Features of the behavior of quasi-trapped solar protons at energies greater than about 100 MeV

Details Features of the behavior of quasi-trapped solar protons at energies greater than about 100 MeV Features of the behavior of quasi-trapped solar protons at energies greater than about 100 MeV

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1836b&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1836-1838. In Russian.

Physics

Energy Spectra, Proton Energy, Solar Protons, Diurnal Variations, Particle Telescopes, Pitch (Inclination)

Scientific paper

Solar-proton-spectrum measurements made in the Apatity (L = 5) are
examined. It is shown that adiabaticity breaks down significantly in the
near-equatorial region at an energy of about 100 MeV even in the dipole
field. In the actual magnetosphere, this breakdown will be even more
acute with significant pitch-angle scattering.

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