A convection-diffusion model for the propagation of the proton-nuclear component of cosmic rays in the Galaxy

Details A convection-diffusion model for the propagation of the proton-nuclear component of cosmic rays in the Galaxy A convection-diffusion model for the propagation of the proton-nuclear component of cosmic rays in the Galaxy

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.2052b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, Russia, Nov. 1-3, 1990, Materialy. A92-40776 16-93) Akademiia Nauk

Computer Science

Convection-Diffusion Equation, Energy Spectra, Galactic Cosmic Rays, Particle Energy, Radiation Distribution, Spatial Distribution, Supernovae

Scientific paper

The propagation of the proton-nuclear component of cosmic rays is
considered within the framework of a convection-diffusion model. It is
concluded that Galactic wind is inessential to the transfer of cosmic
rays in the Galaxy.

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