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 CO6: Hohlraum and X-ray Cavity Physics
2:00 PM–4:48 PM,
Monday, November 5, 2018
OCC
Room: B115-116
Chair: Pierre Michel, Lawrence Livermore National Laboratory
Abstract ID: BAPS.2018.DPP.CO6.5
Abstract: CO6.00005 : 3D wall motion in hohlraum
2:48 PM–3:00 PM
Presenter:
Stephane Laffite
(CEA DAM DIF)
Authors:
Stephane Laffite
(CEA DAM DIF)
Paul Edouard Masson Laborde
(CEA DAM DIF)
Scott Wilks
(LLNL)
Chikang Li
(MIT)
Raphael Riquier
(CEA DAM DIF)
Gilles Kluth
(CEA DAM DIF)
Olivier Morice
(CEA DAM DIF)
Veronique Tassin
(CEA DAM DIF)
Inside a hohlraum, the plasma blow-off of the wall heated by laser beams is a serious concern as this determines how the laser beams propagate through the hohlraum and where they subsequently deposit their energy in the hohlraum. In turn, this determines the X-ray drive that an ICF capsule sees, and therefore impacts the symmetry of the implosion. It is clear that there is here a need to benchmark wall motion in simulations with experimental measurements. Recently, a series of experiments have been carried out on the Omega laser facility to examine such an issue. In an open cylinder, the motion of the laser-driven plasma bubbles was observed with proton radiography. A nearly uniform irradiation of the 59° laser cone with 10 laser spots was compared to the classic irradiation with 5 laser spots for which more 3D effects are expected
We present here 2D and 3D calculations of these experiments. The impact of the 3D is demonstrated: the 3D-calculated bubbles move faster than the 2D-calculated ones. Radial velocities are supersonic (Mach=3-5) and exceed 1000 km/s. However, the 3D calculations still underestimate the experimentally measured bubble motion.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CO6.5
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