In mathematics, a Fourier series, named in honor of Joseph Fourier (1768-1830), is a representation of a periodic function as a sum of periodic functions of the form

which are harmonics of ei x; Fourier was the first to study such series systematically. He applied these series to the solution of the heat equation, publishing his initial results in 1807 and 1811.

Table of contents
1 Definition of Fourier series
2 Convergence of Fourier series
3 General formulation
4 See also

Definition of Fourier series

Suppose f(x) is a complex-valued function of a real number, is periodic with period 2π, and is square integrable over the interval from 0 to 2π. Let

Then the Fourier series representation of f(x) is given by

this is equivalent to representing f(x) as a infinite linear combination of functions of the form , i.e.

Convergence of Fourier series

While the coefficients an and bn can be formally defined for any function for which the integrals make sense, whether the series so defined actually converges to f(x) depends on the properties of f.

A partial answer is that if f is square-integrable then

(this is convergence in the norm of the space ).

That much was proved in the 19th century, as was the fact that if f is piecewise continuous then the series converges at each point of continuity. Perhaps surprisingly, it was not shown until the 1960s that if f is quadratically integrable then the series converges for every value of x except those in some set of measure zero.

General formulation

The useful properties of Fourier series are largely derived from the orthogonality of the functions ei n x. Other sequences of orthogonal functions have similar properties. Examples include sequences of Bessel functions and orthogonal polynomials. Such sequences are commonly the solutions of a differential equation; a large class of useful sequences are solutions of the so-called Sturm-Liouville problems.

See also