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

V. I. Degtyarev G.V. Popov B. S. Xue S.E. Chudnenko

V. I. Degtyarev, G.V. Popov, B. S. Xue, S.E. Chudnenko. Input Parameters for Models of Energetic Electrons Fluxes at the Geostationary Orbit[J]. 空间科学学报, 2005, 25(5): 424-429. doi: 10.11728/cjss2005.05.424
引用本文: V. I. Degtyarev, G.V. Popov, B. S. Xue, S.E. Chudnenko. Input Parameters for Models of Energetic Electrons Fluxes at the Geostationary Orbit[J]. 空间科学学报, 2005, 25(5): 424-429. doi: 10.11728/cjss2005.05.424
V. I. Degtyarev, G.V. Popov, B. S. Xue, S.E. Chudnenko. Input Parameters for Models of Energetic Electrons Fluxes at the Geostationary Orbit[J]. Journal of Space Science, 2005, 25(5): 424-429. doi: 10.11728/cjss2005.05.424
Citation: V. I. Degtyarev, G.V. Popov, B. S. Xue, S.E. Chudnenko. Input Parameters for Models of Energetic Electrons Fluxes at the Geostationary Orbit[J]. Journal of Space Science, 2005, 25(5): 424-429. doi: 10.11728/cjss2005.05.424

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

doi: 10.11728/cjss2005.05.424

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

  • 摘要: The results of cross-correlation analysis between electrons fluxes (with energies of > 0.6 MeV,> 2.0MeV 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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出版历程
  • 收稿日期:  1900-01-01
  • 修回日期:  1900-01-01
  • 刊出日期:  2005-09-15

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