HELIOS 1 energetic particle observations of the solar gamma ray flare events of 7, 21 June 1980 and 3 June 1982

Details HELIOS 1 energetic particle observations of the solar gamma ray flare events of 7, 21 June 1980 and 3 June 1982 HELIOS 1 energetic particle observations of the solar gamma ray flare events of 7, 21 June 1980 and 3 June 1982

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4...98m&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 4 p 98-101 (SEE N85-34729 23-92)

Physics

Anisotropy, Coronal Loops, Coronas, Electron Density (Concentration), Gamma Ray Bursts, Neutron Emission, Particle Acceleration, Particle Flux Density, Particle Precipitation, Photosphere, Solar Flares, Transport Properties, X Ray Spectra, Gamma Ray Spectrometers, Helios 1, Interplanetary Magnetic Fields, Solar Maximum Mission

Scientific paper

The observed characteristics of the energetic particles associated with the solar γ-ray events of 3, 21 June 1980 and 3 June 1982 differ in several important aspects from the typical solar particle increases. They have flat energy spectra, are electron rich and have small precursor increases that begin some hours before the impulsive flare increase.

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