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Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/889
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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.authorPuzović, Jovanen
dc.contributor.authorAničin, I.en
dc.date.accessioned2022-07-12T17:16:58Z-
dc.date.available2022-07-12T17:16:58Z-
dc.date.issued2005-01-01en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/889-
dc.description.abstractThe cosmic-ray intensity record from Belgrade muon detectors in the period 2002-2004 is subjected to power spectra analysis. Statistically significant peaks are found in datasets from both ground and underground (25 m w.e.) detectors. The possible origin of these periodicities is discussed.en
dc.relation.ispartof29th International Cosmic Ray Conference, ICRC 2005en
dc.titleVariations of CR-muon intensity in the declining phase of the 23 <sup>rd</sup> solar cycle in ground and shallow underground dataen
dc.typeConference Paperen
dc.identifier.scopus2-s2.0-84898939330en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84898939330en
dc.relation.volume1en
dc.relation.firstpage249en
dc.relation.lastpage252en
item.openairetypeConference Paper-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
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