[time-nuts] Re: Oncore UT+ EEPROM -

2021-11-29 Thread Poul-Henning Kamp

k1...@att.net writes:

> I have an Oncore UT+ for a project and found that it works fine after
> updating the almanac and getting a 3D fix but it never stores my location
> coordinates in its EEPROM.  Each time I power up it shows all zeroes in Lat,
> Lon, Alt for about an hour or so until it finds satellites.  With Lady
> Heather I tried entering my coordinates and this leads to faster tracking.
> Is this normal Oncore UT+ behavior?  Any advice other than a battery backup.

As far as I know, the EEPROM (Flash?) is only used for code.  The almanac
and other changing info is in battery-backed NOVRAM.

-- 
Poul-Henning Kamp   | UNIX since Zilog Zeus 3.20
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[time-nuts] Oncore UT+ EEPROM -

2021-11-29 Thread k1jos
I have an Oncore UT+ for a project and found that it works fine after
updating the almanac and getting a 3D fix but it never stores my location
coordinates in its EEPROM.  Each time I power up it shows all zeroes in Lat,
Lon, Alt for about an hour or so until it finds satellites.  With Lady
Heather I tried entering my coordinates and this leads to faster tracking.
Is this normal Oncore UT+ behavior?  Any advice other than a battery backup.

 
Jerry NY2KW


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[time-nuts] Re: Seeking advice: Is this the right way to check very short term (below 1s) stability?

2021-11-29 Thread Magnus Danielson via time-nuts

Erik,

Den 2021-11-28 kl. 19:19, skrev Erik Kaashoek:
As the collection of frequency sources and counters in my home lab is 
growing I'd like to understand the performance of the frequency sources.

Two different GPSDO do help to check long term stability.
But the Rubidium frequency standard I have (Accubeat AR60A) is fairly 
unknown and seemingly not of good reputation, more specifically its 
(very) short term stability is doubted.
So how best to check very short term  (below 1s) frequency stability. 
The frequency counters available loose resolution quickly when the 
gate time is reduced below 1 second and high performance phase noise 
measurement equipment is not available so google helped with a search 
for alternative measurement methods.
What I found was a method using two frequency sources, one of the two 
being  a VCO, a mixer and some filters and amplifiers.
By weak locking (large time constant)  the VCO source using the mixer 
as phase detector to the other source, the output of the mixer's IF 
port should carry a voltage real time proportionally to the phase 
difference and by filtering and amplifying it should be possible to 
check for variations in the 1ms-1s range.

Maybe even a scope can see the variations.
When you know the amplification and the full range voltage you can 
even do an absolute measurement.

Would this method work?
Any specific concerns to take note of when doing the measurement?
Removing the DC component (or locking the VCO such that there is no DC 
component) will be crucial I guess but given the slow speed of the 
loop even an ADC->computer->DAC->VCO setup can work.

Any suggestion is welcome.


So, in that region one typically transition into measuring phase noise, 
as for shorter taus your performance will be dominated by the wideband 
white noise, and counters isn't the best tool to analyze that.


The weak locking technique can be used to a limit, but to get good 
results, you need to calibrate it. I suggest you set up the loop in the 
analog domain and only digitize the residual noise. Then inject using a 
synthesizer side-tones to your carrier and know relationship in 
amplitude and frequency offsets, for which then the phase-noise should 
be known, and use that to build a calibration scale. This is described 
in the NIST T&F catalog. You can do that with a varity of sources, but 
eventually you will be limited by the noise of the other oscillator.


I use a cross-correlator setup in the form of TimePod most of the times, 
with quiet references.


Cheers,
Magnus
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[time-nuts] Re: Lowest noise (phase noise and ADEV) method to achieve 10 MHz signal from 5 MHz input

2021-11-29 Thread Wilko Bulte
For those interested, Dave PA5DOF and your's truly are working to get the 
doubler implemented that Luciano has on his website. The first PCB prototype is 
in and has been built and works OK. Some minor tweaks/fixes  will be added to a 
V0.2 PCB. If there is interest I can share the Gerber files. 

The doubler is intended to be hooked up to an Efratom MRK-HLN 5MHz Rb. Our 
shack T&M equipment for the best part requires a 10MHz reference. 

Wilko

> On 29 Nov 2021, at 10:35, tim...@timeok.it wrote:
> 
> 
>   you can use this:
> 
>   
> http://www.timeok.it/wp-content/uploads/2015/08/high-performance-frequency-doublerv1-31.pdf
> 
>   Luciano P. S. Paramithiotti
>   tim...@timeok.it
>   www.timeok.it
> 
>   Da "Matt Huszagh" huszaghm...@gmail.com
>   A time-nuts@lists.febo.com
>   Cc
>   Data Sun, 28 Nov 2021 19:29:58 -0800
>   Oggetto [time-nuts] Lowest noise (phase noise and ADEV) method to achieve 
> 10 MHz signal from 5 MHz input
>   Hi,
> 
>   I've got a 10 MHz distribution amplifier and am considering purchasing a
>   5 MHz reference. Most (not all) of my equipment accepts a 5 MHz
>   reference, but I'd like to be able to use the existing distribution
>   amplifier I have if possible. Therefore, I'm considering ways I might
>   generate a low-noise 10 MHz signal from the 5 MHz reference.
> 
>   An obvious way is to use a doubler. However, as I understand it, even an
>   ideal doubler will add 20log(2)=6 dB of phase noise to the 10 MHz
>   signal. It seems like a possibly more expensive, but lower noise way
>   would be to use a PLL with a divider that locks the divided 10 MHz
>   signal to the 5 MHz input. If the time constant of the loop filter is
>   set long enough, does this avoid the phase noise multiplication issue?
>   From what I've gathered, this is a technique HP used in some of their
>   gear. For example, the 8566 and 8340/1 lock a 100 MHz VCXO to an
>   external reference with a PLL.
> 
>   Any other thoughts on this?
>   Matt
>   ___
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[time-nuts] Re: Project Great

2021-11-29 Thread Bob kb8tq
Hi

All these devices *can* be sensitive to the environment. What degree of 
sensitivity they have is a function of how “nutty” one went on this or that
design. It also is a function of things like cost, size, and power consumption. 

The target market for things like the 5071 is a “we can afford it” sort of 
crew. Even today various government agencies from various countries 
buy the bulk of the 5071’s produced. Yes sorting this out is a bit complicated.
Multi step procurement is pretty common. 

Telecom Rb’s and OCXO’s normally go into a *very* different market. There
is indeed a “good enough” point at which the willingness to pay goes away. 
Temperature stability is one of many things that could be better if more 
money / power / volume was thrown at the problem. 

So no, not a simple single answer.

Bob



> On Nov 29, 2021, at 9:55 AM, Lux, Jim  wrote:
> 
> On 11/29/21 1:57 AM, Hal Murray wrote:
>> j...@luxfamily.com said:
>>> And a lot ofsources may have a low flat spot in the curve, but it
>>> eventually trends up. Except for primary standards like Cs beam.
>> What's magic about "primary standard" or "Cs beam" that keeps the ADEV from
>> trending up?
>> 
> Their ultimate accuracy is dependent only on a invariant physical property 
> that is independent of time.
> 
> A quartz crystal ages. No matter how good your oven is, the frequency will 
> change over a long time.
> 
> Mercury ions, Cs ions (perhaps all ions?) have frequencies that are a 
> fundamental property of the ion.  There might be practical implementation 
> limits or side effects that limit the lowest achievable uncertainty - hot 
> atoms will have higher variance than cold atoms, for instance. So not all Cs 
> primary standards have the same ultimate performance.
> 
> 
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[time-nuts] Re: Project Great

2021-11-29 Thread Lux, Jim

On 11/29/21 1:57 AM, Hal Murray wrote:

j...@luxfamily.com said:

And a lot ofsources may have a low flat spot in the curve, but it
eventually trends up. Except for primary standards like Cs beam.

What's magic about "primary standard" or "Cs beam" that keeps the ADEV from
trending up?

Their ultimate accuracy is dependent only on a invariant physical 
property that is independent of time.


A quartz crystal ages. No matter how good your oven is, the frequency 
will change over a long time.


Mercury ions, Cs ions (perhaps all ions?) have frequencies that are a 
fundamental property of the ion.  There might be practical 
implementation limits or side effects that limit the lowest achievable 
uncertainty - hot atoms will have higher variance than cold atoms, for 
instance. So not all Cs primary standards have the same ultimate 
performance.



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[time-nuts] Re: Project Great

2021-11-29 Thread Magnus Danielson via time-nuts

Hi,

Den 2021-11-29 kl. 10:57, skrev Hal Murray:

j...@luxfamily.com said:

And a lot ofsources may have a low flat spot in the curve, but it
eventually trends up. Except for primary standards like Cs beam.

What's magic about "primary standard" or "Cs beam" that keeps the ADEV from
trending up?


"primary standard" is an overloaded term, so depending on context a 
particular product may suffice to be a "primary standard" in some 
context but not in others. In general a "primary standard" does not need 
external corrections, and some clocks will have less than perfect 
mechanisms for their systematic variations or drift, which does not 
covers the ADEV, as ADEV is not covering systematic properties but is 
only intended to cover random noise. For metrology contexts, "primary 
standards" is only a handful of cesium foutains to achieve frequency 
accuracy, where as the bulk of atomics clocks contribute stability (i.e. 
optimal ADEV).


In telecom, a "Primary Reference Clock (PRC)" or "Primary Reference 
Source (PRS)" ensures frequency within +/- 1E-11, which used to be what 
analog cesiums could achieve. Requirements have since progressed, 
especially for the phase as time is now an added.


So, in general, it's about the repetitive independent generation of 
phase, frequency and drift. Stability in terms of ADEV and TDEV then 
comes in as othogonal requirement.


I think you will find that IEEE Std 1139 and 1193 has further 
refinements as they pop out of the approval and publishing. 1139 draft 
is now in balloting process. We still work on 1193. I also recommend 
having a look at VIM and GUM documents as available from BIPM.


Cheers,
Magnus
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[time-nuts] Re: Lowest noise (phase noise and ADEV) method to achieve 10 MHz signal from 5 MHz input

2021-11-29 Thread Bob kb8tq
Hi

The PLL will have the same 20 log N issue plus a number of other 
problems. The big question is: what are you after? 

If you need something below -175 dbc / Hz far removed, what is 
the application? There may well be better ways to do this or that. 

If you are after -125 dbc / Hz at 1 Hz, that’s a very different need and
the approach to getting it would be significantly different. 

Simple answer is that most equipment is not all that sensitive to phase
noise and that distribution amps have a noise floor. You can go nuts
getting a super quiet reference and it will have no real impact outside
a few very specific applications. ( which likely will need custom “plumbing”).

Bob

> On Nov 28, 2021, at 10:29 PM, Matt Huszagh  wrote:
> 
> Hi,
> 
> I've got a 10 MHz distribution amplifier and am considering purchasing a
> 5 MHz reference. Most (not all) of my equipment accepts a 5 MHz
> reference, but I'd like to be able to use the existing distribution
> amplifier I have if possible. Therefore, I'm considering ways I might
> generate a low-noise 10 MHz signal from the 5 MHz reference.
> 
> An obvious way is to use a doubler. However, as I understand it, even an
> ideal doubler will add 20log(2)=6 dB of phase noise to the 10 MHz
> signal. It seems like a possibly more expensive, but lower noise way
> would be to use a PLL with a divider that locks the divided 10 MHz
> signal to the 5 MHz input. If the time constant of the loop filter is
> set long enough, does this avoid the phase noise multiplication issue?
> From what I've gathered, this is a technique HP used in some of their
> gear. For example, the 8566 and 8340/1 lock a 100 MHz VCXO to an
> external reference with a PLL.
> 
> Any other thoughts on this?
> Matt
> ___
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[time-nuts] Re: HP 5065A on ebay

2021-11-29 Thread paul swed
Poul-Henning
Always fun to take a look and some very attractive starting bids. But then
as time goes by it will get crazy as always. Then $400 or so in shipping
and heavens knows what customes will be. Oh well nice to look.
Thanks
Paul

On Mon, Nov 29, 2021 at 3:28 AM Poul-Henning Kamp 
wrote:

> 
> ew via time-nuts writes:
>
> And there's a 5071A "for parts only" too if anybody feels like an
> adventure:
>
>
> https://www.ebay.com/itm/154720557764?hash=item2406105ac4:g:e~8AAOSwTP5hoOG3
>
> --
> Poul-Henning Kamp   | UNIX since Zilog Zeus 3.20
> p...@freebsd.org | TCP/IP since RFC 956
> FreeBSD committer   | BSD since 4.3-tahoe
> Never attribute to malice what can adequately be explained by incompetence.
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[time-nuts] Re: Project Great

2021-11-29 Thread Poul-Henning Kamp

Hal Murray writes:
> 
> j...@luxfamily.com said:
> > And a lot ofsources may have a low flat spot in the curve, but it
> > eventually trends up. Except for primary standards like Cs beam.
>
> What's magic about "primary standard" or "Cs beam" that keeps the ADEV from 
> trending up?

Primarily (no pun intended) that there are no (relevant) mechanisms of
frequency drift.

Cesium beam standards measure free-flying atoms which means the
only relevant external influence is the black-body radiation, which
is constant, thanks to the thermostatic ovens.

Rubidium standards measure atoms which are confined in a glass-bulb,
which means they literally bounce of the walls all the time.

The resonance we measure is not the real one, but one affected by
the doppler-shift of the atoms speed, ie: velocity without sign,
in the direction of interrogation.

This also broadens the resonance.

I belive the primary source of drift in Rb's are adsorption and
absorption of Rb molecules onto and into the glass itself.  This
causes a drop of gas pressure, which changes the collision dynamics
for the remaining Rb gas, which affects their velocity distribution,
which again moves the "appearant resonance" we measure.

One of the things which set the 5065A apart from "telecom" Rb's is that
there is a side-reservoir which is cooled with a TEC to stabilize the
gas pressure and thus velocity.

If you put your Rb atoms in a fountain instead, they work as well, or
even slightly better than Cs atoms.

-- 
Poul-Henning Kamp   | UNIX since Zilog Zeus 3.20
p...@freebsd.org | TCP/IP since RFC 956
FreeBSD committer   | BSD since 4.3-tahoe
Never attribute to malice what can adequately be explained by incompetence.
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[time-nuts] Re: Lowest noise (phase noise and ADEV) method to achieve 10 MHz signal from 5 MHz input

2021-11-29 Thread Mike Feher
I see you are using two for the phase noise test setup (a common way of
doing it). I am curious about the phase matching between units. From the
results it appears they must be pretty well matched, but did not see any
actual data. Since it is over a very narrow frequency BW it should be no
problem. Thanks & Regards - Mike 

Mike B. Feher, N4FS
89 Arnold Blvd.
Howell NJ 07731
848-245-9115

-Original Message-
From: tim...@timeok.it  
Sent: Monday, November 29, 2021 4:35 AM
To: time-nuts@lists.febo.com
Subject: [time-nuts] Re: Lowest noise (phase noise and ADEV) method to
achieve 10 MHz signal from 5 MHz input


   you can use this:

 
http://www.timeok.it/wp-content/uploads/2015/08/high-performance-frequency-d
oublerv1-31.pdf

   Luciano P. S. Paramithiotti
   tim...@timeok.it
   www.timeok.it

   Da "Matt Huszagh" huszaghm...@gmail.com
   A time-nuts@lists.febo.com
   Cc
   Data Sun, 28 Nov 2021 19:29:58 -0800
   Oggetto [time-nuts] Lowest noise (phase noise and ADEV) method to achieve
10 MHz signal from 5 MHz input
   Hi,

   I've got a 10 MHz distribution amplifier and am considering purchasing a
   5 MHz reference. Most (not all) of my equipment accepts a 5 MHz
   reference, but I'd like to be able to use the existing distribution
   amplifier I have if possible. Therefore, I'm considering ways I might
   generate a low-noise 10 MHz signal from the 5 MHz reference.

   An obvious way is to use a doubler. However, as I understand it, even an
   ideal doubler will add 20log(2)=6 dB of phase noise to the 10 MHz
   signal. It seems like a possibly more expensive, but lower noise way
   would be to use a PLL with a divider that locks the divided 10 MHz
   signal to the 5 MHz input. If the time constant of the loop filter is
   set long enough, does this avoid the phase noise multiplication issue?
   From what I've gathered, this is a technique HP used in some of their
   gear. For example, the 8566 and 8340/1 lock a 100 MHz VCXO to an
   external reference with a PLL.

   Any other thoughts on this?
   Matt
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[time-nuts] Re: Project Great

2021-11-29 Thread Hal Murray


j...@luxfamily.com said:
> And a lot ofsources may have a low flat spot in the curve, but it
> eventually trends up. Except for primary standards like Cs beam.

What's magic about "primary standard" or "Cs beam" that keeps the ADEV from 
trending up?

-- 
These are my opinions.  I hate spam.


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[time-nuts] Re: Lowest noise (phase noise and ADEV) method to achieve 10 MHz signal from 5 MHz input

2021-11-29 Thread timeok


   you can use this:

   
http://www.timeok.it/wp-content/uploads/2015/08/high-performance-frequency-doublerv1-31.pdf

   Luciano P. S. Paramithiotti
   tim...@timeok.it
   www.timeok.it

   Da "Matt Huszagh" huszaghm...@gmail.com
   A time-nuts@lists.febo.com
   Cc
   Data Sun, 28 Nov 2021 19:29:58 -0800
   Oggetto [time-nuts] Lowest noise (phase noise and ADEV) method to achieve 10 
MHz signal from 5 MHz input
   Hi,

   I've got a 10 MHz distribution amplifier and am considering purchasing a
   5 MHz reference. Most (not all) of my equipment accepts a 5 MHz
   reference, but I'd like to be able to use the existing distribution
   amplifier I have if possible. Therefore, I'm considering ways I might
   generate a low-noise 10 MHz signal from the 5 MHz reference.

   An obvious way is to use a doubler. However, as I understand it, even an
   ideal doubler will add 20log(2)=6 dB of phase noise to the 10 MHz
   signal. It seems like a possibly more expensive, but lower noise way
   would be to use a PLL with a divider that locks the divided 10 MHz
   signal to the 5 MHz input. If the time constant of the loop filter is
   set long enough, does this avoid the phase noise multiplication issue?
   From what I've gathered, this is a technique HP used in some of their
   gear. For example, the 8566 and 8340/1 lock a 100 MHz VCXO to an
   external reference with a PLL.

   Any other thoughts on this?
   Matt
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[time-nuts] Re: HP 5065A on ebay

2021-11-29 Thread Poul-Henning Kamp

ew via time-nuts writes:

And there's a 5071A "for parts only" too if anybody feels like an adventure:


https://www.ebay.com/itm/154720557764?hash=item2406105ac4:g:e~8AAOSwTP5hoOG3

-- 
Poul-Henning Kamp   | UNIX since Zilog Zeus 3.20
p...@freebsd.org | TCP/IP since RFC 956
FreeBSD committer   | BSD since 4.3-tahoe
Never attribute to malice what can adequately be explained by incompetence.
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