Shower Simulation Input for Fluorescence Yield Measurements

Details Shower Simulation Input for Fluorescence Yield Measurements Shower Simulation Input for Fluorescence Yield Measurements

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2..607r&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 CORSIKA simulation code has been adapted for an extensive study of the energy release of shower particles during the cascade development. The contributions to the energy deposit from different particle species and energies as well as the typical particle densities are investigated. The dominant contribution stems from electrons and positrons from sub-MeV up to a few hundred MeV, with typical distances between particles exceeding 1 mm for 10 EeV showers. special care is taken of particles falling below the simulation energy threshold which contribute around 10% to the total deposition.

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