Comparison of a sectional and a modal cloud microphysics representations for Venus: VenLA vs. MAD-VenLA

Sabrina Guilbon 1 Anni Määttänen 1 Franck Montmessin 1 Jeremie Burgalat 2 Slimane Bekki 3
1 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
3 STRATO - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
Abstract : 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
Type de document :
Poster
International Venus Conference 2016, Apr 2016, Oxford, United Kingdom. 〈https://venus2016.uk/〉
Liste complète des métadonnées

https://hal-insu.archives-ouvertes.fr/insu-01373846
Contributeur : Catherine Cardon <>
Soumis le : jeudi 29 septembre 2016 - 11:59:03
Dernière modification le : mercredi 19 septembre 2018 - 01:36:52
Document(s) archivé(s) le : vendredi 30 décembre 2016 - 12:51:09

Fichier

Venus_Conf_Oxford-v2.pdf
Fichiers produits par l'(les) auteur(s)

Identifiants

  • HAL Id : insu-01373846, version 1

Collections

Citation

Sabrina Guilbon, Anni Määttänen, Franck Montmessin, Jeremie Burgalat, Slimane Bekki. Comparison of a sectional and a modal cloud microphysics representations for Venus: VenLA vs. MAD-VenLA. International Venus Conference 2016, Apr 2016, Oxford, United Kingdom. 〈https://venus2016.uk/〉. 〈insu-01373846〉

Partager

Métriques

Consultations de la notice

177

Téléchargements de fichiers

42