Jump to content

Prolate spheroidal wave function

From Wikipedia, the free encyclopedia
This is an old revision of this page, as edited by Rjwilmsi (talk | contribs) at 13:07, 11 June 2012 (Format plain DOIs using AWB (8061)). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

In mathematics, the prolate spheroidal wave functions are a set of functions derived by timelimiting and lowpassing, and a second timelimit operation. Let denote the time truncation operator, such that iff x is timelimited within . Similarly, let denote an ideal low-pass filtering operator, such that iff x is bandlimited within . The operator turns out to be linear, bounded and self-adjoint. For we denote with the n-th eigenfunction, defined as

where are the associated eigenvalues. The timelimited functions are the Prolate Spheroidal Wave Functions (PSWFs).

These functions are also encountered in a different context. When solving the Helmholtz equation, , by the method of separation of variables in prolate spheroidal coordinates, , with:

and .

the solution can be written as the product of a radial spheroidal wavefunction and an angular spheroidal wavefunction by with .

The radial wavefunction satisfies the linear ordinary differential equation:

The eigenvalue of this Sturm-Liouville differential equation is fixed by the requirement that must be finite for .

The angular wavefunction satisfies the differential equation:

It is the same differential equation as in the case of the radial wavefunction. However, the range of the variable is different (in the radial wavefunction, ) in the angular wavefunction ).

For these two differential equations reduce to the equations satisfied by the associated Legendre polynomials. For , the angular spheroidal wavefunctions can be expanded as a series of Legendre functions.

Let us note that if one writes , the function satisfies the following linear ordinary differential equation:

which is known as the spheroidal wave equation. This auxiliary equation is used for instance by Stratton in his 1935 article.

There are different normalization schemes for spheroidal functions. A table of the different schemes can be found in Abramowitz and Stegun p. 758. Abramowitz and Stegun (and the present article) follow the notation of Flammer.

In the case of oblate spheroidal coordinates the solution of the Helmholtz equation yields oblate spheroidal wavefunctions.

Originally, the spheroidal wave functions were introduced by C. Niven in 1880 when studying the conduction of heat in an ellipsoid of revolution, which lead to a Helmholtz equation in spheroidal coordinates.

Prolate spheroidal wave functions whose domain is a (portion of) the surface of the unit sphere are more generally called "Slepian functions"[1] (see also Spectral concentration problem). These are of great utility in disciplines such as geodesy[2] or cosmology.[3]

References

  1. ^ F. J. Simons, M. A. Wieczorek and F. A. Dahlen. Spatiospectral concentration on a sphere. SIAM Review, 2006, doi:10.1137/S0036144504445765
  2. ^ F. J. Simons and Dahlen, F. A. "Spherical Slepian functions and the polar gap in Geodesy". Geophysical Journal International, 2006, doi:10.1111/j.1365-246X.2006.03065.x
  3. ^ Dahlen, F. A., and F. J. Simons. "Spectral estimation on a sphere in geophysics and cosmology". Geophysical Journal International, 2008, doi:10.1111/j.1365-246X.2008.03854.x