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
2 GSMA - Groupe de spectrométrie moléculaire et atmosphérique
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
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Poster communications
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https://hal-insu.archives-ouvertes.fr/insu-01373846
Contributor : Catherine Cardon <>
Submitted on : Thursday, September 29, 2016 - 11:59:03 AM
Last modification on : Wednesday, February 5, 2020 - 2:02:11 PM
Long-term archiving on: Friday, December 30, 2016 - 12:51:09 PM

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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. ⟨insu-01373846⟩

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