Atmospheric Physics, Chemistry and Climate
Models
The atmospheric Physics, Chemistry and Climate division is continuously improving and/or developing a hierarchy of models from global coupled atmosphere-ocean-land-ice model to study climate change, to Large Eddy Simulation (LES) model to study small scale physical processes. Some version of these models contain full chemistry of the troposphere and stratosphere, cloud microphysics, detail representation of physical processes like dry and wet convection. Specific configuration has been developed to simulate extraterrestrial atmosphere, in particular Mars. A key component in our models is the radiative transfer calculation of longwave and shortwave radiation with codes developed in-house. Some new parameterization are implemented in specific models to facilitate their evaluation. This is the case of the WRF mesoscale model to test a new representation of clouds microphysics or the transport model GCTMÂ to study ocean productivity by aeolian dust deposition.
Name | Description | Contact |
---|---|---|
CM3 | Coupled Atmosphere Ocean Land Ice model version 3 | Larry Horowitz |
AM3 | Atmospheric Model version 3 | Leo Donner |
AM3strat | Atmospheric Model version 3 with J Austin stratospheric chemistry | John Austin |
AM2 | Atmospheric Model version 2 | |
AM2n | Atmospheric Model version 2 with aerosols and nudging | Paul Ginoux |
Mars-GCM | Global Martian atmospheric model | John Wilson |
GCTM | Global transport model of chemical tracers | Bud Moxim |
WRF | Mesoscale model | Charles Seman |
LES | Large Eddy Simulation Model | Chris Golaz |
Radiation codes | Transfert radiative codes:
|
Dan Schwarzkopf Stuart Feidenreich |
Radiative Forcing | Radiative forcing with stratospheric adjustments | Dan Schwarzkopf |