If the boundary conditions in a physical problem relate to the perimeter of an ellipse, then elliptical coordinates are convenient. These are given by
The two-dimensional wave equation
then becomes
The separated solutions
can be obtained from the
modified Mathieu’s equation (28.20.1) for
and from Mathieu’s
equation (28.2.1) for
, where
is the separation constant and
.
This leads to integral equations and an integral relation between the
solutions of Mathieu’s equation (setting
,
in
(28.32.3)).
Let
be a solution of Mathieu’s equation (28.2.1) and
be a solution of
Also let
be a curve (possibly improper) such that the quantity
approaches the same value when
tends to the endpoints of
.
Then
defines a solution of Mathieu’s equation, provided that (in the case of an
improper curve) the integral converges with respect to
uniformly on
compact subsets of
.
Kernels
can be found, for example, by separating solutions of the wave
equation in other systems of orthogonal coordinates. See
Schmidt and Wolf (1979).
The general paraboloidal coordinate system is linked with Cartesian coordinates via
where
is a parameter,
,
,
and
. When the Helmholtz equation
is separated in this system, each of the separated equations can be reduced to
the Whittaker–Hill equation (28.31.1), in which
are
separation constants. Two conditions are used to determine
. The
first is the
-periodicity of the solutions; the second can be their
asymptotic form. For further information see Arscott (1967) for
, and Urwin and Arscott (1970) for
.