Difference between revisions of "Overview of the Venus PCM"
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In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or WRF (limited area dynamical core). | In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or WRF (limited area dynamical core). | ||
| + | The traditional Venus PCM - LMDZ (formerly know as the IPSL Venus GCM) is the most commonly used version. | ||
| + | |||
| + | == Bibliography == | ||
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| + | TODO: Add reference articles here | ||
| − | [Category:Venus-Model] | + | [[Category:Venus-Model]] |
Revision as of 14:23, 26 May 2023
Welcome to the overview page of the Venus Planetary Climate Model
The Venus PCM (Planetary Climate Model)
In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or WRF (limited area dynamical core).
The traditional Venus PCM - LMDZ (formerly know as the IPSL Venus GCM) is the most commonly used version.
Bibliography
TODO: Add reference articles here
