We investigated with a quasi-geostrophic model convection in an internally heated rapidly rotating sphere. We showed that, in the small Ekman number limit, the kinetic energy of the convective solution becomes time dependent immediately above the onset of convection (relaxation oscillations). We showed that banded structures can develop immediately above the onset in the presence of Ekman pumping. The width of these bands corresponds to a balance between Ekman pumping and bulk viscosity. Then we investigated the dynamo bifurcation. We found that decreasing (resp. increasing) the Roberts (Ekman) number for a given Ekman (Roberts) number one successively obtains supercritical bifurcations, subcritical bifurcations and isola. We showed that fo...
The range of existence and the properties of two essentially different chaotic attractors found in a...
Bistability and hysteresis of magnetohydrodynamic dipolar dynamos generated by turbulent convection ...
A convection-driven multiscale dynamo model is developed in the limit of low Rossby number for the p...
Bifurcations of dynamos in rotating and buoyancy-driven spherical Rayleigh-Bénard convection in an e...
On considère un fluide visqueux conducteur sis entre deux plaques planes, chauffées par en dessous, ...
30 pages, 16 figures, published in JFMInternational audienceWe study nonlinear convection in a rapid...
MAGNETO-CONVECTION IN A RAPIDLY ROTATING SPHERE: NUMERICAL AND EXPERIMENTAL APPROACHES OF THE CONVEC...
In order better to understand the processes that lead to the generation of magnetic fields of finite...
The focus of this study is to investigate primary and secondary bifurcations to weakly nonlinear flo...
International audienceRapidly rotating convection in spherical geometry outside the tangent cylinder...
International audienceWe study numerically an extensive set of dynamo models in rotating spherical s...
The linear stability of the periodic and axisymmetric solutions of the convection in rotating, inter...
The magnetic fields of planets and stars are generated by the motions of electrically conducting flu...
The range of existence and the properties of two essentially different chaotic attractors found in a...
Bistability and hysteresis of magnetohydrodynamic dipolar dynamos generated by turbulent convection ...
A convection-driven multiscale dynamo model is developed in the limit of low Rossby number for the p...
Bifurcations of dynamos in rotating and buoyancy-driven spherical Rayleigh-Bénard convection in an e...
On considère un fluide visqueux conducteur sis entre deux plaques planes, chauffées par en dessous, ...
30 pages, 16 figures, published in JFMInternational audienceWe study nonlinear convection in a rapid...
MAGNETO-CONVECTION IN A RAPIDLY ROTATING SPHERE: NUMERICAL AND EXPERIMENTAL APPROACHES OF THE CONVEC...
In order better to understand the processes that lead to the generation of magnetic fields of finite...
The focus of this study is to investigate primary and secondary bifurcations to weakly nonlinear flo...
International audienceRapidly rotating convection in spherical geometry outside the tangent cylinder...
International audienceWe study numerically an extensive set of dynamo models in rotating spherical s...
The linear stability of the periodic and axisymmetric solutions of the convection in rotating, inter...
The magnetic fields of planets and stars are generated by the motions of electrically conducting flu...
The range of existence and the properties of two essentially different chaotic attractors found in a...
Bistability and hysteresis of magnetohydrodynamic dipolar dynamos generated by turbulent convection ...
A convection-driven multiscale dynamo model is developed in the limit of low Rossby number for the p...