Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/890
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dc.contributor.authorDragić, A.en
dc.contributor.authorBanjanac, R.en
dc.contributor.authorUdovičić, V.en
dc.contributor.authorJoković, D.en
dc.contributor.authorAničin, I.en
dc.contributor.authorPuzović, Jovanen
dc.date.accessioned2022-07-12T17:16:58Z-
dc.date.available2022-07-12T17:16:58Z-
dc.date.issued2005-11-20en
dc.identifier.issn0217-751Xen
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/890-
dc.description.abstractCosmic muon flux is recorded by two plastic scintillator detectors: one located at ground level and the other located in the Belgrade underground laboratory (25 m w.e.). Power spectral analysis of the raw detector data for the period from January 1st 2002 to December 31st 2002 is performed. Similar periodicities are found in both data sets (ground and underground), but with different amplitudes. Main periodicity in the underground detector data has a 26.5 days period, while the highest amplitude signal in the ground detector data has a 243 ± 45 days period. Other signals present in the time series correspond to higher harmonics of the solar rotation period. There is also a wave with a 34.4 days period, whose significance is confirmed by different methods of spectral analysis. The same periodicity is recently found in some processes on the Sun. © World Scientific Publishing Company.en
dc.relation.ispartofInternational Journal of Modern Physics Aen
dc.subjectCosmic muonsen
dc.subjectSolar modulationen
dc.subjectSpectral analysisen
dc.titleComparative study of power spectra of ground and shallow underground muon dataen
dc.typeConference Paperen
dc.identifier.doi10.1142/S0217751X05030570en
dc.identifier.scopus2-s2.0-29844455981en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/29844455981en
dc.relation.issue29en
dc.relation.volume20en
dc.relation.firstpage6953en
dc.relation.lastpage6955en
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
item.cerifentitytypePublications-
item.openairetypeConference Paper-
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