Error control: Computing convergence rates#

Author: Jørgen S. Dokken, Hans Petter Langtangen, Anders Logg

For any numerical method one of the most central questions is its convergence rate: How fast does the error go to zero when the resolution is increased (mesh size decreased).

For the finite element method, this usually corresponds to proving, theoretically or imperically, that the error \(e=u_e-u_h\) is bounded by the mesh size \(h\) to some power \(r\), that is \(\vert\vert e \vert\vert\leq Ch^r\) for some mesh independent constant \(C\). The number \(r\) is called the convergence rate of the method. Note that the different norms like the \(L^2\)-norm \(\vert\vert e\vert\vert\) or the \(H_0^1\)-norm have different convergence rates.

Computing error norms#

We start by creating a manufactured problem, using the same problem as in the solver configuration.

from dolfinx import default_scalar_type
from dolfinx.fem import (Expression, Function, FunctionSpace,
                         assemble_scalar, dirichletbc, form, locate_dofs_topological)
from dolfinx.fem.petsc import LinearProblem
from dolfinx.mesh import create_unit_square, locate_entities_boundary

from mpi4py import MPI
from ufl import SpatialCoordinate, TestFunction, TrialFunction, div, dot, dx, grad, inner

import ufl
import numpy as np


def u_ex(mod):
    return lambda x: mod.cos(2 * mod.pi * x[0]) * mod.cos(2 * mod.pi * x[1])


u_numpy = u_ex(np)
u_ufl = u_ex(ufl)


def solve_poisson(N=10, degree=1):

    mesh = create_unit_square(MPI.COMM_WORLD, N, N)
    x = SpatialCoordinate(mesh)
    f = -div(grad(u_ufl(x)))
    V = FunctionSpace(mesh, ("Lagrange", degree))
    u = TrialFunction(V)
    v = TestFunction(V)
    a = inner(grad(u), grad(v)) * dx
    L = f * v * dx
    u_bc = Function(V)
    u_bc.interpolate(u_numpy)
    facets = locate_entities_boundary(mesh, mesh.topology.dim - 1, lambda x: np.full(x.shape[1], True))
    dofs = locate_dofs_topological(V, mesh.topology.dim - 1, facets)
    bcs = [dirichletbc(u_bc, dofs)]
    default_problem = LinearProblem(a, L, bcs=bcs, petsc_options={"ksp_type": "preonly", "pc_type": "lu"})
    return default_problem.solve(), u_ufl(x)

Now, we can compute the error between the analyical solution u_ex=u_ufl(x) and approximated solution uh. A natural choice might seem to compute (u_ex-uh)**2*ufl.dx.

uh, u_ex = solve_poisson(10)
comm = uh.function_space.mesh.comm
error = form((uh - u_ex)**2 * ufl.dx)
E = np.sqrt(comm.allreduce(assemble_scalar(error), MPI.SUM))
if comm.rank == 0:
    print(f"L2-error: {E:.2e}")
L2-error: 5.28e-02

Sometimes it is of interest to compute the error fo the gradient field, \(\vert\vert \nabla(u_e-u_h)\vert\vert\), often referred to as the \(H_0^1\)-nrom of the error, this can be expressed as

eh = uh - u_ex
error_H10 = form(dot(grad(eh), grad(eh)) * dx)
E_H10 = np.sqrt(comm.allreduce(assemble_scalar(error_H10), op=MPI.SUM))
if comm.rank == 0:
    print(f"H01-error: {E_H10:.2e}")
H01-error: 1.36e+00

Reliable error norm computation#

However, as this gets expanded to u_ex**2 + uh**2 - 2*u_ex*uh. If the error is small, (and the solution itself is of moderate size), this calculation will correspond to subtract two positive numbers u_ex**2 + uh**2\(\sim 1\) and 2*u_ex*u\(\sim 1\) yielding a small number, prone to round-off errors.

To avoid this issue, we interpolate the approximate and exact solution into a higher order function space. Then we subtract the degrees of freedom from the interpolated functions to create a new error function. Then, finally, we assemble/integrate the square difference and take the square root to get the L2 norm.

def error_L2(uh, u_ex, degree_raise=3):
    # Create higher order function space
    degree = uh.function_space.ufl_element().degree()
    family = uh.function_space.ufl_element().family()
    mesh = uh.function_space.mesh
    W = FunctionSpace(mesh, (family, degree + degree_raise))
    # Interpolate approximate solution
    u_W = Function(W)
    u_W.interpolate(uh)

    # Interpolate exact solution, special handling if exact solution
    # is a ufl expression or a python lambda function
    u_ex_W = Function(W)
    if isinstance(u_ex, ufl.core.expr.Expr):
        u_expr = Expression(u_ex, W.element.interpolation_points)
        u_ex_W.interpolate(u_expr)
    else:
        u_ex_W.interpolate(u_ex)

    # Compute the error in the higher order function space
    e_W = Function(W)
    e_W.x.array[:] = u_W.x.array - u_ex_W.x.array

    # Integrate the error
    error = form(ufl.inner(e_W, e_W) * ufl.dx)
    error_local = assemble_scalar(error)
    error_global = mesh.comm.allreduce(error_local, op=MPI.SUM)
    return np.sqrt(error_global)

Computing convergence rates#

Let us consider a sequence of mesh resolutions \(h_0>h_1>h_2\), where \(h_i=\frac{1}{N_i}\) we compute the errors for a range of \(N_i\)s

Ns = [4, 8, 16, 32, 64]
Es = np.zeros(len(Ns), dtype=default_scalar_type)
hs = np.zeros(len(Ns), dtype=np.float64)
for i, N in enumerate(Ns):
    uh, u_ex = solve_poisson(N, degree=1)
    comm = uh.function_space.mesh.comm
    # One can send in either u_numpy or u_ex
    # For L2 error estimations it is reccommended to send in u_numpy
    # as no JIT compilation is required
    Es[i] = error_L2(uh, u_numpy)
    hs[i] = 1. / Ns[i]
    if comm.rank == 0:
        print(f"h: {hs[i]:.2e} Error: {Es[i]:.2e}")
h: 2.50e-01 Error: 2.43e-01
h: 1.25e-01 Error: 7.96e-02
h: 6.25e-02 Error: 2.15e-02
h: 3.12e-02 Error: 5.47e-03
h: 1.56e-02 Error: 1.37e-03

If we assume that \(E_i\) is of the form \(E_i=Ch_i^r\), with unknown constants \(C\) and \(r\), we can compare two consecqutive experiments, \(E_{i-1}= Ch_{i-1}^r\) and \(E_i=Ch_i^r\), and solve for \(r\):

\[r=\frac{\ln(E_i/E_{i-1})}{\ln(h_i/h_{i-1})}\]

The \(r\) values should approac the expected convergence rate (which is typically the polynomial degree + 1 for the \(L^2\)-error.) as \(i\) increases. This can be written compactly using numpy.

rates = np.log(Es[1:] / Es[:-1]) / np.log(hs[1:] / hs[:-1])
if comm.rank == 0:
    print(f"Rates: {rates}")
Rates: [1.61228695 1.89147568 1.97191247 1.99290382]

We also do a similar study for different orders of polynomial spaces to verify our previous claim.

degrees = [1, 2, 3, 4]
for degree in degrees:
    Es = np.zeros(len(Ns), dtype=default_scalar_type)
    hs = np.zeros(len(Ns), dtype=np.float64)
    for i, N in enumerate(Ns):
        uh, u_ex = solve_poisson(N, degree=degree)
        comm = uh.function_space.mesh.comm
        Es[i] = error_L2(uh, u_numpy, degree_raise=3)
        hs[i] = 1. / Ns[i]
        if comm.rank == 0:
            print(f"h: {hs[i]:.2e} Error: {Es[i]:.2e}")
    rates = np.log(Es[1:] / Es[:-1]) / np.log(hs[1:] / hs[:-1])
    if comm.rank == 0:
        print(f"Polynomial degree {degree:d}, Rates {rates}")
h: 2.50e-01 Error: 2.43e-01
h: 1.25e-01 Error: 7.96e-02
h: 6.25e-02 Error: 2.15e-02
h: 3.12e-02 Error: 5.47e-03
h: 1.56e-02 Error: 1.37e-03
Polynomial degree 1, Rates [1.61228695 1.89147568 1.97191247 1.99290382]
h: 2.50e-01 Error: 3.52e-02
h: 1.25e-01 Error: 4.39e-03
h: 6.25e-02 Error: 5.50e-04
h: 3.12e-02 Error: 6.88e-05
h: 1.56e-02 Error: 8.60e-06
Polynomial degree 2, Rates [3.00109101 2.99828073 2.99822291 2.99930786]
h: 2.50e-01 Error: 5.54e-03
h: 1.25e-01 Error: 3.35e-04
h: 6.25e-02 Error: 1.99e-05
h: 3.12e-02 Error: 1.21e-06
h: 1.56e-02 Error: 7.49e-08
Polynomial degree 3, Rates [4.04795047 4.07357659 4.03728992 4.01645269]
h: 2.50e-01 Error: 7.20e-04
h: 1.25e-01 Error: 2.42e-05
h: 6.25e-02 Error: 7.75e-07
h: 3.12e-02 Error: 2.44e-08
h: 1.56e-02 Error: 7.64e-10
Polynomial degree 4, Rates [4.896908   4.96084158 4.98926012 4.99766465]

Infinity norm estimates#

We start by creating a function to compute the infinity norm, the max difference between the approximate and exact solution.

def error_infinity(u_h, u_ex):
    # Interpolate exact solution, special handling if exact solution
    # is a ufl expression or a python lambda function
    comm = u_h.function_space.mesh.comm
    u_ex_V = Function(u_h.function_space)
    if isinstance(u_ex, ufl.core.expr.Expr):
        u_expr = Expression(u_ex, u_h.function_space.element.interpolation_points)
        u_ex_V.interpolate(u_expr)
    else:
        u_ex_V.interpolate(u_ex)
    # Compute infinity norm, furst local to process, then gather the max
    # value over all processes
    error_max_local = np.max(np.abs(u_h.x.array - u_ex_V.x.array))
    error_max = comm.allreduce(error_max_local, op=MPI.MAX)
    return error_max

Running this for various polynomial degrees yields:

for degree in degrees:
    Es = np.zeros(len(Ns), dtype=default_scalar_type)
    hs = np.zeros(len(Ns), dtype=np.float64)
    for i, N in enumerate(Ns):
        uh, u_ex = solve_poisson(N, degree=degree)
        comm = uh.function_space.mesh.comm
        Es[i] = error_infinity(uh, u_numpy)
        hs[i] = 1. / Ns[i]
        if comm.rank == 0:
            print(f"h: {hs[i]:.2e} Error: {Es[i]:.2e}")
    rates = np.log(Es[1:] / Es[:-1]) / np.log(hs[1:] / hs[:-1])
    if comm.rank == 0:
        print(f"Polynomial degree {degree:d}, Rates {rates}")
h: 2.50e-01 Error: 2.73e-01
h: 1.25e-01 Error: 6.96e-02
h: 6.25e-02 Error: 1.75e-02
h: 3.12e-02 Error: 4.38e-03
h: 1.56e-02 Error: 1.10e-03
Polynomial degree 1, Rates [1.96828918 1.9917697  1.99791282 1.99947611]
h: 2.50e-01 Error: 4.85e-02
h: 1.25e-01 Error: 3.65e-03
h: 6.25e-02 Error: 2.37e-04
h: 3.12e-02 Error: 1.50e-05
h: 1.56e-02 Error: 9.38e-07
Polynomial degree 2, Rates [3.73213705 3.94227924 3.98612529 3.99656548]
h: 2.50e-01 Error: 1.08e-02
h: 1.25e-01 Error: 8.13e-04
h: 6.25e-02 Error: 5.86e-05
h: 3.12e-02 Error: 3.80e-06
h: 1.56e-02 Error: 2.41e-07
Polynomial degree 3, Rates [3.72903577 3.79406598 3.94800701 3.97888411]
h: 2.50e-01 Error: 1.63e-03
h: 1.25e-01 Error: 5.23e-05
h: 6.25e-02 Error: 1.67e-06
h: 3.12e-02 Error: 5.25e-08
h: 1.56e-02 Error: 1.64e-09
Polynomial degree 4, Rates [4.96133103 4.96807694 4.99161596 4.99787779]

We observe super convergence for second order polynomials, yielding a fourth order convergence.