Microphysical modeling of the Venusian clouds with the IPSL Venus GCM

Abstract : To understand the Venus atmosphere, LMD and LATMOS laboratories have developed a 3D IPSL Venus Global Climate Model (Lebonnois et al. 2010). In this GCM, the cloud description is simplified. As clouds play a crucial role in radiative transfer, dynamics and generally the climate of Venus, it is necessary to improve the VGCM with a microphysical representation.
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Sabrina Guilbon, Anni Määttänen, Franck Montmessin, Jérémie Burgalat, Sébastien Lebonnois, et al.. Microphysical modeling of the Venusian clouds with the IPSL Venus GCM. European Planetary Science Congress 2017, Sep 2017, Riga, Latvia. pp.EPSC2017-571. ⟨insu-01593730⟩

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