Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions of Extensive Air Showers

Details Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions of Extensive Air Showers Energy Estimation of Ultra High Energy Cosmic Hadrons by Lateral Distribution Functions of Extensive Air Showers

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..424..350g&link_type=abstract

Proceedings of the 9th International Conference of the Hellenic Astronomical Society, proceedings of a conference held 20-24 Sep

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Scientific paper

The determination of energy of Ultra High Energy Cosmic Rays (E ≥ 5×1019 eV) is one of the important issues concerning these particles. For this purpose, Monte Carlo simulations are used to create a large number of vertical and inclined extensive air showers in order to estimate the primary energy based on the lateral distribution function of recorded electrons and muons. This methodology could be applied to all cosmic ray experiments using a surface array of Cerenkov detectors, like, for example, the P. Auger Observatory.

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