Contribution of solar cosmic rays to the formation of the Earth's proton radiation belt

Details Contribution of solar cosmic rays to the formation of the Earth's proton radiation belt Contribution of solar cosmic rays to the formation of the Earth's proton radiation belt

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cosre..47..374l&link_type=abstract

Cosmic Research, Volume 47, Issue 5, pp.374-377

Physics

1

Energetic Trapped Particles, Radiation Belts

Scientific paper

The significance of the contribution of solar protons to fluxes of trapped radiation in the Earth’s outer radiation belt ( L > 2) is estimated for various phases of solar activity. In periods of high solar activity, proton fluxes with the energy 1-5 MeV at L = 2-3 for the bulk of time have SCR as a source, during a minimum of solar activity, trapped proton fluxes are determined by the conventional diffusive mechanism under the action of sudden IMF impulses.

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