Fourier Transform
The Fourier transform is a generalization of the complex Fourier series in the limit as
. Replace
the discrete
with the continuous
while letting
. Then change the sum to an integral,
and the equations become
|
(1)
| |||
|
(2)
|
Here,
|
(3)
| |||
|
(4)
|
is called the forward (
) Fourier transform,
and
|
(5)
| |||
|
(6)
|
is called the inverse (
) Fourier transform.
The notation
is introduced in Trott (2004,
p. xxxiv), and
and
are sometimes
also used to denote the Fourier transform and inverse Fourier transform, respectively
(Krantz 1999, p. 202).
Note that some authors (especially physicists) prefer to write the transform in terms of angular frequency
instead of the oscillation
frequency
. However, this destroys the symmetry,
resulting in the transform pair
|
(7)
| |||
|
(8)
| |||
|
(9)
| |||
|
(10)
|
To restore the symmetry of the transforms, the convention
|
(11)
| |||
|
(12)
| |||
|
(13)
| |||
|
(14)
|
is sometimes used (Mathews and Walker 1970, p. 102).
In general, the Fourier transform pair may be defined using two arbitrary constants
and
as
![]() |
(15)
| ||
![]() |
(16)
|
The Fourier transform
of a function
is implemented the Wolfram
Language as FourierTransform[f,
x, k], and different choices of
and
can be used by
passing the optional FourierParameters->
a, b
option. By default, the Wolfram
Language takes FourierParameters as
. Unfortunately,
a number of other conventions are in widespread use. For example,
is used in
modern physics,
is used in pure mathematics and
systems engineering,
is used in probability theory for
the computation of the characteristic function,
is used in classical physics, and
is used in signal processing.
In this work, following Bracewell (1999, pp. 6-7), it is always assumed that
and
unless
otherwise stated. This choice often results in greatly simplified transforms
of common functions such as 1,
, etc.
Since any function can be split up into even and odd portions
and
,
|
(17)
| |||
|
(18)
|
a Fourier transform can always be expressed in terms of the Fourier cosine transform and Fourier sine transform as
|
(19)
|
A function
has a forward and inverse Fourier
transform such that
![]() |
(20)
|
provided that
1.
exists.
2. There are a finite number of discontinuities.
3. The function has bounded variation. A sufficient weaker condition is fulfillment of the Lipschitz condition
(Ramirez 1985, p. 29). The smoother a function (i.e., the larger the number of continuous derivatives), the more compact its Fourier transform.
The Fourier transform is linear, since if
and
have Fourier
transforms
and
, then
|
(21)
| |||
|
(22)
|
Therefore,
|
(23)
| |||
|
(24)
|
The Fourier transform is also symmetric since
implies
.
Let
denote the convolution,
then the transforms of convolutions of functions have particularly nice transforms,
|
(25)
| |||
|
(26)
| |||
|
(27)
| |||
|
(28)
|
The first of these is derived as follows:
|
(29)
| |||
|
(30)
| |||
|
(31)
| |||
|
(32)
|
where
.
There is also a somewhat surprising and extremely important relationship between the autocorrelation and the Fourier transform
known as the Wiener-Khinchin theorem.
Let
, and
denote the complex conjugate of
, then the Fourier
transform of the absolute square of
is given by
|
(33)
|
The Fourier transform of a derivative
of a function
is simply related to the transform
of the function
itself. Consider
|
(34)
|
Now use integration by parts
|
(35)
|
with
|
(36)
| |||
|
(37)
|
and
|
(38)
| |||
|
(39)
|
then
|
(40)
|
The first term consists of an oscillating function times
. But if the
function is bounded so that
|
(41)
|
(as any physically significant signal must be), then the term vanishes, leaving
|
(42)
| |||
|
(43)
|
This process can be iterated for the
th derivative
to yield
|
(44)
|
The important modulation theorem of Fourier transforms allows
to be expressed
in terms of
as follows,
|
(45)
| |||
|
(46)
| |||
|
(47)
| |||
|
(48)
|
Since the derivative of the Fourier transform is given by
|
(49)
|
it follows that
|
(50)
|
Iterating gives the general formula
|
(51)
| |||
|
(52)
|
The variance of a Fourier transform is
|
(53)
|
and it is true that
|
(54)
|
If
has the Fourier transform
,
then the Fourier transform has the shift property
|
(55)
| |||
|
(56)
|
so
has the Fourier transform
|
(57)
|
If
has a Fourier transform
,
then the Fourier transform obeys a similarity theorem.
|
(58)
|
so
has the Fourier transform
|
(59)
|
The "equivalent width" of a Fourier transform is
|
(60)
| |||
|
(61)
|
The "autocorrelation width" is
|
(62)
| |||
|
(63)
|
where
denotes the cross-correlation
of
and
and
is the complex
conjugate.
Any operation on
which leaves its area
unchanged leaves
unchanged, since
|
(64)
|
The following table summarized some common Fourier transform pairs.
In two dimensions, the Fourier transform becomes
|
(65)
| |||
|
(66)
|
Similarly, the
-dimensional Fourier transform can be
defined for
,
by
![]() |
(67)
| ||
![]() |
(68)
|


![f(x)={int_(-infty)^inftye^(2piikx)[int_(-infty)^inftyf(x)e^(-2piikx)dx]dk for f(x) continuous at x; 1/2[f(x_+)+f(x_-)] for f(x) discontinuous at x,](/images/equations/FourierTransform/NumberedEquation2.gif)


fourier transform




