日本地球惑星科学連合2025年大会

講演情報

[E] ポスター発表

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-CG20] 宇宙・惑星探査の将来計画および関連する機器開発の展望

2025年5月29日(木) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:三谷 烈史(宇宙航空研究開発機構宇宙科学研究所)、桑原 正輝(立教大学)、横田 勝一郎(大阪大学・理学研究科)、長 勇一郎(東京大学理学系研究科地球惑星科学専攻)


17:15 〜 19:15

[PCG20-P12] Development of a Miniaturized Plasma Wave Receiver for CubeSat Using ASIC and Low-Power Processors

*頭師 孝拓1山本 康輔1小嶋 浩嗣2 (1.奈良工業高等専門学校、2.京都大学)

キーワード:プラズマ波動、プラズマ波動観測器、特定用途向け集積回路

The space environment is filled with tenuous plasma, and in-situ observations of plasma waves using plasma wave instruments are essential for studying its properties. In recent years, scientific observations using CubeSats have become increasingly popular. However, traditional plasma wave instruments are too large and resource-intensive to be installed on CubeSats. To address this issue, we have developed a compact plasma wave receiver using an application-specific integrated circuit (ASIC) and a low-power processor.
This receiver performs spectral observations in three frequency bands: DC–1 kHz, 1 kHz–10 kHz, and 10 kHz–100 kHz. Fast Fourier Transform (FFT) is applied to each observation result to obtain spectral data. By lowering the sampling frequency in the low-frequency band, low-power observations become feasible. In addition, ASIC technology is used to implement and miniaturise the analogue circuitry required for such observations.
In addition, FFT processing and the control of the A/D converter and ASIC are performed by a low-power processor, achieving both compactness and power efficiency. We have developed a breadboard model and confirmed that spectral observations in six channels can be achieved within a 9 cm × 9 cm size and a power consumption of less than 1 W.
In this presentation, we report on the details of the ASIC design, the breadboard model, and the performance evaluation of the developed receiver.