57th Annual Meeting of the APS Division of Plasma Physics
Volume 60, Number 19
Monday–Friday, November 16–20, 2015;
Savannah, Georgia
Session GI3: ICF Preheat and Drive
9:30 AM–12:30 PM,
Tuesday, November 17, 2015
Room: Oglethorpe Auditorium
Chair: Felicie Albert, Lawrence Livermore National Laboratory
Abstract ID: BAPS.2015.DPP.GI3.4
Abstract: GI3.00004 : Quantifying the Growth of Cross-Beam Energy Transfer in Polar-Direct-Drive Implosions at the Omega Laser and National Ignition Facilities
11:00 AM–11:30 AM
Preview Abstract
Abstract
Author:
A.K. Davis
(Laboratory for Laser Energetics, U. of Rochester)
Direct-drive inertial confinement fusion requires multiple overlapping laser
beams that can drive the cross-beam energy transfer (CBET) instability. This
instability is of primary concern because it can reduce the laser energy
coupling and can affect the symmetry in a polar-direct-drive (PDD)
configuration. An experiment was designed to determine the CBET growth by
measuring the angularly resolved mass ablation rate and ablation-front
trajectory in a PDD configuration. Adding a thin layer of Si over a CH shell
generates two peaks in x-ray self-emission images that are measured with a
time-resolved pinhole imager. The inner peak is related to the position of
the ablation front and the outer peak corresponds to the position of the
interface of the two layers in the plasma. The emergence of the second peak
is used to measure the time for the laser to burn through the outer layer,
giving the average mass ablation rate of the material. The mass ablation
rate was measured by varying the thickness of the outer silicon layer. The
shell trajectory and mass ablation rate measured in PDD on the pole, where
CBET has little effect, were compared with simulations to validate the
electron thermal-transport model. Excellent agreement was obtained when
using a 2-D nonlocal transport model, and these observables could not be
reproduced with flux-limited models. A similar comparison was performed on
the equator where the CBET growth is large. Without the CBET model, the
shell velocity and mass ablation rate were significantly overestimated by
the simulation. Adding the CBET model reduced the drive on the equator and
reproduced the experimental results.
This material is based upon work supported by the Department of Energy
National Nuclear Security Administration under Award Number DE-NA0001944. In
collaboration with, D. Cao, D. T. Michel, M. Hohenberger, R. Epstein, V. N.
Goncharov, S. X. Hu, I. V. Igumenshchev, J. A. Marozas, D. D. Meyerhofer, P.
B. Radha, S. P. Regan, T. C. Sangster, and D. H. Froula (Laboratory for
Laser Energetics, U. of Rochester); M. Lafon (CEA).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2015.DPP.GI3.4