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Compressible and Thermodynamically-consistent Spectral Model
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Brown-Justin-M/CaTSM
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CCCCCC TTTTTTTT SSSSSS MM MM CCC CCC aaaaaa TT SSS SSS MMM MMM CCC aaa TT SSS MMMMMMMM CCC aaaaaaa TT SSS MM MM MM CCC CCC aaa aaa TT SSS SSS MM MM MM CCCCCC aaaaa a TT SSSSSS MM MM MM ================================================ ================================================ Written by: Justin Brown Contact: jmbrown2@nps.edu README CaTSM is a fluid code designed to solve double-diffusive and microscale fluid problems using compressible physics. The equation state permits linear and ideal gas forms. The code uses the pseudo-spectral method and is periodic horizontally. Initial steps are carried out using a Runge--Kutta/Crank--Nicolson method, but the bulk of the code uses the Adams--Bashforth/Backwards Differentiation Formula. ACKNOWLEDGEMENTS CaTSM was constructed using Stephan Stellmach's PADDI code as a template and similarly adopts the time-stepping schemes from Roger Peyret's "Spectral Methods for Incompressible Viscous Flow." DEPENDENCIES CaTSM depends on the FFTW and NetCDF fortran libraries. It is recommended to use the following versions: FFTW: 3.3.9_1 NetCDF: 4.8.0_1 INSTALL To install CaTSM, use the configure command: ./configure make This will compile the CaTSM executable in the main directory of the code. If the dependencies are not in a standard place or if the fortran compiler does not have a standard name, these can be specified through environment variables to configure. For example, ./configure FC=gfortran-11 FCFLAGS="-I/usr/local/include -L/usr/local/lib" Alternatively, the home directories of FFTW and NetCDF can be specified manually with ./configure FFTW_HOME=/path/to/fftw NETCDF_HOME=/path/to/netcdf RUN To run, CaTSM requires a single parameter file named "parameters" and can be executed from the terminal without arguments. If the file is named something other than parameters, the user can instead run CaTSM name_of_parameter_file The parameter file is a fortran namelist file containing three namelists: grid, parameters, and io. Examples can be found in test/rt or test/sfrt for a standard Rayleigh--Taylor problem without and with double-diffusion, respectively. Additional parameters can be found in the grid_type object definition in src/grid_module.F90, the params_type object definition in src/params_module.F90, and the controllers_type object definition in src/IO/output_module.F90 for the three namelists, respectively. OUTPUTS CaTSM outputs four files during a typical simulation. The names of these files can be specified using the io namelist. The number of steps in between outputs can also be specified using the io namelist. Files ending with ".nc" are in the NetCDF format. data.nc: A full 3D time record of the simulation in physical space. restart.nc: A spectral output at a single time to use as a restart profiles.nc: A time record of vertical profiles diag.csv: A CSV file containing global averages of critical quantities like the heat and salt fluxes and the rms values of the velocities/temperature/ salinity perturbations.
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