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arXiv 2105.01481physics.plasm-ph
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3D 圆柱形 BGK 模型:具有有限速度和极化漂移的电子相空间空洞

3D cylindrical BGK model of electron phase-space holes with finite velocity and polarization drift

Gaëtan Gauthier, Thomas Chust, Olivier Le Contel, Philippe Savoini

AI总结:

本文扩展了3D圆柱形BGK模型,纳入环境磁场强度和背景电子漂移速度的有限效应,以更真实地确定电子相空间空洞中捕获与通过粒子的分布及其存在条件。

摘要:

非线性电子动力学结构在空间和实验磁化等离子体中经常被观测到,称为电子相空间空洞(EHs)。EHs 的存在条件受环境磁场和可能产生它们的电子束参数的影响而变化。本文的目标是扩展由 Chen 等人(2004,2004)开发的具有圆柱几何的 3D Bernstein-Greene-Kruskal(BGK)模型,以同时包含有限效应:(i)环境磁场 $\vec{B}_0$ 的强度,通过修改泊松方程,加入从电子极化电流导出的项;(ii)背景等离子体电子相对于 EH 的漂移速度 $\vec{u}_e$,通过考虑边界条件的速度偏移麦克斯韦分布。这使我们能够更真实地确定形成 EHs 的捕获粒子和通过粒子的分布,以及它们存在的宽度-振幅关系。

英文摘要:

Nonlinear electron kinetic structures are regularly observed in space and experimental magnetized plasmas, called electron phase-space holes (EHs). The existence of EHs is conditioned and varies according to the ambient magnetic field and the parameters of the electron beam(s) that may generate them. The objective of this paper is to extend the 3D Bernstein-Greene-Kruskal (BGK) model with cylindrical geometry developed by Chen et al. (2004,2004) to include simultaneously finite effects due to (i) the strength of the ambient magnetic field $\vec{B}_0$, by modifying the Poisson equation with a term derived from the electron polarization current, and (ii) the drift velocity $\vec{u}_e$ of the background plasma electrons with respect to the EH, by considering velocity-shifted Maxwellian distributions for the boundary conditions. This allows us to more realistically determine the distributions of trapped and passing particles forming the EHs, as well as the width-amplitude relationships for their existence.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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