Mass Composition and Energy Estimation of Primary Cosmic Ray Using Atmospheric Cherenkov Light Reconstruction

Details Mass Composition and Energy Estimation of Primary Cosmic Ray Using Atmospheric Cherenkov Light Reconstruction Mass Composition and Energy Estimation of Primary Cosmic Ray Using Atmospheric Cherenkov Light Reconstruction

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..899..129m&link_type=abstract

SIXTH INTERNATIONAL CONFERENCE OF THE BALKAN PHYSICAL UNION. AIP Conference Proceedings, Volume 899, pp. 129-130 (2007).

Other

Extensive Air Showers, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

Cosmic rays induced by different primaries are simulated using Corsika 6 code and the lateral distributions of atmospheric Cherenkov light are obtained. Approximation of the lateral distributions is proposed. On the basis of solution of inverse problem and the proposed approximation the reconstruction of the shower is carried out and the characteristics of the initial primary particle are estimated.

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