Thermally driven turbulent flows are omnipresent in nature and technology. A good
understanding of the physical principles governing such flows is key for numerous problems …

The Sun is our nearest star; it is also the most important star that determines life on Earth. A
large variety of phenomena observed on the Sun's surface, with potential impact on Earth, is …

Numerical solutions of partial differential equations enable a broad range of scientific
research. The Dedalus project is a flexible, open-source, parallelized computational …

The seventh edition of this classic text outlines the fundamental physical principles of
thermal radiation, as well as analytical and numerical techniques for quantifying radiative …

Thermal turbulence is well known as a potent means to convey heat across space by a
moving fluid. The existence of the boundary layers near the plates, however, bottlenecks its …

In this paper, we investigate and develop scaling laws as a function of external
nondimensional control parameters for heat and momentum transport for nonrotating, slowly …

The observational absence of giant convection cells near the Sun's outer surface is a long-
standing conundrum for solar modelers. We herein propose an explanation. Rotation …

Planetary atmospheres are commonly thought to result from the efficient outgassing of
cooling magma oceans. During this stage, vigorous convective motions in the molten interior …

In turbulent Rayleigh–Bénard (RB) convection with regular, mono-scale, surface roughness,
the scaling exponent, when the smaller roughness elements fully protrude through the …

Transition to the ultimate regime in a radiatively driven convection experiment Page 1 J. Fluid
Mech. (2019), vol. 861, R5, doi:10.1017/jfm.2018.972 journals.cambridge.org/rapids Transition …