Hi jishnu,

With red pitaya,  you have to down convert 20-80 to 0-60 baseband to use
the band fully. As such, it has a cutoff at 65MHz.

Thanks,
Mugundhan

On Mon, 10 Feb 2020, 13:30 Jishnu Nambissan T, <jis...@rri.res.in> wrote:

> Hi Mugundhan,
>
> With red pitaya, can you sample 20-80 MHz without downconversion ? And if
> analog down conversion is required, wouldn't that restrict the usable
> dynamic range (unless a high level mixer is used) ?
>
> Jishnu
>
> ------------------------------
> *From: *"Mugundhan vijayaraghavan" <v.vaishnav151...@gmail.com>
> *To: *"casper" <casper@lists.berkeley.edu>
> *Sent: *Thursday, February 6, 2020 1:06:09 AM
> *Subject: *Re: [casper] Solar Spectrometer Channeliser
>
> Hi Dan,
>
> We have done integration times from 20ms upto a second. There are bursts
> that last for hours, minutes and a few ms to seconds as well.
>
> We have not tried AGC on these bursts since we were aiming to study them
> only. In the 8 bit design, we had 3 bits for background and remaining 5 to
> accommodate bursts.
>
> The red pitaya can still be used if Colm can restrict the band to 20-80
> mhz, because the ionosphere starts cutting of anything below 20mhz
> mostly(depending on the location of course). Then this can be down
> converted to fit into 0-62.5 mhz base band of the red pitaya.
>
> Thanks,
>
> Mugundhan
>
>
>
>
> On Wed, 5 Feb 2020, 22:23 Dan Werthimer, <d...@ssl.berkeley.edu> wrote:
>
>>
>> hi mugundhan,
>>
>> what's the time scale for these bursts?
>> rise and fall times?
>> can you use a AGC circuit (automatic gain control),
>> eg: computer controlled attenuator
>> to turn down the power going into the ADC during the bursts,
>> so you could keep the levels going into the ADC relatively constant?
>> if the rise and fall times are longer than 1ms (the integration time of
>> the spectrometer),
>> then you could adjust the power level for each spectrum, and write down
>> where
>> you set the attenuator for that spectrum, so you could still know the
>> absolute power.
>>
>> if not, there are some 14 bit 200 Msps ADC boards,  and i think the new
>> RFSOC boards/chips have 14 bit ADC's,
>> but you'll have to write a casper yellow interface block for this ADC,
>> as we don't have a 14 bit 200 Msps ADC in the casper library.
>>
>> another possiblity is to multiplex your 80 MHz band, 40 MHz at a time
>> into a red pitaya board,
>> ping ponging back and forth between bands:  0 to 40 MHz for 1 ms, then 40
>> to 80 MHz for the next ms.
>>
>>
>> best wishes,
>>
>> dan
>>
>>
>>
>>
>> On Wed, Feb 5, 2020 at 8:33 AM Mugundhan vijayaraghavan <
>> v.vaishnav151...@gmail.com> wrote:
>>
>>> Hi Dan,
>>>
>>> Usually quiet sun doesn't show such abrupt changes, but bursts do
>>> (easily 40-50dB or more) for bright bursts. We have built 8 bit
>>> spectrometers in 40-80Mhz, but have found then when the burst is pretty
>>> strong, saturation effects starts kicking in.
>>>
>>>
>>> Thanks,
>>> Mugundhan
>>>
>>>
>>> On Wed, 5 Feb 2020, 21:52 Dan Werthimer, <d...@ssl.berkeley.edu> wrote:
>>>
>>>>
>>>> hi colm,
>>>> regarding dynamic range
>>>> ---------------------------------
>>>> for your solar spectrometer, do you need 14 bits of ADC dynamic range?
>>>> it's very unusual in radio astronomy to need that much instantaneous
>>>> dynamic range on the input.
>>>> does the sun vary on short time scales in the radio band by factor of
>>>> 1000 in voltage (1,000,000 in power) ?
>>>> or do you have very strong bursting RFI that is 1000 times the average
>>>> noise voltage (1M in power) in the whole band?
>>>>
>>>> as you probably know, you'll have lots more dynamic range in the output
>>>> power spectrum than the dynamic range of the ADC:
>>>> if you are building a 1024 channel spectrometer with 1 ms integration,
>>>> you'll get about 8 bits more bits of dynamic range above your ADC
>>>> dynamic range in frequency domain voltage,
>>>> which is 16 bits more of dynamic range above your ADC dynamic range in
>>>> power spectra.
>>>> so you'll have about 20 bits of spectral dynamic range if you use an 8
>>>> bit ADC,
>>>> (power spectrum dynamic range of about 1 million in 1 ms with an 8 bit
>>>> ADC, setting noise at 3 bit RMS).
>>>> and 24 bits of spectrral dynamic range for a 10 bit ADC, 28 bits for 12
>>>> bit ADC, and 32 bits for for 14 bit ADC).
>>>>
>>>> regarding boards for your spectrometer
>>>> ---------------------------------------------------
>>>>
>>>> 1) as adam pointed out, the red pitaya is cheap, but sample rate and
>>>> bandwidth don't quite get the specs you need.
>>>>
>>>> 2)  another possibility is to use a snap board, which costs more, but
>>>> can sample 3 inputs at 950 Msps,
>>>> or 6 inputs at 500 Msps, or 12 inputs at 250 Msps with 8 bit ADC's.
>>>> most people populate the snap board with 8 bit ADCs,
>>>> but a few people have populated it with 12 bit ADC's, although the
>>>> sample rate goes down by 8/12.
>>>>
>>>> 3) another possibility is to use a xilinx RFSOC board.  the first gen
>>>> has a bank of 12 bit ADC's  (8 inputs at 4 Gsps, or 16 inputs at 2 Gsps),
>>>> but i think the new generation has 14 bit ADC's ?    the RFSOC boards
>>>> cost more than snaps, but RFSOC was designed
>>>> in dublin, so you can probably get one from xilinx dublin....   the
>>>> ZCU111 board has not been fully casperized yet though.
>>>>
>>>> best wishes,
>>>>
>>>> dan
>>>>
>>>>
>>>>
>>>>
>>>>
>>>> Dan Werthimer
>>>> Marilyn and Watson Alberts Chair
>>>> Astronomy Dept and Space Sciences Lab
>>>> University of California, Berkeley
>>>>
>>>>
>>>> On Wed, Feb 5, 2020 at 5:06 AM Colm Bracken <colmbrac...@gmail.com>
>>>> wrote:
>>>>
>>>>> Hello CASPER people,
>>>>>
>>>>> We are looking to build a spectrometer with not too demanding
>>>>> requirements.
>>>>> Based on the specs below, would the Red Pitaya be up to the job do you
>>>>> think?
>>>>> Or, is there another, better suited (but similarly affordable)
>>>>> solution?
>>>>>
>>>>> Chanel widths: ~< 100 kHz
>>>>> Time sampling: ~< millisecond
>>>>> Polarisation: 2 channels
>>>>> Antenna freq range: 10-85 MHz (total bandwidth of 75 MHz)
>>>>> Digitisation: 14 bit
>>>>>
>>>>> Any advice on this would be great!
>>>>>
>>>>> Thanks in advance,
>>>>> Colm
>>>>> --
>>>>>
>>>>> *Dr Colm Bracken*
>>>>> Lecturer
>>>>> Maynooth University Experimental Physics
>>>>>
>>>>>
>>>>> Maynooth University, Maynooth, Co. Kildare, Ireland.
>>>>>
>>>>> T: +353 1 708 3641
>>>>> E: colm.brac...@mu.ie W: www.maynoothuniversity.ie
>>>>>
>>>>> Follow my work on https://nuim.academia.edu/ColmBracken
>>>>>
>>>>>
>>>>>
>>>>> And
>>>>>
>>>>>
>>>>> Research Associate
>>>>>
>>>>> Astronomy & Astrophysics Section
>>>>> School of Cosmic Physics
>>>>> Dublin Institute for Advanced Studies
>>>>> 31 Fitzwilliam Place
>>>>> Dublin 2, D02 XF86
>>>>>
>>>>>
>>>>>
>>>>> T: +353 1 440 6656 ext 352
>>>>> E: cbrac...@cp.dias.ie W: www.dias.ie/2017/06/22/dr-colm-bracken
>>>>>
>>>>> Follow my work on https://nuim.academia.edu/ColmBracken
>>>>>
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