The material

The source tarball swan4151.tar.gz contains the SWAN source code and consists of the following files:

main program	: swanmain.ftn
pre-processing routines	: swanpre1.ftn
	$\,\,$ swanpre2.ftn
	$\,\,$ SwanBndStruc.ftn90
computational routines	: swancom1.ftn
	$\,\,$ swancom2.ftn
	$\,\,$ swancom3.ftn
	$\,\,$ swancom4.ftn
	$\,\,$ swancom5.ftn
post-processing routines	: swanout1.ftn
	$\,\,$ swanout2.ftn
	$\,\,$ SwanVTKWriteHeader.ftn90
	$\,\,$ SwanVTKWriteData.ftn90
	$\,\,$ SwanVTKPDataSets.ftn90
service routines	: swanser.ftn
	$\,\,$ SwanIntgratSpc.ftn90
routines for Bragg	$\,\,$
scattering	: SwanBraggScat.ftn90
routines for QCM	: SwanQCM.ftn90
routines for ST6 package	: SdsBabanin.ftn90
routines for support
parallel MPI runs	: swanparll.ftn
routines for unstructured	$\,\,$
grids	: SwanReadGrid.ftn90
	$\,\,$ SwanReadADCGrid.ftn90
	$\,\,$ SwanReadTriangleGrid.ftn90
	$\,\,$ SwanReadEasymeshGrid.ftn90
	$\,\,$ SwanInitCompGrid.ftn90
	$\,\,$ SwanCheckGrid.ftn90
	$\,\,$ SwanCreateEdges.ftn90
	$\,\,$ SwanGridTopology.ftn90
	$\,\,$ SwanGridVert.ftn90
	$\,\,$ SwanGridCell.ftn90
	$\,\,$ SwanGridFace.ftn90
	$\,\,$ SwanPrintGridInfo.ftn90
	$\,\,$ SwanFindPoint.ftn90
	$\,\,$ SwanPointinMesh.ftn90
	$\,\,$ SwanBpntlist.ftn90
	$\,\,$ SwanPrepComp.ftn90
	$\,\,$ SwanVertlist.ftn90
	$\,\,$ SwanCompUnstruc.ftn90
	$\,\,$ SwanDispParm.ftn90
	$\,\,$ SwanPropvelX.ftn90
	$\,\,$ SwanSweepSel.ftn90
	$\,\,$ SwanPropvelS.ftn90
	$\,\,$ SwanTranspAc.ftn90
	$\,\,$ SwanTranspX.ftn90
	$\,\,$ SwanGradDepthorK.ftn90
	$\,\,$ SwanGradVel.ftn90
	$\,\,$ SwanDiffPar.ftn90
	$\,\,$ SwanGSECorr.ftn90
	$\,\,$ SwanInterpolatePoint.ftn90
	$\,\,$ SwanInterpolateAc.ftn90
	$\,\,$ SwanInterpolateOutput.ftn90
	$\,\,$ SwanConvAccur.ftn90
	$\,\,$ SwanConvStopc.ftn90
	$\,\,$ SwanThreadBounds.ftn90
	$\,\,$ SwanFindObstacles.ftn90
	$\,\,$ SwanCrossObstacle.ftn90
	$\,\,$ SwanComputeForce.ftn90
routines for parallel,	$\,\,$
unstructured grids	: SwanParallel.ftn90
modules and subroutines	$\,\,$
for netCDF	: nctablemd.ftn90
	$\,\,$ agioncmd.ftn90
	$\,\,$ swn_outnc.ftn90
couplers	: couple2adcirc.ftn90
	$\,\,$ swan2coh.ftn90
routines for installation	: ocpids.ftn
command reading routines	: ocpcre.ftn
miscellaneous routines	: ocpmix.ftn
general modules	: swmod1.ftn
	$\,\,$ swmod2.ftn
modules for XNL	: m_constants.ftn90
	$\,\,$ m_fileio.ftn90
	$\,\,$ serv_xnl4v5.ftn90
	$\,\,$ mod_xnl4v5.ftn90
modules for unstructured	$\,\,$
grids	: SwanGriddata.ftn90
	$\,\,$ SwanGridobjects.ftn90
	$\,\,$ SwanCompdata.ftn90
modules for spectral	$\,\,$
partitioning	: SwanSpectPart.ftn
routines for the fast
Fourier transform	: fftpack51.ftn90

The SWAN source code is written in Fortran 90. Some routines are written in fixed form and depending on your system, the extension may be for or f. Other routines are written in free form and are indicated by extension f90. The conversion from ftn or ftn90 to one of these extensions can be done automatically or manually; see Chapter 3.


You are allow to make changes in the source code of SWAN, but Delft University of Technology will not support modified versions of SWAN. If you want your modifications to be implemented in the authorized version of SWAN (the version on the SWAN homepage), you need to submit these changes to the SWAN team (e-mail: m.zijlema@tudelft.nl).


As a part of the package, fftpack51 is the Fast Fourier Transform library translated to Fortran 90 by John Burkardt of Florida State University.


The SWAN source code is additionally accompanied by the following files:

installation procedures	: INSTALL.README
	$\,\,$ Makefile
	$\,\,$ macros.inc
	$\,\,$ which.cmd
	$\,\,$ platform.pl
	$\,\,$ switch.pl
run procedures	: SWANRUN.README
	$\,\,$ swanrun
	$\,\,$ swanrun.bat
machinefile for parallel	$\,\,$
MPI runs	: machinefile
for concatenation of	$\,\,$
multiple hotfiles	: swanhcat.ftn
	$\,\,$ hcat.nml
edit file	: swan.edt
Matlab scripts for	$\,\,$
unstructured grids	: plotunswan.m
	$\,\,$ plotgrid.m

On the SWAN homepage, you also find some test cases with some output files for making a configuration test of SWAN on your computer. You may compare your results with those in the provided output files. See Chapter 6 for further details.