Simulation of Lateral Distribution Function of Cherenkov Light in Extensive Air Showers for Yakutsk Array
Main Article Content
Abstract
The simulation of Cherenkov light Lateral distribution function (LDF) for
primary particles like primary protons, Iron nuclei, Oxygen, Nitrogen, Calcium,
Neutron and Argon have been performed with CORSIKA code for conditions
and configuration of Yakutsk array in the energy range 1014
-1016 eV for four
zenith angles 0o
, 5
o
, 10o and 15o
. The results of this simulation are compared
with the measurements of Yakutsk array for the same particles and energy
range
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How to Cite
Simulation of Lateral Distribution Function of Cherenkov Light in Extensive Air Showers for Yakutsk Array. (2023). Journal of the College of Basic Education, 18(74), 1-6. https://doi.org/10.35950/cbej.v18i74.8638
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Section
Articles for the humanities and pure sciences
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How to Cite
Simulation of Lateral Distribution Function of Cherenkov Light in Extensive Air Showers for Yakutsk Array. (2023). Journal of the College of Basic Education, 18(74), 1-6. https://doi.org/10.35950/cbej.v18i74.8638