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This is the MATLAB® PDE solver.
PDE Initial-Boundary Value Problem Solver | Description |
|---|---|
Solve initial-boundary value problems for systems of parabolic and elliptic PDEs in one space variable and time. |
PDE Helper Function | Description |
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Evaluate the numerical solution of a PDE using the output of pdepe. |
pdepe solves systems of parabolic and elliptic PDEs in one spatial variable x and time t, of the form
|
| (6-2) |
The PDEs hold for t0 ≤ t ≤ tf and a ≤ x ≤ b. The interval [a, b] must be finite. m can be 0, 1, or 2, corresponding to slab, cylindrical, or spherical symmetry, respectively. If m > 0, then a ≥ 0 must also hold.
In Equation 6-2,
is a
flux term and
is
a source term. The flux term must depend on
. The coupling of the partial derivatives with respect to time is
restricted to multiplication by a diagonal matrix
. The diagonal elements of this matrix
are either identically zero or positive. An element that is identically
zero corresponds to an elliptic equation and otherwise to a parabolic
equation. There must be at least one parabolic equation. An element
of c that corresponds to a parabolic equation can
vanish at isolated values of x if they are mesh
points. Discontinuities in c and/or s due to material interfaces are permitted provided that a mesh point
is placed at each interface.
At the initial time t = t0, for all x the solution components satisfy initial conditions of the form
|
| (6-3) |
At the boundary x = a or x = b, for all t the solution components satisfy a boundary condition of the form
|
| (6-4) |
q(x, t) is a diagonal matrix with elements that are either identically
zero or never zero. Note that the boundary conditions are expressed
in terms of the f rather than partial derivative
of u with respect to x
. Also, of the two coefficients, only p can depend
on u.
The MATLAB PDE solver, pdepe, solves initial-boundary value problems for systems of parabolic and elliptic PDEs in the one space variable x and time t. There must be at least one parabolic equation in the system.
The pdepe solver converts the PDEs to ODEs using a second-order accurate spatial discretization based on a fixed set of user-specified nodes. The discretization method is described in [9]. The time integration is done with ode15s. The pdepe solver exploits the capabilities of ode15s for solving the differential-algebraic equations that arise when Equation 6-2 contains elliptic equations, and for handling Jacobians with a specified sparsity pattern. ode15s changes both the time step and the formula dynamically.
After discretization, elliptic equations give rise to algebraic equations. If the elements of the initial conditions vector that correspond to elliptic equations are not "consistent" with the discretization, pdepe tries to adjust them before beginning the time integration. For this reason, the solution returned for the initial time may have a discretization error comparable to that at any other time. If the mesh is sufficiently fine, pdepe can find consistent initial conditions close to the given ones. If pdepe displays a message that it has difficulty finding consistent initial conditions, try refining the mesh. No adjustment is necessary for elements of the initial conditions vector that correspond to parabolic equations.
The basic syntax of the solver is:
sol = pdepe(m,pdefun,icfun,bcfun,xmesh,tspan)
Note Correspondences given are to terms used in Initial Value Problems. |
The input arguments are
Specifies the symmetry of the problem. m can be 0 = slab, 1 = cylindrical, or 2 = spherical. It corresponds to m in Equation 6-2. | |
Function that defines the components of the PDE. It computes
the terms
[c,f,s] = pdefun(x,t,u,dudx) where x and t are scalars, and u and dudx are vectors that approximate the solution
| |
Function that evaluates the initial conditions. It has the form u = icfun(x) When called with an argument x, icfun evaluates and returns the initial values of the solution components at x in the column vector u. | |
Function that evaluates the terms
[pl,ql,pr,qr] = bcfun(xl,ul,xr,ur,t) where ul is the approximate solution at the left boundary xl = a and ur is the approximate solution at the right boundary xr = b. pl and ql are column vectors corresponding to p and the diagonal of q evaluated at xl. Similarly, pr and qr correspond to xr. When m> 0 and a = 0, boundedness of the solution near x = 0 requires that the f vanish at a = 0. pdepe imposes this boundary condition automatically and it ignores values returned in pl and ql. | |
Vector [x0, x1,
..., xn] specifying the points at which a numerical
solution is requested for every value in tspan. x0 and xn correspond to
Second-order approximation to the solution is made on the mesh
specified in xmesh. Generally, it is best to use
closely spaced mesh points where the solution changes rapidly. pdepe does not select the mesh in
The elements of xmesh must satisfy x0 < x1 < ... < xn. The length of xmesh must be ≥ 3. | |
Vector [t0, t1, ..., tf] specifying the
points at which a solution is requested for every value in xmesh. t0 and tf correspond
to
pdepe performs the time integration with an ODE solver that selects both the time step and formula dynamically. The solutions at the points specified in tspan are obtained using the natural continuous extension of the integration formulas. The elements of tspan merely specify where you want answers and the cost depends weakly on the length of tspan. The elements of tspan must satisfy t0 < t1 < ... < tf. The length of tspan must be ≥ 3. |
The output argument sol is a three-dimensional array, such that
sol(:,:,k) approximates component k of the solution
.
sol(i,:,k) approximates component k of the solution at time tspan(i) and mesh points xmesh(:).
sol(i,j,k) approximates component k of the solution at time tspan(i) and the mesh point xmesh(j).
For more advanced applications, you can also specify as input arguments solver options and additional parameters that are passed to the PDE functions.
Structure of optional parameters that change the default integration properties. This is the seventh input argument. sol = pdepe(m,pdefun,icfun,bcfun,...
xmesh,tspan,options)
See Integrator Options for more information. |
The default integration properties in the MATLAB PDE solver are selected to handle common problems. In some cases, you can improve solver performance by overriding these defaults. You do this by supplying pdepe with one or more property values in an options structure.
sol = pdepe(m,pdefun,icfun,bcfun,xmesh,tspan,options)
Use odeset to create the options structure. Only those options of the underlying ODE solver shown in the following table are available for pdepe. The defaults obtained by leaving off the input argument options are generally satisfactory. Integrator Options tells you how to create the structure and describes the properties.
PDE Properties
Properties Category | Property Name |
|---|---|
Error control | RelTol, AbsTol, NormControl |
Step-size | InitialStep, MaxStep |
Solving the Equation. This example illustrates the straightforward formulation, solution, and plotting of the solution of a single PDE
![]()
This equation holds on an interval
for
times t ≥ 0. At
, the solution satisfies the initial condition
![]()
At
and
, the solution satisfies the boundary conditions
![]()
Note The demo pdex1 contains the complete code for this example. The demo uses subfunctions to place all functions it requires in a single M-file. To run the demo type pdex1 at the command line. See PDE Solver Syntax for more information. |
Rewrite the PDE. Write the PDE in the form
![]()
This is the form shown in Equation 6-2 and expected by pdepe. See Initial Value Problems for more information. For this example, the resulting equation is
![]()
with parameter
and the terms

Code the PDE. Once you rewrite the PDE in the form shown above (Equation 6-2) and identify the terms, you can code the PDE in a function that pdepe can use. The function must be of the form
[c,f,s] = pdefun(x,t,u,dudx)
where c, f, and s correspond to the
,
, and
terms. The code below computes c, f, and s for the example
problem.
function [c,f,s] = pdex1pde(x,t,u,DuDx) c = pi^2; f = DuDx; s = 0;
Code the initial conditions function. You must code the initial conditions in a function of the form
u = icfun(x)
The code below represents the initial conditions in the function pdex1ic.
function u0 = pdex1ic(x) u0 = sin(pi*x);
Code the boundary conditions function. You must also code the boundary conditions in a function of the form
[pl,ql,pr,qr] = bcfun(xl,ul,xr,ur,t)
The boundary conditions, written in the same form as Equation 6-4, are
![]()
and
![]()
The code below evaluates the components
and
of the boundary conditions in the function pdex1bc.
function [pl,ql,pr,qr] = pdex1bc(xl,ul,xr,ur,t) pl = ul; ql = 0; pr = pi * exp(-t); qr = 1;
In the function pdex1bc, pl and ql correspond to the left boundary conditions
(
), and pr and qr correspond to the right boundary condition
.
Select mesh points
for the solution. Before you use the MATLAB PDE solver,
you need to specify the mesh points
at which you want pdepe to
evaluate the solution. Specify the points as vectors t and x.
The vectors t and x play different roles in the solver (see PDE Solver). In particular, the cost and the accuracy of the solution depend strongly on the length of the vector x. However, the computation is much less sensitive to the values in the vector t.
This example requests the solution on the mesh produced by 20 equally spaced points from the spatial interval [0,1] and five values of t from the time interval [0,2].
x = linspace(0,1,20); t = linspace(0,2,5);
Apply the PDE solver. The example calls pdepe with m = 0, the functions pdex1pde, pdex1ic, and pdex1bc, and the mesh defined by x and
t at which pdepe is to evaluate the solution. The pdepe function returns the numerical solution in a three-dimensional
array sol, where sol(i,j,k) approximates
the kth component of the solution,
, evaluated at t(i) and x(j).
m = 0; sol = pdepe(m,@pdex1pde,@pdex1ic,@pdex1bc,x,t);
This example uses @ to pass pdex1pde, pdex1ic, and pdex1bc as function handles to pdepe.
Note See the function_handle (@), func2str, and str2func reference pages, and the @ section of MATLAB Programming Fundamentals for information about function handles. |
View the results. Complete the example by displaying the results:
Extract and display the first solution component.
In this example, the solution
has only one component, but for illustrative
purposes, the example "extracts" it from the three-dimensional
array. The surface plot shows the behavior of the solution.
u = sol(:,:,1);
surf(x,t,u)
title('Numerical solution computed with 20 mesh points')
xlabel('Distance x')
ylabel('Time t')

Display a solution profile at
, the final value of
. In this example,
=
= 2.
figure
plot(x,u(end,:))
title('Solution at t = 2')
xlabel('Distance x')
ylabel('u(x,2)')

Evaluating the Solution. After obtaining and plotting the solution above, you might be interested in a solution profile for a particular value of t, or the time changes of the solution at a particular point x. The kth column u(:,k) (of the solution extracted in step 7) contains the time history of the solution at x(k). The jth row u(j,:) contains the solution profile at t(j).
Using the vectors x and u(j,:), and the helper function pdeval, you can evaluate the solution u and its derivative
at any set of points xout
[uout,DuoutDx] = pdeval(m,x,u(j,:),xout)
The example pdex3 uses pdeval to evaluate the derivative of the solution at xout = 0. See pdeval for details.
This example illustrates the solution of a system of partial
differential equations. The problem is taken from electrodynamics.
It has boundary layers at both ends of the interval, and the solution
changes rapidly for small
.
The PDEs are

where
. The equations hold on
an interval 0 less than or equal to x less than or equal to 1
for times
.
The solution
satisfies the initial conditions
![]()
and boundary conditions

Note The demo pdex4 contains the complete code for this example. The demo uses subfunctions to place all required functions in a single M-file. To run this example type pdex4 at the command line. |
Rewrite the PDE. In the form expected by pdepe, the equations are
![]()
The boundary conditions on the partial derivatives of
have to be written in
terms of the flux. In the form expected by pdepe, the left boundary condition is
![]()
and the right boundary condition is
![]()
Code the PDE. After you rewrite the PDE in the form shown above, you can code it as a function that pdepe can use. The function must be of the form
[c,f,s] = pdefun(x,t,u,dudx)
where c, f, and s correspond to the
,
, and
terms in Equation 6-2.
function [c,f,s] = pdex4pde(x,t,u,DuDx) c = [1; 1]; f = [0.024; 0.17] .* DuDx; y = u(1) - u(2); F = exp(5.73*y)-exp(-11.47*y); s = [-F; F];
Code the initial conditions function. The initial conditions function must be of the form
u = icfun(x)
The code below represents the initial conditions in the function pdex4ic.
function u0 = pdex4ic(x); u0 = [1; 0];
Code the boundary conditions function. The boundary conditions functions must be of the form
[pl,ql,pr,qr] = bcfun(xl,ul,xr,ur,t)
The code below evaluates the components
and
(Equation 6-4) of the boundary conditions in the function pdex4bc.
function [pl,ql,pr,qr] = pdex4bc(xl,ul,xr,ur,t) pl = [0; ul(2)]; ql = [1; 0]; pr = [ur(1)-1; 0]; qr = [0; 1];
Select mesh points
for the solution. The solution changes rapidly for small
. The program selects
the step size in time to resolve this sharp change, but to see this
behavior in the plots, output times must be selected accordingly.
There are boundary layers in the solution at both ends of [0,1], so
mesh points must be placed there to resolve these sharp changes. Often
some experimentation is needed to select the mesh that reveals the
behavior of the solution.
x = [0 0.005 0.01 0.05 0.1 0.2 0.5 0.7 0.9 0.95 0.99 0.995 1]; t = [0 0.005 0.01 0.05 0.1 0.5 1 1.5 2];
Apply the PDE solver. The example calls pdepe with m = 0, the functions pdex4pde, pdex4ic, and pdex4bc, and the mesh defined by x and
t at which pdepe is to evaluate the solution. The pdepe function returns the numerical solution in a three-dimensional
array sol, where sol(i,j,k) approximates
the kth component of the solution,
, evaluated at t(i) and x(j).
m = 0; sol = pdepe(m,@pdex4pde,@pdex4ic,@pdex4bc,x,t);
View the results. The surface plots show the behavior of the solution components.
u1 = sol(:,:,1);
u2 = sol(:,:,2);
figure
surf(x,t,u1)
title('u1(x,t)')
xlabel('Distance x')
ylabel('Time t')

figure
surf(x,t,u2)
title('u2(x,t)')
xlabel('Distance x')
ylabel('Time t')

The following additional examples are available. Type
edit examplename
to view the code and
examplename
to run the example.
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