50th Annual Meeting of the Division of Plasma Physics
Volume 53, Number 14
Monday–Friday, November 17–21, 2008;
Dallas, Texas
Session QI1: Shocks and Shock-Driven Phenomena in High-Energy Density Plasmas
3:00 PM–4:30 PM,
Wednesday, November 19, 2008
Room: Landmark A
Chair: Vladimir Smalyuk, University of Rochester
Abstract ID: BAPS.2008.DPP.QI1.1
Abstract: QI1.00001 : Laboratory blast wave driven instabilities
3:00 PM–3:30 PM
Preview Abstract
Abstract
Author:
Carolyn Kuranz
(University of Michigan)
This presentation discusses experiments
involving the evolution of hydrodynamic instabilities in the
laboratory
under high-energy-density (HED) conditions. These instabilities
are driven
by blast waves, which occur following a sudden, finite release of
energy,
and consist of a shock front followed by a rarefaction wave. When
a blast
wave crosses an interface with a decrease in density, hydrodynamic
instabilities will develop. Instabilities evolving under HED
conditions are
relevant to astrophysics. These experiments include target
materials scaled
in density to the He/H layer in SN1987A. About 5 kJ of laser
energy from the
Omega Laser facility irradiates a 150 $\mu $m plastic layer that
is followed
by a low-density foam layer. A blast wave structure similar to
those in
supernovae is created in the plastic layer. The blast wave
crosses an
interface having a 2D or 3D sinusoidal structure that serves as a
seed
perturbation for hydrodynamic instabilities. This produces
unstable growth
dominated by the Rayleigh-Taylor (RT) instability in the
nonlinear regime.
We have detected the interface structure under these conditions
using x-ray
backlighting. Recent advances in our diagnostic techniques have
greatly
improved the resolution of our x-ray radiographic images. Under
certain
conditions, the improved images show some mass extending beyond
the RT spike
and penetrating further than previously observed or predicted by
current
simulations. The observed effect is potentially of great
importance as a
source of mass transport to places not anticipated by current
theory and
simulation. I will discuss the amount of mass in these spike
extensions, the
associated uncertainties, and hypotheses regarding their origin
We also plan
to show comparisons of experiments using single mode and
multimode as well
as 2D and 3D initial conditions. This work is sponsored by
DOE/NNSA Research
Grants DE-FG52-07NA28058 (Stewardship Sciences Academic
Alliances) and DE-FG52-04NA00064 (National Laser User Facility).
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2008.DPP.QI1.1