Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array

The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the showe...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:JETP letters 2019, Vol.109 (9), p.559-563
Hauptverfasser: Glushkov, A. V., Saburov, A. V.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 563
container_issue 9
container_start_page 559
container_title JETP letters
container_volume 109
creator Glushkov, A. V.
Saburov, A. V.
description The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of (1–30) × 10 17 eV changes from middle nuclei to a purely proton composition.
doi_str_mv 10.1134/S0021364019090091
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2257270481</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2257270481</sourcerecordid><originalsourceid>FETCH-LOGICAL-c1611-ffa35e0494809b8d2740912b02779c88d9bccd27754a891f2a53c326fbf1a5913</originalsourceid><addsrcrecordid>eNp1UMtOwzAQtBBIlMIHcLPEOeB1nDg-Rm15SK2QKCBxihzXbtOSuNgOqFe-nIQicUCcdnd2ZlY7CJ0DuQSI2dWcEApxyggIIggRcIAG0HVRyjJ-iAb9Our3x-jE-zUhAFnMB-hzJr3HI1tvra9CZRtsTTf6ulL4Qe48_qjCCk8a7ZaV9liW9l1jIMCxfsa5UtYtqmaJg8VhpfFYBomNs_X3NGs7u7EOWgXrfG_coy9y0wa_wZN8jnPn5O4UHRn56vXZTx2ip-vJ4-g2mt7f3I3yaaQgBYiMkXGiCRMsI6LMFpSz7k1aEsq5UFm2EKVSHcoTJjMBhsokVjFNTWlAJgLiIbrY-26dfWu1D8Xatq7pThaUJpxywrKeBXuWctZ7p02xdVUt3a4AUvRRF3-i7jR0r_Edt1lq9-v8v-gLe4R9xA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2257270481</pqid></control><display><type>article</type><title>Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array</title><source>SpringerNature Journals</source><creator>Glushkov, A. V. ; Saburov, A. V.</creator><creatorcontrib>Glushkov, A. V. ; Saburov, A. V.</creatorcontrib><description>The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of (1–30) × 10 17 eV changes from middle nuclei to a purely proton composition.</description><identifier>ISSN: 0021-3640</identifier><identifier>EISSN: 1090-6487</identifier><identifier>DOI: 10.1134/S0021364019090091</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Arrays ; Astrophysics and Cosmology ; Atomic ; Biological and Medical Physics ; Biophysics ; Composition ; Cosmic ray showers ; Cosmic rays ; Detectors ; Flux density ; Molecular ; Muons ; Nuclei (nuclear physics) ; Optical and Plasma Physics ; Particle and Nuclear Physics ; Physics ; Physics and Astronomy ; Quantum Information Technology ; Solid State Physics ; Spintronics</subject><ispartof>JETP letters, 2019, Vol.109 (9), p.559-563</ispartof><rights>Pleiades Publishing, Inc. 2019</rights><rights>Copyright Springer Nature B.V. 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c1611-ffa35e0494809b8d2740912b02779c88d9bccd27754a891f2a53c326fbf1a5913</citedby><cites>FETCH-LOGICAL-c1611-ffa35e0494809b8d2740912b02779c88d9bccd27754a891f2a53c326fbf1a5913</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0021364019090091$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0021364019090091$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>315,782,786,27931,27932,41495,42564,51326</link.rule.ids></links><search><creatorcontrib>Glushkov, A. V.</creatorcontrib><creatorcontrib>Saburov, A. V.</creatorcontrib><title>Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array</title><title>JETP letters</title><addtitle>Jetp Lett</addtitle><description>The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of (1–30) × 10 17 eV changes from middle nuclei to a purely proton composition.</description><subject>Arrays</subject><subject>Astrophysics and Cosmology</subject><subject>Atomic</subject><subject>Biological and Medical Physics</subject><subject>Biophysics</subject><subject>Composition</subject><subject>Cosmic ray showers</subject><subject>Cosmic rays</subject><subject>Detectors</subject><subject>Flux density</subject><subject>Molecular</subject><subject>Muons</subject><subject>Nuclei (nuclear physics)</subject><subject>Optical and Plasma Physics</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Information Technology</subject><subject>Solid State Physics</subject><subject>Spintronics</subject><issn>0021-3640</issn><issn>1090-6487</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1UMtOwzAQtBBIlMIHcLPEOeB1nDg-Rm15SK2QKCBxihzXbtOSuNgOqFe-nIQicUCcdnd2ZlY7CJ0DuQSI2dWcEApxyggIIggRcIAG0HVRyjJ-iAb9Our3x-jE-zUhAFnMB-hzJr3HI1tvra9CZRtsTTf6ulL4Qe48_qjCCk8a7ZaV9liW9l1jIMCxfsa5UtYtqmaJg8VhpfFYBomNs_X3NGs7u7EOWgXrfG_coy9y0wa_wZN8jnPn5O4UHRn56vXZTx2ip-vJ4-g2mt7f3I3yaaQgBYiMkXGiCRMsI6LMFpSz7k1aEsq5UFm2EKVSHcoTJjMBhsokVjFNTWlAJgLiIbrY-26dfWu1D8Xatq7pThaUJpxywrKeBXuWctZ7p02xdVUt3a4AUvRRF3-i7jR0r_Edt1lq9-v8v-gLe4R9xA</recordid><startdate>2019</startdate><enddate>2019</enddate><creator>Glushkov, A. V.</creator><creator>Saburov, A. V.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>2019</creationdate><title>Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array</title><author>Glushkov, A. V. ; Saburov, A. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1611-ffa35e0494809b8d2740912b02779c88d9bccd27754a891f2a53c326fbf1a5913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Arrays</topic><topic>Astrophysics and Cosmology</topic><topic>Atomic</topic><topic>Biological and Medical Physics</topic><topic>Biophysics</topic><topic>Composition</topic><topic>Cosmic ray showers</topic><topic>Cosmic rays</topic><topic>Detectors</topic><topic>Flux density</topic><topic>Molecular</topic><topic>Muons</topic><topic>Nuclei (nuclear physics)</topic><topic>Optical and Plasma Physics</topic><topic>Particle and Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Information Technology</topic><topic>Solid State Physics</topic><topic>Spintronics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Glushkov, A. V.</creatorcontrib><creatorcontrib>Saburov, A. V.</creatorcontrib><collection>CrossRef</collection><jtitle>JETP letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Glushkov, A. V.</au><au>Saburov, A. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array</atitle><jtitle>JETP letters</jtitle><stitle>Jetp Lett</stitle><date>2019</date><risdate>2019</risdate><volume>109</volume><issue>9</issue><spage>559</spage><epage>563</epage><pages>559-563</pages><issn>0021-3640</issn><eissn>1090-6487</eissn><abstract>The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of (1–30) × 10 17 eV changes from middle nuclei to a purely proton composition.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0021364019090091</doi><tpages>5</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0021-3640
ispartof JETP letters, 2019, Vol.109 (9), p.559-563
issn 0021-3640
1090-6487
language eng
recordid cdi_proquest_journals_2257270481
source SpringerNature Journals
subjects Arrays
Astrophysics and Cosmology
Atomic
Biological and Medical Physics
Biophysics
Composition
Cosmic ray showers
Cosmic rays
Detectors
Flux density
Molecular
Muons
Nuclei (nuclear physics)
Optical and Plasma Physics
Particle and Nuclear Physics
Physics
Physics and Astronomy
Quantum Information Technology
Solid State Physics
Spintronics
title Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-06T01%3A23%3A34IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Mass%20Composition%20of%20Cosmic%20Rays%20with%20Energies%20above%201017%20eV%20According%20to%20the%20Data%20from%20the%20Muon%20Detectors%20of%20the%20Yakutsk%20EAS%20Array&rft.jtitle=JETP%20letters&rft.au=Glushkov,%20A.%20V.&rft.date=2019&rft.volume=109&rft.issue=9&rft.spage=559&rft.epage=563&rft.pages=559-563&rft.issn=0021-3640&rft.eissn=1090-6487&rft_id=info:doi/10.1134/S0021364019090091&rft_dat=%3Cproquest_cross%3E2257270481%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2257270481&rft_id=info:pmid/&rfr_iscdi=true