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发表刊物：Physics of Plasmas
关键字：Solar wind dynamic pressure,Electromagnetic ion cyclotron waves, Relativistic electron loss
摘要：During enhancement of solar wind dynamic pressure, we observe the periodic emissions of electromagnetic ion cyclotron (EMIC) waves near the nightside geosynchronous orbit (6.6RE). In the hydrogen and helium bands, the different polarized EMIC waves have different influences on relativistic electrons (>0.8MeV). The flux of relativistic electrons is relatively stable if there are only the linearly polarized EMIC waves, but their flux decreases if the left-hand polarized (L-mode) EMIC waves are sufficiently amplified (power spectral density (PSD) 1nT2/Hz). The largeramplitude L-mode waves can cau
合写作者：J. Yu,J. B. Cao,Z. G. Yuan
第一作者：L. Y. Li
一级学科：地球物理学
文献类型：期刊
是否译文：否
发表时间：2016-06-07
收录刊物：SCI
发布期刊链接：http://aip.scitation.org/doi/10.1063/1.4953899