Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/611
DC FieldValueLanguage
dc.contributor.authorMilosavljević, Vladimiren
dc.contributor.authorPoparić, Goranen
dc.date.accessioned2022-07-12T16:01:42Z-
dc.date.available2022-07-12T16:01:42Z-
dc.date.issued2001-01-01en
dc.identifier.issn1063-651Xen
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/611-
dc.description.abstractWe report an advanced numerical procedure for deconvolution of theoretical asymmetric convolution integral of a Gaussian and a plasma broadened spectral line profile [Formula Presented] for spectal lines. Our method determines all broadening parameters, self-consistently and directly from the line profile with minimal assumptions or prior knowledge. This method is useful for obtaining complete information on all plasma parameters directly from the recorded shape of a single line, which is very important in case no other diagnostic methods are available. The method is also convenient for determination of plasma parameters in the case of a symmetrical profile such as Voigt one. © 2001 The American Physical Society.en
dc.relation.ispartofPhysical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topicsen
dc.titleAtomic spectral line free parameter deconvolution procedureen
dc.typeArticleen
dc.identifier.doi10.1103/PhysRevE.63.036404en
dc.identifier.scopus2-s2.0-0035272581en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0035272581en
dc.relation.issue3en
dc.relation.volume63en
item.grantfulltextnone-
item.openairetypeArticle-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
crisitem.author.orcid0000-0002-7805-5189-
Appears in Collections:Journal Article
Show simple item record

SCOPUSTM   
Citations

56
checked on Oct 30, 2024

Page view(s)

18
checked on Nov 4, 2024

Google ScholarTM

Check

Altmetric

Altmetric


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.