Fpga spectrometer commissioning spectrometer description



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FPGA SPECTROMETER COMMISSIONING

  • Spectrometer description

  • How it will be used

  • Where we are at.

  • What needs to be done

  • More info:http://www.naic.edu/~phil/hardware/pdev


Description.. what we bought

  • 20 spectrometer boxes purchased from jeff mock … (jeff who??)

  • 1 box can process 1 beam of alfa.

  • 14 boxes allows for 2 simultaneous alfa experiments.

  • 2 boxes for aeronomy, planetary radar

  • 16 fileservers (each with 4 Tbytes of disc).

  • IF mixer chassis IF to base band (I,Q) (dana)



Description.. 1 box

  • 2 paths each handling 170 MHz Bandwidth

  • A/D.. 12 bit 170 Mhz I Q samplers

  • Digital mixer.

  • Digital low pass filter (decimation 2..1024)

  • Optional time domain data: 4,8,16 bits

  • Polyphase filter bank..16 to 8192 channels.

  • I, polA/B, full stokes power computation.

  • Sum spectra. Output 32,16,8 bit spectral data.

  • Box output I/O rate: 80 Mbytes/sec.



How it will be used

  • Alfa: covers 1225-1525 MHz x 7 beams

  • Galfacts: galaxy full stokes

    • 65Mb/sec * 7 = 450 Mb/sec.
  • Palfa search: Upgrade 100 to 300 MHz BW.

    • 32Mb/sec*7= 225 Mb/sec.
  • Aeronomy: IF sampling, time domain data (Tamara)

    • 32,20,10,.. bandwidths. 32 MHz Bw gets plasma line in 1 band
    • Sampling synced to transmitter pulses and echo return.
  • Planetary Radar: IF sampling, time domain data. (Tamara)

    • 40,20,10,.. Bandwidths with 2,4,8,16 bit samples.
    • Fir filters for CW, sync filters for ranging.
    • Digital doppler correction by interpolating, dropping samples.
  • Single Pixel observations:

    • Use 7*300 MHz bandwidth to cover up tp 2 GHz bw.


Where we are at.

  • Alfa:

    • Hardware
      • 14 spectrometer boxes with 7 mixer chassis installed.
      • 14 file servers installed, 7 in use.
    • Software:
      • Acquires data, writes to disc in pdev or fits format.
  • Aeron:

    • Test data taken in 32Mhz bw Mode
  • Planetary radar

    • 20 MHz bw data taken on saturns rings.


What needs to be done.

  • Hardware/FPGA programming:

    • Resolve radar rfi saturation in PFB butterfly stages. If this is not solved, the lower 170 MHz will be unusable.
    • Take a closer look at birdies generated internally to the boxes.
    • Debug sync filters for planetary radar (Tamara)
    • Debug digital doppler (Tamara).
    • Single pixel.. Need to widen the downstairs IF/LO to handle 2 GHz bw.


What needs to be done (software)

  • Integrate running of spectrometer with GUI.

    • This will take the most time.
  • Fill in all fits header keyword data.

  • Speed up startup configuration of device.

  • Test winking cal, blanking.

  • Automate optimum level setting and configuration for all possible configs.

  • Pulsar users want psrfits format. This is different from the fits files we are generating.

  • Analysis software. Continue developing IDL routines to verify the device operation.

  • Work on system/program documentation (see web site).



When ….

  • Shooting for may 2008 for galfacts alfa observing. This will also enable any of the other alfa spectral line surveys to use the device.

  • Pulsar fits file format will come after galfacts (since palfa is already taking data).

  • Planetary radar/aeronomy needs FPGA programming and Tamara Hall is leaving.

    • Till she leaves, radar/aeronomy work gets priority.
  • 2 GHz single pixel still in the design stages.



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