Solar proton energy spectra derived from gamma-ray observations

Details Solar proton energy spectra derived from gamma-ray observations Solar proton energy spectra derived from gamma-ray observations

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jpsj...54.2100y&link_type=abstract

Physical Society of Japan, Journal (ISSN 0031-9015), vol. 54, June 1985, p. 2100-2103.

Astronomy and Astrophysics

Astronomy

7

Energy Spectra, Gamma Ray Astronomy, Particle Acceleration, Proton Energy, Solar Flares, Solar Protons, Poisson Density Functions

Scientific paper

Energy spectra of accelerated protons at flare sites are derived by comparing the observed ratios of the 4.44 MeV gamma-ray line fluence to the 2.22 MeV gamma-ray line fluence with the calculated ratios. The proton spectra derived for the Apr. 1, 1981, May 13, 1981, Oct. 15, 1981, and June 6, 1982, disk flares do not much vary from flare to flare, and are in agreement with average proton spectra observed in interplanetary space within the errors. It implies that both the protons which produce gamma-ray lines at the sun and those which escape from the sun are probably accelerated by the same mechanism.

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