15th European Turbulence Conference 2015
August 25-28th, 2015, Delft, The Netherlands
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Direct and inverse energy cascades in a forced rotating turbulence experiment


Go-down etc15 Tracking Number 92

Presentation:
Session: Geophysical and astrophysical turbulence 1
Room: Room C
Session start: 10:30 Thu 27 Aug 2015

Frédéric Moisy   moisy@fast.u-psud.fr
Affifliation: Laboratoire FAST, CNRS, Université Paris-Sud, 91405 Orsay, France

Pierre-Philippe Cortet   ppcortet@fast.u-psud.fr
Affifliation: Laboratoire FAST, CNRS, Université Paris-Sud, 91405 Orsay, France

Basile Gallet   basile.gallet@cea.fr
Affifliation: Laboratoire SPHYNX, SPEC, DSM, CEA Saclay, CNRS, 91191 Gif-sur-Yvette, France

Antoine Campagne   campagne@fast.u-psud.fr
Affifliation: Laboratoire FAST, CNRS, Université Paris-Sud, 91405 Orsay, France


Topics: - Geophysical and astrophysical turbulence

Abstract:

We present experimental evidence for a double cascade of kinetic energy in a statistically stationary rotating turbulence experiment. Turbulence is generated by a set of vertical flaps which continuously injects velocity fluctuations towards the center of a rotating water tank. The energy transfers are evaluated from two-point third-order three-component velocity structure functions, which we measure using stereoscopic particle image velocimetry in the rotating frame. Without global rotation, the energy is transferred from large to small scales, as in classical three-dimensional turbulence. For nonzero rotation rates, the horizontal kinetic energy presents a double cascade: a direct cascade at small horizontal scales and an inverse cascade at large horizontal scales. By contrast, the vertical kinetic energy is always transferred from large to small horizontal scales, a behavior reminiscent of the dynamics of a passive scalar in two-dimensional turbulence. At the largest rotation rate the flow is nearly two-dimensional, and a pure inverse energy cascade is found for the horizontal energy. To describe the scale-by-scale energy budget, we consider a generalization of the Kármán-Howarth-Monin equation to inhomogeneous turbulent flows, in which the energy input is explicitly described as the advection of turbulent energy from the flaps through the surface of the control volume where the measurements are performed.