日本地球惑星科学連合2018年大会

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[EE] Eveningポスター発表

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-EM16] Dynamics of Earth's Inner Magnetosphere and Initial Results from Arase

2018年5月22日(火) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:Danny Summers(Memorial University of Newfoundland)、三好 由純(名古屋大学宇宙地球環境研究所)、細川 敬祐(電気通信大学大学院情報理工学研究科、共同)、海老原 祐輔(京都大学生存圏研究所)

[PEM16-P19] Relativistic effect on dispersionless injection associated with substorms

*Tzu-Fang Chang1,2Chio-Zong Cheng2Chih-Yu Chiang2Sunny Wing-Yee Tam2Yoshizumi Miyoshi1Tomoaki Hori1Takefumi Mitani3Takeshi Takashima3Ayako Matsuoka3Mariko Teramoto1 (1.Institute for Space-Earth Environmental Research, Nagoya University, Japan、2.Institute of Space and Plasma Sciences, National Cheng Kung University, Tainan, Taiwan、3.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan)

キーワード:particle injection, dispersionless, substorm, relativistic effect

Substorm dispersionless energetic particle injection to inner magnetosphere has been investigated on the basis of a classical electromagnetic pulse model [Zaharia et al., 2000]. In order to consider the effect of disturbed event on particle transport, relativistic effect is considered in our study to improve non-relativistic calculation results to get better agreement with satellite observation. We combine the ground-based observations and in situ magnetic field and particle data observed from satellites in the inner magnetosphere to investigate the transport of energetic particles associated with the substorms. In this study, the particle drift motion, the adiabatic invariant and particle magnetic moment differ from the previous non-relativistic particle motion model. We simulate the evolution of energetic particle injections during substorms and discuss the difference among non-relativistic, relativistic, and observational results.