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Parameterization of Cherenkov Light Lateral Distribution Function as a Function of the Zenith Angle around the Knee Region

2016/05/01 by Marwah M. Abdulsttar, A. A. Al-Rubaiee, Abdul Halim Kh. Ali +1
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Cherenkov radiation #Dark Matter and Cosmic Phenomena #Function (biology) #Neutrino Physics Research #Nuclear physics #Optics #Physics #Proton #Zenith #astro-ph.HE #astro-ph.IM

paper · pdf · doi:10.18052/www.scipress.com/ilcpa.66.71

published in International Letters of Chemistry Physics and Astronomy 66, 71-78 (SciPress Ltd.) · 9 pages. 6 figures, published in International Letters of Chemistry, Physics and Astronomy Journal

openalex publication_date 2016/05/01 · openalex created_date 2016/06/24 · arxiv created 2016/12/15 · arxiv updated 2016/12/28 · openalex updated_date 2026/08/05

Abstract

Cherenkov light lateral distribution function (CLLDF) simulation was fullfiled using CORSIKA code for configurations of Tunka EAS array for different zenith angles. The parameterization of the CLLDF was carried out as a function of the destance from tehe shower core in extensive air showers (EAS) and zenith angle on the basis of the CORSIKA simulation for primary proton around the knee region with the energy 3.10 15 eV at different zenith angles. The parametrized CLLDF is verified in comparison with the simulation that performed using CORSIKA code for two zenith angles.

Citations