日本地球惑星科学連合2015年大会

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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-EM26] 宇宙プラズマ理論・シミュレーション

2015年5月24日(日) 11:00 〜 12:45 302 (3F)

コンビーナ:*梅田 隆行(名古屋大学 太陽地球環境研究所)、天野 孝伸(東京大学 地球惑星科学専攻)、成行 泰裕(富山大学人間発達科学部)、杉山 徹(独立行政法人海洋研究開発機構 地球情報基盤センター)、中村 匡(福井県立大学)、座長:中村 匡(福井県立大学)、小路 真史(名古屋大学太陽地球環境研究所)

11:30 〜 11:45

[PEM26-10] ヘリコンプラズマ生成の自己無撞着モデル

*諌山 翔伍1羽田 亨1 (1.九州大学総合理工学府)

Helicon plasma is a high-density and low-temperature plasma generated by the electromagnetic (Helicon) wave excited in the plasma. Then, helicon plasma is expected for various applications. On the other hand, there still remain a number of unsolved physical issues regarding how the plasma is generated using the helicon wave. The mechanism of helicon plasma production includes the wave propagation in the plasma (dispersion relation), collisional or non-collisional wave damping and plasma heating, and ionization/recombination of neutral particles which causes time evolution of the dispersion relation. In this study, we use the linear theory of helicon plasma, fluid simulation, and particle simulation to construct self-consist model including these physics.
In previous, we studied the helicon wave propagation and the process of plasma heating. And we showed the efficiency of mode conversion in bulk plasma depends strongly on the magnitudes of dissipations. However, there is a problem that has not been much studied: How do the helicon and TG modes influence the plasma density, electron temperature and their profiles? While the helicon mode is absorbed in the bulk plasma, the TG mode is mostly absorbed near the edge of the plasma. The local power deposition in a helicon plasma is mostly balanced by collision loss. This local power balance can give rise to an inhomogeneous electron temperature profile which is related to time evolution of density profile. In our study, we construct a self-consistent discharge model which includes wave excitation, classical electron heat transfer, and diffusion of charged particles.