Show simple item record

dc.contributor.authorDimitrijevic, Milan S.
dc.contributor.authorSimic, Zoran
dc.contributor.authorValjarević, Aleksandar
dc.contributor.authorYubero, Cristina
dc.date.accessioned2017-11-17T11:27:24Z
dc.date.available2017-11-17T11:27:24Z
dc.date.issued2017
dc.identifier.urihttp://hdl.handle.net/10396/15465
dc.description.abstractSodium is a very important element for the research and analysis of astrophysical, laboratory, and technological plasmas, but neither theoretical nor experimental data on Stark broadening of Na IV spectral lines are present in the literature. Using the modified semiempirical method of Dimitrijević and Konjević, here Stark widths have been calculated for nine Na IV transitions. Na IV belongs to the oxygen isoelectronic sequence, and we have calculated Stark widths belonging to singlets, triplets, and quintuplets, as well as with different parent terms. This is used to discuss similarities within one transition array with different multiplicities and parent terms. Additionally, calculated widths will be implemented in the STARK-B database (http://stark-b.obspm.fr) which is also a part of the Virtual Atomic and Molecular Data Center (VAMDC—http://www.vamdc.org/)es_ES
dc.format.mimetypeapplication/pdfes_ES
dc.language.isoenges_ES
dc.publisherMDPIes_ES
dc.rightshttps://creativecommons.org/licenses/by/4.0/es_ES
dc.sourceAtoms 5(3), 29 (2017)es_ES
dc.subjectStark broadeninges_ES
dc.subjectLine profileses_ES
dc.subjectAtomic dataes_ES
dc.subjectNa IVes_ES
dc.titleStark Widths of Na IV Spectral Lineses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherversionhttp://dx.doi.org/10.3390/atoms5030029es_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record