日本地球惑星科学連合2015年大会

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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] New frontier: Observations of the middle and upper atmospheres from ISS

2015年5月24日(日) 16:15 〜 18:00 A01 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*齊藤 昭則(京都大学大学院理学研究科地球物理学教室)、佐藤 光輝(北海道大学 大学院理学研究院)、大塚 雄一(名古屋大学太陽地球環境研究所)、牛尾 知雄(大阪大学大学院工学研究科情報通信工学部門)、鈴木 睦(宇宙航空研究開発機構宇宙科学研究本部)、座長:牛尾 知雄(大阪大学大学院工学研究科情報通信工学部門)、佐藤 光輝(北海道大学 大学院理学研究院)

16:50 〜 17:10

[PEM11-03] ISS曝露部搭載SEDA-APの観測結果と現状

*古賀 清一1松本 晴久1木本 雄吾1山田 理子1上野 遥1村木 綏2 (1.宇宙航空研究開発機構、2.名古屋大学)

キーワード:SEDA-AP, 宇宙環境

To support future space activities, it is very important to acquire space environmental data related to space radiation degradation of space parts and materials and spacecraft anomalies. Such data are useful for spacecraft design and manned space activity.
On several satellite of the Japan Aerospace Exploration Agency (JAXA) since the Engineering Test Satellite-V (ETS-V), Technical Data Acquisition Equipment (TEDA) and SEDA have been installed for obtaining the data described above.
SEDA-AP measures space environment data on ISS orbit. SEDA-AP comprises common bus equipment supporting launch, RMS handling, the power/communication interface with JEM-EF, an extendible mast that extends the neutron monitor sensor 1 m separate from the bus structure, and equipment that measures space environment data. It has eight environment monitoring sensors, which measure neutrons, heavy ions, plasma, high-energy electrons and protons, atomic oxygen, space debris and dusts.
SEDA-AP was lanced on July 16 in 2009, and attached to Exposed Facility (EF) of "Kibo" on July 25 using the robot arm of "Kibo". Initial checkout was started on August 4 and successfully ended on September 17. The regular operation period ended in 2011. Afterwards, later operation period of three years has started, and operation is being continued now.
We will report the observation results and the current status of SEDA-AP.