Computer Science
Scientific paper
Feb 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977izssr..41q.293d&link_type=abstract
(Mezhdunarodnyi Seminar po Aktivnym Protsessam na Solntse i Probleme Solnechnykh Neitrino, 8th, Leningrad, USSR, Sept. 25-27, 19
Computer Science
Galactic Radiation, Primary Cosmic Rays, Solar Cosmic Rays, Abundance, Chromosphere, Interstellar Radiation, Plasma Turbulence, Solar Flares, Solar Wind
Scientific paper
Subcosmic rays are defined as cosmic rays with energies not exceeding about 0.05 GeV. Arguments are presented in favor of the contention that subcosmic rays are produced by particles entirely of solar origin, mainly from chromospheric flares. It is shown that subcosmic rays cannot be of interplanetary or galactic origin, and indirect evidence is cited for the presence of such particles in interstellar space. The chemical composition and energy spectrum of subcosmic rays observed in interplanetary space are examined along with abundance anomalies, time variations and the radial gradient of the subcosmic-ray flux, and the relative proton and alpha-particle contents of solar cosmic and subcosmic rays. The possibility is considered that subcosmic rays might also be produced and further accelerated in the turbulent transition zone between the solar wind and the interstellar medium.
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