Hi

> On Apr 16, 2022, at 11:55 AM, John Ackermann N8UR <[email protected]> wrote:
> 
> 
> 
> On 4/16/22 09:52, Matthias Welwarsky wrote:
>> Dear list members,
>> in 2020 John Ackermann published an evaluative survey of current day GPS and
>> GNSS receivers (URL below). I have a question about figure 26, which shows,
>> among others, the ADEV of a NEO-M8T against a Cesium reference, with
>> quantization correction applied. The curve shows a significant "bulge" above
>> 1e-10 between about 10s and 100s tau.
>> I'm using a LEA-M8T in my DIY GPSDO, which I think is the same chipset in a
>> slightly different package. I have attached an image worth about 3000 seconds
>> of data, raw 1PPS phase difference against the LO used in the GPSDO. The 
>> GPSDO
>> is locked, not in hold-over mode.
>> The bulge between 10s and 100s is not really visible here. There is a slight
>> bend, but not as pronounced. My explanation is that this is due to the LO
>> being pulled by the GNSS receiver so that it is no longer fully visible. I
>> reason that, were the LO more stable, more loosely coupled to the GNSS, I
>> should see the bulge from figure 26. Would you agree?
> 
> My theory of the ADEV flat spot when the M8T is qErr corrected is that 
> multiple things contribute to noise on the PPS output, and the qErr is only 
> one of them, and it consists of a noise source (clock granularity) that is 
> unrelated to any external analog process.
> 
> Since Qerr has a fixed limit of ± XX nanoseconds (half the receiver clock 
> granularity), its contribution to the PPS noise decreases with longer 
> averaging times.  Meanwhile, the other sources of noise such as ionosphere, 
> etc., are slower and become more pronounced as tau increases.  At around 30 
> seconds, the external noise factors become larger than the qErr.
> 
> So at short tau cancelling out the qErr gets rid of a major noise source and 
> improves ADEV but as tau increases beyond ~30 seconds the qErr contribution 
> is gradually outweighed by the other noise sources and disappears, returning 
> the ADEV slope to its normal -1.
> 
> Also note that in Fig. 26, at tau below 3 seconds it's possible that both the 
> M8T and F9T corrected plots are limited by the TICC resolution, which is 
> around 8e-11 @ 1 second on a good day.  That's below these traces, but may 
> still be high enough to impact the measurement.
> 
> Finally, it looks like you're comparing the raw PPS with an oscillator that 
> is steered by that same PPS.  I have to think their correlation could lead to 
> possible and unpredictable errors.  It would be better to have the OCXO 
> remain unsteered during the measurement.

The only way to make meaningful single comparison measurements of what’s 
going on is to compare to an external “free running” standard that has a 
stability 
adequate to the task. Normally this means an ADEV 5 to 10X better than what
you expect to see on the device under test. 

Bob

> 
> Best,
> John
> ----
> 
>> Best regards,
>> Matthias
>> https://hamsci.org/sites/default/files/publications/2020_TAPR_DCC/
>> N8UR_GPS_Evaluation_August2020.pdf
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