Measurement of the flux and angular distribution of muons produced by cosmic ray neutrinos

Details Measurement of the flux and angular distribution of muons produced by cosmic ray neutrinos Measurement of the flux and angular distribution of muons produced by cosmic ray neutrinos

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55..748b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, USSR, Nov. 1-3, 1990) Akademiia Nauk SSSR, Izvestiia, Seriia Fizich

Other

Cosmic Rays, Muons, Neutrinos, Particle Flux Density, Scintillation Counters, Energetic Particles, Energy Spectra, High Energy Interactions, Monte Carlo Method

Scientific paper

Results of long-term (over 10 yr) scintillation telescope observations of muons produced by cosmic ray neutrinos are presented. The flux of muons with energies above 0.8 GeV, averaged over the lower hemisphere, is estimated at (2.84 + or - 0.17) x 10 to the -13th/sq cm s sr. This result is in good agreement with the results of other similar experiments and with calculated fluxes of muons produced by atmospheric neutrinos.

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