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发表刊物：Journal of Geophysical Research: Space Physics
关键字：Solar wind dynamic pressure, Compression auroras, Substorm auroras, Energetic electron injections
摘要：After the passage of an interplanetary (IP) shock at 06:13 UT on 24 August 2005, the enhancement (>6 nPa) of solar wind dynamic pressure and the southward turning of interplanetary magnetic field (IMF) cause the earthward movement of dayside magnetopause and the drift loss of energetic particles near geosynchronous orbit. The persistent electron drift loss makes the geosynchronous satellites cannot observe the substorm electron injection phenomenon during the two substorm expansion phases (06:57–07:39 UT) on that day. Behind the IP shock, the fluctuations (~0.5–3 nPa) of solar wind dynamic pre
合写作者：Z. Q. Wang
第一作者：L. Y. Li
论文类型：基础研究
一级学科：地球物理学
文献类型：期刊
是否译文：否
发表时间：2018-01-04
收录刊物：SCI
发布期刊链接：http://onlinelibrary.wiley.com/doi/10.1002/2017JA024628/abstract