Flux of upward high-energy muons at the multi-component primary energy spectrum
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The atmospheric neutrino-induced upward muon flux are calculated by using the multi-component primary energy spectrum, CORSIKA EAS simulation code for the reproduction of the atmospheric neutrino spectra and improved parton model for charged-current cross sections. The results are obtained at 0.1-1000 TeV muon energy range and 0-89 degrees zenith angular range.
4 pages, 5 figures, to appear in proceedings of 27th ICRC (Hamburg, August 7-15, 2001)
4 pages, 5 figures, to appear in proceedings of 27th ICRC (Hamburg, August 7-15, 2001)