地球等离子体环境中的太阳风-磁层-电离层相互作用

S. Cowley, J. Davies, A. Grocott, H. Khan, M. Lester, K. McWilliams, S. Milan, G. Provan, P. Sandholt, J. Wild, T. Yeoman
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引用次数: 30

摘要

地球磁层-电离层耦合系统的性质主要由其与太阳风等离子体的相互作用决定,并由磁层顶界面的磁重联介导。因此,地球的磁层动力学主要取决于行星际磁场的同步方向(IMF)。我们通过一些最近的案例研究的结果来说明当前对该系统的理解,并强调了剩余的问题。重点讨论了南向国际货币基金组织间歇期的通量转移事件和亚暴,以及北向国际货币基金组织间歇期的磁层顶和尾过程。我们强调从空间和地面进行的现场和遥感观测相结合的巨大诊断能力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Solar–wind–magnetosphere–ionosphere interactions in the Earth's plasma environment
The properties of the Earth's coupled magnetosphere–ionosphere system are dominated by its interaction with the solar–wind plasma, mediated by magnetic reconnection at the magnetopause interface. As a consequence, Earth's magnetospheric dynamics depend primarily on the concurrent orientation of the interplanetary magnetic field (IMF). We illustrate current understanding of the system through the results of a number of recent case studies and highlight the remaining issues. The discussion centres on flux–transfer events and substorms during intervals of southward IMF and magnetopause and tail processes during intervals of northward IMF. We emphasize the great diagnostic power of combined in situ and remote–sensing observations from space and on the ground.
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