Omnidirectional and vertical fluxes of charged particles in the Earth's atmosphere during solar proton events.

Details Omnidirectional and vertical fluxes of charged particles in the Earth's atmosphere during solar proton events. Omnidirectional and vertical fluxes of charged particles in the Earth's atmosphere during solar proton events.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996radme..26..443b&link_type=abstract

Radiat. Meas., Vol. 26, No. 3, p. 443 - 446

Physics

Solar Cosmic Rays: Protons

Scientific paper

The monitoring of ionizing radiation in the Earth's atmosphere provides a way to detect solar protons with E = 100 - 500 MeV at polar latitudes. At certain periods during solar proton events the experimental results may be understood in terms of the energy-dependent anisotropic angular distribution of solar protons at the top of the atmosphere. The calculation of proton trajectories shows that such a distribution could only be formed inside the magnetosphere.

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