Measurements of low energy electrons and ions during long-lived solar particle events

Details Measurements of low energy electrons and ions during long-lived solar particle events Measurements of low energy electrons and ions during long-lived solar particle events

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ssrv...32..169a&link_type=abstract

(Slovenska Akademia Vied, IAU, and COSPAR, Study of Travelling Interplanetary Phenomena Workshop on Shock Waves in the Solar Cor

Computer Science

8

Ion Distribution, Solar Corpuscular Radiation, Solar Electrons, Solar Flares, Angular Distribution, Energy Spectra, International Sun Earth Explorer 3, Solar X-Rays

Scientific paper

The stream of ions and electrons which appeared in planetary space for about eight days after an April 1979 solar flare exhibited a classic energetic storm particle (ESP) event ion pattern. Distinct populations of these electrons can be identified in association with IMF filaments, and the electron energy spectrum is well fit by a power law exponent of -2.7 during most of the event. The pitch angle distributions of the low energy electrons are found to be complex and to undergo many changes, with weak pitch angle scattering and adiabatic effects playing a role in the shaping of these distributions.

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