%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