Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session GP11: Poster Session III: Basic Plasma Physics: General; Space and Astrophysical Plasmas; ICF Measurement and Computational Techniques, Direct and Indirect Drive; MIF Science and Technology (9:30am-12:30pm)
Tuesday, November 6, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.GP11.98
Abstract: GP11.00098 : Spectroscopic Measurements of the Equatorial Electron Temperature in a NIF Hohlraum Using Mid-Z Tracer Elements**
Presenter:
Klaus Widmann
(Lawrence Livermore Natl Lab)
Authors:
Klaus Widmann
(Lawrence Livermore Natl Lab)
Duane A Liedahl
(Lawrence Livermore Natl Lab)
Stephan A MacLaren
(Lawrence Livermore Natl Lab)
Maria A Barrios
(In-Q-Tel)
Marilyn Beth Schneider
(Lawrence Livermore Natl Lab)
Hui Chen
(Lawrence Livermore Natl Lab)
William A Farmer
(Lawrence Livermore Natl Lab)
Leonard C Jarrott
(Lawrence Livermore Natl Lab)
Oggie Jones
(Lawrence Livermore Natl Lab, Lawrence Livermore Natl Lab)
Robert L Kauffman
(Lawrence Livermore Natl Lab)
Otto L Landen
(Lawrence Livermore Natl Lab)
Nathan Meezan
(Lawrence Livermore Natl Lab)
Mark Sherlock
(Lawrence Livermore Natl Lab)
Daniel Thorn
(Lawrence Livermore Natl Lab)
John D Moody
(Lawrence Livermore Natl Lab)
Spectrally and temporally resolved x-ray emission measurements of highly charged mid-Z ions are used to determine the electron temperature (Te) in the equatorial region of a laser-driven ignition-type NIF hohlraum. A mid-Z tracer “dot” of 400 µm in diameter and 0.16 µm thickness is coated onto the outside of a high-density carbon (HDC) capsule. The measured x-ray spectra are fit using SCRAM simulations and a genetic algorithm to give a peak Te of (2.7 ± 0.4) keV at the hohlraum equator between the HDC capsule and the gold wall. The measurements show a decrease in Te near the hohlraum equator even before the laser drive is turned off giving evidence that the equatorially-directed laser beams are losing their energy before they reach the hohlraum equator. While we find agreement with post-shot simulations when the plasma reaches its peak temperature, some disagreement between the measured and simulated Te remains in the earlier part of the laser heating and also in the temporal signature of the cooling phase near the end of the laser drive. We present a detailed error analysis of the spectroscopic measurements and a discussion of the uncertainty in the derived Te.
**This work was performed under the auspices of the U.S. Department of Energy by LLNL under Contract DE-AC52-07NA27344.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.GP11.98
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