Analysis of the Energy Estimation Algorithm of UHECRs Detected with the Yakutsk Array

Details Analysis of the Energy Estimation Algorithm of UHECRs Detected with the Yakutsk Array Analysis of the Energy Estimation Algorithm of UHECRs Detected with the Yakutsk Array

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....1..385i&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 primary energy estimation method is one of the clue features to deal with using extensive air shower (EAS) technique of ultra-high energy cosmic ray (UHECR) measurements. In this paper we discuss the present status of algorithms used to assign the primary energy to showers detected with the Yakutsk array. special attention is paid to the total flux measurement of the Cherenkov light on the ground which is a basis of the model-indep endent approach to the energy evaluation of EAS original particle. The uncertainty limits of the energy estimation method are analyzed.

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