Fourier series
A Fourier series is an expansion of a periodic
function f(x) in terms of an infinite sum of sines and cosines. Fourier
series make use of the orthogonality
relationships of the sine and cosine functions. The
computation and study of Fourier series is known as harmonic
analysis and is extremely useful as a way to break up an
arbitrary periodic function into a set of simple terms than can be
plugged in, solved individually, and then recombined to obtain the
solution to the original problem or an approximation to it to whatever
accuracy is desired or practical. Examples of successive approximations to
common functions using Fourier series are illustrated above.
In particular, since the superposition
principle holds for solutions of a linear homogeneous ordinary
differential equation, if such an equation can be solved in the case a
single sinusoid, the solution for an arbitrary function is immediately
available by expressing the original function as a Fourier series and then
plugging in the solution for each sinusoidal component. In some special
cases where the Fourier series can be summed in closed form, this
technique can even yield analytic solutions.
Any set of functions that form a complete
orthogonal system have a corresponding generalized
Fourier series analogous to the Fourier series. For example, using
orthogonality of the roots of a Bessel
function of the first kind gives a so-called Fourier-Bessel
series.
The computation of the (usual) Fourier series is based on the integral
identities
for , where is the Kronecker
delta.
Using the method for a generalized
Fourier series, the usual Fourier series involving sines and cosines
is obtained by taking and . Since these functions form a complete
orthogonal system over , the Fourier series of a function
f(x) is given by
 |
(6) |
where
and n = 1, 2, 3, .... Note that the coefficient of the
constant term has been written in a special form compared fo the
general form for a generalized
Fourier series in order to preserve symmetry with the definitions of
and .
A Fourier series converges to the function (equal to the original function at points of
continuity or to the average of the two limits at points of discontinuity)
 |
(10) |
if the function satisfies so-called Dirichlet
conditions.
As a result, near points of discontinuity, a "ringing" known as theGibbs
phenomenon, illustrated above, can occur.
For a function f(x) periodic on an interval instead of , a simple change of variables can be used
to transform the interval of integration from to . Let
Solving for gives , and plugging this in gives
 |
(13) |
Therefore,
Similarly, the function is instead defined on the interval , the above equations simply
become
In fact, for f(x) periodic with period
, any interval can be used, with the choice being one of
convenience or personal preference (Arfken 1985, p. 769).
Thecoefficients for
Fourier series expansions of a few common functions are given in Beyer
(1987, pp. 411-412) and Byerly (1959, p. 51). One of the most
common functions usually analyzed by this technique is the square
wave. The Fourier series for a number of common functions are
summarized in the table below.
| function |
f(x) |
Fourier series |
| Fourier
series--sawtooth wave |
 |
 |
| Fourier
series--square wave |
 |
 |
| Fourier
series--triangle wave |
T(x) |
 |
If a function is even so that
, then is odd. (This
follows since is odd and an even function
times an odd
function is an odd function.)
Therefore, for all n. Similarly, if a function is odd so that
, then is odd. (This
follows since is even and aneven function
times an odd
function is an odd function.)
Therefore, for all n.
The notion of a Fourier series can also be extended to complex coefficients.
Consider a real-valued function f(x). Write
 |
(20) |
Now examine
so
 |
(26) |
The coefficients can
be expressed in terms of those in the Fourier series
For a function periodic in , these become
These equations are the basis for the extremely importantFourier
transform, which is obtained by transforming from a discrete variable to a continuous one as the
length .
|