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Fortran version of the Constrained Spectral Approximation Method

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This repository is an incomplete Fortran version of the Python Constrained Spectral Approximation Method.

The Fortran implementation was meant to be the orographic gravity-wave source for the Multi-scale Gravity-wave Model that is coupled to the German Weather Service's Icosahedral Nonhydrostatic (ICON) model. This codebase builds, runs, and outputs the spectral approximation of topographic data distributed in a geodesic grid cell. However, not all of the latest algorithmic and scientific features have been implemented in the Fortran code.

  • A simple plotter for the output data can be found in notebooks/plotter.ipynb.
  • Namelist files are in scripts.

Note that this codebase uses features from the Fortran 2008 standard.

Requirements

Refer to CMakeLists.txt for more details.

Build

cd trifourtopo
mkdir build
cd build
cmake ..
make

The make command will create two binaries in build/bin:

  • linker
  • four_topo

Run

This codebase uses the USGS GMTED 2010 topographic dataset and an ICON grid.

Before executing four_topo for the spectral analysis, you must link the topographic dataset to the corresponding grid by setting the path in linker.nml and executing build/bin/linker. The program extends the NetCDF grid data with a lookup table to the corresponding data slice in the topographic dataset.

The binary four_topo outputs a NetCDF4 file comprising the computed spectral approximation over all the cells provided in the grid file. The output may be visualised with notebooks/plotter.ipynb.

The notebook nc_compactifie.ipynb creates a regional grid and topographic dataset and may help with debugging and testing.

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Fortran version of the Constrained Spectral Approximation Method

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  • Fortran 96.6%
  • CMake 3.4%