上行和下行电流区的极光粒子加速度特征

G.T. Marklund, T. Karlsson
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引用次数: 13

摘要

为了理解极光粒子加速,有必要考虑整个极光电流回路,从外磁层的发电机到极光电离层,在向上和向下的电流区,通过场向电位降相互解耦。本文的重点是这种电位下降的特征,负责产生极光的加速电子和离子和电子的向上加速。首先,主要根据维京号在加速区内及以上的观测结果,讨论了上行电流区的会聚电场结构的一些特征。其中包括与极光弧相关的高空势和电离层势之间的关系;从现场卫星测量场和粒子估计场向势降的方法;低频电场波动对极光粒子加速和加热的作用。然后简要回顾了Freja最近关于下电流区特性的研究结果,例如引起电离层电子向上加速和垂直加热的强发散电场结构。人们提出了不同的理论模型来解释这些现象。显然,极光场线上的等离子体密度和电离层密度对上下电流区电势结构形成的地点和时间起着根本的作用。对于供给极光电流的电流发生器来说,粒子加速是维持电流通过低等离子体密度区域的必要条件。因此,场向电位的高度分布将强烈依赖于当地的环境等离子体条件,从而随当地的时间、季节和磁活动水平而变化。这些特征可以通过结合不同航天器(如Viking、Polar、Freja、FAST和Astrid-2)在不同高度对场向电位分布的测量来详细研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Characteristics of the auroral particle acceleration in the upward and downward current regions

To understand auroral particle acceleration it is necessary to consider the entire auroral current circuit, from the generator in the outer magnetosphere to the auroral ionosphere, decoupled from each other by field-aligned potential drops in both the upward and downward current regions. This paper focusses on the characteristics of such potential drops responsible for the accelerated electrons that produce the aurora and for the upward acceleration of ions and electrons. First, some features of the converging electric field structures in the upward current region are discussed based predominantly on results from Viking observations within and above the acceleration region. These include the relationship between the high-altitude potential and the ionospheric potential associated with auroral arcs; ways to estimate the field-aligned potential drop from in situ satellite measurements of fields and particles; the role of low-frequency electric field fluctuations for acceleration and heating of auroral particles. A brief review is then given of recent Freja results on characteristics of the downward current region, such as the intense diverging electric field structures that give rise to upward acceleration of ionospheric electrons and perpendicular ion heating. Different theoretical models have been proposed to explain these phenomena. It is clear that the plasma density on auroral field lines and the ionospheric density play a fundamental role for where and when potential structures are formed in the upward and downward current region. For a current generator feeding the auroral currents, particle acceleration is necessary to maintain the current through regions of low plasma density. The altitude distribution of the field-aligned potential will thus depend strongly on the local ambient plasma conditions, and thus vary with local time, season and magnetic activity level. These characteristics could be investigated in detail by combining measurements from various spacecraft (such as Viking, Polar, Freja, FAST, and Astrid-2) at different altitudes with respect to the the field-aligned potential distribution.

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