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Title: | Model uncertainties of local-thermodynamic-equilibrium K-shell spectroscopy | Authors: | Nagayama, T. Bailey, J. E. Mancini, R. C. Iglesias, C. A. Hansen, S. B. Blancard, C. Chung, H. K. Colgan, J. Cosse, P. Faussurier, G. Florido, R. Fontes, C. J. Gilleron, F. Golovkin, I. E. Kilcrease, D. P. Loisel, G. MacFarlane, J. J. Pain, J.-C. Rochau, G. A. Sherrill, M. E. Lee, R. W. |
UNESCO Clasification: | 22 Física | Keywords: | Diagnostics uncertainty Line shape LTE Opacity Plasma diagnostics, et al |
Issue Date: | 2016 | Project: | Implementation of activities described in the Roadmap to Fusion during Horizon 2020 through a Joint programme of the members of the EUROfusion consortium Eurofusión AWP15‐ENR‐01/CE AWP15-ENR-01/CEA-02 |
Journal: | High Energy Density Physics | 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. | URI: | http://hdl.handle.net/10553/42456 | ISSN: | 1574-1818 | DOI: | 10.1016/j.hedp.2016.05.001 | Source: | High Energy Density Physics [ISSN 1574-1818], v. 20, p. 17-22 |
Appears in Collections: | Artículos |
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