Protons and muons in the upper layers of the atmosphere

Details Protons and muons in the upper layers of the atmosphere Protons and muons in the upper layers of the atmosphere

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52.2448v&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Alma-Ata, Kazakh SSR, Sept. 13-15, 1988) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Atmospheric Radiation, Muons, Proton Energy, Upper Atmosphere, Galactic Cosmic Rays, Monte Carlo Method, Solar Activity

Scientific paper

Albedo-proton spectra were calculated for zenith angles of 143-180 deg, 114-127 deg, and 90-102 deg, and for cutoff rigidities of 0.6, 3.0, 7.3, and 15 GV. Calculations are also presented for muons with a cutoff rigidity of 0.6-4.5 GV. It is concluded that the proposed model can be used to analyze proton and muon spectra in the entire zenith-angle range from polar to equatorial regions.

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