Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/848
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dc.contributor.authorDragić, A.en
dc.contributor.authorAničin, I.en
dc.contributor.authorBanjanac, R.en
dc.contributor.authorUdovičić, V.en
dc.contributor.authorJoković, D.en
dc.contributor.authorMaletić, D.en
dc.contributor.authorPuzović, Jovanen
dc.date.accessioned2022-07-12T17:16:53Z-
dc.date.available2022-07-12T17:16:53Z-
dc.date.issued2011-09-09en
dc.identifier.issn1810-6528en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/848-
dc.description.abstractThe proposed influence of cosmic rays on cloud formation is tested for the effect of sudden intensity changes of CR (Forbush decreases) on cloudiness. An attempt is made to widen the investigated period covered by satellite observation of cloudiness. As an indicator of cloud cover, the diurnal temperature range (DTR - a quantity anticorrelated with cloudiness) is used. The superposed epoch analysis on a set of isolated Forbush decreases is conducted and the results for a region of Europe are presented. The effect of Forbush decrease on DTR is statistically significant only if the analysis is restricted to high amplitude FDs (above the threshold value of 7% with the respect to undisturbed CR intensity). The magnitude of the effect on DTR is estimated to be (0.38 ± 0.06) °C. © Author(s) 2011.en
dc.relation.ispartofAstrophysics and Space Sciences Transactionsen
dc.titleForbush decreases - Clouds relation in the neutron monitor eraen
dc.typeArticleen
dc.identifier.doi10.5194/astra-7-315-2011en
dc.identifier.scopus2-s2.0-80052394959en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/80052394959en
dc.relation.issue3en
dc.relation.volume7en
dc.relation.firstpage315en
dc.relation.lastpage318en
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
item.cerifentitytypePublications-
item.openairetypeArticle-
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