Energy spectra of hadrons and leptons in the atmosphere

Details Energy spectra of hadrons and leptons in the atmosphere Energy spectra of hadrons and leptons in the atmosphere

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982izssr..46.2428b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Samarkand, Uzbek SSR, Oct. 27-29, 1981.) Akademiia Nauk SSSR, Izvestiia, Ser

Physics

Energy Spectra, Hadrons, Leptons, Secondary Cosmic Rays, Atmospheric Radiation, Cross Sections, Spectral Energy Distribution

Scientific paper

Differential spectra of hadrons in the 10 to the 11th to 10 to the 15th eV energy region were obtained for atmospheric depths of 60, 260, 690, and 1000 g/cu cm. It is shown that at a depth of 60 g/cu cm the Nikol'skii (1975) spectrum gives the best agreement with the experimental data; the Ryan (1972) spectrum also cannot be excluded. In addition, the Monte Carlo method was used to calculate fluxes of low-energy neutrinos in the atmosphere. Total fluxes of muon and electron neutrinos at an energy of not greater than approximately 200 MeV were 1.13 and 0.75/sq cm s, respectively, while at an energy not greater than approximately 10 MeV these values were 0.011 and 0.035/sq cm s

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