地球磁场的结构,力量平衡和拓
C T Russell1, R J Strangeway2, C Zhao2
1Earth Planetary and Space Sciences, University of California, Los Angeles, CA 90095, USA. ctrussell@igpp.ucla.edu.
概括
地球的磁场,具有影响太阳风相互作用的子层. 复杂的电子流在这个边界上产生磁绳.
科学领域:
- 太空物理
- 血物理
- 地质学
背景情况:
- 磁断层是太阳风与地球磁层相互作用的关键边界层.
- 了解这种相互作用是理解太空天气及其对地球的影响的关键.
研究的目的:
- 为了研究磁停的等离子体和磁力.
- 分析磁断层中的子层结构和电子行为.
- 确定这些因素如何影响太阳风与地球磁层之间的相互作用.
主要方法:
- 使用来自磁层多尺度 (MMS) 任务的多航天器测量.
- 将等离子体和磁力与等离子体压力进行比较
- 检查电子分布函数.
主要成果:
- 磁断层呈现出与离子尺度相似的子层.
- 磁断区内的特定区域的特点是磁场强度低,曲率半径小,电流高.
- 复杂的电子流模式,包括平行和反平行运动,导致磁绳的形成.
结论:
- 磁断是一个具有复杂次层结构的动态边界.
- 电子扩散区域在能量转移过程中起着至关重要的作用.
- 磁绳的形成意味着磁断层的复杂拓,影响太阳风与磁层的合.
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