The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies
The energies of the most energetic extensive air showers observed at the Yakutsk array have been estimated with help of the all detectors readings instead of using of the standard procedure with a parameter s(600). The energy of the most energetic extensive air shower observed at the Yakutsk array h...
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ftdatacite:10.48550/arxiv.0912.1473 2023-05-15T18:45:21+02:00 The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies Dedenko, L. G. Glushkov, A. V. Fedorova, G. F. Knurenko, S. P. Makarov, I. T. Podgrudkov, D. A. Pravdin, M. I. Roganova, T. M. Sleptzov, I. Ye. 2009 https://dx.doi.org/10.48550/arxiv.0912.1473 https://arxiv.org/abs/0912.1473 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 Preprint Article article CreativeWork 2009 ftdatacite https://doi.org/10.48550/arxiv.0912.1473 2022-04-01T14:49:41Z The energies of the most energetic extensive air showers observed at the Yakutsk array have been estimated with help of the all detectors readings instead of using of the standard procedure with a parameter s(600). The energy of the most energetic extensive air shower observed at the Yakutsk array happened to be 200, 200, 180 and 165 EeV with the values of the Xi**2 function per one degree of freedom 0.9, 1., 0.9 and 1.1 for the primary protons and helium, oxygen and iron nuclei accordingly. : 4 pages, 1 figure, 31 ICRC Report 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 Dedenko, L. G. Glushkov, A. V. Fedorova, G. F. Knurenko, S. P. Makarov, I. T. Podgrudkov, D. A. Pravdin, M. I. Roganova, T. M. Sleptzov, I. Ye. The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
The energies of the most energetic extensive air showers observed at the Yakutsk array have been estimated with help of the all detectors readings instead of using of the standard procedure with a parameter s(600). The energy of the most energetic extensive air shower observed at the Yakutsk array happened to be 200, 200, 180 and 165 EeV with the values of the Xi**2 function per one degree of freedom 0.9, 1., 0.9 and 1.1 for the primary protons and helium, oxygen and iron nuclei accordingly. : 4 pages, 1 figure, 31 ICRC |
format |
Report |
author |
Dedenko, L. G. Glushkov, A. V. Fedorova, G. F. Knurenko, S. P. Makarov, I. T. Podgrudkov, D. A. Pravdin, M. I. Roganova, T. M. Sleptzov, I. Ye. |
author_facet |
Dedenko, L. G. Glushkov, A. V. Fedorova, G. F. Knurenko, S. P. Makarov, I. T. Podgrudkov, D. A. Pravdin, M. I. Roganova, T. M. Sleptzov, I. Ye. |
author_sort |
Dedenko, L. G. |
title |
The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
title_short |
The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
title_full |
The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
title_fullStr |
The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
title_full_unstemmed |
The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
title_sort |
possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies |
publisher |
arXiv |
publishDate |
2009 |
url |
https://dx.doi.org/10.48550/arxiv.0912.1473 https://arxiv.org/abs/0912.1473 |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
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.0912.1473 |
_version_ |
1766236394925064192 |