Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/42456
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dc.contributor.authorNagayama, T.en_US
dc.contributor.authorBailey, J. E.en_US
dc.contributor.authorMancini, R. C.en_US
dc.contributor.authorIglesias, C. A.en_US
dc.contributor.authorHansen, S. B.en_US
dc.contributor.authorBlancard, C.en_US
dc.contributor.authorChung, H. K.en_US
dc.contributor.authorColgan, J.en_US
dc.contributor.authorCosse, P.en_US
dc.contributor.authorFaussurier, G.en_US
dc.contributor.authorFlorido, R.en_US
dc.contributor.authorFontes, C. J.en_US
dc.contributor.authorGilleron, F.en_US
dc.contributor.authorGolovkin, I. E.en_US
dc.contributor.authorKilcrease, D. P.en_US
dc.contributor.authorLoisel, G.en_US
dc.contributor.authorMacFarlane, J. J.en_US
dc.contributor.authorPain, J.-C.en_US
dc.contributor.authorRochau, G. A.en_US
dc.contributor.authorSherrill, M. E.en_US
dc.contributor.authorLee, R. W.en_US
dc.date.accessioned2018-11-14T14:06:49Z-
dc.date.available2018-11-14T14:06:49Z-
dc.date.issued2016en_US
dc.identifier.issn1574-1818en_US
dc.identifier.urihttp://hdl.handle.net/10553/42456-
dc.description.abstractLocal-thermodynamic-equilibrium (LTE) K-shell spectroscopy is a common tool to diagnose electron density, ne, and electron temperature, Te, of high-energy-density (HED) plasmas. Knowing the accuracy of such diagnostics is important to provide quantitative conclusions of many HED-plasma research efforts. For example, Fe opacities were recently measured at multiple conditions at the Sandia National Laboratories Z machine (Bailey et al., 2015), showing significant disagreement with modeled opacities. Since the plasma conditions were measured using K-shell spectroscopy of tracer Mg (Nagayama et al., 2014), one concern is the accuracy of the inferred Fe conditions. In this article, we investigate the K-shell spectroscopy model uncertainties by analyzing the Mg spectra computed with 11 different models at the same conditions. We find that the inferred conditions differ by ±20-30% in ne and ±2-4% in Te depending on the choice of spectral model. Also, we find that half of the Te uncertainty comes from ne uncertainty. To refine the accuracy of the K-shell spectroscopy, it is important to scrutinize and experimentally validate line-shape theory. We investigate the impact of the inferred ne and Te model uncertainty on the Fe opacity measurements. Its impact is small and does not explain the reported discrepancies.en_US
dc.languageengen_US
dc.relationImplementation of activities described in the Roadmap to Fusion during Horizon 2020 through a Joint programme of the members of the EUROfusion consortiumen_US
dc.relationEurofusiónen_US
dc.relationAWP15‐ENR‐01/CEen_US
dc.relationAWP15-ENR-01/CEA-02en_US
dc.relation.ispartofHigh Energy Density Physicsen_US
dc.sourceHigh Energy Density Physics [ISSN 1574-1818], v. 20, p. 17-22en_US
dc.subject22 Físicaen_US
dc.subject.otherDiagnostics uncertaintyen_US
dc.subject.otherLine shapeen_US
dc.subject.otherLTEen_US
dc.subject.otherOpacityen_US
dc.subject.otherPlasma diagnosticsen_US
dc.subject.otherX-ray spectroscopyen_US
dc.titleModel uncertainties of local-thermodynamic-equilibrium K-shell spectroscopyen_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.hedp.2016.05.001en_US
dc.identifier.scopus84975256782-
dc.identifier.isi000384802400003-
dc.contributor.authorscopusid25633968700-
dc.contributor.authorscopusid55664000000-
dc.contributor.authorscopusid55230931900-
dc.contributor.authorscopusid35430576000-
dc.contributor.authorscopusid22961691800-
dc.contributor.authorscopusid57203093667-
dc.contributor.authorscopusid55977801500-
dc.contributor.authorscopusid7404007208-
dc.contributor.authorscopusid54790566900-
dc.contributor.authorscopusid6602604993-
dc.contributor.authorscopusid6701629708-
dc.contributor.authorscopusid6505795084-
dc.contributor.authorscopusid7005517473-
dc.contributor.authorscopusid6603580622-
dc.contributor.authorscopusid6603714071-
dc.contributor.authorscopusid6602366876-
dc.contributor.authorscopusid26647552700-
dc.contributor.authorscopusid7201418151-
dc.contributor.authorscopusid35482584300-
dc.contributor.authorscopusid35360460100-
dc.contributor.authorscopusid55871121758-
dc.contributor.authorscopusid13613612800-
dc.description.lastpage22en_US
dc.description.firstpage17en_US
dc.relation.volume20en_US
dc.investigacionCienciasen_US
dc.type2Artículoen_US
dc.contributor.daisngid5309876-
dc.contributor.daisngid674477-
dc.contributor.daisngid30268485-
dc.contributor.daisngid58044-
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dc.contributor.daisngid106974-
dc.utils.revisionen_US
dc.contributor.wosstandardWOS:Nagayama, T-
dc.contributor.wosstandardWOS:Bailey, JE-
dc.contributor.wosstandardWOS:Mancini, RC-
dc.contributor.wosstandardWOS:Iglesias, CA-
dc.contributor.wosstandardWOS:Hansen, SB-
dc.contributor.wosstandardWOS:Blancard, C-
dc.contributor.wosstandardWOS:Chung, HK-
dc.contributor.wosstandardWOS:Colgan, J-
dc.contributor.wosstandardWOS:Cosse, P-
dc.contributor.wosstandardWOS:Faussurier, G-
dc.contributor.wosstandardWOS:Florido, R-
dc.contributor.wosstandardWOS:Fontes, CJ-
dc.contributor.wosstandardWOS:Gilleron, F-
dc.contributor.wosstandardWOS:Golovkin, IE-
dc.contributor.wosstandardWOS:Kilcrease, DP-
dc.contributor.wosstandardWOS:Loisel, G-
dc.contributor.wosstandardWOS:MacFarlane, JJ-
dc.contributor.wosstandardWOS:Pain, JC-
dc.contributor.wosstandardWOS:Rochau, GA-
dc.contributor.wosstandardWOS:Sherrill, ME-
dc.contributor.wosstandardWOS:Lee, RW-
dc.date.coverdateSeptiembre 2016en_US
dc.identifier.ulpgcen_US
dc.description.sjr0,902
dc.description.jcr0,908
dc.description.sjrqQ2
dc.description.jcrqQ4
dc.description.scieSCIE
item.grantfulltextnone-
item.fulltextSin texto completo-
crisitem.project.principalinvestigatorMartel Escobar, Pablo-
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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