Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/309
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dc.contributor.authorDojčinović, Ivanen
dc.contributor.authorTapalaga, Irinelen
dc.contributor.authorPurić, Jagošen
dc.date.accessioned2022-07-12T15:09:04Z-
dc.date.available2022-07-12T15:09:04Z-
dc.date.issued2012-01-01en
dc.identifier.issn0035-8711en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/309-
dc.description.abstractStark width experimental and theoretical data of neutral helium spectral lines have been used to demonstrate their dependence on the upper-level ionization potential within different spectral series. The emphasis is on the term describing structure influence on the studied Stark-width dependences. After establishing these dependences, predictions were made for electron, proton and ionized helium impact contributions to the Stark widths of neutral helium spectral lines that have not been measured experimentally or calculated theoretically until now (transitions from high levels of Hei). The accuracy of the data obtained is comparable with the accuracies of the experimental and theoretical values used in establishing the dependences. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.en
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectAtomic dataen
dc.subjectLine: profilesen
dc.subjectOpacityen
dc.subjectPlasmasen
dc.subjectRadiative transferen
dc.titleStark parameter regularities of neutral helium lines within different spectral seriesen
dc.typeArticleen
dc.identifier.doi10.1111/j.1365-2966.2011.19772.xen
dc.identifier.scopus2-s2.0-83555168161en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/83555168161en
dc.relation.issue1en
dc.relation.volume419en
dc.relation.firstpage904en
dc.relation.lastpage912en
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
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