A class of non-stationary exact solutions of two-dimensional nonlinear Navier–Stokes (NS) equations within a thin rotating spherical shell were found as invariant and approximately invariant solutions. The model is used to describe a simple zonally averaged atmospheric circulation caused by the difference in temperature between the equator and the poles. Coriolis effects are generated by pseudoforces, which support the stable west-to-east flows providing the achievable meteorological flows. The model is superimposed by a stationary latitude dependent flow. Under the assumption of no friction, the perturbed model describes zonal west-to-east flows in the upper atmosphere between the Ferrel and Polar cells. In terms of nonlinear modelin...
We present simulations of atmospheres of Earth-like aquaplanets that are tidally locked to their sta...
International audienceConsistent shallow-water equations are derived on the rotating sphere with top...
The steady flow around a rotating sphere at large Reynolds numbers, up to 105, is obtained and analy...
We derive the conserved vectors for the nonlinear two-dimensional Euler equations describi...
We are interested in the onset of instability of the axisymmetric flow between two concentric spheri...
The article proposes a class of exact solutions of the Navier{Stokes equations for a rotating viscou...
Convection in rotating spherical geometries is an important physical process in planetary and stella...
International audienceSufficient conditions are derived for the linear stability with respect to zon...
The surface zonal winds observed in the giant planets form a complex jet pattern with alternating pr...
This is the final version. Available from the American Meteorological Society via the DOI in this re...
International audienceThe generation of mean flows is a long-standing issue in rotating fluids. Moti...
Sufficient conditions are derived for the linear stability with respect to zonally symmetric perturb...
International audienceZonal flows in rapidly-rotating celestial objects such as the Sun, gas or ice ...
We use a linear shallow-water model to investigate the global circulation of the atmospheres of tida...
We investigate properties of convective solutions of the Boussinesq thermal convection in a moderate...
We present simulations of atmospheres of Earth-like aquaplanets that are tidally locked to their sta...
International audienceConsistent shallow-water equations are derived on the rotating sphere with top...
The steady flow around a rotating sphere at large Reynolds numbers, up to 105, is obtained and analy...
We derive the conserved vectors for the nonlinear two-dimensional Euler equations describi...
We are interested in the onset of instability of the axisymmetric flow between two concentric spheri...
The article proposes a class of exact solutions of the Navier{Stokes equations for a rotating viscou...
Convection in rotating spherical geometries is an important physical process in planetary and stella...
International audienceSufficient conditions are derived for the linear stability with respect to zon...
The surface zonal winds observed in the giant planets form a complex jet pattern with alternating pr...
This is the final version. Available from the American Meteorological Society via the DOI in this re...
International audienceThe generation of mean flows is a long-standing issue in rotating fluids. Moti...
Sufficient conditions are derived for the linear stability with respect to zonally symmetric perturb...
International audienceZonal flows in rapidly-rotating celestial objects such as the Sun, gas or ice ...
We use a linear shallow-water model to investigate the global circulation of the atmospheres of tida...
We investigate properties of convective solutions of the Boussinesq thermal convection in a moderate...
We present simulations of atmospheres of Earth-like aquaplanets that are tidally locked to their sta...
International audienceConsistent shallow-water equations are derived on the rotating sphere with top...
The steady flow around a rotating sphere at large Reynolds numbers, up to 105, is obtained and analy...