Julianne I. Moses

TL;DR: In this article, the meridional variations of diacetylene and methylacetylene mixing ratios in the stratosphere of Saturn's stratosphere were analyzed using the Cassini/CIRS data.

TL;DR: In this paper, the authors investigated how the thermal structure and concentrations of acetylene and ethane have evolved with the changing season on Saturn, and retrieved the vertical temperature profiles and the volume mixing ratios from Δ ν = 15.5 cm -1 Cassini-CIRS observations.

TL;DR: A review of the current knowledge of the molecular, elemental, and isotopic composition and atmospheric chemistry in Saturn's shallow atmosphere can be found in this article, where the authors present the current 1D thermochemical and photochemical models, how these models fare to reproduce the observed composition, and first attempts to design 2D chemical models.

TL;DR: In this paper, the authors outline a number of areas where laboratory or ab initio investigations could fill critical gaps in our ability to model exoplanet atmospheric opacities, clouds, and chemistry.

TL;DR: In this paper, the authors performed laboratory experiments with the PHAZER chamber to simulate haze formation in a range of exoplanet atmospheres (hydrogen-rich, water-rich and carbon dioxide-rich at 300, 400, and 600 K).