Input Parameters for Models of Energetic Electrons Fluxes at the Geostationary Orbit

被引：0
|
作者：
V.I.Degtyarev
G.V.Popov
S.E.Chudnenko
机构：
[1] Russian Academy of Sciences
[2] Irkutsk 664033
[3] Baikal State University of Economics and Law
[4] Institute of Solar-Terrestrial Physics
[5] Siberian Branch
[6] Russia
[7] Departament of Communication Services
来源：
空间科学学报 | 2005年 / 05期
关键词：
Forecast; Energetic electrons; Geostationary orbit; Geomagnetic indices; Solar wind;
D O I：
暂无
中图分类号：
P318 [地磁学]; P353.8 [星际磁场和太阳风];
学科分类号：
070801 ; 070802 ;
摘要：
The results of cross-correlation analysis between electrons fluxes (with energies of > 0.6MeV, > 2.0 MeV and > 4.0MeV), geomagnetic indices and solar wind parameters are shown in the paper. It is determined that the electron fluxes are controlled not only by the geomagnetic indices, but also by the solar wind parameters, and the solar wind velocity demonstrates the best relation with the electron fluxes. Numerical value of the relation efficiency of external parameters with the highly energetic electrons fluxes shows a periodicity. It is presented here the preliminary results of daily averaged electrons fluxes forecast for a day ahead on the basis of the model of neuron networks.
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收藏
页码：424 / 429
页数：6
相关论文
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