Statistical Study of high energy fluxes at GSO:Building on ERR results

Details Statistical Study of high energy fluxes at GSO:Building on ERR results Statistical Study of high energy fluxes at GSO:Building on ERR results

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsm41b2035w&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SM41B-2035

Physics

[2774] Magnetospheric Physics / Radiation Belts

Scientific paper

Error Reduction Ratio analysis produced a surprising result for the solar wind parameters that control the high energy electron fluxes at GSO. It was shown that the solar wind velocity and density are the mist influential parameters. However their relative role changes with energy range. A statistical study that shows effects of solar wind density, velocity and other solar wind parameters on the daily averaged fluxes of energetic electrons at GSO is presented.

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