日本地球惑星科学連合2024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

2024年5月26日(日) 10:45 〜 12:00 105 (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)、Sarris E Sarris(Democritus University of Thrace)、Thomas G Thomas(Dartmouth College)、座長:山本 和弘(東京大学理学研究科)、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)


11:30 〜 11:55

[PEM13-09] Electron microburst induced by chorus waves

★Invited Papers

*Lunjin Chen1 (1.University of Texas at Dallas)

キーワード:radiation belts, wave particle interaction, electron precipitation, chorus waves

During magnetospheric storms, radiation belt electrons are produced and then removed on varying timescales. An efficient loss process is microbursts, strong, transient precipitation of electrons into the lower atmosphere over a wide energy range, from tens of keV to sub-relativistic and relativistic energies (100s keV and above). However, the detailed generation mechanism of microbursts, especially over sub-relativistic and relativistic energies, remains unknown. Here, it is showed that these energetic electron microbursts may be caused by ducted whistler-mode lower-band chorus waves. Using combined observations of equatorial chorus waves from Van Allen Probes and electron precipitation from low-altitude ELFIN, the data-driven simulations demonstrate that the observed microbursts are the result of resonant interaction of electrons with ducted chorus waves rather than nonducted ones. Revealing the physical mechanism behind the microbursts advances our understanding of radiation belt dynamics and its impact on the lower atmosphere and space weather.