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GPU Based Software Correlators - Perspectives for VLBI2010Caused by historical separation and driven by the requirements of the PC gaming industry, Graphics Processing Units (GPUs) have evolved to massive parallel processing systems which entered the area of non-graphic related applications. Although a single processing core on the GPU is much slower and provides less functionality than its counterpart on the CPU, the huge number of these small processing entities outperforms the classical processors when the application can be parallelized. Thus, in recent years various radio astronomical projects have started to make use of this technology either to realize the correlator on this platform or to establish the post-processing pipeline with GPUs. Therefore, the feasibility of GPUs as a choice for a VLBI correlator is being investigated, including pros and cons of this technology. Additionally, a GPU based software correlator will be reviewed with respect to energy consumption/GFlop/sec and cost/GFlop/sec.
Document ID
20110011835
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Hobiger, Thomas
(National Inst. of Information and Communications Technology Japan)
Kimura, Moritaka
(National Inst. of Information and Communications Technology Japan)
Takefuji, Kazuhiro
(National Inst. of Information and Communications Technology Japan)
Oyama, Tomoaki
(National Astronomical Observatory Japan)
Koyama, Yasuhiro
(National Inst. of Information and Communications Technology Japan)
Kondo, Tetsuro
(National Inst. of Information and Communications Technology Japan)
Gotoh, Tadahiro
(National Inst. of Information and Communications Technology Japan)
Amagai, Jun
(National Inst. of Information and Communications Technology Japan)
Date Acquired
August 25, 2013
Publication Date
December 1, 2010
Publication Information
Publication: Proceedings of the Sixth General Meeting of the International VLBI Service for Geodesy and Astrometry
Subject Category
Geophysics
Funding Number(s)
CONTRACT_GRANT: KAKENHI 24241043
Distribution Limits
Public
Copyright
Public Use Permitted.
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