SCARIe: Realtime software correlation Nico Kruithof, Damien Marchal - PowerPoint PPT Presentation

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SCARIe: Realtime software correlation Nico Kruithof, Damien Marchal

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... to generate very high-resolution astronomical images of cosmic radio sources ... from several telescopes is combined to make high resolution images of the sky. ... – PowerPoint PPT presentation

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Title: SCARIe: Realtime software correlation Nico Kruithof, Damien Marchal


1
SCARIeRealtime software correlationNico
Kruithof, Damien Marchal
2
Introduction
  • VLBI
  • Correlation
  • Software correlator
  • SCARIe
  • EXPReS / Fabric
  • Conclusion

3
VLBI
  • VLBI (very large baseline interferometry) is a
    technique, in which widely separated radio
    telescopes observe the same region of sky
    simultaneously, in order to generate very
    high-resolution astronomical images of cosmic
    radio sources
  • Telescopes are usually separated by thousands of
    kilometres
  • Data rates of 32mbps 1gbps per telescope
  • Processing is done at JIVE
  • For one experiment
  • Input 1-100 Terabytes
  • Output 1-100 Gbytes.

4
Larger dish higher resolution
  • Resolution ??? / b
  • Sensitivity ??b2
  • ? wavelength
  • b diameter telescope

Arecibo, Puerto Rico b 305 m
5
Westerbork/Very Large Array
6
VLBI
7
e-VLBI
Past
Today
Results
Today
Research
Today
8
Correlation
  • Combining signals from different telescopes
  • First aligning the signals by
  • Delaying signals
  • Stretch the signals
  • Correlation function
  • Measures the similarity of two signals
  • Integration to enhance the signal to noise ratio

9
Delay correction
  • Received signals from two stations
  • Delay correction
  • Doppler shift / Fringe stopping

10
Correlation function
  • A measure for the similarity of two (relatively
    shifted) functions.
  • Measures the area under the function obtained by
    multiplying one signal with the other shifted
    signal

11
Correlator Design
12
Outline of the nodes
  • Input node
  • Reads the data (at 32 mbps 1 gbps per station)?
  • Extracts the different frequency bands
  • Does the integer delay correction (integer
    number of samples)?
  • Sends two bits samples to the correlator nodes
  • Correlator node
  • Receives samples and converts them to floating
    point values
  • Performs a fractional delay correction
  • Corrects for the Doppler shift
  • Correlates the baselines
  • Output node
  • Sorts the data from the correlator nodes and
    writes it to file

13
DAS-3 / StarPlane
  • DAS-3 Third DAS supercomputer
  • 272 dual AMD Opteron compute nodes, spread out
    over five clusters, located at the four
    universities.
  • StarPlane is the Application Controlled Photonic
    Network connecting the DAS-3 sites

14
EXPReS / FABRIC
  • Collaboration with PSNC for data processing.

15
Success Story FTP Fringe Tests
  • FTP Fringe tests short slices of an experiment
    to test equipment.
  • Cluster running NICTcorrelator broke downin
    May 2007
  • SFXC was successfully used for the last three
    FTP Fringe Tests

16
Benchmarks on DAS-3
  • 40 of realtime (4 telescopes, 256mbps each) on
    30 quad-cores
  • bottleneck is CPU power
  • GPU's / FPGA'scould enhanceperformance

17
Conclusion
  • VLBI is a technique in astronomy in which data
    from several telescopes is combined to make high
    resolution images of the sky.
  • The output of the software correlator has been
    validated and produces similar results as the
    current hardware correlator
  • We are currently benchmarking and optimizing the
    correlator on the DAS-3 cluster.
  • Contact information
  • Nico Kruithof
  • JIVE
  • Kruithof_at_jive.nl
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