相对论强平均磁场中的霍尔磁流体动力学

IF 2.1 3区 物理与天体物理 Q2 PHYSICS, FLUIDS & PLASMAS
Y. Kawazura
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引用次数: 0

摘要

本文提出了一个磁流体动力学模型,描述了在相对论性强平均磁场存在的情况下,波长与离子惯性长度相当的小振幅波动。推导出的方程组与非相对论霍尔还原磁流体动力学(Schekochihin 等,J. Plasma Phys.,第 85 卷,2019 年,905850303)几乎完全相同,区别仅在于考虑了相对论修正的几个常数。这意味着非相对论霍尔机制中固有的动力学阿尔芬湍流和离子回旋湍流的所有特性即使在磁主导机制中也保持不变。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Hall magnetohydrodynamics in a relativistically strong mean magnetic field

This paper presents a magnetohydrodynamic model that describes the small-amplitude fluctuations with wavelengths comparable to ion inertial length in the presence of a relativistically strong mean magnetic field. The set of derived equations is virtually identical to the non-relativistic Hall reduced magnetohydrodynamics (Schekochihin et al., J. Plasma Phys., vol. 85, 2019, 905850303), differing only by a few constants that take into account the relativistic corrections. This means that all the properties of kinetic Alfvén turbulence and ion cyclotron turbulence inherent in the non-relativistic Hall regime persist unchanged even in a magnetically dominated regime.

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来源期刊
Journal of Plasma Physics
Journal of Plasma Physics 物理-物理:流体与等离子体
CiteScore
3.50
自引率
16.00%
发文量
106
审稿时长
6-12 weeks
期刊介绍: JPP aspires to be the intellectual home of those who think of plasma physics as a fundamental discipline. The journal focuses on publishing research on laboratory plasmas (including magnetically confined and inertial fusion plasmas), space physics and plasma astrophysics that takes advantage of the rapid ongoing progress in instrumentation and computing to advance fundamental understanding of multiscale plasma physics. The Journal welcomes submissions of analytical, numerical, observational and experimental work: both original research and tutorial- or review-style papers, as well as proposals for its Lecture Notes series.
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