Features of the proton energy spectrum and the problem of the origin of cosmic rays

Details Features of the proton energy spectrum and the problem of the origin of cosmic rays Features of the proton energy spectrum and the problem of the origin of cosmic rays

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kosis..30..378g&link_type=abstract

Kosmicheskie Issledovaniya (ISSN 0023-4206), vol. 30, no. 3, p. 378-384.

Physics

Energy Spectra, Galactic Cosmic Rays, Proton Energy, Ion Temperature, Muons, Supernovae

Scientific paper

Consideration is given to the anomaly in the cosmic ray proton spectrum at 1-10 TeV and to the detection of high-energy ions in cosmic rays as a possible consequence of the presence of a nearby cosmic ray source. An integral proton spectrum, the relationship of fluxes of protons and alpha particles at different energies, and differential spectra of the vertical muon flux at sea level are illustrated.

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