Haze, Methane, and Carbon Monoxide in Titan’s North Polar Atmosphere from a Cassini/VIMS Specular Transmission Spectrum on the T104 Flyby

We analyze a specular reflection of the Sun off of Titan’s largest sea, Kraken Mare, observed by the Cassini Visual and Infrared Mapping Spectrometer on the T104 flyby (2014 August 21). We use the specularly reflected I / F signal to derive a transmission spectrum. Owing to the low incidence and emi...

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Prif Awduron:	Jason W. Barnes, Connor T. O’Neill, Shannon M. MacKenzie, William J. Miller, Gabriel M. Steward, Maël Es-sayeh, Sebastien Rodriguez, Paul M. Corlies, Jason M. Soderblom
Fformat:	Artigo
Iaith:	Inglês
Cyhoeddwyd:	IOP Publishing 2026-01-01
Cyfres:	The Planetary Science Journal
Pynciau:	Titan Natural satellite atmospheres Transmission spectroscopy
Mynediad Ar-lein:	https://doi.org/10.3847/PSJ/ae40b0
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