On the origin of corotating energetic particle events

Details On the origin of corotating energetic particle events On the origin of corotating energetic particle events

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85.1743s&link_type=abstract

Journal of Geophysical Research, vol. 85, Apr. 1, 1980, p. 1743-1748.

Physics

3

Energetic Particles, Interplanetary Space, Rotating Plasmas, Solar Wind, Particle Acceleration, Pioneer Space Probes, Plasma Temperature, Steady State

Scientific paper

The paper examines energetic corotating particle events produced by acceleration at the forward and reverse shock pair which bounds a corotating interaction region by the process of successive multiple reflections. In the steady state, the energetic particle intensity at the shock depends only on the intensity of shock particles, and measurements of energetic particles show systematic variations between intensities at the forward and reverse shocks. It is concluded that the solar wind is the original particle population that is accelerated in the stationary shocks up to several MeV.

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