日本地球惑星科学連合2014年大会

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インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-CG 宇宙惑星科学複合領域・一般

[P-CG11_28AM2] Instrumentation for space science

2014年4月28日(月) 11:00 〜 12:45 421 (4F)

コンビーナ:*松岡 彩子(宇宙航空研究開発機構 宇宙科学研究所 太陽系科学研究系)、吉川 一朗(東京大学)、座長:松岡 彩子(宇宙航空研究開発機構 宇宙科学研究所 太陽系科学研究系)、吉川 一朗(東京大学)

11:00 〜 11:15

[PCG11-03] ASICを用いた小型プラズマ波動受信器の開発

*頭師 孝拓1萩行 憲輔1大西 啓介1小嶋 浩嗣1山川 宏1 (1.京都大学 生存圏研究所)

Plasma waves are an important physical phenomenon for understanding the electromagnetic environments in space. The plasma wave receiver is roughly divided into two types: a waveform receiver and a spectrum analyzer. Spectrum analyzer provides the frequency spectrums with low noises and high frequency resolution. On the other hand, waveform receiver provides the waveform. Though the waveform has more noise than the spectrum provided by the spectrum analyzer, only the waveform has phase information of a plasma wave. Thus it play a complementary role. However, these plasma wave receivers occupy a large amount of space because of its analog circuits, so a late scientific satellite has only a kind of plasma wave receiver. We have developed miniaturized waveform capture (WFC), a kind of waveform receiver, and sweep frequency analyzer (SFA), a kind of spectrum analyzer, using ASIC (Application Specific Integrated Circuit). We realized 6ch WFC in a chip of 5 mm x 5 mm. We execute experiment expose this chip to radiation. We find that though radiation influence WFC component, especially switched capacitor filter, our WFC fit for the space radiation environment. The SFA has fine frequency resolution, but its time resolution is poor. We propose a new kind of SFA combined with FFT. It has an improved time resolution without losing time resolution. We have developed analog circuits in the new SFA using ASIC technology. Furthermore, we propose the multipoint plasma wave observation system that consisted of some sensor probes using these miniaturized plasma wave receiver. We plan the sounding rocket experiment for performance test of this sensor probe.