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.BO7.3
Abstract: BO7.00003 : Inference of the electron temperature in ICF implosions from X-ray spectra*
9:54 AM–10:06 AM
Presenter:
Grigory Kagan
(Los Alamos Natl Lab)
Authors:
Grigory Kagan
(Los Alamos Natl Lab)
O.L. Landen
(Lawrence Livermore Natl Lab)
D. Svyatskiy
(Los Alamos Natl Lab)
Peter Hakel
(Los Alamos Natl Lab)
C.J. McDevitt
(Los Alamos Natl Lab)
H. Sio
(MIT)
N.V. Kabadi
(MIT)
R.A. Simpson
(MIT)
M. Gatu Johnson
(MIT)
Johan Frenje
(MIT)
Richard David Petrasso
(MIT)
Rahul C Shah
(Lab for Laser Energetics)
Michael J Rosenberg
(Lab for Laser Energetics)
Reuben Epstein
(Lab for Laser Energetics)
Sean P Regan
(Lab for Laser Energetics)
Tirtha R Joshi
(Los Alamos Natl Lab)
Thomas E Weber
(Los Alamos Natl Lab)
Hans Rinderknecht
(Lawrence Livermore Natl Lab)
Daniel Thorn
(Lawrence Livermore Natl Lab)
Marilyn Beth Schneider
(Lawrence Livermore Natl Lab)
David K. Bradley
(Lawrence Livermore Natl Lab)
Joe Kilkenny
(Lawrence Livermore Natl Lab)
Two main approaches to assessing the electron temperature in ICF implosions are now being considered, which are based on measuring, respectively, line emission from a high-Z dopant such as krypton [1] or spectral continuum of 15 to 30 keV from electrons scattering off the D and T ions [2,3]. However, both types of the X-ray emission are due to suprathermal free electrons, which likely deviate from Maxwellian. We present the first theoretical study of both the line and continuum X-ray spectra from the hot-spot accounting for this deviation. In particular, we show that inferring the electron temperature as if the emitting electrons are Maxwellian gives a lower value than the actual one [4].
References
[1] H. Chen et al. Phys. Plasmas 24 (2017) 072715
[2] L. Jarrott, et al. Rev. Sci. Inst. 87 (2016) 11E534
[3] D. B. Thorn et al. Proc. SPIE 10390 (2017) 1039009
[4] G. Kagan et al. https://arxiv.org/abs/1710.01343
*This work is supported by the Laboratory Directed Research and Development program under the auspices of the U.S. Dept. of Energy by the Los Alamos National Security, LLC, Los Alamos National Laboratory under Contract No. DE-AC52-06NA25396.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BO7.3
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