I found all ICs except the VCXO here in the US, from only two sources;
Mouser and Unicorn Electronics. A couple substitutions can be made without
affecting the circuit. The 78L06 is the only change i made... substituting
an LM317L adjustable regulator for the fixed 6-volt reegulator.
I've
Hal wrote:
It would be interesting to measure the propagation delay over a day
or week, and watch the PLL error voltage over a scale of seconds or minutes.
Somewhere I probably still have miles and miles of paper tape that
came out of a WWVB phase comparator for many years BGE (before the
Hi Bob I have just realised that MSF may work diffently?? The Anthorn
signal is monitored by NPL at Teddington, West of London and frequency
off-sets twice a day are published in parts in 10^12 on their
web-site.involving lot of averaging I think. They do not recommend
using the signal
The last NPL MSF Bulletin showing their errors was over 4 years ago:
http://resource.npl.co.uk/time/bulletins/bulletin_archive.html
http://www.npl.co.uk/science-technology/time-frequency/products-and-services/time/msf-radio-time-signal
The error at a receiver over an interval of a couple of days
Hi
It’s not to hard to detect the ionosphere changing and impacting the 60 KHz
signals. If you run one of the old
style strip chart systems it goes nuts as the sunrise or sunset point passes
between you and the transmitter.
At some point the signal may even drop by enough for the receiver to
Jim Lux kirjoitti:
While this is trivial with a GPS receiver, we were thinking about a very
minimalist implementation, with a smart phone as the control interface.
Forget the smart phone - at least if it's un-rooted Android. I'm not
sure how the default time sync is done, it's either by
> On Nov 22, 2015, at 7:47 AM, paul swed wrote:
>
> As mentioned a nice answer to the wwvb modulation change.
> I looked up the parts and it seems that they have gone into the NOS state.
> Though you can get some from digikey and such especially in the SOIC
> package. Also
Please note that this question refers to the branded "Thunderbolt E"
GPSDO, in a silver coloured case with blue label and using a single 24V
supply,
and not the gold coloured "Thunderbolt" that is often found marked "Rev E".
Whilst testing a Thunderbolt E I've observed that the
As mentioned a nice answer to the wwvb modulation change.
I looked up the parts and it seems that they have gone into the NOS state.
Though you can get some from digikey and such especially in the SOIC
package. Also the VCO isn't available.
It appears that the Chinese sight has the lmc6484 and
On Sun, 22 Nov 2015 11:08:50 +0200
Esa Heikkinen wrote:
> > While this is trivial with a GPS receiver, we were thinking about a very
> > minimalist implementation, with a smart phone as the control interface.
>
> Forget the smart phone - at least if it's un-rooted Android. I'm
Hi
The most basic gotcha with WWVB is that propagation can (and does) shift the
carrier more than a full cycle over the course of a day. That’s at 60 KHz, so
one
cycle is a lot (as in 16.666 ppm). Even at one second with a not so great
receiver
and a poor antenna, GPS should give you ~0.01
> I'm familiar with the concept of frequency pulling in oscillators but
> would have expected the Thunderbolt E output to be better buffered than
> this, it's certainly not something I've experienced with the gold cased
> Thunderbolts.
> Before I start probing any deeper I'd be interested
> Iâd have to guess that the PLL would behave better given a 60 kHz reference
> rather than a 1 Hz one. But how stable is that 60 kHz reference after going
> through, what, a thousand miles of ionosphere or so?
One of the reasons for using 60 kHz is to avoid the ionosphere. If you
measure
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