Cosmic ray drift, shock wave acceleration and the anomalous component of cosmic rays

Details Cosmic ray drift, shock wave acceleration and the anomalous component of cosmic rays Cosmic ray drift, shock wave acceleration and the anomalous component of cosmic rays

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8125032p&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Anomalies, Cosmic Rays, Interplanetary Magnetic Fields, Neutral Particles, Particle Acceleration, Shock Waves, Astronomical Models, Diffusion Coefficient, Magnetic Field Configurations, Solar Cycles, Solar Wind

Scientific paper

A model of the anomalous component of the quiet-time cosmic ray flux is presented in which ex-interstellar neutral particles are accelerated continuously in the polar regions of the solar-wind termination shock, and then drift into the equatorial regions of the inner heliosphere. The observed solar-cycle variations, radial gradient, and apparent latitude gradient of the anomalous component are a natural consequence of this model.

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