Comparison of a sectional and a modal cloud microphysics representations for Venus: VenLA vs. MAD-VenLA - INSU - Institut national des sciences de l'Univers Access content directly
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Comparison of a sectional and a modal cloud microphysics representations for Venus: VenLA vs. MAD-VenLA

Sabrina Guilbon
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Anni Määttänen
Franck Montmessin
Slimane Bekki

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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Dates and versions

insu-01373846 , version 1 (29-09-2016)

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  • HAL Id : insu-01373846 , version 1

Cite

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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