181 citations · 2k across the 49 of their papers we have counts for
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Vertical Structure and Color of Jovian Latitudinal Cloud Bands during the Juno Era
Emma K. Dahl, Nancy J. Chanover, Glenn S. Orton +6
The identity of the coloring agent(s) in Jupiter's atmosphere and the exact structure of Jupiter's uppermost cloud deck are yet to be conclusively understood. The Crème Brûlée mode…
Uranus' stratospheric HCl upper limit from Herschel/SPIRE
Nicholas A. Teanby, Patrick G. J. Irwin
Herschel/SPIRE observations of Uranus are used to search for stratospheric hydrogen chloride (HCl) emission at 41.74 cm. HCl was not detected and instead 3 upper limits w…
Detection of Cyclopropenylidene on Titan with ALMA
Conor A. Nixon, Alexander E. Thelen, Martin A. Cordiner +7
We report the first detection on Titan of the small cyclic molecule cyclopropenylidene (c-C3H2) from high sensitivity spectroscopic observations made with the Atacama Large Millime…
Detection of CHCN in Titan's Atmosphere
A. E. Thelen, M. A. Cordiner, C. A. Nixon +6
Titan harbors a dense, organic-rich atmosphere primarily composed of N and CH, with lesser amounts of hydrocarbons and nitrogen-bearing species. As a result of high sensiti…
Jupiter in the ultraviolet: acetylene and ethane abundances in the stratosphere of Jupiter from Cassini observations between 0.15 and 0.19 m
Henrik Melin, Leigh N. Fletcher, Pat G. J. Irwin +1
At wavelengths between 0.15 and 0.19 m, the far-ultraviolet spectrum of Jupiter is dominated by the scattered solar spectrum, attenuated by molecular absorptions primarily by ac…
Understanding and Mitigating Biases when Studying Inhomogeneous Emission Spectra with JWST
Jake Taylor, Vivien Parmentier, Patrick G. J. Irwin +3
Exoplanet emission spectra are often modelled assuming that the hemisphere observed is well represented by a horizontally homogenised atmosphere. However this approximation will li…