53rd Annual Meeting of the APS Division of Plasma Physics
Volume 56, Number 16
Monday–Friday, November 14–18, 2011;
Salt Lake City, Utah
Session BI3: The National Ignition Campaign
9:30 AM–12:30 PM,
Monday, November 14, 2011
Room: Ballroom AC
Chair: Karl Krushelnick, University of Michigan
Abstract ID: BAPS.2011.DPP.BI3.5
Abstract: BI3.00005 : Hot-Spot Mix in Ignition-Scale Implosions at the National Ignition Facility
11:30 AM–12:00 PM
Preview Abstract
Abstract
Author:
S.P. Regan
(Laboratory for Laser Energetics, U. of Rochester)
Ignition of an inertial confinement fusion target depends on the
formation
of a central hot spot with sufficient temperature and areal density.
Radiative and conductive losses from the hot spot can be enhanced by
hydrodynamic instabilities. The concentric spherical layers of
current
National Ignition Facility ignition targets consist of a plastic
ablator
surrounding a thin shell of cryogenic thermonuclear fuel (i.e.,
hydrogen
isotopes), with fuel vapor filling the interior volume.\footnote{
S. W.
Haan\textit{ et al.}, Phys. Plasmas \textbf{18}, 051001 (2011).}
The ablator is doped with
Ge to minimize preheat of the ablator closest to the DT ice
caused by Au
M-band emission from the hohlraum x-ray drive.\footnote{ D. S.
Clark\textit{ et al.}, Phys.
Plasmas \textbf{17}, 052703 (2010).} Richtmyer--Meshkov and
Rayleigh--Taylor
hydrodynamic instabilities seeded by high-mode (50 $< \quad
\lambda \quad <$ 200)
ablator-surface perturbations can cause Ge-doped ablator to mix
into the
interior of the shell at the end of the acceleration
phase.\footnote{ B. A.
Hammel\textit{ et al.}, Phys. Plasmas \textbf{18}, 056310
(2011).} As the shell decelerates,
it compresses the fuel vapor, forming a hot spot. K-shell line
emission from
the ionized Ge that has penetrated into the hot spot provides an
experimental signature of hot-spot mix. The Ge emission from
tritium--hydrogen--deuterium (THD) and DT cryogenic targets and
gas-filled
plastic-shell capsules, which replace the THD layer with a
mass-equivalent
CH layer, was examined. The amount of hot-spot mix mass,
estimated from the
Ge K-shell line brightness using a detailed atomic physics
code,\footnote{J. J. MacFarlane\textit{ et al.}, High Energy
Density Phys. \textbf{3}, 181 (2007).} is
typically below the 100-ng allowance for hot-spot mix.$^{1}$
Predictions of
a simple mix model, based on linear growth of the measured
surface-mass
modulations, are consistent with the experimental results. The
measured
dependence of hot-spot mix on the implosion velocity and on the
high-mode
ablator-surface perturbations will be presented. This work was
supported by
the U.S. Department of Energy Office of Inertial Confinement
Fusion under
Cooperative Agreement No. DE-FC52-08NA28302.
In collaboration with the National Ignition Campaign Mix Working
Group.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2011.DPP.BI3.5