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Supersonic jet and shock interactions

TLDR
Soures et al. as discussed by the authors investigated the propagation of a structured shock front within a radiation-driven target assembly, the formation of a supersonic jet of material, and the subsequent interaction of this jet with an ambient medium in which a second, ablatively driven shock wave is propagating.
Abstract
Supersonic fluid flow and the interaction of strong shock waves to produce jets of material are ubiquitous features of inertial confinement fusion (ICF), astrophysics, and other fields of high energy-density science. The availability of large laser systems provides an opportunity to investigate such hydrodynamic systems in the laboratory, and to test their modeling by radiation hydrocodes. We describe experiments to investigate the propagation of a structured shock front within a radiation-driven target assembly, the formation of a supersonic jet of material, and the subsequent interaction of this jet with an ambient medium in which a second, ablatively driven shock wave is propagating. The density distribution within the jet, the Kelvin–Helmholz roll-up at the tip of the jet, and the jet’s interaction with the counterpropagating shock are investigated by x-ray backlighting. The experiments were designed and modeled using radiation hydrocodes developed by Los Alamos National Laboratory, AWE, and Lawrence Livermore National Laboratory. The same hydrocodes are being used to model a large number of other ICF and high energy-density physics experiments. Excellent agreement between the different simulations and the experimental data is obtained, but only when the full geometry of the experiment, including both laser-heated hohlraum targets (driving the jet and counter-propagating shock), is included. The experiments were carried out at the University of Rochester’s Omega laser [J. M. Soures et al., Phys. Plasmas 3, 2108 (1996)].

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Journal ArticleDOI

Experimental astrophysics with high power lasers and Z pinches

TL;DR: High energy density (HED) laboratory astrophysics as discussed by the authors is a new class of experimental science, wherein the properties of matter and the processes that occur under extreme astrophysical conditions can be examined in the laboratory.
Journal ArticleDOI

The RAGE radiation-hydrodynamic code

TL;DR: RAGE, the 'radiation adaptive grid Eulerian' radiation-hydrodynamics code, is described, including its data structures, its parallelization strategy and performance, its hydrodynamic algorithm(s), its (gray) radiation diffusion algorithm, and some of the considerable amount of verification and validation efforts.
Journal ArticleDOI

The National Ignition Facility: enabling fusion ignition for the 21st century

TL;DR: The National Ignition Facility (NIF) at Lawrence Livermore National Laboratory, when completed in 2008, will contain a 192-beam, 1.8?MJ, 500?TW, ultraviolet laser system together with a 10?m diameter target chamber and room for 100 diagnostics as discussed by the authors.
Journal ArticleDOI

The National Ignition Facility

TL;DR: The National Ignition Facility (NIF) at Lawrence Livermore National Laboratory is a stadium-sized facility that, when completed in 2008, will contain a 192-beam, 1.8-megajoule, 500-terawatt, ultraviolet laser system together with a 10m-diam target chamber and room for 100 diagnostics as discussed by the authors.
Journal ArticleDOI

Architecture of petawatt-class z-pinch accelerators.

TL;DR: In this article, an accelerator architecture that can serve as the basis of the design of petawatt-class $z$-pinch drivers is presented. But it does not include intermediate store transmission lines, multimegavolt gas switches, or a laser trigger system.
References
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Journal ArticleDOI

Development of the indirect‐drive approach to inertial confinement fusion and the target physics basis for ignition and gain

John Lindl
- 01 Nov 1995 - 
TL;DR: In this paper, an approach to fusion that relies on either electron conduction (direct drive) or x rays (indirect drive) for energy transport to drive an implosion is presented.
Journal ArticleDOI

Numerical simulation of turbulent mixing by Rayleigh-Taylor instability

TL;DR: In this article, two-dimensional hydrodynamic codes are used to simulate the growth of perturbations at an interface between two fluids of different density due to Rayleigh-Taylor instability.
Journal ArticleDOI

The mixing transition in turbulent flows

TL;DR: In this paper, the authors proposed a Taylor Reynolds number of ReT = u[prime prime or minute] [lambda]T/v [greater, similar] 100-140 for turbulent mixing.
Journal ArticleDOI

Similarity Criteria for the Laboratory Simulation of Supernova Hydrodynamics

TL;DR: In this paper, the conditions for the applicability of the Euler equations are formulated, based on the analysis of localization, heat conduction, viscosity, and radiation.
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