日本地球惑星科学連合2021年大会

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[J] 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-EM15] 宇宙プラズマ理論・シミュレーション

2021年6月4日(金) 17:15 〜 18:30 Ch.05

コンビーナ:天野 孝伸(東京大学 地球惑星科学専攻)、三宅 洋平(神戸大学計算科学教育センター)、梅田 隆行(名古屋大学 宇宙地球環境研究所)、中村 匡(福井県立大学)

17:15 〜 18:30

[PEM15-P04] PIC simulation on instabilities driven by ring-like energetic-ions: energetic-ion injection model.

*小谷 翼1、樋田 美栄子2、森高 外征雄2、田口 聡1 (1.京都大学理学研究科地球惑星科学専攻地球物理学教室、2.核融合科学研究所)

キーワード:粒子シミュレーション、高速イオン注入、リング状速度分布

It is well-known that instabilities can occur when energetic ions have a ring-like velocity distribution perpendicular to the magnetic field. When a ring speed is larger than the Alfvén speed, electromagnetic fast magnetosonic waves are excited, which are often observed in the Earth’s magnetosphere and are considered to accelerate ions and electrons. On the other hand, when a ring speed is much smaller than the Alfvén speed, electrostatic lower hybrid waves with the resonance frequency, ω LH ∼ √ΩiΩe, are excited, which are often observed in fusion plasma.
Many previous studies for these instabilities solve initial value problems; the density of energetic ions is constant throughout their simulations. They focus on the excitation of the waves and the relaxation of a velocity distribution. However, it is not enough to investigate the developments of the instabilities for a long period because, in the real situations, the injection or loss of energetic ions should occur and leads to the reshaping of the velocity distribution, which can cause further instabilities.
In this meeting, using a one-dimensional, electromagnetic, particle-in-cell code, we study the long-time evolution of the instabilities driven by ring-like energetic ions by an energetic-ion injection model. In this model, the density of energetic ions is zero at first and then increases with time. We also compare these simulation results with the initial value problem and the linear theory.