Halo-disk repenetration of the cosmic particles

Details Halo-disk repenetration of the cosmic particles Halo-disk repenetration of the cosmic particles

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974a%26a....35..339s&link_type=abstract

Astronomy and Astrophysics, vol. 35, no. 3, Oct. 1974, p. 339-344.

Astronomy and Astrophysics

Astrophysics

1

Cosmic Rays, Electron Diffusion, Energy Spectra, Galactic Radiation, Halos, Compton Effect, Energy Dissipation, High Energy Electrons, Interstellar Magnetic Fields, Nonthermal Radiation, Particle Motion, Supernovae, Synchrotron Radiation

Scientific paper

Cosmic electron diffusion characteristics are used to examine the problem of halo-disk repenetration of cosmic particles. Comparison of the results with observed data indicates the repenetration rate can be appreciable. Analysis of the expected nonthermal radiation from the cosmic electron spectrum determined for the disk and halo domains compares favorably with observed astronomical data. Indications of active exchange of cosmic particles between the disk and halo domains suggests supernova explosions as the main source of cosmic rays in the Galaxy.

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