Modeling the HDO cycle with the LMD Mars GCM
Résumé
HDO and the D/H ratio are important in order to understand Mars past and present climate, in particular with regards to the evolution through ages of the Martian water cycle. We present here further modeling developments of the HDO cycle with the LMD Mars GCM (Forget et al. 1999), in continuation of the work presented by L. Rossi in session TP16 ("Modeling of the effect of the MY34 Global Dust Storm on the martian HDO cycle."). These improvements are led with the perspective of comparison with the new observations provided by the Atmospheric Chemistry Suite (ACS) on board the ESA/Roscosmos Trace Gas Orbiter.
Domaines
Astrophysique [astro-ph]| Origine | Fichiers produits par l'(les) auteur(s) |
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