Three-dimensionality of the triadic resonance instability of a plane inertial wave
ORAL
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 degrees depending on the frequency of the primary wave. Thanks 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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Publication: https://arxiv.org/pdf/2107.07937.pdf
Presenters
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Daniel A Mora-Paiba
FAST, CNRS, Université Paris Saclay, Université Paris Saclay
Authors
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Daniel A Mora-Paiba
FAST, CNRS, Université Paris Saclay, Université Paris Saclay
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Eduardo Monsalve
FAST, CNRS, Université Paris Saclay
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Maxime Brunet
FAST, CNRS, Université Paris Saclay
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Thierry Dauxois
Laboratoire de Physique, ENS LYON, CNRS, Université de Lyon, Ecole Normale Superieure de Lyon
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Pierre-Philippe Cortet
FAST, CNRS, Université Paris Saclay