Presentation 2012-07-02
On a Wideband Fast Fourier Transform Using A Piecewise Linear Approximation : Applied to a Radio Telescope Spectrometer
Hiroki NAKAHARA, Hiroyuki NAKANISHI, Tsutomu SASAO,
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Abstract(in English) In a radio telescope, the spectrometer analyzes the radio frequency (RF) received from celestial objects at the frequency domain by performing the fast fourier transform (FFT). The FFT can be realized by the radix 2^k FFT (R2^k FFT). In Radio Astronomy, the number of points for the FFT is larger than that for the general purpose one. Thus, the twiddle factor memory is too large to implement. In this paper, we implement the twiddle factor by the piecewise linear approximation circuit consisting of a small memory, a multiplier, an adder, and a small logic circuit. We analyze the approximation error for the piecewise liner approximation circuits. We implemented the 2^<30> points FFT by the R2^k FFT with the piecewise linear approximation circuit. Compared with other FFT libraries, the R2^k FFT with the piecewise linear approximation using the memory is faster and smaller. Compared with the SETI spectrometer for 2^<27>-FFT in one second, the eight parallelized proposed ones for 2^<27>-FFT is 41.62 times faster, and that for 2^<30>-FFT is 5.20 times faster.
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Paper # CAS2012-8,VLD2012-18,SIP2012-40,MSS2012-8
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Conference Date 2012/6/25(1days)
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Language JPN
Title (in Japanese) (See Japanese page)
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Title (in English) On a Wideband Fast Fourier Transform Using A Piecewise Linear Approximation : Applied to a Radio Telescope Spectrometer
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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 Tsutomu SASAO
3rd Author's Affiliation Department of Creative Informatics, Kyushu Institute of Technology
Date 2012-07-02
Paper # CAS2012-8,VLD2012-18,SIP2012-40,MSS2012-8
Volume (vol) vol.112
Number (no) 116
Page pp.pp.-
#Pages 6
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