Astudy of spectral laws for helical turbulence in the presence of solid body rotation up to Reynolds numbers Re ~ 1 × 105 and down to Rossby numbers Ro ~ 3 × 10-3 is presented. The forcing function is a fully helical flow that can also be viewed as mimicking the effect of atmospheric convective motions. Variants of a model developed previously by Baerenzung et al. are tested in the helical case against direct numerical simulation (DNS), using data from a run on a grid of 15363 points; its efficiency is also contrasted against a spectral largeeddy simulation (LES) by Chollet and Lesieur, as well as an underresolved DNS. The model including the contribution of helicity to the spectral eddy dissipation and eddy noise behaves best, allowing the...
We study the intermittency properties of the energy and helicity cascades in two 15363 direct numeri...
We present a parametric space study of the decay of turbulence in rotating flows combining direct nu...
Rapidly rotating turbulent flow is characterized by the emergence of columnar structures that are re...
We present results from two 15363 direct numerical simulations of rotating turbulence where both ene...
The effect of helicity (velocity-vorticity correlations) is studied in direct numerical simulations ...
Invariance properties of physical systems govern their behaviour: energy conservation in turbulence ...
We present numerical evidence of how three-dimensionalization occurs at small scale in rotating turb...
A subgrid-scale spectral model of rotating turbulent flows is tested against direct numerical simula...
International audienceRecent numerical simulations have shown the strong impact of helicity on homog...
We present numerical evidence on how three-dimensionalization is recovered at small scale in rotatin...
In this thesis, we investigate several properties of rotating turbulent flows. First, we ran several...
The effect of rotation is considered to become important when the Rossby number is sufficiently smal...
We perform numerical simulations of decaying rotating stratified turbulence and show, in the Boussin...
Turbulent mixing in geophysics is often affected by the presence of rotation, which renders the flow...
Copyright © ETC 2013 - 14th European Turbulence Conference.All rights reserved. Rotating turbulent f...
We study the intermittency properties of the energy and helicity cascades in two 15363 direct numeri...
We present a parametric space study of the decay of turbulence in rotating flows combining direct nu...
Rapidly rotating turbulent flow is characterized by the emergence of columnar structures that are re...
We present results from two 15363 direct numerical simulations of rotating turbulence where both ene...
The effect of helicity (velocity-vorticity correlations) is studied in direct numerical simulations ...
Invariance properties of physical systems govern their behaviour: energy conservation in turbulence ...
We present numerical evidence of how three-dimensionalization occurs at small scale in rotating turb...
A subgrid-scale spectral model of rotating turbulent flows is tested against direct numerical simula...
International audienceRecent numerical simulations have shown the strong impact of helicity on homog...
We present numerical evidence on how three-dimensionalization is recovered at small scale in rotatin...
In this thesis, we investigate several properties of rotating turbulent flows. First, we ran several...
The effect of rotation is considered to become important when the Rossby number is sufficiently smal...
We perform numerical simulations of decaying rotating stratified turbulence and show, in the Boussin...
Turbulent mixing in geophysics is often affected by the presence of rotation, which renders the flow...
Copyright © ETC 2013 - 14th European Turbulence Conference.All rights reserved. Rotating turbulent f...
We study the intermittency properties of the energy and helicity cascades in two 15363 direct numeri...
We present a parametric space study of the decay of turbulence in rotating flows combining direct nu...
Rapidly rotating turbulent flow is characterized by the emergence of columnar structures that are re...