Galactic origin of ultrahigh energy cosmic rays
The arrival directions of ultrahigh energy extensive air showers (EAS) by Yakutsk, AGASA, P. Auger array data are analyzed. For the first time, the maps of equal exposition of celestial sphere for the distribution of particles by AGASA and P. Auger arrays data have been constructed. The large-scale...
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ftdatacite:10.48550/arxiv.0902.2609 2023-05-15T18:45:20+02:00 Galactic origin of ultrahigh energy cosmic rays Mikhailov, A. A. 2009 https://dx.doi.org/10.48550/arxiv.0902.2609 https://arxiv.org/abs/0902.2609 unknown arXiv https://dx.doi.org/10.1016/j.nuclphysbps.2009.03.086 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 2009 ftdatacite https://doi.org/10.48550/arxiv.0902.2609 https://doi.org/10.1016/j.nuclphysbps.2009.03.086 2022-04-01T15:05:49Z The arrival directions of ultrahigh energy extensive air showers (EAS) by Yakutsk, AGASA, P. Auger array data are analyzed. For the first time, the maps of equal exposition of celestial sphere for the distribution of particles by AGASA and P. Auger arrays data have been constructed. The large-scale anisotropy of cosmic particles at E>4.1019 eV by Yakutsk, AGASA and P. Auger array data has been detected. The problem of cosmic particle origin is discussed. : 6 pages, 7 figures 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 FOS Physical sciences |
spellingShingle |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences Mikhailov, A. A. Galactic origin of ultrahigh energy cosmic rays |
topic_facet |
High Energy Astrophysical Phenomena astro-ph.HE FOS Physical sciences |
description |
The arrival directions of ultrahigh energy extensive air showers (EAS) by Yakutsk, AGASA, P. Auger array data are analyzed. For the first time, the maps of equal exposition of celestial sphere for the distribution of particles by AGASA and P. Auger arrays data have been constructed. The large-scale anisotropy of cosmic particles at E>4.1019 eV by Yakutsk, AGASA and P. Auger array data has been detected. The problem of cosmic particle origin is discussed. : 6 pages, 7 figures |
format |
Text |
author |
Mikhailov, A. A. |
author_facet |
Mikhailov, A. A. |
author_sort |
Mikhailov, A. A. |
title |
Galactic origin of ultrahigh energy cosmic rays |
title_short |
Galactic origin of ultrahigh energy cosmic rays |
title_full |
Galactic origin of ultrahigh energy cosmic rays |
title_fullStr |
Galactic origin of ultrahigh energy cosmic rays |
title_full_unstemmed |
Galactic origin of ultrahigh energy cosmic rays |
title_sort |
galactic origin of ultrahigh energy cosmic rays |
publisher |
arXiv |
publishDate |
2009 |
url |
https://dx.doi.org/10.48550/arxiv.0902.2609 https://arxiv.org/abs/0902.2609 |
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Yakutsk |
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Yakutsk |
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Yakutsk |
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Yakutsk |
op_relation |
https://dx.doi.org/10.1016/j.nuclphysbps.2009.03.086 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0902.2609 https://doi.org/10.1016/j.nuclphysbps.2009.03.086 |
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1766236386685353984 |