Relativistic solar protons

Details Relativistic solar protons Relativistic solar protons

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975rvgsp..13.1084d&link_type=abstract

Reviews of Geophysics and Space Physics, vol. 13, July 1975, p. 1084-1086, 1095, 1096. NSF-supported research.

Physics

1

Astronomical Models, Particle Acceleration, Relativistic Particles, Solar Activity Effects, Solar Flares, Solar Protons, Angular Distribution, Anisotropy, Energy Spectra, Proton Energy, Proton Flux Density, Solar Physics, Storage

Scientific paper

Recent papers by U.S. scientists on various aspects of high-energy solar protons associated with solar flares are summarized. The intensity profile and energy spectrum of relativistic solar particles are described together with their anisotropic angular distribution at 1 AU. Several models of relativistic-particle propagation are outlined, particularly those which suggest diffusion in the 'solar envelope' (the region out to about 30 solar radii) and longitudinal drift. Proposed models of particle acceleration and storage at the sun are discussed.

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