Day-Night Cloud Asymmetry Inhibits Early Ocean Formation on Venus and Telluric Planets
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en
Communication dans un congrès
Ce document a été publié dans
Ancient Venus Conference 2022, 2022-07, Online. 2022-07p. LPI Contribution No. 2680, id.2009
Résumé en anglais
We will present the results of new 3-D Global Climate Model (GCM) simulations aimed at reproducing the conditions of primordial surface water condensation and thus of the formation of ancient oceans on Venus.
We will present the results of new 3-D Global Climate Model (GCM) simulations aimed at reproducing the conditions of primordial surface water condensation and thus of the formation of ancient oceans on Venus.< Réduire
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