The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …

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 …

Self-sustained convective dynamos in planetary systems operate in an asymptotic regime of
rapid rotation, where a balance is thought to hold between the Coriolis, pressure, buoyancy …

Rayleigh–Bénard convection in rotating spherical shells can be considered as a simplified
analogue of many astrophysical and geophysical fluid flows. Here, we use three …

Thermal interactions between Earth's core and mantle provide the power that maintains the
geomagnetic field. However, the effect of these interactions and, in particular, the …

Ocean worlds are prevalent in the solar system. Focusing on Enceladus, Titan, Europa, and
Ganymede, I use rotating convection theory and numerical simulations to predict ocean …

Convection is a fundamental physical process in the fluid cores of planets. It is the primary
transport mechanism for heat and chemical species and the primary energy source for …

Rotating Rayleigh–Bénard convection is a simple model system used to study the interplay
of buoyant forcing and rotation. Many recent studies have focused on the geostrophic …

Soil-rock mixture (S/RM) is a very complex discontinuous medium material, which is a
multiphase system consisting of high strength rock blocks (Rocks), relatively soft filling …

The geostrophic turbulence in rapidly rotating thermal convection exhibits characteristics
shared by many highly turbulent geophysical and astrophysical flows. In this regime, the …