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

The heat transfer and flow structure in rotating Rayleigh-Bénard convection are strongly
influenced by the Rayleigh (Ra), Prandtl (Pr), and Rossby (Ro) numbers. For Pr≳ 1 and …

Numerical and experimental data for the heat transfer as a function of the Rossby number
Ro in turbulent rotating Rayleigh-Bénard convection are presented for the Prandtl number …

Rotating Rayleigh–Bénard convection is typified by a variety of regimes with very distinct
flow morphologies that originate from several instability mechanisms. Here we present …

We report results from Direct Numerical Simulation (DNS) of rotating Rayleigh–Bénard
convection, regarding the scaling of heat transfer with the Rayleigh number for rotating …

The effect of rotation on the boundary layers (BLs) in a Rayleigh–Bénard system at a
relatively low Rayleigh number, ie, Ra= 4× 10 7⁠, is studied for different Pr by direct …

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

Measurements of the Nusselt number Nu and of properties of the large-scale circulation
(LSC) for turbulent Rayleigh–Bénard convection are presented in the presence of rotation …

Numerical data for the heat transfer as a function of the Prandtl (Pr) and Rossby (Ro)
numbers in turbulent rotating Rayleigh–Bénard convection are presented for Rayleigh …

When the classical Rayleigh–Bénard (RB) system is rotated about its vertical axis roughly
three regimes can be identified. In regime I (weak rotation) the large-scale circulation (LSC) …