Cosmic ray energy spectrum (>10¹⁷ eV) of the Yakutsk EAS array

M. I. Pravdin,A. V. Glushkov,N. A. Djachkovski,Yu. A. Egorov,A. A. Ivanov,V. A. Kolosov,A. D. Krasilnikov,S. P. Knurenko,I. T. Makarov,A. A. Mikhailov,Z. E. Petrov,V. P. Prokhorova,A. V. Sabourov,I. E. Sleptsov,G. G. Struchkov

Bulletin of The Russian Academy of Sciences: Physics（2009）

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摘要

The energy spectrum obtained on the Yakutsk array for the parameter S 600 is compared with the results obtained on the AGASA and HiRes arrays and the latest Pierre Auger Observatory data. The discrepancy in the intensity of the energy spectra obtained in different experiments can be explained by the presence of systematic errors in shower energy estimations.

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Cosmic ray energy spectrum (>1017 eV) of the Yakutsk EAS array

Cosmic ray energy spectrum (>10¹⁷ eV) of the Yakutsk EAS array