An empirical statistical model of the radiation characteristics of solar proton events in near-Earth space.

Details An empirical statistical model of the radiation characteristics of solar proton events in near-Earth space. An empirical statistical model of the radiation characteristics of solar proton events in near-Earth space.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996radme..26..451p&link_type=abstract

Radiat. Meas., Vol. 26, No. 3, p. 451 - 454

Physics

Solar Cosmic Rays: Protons

Scientific paper

Characteristics of solar proton events (SPE) with a maximum flux of 1 cm-2s-1sr-1 (Ep > 10 MeV) in the Earth's orbit over the last three 11-year solar cycles are studied using satellite observations. The number of SPEs responsible for strong disturbances in the 22nd cycle has increased considerably. Based on the set of radiation and heliogeophysical parameters, statistical and empirical radiation situation models are described.

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