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The simulation of the Cherenkov light lateral distribution function (LDF) inExtensive Air Showers (EAS) was perfomed with the CORSIKA code in the energyrange 10^13-10^16 eV for configuration of the Tunka-25 EAS array. On the basisof this simulation we obtained sets of approximating functions for primaryprotons, iron nuclei and gamma-quanta for zenith angles Theta<=20. Thecomparison of the calculated Cherenkov light LDF with that measured with theTunka-25 array has shown an opportunity of primary particle identification anddefinition of its energy around the "knee".

Parametrization for Cherenkov light lateral distribution function in Extensive Air Showers