Extensive air showers without muon component
Extensive air showers of cosmic rays with energies above 5.10**18 eV registered by the Yakutsk array have been analyzed. The existence of showers without muon component is found. Among them we found 5 clusters and these clusters correlate with nearest pulsars. It is found that there exist 4 classes...
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ftdatacite:10.48550/arxiv.astro-ph/0507680 2023-05-15T18:45:24+02:00 Extensive air showers without muon component Mikhailov, A. A. Efremov, N. N. Nikiforova, E. S. 2005 https://dx.doi.org/10.48550/arxiv.astro-ph/0507680 https://arxiv.org/abs/astro-ph/0507680 unknown arXiv 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 Preprint Article article CreativeWork 2005 ftdatacite https://doi.org/10.48550/arxiv.astro-ph/0507680 2022-04-01T16:15:19Z Extensive air showers of cosmic rays with energies above 5.10**18 eV registered by the Yakutsk array have been analyzed. The existence of showers without muon component is found. Among them we found 5 clusters and these clusters correlate with nearest pulsars. It is found that there exist 4 classes of showers. Showers with high content of muons are mainly observed at E> 4.10**19 eV and they are formed most likely by heavy nuclei. : 4 pages, 2 figures, the paper will be publish in Proc. ICRC, Pune, India, 2005 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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unknown |
topic |
Astrophysics astro-ph FOS Physical sciences |
spellingShingle |
Astrophysics astro-ph FOS Physical sciences Mikhailov, A. A. Efremov, N. N. Nikiforova, E. S. Extensive air showers without muon component |
topic_facet |
Astrophysics astro-ph FOS Physical sciences |
description |
Extensive air showers of cosmic rays with energies above 5.10**18 eV registered by the Yakutsk array have been analyzed. The existence of showers without muon component is found. Among them we found 5 clusters and these clusters correlate with nearest pulsars. It is found that there exist 4 classes of showers. Showers with high content of muons are mainly observed at E> 4.10**19 eV and they are formed most likely by heavy nuclei. : 4 pages, 2 figures, the paper will be publish in Proc. ICRC, Pune, India, 2005 |
format |
Report |
author |
Mikhailov, A. A. Efremov, N. N. Nikiforova, E. S. |
author_facet |
Mikhailov, A. A. Efremov, N. N. Nikiforova, E. S. |
author_sort |
Mikhailov, A. A. |
title |
Extensive air showers without muon component |
title_short |
Extensive air showers without muon component |
title_full |
Extensive air showers without muon component |
title_fullStr |
Extensive air showers without muon component |
title_full_unstemmed |
Extensive air showers without muon component |
title_sort |
extensive air showers without muon component |
publisher |
arXiv |
publishDate |
2005 |
url |
https://dx.doi.org/10.48550/arxiv.astro-ph/0507680 https://arxiv.org/abs/astro-ph/0507680 |
geographic |
Yakutsk |
geographic_facet |
Yakutsk |
genre |
Yakutsk |
genre_facet |
Yakutsk |
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/0507680 |
_version_ |
1766236455363936256 |