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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/847
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dc.contributor.authorVitas, Nikolaen_US
dc.contributor.authorDanilović, Sanjaen_US
dc.contributor.authorAtanacković, Olgaen_US
dc.contributor.authorVince, Ištvanen_US
dc.date.accessioned2022-08-15T17:48:53Z-
dc.date.available2022-08-15T17:48:53Z-
dc.date.issued2005-01-01-
dc.identifier.issn03796566en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/847-
dc.description.abstractFormation of Mn I lines potentially suitable for plasma diagnostics is discussed. Synthetic profiles calculated in NLTE conditions with a comprehensive model atom are compared with solar spectrum. Hyperfine structure is taken into account for 37 lines (9 multiplets). The influence of optical pumping by emission from Mg II k line core is discussed.en
dc.relation.ispartofEuropean Space Agency, (Special Publication) ESA SPen_US
dc.subjectFormationen
dc.subjectLineen
dc.subjectPhotosphereen
dc.subjectSunen
dc.titleFormation of neutral manganese lines potentially suitable for plasma diagnosticsen_US
dc.typeConference Paperen_US
dc.relation.publicationProceedings of the 11th European Solar Physics Meeting "The Dynamic Sun: Challenges for Theory and Observations" 2005en_US
dc.identifier.scopus2-s2.0-33644796701-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/33644796701-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage99en_US
dc.relation.lastpage102en_US
dc.relation.issue600en_US
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
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