Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array
The lateral distribution of muons with ~1.0x\sec(θ) GeV in extensive air showers within ~10^{17}-10^{19} eV energy region obtained during different observational periods from November 1987 to June 2013 has been analyzed. Experimental data have been compared to predictions of various hadron interacti...
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ftdatacite:10.48550/arxiv.1311.1570 2023-05-15T18:45:25+02:00 Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array Glushkov, A. V. Sabourov, A. 2013 https://dx.doi.org/10.48550/arxiv.1311.1570 https://arxiv.org/abs/1311.1570 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences article-journal Article ScholarlyArticle Text 2013 ftdatacite https://doi.org/10.48550/arxiv.1311.1570 2022-04-01T13:11:57Z The lateral distribution of muons with ~1.0x\sec(θ) GeV in extensive air showers within ~10^{17}-10^{19} eV energy region obtained during different observational periods from November 1987 to June 2013 has been analyzed. Experimental data have been compared to predictions of various hadron interaction models. The best agreement is observed with QGSJETII-04. Until 1996, the mass composition of cosmic rays with energy below 2x10^{18} eV was significantly lighter than in later periods. : 10 pages, 4 figures. arXiv admin note: substantial text overlap with arXiv:1310.0561 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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topic |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
spellingShingle |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Glushkov, A. V. Sabourov, A. Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
The lateral distribution of muons with ~1.0x\sec(θ) GeV in extensive air showers within ~10^{17}-10^{19} eV energy region obtained during different observational periods from November 1987 to June 2013 has been analyzed. Experimental data have been compared to predictions of various hadron interaction models. The best agreement is observed with QGSJETII-04. Until 1996, the mass composition of cosmic rays with energy below 2x10^{18} eV was significantly lighter than in later periods. : 10 pages, 4 figures. arXiv admin note: substantial text overlap with arXiv:1310.0561 |
format |
Text |
author |
Glushkov, A. V. Sabourov, A. |
author_facet |
Glushkov, A. V. Sabourov, A. |
author_sort |
Glushkov, A. V. |
title |
Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array |
title_short |
Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array |
title_full |
Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array |
title_fullStr |
Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array |
title_full_unstemmed |
Variations of the cosmic ray composition at energy above 0.1 EeV as observed by muon detectors of Yakutsk array |
title_sort |
variations of the cosmic ray composition at energy above 0.1 eev as observed by muon detectors of yakutsk array |
publisher |
arXiv |
publishDate |
2013 |
url |
https://dx.doi.org/10.48550/arxiv.1311.1570 https://arxiv.org/abs/1311.1570 |
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Yakutsk |
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Yakutsk |
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Yakutsk |
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Yakutsk |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1311.1570 |
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1766236467492814848 |