Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-06 Thread Bob Camp
Hi

Fountain's don't work very well in zero G….:)

Bob

On May 6, 2013, at 12:23 AM, Magnus Danielson mag...@rubidium.dyndns.org 
wrote:

 On 05/06/2013 02:29 AM, Mike S wrote:
 On 5/4/2013 2:40 PM, Attila Kinali wrote:
 Can anyone shed some light on why the GPS Cs beams have a worse stability
 than the Rb vapor clocks?
 
 I don't know, but it makes me wonder about things like
 
 1) How sensitive is each to C-field tuning - i.e. for the same change in
 C-field, by how much does each type change in relative frequency? (or
 maybe it's exactly the same, I know nothing about the Zeeman effect) I'd
 think there would be orbital changes in frequency, after all, it's
 orbiting a big magnet.
 
 Rubidium is more sensitive to C-field than Caesium.
 
 2) How tight a lock can be obtained on each? i.e. might the physical
 realizations of Rb clocks have a higher Q-factor?
 
 The Q-value depends on the observation time, and for a Cs-beam this 
 translates into beam-length assuming constant speed. Foutains has much better 
 Q since they have longer observation time. H-masers started as a beam with a 
 bounce-box to prolong the observation time.
 
 Cheers,
 Magnus
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-06 Thread Magnus Danielson
Rather the opposit. They will be really compact and can have long 
observationtime.
Cheers
Magnus

 Originalmeddelande 
Från: Bob Camp li...@rtty.us 
Datum:  
Till: Discussion of precise time and frequency measurement time-nuts@febo.com 
Rubrik: Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs 
 
Hi

Fountain's don't work very well in zero G….:)

Bob

On May 6, 2013, at 12:23 AM, Magnus Danielson mag...@rubidium.dyndns.org 
wrote:

 On 05/06/2013 02:29 AM, Mike S wrote:
 On 5/4/2013 2:40 PM, Attila Kinali wrote:
 Can anyone shed some light on why the GPS Cs beams have a worse stability
 than the Rb vapor clocks?
 
 I don't know, but it makes me wonder about things like
 
 1) How sensitive is each to C-field tuning - i.e. for the same change in
 C-field, by how much does each type change in relative frequency? (or
 maybe it's exactly the same, I know nothing about the Zeeman effect) I'd
 think there would be orbital changes in frequency, after all, it's
 orbiting a big magnet.
 
 Rubidium is more sensitive to C-field than Caesium.
 
 2) How tight a lock can be obtained on each? i.e. might the physical
 realizations of Rb clocks have a higher Q-factor?
 
 The Q-value depends on the observation time, and for a Cs-beam this 
 translates into beam-length assuming constant speed. Foutains has much better 
 Q since they have longer observation time. H-masers started as a beam with a 
 bounce-box to prolong the observation time.
 
 Cheers,
 Magnus
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-05 Thread Attila Kinali
On Sat, 4 May 2013 16:31:42 -0700 (PDT)
Mark Spencer mspencer12...@yahoo.ca wrote:

 The article available for download via this URL contains some history
 about development issues with Rb and Cs Clocks for GPS.   It seems at
 one point after the GPS system was placed into service a development
 program for new Cs GPS clocks failed and by necessity there was a shift
 towards Rb (at least for a period of time.)
  
 http://www.insidegnss.com/node/281

Interesting article. Thanks!

Attila Kinali

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who also happen to be insane and gross.
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-05 Thread Attila Kinali
On Sat, 04 May 2013 21:53:00 -0700
Hal Murray hmur...@megapathdsl.net wrote:

 Radio astronomers use H-masers.  Can I assume that they are mid-term and that 
 H-masers are better than Rb (at mid-term)?

Disclaimer: I'm not into astronomy. What i write below is solely based
on what i've stumbled upon in the last years. It is probably inacurate
and maybe even wrong.


Modern H-Masers outperform both Cs beams and Rb Vapor Gas Cells
siginificantly up to a couple of days to a couple of months.

Which stability (short term or mid term) is exactly used for astronomy
depends on the phenomena they want to observe and how often they
can synchronize their clocks. The three most demanding applications
are probably large antenna arrays, VLBI and pulsar rate measurement.
Large antenna arrays mostly need short term stability, up to a couple
of hours (the length of one observation). VLBI can take multiple
days, depending on the setup. And pulsar rate measurement spans
many months to a couple of years.


Attila Kinali

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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-05 Thread Bob Camp
Hi

All the data is in an adev plot. In this case short is  100 seconds, and long 
is  10,000 seconds. Those are rough numbers, since a really good Rb (like 
Corby's) may cross over a bit earlier. A really crummy Cs (low beam current) 
might not cross over for a couple of days against a well stabilized Rb or 
Maser. A good BVA OCXO will give the Rb a bit more of a run for it's money ….

The cross overs will happen. Where is going to depend entirely on the specific 
individual standards you happen to have. If you are making decisions about 
which of your boxes to use, you have to measure them.

Bob

On May 5, 2013, at 12:53 AM, Hal Murray hmur...@megapathdsl.net wrote:

 
 t...@leapsecond.com said:
 Rule of thumb: quartz is best short term, Rb or H-maser mid-term, and Cs by
 far the best long-term. 
 
 What is short, medium, and long?
 
 Radio astronomers use H-masers.  Can I assume that they are mid-term and that 
 H-masers are better than Rb (at mid-term)?
 
 Does the classic ADEV graph contain all the information, or is it making an 
 assumption that is valid in most cases that allows it to compress/hide lots 
 of information that is interesting for only a few obscure types of 
 applications?
 
 
 -- 
 These are my opinions.  I hate spam.
 
 
 
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-05 Thread WarrenS
All the data is in an adev plot... The cross overs will happen... you have 
to measure them.


True, but then what do you do?
It is not quite as simple or easy as it may sound.

Although it is a good place to start,
for best results in a GPSDO you can not just compare the ADEV crossover 
points of the two frequency sources.

The problem I've seen is that long term ADEV plots generally show a turn-up,
often around the 1000 sec range.
The turn-up in the plot, more often than not, is caused by systematic 
errors, not random noise,

so the turn-up may be scaled incorrectly by the ADEV plot.

The things I've seen that can cause 'premature' turn-up on an ADEV plot are:
Not allowing enough time for the osc to stabilize after turn on,
room temperature variation, outliers and fixed rate ageing.
With careful attention to many details, the turn-up can often be 
significantly reduced.
The effect that each of these errors types have on various disciplined 
control loops varies greatly.


The problem is when the effect that each of these errors has on a 
disciplined control
loop such as a GPSDO is not the same as the effect that they have on the 
ADEV plot,

you can not just use the crossover point of the two plots.

The most extreme example is **fixed** ageing rate of the frequency source 
that is to be disciplined.

A fixed ageing rate drift causes a slope of one turn-up on an ADEV plot
(but has little or no effect on a Hadamard plot).
On the other hand a fixed ageing rate error, which is often the major error 
of a good DOCXO,

has no effect on frequency stability in a basic fixed time constant
disciplined control loop such as used in a TBolt.
It does cause a constant fixed phase error that is a function of the control 
loop's time constant and damping settings,
but that can be removed completely if desired by just changing the control 
loop's cable length setting.

On other types of disciplined control loops, the effect of a fixed ageing
rate error may vary and depends on the type of advanced control loop used.

The effect of temperature variation on a disciplined control loop is another
big variation that can effect ADEV plots and disciplined control loops 
differently.
In the case of a TBolt, delta temperature correction is only applied when 
the unit is in Holdover,

so its effect has to be considered when setting up the GPSDO.
This is why the best way to fix that error source is to not let the 
temperature change or to use a external DOCXO.
Advanced control loops can greatly reduce the effect of changing temperature 
with feed-forward control,

so they may not be nearly as sensitive to temperature variation.

ws

***

Hi

All the data is in an adev plot. In this case short is  100 seconds, and
long is  10,000 seconds. Those are rough numbers, since a really good Rb
(like Corby's) may cross over a bit earlier. A really crummy Cs (low beam
current) might not cross over for a couple of days against a well 
stabilized

Rb or Maser. A good BVA OCXO will give the Rb a bit more of a run for it's
money ..

The cross overs will happen. Where is going to depend entirely on the
specific individual standards you happen to have. If you are making
decisions about which of your boxes to use, you have to measure them.

Bob


*
On May 5, 2013, at 12:53 AM, Hal Murray hmurray at megapathdsl.net wrote:


tvb at leapsecond.com said:

Rule of thumb: quartz is best short term, Rb or H-maser mid-term, and Cs
by far the best long-term.


What is short, medium, and long?

Radio astronomers use H-masers.  Can I assume that they are mid-term and
that H-masers are better than Rb (at mid-term)?

Does the classic ADEV graph contain all the information, or is it making
an assumption that is valid in most cases that allows it to compress/hide
lots of information that is interesting for only a few obscure types of
applications?



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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-05 Thread Mike S

On 5/4/2013 2:40 PM, Attila Kinali wrote:

Can anyone shed some light on why the GPS Cs beams have a worse stability
than the Rb vapor clocks?


I don't know, but it makes me wonder about things like

1) How sensitive is each to C-field tuning - i.e. for the same change in 
C-field, by how much does each type change in relative frequency? (or 
maybe it's exactly the same, I know nothing about the Zeeman effect) I'd 
think there would be orbital changes in frequency, after all, it's 
orbiting a big magnet.


2) How tight a lock can be obtained on each? i.e. might the physical 
realizations of Rb clocks have a higher Q-factor?



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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-05 Thread Magnus Danielson

On 05/06/2013 02:29 AM, Mike S wrote:

On 5/4/2013 2:40 PM, Attila Kinali wrote:

Can anyone shed some light on why the GPS Cs beams have a worse stability
than the Rb vapor clocks?


I don't know, but it makes me wonder about things like

1) How sensitive is each to C-field tuning - i.e. for the same change in
C-field, by how much does each type change in relative frequency? (or
maybe it's exactly the same, I know nothing about the Zeeman effect) I'd
think there would be orbital changes in frequency, after all, it's
orbiting a big magnet.


Rubidium is more sensitive to C-field than Caesium.


2) How tight a lock can be obtained on each? i.e. might the physical
realizations of Rb clocks have a higher Q-factor?


The Q-value depends on the observation time, and for a Cs-beam this 
translates into beam-length assuming constant speed. Foutains has much 
better Q since they have longer observation time. H-masers started as a 
beam with a bounce-box to prolong the observation time.


Cheers,
Magnus
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[time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Attila Kinali
Hi,

Bruce recently mentioned [1], where Fig. 2 shows that the Cs clocks
of the old II and IIA birds are less stable than the Rb clocks of the
newer birds. This struck me as odd and i tried to find out why 
a Cs beam had worse stability than a Rb vabor cell. The only paper comparing
both clocks that i found was [2] which shows in Fig. 2 that the Cs clocks
are less stable even at very small taus. But the only mention of a property
that is worse for the Cs than for the Rb mentioned is that the Rb's are
temperature stabilized while the Cs is not. But i would expect the temperature
effect to be significant from a couple 100s upward, not down to 1s.


Can anyone shed some light on why the GPS Cs beams have a worse stability
than the Rb vapor clocks?


Attila Kinali


[1] GPS clocks in space: Current performance and plans for the future,
by Dass, Freed, Petzinger, Rajan, 2002
http://tycho.usno.navy.mil/ptti/ptti2002/paper18.pdf

[2] Atomic frequency standards for the GPS IIF satelites, 
by Emmer, Watts, 1997
http://www.pttimeeting.org/archivemeetings/1997papers/Vol%2029_19.pdf

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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Tom Van Baak (lab)
Rule of thumb: quartz is best short term, Rb or H-maser mid-term, and Cs by far 
the best long-term.

For GPS clocks the long-term doesn't matter that much since each space clock is 
monitored and updated against the GPS master clock(s) on the ground. 

/tvb (iPhone4)

On May 4, 2013, at 11:40 AM, Attila Kinali att...@kinali.ch wrote:

 Hi,
 
 Bruce recently mentioned [1], where Fig. 2 shows that the Cs clocks
 of the old II and IIA birds are less stable than the Rb clocks of the
 newer birds. This struck me as odd and i tried to find out why 
 a Cs beam had worse stability than a Rb vabor cell. The only paper comparing
 both clocks that i found was [2] which shows in Fig. 2 that the Cs clocks
 are less stable even at very small taus. But the only mention of a property
 that is worse for the Cs than for the Rb mentioned is that the Rb's are
 temperature stabilized while the Cs is not. But i would expect the temperature
 effect to be significant from a couple 100s upward, not down to 1s.
 
 
 Can anyone shed some light on why the GPS Cs beams have a worse stability
 than the Rb vapor clocks?
 
 
Attila Kinali
 
 
 [1] GPS clocks in space: Current performance and plans for the future,
 by Dass, Freed, Petzinger, Rajan, 2002
 http://tycho.usno.navy.mil/ptti/ptti2002/paper18.pdf
 
 [2] Atomic frequency standards for the GPS IIF satelites, 
 by Emmer, Watts, 1997
 http://www.pttimeeting.org/archivemeetings/1997papers/Vol%2029_19.pdf
 
 -- 
 The people on 4chan are like brilliant psychologists
 who also happen to be insane and gross.
-- unknown
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Poul-Henning Kamp
In message bb05041d-f03a-42ac-85c6-467110fc3...@leapsecond.com, Tom Van Baak
 (lab) writes:

Rule of thumb: quartz is best short term, Rb or H-maser mid-term,
and Cs by far the best long-term.

I have never seen a technical description of the Cs used in the
early GPS satellites, but I have seen many references to all sorts
of troubles with them, including a much shorter lifetime than
was hoped for.

-- 
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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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Tom Van Baak (lab)
Note also Galileo uses Rb and H-maser only; no Cs.

/tvb (iPhone4)

On May 4, 2013, at 1:53 PM, Poul-Henning Kamp p...@phk.freebsd.dk wrote:

 In message bb05041d-f03a-42ac-85c6-467110fc3...@leapsecond.com, Tom Van 
 Baak
 (lab) writes:
 
 Rule of thumb: quartz is best short term, Rb or H-maser mid-term,
 and Cs by far the best long-term.
 
 I have never seen a technical description of the Cs used in the
 early GPS satellites, but I have seen many references to all sorts
 of troubles with them, including a much shorter lifetime than
 was hoped for.
 
 -- 
 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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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Mark Spencer
The article available for download via this URL contains some history about 
development issues with Rb and Cs Clocks for GPS.   It seems at one point after 
the GPS system was placed into service a development program for new Cs GPS 
clocks failed and by necessity there was a shift towards Rb (at least for a 
period of time.)
 
http://www.insidegnss.com/node/281
 
I'm also speculating that the end of the cold war may have led to less emphasis 
being placed on the GPS system being able to operate for long periods of time 
without ground based intervention which would have further reduced the need to 
develop new and improved Cs clocks for the new GPS satellites.  (In the cold 
war era I recall seeing estimates of how long the GPS system could operate 
without ground based attention.)
 

 
 
 
 
 
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Bob Camp
Hi

In a ground servo'd system, there is very little need for a Cs beam clock. The 
medium term stability of the Rb's is plenty good enough to allow the ground 
segment to keep up with / correct for what ever the space clocks are doing.

Bob

On May 4, 2013, at 7:31 PM, Mark Spencer mspencer12...@yahoo.ca wrote:

 The article available for download via this URL contains some history about 
 development issues with Rb and Cs Clocks for GPS.   It seems at one point 
 after the GPS system was placed into service a development program for new Cs 
 GPS clocks failed and by necessity there was a shift towards Rb (at least for 
 a period of time.)
  
 http://www.insidegnss.com/node/281
  
 I'm also speculating that the end of the cold war may have led to less 
 emphasis being placed on the GPS system being able to operate for long 
 periods of time without ground based intervention which would have further 
 reduced the need to develop new and improved Cs clocks for the new GPS 
 satellites.  (In the cold war era I recall seeing estimates of how long the 
 GPS system could operate without ground based attention.)
  
 
  
  
  
  
  
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Magnus Danielson

On 05/05/2013 01:31 AM, Mark Spencer wrote:

The article available for download via this URL contains some history about 
development issues with Rb and Cs Clocks for GPS.   It seems at one point after 
the GPS system was placed into service a development program for new Cs GPS 
clocks failed and by necessity there was a shift towards Rb (at least for a 
period of time.)

http://www.insidegnss.com/node/281

I'm also speculating that the end of the cold war may have led to less emphasis 
being placed on the GPS system being able to operate for long periods of time 
without ground based intervention which would have further reduced the need to 
develop new and improved Cs clocks for the new GPS satellites.  (In the cold 
war era I recall seeing estimates of how long the GPS system could operate 
without ground based attention.)


I seem to recall that they even extended the capability with AUTONAV 
functionality, which would significantly prolong the time without ground 
control to 180 days, but beyond the cold war ending, the actual 
performance of the system and also that of the infrastructure has 
allowed a more relaxed situation. Just the long-livety of the birds 
themselves is a factor, and then the precision you achieve by correction 
of time through the regular updates is not too bad.


Also, as many Cs/Rb sats moved to Rb only operation, it has not meant 
any large threat to the system, so launching birds without Cs has been 
less of an issue.


Cheers,
Magnus
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Re: [time-nuts] GSP clock stabilitiy, Rb vs Cs

2013-05-04 Thread Hal Murray

t...@leapsecond.com said:
 Rule of thumb: quartz is best short term, Rb or H-maser mid-term, and Cs by
 far the best long-term. 

What is short, medium, and long?

Radio astronomers use H-masers.  Can I assume that they are mid-term and that 
H-masers are better than Rb (at mid-term)?

Does the classic ADEV graph contain all the information, or is it making an 
assumption that is valid in most cases that allows it to compress/hide lots 
of information that is interesting for only a few obscure types of 
applications?


-- 
These are my opinions.  I hate spam.



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