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Discussion of precise time and frequency measurement

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UTC(LRTE) H-Maser maintenace

J
john@miles.io
Thu, May 28, 2026 4:36 PM

There is probably not much wrong with it, then, if the cavity is putting out a signal.

One thing that can cause some confusion with the Russian masers is degradation of the coaxial capacitor in the HFO.  Both Tom and I have run into that before.  It operates with a high RF voltage across it, and if the insulation breaks down and starts arcing intermittently, some significant EMI can occur before it gets bad enough to stop oscillating completely.  The controller can potentially be affected by that.

-- john

From: Luiz Paulo Damaceno luizpauloeletrico42@gmail.com
Sent: Thursday, May 28, 2026 6:40 AM
To: john@miles.io
Cc: Discussion of precise time and frequency measurement time-nuts@lists.febo.com
Subject: Re: [time-nuts] UTC(LRTE) H-Maser maintenace

Thank you john!

I will verify supply rails with DMM / scope and return the results. For now, Is it an active maser unit. CH1-75A from KVARZ.

Kind regards,

Luiz Paulo

There is probably not much wrong with it, then, if the cavity is putting out a signal. One thing that can cause some confusion with the Russian masers is degradation of the coaxial capacitor in the HFO. Both Tom and I have run into that before. It operates with a high RF voltage across it, and if the insulation breaks down and starts arcing intermittently, some significant EMI can occur before it gets bad enough to stop oscillating completely. The controller can potentially be affected by that. -- john From: Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> Sent: Thursday, May 28, 2026 6:40 AM To: john@miles.io Cc: Discussion of precise time and frequency measurement <time-nuts@lists.febo.com> Subject: Re: [time-nuts] UTC(LRTE) H-Maser maintenace Thank you john! I will verify supply rails with DMM / scope and return the results. For now, Is it an active maser unit. CH1-75A from KVARZ. Kind regards, Luiz Paulo
LP
Luiz Paulo Damaceno
Thu, May 28, 2026 6:13 PM

Attila,

A PLL using the EFC input of the BVA will not work well at these
long time constants. About 1Hz loop bandwidth is the lowest that's
reasonable, I would even draw the line at 10Hz. And only if you
build an active filter using an low-noise opamp. Going lower will
limit your oscillators stability by the noise on the EFC voltage.
You have a 1MΩ resistor, which already produces quite a bit of
noise voltage. And then you use a 50µF capacitor. If it's an
electrolytic capacitor, then the leakage current noise will will destroy
the stability. If it's a ceramic capacitor, then its piezoelectric
properties will couple any acoustic noise and vibration into your
EFC voltage.

Best to ground the EFC voltage and then use a phase/frequency
stepper to shift the frequency of the BVA using a digital control
loop.-

I Did tought that even low noise components that I have here (resistors,
capacitor opamps (like OPA637 and OP37/27)) may contour these issues. Also,
the PLL circuit is temperature-stabilized and mechanical noise poorly
insulated. But you have a good point. I may use some SG384 that I also have
here to remove the frequency offset and actuate in the long term drift to
lock it with the cesium.

If the frequency comb is CEO stabilized (aka f-2f lock) and you can
stabilize its repetition rate using an optical cavity (10cm ULE is
already enough), then you can get better stability than your BVA
in the range up to 10s probably better than 100s, depending on your
setup. If the comb is free running, then the intrinsic instability
of the comb will be larger than the BVA.

We also have an optical cavity that is in progress to lock CEO. But this
will take a while I guess. The comb is repetition rate locked to BVA and
locked itself in the CEO.

Oh nice! Do you already have any publications on this?
I could only find [1] and [2].

Unfortunately that's only the both we have for now... We're ran out of
people working on this and haven't publications for a while.

Luiz Paulo

Em qui., 28 de mai. de 2026 às 12:30, Attila Kinali attila@kinali.ch
escreveu:

A wonderful good afternoon,

On Thu, 28 May 2026 10:37:58 -0300
Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com wrote:

Thank you for the considerations. I've tunned the PLL for 0.00289Hz,

today

i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce

the

error voltage by changing the voltage in a potentiometer, just like a
"volume" control in audio systems. I expect to reduce a bit 0,25 times

day

to day) to archive 1000s loop.

A PLL using the EFC input of the BVA will not work well at these
long time constants. About 1Hz loop bandwidth is the lowest that's
reasonable, I would even draw the line at 10Hz. And only if you
build an active filter using an low-noise opamp. Going lower will
limit your oscillators stability by the noise on the EFC voltage.
You have a 1MΩ resistor, which already produces quite a bit of
noise voltage. And then you use a 50µF capacitor. If it's an
electrolytic capacitor, then the leakage current noise will will destroy
the stability. If it's a ceramic capacitor, then its piezoelectric
properties will couple any acoustic noise and vibration into your
EFC voltage.

Best to ground the EFC voltage and then use a phase/frequency
stepper to shift the frequency of the BVA using a digital control
loop.-

I can only evaluate this using GNSS PPP - by
RTKLib in real time or NRCAN for example and / or CGGTTS files.

I have also available for these measurements a frequency comb from menlo
systems. Can I use repetition rate adev to evaluate the BVA? (locking it

in

a Cs beam and then in BVA + Cs beam)?

If the frequency comb is CEO stabilized (aka f-2f lock) and you can
stabilize its repetition rate using an optical cavity (10cm ULE is
already enough), then you can get better stability than your BVA
in the range up to 10s probably better than 100s, depending on your
setup. If the comb is free running, then the intrinsic instability
of the comb will be larger than the BVA.

We are working in cold atom clocks here also. A Cs fountain and another
kind of cold atom Cs clock. But now, we're in the construction phase. No
measurements being made.

Oh nice! Do you already have any publications on this?
I could only find [1] and [2].

BTW: If you want some known-good reference. The Canadians (IIRC the
NRC itself) sell caesium fountains for a reasonable price.

About getting the maser working again, do you have any experience with

that

maser? Is the KVARZ CH1-75A.

I have never personally worked on a AHM myself. I do know their
working principle and how the electronics is supposed to look.
Unfortunately, I don't know anyone at Kvarz, only at the former
T4-Science.

                     Attila Kinali

[1] "Progress in Brazilian Cesium atomic fountain-BrCsF",
by Rodriguez, Bagnato, Bueno et al, 2016
https://doi.org/10.1109/FCS.2016.7546818

[2] "Progress toward Brazilian cesium fountain second generation",
by Bueno, Rodriguez, Müller, et al. 2018
http://dx.doi.org/10.1088/1742-6596/975/1/012071

--
The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto

Attila, >A PLL using the EFC input of the BVA will not work well at these >long time constants. About 1Hz loop bandwidth is the lowest that's >reasonable, I would even draw the line at 10Hz. And only if you >build an active filter using an low-noise opamp. Going lower will >limit your oscillators stability by the noise on the EFC voltage. >You have a 1MΩ resistor, which already produces quite a bit of >noise voltage. And then you use a 50µF capacitor. If it's an >electrolytic capacitor, then the leakage current noise will will destroy >the stability. If it's a ceramic capacitor, then its piezoelectric >properties will couple any acoustic noise and vibration into your >EFC voltage. >Best to ground the EFC voltage and then use a phase/frequency >stepper to shift the frequency of the BVA using a digital control >loop.- I Did tought that even low noise components that I have here (resistors, capacitor opamps (like OPA637 and OP37/27)) may contour these issues. Also, the PLL circuit is temperature-stabilized and mechanical noise poorly insulated. But you have a good point. I may use some SG384 that I also have here to remove the frequency offset and actuate in the long term drift to lock it with the cesium. >If the frequency comb is CEO stabilized (aka f-2f lock) and you can >stabilize its repetition rate using an optical cavity (10cm ULE is >already enough), then you can get better stability than your BVA >in the range up to 10s probably better than 100s, depending on your >setup. If the comb is free running, then the intrinsic instability >of the comb will be larger than the BVA. We also have an optical cavity that is in progress to lock CEO. But this will take a while I guess. The comb is repetition rate locked to BVA and locked itself in the CEO. >Oh nice! Do you already have any publications on this? >I could only find [1] and [2]. Unfortunately that's only the both we have for now... We're ran out of people working on this and haven't publications for a while. Luiz Paulo Em qui., 28 de mai. de 2026 às 12:30, Attila Kinali <attila@kinali.ch> escreveu: > A wonderful good afternoon, > > On Thu, 28 May 2026 10:37:58 -0300 > Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> wrote: > > > Thank you for the considerations. I've tunned the PLL for 0.00289Hz, > today > > i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce > the > > error voltage by changing the voltage in a potentiometer, just like a > > "volume" control in audio systems. I expect to reduce a bit 0,25 times > day > > to day) to archive 1000s loop. > > A PLL using the EFC input of the BVA will not work well at these > long time constants. About 1Hz loop bandwidth is the lowest that's > reasonable, I would even draw the line at 10Hz. And only if you > build an active filter using an low-noise opamp. Going lower will > limit your oscillators stability by the noise on the EFC voltage. > You have a 1MΩ resistor, which already produces quite a bit of > noise voltage. And then you use a 50µF capacitor. If it's an > electrolytic capacitor, then the leakage current noise will will destroy > the stability. If it's a ceramic capacitor, then its piezoelectric > properties will couple any acoustic noise and vibration into your > EFC voltage. > > Best to ground the EFC voltage and then use a phase/frequency > stepper to shift the frequency of the BVA using a digital control > loop.- > > > I can only evaluate this using GNSS PPP - by > > RTKLib in real time or NRCAN for example and / or CGGTTS files. > > > > I have also available for these measurements a frequency comb from menlo > > systems. Can I use repetition rate adev to evaluate the BVA? (locking it > in > > a Cs beam and then in BVA + Cs beam)? > > If the frequency comb is CEO stabilized (aka f-2f lock) and you can > stabilize its repetition rate using an optical cavity (10cm ULE is > already enough), then you can get better stability than your BVA > in the range up to 10s probably better than 100s, depending on your > setup. If the comb is free running, then the intrinsic instability > of the comb will be larger than the BVA. > > > We are working in cold atom clocks here also. A Cs fountain and another > > kind of cold atom Cs clock. But now, we're in the construction phase. No > > measurements being made. > > Oh nice! Do you already have any publications on this? > I could only find [1] and [2]. > > BTW: If you want some known-good reference. The Canadians (IIRC the > NRC itself) sell caesium fountains for a reasonable price. > > > > About getting the maser working again, do you have any experience with > that > > maser? Is the KVARZ CH1-75A. > > I have never personally worked on a AHM myself. I do know their > working principle and how the electronics is supposed to look. > Unfortunately, I don't know anyone at Kvarz, only at the former > T4-Science. > > > Attila Kinali > > > [1] "Progress in Brazilian Cesium atomic fountain-BrCsF", > by Rodriguez, Bagnato, Bueno et al, 2016 > https://doi.org/10.1109/FCS.2016.7546818 > > [2] "Progress toward Brazilian cesium fountain second generation", > by Bueno, Rodriguez, Müller, et al. 2018 > http://dx.doi.org/10.1088/1742-6596/975/1/012071 > > > > -- > The driving force behind research is the question: "Why?" > There are things we don't understand and things we always > wonder about. And that's why we do research. > -- Kobayashi Makoto >
TV
Tom Van Baak
Fri, May 29, 2026 12:23 AM

Both Tom and I have run into that before.

There's a set of photos of the HFO repair here:

http://www.leapsecond.com/museum/ch175/coil.htm

/tvb

> Both Tom and I have run into that before. There's a set of photos of the HFO repair here: http://www.leapsecond.com/museum/ch175/coil.htm /tvb
AK
Attila Kinali
Fri, May 29, 2026 8:44 PM

Ola Luiz Paulo!

On Thu, 28 May 2026 15:13:08 -0300
Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com wrote:

I Did tought that even low noise components that I have here (resistors,
capacitor opamps (like OPA637 and OP37/27)) may contour these issues.

At first this would seem the case. But once you calculate the
contribution of the various elements needed to control the EFC in
an analog PLL system with extremely low bandwith (or large time
constants), the analog components noise and drift will dominate
the stability, especially with such superb OCXOs like the BVA.
It's really best to just ground the EFC and use a digital scheme,
either some DDS based system like the one from Rick Karlquist[1,2]
and the up-then-down conversion systems like the one formerly sold
by SKK Electronics[3], or some off-the-shelf high resolution frequency
synthesizer.

If you go for the off-the-shelf synthesizer, I would suggest you
set it to a higher frequency and then divide it down. This way
you get lower phase noise, less spurs and higher resolution.
I recommend using something akin to a lambda divider[4], as they are
very simple devices and still achieve close to theoretic performance.

We also have an optical cavity that is in progress to lock CEO. But this
will take a while I guess. The comb is repetition rate locked to BVA and
locked itself in the CEO.

Cool. So you are half way there!
Now you need to lock the frequency comb to an optical cavity.
The trick here is that an optical cavity can reach increadibly
high quality factor Q values. Much higher than anything in the
radio frequency and microwave domain could. The frequency comb
is then used to divide the optical frequency down to RF range
so it can be used in electronic measurements.

This is also the trick behind how the PTB CSF2 reaches the
short to midterm stability of an acvite hydrogen maser [5]

Have a nice weekend!

		Attila Kinali

[1] "A Narrow Band High Resolution Synthesizer Using a Direct
Digital Synthesizer Followed by Repeated Dividing And Mixing",
by Rick Karlquist, 1995

[2] "A 3 to 30MHz High-Resolution Synthesizer Consisting of a
DDS, Divde-and-Mix Modules and a M/N Synthesizer", by Rick Karlquist, 1996

[3] "Characterization of an Auxiliary offset Generator for steering
of H Masers", by Rovera, Abgrall, Siccardi, 2012

[4] "The Sampling Theorem in Pi and Lambda Digital Frequency Dividers",
by Claudio Calosso and Enrico Rubiola, 2013.

[5] "Advances in the accuracy, stability, and reliability of the PTB
primary fountain clocks", by Weyers, Gerginov, Kazda, Rahm, Lipphardt,
Dobrev, and Gibble, 2018
https://doi.org/10.1088/1681-7575/aae008

--
The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto

Ola Luiz Paulo! On Thu, 28 May 2026 15:13:08 -0300 Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> wrote: > I Did tought that even low noise components that I have here (resistors, > capacitor opamps (like OPA637 and OP37/27)) may contour these issues. At first this would seem the case. But once you calculate the contribution of the various elements needed to control the EFC in an analog PLL system with extremely low bandwith (or large time constants), the analog components noise and drift will dominate the stability, especially with such superb OCXOs like the BVA. It's really best to just ground the EFC and use a digital scheme, either some DDS based system like the one from Rick Karlquist[1,2] and the up-then-down conversion systems like the one formerly sold by SKK Electronics[3], or some off-the-shelf high resolution frequency synthesizer. If you go for the off-the-shelf synthesizer, I would suggest you set it to a higher frequency and then divide it down. This way you get lower phase noise, less spurs and higher resolution. I recommend using something akin to a lambda divider[4], as they are very simple devices and still achieve close to theoretic performance. > We also have an optical cavity that is in progress to lock CEO. But this > will take a while I guess. The comb is repetition rate locked to BVA and > locked itself in the CEO. Cool. So you are half way there! Now you need to lock the frequency comb to an optical cavity. The trick here is that an optical cavity can reach increadibly high quality factor Q values. Much higher than anything in the radio frequency and microwave domain could. The frequency comb is then used to divide the optical frequency down to RF range so it can be used in electronic measurements. This is also the trick behind how the PTB CSF2 reaches the short to midterm stability of an acvite hydrogen maser [5] Have a nice weekend! Attila Kinali [1] "A Narrow Band High Resolution Synthesizer Using a Direct Digital Synthesizer Followed by Repeated Dividing And Mixing", by Rick Karlquist, 1995 [2] "A 3 to 30MHz High-Resolution Synthesizer Consisting of a DDS, Divde-and-Mix Modules and a M/N Synthesizer", by Rick Karlquist, 1996 [3] "Characterization of an Auxiliary offset Generator for steering of H Masers", by Rovera, Abgrall, Siccardi, 2012 [4] "The Sampling Theorem in Pi and Lambda Digital Frequency Dividers", by Claudio Calosso and Enrico Rubiola, 2013. [5] "Advances in the accuracy, stability, and reliability of the PTB primary fountain clocks", by Weyers, Gerginov, Kazda, Rahm, Lipphardt, Dobrev, and Gibble, 2018 https://doi.org/10.1088/1681-7575/aae008 -- The driving force behind research is the question: "Why?" There are things we don't understand and things we always wonder about. And that's why we do research. -- Kobayashi Makoto
BK
Bob kb8tq
Sat, May 30, 2026 12:26 PM

Hi

Analog PLL’s can work to a point. Just what that point is has been pretty well gone over already.

The 50 uf cap in this case it something I’d be concerted about.

No capacitor is ever ideal. In this case the “parallel resistance” is worth looking at. Dielectrics (all of them)
leak. That leakage is temperature (and maybe other factors …) dependent. This leads you off in the direction
of things like Teflon dielectrics. That gets both expensive and hard to find.

Bob

On May 28, 2026, at 9:37 AM, Luiz Paulo Damaceno via time-nuts time-nuts@lists.febo.com wrote:

Ola, Attila!

Ok. One "easy" first thing you can do is to more loosely couple
your BVA to your Cs beam standard. If your BVA is well aged,
it is likely to perform better than the Cs beam standard up
to 1000s. If you change the loop-bandwidth of your PLL such
that you get somewhere between 0.01Hz and 0.001Hz, then you
could make better use of your BVA. Of course, that's not
as easy as it sounds. If you have some phase measurement
equipment (e.g. a Timepod, but also a red pitaya would probably
do), you could use the BVA as input to the HROG, then compare
the phase of the HROG output and the Cs beam standard. It would
be then pretty easy to do the PLL loop on some PC and use the
HROG for the control/feedback part.

Thank you for the considerations. I've tunned the PLL for 0.00289Hz, today
i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce the
error voltage by changing the voltage in a potentiometer, just like a
"volume" control in audio systems. I expect to reduce a bit 0,25 times day
to day) to archive 1000s loop. I can only evaluate this using GNSS PPP - by
RTKLib in real time or NRCAN for example and / or CGGTTS files.

I have also available for these measurements a frequency comb from menlo
systems. Can I use repetition rate adev to evaluate the BVA? (locking it in
a Cs beam and then in BVA + Cs beam)?

Ok, so you don't have any legal requirement to keep a continuous
timescale. I guess your primary need is to provide a local realization
of the SI second that is as accurate as possible with as little noise
and uncertainty as possible?

Yes, no legal requirement, here in Brazil, only ONJR has the legal
requirement. Yes, my primary need is to provide a local realization of SI
second with little noise and uncertainty.

We are working in cold atom clocks here also. A Cs fountain and another
kind of cold atom Cs clock. But now, we're in the construction phase. No
measurements being made.

About getting the maser working again, do you have any experience with that
maser? Is the KVARZ CH1-75A.

Abraços,

Luiz Paulo

Em ter., 26 de mai. de 2026 às 11:27, Attila Kinali attila@kinali.ch
escreveu:

Ola Luiz Paulo!

On Tue, 26 May 2026 10:21:03 -0300
Luiz Paulo Damaceno luizpauloeletrico42@gmail.com wrote:

-> I want to achieve long term stability and also short term

performance.

I think both are important to us. I can figure out that things better

than we

have now may need more clocks or a change of base clock.

Ok. One "easy" first thing you can do is to more loosely couple
your BVA to your Cs beam standard. If your BVA is well aged,
it is likely to perform better than the Cs beam standard up
to 1000s. If you change the loop-bandwidth of your PLL such
that you get somewhere between 0.01Hz and 0.001Hz, then you
could make better use of your BVA. Of course, that's not
as easy as it sounds. If you have some phase measurement
equipment (e.g. a Timepod, but also a red pitaya would probably
do), you could use the BVA as input to the HROG, then compare
the phase of the HROG output and the Cs beam standard. It would
be then pretty easy to do the PLL loop on some PC and use the
HROG for the control/feedback part.

-> Quite honestly, given that you are an NMI and we are talking about
a national timescale, I would recommend that you first try to enhance
your resilience against device failures. Having only a single Cs beam
standard, which need a replacement tube every 5 to 20 years (depending
on type and chance), you run the risk of losing your timescale when your
Cs beam standard runs out of Cs.

  • I'm not an NMI, I'm in a university that runs atomic physics
    experiments.

Oh.. sorry. My apologies! I assumed that you were an NMI as it is
rare that non-NMIs contribute to TAI/UTC.

Our UTC time scale is one way for us to have trackability to
Cs frequency realization.

  • Actually we have a second Cs beam that is not running due to this:

have

a second one in case of failure, at least.

Ok, so you don't have any legal requirement to keep a continuous
timescale. I guess your primary need is to provide a local realization
of the SI second that is as accurate as possible with as little noise
and uncertainty as possible?

Then I would focus on getting the hydrogen maser working again
and use it as input to the HROG. That will provide you the best
short to medium term performance.

Then use your phase meter to compare your HROG output and the
Cs beam output. This way you can correct for the drift of the
maser. Use the GNSS system to correct the drift of the Cs beam
standard with a tau in the range of a few weeks to a month.

This is basically what METAS does (minus the Cs fountain that
they periodically run) [1].

BTW: If your research involves optical atomic clocks and their
absolute frequency measurement, you might want to consider getting
a primary frequency standard. In the course of the presentation on the
2025 BIPM recommended frequency list at EFTF last month, Helen Margolis
from NPL did complain about the correlations of absolute frequency
measurements done through UTC, which are very hard to properly handle.

                    Attila Kinali

[1] "METAS new time scale generation system - A progress report"
by Bernier, Dudle and Schlunegger, 2006
http://time.kinali.ch/ptti/2006papers/paper3.pdf

The driving force behind research is the question: "Why?"
There are things we don't understand and things we always
wonder about. And that's why we do research.
-- Kobayashi Makoto


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Hi Analog PLL’s can work to a point. Just what that point is has been pretty well gone over already. The 50 uf cap in this case it something I’d be concerted about. No capacitor is ever ideal. In this case the “parallel resistance” is worth looking at. Dielectrics (all of them) leak. That leakage is temperature (and maybe other factors …) dependent. This leads you off in the direction of things like Teflon dielectrics. That gets both expensive and hard to find. Bob > On May 28, 2026, at 9:37 AM, Luiz Paulo Damaceno via time-nuts <time-nuts@lists.febo.com> wrote: > > Ola, Attila! > >> Ok. One "easy" first thing you can do is to more loosely couple >> your BVA to your Cs beam standard. If your BVA is well aged, >> it is likely to perform better than the Cs beam standard up >> to 1000s. If you change the loop-bandwidth of your PLL such >> that you get somewhere between 0.01Hz and 0.001Hz, then you >> could make better use of your BVA. Of course, that's not >> as easy as it sounds. If you have some phase measurement >> equipment (e.g. a Timepod, but also a red pitaya would probably >> do), you could use the BVA as input to the HROG, then compare >> the phase of the HROG output and the Cs beam standard. It would >> be then pretty easy to do the PLL loop on some PC and use the >> HROG for the control/feedback part. > > Thank you for the considerations. I've tunned the PLL for 0.00289Hz, today > i'm using a 1,1M ohm resistance and 50 uF capacitor. I can also reduce the > error voltage by changing the voltage in a potentiometer, just like a > "volume" control in audio systems. I expect to reduce a bit 0,25 times day > to day) to archive 1000s loop. I can only evaluate this using GNSS PPP - by > RTKLib in real time or NRCAN for example and / or CGGTTS files. > > I have also available for these measurements a frequency comb from menlo > systems. Can I use repetition rate adev to evaluate the BVA? (locking it in > a Cs beam and then in BVA + Cs beam)? > >> Ok, so you don't have any legal requirement to keep a continuous >> timescale. I guess your primary need is to provide a local realization >> of the SI second that is as accurate as possible with as little noise >> and uncertainty as possible? > > Yes, no legal requirement, here in Brazil, only ONJR has the legal > requirement. Yes, my primary need is to provide a local realization of SI > second with little noise and uncertainty. > > We are working in cold atom clocks here also. A Cs fountain and another > kind of cold atom Cs clock. But now, we're in the construction phase. No > measurements being made. > > About getting the maser working again, do you have any experience with that > maser? Is the KVARZ CH1-75A. > > Abraços, > > Luiz Paulo > > Em ter., 26 de mai. de 2026 às 11:27, Attila Kinali <attila@kinali.ch> > escreveu: > >> Ola Luiz Paulo! >> >> On Tue, 26 May 2026 10:21:03 -0300 >> Luiz Paulo Damaceno <luizpauloeletrico42@gmail.com> wrote: >> >>> -> I want to achieve long term stability and also short term >> performance. >>> I think both are important to us. I can figure out that things better >> than we >>> have now may need more clocks or a change of base clock. >> >> Ok. One "easy" first thing you can do is to more loosely couple >> your BVA to your Cs beam standard. If your BVA is well aged, >> it is likely to perform better than the Cs beam standard up >> to 1000s. If you change the loop-bandwidth of your PLL such >> that you get somewhere between 0.01Hz and 0.001Hz, then you >> could make better use of your BVA. Of course, that's not >> as easy as it sounds. If you have some phase measurement >> equipment (e.g. a Timepod, but also a red pitaya would probably >> do), you could use the BVA as input to the HROG, then compare >> the phase of the HROG output and the Cs beam standard. It would >> be then pretty easy to do the PLL loop on some PC and use the >> HROG for the control/feedback part. >> >>> -> Quite honestly, given that you are an NMI and we are talking about >>> a national timescale, I would recommend that you first try to enhance >>> your resilience against device failures. Having only a single Cs beam >>> standard, which need a replacement tube every 5 to 20 years (depending >>> on type and chance), you run the risk of losing your timescale when your >>> Cs beam standard runs out of Cs. >>> - I'm not an NMI, I'm in a university that runs atomic physics >>> experiments. >> >> Oh.. sorry. My apologies! I assumed that you were an NMI as it is >> rare that non-NMIs contribute to TAI/UTC. >> >>> Our UTC time scale is one way for us to have trackability to >>> Cs frequency realization. >>> - Actually we have a second Cs beam that is not running due to this: >> have >>> a second one in case of failure, at least. >> >> Ok, so you don't have any legal requirement to keep a continuous >> timescale. I guess your primary need is to provide a local realization >> of the SI second that is as accurate as possible with as little noise >> and uncertainty as possible? >> >> Then I would focus on getting the hydrogen maser working again >> and use it as input to the HROG. That will provide you the best >> short to medium term performance. >> >> Then use your phase meter to compare your HROG output and the >> Cs beam output. This way you can correct for the drift of the >> maser. Use the GNSS system to correct the drift of the Cs beam >> standard with a tau in the range of a few weeks to a month. >> >> This is basically what METAS does (minus the Cs fountain that >> they periodically run) [1]. >> >> BTW: If your research involves optical atomic clocks and their >> absolute frequency measurement, you might want to consider getting >> a primary frequency standard. In the course of the presentation on the >> 2025 BIPM recommended frequency list at EFTF last month, Helen Margolis >> from NPL did complain about the correlations of absolute frequency >> measurements done through UTC, which are very hard to properly handle. >> >> >> Attila Kinali >> >> >> [1] "METAS new time scale generation system - A progress report" >> by Bernier, Dudle and Schlunegger, 2006 >> http://time.kinali.ch/ptti/2006papers/paper3.pdf >> -- >> The driving force behind research is the question: "Why?" >> There are things we don't understand and things we always >> wonder about. And that's why we do research. >> -- Kobayashi Makoto >> > _______________________________________________ > time-nuts mailing list -- time-nuts@lists.febo.com > To unsubscribe send an email to time-nuts-leave@lists.febo.com