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Numerical simulation of shear-induced instabilities in internal solitary waves

Published online by Cambridge University Press:  22 August 2011

Magda Carr*
Affiliation:
School of Mathematics and Statistics, University of St Andrews, Fife KY16 9SS, UK
Stuart E. King
Affiliation:
School of Mathematics and Statistics, University of St Andrews, Fife KY16 9SS, UK
David G. Dritschel
Affiliation:
School of Mathematics and Statistics, University of St Andrews, Fife KY16 9SS, UK
*
Email address for correspondence: magda@mcs.st-and.ac.uk

Abstract

A numerical method that employs a combination of contour advection and pseudo-spectral techniques is used to simulate shear-induced instabilities in an internal solitary wave (ISW). A three-layer configuration for the background stratification, in which a linearly stratified intermediate layer is sandwiched between two homogeneous ones, is considered throughout. The flow is assumed to satisfy the inviscid, incompressible, Oberbeck–Boussinesq equations in two dimensions. Simulations are initialized by fully nonlinear, steady-state, ISWs. The results of the simulations show that the instability takes place in the pycnocline and manifests itself as Kelvin–Helmholtz billows. The billows form near the trough of the wave, subsequently grow and disturb the tail. Both the critical Richardson number () and the critical amplitude required for instability are found to be functions of the ratio of the undisturbed layer thicknesses. It is shown, therefore, that the constant, critical bound for instability in ISWs given in Barad & Fringer (J. Fluid Mech., vol. 644, 2010, pp. 61–95), namely , is not a sufficient condition for instability. It is also shown that the critical value of required for instability, where is the length of the region in a wave in which and is the half-width of the wave, is sensitive to the ratio of the layer thicknesses. Similarly, a linear stability analysis reveals that (where is the growth rate of the instability averaged over , the period in which parcels of fluid are subjected to ) is very sensitive to the transition between the undisturbed pycnocline and the homogeneous layers, and the amplitude of the wave. Therefore, the alternative tests for instability presented in Fructus et al. (J. Fluid Mech., vol. 620, 2009, pp. 1–29) and Barad & Fringer (J. Fluid Mech., vol. 644, 2010, pp. 61–95), respectively, namely and , are shown to be valid only for a limited parameter range.

Type
Papers
Copyright
Copyright © Cambridge University Press 2011

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Carr et al. supplementary movie

Movie 1. Evolution of the vorticity field for the wave depicted in figure 2 of the manuscript. The wave is defined as stable, little or no disturbance of the pycnocline is seen

Download Carr et al. supplementary movie(Video)
Video 815.4 KB

Carr et al. supplementary movie

Movie 1. Evolution of the vorticity field for the wave depicted in figure 2 of the manuscript. The wave is defined as stable, little or no disturbance of the pycnocline is seen

Download Carr et al. supplementary movie(Video)
Video 584.4 KB

Carr et al. supplementary movie

Movie 2. Evolution of the buoyancy field for the wave depicted in figure 3 of the manuscript. The wave is defined as stable, little or no disturbance of the pycnocline is seen.

Download Carr et al. supplementary movie(Video)
Video 820.7 KB

Carr et al. supplementary movie

Movie 2. Evolution of the buoyancy field for the wave depicted in figure 3 of the manuscript. The wave is defined as stable, little or no disturbance of the pycnocline is seen.

Download Carr et al. supplementary movie(Video)
Video 574.2 KB

Carr et al. supplementary movie

Movie 3. Evolution of the vorticity field for the wave depicted in figure 4 of the manuscript. The wave is defined as weakly unstable. Oscillation of the pycnocline is seen but no persistent coherent billows are formed.

Download Carr et al. supplementary movie(Video)
Video 839.6 KB

Carr et al. supplementary movie

Movie 3. Evolution of the vorticity field for the wave depicted in figure 4 of the manuscript. The wave is defined as weakly unstable. Oscillation of the pycnocline is seen but no persistent coherent billows are formed.

Download Carr et al. supplementary movie(Video)
Video 610.6 KB

Carr et al. supplementary movie

Movie 4. Evolution of the buoyancy field for the wave depicted in figure 5 of the manuscript. The wave is defined as weakly unstable. Oscillation of the pycnocline is seen but no persistent coherent billows are formed

Download Carr et al. supplementary movie(Video)
Video 846.2 KB

Carr et al. supplementary movie

Movie 4. Evolution of the buoyancy field for the wave depicted in figure 5 of the manuscript. The wave is defined as weakly unstable. Oscillation of the pycnocline is seen but no persistent coherent billows are formed

Download Carr et al. supplementary movie(Video)
Video 602.9 KB

Carr et al. supplementary movie

Movie 5. Evolution of the vorticity field for the wave depicted in figure 6 of the manuscript. The wave is defined as unstable. Coherent billows are seen in the pycnocline

Download Carr et al. supplementary movie(Video)
Video 907.9 KB

Carr et al. supplementary movie

Movie 5. Evolution of the vorticity field for the wave depicted in figure 6 of the manuscript. The wave is defined as unstable. Coherent billows are seen in the pycnocline

Download Carr et al. supplementary movie(Video)
Video 692.8 KB

Carr et al. supplementary movie

Movie 6. Evolution of the buoyancy field for the wave depicted in figure 7 of the manuscript. The wave is defined as unstable. Coherent billows are seen in the pycnocline

Download Carr et al. supplementary movie(Video)
Video 894.7 KB

Carr et al. supplementary movie

Movie 6. Evolution of the buoyancy field for the wave depicted in figure 7 of the manuscript. The wave is defined as unstable. Coherent billows are seen in the pycnocline

Download Carr et al. supplementary movie(Video)
Video 655.4 KB