Thanks to the Cassini spacecraft onboard instruments, it has been known that Titan's
ionospheric chemistry is complex and the molecular growth is initiated through the …

Recent observations by the Cassini Orbiter suggest that complex organic chemistry occurs
in the upper atmosphere of Titan. To understand the role of EUV‐VUV light in the complex …

High-energy photons, electrons, and ions initiate ion–neutral chemistry in Titan's upper
atmosphere by ionizing the major neutral species (nitrogen and methane). The Ion and …

The APSIS reactor has been designed to simulate in the laboratory with a VUV synchrotron
irradiation the photochemistry occurring in planetary upper atmospheres. AN 2–CH 4 Titan …

Titan is unique in the solar system as it hosts a dense atmosphere mainly made of molecular
nitrogen N 2 and methane CH 4. The Cassini-Huygens Mission revealed the presence of an …

In the context of recent observations, microphysical models, and laboratory data, a
photochemical model of Titan's atmosphere, including updated chemistry focusing on rate …

The retrieval of data from the Cassini− Huygens mission has revealed much about Titan's
atmospheric-surface system and has precipitated more questions. One of these questions …

Titan, the largest satellite of Saturn, with a dense atmosphere very rich in organics, and
many couplings in the various parts of its “geofluid”, is a reference for studying prebiotic …

The aim of the Titan Haze Simulation (THS) experiment is to contribute to a better
understanding of aerosol formation in Titan's atmosphere through the study of the chemical …

Cassini results indicate that solar photons dominate energy deposition in Titan's upper
atmosphere. These dissociate and ionize nitrogen and methane and drive the subsequent …