2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/40682The 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)High Energy Physics - Phenomenologytext