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 BO7: Measurements and Diagnostics in Inertial Confinement Fusion
9:30 AM–12:30 PM,
Monday, November 5, 2018
OCC
Room: B117-119
Chair: Dan Casey, Lawrence Livermore National Laboratory
Abstract ID: BAPS.2018.DPP.BO7.1
Abstract: BO7.00001 : Diagnosing the hot-spot electron temperature from x-ray continnum emission measurements on NIF and OMEGA implosions*
9:30 AM–9:42 AM
Presenter:
Michael J. MacDonald
(Lawrence Livermore Natl Lab)
Authors:
Michael J. MacDonald
(Lawrence Livermore Natl Lab)
Daniel B. Thorn
(Lawrence Livermore Natl Lab)
Andrew G. MacPhee
(Lawrence Livermore Natl Lab)
Benjamin Bachmann
(Lawrence Livermore Natl Lab)
Dave K. Bradley
(Lawrence Livermore Natl Lab)
Bernard Kozioziemski
(Lawrence Livermore Natl Lab)
Otto L. Landen
(Lawrence Livermore Natl Lab)
Sabrina R. Nagel
(Lawrence Livermore Natl Lab)
Marilyn B. Schneider
(Lawrence Livermore Natl Lab)
Rahul C. Shah
(Lab for Laser Energetics)
Raymond E. Bahr
(Lab for Laser Energetics)
Duc M. Cao
(Lab for Laser Energetics)
Timothy Filkins
(Lab for Laser Energetics)
Sean P. Regan
(Lab for Laser Energetics)
Chuck Sorce
(Lab for Laser Energetics)
Christian Stoeckl
(Lab for Laser Energetics)
Wolfgang R. Theobald
(Lab for Laser Energetics)
Joe D. Kilkenny
(General Atomics)
The hot-spot electron temperature (Te) is a key metric in determining the performance of inertial confinement fusion (ICF) implosions. The Continuum Spectrometer (ConSpec) infers hot-spot Te from the slope of the x-ray continuum emission in the photon energy range of 20 to 30 keV, where ion velocity and opacity effects are negligible. Additionally, the ConSpec provides spatial resolution to resolve background x-ray sources from the hot-spot emission. We present initial x-ray spectra, from which we infer hot-spot Te for DT cryogenic implosions at both the National Ignition Facility (NIF) and the OMEGA laser facility. In the NIF experiments, we infer the hot-spot Te from the continuum emission and measure the emission spectra from the laser deposition region near the hohlraum wall (the gold bubble). For the OMEGA direct-drive implosions, we evaluate the effectiveness of spatially resolving the hot-spot emission in the time-integrated measurement from coronal plasma emission.
*This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344 and 18-ERD-015. This material is based upon work supported by the Department Of Energy National Nuclear Security Administration under Award Number DE NA0001944.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BO7.1
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