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发表刊物：Journal of Geophysical Research: Space Physics,
关键字：Earthward convection, Azimuthal drift loss, Outer radiation belt, Energetic electrons, Pitch angle distribution,
摘要：Utilizing the multi‐point observations by Van Allen Probe A, GOES 13 and 15, we analyzed the competing influences of earthward convection and azimuthal drift loss on the pitch angle distributions of energetic electrons during the simultaneous increases in solar wind flow velocity and pressure. The increase in solar wind speed amplifies the dawn‐dusk convection electric field and causes the earthward transport of energetic electrons, and meanwhile the enhancement of solar wind dynamic pressure causes the inward displacement of dayside magnetopause and triggers the azimuthal drift loss of energetic electrons. The earthward convection of low‐energy electrons (<60 keV) is much faster than their azimuthal drift loss at most pitch angles, and the fast earthward convections make the butterfly‐like electron pitch angle distributions formed early become pancake‐like distributions. The 60–530 keV electrons maintain the butterfly‐like pitch angle distributions during the earthward convections, whereas the high‐energy electrons above 530 keV are not transported to the low‐L shells because of fast drift loss in the high‐L source region. The competition between the earthward convection and the azimuthal drift loss finally determines the pitch angle distributions of energetic electrons near the trapping boundary during the increases in solar wind flow speed and pressure.
第一作者：H. C. Yuan
论文类型：期刊论文
通讯作者：L. Y. Li, +++
一级学科：地球物理学
卷号：129
是否译文：否
CN号：https://agupubs.onli
发表时间：2024-06-23
收录刊物：SCI