日本地球惑星科学連合2022年大会

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[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-EM16] 宇宙プラズマ理論・シミュレーション

2022年5月22日(日) 09:00 〜 10:30 105 (幕張メッセ国際会議場)

コンビーナ:天野 孝伸(東京大学 地球惑星科学専攻)、コンビーナ: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)、コンビーナ:中村 匡(福井県立大学)、座長: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)

09:45 〜 10:00

[PEM16-04] Entropy cascading and structures of distribution function in drift wave turbulence

村上 広暉1、*渡邉 智彦1、前山 伸也1 (1.名古屋大学大学院理学研究科)

キーワード:宇宙プラズマ、乱流、分布関数

High temperature plasmas in space and laboratory are almost collisionless, and the distribution function can be far from the equilibrium state. Fluctuations on the distribution function driven by nonlinear plasma waves or turbulence suffer from filamentation or shearing on the phase space, and the characteristic scale lengths of the perturbed distribution function (delta-f) will be shorter and shorter through the turbulence cascade and the phase mixing until the fine structures are dissipated by collisions. This process plays a key role in the turbulence dissipation or heating in the high temperature plasmas.

In the present work, we consider a drift wave turbulence driven by the ion temperature gradient in a magnetized plasma with weak collisionality. Real and velocity space spectra of the distribution function obtained from the four-dimensional gyrokinetic simulations are investigated by means of the Fourier-Hermite expansions. The entropy variable defined by the L2 norm of delta-f cascades not only in the real wavenumber space, but also in the Hermite spectrum through the ballistic motion of particles. It is noteworthy that fluctuations with high parallel wavenumbers generated in the ExB turbulence induce the fine velocity space structures of delta-f, and that a nearly constant profile of the entropy transfer function is observed with the power-law of the Hermite spectrum of the entropy variable in agreement with a theoretical prediction.

* This work is supported by JSPS KAKENHI Grant Number JP16H04086.