Effect of a standing shock wave on the modulating properties of the solar wind

Details Effect of a standing shock wave on the modulating properties of the solar wind Effect of a standing shock wave on the modulating properties of the solar wind

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2364b&link_type=abstract

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

Physics

Energetic Particles, Galactic Cosmic Rays, Shock Fronts, Solar Wind Velocity, Weak Energy Interactions, Boundary Value Problems, Diffusion Coefficient, Particle Acceleration

Scientific paper

The standing shock wave in the interplanetary medium which limits the supersonic flow region of the solar wind has a significant effect on galactic-cosmic-ray modulation and may be a source of low-energy particles in the heliosphere. This is due to the regular acceleration of cosmic rays near the shock front. The acceleration process is analyzed numerically in an energy range corresponding to possible sources of particles injected at the front.

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