We present a one-dimensional coupled ion-neutral photochemical kinetics and diffusion
model to study the atmospheric composition of Titan in light of new theoretical kinetics …

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 Cosmic Shoreline: The Evidence that Escape Determines which Planets Have Atmospheres,
and what this May Mean for Proxima Centauri B - IOPscience This site uses cookies. By …

We present a comprehensive photochemistry model for exploration of the chemical
composition of terrestrial exoplanet atmospheres. The photochemistry model is designed …

This paper is a review dealing with the photochemistry of Titan's atmosphere and its sources
of uncertainties. It presents current knowledge on the active photochemistry occurring in …

We have developed a one‐dimensional, diurnally averaged, photochemical model for
Jupiter's stratosphere that couples photodissociation, chemical kinetics, vertical diffusion …

We introduce a new 1D coupled Radiative/Convective-Photochemical-Microphysical model
for a planetary atmosphere and apply it to Titan. The model incorporates detailed radiation …

Recently, properties of exoplanet atmospheres have been constrained via multi-wavelength
transit observation, which measures an apparent decrease in stellar brightness during …

The nearby TRAPPIST-1 planetary system is an exciting target for characterizing the
atmospheres of terrestrial planets. The planets e, f, and g lie in the circumstellar habitable …

In this chapter we describe the current knowledge of a selection of collision processes and
chemical reactions of importance to planetary aeronomy. Emphasis is placed on critical …