Origin of cosmic rays

Details Origin of cosmic rays Origin of cosmic rays

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..520g&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Physics

Nuclear Physics

Cosmic Rays, Galactic Radiation, Astronomical Models, Magnetic Field Configurations, Nuclei (Nuclear Physics), Particle Diffusion, Radiation Sources

Scientific paper

The origin of galactic cosmic rays is examined on the basis of cosmic-ray nuclei data (Li, Be, B, H-2 and H-3 nuclei). A one-dimensional diffusion model is developed in which the cosmic ray sources and the interstellar gas are concentrated in the galactic disk. Cosmic ray nuclei diffuse with a coefficient constant throughout the Galaxy and freely enter the intergalactic medium. The mechanism of cosmic ray production is still unclear, but is apparently associated with the resonant scattering of particles on inhomogeneities of the galactic magnetic field.

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