3 papers
astro-ph.EP2026
Cloud and ammonia vertical profiles in the equatorial atmosphere of Jupiter determined from visible to near-IR observations made by VLT/MUSE, Cassini/VIMS, IRTF/SpeX and Juno/JIRAM
Patrick G. J. Irwin, Asier Anguiano-Arteaga, Michelle Colantoni +8
We present a combined cloud/ammonia model for Jupiter's equatorial atmosphere from 0.1 to 10 bar, consistent with observations made at a range of observation geometries from 0.35 t…
astro-ph.EP2025
Using SOFIA's EXES to search for CH and CN in Titan's atmosphere
Zachary C. McQueen, Conor A. Nixon, Curtis de Witt +7
In Titan's atmosphere, the chemistry of small hydrocarbons and nitriles represent an important link from molecular species to the ubiquitous organic haze that gives Titan its chara…
astro-ph.IM2025
archNEMESIS: an open-source Python package for analysis of planetary atmospheric spectra
Juan Alday, Joseph Penn, Patrick G. J. Irwin +2
ArchNEMESIS is an open-source Python package developed for the analysis of remote sensing spectroscopic observations of planetary atmospheres. It is based on the widely used NEMESI…