日本地球惑星科学連合2019年大会

講演情報

[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM11] Dynamics of Magnetosphere and Ionosphere

2019年5月30日(木) 15:30 〜 17:00 A04 (東京ベイ幕張ホール)

コンビーナ:中溝 葵(情報通信研究機構 電磁波研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、藤本 晶子(九州工業大学)、堀 智昭(名古屋大学宇宙地球環境研究所)、座長:北村 成寿(東京大学大学院理学系研究科)、佐藤 由佳(日本工業大学)、西野 真木(名古屋大学宇宙地球環境研究所)

16:30 〜 16:45

[PEM11-30] Development of a miniaturized X-ray imager for GEOspace X-ray imager (GEO-X)

*石川 久美1江副 祐一郎2沼澤 正樹2伊師 大貴2藤谷 麻衣子2大坪 亮太2福島 碧都2鈴木 光2湯浅 辰哉2中嶋 大3平賀 純子4三好 由純5笠原 慧6満田 和久1 (1.宇宙航空研究開発機構/宇宙科学研究所、2.首都大学東京、3.関東学院大学、4.関西学院大学、5.名古屋大学、6.東京大学)

キーワード:X線、磁気圏

A reduction in weight of instrument, especially optics, is a key technique for explorers or small satellite missions. GEO-X (GEOspace X-ray imager) is a Japanese small satellite mission for X-ray observations
of the dayside boundaries of the Earth’s magnetosphere. An instrument is composed of a X-ray telescope
and a radio hard semiconductor pixel detector. Conventional X-ray optics have a trend that optics with better angular resolution have larger ratio of the weight to effective area. Therefore, it is difficult to utilize them for the X-ray planetary mission which has a severe weight limit. Micro pore optics are being developed based on a concept of a miniature optics. An original micro pore optics based on Si micromachining technologies will be used. A CMOS image sensor and a DEPFET (DEPleted P-Channle FET) are candidates for the X-ray detector. These new type semiconductor detectors are radiation hard and have optical light resistance, which are crucial in GEO-X to observe magnetosheaths and cusps near the dayside of the Earth. We report a summary of the instrument design and development for GEO-X.