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dc.contributor.authorBishel, D. T.
dc.contributor.authorMarley, E. V.
dc.contributor.authorSchneider, M. B.
dc.contributor.authorLiedahl, D. A.
dc.contributor.authorHeeter, R. F.
dc.contributor.authorFoord, M. E.
dc.contributor.authorKemp, G. E.
dc.contributor.authorFrank, Y.
dc.contributor.authorEmig, J. A.
dc.contributor.authorNilson, P. M.
dc.contributor.authorChin, D. A.
dc.contributor.authorRygg, J. R.
dc.contributor.authorCollins, G. W.
dc.contributor.authorPérez Callejo, Gabriel 
dc.date.accessioned2024-01-10T17:48:32Z
dc.date.available2024-01-10T17:48:32Z
dc.date.issued2023
dc.identifier.citationPhysics of Plasmas, Julio 2023, v. 30, p. 073303es
dc.identifier.issn1070-664Xes
dc.identifier.urihttps://uvadoc.uva.es/handle/10324/64402
dc.descriptionProducción Científicaes
dc.description.abstractTime-gated Sc K-shell and Ge L-shell spectra are presented from a range of characterized thermodynamic states spanning ion densities of 1e19-1e20cm-3 and plasma temperatures around 2000eV. For the higher densities studied and temperatures from 1000 to 3000 eV, the Sc and Ge x-ray emission spectra are consistent with steady-state calculations from the modern atomic kinetics model SCRAM. At the lower ion densities achieved through plasma expansion, however, the model calculations require a higher plasma temperature to reproduce the observed Ge spectrum. We attribute this to ionization disequilibrium of the Sc because the ionization time scales exceed the hydrodynamic timescale when the inferred temperatures diverge.es
dc.format.mimetypeapplication/pdfes
dc.language.isoenges
dc.publisherAmerican Institute of Physicses
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.titleIonization disequilibrium in K- and L-shell ionses
dc.typeinfo:eu-repo/semantics/articlees
dc.identifier.doi10.1063/5.0151931es
dc.identifier.publicationissue7es
dc.identifier.publicationtitlePhysics of Plasmases
dc.identifier.publicationvolume30es
dc.peerreviewedSIes
dc.description.projectThis work has been supported by the Research Grant No. PID2019-108764RB-I00 from the Spanish Ministry of Science and Innovation.es
dc.identifier.essn1089-7674es
dc.rightsAtribución 4.0 Internacional
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones


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