UHECR Composition Studies with HiRes Stereo Data

Details UHECR Composition Studies with HiRes Stereo Data UHECR Composition Studies with HiRes Stereo Data

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..405a&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

6

Scientific paper

The composition of Ultra High Energy Cosmic Rays (UHECR) was studied with the High Resolution Fly's Eye cosmic ray observatory (HiRes). The QGSJet01 and SIBYLL 2.1 hadronic interaction models were used in the CORSIKA event generator to study predicted elongation rates and Xmax distribution widths in the UHECR regime. The CORSIKA-generated EAS were incorporated directly into a detailed atmospheric and detector Monte Carlo. Elongation rate and Xmax distribution results will be shown for our stereo data.

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