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Cherenkov Light Lateral Distribution Function Estimation as a Function of Zenith Angle

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arxiv 1711.00512 v1 pith:WARLXLFS submitted 2017-10-27 astro-ph.IM astro-ph.HE

Marwah M. Abdulsttar , A. A. Al-Rubaiee This is my paper · ORCID
classification astro-ph.IMastro-ph.HE
keywords functionsimulationzenithcherenkovclldfangleanglescode
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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.

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