日本地球惑星科学連合2018年大会

講演情報

[EE] 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-CG21] 宇宙・惑星探査の将来計画と関連する機器開発の展望

2018年5月21日(月) 09:00 〜 10:30 A01 (東京ベイ幕張ホール)

コンビーナ:亀田 真吾(立教大学理学部)、笠原 慧(東京大学)、尾崎 光紀(金沢大学理工研究域電子情報学系、共同)、吉岡 和夫(東京大学大学院新領域創成科学研究科)、座長:笠原 慧

09:45 〜 10:00

[PCG21-04] SS-520-3 Sounding Rocket Experiment Targeting the Ion Outflow over the Cusp Region: Status Update

*斎藤 義文1小川 泰信2小嶋 浩嗣3 (1.宇宙科学研究所、2.国立極地研究所、3.京都大学 生存圏研究所)

キーワード:観測ロケット、電離大気流出、カスプ

Although Japanese sounding rocket SS-520-3 was planned to be launched from Ny-Ålesund, Svalbard in Spitsbergen in December 2017, the launch was postponed at least by one year due to mal-function of the timer equipment that was found during the final stage of the integration test. The objectives of this sounding rocket are to understand the particle acceleration processes that cause the ion outflow by making in-situ observation of the wave-particle interaction over the dayside cusp region. The wave-particle interaction is going to be resolved by WPIA (Wave Particle Interaction Analyzer) that is newly developed for satellite missions. Since these wave-particle interactions are predicted to be effective above ~800km altitude, a two-stage sounding rocket SS-520 whose apex is higher than ~800km is necessary. The rocket range where SS-520 can be launched over dayside cusp is only SvalRak at Ny-Ålesund in Svalbard. This sounding rocket experiment is a part of the comprehensive observation campaign including ground-based radar (EISCAT Svalbard Radar) and optical observations. SS-520-3 sounding rocket experiment is also one of the projects participating to “A Grand Challenge Initiative (GCI) Cusp program” that is a large-scale international collaboration for targeting advancement in the common understanding of cusp region space physics through coordinated experimental and theoretical research using ground-based instruments, modeling, sounding rocket investigations, and satellite based instruments. All the science payloads of SS-520-3 was manufactured by the end of March 2016. Unit level environment test and calibration has been completed and they are ready for flight in winter 2018-2019.