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The SW model still needs the ICMSH (spectral fields) and ICMGG (gridpoint) files to correctly start. In the idealized case, these are read solely to set the model's spectral and gridpoint resolution and the model will overwrite the initial state read from file (see the code in suspecb.F90).
The model will require the vorticity, divergence, ln(Ps) (contains the geopotential of the free surface) and orography.
The Euler advection scheme can only be run on a regular Gaussian grid however (see below for example).
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A test for the shallow-water model at spectral horizontal resolution T255 is available from the OpenIFS ftp site to try.
This example comes with initial files, namelist and job. The namelist is configured to run the semi-Lagrangian advection. |
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The GRIB files from an existing experiment can also be used to create initial files for the shallow-water model. In the following example, the initial files from the T21 test case distributed with the OpenIFS tarfile are used.
Note that the initial fields themselves are not used with the idealized configurations. The initial files are there to correctly set the grid, hence stl1 is used in this example to get the initial gridpoint file.If you have some existing |
If you have access to the MARS archive at ECMWF then an example of how to retrieve single level fields is:
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