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Instability and transition in finite-amplitude Kelvin–Helmholtz and Holmboe waves

Published online by Cambridge University Press:  26 April 2006

W. D. Smyth  and
W. R. Peltier
W. D. Smyth
Affiliation:
Department of Physics, University of Toronto, Toronto, Ontario, Canada, M5S 1A7
W. R. Peltier
Affiliation:
Department of Physics, University of Toronto, Toronto, Ontario, Canada, M5S 1A7
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Abstract

We investigate the transition to turbulence in a free shear layer which contains a thin central region of stable density stratification. The fluid is assumed to possess Prandtl number significantly larger than unity, and the flow may exhibit either Holmboe or Kelvin–Helmholtz (KH) instability, depending upon the intensity of the stratification. A sequence of two-dimensional nonlinear numerical simulations of flows near the KH–Holmboe transition (i.e. having bulk Richardson numbers near 1/4) clearly illustrates the structural relationship between Holmboe and Kelvin–Helmholtz waves. The time-dependent nonlinear wave states delivered by the simulations are subjected to a three-dimensional normal-mode stability analysis in order to discover the physical processes that might drive the flow towards a turbulent state. Strong secondary instability is found to persist up to large spanwise wavenumbers, with no indication of a preferred lengthscale. These results indicate that secondary instability may lead the flow directly into the turbulent state.

Information

Type
Research Article
Information
Journal of Fluid Mechanics , Volume 228 , July 1991 , pp. 387 - 415
Copyright
© 1991 Cambridge University Press

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