日本地球惑星科学連合2023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-EM13] Dynamics of the Inner Magnetospheric System

2023年5月23日(火) 15:30 〜 16:45 101 (幕張メッセ国際会議場)

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、三好 由純(名古屋大学宇宙地球環境研究所)、Theodore E Sarris(Democritus University of Thrace)、Evan G Thomas(Dartmouth College)、座長:中村 紗都子(名古屋大学宇宙地球環境研究所)、松田 昇也(金沢大学)、山本 和弘(東京大学理学研究科)、三好 由純(名古屋大学宇宙地球環境研究所)、桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)

15:45 〜 16:10

[PEM13-10] Simultaneous macroscale and microscale wave–ion interaction in near-earth space plasmas

★Invited Papers

*Qiugang Zong1 (1.Peking University)

キーワード:wave–ion interaction, EMIC waves, ULF waves

Identifying how energy transfer proceeds from macroscales down to micro-scales in collisionless plasmas is at the forefront of astrophysics and spacephysics. It provides information on the evolution of involved plasma systemsand the generation of high-energy particles in the universe. Here we report twocross-scale energy-transfer events observed by NASA’s Magnetospheric Mul-tiscale spacecraft in Earth’s magnetosphere. In these events, hot ions simul-taneously undergo interactions with macroscale (~105 km) ultra-low-frequencywaves and microscale ( ~ 103 km) electromagnetic-ion-cyclotron (EMIC) waves.The cross-scale interactions cause energy to directly transfer from macro-scales to microscales, and finally dissipate at microscales via EMIC-wave-induced ion energization. The direct measurements of the energy transfer ratein the second event confirm the efficiency of this cross-scale transfer process,whose timescale is estimated to be roughly ten EMIC-wave periods about(1 min). Therefore, these observations experimentally demonstrate thatsimultaneous macroscale and microscale wave-ion interactions provide anefficient mechanism for cross-scale energy transfer and plasma energization inastrophysical and space plasmas