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https://github.com/OPM/opm-simulators.git
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ad0f414c5a
Revision 13e1ab7e1093 introduced well solution vectors (accessed only when wells are present). Update the method call accordingly to restore build.
172 lines
5.5 KiB
C++
172 lines
5.5 KiB
C++
/*
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Copyright 2012 SINTEF ICT, Applied Mathematics.
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This file is part of the Open Porous Media project (OPM).
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OPM is free software: you can redistribute it and/or modify
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it under the terms of the GNU General Public License as published by
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the Free Software Foundation, either version 3 of the License, or
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(at your option) any later version.
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OPM is distributed in the hope that it will be useful,
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but WITHOUT ANY WARRANTY; without even the implied warranty of
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MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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GNU General Public License for more details.
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You should have received a copy of the GNU General Public License
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along with OPM. If not, see <http://www.gnu.org/licenses/>.
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*/
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/// \page tutorial2 Flow Solver for a single phase
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/// \details The flow equations consist of the mass conservation equation
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/// \f[\nabla\cdot u=q\f] and the Darcy law \f[u=-\frac{1}{\mu}K\nabla p.\f] Here,
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/// \f$u\f$ denotes the velocity and \f$p\f$ the pressure. The permeability tensor is
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/// given by \f$K\f$ and \f$\mu\f$ denotes the viscosity.
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///
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/// We solve the flow equations for a carthesian grid and we set the source term
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/// \f$q\f$ be zero except at the left-lower and right-upper corner, where it is equal
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/// with opposite sign (inflow equal to outflow).
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#if HAVE_CONFIG_H
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#include "config.h"
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#endif // HAVE_CONFIG_H
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#include <opm/core/grid.h>
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#include <opm/core/GridManager.hpp>
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#include <opm/core/utility/writeVtkData.hpp>
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#include <cassert>
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#include <cstddef>
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#include <iostream>
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#include <iomanip>
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#include <fstream>
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#include <vector>
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#include <opm/core/linalg/LinearSolverUmfpack.hpp>
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#include <opm/core/pressure/IncompTpfa.hpp>
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#include <opm/core/pressure/FlowBCManager.hpp>
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#include <opm/core/utility/miscUtilities.hpp>
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/// \page tutorial2
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/// \section commentedcode Commented code:
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/// \code
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int main()
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{
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/// \endcode
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/// \page tutorial2
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/// We construct a carthesian grid
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/// \code
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int dim = 3;
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int nx = 40;
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int ny = 40;
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int nz = 1;
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Opm::GridManager grid(nx, ny, nz);
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/// \endcode
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/// \page tutorial2
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/// \details We access the unstructured grid through
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/// the pointer given by \c grid.c_grid(). For more details on unstructured
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/// grid, see grid.h.
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/// \code
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int num_cells = grid.c_grid()->number_of_cells;
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int num_faces = grid.c_grid()->number_of_faces;
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/// \endcode
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/// \page tutorial2
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/// We define the viscosity (unit: cP).
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/// \code
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double mu = 1.0;
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/// \endcode
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/// \page tutorial2
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/// We define the permeability (unit: mD).
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/// \code
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double k = 100.0;
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/// \endcode
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/// \page tutorial2
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/// \details
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/// We set up the permeability tensor and compute the mobility for each cell.
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/// The permeability tensor is flattened in a vector.
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/// \code
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std::vector<double> permeability(num_cells*dim*dim, 0.);
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std::vector<double> mob(num_cells);
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for (int cell = 0; cell < num_cells; ++cell) {
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permeability[9*cell + 0] = k;
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permeability[9*cell + 4] = k;
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permeability[9*cell + 8] = k;
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mob[cell] = 1/mu;
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}
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/// \endcode
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/// \page tutorial2
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/// We choose the UMFPACK linear solver for the pressure solver.
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/// \code
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Opm::LinearSolverUmfpack linsolver;
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/// \endcode
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/// \page tutorial2
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/// We set up the pressure solver
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/// The third argument which corresponds to gravity is set to
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/// zero (no gravity).
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/// \code
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Opm::IncompTpfa psolver(*grid.c_grid(), &permeability[0], 0, linsolver);
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/// \endcode
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/// \page tutorial2
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/// We define the source term.
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/// \code
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std::vector<double> src(num_cells, 0.0);
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src[0] = 100.;
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src[num_cells-1] = -100.;
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/// \endcode
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/// \page tutorial2
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/// \details We set up the boundary conditions. We do not modify them.
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/// By default, we obtain no outflow boundary conditions.
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/// \code
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/// \code
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Opm::FlowBCManager bcs;
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/// \endcode
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/// \page tutorial2
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/// We declare the solution vectors, i.e., the pressure and face
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/// flux vectors we are going to compute. The well solution
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/// vectors are needed for interface compatibility with the
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/// <CODE>solve()</CODE> method of class
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/// <CODE>Opm::IncompTPFA</CODE>.
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/// \code
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std::vector<double> pressure(num_cells);
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std::vector<double> faceflux(num_faces);
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std::vector<double> well_bhp;
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std::vector<double> well_flux;
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/// \endcode
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/// \page tutorial2
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/// \details
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/// We declare the gravity term which is required by the pressure solver (see
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/// Opm::IncompTpfa.solve()). In the absence of gravity, an empty vector is required.
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/// \code
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std::vector<double> omega;
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/// \endcode
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/// \page tutorial2
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/// We call the pressure solver.
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/// \code
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psolver.solve(mob, omega, src, bcs.c_bcs(),
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pressure, faceflux, well_bhp, well_flux);
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/// \endcode
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/// \page tutorial2
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/// We write the results in a file in VTK format.
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/// \code
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std::ofstream vtkfile("tutorial2.vtu");
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Opm::DataMap dm;
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dm["pressure"] = &pressure;
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std::vector<double> cell_velocity;
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Opm::estimateCellVelocity(*grid.c_grid(), faceflux, cell_velocity);
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dm["velocity"] = &cell_velocity;
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Opm::writeVtkData(*grid.c_grid(), dm, vtkfile);
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}
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/// \endcode
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/// \page tutorial2
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/// We read the the vtu output file in \a Paraview and obtain the following pressure
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/// distribution. \image html tutorial2.png
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/// \page tutorial2
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/// \section sourcecode Complete source code.
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/// \include tutorial2.cpp
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