Understanding fluid flows in planetary cores and subsurface oceans, as well as their
signatures in available observational data (gravity, magnetism, rotation, etc.), is a …

A Model of Rotating Convection in Stellar and Planetary Interiors. II. Gravito-inertial Wave
Generation - IOPscience Skip to content IOP Science home Accessibility Help Search all …

Direct numerical simulations are employed to reveal three distinctly different flow regions in
rotating spherical Rayleigh‐Bénard convection. In the high‐latitude region vertical (parallel …

Fluid flow excited by a core oscillating in a rotating spherical cavity is experimentally
investigated. Oscillations are set by an external inertial field so that in the reference frame of …

This work is devoted to an experimental study of the stability of a steady flow in a rotating
spherical cavity with an oscillating core. The case of circular core oscillations in a plane …

The spherical Couette system, consisting of a viscous fluid between two differentially rotating
concentric spheres, is studied using numerical simulations and compared with experiments …

The problem of determining a mean flow induced by longitudinal libration of a rapidly
rotating fluid-filled container bounded by the surfaces of two oppositely oriented right circular …

The existence of triadic resonances in the magnetized spherical Couette system is related to
the development of modulated rotating waves, which are quasiperiodic flows understood in …

Rotating fluids frequently show nonlinear wave interactions and turbulence. This is true in
particular for nonuniformly rotating systems. One example of such a nonuniform rotating …

The spherical Couette system consists of two differentially rotating concentric spheres with
the space in between filled with fluid. We study a regime where the outer sphere is rotating …