Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/326
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dc.contributor.authorTapalaga, I.en_US
dc.contributor.authorDojčinović, Ivanen_US
dc.contributor.authorMilosavljevi, M. K.en_US
dc.contributor.authorPurić, Jagošen_US
dc.date.accessioned2022-07-12T15:11:16Z-
dc.date.available2022-07-12T15:11:16Z-
dc.date.issued2012-03-19-
dc.identifier.issn1323-3580-
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/326-
dc.description.abstractDependences of electron and proton impact Stark width on the upper level ionization potential within different series of the neutral calcium spectral lines have been evaluated and discussed. The similar dependences previously found for the electron impact contribution were also obtained for the proton impact contribution to the Stark broadening. The emphasis is on the term structure influence on the studied Stark width dependences. The influence of the lower transition level and transition term is higher at low temperatures. After establishing these dependences, predictions were made for Stark widths of neutral calcium spectral lines not measured experimentally or calculated theoretically until now. 2012 Astronomical Society of Australia.en_US
dc.relation.ispartofPublications of the Astronomical Society of Australiaen_US
dc.subjectatomic dataen_US
dc.subjectline: profilesen_US
dc.subjectopacityen_US
dc.subjectplasmasen_US
dc.subjectradiative transferen_US
dc.titleStark width regularities within neutral calcium spectral seriesen_US
dc.typeArticleen_US
dc.identifier.doi10.1071/AS11053-
dc.identifier.scopus2-s2.0-84858189028-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84858189028-
dc.relation.issue1en_US
dc.relation.volume29en_US
dc.relation.firstpage20en_US
dc.relation.lastpage28en_US
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
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