310 lines
10 KiB
C++
310 lines
10 KiB
C++
// MFEM Example 18
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//
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// Compile with: make ex18
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//
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// Sample runs:
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//
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// ex18 -p 1 -r 2 -o 1 -s 3
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// ex18 -p 1 -r 1 -o 3 -s 4
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// ex18 -p 1 -r 0 -o 5 -s 6
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// ex18 -p 2 -r 1 -o 1 -s 3
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// ex18 -p 2 -r 0 -o 3 -s 3
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//
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// Description: This example code solves the compressible Euler system of
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// equations, a model nonlinear hyperbolic PDE, with a
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// discontinuous Galerkin (DG) formulation.
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//
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// Specifically, it solves for an exact solution of the equations
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// whereby a vortex is transported by a uniform flow. Since all
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// boundaries are periodic here, the method's accuracy can be
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// assessed by measuring the difference between the solution and
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// the initial condition at a later time when the vortex returns
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// to its initial location.
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//
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// Note that as the order of the spatial discretization increases,
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// the timestep must become smaller. This example currently uses a
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// simple estimate derived by Cockburn and Shu for the 1D RKDG
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// method. An additional factor can be tuned by passing the --cfl
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// (or -c shorter) flag.
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//
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// The example demonstrates user-defined bilinear and nonlinear
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// form integrators for systems of equations that are defined with
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// block vectors, and how these are used with an operator for
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// explicit time integrators. In this case the system also
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// involves an external approximate Riemann solver for the DG
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// interface flux. It also demonstrates how to use GLVis for
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// in-situ visualization of vector grid functions.
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//
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// We recommend viewing examples 9, 14 and 17 before viewing this
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// example.
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#include "mfem.hpp"
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#include <fstream>
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#include <sstream>
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#include <iostream>
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// Classes FE_Evolution, RiemannSolver, and FaceIntegrator
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// shared between the serial and parallel version of the example.
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#include "ex18.hpp"
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// Choice for the problem setup. See InitialCondition in ex18.hpp.
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int problem;
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// Equation constant parameters.
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const int num_equation = 4;
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const real_t specific_heat_ratio = 1.4;
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const real_t gas_constant = 1.0;
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// Maximum characteristic speed (updated by integrators)
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real_t max_char_speed;
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int main(int argc, char *argv[])
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{
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// 1. Parse command-line options.
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problem = 1;
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const char *mesh_file = "../data/periodic-square.mesh";
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int ref_levels = 1;
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int order = 3;
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int ode_solver_type = 4;
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real_t t_final = 2.0;
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real_t dt = -0.01;
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real_t cfl = 0.3;
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bool visualization = true;
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int vis_steps = 50;
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int precision = 8;
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cout.precision(precision);
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OptionsParser args(argc, argv);
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args.AddOption(&mesh_file, "-m", "--mesh",
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"Mesh file to use.");
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args.AddOption(&problem, "-p", "--problem",
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"Problem setup to use. See options in velocity_function().");
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args.AddOption(&ref_levels, "-r", "--refine",
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"Number of times to refine the mesh uniformly.");
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args.AddOption(&order, "-o", "--order",
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"Order (degree) of the finite elements.");
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args.AddOption(&ode_solver_type, "-s", "--ode-solver",
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"ODE solver: 1 - Forward Euler,\n\t"
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" 2 - RK2 SSP, 3 - RK3 SSP, 4 - RK4, 6 - RK6.");
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args.AddOption(&t_final, "-tf", "--t-final",
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"Final time; start time is 0.");
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args.AddOption(&dt, "-dt", "--time-step",
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"Time step. Positive number skips CFL timestep calculation.");
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args.AddOption(&cfl, "-c", "--cfl-number",
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"CFL number for timestep calculation.");
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args.AddOption(&visualization, "-vis", "--visualization", "-no-vis",
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"--no-visualization",
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"Enable or disable GLVis visualization.");
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args.AddOption(&vis_steps, "-vs", "--visualization-steps",
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"Visualize every n-th timestep.");
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args.Parse();
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if (!args.Good())
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{
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args.PrintUsage(cout);
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return 1;
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}
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args.PrintOptions(cout);
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// 2. Read the mesh from the given mesh file. This example requires a 2D
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// periodic mesh, such as ../data/periodic-square.mesh.
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Mesh mesh(mesh_file, 1, 1);
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const int dim = mesh.Dimension();
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MFEM_ASSERT(dim == 2, "Need a two-dimensional mesh for the problem definition");
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// 3. Define the ODE solver used for time integration. Several explicit
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// Runge-Kutta methods are available.
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ODESolver *ode_solver = NULL;
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switch (ode_solver_type)
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{
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case 1: ode_solver = new ForwardEulerSolver; break;
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case 2: ode_solver = new RK2Solver(1.0); break;
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case 3: ode_solver = new RK3SSPSolver; break;
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case 4: ode_solver = new RK4Solver; break;
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case 6: ode_solver = new RK6Solver; break;
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default:
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cout << "Unknown ODE solver type: " << ode_solver_type << '\n';
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return 3;
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}
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// 4. Refine the mesh to increase the resolution. In this example we do
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// 'ref_levels' of uniform refinement, where 'ref_levels' is a
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// command-line parameter.
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for (int lev = 0; lev < ref_levels; lev++)
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{
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mesh.UniformRefinement();
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}
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// 5. Define the discontinuous DG finite element space of the given
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// polynomial order on the refined mesh.
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DG_FECollection fec(order, dim);
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// Finite element space for a scalar (thermodynamic quantity)
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FiniteElementSpace fes(&mesh, &fec);
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// Finite element space for a mesh-dim vector quantity (momentum)
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FiniteElementSpace dfes(&mesh, &fec, dim, Ordering::byNODES);
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// Finite element space for all variables together (total thermodynamic state)
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FiniteElementSpace vfes(&mesh, &fec, num_equation, Ordering::byNODES);
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// This example depends on this ordering of the space.
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MFEM_ASSERT(fes.GetOrdering() == Ordering::byNODES, "");
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cout << "Number of unknowns: " << vfes.GetVSize() << endl;
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// 6. Define the initial conditions, save the corresponding mesh and grid
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// functions to a file. This can be opened with GLVis with the -gc option.
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// The solution u has components {density, x-momentum, y-momentum, energy}.
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// These are stored contiguously in the BlockVector u_block.
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Array<int> offsets(num_equation + 1);
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for (int k = 0; k <= num_equation; k++) { offsets[k] = k * vfes.GetNDofs(); }
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BlockVector u_block(offsets);
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// Momentum grid function on dfes for visualization.
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GridFunction mom(&dfes, u_block.GetData() + offsets[1]);
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// Initialize the state.
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VectorFunctionCoefficient u0(num_equation, InitialCondition);
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GridFunction sol(&vfes, u_block.GetData());
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sol.ProjectCoefficient(u0);
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// Output the initial solution.
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{
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ofstream mesh_ofs("vortex.mesh");
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mesh_ofs.precision(precision);
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mesh_ofs << mesh;
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for (int k = 0; k < num_equation; k++)
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{
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GridFunction uk(&fes, u_block.GetBlock(k));
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ostringstream sol_name;
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sol_name << "vortex-" << k << "-init.gf";
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ofstream sol_ofs(sol_name.str().c_str());
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sol_ofs.precision(precision);
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sol_ofs << uk;
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}
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}
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// 7. Set up the nonlinear form corresponding to the DG discretization of the
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// flux divergence, and assemble the corresponding mass matrix.
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MixedBilinearForm Aflux(&dfes, &fes);
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Aflux.AddDomainIntegrator(new TransposeIntegrator(new GradientIntegrator()));
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Aflux.Assemble();
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NonlinearForm A(&vfes);
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RiemannSolver rsolver;
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A.AddInteriorFaceIntegrator(new FaceIntegrator(rsolver, dim));
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// 8. Define the time-dependent evolution operator describing the ODE
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// right-hand side, and perform time-integration (looping over the time
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// iterations, ti, with a time-step dt).
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FE_Evolution euler(vfes, A, Aflux.SpMat());
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// Visualize the density
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socketstream sout;
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if (visualization)
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{
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char vishost[] = "localhost";
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int visport = 19916;
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sout.open(vishost, visport);
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if (!sout)
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{
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cout << "Unable to connect to GLVis server at "
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<< vishost << ':' << visport << endl;
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visualization = false;
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cout << "GLVis visualization disabled.\n";
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}
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else
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{
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sout.precision(precision);
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sout << "solution\n" << mesh << mom;
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sout << "pause\n";
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sout << flush;
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cout << "GLVis visualization paused."
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<< " Press space (in the GLVis window) to resume it.\n";
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}
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}
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// Determine the minimum element size.
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real_t hmin = 0.0;
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if (cfl > 0)
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{
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hmin = mesh.GetElementSize(0, 1);
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for (int i = 1; i < mesh.GetNE(); i++)
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{
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hmin = min(mesh.GetElementSize(i, 1), hmin);
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}
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}
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// Start the timer.
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tic_toc.Clear();
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tic_toc.Start();
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real_t t = 0.0;
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euler.SetTime(t);
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ode_solver->Init(euler);
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if (cfl > 0)
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{
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// Find a safe dt, using a temporary vector. Calling Mult() computes the
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// maximum char speed at all quadrature points on all faces.
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Vector z(A.Width());
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max_char_speed = 0.;
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A.Mult(sol, z);
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dt = cfl * hmin / max_char_speed / (2*order+1);
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}
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// Integrate in time.
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bool done = false;
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for (int ti = 0; !done; )
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{
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real_t dt_real = min(dt, t_final - t);
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ode_solver->Step(sol, t, dt_real);
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if (cfl > 0)
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{
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dt = cfl * hmin / max_char_speed / (2*order+1);
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}
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ti++;
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done = (t >= t_final - 1e-8*dt);
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if (done || ti % vis_steps == 0)
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{
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cout << "time step: " << ti << ", time: " << t << endl;
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if (visualization)
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{
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sout << "solution\n" << mesh << mom << flush;
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}
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}
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}
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tic_toc.Stop();
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cout << " done, " << tic_toc.RealTime() << "s." << endl;
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// 9. Save the final solution. This output can be viewed later using GLVis:
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// "glvis -m vortex.mesh -g vortex-1-final.gf".
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for (int k = 0; k < num_equation; k++)
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{
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GridFunction uk(&fes, u_block.GetBlock(k));
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ostringstream sol_name;
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sol_name << "vortex-" << k << "-final.gf";
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ofstream sol_ofs(sol_name.str().c_str());
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sol_ofs.precision(precision);
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sol_ofs << uk;
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}
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// 10. Compute the L2 solution error summed for all components.
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if (t_final == 2.0)
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{
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const real_t error = sol.ComputeLpError(2, u0);
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cout << "Solution error: " << error << endl;
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}
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// Free the used memory.
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delete ode_solver;
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return 0;
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}
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