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Seasonal variation of the main gases in Titan's ionosphere from Cassini INMS data

With 13 years of observations, the Ion and Neutral Mass Spectrometer (INMS) on board the Cassini spacecraft has observed the upper atmosphere of Titan through two seasons: northern winter and spring. The complex atmosphere is mainly composed of N2, CH4, H2, and Ar, but many other carbon and nitrogen...

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Autori principali: Coutelier Maélie, Gautier Thomas, Das Koyena, Serigano Joseph, Westlake Joseph, Hörst Sarah M., Trainer Melissa G.
Natura: Artigo
Lingua:Inglês
Pubblicazione: EDP Sciences 2026-04-01
Serie:Astronomy & Astrophysics
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Accesso online:https://www.aanda.org/articles/aa/full_html/2026/04/aa48044-23/aa48044-23.html
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