Presentation 2015-01-29
An AWF Digital Spectrometer for a Radio Telescope
Hiroki NAKAHARA, Hiroyuki NAKANISHI, Kazumasa IWAI,
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Abstract(in English) A radio telescope analyzes radio frequency (RF) received from celestial objects. It consists of an antenna, a receiver, and a spectrometer. The spectrometer converts the time domain into the frequency domain by a FFT operation. In the spectrometer, first, it multiples the window coefficient to the received signal. Second, it applies the FFT operation. Third, it converts to the absolute of a complex number. Finally, to reduce the noise, it accumulates obtained power spectrum. We call this a WFA spectrometer. Since an AD converter is faster than the FPGA, a parallel FFT computation is desired. However, since the amount of hardware for the FFT becomes bottleneck, the conventional WFA does not realized the high-performance analysis. This paper proposes an AWF spectrometer which replaces the order of operations. Since the AWF spectrometer reduces the parallelism of the FFT, it is smaller than the conventional WFA spectrometer. Also, the paper proposes a off-chip memory realization which is highly efficient use of the FPGA. Experimental results show that the proposed AWF spectrometer outperforms conventional spectrometers.
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Paper # VLD2014-122,CPSY2014-131,RECONF2014-55
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Conference Information
Committee RECONF
Conference Date 2015/1/22(1days)
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Registration To Reconfigurable Systems (RECONF)
Language JPN
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Title (in English) An AWF Digital Spectrometer for a Radio Telescope
Sub Title (in English)
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1st Author's Name Hiroki NAKAHARA
1st Author's Affiliation Faculty of Engineering, Kagoshima University()
2nd Author's Name Hiroyuki NAKANISHI
2nd Author's Affiliation Faculty of Science, Kagoshima University
3rd Author's Name Kazumasa IWAI
3rd Author's Affiliation Nobeyama Radio Observatory, NAOJ
Date 2015-01-29
Paper # VLD2014-122,CPSY2014-131,RECONF2014-55
Volume (vol) vol.114
Number (no) 428
Page pp.pp.-
#Pages 6
Date of Issue