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Revision of the energy calibration of the Yakutsk EAS array

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arxiv 1408.6302 v1 pith:XENJ7BIY submitted 2014-08-27 astro-ph.HE

classification astro-ph.HE
keywords energyarrayobtainedyakutskcalculatedcalibrationcompareddetectors
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Responses of surface and underground scintillation detectors of Yakutsk array are calculated for showers initiated by primary particles with energy E0>=1.0E17 eV within the frameworks of QGSJet01 QGSIIJet-II-04, SIBYLL-2.1 and EPOS-LHC hadron interaction models. A new estimation of E0 is obtained with the use of various methods. The resulting energy is lower compared to the obtained with earlier method by factor ~1.33.

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