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_1AM2] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年5月1日(木) 11:00 〜 12:45 312 (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:McCrea Ian(RAL Space, STFC Rutherford Appleton Laboratory)

11:30 〜 11:45

[PEM06-24] 衛星-地上連携観測の重要性:ERGに向けて

*三好 由純1大山 伸一郎1齊藤 慎司1 (1.名古屋大学太陽地球環境研究所)

キーワード:衛星-地上連携観測, ERGプロジェクト

The ERG (Exploration of energization and Radiation in Geospace) is Japanese geospace exploration project. The project focuses on the geospace dynamics in the context of the cross-energy coupling via wave-particle interactions. The project consists of the satellite observation team, the ground-based network observation team, and integrated-data analysis/simulation team. The ERG satellite will be launched in FY2015. Comprehensive instruments for plasma/particles, and field/waves are installed in the ERG satellite to understand the cross-energy coupling system. In the ERG project, several ground-network teams join; magnetometer networks, radar networks, optical imager networks, etc. Moreover, the modeling/simulations play an important role for the quantitative understanding. In this presentation, we will discuss the importance of coordinated observations toward the ERG era. As an example, we show the cooperative observations between the geospace satellite Van Allen Probes an EISCAT to observe the pulsating aurora. The EISCAT measured the height profile of the electron density that can provide the energy of the precipitating electrons. The Van Allen Probes measured the plasma waves in the magnetosphere, which can be used to investigate the origin of the pulsating aurora. In fact, the GEMSIS-RBW simulation that used the observed plasma waves as an input reproduces characteristics of the observed precipitation. Such coordinated observations including the modeling provide a comprehensive view on cause and result.