High-energy cosmic ray diffusion in the Galaxy

Details High-energy cosmic ray diffusion in the Galaxy High-energy cosmic ray diffusion in the Galaxy

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55.2049z&link_type=abstract

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

Physics

Energetic Particles, Galactic Cosmic Rays, Hall Effect, Magnetic Fields, Particle Diffusion, Energy Spectra, Radiation Spectra

Scientific paper

A diffusion model of the propagation of cosmic rays with energies of 10
exp 14 to 10 exp 17 is considered. The possible derivation of a bend in
the observed energy spectrum for 5 x 10 exp 15 eV due to the drift
effect (Hall diffusion) of cosmic rays in the general regular magnetic
field of the Galaxy is discussed.

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