Please use this identifier to cite or link to this item:
http://hdl.handle.net/10553/42456
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Nagayama, T. | en_US |
dc.contributor.author | Bailey, J. E. | en_US |
dc.contributor.author | Mancini, R. C. | en_US |
dc.contributor.author | Iglesias, C. A. | en_US |
dc.contributor.author | Hansen, S. B. | en_US |
dc.contributor.author | Blancard, C. | en_US |
dc.contributor.author | Chung, H. K. | en_US |
dc.contributor.author | Colgan, J. | en_US |
dc.contributor.author | Cosse, P. | en_US |
dc.contributor.author | Faussurier, G. | en_US |
dc.contributor.author | Florido, R. | en_US |
dc.contributor.author | Fontes, C. J. | en_US |
dc.contributor.author | Gilleron, F. | en_US |
dc.contributor.author | Golovkin, I. E. | en_US |
dc.contributor.author | Kilcrease, D. P. | en_US |
dc.contributor.author | Loisel, G. | en_US |
dc.contributor.author | MacFarlane, J. J. | en_US |
dc.contributor.author | Pain, J.-C. | en_US |
dc.contributor.author | Rochau, G. A. | en_US |
dc.contributor.author | Sherrill, M. E. | en_US |
dc.contributor.author | Lee, R. W. | en_US |
dc.date.accessioned | 2018-11-14T14:06:49Z | - |
dc.date.available | 2018-11-14T14:06:49Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 1574-1818 | en_US |
dc.identifier.uri | http://hdl.handle.net/10553/42456 | - |
dc.description.abstract | Local-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.language | eng | en_US |
dc.relation | Implementation of activities described in the Roadmap to Fusion during Horizon 2020 through a Joint programme of the members of the EUROfusion consortium | en_US |
dc.relation | Eurofusión | en_US |
dc.relation | AWP15‐ENR‐01/CE | en_US |
dc.relation | AWP15-ENR-01/CEA-02 | en_US |
dc.relation.ispartof | High Energy Density Physics | en_US |
dc.source | High Energy Density Physics [ISSN 1574-1818], v. 20, p. 17-22 | en_US |
dc.subject | 22 Física | en_US |
dc.subject.other | Diagnostics uncertainty | en_US |
dc.subject.other | Line shape | en_US |
dc.subject.other | LTE | en_US |
dc.subject.other | Opacity | en_US |
dc.subject.other | Plasma diagnostics | en_US |
dc.subject.other | X-ray spectroscopy | en_US |
dc.title | Model uncertainties of local-thermodynamic-equilibrium K-shell spectroscopy | en_US |
dc.type | info:eu-repo/semantics/Article | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1016/j.hedp.2016.05.001 | en_US |
dc.identifier.scopus | 84975256782 | - |
dc.identifier.isi | 000384802400003 | - |
dc.contributor.authorscopusid | 25633968700 | - |
dc.contributor.authorscopusid | 55664000000 | - |
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dc.contributor.authorscopusid | 6505795084 | - |
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dc.contributor.authorscopusid | 35482584300 | - |
dc.contributor.authorscopusid | 35360460100 | - |
dc.contributor.authorscopusid | 55871121758 | - |
dc.contributor.authorscopusid | 13613612800 | - |
dc.description.lastpage | 22 | en_US |
dc.description.firstpage | 17 | en_US |
dc.relation.volume | 20 | en_US |
dc.investigacion | Ciencias | en_US |
dc.type2 | Artículo | en_US |
dc.contributor.daisngid | 5309876 | - |
dc.contributor.daisngid | 674477 | - |
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dc.contributor.daisngid | 1200288 | - |
dc.contributor.daisngid | 106974 | - |
dc.utils.revision | Sí | en_US |
dc.contributor.wosstandard | WOS:Nagayama, T | - |
dc.contributor.wosstandard | WOS:Bailey, JE | - |
dc.contributor.wosstandard | WOS:Mancini, RC | - |
dc.contributor.wosstandard | WOS:Iglesias, CA | - |
dc.contributor.wosstandard | WOS:Hansen, SB | - |
dc.contributor.wosstandard | WOS:Blancard, C | - |
dc.contributor.wosstandard | WOS:Chung, HK | - |
dc.contributor.wosstandard | WOS:Colgan, J | - |
dc.contributor.wosstandard | WOS:Cosse, P | - |
dc.contributor.wosstandard | WOS:Faussurier, G | - |
dc.contributor.wosstandard | WOS:Florido, R | - |
dc.contributor.wosstandard | WOS:Fontes, CJ | - |
dc.contributor.wosstandard | WOS:Gilleron, F | - |
dc.contributor.wosstandard | WOS:Golovkin, IE | - |
dc.contributor.wosstandard | WOS:Kilcrease, DP | - |
dc.contributor.wosstandard | WOS:Loisel, G | - |
dc.contributor.wosstandard | WOS:MacFarlane, JJ | - |
dc.contributor.wosstandard | WOS:Pain, JC | - |
dc.contributor.wosstandard | WOS:Rochau, GA | - |
dc.contributor.wosstandard | WOS:Sherrill, ME | - |
dc.contributor.wosstandard | WOS:Lee, RW | - |
dc.date.coverdate | Septiembre 2016 | en_US |
dc.identifier.ulpgc | Sí | en_US |
dc.description.sjr | 0,902 | |
dc.description.jcr | 0,908 | |
dc.description.sjrq | Q2 | |
dc.description.jcrq | Q4 | |
dc.description.scie | SCIE | |
item.grantfulltext | none | - |
item.fulltext | Sin texto completo | - |
crisitem.project.principalinvestigator | Martel Escobar, Pablo | - |
crisitem.project.principalinvestigator | Martel Escobar, Pablo | - |
crisitem.author.dept | GIR IUNAT: Interacción Radiación-Materia | - |
crisitem.author.dept | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.dept | Departamento de Física | - |
crisitem.author.orcid | 0000-0001-7428-6273 | - |
crisitem.author.parentorg | IU de Estudios Ambientales y Recursos Naturales | - |
crisitem.author.fullName | Florido Hernández, Ricardo Jesús | - |
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