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 differen...
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ftdatacite:10.48550/arxiv.1612.08603 2023-05-15T18:45:18+02:00 Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle Abdulsttar, Marwah M. Al-Rubaiee, A. A. Ali, Abdul Halim Kh. 2016 https://dx.doi.org/10.48550/arxiv.1612.08603 https://arxiv.org/abs/1612.08603 unknown arXiv https://dx.doi.org/10.18052/www.scipress.com/ilcpa.67.21 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences article-journal Article ScholarlyArticle Text 2016 ftdatacite https://doi.org/10.48550/arxiv.1612.08603 https://doi.org/10.18052/www.scipress.com/ilcpa.67.21 2022-04-01T10:48:08Z 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 parameterized CLLDF with that simulated with Yakutsk EAS array is verified. The parameterized CLLDF also is compared with that measured on the Yakutsk EAS array. : 10 pages, 7 figures, published in International Letters of Chemistry, Physics and Astronomy Journal Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
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High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences Abdulsttar, Marwah M. Al-Rubaiee, A. A. Ali, Abdul Halim Kh. Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
description |
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 parameterized CLLDF with that simulated with Yakutsk EAS array is verified. The parameterized CLLDF also is compared with that measured on the Yakutsk EAS array. : 10 pages, 7 figures, published in International Letters of Chemistry, Physics and Astronomy Journal |
format |
Text |
author |
Abdulsttar, Marwah M. Al-Rubaiee, A. A. Ali, Abdul Halim Kh. |
author_facet |
Abdulsttar, Marwah M. Al-Rubaiee, A. A. Ali, Abdul Halim Kh. |
author_sort |
Abdulsttar, Marwah M. |
title |
Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle |
title_short |
Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle |
title_full |
Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle |
title_fullStr |
Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle |
title_full_unstemmed |
Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle |
title_sort |
demonstrating of cosmic ray characteristics by estimating the cherenkov light lateral distribution function for yakutsk array as a function of the zenith angle |
publisher |
arXiv |
publishDate |
2016 |
url |
https://dx.doi.org/10.48550/arxiv.1612.08603 https://arxiv.org/abs/1612.08603 |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
Yakutsk |
op_relation |
https://dx.doi.org/10.18052/www.scipress.com/ilcpa.67.21 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1612.08603 https://doi.org/10.18052/www.scipress.com/ilcpa.67.21 |
_version_ |
1766236348914597888 |