Difference between revisions of "Main Page"
From Planets
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# Long-term volatile/ice cycling on Pluto and Triton | # Long-term volatile/ice cycling on Pluto and Triton | ||
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Revision as of 09:24, 29 March 2023
Welcome to the wiki of the Planetary Climate Models (PCM) family! Our numerical climate models cover a wide range of planets described below.
- With the Generic Models:
- Exoplanets of all kinds (rocky planets, super-Earths, mini-Neptunes, hot Jupiters, etc.)
- Paleoclimates of Solar System planets (e.g., to simulate lakes and glacier on Hesperian/Noachian Mars ; snowball episodes or exploring the Faint Young Sun on Earth ;
formation and stability of early ocean on Venus ; episodes of atmospheric collapse on Titan)
- Giant planets (Jupiter, Saturn, Uranus, Neptune)
- With the Mars Models:
- Present-day Mars climate (with water and dust cycles)
- Recent-Mars paleoclimates (e.g., during Amazonian epoch, to simulate low and high-obliquity epochs)
- Regional and local weathers on Mars (e.g. to simulate weather near Mars rover landing sites)
- With the Venus models:
- Present-day Venus climate
- Regional weather on Venus (e.g. to simulate the convection in the cloud layer)
- With the Titan models:
- Present-day Titan
- Regional and local weather on Titan
- With the Pluto/Triton models:
- Present-day Pluto/Triton climate
- Long-term volatile/ice cycling on Pluto and Triton
You can use the menu on the left to navigate across our webpages.
