Modeling the HDO cycle with the LMD Mars GCM - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2020

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.
Fichier principal
Vignette du fichier
EPSC2020-680.pdf (360.92 Ko) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)

Dates et versions

hal-04492906 , version 1 (06-03-2024)

Identifiants

Citer

Margaux Vals, Loïc Rossi, Franck Montmessin, François Forget, Ehouarn Millour, et al.. Modeling the HDO cycle with the LMD Mars GCM. Europlanet Science Congress 2020, Sep 2020, Online, Unknown Region. pp.EPSC2020-680, ⟨10.5194/epsc2020-680⟩. ⟨hal-04492906⟩
29 Consultations
1 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More