2011
DOI: 10.1016/j.hedp.2011.06.002
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Doppler effects on 3-D non-LTE radiation transport and emission spectra

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Cited by 14 publications
(8 citation statements)
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“…However, none of the numerical codes studied here solve a pressure equation exactly as in Eq. (5). The Athena and the internal NRL codes solve the total energy equation in conservation form, rather than the pressure Eq.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…However, none of the numerical codes studied here solve a pressure equation exactly as in Eq. (5). The Athena and the internal NRL codes solve the total energy equation in conservation form, rather than the pressure Eq.…”
Section: Discussionmentioning
confidence: 99%
“…However, understanding how the physical processes affect the output requires numerical simulation because of the non-linear interaction between the driving circuit, 1 ablation in the case of wire array loads, 2 magnetohydrodynamics (MHD), 3 non-local thermodynamic equilibrium population kinetics, 4 and radiation transport. 5 Simulations combining these features to varying levels of detail have been performed in one dimension (1D) radial, 6,7 2D RÀZ, 3,8-10 2D XÀY, 11,12 3D cylindrical, 13 and 3D Cartesian 14 coordinates.…”
Section: Introductionmentioning
confidence: 99%
“…We also note that analysis by Hansen et al [19] of time-gated K-and L-shell spectra from the same 20-mm-tall Cu wire-array experiment (Z shot 1975) plausibly suggests electron temperature up to 3 keV in the stagnating plasma near the pinch axis (and indeed gradients in electron temperature, density, and velocity were all inferred). Time-dependent behavior of the plasma conditions and spatial gradients must also be considered in developing a detailed picture of z-pinch radiation generation.…”
Section: Resultsmentioning
confidence: 52%
“…While Cu K-shell emission is typically generated only as the plasma stagnates on axis, run-in radiation in the Cu L shell is seen during the final stages of the implosion on Z. Copper and nickel L-shell lines can also be used to diagnose the plasma conditions as has been done for the 20-mm-tall experiment in [19] and [22]; however, here, we focus on Doppler splitting in Ne-like Cu 2p-3s transitions (referred to here as Cu 3F and 3G lines). The radially-resolved, time-gated spectroscopic data are shown in Fig.…”
Section: Resultsmentioning
confidence: 99%
“…However, it is still a work in progress. Recently, Hansen improved the model near the plasma vacuum interface by using a set of rays that are weighted by intensity [15].…”
Section: Mach2 and Tcre Modelsmentioning
confidence: 99%