The formation of complex organic molecules in a reactor filled with gaseous mixtures
possibly reproducing the primitive terrestrial atmosphere and ocean demonstrated more …

With the exception of in situ atmospheric probes, the most useful way to study the
atmospheres of other planets is to observe their electromagnetic spectra through remote …

A global-mean model of coupled neutral and ion chemistry on Titan has been developed.
Unlike the previous coupled models, the model involves ambipolar diffusion and escape of …

In this paper we present an in-depth study of the distributions of various neutral species in
Titan's upper atmosphere, between 950 and 1500 km for abundant species (N2, CH4, H2) …

The photochemistry of N 2 and CH 4 in the atmosphere of Titan leads to a very rich
chemistry which is not well understood. The aim of our study is to improve our understanding …

In this review I summarize the current state of knowledge about the composition of Titan's
atmosphere and our current understanding of the suggested chemistry that leads to that …

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 …

Observations of the Composite InfraRed Spectrometer (CIRS) during the entire nominal
Cassini mission (2004–2008) provide us with an accurate global view of composition and …

This paper reports on the results from an extensive study of all nadir-looking spectra
acquired by Cassini/CIRS during the 44 flybys performed in the course of the nominal …

Stellar occultations observed by the Cassini/UVIS instrument provide unique data that probe
the mesosphere and lower thermosphere of Titan at altitudes between 400 and 1400km …