Anisotropy in the Directions of Arrival of Muon Bundles Detected at the NEVOD Experimental Complex
Results are presented from studying the anisotropy of the flux of very high-energy cosmic rays on the basis of muon bundles. Events were recorded in the period 2012–2018 by the DECOR coordinate-tracking detector, part of the unique research setup of the NEVOD experimental complex. The results from a...
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Veröffentlicht in: | Bulletin of the Russian Academy of Sciences. Physics 2019-08, Vol.83 (8), p.1038-1040 |
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container_title | Bulletin of the Russian Academy of Sciences. Physics |
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creator | Khokhlov, S. S. Amelchakov, M. B. Vorobyev, V. S. Izhbulyakova, Z. T. Kovylyaeva, A. A. |
description | Results are presented from studying the anisotropy of the flux of very high-energy cosmic rays on the basis of muon bundles. Events were recorded in the period 2012–2018 by the DECOR coordinate-tracking detector, part of the unique research setup of the NEVOD experimental complex. The results from analyzing the anisotropy for two samples of events with muon bundles corresponding to different ranges of primary particle energy (
E
> 10
15
eV and
E
> 10
16
eV) are discussed, and estimates are made of dipole anisotropy parameters (amplitude and phase). |
doi_str_mv | 10.3103/S1062873819080185 |
format | Article |
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E
> 10
15
eV and
E
> 10
16
eV) are discussed, and estimates are made of dipole anisotropy parameters (amplitude and phase).</description><identifier>ISSN: 1062-8738</identifier><identifier>EISSN: 1934-9432</identifier><identifier>DOI: 10.3103/S1062873819080185</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Anisotropy ; Bundles ; Bundling ; Cosmic rays ; Dipoles ; Direction of arrival ; Hadrons ; Heavy Ions ; Muons ; Nuclear Physics ; Particle energy ; Physics ; Physics and Astronomy</subject><ispartof>Bulletin of the Russian Academy of Sciences. Physics, 2019-08, Vol.83 (8), p.1038-1040</ispartof><rights>Allerton Press, Inc. 2019</rights><rights>Copyright Springer Nature B.V. 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c1835-ec75480cd44598073463a5cf9c353127362cebe785ca8702219534b166e4330c3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.3103/S1062873819080185$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.3103/S1062873819080185$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,777,781,27905,27906,41469,42538,51300</link.rule.ids></links><search><creatorcontrib>Khokhlov, S. S.</creatorcontrib><creatorcontrib>Amelchakov, M. B.</creatorcontrib><creatorcontrib>Vorobyev, V. S.</creatorcontrib><creatorcontrib>Izhbulyakova, Z. T.</creatorcontrib><creatorcontrib>Kovylyaeva, A. A.</creatorcontrib><title>Anisotropy in the Directions of Arrival of Muon Bundles Detected at the NEVOD Experimental Complex</title><title>Bulletin of the Russian Academy of Sciences. Physics</title><addtitle>Bull. Russ. Acad. Sci. Phys</addtitle><description>Results are presented from studying the anisotropy of the flux of very high-energy cosmic rays on the basis of muon bundles. Events were recorded in the period 2012–2018 by the DECOR coordinate-tracking detector, part of the unique research setup of the NEVOD experimental complex. The results from analyzing the anisotropy for two samples of events with muon bundles corresponding to different ranges of primary particle energy (
E
> 10
15
eV and
E
> 10
16
eV) are discussed, and estimates are made of dipole anisotropy parameters (amplitude and phase).</description><subject>Anisotropy</subject><subject>Bundles</subject><subject>Bundling</subject><subject>Cosmic rays</subject><subject>Dipoles</subject><subject>Direction of arrival</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Muons</subject><subject>Nuclear Physics</subject><subject>Particle energy</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><issn>1062-8738</issn><issn>1934-9432</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1kEtPwzAQhCMEEqXwA7hZ4hywvXZiH0tbHlKhBx7XKHU3kCq1g52g9t_jUiQOiNOONPPNrjZJzhm9BEbh6onRjKscFNNUUabkQTJgGkSqBfDDqKOd7vzj5CSEFaVSai4HyWJk6-A679otqS3p3pFMao-mq50NxFVk5H39WTY7-dA7S657u2wwkAl2MYVLUnbf1OP0dT4h002Lvl6j7SIyduu2wc1pclSVTcCznzlMXm6mz-O7dDa_vR-PZqlhCmSKJpdCUbMUQmpFcxAZlNJU2oAExnPIuMEF5kqaUuWUc6YliAXLMhQA1MAwudj3tt599Bi6YuV6b-PKgnOtRSQlxBTbp4x3IXisijYeXPptwWixe2Xx55WR4XsmxKx9Q__b_D_0BTDrc04</recordid><startdate>20190801</startdate><enddate>20190801</enddate><creator>Khokhlov, S. S.</creator><creator>Amelchakov, M. B.</creator><creator>Vorobyev, V. S.</creator><creator>Izhbulyakova, Z. T.</creator><creator>Kovylyaeva, A. A.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20190801</creationdate><title>Anisotropy in the Directions of Arrival of Muon Bundles Detected at the NEVOD Experimental Complex</title><author>Khokhlov, S. S. ; Amelchakov, M. B. ; Vorobyev, V. S. ; Izhbulyakova, Z. T. ; Kovylyaeva, A. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1835-ec75480cd44598073463a5cf9c353127362cebe785ca8702219534b166e4330c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Anisotropy</topic><topic>Bundles</topic><topic>Bundling</topic><topic>Cosmic rays</topic><topic>Dipoles</topic><topic>Direction of arrival</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Muons</topic><topic>Nuclear Physics</topic><topic>Particle energy</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Khokhlov, S. S.</creatorcontrib><creatorcontrib>Amelchakov, M. B.</creatorcontrib><creatorcontrib>Vorobyev, V. S.</creatorcontrib><creatorcontrib>Izhbulyakova, Z. T.</creatorcontrib><creatorcontrib>Kovylyaeva, A. A.</creatorcontrib><collection>CrossRef</collection><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Khokhlov, S. S.</au><au>Amelchakov, M. B.</au><au>Vorobyev, V. S.</au><au>Izhbulyakova, Z. T.</au><au>Kovylyaeva, A. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Anisotropy in the Directions of Arrival of Muon Bundles Detected at the NEVOD Experimental Complex</atitle><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle><stitle>Bull. Russ. Acad. Sci. Phys</stitle><date>2019-08-01</date><risdate>2019</risdate><volume>83</volume><issue>8</issue><spage>1038</spage><epage>1040</epage><pages>1038-1040</pages><issn>1062-8738</issn><eissn>1934-9432</eissn><abstract>Results are presented from studying the anisotropy of the flux of very high-energy cosmic rays on the basis of muon bundles. Events were recorded in the period 2012–2018 by the DECOR coordinate-tracking detector, part of the unique research setup of the NEVOD experimental complex. The results from analyzing the anisotropy for two samples of events with muon bundles corresponding to different ranges of primary particle energy (
E
> 10
15
eV and
E
> 10
16
eV) are discussed, and estimates are made of dipole anisotropy parameters (amplitude and phase).</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.3103/S1062873819080185</doi><tpages>3</tpages></addata></record> |
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subjects | Anisotropy Bundles Bundling Cosmic rays Dipoles Direction of arrival Hadrons Heavy Ions Muons Nuclear Physics Particle energy Physics Physics and Astronomy |
title | Anisotropy in the Directions of Arrival of Muon Bundles Detected at the NEVOD Experimental Complex |
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