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Coulomb collisional processes in space plasmas; relaxation of suprathermal particle distributions

机译:空间等离子体中的库仑碰撞过程;超热粒子分布的弛豫

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Nonequilibrium distributions of space plasmas are often characterized by extended high-energy tails. This paper provides a detailed analysis of the relaxation of such isotropic nonequilibrium plasmas. We consider an energetic charged species dilutely dispersed in a fully ionized plasma, which acts as a heat bath at equilibrium. The minor constituent is referred to as a "test particle" and collisions between test particles are not included. We study the approach to equilibrium with a finite difference method of solution of the Fokker -Planck equation appropriate for collisions between charged particles. The solution of the Fokker-Planck equation is also presented formally as an expansion in the eigenfunctions of the Fokker-Planck operator. The main objective of the paper is the calculation of the energy-dependent relaxation times of the distribution function. A strong energy dependence for these relaxation times is anticipated since, for Coulomb collisions, the Rutherford cross-section varies with relative speed g as g~(-4). Analogous results for neutral species are presented for comparison in the following paper.
机译:空间等离子体的非平衡分布通常以扩展的高能尾巴为特征。本文提供了此类各向同性非平衡等离子体弛豫的详细分析。我们认为高能带电物质稀疏地分散在完全电离的等离子体中,该等离子体在平衡时充当热浴。微量成分被称为“测试颗粒”,并且不包括测试颗粒之间的碰撞。我们使用适用于带电粒子之间碰撞的Fokker-Planck方程的有限差分法研究平衡方法。福克-普朗克方程的解也作为福克-普朗克算子本征函数的展开形式形式表示。本文的主要目的是计算分布函数的能量相关弛豫时间。对于这些弛豫时间,可以预见到强烈的能量依赖性,因为对于库仑碰撞,卢瑟福横截面随相对速度g随g〜(-4)的变化而变化。在下文中介绍了中性物种的类似结果,以进行比较。

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