日本地球惑星科学連合2021年大会

講演情報

[J] 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-EM15] 宇宙プラズマ理論・シミュレーション

2021年6月4日(金) 10:45 〜 12:15 Ch.06 (Zoom会場06)

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)、座長:諌山 翔伍(九州大学総合理工学研究院)、銭谷 誠司(神戸大学)

10:45 〜 11:00

[PEM15-07] Neutral depletion and the density limit of the helicon plasma

*諌山 翔伍1、篠原 俊二郎2、羽田 亨1、陳 仕宏3 (1.九州大学総合理工学研究院、2.東京農工大学、3.台湾国立中央大学)

キーワード:ヘリコンプラズマ、中性粒子枯渇、密度限界

Neutral depletion is a process in which neutral density decreases due to processes of ionization, neutral heating, and the drag (collision) by ions. In laboratory plasma sources, some experimental [1] and theoretical studies [2] suggest that the neutral depletion plays an important role in determining the plasma transport and the maximum plasma density. The neutral depletion caused by the collision with ions, is known to occur when the plasma pressure is comparable to the neutral gas pressure. If this is the case, the neutrals will naturally be cleared away from the region of high plasma pressure so that the net force balance is maintained. The plasma density consequently saturates to some density limit as the input power is increased. However, the relationship between the neutral depletion and the density limit is not well understood. Physical understanding of this saturation process is important to overcome the density limit of plasma sources.
In our study, we have constructed the self-consistent fluid model to investigate the time evolution of the helicon discharge with the neutral dynamics [3, 4]. In our simulation, the plasma density of ~1019 m-3 is generated, and the neutrals are depleted to ~1020 m-3 under a typical set of experimental parameters. When the input power is increased, the plasma density temporarily grows to ~1020 m-3, but the neutrals are seriously depleted to ~1018 m-3. In this situation, the electron temperature considerably increases since the power absorption (Joule heating) via Coulomb collision still occurs while the loss of energy by the ionization of neutrals becomes very small. As a result, the plasma density decreases to ~1019 m-3 due to the increase of outflow flux which is created by the strong pressure gradient. In this presentation, we discuss the effect of the neutral depletion and the density limit of the helicon plasma.

[1] S. Shinohara, D. Kuwahara, K. Yano and A. Fruchtman, Phys. Plasmas, 23 122108 (2016).
[2] A. Fruchtman, J. Phys. D: Appl. Phys. 50, 473002 (2017) (review paper).
[3] S. Isayama, S. Shinohara, T. Hada and S. H. Chen, Phys. Plasmas, 26 023517 (2019).
[4] S. Isayama, S. Shinohara, T. Hada and S. H. Chen, Phys. Plasmas, 26 053504 (2019).