Abstract

The Boussinesq approximation provides a convenient framework to describe the dynamics of stably-stratified fluids. A fundamental motion in these fluids consists of internal gravity waves, whatever the strength of the stratification. These waves may be unstable through parametric instability, which results in turbulence and mixing. After a brief review of the main properties of internal gravity waves, we show how the parametric instability of a monochromatic internal gravity wave organizes itself in space and time, using energetics arguments and a simple kinematic model. We provide an example, in the deep ocean, where such instability is likely to occur, as estimates of mixing from in situ measurements suggest. We eventually discuss the fundamental role of internal gravity wave mixing in the maintenance of the abyssal thermal stratification. To cite this article: C. Staquet, C. R. Mecanique 335 (2007).

Highlights

  • As discussed in classical textbooks of fluid mechanics and of geophysical fluid dynamics, the Boussinesq approximation is an appropriate framework for describing the dynamics of stably-stratified fluids

  • A direct consequence is that the dispersion relation of a monochromatic internal gravity wave is anisotropic, as we show

  • The dispersion relation of internal gravity waves subjected to rotation has been verified experimentally only recently ([13])

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Summary

Introduction

As discussed in classical textbooks of fluid mechanics (see [1]) and of geophysical fluid dynamics (see [2]), the Boussinesq approximation is an appropriate framework for describing the dynamics of stably-stratified fluids. In the stratosphere, which is the part of the atmosphere comprised between ≃10 and ≃50 km, velocity fluctuations are mostly contributed by internal gravity wave motions These waves partly result from the blowing of the wind over the mountainous Earth surface, as their energy propagates nearly vertically upwards. The ability of internal gravity waves to mix stably-stratified fluids gives them a fundamental role in the deep ocean (cf [9]). These topics are successively addressed in the present article.

Dispersion relation of internal gravity waves
Structure of the emitted wave field
Numerical evidence for the parametric instability
Mechanisms of the parametric instability
Kinematic modelling of the parametric instability
Turbulence and mixing induced by internal gravity waves
The internal tide
Parametric instability of the internal tide
Mixing in the deep ocean
Conclusion
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