John Miles is now hosting the latest Lady Heather 4.0 files. His server is a
little less skeezy than tinyupload.com (which on Windows machines apparently
offers to update your Java with about every click). I've used tinyupload for
years on a Mac, and never got such a "generous" offer. No
Even though nothing to do with time, I found the paper
CESIUM OPTICALLY PUMPED MAGNETOMETERS
http://www.gserentals.co.uk/gse/pdf/Theory%20Cesium%20Optically%20Pumped%20Magnetometers.pdf
to be an interesting read.
I can only imagine what HP and Varian engineers went through
-pete
On Wednesday, April 27, 2016 09:40:05 PM Attila Kinali wrote:
> On Wed, 27 Apr 2016 20:18:10 +0200
>
> Mike Cook wrote:
> > > Use this CW signal on all the telescope stations to phase lock a local
> > > OCXO. Using a good OCXO, it should be possible to use loop bandwidths
>
On Wed, 27 Apr 2016 20:18:10 +0200
Mike Cook wrote:
> > Use this CW signal on all the telescope stations to phase lock a local
> > OCXO. Using a good OCXO, it should be possible to use loop bandwidths
> > in the 0.1-10Hz range. My guess is, that this frequency transfer
Lars,
On 04/27/2016 02:14 PM, Lars Walenius wrote:
Thanks Magnus and Charles,
Could you please explain a little more about this:
Charles wrote:
Loop filters in commercial GPSDOs use algorithms that suppress
systematic ripple on the VCO control related to the comparison frequency.
Magnus
>
> Assuming that you have an amateur radio license, you could use a
> well located central station to transmit a CW signal in the 70cm or
> 23cm band. There should be some effort put into this station
> to make it stable (eg by using a good rubidium as frequency source,
> or even an ensemble)
Greetings Time Nuts,
I read the message below and made a trip to my closest OLLIE's store in
Harrisonburg, VA. I found the book with the assistance of the book area
manager and purchased it. They now have 5 left in Harrisonburg. If you are
interested in the book and have an OLLIE'S nearby it
On Wed, Apr 27, 2016 at 7:21 PM, Bruce Griffiths
wrote:
> Stabilising the GPS receiver antenna temperature is probably a good idea
> particularly if it has bandpass filter(s).
It's not so clear that temperature stabilization of the antenna is
necessary. There have
Lars wrote:
>> What puzzles me is the large hump upwards in DACvalue. Anyone knows what is
>> the reason?
Hal wrote:
>My guess is poor filtering on the initial data when coming out of holdover,
>probably complicated by inadequate testing and/or that case not being
>important.
>
>I'm pretty sure
I've updated my existing LH download page with Mark's new beta version in both
.zip and (Windows) setup.exe formats:
http://www.ke5fx.com/heather/readme.htm
There's also a link to his readme.txt file with Linux build instructions.
(Mark is the best point of contact for anyone with questions on
Thanks Magnus and Charles,
Could you please explain a little more about this:
Charles wrote:
>> Loop filters in commercial GPSDOs use algorithms that suppress
>> systematic ripple on the VCO control related to the comparison frequency.
Magnus wrote:
>It will be there, so you need to manage it
Stabilising the GPS receiver antenna temperature is probably a good idea
particularly if it has bandpass filter(s).
Bruce
On Wednesday, 27 April 2016 9:01 PM, Attila Kinali wrote:
On Wed, 27 Apr 2016 01:30:49 +0200
Ilia Platone wrote:
> I will
It was a joke :)
Interesting the idea of Attila, it can be the less expensive solution:
"Assuming that you have an amateur radio license, you could use a
well located central station to transmit a CW signal in the 70cm or
23cm band. There should be some effort put into this station
to make it
On Wed, Apr 27, 2016 at 7:51 AM, Attila Kinali wrote:
>
>
>
> Another way would be to use L1/L2 receivers with calibrated antennas.
> I know that BIPM has a GPS station that can deliver time transfer
> accuracy <2ns over a distance of several 100km. It could be possible
> to use
A 60kHz receiver is unlikely to be useful for nanosecond timing applications.
Bruce
On Wednesday, 27 April 2016 6:36 PM, Ilia Platone
wrote:
Hi All,
I read from an article about this receiver: C-Max CMMR-6P-60
Can it be useful?
One of the places where I'll
On Wed, 27 Apr 2016 01:30:49 +0200
Ilia Platone wrote:
> I will use a dedicated FPGA design, and the data will be stored into an
> SDXC card (UHS), or an IDE drive (maybe not), in RAW mode (no filesystem).
Please be aware that SDCards performance spec is peak and best
Hi All,
I read from an article about this receiver: C-Max CMMR-6P-60
Can it be useful?
One of the places where I'll setup the telescopes will be in mount
Carpegna, near where I live. There are the repetitors of television and
radio over there. Can the carrier wave of such repetitors be used
On 04/27/2016 01:12 AM, Charles Steinmetz wrote:
Lars wrote:
I have wondered what is meant by a proper digital filter below?
Is a proper digital filter something more than the LP-filter + PI-loop
I use in the DIY Arduino GPSDO?
What is used in commercial GPSDOs?
The loops are
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