We have developed a one-dimensional photochemical and thermochemical kinetics and
diffusion model to study the effects of disequilibrium chemistry on the atmospheric …

The formation of Titan's induced magnetosphere is a unique and important example in the
solar system of a plasma-moon interaction where the moon has a substantial atmosphere …

In this paper, we analyze the strong unidentified emission near 3.28 μm in Titan's upper
daytime atmosphere recently discovered by Dinelli et al. We have studied it by using the …

Fluvial features on Titan have been identified in synthetic aperture radar (SAR) data taken
during spacecraft flybys by the Cassini Titan Radar Mapper (RADAR) and in Descent …

Complex organic materials may exist as haze layers in the atmosphere of Titan and as dark
coloring agents on icy satellite surfaces. Laboratory measurements of optical constants of …

Abstract Observations with the Electron Spectrometer sensor of the Cassini Plasma
Spectrometer (CAPS‐ELS) have revealed the existence of negative ions in Titan's …

The discovery of carbocations and carbanions by Ion Neutral Mass Spectrometer (INMS)
and the Cassini Plasma Spectrometer (CAPS) instruments onboard the Cassini spacecraft in …

Previous authors have suggested that Titan's individual sand particles form by either
sintering or by lithification and erosion. We suggest two new mechanisms for the production …

In this paper, we provide a detailed review of Ganymede's characteristics that are germane
to any consideration of its planetary protection requirements. Ganymede is the largest moon …

The importance of the heavy ions and dust grains for the chemistry and aerosol formation in
Titan's ionosphere has been well established in the recent years of the Cassini mission. In …