Atmospheric muon and neutrino fluxes from 3D simulation

Details Atmospheric muon and neutrino fluxes from 3D simulation Atmospheric muon and neutrino fluxes from 3D simulation

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1033l&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

1

Scientific paper

The muon and neutrino flux are simulated. The program used has successfully reproduced the proton, helium, and e+ /e- spectra measured by AMS. An improved parametrization of the pion production cross section induced by proton on nuclei obtained from a set of data over a broad incident kinetic energy range (0.73-200 GeV), has been used. The simulated muon flux accounts fairly well for the recent measurements at various altitude between sea level and 38 km. The simulated neutrino flux obtained are lower than those reported previously by other groups.

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