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Wall shocks in high-energy-density shock tube experiments

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TLDR
In this paper, the authors demonstrate the effects of wall shocks in experiments performed on the Omega Laser Facility, launching shocks propagating through xenon with speeds above 100 km/s driven by ablation pressures of approximately 50 Mbars.
Abstract
The radiative precursor of a sufficiently fast shock has been observed to drive the vaporization of shock tube material ahead of the shock. The resulting expansion drives a converging blast wave into the gas volume of the tube. The effects of this wall shock may be observed and correlated with primary shock parameters. We demonstrate this process in experiments performed on the Omega Laser Facility, launching shocks propagating through xenon with speeds above 100 km/s driven by ablation pressures of approximately 50 Mbars. Wall shocks in laser experiments, in which the principal shock waves themselves should not be radiative, are also reported—in which the wall shocks have been launched by some other early energy source.

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Citations
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Journal ArticleDOI

Linear and nonlinear waves, by G. B. Whitham. Pp.636. £50. 1999. ISBN 0 471 35942 4 (Wiley).

TL;DR: To the best of our knowledge, there is only one application of mathematical modelling to face recognition as mentioned in this paper, and it is a face recognition problem that scarcely clamoured for attention before the computer age but, having surfaced, has attracted the attention of some fine minds.
Journal ArticleDOI

Crash: A Block-Adaptive-Mesh Code for Radiative Shock Hydrodynamics - Implementation and Verification

TL;DR: The Center for Radiative Shock Hydrodynamics (CRASH) code as mentioned in this paper is a block adaptive mesh code for multi-material radiation hyddynamics, which is an extension of the Block-Adaptive Tree Solarwind Roe Upwind Scheme (BATS-RUS) code with new radiation transfer and heat conduction library and equation-of-state and multigroup opacity solvers.
Journal ArticleDOI

Crash: a block-adaptive-mesh code for radiative shock hydrodynamics—implementation and verification

TL;DR: The CRASH code is an extension of the Block-Adaptive Tree Solarwind Roe Upwind Scheme with a new radiation transfer and heat conduction library and equation-of-state and multi-group opacity solvers, and a suite of verification test problems are presented to demonstrate the accuracy and performance of the algorithms.

Observation of a Hydrodynamically Driven, Radiative Precursor Shock

TL;DR: Observations of a radiative-precursor shock that evolves from a purely hydrodynamic system are presented, and the length and temperature profile of the radiative precursor are examined as the intensity of the laser is varied.
References
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Book

Linear and Nonlinear Waves

G. B. Whitham
TL;DR: In this paper, a general overview of the nonlinear theory of water wave dynamics is presented, including the Wave Equation, the Wave Hierarchies, and the Variational Method of Wave Dispersion.

Physics of shock waves and high-temperature hydrodynamic phenomena

TL;DR: The physics of high-temperature hydrodynamic phenomena is discussed in this article, where the authors present interpretations of the physical basis of shockwave and high temperature hydrodynamics and give practical guidance to those who work with these subjects.
Journal ArticleDOI

Linear and nonlinear waves, by G. B. Whitham. Pp.636. £50. 1999. ISBN 0 471 35942 4 (Wiley).

TL;DR: To the best of our knowledge, there is only one application of mathematical modelling to face recognition as mentioned in this paper, and it is a face recognition problem that scarcely clamoured for attention before the computer age but, having surfaced, has attracted the attention of some fine minds.
Book

Foundations of Radiation Hydrodynamics

TL;DR: In this paper, the great foundation-stones of radiating flows in astrophysics are exposed, and upon them are built the walls of methodology (some understandably incomplete). Concentration is on fundamentals but with only few applications.
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.
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