From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Larry Kayser" <kayser@sympatico.ca>
To: "Talbot Andrew" <ACTALBOT@dera.gov.uk>,  rsgb_lf_group@blacksheep.org
Subject: LF: Re: DDS Board
Date: Wed, 31 May 2000 21:30:45 -0400
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Andy:

Please consider running the pc trace from Pin 18 of the PIC to Pin 8 of the
AD9850 over near the edge of the board and putting some extra contact pads
on the line so it will be possible with minimum risk to get at the FQ_UD
line for external coherent control of the signaling events.  I would also be
prepared to pay a bit more for the board if you had a prototyping area on
the edge of the board, say about 50% of the size of the basic board.

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "George Brown" <george.brown@rsgb.org.uk>
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Subject: LF: SAQ times
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I can confirm the times at which SAQ will be on the air on July 2nd, 
the information coming by e-mail from Lennart Benson at Grimeton.

SAQ is due on the air at:

0830, 0845, 1230 and 1245 UTC.

George Brown, M5ACN.




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Kevin Ravenhill" <kevin.ravenhill@ukonline.co.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Slow CW vs. BPSK etc.
Date: Thu, 1 Jun 2000 09:48:59 +0100
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There's a lot of discussion going on at the moment on the US "LowFER"
mailing list about the relative merits of slow CW versus BPSK (in this case
relating to the COHERENT/AFRICA software by Bill de Carle, VE2IQ). The
general consensus of opinion seems to be that if you are going to use
"machine" modes, BPSK has considerable superiority over any form of slow CW
for the kind of very weak signals often encountered on the LF bands.
Estimates of the effective improvement range from 6dB to 23dB depending on
what factors are taken into account!

At the risk of causing some heated discussion, I'm curious to know the views
of members of this list - particularly in relation to future transatlantic
attempts.

Also, does anyone have an idea of the relative usage of slow CW (QRSs and
related FSK modes) versus modes like PSK31/PSK08 etc, in Europe? My
impression is that various forms of slow CW are still favoured by most
people (and perhaps rightly so, in terms of picking the best/most convenient
mode for what you are trying to do), but I haven't been able to monitor the
LF bands for some time so I don't really know what the current situation is
like.

For anyone who isn't subscribed to the abovementioned list and wishes to
subscribe, send an email to majordomo@qth.net with no title and with
"subscribe lowfer" in the body of the text. You'll get a return email with a
password which has to be sent back, after which you'll be subscribed.

Regards

Kevin, G1HDQ





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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Subject: Re: LF: Diversity reception
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Dear LF Group,
	The Idea of having several widely separated, synchronised 
receivers for diversity reception sounds rather like the 'Very Long 
Baseline Interferometer' techniques used by radioastronomers.

Presumably one could use an existing broadcast carrier, or 
perhaps the TV colour burst signal, as a clock signal for 
synchronisation, to make the system a bit simpler.

Cheers, Jim Moritz
73 de M0BMU


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: Aerial tests.
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Re Jim's aerial tests, I had a word with my pal the (retired) Decca
aerial guru and showed him some of the emails. He said :

(a)	If both aerials are vertically polarised only then there shouldn't be
any difference between their radiated fields if they're radiating the same
power because both are electrically very small. The only difference would
be in their conversion efficiency (RF in to RF out). If there is a genuine
difference in observed field strength then it simply means there is
something wrong in the calculation of ERP - ae efficiency perhaps.
Decca obtained their ae. efficiency figures by feeding with a known
amount of power and making absolute field strength observations
at multiple distant points allowing for different path conductivities.

(b)	If the small one has an assymetric horizontal component (flat-top)
this will complicate matters considerably since it will radiate both 
vertical and
horizontally-polarised and there will be interaction between them that
will affect the radiation pattern. So it would be unlikely to have a circular
polar pattern and this might account for some of the observed variations.
Said it would be better from this viewpoint to make a "T" rather than
a "L", then the horizontal would cancel out.

(c)	Jim's precautions against interaction between aerials were correct
and with the big one grounded there would have been very little, if any.
between the aerials themselves. However, the small one would have been
sharing the earth mat of the big one since it was well within the induction
field so it was probably more efficient than thought.

(d)	The dropped wires were put in simply to increase capacitance back
up to the standard Decca 3750 pf.  All their coils etc were designed for
this figure and it was much cheaper to do this than to have to design and
build new coil systems. Don't forget Decca had to transmit five frequencies
simultaneously every 20 seconds (lane idents) and getting the same power
at the correct phases without any interaction was quite a problem. Hence
the complicated ATU coil setup.

(e)	At one time Decca had a transportable Decca system that used a 100ft
mast with a 100ft radius ground plane (wires run out on the surface). Using
a 500W Tx they used to get ranges of up to 300 miles over water.

(f)	Finally he said the main problem with small aerials was the greatly 
increased
voltages and insulation problems. They always had problems on the transportable
system to the extent they had a man whose job it was to clean all the 
insulators
every morning and they couldn't be located on coasts because the salt water
shorted out everything "in hours".  The 100m aerials were only installed at
a few sites in the early days in the hope of reducing the number of chains 
required
but it turned out skywave was the limiting range factor (screwed up phasing
on which the whole system depended). This meant Decca couldn't be used more
than about 200 miles at night, so later transmitters had smaller and much 
cheaper
aerials (150ft "T") which covered up to 200 miles quite adequately.

Walter G3JKV.



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: Slow CW vs. BPSK etc.
Date: Thu, 1 Jun 2000 11:49:49 +0100
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>There's a lot of discussion going on at the moment on the US "LowFER"
>mailing list about the relative merits of slow CW versus BPSK (in this
case
>relating to the COHERENT/AFRICA software by Bill de Carle, VE2IQ). The
>general consensus of opinion seems to be that if you are going to use
>"machine" modes, BPSK has considerable superiority over any form of
slow CW
>for the kind of very weak signals often encountered on the LF bands.
>Estimates of the effective improvement range from 6dB to 23dB depending
on
>what factors are taken into account!

(Slow) CW vs BPSK etc..

To compare theoretically, firstly we need to make the assumption that
data rates are similar for the two modes.  CW employs a reasonably
efficient variable length coding scheme where character length depends
on letter frequency of occurence.  We need to compare like with like,
and in PSK31 something similar is used.  Both schemes (CW and varicode)
offer about 6 bits per character coding efficiency, not allowing for
inter letter framing pulses.

For a given data rate, there is at least a 6dB advantage to be had in
going from an on / off keyed waveform to a BPSK one.  This is because
the amplitude differnece for the 1 and 0 states is doubled.  For on /off
keying (OOK) it is from 0 to (say) 1 Volt.  For an equivalent BPSK
signal, since the amplitude is plus / minus for 180 degree keying the
total amplitude change is 2 Volts, ie. 6dB better in noise using this
very simple back of an envelope calculation.  

There is further adavantage to be had by using PSK as well.  For OOK a
non coherent detector is usually employed - ie human ears for CW or eyes
for QRSS etc.  Lets we have a perfect operator with golden ears (or
eyes) and   assume these are perfect power detectors for now, in other
words they cannot respond to voltage or phase so are definitely
non-coherent. Various statistical calculations can be made to define at
what level the signal is detectable above noise, but in practice a S/N
value of 10dB is usually the best we can get away with - this is in the
theoretical minimum bandwidth of the signal at roughly half the
signalling rate and does not take into account bandwidth limiting for
spectral reasons.

BPSK, however, is received coherently.  ie voltage is integrated over
the symbol period rather than power, which immediately calls up a square
root term to the detection statistics compared with power.   Again
statistical rules can be applied and Signal to Noise vs. error rate
curves can be generated for minimum bandwidth.  The results usually end
up with a S/N of 6 - 8dB being sufficient for 'reasonable' error rate.
By reasonable, we mean something that will communicate useful
information with errors that the brain can correct for,  - and lets not
get into a discussion of error correction coding.   While coherent
decoding could be applied to OOK signals, what is the point ?  If we go
to the effort of building a coherent detector, then we might as well
make the most of it and use BPSK which is as easy to generate as CW.
(You can even use a changeover realy in the antenna feed as a desperate
last resort)

So we now have something like 6db advantage from peak power alone, and
around another 3dB for coherent vs incoherent detection resulting in 9dB
advantage for PSK over On Off Keying.   I don't know if Coherent offers
the variable length coding to get the average data rate down, if it
doesn't then the advantage is marginally less but this is easily offset
by the heavy error correction that it does have as an option.  

This is a very simple calculation and  communications theory experts
will probably drill all sorts of holes in it, but I bet many of their
arguments will cancel out.   We do actually observe  8 - 10dB S/N
advantage in coherent PSK modes versus incoherent ones such as CW.
Broadly similar arguments apply to SSB vs. AM and no one disputes the
advantage there.

A completely different set of rules apply when noise is non Gaussian
(non white) such as bursts and for ionospheric propagation modes with
multipath, and mean that non coherent modes such as multilevel FSK do
have certain other advantages to offer.

The Shannon theoretical limit for communications in a noisy channel is
(Signaling Rate / Bandwidth, Bn) = LOG2(1 + S/N).    In other words, for
Signalling rate  equal to Bandwidth which is the easy to understand
case,  Signal to Noise equals Unity  =  0dB !!  
Consider CW, the best ears are probably equivalent to 50 Hz bandwidth
and the best operator can probably cope with 24WPM (= 20 Hz) in very
noisy conditions.  S / BW = 0.4 so according to Shannons limit, it ought
to be possible to receive this in a S/N ratio of  2^(0.4) - 1 = 0.32 =
-5dB  (yes, negative S/N !)  In the 200 Hz bandwidth filter usually
employed this becomes -11db S/N

Uncoded PSK itself will nowhere achieve the Shannon limit either, but
with very efficient Turbo error correction coding schemes now appearing,
it is possible to get within 0.7db of it.

PSK31 has a lot to offer on LF, but unfortunately due to the almost
universal use of switching high efficiency power amplifiers and dearth
of tranceivers, is hardly used.   While PSK can be transmitted over non
linear class C/D/E amplifiers, it generates disgusting sidelobes that
beat even key clicks for their annoyance value!

In the Data column in RadCom, in the fundamentals section which will
appear each issue, I am slowly developing an easy intuitive guide to
data communications.  So far three have appeared - any feedback would be
appreciated.

Which reminds me, the deadline for August's issue is only 15 days away !
Must get on with it.

Andy  G4JNT



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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Kevin Ravenhill wrote :

> The general consensus of opinion seems to be that if you are going to use
> "machine" modes, BPSK has considerable superiority over any form of slow CW
> for the kind of very weak signals often encountered on the LF bands.

When you say "machine" modes, are you meaning CW decoded by software or
by the brain (be it aurally or visually) ? There is a profound difference...

73,
Alberto    I2PHD




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: Slow CW vs. BPSK etc.
Date: Thu, 01 Jun 2000 14:58:46 +0300
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On Thu, 1 Jun 2000 09:48:59 +0100, "Kevin Ravenhill"
<kevin.ravenhill@ukonline.co.uk> wrote:

>There's a lot of discussion going on at the moment on the US "LowFER"
>mailing list about the relative merits of slow CW versus BPSK

I think it is appropriate time to remind that some countries have
emission mode limitations on LF (as far as I know A1A is the only mode
allowed in Norway). It should be a good idea for amateurs in these
countries to contact their national amateur radio society and ask them
to discuss lifting the mode limitation with their telecom authorities.

When designing a new mode/protocol the station identification must be
handled in some way, hopefully compatible with ID requirements in most
countries.

Paul OH3LWR
 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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In 22.17 31/05/00 , Dick wrote: 
>
>>
>> To All from PAoSE
>>  
>> ...
>> 73, Dick, PA0SE
>>  
>>  
>> P.S.: Sorry for the vertical line at the left, I don't know how to get rid
>> of it.
>
> </HTML>
>>
>> </x-html> 
>


Stop using Outlook .... ;-)))

73, Marco IK1ODO






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "M. Bruno" <spin@inrete.it>
Subject: LF: Slow CW, BPSK, machine modes
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In 14.06 01/06/00 , hai scritto:
>Kevin Ravenhill wrote :
>
>> The general consensus of opinion seems to be that if you are going to use
>> "machine" modes, BPSK has considerable superiority over any form of slow CW
>> for the kind of very weak signals often encountered on the LF bands.
>
>When you say "machine" modes, are you meaning CW decoded by software or
>by the brain (be it aurally or visually) ? There is a profound difference...
>
>73,
>Alberto    I2PHD
>
>

I agree, visually decoded CW is NOT a machine mode; the final decoding
being done by the operator eye-brain, instaead of ear-brain. 

I found it fascinating for that reason; you have to add some operator skill.

BPSK is a real machine mode; somebody talks about having a large bell calling
him when AFRICA locks on a signal. I see no interest in this, except for
propagation studies. A QSO obtained trying day after day, by previous schedule
and so on, is more rewarding to me.

73, Marco IK1ODO



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: QRSS vs. BPSK, etc.
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Dear LF Group,
	I'm sure that modes such as BPSK have considerable 
technical advantages compared to the slow CW modes. But as in 
most areas of engineering, technical excellence is not the only 
factor.

The advantages of QRSS include the following:

- It is very easy to modify an existing CW station for QRSS 
operation - all that is required are some simple keying circuits and 
leads, and a rather basic PC with some free software.

-QRSS is not demanding on the transmitter/receiver. The duty 
cycle is much the same as normal CW, any transmitter capable of 
on-off keying can be used, all that is required of the receiver is an 
audio output. Exceptional frequency stability is not required.

-There are no synchronisation or clock recovery issues with 
QRSS; also, the PC spectrogram display effectively 'decodes' all 
the signals present in a relatively wide bandwidth. These things 
make random QSO's straightforwards - there is no need to know 
the exact frequency a station is using, the time it will be operating, 
or even to know the exact modulation method that will be used.

In summary, slow CW may not give the very best results, or be a 
particularly satisfying intellectual challenge, but it does give rather 
good results with simple equipment.

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 Slow CW vs. BPSK etc.
Date: Thu, 1 Jun 2000 13:48:32 +0100
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> Kevin Ravenhill wrote :
> 
> >> The general consensus of opinion seems to be that if you are going
> to use
> >> "machine" modes, BPSK has considerable superiority over any form of
> slow CW
> >> for the kind of very weak signals often encountered on the LF
> bands.
> 
>When you say "machine" modes, are you meaning CW decoded by software or
>by the brain (be it aurally or visually) ? There is a profound
difference...


Actually, there probably isn't that much difference in practice, again
comapring like with like.
The ear(or eye) / brain combination serves as a very good error
correction mechanism where the mode being transmitted contains
sufficient redundancy to allow this.  

Examples are CW with it's long and short elements, Hellschreiber with
its pattern of letter shapes and, of course, the enormous redundancy
given by the context and spelling of words which means we can usually
understand text    whxre eveqy wbrd h6a i smeluing misyaki in it .

If this is contrasted with machine generated codes, such as
convolutional and block coding superimposed onto plain ASCII coded text,
then I guess that the fully machine based system can produce very much
better results if you are prepared to accept the overheads.   One major
drawback being that the better an error correction scheme is, the longer
it takes to process all the interleaved data.   One amateur-developed
data mode using 64 parallel tones (MT63) has 10 second overhead on data
at normal typing speed.  Whilst being extremally good at coping with QRM
(it is designed primarily for the HF environment, not white noise) the
10s between typing a character and it's appearing on the receiver's
screen does make for enforced leisurely QSOs. 

For a decent real time communications system, with a reasonable
trade-off of delay against error correction, the machine system probably
is about on a par with a (very good) human ear brain combination.   The
real advantage comes in that the machine can cover a much wider range of
data rate vs. error correction trade off values, instantly, and can
automatically adapt itself to changing propagation condidtions.  Just
compare PSK31 with 20 - 30 WPM CW, it is considerably better.

CW operators do constantly trade off time delay vs S/N.   A few years
ago I once sat on a (windy and rainswept as usual) hilltop taking over
20 minutes to receive a report and locator on 10 GHz using CW - with the
other station sending repeatedly one letter or number at a time in
conjunction with a 144MHz talkback link where I called whenever the
character had been copied.   That equates to something like 0.05 Bits /
second using a protocol which in machine terms would be a multiple
redundant error correcting Automatic reQuest Repeat system. And all just
to set a new personal best distance on this band.   10GHz does not lend
itself to low data rate narrow bandwidth communications so CW is still
of considerably more use there than it is on the LF bands.   So much for
the class A/B licence debate and access to HF bands !

The QSO would have gone something like this :

G4JNT on 2m:		"Send the first number of the report"
G8### on 10GHZ	"1  1  1  1  1  1  1  1  1  1  1  1  1  1  1  "
'jnt			"OK Got that, now the second letter"
G8###			"2  2  2  2  2  2  2  2  2  2  2  2  2  2   2  2
2  2  2  2  2  2  2   2  2  2  2  "
'jnt			"Negative again, again"
G8###			"2  2  2  2  2  2  2  2  2  2  2  2  2  2  2   2
2  2  2  "
etc. etc. 

How much easier if we could have just wound the software down to 0.05
B/s and told it to get on with the job.  Even QRSS can't work on the
higher microwave bands, drift of most systems is a few tens or hundreds
of Hz taking the signal well outside the tuning range of Spect,,,,
Incidently, QSOs like this are common on the uW bands and, before anyone
asks, contest rules have allowances for this dual band operation built
in.

Whilst on this matter, If there are any communication specialists out
there who know of a scheme - is there a way of coding and getting the
full benefit of (say) 0.05 B/s using a spread spectrum waveform 1 - 3kHz
wide (SSB transceiver) that is immune to several 100 Hz of frequency
shift.  The moonbounce community would leap at such a data scheme as
well as the uW operators

Not a very LF orientated ramble for this reflector, but ..........

Andy  G4JNT


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Kevin Ravenhill" <kevin.ravenhill@ukonline.co.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
References: <003e01bfcba6$70b54200$ac1886d4@kevin> <393648EF.ADBCDF55@usa.net>
Subject: Re: LF: Slow CW vs. BPSK etc.
Date: Thu, 1 Jun 2000 14:44:15 +0100
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> When you say "machine" modes, are you meaning CW decoded by software or
> by the brain (be it aurally or visually) ? There is a profound
difference...
>
> 73,
> Alberto    I2PHD

By "machine" modes, I mean anything which requires a PC or other
hard/software to change the raw CW+QRM/QRN audio input into something which
can be interpreted by human senses (usually involving translating the signal
from audible to visible form). This is in contrast to direct aural decoding
of CW by the brain, filter-assisted or otherwise, which generally requires a
lot more human "processing power".

Apart from the obvious i.e. the various decoders with text output, I would
put software such as Spectran (VY NICE program, by the way!), Spectrogram,
etc. in the "machine modes" category. This is because it takes a wanted
audio signal which is buried in QRM/QRN and therefore indistinguishable, and
translates it into a visual form, separating it from the unwanted stuff as a
discrete trace on a screen. The only part the brain is required to play in
this process is to interpret the trace as letters and numbers - most of the
hard work has been done already.

Hope this explanation is reasonably coherent!

Regards

Kevin, G1HDQ.





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: Slow CW vs. BPSK etc.
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> When you say "machine" modes, are you meaning CW decoded by software or by
> the brain (be it aurally or visually) ? There is a profound difference...
> 73, Alberto    I2PHD

This is all-important. Extremely weak stations require considerable 
additional work by the 'computer between the ears' to decipher 
what is signal and what is noise on the screen - just like aural 
Morse, but visual. This accounts for several extra dB of gain, and 
however slow you send the Morse, this advantage is still available. 
It would take a very sophisticated computer to be as good. 

There are, of course, advantages in having modes with little or no 
manual intervention. Suppose, for instance, it were possible to 
monitor for a transatlantic beacon and raise an alarm when a 
callsign (or some pattern) was recognised by the computer. This 
may be where BPSK comes into its own as being superior other 
purely machine-read modes.






Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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From: "Mike Dennison" <mike.dennison@rsgb.org.uk>
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Subject: Re: LF: Slow CW vs. BPSK etc.
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G2HDQ wrote:
> Apart from the obvious i.e. the various decoders with text output, I would
> put software such as Spectran (VY NICE program, by the way!), Spectrogram,
> etc. in the "machine modes" category. This is because it takes a wanted
> audio signal which is buried in QRM/QRN and therefore indistinguishable,
> and translates it into a visual form, separating it from the unwanted
> stuff as a discrete trace on a screen. The only part the brain is required
> to play in this process is to interpret the trace as letters and numbers -
> most of the hard work has been done already.
> 

See my other message. If the only work was to interpret the trace 
as letters and numbers, it would be trivial for a bit more coding to 
be included to do just that - and of course 'strong' signals (ie those 
that are louder than a mere 10db below noise) come into this 
category. However, it is quite possible to dig much deeper than this 
by using the brain to work out what is rubbish and what is signal. 
Most machines are quite incapable of ignoring static and other 
noise. 

In the few reports I have read about the various PSK modes, they 
appear to have similar error rate to CW, which is very impressive for 
something read by a machine (conventional CW read by a machine 
is terrible in the presence of QRM), but at sub-noise levels the error 
rate increases. This is not the case with visual CW modes for the 
reasons mentioned above. Of course, very low bit rate PSK may 
well be a different matter, and that is really comparing like for like.


Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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: Re: LF: Slow CW vs. BPSK etc.
References: <003e01bfcba6$70b54200$ac1886d4@kevin> <393648EF.ADBCDF55@usa.net> <002701bfcbcf$b0c2f9e0$f41a86d4@kevin>
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Kevin Ravenhill wrote:

> ......... The only part the brain is required to play in
> this process is to interpret the trace as letters and numbers - most of the
> hard work has been done already.
>

I have to disagree. The brain has also the task to sort out white spots, caused
by noise, from true signal lines (or fragmented fractions of them).
And this is where the powerful pattern recognition mechanism embedded in our
personal  'CPU' plays an invaluable role. Wonder why the AI (Artificial Intelligence)
so much touted a decade and half ago hasn't taken off as they would have been
expected ? So far the brain has mainly resisted to divulge the secrets of its inner
algorithmical working. The only pale approximations to it are the neural networks,
which aren't a technological breakthough, at least with the present state of  art.

73
Alberto    I2PHD





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
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Subject: LF: QRS, BPSK and diversity
Date: Thu, 1 Jun 2000 20:19:04 +0100
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Hi all, I monitored Dave G3YXM's attempts to make a PSK31 with Reino OH1TN
earlier in the year (or was it last year now). I could see the signal from
Reino easily on FFTDSP4 (not one of the most sensitive of DSP waterfall
displays available these days) but using the soundcard PSK31 decoder I could
not copy a signal at all from Reino, though I had a perfect copy of Dave so
the system was working. It may be that the soundcard decoder is not the most
sensitive, but that test showed that Dave (with a better aerial than me)
could only get PSK31 copy when Reino was fully R5 on hand-keyed morse (not
even QRS).  I suspect the power output from both Dave and Reino was probably
down about 3dB on their normal CW power, due to the need to use a linear
system for PSK31.  I await Andy's experiments with interest.

Several of us have recently copied a QRS beacon from Marco running an
estimated 1mW ERP south of the Alps (900kms from me) I think this is well
into the area of powers being radiated by the Lowfer beacons allowing for
their frequency 50% higher, so their aerials are twice as efficient. Also I
suspect the Lowfer beacon keepers who radiate BPSK may be the more technical
ones who have the more efficient stations.

I think it may be a case of 'horses for courses' and it all depends what you
wish to achieve.

On the diversity topic, strangely enough I related it to the astronomers
correlation proceedures as well Jim, but am I wrong or is it a case of
diminishing returns? I suspect you have to double the number of aerials for
each 3dB. Four aerials is feasible but gives only 6dB and we would need
eight aerials for 9dB which would be a bit of an epic. I did once write a
simulation of this using an FFT writen in Basic (a sort of Slow Fast Fourier
Transform!) with uncorrelated random noise masking the wanted signal. It
certainly works but got the feeling that it was a lot of effort for a fairly
small return. We are not interested in locating a source accurately, as are
the astronomers so we do not use one of the main points of the VLBA, its
spatial resolution.

All interesting stuff.
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: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
Subject: LF: BPSK's, not all the same.
Date: Thu, 1 Jun 2000 21:33:53 -0400
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The thread that has been running about BPSK / QRS CW covers the technical
issues, but I sense there is an assumption that BPSK as per AFRICA/COHERENT
by Bill de Carle and the PSK31 (and it's variants) by G3PLX are radically
different implementations of PSK.

The purpose of this note is to stimulate a discussion of the differences
between the two systems.

For starters, PSK31 was defined by Peter Martinez, G3PLX, as being for
"keyboard to keyboard" types of applications.  This is a new system
implementation of what we used to call "Green Keys" type of teletype
operation.  The basic tenet as I understand it is for keyboard to keyboard
QSO's over the radio.

In the very opposite sense, C-BPSK as implemented in Coherent/Africa by Bill
de Carle, VE2IQ, will accommodate users who wish to use the package for
Keyboard to Keyboard, but the REAL PURPOSE of the programs is to get down
and dig a signal out of the mud, to do so with the single determination of
finding a signal and using every mathematical resource available to pull
that signal out of the noise.

The application of these packages should take into consideration the job
that is desired to be done.  Using PSK31 to  work over the North Atlantic on
136 would be a gross misapplication of the software unless there was certain
knowledge that the task can in fact be accomplished within a reasonable time
period.  On the other hand Coherent/Africa  will patiently wait for months
or even years with a minimum of demands on the users for a signal to pop out
of the noise.

The technical discussion are enlightening and really great but the
discussion also needs to consider what the objectives are for the experiment
that the user desires to perform.  It is obvious to me that there is a need
to identify what applications can make the best use of the existing software
programs such as QRS CW, PSK31, and Coherent/Africa.  If careful attention
is given to the details of the system requirements then at the end of the
day the software system developers will have new opportunities to make their
systems stay on the leading edge of performance.

Larry
VA3LK





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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Slow CW vs. BPSK. & Computer modes
Date: Fri, 2 Jun 2000 09:21:17 +0100
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>This is all-important. Extremely weak stations require considerable 
>additional work by the 'computer between the ears' to decipher 
>what is signal and what is noise on the screen - just like aural 
>Morse, but visual. This accounts for several extra dB of gain, and 
>however slow you send the Morse, this advantage is still available. 
>It would take a very sophisticated computer to be as good. 

NO !  With these modes the computer is not doing anything to aid
extraction of the signal that could not be done with conventional
hardware.    The 'several extra dB gain' is just there because more
noise has been filtered out.  The brain is just looking at amplitude
changes in this narrow bandwidth and integrating over the signalling
period (looking at brightness over the length of a dot). 

All Spect....  is,  is a bank of narrow filters.   There is nothing in
theory to stop you making a crystal filter, or a whole bank of them this
narrow.   For a display mechanism, a chart recorder - multiple pen ones
are available.    All this technology was available in the 1950s as I'm
sure those who were around in that era will remember.

All the computer does is make this much simpler and cheaper and
available to everyone, it is only a filter and display mechanism so
please can we stop referring to Spect...   as computer modes.   It can
be done in other ways.

Coherent etc and PSK31 are computer modes,  SPECT..... is not, it is
only a filter bank and display.

Real computer / DSP modes mean making use of coherent detection and
error correction - and have nothing to do with the speed of the
signalling.   

There seems to be no appreciation on this newsgroup of the real value of
coherent detection - that is, having phase information available when
the signal is decoded and coherently locking to the signal carrier and
bit  timing.   Simple theory, as I covered in a previous email, shows
mathematically the considerable theoretical advantage of coherent
detection over non coherent, there is no dispute about this.

SO unless your ears / eyes can respond to signal phase, is doesn't
matter how much personal pride says that the brain is a marvelous
computer, is will never compete against PSK  :  

Given the same TOTAL overall signalling speed and comparing like with
like on the end to end link.

Repeating CW characters time and time again has to be compared with true
error correction and low data rate signalling.

Computer error correction does the same job as the eye interpreting
between the dots on Spect...,   and with well chosen codes can do an
awful lot better.  These optimum codes are only just beginning to appear
thanks primarily to the huge research effort funded by the mobile phone
industry, but hopefully Coherent etc will soon make use of them - the
equations are public information.  The maths is similar, just the
implementation different.

Coherent etc and PSK31 are computer modes,  Spect... is not.

Andy  G4JNT


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Kevin Ravenhill" <kevin.ravenhill@ukonline.co.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: BPSK and other modes
Date: Fri, 2 Jun 2000 09:43:09 +0100
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The comments from Larry, VA3LK echo my thoughts to a large extent. I feel
that, FOR CERTAIN SITUATIONS e.g. transatlantic attempts, BPSK as
implemented in Coherent/Africa is specifically designed for the job and
would probably stand a better chance of success than, say, PSKxx or QRSS,
given adequate phase stability of the propagation path. It certainly seems
to have been used with success in the USA, with Part 15 LowFER beacons (<1mW
ERP?) apparently producing reliable copy over paths of 1600km+ under the
right conditions.

Having said this, I believe the US LowFER distance record may still be
USA-Hawaii using standard CW! It is, indeed, very much a case of "horses for
courses" and I certainly wouldn't make a blanket claim that any one mode is
superior to any others. Basically, like everything in this hobby, it comes
down to using whatever you are comfortable with and/or have the kit for.

Lastly, and with reference to recent comments on the reflector, perhaps a
more correct term than "machine modes" would be "machine-assisted modes"!

Regards

Kevin, G1HDQ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: BPSK and other modes
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> Lastly, and with reference to recent comments on the reflector, perhaps a
> more correct term than "machine modes" would be "machine-assisted modes"!
> Regards
> Kevin, G1HDQ

At the risk of winding everyone up, what is "machine assisted"? 
What is the difference between DSP for audio reception and DSP 
for screen reception? Or is the analogue filter a machine, or the 
receiver itself?

In trying to formulate the rules for the Peter Bobeck Award, we 
agonised over this sort of thing, and concluded that if you are going 
to make any distinction at all, it should be related to the time taken 
to conclude the QSO (the bit rate in data terms). If it takes an hour 
to exchange reports and calls, this is arguably a different level of 
achievement to taking a few minutes, no matter whether you repeat 
CW or SSB over and over (and who hasn't done that from time to 
time?) or have very long dots, or a clever redundancy arrangement.


Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
References: <4.2.0.58.20000601105903.0097a890@mail.pncl.co.uk>
Subject: LF: Re: Aerial tests.
Date: Fri, 2 Jun 2000 13:41:08 +0200
Organization: Freeler
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To All from PA0SE

Walter Blanchard quoted the RACAL expert who has in the past  designed the
Decca antennas as follows:

>(...)  If the small one has an assymetric horizontal component (flat-top)
> this will complicate matters considerably since it will radiate both
> vertical and
> horizontally-polarised and there will be interaction between them that
> will affect the radiation pattern. So it would be unlikely to have a
circular
> polar pattern and this might account for some of the observed variations.

This is not confirmed by computer simulation.

Computer program AO by Brian Beezley, K6STI, shows  for the L-antenna over
medium ground  an almost perfect omnidirectional radiation pattern. The
deviation
from a circle is no  more than about 0.1dB.

The program also shows that the maximum of the horizontally polarised wave
is straight up and 21.1dB down on the maximum of the vertically polarised
wave.
The latter maximum occurs under an angle of 12 degrees (direct + reflected
wave).
In the region where the inverse distance law is applicable the space in the
vertical radiation pattern between  zero degrees and the lobe under 12
degrees is filled by the surface wave.

73, Dick, PA0SE






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <134.200006021150@gemini>
From: "James Moritz" <j.r.moritz@herts.ac.uk>
Organization: University of Hertfordshire
To: rsgb_lf_group@blacksheep.org
Date: Fri, 2 Jun 2000 12:57:58 +0000
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Subject: LF: Litz wire stripping method
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Dear LF Group,
	I recently salvaged some thick litz wire, and have been trying to 
find a workable method of stripping the insulation. The enamel is of 
the older, dark coloured type, which cannot be removed by dipping 
in molten solder. The overall conductor thickness is about 4mm 
with 729 strands, and a spirit burner as previously suggested on 
this reflector just does not make any impression. A blowtorch does, 
but also burns away the outer strands and the plastic sheathing. I 
believe chemical strippers are available, but have to be melted at 
high temperature, and then neutralised afterwards.

However, the following seems to work quite well - strip about 50mm 
of the plastic sheathing, and wrap the end 25mm of wire strands 
tightly in a piece of copper foil (such as can be peeled off some 
PCB laminate, or the type used for EMC shielding). Wrap a smaller 
piece of foil around the 12mm of wire strands nearest the stripped 
back sheathing, and grip with a pair of pliers - this acts as a 
heatsink to protect the sheathing. Heat the foil covered end red hot 
with a blowtorch. The enamel burns off with a small flame at the 
end of the foil, while the foil protects the copper strands from the 
blowtorch flame. When the flame goes out, leave to cool and 
unwrap the foil. The wire strands are coated in black, shiny 
residue, which can be cleaned off by rubbing the end of the wire 
against the bottom of a shallow dish full of water, as if cleaning a 
paint brush. Somewhat suprisingly, this leaves clean, shiny strands 
of copper that can be soldered in the usual way.

Just thought this might be useful to know,
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: <001101bfcc87$1060e4e0$0d5a883e@iway.co.uk>
From: "Robin Greenwood" <robin@g3lba.freeserve.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <134.200006021150@gemini>
Subject: LF: Re: Litz wire stripping method
Date: Fri, 2 Jun 2000 12:38:23 +0100
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Splay wires slightly, heat in a methelated spirit flame. until red hot then
plunge into a small pot of Meths  It comes out clean. Do this cautiously and
outside...!!!..
Robin G3LBA
----- Original Message -----
From: "James Moritz" <j.r.moritz@herts.ac.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: 02 June 2000 13:57
Subject: LF: Litz wire stripping method


> Dear LF Group,
> I recently salvaged some thick litz wire, and have been trying to
> find a workable method of stripping the insulation. The enamel is of
> the older, dark coloured type, which cannot be removed by dipping
> in molten solder. The overall conductor thickness is about 4mm
> with 729 strands, and a spirit burner as previously suggested on
> this reflector just does not make any impression. A blowtorch does,
> but also burns away the outer strands and the plastic sheathing. I
> believe chemical strippers are available, but have to be melted at
> high temperature, and then neutralised afterwards.
>
> However, the following seems to work quite well - strip about 50mm
> of the plastic sheathing, and wrap the end 25mm of wire strands
> tightly in a piece of copper foil (such as can be peeled off some
> PCB laminate, or the type used for EMC shielding). Wrap a smaller
> piece of foil around the 12mm of wire strands nearest the stripped
> back sheathing, and grip with a pair of pliers - this acts as a
> heatsink to protect the sheathing. Heat the foil covered end red hot
> with a blowtorch. The enamel burns off with a small flame at the
> end of the foil, while the foil protects the copper strands from the
> blowtorch flame. When the flame goes out, leave to cool and
> unwrap the foil. The wire strands are coated in black, shiny
> residue, which can be cleaned off by rubbing the end of the wire
> against the bottom of a shallow dish full of water, as if cleaning a
> paint brush. Somewhat suprisingly, this leaves clean, shiny strands
> of copper that can be soldered in the usual way.
>
> Just thought this might be useful to know,
> 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, 02 Jun 2000 15:38:12 +0200
From: "Alberto di Bene" <dibene@usa.net>
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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Slow CW vs. BPSK. & Computer modes
References: <3617AC3245C2D1118A840000F805359C01AB8C85@pdw-mercury-1.dera.gov.uk>
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Talbot Andrew wrote:

> [snip]
> There seems to be no appreciation on this newsgroup of the real value of
> coherent detection - that is, having phase information available when
> the signal is decoded and coherently locking to the signal carrier and
> bit  timing.   Simple theory, as I covered in a previous email, shows
> mathematically the considerable theoretical advantage of coherent
> detection over non coherent, there is no dispute about this.
> [snip]

Andy,
                 from a theoretical point of view you are damn right. But I am
not so sure that LF/HF propagation can preserve phase coherence and
with it the decoding gain achieved with coherent detection, unless you are
willing to use some extra bandwidth to transmit phase information.
But, then, I am not a propagation expert, so my comments stop here.

73,
Alberto   I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Kevin Ravenhill" <kevin.ravenhill@ukonline.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <E12xnko-0000M8-00@mserv1c.u-net.net>
Subject: LF: Definitions
Date: Fri, 2 Jun 2000 14:59:24 +0100
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> At the risk of winding everyone up, what is "machine assisted"?
> What is the difference between DSP for audio reception and DSP
> for screen reception? Or is the analogue filter a machine, or the
> receiver itself?

Hmm. I had a feeling it was a bad idea to send that last posting....

OK, so it's a matter of the language you choose. I don't want to get into
precise and pedantic definitions of what does or does not constitute a
"machine" - this was never my intention and frankly I can't see why it
should be such an issue.

All I was originally trying to convey was the difference, as I saw it,
between using the ear/brain combination to directly interpret an audio
signal (if you like, the definition of a "classic" amateur radio voice or CW
contact) as opposed to any method which involves converting the audio signal
into something which isn't audio any more, but which then allows human
interpretation which would otherwise have been very difficult or impossible.
I used "machine" for want of anything better - feel free to substitute
whatever language you're happy with.

To sum up, apologies if my postings are anything other than in perfectly
clear English and of precise technical correctness - I will try to ensure
that they are of the highest standard in future. Can we get back to the
original subject now, please?

Regards

Kevin, G1HDQ.



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'" <rsgb_lf_group@blacksheep.org>
Cc: harry@woodhou.freeserve.co.uk
Subject: LF: Decca Loading coils for sale
Date: Fri, 2 Jun 2000 16:00:28 +0100
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Harry Woodhouse G3MFW from St. Austell Cornwall wrote to me re. the
following :

He went to the Scilly Isles last month and dismantled the antenna
loading coils of the Decca station there.  Then, with the aid of
wheelbarrow and hired lorry, got them to the cargo boat for Penzance and
home in a Landrover (quote "Phew !!")

He wants to dispose of three of them and is asking £32 for each which
just covers the cost of the recovery.  They cannot be packed into crates
for sending on, so anyone who wants them will need to collect from St.
Austell.

If nothing else, they are an excellent low cost source of 729 strand
Litz wire, but are "A fatal combination of Fragile and Heavy".  Details
of similar (identical ?) coils are on Mike  G3XDV's LF Website.
Dimensions are 914mm OD x 480mm ID x 230mm thick and weigh in th eregion
of 25kg each.

I suggest if you are interested, you contact Harry direct on  01726
73608.   While he is on EMail, this is only collected once a week on
Mondays, so this would not appear to be a good method.  He does not want
to cope with the flood of EMails this reflector generates. 

Personally, I would have thought an auction might be more in order.

Andy  G4JNT


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 02 Jun 2000 19:14:43
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: Slow CW vs. BPSK etc.
In-reply-to: <003e01bfcba6$70b54200$ac1886d4@kevin>
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Hello Kevin,

I took part in some PSK31 tests (receiving only) with G3YXM and I was not
very impressed by PSK31. At levels were it gave a more or less usable copy
the signal was strong enough to be copied in normal CW.
I cannot tell you about BPSK (COHERENT/AFRICA sofware) but the statement
that it by far superior to QRSS or DFCW is hard to believe, for some sipmle
physical facts :
1. due to its nature BPSK has an advantage of 6dB over a 'normal' signal at
the same baudrate
2. the SNR (signal to noise ratio) is, regardless of what mode you are
using, dependent on the bandwidth of the signal. Reducing the bandwidth to
half will improve SNR by 3dB.

>From what I understand a baudrate of 10Hz is used for BPSK on LF (what
means a minimal bandwidth of 10Hz), so that means that it would have the
same efficieny as an other signal at 2.5Hz (what equals a dotlenght of 0.4
seconds or a speed of 3WPM).
The QRSS standard (in Europe) is a dotlength of 3 seconds (= bandwidth of
0.333Hz) and using DFCW a dotlength of 10 seconds (= 0.1Hz bandwidth) can
be used (at the same 'QSO speed'). The 'sliding technique' used by I2PHD in
his program SPECTRAN allows the use of the minimal bandwidth.
So even taking the 6dB advantage of BPSK into account QRSS / DFCW have a 9
to 14dB better SNR, because the can be copied at a much narrower bandwidth .

Please do not misunderstand me, I believe that BPSK is probably the best
mode in the WPM (words per minute) datatransfer range. But I do not think
that it can compete with modes with a MPW (minutes per word) datatransfer
that can be copied at a 30 to 100 times narrower bandwidth.

Besides that : while QRSS /DFCW can be used with a class E amp. (efficiency
close to 100%), BPSK needs a linear amp (efficiency 70%), a 1.5dB
disadvantage for BPSK.

73, Rik  ON7YD


At 09:48 1/06/00 +0100, you wrote:
>There's a lot of discussion going on at the moment on the US "LowFER"
>mailing list about the relative merits of slow CW versus BPSK (in this case
>relating to the COHERENT/AFRICA software by Bill de Carle, VE2IQ). The
>general consensus of opinion seems to be that if you are going to use
>"machine" modes, BPSK has considerable superiority over any form of slow CW
>for the kind of very weak signals often encountered on the LF bands.
>Estimates of the effective improvement range from 6dB to 23dB depending on
>what factors are taken into account!
>
>At the risk of causing some heated discussion, I'm curious to know the views
>of members of this list - particularly in relation to future transatlantic
>attempts.
>
>Also, does anyone have an idea of the relative usage of slow CW (QRSs and
>related FSK modes) versus modes like PSK31/PSK08 etc, in Europe? My
>impression is that various forms of slow CW are still favoured by most
>people (and perhaps rightly so, in terms of picking the best/most convenient
>mode for what you are trying to do), but I haven't been able to monitor the
>LF bands for some time so I don't really know what the current situation is
>like.
>
>For anyone who isn't subscribed to the abovementioned list and wishes to
>subscribe, send an email to majordomo@qth.net with no title and with
>"subscribe lowfer" in the body of the text. You'll get a return email with a
>password which has to be sent back, after which you'll be subscribed.
>
>Regards
>
>Kevin, G1HDQ
>
>
>
>
>


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Larry,
Where can we learn more about BPSK, and in particular AFRICA/COHERENT by
Bill de Carle?
John, G4CNN





_______________________________________________________
Get 100% FREE Internet Access powered by Excite
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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,
	Some comments on G3JKV's recent E-mail -

I calculated the ERP on the basis of the measured antenna current 
and estimated radiation resistance of the two antennas. Part of the 
reasoning behind this was that the antenna efficiency would not be 
an issue; the radiated power is just I squared times the radiation 
resistance, and the calculated radiation resistance is a function 
only of the antenna geometry, and not it's losses. In principle at 
least, the only result of improved efficiency due to the Decca earth 
mat would be to reduce the amount of transmitter power required to 
produce the measured value of antenna current. So antenna 
efficiency did not actually enter into the calculation of ERP, and the 
presence or absence of the Decca earth would not have affected 
the result of the calculation. 

Having said that, clearly the ERP calculations are wrong, because 
there was a significant difference in signal strength, and so by 
definition ERP, between the two antennas, where the calculations 
said they should be the same. Unfortunately, my field strength 
measuring equipment is not accurate enough to say for certain that 
this was because the small antenna was producing more ERP than 
it should, or that the Decca antenna was producing less than it 
should. However, it is probably easier to believe the former, since 
the assumptions on which the calculations are based are more 
nearly met by the Decca antenna than the small inverted L.

I don't know if this experiment has much to tell us about the 
presence or absence of horizontally polarised signals; however, 
the ferrite rod antenna I used to measure field strengths showed 
the difference in field strength of roughly 4dB observed by nearly 
everyone else, and should not have been sensitive to horizontally 
polarised signals (ie. vertical H field).

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: <7d.5af4eef.26695c95@aol.com>
Date: Fri, 2 Jun 2000 14:53:09 EDT
Subject: Re: LF: Slow CW vs. BPSK etc.
To: rsgb_lf_group@blacksheep.org
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 >There's a lot of discussion going on at the moment on the US "LowFER"
 >mailing list about the relative merits of slow CW versus BPSK 

Indeed there has been.  Some of it has gotten rather silly and occasionally a 
bit abusive, in fact.  I'm glad to see the discussion has been more civilized 
here, although there are still evident tendencies to compare apples with 
oranges and to draw too many conclusions from accepted premises.

Some of the rather extreme arguments in favor of BPSK and similar modes tend 
to count the same chickens twice; perhaps more often, for those claiming 23db 
advantages <grin>.

The most credible proponents say that, for a given bit rate, coherent methods 
have a 9db advantage.  Andy Talbot's post yesterday argues this case well.  
Six decibels are the result of the effective doubling of detected signal 
output by one state of the received signal adding in-phase and the other 
adding out of phase in the detector.  Integration of voltage over the symbol 
period accounts for the other three.  The latter effect is a direct 
consequence of coherence (one might call it the definition of coherent 
detection), and the former requires coherence to exist before it can be 
true...or for any detection to exist at all.  With coherence, a BPSK-based 
mode has a 9db advantage over on-off keying detected non-coherently, or 6db 
over coherent CW.

Does this mean, therefore, that BPSK is inherently "better" than Slow CW?  
Andy was careful to preface his comments with the qualification, "To compare 
theoretically, firstly we need to make the assumption that data rates are 
similar for the two modes."  However, there is an additional qualifier that 
follows from all this: we must also assume that coherence _can_ in fact be 
achieved and maintained over the duration of enough symbols for the message 
to be reconstructed.

If this latter condition cannot be met, then PSK-based modes have no 
advantage.  They simply don't work at all.

The traditional technique of reducing data rates and narrowing communication 
bandwidth only work for coherent methods to the extent that the path between 
the transmitter and receiver is stable enough to accomodate the slower bit 
rate.  It doesn't matter if the sender and receiver are using perfectly 
synchronized atomic clock frequency standards: if propagation effects distort 
the all-crucial phase information enough during each individual symbol, the 
symbol will not be recovered.

Hence, for a given propagation mode--and, where the ionosphere is involved, 
this is also a function of carrier frequency, path length, launch angle, 
geomagnetic conditions, and so on--there will be some _minimum_ data rate 
below which a given coherent method will not work.  Weak-signal reception 
techniques based on power integration over extremely narrow bandwidths (i.e., 
spectral analysis techniques) do not suffer nearly as strongly from the same 
effects.

Let's re-evaluate the numbers in this light.  Suppose, over a given long 
path, we find that BPSK will let us receive an acceptable percentage of a 
transmission at 10 bits per second, but faster rates are limited by noise and 
slower rates are limited by phase errors in the propagating medium.  To 
achieve the same result, we would have to slow down our on-off keying by 9db, 
to roughly one dot per second.

Now, however, let's suppose that either the noise levels increase, or we 
attempt to receive the same signal over a greater distance.  We can't slow 
the speed of the BPSK transmission any further without losing the ability to 
recover it coherently; which is to say, at all.  Yet, we can slow down the CW 
transmission and tighten the resolution of our receiving software and 
continue the exchange of information.

(This can't be done without limit, of course.  At some point, propagation 
phase shifts will spread the spectrum of the on-off carrier enough to 
disperse it across multiple channels, considering how narrow the detected 
channels have become at that point, and the analog signal-to-noise ratio will 
then rapidly collapse too.)

I don't follow the BPSK e-mail group, so this may not be the most current 
information, but as far as I am aware, the best LF DX results with BPSK over 
here have been at 100 and 200 milliseconds per bit.  Some have tried 500 and 
1000 milliseconds, but have not done as well; whereas on HF, rates of 50 
milliseconds per bit or faster seem most effective.

If 200 milliseconds per bit turns out to be the lowest practical speed for 
longwave DX, then we already know that Slow CW at 3 seconds per bit should be 
able to match its data recovery performance if the time penalty is 
acceptable.  We also know that 10 seconds per dot, or longer, is entirely 
feasible with the available receiving software.  The only thing we don't know 
is how Slow CW performs under conditions of very long paths at LF, on the 
order of 1600km or more at 5mw radiated power, for which we do have some 
experience with BPSK.

The essential point is that there are conditions below which coherent methods 
cannot work at all, but in which other (slow) weak-signal methods may provide 
at least a chance of getting signal through.  There's room for a lot of 
experimentation with these "different horses!"

73,
John  KD4IDY


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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Subject: Re: LF: Slow CW vs. BPSK etc.
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R


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 2 Jun 2000 16:08:39 +0100
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Re: Aerial tests.
References: <4.2.0.58.20000601105903.0097a890@mail.pncl.co.uk> <000301bfcc87$d6d381a0$9dd699d4@w8k3f0>
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In message <000301bfcc87$d6d381a0$9dd699d4@w8k3f0>, Dick Rollema
<d.w.rollema@freeler.nl> writes
>To All from PA0SE
>
>Walter Blanchard quoted the RACAL expert who has in the past  designed the
>Decca antennas as follows:
>
>>(...)  If the small one has an assymetric horizontal component (flat-top)
>> this will complicate matters considerably since it will radiate both
>> vertical and
>> horizontally-polarised and there will be interaction between them that
>> will affect the radiation pattern. So it would be unlikely to have a
>circular
>> polar pattern and this might account for some of the observed variations.
>
>This is not confirmed by computer simulation.
>
>Computer program AO by Brian Beezley, K6STI, shows  for the L-antenna over
>medium ground  an almost perfect omnidirectional radiation pattern. The
>deviation
>from a circle is no  more than about 0.1dB.
>
>The program also shows that the maximum of the horizontally polarised wave
>is straight up and 21.1dB down on the maximum of the vertically polarised
>wave.
>The latter maximum occurs under an angle of 12 degrees (direct + reflected
>wave).
>In the region where the inverse distance law is applicable the space in the
>vertical radiation pattern between  zero degrees and the lobe under 12
>degrees is filled by the surface wave.

And yet did not Marconi use a vertical antenna with a long horizontal
wire to obtain directivity from Cape Race? When the original aerials
came down in a gale he found equal or stronger signal strengths using an
inverted 'L' with the arm pointing the right way.

Mike
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
Message-ID: <c.5f80486.26696458@aol.com>
Date: Fri, 2 Jun 2000 15:26:16 EDT
Subject: Re: LF: Slow CW vs. BPSK etc.
To: rsgb_lf_group@blacksheep.org
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Rik posted while I was still struggling to finish typing mine.  If he had 
been a bit faster or I had been a bit slower, I could have addressed some 
part of the bandwidth issue. <g>

The necessary bandwidth of these methods may be correct as stated, but the 
actual radiated bandwidths may not be.  North American-style BPSK, a least 
that which is generated in LowFER transmitters, is not particularly 
spectrum-efficient.  It's a constant-envelope type, which means it can be 
amplified in high-efficiency stages (provided the output tuning isn't too 
sharp).  The extra sidebands are not a problem since we have 30kHz in which 
to play, and negligible radiated power to start with.  PSK31 gains its 
spectrum efficiency through envelope shaping, but that same requirement 
probably makes it a lot more susceptible to impulse noise than its 
brute-force BPSK counterpart.
 
As I mentioned in my previous message, I agree with Rik's assessment that 
narrower bandwidths with QRSS give us another window of opportunity for 
communication below signal levels where pure digital modes fall over the 
cliff edge.  The window is not limitless, because propagation-related phase 
shifts will eventually impact very narrow communication channels in the 
analog domain too.  Still, I think that window needs to be explored fully, 
and not dismissed out of hand just because it's slower or lacks digital 
purity.

73,
John


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: Fri, 2 Jun 2000 15:45:54 EDT
Subject: Re: LF: BPSK's, not all the same.
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John, G4CNN writes:
<< Where can we learn more about BPSK, and in particular AFRICA/COHERENT by
 Bill de Carle? >>

The links on the LWCA "LF Ham and Digital" page 
(lwca.org/sitepage/lfham/lfham.htm), although not always as current as I'd 
like to maintain them, are a good place to start.  There are two links in 
particular which should help:
Bill de Carle's own site  -  http://www.ietc.ca/home/bill/bbs.htm
An article by Lyle Koehler - http://www.computerpro.com/~lyle/watsbpsk.htm

73,
John


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Data: Fri, 02 Jun 2000 20:48:04 +0100
To: rsgb_lf_group@blacksheep.org
From: "M. Bruno" <spin@inrete.it>
Subject: LF: M8 solar flare now .........
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For anyone interested, an M- class (currently M8 level and rising) solar flare
is in progress now (1947z).

http://www.sec.noaa.gov/rt_plots/xray_5m.cgi

73, Marco IK1ODO



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Message-ID: <00a001bfccf0$5c740d30$0a00a8c0@server1.ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: BPSK's, not all the same.
Date: Fri, 2 Jun 2000 20:11:50 -0400
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John:

>Where can we learn more about BPSK, and in particular AFRICA/COHERENT by
>Bill de Carle?


http://www.alltel.net/~k3pgp/opening.htm

Look at this URL John and then look down for Bill Cantrell's articles about
"BPSK Adventures".

A good read and an even better eye-opener about BPSK.   Someone else gave
you the URL for the two other good items available.

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Bessel bandpass filter?
References: <E12xQYh-00044o-00@mserv1a.u-net.net>
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Thanks for reading this,

I'm doing some study on audio bandpass filters before building a
different variant of the PA0LQ stagger tuned filter.  Texts suggest that
the type of multiple feed back (MFB) op amp filter should not use a Q of
greater than about 5, for performance stability, but the PA0LQ design
has a Q of just over 30 per stage.  I'm going to try a much lower Q and
pass band width of 150 Hz or so, and also 800 Hz centre frequency.  My
thinking is that several sidebands are needed to give reasonable rates
of rise and fall times of the keyed signal, and a square wave has odd
harmonics.  I have also read the SM7CMY thesis and there is mention of a
"critical bandwidth" that seems to me to be typically around 150 Hz. 
The human brain is part of the overall aural filter.  It seems that
selected stagger tuning is the "answer" to minimising ringing in the
(electronic) filter.  I guess I will find out in due course if a 150 Hz
stagger tuned version "sounds better".

For anyone considering active filter variants, there is design
information on page 16.28 of the 1999 ARRL Handbook, for a single
stage.  For the desired application, the mulit stage stagger tuning
still needs to be somehow worked out!

But the intended thrust of this email is to ask about if anyone can find
a reference to a BESSEL BANDPASS filter.  Text books all say that the
Bessel low pass filter has the most linear phase response (best group
delay) of the basic range of filters (Butterworth, Chebyshev, elliptic,
Bessel).  But I can not find any reference to a BANDPASS variant of the
Bessel filter.  I have a feeling that it is not realisable
mathematically, and that is why it is obvious by its absence as a text
book band pass filter, but if there is a filter theory guru on the
reflector I would dearly like to hear a response.

73, Bob ZL2CA



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: WarmSpgs@aol.com
Message-ID: <3b.5b0ebd6.2669f0ef@aol.com>
Date: Sat, 3 Jun 2000 01:26:07 EDT
Subject: Re: LF: Bessel bandpass filter?
To: rsgb_lf_group@blacksheep.org
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Hi Bob,

Bessel filters do have wonderful group delay characteristics, and a bandpass 
version is entirely mathematically realisable...but not especially useful.  
The skirts of such a filter are so gentle that there is little point in using 
it for communications audio filtering unless you used many, many stages.  If 
you were to do that, however, the inevitable minor defects in the physical 
realisation would likely result in phase characteristics little better than a 
simpler Butterworth design of comparable steepness.

It is not an absolute requirement to have linear phase over the entire band 
of interest; only enough of it to allow the shape of the more-or-less square 
wave envelope to be reproduced without excessive overshoot.  (This could be 
as little as 50 Hz of the overall bandwidth for normal CW.)  We have been 
using brick-wall highpass and lowpass filters in broadcast audio paths for 
some time now, exhibiting virtually no ringing or overshoot.  This is done 
partly by incorporating active phase shift networks to compensate for the 
normal huge group delay excursions in the elliptical designs needed to 
achieve the required rolloff characteristics.  Alas, design formulae for some 
of the fancier implementations are hard to come by.

73,
John KD4IDY


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Graeme Zimmer" <gzimmer@bigpond.com>
To: rsgb_lf_group@blacksheep.org,  vernall@xtra.co.nz
References: <E12xQYh-00044o-00@mserv1a.u-net.net> <393881DE.3D9D@xtra.co.nz>
Subject: LF: Re: Bessel bandpass filter?
Date: Sat, 3 Jun 2000 15:39:15 +1000
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Hi Bob,

> But the intended thrust of this email is to ask about if anyone can find
> a reference to a BESSEL BANDPASS filter.

"Electronic Filter Design Handbook" by Williams and Taylor
has a section on "Capacitive Coupled Resonant" bandpass filters.
(These are the kind where a number of parallel tuned circuits are coupled
together via capacitors)

The book offers a table for Bessel parameters.

It does a design for "constant delay over passband" bandpass using the
Bessel tables...

Let me know if you could use a photocopy of a few pages.....

......................... Zim ............. VK3GJZ



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: LF: SV: Re: Bessel bandpass filter?
Date: Sat, 3 Jun 2000 09:30:39 +0200
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>> a reference to a BESSEL BANDPASS filter.

There's a nice software called "Filter Wiz Pro" which can be downloaded at:
http://www.schematica.com/Fil_Xfer/Transfer.htm

The unregistered version has some masked componet values in the circuit diagrams.

73
Christer
sm6pxj






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Graeme Zimmer" <gzimmer@bigpond.com>
To: rsgb_lf_group@blacksheep.org
Cc: vernall@xtra.co.nz
Subject: LF: Re: Bessel bandpass filter?
Date: Sat, 3 Jun 2000 17:46:36 +1000
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Hi Bob,

> But the intended thrust of this email is to ask about if anyone can find
> a reference to a BESSEL BANDPASS filter.

"Electronic Filter Design Handbook" by Williams and Taylor
has a section on "Capacitive Coupled Resonant" bandpass filters.
(These are the kind where a number of parallel tuned circuits are coupled
together via capacitors)

The book offers a table for Bessel parameters.

It does a design for "constant delay over passband" bandpass using the
Bessel tables...

Let me know if you could use a photocopy of a few pages.....

......................... Zim ............. VK3GJZ




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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WarmSpgs@aol.com wrote:
> 
> Hi Bob,
> 
> Bessel filters do have wonderful group delay characteristics, and a bandpass
> version is entirely mathematically realisable...but not especially useful.

I was not planning to use one.  My query was about apparent lack of a
band pass version being mentioned in text books.

> The skirts of such a filter are so gentle that there is little point in using
> it for communications audio filtering unless you used many, many stages.  If
> you were to do that, however, the inevitable minor defects in the physical
> realisation would likely result in phase characteristics little better than a
> simpler Butterworth design of comparable steepness.

Yes.  It seems the stagger tuned Butterworth is the design to go for.
 
> It is not an absolute requirement to have linear phase over the entire band
> of interest; only enough of it to allow the shape of the more-or-less square
> wave envelope to be reproduced without excessive overshoot.  (This could be
> as little as 50 Hz of the overall bandwidth for normal CW.)  We have been
> using brick-wall highpass and lowpass filters in broadcast audio paths for
> some time now, exhibiting virtually no ringing or overshoot.  This is done
> partly by incorporating active phase shift networks to compensate for the
> normal huge group delay excursions in the elliptical designs needed to
> achieve the required rolloff characteristics.  Alas, design formulae for some
> of the fancier implementations are hard to come by.
> 
> 73,
> John KD4IDY

What I am not sure of is how to stagger the stages of bandpass active
filters.  However, they can easily be tweaked, and applying "input
beeping" and using a scope to minimise ringing in the output seems to be
a good experimental way of adjusting it for the desired characteristic.

Thanks for the comments.

Bob ZL2CA




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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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: SV: Re: Bessel bandpass filter?
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C Andersson wrote:
> 
> >> a reference to a BESSEL BANDPASS filter.
> 
> There's a nice software called "Filter Wiz Pro" which can be downloaded at:
> http://www.schematica.com/Fil_Xfer/Transfer.htm
> 
> The unregistered version has some masked componet values in the circuit diagrams.
> 
> 73
> Christer
> sm6pxj

Thanks for the URL info.  I will check it out.

Bob ZL2CA



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 03 Jun 2000 11:20:23 -0500
Subject: LF: FilterCAD
From: "Mitch Powell" <PowellM@claven.fanshawec.on.ca>
To: vernall@xtra.co.nz
Cc: rsgb_lf_group@blacksheep.org
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<HTML>
<HEAD>
<TITLE>FilterCAD</TITLE>
</HEAD>
<BODY BGCOLOR="#FFFFFF">
<TT>Bob:<BR>
Try the following site - for filter design - I believe you can enter the parameters, and the filter is designed on the spot.<BR>
<BR>
FILTERCAD WEB SITE INFO<BR>
<BR>
www.linear.com/apps/download.html &nbsp;&nbsp;&nbsp;- &nbsp;download information<BR>
<BR>
www.linear.com/apps/ &nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;- &nbsp;&nbsp;lots of application notes<BR>
<BR>
www.linear.com/source_html/form_sent_software.html&nbsp;&nbsp;&nbsp; - the actual download site<BR>
<BR>
73<BR>
Mitch &nbsp;&nbsp;&nbsp;&nbsp;VE3OT</TT>
</BODY>
</HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: communications systems
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Having read and studied many messages lately about various modes and
advantages of one over another. BPSK, PSK31, SLOW CW, NORMAL CW etc
My conclusion like I have always stated is that NORMAL CW or SLOW CW is
more suitable on LF for what we are trying to achieve, especially long
distance dx, and short exchanges of information like callsigna and RST.
If one wants to shift large volumes of traffic then use data modes and
suitable frequencies like vhf/uhf and satellites, where noise is mimimal
and phase distortion due to propagation anomalies is also mimimal.
Propagation conditions on LF with all the environmental noise and high
static levels that most users of the band complain about plus low
transmitter power of a max of 1w is more suited to the use of
CW where a mimimum of fuss and equipment is required. The operators
ideally should be fully competent and experienced in CW.

On the question of machine v manual modes.
If one uses a computer to visually read slow cw that cannot be heard
aurally then it must be a machine function system, otherwise the message
or qso could not be conducted.
In most cases the very slow cw that I have seen on a screen can be read
directly from the speaker and in this case is not considered a machine
system. If one is totally dependent on a machine to send and receive
very slow cw then it must be considered a machine system.
The machine/computer with suitable software is converting the audio into
a visual format, and with FFT,  processing the signal. If automated
sending is used, again this is a machine generated system.
The operator participation using a computer for sending/receiving very
slow cw is no different to sending/receiving PSK31.
You must read the screen in both cases to get the message and you must
type the message information to send it.
Another factor to consider. Very slow morse generated/received by a
computer does not require the operator to know the morse code. The
message is typed to be sent and instead of reading the received dots and
dashes on the screen, existing software can be modified to print out the
message.
A couple of professional cw operators one at each end of the proposed
transatlantic link will achieve the object. There is no need for
synchronised atomic clocks and bandwidths of 0.00000000007hz
Keep it simple and all can enjoy and verify it.
If someone using the new Hydrogen/Stentlesch clock and a b/w of
0.0000000000000000000007 hz told us that they had made the first qso
across the atlantic on 136 khz, how would the rest of us  know if they
were telling the truth. Would they qualify for any awards?????
73 de G3KEV








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: MODES AND ANTENNAS
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There is such a diverse opinion about antennas both little and large and
modes one versus the other that the best course of action is for each
individual to build and use what they think is best for them.
There is an abundance of theoritical discussion going on that bears no
relationship to REALITY.
Too many assumptions, and too wide of the mark when one tries to
implement them.
The real proof of success will be judged by listening on LF to signals
being emitted from the various sources. Those doing the job properly
will be obvious from the strength of the signals received.
Data modes would not fair very well today with static crashes S9 plus
40, but I could manage a short exchange of RST and callsign on CW
without difficulty.
73 de G3KEV





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "'Geri' Kinzel, DK8KW" <DK8KW@compuserve.com>
Subject: LF: MODES AND ANTENNAS
To: rsgb_lf_group@blacksheep.org
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G3KEV wrote:

>There is such a diverse opinion about antennas both little and large and
>modes one versus the other that the best course of action is for each
>individual to build and use what they think is best for them.<

Mal, 

I do not always agree with what you say, but here I fully agree. May the
people using small antennas be happy with their system and the people who
have the ability to erect large antenna arrays use those. Same is true for
the most suitable mode. I like to conduct experiments to see what is
suitable to me, sometimes it depends on my mood. I have the ability to
cross the channel (not the Atlantic, yet), but I have just build a QRP LF
transmitter and was happy that Wil in PA was able to copy me. So thats what
counts: have fun and try what you think is best suitable for what you want
to reach.

May your god be with you!

Best 73 

Geri, DK8KW (W1KW)

P.S.: I was a keen 50 MHz operator until the band became too crowded ...
too easy to work into the states or other dx ... will be back when sunspots
disappear ... more fun! 


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: <22021.200005301550@gemini>
Subject: LF: Re: Big & Small antennas - Reply to comments
Date: Sat, 3 Jun 2000 19:24:44 +0100
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----- Original Message -----
From: James Moritz <j.r.moritz@herts.ac.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Tuesday, May 30, 2000 5:57 PM
Subject: LF: Big & Small antennas - Reply to comments


> Possible Causes:
>
> My money is on the increased field strengths being due to fields
> and currents under the ground surface, resulting in greater
> effective height of the antenna. Obviously, this needs more
> investigation, which I hope to try later. By the way, have any of the
> cave radio community made underground field strength
> measurements?

Yes, we have. There is a piece on earth electrode based cave radio
experiments in issue 40 of the Cave Radio & Electronics Group Journal (ISSN
1361-4800). See also http://www.mcrosolv.demon.co.uk/caves.org/radio/ to
search for articles using David Gibson's on-line digest.

73 de
John Rabson G3PAI








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 03 Jun 2000 19:32:13 +0100
To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: Re: LF: Re: Aerial tests.
In-reply-to: <000301bfcc87$d6d381a0$9dd699d4@w8k3f0>
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At 13:41 02/06/00 +0200, you wrote:
>To All from PA0SE
>
>Walter Blanchard quoted the RACAL expert who has in the past  designed the
>Decca antennas as follows:
>
> >(...)  If the small one has an assymetric horizontal component (flat-top)
> > this will complicate matters considerably since it will radiate both
> > vertical and
> > horizontally-polarised and there will be interaction between them that
> > will affect the radiation pattern. So it would be unlikely to have a
>circular
> > polar pattern and this might account for some of the observed variations.
>
>This is not confirmed by computer simulation.
>
>Computer program AO by Brian Beezley, K6STI, shows  for the L-antenna over
>medium ground  an almost perfect omnidirectional radiation pattern. The
>deviation
>from a circle is no  more than about 0.1dB.
>
>The program also shows that the maximum of the horizontally polarised wave
>is straight up and 21.1dB down on the maximum of the vertically polarised
>wave.
>The latter maximum occurs under an angle of 12 degrees (direct + reflected
>wave).
>In the region where the inverse distance law is applicable the space in the
>vertical radiation pattern between  zero degrees and the lobe under 12
>degrees is filled by the surface wave.

Dick,

I haven't got AO so could you see what it says about the following:

An inverted-L half-wave resonant at 1950 kHz, vertical section  25m high,
horizontal  55m long.  What does it predict the VERTICALLY-POLARISED
horizontal polar pattern to be ?
I know the answer, because I've measured it, I just want to know what
your AO says!

Walter G3JKV.




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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Mitch Powell wrote:
> 
> Bob:
> Try the following site - for filter design - I believe you can enter
> the parameters, and the filter is designed on the spot.
> 
> FILTERCAD WEB SITE INFO
> 
> www.linear.com/apps/download.html    -  download information
> 
> www.linear.com/apps/         -   lots of application notes
> 
> www.linear.com/source_html/form_sent_software.html    - the actual
> download site
> 
> 73
> Mitch     VE3OT

Thanks Mitch, I will check that out as well.

73, Bob




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Re: Bessel bandpass filter?
References: <001401bfcd2f$d96512a0$095b868b@zimslaptop>
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Graeme Zimmer wrote:
> 
> Hi Bob,
> 
> > But the intended thrust of this email is to ask about if anyone can find
> > a reference to a BESSEL BANDPASS filter.
> 
> "Electronic Filter Design Handbook" by Williams and Taylor
> has a section on "Capacitive Coupled Resonant" bandpass filters.
> (These are the kind where a number of parallel tuned circuits are coupled
> together via capacitors)
> 
> The book offers a table for Bessel parameters.
> 
> It does a design for "constant delay over passband" bandpass using the
> Bessel tables...
> 
> Let me know if you could use a photocopy of a few pages.....
> 
> ......................... Zim ............. VK3GJZ

My first reply was direct to Zim, but I should also acknowledge it to
reflector reader:

I would like a copy, thanks for the offer Zim.

I'm intending to build an active filter equivalent, where each stage is
practically independent of others, which is different to the mutually
coupled passive filter, but the design info would be interesting in its
own right.

73, Bob




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 3 Jun 2000 18:46:18 EDT
Subject: LF: GPS Frequency reference.
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I've been looking for a high stability source to act as a timebase for a 
frequency counter and for a PLL reference.

I notice that the older Magellan GPS300 is available at $ 99.

Does anyone know if:

1)  The GPS300 has a 1Hz pulse output. (Or any other sensible frequency with 
high accuracy)

2)   It can display Maidenhead locators.

73

David  G0MRF


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Subject: LF: Kits and Bits
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With apologies to the group.

a) Glenn W7GS.     
Unable to reply to your enquiry via your hotmail address. Messages are 
bounced.


Help /qsp pse.

David  G0MRF


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: FilterCAD
Date: Sun, 4 Jun 2000 19:32:55 +1200
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----- Original Message -----
From: vernall <vernall@xtra.co.nz>
To: <rsgb_lf_group@blacksheep.org>
Sent: Sunday, June 04, 2000 8:46 AM
Subject: Re: LF: FilterCAD

I downloaded the 'full catastrophe' from the LTC (Linear Technology) site
some time back but it's on the pc at work. Output of the filter design pgm
is in terms of varoius LTC op amps etc but useful if you want to get an
appreciation of what may be needed to achieve a given spec. Can't recall the
options available but I dare say yu will have a peek anyway! The
handbook(downloadable too) for use with the software is quite interesting as
well.
73
Dave, ZL3FJ



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andy Talbot" <drassew2@interalpha.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: GPS Frequency reference.
Date: Sun, 4 Jun 2000 09:25:58 +0100
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I have the Magellan Trailblazer, oldish GPS handheld circa 1994.   There are
no 1s pulses anywhere to be found on it, and the unit only displays NGR,
Lat/Long or UTM.

Look at the TAPR website for their deals on Garmin GPS25 and other boards.
It is much faster locking up than the old Magellan and has 1s pulses

Andy  G4JNT


-----Original Message-----
From: G0MRF@aol.com <G0MRF@aol.com>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 04 June 2000 00:20
Subject: LF: GPS Frequency reference.


>I've been looking for a high stability source to act as a timebase for a
>frequency counter and for a PLL reference.
>
>I notice that the older Magellan GPS300 is available at $ 99.
>
>Does anyone know if:
>
>1)  The GPS300 has a 1Hz pulse output. (Or any other sensible frequency
with
>high accuracy)
>
>2)   It can display Maidenhead locators.
>
>73
>
>David  G0MRF
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sun, 04 Jun 2000 10:01:28 +0100
To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: Re: LF: GPS Frequency reference.
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David,

Your query:

>I've been looking for a high stability source to act as a timebase for a
>frequency counter and for a PLL reference.
>
>I notice that the older Magellan GPS300 is available at $ 99.
>
>Does anyone know if:
>
>1)  The GPS300 has a 1Hz pulse output. (Or any other sensible frequency with
>high accuracy)
>
>2)   It can display Maidenhead locators.

I haven't been following this thread so not sure what you
actually want these for, but a word of warning.
These cheapo GPS's either (a) will not have any outputs,
or (b) timing-wise they won't be worth a damn if you
want any real accuracy.
They use the cheapest VXO they can and depend on the
software to hold time so it's very jittery.
Are you looking for accurate relative time or accurate absolute
time? - there's a big difference.
Why don't you use MSF?  It's very easy to filter out
the 60 kHz carrier and divide down to whatever you want -
even I can do it!  And it's based on one of the frequency
standards that USNO uses for GPS.
You could always buy an MSF clock module from Maplin for
a few quid and dig into it to pull out what you want.
Have a word with Dr John Laverty at NPL - he supplies the
controlling timing reference for MSF and is happy to talk
to anyone about time and timing references.

Walter G3JKV.






Walter G3JKV.



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
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Subject: Re: LF: Re: Aerial tests.
Date: Sun, 4 Jun 2000 11:48:43 +0200
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To All from PA0SE

In an earlier e-mail I wrote:

> >Computer program AO by Brian Beezley, K6STI, shows  for the L-antenna
over
> >medium ground  an almost perfect omnidirectional radiation pattern. The
> >deviation
> >from a circle is no  more than about 0.1dB.

Mike Powell commented:

> And yet did not Marconi use a vertical antenna with a long horizontal
> wire to obtain directivity from Cape Race? When the original aerials
> came down in a gale he found equal or stronger signal strengths using an
> inverted 'L' with the arm pointing the right way.

Mike,

It depends on the length of the horizontal part af the antenna.

Jim used only 42m.

When the top is increased to 0.1 wavelength than a F/B-ratio of 2.23dB
results.

With a top of 0.25 wavelength F/B becomes 3.51dB.


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>
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Subject: Re: LF: Re: Aerial tests.
Date: Sun, 4 Jun 2000 12:57:58 +0200
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G3JKC wrote:

> Dick,

>
> I haven't got AO so could you see what it says about the following:
>
> An inverted-L half-wave resonant at 1950 kHz, vertical section  25m high,
> horizontal  55m long.  What does it predict the VERTICALLY-POLARISED
> horizontal polar pattern to be ?
> I know the answer, because I've measured it, I just want to know what
> your AO says!
>
> Walter G3JKV.


Walter,

I will send you the patterns (vertical polarisation, horizontal and vertical
pattern) as attachments to a direct e-mail because the reflector does not
accept these.

73, Dick, PA0SE



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Photons again...
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If verified, an interesting development,
Andre' N4ICK

>  http://www.sunday-times.co.uk/news/pages/sti/2000/06/04/stifgnusa01007.html



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Having read and studied many messages lately about various modes and
advantages of one over another. BPSK, PSK31, SLOW CW, NORMAL CW etc
My conclusion like I have always stated is that NORMAL CW or SLOW CW is
more suitable on LF for what we are trying to achieve, especially long
distance dx, and short exchanges of information like callsigna and RST.
If one wants to shift large volumes of traffic then use digital/data
modes and
suitable frequencies like vhf/uhf and satellites, where noise is mimimal
and phase distortion due to propagation anomalies is also mimimal.
Propagation conditions on LF with all the environmental noise and high
static levels that most users of the band complain about plus low
transmitter power of a max of 1w is more suited to the use of
CW where a mimimum of fuss and equipment is required. The operators
ideally should be fully competent and experienced in CW.

On the question of machine v manual modes.
If one uses a computer to visually read slow cw that cannot be heard
aurally then it must be a machine function system, otherwise the message
or qso could not be conducted.
In most cases the very slow cw that I have seen on a screen can be read
directly from the speaker and in this case is not considered a machine
system. If one is totally dependent on a machine to send and receive
very slow cw then it must be considered a machine system.
The machine/computer with suitable software is converting the audio into
a visual format, and with FFT,  processing the signal. If automated
sending is used, again this is a machine generated system.
The operator participation using a computer for sending/receiving very
slow cw is no different to sending/receiving PSK31.
You must read the screen in both cases to get the message and you must
type the message information to send it.
Another factor to consider. Very slow morse generated/received by a
computer does not require the operator to know the morse code. The
message is typed to be sent and instead of reading the received dots and
dashes on the screen, existing software can be modified to print out the
message.
A couple of professional cw operators one at each end of the proposed
transatlantic link will achieve the object. There is no need for
synchronised atomic clocks and bandwidths of 0.00000000007hz
Keep it simple and all can enjoy and verify it.
If someone using the new Hydrogen/Stentlesch clock and a b/w of
0.0000000000000000000007 hz told us that they had made the first qso
across the atlantic on 136 khz, how would the rest of us  know if they
were telling the truth. Would they qualify for any awards?????
73 de G3KEV




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James Moritz wrote:

> Dear LF Group,
>         Some comments on G3JKV's recent E-mail -
>
> I calculated the ERP on the basis of the measured antenna current
> and estimated radiation resistance of the two antennas. Part of the
> reasoning behind this was that the antenna efficiency would not be
> an issue; the radiated power is just I squared times the radiation
> resistance, and the calculated radiation resistance is a function
> only of the antenna geometry, and not it's losses. In principle at
> least, the only result of improved efficiency due to the Decca earth
> mat would be to reduce the amount of transmitter power required to
> produce the measured value of antenna current. So antenna
> efficiency did not actually enter into the calculation of ERP, and the
> presence or absence of the Decca earth would not have affected
> the result of the calculation.
>
> Having said that, clearly the ERP calculations are wrong because

> there was a significant difference in signal strength, and so by
> definition ERP, between the two antennas, where the calculations
> said they should be the same.

Unfortunately this makes the whole comparison tests between the small inv
L and the large vertical
FLAWED. Next time compare the large vertical against a small 9 metre
vertical without any horizontal wires. Resonate each vertical in turn and
check the reports. I will put my money on the large vertical.
G3KEV

> Unfortunately, my field strength
> measuring equipment is not accurate enough to say for certain that
> this was because the small antenna was producing more ERP than
> it should, or that the Decca antenna was producing less than it
> should. However, it is probably easier to believe the former, since
> the assumptions on which the calculations are based are more
> nearly met by the Decca antenna than the small inverted L.
>
> I don't know if this experiment has much to tell us about the
> presence or absence of horizontally polarised signals; however,
> the ferrite rod antenna I used to measure field strengths showed
> the difference in field strength of roughly 4dB observed by nearly
> everyone else, and should not have been sensitive to horizontally
> polarised signals (ie. vertical H field).
>
> Cheers, Jim Moritz
> 73 de M0BMU




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Date: Sun, 4 Jun 2000 13:43:08 +0100
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Re: Aerial tests.
References: <4.2.0.58.20000601105903.0097a890@mail.pncl.co.uk> <000301bfcc87$d6d381a0$9dd699d4@w8k3f0> <OpcBAIA338N5EwXR@pickmere.demon.co.uk> <003701bfce1a$2a24f580$93fb88d4@w8k3f0>
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In message <003701bfce1a$2a24f580$93fb88d4@w8k3f0>, Dick Rollema
<d.w.rollema@freeler.nl> writes
>To All from PA0SE
>
>In an earlier e-mail I wrote:
>
>> >Computer program AO by Brian Beezley, K6STI, shows  for the L-antenna
>over
>> >medium ground  an almost perfect omnidirectional radiation pattern. The
>> >deviation
>> >from a circle is no  more than about 0.1dB.
>
>Mike Powell commented:
>
>> And yet did not Marconi use a vertical antenna with a long horizontal
>> wire to obtain directivity from Cape Race? When the original aerials
>> came down in a gale he found equal or stronger signal strengths using an
>> inverted 'L' with the arm pointing the right way.
>
>Mike,
>
>It depends on the length of the horizontal part af the antenna.
>
>Jim used only 42m.
>
>When the top is increased to 0.1 wavelength than a F/B-ratio of 2.23dB
>results.
>
>With a top of 0.25 wavelength F/B becomes 3.51dB.

Thanks, Dick

Considering the poor receivers in use at the time and the ratio of
vertical to horizontal (1:1?) I would have expected a bigger
improvement.

Mike 
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andy Talbot" <drassew2@interalpha.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: GPS Frequency reference.
Date: Sun, 4 Jun 2000 20:35:28 +0100
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One PPS output on the Garmin GPS25 is specified at 1us accuracy.  This ought
to be adequate if the PLL has a long enough time constant.  I use mine to
drive the B input of a counter timer and using teh A/B * 10^n functionm can
get gating times of 10000s

Have a look at the Brooks Sheera GPS Disiplined frequency standard in QST
last year or the year before sometime.  I've got a copy somwhere if you're
stuck

Andy  G4JNT


-----Original Message-----
From: Walter Blanchard <blanch@pncl.co.uk>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 04 June 2000 10:37
Subject: Re: LF: GPS Frequency reference.


>David,
>
>Your query:
>
>>I've been looking for a high stability source to act as a timebase for a
>>frequency counter and for a PLL reference.
>>
>>I notice that the older Magellan GPS300 is available at $ 99.
>>
>>Does anyone know if:
>>
>>1)  The GPS300 has a 1Hz pulse output. (Or any other sensible frequency
with
>>high accuracy)
>>
>>2)   It can display Maidenhead locators.
>
>I haven't been following this thread so not sure what you
>actually want these for, but a word of warning.
>These cheapo GPS's either (a) will not have any outputs,
>or (b) timing-wise they won't be worth a damn if you
>want any real accuracy.
>They use the cheapest VXO they can and depend on the
>software to hold time so it's very jittery.
>Are you looking for accurate relative time or accurate absolute
>time? - there's a big difference.
>Why don't you use MSF?  It's very easy to filter out
>the 60 kHz carrier and divide down to whatever you want -
>even I can do it!  And it's based on one of the frequency
>standards that USNO uses for GPS.
>You could always buy an MSF clock module from Maplin for
>a few quid and dig into it to pull out what you want.
>Have a word with Dr John Laverty at NPL - he supplies the
>controlling timing reference for MSF and is happy to talk
>to anyone about time and timing references.
>
>Walter G3JKV.
>
>
>
>
>
>
>Walter G3JKV.
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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g3kev wrote:
snip
> If someone using the new Hydrogen/Stentlesch clock and a b/w of
> 0.0000000000000000000007 hz told us that they had made the first qso
> across the atlantic on 136 khz, how would the rest of us  know if they
> were telling the truth. Would they qualify for any awards?????
> 73 de G3KEV

Sounds to me to be a sour grapes comment from a "CW for ever" believer? 
The stations of such a QSO would of course have their self-reward for
the achievement, even if there is a level of keeping high tech at arms
length from others.  The amateur is progressive?

Bob ZL2CA




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Sorry no Dx Cluster spots from GB7DXM
Date: Sun, 4 Jun 2000 23:20:20 +0100
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Hi all, I am sorry to say that the local DX Cluster crashed late last week
and there are no entries on it for LF.
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: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
Subject: LF: a really weak signal in Canada....
Date: Sun, 4 Jun 2000 20:06:39 -0400
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Greetings:

Bill de Carle has aggressively gone after my ultra weak signal on 137.710
and managed to copy it.  He sent the following email to the LowFer
reflector, I am resending it here for those who might be interested.  With
the antenna finally up here I am working on the test set so I can tune up
the antenna.  The signal is QRS CW at the speed of .4 WPM.

Quote
I don't know if this has been tried before, but I just tried it and it
worked nicely.

The general idea is to record an ultra-slow CW signal, then to play it
back speeded up so the human operator can copy the CW message by ear
at normal speed.  Ham operators have years of experience trying to dig
weak CW signals out of the noise - by ear - not by looking at a picture
on a computer monitor.

I used VA3LK's ultra-weak test signal.
Using FFTZZ, I knew the signal was being received at 803 Hz - after some
minutes of integration, the spectral line came up out of the noise, so I
knew beforehand what the exact frequency was.  Unfortunately the signal
was way too weak to be able to decode by any spectral display technique
available to me, so I hit upon the idea of time-compression.

I recorded some 578 seconds of audio to hard disk at 7200 samples per sec.
Then I post-processed that file as follows:

1.  Run it through a narrow bandpass filter centered on 803 Hz.

2.  Multiply the resulting data with a sinewave at 825.4 Hz - that
    acts like a mixer producing sum and difference frequencies at
    1628.4 and 22.4 Hz respectively.

3.  Run that waveform through a 32-point FIR lowpass filter to keep
    only the 22.4 Hz component.

4.  Keep only 1 resulting filtered sample out of 32 - essentially
    compressing the total recording time by a factor of 32.

5.  Make it into a .wav file specified as sampled at 8000 s/s and
    lasting 16.25 seconds.

When I played the 16.25 second wav file back I could actually hear the
CW at a reasonable speed (about 35.5 times faster than it was transmitted)
and at a reasonable tone (about 800 Hz).  The ident was easily recognized.

It worked on first try.  I will now optimize the filter coefficients and
write a single program to go directly from digitized samples on disk at
7200 s/s to a .wav file time-compressed at 8000 s/s.

Anybody else tried this?

Bill VE2IQ

Unquote

I have the .WAV file and will send to anyone who asks.

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
Date: Sun, 4 Jun 2000 21:27:20 -0400
Subject: Re: LF: a really weak signal in Canada....
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Hi Larry

when you get a list together include it to me 

a really novel idea

Bob

I have the .WAV file and will send to anyone who asks.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: LF: Signal Strength Measurements by OH2LX, 05 June 2000
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Signal strength measurements of various LF stations by OH2LX:
------------------------------------------------------------------
Day ------------------   29May 30May 31May 01Jun 02Jun 03Jun 04Jun
                          MON   TUE   WED   THU   FRI   SAT   SUN 
Time, UTC ------------    2040- 2020- 2030- 2035- 2035- 2040- 2030-
------------------------------------------------------------------
kHz    Stn   d,km  AZI          Indicated ESH2 input, dBmW
------------------------------------------------------------------
 68.9 DHJ58? 1115, 242    -99  -105  -101  -102   -99  -101  -103
------------------------------------------------------------------
 73.3 Rugby, 1825, 252,  -107  -107  -105  -106  -104  -104  -106
------------------------------------------------------------------
 75.0   HBG, 1992, 226,  -104  -103  -107  -104  -103  -102  -106
------------------------------------------------------------------
 77.5 DCF77, 1543, 228,   -89   -90   -92   -89   -87   -87   -92
------------------------------------------------------------------
128.9 DCF49, 1544, 228,   -95   -93   -89   -91   -87   -92   -96
------------------------------------------------------------------
138.8 DBF39, 1221, 226,   -85   -85   -85   -85   -83   -96   -85
------------------------------------------------------------------
135.8   SXV, 2490, 182,  -103  -112  -104  -106  -116  -106  -107*
------------------------------------------------------------------
137.0   CFH, 5750, 295,   Nil   Nil   Nil   Nil   Nil   Nil   Nil
------------------------------------------------------------------
* One deep minimum observed practically every evening (fade)
------------------------------------------------------------------
03June 1932 OH1TN -112; 1946:-112; 1953:-112; 2000:-112  (clg CQ)
             2006:-111; 2013:-111; 2040:-112; 2045:-112; 2106:-112
------------------------------------------------------------------
(R&S ESH2/---- 10m coax----/1:10/-----15m wire-----):
 Noise level with antenna: with 200Hz IF BandWidth: 
-24..-20 dB(uV), -131..-127dBmW (varies with frq, qrm, qrn etc)
------------------------------------------------------------------
End of message of 05th June 2000, 0700 UTC, from OH2LX
----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: a really weak signal in Canada....
Date: Mon, 5 Jun 2000 09:27:35 +0100
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>From VE2IQ
>It worked on first try.  I will now optimize the filter coefficients
and
>write a single program to go directly from digitized samples on disk at
>7200 s/s to a .wav file time-compressed at 8000 s/s.

>Anybody else tried this?

Yes- 

It was a bit of fun after my 393km 73kHz contact with G3PLX in 1997
using 50 second dot CW.  Peter recorded my signals in I/Q format after
mixing down to zero IF at a sampling rate of  6.25 Hz, then sent me the
raw data file.   I treated this as if it were sampled at a much higher
rate - trivial in DSP by just pretending it is at a higher rate -
effectively multiplying the signalling by 1000 times.  Then upconverted
to audio by multiplying the I/Q pairs by SIN / COS samples of a tone of
800 Hz.  The resulting samples were then stored in a .WAV file which
could be played back conventionally.

50s dots became 50ms which was about 24 WPM (which 'JNT could copy coz
he knew what was being sent).   A signal comfortably visible on the
screen (10 - 15dB S/N in 0.05 Hz bandwidth) became a conventional CW
signal easy to copy - with the same S/N effectively in 50Hz bandwidth.
Incidently, there was no ringing on this in spite of the narrow filter
due to the ability to perfectly optimise DSP filtering.

When we tried with weaker signals, it was interesting, but probably not
surprising that a signal that became difficult to see also became
difficult to hear.  To my mind, and memory of three years ago, the
results for audio and visual were very similar.

Doing the same rate conversion on an early evening to late morning
3.5MHz Dopplergram recording, (see G3PLX's article in RadCom a couple of
years ago), resulted in the most wonderful 'whale' like whistling and
tones as the ionosphere shifted the signal up and down and introduced
extra components.  Another in the 'natural sounds' series -  wonder if a
recording company would be interested ?

Andy  G4JNT

> Quote
> I don't know if this has been tried before, but I just tried it and it
> worked nicely.
> 
> The general idea is to record an ultra-slow CW signal, then to play it
> back speeded up so the human operator can copy the CW message by ear
> at normal speed.  Ham operators have years of experience trying to dig
> weak CW signals out of the noise - by ear - not by looking at a
> picture
> on a computer monitor.
> 
> I used VA3LK's ultra-weak test signal.
> Using FFTZZ, I knew the signal was being received at 803 Hz - after
> some
> minutes of integration, the spectral line came up out of the noise, so
> I
> knew beforehand what the exact frequency was.  Unfortunately the
> signal
> was way too weak to be able to decode by any spectral display
> technique
> available to me, so I hit upon the idea of time-compression.
> 
> I recorded some 578 seconds of audio to hard disk at 7200 samples per
> sec.
> Then I post-processed that file as follows:
> 
> 1.  Run it through a narrow bandpass filter centered on 803 Hz.
> 
> 2.  Multiply the resulting data with a sinewave at 825.4 Hz - that
>     acts like a mixer producing sum and difference frequencies at
>     1628.4 and 22.4 Hz respectively.
> 
> 3.  Run that waveform through a 32-point FIR lowpass filter to keep
>     only the 22.4 Hz component.
> 
> 4.  Keep only 1 resulting filtered sample out of 32 - essentially
>     compressing the total recording time by a factor of 32.
> 
> 5.  Make it into a .wav file specified as sampled at 8000 s/s and
>     lasting 16.25 seconds.
> 
> When I played the 16.25 second wav file back I could actually hear the
> CW at a reasonable speed (about 35.5 times faster than it was
> transmitted)
> and at a reasonable tone (about 800 Hz).  The ident was easily
> recognized.
> 
> It worked on first try.  I will now optimize the filter coefficients
> and
> write a single program to go directly from digitized samples on disk
> at
> 7200 s/s to a .wav file time-compressed at 8000 s/s.
> 
> Anybody else tried this?
> 
> Bill VE2IQ
> 
> Unquote
> 
> I have the .WAV file and will send to anyone who asks.
> 
> Larry
> VA3LK
> 
> 
> 
> 


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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: Re: LF: a really weak signal in Canada....
References: <003201bfce81$f1a552f0$0a00a8c0@server1.ThreeLakes.ca>
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Larry Kayser wrote:

> Greetings:
>
> Quote
> I don't know if this has been tried before, but I just tried it and it
> worked nicely.
> [snip]
> I recorded some 578 seconds of audio to hard disk at 7200 samples per sec.
> [snip]

Seems really a good idea, which could attract also the
die-hard CW-must-be-copied-by-ears crop around.

Just one simple question : why 7200 samples/sec ? It is not a standard
sound card sampling rate. Is there a specific reason for this sampling speed ?
Perhaps Bill was using an external A/D converter. For the technique to
become widespread and accepted by many (all), it shouldn't rely on an
ad-hoc hardware. Modern sound cards have superb A/D converters,
so why not use them ?

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>
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Subject: Re: LF: Bessel bandpass filter?
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Dear LF Group,

ZL2CA wrote: 
> But the intended thrust of this email is to ask about if anyone can find a
> reference to a BESSEL BANDPASS filter.  Text books all say that the Bessel
> low pass filter has the most linear phase response (best group delay) of
> the basic range of filters (Butterworth, Chebyshev, elliptic, Bessel). 
> But I can not find any reference to a BANDPASS variant of the Bessel
> filter.  I have a feeling that it is not realisable mathematically, and
> that is why it is obvious by its absence as a text book band pass filter,
> but if there is a filter theory guru on the reflector I would dearly like
> to hear a response.

Not sure if I could be called a 'filter guru', but I have a fair bit of 
experience designing filters. It is a huge area, and difficult to 
scratch the surface, but here are some useful bits of info:

You won't find tables of Bessel or other bandpass filter values very 
often - this is because the standard filter design procedure starts 
with a normalised low pass design (ie. designed for 1ohm source & 
load, 1rad/s cut off frequency) and transforms it into whatever low- 
high-, bandpass, or bandstop filter you desire. So the Bessel low 
pass tables are where you need to start to design a Bessel 
bandpass filter. For passive LC filters, these are usually given as a 
table of L and C values, but active filter designs usually start from 
the tables of pole locations (these effectively specify the cut off 
frequency and Q of each section of the filter).

The reason for doing this is that the possible permutations of 
bandwidths and centre frequencies are more or less infinite, so 
tabulating all the values would be impossible.

An alternative is the 'coupled resonator' approach, which is 
normally reserved for passive bandpass filters with bandwidths 
less than 5 or 10% of the centre frequency. This uses tables of k 
and q values for different types of filter response.

As to how to do it, the A.B. Williams / F.J. Taylor 'Electronic filter design 
handbook' is excellent for passive LC and active designs, and includes 
many worked examples and formulas for different types of circuit suitable 
for different applications. Later editions have a section on digital filters too. 
The bible for passive designs including crystal filters is A.I. Zverev's 
'Handbook of filter synthesis'. These are the two references I have used most, 
but there are others too.

As to different types of filter response, there is always 
compromise. Filters with sharp cut-off always have poor transient 
response, those with good transient response have lousy skirt 
selectivity. So Chebyshev and eliptic filters have lots of ringing and 
overshoot, but good selectivity, while Bessel, Gaussian, linear 
phase etc. have little ringing and overshoot, but poor selectivity. 
Increasing the number of poles (in a bandpass filter the number of 
resonators) will improve the selectivity / transient response trade-
off, but require higher Q for each element, and greater precision in 
component values, and have higher insertion losses.

There are also many compromise filter responses, which have both 
reasonable transient response and selectivity. These include the 
Butterworth, and various 'transitional' responses. I have had good 
results with 100 and 250Hz, 5 pole CW filters using a 'transitional 
Gaussian to -6dB' response; this has a rounded response like a 
Bessel filter until it falls of by 6dB, when the skirts get steeper like 
a Chebyshev filter. I was impressed by the 'crispness' of CW 
through these filters.

In general, any passive filter design can also be implemented using 
an active filter and vice versa. Passive filters have lower 
component count and better dynamic range, and work better at 
high frequencies. Active filters do not require inductors, and are 
better suited to very narrow band filters where very high Q is 
required. It seems to be difficult to design a passive CW audio 
filter with a bandwidth much less than about 50Hz, due to the finite 
Q of inductors available. This is fairly easy with active filters, but 
requires the use of multiple op-amp filter sections, rather than the 
single op-amp multiple feedback circuits. It gets increasingly 
difficult to make good active filters at high frequencies, but the 
audio range is no problem. Whether active or passive, it is usually 
neccessary to trim component values with narrow filters.

 For audio filters, BiFET op amps like TL071/81, LF351 etc and 
their dual and quad variants are a much better choice than 741 
type op amps; their lower bias currents make for more choice in 
the range of resistor and capacitor values. Some of the newer 
CMOS op-amps are good too, but relatively costly. The most 
important op-amp parameter for filters is the gain-bandwidth 
product - the higher it is, the higher the filter Q that can be obtained 
with a given circuit.

There are usually many ways of producing a given filter 
performance; it's best to have a read of one of the handbooks 
before you start.

Hope this E-mail is legible - something funny has happened to the 
text wrap on this software!

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 a really weak signal in Canada....
Date: Mon, 5 Jun 2000 14:57:30 +0100
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It's been my experience that Soundcards replaying .WAV files can usually
cope with any sampling rate above 5513Hz, although the resultant
frequency generated may not be very accurate. The speeded up ones I
tried were at 6250Hz

One way to test, is to use a hex editor to access the header information
in a .WAV file and just change the value of sampling rate, then see how
well it can be replayed.

Andy  G4JNT


> ----------
> From: 	Alberto di Bene[SMTP:dibene@usa.net]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-05 13:22
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	Re: LF: a really weak signal in Canada....
> 
> Larry Kayser wrote:
> 
> > Greetings:
> >
> > Quote
> > I don't know if this has been tried before, but I just tried it and
> it
> > worked nicely.
> > [snip]
> > I recorded some 578 seconds of audio to hard disk at 7200 samples
> per sec.
> > [snip]
> 
> Seems really a good idea, which could attract also the
> die-hard CW-must-be-copied-by-ears crop around.
> 
> Just one simple question : why 7200 samples/sec ? It is not a standard
> sound card sampling rate. Is there a specific reason for this sampling
> speed ?
> Perhaps Bill was using an external A/D converter. For the technique to
> become widespread and accepted by many (all), it shouldn't rely on an
> ad-hoc hardware. Modern sound cards have superb A/D converters,
> so why not use them ?
> 
> 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: "Dave Sergeant" <sergeantd@compuserve.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: 'Dyed in the wood CW'
Date: Mon, 5 Jun 2000 15:43:19 +0100
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>From Dave G3YMC

There has been some stinging comment on here in recent days on 'dyed in the
wood' CW operators, which perhaps I have to admit to being.  The implication
is that if you persue such modes you are a little dated and should be using
fancy digital thingemy modes these days.  Having spent a most enjoyable
weekend in HF NFD on Top Band it is very apparent that CW is very far from a
dead mode, and anybody who cares to listen to the CW parts of the HF bands
during a major contest will see that it is very much still alive.  In spite
of high static levels there was no shortage of stations able to have quick
exchanges at the normal speeds of 25-30 wpm.

It was commented on here recently that users of the band should use the
modes they wish to use, and any method of having a QSO is equally valid.
Let us stop the bickering - if you want to develop high tech DSP algorithms
etc that is fine, however please accept that some wish to use normal amateur
techniques as well.

Cheers Dave
dsergeant@iee.org
http://ourworld.compuserve.com/homepages/sergeantd




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, 5 Jun 2000 15:34:33 +0100
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I have been playing around with feeding differently derived audio into 
the two halves of stereo headphones with some interesting results. 
I will report in detail when the tests are complete. In short, it is 
certainly possible to improve headphone reception, both in terms of 
close-in selectivity and resistance to static.

One question. How do I make an electronic circuit to delay a 
broadband audio signal by about one-thousandth of a second, 
without resorting to DSP? Any genius out there with a simple 
circuit? And yes I do know about the methods (that were originally 
used for electric guitar echo) such as connecting the diaphragms of 
a loudspeaker and a microphone by using a spring, and also the 
tape recorder method.



Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: 'Dyed in the wood CW'
References: <000e01bfcefc$b56c0920$282878d5@dave>
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I agree, and agree again.

As the editor of the French edition of CQ, and I guess my American
collegues will agree, the latest results of our CW contests confirm that
CW has never been so popular.

On a more personal basis, outside-contest CW is also well and alive.

However, one must not discard all those digital modes which are
obviously very useful when it comes to narrow band reception.

I think it's just different, and maybe complementary.

73, Mark, F6JSZ

Dave Sergeant a *crit :
> 
> >From Dave G3YMC
> 
> There has been some stinging comment on here in recent days on 'dyed in the
> wood' CW operators, which perhaps I have to admit to being.  The implication
> is that if you persue such modes you are a little dated and should be using
> fancy digital thingemy modes these days.  Having spent a most enjoyable
> weekend in HF NFD on Top Band it is very apparent that CW is very far from a
> dead mode, and anybody who cares to listen to the CW parts of the HF bands
> during a major contest will see that it is very much still alive.  In spite
> of high static levels there was no shortage of stations able to have quick
> exchanges at the normal speeds of 25-30 wpm.
> 
> It was commented on here recently that users of the band should use the
> modes they wish to use, and any method of having a QSO is equally valid.
> Let us stop the bickering - if you want to develop high tech DSP algorithms
> etc that is fine, however please accept that some wish to use normal amateur
> techniques as well.
> 
> Cheers Dave
> dsergeant@iee.org
> http://ourworld.compuserve.com/homepages/sergeantd


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: 'Dyed in the wood CW'
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> >From Dave G3YMC
> 
> There has been some stinging comment on here in recent days on 'dyed in
> the wood' CW operators, which perhaps I have to admit to being.  The
> implication is that if you persue such modes you are a little dated and
> should be using fancy digital thingemy modes these days.  
[cut]
> Let us stop the bickering - if you want to develop high tech DSP
> algorithms etc that is fine, however please accept that some wish to use
> normal amateur techniques as well.


Who are you calling abnormal! Seriously, though, as a very keen 
CW operator (I do have a microphone but you'd have to give me a 
day's notice to find it), the really encouraging thing about LF is that 
it has demonstrated many of the benefits of this fine old mode - low 
bandwidth, tolerant of low S/N ratio, simple to execute, and good 
fun. Several regular ops have re-learned Morse simply to use the 
band. It will be a long time before the more complex modes match 
every one of those advantages, even if they excel at one or two.

Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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: Re: LF: 'Dyed in the wood CW'
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Dave Sergeant wrote:

> >From Dave G3YMC
>
> There has been some stinging comment on here in recent days on 'dyed in the
> wood' CW operators, which perhaps I have to admit to being.  The implication
> is that if you persue such modes you are a little dated and should be using
> fancy digital thingemy modes these days.
> [snip]
>

Dave,
               frankly I don't know whether you were addressing me for
an half sentence I put in my last message to the reflector.
The English language is full of subtleties that escape to a non-native speaker.
If you took my sentence as dismissive of aural CW, perhaps I didn't make
my thoughts clear enough. As a matter of fact, I sometimes enjoy listening
to CW, though my skills are far from being perfect.
What I meant was a sort of criticism of the komeinist position that says
that  "if it ain't copied by ears, it's rubbish". I wasn't trying to convey any
other subliminal message. And, from what you say, you don't certainly
qualify as a target for that my comment.

Cheers,
Alberto    I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Clifford Buttschardt" <cbuttsch@slonet.org>
To: "Mike Dennison" <mike.dennison@rsgb.org.uk>
Cc: rsgb_lf_group@blacksheep.org
Subject: Re: LF: Copying CW
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There are chips called "bucket brigade" delay lines that will do this job
easily.  Radio Shack and Digi-Key here in the States would have them.  I'd
check MAPLEN (spelling could be wrong here!) using that terminology.
Cliff K7RR


On Mon, 5 Jun 2000, Mike Dennison wrote:

> I have been playing around with feeding differently derived audio into 
> the two halves of stereo headphones with some interesting results. 
> I will report in detail when the tests are complete. In short, it is 
> certainly possible to improve headphone reception, both in terms of 
> close-in selectivity and resistance to static.
> 
> One question. How do I make an electronic circuit to delay a 
> broadband audio signal by about one-thousandth of a second, 
> without resorting to DSP? Any genius out there with a simple 
> circuit? And yes I do know about the methods (that were originally 
> used for electric guitar echo) such as connecting the diaphragms of 
> a loudspeaker and a microphone by using a spring, and also the 
> tape recorder method.
> 
> 
> 
> Mike, G3XDV (IO91VT)
> http://www.dennison.demon.co.uk/activity.htm
> 
> 
> 



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 05 Jun 2000 13:47:48 -0400
From: "Steve Dove" <dsp@hifidelity.com>
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Hi Mike,

Ooooh, analogue.  I remember that.

Possibly still available (I checked the Digikey book without success, but
RS etc. maybe?) would be bucket-brigade delay lines, which were used
extensively for audio effects (delay / spin / reverb etc.) in the olde
days.  Recoton was a manufacturer if memory serves, as I think were
NatSemi, but they've been shedding even less esoteric product than that in
recent years.

They had only so-so noise performance, but their dynamic range would be
plenty good enough for what you're suggesting.  The through delay is
varied by clocking their fixed-length chain of buckets faster or slower.

        73

                Steve        W3EEE  /  G3YDV



Mike Dennison wrote:

> I have been playing around with feeding differently derived audio into
> the two halves of stereo headphones with some interesting results.
> I will report in detail when the tests are complete. In short, it is
> certainly possible to improve headphone reception, both in terms of
> close-in selectivity and resistance to static.
>
> One question. How do I make an electronic circuit to delay a
> broadband audio signal by about one-thousandth of a second,
> without resorting to DSP? Any genius out there with a simple
> circuit? And yes I do know about the methods (that were originally
> used for electric guitar echo) such as connecting the diaphragms of
> a loudspeaker and a microphone by using a spring, and also the
> tape recorder method.
>
> Mike, G3XDV (IO91VT)
> http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Steve Dove" <dsp@hifidelity.com>
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Hi Mike,

Reticon was who I meant, however they seemed to have skipped out of that town,
too.  A further 30 seconds perusal of the Digikey book turned up a bunch of
Panasonic parts of various lengths and permutations.  For a millisecond or two
even the shortest devices would be adequate (sampling-rate limitations rule
here just as they do in digital);  at a stab I'd say the 8-pin DIP MN3009
256-bucket alleged 'low-noise' part at $4.84 would be the one.  It with a 555
to clock it is basically all you'd need.

Other parts listed are MN3003,8,10,11,12, MN3204,6,8,9 and 14 if that helps
you source them closer to home.

        73

                Steve


Steve Dove wrote:

> Hi Mike,
>
> Ooooh, analogue.  I remember that.
>
> Possibly still available (I checked the Digikey book without success, but
> RS etc. maybe?) would be bucket-brigade delay lines, which were used
> extensively for audio effects (delay / spin / reverb etc.) in the olde
> days.  Recoton was a manufacturer if memory serves, as I think were
> NatSemi, but they've been shedding even less esoteric product than that in
> recent years.
>
> They had only so-so noise performance, but their dynamic range would be
> plenty good enough for what you're suggesting.  The through delay is
> varied by clocking their fixed-length chain of buckets faster or slower.
>
>         73
>
>                 Steve        W3EEE  /  G3YDV
>
> Mike Dennison wrote:
>
> > I have been playing around with feeding differently derived audio into
> > the two halves of stereo headphones with some interesting results.
> > I will report in detail when the tests are complete. In short, it is
> > certainly possible to improve headphone reception, both in terms of
> > close-in selectivity and resistance to static.
> >
> > One question. How do I make an electronic circuit to delay a
> > broadband audio signal by about one-thousandth of a second,
> > without resorting to DSP? Any genius out there with a simple
> > circuit? And yes I do know about the methods (that were originally
> > used for electric guitar echo) such as connecting the diaphragms of
> > a loudspeaker and a microphone by using a spring, and also the
> > tape recorder method.
> >
> > Mike, G3XDV (IO91VT)
> > http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Copying CW
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In message <E12yyDT-00049o-00@mserv1b.u-net.net>, Mike Dennison
<mike.dennison@rsgb.org.uk> writes
>I have been playing around with feeding differently derived audio into 
>the two halves of stereo headphones with some interesting results. 
>I will report in detail when the tests are complete. In short, it is 
>certainly possible to improve headphone reception, both in terms of 
>close-in selectivity and resistance to static.
>
>One question. How do I make an electronic circuit to delay a 
>broadband audio signal by about one-thousandth of a second, 
>without resorting to DSP? Any genius out there with a simple 
>circuit? And yes I do know about the methods (that were originally 
>used for electric guitar echo) such as connecting the diaphragms of 
>a loudspeaker and a microphone by using a spring, and also the 
>tape recorder method.

The method we used at a TV station I once worked for was to use a long
corridor with a mic and a loudspeaker!

Mike
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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I wish to thank Jim M0BMU for his good summary comments on filter
design, including Bessel types.

I do not have either of the two reference books Jim named and I will
request the public library to seek them on interloan.

While I happen to have quite a good selection of salvaged high Q audio
inductors, as for the PA0LQ filter, any confirmed good design is of
wider applicability to others if it is an active filter type (and using
good op amps).  While a coupled passive filter may give good results, it
is closer to a special one-off result if the inductor types are hard to
acquire.  Also if it needs a high impedance load, then it could need an
op amp anyway, so it would not be an entirely passive circuit as an
accessory.  I'm going to include an audio PA chip so the accessory
filter can have a volume control and feed a loudspeaker or low impedance
headphones or a PC sound card.

Suggestions of others resulted in some PC CAD software being downloaded,
and this is mostly of the "demo" or "knobbled" variety as it is "free". 
I have found it to be very interesting where group delay curves are
available.  However, as at present I have yet to find out what results
from selected stagger tuning (of isolated resonators, using active
filters).

73, Bob ZL2CA




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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TRANS-PACIFIC LF TEST SCHEDULE                        6 June 2000

Arrangements have been made for a number of West Coast stateside LF
listeners to 
find out what they can receive from ZL LF test transmissions.  The
timing is 
Saturday night 17 June (New Zealand time) which is Friday night and
Saturday 
morning California time.  It is intended to also try again on Saturday
24 June, 
but subject to review, depending on what is reported for 17 June.  The
following 
table shows the respective sunset and sunrise times:

              ZL sunset      CA sunrise     ZL sunrise
              =========      ==========     ==========
   17 June    0455 UTC       1252 UTC       1950 UTC
   24 June    0457           1253           1952

The timing happens to be around the longest day (mid summer) in the
northern 
hemisphere, which of course corresponds to the longest night in the
southern 
hemisphere (mid winter).

The following stations intend to be transmitting:

    ZL1WB  181.42 kHz
    ZL6QH  182.10 kHz  (operated by ZL2BBJ and ZL2CA)
    ZL3PN  182.70 kHz
    ZL4MD  183.50 kHz
    ZL3VN  184.00 kHz
    ZL3JE  184.50 kHz
    ZL4OL  185.00 kHz
    AX2TAR 176.50 kHz  (VK7ZAL, Tasmania, Australia)

The station with highest radiated power is likely to be the Quartz Hill
station 
ZL6QH.  It is intended to run ZL6QH as a continuous beacon transmission,
from 
around 0400 - 2000 UTC on 17 June.  This covers times for many "dark"
paths, both 
east and west.

AX2TAR is also planning to run continuously, from 0630 - 1300 UTC on 17
June.

All other stations will definitely try to be transmitting for around
half an hour 
either side of ZL sunset time as well as the California sunrise time. 
As each 
station has a unique test frequency, there is no co-channel pile-up. 
Frequencies 
have already been checked for not coinciding with local QRM for
receiving stations 
in California. 

In general, stations will attempt to maintain their assigned carrier
frequency 
within 10 Hz.  In general emissions will be conventional CW at around 5
wpm.

Reception reports are welcomed.  Email to reflector sites would
generally be the 
fastest and most effective way to disseminate reports.

Bob ZL2CA




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: <E12yyDT-00049o-00@mserv1b.u-net.net>
Subject: LF: Re: Copying CW
Date: Tue, 6 Jun 2000 13:24:44 +0200
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To All from PA0SE

Mike, G3XDV, wrote

> I have been playing around with feeding differently derived audio into
> the two halves of stereo headphones with some interesting results.
> I will report in detail when the tests are complete. In short, it is
> certainly possible to improve headphone reception, both in terms of
> close-in selectivity and resistance to static.

I have tested "pseudo-stereophonic" reception of CW by feeding the halves of
a stereo headphone via series tuned circuits resonating at  1002 and 842Hz
(922 ± 80Hz)  respectively.
At first the result  was pleasant; it sounded like being in a room with the
wanted 922Hz signal in the centre. But it did not take me long to find out
that it contributed absolutely nothing to the readibility of signals under
difficult conditions.

It proved again that our sophisticated ear/brain system cannot be helped by
such primitive contraptions.

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: Re: LF: Re: Copying CW
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Dick, PA0SE wrote:
> I have tested "pseudo-stereophonic" reception of CW by feeding the halves
> of a stereo headphone via series tuned circuits resonating at  1002 and
> 842Hz (922 ± 80Hz)  respectively. At first the result  was pleasant; it
> sounded like being in a room with the wanted 922Hz signal in the centre.
> But it did not take me long to find out that it contributed absolutely
> nothing to the readibility of signals under difficult conditions.
> It proved again that our sophisticated ear/brain system cannot be helped
> by such primitive contraptions.

Yes, I'm aware of this but am keeping an open mind. I have already 
done some interesting tests that combine some of the advantages 
of both analogue and digital techniques. One crude test last 
weekend produced significantly better readability of a weak station 
in heavy static than was available either direct from my radio, or via 
a DSP unit.

What sparked off this idea was the number of people who agreed 
that listening to a pair of headphones on the bench gave them 
better reception than when the phones were on the head. Therefore 
there appears to be at least one uninvestigated way of enhancing 
reception which at present relies on chance and acoustics.

I agree that all theoretical work tends to ignore the colossal 
advantage of using the brain, but I am not a theorist and would like 
to find ways of helping the brain along a bit.

Thanks very much to all those who replied re time delays.

As soon as I have reached some conclusions I will report my 
results - or that Dick is indeed right and the brain can't be helped at 
all!



Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 6 Jun 2000 15:57:31 +0100
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Re: Copying CW
References: <001701bfcfa9$ea7322e0$1fd499d4@w8k3f0> <E12zIkh-0003zU-00@mserv1b.u-net.net>
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In message <E12zIkh-0003zU-00@mserv1b.u-net.net>, Mike Dennison
<mike.dennison@rsgb.org.uk> writes
>Dick, PA0SE wrote:
>> I have tested "pseudo-stereophonic" reception of CW by feeding the halves
>> of a stereo headphone via series tuned circuits resonating at  1002 and
>> 842Hz (922 ± 80Hz)  respectively. At first the result  was pleasant; it
>> sounded like being in a room with the wanted 922Hz signal in the centre.
>> But it did not take me long to find out that it contributed absolutely
>> nothing to the readibility of signals under difficult conditions.
>> It proved again that our sophisticated ear/brain system cannot be helped
>> by such primitive contraptions.
>
>Yes, I'm aware of this but am keeping an open mind. I have already
>done some interesting tests that combine some of the advantages
>of both analogue and digital techniques. One crude test last
>weekend produced significantly better readability of a weak station
>in heavy static than was available either direct from my radio, or via
>a DSP unit.
>
>What sparked off this idea was the number of people who agreed
>that listening to a pair of headphones on the bench gave them
>better reception than when the phones were on the head. Therefore
>there appears to be at least one uninvestigated way of enhancing
>reception which at present relies on chance and acoustics.
>
>I agree that all theoretical work tends to ignore the colossal
>advantage of using the brain, but I am not a theorist and would like
>to find ways of helping the brain along a bit.
>
>Thanks very much to all those who replied re time delays.
>
>As soon as I have reached some conclusions I will report my
>results - or that Dick is indeed right and the brain can't be helped at
>all!

Don't forget the old trick of fixing a loudspeaker to the end of a pipe
and using the organ pipe resonance frequency. Quite common in the 40s
and 50s. I wonder if two could be used, tuned to different frequencies
and placed at opposite ends of the room?

73


Mike 
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Prof R. Jennison" <boffin1@compuserve.com>
Subject: LF: Copying CW
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Mike,
We used to use delay lines!
Roger.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Peter Dodd" <g3ldo@zetnet.co.uk>
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Subject: LF: Re: Antenna Z measurements at LF
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 Measurement of Antenna System Impedance at LF

Although a suitable matching transformer can be arrived at 
empirically the design can be simplified if the antenna feed 
impedance is known. An impedance value will also give you some idea 
of how good your ground system is, once you have estimated the coil 
loss. There may be other uses.

The method of measuring impedance I use is called the 3 Meter 
Impedance Measuring Method (3m Z Bridge) and I have used it for the 
last 20 years on HF. It is described in more detail in 'The Antenna 
Experimenter's Guide'  (from RSGB Bookshop).
The 3-meter impedance measurement technique is very simple. It 
compares the unknown impedance with a fixed standard impedance, (a 50 
ohm resistor and a .01uF capacitor). An excitation source (signal 
generator) applies an RF voltage to the standards and diode 
voltmeters, selected by a switch allow digital voltmeter readings to 
be made at various points. Impedance is indicated by the ratio of 
three voltmeter readings. One additional reading allows in-place 
calibration of the reference capacitor and the second permits several 
solutions for the unknown impedance, thus giving an indication of the 
random errors that may be present in the data.
Impedance values are derived from the voltage data by calculation. 
However, this may be simplified by using a graphic method (using 
graph paper and a pair of compasses and a ruler) or a computer. The 
BASIC (do you remember that stuff?) source code is available at the 
RSGB Web site <www.rsgb.org>  If you download it as a text file it 
will run in Q-Basic - I dont know about Visual Basic.
If you are using the standard Marconi antenna measure the feedpoint 
impedance from the bottom of the loading coil and earth.

The following measured impedances in the range 136.4 to 138kHz 
indicate some errors just below 137kHz, which I have not yet identified. 

G3LDO_LF_Antenna
 
                    Results        +/-Errors
Freq MHz   Res      jX       Res    jX
----------------------------------------
 .1364       37.9   - 29.4      2      2.1
 .1366       37.4   - 22.8      4.6    5.3
 .1368       33.5   - 22.2     5.1    5.7
 .1370       33.4   - 17.3      5.8    7.4
 .1372       35.6   - 8.8       2.8    3.5
 .1374       36.4   -0 1        1.7    2
 .1376       36.9   +0 5       1.1    1.3
 .1378       36.5   + 13.3    1      1.3
 .1380       38.1   + 21       1.1    1.8

The above measurements were made in the late afternoon when the 
ground was relatively dry. In the morning the resistance was above 
40ohms and resonance was around 136.8kHz. 

A full description will appear in the forthcoming LF Book.



-- 
Regards, Peter, G3LDO

<g3ldo@zetnet.co.uk>






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 6 Jun 2000 23:00:30 +0100
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Copying CW
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In message <200006061702_MC2-A7C1-1189@compuserve.com>, Prof R. Jennison
<boffin1@compuserve.com> writes
>Mike,
>We used to use delay lines!

We were too poor to afford a delay line!

TWW, Cardiff 1959.

Mike
-- 
M.J.Powell


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Subject: Re: LF: Re: Copying CW
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Greetings,


> Don't forget the old trick of fixing a loudspeaker to the end of a pipe
> and using the organ pipe resonance frequency. 

Re Resonant Loudspeakers..

You might like to look at   http://www.io.com/~maddog/hamradio/res_spkr.htm

cheers ................... Zim



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
Subject: Re: LF: a really weak signal in Canada....
Date: Tue, 6 Jun 2000 21:28:59 -0400
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Alberto:

>> I recorded some 578 seconds of audio to hard disk at 7200 samples per
sec.
>> [snip]
>
>Seems really a good idea, which could attract also the
>die-hard CW-must-be-copied-by-ears crop around.
>
>Just one simple question : why 7200 samples/sec ? It is not a standard
>sound card sampling rate. Is there a specific reason for this sampling
speed ?
>Perhaps Bill was using an external A/D converter. For the technique to
>become widespread and accepted by many (all), it shouldn't rely on an
>ad-hoc hardware. Modern sound cards have superb A/D converters,
>so why not use them ?


Yes, your right sound cards today are at least good.  However Bill started
his work way back and he uses a small card that implements in discrete logic
a Sigma Delta A/D, published in QST in 1992.  The card runs the serial port
at 115200 baud with 10 of the 16 bits being a full async character with
start bit, 8 data bits, and a stop bit.  the blank 6 bits let the processor
get some work done between data characters.

http://www.ietc.ca/home/bill/bbs.htm

if you go and look and download some of the material at Bills web site you
can see how he does things.

>For the technique to
>become widespread and accepted by many (all), it shouldn't rely on an
>ad-hoc hardware.

Fair opinion for you Alberto, possibly relevant in your terms.

>Modern sound cards have superb A/D converters,
>so why not use them ?

Computer sound cards did not exist when Bill started his work, since they
were not available they were not used.  Having been around A/D converters
for many years, the superlative of "superb A/D converters" seems to have a
degree of hyperbole from my perspective.

Bill will probably speak to the sound card issue at some point in the
future, that is his choice of course.

In the interim he has done DSP work that is superb for weak signal work and
has been demonstrated to perform excellently.

Larry
VA3LK





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: Formula
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I found the following in an article recently.

Quote:

"The intensity E (known as the field strength) of a transmission
at a distance D from a source transmitting P watts of RF power via
a half-wave dipole in a free, unobstructed space, can be estimated
using the formula:

E=(7*sqrt (P))/D.

Thus, for a 2 watt transmitter, the theoretical field strength in free
space at one metre distance is approximately 10 V/m and at 100 metres
distance 0.1 V/m"

This formula is new to me and I can't find it in any
textbooks I have.  Since it ignores frequency shouldn't
it be power flux per unit area and not field strength?
Can anyone tell me where it comes from?

Walter G3JKV.




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: Formula
Date: Wed, 7 Jun 2000 11:42:27 +0100
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Walter  et al :- 

Doesn't specifying a dipole as the radiator automatically take antenna
aperture into account, and cancels out frequency from the equation ?  So
if you take just the spreading out of the total power over the area of a
sphere :

Watts per m^2  =  P . / (D ^ 2  x  4.pi)	
and  E ( V/m )  = SQTR( Power x. Resistance of free space )
so   Volts / m   =   SQRT(W/m^2  *   Z free space)   =   SQRT(P x 377 /
4.pi / D^2)

= SQRT(P) * 30 / D  

A dipole has a gain of 1.64 (power) so its "voltage gain" could be said
to be 1.28
so I reckon the formula should read    E  (V/m)  =    38.4 . SQRT(P) / D
(all in SI units of course)

Some way off a value of 7, but in the right region.   Can anyone spot if
I've slipped a digit or something ?

Andy  G4JNT

> ----------
> From: 	Walter Blanchard[SMTP:blanch@pncl.co.uk]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-07 10:25
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	LF: Formula
> 
> I found the following in an article recently.
> 
> Quote:
> 
> "The intensity E (known as the field strength) of a transmission
> at a distance D from a source transmitting P watts of RF power via
> a half-wave dipole in a free, unobstructed space, can be estimated
> using the formula:
> 
> E=(7*sqrt (P))/D.
> 
> Thus, for a 2 watt transmitter, the theoretical field strength in free
> space at one metre distance is approximately 10 V/m and at 100 metres
> distance 0.1 V/m"
> 
> This formula is new to me and I can't find it in any
> textbooks I have.  Since it ignores frequency shouldn't
> it be power flux per unit area and not field strength?
> Can anyone tell me where it comes from?
> 
> Walter G3JKV.
> 
> 
> 


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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, 7 Jun 2000 11:29:26 +0100
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Yesterday there were three major solar flares (two X class and an 
M).

There should be a major impact on LF conditions as a result, as 
well as auroras and HF fade-out.

See http://www.dxlc.com/solar/ for more info.


Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "cesare tagliabue" <cestag@dada.it>
To: rsgb_lf_group@blacksheep.org
Subject: LF: R: Formula
Date: Wed, 7 Jun 2000 13:11:26 +0200
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            Hi Walter
        The formula is derived from the general one that is: E =
SQR(30*P*G)/D. Being the gain G of an half-wave dipole equal to 1.64,
30*1.64 = 49.2, rounded to integer and written out of the square root it
becomes 7. E is the field strength in V/mt, provided that P is in Watts and
D in meter; in fact the field strength is independent from frequency.
        73  Cesare

Cesare Tagliabue   I 5 TGC
e-mail: cestag@dada.it
url: http://www.dadacasa.com/i5tgc

-----Messaggio originale-----
Da: Walter Blanchard <blanch@pncl.co.uk>
A: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Data: mercoledì 7 giugno 2000 11.58
Oggetto: LF: Formula


>I found the following in an article recently.
>
>Quote:
>
>"The intensity E (known as the field strength) of a transmission
>at a distance D from a source transmitting P watts of RF power via
>a half-wave dipole in a free, unobstructed space, can be estimated
>using the formula:
>
>E=(7*sqrt (P))/D.
>
>Thus, for a 2 watt transmitter, the theoretical field strength in free
>space at one metre distance is approximately 10 V/m and at 100 metres
>distance 0.1 V/m"
>
>This formula is new to me and I can't find it in any
>textbooks I have.  Since it ignores frequency shouldn't
>it be power flux per unit area and not field strength?
>Can anyone tell me where it comes from?
>
>Walter G3JKV.
>
>
>
>



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 sent:      	Wed, 07 Jun 2000 10:25:14 +0100
To:             	rsgb_lf_group@blacksheep.org
From:           	Walter Blanchard <blanch@pncl.co.uk>
Subject:        	LF: Formula
Send reply to:  	rsgb_lf_group@blacksheep.org

> I found the following in an article recently.
> 
> Quote:
> 
> "The intensity E (known as the field strength) of a transmission
> at a distance D from a source transmitting P watts of RF power via
> a half-wave dipole in a free, unobstructed space, can be estimated
> using the formula:
> 
> E=(7*sqrt (P))/D.

Dear Walter & Group,

If the propagating wave is a transverse electromagnetic wave 
(which it will be a reasonable distance from the antenna, in 'free 
space'), the electric (E volts/m) and magnetic (H amps/m) fields are 
proportional; E/H = 120pi ohms. This 'free space wave impedance' 
is about 377ohms and is a constant provided the permeability and 
permittivity of the medium is the same as a vacuum, or air is near 
enough. This comes about ultimately from the definitions of volts 
and amps. E times H has the dimensions of watts/sq. metre and so 
is called the power density, S. A bit of algebra gives you power 
density S = (Esquared)/120pi (compare with P = (Vsquared)/R), so 
measuring E is effectively also a measure of power density, and 
also a measure of H. Rearranging this gives E = sqrt(120piS)

If the antenna in free space radiated equally in all directions, (ie. 
an 'isotropic radiator'), at a distance d the radiated power P would 
be evenly distributed over the surface of a sphere of radius d. the 
surface of the sphere would have an area 4pi(d squared), so 
power density would be S = P / 4pi(d squared). Putting this value of 
power density into the equation for E gives 
E= sqrt (30P/(d squared), or E= 5.477 sqrt(P)/d.

This applies to an isotropic radiator, but all real antennas have a 
directional pattern, and so in the direction of their maximum 
radiation, the power density is increased by a factor D (note not d, 
the distance), the directivity or directional gain. This makes E = 
5.477 sqrt (PD)/d.

The value of D depends on the geometry and voltage and current 
distribution of the antenna. It's quite complex to work out, but can 
be done for simple antennas - refer to an antenna text book for 
details! - it can be calculated by programs such as EZNEC for 
more complicated antennas. For a half wave dipole it is 1.64, for a 
short monopole it is 3. Putting D = 1.64 into the formula gives
E = 7.01 sqrt (P) / d for a half wave dipole,

E = 9.49 sqrt (P) / d for a short monopole. 

Hope that is some help,
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: R: Formula
Date: Wed, 7 Jun 2000 12:54:34 +0100
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Ah -
I'd taken the factor of 30 outside the square root then.  Careless !!

Andy  'JNT

> ----------
> From: 	cesare tagliabue[SMTP:cestag@dada.it]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-07 12:11
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	LF: R: Formula
> 
>             Hi Walter
>         The formula is derived from the general one that is: E =
> SQR(30*P*G)/D. Being the gain G of an half-wave dipole equal to 1.64,
> 30*1.64 = 49.2, rounded to integer and written out of the square root
> it
> becomes 7. E is the field strength in V/mt, provided that P is in
> Watts and
> D in meter; in fact the field strength is independent from frequency.
>         73  Cesare
> 
> Cesare Tagliabue   I 5 TGC
> e-mail: cestag@dada.it
> url: http://www.dadacasa.com/i5tgc
> 
> -----Messaggio originale-----
> Da: Walter Blanchard <blanch@pncl.co.uk>
> A: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
> Data: mercoledì 7 giugno 2000 11.58
> Oggetto: LF: Formula
> 
> 
> >I found the following in an article recently.
> >
> >Quote:
> >
> >"The intensity E (known as the field strength) of a transmission
> >at a distance D from a source transmitting P watts of RF power via
> >a half-wave dipole in a free, unobstructed space, can be estimated
> >using the formula:
> >
> >E=(7*sqrt (P))/D.
> >
> >Thus, for a 2 watt transmitter, the theoretical field strength in
> free
> >space at one metre distance is approximately 10 V/m and at 100 metres
> >distance 0.1 V/m"
> >
> >This formula is new to me and I can't find it in any
> >textbooks I have.  Since it ignores frequency shouldn't
> >it be power flux per unit area and not field strength?
> >Can anyone tell me where it comes from?
> >
> >Walter G3JKV.
> >
> >
> >
> >
> 
> 


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Walter Blanchard wrote:
> 
> I found the following in an article recently.
> 
> Quote:
> 
> "The intensity E (known as the field strength) of a transmission
> at a distance D from a source transmitting P watts of RF power via
> a half-wave dipole in a free, unobstructed space, can be estimated
> using the formula:
> 
> E=(7*sqrt (P))/D.
> 
> Thus, for a 2 watt transmitter, the theoretical field strength in free
> space at one metre distance is approximately 10 V/m and at 100 metres
> distance 0.1 V/m"
> 
> This formula is new to me and I can't find it in any
> textbooks I have.  Since it ignores frequency shouldn't
> it be power flux per unit area and not field strength?
> Can anyone tell me where it comes from?
> 
> Walter G3JKV.

In free space, field strength for a given radiated power is independent
of frequency.  This is basically the case for a point source radiator
surrounded by an imaginary sphere, and the power flux density is
constant for any given same area of the imaginary sphere.  This is not
to say that the received power using a reference antenna is independent
of frequency: it is not.  For the likes of half wave dipoles, receiving
aperture has a -6 dB per octave relationship with increasing frequency. 
So field strength is independent of frequency, but received power is -6
dB/octave.

Whatever, at LF we hardly ever encounter "free space" around our
antennas.  Free space is a concept for VHF and higher frequencies as far
as ground-based radio stations are concerned.

73, Bob ZL2CA



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 7 Jun 2000 09:28:12 -0400
From: "DEREK ATTER" <DATTER@compuserve.com>
Subject: LF: Decca Loading coils, 1Kw Transmitters, Litz wire etc.
To: rsgb_lf_group@blacksheep.org
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The Crawley Club have managed to collect a number of  items of hardware
from the redundant Decca stations before they were scrapped. These  include
several of the 1.2Kw  transmitters,  a considerable amount of Litz wire of
various gauges, one or two variometers, several of the large loading coils
described on Mike G3XDV's website plus a number of high stability 5Mhz xtal
oscillators.

   The Club propose to offer these for disposal among the LF fraternity at
modest prices to cover the transport costs from site plus a donation to
local clubs for their efforts in collecting and storing the equipment.  The
the Club does not  wish to get  involved in arranging delivery so equipment
will have to be collected from Crawley.  Anyone interested please contact
me for information on details on prices etc. by phone on 01293 520424 or by
E-mail at. (datter@compuserve.com) 
    The Crawley Club are hosting the South Eastern session of the 
Microwave Round Table this coming Sunday, 11th June.   The morning session
starting at 10 am will include a small 'bring and buy' sale at which the LF
items will be also be available.       Information on the ex-Decca items
will also be posted on the Crawley Club website at
www://http.bigfoot.com/~crawleyarc/

Further details of the some of the hardware:

Tranmitters :      1.2Kw RF out from 3 separate PA modules each with 4
power MOSFETs  operating in class "D" in a bridge   configuration.  The
units are rack mounted with integral driver and protection circuitry in
each module. RF drive input 3V  pk-pk.
  DC input supplies 67.5V about 25A and 24V at 1A.  Technical info and
circuit diagrams are available.  Depending on demand we  could split up
some TX units into individual PA modules each nominally rated at  400W but
believed capable of about 600W each.
 
Litz Wire :  In addition to the large loading  coils ( about 900mm diam  x
250mm wide with 729 strand Litz wire) we have a variety of different gauges
from quite thin up to some about 3mm diam double cotton covered with large
number of strands. Probably the most interesting to LF'ers  is a quantaty
of  2mm and 3mm diam Litz wire with a thin outer sheath of polythene or
similar (may be PTFE ?) which will have a much higher insulation rating
than the usual cotton covered  variety which will reduce turn-turn voltage
breakdown for loading coil use.
                73 de Derek Atter,  G3GRO


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'" <rsgb_lf_group@blacksheep.org>
Cc: "'KZY'" <Paul@HF-Inst.co.uk>,  chris@hf-inst.co.uk
Subject: LF: DDS Board Progress
Date: Wed, 7 Jun 2000 14:57:27 +0100
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The AD9850 DDS Board is now with the PCB manufacturers.  I went there
yesterday to check the solder mask, and had a fascinating trip round the
factory looking at PCB manufacture and SMT component pick and place
mounting.  Delivery is still quoted as 30 days so we have about 3 - 4
weeks left as these are being batched with other PCBs.

Price of the PCB will probably be £8.00, plus p&p whatever that will
come out at.  HF Instruments will also coordinate a bulk purchase of
AD9850 chips and some AD9851 devices too (see below), prices still to be
fixed.   I have also been told that it will be possible to supply chips
mounted on the PCB for those frightened by the thought of soldering 28
0.65mm spaced pins - although its not as difficult as you might think
especially with a solder mask there to help avoid shorts underneath.

The AD9851 DDS chip is pin compatible with the AD9850 device and has an
internal x6 clock multiplier allowing it to be used with up to a 30 MHz
oscillator to give a clock freqeuncy to 180 MHz - output range can then
go from DC to 70 MHz in steps of 0.04 Hz.   For LF use however, I would
still recommend the AD9850 device with a drive frequency of 4 - 5 MHz
giving mHz steps.   
One interesting aspect that comes out of the 9851 data sheet is the use
of the aliassed DDS products, after bandPASS filtering, to generate
frequencies in the VHF range up to 100s of MHz.   Very useful to
microwavers.

Andy  G4JNT


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Re: Copying CW
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Dick Rollema wrote:

> To All from PA0SE
>
> Mike, G3XDV, wrote
>
> > I have been playing around with feeding differently derived audio into
> > the two halves of stereo headphones with some interesting results.
> > I will report in detail when the tests are complete. In short, it is
> > certainly possible to improve headphone reception, both in terms of
> > close-in selectivity and resistance to static.
>
> I have tested "pseudo-stereophonic" reception of CW by feeding the halves of
> a stereo headphone via series tuned circuits resonating at  1002 and 842Hz
> (922 ± 80Hz)  respectively.
> At first the result  was pleasant; it sounded like being in a room with the
> wanted 922Hz signal in the centre. But it did not take me long to find out
> that it contributed absolutely nothing to the readibility of signals under
> difficult conditions.

You are correct, this has all been tried before years ago and proved useless.
The only solution is to become a compentent cw operator. You will then be able
to read cw under all adverse conditions. which is often the case of HF/LF. And
cw is far from DEAD. It is virtually impossible to find a slot
on the cw portion of any band  especially during a contest. How about a high
speed cw contest on 136 khz.
Is there such a thing as a BPSK, PTOR or PSK31 contest ???????????
G3KEV



>
>
> It proved again that our sophisticated ear/brain system cannot be helped by
> such primitive contraptions.
>
> 73, Dick, PA0SE




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 7 Jun 2000 10:17:00 -0700 (PDT)
From: "john sexton" <computernetworks@excite.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Solar flares
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Hi All,

Thought the following might be of interest:

Space Weather News for June 6, 2000 

An intense "X-class" solar flare today was followed by a full-halo coronal 
mass ejection.  Material from the leading edge of the disturbance is 
expected to arrive on Thursday, June 8, with possible auroral displays to 
follow.  For images and updates please visit http://www.spaceweather.com

John, G4CNN





_______________________________________________________
Get 100% FREE Internet Access powered by Excite
Visit http://freelane.excite.com/freeisp



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: Re: LF: a really weak signal in Canada....
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Larry Kayser wrote:

>
> >Modern sound cards have superb A/D converters,
> >so why not use them ?
>
> Computer sound cards did not exist when Bill started his work, since they
> were not available they were not used.  Having been around A/D converters
> for many years, the superlative of "superb A/D converters" seems to have a
> degree of hyperbole from my perspective.
>

'Superb' in this context refers of course to the adequateness (sp?) to the task.
Having 16 bits of resolutions, and, for the best cards, a noise floor approaching
-90 dB, seems to be much more than adequate for whatever radio-received
audio-range signals one could need to process. For hi-fi applications, this doesn't
hold any more, of course.

>
> In the interim he has done DSP work that is superb for weak signal work and
> has been demonstrated to perform excellently.
>

Yes, his work is excellent, and if/when he will port it to a sound card, it will surely be
a winner also in terms of number of users.

73
Alberto    I2PHD




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 08 Jun 2000 09:01:10 +0100
To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: LF: Formula
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Thanks, chaps. Old grey cells getting scrambled by all the RF
over the years, I guess!
Walter G3JKV.


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From: "Gasparik Richard" <Richard.Gasparik@siemens.sk>
To: "Rsgb_Lf_Group \(E-mail\)" <rsgb_lf_group@blacksheep.org>
Subject: LF: LF PA with tube...
Date: Thu, 8 Jun 2000 11:18:06 +0200
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Hi all...

Anybody have an idea how to build an power amplifier with single tube ?
I have some GU81's. They needs about Ua=2000 V and Ia(max)=600mA.
I calculated Pi match, but values of capacitors are to high...anybody knows
how to do it other way ?
Thank you very much for all info...

Rich OM2TW


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Koenig, Wolfgang" <Wolfgang.Koenig@vs.dasa.de>
To: rsgb_lf_group@blacksheep.org
Subject: LF: AW: Sorry no Dx Cluster spots from GB7DXM
Date: Thu, 8 Jun 2000 12:40:26 +0200
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Hallo Group,

there was only one spot on db0mdx last weekend:

   136.7  OZ1KMR       2-Jun-2000 1610Z                           <dl3fdo>

I was not able to be qrv on lf or spot any station because I was involved in
the FD-activity of DL0UL/p.

Hope to be qrv during whitsuntide. hopefully the static crashes keep low.

73 de dl1san wolf

-----Ursprüngliche Nachricht-----
Von: Alan Melia [mailto:Alan.Melia@btinternet.com]
Gesendet am: Montag, 5. Juni 2000 00:20
An: rsgb_lf_group
Betreff: LF: Sorry no Dx Cluster spots from GB7DXM

Hi all, I am sorry to say that the local DX Cluster crashed late last week
and there are no entries on it for LF.
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: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: LF PA with tube...
Date: Thu, 8 Jun 2000 12:52:44 +0100
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>Anybody have an idea how to build an power amplifier with single tube ?
>I have some GU81's. They needs about Ua=2000 V and Ia(max)=600mA.
>I calculated Pi match, but values of capacitors are to high...anybody
knows
>how to do it other way ?
>Thank you very much for all info...

>Rich OM2TW

Sell it and get some power Mosfets..........

More seriously though, what is wrong with this pi-network ?  assuming an
Rl for the valve of 2000V / 0.6 A  = 3300 ohms  which will allow over
1kW out, a pi match with Q of 12 to get to 50 ohms needs

Cin = 4nF (rated 4kV plus) 
L = 361uH
Cout 23.3nF	Rated 500V.

The first one is slightly tricky, but high voltage ceramic caps up to
10kV do exist up to a few nF do exist, so connect them in parallel to
tune.  Cout is no problem.  The inductor could be 140 - 150 turns of 2mm
wire on an 80mm diameter former.  Get hold of some Litz wire from old
Decca transmitter loading coils.   The DC choke will be interesting
though.   An LOT of turns on a ferrite core, and remember it has to be
gapped or a dust core as it has DC flowing.  Alternatively feed in the
DC through a more modest choke at the 50 ohm point in which case Cout
has to be rated at 3kV and another blocking cap of say 100n rated 3kV is
needed.

Alternatively find the biggest ferrite core suitable for switch mode PSU
you can lay your hands on and wind an output transformer. Even stack
cores if you have to.   Minimum number of turns for a given ferrite core
area is given by :   N = Vrf(RMS) / (4.44. F . A . B)
Using B = 0.2 Tesla (suitable for most SMPSU ferrite materials), A = 300
x 10^-6 m^2 for a large SMPSU core and V = 3kV, at 137kHz gives minimum
number of turns of just 55.  Transformation ratio = SQRT(3300 / 50) =
8.2 : 1   Remember the winding has to be insulated for 3 - 4kV and DC
flowing through it could present a problem of saturation, so monitor
core temperature carefully. 100deg is usually OK provided the wire can
take it.  You will also need an output low pass filter but component
values here are a bit less restrictive.

It is all a lot easier, even at the 1kW level, with solid state devices.

Andy  G4JNT

> ----------
> From: 	Gasparik Richard[SMTP:Richard.Gasparik@siemens.sk]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-08 10:18
> To: 	Rsgb_Lf_Group (E-mail)
> Subject: 	LF: LF PA with tube...
> 
> Hi all...
> 


-- 
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: "g3kev" <g3kev@netscapeonline.co.uk>
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There is an on/off (A1A)keyed reversals transmission on 138.15 khz. This
is possibly a fixed frequency ionospheric sounder. I could also hear it
in GI. Can anyone else hear it ?
de G3KEV





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "M & S" <sovergne@club-internet.fr>
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Hi Mal & group,

I can hear 'something', but not strong enough to be readable.

73, Mark, F6JSZ

---

http://perso.club-internet.fr/sovergne

---

g3kev a *crit :
> 
> There is an on/off (A1A)keyed reversals transmission on 138.15 khz. This
> is possibly a fixed frequency ionospheric sounder. I could also hear it
> in GI. Can anyone else hear it ?
> de G3KEV


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Tune to 137.60kHz and use Spectran set at Resolution 0.125Hz and 
speed about one fifth from bottom of scale - 
and tell us what you see!








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave" <dave@picks.f9.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <2000060818414368199@zetnet.co.uk>
Subject: LF: Re: Re: Mystery
Date: Thu, 8 Jun 2000 22:00:35 +0100
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Yes I noticed that...
Looks like sawteeth on Spectrogram but in little steps rather than smooth
drift.
About S7 here.

Dave G3YXM


> Tune to 137.60kHz and use Spectran set at Resolution 0.125Hz and
> speed about one fifth from bottom of scale -
> and tell us what you see!
>
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Gaspard De Wilde" <on4zk@vt4.net>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Re: Mystery
Date: Thu, 8 Jun 2000 23:19:22 +0200
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hello  
I remark a broad band about 8Hz width centert around  137600 hz
 some intensity modulation on???????
-----Oorspronkelijk bericht-----
Van: Peter Dodd <g3ldo@zetnet.co.uk>
Aan: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Datum: donderdag 8 juni 2000 21:12
Onderwerp: LF: Re: Mystery


>Tune to 137.60kHz and use Spectran set at Resolution 0.125Hz and 
>speed about one fifth from bottom of scale - 
>and tell us what you see!
>
>
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Copying Slow CW by Ear
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Bill VE2IQ announced his new time-crunching software Thursday for recording 
QRS transmissions via the sigma-delta converter and playing them back at an 
accelerated rate through a regular PC sound card for conventional aural 
"decoding."

The text of the announcement is available at:
http://lwca.org/miscdocs/crunch.htm
It contains links to download the software.

73,
John  KD4IDY



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This interesting post appeared on the lowfer mailing list last night. It gives
more information on the CRUNCH program.

Stewart G3YSX

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Dick Rollema wrote:

> To All from PA0SE
>
> Walter Blanchard quoted the RACAL expert who has in the past  designed the
> Decca antennas as follows:
>
> >(...)  If the small one has an assymetric horizontal component (flat-top)
> > this will complicate matters considerably since it will radiate both
> > vertical and
> > horizontally-polarised and there will be interaction between them that
> > will affect the radiation pattern. So it would be unlikely to have a
> circular
> > polar pattern and this might account for some of the observed variations.
>
> This is not confirmed by computer simulation.
>

Shouldn't you say "Computer simulations do not model this". Decca did a lot of
measurements when they developed Navigator, and the physics always has the last
word. The question should therefore be "what is wrong with the computer model?"

Stewart G3YSX



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Yesterday evening I suggested that you all try and look for the 
mystery signal on 137.60kHz

There were a couple of reports but no one guessed what it was.

How about trying again tonight


Use Spectran set at Resolution 0.125Hz and speed about one fifth from 
bottom of scale. Let it integrate for at least half a page. It might 
also work using Spectrogram on similar settings.

Tell us what you see!



-- 
Regards, Peter, G3LDO

<g3ldo@zetnet.co.uk>






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Gasparik Richard" <Richard.Gasparik@siemens.sk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: [Fwd: [Lowfer] New software available for copying weak QRS-CW]
Date: Fri, 9 Jun 2000 14:11:14 +0200
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Hi LF-ers...

That's great...easy to copy va3lk.wav...no problem.
Congrats to such a good idea.
Best regards...and have a nice weekend.

Rich OM2TW

> -----Original Message-----
> From:	Stewart Bryant [SMTP:stewart.bryant@virgin.net]
> Sent:	9. jún 2000 8:18
> To:	rsgb_lf_group@blacksheep.org
> Subject:	LF: [Fwd: [Lowfer] New software available for copying weak
> QRS-CW]
> 
> This interesting post appeared on the lowfer mailing list last night. It
> gives
> more information on the CRUNCH program.
> 
> Stewart G3YSX << Message: [Lowfer] New software available for copying weak
> QRS-CW >> 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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> > This is not confirmed by computer simulation.
> >
>
> Shouldn't you say "Computer simulations do not model this". Decca did a
lot of
> measurements when they developed Navigator, and the physics always has the
last
> word. The question should therefore be "what is wrong with the computer
model?"
>
> Stewart G3YSX

The computer did not simulate the Decca mast but the small L-antenna used by
Jim.

73, Dick, PA0SE



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: 137.600.....Hell its Andy
Date: Fri, 9 Jun 2000 17:24:39 +0100
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Hi Peter, yes the secret is having the scroll rate rate ....good 'O' signal
here just after 1600z.....interesting.
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: "Alan Melia" <Alan.Melia@btinternet.com>
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Subject: LF: 137600 ....more..
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Hi all the only trouble is that a lot of us use LSB on 136 to drop DCF39
over the edge of the filter.......this results in and upside down
message....literally.

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: "Andy Talbot" <drassew2@interalpha.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: 137600 ....more..
Date: Fri, 9 Jun 2000 21:46:53 +0100
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In that case, use vertical scrolling and turn your head sideways, that gives
the proper mirror image doesn't it ?
I'm not turning it upside down !

Andy

-----Original Message-----
From: Alan Melia <Alan.Melia@btinternet.com>
To: rsgb_lf_group <rsgb_lf_group@blacksheep.org>
Date: 09 June 2000 21:39
Subject: LF: 137600 ....more..


>Hi all the only trouble is that a lot of us use LSB on 136 to drop DCF39
>over the edge of the filter.......this results in and upside down
>message....literally.
>
>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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> Hi all the only trouble is that a lot of us use LSB on 136 to drop DCF39
> over the edge of the filter.......this results in and upside down
> message....literally.

How do you use the Spectran frequency scale when you are on LSB?

If you tune the receiver to 137kHz USB then the scale on Spectran is meaningful
For example 137kHz on the Rx,  plus a Spectran reading of 600  = 137.600kHz.

The receiver is set to SSB bandwidth and any strong out of band 
signal can be attenuated using the IF SLOPE TUNING.

This seems simple to me - but is there a better way?

The TS-850 has a 1Hz tuning resolution but a 10Hz readout resolution. 
The fix is the set the receiver frequency at the point where it 
changes from 136.99 to 137.00. 

-- 
Regards, Peter, G3LDO

<g3ldo@zetnet.co.uk>








From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Peter, 
The secret is to be patient. My first reaction was there was nothing there, 
but after waiting a whole page, all was revealed. It reminds me of sky
writing.
I hope that Andy is going to explain to us all, what it is all about, i.e. 
is it just fun or is there a serious purpose? Nothing wrong with fun by the 
way. 
It is interesting how it varies in intensity with time of day. At 17.00
today, it was very clear, but by 22.30 had faded considerably.

                     John, G4CNN 





_______________________________________________________
Get 100% FREE Internet Access powered by Excite
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To: rsgb_lf_group@blacksheep.org
From: les@highnoonfilm.com
Subject: Re: LF: Copying Slow CW by Ear
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At 12:27 AM 6/9/00 EDT, you wrote:
>Bill VE2IQ announced his new time-crunching software Thursday for recording 
>QRS transmissions via the sigma-delta converter and playing them back at an 
>accelerated rate through a regular PC sound card for conventional aural 
>"decoding."
>
>The text of the announcement is available at:
>http://lwca.org/miscdocs/crunch.htm
>It contains links to download the software.
>
>73,
>John  KD4IDY


John,

I may QSY my beacon, XMGR to 187.500khz. I need to know if that's
a clear frequency for you. According to my computer, you're only
129 miles from my location, so you may be my best bet for 
a reception this fall.

Les Rayburn, KT40Z
4919 Cox Cove
Helena, AL 35080
(205) 253-4867 CELL




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andy Talbot" <drassew2@interalpha.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Re: Mystery
Date: Sat, 10 Jun 2000 09:35:08 +0100
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Peter has asked me for a write up for the LF Book, so full details will
appear there.  But basically it was a bit of fun to show how something can
be done with a DDS in real time other than just using it as a simple
frequency source.

The mode is more commonly known as Hellschreiber, or at least one of its
varients,  and is available for Soundcard and EVM with an SSB transmitter
(with transverter for LF).  However, that is a wide band system using up to
1kHz bandwidth.   What I did was take the technique a stage further and use
a DDS to generate a narrow band version for use with Spectran.  It can go
narrower, in fact today I may try a 5 Hz version.  DSP derived versions can
transmit the tones in parallel, leading to proper vertical lines, but need
linear transmitters.  This one -at-a-time frequency version is called
Sequential Multi Tone Hellscheiber or SMT Hell.    Hellschreiber comes
within the term "Fuzzy Modes"  like SLOWCW etc where there is a crossover
between data and human interpretation.

See how it compares with medium speed CW  - whatever would be transmitted in
10 Hz bandwidth.

I'll change to a 5 Hz version around Midday today

Incidently, to save tying up a useful computer just generating a message
repeatedly, I've pressed an ancient 10MHz 286 Laptop into service.   Who
needs Pentium 400s for Data comms ?

Andy  G4JNT


-----Original Message-----
From: john sexton <computernetworks@excite.com>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 09 June 2000 23:12
Subject: LF: Re: Mystery


>
>Hi Peter,
>The secret is to be patient. My first reaction was there was nothing there,
>but after waiting a whole page, all was revealed. It reminds me of sky
>writing.
>I hope that Andy is going to explain to us all, what it is all about, i.e.
>is it just fun or is there a serious purpose? Nothing wrong with fun by the
>way.
>It is interesting how it varies in intensity with time of day. At 17.00
>today, it was very clear, but by 22.30 had faded considerably.
>
>                     John, G4CNN
>
>
>
>
>
>_______________________________________________________
>Get 100% FREE Internet Access powered by Excite
>Visit http://freelane.excite.com/freeisp
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andy Talbot" <drassew2@interalpha.co.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: SMT-Hell on 137.6kHz
Date: Sat, 10 Jun 2000 12:22:09 +0100
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The signal is now running using a 5 Hz bandwidth on 137.6kHz.
Change Spectran settings to 0.06 Hz resolution and adjust the speed control
for best looking copy.   Be patient....
Each pixel is timed for 1.2 seconds with an 8x8 Font.

Andy  G4JNT



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave" <dave@picks.f9.co.uk>
To: rsgb_lf_group@blacksheep.org
References: <000901bfd2ce$57620200$2fe11ac3@g4jnt>
Subject: LF: Re: SMT-Hell on 137.6kHz
Date: Sat, 10 Jun 2000 12:54:00 +0100
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Andy et al.

Some screenshots are at http://www.picks.f9.co.uk/newspic22.htm
I left the bandwidth at 0.12 and slowed down the scan for the 5Hz version
and it still looks cleaner than the 10Hz.

Dave G3YXM.


> The signal is now running using a 5 Hz bandwidth on 137.6kHz.
> Change Spectran settings to 0.06 Hz resolution and adjust the speed
control
> for best looking copy.   Be patient....
> Each pixel is timed for 1.2 seconds with an 8x8 Font.
>
> Andy  G4JNT
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 10 Jun 2000 08:46:10 -0400 (EDT)
From: "Bill de Carle" <ab196@valleynet.on.ca>
To: rsgb_lf_group@blacksheep.org
Subject: LF: My ISP having difficulties
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My apology to anyone trying to download the CRUNCH software from my
regular webpage www.ietc.ca/home/bill/bbs.htm - my local ISP,
ietc.ca was bought out by another company (COGECO) recently and
it seems they are having difficulties getting things changed over.

I have been unable to send or receive e-mails from my regular
account over the past few hours and no doubt the web page at
ietc is inaccessible as well.

Hope they get it all sorted out soon.
Sorry for the difficulties.

Bill VE2IQ





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Andy,
Thanks for the explanation. As I am sure you know HellSchreiber, means
Bright Writer, which this certainly is.
This PM noticed that it had reduced to 5 Hz, so I decreased the resolution
to 0.064 and the speed to one division (approx 1/12). It is just as legible
as before. However I am noticing a long period fading and recovery of some
hours.
73
John, G4CNN





_______________________________________________________
Get 100% FREE Internet Access powered by Excite
Visit http://freelane.excite.com/freeisp



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 10 Jun 2000 11:18:21 -0400 (EDT)
From: "Bill de Carle" <ab196@valleynet.on.ca>
To: rsgb_lf_group@blacksheep.org,  lowfer@qth.net
Subject: LF: CRUNCH V2.1
Message-ID: <Pine.LNX.3.91.1000610111330.8305A-100000@valley1.valleynet.on.ca>
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CRUNCH V2.1 is up on my web page at IETC.CA -
Even though most DNS's will tell your browser that www.ietc.ca does
not exist, I found you can still download it (at least for a while)
by connecting with the IP address, bypassing your nameserver.

Just tell your browser to go to 24.226.220.15/home/bill/bbs.htm

It works for me!

And you will probably get very good download performance because
I kinda doubt anyone else is accessing web pages on IETC today :-)

Bill VE2IQ




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 10 Jun 2000 19:46:19 +0100
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Re: Re: Mystery
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In message <28540596.960642412155.JavaMail.imail@bubbles.excite.com>,
john sexton <computernetworks@excite.com> writes
>
>Hi Andy,
>Thanks for the explanation. As I am sure you know HellSchreiber, means
>Bright Writer, which this certainly is.

I thought it was because it was invented by Dr. Hell. A rare German pun,
perhaps?

Mike
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000e01bfd327$7fb1b080$659101d5@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: SMT-Hell and Spectran.
Date: Sat, 10 Jun 2000 22:59:58 +0100
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Hi all, cor I have a pain in the neck (or do I mean I am being a pain in the
neck?) I have to drink me beer through a straw now Andy. I decided an easier
way was to relearn a skill I developed many years ago when I worked in
London and was too mean (or too late ) to buy a paper before boarding the
tube-train. I got very good at reading upside-down.....Its a skill you never
forget...bit like morse I suppose....just need to practice it. The 5Hz
signal was readable all day and only started to get difficult after dark as
the noise came up. I found I needed a time-scale of 3000 and 5.5k sample
rate, with 16k points on Spectrogram which may be why some didn't decode it

Peter I run the rx permanently on 138.100kHz LSB and put and offset into
Spectran (the latest build) The problem is the RX is in a different room to
the PC running Win95 and Spectran. I dont use narrow filters for the PC
modes as if doesn't help, but I can listen on the PC speaker to other QSOs
and CQs up the band. I just find that LSB gives the best 'whole band' view
that way which I monitor on FFTDSP4 alongside the radio. That is sensitive
enough to show traces from signals I cannot read, with the 500Hz filter and
the outboard 80Hz audio filter. FFTDSP4 doesn't have an offset so I have a
paper scale pasted to the monitor screen surround.

Great fun and some nice pictures for the next time I have to give a Club
talk.
Does anyone run the mechanical Hell' in this country? I think I once saw one
in action many years ago. From memory the display was produced by a
continously rotating helix which was brought into contact with the moving
paper strip by a solenoid. Quite ingenious!

Cheers de Alan G3NYK
Alan.Melia@btinternet.com




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From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: rsgb_lf_group@blacksheep.org
Cc: "Koos Fockens, PA0KDF" <K.Fockens@iaf.nl>
References: <000e01bfd327$7fb1b080$659101d5@default>
Subject: LF: Re: Hellschreiber
Date: Sun, 11 Jun 2000 09:39:57 +0200
Organization: Freeler
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> Does anyone run the mechanical Hell' in this country? I think I once saw
one
> in action many years ago. From memory the display was produced by a
> continously rotating helix which was brought into contact with the moving
> paper strip by a solenoid. Quite ingenious!
>
> Cheers de Alan G3NYK
> Alan.Melia@btinternet.com

Hello Alan and others,

There are several ones in your country Alan, eg at the Science Museum.

I also worked G's using a machine, for instance the late G5XB and others
whose calls I  can't remember.

I have one on "permanent" loan from PA0AOB and are using it on the air
since 1976.

There is a  Hellschreiber meeting on Sundays at 14.30 UTC (in winter 15.40
UTC) at about
3580kHz using the "Feldhell" system.

You can learn a lot about the Hellschreiber by visiting one of the
websites of Murray Greenman, ZLBPU, for instance:

http://www..qsl.net/zl1bpu/FUZZY/History/history.html

Software for it can be downloaded from

http://www.qsl.net/zl1bpu/FUZZY/starting.html

Murray can be contacted at  as149@detroit.freenet.org

An informative article on the Hellscreiber by ZL1BPU can be found in QST
January 2000: "Let's See you in Hellschreiber". It contains a photograph of
"my" machine.

73, Dick, PAoSE







From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Sorry no Cluster spots for June 10/11 from GB7DXM
Date: Sun, 11 Jun 2000 21:33:32 +0100
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Hi All, there are no Cluster spots for LF on my local Cluster node again
this week. There has been a lot of static , and there seemed very little
activity this morning. Roll on the autumn (well maybe not TOO quickly!)

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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To: rsgb_lf_group@blacksheep.org
From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: LF: Signal Strength Measurements by OH2LX, 12 June 2000
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Signal strength measurements of various LF stations by OH2LX:
------------------------------------------------------------------
Day ------------------   05Jun 06Jun 07Jun 08Jun 08Jun 10Jun 11Jun
                          MON   TUE   WED   THU   FRI   SAT   SUN 
Time, UTC ------------    2045- 2015- 2100- 2045- 2055- 2040- 2055-
------------------------------------------------------------------
kHz    Stn   d,km  AZI          Indicated ESH2 input, dBmW
------------------------------------------------------------------
 68.9 DHJ58? 1115, 242   -105  -101   -98  -104   -98  -104   -99
------------------------------------------------------------------
 73.3 Rugby, 1825, 252,  -105  -106  -105  -104   Nil  -105  -105
------------------------------------------------------------------
 75.0   HBG, 1992, 226,  -102  -107  -108  -104   -97  -107  -105
------------------------------------------------------------------
 77.5 DCF77, 1543, 228,   -90   -94   -93   -89   -87   -93   -92
------------------------------------------------------------------
128.9 DCF49, 1544, 228,   -92   -93   -85   -94   -91   -93   -88
------------------------------------------------------------------
138.8 DBF39, 1221, 226,   -86   -92   -84   -90   -85   -91   -89
------------------------------------------------------------------
135.8   SXV, 2490, 182,  -108  -108  -105  -111  -104  -105  -107
------------------------------------------------------------------
137.0   CFH, 5750, 295,   Nil   Nil   Nil   Nil   Nil   Nil   Nil
------------------------------------------------------------------
(R&S ESH2/---- 10m coax----/1:10/-----15m wire-----):
 Noise level with antenna: with 200Hz IF BandWidth: 
-24..-20 dB(uV), -131..-127dBmW (varies with frq, qrm, qrn etc)
------------------------------------------------------------------
End of message of 12th June 2000, 0700 UTC, from OH2LX
------------------------------------------------------------------
------------------------------------------------------------------
DISCUSSION: In RadCom May 2000, (p 95) "the last Word" C J Osborne,
G3XIZ writes about "Watt Nonsense" and suggests: "Ditch dBW and
use watts...". In RadCom June 2000 Peter Chadwick, G3RZP comments
under caption: "The much Maligned dBW"; G3RZP writes: "..it (dBW)
came from the use of dBm for measuring receiver sensitivity, which
originated from the radar/electronic warfare community, where
matched impedances and received powers were the major parameters
of interest ..... dBm is the power in decibels relative to 1mW,
which would be provided to the equipment if the load impedance
was 50 ohms - a lot of assumptions...".

OH2LX: Actually there is no reason to tabulate my measurements
in dBmW. I wouldn't even dream of using "received power" unless
I use for measurements a genuine MEASURING RECEIVER, an R&S ESH2.

Note: In my case approximate field strength (around 136 kHz) is:
F-s (dBuV/m) = dBmW + 127dB,  e.g. -127dBmW + 127dB = 0 dBuV/m.
(have not yet attempted to calibrate it around 70-80 kHz).
----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


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: Mon, 12 Jun 2000 04:56:34 EDT
Subject: LF: Decca Users Group?
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I understand there are now several reflector members who now own ex-Decca 
Transmitters.

Is anyone interested in a temporary 'Decca Users group' for the purposes of 
exchanging information on modifying the transmitters for use on the amateur 
LF bands?

I hope to have my one operational by this Friday!  (Unrealistic enthusiasm) 
and would like to exchange thoughts on calamity avoidance.

73

David



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: 137600 ....more..
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> 
> > Hi all the only trouble is that a lot of us use LSB on 136 to drop DCF39
> > over the edge of the filter.......this results in and upside down
> > message....literally.
> 
> How do you use the Spectran frequency scale when you are on LSB?
> 


I use LSB for this reason, too, and had troubles with Andy's Hell 
until I twigged that a dot at the top of a series of symbols probably 
wasn't right.

As for using the frequency scale on Spectran or Spectrogram. I 
just wouldn't do it. The simplest way of calibrating your receiver is 
to put VFO 1 on 60.000kHz, adjust Spectran or your RIT so that 
the signal appears in a convenient place on the screen (say, 
600Hz), then switch to VFO 2. When the dial says 137.700kHz 
any signal on that frequency should appear at 600Hz on the 
screen. This assumes a 1Hz read-out of course, but it does 
eliminate all calibration errors and you don't have to set the receiver 
or Spectran to a wide setting to make it work.

Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 15:25:26 +0200
From: "Valerio Gabbani" <valerio@dii.unisi.it>
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Hello all,
i got an object that seems to be a TXCO but i need some info about how
to use it.
The manufacturer is Siemens, the device looks like e black
cilinder,diameter about 6.5 cm and 9 cm high, with a 9 poles circular
male connector (similar to octal type) on the bottom and on the top the
following inscription:

"Siemens
Schwingquarz-thermostat
4,000000 Mhz
70° C   20V 14W
Q91502-A4000-E-1".

If there is someone reading the reflector that knows  the output
connector pin map please tell me !

Thanks in advance

'73, Valerio (IK5ZPV)



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: MarkusVester@aol.com
Message-ID: <9c.48eaab3.26764cbb@aol.com>
Date: Mon, 12 Jun 2000 10:24:59 EDT
Subject: LF: Chirped MT-Hell and Fourier-SSTV
To: rsgb_lf_group@blacksheep.org
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Hi Geri, hi group,

encouraged by the "Mystery Signal" discussion, I had an enjoyable qso with 
DK8KW  today, sending out a couple of pictures around 137.73 kHz. I had been 
experimenting with fourier image transmission for a while.

The modulation I used is similar to parallel multitone hell (MT Hell) as 
described on ZLBPU's page. For n lines and a column duration of T only the 
optimal total bandwidth of n/T is required. It's disadvantage is a linear 
transmitter with a high crest factor (peak to average ratio), as for a bright 
vertical line all the energy is concentrated in a narrow sin(t)/t pulse, only 
T/n long. 

As phase is not displayed in the received spectrograms, a chirp filter can be 
used to smear out the same energy over the symbol time T, reducing peak power 
by a factor of n for chirped multi-tone (CMT). Its easy and efficient to 
apply a quadratic phase term to the image intensity before the FFT.

For a full white image, the resulting sweep signal looks similar to the SMT 
(sequential multitone) mode Andy used in his experiments. But for a single 
horizontal line, SMT would transmit a series of full-power pulses of  short 
duration T/n. To separate these spectrally, the rx would have to use a 
bandwidth of n/T for each channel, or n*n/T for the full image height. Thus, 
SMT is less bandwidth-efficient by that factor of n compared to MT or CMT. 
This makes CMT interesting for fast "high resolution" grey-scale image 
transfer like the 64*64 pixel portraits I have sent to Walter and Geri.

So, where's the catch, besides the linear tx? Theoretically, there could be a 
"reversed chirp" luminosity pattern in the image, refocussing all the smeared 
energy into a high peak. For random images, the crest factor would be on the 
order of sqrt(n) regardless of any phase modulation scheme. But as pixel 
values are always positive, the image has a strong spatial zero-frequency 
component, and thus chirping still helps. Practically I found that an extra 
6dB dynamic headroom was usually sufficient. When precalculating the sound 
data, one could always scale them down or try a reversed chirp direction.  

In the current implementation, a QBasic program transforms a bmp image to a 
1MB wav file. I can play this to my SSB rig with a second instance of gram 
using "Scan File", while leaving the "Scan Input" monitor running. Due to 
limited FFT size (8192) and playback sample rate (11025 Hz), minimum 
bandwidth is 1.3 Hz per line. Its fast, but too wide for the LF qrss band and 
rather tall on an 86 Hz display, so I will try to use 64*0.33 Hz in the 
future.

So much for now, 73 cu
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: Mon, 12 Jun 2000 10:25:10 EDT
Subject: LF: Russian ALPHA qrt ?
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Hello group,

yesterday I checked the very low end and wondered that I didn't see a trace 
of the familiar ALPHA beeps. Today nothing either on any of their qrgs 
11.905, 12.089, 12.667 and 14.88 kHz. With precise GPS, are they finally gone 
for good now, following the fate of OMEGA? Hearing all four beacons certainly 
was an excellent rx test, but natural-radio listeners will probably enjoy the 
lack of qrm. One I would NOT miss would be the 124 kHz DGPS service from 
Mainflingen with all its noisy intermodulation...

73s de Markus, DF6NM 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 17:45:44 +0300
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From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: Re: LF: Russian ALPHA qrt ?
In-reply-to: <c1.40d85f4.26764cc6@aol.com>
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Hello Markus and others,

It has been common to Alpha since 1970
to be qrt for shorter and longer periods.
The 5th Alpha station Seydi has been off
air totally but even Revda has been on.
A while ago I thought Mars-75 went qrt
but after a few days it came back.
73 de Vaino, OH2LX








At 10:25 12.6.2000 EDT, you wrote:
>Hello group,
>
>yesterday I checked the very low end and wondered that I didn't see a trace 
>of the familiar ALPHA beeps. Today nothing either on any of their qrgs 
>11.905, 12.089, 12.667 and 14.88 kHz. With precise GPS, are they finally
gone 
>for good now, following the fate of OMEGA? Hearing all four beacons
certainly 
>was an excellent rx test, but natural-radio listeners will probably enjoy
the 
>lack of qrm. One I would NOT miss would be the 124 kHz DGPS service from 
>Mainflingen with all its noisy intermodulation...
>
>73s de Markus, DF6NM 

----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 13:19:13 -0400
From: "'Geri' Kinzel, DK8KW" <DK8KW@compuserve.com>
Subject: LF: Re: LF Chirped MT-Hell and Fourier-SSTV
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Hello LF-friends,

a picture of Markus', DF6NM's transmission in Slow-Hell can be found at

                http://www.qru.de/df6nm-hell.html

Best 73

Geri, DK8KW (W1KW)
http://www.qru.de


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 10:28:25 -0700 (PDT)
From: "john sexton" <computernetworks@excite.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: HellSchreiber
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Hi Mitch and All,

Mitch VE3OT wrote that HellSchreiber is named after the inventor, Dr. Hell.

You are of course right Mitch. It just goes to show how a little knowledge
is a dangerous thing, hi! I thought I knew German reasonably well. My only
defence is that the family name Bright is also common in English. Maybe it
was indeed meant to be a pun as you suggest? Who knows what was in his mind
when he named it? The name reminded me of what we used to call Legible Text,
which we puched at the beginning of our Computer tapes, although we became
quite proficient at reading ASCII on paper tapes. This was a long time ago,
when computers were rare and viewed as electronic brains, instead of as
glorified typewriters for modern secretaries.

John, G4CNN





_______________________________________________________
Get 100% FREE Internet Access powered by Excite
Visit http://freelane.excite.com/freeisp



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 10:30:05 -0700 (PDT)
From: "john sexton" <computernetworks@excite.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: RTTY station
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Hi All,

Can anyone tell me what the RTTY station on 136.648 is? This appears to be
the spacing frequency, and there appears to be a marking frequency only 20
Hz lower.

John, G4CNN







_______________________________________________________
Get 100% FREE Internet Access powered by Excite
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Guido Roels" <on6rl@pi.be>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Audio filters
Date: Mon, 12 Jun 2000 20:20:08 +0100
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Hello everyone,

Lately I obtained two AF filters. 
One is marked as:

     FILTER BAND PASS
     5915-99-920-1117
     500 C/S  TX & RX

The other one:

     FILTER BAND PASS
     5915-99-920-1118
     700 C/S  TX & RX

Dimensions about 8cm cube and with a DB-9 male connector fitted on top.
As they are painted in the well known RACAL RA-17 green I suppose they 
are RACAL origin.
I have measured the B/W and it's about 180Hz by 6dB when connected to
600R.

Anyone in the group who knows more about this specimen?

Best regards,

Guido, ON6RL.





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 21:48:04 +0100
To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: LF: Russian ALPHA qrt ?
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Hi Markus,

The Alpha operators probably haven't paid their electricity bill.
There were three Russian high-ups at a conference I went to
recently who had some say in operating that system and they
said that when it came to a choice between paying their salaries
and paying the electricity guess which won! Also said they
were having some problems keeping Chaika on the air for the
same reason.

Walter G3JKV.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 21:41:08 +0100
To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: LF: Decca Users Group
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G0MRF wrote:

>I understand there are now several reflector members who now own ex-Decca
>Transmitters.
>
>Is anyone interested in a temporary 'Decca Users group' for the purposes of
>exchanging information on modifying the transmitters for use on the amateur
>LF bands?
>
>I hope to have my one operational by this Friday!  (Unrealistic enthusiasm)
>and would like to exchange thoughts on calamity avoidance.

I've been asking those who get one to do just this - did I miss you
on Sunday, David?  I can get to the guys who designed them if
necessary so just put queries on this reflector, and if nobody else can
answer I'll buy them a beer and get "horses' mouth" advice.
We ex-Decca narks meet once a month at a local pub.

Walter G3JKV.



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 12 Jun 2000 20:01:42 +0100
To: rsgb_lf_group@blacksheep.org
From: "M.J.Powell" <mike@pickmere.demon.co.uk>
Subject: Re: LF: Re: HellSchreiber
References: <18823271.960830905371.JavaMail.imail@bubbles.excite.com>
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In message <18823271.960830905371.JavaMail.imail@bubbles.excite.com>,
john sexton <computernetworks@excite.com> writes
>Hi Mitch and All,
>
>Mitch VE3OT wrote that HellSchreiber is named after the inventor, Dr. Hell.
>
>You are of course right Mitch. It just goes to show how a little knowledge
>is a dangerous thing, hi! I thought I knew German reasonably well. My only
>defence is that the family name Bright is also common in English. Maybe it
>was indeed meant to be a pun as you suggest? Who knows what was in his mind
>when he named it? The name reminded me of what we used to call Legible Text,
>which we puched at the beginning of our Computer tapes, although we became
>quite proficient at reading ASCII on paper tapes. This was a long time ago,
>when computers were rare and viewed as electronic brains, instead of as
>glorified typewriters for modern secretaries.

Not Mitch. Twas me!

Mike
-- 
M.J.Powell


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: rsgb_lf_group@blacksheep.org
Date: Mon, 12 Jun 2000 18:57:47 -0400
Subject: Re: LF: 137600 ....more..
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FYI  Mikes method is the same one I use. The receiver I use for an IF has
a variable
Offset which I attempt to keep at 600 Cycles. However over time the Knob
gets moved
I have always made it a routine when checking something new to do a 60
Khz check before
looking at the specific frequency I wish to check.  Gives that little
added
confidence     HI

Bob


>ju>to put VFO 1 on 60.000kHz, adjust Spectran or your RIT so that 
>the signal appears in a convenient place on the screen (say, 
>600Hz), then switch to VFO 2. When the dial says 137.700kHz 
>any signal on that frequency should appear at 600Hz on the 
>screen. This assumes a 1Hz read-out of course, but it does 
>eliminate all calibration errors and you don't have to set the 
>receiver 
>or Spectran to a wide setting to make it work.
>
>Mike, G3XDV (IO91VT)
>http://www.dennison.demon.co.uk/activity.htm
>
>


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
Subject: LF: Surplus 5 MHz frequency standards?
Date: Mon, 12 Jun 2000 19:12:25 -0400
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Greetings:

Recently on this reflector there was reference to the availability of some 5
MHz frequency standards.  An issue has come up here and I sure could use an
extra standard to make life a little easier on a small side project.  If any
of those surplus items are still available I sure would like to get a price
ASAP.

Larry
VA3LK





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Date: Mon, 12 Jun 2000 23:39:43 -0500
Subject: Re: LF: Re: HellSchreiber
From: "Mitch Powell" <PowellM@claven.fanshawec.on.ca>
To: rsgb_lf_group@blacksheep.org
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>>
>>Mitch VE3OT wrote that HellSchreiber is named after the inventor, Dr. Hell.

> Not Mitch. Twas me!
>
> Mike
> --
> M.J.Powell

Thanks for the correction Mike - appreciate the confirmation that
my mind was not slipping !!

Mitch
> 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 13 Jun 2000 09:37:36 +0300
To: rsgb_lf_group@blacksheep.org
From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: Re: LF: Russian ALPHA qrt ?
In-reply-to: <4.2.0.58.20000612214414.0097dd50@mail.pncl.co.uk>
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Walter,

You are no doubt right about the reason for
Alpha etc qrt, I know one Russian captain...
Four Alpha stations were on and off during the
first four months of 2000, including Revda.
The official USSR name for Alpha is RSDN-20
where D stands for long-range (dalnoye).
 
Russians place Mars-75 system in its own
category "sinteziruyemim" and my old friend
suggested that Decca also is a "synthesized"
system, I always thought Decca belongs to
"cw hyperbolic" category, What say?
Loran is a "(im)pulse hyperbolic" system.
In Mars all the other frequencies are said
to be "synthesized" from the main frequency.
The Russian language is not very easy...
73 de Vaiski




At 21:48 12.6.2000 +0100, you wrote:
>Hi Markus,
>
>The Alpha operators probably haven't paid their electricity bill.
>There were three Russian high-ups at a conference I went to
>recently who had some say in operating that system and they
>said that when it came to a choice between paying their salaries
>and paying the electricity guess which won! Also said they
>were having some problems keeping Chaika on the air for the
>same reason.
>
>Walter G3JKV.

----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <002301bfd518$5d450900$290e35d5@w8k3f0>
From: "Dick Rollema" <d.w.rollema@freeler.nl>
To: "LF-Group" <rsgb_lf_group@blacksheep.org>
Cc: "Murray Greenman" <as149@detroit.freenet.org>, 
 "Koos Fockens, PA0KDF" <K.Fockens@iaf.nl>,
 "Cas Caspers, PA0CSC" <cas.caspers@hetnet.nl>, 
 "Arthur Bauer, PA0AOB" <aobauer@compuserve.com>
Subject: LF: Fw: Hellschreiber History
Date: Tue, 13 Jun 2000 11:16:52 +0200
Organization: Freeler
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To All from PAoSE

In my e-mail of June 11 2000 9.39 I gave the URL of one of ZL1BPU's websites
on which the history of the Hellschreiber can be found.
When afterwards I tried to visit it there was no access.
Asking ZL1BPU what could be the cause of the failure Murray replied as
follows:

> Dick,
>
> The URL that was posted was wrong. It had an extra dot in it!
>
> This one definitely works, because I just tried it:
>
> http://www.qsl.net/zl1bpu/FUZZY/History/History.html
>
> And yes, your mechanical machine has it's picture there too.
>
> By the way, Mike KF4HEY are putting together a new and better "History"
> site, to be hosted by Mike. Look out for that when it is ready!
>
> 73,
>
> Murray ZL1BPU


I can fully recommend visiting the site; it  gives an excellent overview of
the Hell system of teleprinting.

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: Tue, 13 Jun 2000 12:18:34 +0100
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Subject: LF: Litz
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A couple of weeks ago, I connected up my ex-Puckeridge giant 
Litz coil (see my web site for a picture). I used a variation of the 
stripping/soldering method described by Jim, M0BMU. He 
recommended wrapping copper foil around the wires and then 
applying a blowlamp. I used kitchen aluminium foil which worked 
OK. The only failure I had was when I stripped too little of the PTFE 
insulation off  and the melting PTFE coated the wires with a black 
goo that was impossible to remove.

The resultant coils - they are all different; mine has four parallel-
wound windings - each had less than one ohm DC resistance. I 
connected up one winding, and the antenna (plus the coil at the top 
of the mast) resonated at 150kHz. Connecting another in series 
reduced the frequency to 88kHz. This is not the sort of coil you can 
tap so it was back to the old dustbin to supplement a single Litz 
coil. I haven't yet tried three windings to get to 73kHz. The built-in 
variometer changes the frequency by only a few kHz.

My antenna current has increased by 20 per cent and there is 
obviously a higher Q as I have had to prevent the pa from oscillating 
on key up.

When we were first experimenting with LF there was a lot of 
discussion about Litz wound inductors. The conclusion then was 
that any advantage would be small compared with earth and other 
losses. I think that was true, but it does show that once you have 
reduced the other losses as far as possible there is some 
advantage in going for a properly wound low-loss coil.

Next projects - a shed for the big loading coil (though perhaps one 
of those plastic luggage boxes that sit on top of cars would do) and 
a Litz-wound mast-head inductor.

Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Re: RTTY station
Date: Tue, 13 Jun 2000 15:47:51 +0100
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Hi John, I think Markus told me that was an intermod product from DCF39/42
...I will copy Markus's message direct to you John.
Cheers de Alan G3NYK
Alan.Melia@btinternet.com

-----Original Message-----
From: john sexton <computernetworks@excite.com>
To: rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date: 13 June, 2000 7:36 AM
Subject: LF: Re: RTTY station


>Hi All,
>
>Can anyone tell me what the RTTY station on 136.648 is? This appears to be
>the spacing frequency, and there appears to be a marking frequency only 20
>Hz lower.
>
>John, G4CNN
>
>
>
>
>
>
>
>_______________________________________________________
>Get 100% FREE Internet Access powered by Excite
>Visit http://freelane.excite.com/freeisp
>
>



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: Re: HellSchreiber
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Hi Mike,
Not my day for getting things right is it! Unfortunately I had deleted the
original E-mail and could only remember that it was M. Powell. Curiously
there are two of you!
Thanks for putting me straight.
John





_______________________________________________________
Get 100% FREE Internet Access powered by Excite
Visit http://freelane.excite.com/freeisp



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Tue, 13 Jun 2000 23:19:17 -0700 (PDT)
From: "wolfgang koenig" <dl1san@yahoo.com>
Subject: Re: LF: Sorry no Cluster spots for June 10/11 from GB7DXM
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Hallo Group,

we had some activity on LF last Monday (12. Jun)
morning. The band was quiet without static crashes. I
heared a few stations :

DJ2EY 559,
DL3FDO 559,
DJ1RL 559 in qso with df8zr 559,
DJ7RD 599,
DL0FTZ/P 549,
OZ8NJ 439

73 de dl1san Wolf


--- Alan Melia <Alan.Melia@btinternet.com> wrote:
> Hi All, there are no Cluster spots for LF on my
> local Cluster node again
> this week. There has been a lot of static , and
> there seemed very little
> activity this morning. Roll on the autumn (well
> maybe not TOO quickly!)
> 
> Cheers de Alan G3NYK
> Alan.Melia@btinternet.com
> 
> 
> 


__________________________________________________
Do You Yahoo!?
Yahoo! Photos -- now, 100 FREE prints!
http://photos.yahoo.com


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Peter Dodd" <g3ldo@zetnet.co.uk>
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The Industrial museum at Amberley put on 'theme' weekends, such as 
model steam engines or vintage cars etc. This coming weekend we are 
having a 'cats whisker' theme - some the vintage kit that the museum 
has is up and running. I have volenteered to operated an amateur 
station comprising the old 'breadboard' layout, probably on 7MHz. 
Hopefully there will be a demonstration of 40 line mechanical scanned 
TV. I have not planned to operate the LF station but that might change. 


-- 
Regards, Peter, G3LDO

<g3ldo@zetnet.co.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: Wed, 14 Jun 2000 12:45:33 +0000
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Dear LF group,
	Looking through my box of crystals recently, I found some 
operating in the range 30 - 40kHz. They are in glass envelopes, 
and I noticed that the metalisation on each side of the quartz plate 
is divided into two halves, giving four electrodes. On some units, all 
four electrodes are connected to seperate pins, while on others 
two diagonally oposite electrodes are commoned, giving only 3 
external connections. They look a little like 2 pole monolithic crystal 
filters, but have no bandwidth marked on them, and I have not 
heard of such filters being used at low frequencies.

Does anybody know how these 3 and 4 terminal crystals are 
used? Just curious really.

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Thu, 15 Jun 2000 09:36:03 +0100
To: rsgb_lf_group@blacksheep.org
From: "Brian Rogerson" <brian@esoterica.pt>
Subject: LF: Beacon on 2200m
Cc: alberto.dinis@icp.pt,  carlos.carvalho@icp.pt
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Goodmorning to all,

Having just finished assembling and adjusting the aerial tuning
and matching unit, I was wondering if some kind person would
transmit a beacon signal.  The band is exceptionally quiet now
after a fairly noisy night.  I cannot transmit since I am still
waiting for a license to be issued and the transmitter is not
complete.

73's de Brian, CT1DRP, IN51QD




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'" <rsgb_lf_group@blacksheep.org>
Subject: LF: The secret is out
Date: Fri, 16 Jun 2000 11:18:39 +0100
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Now that the 'mystery signal' of last week has been identified and
decoded by a number of people, I'll be transmitting Low Speed Sequential
Multi Tone Hellschreiber again this weekend on 137.6kHz, this time with
bandwidths of 20Hz and 2.5Hz.  Time duration per pixel will be scaled in
line with the frequency deviation in proportion to the tests last
weekend, so around 0.3s / pixel for the 20 Hz version and 2.5s for the
2.5Hz version.   These correspond to 19 seconds and 2.67 minutes per
character respectively.  Power will be in the 50 - 100 Watt region to
the antenna, giving 5 - 10mW (or probably less) ERP.

If anyone would like these parameters varied let me know on the other
EMail account G4JNT@ARRL.ORG or via the reflector and I hope to be able
to accomodate this. You can also try phoning on 01489 787424 but expect
to get an answering machine as I'll be in the garden most of the day
building a conservatory and getting irradiated by the RF fields from
overhead !

Unfortunately, Dave and Mike, LSB is not an currently an option, so for
now get a mirror / scroll vertically / practise reading back to front.
I could alter the software in the future for this mode though, or even
transmit USB and LSB simultaneously, one above the other.  Presumably
that becomes ISB.  

Three other fonts are available, a simple 5x7 font similar to the
original Hellschreiber one, though reported by G3LDO to be not as good
as the 8x8 I was using;  and larger 8x14 and 8x16 fonts which probably
have nothing to offer - on local strong signal copy anyway.

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.


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: EMail address correction
Date: Fri, 16 Jun 2000 15:09:57 +0100
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That should read    g4jnt@arrl.net 
 not .org as stated.

Andy  G4JNT

>If anyone would like these parameters varied let me know on the other
>EMail account ..........


-- 
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is private and is intended solely for the intended recipient(s).
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prohibited and may be unlawful.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sat, 17 Jun 2000 08:38:58 +0100
To: rsgb_lf_group@blacksheep.org
From: "Tom Boucher" <tom@telemetry.demon.co.uk>
Subject: LF: Cut short in mid-QSO!
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Hello LF Folk

I don't know if Bob G8RW monitors this reflector, if so, apologies for
disappearing mid QSO on 136KHz at 0715 Z this morning. We are having
some strong winds and my antenna must have blown against a branch, arced
and broken. So that's another job for this week-end!

73, Tom G3OLB


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "f5maf" <f5maf@free.fr>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Cut short in mid-QSO!
Date: Sat, 17 Jun 2000 14:53:21 +0200
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Hi Tom I have listened you this morning on 136.750 at 07:15AM with good
signal
on 2meters loop and 10 meters vertical antenna.
But I would like to record you but you had qrt (at about 07:20).

Best 73
Marc F5MAF JN03PP

-----Message d'origine-----
De : Tom Boucher <tom@telemetry.demon.co.uk>
À : rsgb_lf_group@blacksheep.org <rsgb_lf_group@blacksheep.org>
Date : samedi 17 juin 2000 10:15
Objet : LF: Cut short in mid-QSO!


>Hello LF Folk
>
>I don't know if Bob G8RW monitors this reflector, if so, apologies for
>disappearing mid QSO on 136KHz at 0715 Z this morning. We are having
>some strong winds and my antenna must have blown against a branch, arced
>and broken. So that's another job for this week-end!
>
>73, Tom G3OLB
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Cut short in mid-QSO!
References: <ks+XHAASsyS5EwrB@telemetry.demon.co.uk>
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Hi Tom,

Bob doesn't monitor the reflector, but I have relayed your
message to him.

Bob sends his 73, and hopes to work you again soon.

Regards to all,
Steve GW4ALG



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

What I presume was the 20Hz bandwidth signal transmitted in the morning, was
quite readable, but weak. How do we give reports for these transmissions?

The 2.5Hz bandwidth signal was bright and clear on Spectran around 17.00
local. The following settings worked well for me:
0.32 Hz resolution (finest)
Speed setting to second slot on scale from bottom.

John, G4CNN, Caversham, Reading (Not up on the hill beside the BBC
monitoring station, but down in a hollow, known locally as Bugs Bottom!)
Rx: AOR 7030 (CW setting)
Antenna: G3LNP loop, oriented East - West.






_______________________________________________________
Get 100% FREE Internet Access powered by Excite
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andy Talbot" <drassew2@interalpha.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: Re: LF: The secret is out
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Tomorrow, I may run much lower power on 5Hz or 2.5Hz span.  So if the signal
appears much weaker than today's it will be because I'm using a 10 Watt
amplifier module instead of the usual 250W job (throtted back to 130W
today).

Andy  G4JNT




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Date: Sun, 18 Jun 2000 07:55:32 +0100
To: rsgb_lf_group@blacksheep.org
From: "Tom Boucher" <tom@telemetry.demon.co.uk>
Subject: LF: Broken antennas
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Thanks Steve for the QSP and thanks also to Marc and Alan for reports. I
put my 1100 ft long wire back up but it's even lower than before. Quite
difficult dis-entangling halyards and wires from trees especially when
the wind is blowing hard and the trees are in full leaf!

73, Tom G3OLB


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 June at GB7DXM
Date: Mon, 19 Jun 2000 00:02:08 +0100
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Hi All, not a lot of activity heard here this weekend but maybe I was
listening at the wrong time (I'm too lazy to get up early!). Static levels
were fairly reasonable considering the very warm weather. Good solid 'O'
signals on QRS on Saturday from Petr OK1FIG but then he was probably audible
as well, also heard PA0BWL and DF0WD at good strength. LX1PD is a call I
have not heard for a while which surfaced again this week. Out most of
Sunday so no log.

Good copy of Andy's 2.5Hz SMT Hell on Spectran. I am not sure but I suspect
he was being copied further east as I saw "HELL ?" and later Petr and Marcus
DF6NM discussing Hell on QRS/DFCW at 1630z. (Spectrogram 0.3Hz, 1000msec
time scale)
There was a reasonable catch on the cluster this week with one or two new
calls helping Wolf out with postings. Note an HA6 posting ....does this mean
Hungary is due to have the band released? I must admit to not having heard
any F callsigns yet. Hopefully Brian's (CT1DRP) persistance in CT1 will pay
off soon, before the November transatlatic schedules with luck. It might be
worth quoting those dates to your authorities Brian just to show that there
is international activity and experiments.

Cluster spots below, 1800.0 slot still not usable here as it is full of
inane stateside chatter via an internet cluster link.
G3NYK de GB7DXM   18-Jun 2222Z >
   136.5  OK1DTN      18-Jun-2000 1848Z  now-like ever-vy gd
<HA6PC>
   136.7  DK6NI       18-Jun-2000 1309Z  cq
<DL6SN>
   136.5  DJ2EY       18-Jun-2000 1121Z  cq
<DL6SN>
   136.9  OK1DTN      18-Jun-2000 1120Z  cq
<DL6SN>
   136.6  DF0WD       18-Jun-2000 1043Z  529 qso with dk6ni 539
<DL1SAN>
   137.0  PA0BWL      18-Jun-2000 1036Z  in qso w DL1SAN
<DF0WD>
   137.0  PA0BWL      18-Jun-2000 1029Z  529 cq
<DL1SAN>
   136.9  DF0WD       18-Jun-2000 1005Z  cq
<DL6SN>
   136.7  DJ2EY       18-Jun-2000 0936Z  559 cq
<DL1SAN>
   136.4  OK1DTN      18-Jun-2000 0911Z  549 cq
<DL1SAN>
   136.6  DK6NI       18-Jun-2000 0849Z  549
<DL1SAN>
   137.0  G3YXM       18-Jun-2000 0828Z  vy strong on my magn. Loop
<DL3FDO>
   137.3  DF8ZR       18-Jun-2000 0807Z  in qso with df6nm
<DL6SN>
   136.5  DJ9IE       18-Jun-2000 0805Z  in qso with oz8nj
<DL6SN>
   136.3  DJ2LF       18-Jun-2000 0802Z  cq
<DL6SN>
   136.7  DL3FDO      18-Jun-2000 0800Z
<DL6SN>
   136.9  OZ8NJ       18-Jun-2000 0720Z  in qso with ok1fig
<DL6SN>
   136.3  IK5ZPV      18-Jun-2000 0711Z  in qso with ok1dtn
<DL6SN>
   137.0  OK1FIG      18-Jun-2000 0704Z
<DL6SN>
   136.7  OK1FIG      18-Jun-2000 0649Z  569 cq
<DL1SAN>
   136.3  HB2ASB      18-Jun-2000 0648Z  579 cq
<DL1SAN>
   137.0  G3OLB       17-Jun-2000 1313Z
<DL3FDO>
   136.8  OK1FIG      17-Jun-2000 1110Z  559 cq
<DL1SAN>
   136.6  DJ7RD       17-Jun-2000 0932Z  579 cq
<DL1SAN>
   136.6  DK6NI       17-Jun-2000 0823Z  539 just wkd
<DL1SAN>
   136.9  OK1DTN      17-Jun-2000 0610Z  559 cq
<DL1SAN>
   136.5  LX1PD       12-Jun-2000 1207Z
<DL3FDO>
   136.9  DL0FTZ/P    12-Jun-2000 0904Z  549
<DL1SAN>
G3NYK de GB7DXM   18-Jun 2225Z >

Cheers and 73 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: "Petr Maly" <p.maly@gmc.net>
To: "136 group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Screen shot of Slow-HELL of DF6NM
Date: Mon, 19 Jun 2000 09:52:27 +0200
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Hello LF'ers

On Saturday I had cross-mode (Visual-CW/Slow-HELL) QSO with Marcus, DF6NM.
Take a look to screenshot from Spectran:
http://mujweb.cz/www/ok1fig/H_galler.htm

I regret I missed LX1PD, new country for me.

73, Petr, OK1FIG




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: LF: Signal Strength Measurements by OH2LX, 19 June 2000
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Signal strength measurements of various LF stations by OH2LX:
------------------------------------------------------------------
Day ------------------   12Jun 13Jun 14Jun 15Jun 16Jun 17Jun 18Jun
                          MON   TUE   WED   THU   FRI   SAT   SUN 
Time, UTC ------------    2050- 2040- 2035- 2045- 2050- 2030- 2045-
------------------------------------------------------------------
kHz    Stn   d,km  AZI          Indicated ESH2 input, dBmW
------------------------------------------------------------------
 68.9 DHJ58? 1115, 242    -98  -103  -100  -103  -102   -96  -102
------------------------------------------------------------------
 73.3 Rugby, 1825, 252,  -104  -105  -106  -104  -105c -105c -103c
------------------------------------------------------------------
 75.0   HBG, 1992, 226,  -104  -105  -107  -105  -107  -108  -105
------------------------------------------------------------------
 77.5 DCF77, 1543, 228,   -89   -92   -93   -90   -91   -94   -89
------------------------------------------------------------------
128.9 DCF49, 1544, 228,   -97   -93   -93   -91   -93   -96   -94
------------------------------------------------------------------
138.8 DBF39, 1221, 226,   -89   -89   -91   -89   -87   -92   -91
------------------------------------------------------------------
135.8   SXV, 2490, 182,  -112  -109  -108  -113  -108  -107  -106
------------------------------------------------------------------
137.0   CFH, 5750, 295,   Nil   Nil   Nil   Nil   Nil   Nil   Nil
------------------------------------------------------------------
(R&S ESH2/---- 10m coax----/1:10/-----15m wire-----):
 Noise level with antenna: with 200Hz IF BandWidth: 
-24..-20 dB(uV), -131..-127dBmW (varies with frq, qrm, qrn etc)
------------------------------------------------------------------
73.3: - c = carrier not identified, assumed to be Rugby
------------------------------------------------------------------
End of message of 19th June 2000, 0800 UTC, from OH2LX
------------------------------------------------------------------

----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


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'" <rsgb_lf_group@blacksheep.org>
Subject: LF: Very Slow Hell
Date: Mon, 19 Jun 2000 09:55:09 +0100
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Yesterday (Sunday) I was transmitting a low power slow Hellschreiber
beacon signal all day.  Signal width was 2.5Hz / Pixel rate 2s  on
137.6kHz.  Power to the antenna was 6 Watts with ERP around 0.6mW.  Did
anyone see anything ?

Andy G4JNT


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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 19 Jun 2000 13:26:57 +0100
To: rsgb_lf_group@blacksheep.org
From: "Walter Blanchard" <blanch@pncl.co.uk>
Subject: Re: LF: Very Slow Hell
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At 09:55 19/06/00 +0100, you wrote:
>Yesterday (Sunday) I was transmitting a low power slow Hellschreiber
>beacon signal all day.  Signal width was 2.5Hz / Pixel rate 2s  on
>137.6kHz.  Power to the antenna was 6 Watts with ERP around 0.6mW.  Did
>anyone see anything ?

Yes, received here OK but must say it's a bit impractical.  I only have
Spectrogram and to get the aspect ratio right I needed to have a 20000
mS scan time - far too long. Your 20 Hz on Saturday was far better and
much quicker - 500 mS scan.

Walter G3JKV - Dorking, IO91UF. 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Hi Andy,
I didn't have much time on Sunday, but did look briefly around 11.30 local.
It was just visible, but very weak. Knowing what the letters were, made it
possible to identify it.
John, G4CNN





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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: Very Slow Hell
Date: Mon, 19 Jun 2000 19:07:13 +0100
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Andy.

I did run Spectran at 0.086? setting and could plainly see the signal but
far too stretched out due to my speed setting being too fast. As it had
taken about an hour to build it up I didn't try again....
It would have been easily readable with the right settings although I could
hear nothing.

73, Dave G3YXM.

> Yesterday (Sunday) I was transmitting a low power slow Hellschreiber
> beacon signal all day.  Signal width was 2.5Hz / Pixel rate 2s  on
> 137.6kHz.  Power to the antenna was 6 Watts with ERP around 0.6mW.  Did
> anyone see anything ?
>
> 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.
>
>



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: Very Slow Hell trial results
Date: Tue, 20 Jun 2000 08:44:18 +0100
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That was the idea of the low power transmission.  It looks as if there
may still be some work to be done on optimising the pixel duration
against particular decoding software settings - Spectrogram does not
seem particularly useful except for the widest version tried - and at
20Hz bandwidth this defeats the purpose I had in mind.

It would be a difficult test to arange, but I wonder if there is any
fair way to compare readability of Slow SMT Hell with Slow CW using
equivalent bandwidth and equivalent time versions of both. Calculation
should give most of the answers and needs doing anyway to find
comparable speeds/bandwidths for a fair testing programme.  Then perhaps
I could transmit alternate modes throughout a day for some serious
measurements.
Walter, I suggest you get a copy of Spectan - Hi.

Andy  G4JNT

>>beacon signal all day.  Signal width was 2.5Hz / Pixel rate 2s  on
>>137.6kHz.  Power to the antenna was 6 Watts with ERP around 0.6mW. 

>Yes, received here OK but must say it's a bit impractical.  I only have
>Spectrogram and to get the aspect ratio right I needed to have a 20000
>mS scan time - far too long. Your 20 Hz on Saturday was far better and
>much quicker - 500 mS scan.	Walter G3JKV

>It was just visible, but very weak. Knowing what the letters were, made
it
>possible to identify it.	John, G4CNN

>I did run Spectran at 0.086? setting and could plainly see the signal
but
>far too stretched out due to my speed setting being too fast. As it had
>taken about an hour to build it up I didn't try again....
>It would have been easily readable with the right settings although I
could
>hear nothing.	Dave G3YXM.



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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Information of interest:

What is different about the CFA? As an example, a CFA only 21 feet (6.5
m) tall, located at Tanta in the center of Egypt, provides AM broadcast
service at 1.16 MHz (258 Meters) to millions of people from Cairo north
to the coast. Certified measurements provide evidence that this small
CFA produces a radiated signal almost 6 dB stronger than the previous
1/4 wavelength vertical broadcast tower which was 211 feet (65 Meters)
tall. To express the performance a different way >> with the tall tower,
a 100,000 watt transmitter was required for the desired coverage. With
the miniature CFA the same coverage was attained with the transmitter
power reduced to 30,000 watts.

As seen on:
http://www.antennex.com/

73, Mark, F6JSZ
http://perso.club-internet.fr/sovergne


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: CFA Antenna: miraculous?
Date: Tue, 20 Jun 2000 16:00:34 +0100
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The real question is, why was the quarter wave antenna worse, not why
was the CFA so good.  A 1/4 monopole can approach 100% efficiency and
can be 3dB up on a dipole when erected properly - in which case any
other single element antenna cannot have any MORE gain.  

As Egypt is surrounded by sand, doesn't it look like a ground
conductivity issue destroying the efficiency of the conventional
radiator.  As the CFA is less dependant on a ground for termination of
the Reactive fields it could just possibly be better in these
circumstances.

All the CFAs built and tested at higher freqs have never been as good as
the dipoles or similar they were supposed to replace.  In fact usually
6dB or more worse

Andy  G4JNT


> ----------
> From: 	M & S[SMTP:sovergne@club-internet.fr]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-20 14:48
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	LF: CFA Antenna: miraculous?
> 
> Information of interest:
> 
> What is different about the CFA? As an example, a CFA only 21 feet
> (6.5
> m) tall, located at Tanta in the center of Egypt, provides AM
> broadcast
> service at 1.16 MHz (258 Meters) to millions of people from Cairo
> north
> to the coast. Certified measurements provide evidence that this small
> CFA produces a radiated signal almost 6 dB stronger than the previous
> 1/4 wavelength vertical broadcast tower which was 211 feet (65 Meters)
> tall. To express the performance a different way >> with the tall
> tower,
> a 100,000 watt transmitter was required for the desired coverage. With
> the miniature CFA the same coverage was attained with the transmitter
> power reduced to 30,000 watts.
> 
> As seen on:
> http://www.antennex.com/
> 
> 73, Mark, F6JSZ
> http://perso.club-internet.fr/sovergne
> 


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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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Talbot Andrew a *crit :
> 
> The real question is, why was the quarter wave antenna worse, not why
> was the CFA so good.  A 1/4 monopole can approach 100% efficiency and
> can be 3dB up on a dipole when erected properly - in which case any
> other single element antenna cannot have any MORE gain.

Thank you, Andy. That DOES confirm what I thought. I just found this
information on the Net and wondered if there was something extraordinary
about it, just in case any lowfer had experimented the stuff...

73, Mark, F6JSZ
Soon on the air: just a small problem with the antenna; JN04PX.

"There was an owl who sat in an oak,
The more he heard, the less he spoke,
The more he spoke, the less he heard,
Why not copy that wise old bird ?"

---


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: re CFA antennas
Date: Tue, 20 Jun 2000 20:07:38 +0100
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Hi Mark, I think we are all waiting for the proposed station on the I of Man
to start transmission so we can compare it with the strength we received
from the "two Daves and Graham" LF expedition.

If you have not seen them there is a good exposition of the theory aspects
on
http://www.ee.surrey.ac.uk/Personal/D.Jefferies/poynting.html
There was also a report of experiments done by or on behalf of John Belrose
VE2CV. I do not have a site URL for this. John's e-mail address is given as
john.belrose@crc.ca  
and a URL is given for the pictures and wire model as
http://members.home.net/propagation/cfa.html
This may lead to the text of the experimental report.

These are not the sarcastic knocking copy that has been around but are
reasoned reports saying that the claimed results have yet to be
duplicated..........remember 'Cold Fusion' !!

It could be the next breakthough but don't hold your breath.

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: "Peter Dodd" <g3ldo@zetnet.co.uk>
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Subject: LF: Re:  CFA Antenna: miraculous?
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The CFA antenna is made by Hately Antenna Technology (GM3HAT). Every 
month for many years now the RSGB has carried an advertisment for 
this company. (until May, when the advertisment said they were moving 
QTH and don't try and contact them until further notice)

One outstanding characteristic of this antenna is the lack of 
information on it - after all these years.

The other characteristic is the lack of comparitive test (review) 
information on it - after all these years.

The Wireless World (now Electronics World + Wireless World) did 
several articles on the CFA but there was never enough information to 
duplicate it. Finally an article 'CFA - RIP' appeared in May 1993 (I 
have a copy), where a test version of the CFA radiation was -23dB 
relative to a reference dipole. However, the radiation level did not 
vary as the phase angle (using the phasing unit) was changed, 
therefore it was not performing as the theory said it should.

The <www.antennex.com> website promises information  - at a price. 

Has any one used a CFA (or knows of someone who has used one) on any band?

  

-- 
Regards, Peter, G3LDO

<g3ldo@zetnet.co.uk>






From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 21 Jun 2000 10:36:59
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: CFA Antenna: miraculous?
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I have been looking for information on the CFA antenna and found some on
internet. Links to them are found on my webpage :
http://www.qsl.net/on7yd/136lit.htm
(3 last articles)

Who would not be interested in a compact antenna with the performance of a
quarter-wave ? 
Most of us would even be more than happy to accept a loss of 20dB referred
to a quarter-wave ... but :

- If you convert 6.5m on 16Mhz to 136kHz, the antenna is still 55m high
- Building (and adjusting) the antenna will be far more complicated and
expensive than making a simple vertical or loop antenna.
-So far I have not found any report that a CFA antenna has been built by a
ham for any frequency.
- While other antennas for 136kHz mainly consist of wires and are rather
invisible, the CFA seems to be a massive construction, so a height of 5 to
10 meters will be the limit that most hams can achieve without getting into
trouble with the neighbourgs and the authorities. Converted back to 1.16MHz
this would mean a height of 1 meter or less.

It might be a good idea to try it on topband or even on 80m, let's see what
it is worth there.

73, Rik  ON7YD



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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Re:  CFA Antenna
Date: Wed, 21 Jun 2000 09:47:37 +0100
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Can anyone identify the issue(s) of Wireless World where it first
appeared.  It would be interesting to extract them from the archives and
read up on just what was published

Andy  G4JNT

> ----------
> From: 	Peter Dodd[SMTP:g3ldo@zetnet.co.uk]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-21 07:51
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	LF: Re:  CFA Antenna: miraculous?
> 
> 
> The CFA antenna is made by Hately Antenna Technology (GM3HAT). Every 
> month for many years now the RSGB has carried an advertisment for 
> this company. (until May, when the advertisment said they were moving 
> QTH and don't try and contact them until further notice)
> 
> One outstanding characteristic of this antenna is the lack of 
> information on it - after all these years.
> 
> The other characteristic is the lack of comparitive test (review) 
> information on it - after all these years.
> 
> The Wireless World (now Electronics World + Wireless World) did 
> several articles on the CFA but there was never enough information to 
> duplicate it. Finally an article 'CFA - RIP' appeared in May 1993 (I 
> have a copy), where a test version of the CFA radiation was -23dB 
> relative to a reference dipole. However, the radiation level did not 
> vary as the phase angle (using the phasing unit) was changed, 
> therefore it was not performing as the theory said it should.
> 
> The <www.antennex.com> website promises information  - at a price. 
> 
> Has any one used a CFA (or knows of someone who has used one) on any
> band?
> 
>   
> 
> -- 
> Regards, Peter, G3LDO
> 
> <g3ldo@zetnet.co.uk>
> 
> 


-- 
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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, 
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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: Re: LF: Re:  CFA Antenna: miraculous?
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The CFA was described in Radio Today magazine last October. In 
the Feb 2000 edition a phasing unit (essential to correct operation) 
for an 80m CFA was described.

Back numbers are available from sales@rsgb.org.uk

End of advert.



Mike Dennison, G3XDV
Publications Manager

* RadCom * Ham Radio Today * GB2RS News *
* RSGB Books and CDs *

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

RSGB - UK AMATEUR RADIO



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Aldo Marchetto" <a.marchetto@iii.to.cnr.it>
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Subject: Re: LF: CFA Antenna: miraculous?
In-reply-to: <3.0.1.16.20000621103659.0af713fc@mail.cc.kuleuven.ac.be>
References: <394F7643.7AC83ACF@club-internet.fr>
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I agree with you that CFAs seen in the literarture are too big for 
135 kHz, and not enough efficient

To avoid to be flamed, I states immediately that I'm not a supporter 
nor a detractor of CFA, but I'm only intrigued to see the results of 
accurate testing of the antenna 

>-So far I have not found any report that a CFA antenna has been 
>built by a ham for any frequency.

On the contrary, I read on the Antennex magazine that some OM have 
built CFA for 40 and 80 m, someone are testing one for 160 m and 
someone also reported a CFA working in VHF (around 100 MHz)

I had some interesting exchange of e-mail with some of them and I too 
I built one for 40/80 meters, 25 cm high.
However in most cases (mine included) there was no measurement of the
actual performance of the antenna.

Most of the OM which built CFAs (including me) did some QSO in the 
range of 1000 km with the antenna indoor, reported satisfaction or 
unsatisfaction, but had no instrument or experience to make an 
accurate comparison among HF antennas.

CFA antennas for the ham bands can also be purchased:
in December 8th, 1999, G3SMW trasmitted a 10-W beacon Hellschreiber 
signal in 20 meters using a commercial Crossed-Field (Horizontal 
Monoband Loop) Antenna 10m above ground, and got several reports.
I received his signal in Northern Italy with signals comparable to 
other G or PA stations running 100 watts to ground planes. However 
this is only an episodic report, and he was not trying to test the 
performance of this antenna (we were testing the relative performance 
of different Hellschreiber codes).

I found only two papers reporting field strenght measurement, one 
from supporters and one from a dectractor of CFAs:

1) WA6HZT and N6YIP in Antennex (June 2000) report a loss of 24 db 
respect to the filed strenght predicted by models for a 
quarter wave monopole with 120 radials, for their 1.6-m high CFA on 
160 meters. However they declare that this result is provisional, 
while they are still trying to build better tuning networks.

2) VE2CV in the same journal reports a radiation efficiency of about 
1% for his 1.2-m high CFA on 80 meters

In my opinion most of the debate is related on the claims that the 
CFA should perform as well or better than a quarter wave monopole.
Probably it would be more proficient evaluate it against other 
antenna of similar height.

It has also been supposed that CFA could represent an alternative way 
to feed a short, fat monopole and, in this case, it would be 
interesting to evaluate advantages and disadvantages of this 
alternative feeding.

73 Aldo IZ1ANT




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 21 Jun 2000 13:53:02
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: CFA Antenna: miraculous?
In-reply-to: <E134iLB-0001Lr-00@post.thorcom.com>
References: <3.0.1.16.20000621103659.0af713fc@mail.cc.kuleuven.ac.be> <394F7643.7AC83ACF@club-internet.fr>
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>I found only two papers reporting field strenght measurement, one 
>from supporters and one from a dectractor of CFAs:
>
>1) WA6HZT and N6YIP in Antennex (June 2000) report a loss of 24 db 
>respect to the filed strenght predicted by models for a 
>quarter wave monopole with 120 radials, for their 1.6-m high CFA on 
>160 meters. However they declare that this result is provisional, 
>while they are still trying to build better tuning networks.
>
>2) VE2CV in the same journal reports a radiation efficiency of about 
>1% for his 1.2-m high CFA on 80 meters

This would mean that a 0.015 lambda CFA has a gain of about -20dB (2) and a
0.01 lambda CFA has a gain of about -24dB (1). 
Extrapolating this figures would lead to -30/-35dB for a 10m high CFA on
136kHz (about 0.005 lambda) and -35/-40dB for 6m high CFA.
These are values that one can achieve with a decent T or inverted-L antenna
of the same height.

I do not doubt that the CFA principle works, but when the size of the
antenna becomes very small (compared to wavelength) you will get high
losses. For a short vertical these are mainly in the 'surrounding'
(grounds, nearby objects) while for the CFA (as for the magnetic loop)
these are probably within the antenna. This could make the CFA a valid
alternative for those sufferering from very high groundloss.

73, Rik  ON7YD


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: <3617AC3245C2D1118A840000F805359C01AB8CCF@pdw-mercury-1.dera.gov.uk>
Subject: LF: Re: Re:  CFA Antenna
Date: Wed, 21 Jun 2000 15:48:47 +0200
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> Can anyone identify the issue(s) of Wireless World where it first
> appeared.  It would be interesting to extract them from the archives and
> read up on just what was published
>
> Andy  G4JNT
>

The article appeared in Electronics & Wireless World of March 1989:

F.M. Kabbay, M.C. Hately and B.G. Stewart: "Maxwell's equations and the
Crossed Field Antenna".


73, Dick Rollema, PA0SE




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: CFA Antenna: miraculous?
References: <3.0.1.16.20000621103659.0af713fc@mail.cc.kuleuven.ac.be> <394F7643.7AC83ACF@club-internet.fr> <3.0.1.16.20000621135302.12f7ace4@mail.cc.kuleuven.ac.be>
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Hi Rick, Hi all,


I'll be constructing one of these antennas starting from next weekend.
All the literature about it seem's so interesting that I will absolutely
try one.

I'll start with 160 meters and give you the results.

Then, I'll try one for 136 kHz

In the mean time, my full-size dipole has been repaired with success.
Reception is very good. Just wait for that big signal from the
south-west of France...

73, Mark, F6JSZ
JN04PX
http://perso.club-internet.fr/sovergne

Rik Strobbe a *crit :
> 
> >I found only two papers reporting field strenght measurement, one
> >from supporters and one from a dectractor of CFAs:
> >
> >1) WA6HZT and N6YIP in Antennex (June 2000) report a loss of 24 db
> >respect to the filed strenght predicted by models for a
> >quarter wave monopole with 120 radials, for their 1.6-m high CFA on
> >160 meters. However they declare that this result is provisional,
> >while they are still trying to build better tuning networks.
> >
> >2) VE2CV in the same journal reports a radiation efficiency of about
> >1% for his 1.2-m high CFA on 80 meters
> 
> This would mean that a 0.015 lambda CFA has a gain of about -20dB (2) and a
> 0.01 lambda CFA has a gain of about -24dB (1).
> Extrapolating this figures would lead to -30/-35dB for a 10m high CFA on
> 136kHz (about 0.005 lambda) and -35/-40dB for 6m high CFA.
> These are values that one can achieve with a decent T or inverted-L antenna
> of the same height.
> 
> I do not doubt that the CFA principle works, but when the size of the
> antenna becomes very small (compared to wavelength) you will get high
> losses. For a short vertical these are mainly in the 'surrounding'
> (grounds, nearby objects) while for the CFA (as for the magnetic loop)
> these are probably within the antenna. This could make the CFA a valid
> alternative for those sufferering from very high groundloss.
> 
> 73, Rik  ON7YD


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: Reference sound for shrinking
Date: Thu, 22 Jun 2000 09:14:25 +0200
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Hello LF'ers

Does anybody have recorded sound of Visual-CW (as *.WAV with reasonable
length) where the signal is not hearable by ear? Could we have such a
reference sound to compare the results of processing? I would like to try to
shrink the sound in SW like SoundForge or CoolEdit and compare results with
the others, mainly with Bill.

73, Petr, OK1FIG





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> Does anybody have recorded sound of Visual-CW (as *.WAV with reasonable
> length) where the signal is not hearable by ear? Could we have such a
> reference sound to compare the results of processing? I would like to try
> to shrink the sound in SW like SoundForge or CoolEdit and compare results
> with the others, mainly with Bill.
> 
> 73, Petr, OK1FIG
>

Petr,

On my web site is a .WAV of a transmission made in 1998 by the 
late Peter Bobeck as DA0LF. The Morse has a 20s dot period. It is 
1.3Mb and lasts for 2 minutes, during which he sends a dash and a 
dot! He is not quite inaudible but certainly would have been 
unreadable at normal speeds as the signal is only just perceptible. 
The page also gives spectrograms traces of the signal - absolutely 
100% with no noise.

http://www.dennison.demon.co.uk/da0lf621.htm

73


Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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: <E1353Ki-00000n-00@mserv1d.u-net.net>
Subject: Re: LF: Reference sound for shrinking
Date: Thu, 22 Jun 2000 12:36:19 +0200
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----- Original Message -----
From: Mike Dennison <mike.dennison@rsgb.org.uk>
To: <rsgb_lf_group@blacksheep.org>
Sent: Thursday, June 22, 2000 11:24 AM
Subject: Re: LF: Reference sound for shrinking


> > Does anybody have recorded sound of Visual-CW (as *.WAV with reasonable
> > length) where the signal is not hearable by ear? Could we have such a
> > reference sound to compare the results of processing? I would like to
try
> > to shrink the sound in SW like SoundForge or CoolEdit and compare
results
> > with the others, mainly with Bill.
> >
> > 73, Petr, OK1FIG
> >
>
> Petr,
>
> On my web site is a .WAV of a transmission made in 1998 by the
> late Peter Bobeck as DA0LF. The Morse has a 20s dot period. It is
> 1.3Mb and lasts for 2 minutes, during which he sends a dash and a
> dot! He is not quite inaudible but certainly would have been
> unreadable at normal speeds as the signal is only just perceptible.
> The page also gives spectrograms traces of the signal - absolutely
> 100% with no noise.
>
> http://www.dennison.demon.co.uk/da0lf621.htm
>
> 73
>
Thank you. It is not a typical sound we need to process, but I will try it
also. In any way, it will be a big honour for me to process Peter Bobek's
tranmission. Does he know....?

73, Petr

>
> Mike, G3XDV (IO91VT)
> http://www.dennison.demon.co.uk/activity.htm
>
>
>



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: "136 group" <rsgb_lf_group@blacksheep.org>
From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: LF: Reference sound for shrinking
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While writing histories - at the moment about
the first Sputniks - let me recall a tape recording
made by our friend Lenna, OH1NL on the 11th April 1964
of the 1st 144 MHz EME QSO. The original recording was
played to numerous hams, some of them heard something
but heard nothing at all. Much depends on the individual
person's abilities to trace and 'decode' the A1 signal
from below the noise, even with the same arrangement.

Petr's suggestion is OK, would be interested to get
such copy and still looking for Lenna's recording.

73 de Vaino, OH2LX (I have a copy of SM7CMY's thesis)






Hello LF'ers

Does anybody have recorded sound of Visual-CW (as *.WAV with reasonable
length) where the signal is not hearable by ear? Could we have such a
reference sound to compare the results of processing? I would like to try to
shrink the sound in SW like SoundForge or CoolEdit and compare results with
the others, mainly with Bill.

73, Petr, OK1FIG





----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


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: Shrinking sounds - fiasco
Date: Fri, 23 Jun 2000 09:56:46 +0200
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Hello all
Yesterday I spent a while with shrinking WAV's in SoundForge and CoolEdit.
In the original file (da0lf), there is nothing heard by ear, but when the
file is open in the Gram, the signal trace is clearly visible. I tried to
shrink to 50% of the previous length as a first step. I could not hear
anything either. When I opened the new file in the Gram, the signal
disappeared completely. I guess the main reason is that unlike the Bill's
method, this one doesn't lead to narrowing the bandwidth. Simply, it doesn't
work. I must try Bill's software.

73, Petr, OK1FIG





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Brown" <tractorb@ihug.co.nz>
To: rsgb_lf_group@blacksheep.org
References: <003301bfdce8$94309b00$2301a8c0@maly.cz.gmc.net>
Subject: LF: Re: Shrinking sounds - fiasco
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A good test  .WAV file is the  Z2 file that is still I think the best LOWFER
beacon aural DX,  a mainland USA LOWFER beacon copied in Hawaii on a
portable setup. I have a copy of the wave file  here but I believe it is
available ex the K0LR web site.




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: Shrinking sounds - fiasco
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---Second bit of message having hit the send button by accident!!!!

The Z2 wav file is quite a challenge aurally as well. I had to listen to it
several times before I could pick out the callsign.
73
Dave, ZL3FJ



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: Shrinking sounds - fiasco
Date: Fri, 23 Jun 2000 10:27:59 +0100
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You will not be able to shrink files and make them audible without
processing the .WAV file data considerably.  Merely changing the
sampling rate will do nothing to improve readability.   The stages
necessary are  :

1)	Take the off air signal recording at (say) 8000 Hz sampling rate

2)	Digitally mix down to some arbitrarily low frequency by
multiplying each waveform sample by COS and SIN samples of a digital
local oscillator signal.

3)	Filter to the necessary sub-Hz bandwidth centred on the signal
of interest .  This stage is what makes the signal 'audible' and brings
it out of the noise.

4)	Decimate this filtered data to a much lower sampling rate by
just taking one sample out of every (say) 256 . Save as if it were a
.WAV file giving the data sampled at 31.25 Hz.  Choose a decimated
sampling rate adequate to meet the Nyquist criteria of the bandpass
filtered signal

5)	Re label the .WAV file to make it 'think' the sampling rate is
8000Hz and replay.  The result will be a tone centred on 256 * the mixed
down frequency with a bandwidth 256 * the filtered bandwidth.

All the numbers can of course be changed arbitrarily provided teh rules
for sampling and Nyquist are adhered to.  As you can see, the process is
not as straighforward as some have lead to believe on this reflector.  
For anyone contemplating writing software to do this, note that stages
3) and 4) can be taken together - if using an FIR filter, the filtering
process needs to be done for each decimated sample only - this saves
considerable processing overhead for the long filter tap lengths
necessary

I have software to do this process for other (non-amateur) signal
analysis purposes and use an intermediate I/Q file format where signals
are first mixed down to zero centre frequency and stored in their
complex form with a spectrum ranging from minus to plus half the
sampling rate.  Processing is then more straightforward as bandpass
filtering becomes lowpass etc.  After decimation a final conversion to
.WAV format is then made and the tone frequency and false sampling rate
can be set arbitrarily.

The most fascinating signal produced this way was a Dopplergram of a
carrier on 3.572MHz recorded overnight and played back 500 times faster.
The ionospheric Doppler shifts and multipath result in sounds not unlike
those of Whales talking !

Andy  G4JNT
> ----------
> From: 	Petr Maly[SMTP:p.maly@gmc.net]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-23 08:56
> To: 	136 group
> Subject: 	LF: Shrinking sounds - fiasco
> 
> Hello all
> Yesterday I spent a while with shrinking WAV's in SoundForge and
> CoolEdit.
> In the original file (da0lf), there is nothing heard by ear, but when
> the
> file is open in the Gram, the signal trace is clearly visible. I tried
> to
> shrink to 50% of the previous length as a first step. I could not hear
> anything either. When I opened the new file in the Gram, the signal
> disappeared completely. I guess the main reason is that unlike the
> Bill's
> method, this one doesn't lead to narrowing the bandwidth. Simply, it
> doesn't
> work. I must try Bill's software.
> 
> 73, Petr, OK1FIG
> 
> 
> 
> 


-- 
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Shrinking sounds - fiasco
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On Fri, 23 Jun 2000 09:56:46 +0200, "Petr Maly" <p.maly@gmc.net>
wrote:

>Hello all
>Yesterday I spent a while with shrinking WAV's in SoundForge and CoolEdit.
>In the original file (da0lf), there is nothing heard by ear, but when the
>file is open in the Gram, the signal trace is clearly visible. I tried to
>shrink to 50% of the previous length as a first step. I could not hear
>anything either. When I opened the new file in the Gram, the signal
>disappeared completely.

Just a check, but what method did you use to shrink these files ?

Any pesky lossy psychoacoustic compression method such as MP3, Musicam
etc. is definitely NOT suitable for compressing such files. The idea
with all the psychoacoustic compression is to remove all the data that
is not going to be _heard_ due to masking by a strong nearby signal or
by wideband noise (as in this case).

If you use some kind of compression, make sure that you are using some
_lossless_ compression method.

Paul OH3LWR



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From: "Paul Keinanen" <keinanen@sci.fi>
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To: rsgb_lf_group@blacksheep.org
Subject: LF: Re: Shrinking sounds - fiasco
Date: Fri, 23 Jun 2000 15:48:12 +0300
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On Fri, 23 Jun 2000 10:27:59 +0100, Talbot Andrew
<ACTALBOT@dera.gov.uk> wrote:


>1)	Take the off air signal recording at (say) 8000 Hz sampling rate

>2)	Digitally mix down to some arbitrarily low frequency 

>3)	Filter to the necessary sub-Hz bandwidth centred on the signal

>4)	Decimate this filtered data to a much lower sampling rate by
>just taking one sample out of every (say) 256 . 

>For anyone contemplating writing software to do this, note that stages
>3) and 4) can be taken together - if using an FIR filter, the filtering
>process needs to be done for each decimated sample only - this saves
>considerable processing overhead for the long filter tap lengths
>necessary


If you plan to combine steps 3) and 4) by doing first decimating and
then narrow band (sub-Hz) filtering, shouldn't you low pass filter the
signal produced by the mixdown at 2) to have a bandwidth less than 15
Hz for the final 31.25 Hz sample rate to meet the Nyquist criteria ?

Paul OH3LWR




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
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Subject: Re: LF: Shrinking sounds - fiasco
Date: Fri, 23 Jun 2000 15:10:24 +0200
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Paul, you haven't read the previous messages, have you. We don't talk about
compressing sound files.

Petr, OK1FIG

----- Original Message -----
From: Paul Keinanen <keinanen@sci.fi>
To: <rsgb_lf_group@blacksheep.org>
Sent: Friday, June 23, 2000 1:04 PM
Subject: Re: LF: Shrinking sounds - fiasco


> On Fri, 23 Jun 2000 09:56:46 +0200, "Petr Maly" <p.maly@gmc.net>
> wrote:
>
> >Hello all
> >Yesterday I spent a while with shrinking WAV's in SoundForge and
CoolEdit.
> >In the original file (da0lf), there is nothing heard by ear, but when the
> >file is open in the Gram, the signal trace is clearly visible. I tried to
> >shrink to 50% of the previous length as a first step. I could not hear
> >anything either. When I opened the new file in the Gram, the signal
> >disappeared completely.
>
> Just a check, but what method did you use to shrink these files ?
>
> Any pesky lossy psychoacoustic compression method such as MP3, Musicam
> etc. is definitely NOT suitable for compressing such files. The idea
> with all the psychoacoustic compression is to remove all the data that
> is not going to be _heard_ due to masking by a strong nearby signal or
> by wideband noise (as in this case).
>
> If you use some kind of compression, make sure that you are using some
> _lossless_ compression method.
>
> Paul OH3LWR
>
>
>



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: Shrinking sounds - fiasco
Date: Fri, 23 Jun 2000 14:27:53 +0100
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Well, the way I do it is to use a mixed down frequency centred on zero
and use low pass filtering to give bandpass when mixed back up for
listening.  As described the method would need some low pass filtering
as part of the initial mixing down process.  

Filtering may well also be needed in the final upconversion process

Andy

>>3) and 4) can be taken together - if using an FIR filter, the
filtering
>>process needs to be done for each decimated sample only - this saves
>>considerable processing overhead for the long filter tap lengths
>>necessary
>
>
>If you plan to combine steps 3) and 4) by doing first decimating and
>then narrow band (sub-Hz) filtering, shouldn't you low pass filter the
>signal produced by the mixdown at 2) to have a bandwidth less than 15
>Hz for the final 31.25 Hz sample rate to meet the Nyquist criteria ?
>
>Paul OH3LWR





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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <000e01bfdd27$ee3866c0$a258063e@default>
From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: CFH and solar event??
Date: Fri, 23 Jun 2000 16:21:54 +0100
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Hi All, as a result of some converstaions with Brian CT1DRP I have
determined that CFH the Canadian Navy station located at Halifax in Nova
Scotia is back on air again. The reason I missed it, was that at this time
of year it only becomes 'visible' after about 2400z. A couple of nights
monitoring has confirmed to my satisfaction that the FSK (I think!) signal
on 137 is our old friend, back on a new state-of-the-art transmitter. The
profile of the appearance and peaks correlates well with the darkness path
and what we know from monitoring earlier in the year. The modulation looks
different to that which we saw transmitted between Jan 2000 and its switch
off in May. It now looks more like the signal I saw in the first half of
1999 before it was switched off at the end of August.

So far so good......now for the real excitement!!  By chance at 1449z today
I noticed that there was an FSK signal visible on FFTDSP4 on exactly 137.00
+/_42.5 Hz shift FSK. I dont know when it appeared first but by 1459z is had
faded into the noise at this location. This looks very much like flare
activity that has been reported before by Larry I think. Does anyone have
the solar information. I suspect I missed anything up to 20 to 30 minutes of
the event, which would put the particle cloud arrival at about 1420z to
1430, probably timing the event on the sun to sometime Wednesday. Ironically
the only station heard on the band was G8RW pumping away unanswered CQs.

Now that CFH is back it looks as though we might have a warning signal of
these events if we can get reports of the likely flares posted to the
reflector in time.

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: "Steve Olney" <ollaneg@zeta.org.au>
To: rsgb_lf_group@blacksheep.org
References: <394F7643.7AC83ACF@club-internet.fr>
Subject: LF: Re: CFA Antenna: miraculous?
Date: Sat, 24 Jun 2000 06:49:36 +1000
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G'day All,

Here in Sydney Australia we have (had) a CFA installation in commercial use.
I have done relative FS measurements (single point) at a distance of 60Km
and can report that the CFA antenna is NOT working as the inventors say it
will.   The signal (giving all advantage to the CFA) is about 8dB down on
similar standard antenna radiating stations.

The facts (and these are not disputed by anyone - only ignored) are:

- that the antenna was designed, constructed, tuned and re-tuned by one of
the inventors. (No faulty installation one would have to assume).

- the station power had to be reduced from its allowed 400W to 200W due to
it interfering with nearby services.  (CFA is supposed to be an antenna with
little near-field interaction).

- the station owners reconfigured the antenna to be fed as a standard short
fat monopole because they obtained an increased FS with configuration as
against the "superior" CFA.

- the station is in the expensive process of moving their transmitting site
elsewhere to use a standard antenna and is offering the CFA antenna to any
sucker - sorry, buyer.

CFA - miraculous?  Certainly, unfortunately I don't believe in miracles -
only repeatable measurements :-)

73s Steve Olney (VK2ZTO/AXSO - QF56IK : Lat -33 34 07, Long +150 44 40)
=============================================
HomePage URLs:
http://www.qsl.net/vk2zto
http://www.zeta.org.au/~ollaneg

Containing:-
Laser Comms DX
LF Experimentation
Amateur Radio Astronomy
=============================================



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 23 Jun 2000 16:46:05 -0500
To: lowfer@qth.net
Subject: LF: LFCC Award Proposal
Cc: rsgb_lf_group@blacksheep.org
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PROPOSAL TO ESTABLISH A LOW FREQUENCY CENTURY CLUB AWARD (LFCC)
By Les Rayburn, KT4OZ
June 23, 2000


Objective: To outline a set of suggested guidelines for the establishment
of an award
targeted at the users of the Low Frequency (Below 500Khz) spectrum. This
award would 
encourage more activity on LF, and spur users to pursue multiple endorsements.

Governing Body: Ideally, an LF organization like the Longwave Club of
America. Failing that
alternate bodies might include AMRAD, RGSB, or ARRL. 

Award: Certificate, with endorsement stickers.

Program Brief: This award would be open to amateur radio operators,
lowfers, longwave listeners,
and maritime operators.  Operators would be required to submit QSL cards, or
other verification proof to the governing body to be checked for
completeness and accuracy.
The decision of the governing body would be final and not available for
review. 

Certificates would be numbered beginning with LFCC #1 (* See Note Below)

Certificates to be awarded according to the guidelines below:


0-100Khz (VLF Endorsement): Award would be granted to those operators who
could verify 
reception of stations in 25 Maidenhead grid squares. Endorsements for each
additional 25 stations.


76Khz (Amateur VLF Endorsement): Award would be granted to those operators
who could verify two way contacts with or
reception of stations in 10 Maidenhead grid squares. Endorsements for each
additional 10 grid squares.

Amateurs who operate in the 76Khz range would be required to provide proof
of either reception of their
station, other stations, or two way contacts to qualify. No contacts with
non amateur stations can count towards
this endorsement. LF Listeners would receive the Amateur VLF DX Endorsement. 


136Khz (Amateur LF Endorsement): Award would be granted to those operators
who could verify two way contacts with or
reception of stations in 25 Maidenhead grid squares. Endorsements for each
additional 25 grid squares.

Amateurs who operate in the 136Khz range would be required to provide proof
of either reception of their
station, other stations, or two way contacts to qualify. No contacts with
non amateur stations can count towards
this endorsement. LF Listeners would receive the Amateur LF DX Endorsement.


160-190Khz (Lowfer Endorsement): Award would be granted to those operators
who can verify reception of their
LF beacon in at least 10 Maidenhead grid squares. Endorsements for each
additional 5 grid squares. 

LF Listeners (including beacon operators) could also receive the Lowfer DX
Endorsement for reception of lowfer
beacons in at least 5 grid squares. Endorsements for each additional 5 grid
squares. 

100Khz-500Khz (LF Endorsement): Award would be granted to those operators
who could verify reception of stations in 
at least 100 Maidenhead grid squares. Endorsements for each additional 50
grid squares.

This stations could include any combination of NDB, TWIB, Maritime
stations, broadcasting, etc. 


Basic Rules: Verification could be in the form of a QSL card, verification
letter, or other supporting documentation. The 
governing body would appoint a chairman to inspect and return these
verifications. Any operator submitting
false or suspect documentation will have those cards marked by the Chairman
and their application of LFCC
returned. There is no appeal. Operators must resubmit application without
those documents judged to be
false or suspect. 

Basic costs would be covered in the application fee (Suggestion $10-$20). 

Contacts and receptions must have occurred on or before 1980 (I doubt that
reliable frequency listings
exist much before this date.)


Comments: Many LF operators would already qualify for this award. In the
case of veteran NDB dx'ers
they might even qualify for several endorsement stickers! But for many of
us, it would represent
a goal that was realistic and achievable...but difficult enough to
encourage effort. 

There are many out there who object to "paper-chasing" of any kind on the
low frequencies, and this
is understandable. However, if we hope to see amateur allocations grow and
foster in this band,
activity is what we need. Also many of us Lowfers do not have even a single
serious LF listener
within the normal range of our stations, growth is important in these areas
too.

I would further suggest that honorary LFCC's be granted to recognize those
pioneers
of the band who are no longer living or inactive. For example, Ken Cornell,
or Vince Pinto.


Comments are welcome.






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: LFCC Award Proposal
References: <3.0.3.32.20000623165020.007e79d0@highnoonfilm.com>
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Hi Les,


Your proposal is very interesting.

However, the French edition of CQ magazine has already proposed the LFCC
and the award is supposed to be available diring autumn this year...

The brand "LFCC" is now a trademark (yes, we are 'commercial' guys...

73, Mark, F6JSZ

P.S. We formerly did a survey on this mailing list, and response was
quite positive.

les@highnoonfilm.com a *crit :
> 
> 
> 
> PROPOSAL TO ESTABLISH A LOW FREQUENCY CENTURY CLUB AWARD (LFCC)
> By Les Rayburn, KT4OZ
> June 23, 2000
> 
> Objective: To outline a set of suggested guidelines for the establishment
> of an award
> targeted at the users of the Low Frequency (Below 500Khz) spectrum. This
> award would
> encourage more activity on LF, and spur users to pursue multiple endorsements.
> 
> Governing Body: Ideally, an LF organization like the Longwave Club of
> America. Failing that
> alternate bodies might include AMRAD, RGSB, or ARRL.
> 
> Award: Certificate, with endorsement stickers.
> 
> Program Brief: This award would be open to amateur radio operators,
> lowfers, longwave listeners,
> and maritime operators.  Operators would be required to submit QSL cards, or
> other verification proof to the governing body to be checked for
> completeness and accuracy.
> The decision of the governing body would be final and not available for
> review.
> 
> Certificates would be numbered beginning with LFCC #1 (* See Note Below)
> 
> Certificates to be awarded according to the guidelines below:
> 
> 0-100Khz (VLF Endorsement): Award would be granted to those operators who
> could verify
> reception of stations in 25 Maidenhead grid squares. Endorsements for each
> additional 25 stations.
> 
> 73Khz (Amateur VLF Endorsement): Award would be granted to those operators
> who could verify two way contacts with or
> reception of stations in 10 Maidenhead grid squares. Endorsements for each
> additional 10 grid squares.
> 
> Amateurs who operate in the 73Khz range would be required to provide proof
> of either reception of their
> station, other stations, or two way contacts to qualify. No contacts with
> non amateur stations can count towards
> this endorsement. LF Listeners would receive the Amateur VLF DX Endorsement.
> 
> 136Khz (Amateur LF Endorsement): Award would be granted to those operators
> who could verify two way contacts with or
> reception of stations in 25 Maidenhead grid squares. Endorsements for each
> additional 25 grid squares.
> 
> Amateurs who operate in the 136Khz range would be required to provide proof
> of either reception of their
> station, other stations, or two way contacts to qualify. No contacts with
> non amateur stations can count towards
> this endorsement. LF Listeners would receive the Amateur LF DX Endorsement.
> 
> 160-190Khz (Lowfer Endorsement): Award would be granted to those operators
> who can verify reception of their
> LF beacon in at least 10 Maidenhead grid squares. Endorsements for each
> additional 5 grid squares.
> 
> LF Listeners (including beacon operators) could also receive the Lowfer DX
> Endorsement for reception of lowfer
> beacons in at least 5 grid squares. Endorsements for each additional 5 grid
> squares.
> 
> 100Khz-500Khz (LF Endorsement): Award would be granted to those operators
> who could verify reception of stations in
> at least 100 Maidenhead grid squares. Endorsements for each additional 50
> grid squares.
> 
> This stations could include any combination of NDB, TWIB, Maritime
> stations, broadcasting, etc.
> 
> Basic Rules: Verification could be in the form of a QSL card, verification
> letter, or other supporting documentation. The
> governing body would appoint a chairman to inspect and return these
> verifications. Any operator submitting
> false or suspect documentation will have those cards marked by the Chairman
> and their application of LFCC
> returned. There is no appeal. Operators must resubmit application without
> those documents judged to be
> false or suspect.
> 
> Basic costs would be covered in the application fee (Suggestion $10-$20).
> 
> Contacts and receptions must have occurred on or before 1980 (I doubt that
> reliable frequency listings
> exist much before this date.)
> 
> Comments: Many LF operators would already qualify for this award. In the
> case of veteran NDB dx'ers
> they might even qualify for several endorsement stickers! But for many of
> us, it would represent
> a goal that was realistic and achievable...but difficult enough to
> encourage effort.
> 
> There are many out there who object to "paper-chasing" of any kind on the
> low frequencies, and this
> is understandable. However, if we hope to see amateur allocations grow and
> foster in this band,
> activity is what we need. Also many of us Lowfers do not have even a single
> serious LF listener
> within the normal range of our stations, growth is important in these areas
> too.
> 
> I would further suggest that honorary LFCC's be granted to recognize those
> pioneers
> of the band who are no longer living or inactive. For example, Ken Cornell,
> or Vince Pinto.
> 
> Comments are welcome.


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
Subject: LF: Re: CFH and solar event??
Date: Fri, 23 Jun 2000 18:30:57 -0400
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Alan and LF group:

>now for the real excitement!!  By chance at 1449z today
>I noticed that there was an FSK signal visible on FFTDSP4 on exactly 137.00
>+/_42.5 Hz shift FSK. I dont know when it appeared first but by 1459z is
had
>faded into the noise at this location. This looks very much like flare
>activity that has been reported before by Larry I think. Does anyone have
>the solar information.

Yes!

from the IPS message

IPS FLARE ALERT - PART B
ESTIMATED END TIME OF FLARE
ISSUE TIME: Sat Jun 24 00:45:48 EST 2000
++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Current X-ray Flux : 1.79e-05 (M1.8)
Maximum X-ray Flux of 2.89e-05 (M2.9) at 14:29 UT
Estimated Flare End (below M1.0 level) at 14:55 UT

Further Information Will Be Issued At the End of the Event
++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++

And yes, CFH is back on, loud here of course.

There was also an event earlier in the day, see following

IPS FLARE ALERT - PART C
PRELIMINARY FLARE DETAILS AT END OF FLARE
ISSUE TIME: Fri Jun 23 14:20:38 EST 2000
++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
Approximate Flare Start  :  23-06-2000 0359 UT
Approximate Flare Maximum:  23-06-2000 0409 UT  at Flux M 2.3
Approximate Flare End    :  23-06-2000 0419 UT
++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++


So we might think that it took some 10 hours for the faster material to get
here, or was it the real fast stuff the occured as you heard the signal?

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Peter Dodd" <g3ldo@zetnet.co.uk>
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Steve Olney said

> Here in Sydney Australia we have (had) a CFA installation in commercial use.
> I have done relative FS measurements (single point) at a distance of 60Km
> and can report that the CFA antenna is NOT working as the inventors say it will.  

In my early days of Ham radio I visited a radio ham who used one of 
those old metal spring double beds as an antenna. The bed was 
connected to the hot end of the ATU and the other to the water pipe 
of a sink that was also in the room. As I recall he seemed to work 
around the UK on 80m using it. I called it the Sleep Mode Antenna (SMA).

The Electronics World and Wireless World articles referring tothe CFA 
antenna (I think G4JNT asked) are:

Maxwell's Equations and the Crossed Field Antenna, March 1989
The Crossed Field Antenna in Practice, Nov 1989
CFA Experiments, March 1990
CFA Working Assumption, Dec 1990
CFA-RIP, May 1993

The last article is a documented project, part of a final year 
Electronic and Electrical Engineering degree course project, by Colin 
Davis to test the CFA antenna. His conclusion disputes the hypothesis 
behind the CFA antenna and cast doubts on its performance claims.
  

-- 
Regards, Peter, G3LDO

<g3ldo@zetnet.co.uk>






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: Shrinking sounds - fiasco
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From:           	Paul Keinanen <keinanen@sci.fi>
To:             	rsgb_lf_group@blacksheep.org
Subject:        	LF: Re: Shrinking sounds - fiasco
Date sent:      	Fri, 23 Jun 2000 15:48:12 +0300
Send reply to:  	rsgb_lf_group@blacksheep.org

> On Fri, 23 Jun 2000 10:27:59 +0100, Talbot Andrew
> <ACTALBOT@dera.gov.uk> wrote:
> 
> 
> >1)	Take the off air signal recording at (say) 8000 Hz sampling rate
> 
> >2)	Digitally mix down to some arbitrarily low frequency 
> 
> >3)	Filter to the necessary sub-Hz bandwidth centred on the signal
> 
> >4)	Decimate this filtered data to a much lower sampling rate by
> >just taking one sample out of every (say) 256 . 
> 
> >For anyone contemplating writing software to do this, note that stages
> >3) and 4) can be taken together - if using an FIR filter, the filtering
> >process needs to be done for each decimated sample only - this saves
> >considerable processing overhead for the long filter tap lengths
> >necessary
> 
> 
> If you plan to combine steps 3) and 4) by doing first decimating and
> then narrow band (sub-Hz) filtering, shouldn't you low pass filter the
> signal produced by the mixdown at 2) to have a bandwidth less than 15
> Hz for the final 31.25 Hz sample rate to meet the Nyquist criteria ?
> 
> Paul OH3LWR
>
 
Yes, a decimation must be preceded by a decimation filter. The output 
of this filter is only needed at the decimated rate. So, you will 
compute the FIR algorithm at the decimated rate. But the input buffer 
is at the full sample rate. And this full rate is the design rate of 
the filter. Since the pass band and the stop band are very narrow 
only very few coefficients are necessary. Usually halfband filters 
are used with less than 10 non vanishing coefficients.

Interpolation filters have to run at the up-sampled output rate. 
If the alias-suppression must be the same as with the decimation 
then the interpolation is the most costly operation of the filter. 

I made a universal multirate filter for adjustable bandwidth 
0.01 Hz ... 3kHz at -130 dB and adjustable input and output 
frequencies running on the DSP56002EVM in real time. This filter 
uses a very efficient bandpass decimation and interpolation with 
halfband filters. It is available on request.

If you have MATLAB (Student Edition or full, Ver. 5.0 or higher) 
an interactive DSP-Lecture including multirate filter design 
(Chapter 13) is available on request. 

73 de Klaus, DJ5HG





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: LF: Re: CFH and solar event??
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>From Dave G3YMC

For your information, CFH was audible at S5 on Thursday 22nd June at 0600z, some
2 hours after local sunrise.  This would be before the recent storms, so it may
indicate that CFH can be heard at all sorts of unexpected times.  Perhaps their
recent engineering work has increased their signal?

Cheers Dave
dsergeant@iee.org
http://ourworld.compuserve.com/homepages/sergeantd




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Andy Talbot" <drassew2@interalpha.co.uk>
To: "LF Group" <rsgb_lf_group@blacksheep.org>
Subject: LF: SMT Hell
Date: Sat, 24 Jun 2000 22:53:19 +0100
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For information, I am transmitting a 2.5 Hz wide SMT Hell signal
continuously on 137.6kHz with pixel duration 2s.  Use Spectran at 0.031 Hz
resolution and about 40 - 50% speed, averaging off.   Power output is 5
Watts RF to the antenna, about -33dBW ERP.

However, there may be a short break sometime tomorrow (Sunday) while I
re-route the coax feed to the antenna.

Andy  G4JNT



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Andy..
Using SpectroGram here, any idea what the best value
for the time scale in msec is.
Running it at 3000Msec now but traces are very weak.

73 de Ko, NL9222

----------
> From: Andy Talbot <drassew2@interalpha.co.uk>
> To: LF Group <rsgb_lf_group@blacksheep.org>
> Subject: LF: SMT Hell
> Date: Saturday, June 24, 2000 11:53 PM
> 
> For information, I am transmitting a 2.5 Hz wide SMT Hell signal
> continuously on 137.6kHz with pixel duration 2s.  Use Spectran at 0.031
Hz
> resolution and about 40 - 50% speed, averaging off.   Power output is 5
> Watts RF to the antenna, about -33dBW ERP.
> 
> However, there may be a short break sometime tomorrow (Sunday) while I
> re-route the coax feed to the antenna.
> 
> Andy  G4JNT
> 


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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To: dsp-weak-signal@qth.net,  rsgb_lf_group@blacksheep.org
From: "Bill de Carle" <bill@ietc.ca>
Subject: LF: Raw audio on my web page
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If anybody's interested, I just posted an audio file to my web page.
It was recorded yesterday morning while I was listening to VA3LK on
137.71 Khz.

Sample rate is 8000 samples per second, each sample consists of one
8-bit *signed* byte - i.e. the range is -128 to 127.

The signal is relatively strong but there is a lot of noise - I'd
be very interested to know how the spectrogram-type programs handle
this kind of data.

It's nearly 2 megabytes long, so will take a while to download.
I don't know how long I can leave it up there.

You can download the file called SATRAW.ZIP from my web page at:

www.ietc.ca/home/bill/bbs.htm

Bill VE2IQ



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<DIV>&nbsp;</DIV>
<DIV><FONT color=#000000 size=2>In english (bad) after</FONT></DIV>
<DIV><FONT color=#000000 size=2></FONT>&nbsp;</DIV>
<DIV><FONT color=#000000 size=2>Quel est l'adresse du sit web de la station 
mus&eacute;e SAQ (Grimeton&nbsp; Su&eacute;de) car apparemment le site serait 
inactif ? Le but est d'avoir la fr&eacute;quence exacte et les heures de la 
transmission du 2 juillet.</FONT></DIV>
<DIV><FONT color=#000000 size=2>73 de Daniel&nbsp; F1TAY</FONT></DIV>
<DIV><FONT color=#000000 size=2></FONT>&nbsp;</DIV>
<DIV><FONT color=#000000 size=2>Adress of web site of museum radio station SAQ 
(Grimeton, Sweden) ? Exact QRG and QTR of SAQ&nbsp; 2 july transmission ? 
Excused my very bad english.</FONT></DIV>
<DIV><FONT color=#000000 size=2>73 of Daniel&nbsp; F1TAY</FONT></DIV>
<DIV><FONT color=#000000 size=2>&nbsp;</FONT></DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Sun, 25 Jun 2000 13:20:56 EDT
Subject: Re: LF: GRIMETON
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Daniel  F1TAY a *crit :
>Quel est l'adresse du sit web de la station musée SAQ (Grimeton  Suéde) car 
>apparemment le site serait inactif ? Le but est d'avoir la fréquence exacte 
et les >heures de la transmission du 2 juillet.

http://www.telemuseum.se/grimeton/jubilee.html

They have changed the home page addresses this year.  The English index page 
is now:  http://www.telemuseum.se/Grimeton/defaulte.html

73,
John


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From: "John Rabson" <word.factory@zetnet.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Fw: Radiostation Grimeton
Date: Sun, 25 Jun 2000 18:23:48 +0100
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD><TITLE>Radiostationen Grimeton</TITLE>
<META content="text/html; charset=iso-8859-1" http-equiv=Content-Type><BASE 
href=http://www.telemuseum.se/grimeton/jubilee.html>
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<BODY bgColor=white>
<DIV>&nbsp;</DIV>
<DIV style="FONT: 10pt arial">----- Original Message ----- 
<DIV style="BACKGROUND: #e4e4e4; font-color: black"><B>From:</B> <A 
href="mailto:d.w.rollema@freeler.nl" title=d.w.rollema@freeler.nl>Dick 
Rollema</A> </DIV>
<DIV><B>To:</B> <A href="mailto:rsgb_lf_group@blacksheep.org" 
title=rsgb_lf_group@blacksheep.org>LF-Group</A> </DIV>
<DIV><B>Sent:</B> Wednesday, May 31, 2000 7:52 PM</DIV>
<DIV><B>Subject:</B> LF: Radiostation Grimeton</DIV></DIV>
<DIV><BR></DIV>
<DIV><FONT size=4>From the website:</FONT></DIV>
<TABLE border=0 cellPadding=0 cellSpacing=5 width=749>
  <TBODY>
  <TR>
    <TD width=169><IMG height=1 src="pics/prick.gif" width=167></TD>
    <TD><IMG alt="RADIOSTATIONEN GRIMETON" height=89 src="pics/griheade.jpg" 
      width=555></TD></TR>
  <TR>
    <TD bgColor=#ddddff vAlign=top width=169><A href="grimeng.html" 
      onmouseout="swapImage('station','pics/abubblu.gif')" 
      onmouseover="swapImage('station','pics/abubred.gif'); window.status='About the radio station';return true"><B><IMG 
      align=middle border=0 height=30 name=station src="pics/abubblu.gif" 
      width=30>THE STATION</B></A><B><BR><A href="preserve.html" 
      onmouseout="swapImage('bevara','pics/abubblu.gif')" 
      onmouseover="swapImage('bevara','pics/abubred.gif'); window.status='About the preservation';return true"><IMG 
      align=middle alt=BEVARANDE border=0 height=30 name=bevara 
      src="pics/abubblu.gif" width=30>PRESERVATION</A><BR><A href="new.html" 
      onmouseout="swapImage('vadnu','pics/abubblu.gif')" 
      onmouseover="swapImage('vadnu','pics/abubred.gif'); window.status='What is going on';return true"><IMG 
      align=middle alt="Vad nytt" border=0 height=30 name=vadnu 
      src="pics/abubblu.gif" width=30>WHAT'S GOING ON?</A><BR><IMG align=middle 
      alt=JUBILEUM border=0 height=30 name=jubileum src="pics/abubblu.gif" 
      width=30>JUBILEE<BR><A href="visit.html" 
      onmouseout="swapImage('besok','pics/abubblu.gif')" 
      onmouseover="swapImage('besok','pics/abubred.gif'); window.status='Come to the station';return true"><IMG 
      align=middle alt=BESOK border=0 height=30 name=besok 
      src="pics/abubblu.gif" width=30>VISITORS INFO</A></B></TD>
    <TD vAlign=top>
      <H2>The radio station Grimeton celebrates 75year anniversary on July 2nd, 
      2000.</H2>
      <P>H M King Gustaf V performed the official inauguration of the Swedish 
      transmitting station for wireless telegraphy to America in July 1925. The 
      75years anniversary of the royal opening ceremony will be celebrated at an 
      open house event at the second of July 2000.</P>
      <P>The great radio station with callsign SAQ at Grimeton, has a 
      alternating-current generator (alternator) as transmitter. It was 
      constructed by a Swede, Ernst F W Alexanderson, and was built in USA by 
      General Electric. The alternator produce still 200 kW to the six antennas 
      at 17,2 kHz. The Grimeton radio station is the only one left in the whole 
      world.</P>
      <P>The open house event take place 8am - 2pm (GMT) Sunday the second of 
      July 2000.</P>
      <P>The transmitter will go on air at 8.30 and 8.45am. 0.30 and 0.45pm 
      (GMT)</P>
      <P>During the jubilee the callsign SA6Q will be QRV on two stations for 
      listening reports.</P>
      <P>
      <TABLE border=0 cellPadding=0 cellSpacing=5 width=250>
        <TBODY>
        <TR>
          <TD>&nbsp;</TD>
          <TD><B>Frequency</B></TD>
          <TD><B>Mod </B></TD></TR>
        <TR>
          <TD><B>Station 1</B></TD>
          <TD>3515 +- 5 kHz</TD>
          <TD>CW</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>3740 +- 5 kHz</TD>
          <TD>SSB</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>7015 +- 5 kHz</TD>
          <TD>CW</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>7050 +- 5 kHz</TD>
          <TD>SSB</TD></TR>
        <TR>
          <TD><B>Station 2</B></TD>
          <TD>14035 +- 5kHz</TD>
          <TD>CW</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>14215 +- 5 kHz</TD>
          <TD>SSB</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>21030 +- 5kHz</TD>
          <TD>CW</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>21205 +- 5 kHz</TD>
          <TD>SSB</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>28030 +- 5 kHz</TD>
          <TD>CW</TD></TR>
        <TR>
          <TD>&nbsp;</TD>
          <TD>28415 +- 5 kHz</TD>
          <TD>SSB</TD></TR></TBODY></TABLE></P>
      <P><BR>e-mail: grimeton-radio@telia.se<BR>Fax: 0340-67 41 95, Phone: 
      0340-67 42 51<BR></P></TD></TR></TBODY></TABLE>
<P>2000-03-25 <A 
href="mailto:grimeton-radio@telia.se">grimeton-radio@telia.se</A> 
<P>
<P>Thanks Christer, SM6PXJ, for the hint! 
<P>73,&nbsp; Dick, PA0SE</P></BODY></HTML>

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--------------050701040700050504050002--

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: DX Cluster spots for June 24/25th at GB7DXM
Date: Sun, 25 Jun 2000 22:19:14 +0100
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Hi All, first the return of CFH is confirmed by Larry. It seems to be
visible between about 2400z and 0600z here, reaching the same sort of
strength I saw it in the winter. Unfortunately our man-on-the-spot Jean-Marc
has moved west now so we have no way of confiming that it is still radiating
the same power it was before the TX change. The enhanced daytime trace that
I reported on Friday (1449-1459z) seems to correlate with an M2 X-ray burst
(Thanks to Larry for that gen). I only saw the estimated last 10 minutes of
what was probably a 30 minute event, and the peak strength was certainly
within about 6dB of the peak night-time strength. Did anyone see enhancement
from the delayed particle streams, maybe Sunday?


Stations heard here on what seemed like a fairly low activity weekend
G8RW,PA0SE,PA0BWL,DJ9IE,G3XDV,  all at good strength, and a call I have not
heard before G0VXG who was 559 here on Sat at 1803z on an unanswered CQ.
Good copy from Andy's 2.5Hz 5watt SMT-Hell after a bit of playing with the
parameters on Spectran. He would have been an easy 'O' signal on Spectrogram
(0.7Hz) on QRS CW. Which just goes to show how far 5 watts will travel !
There were two stations on Sunday morning with DFCW, I suspect at one stage
Markus DF6NM may have been working Valerio. I did decode the name but was
running 'gram too slowly to get an full decode easily on a weakish signal.
If it was Valerio IK1ZPV I did not copy his signal at that time. Was there a
bust of 5Hz Hell in the transmission Markus?

Spots from the cluster follow, no G stations logged :-

   136.7  DL3FDO      25-Jun-2000 0952Z  cq    <DL6SN>
   136.5  DK6NI       25-Jun-2000 0925Z  cq    <DL6SN>
   136.8  OK1DTN      25-Jun-2000 0909Z  cq    <DL6SN>
   136.8  OK1DTN      25-Jun-2000 0903Z        <DL3FDO>
   136.9  DJ2EY       25-Jun-2000 0804Z  559 cq<DL1SAN>
   136.7  DJ2EY       25-Jun-2000 0713Z            <DL6SN>
   136.8  OK1DTN      25-Jun-2000 0653Z  539 in JN58AU<DL6SN>
   136.7  OK1DTN      25-Jun-2000 0647Z  559 cq<DL1SAN>
   136.5  OK1DTN      18-Jun-2000 1848Z  now-like ever-vy gd<HA6PC>
G3NYK de GB7DXM   25-Jun 1900Z >

73 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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To: rsgb_lf_group@blacksheep.org
From: =?iso-8859-1?Q?V=E4in=F6_Lehtoranta?= <vaiski@dlc.fi>
Subject: LF: Signal Strength Measurements by OH2LX, 26 June 2000
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Signal strength measurements of various LF stations by OH2LX:

VLF NAV system "Alpha" has been back since the 20th June...
------------------------------------------------------------------
Day ------------------   19Jun 20Jun 21Jun 22Jun 23Jun 24Jun 25Jun
                          MON   TUE   WED   THU   FRI   SAT   SUN 
Time, UTC ------------    2055- 2110- 2050- 2055- 2045- 2050- 2050-
------------------------------------------------------------------
kHz    Stn   d,km  AZI          Indicated ESH2 input, dBmW
------------------------------------------------------------------
 68.9 DHJ58? 1115, 242   -103  -103  -105   Nil   Nil   Nil   Nil
------------------------------------------------------------------
 73.3 Rugby, 1825, 252,  -105c -104c -104c -106c -105c -106  -105
------------------------------------------------------------------
 75.0   HBG, 1992, 226,  -107  -102  -105  -109  -107  -111  -109
------------------------------------------------------------------
 77.5 DCF77, 1543, 228,   -91   -85   -90   -89   -91   -91   -92
------------------------------------------------------------------
128.9 DCF49, 1544, 228,   -93   -87  -103   -96   -95   -93   -97
------------------------------------------------------------------
138.8 DBF39, 1221, 226,   -89   -91   -93   -89   -91   -90   -95
------------------------------------------------------------------
135.8   SXV, 2490, 182,  -101  -109  -115  -110  -107  -109  -110
------------------------------------------------------------------
137.0   CFH, 5750, 295,   Nil   Nil   Nil   Nil   Nil   Nil   Nil
------------------------------------------------------------------
(R&S ESH2/---- 10m coax----/1:10/-----15m wire-----):
 Noise level with antenna: with 200Hz IF BandWidth: 
-24..-20 dB(uV), -131..-127dBmW (varies with frq, qrm, qrn etc)
------------------------------------------------------------------
73.3: - c = carrier not identified, assumed to be Rugby
------------------------------------------------------------------
End of message of 26th June 2000, 0800 UTC, from OH2LX
------------------------------------------------------------------
----------------------------------------------------------
V.K.Lehtoranta, OH2LX, POBox 50, FIN-05401 Jokela, Finland
------ Tel: +358-9-4173965 ---- Fax: +358-9-4173961 ------
E-mail: vaiski@dlc.fi - alias: oh2lx@dlc.fi & oh2lx@sral.fi


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: New Spectrogram - "EasyGram"
Date: Mon, 26 Jun 2000 09:22:18 +0200
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<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 4.0 Transitional//EN">
<HTML><HEAD>
<META content="text/html; charset=iso-8859-2" http-equiv=Content-Type>
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<STYLE></STYLE>
</HEAD>
<BODY bgColor=#ffffff>
<DIV><FONT face=Arial size=2>Hello LowFers</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I have made my own user interface for Spectrum.dll 
(by R.S.Horne).&nbsp;My&nbsp;interface provides the same functionality as 
Spectrogram, but it has a more user-friendly access. Main 
differences:</FONT></DIV>
<DIV><FONT face=Arial size=2>1. All the settings can be done while scanning runs 
(like Spectran)</FONT></DIV>
<DIV><FONT face=Arial size=2>2. The picture moves in a separate window. This 
enables to change the size and position of the window (don't do it with mouse 
but by entering numbers in configuration). Also, the scanning window can be 
maximized accross the whole screen.</FONT></DIV>
<DIV><FONT face=Arial size=2>3. All the settings can be saved to a 
"profile".&nbsp;Once the profile is defined, you can select all the settings at 
once by selecting the profile - item in a combo box. This includes also position 
and size of the scanning window.</FONT></DIV>
<DIV><FONT face=Arial size=2>4. Vertical (waterfall) scanning is 
possible.</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2>I created it during weekend so that it is not fully 
finished yet and therefore it is an Alpha version. Also, help is missing and 
"about box" with thanks to the author of Spectrum.dll.</FONT></DIV>
<DIV><FONT face=Arial size=2>Download the file from:</FONT></DIV>
<DIV><FONT face=Arial size=2><A 
href="http://mujweb.cz/www/ok1fig/EasyGram.htm">http://mujweb.cz/www/ok1fig/EasyGram.htm</A></FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV><FONT face=Arial size=2></FONT><FONT face=Arial size=2>73, Petr 
OK1FIG</FONT></DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV>
<DIV>&nbsp;</DIV></BODY></HTML>

From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 26 Jun 2000 10:36:01
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: Re: LF: LFCC Award Proposal
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>PROPOSAL TO ESTABLISH A LOW FREQUENCY CENTURY CLUB AWARD (LFCC)
>By Les Rayburn, KT4OZ
>
> ...
>
>0-100Khz (VLF Endorsement): Award would be granted to those operators who
>could verify reception of stations in 25 Maidenhead grid squares.
Endorsements
>for each additional 25 stations.
>
>76Khz (Amateur VLF Endorsement): Award would be granted to those operators
>who could verify two way contacts with or reception of stations in 10 
>Maidenhead grid squares. Endorsements for each additional 10 grid squares.
>
> ...
>
>136Khz (Amateur LF Endorsement): Award would be granted to those operators
>who could verify two way contacts with or reception of stations in 25 
>Maidenhead grid squares. Endorsements for each additional 25 grid squares.
>

Good idea, but is does not agree with the 'official ranges' :
VLF = 3 to 30kHz
LF = 30 to 300 kHz
So the 75kHz UK allocation is actually LF, not VLF

73, Rik ON7YD



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From: "Talbot Andrew" <ACTALBOT@dera.gov.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: Re: SMT Hell
Date: Mon, 26 Jun 2000 09:37:50 +0100
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No, the version of Spectrogram I use does not have the time delay
function.  Use Spectran instead.  For this 2.5Hz mode Gram will not go
narrow enough I suspect. even if you do get the delay right.

Andy G4JNT


> ----------
> From: 	Ko Versteeg[SMTP:nl9222tv@tref.nl]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-25 10:35
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	LF: Re: SMT Hell
> 
> Andy..
> Using SpectroGram here, any idea what the best value
> for the time scale in msec is.
> Running it at 3000Msec now but traces are very weak.
> 
> 73 de Ko, NL9222
> 
> ----------
> > From: Andy Talbot <drassew2@interalpha.co.uk>
> > To: LF Group <rsgb_lf_group@blacksheep.org>
> > Subject: LF: SMT Hell
> > Date: Saturday, June 24, 2000 11:53 PM
> > 
> > For information, I am transmitting a 2.5 Hz wide SMT Hell signal
> > continuously on 137.6kHz with pixel duration 2s.  Use Spectran at
> 0.031
> Hz
> > resolution and about 40 - 50% speed, averaging off.   Power output
> is 5
> > Watts RF to the antenna, about -33dBW ERP.
> > 
> > However, there may be a short break sometime tomorrow (Sunday) while
> I
> > re-route the coax feed to the antenna.
> > 
> > Andy  G4JNT
> > 
> 


-- 
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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: Mon, 26 Jun 2000 12:19:58 +0100
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> So we might think that it took some 10 hours for the faster material to
> get here, or was it the real fast stuff the occured as you heard the
> signal?

The only time I have recorded an enhancement of the reception of 
CFH coincided exactly with a major flare so the suggestion is "the 
real fast stuff". If true, this is bad news as we really need some 
warning if we are to make the best of a short enhancement. 
Interestingly this occasion was the day after some other flares, so 
perhaps it needs both.

See http://www.dennison.demon.co.uk/mike/cfh.htm



Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Mon, 26 Jun 2000 12:30:58 +0100
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> > Here in Sydney Australia we have (had) a CFA installation in commercial
> > use. I have done relative FS measurements (single point) at a distance
> > of 60Km and can report that the CFA antenna is NOT working as the
> > inventors say it will.  
> 
> In my early days of Ham radio I visited a radio ham who used one of 
> those old metal spring double beds as an antenna. The bed was 
> connected to the hot end of the ATU and the other to the water pipe 
> of a sink that was also in the room. As I recall he seemed to work 
> around the UK on 80m using it. I called it the Sleep Mode Antenna (SMA).

Many years ago, RadCom (actually it was the RSGB BUlletin in 
those days) ran a superb April spoof. It described an antenna 
comprising two circular plates joined by vertical bars like a cage. 
The clever bit was that the bars were spaced logarithmically from 
each other. More complex calculation went into where to attach the 
feedpoint - a single wire - off centre of the lower plate.

This was all fascinating and believable until you got to the final 
sentence whch said that for best results the single wire feeder 
should be vertical and at least a quarter wavelength, tuned against 
a good ground.

This was probably aimed at a popular short loaded antenna of the 
day called a Joystick, but which was also called the VFA (variable 
frequency antenna).


Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



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: VON DER LEY 18m fiberglass masts
Date: Tue, 27 Jun 2000 12:26:37 +0100
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I intend ordering either one or two of the 18m fiberglass 
masts produced in Germany by VON DER LEY and wondered if anyone
else in the UK would be interested in ordering one at the same
time, to cut down on the transport costs.

The last time I checked the masts cost about 160 pounds including
transport from Germany.

73s Tracey G5VU





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Dave Goodwin VE2ZP/VE9CB" <VE2ZP@sympatico.ca>
To: "137kHz" <rsgb_lf_group@blacksheep.org>
Subject: LF: VA3LK Beacon Heard by VE2ZP
Date: Tue, 27 Jun 2000 10:38:47 -0400
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This morning, Tuesday 27 June, from 0600-0620z (2am local), I copied Larry
VA3LK's beacon on 137.71kHz.  VA3LK sounded about s4, compared to CFH which
was s8 from 1200km away.  At 1430z (10.30am local), VA3LK was slightly
weaker.

Larry's signal was certainly strong enough for a conventional CW contact.
It is quite an adjustment to copy morse at 0.4wpm.

Larry's location is less than 200km from here (near Ottawa), so this is no
great DX, but this is the first Amateur LF signal I have heard to date.
Larry is probably the only Canadian Amateur transmitting on LF at present.

73,

Dave VE2ZP



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Petr's Easygram
Date: Tue, 27 Jun 2000 20:32:45 +0100
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Hi all. Petr has done a nice job of front-ending Robert's software. The
major advantage is to be able to adjust the parameters without losing, and
having to restart, the display. It will be interesting to see if those who
have trouble with Robert's original version, find they can access the 5000
samples/s facility via Petr's menu. There are yet some interesting
parts.....I am trying to work out how to use a bandwidth of
-10Hz, before he removes it from the menu!

I'm afraid I may have messed up the LF DX as I have already posted him a
substantial 'Wish List' !! Petr doesn't say so (unless its in the
'manual'....and nobody reads those  .......do they!) but I assume it will
require Win95/98/2000 as does the original.

Nice piece of work Petr, thanks for your efforts.
73 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: "Michael Probert" <mike@boxernet.demon.co.uk>
To: rsgb_lf_group@blacksheep.org
Subject: LF: RE: VON DER LEY 18m fiberglass masts
Date: Tue, 27 Jun 2000 10:55:59 +0100
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-----Original Message-----
From: majordom@post.thorcom.com [mailto:majordom@post.thorcom.com]On
Behalf Of tracey.gardner
Sent: 27 June 2000 12:27
To: rsgb_lf_group@blacksheep.org
Subject: LF: VON DER LEY 18m fiberglass masts



I intend ordering either one or two of the 18m fiberglass 
masts produced in Germany by VON DER LEY and wondered if anyone
else in the UK would be interested in ordering one at the same
time, to cut down on the transport costs.

The last time I checked the masts cost about 160 pounds including
transport from Germany.

73s Tracey G5VU
njdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjdjnvnvnvn
vnvnvvmmmvmvvnbvhffufuyryurrririririrryryryrggdyututut





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Message-ID: <003601bfe0e8$bae186c0$0a00a8c0@server1.ThreeLakes.ca>
From: "Larry Kayser" <kayser@sympatico.ca>
To: rsgb_lf_group@blacksheep.org
Subject: LF: Wire, for LF Antennas
Date: Wed, 28 Jun 2000 06:06:12 -0400
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Greetings:

Preparations continue for TransAtlantic II, the test transmissions from here
in Eastern Ontario on 137.710 kHz are now heard widely in the USA and
Canada.

Moving forward through the lists of things and issues to be worked on, the
subject of WIRE for LF antennas comes up.  The objective of this email is to
have a discussion with active LF amateurs that will ensure for me at the end
of the day that the best alternatives have been discovered and considered
for use here.

The current antenna here for the test transmissions is made from what we
here call common antenna wire, 7 strands of semi hard copper wire, commonly
known as 7/24.  For LF the type of wire is marginal, when used for long
spans it stretches and anneals, becomes eventually very brittle and fails.
A lousy wire solution for long spans associated with LF antennas.  The LF
test antenna here is far from optimum because I simply do not dare to
stretch the wire harder with the rope that pulls the antenna away from the
supporting tower.

The alternative selections available here are very limited.  There is a
reasonable quantity of semi hard drawn solid copper wire #12, commonly used
by the Broadcast Station industry.  I use this for MF/HF antennas but it is
also subject to annealing and stretching.

We have available an insulated wire known variously as "FlexWeave", similar
to Litz wire but without the shellac to hold the wire together.  This is
around 75 and 150 strands in the two sizes that are usually available.  The
issue here again is strength, 150 Meter spans do not last very long.

The last is the good old copper clad steel wire, not much copper any more
but usually pretty good for long spans.  Sources of this product are
limited, a good source here in Canada would be a help.

What are the other alternatives that you are using in your setup?  Why are
they good?  What is the usual cost in your area?  If you were looking at
spans of up to 300 Meters what would you use for an antenna wire?

Not a glorious subject, but one which is important to the LF community.
Your comments are solicited.

Larry
VA3LK





From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 28 Jun 2000 11:24:41 +0100
To: rsgb_lf_group@blacksheep.org
From: "Brian Rogerson" <brian@esoterica.pt>
Subject: Re: LF: Wire, for LF Antennas
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Aluminium?

Much lighter so you can use larger diameters.  I use it extensively now,
without
problem to date but can only claim a 40m span folded dipole with 2.5mm
diameter wire.

Brian, CT1DRP

At 06:06 28/06/00 -0400, you wrote:
>Greetings:
>
>Preparations continue for TransAtlantic II, the test transmissions from here
>in Eastern Ontario on 137.710 kHz are now heard widely in the USA and
>Canada.
>
>Moving forward through the lists of things and issues to be worked on, the
>subject of WIRE for LF antennas comes up.  The objective of this email is to
>have a discussion with active LF amateurs that will ensure for me at the end
>of the day that the best alternatives have been discovered and considered
>for use here.
>
>The current antenna here for the test transmissions is made from what we
>here call common antenna wire, 7 strands of semi hard copper wire, commonly
>known as 7/24.  For LF the type of wire is marginal, when used for long
>spans it stretches and anneals, becomes eventually very brittle and fails.
>A lousy wire solution for long spans associated with LF antennas.  The LF
>test antenna here is far from optimum because I simply do not dare to
>stretch the wire harder with the rope that pulls the antenna away from the
>supporting tower.
>
>The alternative selections available here are very limited.  There is a
>reasonable quantity of semi hard drawn solid copper wire #12, commonly used
>by the Broadcast Station industry.  I use this for MF/HF antennas but it is
>also subject to annealing and stretching.
>
>We have available an insulated wire known variously as "FlexWeave", similar
>to Litz wire but without the shellac to hold the wire together.  This is
>around 75 and 150 strands in the two sizes that are usually available.  The
>issue here again is strength, 150 Meter spans do not last very long.
>
>The last is the good old copper clad steel wire, not much copper any more
>but usually pretty good for long spans.  Sources of this product are
>limited, a good source here in Canada would be a help.
>
>What are the other alternatives that you are using in your setup?  Why are
>they good?  What is the usual cost in your area?  If you were looking at
>spans of up to 300 Meters what would you use for an antenna wire?
>
>Not a glorious subject, but one which is important to the LF community.
>Your comments are solicited.
>
>Larry
>VA3LK
>
>
>
>
>
>




From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Wed, 28 Jun 2000 13:15:47 +0100
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From: "Tom Boucher" <tom@telemetry.demon.co.uk>
Subject: LF: Antenna Wire
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Larry & all

My 1100 ft horizontal long wire is made from 32 X 0.2mm thin wall PVC
covered, 10 amp plain annealed copper wire, Arrow Stock No: 438095B,
cost 30.42 pounds per 500m reel.

Maximum length between halyards was about 200 feet or so and this stayed
up without trouble for 8 months. However, I foolishly disposed of one
halyard which resulted in a run of around 400 feet which did not last,
and with the winds of late, have been unable to keep it up in the air.

Current plan is to replace halyards, limiting maximum span to 200 ft and
stick with the same wire which seems to be relatively strong and light
weight. If that doesn't work, perhaps try a thicker wire - Arrow have 21
X 0.3mm at GBP46/500m or 28 X 0.3 at GBP54/500m - unless someone comes
up with a better idea.

Brian, where did you obtain your alumin(i)um wire?

73, Tom G3OLB.


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Petr's Easygram
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G3NYK wrote:

>I am trying to work out how to use a bandwidth of -10Hz, before
> he removes it from the menu!

Don't remove this one. It should give better than infinite signal to 
noise ratio. You should be able to light a small city with the output 
from a signal that you just thought might be on the air.



Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.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 LF Group,
	
I believe most LF amateurs favour string for their antennas - 
preferably well soaked in brine to maximise conductivity...

But seriously, I have found 24/0.2 or 32/0.2 stranded PVC 
insulated wire suprisingly robust - it has put up with winter gales 
and so on in spans up to 40m, even though the trees it is attached 
to wave about a lot in the wind. It seems to put up with flexing a lot 
better than solid wire, and the sheathing prevents corrosion. I don't 
suppose it is very useful as a mechanical support, though, and if 
you are lucky enough to have room for longer spans, it might not 
be up to the job.

Cheers, Jim Moritz
73 de M0BMU


From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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> Preparations continue for TransAtlantic II, the test transmissions from
> here in Eastern Ontario on 137.710 kHz are now heard widely in the USA and
> Canada.

Larry,

It would help if you could give an idea of the sort of distances being 
covered and what you believe your erp is now. Nothing seen at my 
end at 0200UTC last night even though CFH was S9.

73


Mike, G3XDV (IO91VT)
http://www.dennison.demon.co.uk/activity.htm



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Subject: Re: LF: Petr's Easygram
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>>I am trying to work out how to use a bandwidth of -10Hz, before
>> he removes it from the menu!
 
 >Don't remove this one. It should give better than infinite signal to 
 >noise ratio. You should be able to light a small city with the output 
 >from a signal that you just thought might be on the air.

Actually, I suspect it would take a bandwidth closer to -30Hz to achieve that 
much output.  But I'm having a little trouble with the maths necessary to 
prove it.  This dividing by zero business is harder than I thought....

73,
John  KD4IDY



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: robin@g3lba.freeserve.co.uk
To: rsgb_lf_group@blacksheep.org
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Subject: Re: LF: Petr's Easygram
Date: Wed, 28 Jun 2000 18:24:43 +0100
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Dividing by Zero is easy.... My Windows PC tries it all the time!!
Robin
----- Original Message -----
From: <WarmSpgs@aol.com>
To: <rsgb_lf_group@blacksheep.org>
Sent: Wednesday, June 28, 2000 5:41 PM
Subject: Re: LF: Petr's Easygram


> >>I am trying to work out how to use a bandwidth of -10Hz, before
> >> he removes it from the menu!
>
>  >Don't remove this one. It should give better than infinite signal to
>  >noise ratio. You should be able to light a small city with the output
>  >from a signal that you just thought might be on the air.
>
> Actually, I suspect it would take a bandwidth closer to -30Hz to achieve
that
> much output.  But I'm having a little trouble with the maths necessary to
> prove it.  This dividing by zero business is harder than I thought....
>
> 73,
> John  KD4IDY
>
>
>



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: Wed, 28 Jun 2000 18:17:31 EDT
Subject: Re: LF: Petr's Easygram
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In a message dated 6/28/00 2:27:18 PM Eastern Daylight Time, 
robin@g3lba.freeserve.co.uk writes:

<< Dividing by Zero is easy.... My Windows PC tries it all the time!! >>

If it succeeds, please advise soonest.  Will make generous offer.  :)



From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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From: "Alan Melia" <Alan.Melia@btinternet.com>
To: "rsgb_lf_group" <rsgb_lf_group@blacksheep.org>
Subject: LF: Antenna wire materials
Date: Wed, 28 Jun 2000 20:26:24 +0100
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Hi Larry, I will fly this through the reflector so it can generate some
Flak. It occurs to me that you are having separate TX and RX sites......so
presumably separate aerials.
I would not think that you want to transmit into a very long wire (though
several do quite successfully) but that your main interest in this would be
in receive as a Beverage format. My reason for saying this is that I suspect
that wire resistance is not quite so much an issue on a receive aerial, so
you could probably use a steel/copper stranded mix for a long span. You do
not want to put a lot of effort into the erection of many support masts for
such a short period.  I am aware that a good TX antenna is usually a good RX
antenna, but the reverse is not necessarily true (e.g. small loop)

Now, at the risk of creating a furore, in the case on an 'L' or a 'T'
antenna for TX, the current flowing in the vertical section is all important
so this needs to be thick and low resistance, but when it gets up into the
top section it doesn't matter so much as this is all 'top loading' so
several smaller lighter wires would do. You could even use telephone
'drop-wire' (steel/copper stranded mix, you can see my upbringing, but I
don't know whether your telcos have a different name for it ) the current in
these wires is supposed to be lost to radiation so what matter if a bit is
lost in resistance?.  That is a challenge to the modellers to calculate how
many tenths of a dB you will loose with resistive top wires.  I am assuming
you will not want to transit on a low horizontal dipole, because too much of
the power would be lost straight up in the air.

On top of these you will need to consider the kind of wire for kite use (I
think you said you had found a kite specialist)  Dave and Mike are better
sources on that topic.

Hopefully my misconceptions can be corrected with experimental experience,
but I do like to look at problems from strange angles, if not quite
laterally.

Cheers de Alan G3NYK
Alan.Melia@btinternet.com




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In a message dated 6/28/00 11:21:39 AM GMT Daylight Time, kayser@sympatico.ca 
writes:

<< Moving forward through the lists of things and issues to be worked on, the
 subject of WIRE for LF antennas comes up.  The objective of this email is to
 have a discussion with active LF amateurs that will ensure for me at the end
 of the day that the best alternatives have been discovered and considered
 for use here. >>

Hi All.
I've tried various insulated stranded copper 'equipment' wire which is OK in 
short runs, or for a short time.
The Whitton club antenna, and the /P antenna used at Hastings is standard 
hard drawn copper in UK 16 gauge ( apx. 1.7mm dia )
The clubs 234 foot has been in place for 2 years without problem but the 
extra tension to raise 300m would be considerable.   Price here is £15 per 
100m.

The resistive losses in the antenna should be minor compared to the losses in 
the coil / ground system.

How about a thin steel cable under a lot of tension, used to support a lower 
loss copper radiator. As in power distribution between pylons?

73


David  G0MRF


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
Subject: LF: Louis, G5RV, Silent Key
Date: Thu, 29 Jun 2000 08:50:23 -0400
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I have just had a short email on the FOC reflector saying that Louis, G5RV
has passed away at noon UK time yesterday.

Larry
VA3LK





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: Louis, G5RV, Silent Key
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> I have just had a short email on the FOC reflector saying that Louis, G5RV
> has passed away at noon UK time yesterday.

See the rsgb web site for more info.





Mike Dennison, G3XDV
Publications Manager

* RadCom * Ham Radio Today * GB2RS News *
* RSGB Books and CDs *

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

RSGB - UK AMATEUR RADIO



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: Wire, for LF Antennas
References: <003601bfe0e8$bae186c0$0a00a8c0@server1.ThreeLakes.ca>
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Larry,

Mentioned for completeness, at the Quartz Hill ZL6QH DX station, of
which I am a member, we decided to use high tensile 12 gauge galvanised
steel wire for replacement of any of the long Vee antennas.  Legs are
typically 250 to 300 metres long.  We modelled the situation and found
that losses were only fractional compared to using hard drawn copper. 
Some have been installed for over a year, and Wellington has a
reputation for being "Windy Wellington".  The 12 gauge high tensile
galvanised steel wire is in regular use for fences on New Zealand farms,
so is cheap and available.

The ZL6QH Vees are all fairly high (surge) impedance wires at the MF/HF
bands and that is why a few more ohms of surface resistance does not
give rise to a significant loss factor.

An LF antenna may well be a low resistance affair where series
resistance in the "top loading" is significant, at least for
transmitting efficiency.  I think another reply on the reflector
mentioned using copper for an "upwire" and galvanised steel for the top
loading.  In terms of "bang for buck" it could pay to concentrate on a
higher upwire than wider top loading.

73, Bob



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: RE: LF: Wire, for LF Antennas
Date: Fri, 30 Jun 2000 08:37:29 +0100
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There is also the issue of reduced skin depth and extra losses when
using steel wire, or any other magnetic material for that matter.   Skin
depth reduces as the square root of relative permeability, which for
steel wire is several thousand.

Did the modelling of the MF atnennas take this magnetic wire effect into
account, although at those frequencies much of the current will be
concentrated in the zinc galvanising so reducing the Ur losses.

As you say, the high impedance of these antenna will not show up the
losses in the wire nearly as much as using steel wire at LF where skin
depth is 0.2mm or so.

Andy  G4JNT


> ----------
> From: 	vernall[SMTP:vernall@xtra.co.nz]
> Reply To: 	rsgb_lf_group@blacksheep.org
> Sent: 	2000-06-30 07:46
> To: 	rsgb_lf_group@blacksheep.org
> Subject: 	Re: LF: Wire, for LF Antennas
> 
> Larry,
> 
> Mentioned for completeness, at the Quartz Hill ZL6QH DX station, of
> which I am a member, we decided to use high tensile 12 gauge
> galvanised
> steel wire for replacement of any of the long Vee antennas.  Legs are
> typically 250 to 300 metres long.  We modelled the situation and found
> that losses were only fractional compared to using hard drawn copper. 
> Some have been installed for over a year, and Wellington has a
> reputation for being "Windy Wellington".  The 12 gauge high tensile
> galvanised steel wire is in regular use for fences on New Zealand
> farms,
> so is cheap and available.
> 
> The ZL6QH Vees are all fairly high (surge) impedance wires at the
> MF/HF
> bands and that is why a few more ohms of surface resistance does not
> give rise to a significant loss factor.
> 
> An LF antenna may well be a low resistance affair where series
> resistance in the "top loading" is significant, at least for
> transmitting efficiency.  I think another reply on the reflector
> mentioned using copper for an "upwire" and galvanised steel for the
> top
> loading.  In terms of "bang for buck" it could pay to concentrate on a
> higher upwire than wider top loading.
> 
> 73, Bob
> 
> 


-- 
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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, 
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From rsgb_lf_group@blacksheep.org Sun Jan 01 00:00:00 1970
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Date: Fri, 30 Jun 2000 12:14:47
To: rsgb_lf_group@blacksheep.org
From: "Rik Strobbe" <rik.strobbe@fys.kuleuven.ac.be>
Subject: RE: LF: Wire, for LF Antennas
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At 08:37 30/06/00 +0100, G4JNT wrote:
>There is also the issue of reduced skin depth and extra losses when
>using steel wire, or any other magnetic material for that matter.   Skin
>depth reduces as the square root of relative permeability, which for
>steel wire is several thousand.

Following might be interesting :

Aluminium has a lower conductivity compared to Copper (1.76 lower) but has
a higher skin-depth (on 136kHz : .18mm for Cu, 0.24 for Al).
The result is that for wires with a diameter of more than 1mm Al is only
32% worse than Cu. Or otherwise, a 1.3mm Al wire will have the same losses
as a 1mm Cu wire while the weight of 1.3mm Al wire is only half of 1mm Cu
wire.

73, Rik  ON7YD



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Date: Fri, 23 Jun 2000 16:50:20 -0500
To: lowfer@qth.net
Subject: LF: LFCC Award Proposal
Cc: rsgb_lf_group@blacksheep.org
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PROPOSAL TO ESTABLISH A LOW FREQUENCY CENTURY CLUB AWARD (LFCC)
By Les Rayburn, KT4OZ
June 23, 2000


Objective: To outline a set of suggested guidelines for the establishment
of an award
targeted at the users of the Low Frequency (Below 500Khz) spectrum. This
award would 
encourage more activity on LF, and spur users to pursue multiple endorsements.

Governing Body: Ideally, an LF organization like the Longwave Club of
America. Failing that
alternate bodies might include AMRAD, RGSB, or ARRL. 

Award: Certificate, with endorsement stickers.

Program Brief: This award would be open to amateur radio operators,
lowfers, longwave listeners,
and maritime operators.  Operators would be required to submit QSL cards, or
other verification proof to the governing body to be checked for
completeness and accuracy.
The decision of the governing body would be final and not available for
review. 

Certificates would be numbered beginning with LFCC #1 (* See Note Below)

Certificates to be awarded according to the guidelines below:


0-100Khz (VLF Endorsement): Award would be granted to those operators who
could verify 
reception of stations in 25 Maidenhead grid squares. Endorsements for each
additional 25 stations.


73Khz (Amateur VLF Endorsement): Award would be granted to those operators
who could verify two way contacts with or
reception of stations in 10 Maidenhead grid squares. Endorsements for each
additional 10 grid squares.

Amateurs who operate in the 73Khz range would be required to provide proof
of either reception of their
station, other stations, or two way contacts to qualify. No contacts with
non amateur stations can count towards
this endorsement. LF Listeners would receive the Amateur VLF DX Endorsement. 


136Khz (Amateur LF Endorsement): Award would be granted to those operators
who could verify two way contacts with or
reception of stations in 25 Maidenhead grid squares. Endorsements for each
additional 25 grid squares.

Amateurs who operate in the 136Khz range would be required to provide proof
of either reception of their
station, other stations, or two way contacts to qualify. No contacts with
non amateur stations can count towards
this endorsement. LF Listeners would receive the Amateur LF DX Endorsement.


160-190Khz (Lowfer Endorsement): Award would be granted to those operators
who can verify reception of their
LF beacon in at least 10 Maidenhead grid squares. Endorsements for each
additional 5 grid squares. 

LF Listeners (including beacon operators) could also receive the Lowfer DX
Endorsement for reception of lowfer
beacons in at least 5 grid squares. Endorsements for each additional 5 grid
squares. 

100Khz-500Khz (LF Endorsement): Award would be granted to those operators
who could verify reception of stations in 
at least 100 Maidenhead grid squares. Endorsements for each additional 50
grid squares.

This stations could include any combination of NDB, TWIB, Maritime
stations, broadcasting, etc. 


Basic Rules: Verification could be in the form of a QSL card, verification
letter, or other supporting documentation. The 
governing body would appoint a chairman to inspect and return these
verifications. Any operator submitting
false or suspect documentation will have those cards marked by the Chairman
and their application of LFCC
returned. There is no appeal. Operators must resubmit application without
those documents judged to be
false or suspect. 

Basic costs would be covered in the application fee (Suggestion $10-$20). 

Contacts and receptions must have occurred on or before 1980 (I doubt that
reliable frequency listings
exist much before this date.)


Comments: Many LF operators would already qualify for this award. In the
case of veteran NDB dx'ers
they might even qualify for several endorsement stickers! But for many of
us, it would represent
a goal that was realistic and achievable...but difficult enough to
encourage effort. 

There are many out there who object to "paper-chasing" of any kind on the
low frequencies, and this
is understandable. However, if we hope to see amateur allocations grow and
foster in this band,
activity is what we need. Also many of us Lowfers do not have even a single
serious LF listener
within the normal range of our stations, growth is important in these areas
too.

I would further suggest that honorary LFCC's be granted to recognize those
pioneers
of the band who are no longer living or inactive. For example, Ken Cornell,
or Vince Pinto.


Comments are welcome.







