Three-dimensionality of the triadic resonance instability of a plane inertial wave

Daniel Odens Mora, Eduardo Monsalve, Maxime Brunet, Thierry Dauxois, and Pierre-Philippe Cortet
Phys. Rev. Fluids 6, 074801 – Published 27 July 2021

Abstract

We analyze theoretically and experimentally the triadic resonance instability (TRI) of a plane inertial wave in a rotating fluid. Building on the classical triadic interaction equations between helical modes, we show by numerical integration that the maximum growth rate of the TRI is found for secondary waves that do not propagate in the same vertical plane as the primary wave (the rotation axis is parallel to the vertical). In the inviscid limit, we prove this result analytically, in which case the change in the horizontal propagation direction induced by the TRI evolves from 60 to 90 depending on the frequency of the primary wave. Due to a wave generator with a large spatial extension in the horizontal direction of invariance of the forced wave, we are able to report experimental evidence that the TRI of a plane inertial wave is three dimensional. The wave vectors of the secondary waves produced by the TRI are shown to match the theoretical predictions based on the maximum growth rate criterion. These results reveal that the triadic resonant interactions between inertial waves are very efficient at redistributing energy in the horizontal plane, normal to the rotation axis.

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  • Received 25 March 2021
  • Accepted 15 July 2021

DOI:https://doi.org/10.1103/PhysRevFluids.6.074801

©2021 American Physical Society

Physics Subject Headings (PhySH)

Fluid Dynamics

Authors & Affiliations

Daniel Odens Mora1, Eduardo Monsalve1, Maxime Brunet1, Thierry Dauxois2, and Pierre-Philippe Cortet1,*

  • 1Université Paris-Saclay, CNRS, FAST, 91405 Orsay, France
  • 2Université de Lyon, ENS de Lyon, CNRS, Laboratoire de Physique, 69342 Lyon, France

  • *pierre-philippe.cortet@universite-paris-saclay.fr

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Issue

Vol. 6, Iss. 7 — July 2021

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