I am looking for an HP 10638A degausser for an HP5061B Cesium Beam Standard.
Does anyone have one that they are willing to sell?
Short of that, does anyone have a schematic for the degausser they're willing
to share with me?
Thanks!
Jeff
Jeffrey K. Okamitsu, PhD, MBA
+1-609-638-5402
I've been looking for one for ages. They're out there, but at outrageous
prices.
ManualsPlus sells a very nice reprint manual with schematics.
If you're patient, I just started building a replacement using most of
the original circuitry. I'd be happy to make board files available, or a
board
Skip,
I've successfully converted my TS2100 IRIG to a GPS model along with several
other people. As far as I know, the Oncore module was never used (maybe a
planned future upgrade), but the ACE-III modules work just fine.
The trick is you need to make a temporary interface with your ACE-III and
Gerhard -- the discussion between you and Bruce has been very
interesting. I asked a VLBI colleague to look over your design and he
had this comment.
In VLBI, H-Maser frequency standards used to generate local
oscillators at microwave frequencies. We have problems with amplitude
Hi,
I listened today the WWW station and I've found it on 9.996 Mhz instead of
10.000Mhz and my receiver is fairly well calibrated and I was within the narrow
CW filter.
I thought the WWW was precisely on 10Mhz.
Do you have some explaination?
How many WWW station worldwilde are there and what
In message [EMAIL PROTECTED], Gerhard Hoffmann write
s:
The question is more if the 100r * 100u do anything to de-noise
the LED voltage. Close to the carrier probably not. The problem is
that you nowhere get exact numbers to base a decision on.
Be aware that LED's work both ways: current-light
In message [EMAIL PROTECTED], Gerhard Hoffmann write
s:
The question is more if the 100r * 100u do anything to de-noise
the LED voltage. Close to the carrier probably not. The problem is
that you nowhere get exact numbers to base a decision on.
Be aware that LED's work both ways: current-light
You don't normally listen to a CW signal at zero beat, so many receivers
apply a BFO offset to make the CW tone audible at a comfortable frequency.
This is usually more like 800 Hz than 4 kHz, though, so you could still have
a calibration error somewhere.
-- john, KE5FX
-Original
You heard the Russian station RWM (.-. .-- --) which transmits on 4996,
9996, 14996 and maybe 19996. It is the easiest to receive station in Europe,
quite strong signal.
73,
Antonio I8IOV
Hi,
I listened today the WWW station and I've found it on 9.996 Mhz instead of
10.000Mhz and my
there.
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Poul-Henning Kamp wrote:
In message [EMAIL PROTECTED], Gerhard Hoffmann write
s:
The question is more if the 100r * 100u do anything to de-noise
the LED voltage. Close to the carrier probably not. The problem is
that you nowhere get exact numbers to base a decision on.
Be aware
Tom Clark, K3IO wrote:
Gerhard -- the discussion between you and Bruce has been very
interesting. I asked a VLBI colleague to look over your design and he
had this comment.
In VLBI, H-Maser frequency standards used to generate local
oscillators at microwave frequencies. We
At 05:54 PM 9/25/2008, f5bqp_pfm wrote...
Hi John,
No no, I'm sure of my cal, but not sure of the station
I've tried to find a list of the WWW stations without success.
Try searching for WWV, instead.
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Bruce Griffiths wrote:
Tom Clark, K3IO wrote:
Gerhard -- the discussion between you and Bruce has been very
interesting. I asked a VLBI colleague to look over your design and he
had this comment.
In VLBI, H-Maser frequency standards used to generate local
oscillators at
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