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.
@article{arxiv.1711.00512,
title = {Cherenkov Light Lateral Distribution Function Estimation as a Function of Zenith Angle},
author = {Marwah M. Abdulsttar and A. A. Al-Rubaiee},
journal= {arXiv preprint arXiv:1711.00512},
year = {2017}
}
Comments
7 pages, 4 figures, Journal of Applied Physical Science International