Fourier transform

Fourier transforms
	Continuous Fourier transform
	Fourier series
	Discrete Fourier transform
	Discrete-time Fourier transform
	Related transforms

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This article specifically discusses Fourier transformation of functions on the real line; for other kinds of Fourier transformation, see Fourier analysis and list of Fourier-related transforms.

In mathematics, the Fourier transform is an operation that transforms one complex-valued function of a real variable into another. The new function, often called the frequency domain representation of the original function, describes which frequencies are present in the original function. This is in a similar spirit to the way that a chord of music can be described by notes that are being played. In effect, the Fourier transform decomposes a function into oscillatory functions. The Fourier transform (FT) is similar to many other operations in mathematics which make up the subject of Fourier analysis. In this specific case, both the domains of the original function and its frequency domain representation are continuous and unbounded. The term Fourier transform can refer to both the frequency domain representation of a function or to the process/formula that "transforms" one function into the other.

[edit] Definition

There are several common conventions for defining the Fourier transform of an integrable function ƒ : R → C (Kaiser 1994). This article will use the definition:

$\hat{f}(\xi) := \int_{-\infty}^{\infty} f(x)\ e^{- 2\pi i x \xi}\,dx,$ for every real number ξ. (This letter is the lowercase Greek letter Xi).

When the independent variable x represents time (with SI unit of seconds), the transform variable ξ represents ordinary frequency (in hertz). Under suitable conditions, ƒ can be reconstructed from $\hat f$ by the inverse transform:

$f(x) = \int_{-\infty}^{\infty} \hat{f}(\xi)\ e^{2 \pi i x \xi}\,d\xi,$ for every real number x.

For other common conventions and notations see the sections Other conventions and Other notations below.

[edit] Introduction

[edit] Properties of the Fourier transform

An integrable function is a function ƒ on the real line that is Lebesgue-measurable and satisfies

$\int_{-\infty}^\infty |f(x)| \, dx < \infty.$

[edit] Basic properties

Given integrable functions f(x), g(x), and h(x) denote their Fourier transforms by $\hat{f}(\xi)$ , $\hat{g}(\xi)$ , and $\hat{h}(\xi)$ respectively. The Fourier transform has the following basic properties (Pinsky 2002).

Linearity: For any complex numbers a and b, if h(x) = aƒ(x) + bg(x), then $\hat{h}(\xi)=a\cdot \hat{f}(\xi) + b\cdot\hat{g}(\xi).$
Translation: For any real number x₀, if h(x) = ƒ(x − x₀), then $\hat{h}(\xi)= e^{-2\pi i x_0\xi }\hat{f}(\xi).$
Modulation: For any real number ξ₀, if h(x) = e^2πixξ₀ƒ(x), then $\hat{h}(\xi) = \hat{f}(\xi-\xi_{0})$ .
Scaling: For all non-zero real numbers a, if h(x) = ƒ(ax), then $\hat{h}(\xi)=\frac{1}{|a|}\hat{f}\left(\frac{\xi}{a}\right)$ . The case a = −1 leads to the time-reversal property, which states: if h(x) = ƒ(−x), then $\hat{h}(\xi)=\hat{f}(-\xi)$ .
Conjugation: If $h(x)=\overline{f(x)}$ , then $\hat{h}(\xi) = \overline{\hat{f}(-\xi)}.$
Convolution: If $h(x)=\left(f*g\right)(x)$ , then $\hat{h}(\xi)=\hat{f}(\xi)\cdot \hat{g}(\xi).$

[edit] Uniform continuity and the Riemann-Lebesgue lemma

The Fourier transform of integrable functions have additional properties that do not always hold. The Fourier transform of integrable functions ƒ are uniformly continuous and $\|\hat{f}\|_{\infty}\leq \|f\|_1$ (Katznelson 1976). The Fourier transform of integrable functions also satisfy the Riemann-Lebesgue lemma which states that (Stein & Weiss 1971)

$\hat{f}(\xi)\to 0\text{ as }|\xi|\to \infty.\,$

The Fourier transform $\hat f$ of an integrable function ƒ is bounded and continuous, but need not be integrable. It is not possible in general to write the inverse transform as a Lebesgue integral. However, when both ƒ and $\hat f$ are integrable, the following inverse equality holds true for almost every x:

$f(x) = \int_{-\infty}^\infty \hat f(\xi) e^{2 i \pi x \xi} \, d\xi.$

Almost everywhere, ƒ is equal to the continuous function given by the right-hand side. If ƒ is given as continuous function on the line, then equality holds for every x.

A consequence of the preceding result is that the Fourier transform is injective on L¹(R).

[edit] The Plancherel theorem and Parseval's theorem

Let f(x) and g(x) be integrable, and let $\hat{f}(\xi)$ and $\hat{g}(\xi)$ be their Fourier transforms. If f(x) and g(x) are also square-integrable, then we have Parseval's theorem (Rudin 1987, p. 187):

$\int_{-\infty}^{\infty} f(x) \overline{g(x)} \, dx = \int_{-\infty}^\infty \hat{f}(\xi) \overline{\hat{g}(\xi)} \, d\xi,$

where the bar denotes complex conjugation.

The Plancherel theorem, which is equivalent to Parseval's theorem, states (Rudin 1987, p. 186):

$\int_{-\infty}^\infty \left| f(x) \right|^2\, dx = \int_{-\infty}^\infty \left| \hat{f}(\xi) \right|^2\, d\xi.$

The Plancherel theorem makes it possible to define the Fourier transform for functions in L²(R), as described in Generalizations below. The Plancherel theorem has the interpretation in the sciences that the Fourier transform preserves the energy of the original quantity. It should be noted that depending on the author either of these theorems might be referred to as the Plancherel theorem or as Parseval's theorem.

See Pontryagin duality for a general formulation of this concept in the context of locally compact abelian groups.

[edit] Uncertainty principle

Generally speaking, the more concentrated f(x) is, the more spread out its Fourier transform $\hat{f}(\xi)$ must be. In particular, the scaling property of the Fourier transform may be seen as saying: if we "squeeze" a function in x, its Fourier transform "stretches out" in ξ. It is not possible to arbitrarily concentrate both a function and its Fourier transform.

The trade-off between the compaction of a function and its Fourier transform can be formalized in the form of an Uncertainty Principle. Suppose ƒ(x) is an integrable and square-integrable function. Without loss of generality, assume that ƒ(x) is normalized:

$\int_{-\infty}^\infty |f(x)|^2 \,dx=1.$

It follows from the Plancherel theorem that $\hat{f}(\xi)$ is also normalized.

The spread around x = 0 may be measured by the dispersion about zero (Pinsky 2002) defined by

$D_0(f)=\int_{-\infty}^\infty x^2|f(x)|^2\,dx.$

In probability terms, this is the second moment of $|f(x)|^2\,\!$ about zero.

The Uncertainty principle states that, if ƒ(x) is absolutely continuous and the functions x·ƒ(x) and ƒ′(x) are square integrable, then

$D_0(f)D_0(\hat{f}) \geq \frac{1}{16\pi^2}$ (Pinsky 2002).

The equality is attained only in the case $f(x)=C_1 \, e^{{- \pi x^2}/{\sigma^2}}$ (hence $\quad \hat{f}(\xi)= \sigma C_1 \, e^{-\pi\sigma^2\xi^2}$ ) where σ > 0 is arbitrary and C₁ is such that ƒ is L²–normalized (Pinsky 2002). In other words, where ƒ is a (normalized) Gaussian function, centered at zero.

In fact, this inequality implies that:

$\left(\int_{-\infty}^\infty (x-x_0)^2|f(x)|^2\,dx\right)\left(\int_{-\infty}^\infty(\xi-\xi_0)^2|\hat{f}(\xi)|^2\,d\xi\right)\geq \frac{1}{16\pi^2}$

for any $x_0, \, \xi_0$ in R (Stein & Shakarchi 2003).

In quantum mechanics, the momentum and position wave functions are Fourier transform pairs, to within a factor of Planck's constant. With this constant properly taken into account, the inequality above becomes the statement of the Heisenberg uncertainty principle (Stein & Shakarchi 2003).

[edit] Poisson summation formula

Main article: Poisson summation formula

The Poisson summation formula provides a link between the study of Fourier transforms and Fourier Series. Given an integrable function ƒ in L¹(Rⁿ) we can consider the periodization of ƒ given by

$\bar f(x)=\sum_{k\in\mathbb{Z}^n} f(x+k).$

Then the Poisson summation formula relates the Fourier series of $\bar f$ to the Fourier transform of ƒ. Specifically it states that the Fourier series of $\bar f$ is given by:

$\bar f(x) \sim \sum_{k\in\mathbb{Z}^n} \hat{f}(k)e^{2\pi i k\cdot x}.$

The Poisson summation formula maybe used to derive Landau's asymptotic formula for the number of lattice points in a large Euclidean sphere. It can also be used to show that if an integrable function, ƒ, and $\hat f$ both have compact support then ƒ = 0 (Pinsky 2002).

[edit] Convolution theorem

Main article: Convolution theorem

The Fourier transform translates between convolution and multiplication of functions. If ƒ(x) and g(x) are integrable functions with Fourier transforms $\hat{f}(\xi)$ and $\hat{g}(\xi)$ respectively, and if the convolution of ƒ and g exists and is absolutely integrable, then the Fourier transform of the convolution is given by the product of the Fourier transforms $\hat{f}(\xi)$ and $\hat{g}(\xi)$ (under other conventions for the definition of the Fourier transform a constant factor may appear).

This means that if:

$h(x) = (f*g)(x) = \int_{-\infty}^\infty f(y)g(x - y)\,dy,$

where ∗ denotes the convolution operation, then:

$\hat{h}(\xi) = \hat{f}(\xi)\cdot \hat{g}(\xi).$

In linear time invariant (LTI) system theory, it is common to interpret g(x) as the impulse response of an LTI system with input ƒ(x) and output h(x), since substituting the unit impulse for ƒ(x) yields h(x) = g(x). In this case, $\hat{g}(\xi)$ represents the frequency response of the system.

Conversely, if ƒ(x) can be decomposed as the product of two square integrable functions p(x) and q(x), then the Fourier transform of ƒ(x) is given by the convolution of the respective Fourier transforms $\hat{p}(\xi)$ and $\hat{q}(\xi)$ .

[edit] Cross-correlation theorem

Main article: Cross-correlation

In an analogous manner, it can be shown that if h(x) is the cross-correlation of ƒ(x) and g(x):

$h(x)=(f\star g)(x) = \int_{-\infty}^\infty \overline{f(y)}\,g(x+y)\,dy$

then the Fourier transform of h(x) is:

$\hat{h}(\xi) = \overline{\hat{f}(\xi)}\,\hat{g}(\xi).$

[edit] Eigenfunctions

One important choice of an orthonormal basis for L²(R) is given by the Hermite functions

${\psi}_n(x) = \frac{2^{1/4}}{\sqrt{n!}} \, e^{-\pi x^2}H_n(2x\sqrt{\pi}),$

where $H n (x)$ are the "probabilist's" Hermite polynomials, defined by H_n(x) = (−1)ⁿexp(x²/2) Dⁿ exp(−x²/2). Under this convention for the Fourier transform, we have that

$\hat\psi_n(\xi) = (-i)^n {\psi}_n(\xi) .$

In other words, the Hermite functions form a complete orthonormal system of eigenfunctions for the Fourier transform on L²(R) (Pinsky 2002). However, this choice of eigenfunctions is not unique. There are only four different eigenvalues of the Fourier transform (±1 and ±i) and any linear combination of eigenfunctions with the same eigenvalue gives another eigenfunction. As a consequence of this, it is possible to decompose L²(R) as a direct sum of four spaces H₀, H₁, H₂, and H₃ where the Fourier transform acts on H_k simply by multiplication by i^k. This approach to define the Fourier transform is due to N. Wiener (Duoandikoetxea 2001). The choice of Hermite functions is convenient because they are exponentially localized in both frequency and time domains, and thus give rise to the fractional Fourier transform used in time-frequency analysis^{[citation needed]}.

[edit] Spherical harmonics

Let the set of homogeneous harmonic polynomials of degree k be denoted by ${\mathcal A}_k$ . The set ${\mathcal A}_k$ are known as the solid spherical harmonics. The solid spherical harmonics play a similar role to the Hermite polynomials in higher dimensions. Specifically, if f(x) = e^−π|x|²P(x) for some P(x) in ${\mathcal A}_k$ , then $\hat{f}(\xi)=i^{-k}f(\xi)$ . Let the set ${\mathcal H}_k$ be the closure in L²(Rⁿ) of linear combinations of functions of the form f(|x|)P(x) where P(x) is in ${\mathcal A}_k$ . The space L²(Rⁿ) is then a direct sum of the spaces ${\mathcal H}_k$ and the Fourier transform maps each space ${\mathcal H}_k$ to itself and is possible to characterize the action of the Fourier transform on each space ${\mathcal H}_k$ (Stein & Weiss 1971). Let ƒ(x) = ƒ₀(|x|)P(x) (with P(x) in ${\mathcal A}_k$ ), then $\hat{f}(\xi)=F_0(|\xi|)P(\xi)$ where

$F_0(r)=2\pi i^{-k}r^{-(n+2k-2)/2}\int_0^\infty f_0(s)J_{(n+2k-2)/2}(2\pi rs)s^{(n+2k)/2}\,ds.$

Here J_{(n + 2k − 2)/2} denotes the Bessel function of the first kind with order (n + 2k − 2)/2. When k = 0 this gives a useful formula for the Fourier transform of a radial function (Grafakos 2004).

[edit] Generalizations

[edit] Fourier transform on other function spaces

It is possible to extend the definition of the Fourier transform to other spaces of functions. Since compactly supported smooth functions are integrable and dense in L²(R), the Plancherel theorem allows us to extend the definition of the Fourier transform to general functions in L²(R) by continuity arguments. Further $\mathcal{F}$ : L²(R) → L²(R) is a unitary operator (Stein & Weiss 1971, Thm. 2.3). Many of the properties remain the same for the Fourier transform. The Hausdorff-Young inequality can be used to extend the definition of the Fourier transform to include functions in L^p(R) for 1 ≤ p ≤ 2. Unfortunately, further extensions become more technical. The Fourier transform of functions in L^p for the range 2 < p < ∞ requires the study of distributions (Katznelson 1976). In fact, it can be shown that there are functions in L^p with p>2 so that the Fourier transform is not defined as a function (Stein & Weiss 1971).

[edit] Multi-dimensional version

The Fourier transform can be in any arbitrary number of dimensions n. As with the one-dimensional case there are many conventions, for an integrable function ƒ(x) this article takes the definition:

$\hat{f}(\xi) = \mathcal{F}(f)(\xi) = \int_{\R^n} f(x) e^{-2\pi i x\cdot\xi} \, dx$

where x and ξ are n-dimensional vectors, and x · ξ is the dot product of the vectors. The dot product is sometimes written as $\left\langle x,\xi \right\rangle$ .

All of the basic properties listed above hold for the n-dimensional Fourier transform, as do Plancherel's and Parseval's theorems. When the function is integrable, the Fourier transform is still uniformly continuous and the Riemann-Lebesgue lemma holds. (Stein & Weiss 1971)

In higher dimensions it becomes interesting to study restriction problems for the Fourier transform. The Fourier transform of an integrable function is continuous and the restriction of this function to any set is defined. But for a square-integrable function the Fourier transform could be a general class of square integrable functions. As such, the restriction of the Fourier transform of an L²(Rⁿ) function cannot be defined on sets of measure 0. It is still an active area of study to understand restriction problems in L^p for 1 < p < 2. Surprisingly, it is possible in some cases to define the restriction of a Fourier transform to a set S, provided S has non-zero curvature. The case when S is the unit sphere in Rⁿ is of particular interest. In this case the Thomas-Stein restriction theorem states that the restriction of the Fourier transform to the unit sphere in Rⁿ is a bounded operator on L^p provided 1 ≤ p ≤ (2n + 2) / (n + 3).

One notable difference between the Fourier transform in 1 dimension versus higher dimensions concerns the partial sum operator. For a given integrable function ƒ, consider the function ƒ_R defined by:

$f_R(x) = \int_{S_R}\hat{f}(\xi) e^{2\pi ix\cdot\xi}\, d\xi, \quad x \in \mathbb{R}^n.$

Suppose in addition that ƒ is in L^p(Rⁿ). For n = 1 and 1 < p < ∞, if one takes S_R = (−R, R), then ƒ_R converges to ƒ in L^p as R tends to infinity, by the boundedness of the Hilbert Transform. Naively one may hope the same holds true for n > 1. In the case that S_R is taken to be a cube with side length R, then convergence still holds. Another natural candidate is the Euclidean ball S_R = {ξ : |ξ| < R}. In order for this partial sum operator to converge, it is necessary that the multiplier for the unit ball be bounded in L^p(Rⁿ). For n ≥ 2 it is a celebrated theorem of Charles Fefferman that the multiplier for the unit ball is never bounded unless p = 2 (Duoandikoetxea 2001). In fact, when p ≠ 2, this shows that not only may ƒ_R fail to converge to ƒ in L^p, but for some functions ƒ ∈ L^p(Rⁿ), ƒ_R is not even an element of L^p.

[edit] Fourier–Stieltjes transform

The Fourier transform of a finite Borel measure μ on Rⁿ is given by (Pinsky 2002):

$\hat\mu(\xi)=\int_{\mathbb{R}^n} \mathrm{e}^{-2\pi i x \cdot \xi}\,d\mu.$

This transform continues to enjoy many of the properties of the Fourier transform of integrable functions. One notable difference is that the Riemann-Lebesgue lemma fails for measures (Katznelson 1976). In the case that dμ = ƒ(x) dx, then the formula above reduces to the usual definition for the Fourier transform of ƒ.

The Fourier transform may be used to give a characterization of continuous measures. Bochner's theorem characterizes which functions may arise as the Fourier-Stieltjes transform of a measure (Katznelson 1976).

Furthermore, the Dirac delta function is not a function but it is a finite Borel measure. Its Fourier transform is a constant function (whose specific value depends upon the form of the Fourier transform used).

[edit] Tempered distributions

The Fourier transform maps the space of Schwartz functions to itself, and gives a homeomorphism of the space to itself (Stein & Weiss 1971). Because of this it is possible to define the Fourier transform of tempered distributions. These include all the integrable functions mentioned above and have the added advantage that the Fourier transform of any tempered distribution is again a tempered distribution.

The following two facts provide some motivation for the definition of the Fourier transform of a distribution. First let ƒ and g be integrable functions, and let $\hat{f}$ and $\hat{g}$ be their Fourier transforms respectively. Then the Fourier transform obeys the following multiplication formula (Stein & Weiss 1971),

$\int_{\mathbb{R}^n}\hat{f}(x)g(x)\,dx=\int_{\mathbb{R}^n}f(x)\hat{g}(x)\,dx.$

Secondly, every integrable function ƒ defines a distribution T_ƒ by the relation

$T_f(\varphi)=\int_{\mathbb{R}^n}f(x)\varphi(x)\,dx$ for all Schwartz functions φ.

In fact, given a distribution T, we define the Fourier transform by the relation

$\hat{T}(\varphi)=T(\hat{\varphi})$ for all Schwartz functions φ.

It follows that $\hat{T}_f=T_{\hat{f}}$ .

Distributions can be differentiated and the above mentioned compatibility of the Fourier transform with differentiation and convolution remains true for tempered distributions.

[edit] Locally compact abelian groups

The Fourier transform may be generalized to any locally compact Abelian group. A locally compact abelian group is an abelian group which is at the same time a locally compact Hausdorff topological space so that the group operations are continuous. If G is a locally compact abelian group, it has a translation invariant measure μ, called Haar measure. For a locally compact abelian group G it is possible to place a topology on the set of characters $\hat G$ so that $\hat G$ is also a locally compact abelian group. For a function ƒ in L¹(G) it is possible to define the Fourier transform by (Katznelson 1976):

$\hat{f}(\xi)=\int_G \xi(x)f(x)\,d\mu\qquad\text{for any }\xi\in\hat G.$

[edit] Applications

[edit] Analysis of differential equations

Fourier transforms, and the closely related Laplace transforms are widely used in solving differential equations. The Fourier transform is compatible with differentiation in the following sense: if f(x) is a differentiable function with Fourier transform $\hat{f}(\xi)$ , then the Fourier transform of its derivative is given by $2\pi i\xi\hat{f}(\xi)$ . This can be used to transform differential equations into algebraic equations. Note that this technique only applies to problems whose domain is the whole set of real numbers. By extending the Fourier transform to functions of several variables partial differential equations with domain Rⁿ can also be translated into algebraic equations.

[edit] Domain and range of the Fourier transform

It is often desirable to have the most general domain for the Fourier transform as possible. The definition of Fourier transform as an integral naturally restricts the domain to the space of integrable functions. Unfortunately, there is no simple characterizations of which functions are Fourier transforms of integrable functions (Stein & Weiss 1971). It is possible to extend the domain of the Fourier transform in various ways, as discussed in generalizations above. The following list details some of the more common domains and ranges on which the Fourier transform is defined.

The space of Schwartz functions is closed under the Fourier transform. Schwartz functions are rapidly decaying functions and do not include all functions which are relevant for the Fourier transform. More details may be found in (Stein & Weiss 1971).

The space L¹ of Lebesgue integrable functions maps into C₀, the space of continuous functions that tend to zero at infinity.

The space L² is closed under the Fourier transform, but here the Fourier transform is no longer defined by integration.

The space L^p maps into the space L^q, where 1/p + 1/q = 1 and 1 ≤ p ≤ 2 (Hausdorff-Young inequality).

The set of tempered distributions is closed under the Fourier transform. Tempered distributions are also a form of generalization of functions. It is in this generality that one can define the Fourier transform of objects like the Dirac comb.

[edit] Other notations

Other common notations for $\hat{f}(\xi)$ are: $\mathcal F(\xi)$ , $\mathcal{F}\left(f\right)(\xi)$ , $\left(\mathcal{F}f\right)(\xi)$ , $\mathcal{F}(f)$ , $\mathcal F(\omega)$ , $\mathcal F(j\omega)$ , $\mathcal{F}\{f\}$ and $\mathcal{F} \left(f(t)\right).$ Though less commonly other notations are used. Denote the Fourier transform by a capital letter corresponding to the letter of function being transformed (such as f(x) and F(ξ)) is especially common in the sciences and engineering. In electronics, the omega (ω) is often used instead of ξ due to its interpretation as angular frequency, sometimes it is written as F(jω), where j is the imaginary unit, to indicate its relationship with the Laplace transform, and sometimes it is replaced with 2πf in order to use common frequency.

The interpretation of the complex function $\hat{f}(\xi)$ may be aided by expressing it in polar coordinate form: $\hat{f}(\xi)=A(\xi)e^{i\varphi(\xi)}$ in terms of the two real functions A(ξ) and φ(ξ) where:

$A(\xi) = |\hat{f}(\xi)|, \,$

is the amplitude and

$\varphi (\xi) = \arg \big( \hat{f}(\xi) \big),$

is the phase (see arg function).

Then the inverse transform can be written:

$f(x) = \int _{-\infty}^{\infty} A(\xi)\ e^{ i(2\pi \xi x +\varphi (\xi))}\,d\nu,$

which is a recombination of all the frequency components of ƒ(x). Each component is a complex sinusoid of the form e^2πixξ whose amplitude is A(ξ) and whose initial phase angle (at x = 0) is φ(ξ).

The Fourier transform maybe thought of as a mapping on function spaces. This mapping is here denoted $\mathcal{F}$ and $\mathcal{F}(f)$ is used to denote the Fourier transform of the function f. This mapping is linear, which means that $\mathcal{F}$ can also be seen as a linear transformation on the function space and implies that the standard notation in linear algebra of applying a linear transformation to a vector (here the function f) can be used to write $\mathcal{F} f$ instead of $\mathcal{F}(f)$ . Since the result of applying the Fourier transform is again a function, we can be interested in the value of this function evaluated at the value ξ for its variable, and this is denoted either as $\mathcal{F}(f)(\xi)$ or as $(\mathcal{F} f)(\xi)$ . Notice that in the former case, it is implicitly understood that $\mathcal{F}$ is applied first to f and then the resulting function is evaluated at ξ, not the other way around.

In mathematics and various applied sciences it is often necessary to distinguish between a function f and the value of f when its variable equals x, denoted f(x). This means that a notation like $\mathcal{F}(f(x))$ formally can be interpreted as the Fourier transform of the values of f at x. Despite this flaw, the previous notation appears frequently, often when a particular function or a function of a particular variable is to be transformed. For example, $\mathcal{F}( \mathrm{rect}(x) ) = \mathrm{sinc}(\xi)$ is sometimes used to express that the Fourier transform of a rectangular function is a sinc function, or $\mathcal{F}(f(x+x_{0})) = \mathcal{F}(f(x)) e^{2\pi i \xi x_{0}}$ is used to express the shift property of the Fourier transform. Notice, that the last example is only correct under the assumption that the transformed function is a function of x, not of x₀.

[edit] Other conventions

There are three common conventions for defining the Fourier transform. The Fourier transform is often written in terms of angular frequency: ω = 2πξ whose units are radians per second.

The substitution ξ = ω/(2π) into the formulas above produces this convention:

$\hat{f}(\omega) = \int_{\mathbb{R}^n} f(x) e^{- i\omega\cdot x}\,dx$

Under this convention, the inverse transform becomes:

$f(x) = \frac{1}{(2\pi)^n} \int_{\mathbb{R}^n} \hat{f}(\omega)e^{ i\omega \cdot x}\,d\omega.$

Unlike the convention followed in this article, when the Fourier transform is defined this way it no longer a unitary transformation on L²(Rⁿ). There is also less symmetry between the formulas for the Fourier transform and its inverse.

Another popular convention is to split the factor of (2π)ⁿ evenly between the Fourier transform and its inverse, which leads to definitions:

$\hat{f}(\omega) = \frac{1}{(2\pi)^{n/2}} \int_{\mathbb{R}^n} f(x) e^{- i\omega\cdot x}\,dx$

$f(x) = \frac{1}{(2\pi)^{n/2}} \int_{\mathbb{R}^n} \hat{f}(\omega) e^{ i\omega \cdot x}\,d\omega.$

Under this convention the Fourier transform is again a unitary transformation on L²(Rⁿ). It also restores the symmetry between the Fourier transform and its inverse.

Variations of all three conventions can be created by conjugating the complex-exponential kernel of both the forward and the reverse transform. The signs must be opposites. Other than that, the choice is (again) a matter of convention.

Summary of popular forms of the Fourier transform
ordinary frequency ξ (hertz)	unitary	$\hat{f}_1(\xi)\ \stackrel{\mathrm{def}}{=}\ \int_{\mathbb{R}^n} f(x) e^{-2 \pi i x\cdot\xi}\, dx = \hat{f}_2(2 \pi \xi)=(2 \pi)^{n/2}\hat{f}_3(2 \pi \xi)$ $f(x) = \int_{\mathbb{R}^n} \hat{f}_1(\xi) e^{2 \pi i x\cdot \xi}\, d\xi \$
angular frequency ω (rad/s)	non-unitary	$\hat{f}_2(\omega) \ \stackrel{\mathrm{def}}{=}\int_{\mathbb{R}^n} f(x) e^{-i\omega\cdot x} \, dx \ = \hat{f}_1 \left ( \frac{\omega}{2 \pi} \right ) = (2 \pi)^{n/2}\ \hat{f}_3(\omega)$ $f(x) = \frac{1}{(2 \pi)^n} \int_{\mathbb{R}^n} \hat{f}_2(\omega) e^{i \omega\cdot x} \, d \omega \$
angular frequency ω (rad/s)	unitary	$\hat{f}_3(\omega) \ \stackrel{\mathrm{def}}{=}\ \frac{1}{(2 \pi)^{n/2}} \int_{\mathbb{R}^n} f(x) \ e^{-i \omega\cdot x}\, dx = \frac{1}{(2 \pi)^{n/2}} \hat{f}_1\left(\frac{\omega}{2 \pi} \right) = \frac{1}{(2 \pi)^{n/2}} \hat{f}_2(\omega)$ $f(x) = \frac{1}{(2 \pi)^{n/2}} \int_{\mathbb{R}^n} \hat{f}_3(\omega)e^{i \omega\cdot x}\, d \omega \$

[edit] Tables of important Fourier transforms

The following tables record some closed form Fourier transforms. For functions ƒ(x) , g(x) and h(x) denote their Fourier transforms by $\hat{f}$ , $\hat{g}$ , and $\hat{h}$ respectively. Only the three most common conventions are included.

[edit] Functional relationships

The Fourier transforms in this table may be found in (Erdélyi 1954) or the appendix of (Kammler 2000)

	Function	Fourier transform unitary, ordinary frequency	Fourier transform unitary, angular frequency	Fourier transform non-unitary, angular frequency	Remarks
	$f(x)\,$	$\hat{f}(\xi)=$ $\int_{-\infty}^{\infty}f(x) e^{-2\pi i x\xi}\, dx$	$\hat{f}(\omega)=$ $\frac{1}{\sqrt{2 \pi}} \int_{-\infty}^{\infty} f(x) e^{-i \omega x}\, dx$	$\hat{f}(\nu)=$ $\int_{-\infty}^{\infty}f(x) e^{-i \nu x}\, dx$
101	$a\cdot f(x) + b\cdot g(x)\,$	$a\cdot \hat{f}(\xi) + b\cdot \hat{g}(\xi)\,$	$a\cdot \hat{f}(\omega) + b\cdot \hat{g}(\omega)\,$	$a\cdot \hat{f}(\nu) + b\cdot \hat{g}(\nu)\,$	Linearity
102	$f(x - a)\,$	$e^{-2\pi i a \xi} \hat{f}(\xi)\,$	$e^{- i a \omega} \hat{f}(\omega)\,$	$e^{- i a \nu} \hat{f}(\nu)\,$	Shift in time domain
103	$e^{ 2\pi iax} f(x)\,$	$\hat{f} \left(\xi - a\right)\,$	$\hat{f}(\omega - 2\pi a)\,$	$\hat{f}(\nu - 2\pi a)\,$	Shift in frequency domain, dual of 102
104	$f(a x)\,$	$\frac{1}{\|a\|} \hat{f}\left( \frac{\xi}{a} \right)\,$	$\frac{1}{\|a\|} \hat{f}\left( \frac{\omega}{a} \right)\,$	$\frac{1}{\|a\|} \hat{f}\left( \frac{\nu}{a} \right)\,$	If $\|a\|\,$ is large, then $f(a x)\,$ is concentrated around 0 and $\frac{1}{\|a\|}\hat{f} \left( \frac{\omega}{a} \right)\,$ spreads out and flattens.
105	$\hat{f}(x)\,$	$f(-\xi)\,$	$f(-\omega)\,$	$2\pi f(-\nu)\,$	Here $\hat{f}$ needs to be calculated using the same method as Fourier transform column. Results from swapping "dummy" variables of $t \,$ and $\omega \,$ .
106	$\frac{d^n f(x)}{dx^n}\,$	$(2\pi i\xi)^n \hat{f}(\xi)\,$	$(i\omega)^n \hat{f}(\omega)\,$	$(i\nu)^n \hat{f}(\nu)\,$
107	$x^n f(x)\,$	$\left (\frac{i}{2\pi}\right)^n \frac{d^n \hat{f}(\xi)}{d\xi^n}\,$	$i^n \frac{d^n \hat{f}(\omega)}{d\omega^n}$	$i^n \frac{d^n \hat{f}(\nu)}{d\nu^n}$	This is the dual of 106
108	$(f * g)(x)\,$	$\hat{f}(\xi) \hat{g}(\xi)\,$	$\sqrt{2\pi} \hat{f}(\omega) \hat{g}(\omega)\,$	$\hat{f}(\nu) \hat{g}(\nu)\,$	The notation $f * g$ denotes the convolution of $f$ and $g$ — this rule is the convolution theorem
109	$f(x) g(x)\,$	$(\hat{f} * \hat{g})(\xi)\,$	$(\hat{f} * \hat{g})(\omega) \over \sqrt{2\pi}\,$	$\frac{1}{2\pi}(\hat{f} * \hat{g})(\nu)\,$	This is the dual of 108
110	For $f (x)$ a purely real even function	$\hat{f}(\omega)$ , $\hat{f}(\xi)$ and $\hat{f}(\nu)\,$ are purely real even functions.
111	For $f (x)$ a purely real odd function	$\hat{f}(\omega)$ , $\hat{f}(\xi)$ and $\hat{f}(\nu)$ are purely imaginary odd functions.

[edit] Square-integrable functions

The Fourier transforms in this table may be found in (Campbell & Foster 1948), (Erdélyi 1954), or the appendix of (Kammler 2000)

	Function	Fourier transform unitary, ordinary frequency	Fourier transform unitary, angular frequency	Fourier transform non-unitary, angular frequency	Remarks
	$f (x)$	$\hat{f}(\xi)=$ $\int_{-\infty}^{\infty}f(x) e^{-2\pi ix\xi}\,dx$	$\hat{f}(\omega)=$ $\frac{1}{\sqrt{2 \pi}} \int_{-\infty}^{\infty} f(x) e^{-i \omega x}\, dx$	$\hat{f}(\nu)=$ $\int_{-\infty}^{\infty} f(x) e^{-i\nu x}\, dx$
201	$\operatorname{rect}(a x) \,$	$\frac{1}{\|a\|}\cdot \operatorname{sinc}\left(\frac{\xi}{a}\right)$	$\frac{1}{\sqrt{2 \pi a^2}}\cdot \operatorname{sinc}\left(\frac{\omega}{2\pi a}\right)$	$\frac{1}{\|a\|}\cdot \operatorname{sinc}\left(\frac{\nu}{2\pi a}\right)$	The rectangular pulse and the normalized sinc function, here defined as sinc(x) = sin(πx)/(πx)
202	$\operatorname{sinc}(a x)\,$	$\frac{1}{\|a\|}\cdot \operatorname{rect}\left(\frac{\xi}{a} \right)\,$	$\frac{1}{\sqrt{2\pi a^2}}\cdot \operatorname{rect}\left(\frac{\omega}{2 \pi a}\right)$	$\frac{1}{\|a\|}\cdot \operatorname{rect}\left(\frac{\nu}{2 \pi a}\right)$	Dual of rule 201. The rectangular function is an ideal low-pass filter, and the sinc function is the non-causal impulse response of such a filter.
203	$\operatorname{sinc}^2 (a x)$	$\frac{1}{\|a\|}\cdot \operatorname{tri} \left( \frac{\xi}{a} \right)$	$\frac{1}{\sqrt{2\pi a^2}}\cdot \operatorname{tri} \left( \frac{\omega}{2\pi a} \right)$	$\frac{1}{\|a\|}\cdot \operatorname{tri} \left( \frac{\nu}{2\pi a} \right)$	The function tri(x) is the triangular function
204	$\operatorname{tri} (a x)$	$\frac{1}{\|a\|}\cdot \operatorname{sinc}^2 \left( \frac{\xi}{a} \right) \,$	$\frac{1}{\sqrt{2\pi a^2}} \cdot \operatorname{sinc}^2 \left( \frac{\omega}{2\pi a} \right)$	$\frac{1}{\|a\|} \cdot \operatorname{sinc}^2 \left( \frac{\nu}{2\pi a} \right)$	Dual of rule 203.
205	$e^{- a x} u(x) \,$	$\frac{1}{a + 2 \pi i \xi}$	$\frac{1}{\sqrt{2 \pi} (a + i \omega)}$	$\frac{1}{a + i \nu}$	The function u(x) is the Heaviside unit step function and a>0.
206	$e^{-\alpha x^2}\,$	$\sqrt{\frac{\pi}{\alpha}}\cdot e^{-\frac{(\pi \xi)^2}{\alpha}}$	$\frac{1}{\sqrt{2 \alpha}}\cdot e^{-\frac{\omega^2}{4 \alpha}}$	$\sqrt{\frac{\pi}{\alpha}}\cdot e^{-\frac{\nu^2}{4 \alpha}}$	This shows that, for the unitary Fourier transforms, the Gaussian function exp(−αx²) is its own Fourier transform for some choice of α. For this to be integrable we must have Re(α)>0.
207	$\operatorname{e}^{-a\|x\|} \,$	$\frac{2 a}{a^2 + 4 \pi^2 \xi^2}$	$\sqrt{\frac{2}{\pi}} \cdot \frac{a}{a^2 + \omega^2}$	$\frac{2a}{a^2 + \nu^2}$	For a>0.
208	$\frac{J_n (x)}{x} \,$	$\frac{2 i}{n} (-i)^n \cdot U_{n-1} (2 \pi \xi)\,$ $\cdot \ \sqrt{1 - 4 \pi^2 \xi^2} \operatorname{rect}( \pi \xi )$	$\sqrt{\frac{2}{\pi}} \frac{i}{n} (-i)^n \cdot U_{n-1} (\omega)\,$ $\cdot \ \sqrt{1 - \omega^2} \operatorname{rect} \left( \frac{\omega}{2} \right)$	$\frac{2 i}{n} (-i)^n \cdot U_{n-1} (\nu)\,$ $\cdot \ \sqrt{1 - \nu^2} \operatorname{rect} \left( \frac{\nu}{2} \right)$	The functions J_n (x) are the n-th order Bessel functions of the first kind. The functions U_n (x) are the Chebyshev polynomial of the second kind. See 315 and 316 below.
209	$\operatorname{sech}(a x) \,$	$\frac{\pi}{a} \operatorname{sech} \left( \frac{\pi^2}{ a} \xi \right)$	$\frac{1}{a}\sqrt{\frac{\pi}{2}}\operatorname{sech}\left( \frac{\pi}{2 a} \omega \right)$	$\frac{\pi}{a}\operatorname{sech}\left( \frac{\pi}{2 a} \nu \right)$	Hyperbolic secant is its own Fourier transform

[edit] Distributions