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...

Descripció completa

Dades bibliogràfiques

Autors principals:	Coutelier Maélie, Gautier Thomas, Das Koyena, Serigano Joseph, Westlake Joseph, Hörst Sarah M., Trainer Melissa G.
Format:	Artigo
Idioma:	Inglês
Publicat:	EDP Sciences 2026-04-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	methods: data analysis planets and satellites: atmospheres planets and satellites: composition planets and satellites: individual: titan
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/04/aa48044-23/aa48044-23.html
Etiquetes:	Afegir etiqueta Sense etiquetes, Sigues el primer a etiquetar aquest registre!