An accurate description of turbulent core convection is necessary in order to build robust
models of planetary core processes. Towards this end, we focus here on the physics of …

The heat transfer scaling theories for Rayleigh‐Bénard convection (RBC) are reviewed and
discussed for configurations with and without rotation and magnetic fields. Scaling laws are …

Turbulent Rayleigh-Bénard convection displays a large-scale order in the form of rolls and
cells on lengths larger than the layer height once the fluctuations of temperature and velocity …

Rapidly rotating Rayleigh–Bénard convection is studied using an asymptotically reduced
equation set valid in the limit of low Rossby numbers. Four distinct dynamical regimes are …

Numerical simulations of three-dimensional rapidly rotating Rayleigh–Bénard convection
are performed by employing an asymptotic quasi-geostrophic model that incorporates the …

Here we summarize the results from our direct numerical simulations (DNS) and
experimental measurements on rotating Rayleigh–Bénard (RB) convection. Our …

It is proposed that critical balance–a scale-by-scale balance between the linear propagation
and nonlinear interaction time scales–can be used as a universal scaling conjecture for …

A reduced model is developed for low-Rossby-number convection in a plane layer geometry
with no-slip upper and lower boundaries held at fixed temperatures. A complete description …

The interplay between convective, rotational and magnetic forces defines the dynamics
within the electrically conducting regions of planets and stars. Yet their triadic effects are …

This work studies two-dimensional fixed-flux Rayleigh–Bénard convection with periodic
boundary conditions in both horizontal and vertical directions and analyses its dynamics …