  The simulation of Cherenkov light lateral distribution function (CLLDF) in
Extensive Air Showers (EAS) was performed by using the Monte Carlo CORSIKA code
for configurations of Tunka-133 EAS Cherenkov array. This simulation was
carried out for different primary particles (e+, e-, p, O, Ar and Fe) around
the knee region with the energy 3.10^15 eV at different zenith angles. By
depending on the Breit-Wigner function a parameterization of CLLDF was
reconstructed on the basis of this simulation as a function of the zenith
angle. The parameterized CLLDF was verified for four fixed zenith angles in
comparison with the simulation that performed using CORSIKA code for each
primary particle.
