Please use this identifier to cite or link to this item: http://hdl.handle.net/10553/47992
DC FieldValueLanguage
dc.contributor.authorMancini, R. C.en_US
dc.contributor.authorIglesias, C. A.en_US
dc.contributor.authorFerri, S.en_US
dc.contributor.authorCalisti, A.en_US
dc.contributor.authorFlorido, R.en_US
dc.contributor.otherFlorido, Ricardo-
dc.contributor.otherCalisti, Annette-
dc.date.accessioned2018-11-23T18:05:57Z-
dc.date.available2018-11-23T18:05:57Z-
dc.date.issued2013en_US
dc.identifier.issn1574-1818en_US
dc.identifier.urihttp://hdl.handle.net/10553/47992-
dc.description.abstractThe effect of the interference term in the electron broadening of the Li-like satellites to the Ar Heβ line has been investigated in the standard Stark broadening theory. Although the interference term has negligible or small effect on satellite lines with spectator electrons in n = 2 and n = 3 shells, it shows significant narrowing for lines with n = 4 spectator electrons. Nevertheless, the improved n = 4 satellite line shape makes a small difference in the emergent intensity distribution of the composite spectral feature. Accordingly, this change in line shape does not affect previous diagnosis of plasma conditions in Ar-doped ICF implosion cores.en_US
dc.languageengen_US
dc.relationDeterminación de Propiedades Radiativas, Termodinamicas y Diagnosis Espectroscopica de Plasmas de Interés Científico-Tecnológicoen_US
dc.relation.ispartofHigh Energy Density Physicsen_US
dc.sourceHigh Energy Density Physics [ISSN 1574-1818], v. 9 (4), p. 731-736en_US
dc.subject2207 Física atómica y nuclearen_US
dc.subject.otherSpectral line shapes-
dc.subject.otherStark broadening-
dc.subject.otherRadiative properties-
dc.subject.otherICF diagnostics-
dc.titleThe effect of improved satellite line shapes on the argon Heβ spectral featureen_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.hedp.2013.08.002en_US
dc.identifier.scopus84878872243-
dc.identifier.isi000328183200011-
dcterms.isPartOfHigh Energy Density Physics-
dcterms.sourceHigh Energy Density Physics[ISSN 1574-1818],v. 9 (4), p. 731-736-
dc.contributor.authorscopusid35430576000-
dc.contributor.authorscopusid22961691800-
dc.contributor.authorscopusid7101638564-
dc.contributor.authorscopusid56219688400-
dc.contributor.authorscopusid6505795084-
dc.description.lastpage736en_US
dc.identifier.issue4-
dc.description.firstpage731en_US
dc.relation.volume9en_US
dc.investigacionCiencias-
dc.type2Artículoen_US
dc.identifier.wosWOS:000328183200011-
dc.contributor.daisngid27815-
dc.contributor.daisngid30268485-
dc.contributor.daisngid58044-
dc.contributor.daisngid1090357-
dc.contributor.daisngid85747-
dc.contributor.daisngid236941-
dc.contributor.daisngid835287-
dc.identifier.investigatorRIDH-5513-2015-
dc.identifier.investigatorRIDNo ID-
dc.description.numberofpages6en_US
dc.utils.revision-
dc.contributor.wosstandardWOS:Mancini, RC-
dc.contributor.wosstandardWOS:Iglesias, CA-
dc.contributor.wosstandardWOS:Ferri, S-
dc.contributor.wosstandardWOS:Calisti, A-
dc.contributor.wosstandardWOS:Florido, R-
dc.date.coverdateDiciembre 2013en_US
dc.identifier.ulpgces
dc.contributor.buulpgcBU-BASen_US
dc.description.sjr0,978
dc.description.jcr1,519
dc.description.sjrqQ2
dc.description.jcrqQ3
dc.description.scieSCIE
item.grantfulltextnone-
item.fulltextSin texto completo-
crisitem.project.principalinvestigatorMartel Escobar, Pablo-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.orcid0000-0001-7428-6273-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.fullNameFlorido Hernández, Ricardo Jesús-
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