Estimation of Primary Cosmic Ray Energy Registered at the EAS Yakutsk Array

Details Estimation of Primary Cosmic Ray Energy Registered at the EAS Yakutsk Array Estimation of Primary Cosmic Ray Energy Registered at the EAS Yakutsk Array

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..393g&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 energy for primary particles generating showers in the energy interval of 1017 - 1019 eV is estimated by using EAS Cerenkov light data at the Yakutsk array. For vertical showers the main relations between the energy and measured parameters S 300 and S 600 obtained by the calorimetric method are given. S 300 and S 600 depending on a zenith angle are studied. The change of these parameters in the wide region of atmospheric depth can be described as a sum of two exponents with strongly different attenuation lengths.

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