Some Characteristics of Extensive Air Showers at Chacaltaya Observation Level

Details Some Characteristics of Extensive Air Showers at Chacaltaya Observation Level Some Characteristics of Extensive Air Showers at Chacaltaya Observation Level

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..247m&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

One of the principle problems in high energy astrophysics are the investigations of cosmic rays, precisely their spectrum and mass composition. In this paper in attempt to facilitate future experiments based on different technics and registration of different components of extensive air showers some characteristics are simulated using CORSIKA code. In the very interesting energy range 1012 - 1016 eV for primary proton and gamma quanta and 1012 - 1016 eV for primary iron and helium the lateral distributions of Cerenkov light, electron, muons and hadrons are obtained for Chacaltaya observation level (536g /cm2).

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