Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/616
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dc.contributor.authorMilosavljević, Vladimiren
dc.contributor.authorDjeniže, Stevaen
dc.date.accessioned2022-07-12T16:01:42Z-
dc.date.available2022-07-12T16:01:42Z-
dc.date.issued2002-11-25en
dc.identifier.issn0375-9601en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/616-
dc.description.abstractOn the basis of the observed asymmetry of 26 Ne I spectral line profiles (in the 3s-3p and 3p-4d transitions) we have obtained their ion broadening parameters (A) caused by influence of ion microfield to the line broadening mechanism. They are the first A data obtained experimentally in the NeI spectrum and 16 from them are the first data in this field. The linear, low-pressure, pulsed arc has been used as a plasma source operated in neon at 33 000 and 36 500 K electron temperatures and 6.7 × 1022 and 8.8 × 1022 m-3 electron densities. Our A values have been compared to the unique theoretical ones and very high disagreement was found among them. We have found stronger influence of the ion contribution to the Ne I line profiles than the semiclassical theoretical approximation provides. © 2002 Elsevier Science B.V. All rights reserved.en
dc.relation.ispartofPhysics Letters, Section A: General, Atomic and Solid State Physicsen
dc.titleIon contribution to the Ne I spectral lines broadeningen
dc.typeArticleen
dc.identifier.doi10.1016/S0375-9601(02)01354-3en
dc.identifier.scopus2-s2.0-0037175604en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0037175604en
dc.relation.issue1-2en
dc.relation.volume305en
dc.relation.firstpage70en
dc.relation.lastpage74en
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.openairetypeArticle-
crisitem.author.orcid0000-0002-7805-5189-
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