2016/06/01 by Marwah M. Abdulsttar, A. A. Al-Rubaiee, A.A. Al-Rubaiee +2
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Cherenkov radiation #Cosmic ray #Dark Matter and Cosmic Phenomena #Distribution function #Function (biology) #Parameterized complexity #Radiation Detection and Scintillator Technologies #Zenith #astro-ph.HE #astro-ph.IM
paper · pdf · open access · doi:10.18052/www.scipress.com/ilcpa.67.21
published in International Letters of Chemistry Physics and Astronomy 67, 21-30 (SciPress Ltd.) · 10 pages, 7 figures, published in International Letters of Chemistry, Physics and Astronomy Journal
openalex publication_date 2016/06/01 · openalex created_date 2016/07/22 · arxiv created 2016/12/15 · arxiv updated 2016/12/28 · openalex updated_date 2026/08/05
Cherenkov light lateral distribution function (CLLDF) in Extensive Air Showers (EAS) for different primary particles (e - , n , p, F, K and Fe) was simulated using CORSIKA code for conditions and configurations of Yakutsk EAS array with the fixed primary energy 3 PeV around the knee region at different zenith angles. Basing on the results of CLLDF numerical simulation, sets of approximated functions are reconstructed for different primary particles as a function of the zenith angle. A comparison of the parametrized CLLDF with that simulated with Yakutsk EAS array is verified.The parameterized CLLDF also is compared with that measured on the Yakutsk EAS array.