> record the duration of each cycle directly
> 5) Double wide cycles are detectable but missed cycles are not.
What do you mean by a double wide cycle?
What do you mean by a missed cycle?
They seem like the same thing - if you miss one, the next one will be twice
as wide.
> Here are the
> On Apr 11, 2016, at 2:31 PM, Tom Van Baak wrote:
>
>
> 6) picPET output is directly readable by TimeLab via serial/USB.
This one line item twigged my interest.
Dedicating my 53220A to certain long running tasks that don’t require its full
capabilities irks me a
Hi
If you *do* want to go with the fancy ADC approach, there are MCU’s that are
built specifically for
power meter applications. They have cool stuff like 24 bit ADC’s and DSP
capability. Since the
target it high volume, the cost is sub $10 …
That’s still an IF by the way. It’s still not at
Hi Jay,
> Q1: Assuming the schmitt trigger in the picPET triggers at a consistent
> point in the waveform, the frequency at any given cycle is easy to
> calculate: 1.0 / (timestamp2 - timestamp1)...but, is there a better
> way? That method just feels... naive, for some reason.
Ah! if it
At 11:46 AM 4/11/2016, Tom Van Baak wrote:
Another way might be to use single-channel common view GPS. I've not
checked recently to see if 100 ps is possible over a 1 km baseline.
If so that would be a less expensive solution. Someone should dig
into the RINEX mode of the ublox 6T. It's on my
Its an intensity interferometer, there are no fringes.
The SNR is such thatseveral hours of integration are required.
If this method is at all feasible each telescope would likely need a hydrogen
maser or equivalent for such a technique to be useful.
More frequent phase comparisons allow
I have not followed this closely. Why not use the data itself? The
theoretical pattern for the telescope pair can be calculated. Even
though the signals are not i.i.d, from phototubes, the data can be slid
along and the delay pattern established and compared to the theoretical
pattern? Timing
On Mon, 11 Apr 2016 19:58:33 +0200
Attila Kinali wrote:
> The baseline is not the problem in this case, but the delay within
> the GPS receivers and the cables. To keep their variation below 1ns
> is already quite a challenge. The usual method for this is to have
> the whole
If using this system can the relative positions of the telescopes be
calculated also? You said the delay corresponding with 1mm is about 1ps,
so during processing we'd calculate the relative positions also using
delays between the various stations, if using common-view pulses at a
different
>> A more modern name for a synchronous motor is a permanent magnet stepper
>> motor. Any PM stepper, and a couple of microfarad capacitor becomes a
>> synchronous motor when connected to the power line.
I've seen a data sheet for a motor that's actually spec'd for both uses.
I don't know how
Good afternoon
I own a RTOS ( OS-9) and I have recently had some inquires about
support for 1588.
Does anyone have a suggestion for a grandmaster 1588 source ? In my
office I do not have a requirement for precise time at this time, but i
do have a couple of servers andserve3ral systems
On Mon, 11 Apr 2016 09:46:17 -0700
"Tom Van Baak" wrote:
> Another way might be to use single-channel common view GPS. I've not
> checked recently to see if 100 ps is possible over a 1 km baseline. If so
> that would be a less expensive solution. Someone should dig into the
Bruce,
So the time tag information will be processed off-line. In that case there's no
requirement for real-time clock synchronization, is there? Why not let each
station's clock free-run and provide periodic external pings amongst the
stations as a way to continuously calibrate all the
IMHO the transients and harmonic content, are more interesting than the
60Hz frequency!
But if the 60Hz frequency with superb rejection of transients is the only
goal:
The 60Hz line clock chips of the 1970's used the LV transformer secondary,
a single pole of RC low-pass filtering to get rid of
On Wed, 6 Apr 2016 18:21:43 -0700, you wrote:
>...
>
>Q1: Assuming the schmitt trigger in the picPET triggers at a consistent
>point in the waveform, the frequency at any given cycle is easy to
>calculate: 1.0 / (timestamp2 - timestamp1)...but, is there a better
>way? That method just
If all independent clocks is stable enough, then correlation between of
them could be re-considered after the data will be collected, I think.
On 2016-04-11 01:00, Bruce Griffiths wrote:
There is a proposal to use multiple light bucket style optical
telescopes to do Intensity stellar
On 4/11/16 1:40 AM, Björn wrote:
Hi Bruce,
For such short baselines single frequency GNSS should be able to keep fixed
integer solutions. Not sure how much money thas is going to save, since you
might need timing specific geodetic receivers to get external 10MHz input.
Did you consider
Hi
Is there a “common view” to a TV station or an FM radio station or a cell tower
or ….
Carrier phase works on terrestrial signals. If you have one with a stable
enough career and
a complex enough modulation to work out which cycle is which, it might be a
cheaper approach.
Bob
> On Apr
Hi Bruce,
For such short baselines single frequency GNSS should be able to keep fixed
integer solutions. Not sure how much money thas is going to save, since you
might need timing specific geodetic receivers to get external 10MHz input.
Did you consider implementing time transfer using time
bruce.griffi...@xtra.co.nz said:
> There is a proposal to use multiple light bucket style optical telescopes to
> do Intensity stellar Interferometry over short baselines (up to perhaps 1km
> or so) by using independent clocks to time tag photon arrivals.
> The relative positions of the
Dear Bruce
Posted too hastily ...
Since you don't care about absolute time, maybe using identical receivers
you might be able to get a few hundred ps synchronization using a PPP
solution, for example.
Attached is 6 months of data for two Javad receivers, with daily PPP
solutions. The antennas
As alternative to independent clocks and single photon tagging, we
considered to use TDCs: a possible solution would be radio cross links
between the telescopes that drive the start/stop signals of the TDCs,
then we'd tag only the lapses between photon detection from each
telescope. In this way a
Dear Bruce
I think it will be very difficult to achieve synchronization at the level
you want using GNSS signals. The BIPM would only claim 2 ns accuracy for
calibration of the delays in a GNSS receiver plus antenna. When you process
carrier phase data, you typically see jumps at the day boundary
Hi,
I would look at White Rabbit and fibre.
Now, you say you can't use fibre. If you have line of sight you may use
microwave (but not WLAN) or laser for a medium.
I would *really* consider pulling fiber after all. After that it is
relatively cheap to achieve the rest.
Cheers,
Magnus
On
There is a proposal to use multiple light bucket style optical telescopes to do
Intensity stellar Interferometry over short baselines (up to perhaps 1km or
so) by using independent clocks to time tag photon arrivals. store the time
tags and process the data off line. Depending on the time tag
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