A high resolution study of the Martian water cycle with a global climate model

Alizée Pottier (1, 2) , Franck Montmessin (1) , François Forget (2) , Thomas Navarro (2) , Ehouarn Millour (2) , Jean-Baptiste Madeleine (2) , Aymeric Spiga (2)

1 PLANETO - LATMOS
2 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)

The martian water cycle's main source is the northern polar cap. Running high resolution models, up to 360° per 180°, help better resolve this ice cap, and better mimic the gradual retreat of the seasonal cap. Atmospheric circulation is also better resolved. Water vapor advection and the subsequent formation of clouds quite differ when we compare these brand new high resolution simulations and the usual lower resolution ones at 64 per 48 grid points.

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Astrophysique stellaire et solaire [astro-ph.SR]; Physique Atmosphérique et Océanique [physics.ao-ph]

Alizée Pottier, Franck Montmessin, François Forget, Thomas Navarro, Ehouarn Millour, et al.. A high resolution study of the Martian water cycle with a global climate model. European Planetary Science Congress 2015, Sep 2015, Nantes, France. pp.EPSC2015-215. ⟨insu-01217131⟩