Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle

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 differ...

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Bibliographic Details
Published in:International Letters of Chemistry, Physics and Astronomy
Main Authors: Abdulsttar, Marwah M., Al-Rubaiee, A.A., Ali, Abdul Halim K.
Format: Article in Journal/Newspaper
Language:unknown
Published: SciPress Ltd 2016
Subjects:
Psychiatry and Mental health
Neuropsychology and Physiological Psychology
Yakutsk
Online Access:http://dx.doi.org/10.18052/www.scipress.com/ilcpa.67.21
https://www.scipress.com/ILCPA.67.21.pdf
Description
Summary: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.

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