The spectrum of flare protons in the low-energy range

Details The spectrum of flare protons in the low-energy range The spectrum of flare protons in the low-energy range

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981kosis..19..704d&link_type=abstract

Kosmicheskie Issledovaniia, vol. 19, Sept.-Oct. 1981, p. 704-711. In Russian.

Computer Science

Energy Spectra, Proton Energy, Solar Flares, Solar Protons, Energy Dissipation, Particle Acceleration, Prognoz Satellites, Solar Cosmic Rays

Scientific paper

An analysis is presented of the spectra of flare protons in the 0.08-150 MeV energy range, measured at about 1 AE on the Prognoz-6 satellite. The spectral data are compared with the energy dependence of the observation time of the maximum flux of flare protons. It is shown that changes in the slope in the spectrum and in the energy dependence of maximum times occur at approximately the same energy. Energy losses of protons in the interplanetary medium due to adiabatic cooling are determined. This effect is significant for protons with energies less than 1 MeV, and, in the case of flares of low importance, plays a decisive role in the formation of the spectrum of the observed flare protons.

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