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-CG 宇宙惑星科学複合領域・一般

[P-CG31] 宇宙科学・探査の将来計画と関連する機器・技術の現状と展望

2015年5月28日(木) 14:15 〜 16:00 202 (2F)

コンビーナ:*平原 聖文(名古屋大学太陽地球環境研究所)、小嶋 浩嗣(京都大学生存圏研究所)、高橋 幸弘(北海道大学・大学院理学院・宇宙理学専攻)、鈴木 睦(宇宙航空研究開発機構宇宙科学研究本部)、座長:高橋 幸弘(北海道大学・大学院理学院・宇宙理学専攻)、鈴木 睦(宇宙航空研究開発機構宇宙科学研究本部)

14:15 〜 14:30

[PCG31-10] 宇宙空間からの電離圏・熱圏・中間圏の観測

*齊藤 昭則1 (1.京都大学)

キーワード:電離圏, 中間圏, 熱圏, プラズマ圏, 衛星撮像観測

A micro satellite for imaging of the ionosphere-thermosphere-mesosphere-plasmasphere is being designed in aiming to be launched in the low-earth orbit. This new observation is expected to clarify the upper atmospheric processes that have been partially found by the ground-based techniques and the ISS-IMAP missions from the international space station. The new satellite can observe the Earth's upper atmosphere with a wide field of view that cannot be observed from ground-based instruments. Main targets of the observation are: (1) generation, evolution and decay mechanisms of mesoscale structures in the mesosphere and the ionosphere, (2) longitudinal and regional characteristics of the atmospheric gravity waves and tidal waves in the mesosphere, (3) disturbances of the thermosphere associated with the geomagnetic storms, (4) electron density distribution in the plasmasphere and its effect on GPS radio waves, (5) the ionospheric effect on the radio waves and development of the correction technique. Coordinated study among the satellite, ground-based instruments and numerical models is expected to expand our knowledge of the mesosphere, thermosphere, ionosphere and plasmasphere from the equatorial to the polar regions. The coupling mechanisms among high-, mid-, and low latitude regions, and between lower and upper atmosphere will be elucidated by this space-borne observation.