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Solving the corner-turning problem for large interferometers

delete2010-10-12
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OA
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A
Andrew Lutomirski *
M
Max Tegmark
N
N. Sánchez
L
Leo C. Stein
W
W. L. Urry
M
Matías Zaldarriaga
DOI:10.1111/j.1365-2966.2010.17587.xdelete
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Abstract

Abstract

En 中文
The so-called corner-turning problem is a major bottleneck for radio telescopes with large numbers of antennas. The problem is essentially that of rapidly transposing a matrix that is too large to store on one single device; in radio interferometry, it occurs because data from each antenna need to be routed to an array of processors each of which will handle a limited portion of the data (say, a frequency range) but requires input from each antenna. We present a low-cost solution allowing the correlator to transpose its data in real time, without contending for bandwidth, via a butterfly network requiring neither additional RAM memory nor expensive general-purpose switching hardware. We discuss possible implementations of this using FPGA, CMOS, analog logic and optical technology, and conclude that the corner-turner cost can be small even for upcoming massive radio arrays.
Keywords:
methods: data analysis
techniques: interferometric
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Journal

Monthly Notices of the Royal Astronomical Society cover
Monthly Notices of the Royal Astronomical Society
IF:
4.8
Papers:
7.0W
Citations:
25.0W

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U
University of California Berkeley
Scholars:
3.5W
Papers: 2.8W
Citations: 11.3W
University of California System cover
University of California System
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Papers: 33.7W
Citations: 6.6K