Resonant Triad Instability in Stratified Fluids
Sylvain Joubaud (Phys-ENS), James Munroe, Philippe Odier (Phys-ENS),, Thierry Dauxois (Phys-ENS)

TL;DR
This paper presents the first experimental measurement of the growth rate of resonant triad instability in stratified fluids, comparing results with theoretical predictions to enhance understanding of energy transfer in geophysical and astrophysical flows.
Contribution
It provides the first experimental quantification of the growth rate of resonant triad instability in stratified fluids, validating theoretical models.
Findings
Measured growth rates match theoretical predictions.
Resonant triad instability facilitates energy transfer to smaller scales.
Experimental data supports the role of internal waves in fluid mixing.
Abstract
Internal gravity waves contribute to fluid mixing and energy transport, not only in oceans but also in the atmosphere and in astrophysical bodies. We provide here the first experimental measurement of the growth rate of a resonant triad instability (also called parametric subharmonic instability) transferring energy to smaller scales where it is dissipated. We make careful and quantitative comparisons with theoretical predictions for propagating vertical modes in laboratory experiments.
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