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平静时期太阳风中晕外电子的角分布规律(英文)
杨柳 ; 王玲华 ; 李刚 ; 何建森 ; 涂传诒
2016
关键词角分布 anisotropy instrument angular quiet traveling turbulence inward anisotropic possibility
英文摘要The angular distribution of superhalo electrons provides important information on the generation of superhalo electrons in the solar wind.Here we present a comprehensive study of the angular distribution of~20–200 keV superhalo electrons measured at 1 AU by the WIND 3DP instrument during quiet times from 1995 January through 2005 December.For a given energy,we define the anisotropy of superhalo electrons(with respect to the interplanetary magnetic field)as A=2*(Jout+Jin)/(Jout-Jin),where Jout(Jin)is the observed differential flux of electrons traveling; The angular distribution of superhalo electrons provides important information on the generation of superhalo electrons in the solar wind.Here we present a comprehensive study of the angular distribution of~20–200 keV superhalo electrons measured at 1 AU by the WIND 3DP instrument during quiet times from 1995 January through 2005 December.For a given energy,we define the anisotropy of superhalo electrons(with respect to the interplanetary magnetic field)as A=2*(Jout+Jin)/(Jout-Jin),where Jout(Jin)is the; 中国地球物理学会、中国地震学会、全国岩石学与地球动力学研讨会组委会、中国地质学会构造地质学与地球动力学专业委员会、中国地质学会区域地质与成矿专业委员会; 1
语种英语
出处2016中国地球科学联合学术年会
内容类型其他
源URL[http://ir.pku.edu.cn/handle/20.500.11897/487324]  
专题地球与空间科学学院
推荐引用方式
GB/T 7714
杨柳,王玲华,李刚,等. 平静时期太阳风中晕外电子的角分布规律(英文). 2016-01-01.
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