The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers

In terms of the quark-gluon string model the analysis of the classic procedure to estimate the energy of giant air showers with help of the parameter s(600) (a density of energy deposition in the scintillator at a distance of 600 m from the shower core) have been carried out. Simulations of the sign...

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Main Authors: Dedenko, L. G., Podgrudkov, D. A., Roganova, T. M., Fedorova, G. F., Fedunin, E. Yu., Shozieev, G. P.
Format: Text
Language:unknown
Published: arXiv 2007
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Online Access:https://dx.doi.org/10.48550/arxiv.astro-ph/0703015
https://arxiv.org/abs/astro-ph/0703015
id ftdatacite:10.48550/arxiv.astro-ph/0703015
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spelling ftdatacite:10.48550/arxiv.astro-ph/0703015 2023-05-15T18:45:28+02:00 The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers Dedenko, L. G. Podgrudkov, D. A. Roganova, T. M. Fedorova, G. F. Fedunin, E. Yu. Shozieev, G. P. 2007 https://dx.doi.org/10.48550/arxiv.astro-ph/0703015 https://arxiv.org/abs/astro-ph/0703015 unknown arXiv https://dx.doi.org/10.1134/s1063778807100122 Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004 http://arxiv.org/licenses/assumed-1991-2003/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2007 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0703015 https://doi.org/10.1134/s1063778807100122 2022-04-01T15:40:29Z In terms of the quark-gluon string model the analysis of the classic procedure to estimate the energy of giant air showers with help of the parameter s(600) (a density of energy deposition in the scintillator at a distance of 600 m from the shower core) have been carried out. Simulations of the signal s(600) with help of the CORSIKA code in terms of the hybrid scheme show energy estimates which are approximately a factor of 1.6 times lower than adopted at the Yakutsk array. The energy estimates calculated with the help of the Cherenkov radiation coincide with the experimental data. Simulations of deposited energy distributions in the atmosphere with help of the GEANT4 code and the CORSIKA code show that more than 20% of this energy may be deposited at distances above 100 m from the shower axis. : 10 pages, 5 figures Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Astrophysics astro-ph
FOS Physical sciences
spellingShingle Astrophysics astro-ph
FOS Physical sciences
Dedenko, L. G.
Podgrudkov, D. A.
Roganova, T. M.
Fedorova, G. F.
Fedunin, E. Yu.
Shozieev, G. P.
The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
topic_facet Astrophysics astro-ph
FOS Physical sciences
description In terms of the quark-gluon string model the analysis of the classic procedure to estimate the energy of giant air showers with help of the parameter s(600) (a density of energy deposition in the scintillator at a distance of 600 m from the shower core) have been carried out. Simulations of the signal s(600) with help of the CORSIKA code in terms of the hybrid scheme show energy estimates which are approximately a factor of 1.6 times lower than adopted at the Yakutsk array. The energy estimates calculated with the help of the Cherenkov radiation coincide with the experimental data. Simulations of deposited energy distributions in the atmosphere with help of the GEANT4 code and the CORSIKA code show that more than 20% of this energy may be deposited at distances above 100 m from the shower axis. : 10 pages, 5 figures
format Text
author Dedenko, L. G.
Podgrudkov, D. A.
Roganova, T. M.
Fedorova, G. F.
Fedunin, E. Yu.
Shozieev, G. P.
author_facet Dedenko, L. G.
Podgrudkov, D. A.
Roganova, T. M.
Fedorova, G. F.
Fedunin, E. Yu.
Shozieev, G. P.
author_sort Dedenko, L. G.
title The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
title_short The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
title_full The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
title_fullStr The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
title_full_unstemmed The use of the Cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
title_sort use of the cherenkov radiation and the fluorescence light to calibrate the energy of giant air showers
publisher arXiv
publishDate 2007
url https://dx.doi.org/10.48550/arxiv.astro-ph/0703015
https://arxiv.org/abs/astro-ph/0703015
geographic Yakutsk
geographic_facet Yakutsk
genre Yakutsk
genre_facet Yakutsk
op_relation https://dx.doi.org/10.1134/s1063778807100122
op_rights Assumed arXiv.org perpetual, non-exclusive license to distribute this article for submissions made before January 2004
http://arxiv.org/licenses/assumed-1991-2003/
op_doi https://doi.org/10.48550/arxiv.astro-ph/0703015
https://doi.org/10.1134/s1063778807100122
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