Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background

Results are presented that were obtained by analysing the arrival directions of E0 > 8x10**18 eV primary cosmic rays recorded at the Yakutsk array over the period between 1974 and 2003 and at the SUGAR array (Australia). The greatest primary cosmic ray flux is shown to arrive from the region of v...

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Main Author: Glushkov, A. V.
Format: Text
Language:unknown
Published: arXiv 2012
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Yakutsk
Online Access:https://dx.doi.org/10.48550/arxiv.1202.5345
https://arxiv.org/abs/1202.5345
id ftdatacite:10.48550/arxiv.1202.5345
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spelling ftdatacite:10.48550/arxiv.1202.5345 2023-05-15T18:45:25+02:00 Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background Glushkov, A. V. 2012 https://dx.doi.org/10.48550/arxiv.1202.5345 https://arxiv.org/abs/1202.5345 unknown arXiv https://dx.doi.org/10.1134/s1063778808080103 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 2012 ftdatacite https://doi.org/10.48550/arxiv.1202.5345 https://doi.org/10.1134/s1063778808080103 2022-04-01T14:00:42Z Results are presented that were obtained by analysing the arrival directions of E0 > 8x10**18 eV primary cosmic rays recorded at the Yakutsk array over the period between 1974 and 2003 and at the SUGAR array (Australia). The greatest primary cosmic ray flux is shown to arrive from the region of visible intersection of the planes of the Galaxy and the Supergalaxy (local supercluster of galaxies) at a galactic longitude of about 137 degres. On a global scale, the lowest temperature of the cosmic microwave background is typical of this region. : 4 pages, 2 figures Text Yakutsk DataCite Metadata Store (German National Library of Science and Technology) Yakutsk
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
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.
Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
topic_facet High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
description Results are presented that were obtained by analysing the arrival directions of E0 > 8x10**18 eV primary cosmic rays recorded at the Yakutsk array over the period between 1974 and 2003 and at the SUGAR array (Australia). The greatest primary cosmic ray flux is shown to arrive from the region of visible intersection of the planes of the Galaxy and the Supergalaxy (local supercluster of galaxies) at a galactic longitude of about 137 degres. On a global scale, the lowest temperature of the cosmic microwave background is typical of this region. : 4 pages, 2 figures
format Text
author Glushkov, A. V.
author_facet Glushkov, A. V.
author_sort Glushkov, A. V.
title Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
title_short Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
title_full Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
title_fullStr Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
title_full_unstemmed Anisotropy of Arrival Directions of E0 > 8 x 10**18 eV Cosmic Rays and Cosmic Microwave Background
title_sort anisotropy of arrival directions of e0 > 8 x 10**18 ev cosmic rays and cosmic microwave background
publisher arXiv
publishDate 2012
url https://dx.doi.org/10.48550/arxiv.1202.5345
https://arxiv.org/abs/1202.5345
geographic Yakutsk
geographic_facet Yakutsk
genre Yakutsk
genre_facet Yakutsk
op_relation https://dx.doi.org/10.1134/s1063778808080103
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1202.5345
https://doi.org/10.1134/s1063778808080103
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