Mechanisms of auroral particle acceleration

G. Haerendel
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引用次数: 4

Abstract

The paper deals with the conditions enabling auroral acceleration, the coupling of the various processes involved, and the feedback mechanisms on the source of energy and mass. Particular emphasis is given to the energy flow, for which four different paths are identified, whose efficiencies and time-scales are being compared. Furthermore, the necessary ingredients of auroral arc formation are discussed, among which current filamentation and dynamical feedback on the source plasma are still largely unknown elements. The paper closes with a conjecture about the origin of auroral folds and curls, which is attributed to the evacuation process of the topside ionosphere, the ensuing modification of the electric potential distribution, generation of small-scale shear flows and their instability.

极光粒子加速的机制
本文讨论了使极光加速的条件,所涉及的各种过程的耦合,以及能量和质量来源的反馈机制。特别强调的是能量流动,其中确定了四种不同的途径,并对其效率和时间尺度进行了比较。此外,还讨论了极光弧形成的必要因素,其中电流丝化和源等离子体的动态反馈在很大程度上仍然是未知的因素。本文最后提出了一个关于极光褶皱和极光卷曲起源的猜想,认为这是由于上层电离层的疏散过程、电势分布的改变、小尺度剪切流的产生及其不稳定性造成的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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