Titan is the only moon with a substantial atmosphere, the only other thick N2 atmosphere
besides Earth's, the site of extraordinarily complex atmospheric chemistry that far surpasses …

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 …

We use a 3‐D general circulation model to compare the primitive Martian hydrological cycle
in “warm and wet” and “cold and icy” scenarios. In the warm and wet scenario, an …

In this paper, the effect of a simple convection scheme on the zonally averaged tropical
general circulation is examined within an idealized moist GCM to obtain broad …

Cassini RADAR observations now permit an initial assessment of the inventory of two
classes, presumed to be organic, of Titan surface materials: polar lake liquids and equatorial …

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 …

Cassini's Imaging Science Subsystem (ISS) has been observing Titan since April 2004,
compiling a nearly global surface map and monitoring the surface and atmosphere for …

Efforts to characterize extrasolar giant planet (EGP) atmospheres have so far emphasized
planets within 0.05 AU of their stars. Despite this focus, known EGPs populate a continuum …

Simulation results are presented from a new general circulation model (GCM) of Titan, the
Titan Atmospheric Model (TAM), which couples the Flexible Modeling System (FMS) spectral …