Add to ORKGThe convective stability of a viscous liquid in spherical layers is investigated taking into consideration rotation, the latitudinal temperature gradient, and shear flow. The results of calculating nonlinear convective motion in spherical layers are examined. A discussion is given of the applicability of the results obtained to studying convection in astrophysical objects
The study of thermal convection in rotating spherical geometry is fundamental to explain many geophy...
A wide range of fluid flows occur within astrophysical bodies such as stars and planets. In particul...
A wide range of fluid flows occur within astrophysical bodies such as stars and planets. In particul...
The principal concern of this paper is with the thermal convective instabilities of a non-uniformly ...
The numerical investigation of convective flows in the radial force field caused by an oscillating e...
The principal concern of this paper is with the thermal convective instabilities of a non-uniformly ...
Steady state, axisymmetric motions of a Boussineaq fluid continued in rotating spherical anmulus are...
Many celestial objects are thought to host interfaces between convective and stable stratified inter...
Convective stability and thermodynamic properties of infinite horizontal thin polytropic layer subje...
A formulation of the fluid dynamics of convective regions is developed which leads to an analytical ...
Tesi per compendi de publicacionsThe study of thermal convection in rotating spherical geometry is f...
Tesi per compendi de publicacionsThe study of thermal convection in rotating spherical geometry is f...
The convective flow of a self gravitating sphere of Boussinesq fluid for small Reynolds and Peclet n...
Bottom-heated convection in rotating spherical shells provides a simple analogue for many astrophysi...
Thesis (M.S.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1969.Bi...
The study of thermal convection in rotating spherical geometry is fundamental to explain many geophy...
A wide range of fluid flows occur within astrophysical bodies such as stars and planets. In particul...
A wide range of fluid flows occur within astrophysical bodies such as stars and planets. In particul...
The principal concern of this paper is with the thermal convective instabilities of a non-uniformly ...
The numerical investigation of convective flows in the radial force field caused by an oscillating e...
The principal concern of this paper is with the thermal convective instabilities of a non-uniformly ...
Steady state, axisymmetric motions of a Boussineaq fluid continued in rotating spherical anmulus are...
Many celestial objects are thought to host interfaces between convective and stable stratified inter...
Convective stability and thermodynamic properties of infinite horizontal thin polytropic layer subje...
A formulation of the fluid dynamics of convective regions is developed which leads to an analytical ...
Tesi per compendi de publicacionsThe study of thermal convection in rotating spherical geometry is f...
Tesi per compendi de publicacionsThe study of thermal convection in rotating spherical geometry is f...
The convective flow of a self gravitating sphere of Boussinesq fluid for small Reynolds and Peclet n...
Bottom-heated convection in rotating spherical shells provides a simple analogue for many astrophysi...
Thesis (M.S.)--Massachusetts Institute of Technology, Dept. of Earth and Planetary Sciences, 1969.Bi...
The study of thermal convection in rotating spherical geometry is fundamental to explain many geophy...
A wide range of fluid flows occur within astrophysical bodies such as stars and planets. In particul...
A wide range of fluid flows occur within astrophysical bodies such as stars and planets. In particul...