Albedo gamma-rays from cosmic ray interactions on the solar surface

Details Albedo gamma-rays from cosmic ray interactions on the solar surface Albedo gamma-rays from cosmic ray interactions on the solar surface

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..220..227s&link_type=abstract

In: High energy gamma-ray astronomy; Proceedings of the International Conference, Ann Arbor, MI, Oct. 2-5, 1990 (A93-25001 08-93

Astronomy and Astrophysics

Astronomy

Albedo, Elementary Particle Interactions, Gamma Ray Astronomy, Solar Cosmic Rays, Interplanetary Magnetic Fields, Neutron Distribution, Solar Flux, Solar Neutrinos

Scientific paper

We estimate the flux of gamma-rays that result from collisions of high energy galactic cosmic rays with the solar atmosphere. The high energy photon flux should be observable by the GRO, although details of our results are sensitive to assumptions about cosmic ray propagation through the magnetic fields of the inner solar system. We also estimate the neutrino and neutron fluxes resulting from the same process.

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