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The Venus Climate Database Project
The
Venus Climate Database
(web interface)
To get the full version, please follow this
link
or contact
sebastien.lebonnois@lmd.ipsl.fr,ehouarn.millour@lmd.ipsl.fr
The IPSL
Venus Climate Model
Our Venus GCM includes a full radiative transfert and accounts for atmospheric composition and cloud microphysics. It routinely resolves circulation from the surface to 100km, but may also include the thermosphere up to ~250km (
Lebonnois et al.
2010
,
2016
,
2018
,
Gilli et al.
2017
,
2021
,
Garate-Lopez and Lebonnois
2018
,
Navarro et al.
2021
).
The Venus GCM is freely available; contact
Sébastien Lebonnois
The
Venus Mesoscale Model
(
Lefevre et al.
2017
,
2018
,
2020
) : The WRF dynamical core, coupled to the Venus GCM's physics package, enables to study meso- and micro-scale processes such as convection or small scale gravity waves. Contact
Aymeric Spiga
Related
:
Virtual Observatory data access through the
VESPA
(Virtual European Solar and Planetary Access) portal:
http://vespa.obspm.fr/planetary/data/display/?&service_id=ivo://lmd.jussieu/vcd/q/epn_core&service_type=epn
VCD VESPA service
user Manual
The Planetary Climates Database Project