separate units would cancel out for two GPSDOs but add for the
> Cs.
>
> Bob
>
>
>
>
> -----
> From: Bruce Griffiths <bruce.griffi...@xtra.co.nz>
> To: Bob Stewart <b...@evoria.net>; Dis
me conditions, yet the ADEV of the Cs is obviously not as good as
> that of the GPSDO. Also, the ADEV of the GPSDO pretty much tracks what is to
> be expected when run on a good 5370, isn't it?
>
> Bob
>
>
>
> ---------
>
bably be useful
> for such measurements."
>
> What would such an "inexpensive" device be? What's inexpensive for you
> would probably be way out of my reach.
>
> Bob
>
>
>
>
> ---
. Of course, I don't know anything more than that. Correct?
>
> Bob
>
>
> From: Bruce Griffiths <bruce.griffi...@xtra.co.nz>
> To: Bob Stewart <b...@evoria.net>; Discussion of precise time and frequency
> measurement <time-nuts@febo.com>
> Sent: Saturd
Bob
That doesn't seem inconsistent with the specs given the contribution of the
5370A to the measured ADEV is likely to be of the same order as the PRS45A
spec. The ADEV of the GPSDO also needs to be taken into account. The
contribution of the 5370A to ADEV will gradually become insignificant
"cells".
Bruce
On Thursday, 23 February 2017 3:09 PM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
It would be better to lock the laser to a suitable optical absorption line or
other optical transition.Long term stability can be better than an optical
For a spherical body of uniform density the value of g below the surface is
proportional to the radial distance of the location from the centre of the
sphere. For a spherically symmetric body only the mass contained within the
sphere below the point has any effect on the measured value of g.
On Tuesday, February 21, 2017 11:13:34 AM Rhoderick Beery wrote:
> Greetings Time-Nuts!
>
> I'm a physics theorist interested in performing an experiment to measure
> the gravitational time dilation beneath the surface of the Earth. Boulby
> Labs in the UK is 1.1 km down which would generate a
An entire room kept near to absolute zero with a simple door access???Unlikely,
likely the writer is unfamiliar with science/engineering.
Bruce
On Saturday, 14 January 2017 11:39 AM, Gary Woods
wrote:
Hydrogen maser in radio astronomy to sync worldwide
Angus
Read the paper I posted on the current state of the art.
ADEV ~ 2E-13/SQRT(Tau) is feasible with large cells and using a laser instead
of rubidium lamp.In principle, one can use the same cell to lock the laser to
the rubidium absorption line and lock the microwave signal.Suitable laser
One could always use a cryo pump.
The following paper is a summary of the current state of the art for rubidium
vapour frequency
standards:http://www.euramet.org/Media/docs/Repository/A169/IND55/micalizio_02182015.pdf
Bruce
On Wednesday, 11 January 2017 5:15 PM, Ole Petter Ronningen
of the diffusing coating
(typically Barium sulphate with an organic binder). Roughening (fine grind
followed by HF etch for stress relief) the outer surface of the cell is also
advisable to eliminate light pipe effects in the cell wall.
Bruce
On Wednesday, 11 January 2017 3:54 PM, Bruce Griffiths
A possible RF chain for a Rubidium standard using off the shelf parts plus a
couple of custom microwave filters:https://arxiv.org/pdf/1204.4215.pdf
Bruce
On Wednesday, 11 January 2017 2:10 PM, Bob Camp wrote:
Hi
The gotcha is that 5065’s never were a popular item in
:33 PM Bruce Griffiths wrote:
> Possible sources of Rubium vapour
>
cells:https://www.thorlabs.com/newgrouppage9.cfm?objectgroup_id=1470
>
> http://www.precisionglassblowing.com/custom-solutions/optical-glassware/vapo
> r-wavelength-reference-cells/
>
> https://www.sach
andard …. not really
easy at all.
Bob
> On Jan 8, 2017, at 3:55 PM, Bruce Griffiths <bruce.griffi...@xtra.co.nz>
> wrote:
>
> The rubidium standard appears much more manageable given that the cavity
> dimensions are somewhat more compact and rubidium vapour cells are readily
> a
You could try a cavity like the one in;http://tf.nist.gov/general/pdf/156.pdf
This avoids the requirement for a fused quartz storage bulb.
Bruce
On Sunday, 8 January 2017 11:33 PM, timeok wrote:
Hi,
the thought of being able to work on building a H Maser has always
January 2017 11:46 AM, Bob Camp <kb...@n1k.org> wrote:
Hi
> On Jan 2, 2017, at 5:02 PM, Bruce Griffiths <bruce.griffi...@xtra.co.nz>
> wrote:
>
>
> Maybe a waterjet cutter would imapct less on the shielding properties of
> tthe mumetal?
>
Maybe …. pretty
Make that a dual rate moon camera.These were used to measure variations in
Earth's rotation period.
Bruce
On Tuesday, 3 January 2017 11:10 AM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
Carter did have a couple of small historic brass transit instruments which
were neve
2017 10:35 AM, Will Kimber <zl1...@gmx.com> wrote:
Apologies Bruce,
It is a good many years since I was there last.
Cheers,
Will
On 01/03/2017 12:40 AM, Bruce Griffiths wrote:
> You mean the Dominion observatory surely not Carter. It was close by and also
> had a Danjon Astrol
Maybe a waterjet cutter would imapct less on the shielding properties of
tthe mumetal?
Bruce
On Monday, January 02, 2017 12:58:55 PM Bob Camp wrote:
> Hi
>
> > On Jan 1, 2017, at 7:31 PM, wb6bnq wrote:
> >
> > Hello Mathias,
> >
> > I think you did not quite understand how
You mean the Dominion observatory surely not Carter. It was close by and also
had a Danjon Astrolabe.
Bruce
On Tuesday, 3 January 2017 12:10 AM, Hal Murray
wrote:
tract...@ihug.co.nz said:
> The 'landline' networks also have significant (and variable)
Attila
Lookup "Stellar compass" as used for determining space probe attitude.Can also
be used to determine the direction of the centre of an image of a field of
bright stars.Subarcsecond accuracy is fairly routine.Pattern recognition
techniques combined with measures of the relative brightness
Yes, the very low frequency noise of these regulators isn't anywhere near as
impressive as their high frequency noise.However for some RF circuits the low
frequency power supply noise may not be as significant as other effects.
Bruce
On Thursday, 8 December 2016 2:59 PM, Gerhard Hoffmann
device currently available.
On 11/24/2016 01:03 PM, Bruce Griffiths wrote:
> John
>
> There is an application note or similar on the 53230A that indicates that
> the single shot noise for time interval measurement is typically about 13ps
> or so.
>
> Bruce
> On Thursday,
John
There is an application note or similar on the 53230A that indicates that
the single shot noise for time interval measurement is typically about 13ps
or so.
Bruce
On Thursday, November 24, 2016 09:43:54 AM John Ackermann N8UR
wrote:
> Hi Anders --
>
> Thanks, and thanks for the info on
1-2ps rms single shot noise timestamping is feasible with embedded (occurs as
part of the interpolation process) interpolator calibration. Only calibration
of the differential delay between channels is required, as is required by all
such instruments.
However the cost for such a timestamping
With no internal PLL to generate a higher internal frequency than the 25MHz
MCLK, that 1MHz waveform looks a bit too smooth for an unfiltered 1MHz output.
Bruce
On Friday, 18 November 2016 5:12 PM, Richard (Rick) Karlquist
wrote:
Trying to figure out what "Iout
On Thursday, November 10, 2016 02:23:19 PM xaos wrote:
> I wonder if there is a way to get a voltage standard out of a frequency
> standard (GPS Disciplined).
> I think the big problem is probably voltage stability due to temperature
> variations.
>
> Any thoughts on this ?
>
> -George
>
> On
Neither Rb cells nor isolators are difficult to source.They are both catalog
items. However if using a cavity it may need to be tailored to the available
cells.Walk-off isolators using double refraction are somewhat more convenient
than those requiring a strong magnetic field.
Bruce
On
On Saturday, November 05, 2016 12:12:18 PM Tom Van Baak wrote:
> See C13 in the attached photo. I need to replace some blown caps on a
few
> boards [1]. In one instance the cap got so hot it melted itself off the
> board. Quiet convenient, actually -- it acts like its own fuse -- but I
> don't
Ilia
Circuit diagrams are posted here from time to time, so it should be OK.
Bruce
On Saturday, 5 November 2016 7:02 PM, Ilia Platone
wrote:
Hi, and thank you for these suggestions.
Currently this project becomes reality (slowly): this kind of
The N resonance discussedd
in:http://walsworth.physics.harvard.edu/publications/2005_Smallwood_HUBAThesis.pdf
May be a better bet than traditional CPT.
Bruce
On Saturday, 5 November 2016 12:17 PM, Magnus Danielson
wrote:
Poul-Henning,
On 11/05/2016 12:04
Hej Magnus
A quarter waveplate doesn't depolarise, it can however convert a linearly
polarised beam to a circularly polarised one.If you really need to depolarise a
laser beam, scattering from a colloidal suspension of Titanium dioxide is very
effective.There are no macroscopic moving
On Friday, November 04, 2016 09:27:59 PM Poul-Henning Kamp wrote:
>
> In message <2af27ebe-9200-c348-c89b-b98f9c973...@karlquist.com>,
"Richard
> (Rick) Karlquist" w
> rites:
> >Also, one of the Rb isotopes is slightly radioactive.
> >35 years ago, the guy in the next cubicle got away
Suitable ECDL laser for Rb
clock:https://www.sacher-laser.com/home/industrial-lasers/point_and_line_laser_module.html
the 784.8 nm version has 0.2nm of tuning range,
Bruce
On Friday, 4 November 2016 2:43 PM, Tim Shoppa wrote:
Zero. But the answer is also zero for a
at the University of Neuchatel.
Bruce
On Friday, 4 November 2016 11:58 AM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
There is at least one recent thesis where a dual resonance rubidium vapor cell
was built and used to lock a low noise OCXO,The machining of the cavity didnt
There is at least one recent thesis where a dual resonance rubidium vapor cell
was built and used to lock a low noise OCXO,The machining of the cavity didnt
appear particularly challenging nor did the locking of the laser to the
relevant wavelength using an auxiliary rubidium vapour cell.IIRC
Another issue is that the finer the timestamp quantisation step size the larger
the signal of interest (Intensity correlation). The signal doesn't vanish as
the timestamp quantisation step size increases however the signal decreases
requiring a longer observation time to achieve a given SNR.
10us deadtime is somewhat excessive for average detection rates much greater
than 1kcps (kilo counts/sec).Higher rates will tend to have the correlations
between detectors suppressed. This will be particulalrly acute for Intensity
correlations.Active detector (Geiger mode APD) quenching is
On Thursday, October 20, 2016 08:12:12 PM Attila Kinali wrote:
> On Thu, 20 Oct 2016 10:59:21 +0100
>
> "David J Taylor" wrote:
> > Actually, of the 15 Raspberry Pi cards I have only one is used in a
> > graphics application.
>
> Yes, the rpi are used for all kind
On Thursday, September 22, 2016 01:37:02 AM Gerhard Hoffmann wrote:
> Am 22.09.2016 um 00:24 schrieb Bruce Griffiths:
> > Another issue is the requirement to trim the current sink for low
output
> > offset.
>
> And _that_ FET is made from Unobtainium.
>
> > If o
On Wednesday, September 21, 2016 08:59:18 PM Attila Kinali wrote:
> On Wed, 21 Sep 2016 09:16:18 -0700
>
> Dan Rae wrote:
> > On 9/21/2016 9:01 AM, David C. Partridge wrote:
> > > Yes, I fear a timepod is a bit out of my budget (I can dream tho').
> > > Over here in the UK
On Tuesday, September 20, 2016 01:53:49 PM Tim Lister wrote:
> On Tue, Sep 20, 2016 at 12:56 PM, Bryan _
wrote:
> > May also want to check the output amplitude. If memory serves me
correct
> > it is very common for a capacitor inside this model number to fail. It
> > can be
on set internally to the analyser.
The results are attached.
Dave
-Original Message-
From: time-nuts [mailto:time-nuts-boun...@febo.com] On Behalf Of Bruce Griffiths
Sent: 18 September 2016 12:52
To: Discussion of precise time and frequency measurement
Subject: Re: [time-nuts] Thunderbolt
The signal level is also very low.
Brue
On Sunday, 18 September 2016 11:47 PM, Magnus Danielson
wrote:
The phase-noise still looks fairly high. How do you measure this?
Cheers,
Magnus
On 09/18/2016 01:27 PM, David C. Partridge wrote:
> Now that's
The PN should be considerably lower than that even with the noisy output buffer
the PN floor should be considerably lower (>40db lower). The OCXO by itself
should have somewhat lower PN.
Bruce
On Sunday, 18 September 2016 11:14 PM, David C. Partridge
wrote:
Also avoids thermomechanical fatigue failure in the Peltier device.
On Wednesday, 7 September 2016 12:14 AM, jimlux
wrote:
On 9/6/16 1:19 AM, Adrian Godwin wrote:
> On Tue, Sep 6, 2016 at 4:24 AM, Bob Darlington
> wrote:
>
>> Rick,
>>
>>
Post should have been:
Acts like noise current flowing in the voltage setting network (R || C).Flicker
noise appears to kick in below 1Hz or so.
Bruce
On Thursday, 1 September 2016 8:23 PM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
Acts like current noise f
~22nV/rtHz) isn't significant in comparison with other sources.
Bruce
On Thursday, 1 September 2016 5:56 PM, Gerhard Hoffmann <dk...@arcor.de>
wrote:
Am 01.09.2016 um 06:07 schrieb Bruce Griffiths:
> I have a quad LT3042 PCB that I must get around to assembling.One potential
Just split the 1uF coupling cap into 2x 2u2 in series in the Cuk dc-dc
converter add a 1:1 transformer (should be small at 2MHz) between the pair of
2u2 caps to produce a floating output and use an LT3042 as a post
regulator.With a mains transformer input supply a separate isolated winding for
If onen is going to use a dc-dc converter the Cuk converter used here is a nice
topology in that it can have low input and output ripple currents. However
input and output filters like the Murata BNX002/BNX005 series would have been
useful as would an LM3042 linear post regulator for the -12V
wrote:
From: Bruce Griffiths
You'd need a rather thick copper jacket to shield effectively against the
50Hz magnetic field.
Bruce
==
Would mu-metal be any use?
https://en.wikipedia.org/wiki/Mu-metal
http://mumetal.co.uk/
Cheers,
David
--
SatSignal Software - Q
the EM field?
André Esteves
2016-08-25 0:33 GMT+01:00 Bruce Griffiths <bruce.griffi...@xtra.co.nz>:
> The Kerr effect is Proportional to the square of the field so one would
> expect a strong 100Hz component from this.
>
> The magneto optical Kerr eefect which rotates the plane of
The Kerr effect is Proportional to the square of the field so one would
expect a strong 100Hz component from this.
The magneto optical Kerr eefect which rotates the plane of polarisation is
linear however.
Bruce
On Wednesday, August 24, 2016 07:04:31 AM Bob kb8tq wrote:
> Hi
>
> I would not
The stability of the typical GPS receiver oscillator is usually inadequate to
be useful as a GPSDO. An OCXO (as in the Trimble Thunderbolt for example) or
equivalent is usually required. One can't usually just add a varicap to adjust
the frequency of a packaged oscillator. If an external
On Friday, August 12, 2016 12:21:55 PM David wrote:
> On Fri, 12 Aug 2016 13:56:40 +0200, you wrote:
> >Hi everyone,
> >
> >On 2016-08-11 21:06:12, Attila Kinali wrote:
> >> Hoi Bert,
> >>
> >> I'm asking, because if you go the way of using a CPLD anyways, you
could
> >> throw in another $2 for
On Tuesday, August 02, 2016 01:03:58 PM Gerhard
Hoffmann wrote:
> Am 02.08.2016 um 09:14 schrieb Bruce Griffiths:
>
>
> ... and a screen dump for the LTspice challenged
>
> ;-) Gerhard
Uually a zero is needed in the bias stabilisation loop to
eliminate low frequency ga
the conventional approach.
Bruce
On Tuesday, 2 August 2016 6:19 PM, Alex Pummer <a...@pcscons.com> wrote:
Ja Gerhard, bitte schicke mir den LTSpice file,
Danke im Voraus und
73
KJ6UHN
Alex
On 8/1/2016 6:34 PM, Gerhard Hoffmann wrote:
> Am 02.08.2016 um 02:42 schrieb Bruce Griffiths:
"I'm working on a new amplifier based on IF3602 or BF862 FETs that can
use 10u foil only."
Similar to that published by Groner in Linear Audio?
Bruce
On Tuesday, 2 August 2016 12:12 PM, Gerhard Hoffmann wrote:
Am 01.08.2016 um 22:16 schrieb David:
> This duplicates the
art.This issue was discussed on
the list some time ago,
Bruce
On Friday, 29 July 2016 6:31 AM, Attila Kinali <att...@kinali.ch> wrote:
On Fri, 22 Jul 2016 08:19:43 + (UTC)
Bruce Griffiths <bruce.griffi...@xtra.co.nz> wrote:
> No, the first one merely uses a pair of casc
On Wednesday, July 27, 2016 08:55:20 PM Robert LaJeunesse wrote:
> The concept of track & hold was well understood in 1966 and documented in
> the classic Philbrick Researches amplifier application book, now available
> at
>
The PFC power supply architecture I had in mind uses a flyback inverter to
regulate the input rail voltage for the output dc-dc converter stage. The
flyback stage peak current is modulated by a sinewave. A feedback loop adjusts
the effective amplitude of this sinusoidal modulation to regulate
The PFC stage needs a line frequency sinewave reference, if this is produced by
attenuating the line input, then it may not function well with badly distorted
line input waveforms (modified sine, square wave etc).Phase locking a sinewave
to the line input may be a better approach.
Bruce
The AD5791 evaluation board has an unpopulated area for what appears to be an
LTZ1000 reference circuit.
Bruce
On Sunday, 24 July 2016 7:00 AM, Attila Kinali wrote:
On Fri, 22 Jul 2016 12:15:25 -0500
David wrote:
> If you expect analog
No, the first one merely uses a pair of cascaded heterodyne PLLs as shown on p3
of the manual.A diophantine setup may be useful here if one wished to construct
something similar.
Bruce
From: Anders Wallin
To: Discussion of precise time and frequency
The most effective approach would be to design a replacement with lower jitter
(< 5ps ) and lower power consumption (< 10W??).The hard/interesting part is the
higher resolution lower jitter interpolator.Preliminary testing suggests this
part isnt as difficult as first thought.
As soon (within a
I can't seem to get the line related spurs much below -170dBc/Hz for the
fundamental and -180dBc/Hz for the line frequency related harmonics. Everything
was bolted down to a 12mm thick aluminium slab. Avoiding an Earth loop by
isolating the Timepod Ch0 and CH2 inputs from the aluminium plate
The optimum sine to square converter is embodied in the Collins style limiter
approach consisting of a cascade of limiting amplifiers each with suitable
individual gain and individual bandwidth, the gain and bandwidth increasing for
each successive stage until the output slew rate is sufficient
On Sunday, June 19, 2016 07:23:09 PM Attila Kinali wrote:
> Good evening,
>
> I have recently been looking into BJT's and their switching properties.
> Because a time-to-amplitude converter does similar things as I would like
> to, I have been looking in what people do with those. First thing
It almost sounds like something has been found not to be ROHS compliant.Could
be as simple as the alodined (conventional process uses hexavalent chromium )
case or perhaps a non ROHS part was used.
Bruce
On Sunday, 19 June 2016 8:02 PM, John Miles wrote:
> On 6/18/16
be required.
Bruce
On Tuesday, 14 June 2016 6:01 PM, Chris Caudle <ch...@chriscaudle.org>
wrote:
On Mon, June 13, 2016 9:38 pm, Bruce Griffiths wrote:
> If the quantisation noise is random and spread uniformly over the Nyquist
> bandwidth (~40MHz??) then the noise floor is about -82
The subsequent all digital mixdown and low pass filtering, if done correctly,
will increase the resolution provided that the signal and reference periods are
uniformly sampled at a sufficient equivalent number of points. But with a
starting point some 70dB or more behind an ADC, the system
or less.
The problem lies in ensuring that the quantisation noise is actually
random..With a high resolution RF ADC internal noise is usually sufficient (>=
1 lsb)) to ensure this.
Bruce
On Tuesday, 14 June 2016 2:11 PM, Bruce Griffiths
<bruce.griffi...@xtra..co.nz&
have lower phase
noise than CMOS at low offset frequencies.
Bruce
On Monday, 13 June 2016 8:12 PM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
Adjusting the sampling clock frequency so that is neither a harmonic nor a
harmonic of a subharmonic of either of the clock frequ
Adjusting the sampling clock frequency so that is neither a harmonic nor a
harmonic of a subharmonic of either of the clock frequencies being compared
ensures that each clock waveform isnt repeatedly sampled at a small set of
points.i.e.
fsample != (m/n)*ftest
andfsample != (p/q)*freference
Perhaps a location for an alternate receiver used in another model/version that
shared the same PCB albeit populated with different OCXOs etc?.
Interesting that 2 ocxos appear to be in use.
Bruce
On Sunday, 5 June 2016 5:53 PM, Charles Steinmetz
wrote:
Isn't
More likely the missing GPS receiver board is installed over the ground plane.
Bruce
On Sunday, 5 June 2016 4:11 PM, Hui Zhang wrote:
Dear group:
Does anyone familiar with this Symmtricom GPSDO board? I have searched on
internet but I have not found any manual or
, the crystal
parameters can be extracted without knowledge of the phase shift.
Bruce
On Saturday, 4 June 2016 11:01 PM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
On reflection, building a jig to measure the crystal transmission as a
function of frequency may be much easie
Some idea of the crystal equivalent circuit at the oscillation frequency would
help considerably. Usually lower frequency crystals have a considerably higher
series resistance than those operated at 1MHz or above.
At frequencies below 100kHz or so a Meacham bridge using something likke a
to design a suitable
oscillator circuit. Measuring the location of spurious resonances may also be
useful.
Bruce
On Saturday, 4 June 2016 9:52 PM, Bruce Griffiths
<bruce.griffi...@xtra..co.nz> wrote:
Some idea of the crystal equivalent circuit at the oscillation frequency would
Microdot (now available from TE connectivity) made these for 50 ohm, 75 ohm and
93 ohm coax. Digikey have 50 ohm coax male versions.
Bruce
On Saturday, 4 June 2016 3:02 PM, Tom Miller
wrote:
I've seen these used for accelerometer cables.
t; On May 28, 2016, at 11:04 AM, Bruce Griffiths <bruce.griffi...@xtra.co.nz>
> wrote:
>
> One can just measure the TDEV performance.I can measure the TDEV performance
> at 10MHz later today if that's useful.It should be somewhat similar to the
> singl
On Sunday, 29 May 2016 2:04 AM, Attila Kinali <att...@kinali.ch> wrote:
On Sat, 28 May 2016 08:47:45 + (UTC)
Bruce Griffiths <bruce.griffi...@xtra.co.nz> wrote:
> This SDR setup appears to have a higher PN (at least 2 ADC's per signal
> are required to achieve lower PN ) than
A low pass filter will reduce the source broadband noise aliased into the ADC
output signal.
Using the LVDS ADC outputs rather than the CMOS outputs may help in reducing
noise generated on the board. NB the ADC performance is specified when the LVDS
outputs are used.
This SDR setup appears to
lone V SoC FPGA running at 800MHz. Installments to his series have
been slow coming, but I've been wondering if this could be the basis for a
Timepod type of unit.
Bob
On Fri, 5/27/16, Bruce Griffiths <bruce.griffi...@xtra.co.nz> wrote:
circuitry may degrade the performance compared to that
achieved with lower maximum sampling rate ADC pairs.
Bruce
On Saturday, 28 May 2016 4:01 PM, Bob Camp <kb...@n1k.org> wrote:
Hi
> On May 27, 2016, at 8:17 PM, Bruce Griffiths <bruce.griffi...@xtra.co.nz>
> wrote
than
that of the TI ADC used in the ETTUS 210 SDR.
Bruce
On Saturday, 28 May 2016 3:08 PM, Bruce Griffiths
<bruce.griffi...@xtra..co.nz> wrote:
The Red Pitaya FPGA may be a little too small.Its not clear if a single chip
ADC is used.If not, the performance will suffer.Dc c
The Red Pitaya FPGA may be a little too small.Its not clear if a single chip
ADC is used.If not, the performance will suffer.Dc coupled inputs will degrade
the performance somewhat compared to transformer coupled inputs.
Input bandwidth would be around 40MHz or so for the Nyquist band of
On Thursday, May 26, 2016 06:40:26 PM Bob Camp wrote:
> Hi
>
> Very interesting paper, thanks for sharing !!
>
> One question:
>
> In many DMTD (and single mixer) systems, a lowpass and high pass filter are
> applied to the signal coming out of the mixer. This is done to improve the
> zero
However the value of the second time constant in the active PI filter required
to achieve reasonable damping will be around 1600 seconds. This corresponds to
an active PI filter proportional gain of 16.
Bruce
On Wednesday, 25 May 2016 3:20 PM, Bruce Griffiths
<bruce.griffi...@xtra.co
When comparing a 10MHz OCXO divided down to 1Hz with a GPS PPS signal, the
effective VCO gain (Ko/N) is likely to be around 6E-7 rad/s/V (eg HP10811A) and
the phase detector gain around 1V/rad. Consequently a PLL loop bandwidth of
100uHz only requires an Integrator time constant of around 100
The grid current of most tubes (apart from electrometer tubes operated at low
voltage) is much larger than most FETs (apart from very large area ones).. The
other issue with tube grid currents is that zero current corresponds to a
delicate balance between electon and ion currents so the grid
Search for 105B on Didier's site.There are 2 files that contain the relevant
schematics and change data for versions with10811A's. Although my 10811A
equipped HP105B variant appears to have the old power supply with MC1468's
rather than the later version using LM317's.
Bruce
On
PM, Bruce Griffiths
<bruce.griffi...@xtra..co.nz> wrote:
The input noise of a 125 series gate will be far larger than the noise at the
mixer output at the beat frequency. A 125 may be useful as the output stage of
a Collins style limiter chain wherein which the gain and bandwidth o
by ensuring that the DDS
only contributes a small fraction of the offset frequency.
At least a modular system will allow these issues to be explored.
Bruce
On Thursday, 12 May 2016 5:00 PM, Bruce Griffiths
<bruce.griffi...@xtra..co.nz> wrote:
For DMTD service with an offset fre
raises the ugly sepctre of unwanted close in
spurs, unless one chooses one of the magic frequency outputs that is free of
such spurs.
Bruce
On Thursday, 12 May 2016 3:33 PM, Bruce Griffiths
<bruce.griffi...@xtra..co.nz> wrote:
For DMTD service with an offset frequency of 100Hz o
For DMTD service with an offset frequency of 100Hz or less the flicker phase
noise of the mixer is more important than its wideband PN floor.The RDP series
phase detectors are amongst the lowest PN noise mixer/phase detectors
commercially available. They are considerably quieter than the TUF
Bruce
On Tuesday, 10 May 2016 9:17 PM, Attila Kinali <att...@kinali.ch> wrote:
Hoi Bruce,
On Mon, 9 May 2016 23:34:24 + (UTC)
Bruce Griffiths <bruce.griffi...@xtra.co.nz> wrote:
> Its probably easier/cheaper to construct a suitable filter for a GSPS ADC
> than
custom IC is probably the
only effective solution for such a TAC. The somewhat heroic measures employed
in the Wavecrest counters is perhaps the limit of discrete construction
techniques.
Bruce
On Tuesday, 10 May 2016 1:08 AM, Bruce Griffiths
<bruce.griffi...@xtra.co.nz> wrote:
Since the GSPS sampling ADCs all appear to use an input buffer with relatively
low value resistors between the differential inputs or connected to a midpoint
bias voltage, some kind of high impedance buffer is needed between the TAC
capacitor and the ADC input when using such ADCs. The highest
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