%0 Journal Article
%T Modelling Energetic Electrons by a Kappa-Loss-Cone Distribution at Geostationary Orbit
%A XIAO Fu-Liang
%A ZHOU Qing-Hua
%A HE Hui-Yong
%A
肖伏良
%A 周庆华
%A 贺慧勇
%J 中国物理快报
%D 2007
%I
%X We adopt a recently developed relativistic kappa-loss-cone (KLC) distribution to model energetic electrons energy spectra observed at the geostationary orbit in the storm of 3--4 November 1993. The KLC distribution is found to fit well with the observed data from four satellites during different universal times. This suggests that the electron flux obeys the power-law not only at the lower energies but also at the relativistic energies, and the KLC distribution may provide a better understanding of environments in those space plasmas where relativistic electrons are present.
%K 52
%K 27
%K Ny
%K 94
%K 30
%K -d
%K 95
%K 75
%K -z
模型
%K 能量
%K 电子分布
%K 静止轨道
%U http://www.alljournals.cn/get_abstract_url.aspx?pcid=6E709DC38FA1D09A4B578DD0906875B5B44D4D294832BB8E&cid=47EA7CFDDEBB28E0&jid=E27DA92E19FE279A273627875A70D74D&aid=03664AC44D4808184AE8BF2834BC774F&yid=A732AF04DDA03BB3&vid=B91E8C6D6FE990DB&iid=DF92D298D3FF1E6E&sid=37904DC365DD7266&eid=DE12191FBD62783C&journal_id=0256-307X&journal_name=中国物理快报&referenced_num=0&reference_num=0