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Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/76
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dc.contributor.authorObradović, Bratislaven
dc.contributor.authorIvković, M.en
dc.contributor.authorIvković, Sašaen
dc.contributor.authorCvetanović, N.en
dc.contributor.authorSretenović, Goranen
dc.contributor.authorKovačević, Vesnaen
dc.contributor.authorKrstić, I. B.en
dc.contributor.authorKuraica, Miloraden
dc.date.accessioned2022-06-30T14:38:36Z-
dc.date.available2022-06-30T14:38:36Z-
dc.date.issued2016-01-01en
dc.identifier.issn0004-640Xen
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/76-
dc.description.abstractSeveral examples of Stark spectral line shifts from different laboratory plasma experiments are presented. The difference is outlined between the Stark shift caused by the micro field of charged particles on one side and the Stark shift caused by macroscopic electric field occurring in plasma sheaths on the other. In the first case the shift is used for testing of the Stark shifting theory and/or measurement of density of electrons while in the second it is used for measurement of macroscopic electric field strength. It is shown that inhomogeneity of the plasma can be used to provide the reference nonshifted lines for exact evaluation of the shift magnitude.en
dc.relation.ispartofAstrophysics and Space Scienceen
dc.subjectSpectroscopyen
dc.subjectStark shiften
dc.titleInhomogeneity in laboratory plasma discharges and Stark shift measurementen
dc.typeArticleen
dc.identifier.doi10.1007/s10509-015-2620-0en
dc.identifier.scopus2-s2.0-84951270176en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84951270176en
dc.relation.issue1en
dc.relation.volume361en
dc.relation.firstpage1en
dc.relation.lastpage6en
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
crisitem.author.orcid0000-0002-3221-7779-
crisitem.author.orcid0000-0003-4817-4723-
crisitem.author.orcid0000-0002-8575-1668-
crisitem.author.orcid0000-0001-8201-8500-
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