Changes between Version 38 and Version 39 of doc/tec/nesting
- Timestamp:
- Nov 2, 2020 2:22:13 PM (4 years ago)
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doc/tec/nesting
v38 v39 41 41 The PALM model can be nested into any larger-scale model of your choice (COSMO, WRF, etc.), subject to the condition that the data in the dynamic input file is readable, i.e. with horizontal and vertical dimensions as expected by PALM. 42 42 Boundary data need to be provided for each boundary grid point at the lateral ''xz, yz''-layers as well as at the top boundary. 43 To date, the pre-processing tool [wiki:doc/app/iofiles/inifor INIFOR] is available which can convert output data from the COSMO model into PALM-readable boundary data. A [wiki:doc/app/iofiles/wrf_interface set of scripts] is available for generating the dynamic input file from the output of a WRF simulation, which also supports optional CAMx output files for preparing the initial and boundary conditions for the [wiki:doc/tec/chem chemistry model]. \\\\43 To date, the pre-processing tool [wiki:doc/app/iofiles/inifor INIFOR] is available which can convert output data from the COSMO model into PALM-readable boundary data. A [wiki:doc/app/iofiles/wrf_interface WRF interface] is available for generating the dynamic input file from the output of a WRF simulation, which also supports optional CAMx output files for preparing the initial and boundary conditions for the [wiki:doc/tec/chem chemistry model]. \\\\ 44 44 45 45 Larger-scale model output data do not encompass any resolved-scale turbulence but turbulence is completely parametrized.
