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 …

The entry, descent and landing of Schiaparelli, the ExoMars Entry, descent and landing
Demonstrator Module (EDM), offered a rare (once-per-mission) opportunity for in situ …

The presence of winds in Titan's lower and middle atmosphere has been determined by a
variety of techniques, including direct measurements from the Huygens Probe over 0–150 …

Abstract Pluto, Titan and Triton all have low-temperature environments with an N2, CH4 and
CO atmospheric composition in which solar radiation drives an intense organic …

The temperature structure of Titan's upper atmosphere exhibits large variability resulting
from numerous spatially and temporally irregular external energy sources, seasonal …

We present a detailed model for the vibrational population of all non pre-dissociating excited
electronic states of N 2, as well as for the ground and ionic states, in Titan's atmosphere. Our …

We use two independent General Circulation Models (GCMs) to estimate surface winds at
Titan's Ligeia Mare (78° N, 250° W), motivated by a proposed mission to land a floating …

Abstract On 19th October 2016 Schiaparelli module of the ExoMars 2016 mission flew
through the Mars atmosphere. After successful entry and descent under parachute, the …

Analysis of the Cassini Ion Neutral Mass Spectrometer data reveals the omnipresence of
density waves in various constituents of Titan's upper atmosphere, with quasi‐periodical …

The Huygens probe recorded atmospheric temperatures during its parachute descent
through the atmosphere of Titan. A careful analysis of these data reveals for the first time …