally used for BPSK, 2250 
characters per hour can be transmitted, far higher than is actually 
required. So the bit rate could be greatly reduced, and/or the 
coding altered to a greatly increased number of bits per character, 
hopefully improving the readability of the signal. Reducing the 
overall speed by a factor as much as 45 would still meet condition 
1. To fit into a 10Hz bandwidth, the bit rate would have to be 2.5 
bits/sec (MS400) or less, so you could encode each character with 
up to 180 bits if you wanted to. Or, sticking with 16 bit codes, 0.22 
bits/second (MS4500) would still be OK. What we want is the best 
trade off between bit rate and encoding for very poor signal to 
noise ratio. I don't know a great deal about this subject, but I 
expect some readers of this reflector already know the answer. 

Beacon signals are a bit different; here, the only requirement is to 
positively identify the signal, and make some estimate of the signal 
level. An on-off keyed carrier with a simple repeating pattern and a 
well defined frequency is easily identified with simple equipment, 
and has the advantage of flexibility at the receiving end - you can 
make the bandwidth arbitrarily narrow, or perhaps take advantage 
of the coherent nature of the signal, to improve detection 
capability. You can also monitor several signals at once.

So any suggestions/comments would be welcome -     well, almost 
any! By the way, I now have BPSK at up to 1200W PEP from my 
Decca TX, if anyone would like a sked/tests, etc.

Cheers, Jim Moritz
73 de M0BMU




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 18:39:08
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: WOLF Mode Records!
In-reply-to: <5.0.2.1.0.20010303105753.02bda910@highnoonfilm.com>
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At 11:15 3/03/01 -0600, N1LF wrote:
>...
>The results were:
>
>CW (by ear) -18db below the noise
>QRSS (3 sec dots) -27db below the noise
>QRSS(S) (60 sec dots) -31db below the noise
>WOLF -40db below the noise
>...

The above figures seem a bit strange to me :
QRSS at 60 sec/dot should be 13dB better than QRSS at 3 sec/dot. I won't
argue about 1..2 dB more or less, but a difference of 9dB (4dB vs 13dB)
seems hard to believe.
Recent tests (eg. the QSO between G3XDV and CT1DRP) have shown even between
3 sec/dot and 10 sec/dot there is a significant difference (from a bare 'T'
to a solid 'O') that is probably close to 4dB.

Also the 9dB between 'by ear' and 3 sec/dot seems rather conservative,
other tests (eg. those done by DK8KW) have shown a 15dB difference.

I'm not saying that WOLF is not superior to QRSS, but the above figures
seem not correct to me.

73, Rik  ON7YD



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 18:22:29
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: LF: new version of QRS (v3.04)
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Hello all,

I have a new version of QRS available that is adapted to the recent needs
for longer dotlengths with more accurate timing.
New features :
- dotlengths up to 1 hour (OK, very long ... but I tried to be 'on the save
side' for future developements)
- possibility to syncronize transmission to the PC timer (eg. let the
dots/dashes start exactly on the full minute at 60 sec/dot), I believe
there is some gain to achieve if the receiver exactly knows when the dots
start and stop
- more precize timing, as the minimal errors that were not noticed at 3
sec./dot can become annoying at 60 sec./dot
- improved QSK behaviour

This new version can be (temporarily) downloaded from

http://www.qsl.net/on7yd/QRS/qrs304.zip

for final testing, if I get no bug reports within the next days it will be
released via the known webpages.

My thanks go to G3AQC and M0BMU who did a lot of testing over the last
weeks and helped me to get all bug out (fingers crossed).

Please do not put this version on other web places (yet) until I'm sure it
is 100% bugfree and give an official release.

73, Rik  ON7YD

PS : I'm working on some soundcard output, hope to get it ready soon.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 08:45:34 -0600
To: rsgb_lf_group@blacksheep.org
From: "Les Rayburn" <les@highnoonfilm.com>
Subject: LF: WOLF Mode Records!
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On this side of the Atlantic, US Lowfers are experimenting with a new weak 
signal mode
called "WOLF" developed by Stewart Nelson, KK7KA. It has proven to be far 
superior
to QRSS(S) mode in both off air and on-air tests to date.

Lyle Koehler, K0LR conducted off air tests where he mixed a random sample 
of LF noise
with the desired signals from a variety of modes. The results were:

CW (by ear) -18db below the noise
QRSS (3 sec dots) -27db below the noise
QRSS(S) (60 sec dots) -31db below the noise
WOLF -40db below the noise

These tests have been further confirmed by on-air tests as well. Despite 
the Springtime
QRN, record breaking receptions in WOLF mode have been made in the past few
days including Stewart's reception of the XM(GR) beacon at a distance of 
1,874 miles
with a 1 watt input (2 milliwatt ERP) beacon.

I urge LF'ers on both sides of the pond to investigate this exciting new 
mode. It offers
the promise of Trans-Atlantic QSO's even with current US power limits...and 
certainly
with the type of ERP common in Europe and Canada.

Please note that not only is the weak signal performance of this mode 
superior to QRSS
but also that more information can be passed in a given time frame. 
Currently, WOLF uses
a 15 byte message format that can be totally unknown to the receiving 
station (AS WAS
THE CASE IN ALL TEST TRANSMISSIONS SO FAR) resulting in little doubt that
an actual reception or QSO has occurred.

More info can be found on the Noise Floor Web site:

http://www.highnoonfilm.com/xmgr/updates/wolf.htm

73,







Les Rayburn, N1LF
4919 Cox Cove
Helena, AL 35080
XMGR 184.900khz
1LF 187.300khz





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 03 Mar 2001 11:15:43 -0600
To: rsgb_lf_group@blacksheep.org
From: "Les Rayburn" <les@highnoonfilm.com>
Subject: LF: WOLF Mode Records!
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On this side of the Atlantic, US Lowfers are experimenting with a new weak 
signal mode
called "WOLF" developed by Stewart Nelson, KK7KA. It has proven to be far 
superior
to QRSS(S) mode in both off air and on-air tests to date.

Lyle Koehler, K0LR conducted off air tests where he mixed a random sample 
of LF noise
with the desired signals from a variety of modes. The results were:

CW (by ear) -18db below the noise
QRSS (3 sec dots) -27db below the noise
QRSS(S) (60 sec dots) -31db below the noise
WOLF -40db below the noise

These tests have been further confirmed by on-air tests as well. Despite 
the Springtime
QRN, record breaking receptions in WOLF mode have been made in the past few
days including Stewart's reception of the XM(GR) beacon at a distance of 
1,874 miles
with a 1 watt input (2 milliwatt ERP) beacon.

I urge LF'ers on both sides of the pond to investigate this exciting new 
mode. It offers
the promise of Trans-Atlantic QSO's even with current US power limits...and 
certainly
with the type of ERP common in Europe and Canada.

Please note that not only is the weak signal performance of this mode 
superior to QRSS
but also that more information can be passed in a given time frame. 
Currently, WOLF uses
a 15 byte message format that can be totally unknown to the receiving 
station (AS WAS
THE CASE IN ALL TEST TRANSMISSIONS SO FAR) resulting in little doubt that
an actual reception or QSO has occurred.

More info can be found on the Noise Floor Web site:

http://www.highnoonfilm.com/xmgr/updates/wolf.htm

73,







Les Rayburn, N1LF
4919 Cox Cove
Helena, AL 35080
XMGR 184.900khz
1LF 187.300khz





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Date: Tue, 6 Mar 2001 14:56:53 -0000
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Subject: Re: LF: Transatlantic: on now
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> mike.dennison schrieb:
> > I am transmitting tonight on 135.9230kHz 120s dashes, 60s dots - "G3XDV".
> > Mike, G3XDV

> Hi Mike and all,
> I made a screenshot from ARGO-30dots on 135.922.0 kHz +/- at 0045 todays morning 
> (06.03.01). guess your signal, Mike, was the strong one with 60/120sec. but I 
> couldn`t read "G3XDV".
> And who were the others above and below (urs) ?
> 
> I do read in the first line: HEE EEEH
>                 second line: MUEL
>                  third line: DFZNM.
> Uwe, dj8wx, jo43sv, ant: inv.Ve with 340m es 400m lws. 

Uwe,

The top signal was mine. I make 120s 'dashes' from four 30s dashes on my 
keyer, and 60s 'dots' from two 30s dashes! So in your e-mail H = dash and 
E = dot, so the top line reads 'DV'. Half close your eyes and it works fine. 
Using the 60s setting in Argo, it looks like continuous dots and dashes.

The next line - the strong one - I presume was M0BMU, and the third one is 
DF6NM.

Thanks for the pic - very interesting. Looks like I still have some way to go to 
reach M0BMU's signal.

73


Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re. Transatlantic.
Date: Tue, 6 Mar 2001 15:12:35 -0000
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<DIV><FONT face=Arial size=2>Hi John and All,</FONT></DIV>
<DIV><FONT face=Arial size=2>Glad to hear that there is still some TA 
propagation. I will run DFCW tonight using 30 sec dots. Dot freq. 135,921.5 dash 
freq.</FONT></DIV>
<DIV><FONT face=Arial size=2>135.922. I am very intrested to see wether this 
mode gets through, and would appreciate any reports Start time 
20:00utc</FONT></DIV>
<DIV><FONT face=Arial size=2>73s Laurie. G3AQC.&nbsp;</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 06 Mar 2001 15:43:38
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Transatlantic: on now
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Hallo Uli,

Das obere Signal ist Mike (DV = Ende seines Rufzeichens)
Das mittlere Signal ist mir unbekant, aber es schaut recht stark aus
Das untere Signal ist DF6NM

73, Rik  ON7YD




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Date: Tue, 06 Mar 2001 14:26:26 -0800
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Last night M0BMU was visible with good signals.  At times he was chopped
up by local 60Hz harmonics.
       Did not see G3XDV.  But was using 30 sec dots.  Can't use version
of ARGO I haveon 60 second dots

   Will be looking tonight agn 73 de John VE1ZJ



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Subject: Re: LF: Transatlantic: on now
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This is a multi-part message in MIME format.
--------------080501090500050203030306
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mike.dennison schrieb:
> I am transmitting tonight on 135.9230kHz 120s dashes, 60s dots - "G3XDV".
>
> Mike, G3XDV
>
>
Hi Mike and all,
I made a screenshot from ARGO-30dots on 135.922.0 kHz +/- at 0045 todays morning 
(06.03.01). guess your signal, Mike, was the strong one with 60/120sec. but I 
couldn`t read "G3XDV".
And who were the others above and below (urs) ?

I do read in the first line: HEE EEEH
                second line: MUEL
                 third line: DFZNM.
Regards
Uwe, dj8wx, jo43sv, ant: inv.Ve with 340m es 400m lws. 
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--------------080501090500050203030306--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000401c0a5ba$00fdb160$bd04073e@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: DX Cluster spots for 3/4th Mar at GB7DXM
Date: Mon, 5 Mar 2001 21:06:29 -0000
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Hi all, not a lot of serious listening from me this last week. I have heard
Finbar EI0CF fairly regularly, looking for continental stations.He seems to
be having difficulty catching continental stations. Maybe they used to hear
some of the big signals in England working him first, and they are not
realising his presence now. Finbar has a DECCA TX  and an aerial with 230m
of top-load at about 18m high. He is quite consistently 569 at this location
in daytime. It is worth noting that Finbar has QRSS available now, if you
can't reach otherwise.  He still reckons he needs a bit a practice at it
yet!

Also heard at better strength than normal, I think, was Colin G3KMP in
Hastings....maybe some aerial improvements, but he was as strong if not
stronger than Bill G0AKY last time I heard them. Mike, G3XDV, Tom G3OLB,
Peter G3LDO, Dave G3YXM, and Laurie G3AQC have been heard from time to time
pounding through. Most afternoons last week and today DJ9IE has been easily
copiable on the speaker here and has been worked by a number of stations.
Hopefully, John G3CCH may be heard again soon, and may also be joining us on
the 'Inet' .He is considering a new 'exciter' (one with less drift than the
FT-77) and may be trawling for opinions. G6NB and G8RW are regular singals
also.

A weeks worth of continuous strength recording of SXV (Marathon) on 135.7/8
kHz has proved that this signal seems to respond to geomagnetic disturbances
in similar ways to those I have seen on CFH. The recent Coronal Mass
Ejection produced some overnight plots with rapid and deep fading. It also
showed the situation where the best strengths were at or around 2400z with
the overall trend being continuously downward ( increasing absorption ??)
for the rest of the darkness. Most normal undisturbed nights show a fairly
constant signal from 2400z through to about 0500z.  So, it could well be
that there is some useful propagtion information to be gained. I will keep
you all updated with any progress on that front. Rik has offered to host
these plots later on his web site.

I note a call I have not seen before on the spotting side ..G3ZES...so maybe
a new station on the band soon??
Cluster spots follow:-
   137.7  IK5ZPV       4-Mar-2001 1743Z  cq qrss
<DL6SN>
   137.5  IK5ZPV       4-Mar-2001 1744Z  QRSSS CQ 589
<S59A>
   136.7  DK6NI        4-Mar-2001 1737Z  cq
<DL6SN>
   136.7  F6BWO        4-Mar-2001 1548Z  cq
<DL6SN>
   137.7  PA0BWL       4-Mar-2001 1241Z  qrss
<OM2TW>
   137.7  IK5ZPV       4-Mar-2001 1100Z  cq qrss
<DL6SN>
   137.7  IK5ZPV       4-Mar-2001 1015Z
<OM2TW>
   136.4  F6BWO        4-Mar-2001 1003Z  419 in jn58au
<DL6SN>
   136.5  DJ7RD        4-Mar-2001 0951Z  cq
<DL6SN>
   137.7  OM2TW        4-Mar-2001 0847Z  qrss
<DL6SN>
   137.7  PA0BWL       3-Mar-2001 1417Z  cq qrss
<DL6SN>
   136.5  OK1DTN       3-Mar-2001 1404Z
<DL6SN>
   136.5  OK1DTN       3-Mar-2001 1045Z  cq
<DL6SN>
   136.5  DJ9IE        3-Mar-2001 1045Z
<OM2TW>
   137.0  OK1DTN       3-Mar-2001 1020Z  strong
<OM2TW>
   136.6  DJ9IE        3-Mar-2001 0915Z
<DL6SN>
   136.9  G8RW         2-Mar-2001 2041Z  559 CQ
<G3ZES>
   136.6  DJ9IE        2-Mar-2001 2014Z  cq for test 559
<G3ZES>
   136.7  DL3FDO       1-Mar-2001 1757Z
<DL6SN>
   136.6  ON6ND       26-Feb-2001 1910Z  ON6ND 559 DJ9IE 559 <G3ZES>
   G3NYK de GB7MRS  5-Mar-2001 2029Z >

Cheers de Alan G3NYK    JO02PB
Alan.Melia@btinternet.com




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 05 Mar 2001 15:50:03 +0000
Subject: LF: Re: QSB on LF
From: "Mitch Powell" <PowellM@claven.fanshawec.on.ca>
To: andre.kesteloot@ieee.org
Cc: rsgb_lf_group@blacksheep.org
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Andre: Just to add to the confusion (?) let me add the followiing, 
based on extensive daily monitoring of AMRAD WA2XTF/12 at Front Royal
Virginia, a distance of 324 mi ( 520 kM). The WA2XTF signal appears
with great rugularity before local sunrise and is solid copy with no
QSB noticed through the observation period. At present ( 1545 EST)
(2045Z) the signal is audible and solid trace at the same time using
ARGO and Spectrogram. QSB has not been a problem, and the signal is a
steady and solid reference as I experiment throughout the winter with
different antenna configurations / preamps.
I believe you use a 1500 foot ( ~500m ) longwire - so I can certainly
guarantee I will receive your signal over a 12 hour period, well past
sunset. Later ( 2100 EST) 02Z ) the signal is very weak and disappears
normally until re-appearing with the sun !
For your information.

73
Mitch VE3OT

----------
>From: "Andre' Kesteloot" <andre.kesteloot@ieee.org>
>To: lf-amrad <lf@amrad.org>, Mitch Powell VE3OT
<PowellM@claven.fanshawec.on.ca>
>Subject: QSB on LF
>Date: Mon, Mar 5, 2001, 0:33pm
>

>
>
> Rik Strobbe wrote:
>
>> Have heard OK1DTN for the last 2 weeks several times with good signals,
>> from 559 up to 589. But so far I always called him in vain.
>> Most of the time he has a fair amount of QSB on his signal (compared to
>> others at the same distance).
>> I wouldn't be surprised if he was running a long wire antenna, I getting
>> the impression that stations with relatively long wire antennas have more
>> QSB than those with small toploads or pure verticals.
>> Could it be that long wires radiate at steeper angles and thus produce more
>> skywave ?
>>
>> 73, Rik  ON7YD
>>
>> At 10:41 5/03/01 +0100, you wrote:
>> >To All from PA0SE
>> >
>> >I worked OK1BTN on 25 February; sent 569, received 229. Heard G3YXM and
>> >ON6ND working him as well.
>> >
>> >73, Dick, PA0SE
>
> 


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
Subject: LF: Transatlantic: on now
Date: Mon, 5 Mar 2001 20:33:12 -0000
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I am transmitting tonight on 135.9230kHz 120s dashes, 60s dots - "G3XDV".

Mike, G3XDV



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
References: <001a01c0a4f2$8791e3e0$906568d5@oemcomputer> <3.0.1.16.20010305121327.2dbfd9fc@mail.cc.kuleuven.ac.be>
Subject: Re: LF: Re: OK QSO
Date: Mon, 5 Mar 2001 20:02:31 +0100
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Hello All

I think Rik is right , looking abt the difference between long wire and
toploaded vertical .
My first qso with Ruda OK1DTN  on 11-2-2001   give 3-3-9     rcvd  4-3-9
My second qso with Ruda was on       25-2-2001   give 5-7-9     rcvd  4-3-9
So my vert. was stable , and big difference on His sig. , unless He uses now
an amplifier .

Best 73 to All
Werner  ON6ND


----- Original Message -----
From: Rik Strobbe <rik.strobbe@fys.kuleuven.ac.be>
To: <rsgb_lf_group@blacksheep.org>
Sent: Monday, March 05, 2001 12:13 PM
Subject: Re: LF: Re: OK QSO


> Have heard OK1DTN for the last 2 weeks several times with good signals,
> from 559 up to 589. But so far I always called him in vain.
> Most of the time he has a fair amount of QSB on his signal (compared to
> others at the same distance).
> I wouldn't be surprised if he was running a long wire antenna, I getting
> the impression that stations with relatively long wire antennas have more
> QSB than those with small toploads or pure verticals.
> Could it be that long wires radiate at steeper angles and thus produce
more
> skywave ?
>
> 73, Rik  ON7YD
>
> At 10:41 5/03/01 +0100, you wrote:
> >To All from PA0SE
> >
> >I worked OK1BTN on 25 February; sent 569, received 229. Heard G3YXM and
> >ON6ND working him as well.
> >
> >73, Dick, PA0SE
>
>
>









From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
To: rsgb_lf_group@blacksheep.org
Date: Mon, 5 Mar 2001 14:43:25 -0000
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Subject: Re: LF: Re: OK QSO
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> I am a little puzzled about the three different OK call signs that are
> reported to have been worked: OK1DRT, OK1BTN, OK1DTN. Are these really three
> new stations?
> The only one I have heard is OK1DTN, 549 here.
> 73, John, G4CNN

Sorry, brain failed after a long weekend. The station was OK1DTN as reported 
in my first e-mail, not DRT as in my second.



Mike, G3XDV (IO91VT)
http://www.lf.thersgb.net



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To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: OK QSO
In-reply-to: <9912547.983797554504.JavaMail.imail@chilly.excite.com>
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Hello John,

that mail came through twice ...
The only one I heard OK1DTN.

Rik

At 05:05 5/03/01 -0800, you wrote:
>Hi All,
>I am a little puzzled about the three different OK call signs that have been
>worked: OK1DRT, OK1BTN, OK1DTN. Are there really three new stations?
>The only one that I have heard is OK1DTN, 549 here.
>73, John, G4CNN



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 5 Mar 2001 05:08:45 -0800 (PST)
From: "john sexton" <computernetworks@excite.com>
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Subject: Re: LF: Re: OK QSO
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Hi All,
I am a little puzzled about the three different OK call signs that are
reported to have been worked: OK1DRT, OK1BTN, OK1DTN. Are these really three
new stations?
The only one I have heard is OK1DTN, 549 here.
73, John, G4CNN





_______________________________________________________
Send a cool gift with your E-Card
http://www.bluemountain.com/giftcenter/




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 5 Mar 2001 05:05:44 -0800 (PST)
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Subject: Re: LF: Re: OK QSO
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Hi All,
I am a little puzzled about the three different OK call signs that have been
worked: OK1DRT, OK1BTN, OK1DTN. Are there really three new stations?
The only one that I have heard is OK1DTN, 549 here.
73, John, G4CNN





_______________________________________________________
Send a cool gift with your E-Card
http://www.bluemountain.com/giftcenter/




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 05 Mar 2001 12:13:27
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Re: OK QSO
In-reply-to: <002601c0a558$888e34e0$cc9e74d5@w8k3f0>
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Have heard OK1DTN for the last 2 weeks several times with good signals,
from 559 up to 589. But so far I always called him in vain.
Most of the time he has a fair amount of QSB on his signal (compared to
others at the same distance).
I wouldn't be surprised if he was running a long wire antenna, I getting
the impression that stations with relatively long wire antennas have more
QSB than those with small toploads or pure verticals.
Could it be that long wires radiate at steeper angles and thus produce more
skywave ?

73, Rik  ON7YD

At 10:41 5/03/01 +0100, you wrote:
>To All from PA0SE
>
>I worked OK1BTN on 25 February; sent 569, received 229. Heard G3YXM and
>ON6ND working him as well.
>
>73, Dick, PA0SE



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: rsgb_lf_group@blacksheep.org
References: <001a01c0a4f2$8791e3e0$906568d5@oemcomputer>
Subject: LF: Re: OK QSO
Date: Mon, 5 Mar 2001 10:41:07 +0100
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To All from PA0SE

I worked OK1BTN on 25 February; sent 569, received 229. Heard G3YXM and
ON6ND working him as well.

73, Dick, PA0SE

----- Oorspronkelijk bericht -----
Van: mike.dennison <mike.dennison@ntlworld.com>
Aan: <rsgb_lf_group@blacksheep.org>
Verzonden: zondag 4 maart 2001 22:29
Onderwerp: LF: OK QSO


> Further to yesterday's message about hearing OK1DRT. I worked him today
(Sun
> 4 March) and gave him 539. He gave me 229 and it was a struggle but
> eventually successful.
>
> 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: "mike.dennison" <mike.dennison@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: OK QSO
Date: Sun, 4 Mar 2001 21:29:38 -0000
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Further to yesterday's message about hearing OK1DRT. I worked him today (Sun
4 March) and gave him 539. He gave me 229 and it was a struggle but
eventually successful.

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: "Alan Melia" <Alan.Melia@btinternet.com>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: spearker qrm
Date: Sun, 4 Mar 2001 12:27:50 -0000
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Hi Lary I have certainly come across that in the distant past when I used to
run RTTY (not using a pc). I wondered why I used to get a corrupt char if I
coughed !! It turned out to be the speaker acting as a mic and putting qrm
into the TU. The radios I use at the moment have audio take off before the
vol control so I dont get problems like that.

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: "cesare tagliabue" <cestag@dada.it>
To: "LF group" <rsgb_lf_group@blacksheep.org>
Subject: LF: new station
Date: Sun, 4 Mar 2001 21:35:17 +0100
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD W3 HTML//EN">
<HTML>
<HEAD>

<META content=text/html;charset=iso-8859-1 http-equiv=Content-Type>
<META content='"MSHTML 4.72.3110.7"' name=GENERATOR>
</HEAD>
<BODY bgColor=#ffffff>
<DIV><FONT color=#000000 size=2>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; <FONT 
color=#000000>Hi all</FONT></FONT></DIV>
<DIV><FONT color=#000000 size=2><FONT 
color=#000000></FONT>&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; This afternoon 
Sun 4 March, around 14.15 UTC I've heard the new OK station OK1DTN calling CQ, 
the signal was very strong, 579 here in Florence; this station seems to be well 
equipped.</FONT></DIV>
<DIV><FONT color=#000000 size=2></FONT><FONT size=2>&nbsp; 73&nbsp; 
Cesare</FONT></DIV>
<DIV><FONT size=2></FONT>&nbsp;</DIV>
<DIV><FONT color=#000000 size=2>Cesare Tagliabue&nbsp;&nbsp; I 5 
TGC<BR>WW-Loc&nbsp; JN53PS<BR>e-mail: <A 
href="mailto:cestag@dada.it">cestag@dada.it</A><BR>url: <A 
href="http://www.dadacasa.com/i5tgc">http://www.dadacasa.com/i5tgc</A><BR></FONT></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>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010228102047.2cdfe722@mail.cc.kuleuven.ac.be> <14YH76-07vfRgC@fwd04.sul.t-online.com> <005001c0a43c$479230d0$0a00a8c0@ThreeLakes.ca>
Subject: LF: Re: 136kHz transmissions
Date: Sun, 4 Mar 2001 20:19:18 -0000
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Larry  said
> I have been having a bit of a problem receiving LF signals with ARGO, I am
> not able to see the signals due to interference.  I have been looking for
> G3LDO with 60 seconds dits and nil just more and more interference.

One of the reasons that have probably made it difficult to receive my
transmissions is that I haven't been transmitting. I put out an e-mail
message on the 18th Feb that I would be transmitting on the morning of the
19th and although I did transmit there was no response of any sort.

The cost of power over here in the UK is not cheap, and to run a transmitter
through the night takes around 6 to 8kW/hrs. Now, while the government has
granted us pensioners an extra £200 for heating costs for the winter months,
we still have to be careful if we are not to run up large energy bills.

I am quite happy to make transmissions over limited periods of time, where
they have the chance of being more effective.
If there is interest I will transmit this week (Monday to Friday) from 0530
to 0630 on 135.920 using a dot period that allows the call to be sent within
the hour.

Anyone interested?

Regards,
Peter, G3LDO

<g3ldo@ukonline.co.uk>







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To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: Re: LF: corrections
In-reply-to: <3AA1455E.224CEB80@netscapeonline.co.uk>
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At 19:26 03/03/01 Saturday, G3KEV wrote:
>There seems to be so many mistakes in the latest COMIC. Who did the
>proof reading before publication? Can I get a hardback of the
>corrections? There is no excuse for this amateurish edition.
>I bought the original version and could not see the CARTOONS, they were
>BLACKED out.
>I still have it as proof if anyone would like to try and identify what
>noddy is trying to illustrate.
>The cover was scuffed when I got it, the internal pages were photo
>copied. Did I get a second hand copy? During my time at College this
>sort of presentation would have been a FAILURE. I suppose today with
>only 30% required for a degree pass at University  this is accepatable
>to some!!!!!!

Why not try writing one yourself then?
You seem to know it all.

Walter G3JKV.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: New stations
References: <003b01c0a40e$65144ae0$296468d5@oemcomputer>
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Mike G3XDV wrote:

> This morning, Sat 3 March, I heard OK1DTN whose CW was 439. 
> He worked SM6PXJ exchanging S3 reports. He did not reply to my calls.
> 
> Also worked ON7ZO for the first time - sent 569, received 579.

I also worked ON7ZO for the first time today (Sunday).  I called
him immediately after he signed with Bill G0AKY.  I sent 559,
received 419, using my 12 m vertical.  A flashover in the
variometer interrupted the QSO for a few minutes, but, after I
had brushed away the carbon deposits, we completed OK.  Nice to
hear another new station on the band.  

Regards to all,
Steve GW4ALG



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: "rsgb lf group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Re. QRS
Date: Sun, 4 Mar 2001 07:50:32 -0000
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Hi All,
Hava a look at Riks latest DFCW with half element spacing.Now running
on135.922
use Argo on 10sec dots.I will run it for 2 hours. 73s Laurie.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Vernall" <vernall@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010228102047.2cdfe722@mail.cc.kuleuven.ac.be> <14YH76-07vfRgC@fwd04.sul.t-online.com> <005001c0a43c$479230d0$0a00a8c0@ThreeLakes.ca>
Subject: LF: Re: Interference to ARGO, a surprise
Date: Sun, 4 Mar 2001 13:36:48 +1300
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Larry,

You have found an oddball way of getting unwanted local audio.
> I have been having a bit of a problem receiving LF signals with ARGO, I am
> not able to see the signals due to interference.  I have been looking for
> G3LDO with 60 seconds dits and nil just more and more interference.
>
> Today I did a methodical series of test and I have found that the speaker
I
> have been clip leading into the circuit so I can listen to what is going
on,
> straight noise of course, is in fact reacting to the large blowers I have
> running in my remote site.  The Blowers are the source of interference
that
> has been driving me almost nuts looking for the source.
>
> Have any of the others had local speakers become a visible component in
> their receivning systems?

Also beware of laptops that have onboard microphones.  I was mystified as to
how the Argo screen was apparently working when the audio lead was
unplugged, but it was an audio (sound wave) path via the microphone.

73, Bob ZL2CA



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010228102047.2cdfe722@mail.cc.kuleuven.ac.be> <14YH76-07vfRgC@fwd04.sul.t-online.com>
Subject: LF: Interference to ARGO, a surprise
Date: Sat, 3 Mar 2001 18:47:11 -0500
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Greetings All:

I have been having a bit of a problem receiving LF signals with ARGO, I am
not able to see the signals due to interference.  I have been looking for
G3LDO with 60 seconds dits and nil just more and more interference.

Today I did a methodical series of test and I have found that the speaker I
have been clip leading into the circuit so I can listen to what is going on,
straight noise of course, is in fact reacting to the large blowers I have
running in my remote site.  The Blowers are the source of interference that
has been driving me almost nuts looking for the source.

Have any of the others had local speakers become a visible component in
their receivning systems?

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Vernall" <vernall@xtra.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <001401c0a3fd$2ac9de60$248801d4@g4jnt>
Subject: LF: Re: Re: test
Date: Sun, 4 Mar 2001 09:10:11 +1300
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> No messages from this reflector - is it working properly, or in quarantine
> for Foot and Mouth :-(
> Andy  'JNT

Andy,

Just as a precaution, please run your files through a disinfectant bath
before forwarding them to the reflector :-)

73, Bob ZL2CA



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 3 Mar 2001 20:53:6 +0100
From: "Ko Versteeg" <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org
Subject: Re: Re: LF: Re: test
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At 3/3/01 10:48:00, you wrote:
>
>What suffering withdrawal symptoms? hi (:-)
>John, G4CNN


John.
Not really ;-)
It has been quiet for days so i decided to test to see if there was still a server on the other side.
No Content (subject) came from the split server idea so we don't have to check all mail (i read 'em all)

The lack of activity comes in handy so i can celebrate the new job, i finally managed
to escape from the "black hole"..
Perhaps more to do tomorrow on 136, ready for 73 aswell.

73 de Ko, NL9222.




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "gii3kev" <gii3kev@netscapeonline.co.uk>
Organization: Netscape Online member
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There seems to be so many mistakes in the latest COMIC. Who did the
proof reading before publication? Can I get a hardback of the
corrections? There is no excuse for this amateurish edition.
I bought the original version and could not see the CARTOONS, they were
BLACKED out.
I still have it as proof if anyone would like to try and identify what
noddy is trying to illustrate.
The cover was scuffed when I got it, the internal pages were photo
copied. Did I get a second hand copy? During my time at College this
sort of presentation would have been a FAILURE. I suppose today with
only 30% required for a degree pass at University  this is accepatable
to some!!!!!!

G3KEV






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 3 Mar 2001 10:48:07 -0800 (PST)
From: "john sexton" <computernetworks@excite.com>
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Subject: Re: LF: Re: test
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What suffering withdrawal symptoms? hi (:-)
John, G4CNN





_______________________________________________________
Send a cool gift with your E-Card
http://www.bluemountain.com/giftcenter/




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From: "mike.dennison" <mike.dennison@ntlworld.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: New stations
Date: Sat, 3 Mar 2001 18:18:40 -0000
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This morning, Sat 3 March, I heard OK1DTN whose CW was 439. He worked SM6PXJ
exchanging S3 reports. He did not reply to my calls.

Also worked ON7ZO for the first time - sent 569, received 579.

Mike, G3XDV



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <01C0A3DB.49DD9E80.esanders@erols.com>
From: "Nan and Sandy Sanders" <esanders@erols.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Re: test
Date: Sat, 3 Mar 2001 12:11:35 -0500
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 What do LF waves and viruses have in common ? I wonder if foot and Mouth is affected the same way?

 http://www.nationalpost.com/home/story.html?f=/stories/20010302/489917.html 

				Sandy
				WB5MMB

----------
From: 	Andrew Talbot[SMTP:G4JNT@thersgb.net]
Reply To: 	rsgb_lf_group@blacksheep.org
Sent: 	Saturday, March 03, 2001 11:15 AM
To: 	rsgb_lf_group@blacksheep.org
Subject: 	LF: Re: test 

No messages from this reflector - is it working properly, or in quarantine
for Foot and Mouth :-(
Andy  'JNT

-----Original Message-----
From: Ko Versteeg <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 03 March 2001 11:52
Subject: LF: test [no content]


>
>
>
>






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From: "Andrew Talbot" <G4JNT@thersgb.net>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: test
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No messages from this reflector - is it working properly, or in quarantine
for Foot and Mouth :-(
Andy  'JNT

-----Original Message-----
From: Ko Versteeg <nl9222@wanadoo.nl>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 03 March 2001 11:52
Subject: LF: test [no content]


>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Ko Versteeg" <nl9222@wanadoo.nl>
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Subject: LF: test [no content]
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "LAWRENCE MAYHEAD" <laurie@g3aqc.freeserve.co.uk>
To: "rsgb lf group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Re. Beacon
Date: Thu, 1 Mar 2001 22:37:29 -0000
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I am running the beacon tonight as usual (135.922 kHz ) but Dexter reports
heavy QRN still.Perhaps we have run out of the low noise conditions for this
winter! I will await further information and advise when I am going to
Transmit again. 73s to all.
Laurie.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Hans-Joachim Brandt" <hajo.brandt.dj1zb@t-online.de>
To: rsgb_lf_group@blacksheep.org
References: <3.0.1.16.20010228102047.2cdfe722@mail.cc.kuleuven.ac.be>
Subject: Re: LF: RE: Icom IC-746 on LF
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Dear all,

concerning the beginning of LF amateur operation in Germany I must confess that 
a very detailed description of the equipment used has never been published but I 
think that the contribution below by ON7YD should be corrected:

Just before the Ham Radio Fair at the end of June 1997 at Friedrichshafen our 
administration had isssued two provisional licences for DA0LF (Peter Bobek, 
DJ8WL) and DA0VLF (Dr. Hartmut Buettig, DL1VDL, DARC HF manager) for a 
transmitter power of 100 watts (now we still have 20 watts nominal only). Time 
for preparations were very short, nobody could even think of a 100 watts PA. For 
DA0LF Peter Bobek employed his Hagenuk receiver and exciter with an output of 
200 mW to a random wire. For DA0VLF "Hardy" Buettig had prepared a 20 watts PA 
and a loop aerial, but could not contribute anything for receive and for driving 
his PA. Therefore he was very glad that I could supply him with a passive LF 
converter to 14 MHz (then used with a TS-50 behind, showing 14.136.6 on the 
dial) and a crystal mixer exciter which produced just 3 watts output when 
combinded with Hardy's PA. Coupling between the random wire and the LF loop even 
within the same exhibition hall was rather poor, but a few meters of wire 
connected to the loop did not detune it but improved reception on both sides 
considerably. RST had been about 579. At the stand of the DARC HF referate a lot 
of visitors took the chance to have a first qso on LF and to receive a special 
QSL card.

I myself could not travel to Friedrichshaven that year, because my third son had 
decided to marry just on Friday of that weekend!      

In another cq-DL article (5/1998) Peter Bobek reported that to increase his LF 
power to 50 watts for his long-range qrss tests he had used a push-pull power 
amplifier with two MRF454 employing "completely inadequate cores for LF". This 
may have been the PA needing more cooling for the output transformer than for 
the transistors. 

73 Ha-Jo, DJ1ZB


Rik Strobbe schrieb:
> Hello group,
>
> Most HF-rigs have a "push-pull" PA that has an input and output
> transformer. It are most likely these transformers that determine the lower
> frequency limit.
> I believe to have read an article in CQ-DL about the first 136kHz
> transmissions between DA0LF and DA0VLF in Friedrichshafen (1997 ?). One of
> the stations used a 100W HF push-pull PA to get 20W on 136kHz and they
> needed a fan, not to cool the transistor but to cool the output
> transformer. So even if you get your HF rig running on 136kHz I suggest to
> limit the output to a few Watt in order to avoid a 'meltdown' of the output
> transformer.
>
> 73, Rik  ON7YD
>
>
> At 08:43 28/02/01 -0000, you wrote:
> >I don't know those particular mods, but my IC746 was supplied (quite
> >intentionally) with all band transmit capability.  However, the
> >transmitter is still inhibited when trying to operate below 1.5MHz as
> >the PA cannot cope below this frequency.   Presumably the MARS mods you
> >mention only require transmission at a few other HF freqs so the 100kHz
> >lower limit could be a misunderstanding / typo on the authors part.
> >
> >The firm supplying it told me in no uncertain terms that the guarantee
> >was only valid for transmission in the amateur bands, but Icom confirmed
> >the rig is quite happy transmitting over the whole HF spectrum, but
> >trouble would come if trying to transmit in the 30 - 45MHz region as it
> >would still be trying to use the 30MHz low pass output filter.  Also VHF
> >transmission much outside 140-150MHz would cause problems, again due to
> >the output filter.
> >
> >Andy
> >
> >
> >> -----Original Message-----
> >> From: Jonathan Jesse [mailto:w1jhj@netzero.net]
> >> Sent: 2001-02-27 18:43
> >> To: rsgb_lf_group@blacksheep.org; lowfer@qth.net
> >> Subject: LF: Icom IC-746 on LF
> >> 
> >> 
> >> 
> >> While surfing around the "net" for specifications on Icom's 
> >> IC-746 HF/VHF
> >> transceiver, I found a modification to open the transmit 
> >> capabilities  (so
> >> called MARS/CAP mod).  Reading on, I found that the author 
> >> stated that this
> >> mod will open the transmit from 100khz to 60mhg.  100khz?  
> >> Has anyone tried
> >> and or confirmed this?
> >> 
> >> Thanks,
> >> Jon W1JHJ
> >> Jon
> >> W1JHJ
> >> Plymouth, MA
> >> FN41qw
> >> http://geocities.com/ws1k.rm
> >> 
> >> Shop online without a credit card
> >> http://www.rocketcash.com
> >> RocketCash, a NetZero subsidiary
> >> 
> >
> >
> >-- 
> >The Information contained in this E-Mail and any subsequent correspondence
> >is private and is intended solely for the intended recipient(s).
> >For those other than the recipient any disclosure, copying, distribution, 
> >or any action taken or omitted to be taken in reliance on such information is
> >prohibited and may be unlawful.
> >
> >
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "John Andrews" <w1tag@charter.net>
To: "James Moritz" <j.r.moritz@herts.ac.uk>
Cc: rsgb_lf_group@blacksheep.org
References: <16473.200103231813@gemini>
Subject: LF: Re: [Lowfer] Wolf BPSK from the UK
Date: Fri, 23 Mar 2001 14:22:31 -0500
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Jim,

I will be trying again tonight, at least from 0100 to 0230. Attempted on
Tuesday and Wednesday, but nothing was heard/deciphered. On both evenings,
there was no sign of any other transatlantic activity, either.  My local
conditions were fairly quiet, with the strong carrier on 137 kHz having
departed, at least temporarily.

John Andrews, W1TAG




