Changes between Version 37 and Version 38 of doc/tec/nesting

Timestamp:

Nov 2, 2020 2:19:51 PM (4 years ago)

Author:

pavelkrc

Comment:

--

doc/tec/nesting

@@ -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. 
 Boundary data need to be provided for each boundary grid point at the lateral ''xz, yz''-layers as well as at the top boundary.  
-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 (not available for WRF so far).  \\\\
+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]. \\\\
 
 Larger-scale model output data do not encompass any resolved-scale turbulence but turbulence is completely parametrized.