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Current Sheets in the Earth Magnetotail: Plasma and Magnetic Field Structure with Cluster Project Observations

机译:地球磁尾中的当前工作表:具有群集项目观测的等离子体和磁场结构

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摘要

Thin current sheets having kinetic scales are an important plasma structure, where the magnetic energy dissipation and charged particle acceleration are the most effective. It is believed that such current sheets are self-consistently formed by the specific nonadiabatic dynamics of charged particles and play a critical role in many space plasma and astrophysical objects. Current sheets in the near-Earth plasma environment, e.g., the magnetotail current sheet, are readily available for in-situ investigations. The dedicated multi-spacecraft Cluster mission have revealed basic properties of this current sheet, which are presented in this review: typical spatial profiles of magnetic field and current density, distributions of plasma temperature and density, role of heavy ions and electron currents, etc. Being important for the Earth magnetosphere physics, the new knowledge also could provide the basis for advancement in general plasma physics as well as in plasma astrophysics.
机译:具有动力学尺度的薄电流片是重要的等离子体结构,其中磁能耗散和带电粒子加速是最有效的。据信,这样的电流片是由带电粒子的特定非绝热动力学自洽形成的,并且在许多空间等离子体和天体物理学中起着至关重要的作用。近地等离子体环境中的当前薄片,例如磁尾电流薄片,很容易用于现场研究。专门的多空飞行器群任务揭示了该电流表的基本特性,在本综述中将进行介绍:磁场和电流密度的典型空间分布,等离子体温度和密度的分布,重离子和电子流的作用等。对于地球磁层物理学很重要,新知识还可以为一般等离子体物理学以及等离子体天体物理学的进步提供基础。

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