• Title of article

    Enabling a high throughput real time data pipeline for a large radio telescope array with GPUs Original Research Article

  • Author/Authors

    R.G. Edgar، نويسنده , , M.A. Clark، نويسنده , , Ryan K. Dale، نويسنده , , D.A Mitchell، نويسنده , , S.M. Ord، نويسنده , , R.B. Wayth، نويسنده , , H. Pfister، نويسنده , , L.J. Greenhill، نويسنده ,

  • Issue Information
    ماهنامه با شماره پیاپی سال 2010
  • Pages
    8
  • From page
    1707
  • To page
    1714
  • Abstract
    The Murchison Widefield Array (MWA) is a next-generation radio telescope currently under construction in the remote Western Australia Outback. Raw data will be generated continuously at 5 GiB s−1, grouped into 8 s cadences. This high throughput motivates the development of on-site, real time processing and reduction in preference to archiving, transport and off-line processing. Each batch of 8 s data must be completely reduced before the next batch arrives. Maintaining real time operation will require a sustained performance of around 2.5 TFLOP s−1 (including convolutions, FFTs, interpolations and matrix multiplications). We describe a scalable heterogeneous computing pipeline implementation, exploiting both the high computing density and FLOP-per-Watt ratio of modern GPUs. The architecture is highly parallel within and across nodes, with all major processing elements performed by GPUs. Necessary scatter-gather operations along the pipeline are loosely synchronized between the nodes hosting the GPUs. The MWA will be a frontier scientific instrument and a pathfinder for planned peta- and exa-scale facilities.
  • Keywords
    Radio telescopes and instrumentation , Mathematical procedures and computer techniques , Heterodyne receivers , Computer science and technology
  • Journal title
    Computer Physics Communications
  • Serial Year
    2010
  • Journal title
    Computer Physics Communications
  • Record number

    1138029