Abstract
Responses of surface and underground scintillation detectors of Yakutsk array are calculated for showers initiated by primary particles with energy within the frameworks of QGSJet01d, QGSJet-II-04, SIBYLL-2.1, and EPOS-LHC hadron interaction models. A new estimation of is obtained with the use of various methods. The resulting energy is lower compared to the obtained with earlier method by a factor of .
- Received 25 April 2014
DOI:https://doi.org/10.1103/PhysRevD.90.012005
© 2014 American Physical Society