2016
DOI: 10.1103/physrevlett.117.225001
|View full text |Cite
|
Sign up to set email alerts
|

Late-Time Mixing Sensitivity to Initial Broadband Surface Roughness in High-Energy-Density Shear Layers

Abstract: Using a large volume high-energy-density fluid shear experiment (8.5 cm 3 ) at the National Ignition Facility, we have demonstrated for the first time the ability to significantly alter the evolution of a supersonic sheared mixing layer by controlling the initial conditions of that layer. By altering the initial surface roughness of the tracer foil, we demonstrate the ability to transition the shear mixing layer from a highly ordered system of coherent structures to a randomly ordered system with a faster grow… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
6
0

Year Published

2017
2017
2022
2022

Publication Types

Select...
9
1

Relationship

0
10

Authors

Journals

citations
Cited by 26 publications
(6 citation statements)
references
References 41 publications
0
6
0
Order By: Relevance
“…RMI differs significantly from Kelvin-Helmholtz instability (KHI) and closely related Rayleigh-Taylor instability (RTI) a) UK Ministry of Defence c Crown Owned Copyright 2019/AWE b) Electronic mail: ben.thornber@sydney.edu.au in that the driving is impulsive. With a sufficiently strong impulse, time to develop, and high Reynolds number, linear growth will be followed by a transition to turbulence, where velocity fluctuations decay in time, and the layer grows at a relatively slow rate ∝ t θ with θ ≈ 0.2 to 1 (possible if dominated by linear modes, although a fully turbulent layer is limited to 8 θ ≤ 2/3) with a strong dependence on initial conditions [9][10][11][12][13][14][15] . As an example θ ≈ 0.29 for the configuration studied in this paper 16 , compared to KHI (∝ t) and RTI (∝ t 2 ).…”
Section: Introductionmentioning
confidence: 99%
“…RMI differs significantly from Kelvin-Helmholtz instability (KHI) and closely related Rayleigh-Taylor instability (RTI) a) UK Ministry of Defence c Crown Owned Copyright 2019/AWE b) Electronic mail: ben.thornber@sydney.edu.au in that the driving is impulsive. With a sufficiently strong impulse, time to develop, and high Reynolds number, linear growth will be followed by a transition to turbulence, where velocity fluctuations decay in time, and the layer grows at a relatively slow rate ∝ t θ with θ ≈ 0.2 to 1 (possible if dominated by linear modes, although a fully turbulent layer is limited to 8 θ ≤ 2/3) with a strong dependence on initial conditions [9][10][11][12][13][14][15] . As an example θ ≈ 0.29 for the configuration studied in this paper 16 , compared to KHI (∝ t) and RTI (∝ t 2 ).…”
Section: Introductionmentioning
confidence: 99%
“…Numerical data are advantageous for LWN model validation because higher order quantities such as spectra can be extracted for more detailed comparisons. While experimental efforts do not carry the same granularity of information as simulations, the LANL also has invested resources in high energy density experiments to study shocked and sheared mixing [118], which could also be used as validation data for global mean quantities of interest. In the realm of single and two-fluid mixing, the data appear to be quite extensive.…”
Section: Discussionmentioning
confidence: 99%
“…Another series of HEDP turbulent experiments were developed in a shock-shear driven planar geometry on OMEGA and NIF [171][172][173]. Starting from initial surface roughness, signatures of 3D self-similar turbulent evolution were measured [174].…”
Section: (B) Fundamental High-energy-density Hydrodynamicsmentioning
confidence: 99%