- Working Groups
As a deep time modeler, you are responsible for creating a new topography file which you will point to in the user_nl_cam namelist. You also specify trace gas constituents and the solar constant in user_nl_cam, if they differ from pre-industrial. The CESM User Guide describes the user namelist functionality in CESM1.
The atmosphere component model requires initial boundary conditions, including fractional landcover (LANDFRAC), topography (PHIS), surface roughness, (SGH), and high resolution surface roughness (SGH30), and an aerosol scaling factor (LANDM_COSLAT). For deep time, surface roughness is approximated by multiplying the surface topography by 0.3 and 0.1, respectively.
NOTE: Angular, highly variable topography can cause instability in the CAM atmosphere model that is difficult to detect but may cause the model to crash without errors. We recommend that you smooth your high resolution (10min) topography to reduce the likelihood of model instabilities. We provide a rudimentary smoothing program for this purpose. The code allows you to set the number of smoothing passes (niter) you make over your initial topography, and produces a latitudinal cross section for comparison.
ncdata: initial state
You can initialize your deep time simulation from a default cesm initial file (e.g., cami_0000-01-01_1.9x2.5_L30_c070703.nc), by setting the the ice initial condition to zero in the ice model namelist (user_nl_cice: ice_ic='none').
Solar constant and trace gases
|co2vmr||CO2 volume mixing ratio|
|ch4vmr||CH4 volume mixing ratio|
|n20vmr||N2O volume mixing ratio|
|f11vmr1||CFC11 volume mixing ratio|
|f12vmr1||CFC12 volume mixing ration|
1 For deep time paleo experiments, F11VMR and F12VMR should be set to 0.