We review our current knowledge of the atmospheric dynamics of Venus prior to the
Akatsuki mission, in the altitude range from the surface to approximately the cloud tops …

Tide-locked planets are planets in which tidal stresses from the host star have spun down
the planet's rotation to the point where its length of sidereal day equals its length of year. In a …

The increasing richness of exoplanet observations has motivated a variety of three-
dimensional (3D) atmospheric circulation models of these planets. Under strongly irradiated …

A planetary atmosphere is the outer gas layer of a planet. Besides its scientific significance
among the first and most accessible planetary layers observed from space, it is closely …

Using a 3D general circulation model (GCM), we investigate the sensitivity of the climate of
tidally locked Earthlike exoplanets, Trappist-1e and Proxima Centauri b, to the choice of a …

The recent discoveries of terrestrial exoplanets and super-Earths extending over a broad
range of orbital and physical parameters suggest that these planets will span a wide range …

We have developed a new 3-dimensional climate model for Titan's atmosphere, using the
physics of the IPSL Titan 2-dimensional climate model with the current version of the LMDZ …

Using a 3D general circulation model, we demonstrate that a confirmed rocky exoplanet and
a primary observational target, TRAPPIST-1e presents an interesting case of climate …

The superrotation of the atmospheres of Venus and Titan has puzzled dynamicists for many
years and seems to put these planets in a very different dynamical regime from most other …

Over the past decade, the Cassini-Huygens mission to the Saturn system has revolutionized
our understanding of Titan and its climate. Veiled in a thick organic haze, Titan's visible …