The energy spectrum of the continuous flux of solar cosmic rays and its variation in time

Details The energy spectrum of the continuous flux of solar cosmic rays and its variation in time The energy spectrum of the continuous flux of solar cosmic rays and its variation in time

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974izkaz.......63k&link_type=abstract

Akademiia Nauk Kazakhskoi SSR, Izvestiia, Seriia Fiziko-Matematicheskaia, July-Aug. 1974, p. 63-66. In Russian.

Physics

Energy Spectra, Solar Cosmic Rays, Solar Protons, Time Response, Chromosphere, Continuous Radiation, Galactic Radiation, Helium, Particle Flux Density, Periodic Variations, Solar Activity Effects, Solar Flux

Scientific paper

It is shown that the energy spectrum of solar cosmic particles can be described by a power function and that the upper bound of the spectrum is shifted to the region of high energies with increased solar activity. The energy spectrum of the continuous flux of solar protons becomes more rigid with decreasing energy and is similar to the spectrum of galactic cosmic rays. Data are discussed which argue in favor of the solar origin of low-energy cosmic electrons.

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