日本地球惑星科学連合2019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] 内部磁気圏

2019年5月29日(水) 09:00 〜 10:30 A04 (東京ベイ幕張ホール)

コンビーナ:海老原 祐輔(京都大学生存圏研究所)、Danny Summers(Memorial University of Newfoundland)、三好 由純(名古屋大学宇宙地球環境研究所)、齊藤 慎司(名古屋大学 大学院理学研究科)、座長:Shinji Saito(ISEE, Nagoya University)、海老原 祐輔(京都大学生存圏研究所)

10:00 〜 10:15

[PEM13-15] Generation Mechanism of Non-thermal Continuum Radiation

*大村 善治1Horky Miroslav1,2 (1.京都大学生存圏研究所、2.Department of Space Physics, Institute of Atmospheric Physics, Czech Academy of Sciences)

キーワード:波動粒子相互作用、非線形過程、プラズマポーズ

We study a possible nonlinear mechanism which could be responsible for generation of the non-thermal continuum radiation. We propose a theoretical model and perform numerical simulations using a 2-D electromagnetic particle code (KEMPO2) [1] to verify the mechanism [2]. In the simulation system, we have density gradient and ring beam electrons in the dense region as a source of electrostatic waves through ring-beam instability. These electrostatic waves cause non-gyrotropy of the ring velocity distribution which is necessary for generation of the harmonic waves. Velocity component Vy together with magnetic field Bz of the generated Z-mode waves creates Lorentz force in the x-direction (along the magnetic field). Hence, oscillating energetic electrons work as an anntenna emiting O-mode waves to the low density region. Electromagnetic O-mode waves are emitted at harmonics of the cyclotron frequency up to the maximal plasma frequency of the high density region, and they are observed as non-thermal continuum radiation in the low density region.

References:
[1] M. Horky, Y. Omura, and O. Santolik, Particle simulation of electromagnetic emissions from electrostatic instability driven by an electron ring beam on the density gradient, Physics of Plasmas 25, 042905, doi: 10.1063/1.5025912, 2018.
[2] M. Horky, and Y. Omura, Novel nonlinear mechanism of the generation of non-thermal continuum radiation, Physics of Plasmas 26, 2019.