We present a suite of seven 3D supernova simulations of non-rotating low-mass progenitors
using multigroup neutrino transport. Our simulations cover single star progenitors with zero …

The atmospheres of synchronously rotating exoplanets are intrinsically 3D, and fast vertical
and horizontal winds are expected to mix the atmosphere, driving the chemical composition …

Spectral features in the observed spectra of exoplanets depend on the composition of their
atmospheres. A good knowledge of the main atmospheric processes that drive the chemical …

We present WASP-43b climate simulations with deep wind jets (down to 700 bar) that are
linked to retrograde (westward) flow at the equatorial day side for p< 0.1 bar. Retrograde …

The era of atmospheric characterization of terrestrial exoplanets is just around the corner.
Modeling prior to observations is crucial in order to predict the observational challenges and …

We have designed and developed, from scratch, a global circulation model (GCM) named
THOR that solves the three-dimensional nonhydrostatic Euler equations. Our general …

General circulation models (GCMs) provide context for interpreting multiwavelength,
multiphase data of the atmospheres of tidally locked exoplanets. In the current study, the non …

Sub-Neptunes (planets with radii between 2 and 4 R⊕) are abundant around M-dwarf stars,
yet the atmospheric dynamics of these planets is relatively unexplored. In this paper, we aim …

The atmospheric circulation of tidally locked planets is dominated by a superrotating
eastward equatorial jet. We develop a predictive theory for the formation of this jet …

Consider an incompressible fluid in a region Ωf flowing both ways across an interface into a
porous media domain Ωp saturated with the same fluid. The physical processes in each …