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A spectrum of cosmic rays within energy range 10^15 - 3x10^17 eV was derivedfrom the data of the small Cherenkov setup, which is a part of the Yakutskcomplex EAS array. In this, work a new series of observation is covered. Theseobservations lasted from 2000 till 2010 and resulted in increased number ofregistered events within interval 10^16 - 10^18 eV, which in turn made itpossible to reproduce cosmic ray spectrum in this energy domain with betterprecision. A sign of a thin structure is observed in the shape of the spectrum.It could be related to the escape of heavy nuclei from our Galaxy. Cosmic raymass composition was obtained for the energy region 10^16 - 10^18 eV. A jointanalysis of spectrum and mass composition of cosmic rays was performed.Obtained results are considered in the context of theoretical computations thatwere performed with the use of hypothesis of galactic and meta-galactic originof cosmic rays.

Spectrum and mass composition of cosmic rays in the energy range 10^15-10^18 eV derived from the Yakutsk array data