Change in the spectrum of low-energy protons during their passage through the solar corona

Details Change in the spectrum of low-energy protons during their passage through the solar corona Change in the spectrum of low-energy protons during their passage through the solar corona

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pazh....3..469z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 3, Oct. 1977, p. 469-473. In Russian.

Astronomy and Astrophysics

Astronomy

Energy Spectra, Plasma-Particle Interactions, Proton Energy, Solar Corona, Solar Protons, Energy Dissipation, Energy Transfer, Particle Acceleration, Particle Collisions, Spectral Energy Distribution

Scientific paper

The shape of the proton spectrum over the energy range from 20 to 1000 keV at a distance of 1 AU after passage through a specific amount of matter in the solar corona is obtained on the assumption of an initial power-law spectrum. Energy losses experienced by soft protons in the storage region near the sun are computed, and the change in proton spectral shape that occurs during propagation in the corona is analyzed. Analytical results are briefly evaluated for different values of the governing parameters.

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