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NAME

       r3.gwflow  - Numerical calculation program for transient, confined groundwater flow in three dimensions.

KEYWORDS

       raster3d, groundwater flow, voxel, hydrology

SYNOPSIS

       r3.gwflow
       r3.gwflow --help
       r3.gwflow   [-mf]   phead=name   status=name   hc_x=name  hc_y=name  hc_z=name   [sink=name]   yield=name
       [recharge=name]  output=name  [velocity_x=name]   [velocity_y=name]    [velocity_z=name]    [budget=name]
       dtime=float   [maxit=integer]    [error=float]    [solver=name]    [--overwrite]   [--help]   [--verbose]
       [--quiet]  [--ui]

   Flags:
       -m
           Use 3D raster mask (if exists)

       -f
           Use a full filled quadratic linear equation system, default is a sparse linear equation system.

       --overwrite
           Allow output files to overwrite existing files

       --help
           Print usage summary

       --verbose
           Verbose module output

       --quiet
           Quiet module output

       --ui
           Force launching GUI dialog

   Parameters:
       phead=name [required]
           Input 3D raster map with initial piezometric heads in [m]

       status=name [required]
           Input 3D raster map providing the status for each cell, = 0 - inactive, 1 - active, 2 - dirichlet

       hc_x=name [required]
           Input 3D raster map with the x-part of the hydraulic conductivity tensor in [m/s]

       hc_y=name [required]
           Input 3D raster map with the y-part of the hydraulic conductivity tensor in [m/s]

       hc_z=name [required]
           Input 3D raster map with the z-part of the hydraulic conductivity tensor in [m/s]

       sink=name
           Input 3D raster map with sources and sinks in [m^3/s]

       yield=name [required]
           Specific yield [1/m] input 3D raster map

       recharge=name
           Recharge input 3D raster map in m^3/s

       output=name [required]
           Output 3D raster map storing the piezometric head result of the numerical calculation

       velocity_x=name
           Output 3D raster map storing the groundwater filter velocity vector part in x direction [m/s]

       velocity_y=name
           Output 3D raster map storing the groundwater filter velocity vector part in y direction [m/s]

       velocity_z=name
           Output 3D raster map storing the groundwater filter velocity vector part in z direction [m/s]

       budget=name
           Output 3D raster map storing the groundwater budget for each cell [m^3/s]

       dtime=float [required]
           The calculation time in seconds
           Default: 86400

       maxit=integer
           Maximum number of iteration used to solve the linear equation system
           Default: 10000

       error=float
           Error break criteria for iterative solver
           Default: 0.000001

       solver=name
           The type of solver which should solve the symmetric linear equation system
           Options: cg, pcg, cholesky
           Default: cg

DESCRIPTION

       This numerical module calculates implicit transient and steady state, confined groundwater flow in  three
       dimensions based on volume maps and the current 3D region settings.  All initial- and boundary-conditions
       must be provided as volume maps.  The unit in the location must be meters.

       This module is sensitive to mask settings. All cells which are outside the mask are ignored  and  handled
       as no flow boundaries.

       The  module  calculates  the  piezometric  head  and  optionally  the water balance for each cell and the
       groundwater velocity field in 3 dimensions.  The vector components can be  visualized  with  ParaView  if
       they are exported with r3.out.vtk.

       The  groundwater  flow will always be calculated transient.  For steady state computation the user should
       set the timestep to a large number (billions of seconds) or set the specific yield raster map to zero.

NOTES

       The groundwater flow calculation is  based  on  Darcy’s  law  and  a  numerical  implicit  finite  volume
       discretization. The discretization results in a symmetric and positive definite linear equation system in
       form of Ax = b, which must be solved. The groundwater  flow  partial  differential  equation  is  of  the
       following form:

       (dh/dt)*S = div (K grad h) + q

       In detail for 3 dimensions:

       (dh/dt)*S = Kxx * (d^2h/dx^2) + Kyy * (d^2h/dy^2) + Kzz * (d^2h/dz^2) + q

           •   h -- the piezometric head im meters [m]

           •   dt -- the time step for transient calculation in seconds [s]

           •   S -- the specific yield  [1/m]

           •   b -- the bottom surface of the aquifer meters [m]

           •   Kxx -- the hydraulic conductivity tensor part in x direction in meter per second [m/s]

           •   Kyy -- the hydraulic conductivity tensor part in y direction in meter per seconds [m/s]

           •   Kzz -- the hydraulic conductivity tensor part in z direction in meter per seconds [m/s]

           •   q - inner source/sinc in [1/s]

       Two  different  boundary conditions are implemented, the Dirichlet and Neumann conditions. By default the
       calculation area is surrounded by homogeneous Neumann boundary conditions. The calculation  and  boundary
       status of single cells can be set with the status map, the following cell states are supported:

           •   0  ==  inactive - the cell with status 0 will not be calculated, active cells will have a no flow
               boundary to an inactive cell

           •   1 == active - this cell is used for groundwater calculation, inner sources  can  be  defined  for
               those cells

           •   2  == Dirichlet - cells of this type will have a fixed piezometric head value which do not change
               over time

       Note that all required raster maps are read into main memory. Additionally  the  linear  equation  system
       will  be  allocated,  so  the  memory consumption of this module rapidely grow with the size of the input
       maps.

       The resulting linear equation system Ax = b can be solved with several solvers. An iterative solvers with
       sparse  and  quadratic  matrices  support  is implemented.  The conjugate gradients method with (pcg) and
       without (cg) precondition.  Additionally a direct Cholesky solver is available. This direct  solver  only
       work  with normal quadratic matrices, so be careful using them with large maps (maps of size 10.000 cells
       will need more than one Gigabyte of RAM). The user should always prefer to use a sparse matrix solver.

EXAMPLE 1

       This small script creates a working groundwater flow area and  data.  It  cannot  be  run  in  a  lat/lon
       location.
       # set the region accordingly
       g.region res=25 res3=25 t=100 b=0 n=1000 s=0 w=0 e=1000 -p3
       #now create the input raster maps for a confined aquifer
       r3.mapcalc expression="phead = if(row() == 1 && depth() == 4, 50, 40)"
       r3.mapcalc expression="status = if(row() == 1 && depth() == 4, 2, 1)"
       r3.mapcalc expression="well = if(row() == 20 && col() == 20 && depth() == 2, -0.25, 0)"
       r3.mapcalc expression="hydcond = 0.00025"
       r3.mapcalc expression="syield = 0.0001"
       r.mapcalc  expression="recharge = 0.0"
       r3.gwflow solver=cg phead=phead statuyield=status hc_x=hydcond hc_y=hydcond  \
          hc_z=hydcond sink=well yield=syield r=recharge output=gwresult dt=8640000 vx=vx vy=vy vz=vz budget=budget
       # The data can be visualized with ParaView when exported with r3.out.vtk
       r3.out.vtk -p in=gwresult,status,budget vector=vx,vy,vz out=/tmp/gwdata3d.vtk
       #now load the data into ParaView
       paraview --data=/tmp/gwdata3d.vtk

EXAMPLE 2

       This will create a nice 3D model with geological layer with different hydraulic conductivities. Make sure
       you are not in a lat/lon projection.
       # set the region accordingly
       g.region res=15 res3=15 t=500 b=0 n=1000 s=0 w=0 e=1000
       #now create the input raster maps for a confined aquifer
       r3.mapcalc expression="phead = if(col() == 1 && depth() == 33, 50, 40)"
       r3.mapcalc expression="status = if(col() == 1 && depth() == 33, 2, 1)"
       r3.mapcalc expression="well = if(row() == 20 && col() == 20 && depth() == 3, -0.25, 0)"
       r3.mapcalc expression="well = if(row() == 50 && col() == 50 && depth() == 3, -0.25, well)"
       r3.mapcalc expression="hydcond = 0.0025"
       r3.mapcalc expression="hydcond = if(depth() < 30 && depth() > 23 && col() < 60, 0.000025, hydcond)"
       r3.mapcalc expression="hydcond = if(depth() < 20 && depth() > 13 && col() >  7, 0.000025, hydcond)"
       r3.mapcalc expression="hydcond = if(depth() < 10 && depth() >  7 && col() < 60, 0.000025, hydcond)"
       r3.mapcalc expression="syield = 0.0001"
       r3.gwflow solver=cg phead=phead statuyield=status hc_x=hydcond hc_y=hydcond  \
          hc_z=hydcond sink=well yield=syield output=gwresult dt=8640000 vx=vx vy=vy vz=vz budget=budget
       # The data can be visualized with paraview when exported with r3.out.vtk
       r3.out.vtk -p in=gwresult,status,budget,hydcond,well vector=vx,vy,vz out=/tmp/gwdata3d.vtk
       #now load the data into paraview
       paraview --data=/tmp/gwdata3d.vtk

SEE ALSO

        r.gwflow, r.solute.transport, r3.out.vtk

AUTHOR

       Sören Gebbert

       This work is based on the Diploma Thesis of Sören Gebbert available here at Technical University  Berlin,
       Germany.

SOURCE CODE

       Available at: r3.gwflow source code (history)

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       © 2003-2019 GRASS Development Team, GRASS GIS 7.8.2 Reference Manual