Primary-particle spectrum from extensive-air-shower data in the energy region from 10 to the 8th power to 10 to the 10th power GeV

Details Primary-particle spectrum from extensive-air-shower data in the energy region from 10 to the 8th power to 10 to the 10th power GeV Primary-particle spectrum from extensive-air-shower data in the energy region from 10 to the 8th power to 10 to the 10th power GeV

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40.1035d&link_type=toc

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Mathematics

Probability

Atmospheric Attenuation, Cosmic Ray Showers, Energy Spectra, High Energy Electrons, Primary Cosmic Rays, Spatial Distribution, Monte Carlo Method, Muons, Pions, Probability Distribution Functions, Vertical Distribution

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