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Cherenkov light lateral distribution function (CLLDF) in Extensive AirShowers (EAS) for different primary particles (e-, n , p, F, K and Fe) wassimulated using CORSIKA code for conditions and configurations of Yakutsk EASarray with the fixed primary energy 3 PeV around the knee region at differentzenith angles. Basing on the results of CLLDF numerical simulation, sets ofapproximated functions are reconstructed for different primary particles as afunction of the zenith angle. A comparison of the parameterized CLLDF with thatsimulated with Yakutsk EAS array is verified. The parameterized CLLDF also iscompared with that measured on the Yakutsk EAS array.

international letters of chemistry, physics and astronomy

Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov  Light Lateral Distribution Function for Yakutsk Array as a Function of the  Zenith Angle