Energetic solar cosmic rays in the outer heliosphere

Details Energetic solar cosmic rays in the outer heliosphere Energetic solar cosmic rays in the outer heliosphere

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...10..385g&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Late Papers. Volume 10 (A85-22801

Physics

Heliosphere, Solar Cosmic Rays, Solar Flares, Solar Protons, Anisotropy, Explorer 50 Satellite, Particle Telescopes, Pioneer Space Probes, Radiant Flux Density, Shock Waves

Scientific paper

Intermediate-energy protons (3.5-56 MeV) in the outer heliosphere are studied using data from the GSFC-UNH cosmic-ray telescopes on Pioneer 10 and 11. Flux and anisotropy information in this energy region is used to investigate the properties of the solar-flare-associated flux increases detected between September 1977 and September 1982 for radial distances between 5.8 and 28.5 AU. A propagation model is discussed, and its predictions for the 3-5 MeV protons are presented in diagrams.

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