2006 48th Annual Meeting of the Division of Plasma Physics
Monday–Friday, October 30–November 3 2006;
Philadelphia, Pennsylvania
Session RI1: Direct Drive ICF
3:00 PM–5:00 PM,
Wednesday, November 1, 2006
Philadelphia Marriott Downtown
Room: Grand Salon ABF
Chair: Stephen Craxton, University of Rochester
Abstract ID: BAPS.2006.DPP.RI1.1
Abstract: RI1.00001 : Laser-Energy Coupling, Mass Ablation Rate, and Shock-Heating in Direct-Drive ICF
3:00 PM–3:30 PM
Preview Abstract
Abstract
Author:
S.P. Regan
(Laboratory for Laser Energetics, U. of Rochester)
Direct-drive laser-energy coupling, mass ablation rate, and
shock-heating
are experimentally studied on the OMEGA Laser System to validate
hydrodynamics simulations. High-gain, direct-drive inertial
confinement
fusion (ICF) target implosions require accurate predictions of
the shell
adiabat \textit{$\alpha $} (entropy), defined as the pressure in
the main fuel layer to the
Fermi-degenerate pressure. Since the minimum energy for ignition
scales as
$E_{min}\sim $ \textit{$\alpha $}$^{1.9}$ and the
Rayleigh--Taylor ablative stabilization
term is proportional to the ablation velocity $V_{a}\sim $
\textit{$\alpha $}$^{3/5}$; a
balance must be struck. The temporal pulse shape of the laser
irradiation
determines the adiabat. A series of experiments in spherical and
planar
geometries with CH targets have measured the laser absorption,
mass ablation
rate, and the amount of shock heating in the target. Time-resolved
measurements of laser absorption in the corona are performed on
spherical
implosion experiments. The mass ablation rate is inferred from
time-resolved
Ti K-shell spectroscopic measurements of nonaccelerating, solid
CH spherical
targets with a buried tracer layer of Ti. The amount of shock
heating is
diagnosed in planar-CH-foil targets using two techniques:
time-resolved
x-ray absorption spectroscopy and noncollective spectrally
resolved x-ray
scattering. The predicted shell conditions are close to the
experimental
results. A detailed comparison of the experimental results and the
simulations will be presented. This work was supported by the U.S.
Department of Energy Office of Inertial Confinement Fusion under
Cooperative
Agreement No. DE-FC52-92SF19460. Contributors: H. Sawada, D. Li,
V. N.
Goncharov, R. Epstein, J. A. Delettrez, J. P. Knauer, J. A.
Marozas, F. J.
Marshall, R. L. McCrory, P. W. McKenty, D. D. Meyerhofer, P. B.
Radha, W.
Seka, T. C. Sangster, S. Skupsky, V. A. Smalyuk, LLE/UR, R. Mancini,
University of Nevada, S.H. Glenzer, O. Landen \textit{LLNL, }G.
Gregori, \textit{RAL}
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2006.DPP.RI1.1