Jan 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ssrv...64..183d&link_type=abstract
Space Science Reviews, vol. 64, p. 183
Other
11
Solar Cosmic Rays, Solar Flares, Chromosphere, Radiation Hazards, Earth Atmosphere, Energy Spectra, Abundance, Particle Acceleration, Positrons, Neutrons
Scientific paper
Results are presented of the experimental and theoretical investigations of the results of the properties of solar cosmic rays from ground events. Important information from solar experimental data relating to ground events observed on September and October 1989 and May 1990 is discussed. Some experimental evidence of acceleration processes in phenomena associated with flares and the long-term (solar cycle) variation of the average flux of solar cosmic rays is discussed. Solar cosmic ray propagation in the corona, interplanetary space, and in the terrestrial magnetosphere is also discussed. It is noted that the energy spectrum of the solar cosmic rays varied very strongly from one flare to another. An investigation is undertaken of the chemical and isotopic contents of solar cosmic rays, including the composition of some individual solar cosmic-ray events and the statistical regularities of solar cosmic-ray chemical composition. A discussion of the peculiarities of He-3- and heavy-nucleus-rich events concludes this study.
Dorman Lev I.
Venkatesan D.
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