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-P07] Ion optics of the ±45° angular scanning deflectors for space plasma instruments

北村 悠稀1、*横田 勝一郎1笠原 慧2寺田 健太郎1 (1.大阪大学大学院・理学研究科、2.東京大学大学院・理学系研究科)

キーワード:宇宙プラズマ計測、静電分析器、視野掃引

For three-dimensional energy analysis of low-energy ions and electrons in space, the top-hat electrostatic method has usually been applied because of its large geometric factor and uniform angular response while requiring relatively few resources. Typical top-hat spectrometers provide a wide field of view (FOV) (360° x ~5°), appropriate energy resolution (~10%), and an energy range from a few electronvolts to a few ten kilo-electronvolts, a reasonable geometric factor (~10-4 cm2 sr eV/eV), and good sunlight rejection by means of small weight, size and power. Complete spherical FOV (4pi steradian) is enabled by the spin motion of the spacecraft. In almost all optical experiments, however, three-axis stabilized satellites are preferred because most experiments require observation in the direction of the planetary atmosphere or surface. Three-axis stabilized satellites intrinsically restrict the FOV of top-hat analyzers to a plane. Electrostatic angular scanning derived from the differential ion flux probe is an effective way to extend the FOV while placing only small demands on resources. Furthermore, angular scanning deflectors and top-hat electrostatic analyzers form an excellent combination to provide hemispherical coverage of the FOV even on three-axis stabilized planetary explorers such as KAGUYA and Martian Moons eXploration (MMX). Therefore, we studied ion optics of the angular scanning deflectors of spaceborne low-energy particle experiments. Numerical models were used to comprehensively examine various geometries of the deflectors and evaluate the performance of each one in terms of deflection characteristics (±45°), energy-angle response, and sensitivity. An analytical model was developed to evaluate the performance of the deflector with respect to the geometry in all parameters. We confirmed that the outputs of the analytical model agree with that of the numerical model with an accuracy of approximately 10%. Here, we present the details of the ion optics for the deflector of the low-energy particle instruments, the analytical model we developed, and its evaluation.