PDEONE Example A:
Supposed one wanted to solve the following system of partial
differential equations on the interval [0,1].
This we recognized as Burgers' equation with the addition of a
diffusive term. We desire the solution of the PDE above with
boundary conditions given by
here is an exact solution to the PDE given by
With initial conditions given by
This corresponds to the first example in the original reference to
PDEONE (given above). This is quite simple to solve with the
pdeone gateway in octave. First the user must specify an octave
function "F.m" which evaluates the right hand side of the PDE
expressed in the following form
The incoming arguments to the octave function F.m are t,x,u,ux,
and duxx. Here t is the scalar time, x the scalar grid point, u a
vector of the NPDE unknowns, ux a vector of the x derivatives of
these unknowns, and duxx is a matrix expressing the
following derivatives
With the background we can write our F.m function for evaluating the right hand
side of our PDEs. In addition to F.m, PDEONE requires the
information on the diffusion coefficients D. This is provided in
the form of a function
D.m.
PDEONE requires the boundary conditions of the form
To implement this in octave we must specify three boundary
functions with input arguments t,x, and u (with the same meanings as
above):
BNDRY_ALPHA.m,
BNDRY_BETA.m, and
BNDRY_GAMMA.m. In
the implementation BNDRY_GAMMA.m we can see one of the powers of implementing PDEs
in octave. In that function we call another octave function
truesol.m representing an
octave implementation of the true solution
above.
Finally the user must specify the initial conditions. In this
example we can use the same function "truesol.m". The two inputs
to the initial condition function are t and x. Here t is a scalar
input of time but in this case x is a vector of grid points where
the initial conditions are desired. Note, that to work properly
this function must be vectorized meaning that it can
return a matrix (of dimension [NPDE,Number of Grid Points]) of
initial conditions.
Once this code is written a person can call "pdeone.m". Here we
present an example pdeone_Script.m driver file. Note: Since
this problem is in Cartesian the constant c=0. Since this is the
default, there is no need to specify anything additional.
Finally, we can reap the benefits of our work by viewing the
solution to our problem:
Note that this is a replica of the plot given in the Sincovec and
Madsen paper.
John Weatherwax
Last modified: Thu Jan 5 21:46:29 EST 2006