Simulation of Atmospheric Neutrino Fluxes with CORSIKA

Details Simulation of Atmospheric Neutrino Fluxes with CORSIKA Simulation of Atmospheric Neutrino Fluxes with CORSIKA

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....3.1403w&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

The three dimensional Monte Carlo simulation code CORSIKA is used to calculate the fluxes of atmospheric neutrinos with the hadronic interaction models DPMJET, VENUS, and UrQMD. For this purpose the original CORSIKA is extended by a parametrization of the solar modulation and a microscopic calculation of the directional dependence of the geomagnetic cut-off functions. A precise description for the geography of the Earth has been included by a digital elevation model, tables for the local magnetic field in the atmosphere, and various atmospheric models for different geographic latitudes and annual seasons. The neutrino fluxes obtained are compared with other calculations.

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