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astro-ph.EP2024
A photochemical PHO network for hydrogen-dominated exoplanet atmospheres
Elspeth K. H. Lee, Shang-Min Tsai, Julianne I. Moses +3
Due to the detection of phosphine PH3 in the Solar System gas giants Jupiter and Saturn, PH3 has long been suggested to be detectable in exosolar substellar atmospheres too. Howeve…
astro-ph.EP2023
Structure, variability, and origin of the low-latitude nightglow continuum between 300 and 1,800 nm: Evidence for HO emission in the near-infrared
Stefan Noll, John M. C. Plane, Wuhu Feng +5
The Earth's mesopause region between about 75 and 105 km is characterised by chemiluminescent emission from various lines of different molecules and atoms. This emission was and is…