日本地球惑星科学連合2014年大会

講演情報

インターナショナルセッション(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-EM06_1AM1] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年5月1日(木) 09:00 〜 10:45 312 (3F)

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(名古屋大学太陽地球環境研究所)、橋口 浩之(京都大学生存圏研究所)、座長:小川 泰信(国立極地研究所)

09:00 〜 09:30

[PEM06-17] 電磁気圏・超高層大気の広域多点観測の将来の方向性

*塩川 和夫1大塚 雄一1 (1.名古屋大学太陽地球環境研究所)

キーワード:広域多点観測, 電離圏, 磁気圏, 超高層大気, 将来計画

Multi-point ground-based instruments are powerful tools to investigate global dynamics of the magnetosphere, ionosphere, and the upper atmosphere. Airglow imagers and multi-point GPS receivers provide two- and three-dimensional view of these regions. The ring-current and radiation-belt particles in the inner magnetosphere round the earth with a time scale from a few tens of minutes to a few hours. Interactions of these particles with Pc5 (times scale of ~minutes), Pc1 (~Hz) and VLF/ELF chorus (~kHz) causes acceleration and loss of these particles. Thus, longitudinal chain of ground-based stations to observe these various waves and auroras is essentially needed to understand the acceleration and loss of the plasma in the inner magnetosphere. The auroral energy input from the solar wind and magnetosphere to the high-latitude ionosphere is a major energy source of the dynamic variation of the upper atmosphere. Intense convective activity in the equatorial troposphere gives another energy source of the dynamic variation of the upper atmosphere. Thus, meridional chain stations are essentially needed to understand these dynamic variations and their global coupling. In this presentation we discuss possible future directions of these ground-based network observations to understand the global dynamics of the magnetosphere, ionosphere, and the upper atmosphere.