Energy losses of cosmic rays in a two-component model of the cosmic medium

Details Energy losses of cosmic rays in a two-component model of the cosmic medium Energy losses of cosmic rays in a two-component model of the cosmic medium

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2306k&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Computer Science

Aerospace Environments, Cosmic Rays, Energetic Particles, Energy Dissipation, Two Dimensional Models, Electromagnetic Fields, Magnetic Clouds, Particle Mass

Scientific paper

The two-component model of the cosmic medium consists of (1) a moving background plasma with a frozen-in magnetic field and (2) an ensemble of magnetic clouds moving at a velocity that differs from that of the background plasma. Cosmic-ray energy losses in this model are considered; the propagation of electrons in the interstellar medium is considered as an example.

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