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

The cores of main sequence intermediate-and high-mass stars are convective. Mixing at the
radiative–convective boundary, waves excited by the convection, and magnetic fields …

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 …

We investigate heat transport associated with compositionally driven convection driven by
crystallization at the ocean–crust interface in accreting neutron stars, or growth of the solid …

About 10 per cent of intermediate-and high-mass dwarf stars are observed to host a strong
large-scale magnetic field at their surface, which is thought to be of fossil field origin …

This study investigates the adjustment of large‐scale localized buoyancy anomalies in mid‐
latitude regions and the nonlinear evolution of associated condensation patterns in both …

Massive stars die in catastrophic explosions that seed the interstellar medium with heavy
elements and produce neutron stars and black holes. Predictions of the explosion's …

By means of a new multilayer pseudo‐spectral moist‐convective thermal rotating shallow‐
water (mcTRSW) model in a full sphere, we present a possible equatorial adjustment …

The magnetic dynamo cycle of the Sun features a distinct pattern: a propagating region of
sunspot emergence appears around 30° latitude and vanishes near the equator every 11 …

We present a simulation code which can solve a broad range of partial differential equations
in a full sphere. The code expands tensorial variables in a spectral series of spin-weighted …