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dc.contributor.authorTrzaska, Wladyslaw Henryk
dc.contributor.authorSlupecki, Maciej
dc.contributor.authorBandac, Iulian
dc.contributor.authorBayo, Alberto
dc.contributor.authorBettini, Alessandro
dc.contributor.authorBezrukov, Leonid
dc.contributor.authorEnqvist, Timo
dc.contributor.authorFazliakhmetov, Almaz
dc.contributor.authorIanni, Aldo
dc.contributor.authorInzhechik, Lev
dc.contributor.authorJoutsenvaara, Jari
dc.contributor.authorKuusiniemi, Pasi
dc.contributor.authorLoo, Kai
dc.contributor.authorLubsandorzhiev, Bayarto
dc.contributor.authorNozik, Alexander
dc.contributor.authorPeña Garay, Carlos
dc.contributor.authorPoliakova, Maria
dc.date.accessioned2019-09-02T05:40:41Z
dc.date.available2019-09-02T05:40:41Z
dc.date.issued2019
dc.identifier.citationTrzaska, W. H., Slupecki, M., Bandac, I., Bayo, A., Bettini, A., Bezrukov, L., Enqvist, T., Fazliakhmetov, A., Ianni, A., Inzhechik, L., Joutsenvaara, J., Kuusiniemi, P., Loo, K., Lubsandorzhiev, B., Nozik, A., Peña Garay, C., & Poliakova, M. (2019). Cosmic-ray muon flux at Canfranc Underground Laboratory. <i>European Physical Journal C</i>, <i>79</i>(8), Article 721. <a href="https://doi.org/10.1140/epjc/s10052-019-7239-9" target="_blank">https://doi.org/10.1140/epjc/s10052-019-7239-9</a>
dc.identifier.otherCONVID_32657951
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/65387
dc.description.abstractResidual flux and angular distribution of high-energy cosmic muons have been measured in two underground locations at the Canfranc Underground Laboratory (LSC) using a dedicated Muon Monitor. The instrument consists of three layers of fast scintillation detector modules operating as 352 independent pixels. The monitor has a flux-defining area of 1 m2 and covers all azimuth angles, and zenith angles up to 80∘ . The measured integrated muon flux is (5.26±0.21)×10−3 m−2s−1 in the Hall A of the LAB2400 and (4.29±0.17)×10−3 m−2s−1 in LAB2500. The angular dependence is consistent with the known profile and rock density of the surrounding mountains. In particular, there is a clear maximum in the flux coming from the direction of the Rioseta valley.en
dc.format.mimetypeapplication/pdf
dc.languageeng
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofseriesEuropean Physical Journal C
dc.rightsCC BY 4.0
dc.subject.otherhigh-energy cosmic muons
dc.titleCosmic-ray muon flux at Canfranc Underground Laboratory
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-201909023992
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.contributor.oppiaineYdin- ja kiihdytinfysiikan huippuyksikköfi
dc.contributor.oppiaineFysiikkafi
dc.contributor.oppiaineCentre of Excellence in Nuclear and Accelerator Based Physicsen
dc.contributor.oppiainePhysicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.type.coarhttp://purl.org/coar/resource_type/c_2df8fbb1
dc.description.reviewstatuspeerReviewed
dc.relation.issn1434-6044
dc.relation.numberinseries8
dc.relation.volume79
dc.type.versionpublishedVersion
dc.rights.copyright© The Author(s) 2019
dc.rights.accesslevelopenAccessfi
dc.subject.ysohiukkasfysiikka
dc.subject.ysokosminen säteily
dc.subject.ysoilmaisimet
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p15576
jyx.subject.urihttp://www.yso.fi/onto/yso/p14258
jyx.subject.urihttp://www.yso.fi/onto/yso/p4220
dc.rights.urlhttps://creativecommons.org/licenses/by/4.0/
dc.relation.doi10.1140/epjc/s10052-019-7239-9
jyx.fundinginformationWe gratefully acknowledge the help and support from the directorate and staff of the Canfranc Underground Laboratory during the design, planning, construction and data acquisition phases of this project. This work has been supported in part by the Council of Oulu Region, the European Union Regional Development Fund, and by the grant of the Ministry of Education and Science of the Russian Federation number 3.3008.2017.
dc.type.okmA1


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