抄録
A radio astronomy telescope with a wide field of view is an efficient tool for locating transient radio sources in space as supernova explosions. A promising method of designing this type of telescope is to apply Fourier transformation to the output signals from a phased array antenna. The implementation of a high-speed parallel FFT processor to an eight-element linear phased array antenna output is reported. Small size and low-power consumption are achieved by utilizing conventional digital video signal processing LSIs. In the pilot system, arithmetic operation up to a speed of 2.7 giga operations per second has been attained. The basic operation has been confirmed by solar observation.
| 本文言語 | English |
|---|---|
| ページ（範囲） | 109-117 |
| ページ数 | 9 |
| ジャーナル | Electronics and Communications in Japan, Part III: Fundamental Electronic Science (English translation of Denshi Tsushin Gakkai Ronbunshi) |
| 巻 | 72 |
| 号 | 5 |
| 出版ステータス | Published - 1989 5月 |
| 外部発表 | はい |
ASJC Scopus subject areas
- 電子工学および電気工学