Comparison of a sectional and a modal cloud microphysics representations for Venus: VenLA vs. MAD-VenLA
Résumé
Here, we present a status report of MAD-VenLA. The results of the thermodynamical equilibrium and the homogeneous nucleation are similar between VenLA and MAD-VenLA. For the condensational process, with the same initial state and particle distribution, we can see a difference between MAD-VenLA and VenLA. In fact, the sectional model condense more than the modal representation. The validation of MAD-VenLA will be done with all processes and a comparison with baseline high-resolution models in literature
Domaines
Astrophysique [astro-ph]Origine | Fichiers produits par l'(les) auteur(s) |
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