点击次数：
发表刊物：Journal of Geophysical Research: Space Physics
关键字：Earth's Radiation Belts;Solar Wind Plasma Flow;Interplanetary Magnetic Field
摘要：Based on the statistical data measured by Van Allen Probes from 2012 to 2016, we analyzed the effects of solar wind plasma flow and interplanetary magnetic field (IMF) on the spatial distribution of Earth's radiation belt electrons (>100 keV). The statistical results indicate that the increases in solar wind plasma density and flow speed can exert different effects on the spatial structure of the radiation belts. The high solar wind plasma density ( 6 cm−3)/flow pressure ( 2.5 nPa) and a large southward IMF (Bz < −6nT) usually appear in the front of high‐speed solar wind streams ( 450 km/s),
合写作者：S. S. Yang,J. Yu
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：2019-12-30
收录刊物：SCI
发布期刊链接：https://agupubs-onlinelibrary-wiley-com-443.e2.buaa.edu.cn/doi/abs/10.1029/2019JA027284