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-EM15] 太陽地球系結合過程の研究基盤形成

2019年5月30日(木) 13:45 〜 15:15 A01 (東京ベイ幕張ホール)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:小川 泰信

13:45 〜 14:00

[PEM15-12] Mini/Micro Satellite Constelaltion for the study of LAI coupling

*小山 孝一郎1,2,3 (1.国立成功プラズマ宇宙科学研究所  台湾、2.九州大学国際宇宙天気・教育センター、3.(株)アジア宇宙環境研究コンソーシアム)

キーワード:EAI結合、衛星観測、国際協力

Recent Studies show that ionosphere influenced by Thunder cloud, Typhoon, Sudden Stratosphere warming, Earth quake, and so on. Possible atmosphere perturbation to generate Radio wave scintillation is still not confirmed by observation in spite of the long history of radio scintillation research. Since 1970’s, no break through is found in ionosphere physics. The reason is the lack of information of the atmosphere below which is needed simultaneously with ionopshere information. We propose here the satellite constellation of /Pico /mini satellites combined with one /two small satellite (200-500 Kg). Pico/mini satellite should be constellation to measure basic ionosphere parameter. These are electron density, temperature, ion temperature, ion mass, electric field, and neutral wind at ionosphere height. Information on the atmospheric wind down to ground surface below 120 km should be simultaneously measured. This means that we need photometric instruments such as TIDI and SABAR accommodated in TIMED satellite or instruments to measure electromagnetic waves radiated by neutral particles. These observations can be done through international collaboration.

References
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