Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster
The cluster of ultra-high-energy cosmic rays observed by the AGASA, HiRes and Yakutsk experiments is studied with respect to possible deflections of particles in regular magnetic fields. Best-fit positions of a potential source of these clustered particles are found, with account of the errors in en...
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ftdatacite:10.48550/arxiv.astro-ph/0505262 2023-05-15T18:45:22+02:00 Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster Troitsky, S. V. 2005 https://dx.doi.org/10.48550/arxiv.astro-ph/0505262 https://arxiv.org/abs/astro-ph/0505262 unknown arXiv https://dx.doi.org/10.1016/j.astropartphys.2006.07.006 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 2005 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0505262 https://doi.org/10.1016/j.astropartphys.2006.07.006 2022-04-01T16:05:55Z The cluster of ultra-high-energy cosmic rays observed by the AGASA, HiRes and Yakutsk experiments is studied with respect to possible deflections of particles in regular magnetic fields. Best-fit positions of a potential source of these clustered particles are found, with account of the errors in energy estimation, both in the frameworks of particular models of the Galactic magnetic field and treating the direction and the amount of deflection as free parameters. The study suggests that an unknown regular component of either Galactic or extragalactic magnetic field may dominate over modelled components in the direction of the cluster. Possible sources of the cosmic rays in that direction are considered. : 18 pages, 3 eps figures, iopart.cls 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 |
Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences Troitsky, S. V. Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
The cluster of ultra-high-energy cosmic rays observed by the AGASA, HiRes and Yakutsk experiments is studied with respect to possible deflections of particles in regular magnetic fields. Best-fit positions of a potential source of these clustered particles are found, with account of the errors in energy estimation, both in the frameworks of particular models of the Galactic magnetic field and treating the direction and the amount of deflection as free parameters. The study suggests that an unknown regular component of either Galactic or extragalactic magnetic field may dominate over modelled components in the direction of the cluster. Possible sources of the cosmic rays in that direction are considered. : 18 pages, 3 eps figures, iopart.cls |
format |
Text |
author |
Troitsky, S. V. |
author_facet |
Troitsky, S. V. |
author_sort |
Troitsky, S. V. |
title |
Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster |
title_short |
Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster |
title_full |
Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster |
title_fullStr |
Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster |
title_full_unstemmed |
Magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the AGASA-HiRes-Yakutsk cluster |
title_sort |
magnetic deflections and possible sources of the ultra-high-energy cosmic rays in the agasa-hires-yakutsk cluster |
publisher |
arXiv |
publishDate |
2005 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0505262 https://arxiv.org/abs/astro-ph/0505262 |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
Yakutsk |
op_relation |
https://dx.doi.org/10.1016/j.astropartphys.2006.07.006 |
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/0505262 https://doi.org/10.1016/j.astropartphys.2006.07.006 |
_version_ |
1766236407717691392 |