Rotation with thermally induced buoyancy governs many astrophysical and geophysical
processes in the atmosphere, ocean, sun, and Earth's liquid-metal outer core. Rotating …

Tuning transport properties through the manipulation of elementary structures has achieved
great success in many areas, such as condensed matter physics. However, the ability to …

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 …

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 …

We present laboratory and numerical models investigating the behavioural regimes of
rapidly rotating convection in high-latitude planetary core-style settings. Our combined …

We studied the flow organization and heat transfer properties in two-dimensional and three-
dimensional Rayleigh–Bénard cells that are imposed with different types of wall shear. The …

We study the influence of thermal boundary conditions on large aspect ratio Rayleigh–
Bénard convection by a joint analysis of experimental and numerical data sets for a Prandtl …

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

Thermal convection is the dominant mechanism of energy transport in the outer envelope of
the Sun (one-third by radius). It drives global fluid circulations and magnetic fields observed …

We conduct numerical investigations on turbulent Rayleigh–Bénard (RB) convection
modulated by oscillating filaments, where an array of active filaments is adhered to the …