Pitch angle distributions of 35-1000 keV protons at quasi-perpendicular interplanetary shocks

Details Pitch angle distributions of 35-1000 keV protons at quasi-perpendicular interplanetary shocks Pitch angle distributions of 35-1000 keV protons at quasi-perpendicular interplanetary shocks

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..178b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 178-181 (SEE N85-34729 23-92)

Physics

Distribution Functions, Interplanetary Medium, Pitch (Inclination), Shock Waves, Solar Wind, International Sun Earth Explorer 3, Particle Acceleration

Scientific paper

The characteristic features of the scatter-free acceleration process near perpendicular shocks are examined in the upstream and downstream pitch angle distributions of 35 - 1000 keV protons. Reasonable quantitative agreement is found between theoretical predictions and observations. The role played by "bottle" geometries, leading to enhanced acceleration, is highlighted.

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