The connection between solar wind velocity variations and the physical and empirical models for electron fluxes in near-Earth space.

Details The connection between solar wind velocity variations and the physical and empirical models for electron fluxes in near-Earth space. The connection between solar wind velocity variations and the physical and empirical models for electron fluxes in near-Earth space.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996radme..26..405g&link_type=abstract

Radiat. Meas., Vol. 26, No. 3, p. 405 - 408

Physics

Solar-Terrestrial Relations

Scientific paper

Long duration predictions of energetic electron fluxes in near-Earth space is obtained using calculated models. However the existing calculated models, constructed on the basis of experimental data, usually do not sufficiently take into account the variations of the solar wind velocity. Many experiments on satellites show that the energetic electron flux intensity in magnetosheath, magnetopause and geosynchronous orbits depends on the solar wind velocity. A method for determining the dependence observed in physical and empirical models for energetic electron fluxes in near-Earth cosmic space is suggested.

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