----- Original Message -----
Sent: Saturday, January 21, 2006 3:14
PM
Subject: LF: Re: Re: TA 21 JAN 06
Mal
Yes, I seem to have no problem seeing you
whenever you're on.
I would recommend 136.3165 khz as
that will put you out in the open even if M0BMU is on the air. Will look
for you in QRSS20 or 10 starting around 0000Z.
Jay.
I will tx on 136.3165 khz, hope to be on tonight
if all goes to plan.
73 and gl de Mal/G3KEV
We have another rain/snow storm on the
way so things may be a bit noisey but will
be watching in any case.
Jay, W1VD
----- Original Message -----
Sent: Saturday, January 21, 2006 9:37
AM
Subject: LF: Re: TA 21 JAN 06
----- Original Message -----
From: Jay
Rusgrove
To: [email protected]
Sent: Saturday, January 21, 2006 12:24 PM
Subject: LF: TA
21 JAN 06
Good signal levels, low static but some rapid
fading. CT1DRP and DJ8WX present as usual...will be happy to watch for others
as well!
Captures: http://www.w1vd.com/gallery2006.html
Mal...saw some QRM on CT1DRP's lower DFCW frequency but didn't
figure out what it was until after you had QRT. Would be helpful if you could
move to a clear frequency. See capture below - plenty of open area but
remember higher QRSS speeds reduce frequency resolution.
Hi
Jay
Tnx the shots and info. I will try 136.3175 khz, it looks clear
at your end except you prefer another freq. My signal looks strong enough for
qrs 10 or 20 if you open up the b/width. I usually work around midnight to
around 0100 z for about an hour but could start earlier. Every time I transmit
you are able to see my signal at qrs 10 to 20. I have been seen in the past at
qrs 3 but the monitored b/width needs to be set for my speed.
I
usually monitor at 10 or 20 at this end and can see the lower qrs speeds with
elongated dots/dashes and narrower looking shift in the case of dfcw but it
works well and I can see them all. In the past I have monitored TR signals in
the qrs 3 mode and the dots/dashes are a mile long but perfectly
readable.
73 and appreciate your reporting of sigs from over
here.
de Mal/G3KEV
