Physics
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc...12..235k&link_type=abstract
IN: International Cosmic Ray Conference, 18th, Bangalore, India. August 22-September 3, 1983, Invited and Rapporteur Papers. Vol
Physics
2
Energetic Particles, Gamma Rays, Particle Acceleration, Solar Atmosphere, Solar Flares, Solar Wind, Abundance, Electron Acceleration, Energy Spectra, Isotopes, Neutrons
Scientific paper
Observations and theoretical investigations of the physical characteristics of solar energetic particles, gamma rays, and neutrons are briefly reviewed. Attention is given to such topics as: the relationship between particle acceleration and the thermal and magnetic properties of the solar plasma; the energy spectra of cosmic rays; and the elemental and isotopic composition of solar particles. Observational data from the Solar Maximum Mission, Hinotori, and ISEE-3 satellites are discussed within the framework of current theories concerning the physical properties of solar gamma-rays and neutrons with energies above 0.3 MeV; photon emission from solar flares at energies above 10 MeV; and type II and type IV radio bursts due to gamma-ray line flares. The connection between proton and electron acceleration processes during the impulsive phase of a solar flare event is discussed in detail.
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