Energy spectrum of cosmic rays at E_0>1017 eV by the Yakutsk eas array data

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Scientific paper

The energy spectrum of primary cosmic rays with the energy EO > 1017 eV by using the Yakutsk EAS array data is presented. The experimentally obtained relation between EO and S300 (the particle density at the distance of 300 m from a shower core) and the comparison with calculations according to the QGSJet model are given. The irregularity of a spectrum form in the region of 2ṡ1018 - 4ṡ1019 eV using the single parameter S300 is also investigated. The obtained energy spectrum is compared with the last AGASA results.

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