Fourier transform
A Fourier transform (FT) is a mathematical transform that decomposes functions depending on space or time into functions depending on spatial frequency or temporal frequency. That process is also called analysis. An example application would be decomposing the waveform of a musical chord into terms of the intensity of its constituent pitches. The term Fourier transform refers to both the frequency domain representation and the mathematical operation that associates the frequency domain representation to a function of space or time.
The Fourier transform of a function is a complexvalued function representing the complex sinusoids that comprise the original function. For each frequency, the magnitude (absolute value) of the complex value represents the amplitude of a constituent complex sinusoid with that frequency, and the argument of the complex value represents that complex sinusoid's phase offset. If a frequency is not present, the transform has a value of 0 for that frequency. The Fourier transform is not limited to functions of time, but the domain of the original function is commonly referred to as the time domain. The Fourier inversion theorem provides a synthesis process that recreates the original function from its frequency domain representation.
Functions that are localized in the time domain have Fourier transforms that are spread out across the frequency domain and vice versa, a phenomenon known as the uncertainty principle. The critical case for this principle is the Gaussian function, of substantial importance in probability theory and statistics as well as in the study of physical phenomena exhibiting normal distribution (e.g., diffusion). The Fourier transform of a Gaussian function is another Gaussian function. Joseph Fourier introduced the transform in his study of heat transfer, where Gaussian functions appear as solutions of the heat equation.
The Fourier transform can be formally defined as an improper Riemann integral, making it an integral transform, although this definition is not suitable for many applications requiring a more sophisticated integration theory.^{[note 1]} For example, many relatively simple applications use the Dirac delta function, which can be treated formally as if it were a function, but the justification requires a mathematically more sophisticated viewpoint.^{[note 2]}
The Fourier transform can also be generalized to functions of several variables on Euclidean space, sending a function of 3dimensional 'position space' to a function of 3dimensional momentum (or a function of space and time to a function of 4momentum). This idea makes the spatial Fourier transform very natural in the study of waves, as well as in quantum mechanics, where it is important to be able to represent wave solutions as functions of either position or momentum and sometimes both. In general, functions to which Fourier methods are applicable are complexvalued, and possibly vectorvalued.^{[note 3]} Still further generalization is possible to functions on groups, which, besides the original Fourier transform on R or R^{n} (viewed as groups under addition), notably includes the discretetime Fourier transform (DTFT, group = Z), the discrete Fourier transform (DFT, group = Z mod N) and the Fourier series or circular Fourier transform (group = S^{1}, the unit circle ≈ closed finite interval with endpoints identified). The latter is routinely employed to handle periodic functions. The fast Fourier transform (FFT) is an algorithm for computing the DFT.
Definition
There are several common conventions for defining the Fourier transform of an integrable function [math]\displaystyle{ f: \mathbb{R} \to \mathbb{C} }[/math].^{[1]}^{[2]} One of them is:
[math]\displaystyle{ \hat{f}(\xi) = \int_{\infty}^{\infty} f(x)\ e^{i 2\pi \xi x}\,dx,\quad \forall\ \xi \in \mathbb R. }[/math] 

( ) 
The transform of function [math]\displaystyle{ f(x) }[/math] at frequency [math]\displaystyle{ \xi }[/math] is given by the complex number [math]\displaystyle{ \hat{f}(\xi) }[/math]. Evaluating Eq.1 for all values of [math]\displaystyle{ \xi }[/math] produces the frequencydomain function. The Fourier transform is denoted here by adding a circumflex to the symbol of the function. When the independent variable represents time (often denoted by [math]\displaystyle{ t }[/math] instead of [math]\displaystyle{ x }[/math]), the transform variable represents frequency (often denoted by [math]\displaystyle{ f }[/math] instead of [math]\displaystyle{ \xi }[/math]). For example, if time is measured in seconds, then frequency is in hertz.
For realvalued [math]\displaystyle{ f(x), }[/math] Eq.1 has the symmetry property [math]\displaystyle{ \hat f(\xi) = \hat f^*(\xi), }[/math] where [math]\displaystyle{ \hat f^*(\xi) }[/math] is the complex conjugate of [math]\displaystyle{ \hat f(\xi) }[/math]. The Fourier transform can therefore be reduced to:
[math]\displaystyle{ \hat f(\xi) = \left\{ \begin{align} &\int_{\infty}^{\infty} f(x)\ e^{i 2\pi \xi x}\,dx,\ &\xi \ge 0\\ &\hat f^*(\xi)&\xi \lt 0\\ \end{align} \right., }[/math]
which means that negative values of the frequency, [math]\displaystyle{ \xi, }[/math] are unnecessary in this context.
Under suitable conditions [math]\displaystyle{ f }[/math] can be represented as a recombination of complex exponentials of all possible frequencies:
[math]\displaystyle{ f(x) = \int_{\infty}^{\infty} \hat f(\xi)\ e^{i 2 \pi \xi x}\,d\xi,\quad \forall\ x \in \mathbb R, }[/math] 

( ) 
which, for realvalued [math]\displaystyle{ f(x), }[/math] reduces to:
[math]\displaystyle{ \begin{align} f(x) &= 2 \int_{0}^{\infty}\operatorname{Re} \left(\hat {f}(\xi)\cdot e^{i 2\pi \xi x}\right)d\xi\\ &=2 \int_{0}^{\infty} \left( \operatorname{Re}(\hat {f}(\xi))\cdot\cos(2\pi \xi x) \operatorname{Im}(\hat {f}(\xi))\cdot\sin(2\pi \xi x) \right)d\xi. \end{align} }[/math]
The complex number, [math]\displaystyle{ \hat{f}(\xi) }[/math], conveys both amplitude and phase of frequency [math]\displaystyle{ \xi }[/math]. Eq.2 is known as the Fourier inversion theorem, and was first introduced in Fourier's Analytical Theory of Heat,^{[3]}^{[4]} although a proof by modern standards was not given until much later.^{[5]}^{[6]} The functions [math]\displaystyle{ f }[/math] and [math]\displaystyle{ \hat{f} }[/math] are often referred to as a Fourier integral pair or Fourier transform pair.^{[7]} A common notation for designating transform pairs is:^{[8]}
 [math]\displaystyle{ f(x)\ \stackrel{\mathcal{F}}{\longleftrightarrow}\ \hat f(\xi) }[/math].
For other common conventions and notations, including using the angular frequency ω instead of the ordinary frequency ξ, see Other conventions and Other notations below. The Fourier transform on Euclidean space is treated separately, in which the variable x often represents position and ξ momentum. The conventions chosen in this article are those of harmonic analysis, and are characterized as the unique conventions such that the Fourier transform is both unitary on L^{2} and an algebra homomorphism from L^{1} to L^{∞}, without renormalizing the Lebesgue measure.^{[9]}
Many other characterizations of the Fourier transform exist. For example, one uses the Stone–von Neumann theorem: the Fourier transform is the unique unitary intertwiner for the symplectic and Euclidean Schrödinger representations of the Heisenberg group.
History
In 1822, Fourier claimed (see Joseph Fourier § The Analytic Theory of Heat) that any function, whether continuous or discontinuous, can be expanded into a series of sines.^{[10]} That important work was corrected and expanded upon by others to provide the foundation for the various forms of the Fourier transform used since.
Introduction
Although Fourier series can represent periodic waveforms as the sum of harmonicallyrelated sinusoids, Fourier series can't represent nonperiodic waveforms. However, the Fourier transform is able to represent nonperiodic waveforms as well. It achieves this by applying a limiting process to lengthen the period of any waveform to infinity and then treating that as a periodic waveform.^{[11]}
In the study of Fourier series, the Fourier coefficients represent the amplitude of each harmonicallyrelated sinusoid present in the Fourier series of a periodic function f. Similarly, the Fourier transform represents the amplitude and phase of every sinusoid present in a (possibly nonperiodic) function f.
The Fourier transform uses an integral (or "continuous sum") that exploits properties of sine and cosine to recover the amplitude and phase of each sinusoid in a Fourier series. The inverse Fourier transform recombines these waves using a similar integral to reproduce the original function.
Use of complex sinusoids to represent real sinusoids
To simplify the math, it is desirable to write the Fourier series as a sum of complex exponentials (see Fourier series § Exponential form). Each complex exponential or complex sinusoid of frequency ξ can be expressed using Euler's formula as the sum of a cosine wave of frequency ξ for the real component plus a sine wave also of frequency ξ for the imaginary component:
 [math]\displaystyle{ \begin{align} e^{2\pi i \xi x} &= \cos(2\pi \xi x) + i \sin(2\pi \xi x) \end{align} }[/math]
Expressing real sinusoids as complex sinusoids makes it necessary for the Fourier coefficients [math]\displaystyle{ c_n }[/math]to be complex valued, but has the benefit of compactly representing all necessary information about each frequency. The usual interpretation of this complex number is that [math]\displaystyle{ \left\vert c_n \right\vert }[/math] (its magnitude) gives the amplitude and [math]\displaystyle{ \arg (c_n) }[/math] (its argument) gives the phase of the complex sinusoid for that coefficient.
These complex exponentials may have negative frequency. For example, both complex sinusoids e^{2πiξx} and e^{−2πiξx} complete one cycle per unit of x, but the first represents a positive frequency while the second represents a negative frequency. Positive frequency can be understood as rotating counterclockwise about the complex plane while negative frequency can be understood as rotating clockwise about the complex plane. When complex sinusoids are interpreted as a helix in threedimensions (with the third dimension being the imaginary component), negating the frequency simply changes the handedness of the helix.^{[12]}
Real sine and cosine waves can be recovered from the complex exponential representation of sinusoids. For example, a corollary to Euler's formula allows expressing cosine and sine waves as either the real or imaginary part of a complex sinusoid or as a weighted sum of two complex sinusoids of opposite frequency:
 [math]\displaystyle{ \begin{align} \cos(2\pi \xi x) &= \operatorname{Re} \left(e^{2\pi i \xi x}\right) =\tfrac{1}{2} e^{2\pi i \xi x} + \tfrac{1}{2} e^{2\pi i \xi x}, \\ \sin(2\pi \xi x) &= \operatorname{Im} \left(e^{2\pi i \xi x}\right) =\tfrac{1}{2i} e^{2\pi i \xi x}  \tfrac{1}{2i} e^{2\pi i \xi x}. \end{align} }[/math]
Consequently, a general form of any real sinusoid (with frequency ξ, phase shift θ, and amplitude A) can be expressed as the sum of two complex sinusoids of opposite frequency (ξ and ξ) but equal magnitude (A/2) and with the phase shift θ embedded in both their complex coefficients:
 [math]\displaystyle{ \begin{align} A \cos(2\pi \xi x + \theta) &= \tfrac{A}{2} e^{2\pi i \xi x + i \theta} + \tfrac{A}{2} e^{2\pi i \xi x  i \theta} = \tfrac{A e^{i \theta}}{2} e^{2\pi i \xi x} + \tfrac{A e^{i \theta}}{2} e^{2\pi i \xi x} . \end{align} }[/math]
Hence, every real sinusoid (and real signal) can be considered to consist of a positive and negative frequency, whose imaginary components cancel but whose real components contribute equally to form the real signal.
To avoid the use of complex numbers and negative frequencies, the sine and cosine transforms together can be used as an equivalent alternative form of the Fourier transform.
Fourier transform for functions that are zero outside an interval
There is a close connection between the definition of Fourier series and the Fourier transform for functions f that are zero outside an interval. For such a function, we can calculate its Fourier series on any interval that includes the points where f is not zero. The Fourier transform is also defined for such a function. As we increase the length of the interval in which we calculate the Fourier series, then the Fourier series coefficients begin to resemble the Fourier transform and the sum of the Fourier series of f begins to resemble the inverse Fourier transform. More precisely, suppose T is large enough that the interval [−T/2, T/2] contains the interval in which f is not zero. Then, the nth series coefficient c_{n} is given by:
 [math]\displaystyle{ c_n = \frac{1}{T} \int_{\frac{T}{2}}^\frac{T}{2} f(x)\, e^{2\pi i\left(\frac{n}{T}\right) x} \, dx. }[/math]
Comparing this to the definition of the Fourier transform, it follows that:
 [math]\displaystyle{ c_n = \frac{1}{T}\hat f\left(\frac{n}{T}\right) }[/math]
since f(x) is zero outside [−T/2, T/2]. Thus, the Fourier coefficients are equal to the values of the Fourier transform sampled on a grid of width 1/T, multiplied by the grid width 1/T.
Under appropriate conditions, the Fourier series of f will equal the function f. In other words, f can be written:
 [math]\displaystyle{ f(x)=\sum_{n=\infty}^\infty c_n\, e^{2\pi i\left(\frac{n}{T}\right) x} =\sum_{n=\infty}^\infty \hat{f}(\xi_n)\ e^{2\pi i\xi_n x}\Delta\xi, }[/math]
where the last sum is simply the first sum rewritten using the definitions ξ_{n} = n/T, and Δξ = n + 1/T − n/T = 1/T.
This second sum is a Riemann sum. By letting T → ∞ it will converge to the integral for the inverse Fourier transform as expressed above. Under suitable conditions, this argument may be made precise.^{[13]}
Example
The following figures provide a visual illustration how the Fourier transform measures whether a frequency is present in a particular function. The depicted function f(t) = cos(6πt) e^{−πt2} oscillates at 3 Hz (if t measures seconds) and tends quickly to 0. (The second factor in this equation is an envelope function that shapes the continuous sinusoid into a short pulse. Its general form is a Gaussian function). This function was specially chosen to have a real Fourier transform that can be easily plotted. The first image contains its graph. In order to calculate [math]\displaystyle{ \hat{f}(3) }[/math] we must integrate e^{−2πi(3t)}f(t). The second image shows the plot of the real and imaginary parts of this function. The real part of the integrand is almost always positive, because when f(t) is negative, the real part of e^{−2πi(3t)} is negative as well. Because they oscillate at the same rate, when f(t) is positive, so is the real part of e^{−2πi(3t)}. The result is that when you integrate the real part of the integrand you get a relatively large number (in this case 1/2). On the other hand, when you try to measure a frequency that is not present, as in the case when we look at [math]\displaystyle{ \hat{f}(5) }[/math], you see that both real and imaginary component of this function vary rapidly between positive and negative values, as plotted in the third image. Therefore, in this case, the integrand oscillates fast enough so that the integral is very small and the value for the Fourier transform for that frequency is nearly zero.
The general situation may be a bit more complicated than this, but this in spirit is how the Fourier transform measures how much of an individual frequency is present in a function f(t).
Properties of the Fourier transform
Here we assume f(x), g(x) and h(x) are integrable functions: Lebesguemeasurable on the real line satisfying: [math]\displaystyle{ \int_{\infty}^\infty f(x) \, dx \lt \infty. }[/math]
We denote the Fourier transforms of these functions as f̂(ξ), ĝ(ξ) and ĥ(ξ) respectively.
Basic properties
The Fourier transform has the following basic properties:^{[14]}
Linearity
 For any complex numbers a and b, if h(x) = af (x) + bg(x), then ĥ(ξ) = a · f̂(ξ) + b · ĝ(ξ).
Translation / time shifting
 For any real number x_{0}, if h(x) = f(x − x_{0}), then ĥ(ξ) = e^{−2πix0ξ} f̂(ξ).
Modulation / frequency shifting
 For any real number ξ_{0}, if h(x) = e^{2πixξ0} f(x), then ĥ(ξ) = f̂(ξ − ξ_{0}).
Time scaling
 For a nonzero real number a, if h(x) = f(ax), then
 [math]\displaystyle{ \hat{h}(\xi)=\frac{1}{a}\hat{f}\left(\frac{\xi}{a}\right). }[/math]
 The case a = −1 leads to the timereversal property, which states: if h(x) = f(−x), then ĥ(ξ) = f̂(−ξ).
Conjugation
 If h(x) = f(x), then
 [math]\displaystyle{ \hat{h}(\xi) = \overline{\hat{f}(\xi)}. }[/math]
 In particular, if f is real, then one has the reality condition
 [math]\displaystyle{ \hat{f}(\xi)=\overline{\hat{f}(\xi)}, }[/math]
 that is, f̂ is a Hermitian function. And if f is purely imaginary, then
 [math]\displaystyle{ \hat{f}(\xi)=\hat{f}(\xi). }[/math]
Real and imaginary part in time
 If [math]\displaystyle{ h(x) = \Re{(f(x))} }[/math], then [math]\displaystyle{ \hat{h}(\xi) = \frac{1}{2}\left(\hat{f}(\xi) + \overline{\hat{f}(\xi)}\right) }[/math].
 If [math]\displaystyle{ h(x) = \Im{(f(x))} }[/math], then [math]\displaystyle{ \hat{h}(\xi) = \frac{1}{2i}\left(\hat{f}(\xi)  \overline{\hat{f}(\xi)}\right) }[/math].
The zero frequency component
 Substituting ξ = 0 in the definition, we obtain
 [math]\displaystyle{ \hat{f}(0) = \int_{\infty}^{\infty} f(x)\,dx. }[/math]
 That is the same as the integral of f over all its domain and is also known as the average value or DC bias of the function.
Invertibility and periodicity
Under suitable conditions on the function [math]\displaystyle{ f }[/math], it can be recovered from its Fourier transform [math]\displaystyle{ \hat{f} }[/math]. Indeed, denoting the Fourier transform operator by [math]\displaystyle{ \mathcal{F} }[/math], so [math]\displaystyle{ \mathcal{F} f := \hat{f} }[/math], then for suitable functions, applying the Fourier transform twice simply flips the function: [math]\displaystyle{ (\mathcal{F}^2 f)(x) = f(x) }[/math], which can be interpreted as "reversing time". Since reversing time is twoperiodic, applying this twice yields [math]\displaystyle{ \mathcal{F}^4(f) = f }[/math], so the Fourier transform operator is fourperiodic, and similarly the inverse Fourier transform can be obtained by applying the Fourier transform three times: [math]\displaystyle{ \mathcal{F}^3(\hat{f}) = f }[/math]. In particular the Fourier transform is invertible (under suitable conditions).
More precisely, defining the parity operator [math]\displaystyle{ \mathcal{P} }[/math] such that [math]\displaystyle{ (\mathcal{P} f)(x) = f(x) }[/math], we have:
 [math]\displaystyle{ \begin{align} \mathcal{F}^0 &= \mathrm{id}, \\ \mathcal{F}^1 &= \mathcal{F}, \\ \mathcal{F}^2 &= \mathcal{P}, \\ \mathcal{F}^3 &= \mathcal{F}^{1} = \mathcal{P} \circ \mathcal{F} = \mathcal{F} \circ \mathcal{P}, \\ \mathcal{F}^4 &= \mathrm{id} \end{align} }[/math]
These equalities of operators require careful definition of the space of functions in question, defining equality of functions (equality at every point? equality almost everywhere?) and defining equality of operators – that is, defining the topology on the function space and operator space in question. These are not true for all functions, but are true under various conditions, which are the content of the various forms of the Fourier inversion theorem.
This fourfold periodicity of the Fourier transform is similar to a rotation of the plane by 90°, particularly as the twofold iteration yields a reversal, and in fact this analogy can be made precise. While the Fourier transform can simply be interpreted as switching the time domain and the frequency domain, with the inverse Fourier transform switching them back, more geometrically it can be interpreted as a rotation by 90° in the time–frequency domain (considering time as the xaxis and frequency as the yaxis), and the Fourier transform can be generalized to the fractional Fourier transform, which involves rotations by other angles. This can be further generalized to linear canonical transformations, which can be visualized as the action of the special linear group SL_{2}(R) on the time–frequency plane, with the preserved symplectic form corresponding to the uncertainty principle, below. This approach is particularly studied in signal processing, under time–frequency analysis.
Units and duality
The frequency variable must have inverse units to the units of the original function's domain (typically named t or x). For example, if t is measured in seconds, ξ should be in cycles per second. If the scale of time is in units of 2π seconds, then another greek letter ω typically is used instead to represent angular frequency (where ω = 2πξ) in units of radians per second. If using x for units of length, then ξ must be in inverse length, e.g., wavenumbers. That is to say, there are two versions of the real line: one which is the range of t and measured in units of t, and the other which is the range of ξ and measured in inverse units to the units of t. These two distinct versions of the real line cannot be equated with each other. Therefore, the Fourier transform goes from one space of functions to a different space of functions: functions which have a different domain of definition.
In general, ξ must always be taken to be a linear form on the space of its domain, which is to say that the second real line is the dual space of the first real line. See the article on linear algebra for a more formal explanation and for more details. This point of view becomes essential in generalisations of the Fourier transform to general symmetry groups, including the case of Fourier series.
That there is no one preferred way (often, one says "no canonical way") to compare the two versions of the real line which are involved in the Fourier transform—fixing the units on one line does not force the scale of the units on the other line—is the reason for the plethora of rival conventions on the definition of the Fourier transform. The various definitions resulting from different choices of units differ by various constants.
Let [math]\displaystyle{ \hat f_1(\xi) }[/math] be the form of the Fourier transform in terms of ordinary frequency ξ.
Because [math]\displaystyle{ \xi = \tfrac{\omega}{2 \pi} }[/math], the alternative form [math]\displaystyle{ \hat f_3(\omega) }[/math] (which Fourier transform § Other conventions calls the nonunitary form in angular frequency) has no factor in its definition
 [math]\displaystyle{ \begin{align} \hat{f}_3(\omega) \ &\stackrel{\mathrm{def}}{=}\ \int_{\infty}^{\infty} f(x)\cdot e^{i\omega\cdot x}\, dx = \hat{f}_1 \left(\frac{\omega}{2 \pi}\right) \end{align} }[/math]
but has a factor of [math]\displaystyle{ \tfrac{1}{2 \pi} }[/math] in its corresponding inversion formula
 [math]\displaystyle{ \begin{align} f(x) &= \frac{1}{2 \pi} \int_{\infty}^{\infty} \hat{f}_3(\omega)\cdot e^{i \omega\cdot x}\, d\omega . \end{align} }[/math]
An alternative form [math]\displaystyle{ \hat f_2(\omega) }[/math] (which Fourier transform § Other conventions calls the unitary form in angular frequency) has a factor of [math]\displaystyle{ \tfrac{1}{\sqrt{2 \pi}} }[/math] in its definition
 [math]\displaystyle{ \begin{align} \hat{f}_2(\omega)\ &\stackrel{\mathrm{def}}{=}\ \frac{1}{\sqrt{2 \pi}} \int_{\infty}^{\infty} f(x)\cdot e^{i \omega\cdot x}\, dx \end{align} }[/math]
and also has that same factor of [math]\displaystyle{ \tfrac{1}{\sqrt{2 \pi}} }[/math] in its corresponding inversion formula, producing a symmetrical relationship
 [math]\displaystyle{ \begin{align} f(x) &= \frac{1}{\sqrt{2 \pi}} \int_{\infty}^{\infty} \hat{f}_2(\omega)\cdot e^{i \omega\cdot x}\, d\omega . \end{align} }[/math]
In other conventions, the Fourier transform has i in the exponent instead of −i, and vice versa for the inversion formula. Effectively that defines [math]\displaystyle{ e^{i 2\pi \xi x}, \xi \gt 0 }[/math] as a negative frequency, because the corresponding spectral component is [math]\displaystyle{ \hat f(\xi). }[/math] But many of the identities involving the Fourier transform remain valid in those conventions, provided all terms that explicitly involve i have it replaced by −i. To add further confusion, be aware that since electrical engineers use the letter i to represent current, their form of the transform typically uses the letter j for the imaginary unit instead of i.
When using dimensionless units, the constant factors might not even be written in the transform definition. For instance, in probability theory, the characteristic function Φ of the probability density function f of a random variable X of continuous type is defined without a negative sign in the exponential, and since the units of x are ignored, there is no 2π either:
 [math]\displaystyle{ \phi (\lambda) = \int_{\infty}^\infty f(x) e^{i\lambda x} \,dx. }[/math]
(In probability theory, and in mathematical statistics, the use of the Fourier—Stieltjes transform is preferred, because so many random variables are not of continuous type, and do not possess a density function, and one must treat not functions but distributions, i.e., measures which possess "atoms".)
From the higher point of view of group characters, which is much more abstract, all these arbitrary choices disappear, as will be explained in the later section of this article, which treats the notion of the Fourier transform of a function on a locally compact Abelian group.
Uniform continuity and the Riemann–Lebesgue lemma
The Fourier transform may be defined in some cases for nonintegrable functions, but the Fourier transforms of integrable functions have several strong properties.
The Fourier transform f̂ of any integrable function f is uniformly continuous and^{[15]}
 [math]\displaystyle{ \left\\hat{f}\right\_\infty \leq \left\f\right\_1 }[/math]
By the Riemann–Lebesgue lemma,^{[16]}
 [math]\displaystyle{ \hat{f}(\xi) \to 0\text{ as }\xi \to \infty. }[/math]
However, [math]\displaystyle{ \hat{f} }[/math] need not be integrable. For example, the Fourier transform of the rectangular function, which is integrable, is the sinc function, which is not Lebesgue integrable, because its improper integrals behave analogously to the alternating harmonic series, in converging to a sum without being absolutely convergent.
It is not generally possible to write the inverse transform as a Lebesgue integral. However, when both f and [math]\displaystyle{ \hat{f} }[/math] are integrable, the inverse equality
 [math]\displaystyle{ f(x) = \int_{\infty}^\infty \hat f(\xi) e^{2 i \pi x \xi} \, d\xi }[/math]
holds almost everywhere. That is, the Fourier transform is injective on L^{1}(R). (But if f is continuous, then equality holds for every x.)
Plancherel theorem and Parseval's theorem
Let f(x) and g(x) be integrable, and let f̂(ξ) and ĝ(ξ) be their Fourier transforms. If f(x) and g(x) are also squareintegrable, then the Parseval formula follows:^{[17]}
 [math]\displaystyle{ \langle f, g\rangle_{L^{2}} = \int_{\infty}^{\infty} f(x) \overline{g(x)} \,dx = \int_{\infty}^\infty \hat{f}(\xi) \overline{\hat{g}(\xi)} \,d\xi, }[/math]
where the bar denotes complex conjugation.
The Plancherel theorem, which follows from the above, states that^{[18]}
 [math]\displaystyle{ \f\_{L^{2}} = \int_{\infty}^\infty \left f(x) \right^2\,dx = \int_{\infty}^\infty \left \hat{f}(\xi) \right^2\,d\xi. }[/math]
Plancherel's theorem makes it possible to extend the Fourier transform, by a continuity argument, to a unitary operator on L^{2}(R). On L^{1}(R) ∩ L^{2}(R), this extension agrees with original Fourier transform defined on L^{1}(R), thus enlarging the domain of the Fourier transform to L^{1}(R) + L^{2}(R) (and consequently to L^{p}(R) for 1 ≤ p ≤ 2). Plancherel's theorem has the interpretation in the sciences that the Fourier transform preserves the energy of the original quantity. The terminology of these formulas is not quite standardised. Parseval's theorem was proved only for Fourier series, and was first proved by Lyapunov. But Parseval's formula makes sense for the Fourier transform as well, and so even though in the context of the Fourier transform it was proved by Plancherel, it is still often referred to as Parseval's formula, or Parseval's relation, or even Parseval's theorem.
See Pontryagin duality for a general formulation of this concept in the context of locally compact abelian groups.
Poisson summation formula
The Poisson summation formula (PSF) is an equation that relates the Fourier series coefficients of the periodic summation of a function to values of the function's continuous Fourier transform. The Poisson summation formula says that for sufficiently regular functions f,
 [math]\displaystyle{ \sum_n \hat f(n) = \sum_n f (n). }[/math]
It has a variety of useful forms that are derived from the basic one by application of the Fourier transform's scaling and timeshifting properties. The formula has applications in engineering, physics, and number theory. The frequencydomain dual of the standard Poisson summation formula is also called the discretetime Fourier transform.
Poisson summation is generally associated with the physics of periodic media, such as heat conduction on a circle. The fundamental solution of the heat equation on a circle is called a theta function. It is used in number theory to prove the transformation properties of theta functions, which turn out to be a type of modular form, and it is connected more generally to the theory of automorphic forms where it appears on one side of the Selberg trace formula.
Differentiation
Suppose f(x) is an absolutely continuous differentiable function, and both f and its derivative f′ are integrable. Then the Fourier transform of the derivative is given by
 [math]\displaystyle{ \widehat{f'\,}(\xi) = \mathcal{F}\left\{ \frac{d}{dx} f(x)\right\} = 2\pi i\xi\hat{f}(\xi). }[/math]
More generally, the Fourier transformation of the nth derivative f^{(n)} is given by
 [math]\displaystyle{ \widehat{f^{(n)}}(\xi) = \mathcal{F}\left\{ \frac{d^n}{dx^n} f(x) \right\} = (2\pi i\xi)^n\hat{f}(\xi). }[/math]
By applying the Fourier transform and using these formulas, some ordinary differential equations can be transformed into algebraic equations, which are much easier to solve. These formulas also give rise to the rule of thumb "f(x) is smooth if and only if f̂(ξ) quickly falls to 0 for ξ → ∞." By using the analogous rules for the inverse Fourier transform, one can also say "f(x) quickly falls to 0 for x → ∞ if and only if f̂(ξ) is smooth."
Convolution theorem
The Fourier transform translates between convolution and multiplication of functions. If f(x) and g(x) are integrable functions with Fourier transforms f̂(ξ) and ĝ(ξ) respectively, then the Fourier transform of the convolution is given by the product of the Fourier transforms f̂(ξ) and ĝ(ξ) (under other conventions for the definition of the Fourier transform a constant factor may appear).
This means that if:
 [math]\displaystyle{ h(x) = (f*g)(x) = \int_{\infty}^\infty f(y)g(x  y)\,dy, }[/math]
where ∗ denotes the convolution operation, then:
 [math]\displaystyle{ \hat{h}(\xi) = \hat{f}(\xi)\cdot \hat{g}(\xi). }[/math]
In linear time invariant (LTI) system theory, it is common to interpret g(x) as the impulse response of an LTI system with input f(x) and output h(x), since substituting the unit impulse for f(x) yields h(x) = g(x). In this case, ĝ(ξ) represents the frequency response of the system.
Conversely, if f(x) can be decomposed as the product of two square integrable functions p(x) and q(x), then the Fourier transform of f(x) is given by the convolution of the respective Fourier transforms p̂(ξ) and q̂(ξ).
Crosscorrelation theorem
In an analogous manner, it can be shown that if h(x) is the crosscorrelation of f(x) and g(x):
 [math]\displaystyle{ h(x) = (f \star g)(x) = \int_{\infty}^\infty \overline{f(y)}g(x + y)\,dy }[/math]
then the Fourier transform of h(x) is:
 [math]\displaystyle{ \hat{h}(\xi) = \overline{\hat{f}(\xi)} \cdot \hat{g}(\xi). }[/math]
As a special case, the autocorrelation of function f(x) is:
 [math]\displaystyle{ h(x) = (f \star f)(x) = \int_{\infty}^\infty \overline{f(y)}f(x + y)\,dy }[/math]
for which
 [math]\displaystyle{ \hat{h}(\xi) = \overline{\hat{f}(\xi)}\hat{f}(\xi) = \left\hat{f}(\xi)\right^2. }[/math]
Eigenfunctions
One important choice of an orthonormal basis for L^{2}(R) is given by the Hermite functions
 [math]\displaystyle{ \psi_n(x) = \frac{\sqrt[4]{2}}{\sqrt{n!}} e^{\pi x^2}\mathrm{He}_n\left(2x\sqrt{\pi}\right), }[/math]
where He_{n}(x) are the "probabilist's" Hermite polynomials, defined as
 [math]\displaystyle{ \mathrm{He}_n(x) = (1)^n e^{\frac{x^2}{2}}\left(\frac{d}{dx}\right)^n e^{\frac{x^2}{2}} }[/math]
Under this convention for the Fourier transform, we have that
 [math]\displaystyle{ \hat\psi_n(\xi) = (i)^n \psi_n(\xi) }[/math].
In other words, the Hermite functions form a complete orthonormal system of eigenfunctions for the Fourier transform on L^{2}(R).^{[14]} 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 L^{2}(R) as a direct sum of four spaces H_{0}, H_{1}, H_{2}, and H_{3} where the Fourier transform acts on He_{k} simply by multiplication by i^{k}.
Since the complete set of Hermite functions provides a resolution of the identity, the Fourier transform can be represented by such a sum of terms weighted by the above eigenvalues, and these sums can be explicitly summed. This approach to define the Fourier transform was first done by Norbert Wiener.^{[19]} Among other properties, Hermite functions decrease exponentially fast in both frequency and time domains, and they are thus used to define a generalization of the Fourier transform, namely the fractional Fourier transform used in time–frequency analysis.^{[20]} In physics, this transform was introduced by Edward Condon.^{[21]}
Connection with the Heisenberg group
The Heisenberg group is a certain group of unitary operators on the Hilbert space L^{2}(R) of square integrable complex valued functions f on the real line, generated by the translations (T_{y} f)(x) = f (x + y) and multiplication by e^{2πixξ}, (M_{ξ} f)(x) = e^{2πixξ} f (x). These operators do not commute, as their (group) commutator is
 [math]\displaystyle{ \left(M^{1}_\xi T^{1}_yM_\xi T_yf\right)(x) = e^{2\pi i y\xi}f(x) }[/math]
which is multiplication by the constant (independent of x) e^{2πiyξ} ∈ U(1) (the circle group of unit modulus complex numbers). As an abstract group, the Heisenberg group is the threedimensional Lie group of triples (x, ξ, z) ∈ R^{2} × U(1), with the group law
 [math]\displaystyle{ \left(x_1, \xi_1, t_1\right) \cdot \left(x_2, \xi_2, t_2\right) = \left(x_1 + x_2, \xi_1 + \xi_2, t_1 t_2 e^{2\pi i \left(x_1\xi_1 + x_2\xi_2 + x_1\xi_2\right)}\right). }[/math]
Denote the Heisenberg group by H_{1}. The above procedure describes not only the group structure, but also a standard unitary representation of H_{1} on a Hilbert space, which we denote by ρ : H_{1} → B(L^{2}(R)). Define the linear automorphism of R^{2} by
 [math]\displaystyle{ J \begin{pmatrix} x \\ \xi \end{pmatrix} = \begin{pmatrix} \xi \\ x \end{pmatrix} }[/math]
so that J^{2} = −I. This J can be extended to a unique automorphism of H_{1}:
 [math]\displaystyle{ j\left(x, \xi, t\right) = \left(\xi, x, te^{2\pi i x\xi}\right). }[/math]
According to the Stone–von Neumann theorem, the unitary representations ρ and ρ ∘ j are unitarily equivalent, so there is a unique intertwiner W ∈ U(L^{2}(R)) such that
 [math]\displaystyle{ \rho \circ j = W \rho W^*. }[/math]
This operator W is the Fourier transform.
Many of the standard properties of the Fourier transform are immediate consequences of this more general framework.^{[22]} For example, the square of the Fourier transform, W^{2}, is an intertwiner associated with J^{2} = −I, and so we have (W^{2}f)(x) = f (−x) is the reflection of the original function f.
Complex domain
The integral for the Fourier transform
 [math]\displaystyle{ \hat f (\xi) = \int _{\infty}^\infty e^{2\pi i \xi t} f(t) \, dt }[/math]
can be studied for complex values of its argument ξ. Depending on the properties of f, this might not converge off the real axis at all, or it might converge to a complex analytic function for all values of ξ = σ + iτ, or something in between.^{[23]}
The Paley–Wiener theorem says that f is smooth (i.e., ntimes differentiable for all positive integers n) and compactly supported if and only if f̂ (σ + iτ) is a holomorphic function for which there exists a constant a > 0 such that for any integer n ≥ 0,
 [math]\displaystyle{ \left\vert \xi ^n \hat f(\xi) \right\vert \leq C e^{a\vert\tau\vert} }[/math]
for some constant C. (In this case, f is supported on [−a, a].) This can be expressed by saying that f̂ is an entire function which is rapidly decreasing in σ (for fixed τ) and of exponential growth in τ (uniformly in σ).^{[24]}
(If f is not smooth, but only L^{2}, the statement still holds provided n = 0.^{[25]}) The space of such functions of a complex variable is called the Paley—Wiener space. This theorem has been generalised to semisimple Lie groups.^{[26]}
If f is supported on the halfline t ≥ 0, then f is said to be "causal" because the impulse response function of a physically realisable filter must have this property, as no effect can precede its cause. Paley and Wiener showed that then f̂ extends to a holomorphic function on the complex lower halfplane τ < 0 which tends to zero as τ goes to infinity.^{[27]} The converse is false and it is not known how to characterise the Fourier transform of a causal function.^{[28]}
Laplace transform
The Fourier transform f̂(ξ) is related to the Laplace transform F(s), which is also used for the solution of differential equations and the analysis of filters.
It may happen that a function f for which the Fourier integral does not converge on the real axis at all, nevertheless has a complex Fourier transform defined in some region of the complex plane.
For example, if f(t) is of exponential growth, i.e.,
 [math]\displaystyle{ \vert f(t) \vert \lt C e^{a\vert t\vert} }[/math]
for some constants C, a ≥ 0, then^{[29]}
 [math]\displaystyle{ \hat f (i\tau) = \int _{\infty}^\infty e^{ 2\pi \tau t} f(t) \, dt, }[/math]
convergent for all 2πτ < −a, is the twosided Laplace transform of f.
The more usual version ("onesided") of the Laplace transform is
 [math]\displaystyle{ F(s) = \int_0^\infty f(t) e^{st} \, dt. }[/math]
If f is also causal, and analytical, then: [math]\displaystyle{ \hat f(i\tau) = F(2\pi\tau). }[/math] Thus, extending the Fourier transform to the complex domain means it includes the Laplace transform as a special case in the case of causal functions—but with the change of variable s = 2πiξ.
From another, perhaps more classical viewpoint, the Laplace transform by its form involves an additional exponential regulating term which lets it converge outside of the imaginary line where the Fourier transform is defined. As such it can converge for at most exponentially divergent series and integrals, whereas the original Fourier decomposition cannot, enabling analysis of systems with divergent or critical elements. Two particular examples from linear signal processing are the construction of allpass filter networks from critical comb and mitigating filters via exact polezero cancellation on the unit circle. Such designs are common in audio processing, where highly nonlinear phase response is sought for, as in reverb.
Furthermore, when extended pulselike impulse responses are sought for signal processing work, the easiest way to produce them is to have one circuit which produces a divergent time response, and then to cancel its divergence through a delayed opposite and compensatory response. There, only the delay circuit inbetween admits a classical Fourier description, which is critical. Both the circuits to the side are unstable, and do not admit a convergent Fourier decomposition. However, they do admit a Laplace domain description, with identical halfplanes of convergence in the complex plane (or in the discrete case, the Zplane), wherein their effects cancel.
In modern mathematics the Laplace transform is conventionally subsumed under the aegis Fourier methods. Both of them are subsumed by the far more general, and more abstract, idea of harmonic analysis.
Inversion
If f̂ is complex analytic for a ≤ τ ≤ b, then
 [math]\displaystyle{ \int _{\infty}^\infty \hat f (\sigma + ia) e^{ 2\pi i \xi t} \, d\sigma = \int _{\infty}^\infty \hat f (\sigma + ib) e^{ 2\pi i \xi t} \, d\sigma }[/math]
by Cauchy's integral theorem. Therefore, the Fourier inversion formula can use integration along different lines, parallel to the real axis.^{[30]}
Theorem: If f(t) = 0 for t < 0, and f(t) < Ce^{at} for some constants C, a > 0, then
 [math]\displaystyle{ f(t) = \int_{\infty}^\infty \hat f(\sigma + i\tau) e^{2 \pi i\xi t} \, d\sigma, }[/math]
for any τ < −a/2π.
This theorem implies the Mellin inversion formula for the Laplace transformation,^{[29]}
 [math]\displaystyle{ f(t) = \frac 1 {2\pi i} \int_{bi\infty}^{b+i\infty} F(s) e^{st}\, ds }[/math]
for any b > a, where F(s) is the Laplace transform of f(t).
The hypotheses can be weakened, as in the results of Carleman and Hunt, to f(t) e^{−at} being L^{1}, provided that f is of bounded variation in a closed neighborhood of t (cf. DirichletDini theorem), the value of f at t is taken to be the arithmetic mean of the left and right limits, and provided that the integrals are taken in the sense of Cauchy principal values.^{[31]}
L^{2} versions of these inversion formulas are also available.^{[32]}
Fourier transform on Euclidean space
The Fourier transform can be defined in any arbitrary number of dimensions n. As with the onedimensional case, there are many conventions. For an integrable function f(x), this article takes the definition:
 [math]\displaystyle{ \hat{f}(\boldsymbol{\xi}) = \mathcal{F}(f)(\boldsymbol{\xi}) = \int_{\R^n} f(\mathbf{x}) e^{2\pi i \mathbf{x}\cdot\boldsymbol{\xi}} \, d\mathbf{x} }[/math]
where x and ξ are ndimensional vectors, and x · ξ is the dot product of the vectors. Alternatively, ξ can be viewed as belonging to the dual vector space [math]\displaystyle{ \R^{n\star} }[/math], in which case the dot product becomes the contraction of x and ξ, usually written as ⟨x, ξ⟩.
All of the basic properties listed above hold for the ndimensional Fourier transform, as do Plancherel's and Parseval's theorem. When the function is integrable, the Fourier transform is still uniformly continuous and the Riemann–Lebesgue lemma holds.^{[16]}
Uncertainty principle
Generally speaking, the more concentrated f(x) is, the more spread out its Fourier transform f̂(ξ) 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 tradeoff between the compaction of a function and its Fourier transform can be formalized in the form of an uncertainty principle by viewing a function and its Fourier transform as conjugate variables with respect to the symplectic form on the time–frequency domain: from the point of view of the linear canonical transformation, the Fourier transform is rotation by 90° in the time–frequency domain, and preserves the symplectic form.
Suppose f(x) is an integrable and squareintegrable function. Without loss of generality, assume that f(x) is normalized:
 [math]\displaystyle{ \int_{\infty}^\infty f(x)^2 \,dx=1. }[/math]
It follows from the Plancherel theorem that f̂(ξ) is also normalized.
The spread around x = 0 may be measured by the dispersion about zero^{[33]} defined by
 [math]\displaystyle{ D_0(f)=\int_{\infty}^\infty x^2f(x)^2\,dx. }[/math]
In probability terms, this is the second moment of f(x)^{2} about zero.
The uncertainty principle states that, if f(x) is absolutely continuous and the functions x·f(x) and f′(x) are square integrable, then^{[14]}
 [math]\displaystyle{ D_0(f)D_0\left(\hat{f}\right) \geq \frac{1}{16\pi^2} }[/math].
The equality is attained only in the case
 [math]\displaystyle{ \begin{align} f(x) &= C_1 \, e^{\pi \frac{x^2}{\sigma^2} }\\ \therefore \hat{f}(\xi) &= \sigma C_1 \, e^{\pi\sigma^2\xi^2} \end{align} }[/math]
where σ > 0 is arbitrary and C_{1} = ^{4}√2/√σ so that f is L^{2}normalized.^{[14]} In other words, where f is a (normalized) Gaussian function with variance σ^{2}, centered at zero, and its Fourier transform is a Gaussian function with variance σ^{−2}.
In fact, this inequality implies that:
 [math]\displaystyle{ \left(\int_{\infty}^\infty (xx_0)^2f(x)^2\,dx\right)\left(\int_{\infty}^\infty(\xi\xi_0)^2\left\hat{f}(\xi)\right^2\,d\xi\right)\geq \frac{1}{16\pi^2} }[/math]
for any x_{0}, ξ_{0} ∈ R.^{[13]}
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.^{[34]}
A stronger uncertainty principle is the Hirschman uncertainty principle, which is expressed as:
 [math]\displaystyle{ H\left(\leftf\right^2\right)+H\left(\left\hat{f}\right^2\right)\ge \log\left(\frac{e}{2}\right) }[/math]
where H(p) is the differential entropy of the probability density function p(x):
 [math]\displaystyle{ H(p) = \int_{\infty}^\infty p(x)\log\bigl(p(x)\bigr) \, dx }[/math]
where the logarithms may be in any base that is consistent. The equality is attained for a Gaussian, as in the previous case.
Sine and cosine transforms
Fourier's original formulation of the transform did not use complex numbers, but rather sines and cosines. Statisticians and others still use this form. An absolutely integrable function f for which Fourier inversion holds can be expanded in terms of genuine frequencies (avoiding negative frequencies, which are sometimes considered hard to interpret physically^{[35]}) λ by
 [math]\displaystyle{ f(t) = \int_0^\infty \bigl( a(\lambda ) \cos( 2\pi \lambda t) + b(\lambda ) \sin( 2\pi \lambda t)\bigr) \, d\lambda. }[/math]
This is called an expansion as a trigonometric integral, or a Fourier integral expansion. The coefficient functions a and b can be found by using variants of the Fourier cosine transform and the Fourier sine transform (the normalisations are, again, not standardised):
 [math]\displaystyle{ a (\lambda) = 2\int_{\infty}^\infty f(t) \cos(2\pi\lambda t) \, dt }[/math]
and
 [math]\displaystyle{ b (\lambda) = 2\int_{\infty}^\infty f(t) \sin(2\pi\lambda t) \, dt. }[/math]
Older literature refers to the two transform functions, the Fourier cosine transform, a, and the Fourier sine transform, b.
The function f can be recovered from the sine and cosine transform using
 [math]\displaystyle{ f(t) = 2\int_0 ^{\infty} \int_{\infty}^{\infty} f(\tau) \cos\bigl( 2\pi \lambda(\taut)\bigr) \, d\tau \, d\lambda. }[/math]
together with trigonometric identities. This is referred to as Fourier's integral formula.^{[29]}^{[36]}^{[37]}^{[38]}
Spherical harmonics
Let the set of homogeneous harmonic polynomials of degree k on R^{n} be denoted by A_{k}. The set A_{k} consists of the solid spherical harmonics of degree k. The solid spherical harmonics play a similar role in higher dimensions to the Hermite polynomials in dimension one. Specifically, if f(x) = e^{−πx2}P(x) for some P(x) in A_{k}, then f̂(ξ) = i^{−k} f(ξ). Let the set H_{k} be the closure in L^{2}(R^{n}) of linear combinations of functions of the form f(x)P(x) where P(x) is in A_{k}. The space L^{2}(R^{n}) is then a direct sum of the spaces H_{k} and the Fourier transform maps each space H_{k} to itself and is possible to characterize the action of the Fourier transform on each space H_{k}.^{[16]}
Let f(x) = f_{0}(x)P(x) (with P(x) in A_{k}), then
 [math]\displaystyle{ \hat{f}(\xi)=F_0(\xi)P(\xi) }[/math]
where
 [math]\displaystyle{ F_0(r) = 2\pi i^{k}r^{\frac{n+2k2}{2}} \int_0^\infty f_0(s)J_\frac{n+2k2}{2}(2\pi rs)s^\frac{n+2k}{2}\,ds. }[/math]
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.^{[39]} This is essentially the Hankel transform. Moreover, there is a simple recursion relating the cases n + 2 and n^{[40]} allowing to compute, e.g., the threedimensional Fourier transform of a radial function from the onedimensional one.
Restriction problems
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 squareintegrable function the Fourier transform could be a general class of square integrable functions. As such, the restriction of the Fourier transform of an L^{2}(R^{n}) 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 nonzero curvature. The case when S is the unit sphere in R^{n} is of particular interest. In this case the Tomas–Stein restriction theorem states that the restriction of the Fourier transform to the unit sphere in R^{n} 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. Consider an increasing collection of measurable sets E_{R} indexed by R ∈ (0,∞): such as balls of radius R centered at the origin, or cubes of side 2R. For a given integrable function f, consider the function f_{R} defined by:
 [math]\displaystyle{ f_R(x) = \int_{E_R}\hat{f}(\xi) e^{2\pi ix\cdot\xi}\, d\xi, \quad x \in \mathbb{R}^n. }[/math]
Suppose in addition that f ∈ L^{p}(R^{n}). For n = 1 and 1 < p < ∞, if one takes E_{R} = (−R, R), then f_{R} converges to f 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 E_{R} is taken to be a cube with side length R, then convergence still holds. Another natural candidate is the Euclidean ball E_{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}(R^{n}). For n ≥ 2 it is a celebrated theorem of Charles Fefferman that the multiplier for the unit ball is never bounded unless p = 2.^{[19]} In fact, when p ≠ 2, this shows that not only may f_{R} fail to converge to f in L^{p}, but for some functions f ∈ L^{p}(R^{n}), f_{R} is not even an element of L^{p}.
Fourier transform on function spaces
On L^{p} spaces
On L^{1}
The definition of the Fourier transform by the integral formula
 [math]\displaystyle{ \hat{f}(\xi) = \int_{\mathbb{R}^n} f(x)e^{2\pi i \xi\cdot x}\,dx }[/math]
is valid for Lebesgue integrable functions f; that is, f ∈ L^{1}(R^{n}).
The Fourier transform F : L^{1}(R^{n}) → L^{∞}(R^{n}) is a bounded operator. This follows from the observation that
 [math]\displaystyle{ \left\vert\hat{f}(\xi)\right\vert \leq \int_{\mathbb{R}^n} \vert f(x)\vert \,dx, }[/math]
which shows that its operator norm is bounded by 1. Indeed, it equals 1, which can be seen, for example, from the transform of the rect function. The image of L^{1} is a subset of the space C_{0}(R^{n}) of continuous functions that tend to zero at infinity (the Riemann–Lebesgue lemma), although it is not the entire space. Indeed, there is no simple characterization of the image.
On L^{2}
Since compactly supported smooth functions are integrable and dense in L^{2}(R^{n}), the Plancherel theorem allows us to extend the definition of the Fourier transform to general functions in L^{2}(R^{n}) by continuity arguments. The Fourier transform in L^{2}(R^{n}) is no longer given by an ordinary Lebesgue integral, although it can be computed by an improper integral, here meaning that for an L^{2} function f,
 [math]\displaystyle{ \hat{f}(\xi) = \lim_{R\to\infty}\int_{x\le R} f(x) e^{2\pi i x\cdot\xi}\,dx }[/math]
where the limit is taken in the L^{2} sense. (More generally, you can take a sequence of functions that are in the intersection of L^{1} and L^{2} and that converges to f in the L^{2}norm, and define the Fourier transform of f as the L^{2} limit of the Fourier transforms of these functions.^{[41]})
Many of the properties of the Fourier transform in L^{1} carry over to L^{2}, by a suitable limiting argument.
Furthermore, F : L^{2}(R^{n}) → L^{2}(R^{n}) is a unitary operator.^{[42]} For an operator to be unitary it is sufficient to show that it is bijective and preserves the inner product, so in this case these follow from the Fourier inversion theorem combined with the fact that for any f, g ∈ L^{2}(R^{n}) we have
 [math]\displaystyle{ \int_{\mathbb{R}^n} f(x)\mathcal{F}g(x)\,dx = \int_{\mathbb{R}^n} \mathcal{F}f(x)g(x)\,dx. }[/math]
In particular, the image of L^{2}(R^{n}) is itself under the Fourier transform.
On other L^{p}
The definition of the Fourier transform can be extended to functions in L^{p}(R^{n}) for 1 ≤ p ≤ 2 by decomposing such functions into a fat tail part in L^{2} plus a fat body part in L^{1}. In each of these spaces, the Fourier transform of a function in L^{p}(R^{n}) is in L^{q}(R^{n}), where q = p/p − 1 is the Hölder conjugate of p (by the Hausdorff–Young inequality). However, except for p = 2, the image is not easily characterized. Further extensions become more technical. The Fourier transform of functions in L^{p} for the range 2 < p < ∞ requires the study of distributions.^{[15]} 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.^{[16]}
Tempered distributions
One might consider enlarging the domain of the Fourier transform from L^{1} + L^{2} by considering generalized functions, or distributions. A distribution on R^{n} is a continuous linear functional on the space C_{c}(R^{n}) of compactly supported smooth functions, equipped with a suitable topology. The strategy is then to consider the action of the Fourier transform on C_{c}(R^{n}) and pass to distributions by duality. The obstruction to doing this is that the Fourier transform does not map C_{c}(R^{n}) to C_{c}(R^{n}). In fact the Fourier transform of an element in C_{c}(R^{n}) can not vanish on an open set; see the above discussion on the uncertainty principle. The right space here is the slightly larger space of Schwartz functions. The Fourier transform is an automorphism on the Schwartz space, as a topological vector space, and thus induces an automorphism on its dual, the space of tempered distributions.^{[16]} The tempered distributions include all the integrable functions mentioned above, as well as wellbehaved functions of polynomial growth and distributions of compact support.
For the definition of the Fourier transform of a tempered distribution, let f and g be integrable functions, and let f̂ and ĝ be their Fourier transforms respectively. Then the Fourier transform obeys the following multiplication formula,^{[16]}
 [math]\displaystyle{ \int_{\mathbb{R}^n}\hat{f}(x)g(x)\,dx=\int_{\mathbb{R}^n}f(x)\hat{g}(x)\,dx. }[/math]
Every integrable function f defines (induces) a distribution T_{f} by the relation
 [math]\displaystyle{ T_f(\varphi)=\int_{\mathbb{R}^n}f(x)\varphi(x)\,dx }[/math]
for all Schwartz functions φ. So it makes sense to define Fourier transform T̂_{f} of T_{f} by
 [math]\displaystyle{ \hat{T}_f (\varphi)= T_f\left(\hat{\varphi}\right) }[/math]
for all Schwartz functions φ. Extending this to all tempered distributions T gives the general definition of the Fourier transform.
Distributions can be differentiated and the abovementioned compatibility of the Fourier transform with differentiation and convolution remains true for tempered distributions.
Generalizations
Fourier–Stieltjes transform
The Fourier transform of a finite Borel measure μ on R^{n} is given by:^{[43]}
 [math]\displaystyle{ \hat\mu(\xi)=\int_{\mathbb{R}^n} e^{2\pi i x \cdot \xi}\,d\mu. }[/math]
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.^{[15]} In the case that dμ = f(x) dx, then the formula above reduces to the usual definition for the Fourier transform of f. In the case that μ is the probability distribution associated to a random variable X, the Fourier–Stieltjes transform is closely related to the characteristic function, but the typical conventions in probability theory take e^{ixξ} instead of e^{−2πixξ}.^{[14]} In the case when the distribution has a probability density function this definition reduces to the Fourier transform applied to the probability density function, again with a different choice of constants.
The Fourier transform may be used to give a characterization of measures. Bochner's theorem characterizes which functions may arise as the Fourier–Stieltjes transform of a positive measure on the circle.^{[15]}
Furthermore, the Dirac delta function, although not a function, is a finite Borel measure. Its Fourier transform is a constant function (whose specific value depends upon the form of the Fourier transform used).
Kaniadakis κFourier transform
The Kaniadakis κFourier transform is a κdeformation of the Fourier transform, associated with the Kaniadakis statistics, which is defined as:^{[44]}
 [math]\displaystyle{ {\cal F}_\kappa[f(x)](\omega)={1\over\sqrt{2\,\pi}}\int\limits_{\infty}\limits^{+\infty}f(x)\, {\exp(i\,x_{\{\kappa\}}\,\omega_{\{\kappa\}})\over\sqrt{1+\kappa^2\,x^2}} \,d x }[/math]
where [math]\displaystyle{ z_{\{\kappa\}}=\frac{1}{\kappa}\, {\rm arcsinh} \,(\kappa\,z) }[/math] is a κnumber and [math]\displaystyle{ 0 \leq \kappa \lt 1 }[/math] is the entropic index linked with the Kaniadakis entropy.
The κFourier transform is based on the κFourier series,^{[45]} in which the classical Fourier series and Fourier transform are particular case in the [math]\displaystyle{ \kappa \rightarrow 0 }[/math] limiting case. This transform imposes an asymptotically logperiodic behavior (or κdeformed phase by deforminh [math]\displaystyle{ \omega }[/math]) and a damping factor following a waveletlike behavior ([math]\displaystyle{ \sqrt{1+\kappa^2\,x^2} }[/math]).
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 that is at the same time a locally compact Hausdorff topological space so that the group operation is 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, the set of irreducible, i.e. onedimensional, unitary representations are called its characters. With its natural group structure and the topology of pointwise convergence, the set of characters Ĝ is itself a locally compact abelian group, called the Pontryagin dual of G. For a function f in L^{1}(G), its Fourier transform is defined by^{[15]}
 [math]\displaystyle{ \hat{f}(\xi)=\int_G \xi(x)f(x)\,d\mu\qquad\text{for any }\xi\in\hat G. }[/math]
The Riemann–Lebesgue lemma holds in this case; f̂(ξ) is a function vanishing at infinity on Ĝ.
The Fourier transform on T=R/Z is an example; here T is a locally compact abelian group, and the Haar measure μ on T can be thought of as the Lebesgue measure on [0,1). Consider the representation of T on the complex plane C that is a 1dimensional complex vector space. There are a group of representations (which are irreducible since C is 1dim) [math]\displaystyle{ \{e_{k}: T\rightarrow GL_{1}(C)=C^{*}\mid k\in Z\} }[/math] where [math]\displaystyle{ e_{k}(x)=e^{2\pi ikx} }[/math] for [math]\displaystyle{ x\in T }[/math].
The character of such representation, that is the trace of [math]\displaystyle{ e_{k}(x) }[/math] for each [math]\displaystyle{ x\in T }[/math] and [math]\displaystyle{ k\in Z }[/math], is [math]\displaystyle{ e^{2\pi i kx} }[/math] itself. In the case of representation of finite group, the character table of the group G are rows of vectors such that each row is the character of one irreducible representation of G, and these vectors form an orthonormal basis of the space of class functions that map from G to C by Schur's lemma. Now the group T is no longer finite but still compact, and it preserves the orthonormality of character table. Each row of the table is the function [math]\displaystyle{ e_{k}(x) }[/math] of [math]\displaystyle{ x\in T, }[/math] and the inner product between two class functions (all functions being class functions since T is abelian) [math]\displaystyle{ f,g \in L^{2}(T, d\mu) }[/math] is defined as [math]\displaystyle{ \langle f,g\rangle=\frac{1}{T}\int_{[0,1)}f(y)\overline{g}(y)d\mu(y) }[/math] with the normalizing factor [math]\displaystyle{ T=1 }[/math]. The sequence [math]\displaystyle{ \{e_{k}\mid k\in Z\} }[/math] is an orthonormal basis of the space of class functions [math]\displaystyle{ L^{2}(T,d\mu) }[/math].
For any representation V of a finite group G, [math]\displaystyle{ \chi_{v} }[/math] can be expressed as the span [math]\displaystyle{ \sum_{i} \left\langle \chi_{v},\chi_{v_{i}} \right\rangle \chi_{v_{i}} }[/math] ([math]\displaystyle{ V_{i} }[/math] are the irreps of G), such that [math]\displaystyle{ \left\langle \chi_{v},\chi_{v_{i}} \right\rangle = \frac{1}{G}\sum_{g\in G}\chi_{v}(g)\overline{\chi}_{v_{i}}(g) }[/math]. Similarly for [math]\displaystyle{ G=T }[/math] and [math]\displaystyle{ f\in L^{2}(T,d\mu) }[/math], [math]\displaystyle{ f(x)=\sum_{k\in Z}\hat{f}(k)e_{k} }[/math]. The Pontriagin dual [math]\displaystyle{ \hat{T} }[/math] is [math]\displaystyle{ \{e_{k}\}(k\in Z) }[/math] and for [math]\displaystyle{ f\in L^{2}(T,d\mu) }[/math], [math]\displaystyle{ \hat{f}(k)=\frac{1}{T}\int_{[0,1)}f(y)e^{2\pi iky}dy }[/math] is its Fourier transform for [math]\displaystyle{ e_{k}\in \hat{T} }[/math].
Gelfand transform
The Fourier transform is also a special case of Gelfand transform. In this particular context, it is closely related to the Pontryagin duality map defined above.
Given an abelian locally compact Hausdorff topological group G, as before we consider space L^{1}(G), defined using a Haar measure. With convolution as multiplication, L^{1}(G) is an abelian Banach algebra. It also has an involution * given by
 [math]\displaystyle{ f^*(g) = \overline{f\left(g^{1}\right)}. }[/math]
Taking the completion with respect to the largest possibly C*norm gives its enveloping C*algebra, called the group C*algebra C*(G) of G. (Any C*norm on L^{1}(G) is bounded by the L^{1} norm, therefore their supremum exists.)
Given any abelian C*algebra A, the Gelfand transform gives an isomorphism between A and C_{0}(A^), where A^ is the multiplicative linear functionals, i.e. onedimensional representations, on A with the weak* topology. The map is simply given by
 [math]\displaystyle{ a \mapsto \bigl( \varphi \mapsto \varphi(a) \bigr) }[/math]
It turns out that the multiplicative linear functionals of C*(G), after suitable identification, are exactly the characters of G, and the Gelfand transform, when restricted to the dense subset L^{1}(G) is the Fourier–Pontryagin transform.
Compact nonabelian groups
The Fourier transform can also be defined for functions on a nonabelian group, provided that the group is compact. Removing the assumption that the underlying group is abelian, irreducible unitary representations need not always be onedimensional. This means the Fourier transform on a nonabelian group takes values as Hilbert space operators.^{[46]} The Fourier transform on compact groups is a major tool in representation theory^{[47]} and noncommutative harmonic analysis.
Let G be a compact Hausdorff topological group. Let Σ denote the collection of all isomorphism classes of finitedimensional irreducible unitary representations, along with a definite choice of representation U^{(σ)} on the Hilbert space H_{σ} of finite dimension d_{σ} for each σ ∈ Σ. If μ is a finite Borel measure on G, then the Fourier–Stieltjes transform of μ is the operator on H_{σ} defined by
 [math]\displaystyle{ \left\langle \hat{\mu}\xi,\eta\right\rangle_{H_\sigma} = \int_G \left\langle \overline{U}^{(\sigma)}_g\xi,\eta\right\rangle\,d\mu(g) }[/math]
where U^{(σ)} is the complexconjugate representation of U^{(σ)} acting on H_{σ}. If μ is absolutely continuous with respect to the leftinvariant probability measure λ on G, represented as
 [math]\displaystyle{ d\mu = f \, d\lambda }[/math]
for some f ∈ L^{1}(λ), one identifies the Fourier transform of f with the Fourier–Stieltjes transform of μ.
The mapping
 [math]\displaystyle{ \mu\mapsto\hat{\mu} }[/math]
defines an isomorphism between the Banach space M(G) of finite Borel measures (see rca space) and a closed subspace of the Banach space C_{∞}(Σ) consisting of all sequences E = (E_{σ}) indexed by Σ of (bounded) linear operators E_{σ} : H_{σ} → H_{σ} for which the norm
 [math]\displaystyle{ \E\ = \sup_{\sigma\in\Sigma}\left\E_\sigma\right\ }[/math]
is finite. The "convolution theorem" asserts that, furthermore, this isomorphism of Banach spaces is in fact an isometric isomorphism of C*algebras into a subspace of C_{∞}(Σ). Multiplication on M(G) is given by convolution of measures and the involution * defined by
 [math]\displaystyle{ f^*(g) = \overline{f\left(g^{1}\right)}, }[/math]
and C_{∞}(Σ) has a natural C*algebra structure as Hilbert space operators.
The Peter–Weyl theorem holds, and a version of the Fourier inversion formula (Plancherel's theorem) follows: if f ∈ L^{2}(G), then
 [math]\displaystyle{ f(g) = \sum_{\sigma\in\Sigma} d_\sigma \operatorname{tr}\left(\hat{f}(\sigma)U^{(\sigma)}_g\right) }[/math]
where the summation is understood as convergent in the L^{2} sense.
The generalization of the Fourier transform to the noncommutative situation has also in part contributed to the development of noncommutative geometry. In this context, a categorical generalization of the Fourier transform to noncommutative groups is Tannaka–Krein duality, which replaces the group of characters with the category of representations. However, this loses the connection with harmonic functions.
Alternatives
In signal processing terms, a function (of time) is a representation of a signal with perfect time resolution, but no frequency information, while the Fourier transform has perfect frequency resolution, but no time information: the magnitude of the Fourier transform at a point is how much frequency content there is, but location is only given by phase (argument of the Fourier transform at a point), and standing waves are not localized in time – a sine wave continues out to infinity, without decaying. This limits the usefulness of the Fourier transform for analyzing signals that are localized in time, notably transients, or any signal of finite extent.
As alternatives to the Fourier transform, in time–frequency analysis, one uses time–frequency transforms or time–frequency distributions to represent signals in a form that has some time information and some frequency information – by the uncertainty principle, there is a tradeoff between these. These can be generalizations of the Fourier transform, such as the shorttime Fourier transform or fractional Fourier transform, or other functions to represent signals, as in wavelet transforms and chirplet transforms, with the wavelet analog of the (continuous) Fourier transform being the continuous wavelet transform.^{[20]}
Applications
Linear operations performed in one domain (time or frequency) have corresponding operations in the other domain, which are sometimes easier to perform. The operation of differentiation in the time domain corresponds to multiplication by the frequency,^{[note 4]} so some differential equations are easier to analyze in the frequency domain. Also, convolution in the time domain corresponds to ordinary multiplication in the frequency domain (see Convolution theorem). After performing the desired operations, transformation of the result can be made back to the time domain. Harmonic analysis is the systematic study of the relationship between the frequency and time domains, including the kinds of functions or operations that are "simpler" in one or the other, and has deep connections to many areas of modern mathematics.
Analysis of differential equations
Perhaps the most important use of the Fourier transformation is to solve partial differential equations. Many of the equations of the mathematical physics of the nineteenth century can be treated this way. Fourier studied the heat equation, which in one dimension and in dimensionless units is
 [math]\displaystyle{ \frac{\partial^2 y(x,t)}{ \partial^2 x } =\frac{\partial y(x,t) }{ \partial t}. }[/math]
The example we will give, a slightly more difficult one, is the wave equation in one dimension,
 [math]\displaystyle{ \frac{\partial^2y(x,t)}{\partial^2 x }=\frac{\partial^2y(x,t)}{\partial^2t}. }[/math]
As usual, the problem is not to find a solution: there are infinitely many. The problem is that of the socalled "boundary problem": find a solution which satisfies the "boundary conditions"
 [math]\displaystyle{ y(x,0) = f(x) , \qquad \frac{\partial y(x,0) }{ \partial t}= g(x). }[/math]
Here, f and g are given functions. For the heat equation, only one boundary condition can be required (usually the first one). But for the wave equation, there are still infinitely many solutions y which satisfy the first boundary condition. But when one imposes both conditions, there is only one possible solution.
It is easier to find the Fourier transform ŷ of the solution than to find the solution directly. This is because the Fourier transformation takes differentiation into multiplication by the Fourierdual variable, and so a partial differential equation applied to the original function is transformed into multiplication by polynomial functions of the dual variables applied to the transformed function. After ŷ is determined, we can apply the inverse Fourier transformation to find y.
Fourier's method is as follows. First, note that any function of the forms
 [math]\displaystyle{ \cos\bigl(2\pi\xi(x\pm t)\bigr) \mbox{ or } \sin\bigl(2\pi\xi(x \pm t)\bigr) }[/math]
satisfies the wave equation. These are called the elementary solutions.
Second, note that therefore any integral
 [math]\displaystyle{ y(x,t) = \int_{0}^{\infty} a_+(\xi)\cos\bigl(2\pi\xi(x +t)\bigr) + a_(\xi)\cos\bigl(2\pi\xi(x t)\bigr) + b_+(\xi)\sin\bigl(2\pi\xi(x +t)\bigr) + b_(\xi)\sin\left(2\pi\xi(x t)\right) \, d\xi }[/math]
(for arbitrary a_{+}, a_{−}, b_{+}, b_{−}) satisfies the wave equation. (This integral is just a kind of continuous linear combination, and the equation is linear.)
Now this resembles the formula for the Fourier synthesis of a function. In fact, this is the real inverse Fourier transform of a_{±} and b_{±} in the variable x.
The third step is to examine how to find the specific unknown coefficient functions a_{±} and b_{±} that will lead to y satisfying the boundary conditions. We are interested in the values of these solutions at t = 0. So we will set t = 0. Assuming that the conditions needed for Fourier inversion are satisfied, we can then find the Fourier sine and cosine transforms (in the variable x) of both sides and obtain
 [math]\displaystyle{ 2\int_{\infty}^\infty y(x,0) \cos(2\pi\xi x) \, dx = a_++a_ }[/math]
and
 [math]\displaystyle{ 2\int_{\infty}^\infty y(x,0) \sin(2\pi\xi x) \, dx = b_++b_. }[/math]
Similarly, taking the derivative of y with respect to t and then applying the Fourier sine and cosine transformations yields
 [math]\displaystyle{ 2\int_{\infty}^{\infty} \frac{\partial y(u,0)}{\partial t} \sin (2\pi\xi x) \, dx = (2\pi\xi)\left(a_++a_\right) }[/math]
and
 [math]\displaystyle{ 2\int_{\infty}^\infty \frac{\partial y(u,0)}{\partial t} \cos (2\pi\xi x) \, dx = (2\pi\xi)\left(b_+b_\right). }[/math]
These are four linear equations for the four unknowns a_{±} and b_{±}, in terms of the Fourier sine and cosine transforms of the boundary conditions, which are easily solved by elementary algebra, provided that these transforms can be found.
In summary, we chose a set of elementary solutions, parametrized by ξ, of which the general solution would be a (continuous) linear combination in the form of an integral over the parameter ξ. But this integral was in the form of a Fourier integral. The next step was to express the boundary conditions in terms of these integrals, and set them equal to the given functions f and g. But these expressions also took the form of a Fourier integral because of the properties of the Fourier transform of a derivative. The last step was to exploit Fourier inversion by applying the Fourier transformation to both sides, thus obtaining expressions for the coefficient functions a_{±} and b_{±} in terms of the given boundary conditions f and g.
From a higher point of view, Fourier's procedure can be reformulated more conceptually. Since there are two variables, we will use the Fourier transformation in both x and t rather than operate as Fourier did, who only transformed in the spatial variables. Note that ŷ must be considered in the sense of a distribution since y(x, t) is not going to be L^{1}: as a wave, it will persist through time and thus is not a transient phenomenon. But it will be bounded and so its Fourier transform can be defined as a distribution. The operational properties of the Fourier transformation that are relevant to this equation are that it takes differentiation in x to multiplication by 2πiξ and differentiation with respect to t to multiplication by 2πif where f is the frequency. Then the wave equation becomes an algebraic equation in ŷ:
 [math]\displaystyle{ \xi^2 \hat y (\xi, f) = f^2 \hat y (\xi, f). }[/math]
This is equivalent to requiring ŷ(ξ, f) = 0 unless ξ = ±f. Right away, this explains why the choice of elementary solutions we made earlier worked so well: obviously f̂ = δ(ξ ± f) will be solutions. Applying Fourier inversion to these delta functions, we obtain the elementary solutions we picked earlier. But from the higher point of view, one does not pick elementary solutions, but rather considers the space of all distributions which are supported on the (degenerate) conic ξ^{2} − f^{2} = 0.
We may as well consider the distributions supported on the conic that are given by distributions of one variable on the line ξ = f plus distributions on the line ξ = −f as follows: if Φ is any test function,
 [math]\displaystyle{ \iint \hat y \phi(\xi,f) \, d\xi \, df = \int s_+ \phi(\xi,\xi) \, d\xi + \int s_ \phi(\xi,\xi) \, d\xi, }[/math]
where s_{+}, and s_{−}, are distributions of one variable.
Then Fourier inversion gives, for the boundary conditions, something very similar to what we had more concretely above (put Φ(ξ, f) = e^{2πi(xξ+tf)}, which is clearly of polynomial growth):
 [math]\displaystyle{ y(x,0) = \int\bigl\{s_+(\xi) + s_(\xi)\bigr\} e^{2\pi i\xi x+0} \, d\xi }[/math]
and
 [math]\displaystyle{ \frac{\partial y(x,0)}{\partial t} = \int\bigl\{s_+(\xi)  s_(\xi)\bigr\} 2\pi i \xi e^{2\pi i\xi x+0} \, d\xi. }[/math]
Now, as before, applying the onevariable Fourier transformation in the variable x to these functions of x yields two equations in the two unknown distributions s_{±} (which can be taken to be ordinary functions if the boundary conditions are L^{1} or L^{2}).
From a calculational point of view, the drawback of course is that one must first calculate the Fourier transforms of the boundary conditions, then assemble the solution from these, and then calculate an inverse Fourier transform. Closed form formulas are rare, except when there is some geometric symmetry that can be exploited, and the numerical calculations are difficult because of the oscillatory nature of the integrals, which makes convergence slow and hard to estimate. For practical calculations, other methods are often used.
The twentieth century has seen the extension of these methods to all linear partial differential equations with polynomial coefficients, and by extending the notion of Fourier transformation to include Fourier integral operators, some nonlinear equations as well.
Fourier transform spectroscopy
The Fourier transform is also used in nuclear magnetic resonance (NMR) and in other kinds of spectroscopy, e.g. infrared (FTIR). In NMR an exponentially shaped free induction decay (FID) signal is acquired in the time domain and Fouriertransformed to a Lorentzian lineshape in the frequency domain. The Fourier transform is also used in magnetic resonance imaging (MRI) and mass spectrometry.
Quantum mechanics
The Fourier transform is useful in quantum mechanics in two different ways. To begin with, the basic conceptual structure of quantum mechanics postulates the existence of pairs of complementary variables, connected by the Heisenberg uncertainty principle. For example, in one dimension, the spatial variable q of, say, a particle, can only be measured by the quantum mechanical "position operator" at the cost of losing information about the momentum p of the particle. Therefore, the physical state of the particle can either be described by a function, called "the wave function", of q or by a function of p but not by a function of both variables. The variable p is called the conjugate variable to q. In classical mechanics, the physical state of a particle (existing in one dimension, for simplicity of exposition) would be given by assigning definite values to both p and q simultaneously. Thus, the set of all possible physical states is the twodimensional real vector space with a paxis and a qaxis called the phase space.
In contrast, quantum mechanics chooses a polarisation of this space in the sense that it picks a subspace of onehalf the dimension, for example, the qaxis alone, but instead of considering only points, takes the set of all complexvalued "wave functions" on this axis. Nevertheless, choosing the paxis is an equally valid polarisation, yielding a different representation of the set of possible physical states of the particle which is related to the first representation by the Fourier transformation
 [math]\displaystyle{ \phi(p) = \int \psi (q) e^{2\pi i \frac{pq}{h}}\, dq. }[/math]
Physically realisable states are L^{2}, and so by the Plancherel theorem, their Fourier transforms are also L^{2}. (Note that since q is in units of distance and p is in units of momentum, the presence of Planck's constant in the exponent makes the exponent dimensionless, as it should be.)
Therefore, the Fourier transform can be used to pass from one way of representing the state of the particle, by a wave function of position, to another way of representing the state of the particle: by a wave function of momentum. Infinitely many different polarisations are possible, and all are equally valid. Being able to transform states from one representation to another is sometimes convenient.
The other use of the Fourier transform in both quantum mechanics and quantum field theory is to solve the applicable wave equation. In nonrelativistic quantum mechanics, Schrödinger's equation for a timevarying wave function in onedimension, not subject to external forces, is
 [math]\displaystyle{ \frac{\partial^2}{\partial x^2} \psi(x,t) = i \frac h{2\pi} \frac{\partial}{\partial t} \psi(x,t). }[/math]
This is the same as the heat equation except for the presence of the imaginary unit i. Fourier methods can be used to solve this equation.
In the presence of a potential, given by the potential energy function V(x), the equation becomes
 [math]\displaystyle{ \frac{\partial^2}{\partial x^2} \psi(x,t) + V(x)\psi(x,t) = i \frac h{2\pi} \frac{\partial}{\partial t} \psi(x,t). }[/math]
The "elementary solutions", as we referred to them above, are the socalled "stationary states" of the particle, and Fourier's algorithm, as described above, can still be used to solve the boundary value problem of the future evolution of ψ given its values for t = 0. Neither of these approaches is of much practical use in quantum mechanics. Boundary value problems and the timeevolution of the wave function is not of much practical interest: it is the stationary states that are most important.
In relativistic quantum mechanics, Schrödinger's equation becomes a wave equation as was usual in classical physics, except that complexvalued waves are considered. A simple example, in the absence of interactions with other particles or fields, is the free onedimensional Klein–Gordon–Schrödinger–Fock equation, this time in dimensionless units,
 [math]\displaystyle{ \left (\frac{\partial^2}{\partial x^2} +1 \right) \psi(x,t) = \frac{\partial^2}{\partial t^2} \psi(x,t). }[/math]
This is, from the mathematical point of view, the same as the wave equation of classical physics solved above (but with a complexvalued wave, which makes no difference in the methods). This is of great use in quantum field theory: each separate Fourier component of a wave can be treated as a separate harmonic oscillator and then quantized, a procedure known as "second quantization". Fourier methods have been adapted to also deal with nontrivial interactions.
Signal processing
The Fourier transform is used for the spectral analysis of timeseries. The subject of statistical signal processing does not, however, usually apply the Fourier transformation to the signal itself. Even if a real signal is indeed transient, it has been found in practice advisable to model a signal by a function (or, alternatively, a stochastic process) which is stationary in the sense that its characteristic properties are constant over all time. The Fourier transform of such a function does not exist in the usual sense, and it has been found more useful for the analysis of signals to instead take the Fourier transform of its autocorrelation function.
The autocorrelation function R of a function f is defined by
 [math]\displaystyle{ R_f (\tau) = \lim_{T\rightarrow \infty} \frac{1}{2T} \int_{T}^T f(t) f(t+\tau) \, dt. }[/math]
This function is a function of the timelag τ elapsing between the values of f to be correlated.
For most functions f that occur in practice, R is a bounded even function of the timelag τ and for typical noisy signals it turns out to be uniformly continuous with a maximum at τ = 0.
The autocorrelation function, more properly called the autocovariance function unless it is normalized in some appropriate fashion, measures the strength of the correlation between the values of f separated by a time lag. This is a way of searching for the correlation of f with its own past. It is useful even for other statistical tasks besides the analysis of signals. For example, if f(t) represents the temperature at time t, one expects a strong correlation with the temperature at a time lag of 24 hours.
It possesses a Fourier transform,
 [math]\displaystyle{ P_f(\xi) = \int_{\infty}^\infty R_f (\tau) e^{2\pi i \xi\tau} \, d\tau. }[/math]
This Fourier transform is called the power spectral density function of f. (Unless all periodic components are first filtered out from f, this integral will diverge, but it is easy to filter out such periodicities.)
The power spectrum, as indicated by this density function P, measures the amount of variance contributed to the data by the frequency ξ. In electrical signals, the variance is proportional to the average power (energy per unit time), and so the power spectrum describes how much the different frequencies contribute to the average power of the signal. This process is called the spectral analysis of timeseries and is analogous to the usual analysis of variance of data that is not a timeseries (ANOVA).
Knowledge of which frequencies are "important" in this sense is crucial for the proper design of filters and for the proper evaluation of measuring apparatuses. It can also be useful for the scientific analysis of the phenomena responsible for producing the data.
The power spectrum of a signal can also be approximately measured directly by measuring the average power that remains in a signal after all the frequencies outside a narrow band have been filtered out.
Spectral analysis is carried out for visual signals as well. The power spectrum ignores all phase relations, which is good enough for many purposes, but for video signals other types of spectral analysis must also be employed, still using the Fourier transform as a tool.
Other notations
Other common notations for f̂(ξ) include:
 [math]\displaystyle{ \tilde{f}(\xi),\ \tilde{f}(\omega),\ F(\xi),\ \mathcal{F}\left(f\right)(\xi),\ \left(\mathcal{F}f\right)(\xi),\ \mathcal{F}(f),\ \mathcal F(\omega),\ F(\omega),\ \mathcal F(j\omega),\ \mathcal{F}\{f\},\ \mathcal{F} \bigl(f(t)\bigr),\ \mathcal{F} \bigl\{f(t)\bigr\}. }[/math]
Denoting 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, 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 written informally as F(2πf) in order to use ordinary frequency. In some contexts such as particle physics, the same symbol [math]\displaystyle{ f }[/math] may be used for both for a function as well as it Fourier transform, with the two only distinguished by their argument: [math]\displaystyle{ f(k_1 + k_2) }[/math] would refer to the Fourier transform because of the momentum argument, while [math]\displaystyle{ f(x_0 + \pi \vec r) }[/math] would refer to the original function because of the positional argument. Although tildes may be used as in [math]\displaystyle{ \tilde{f} }[/math] to indicate Fourier transforms, tildes may also be used to indicate a modification of a quantity with a more Lorentz invariant form, such as [math]\displaystyle{ \tilde{dk} = \frac{dk}{(2\pi)^32\omega} }[/math], so care must be taken.
The interpretation of the complex function f̂(ξ) may be aided by expressing it in polar coordinate form
 [math]\displaystyle{ \hat f(\xi) = A(\xi) e^{i\varphi(\xi)} }[/math]
in terms of the two real functions A(ξ) and φ(ξ) where:
 [math]\displaystyle{ A(\xi) = \left\hat f(\xi)\right, }[/math]
is the amplitude and
 [math]\displaystyle{ \varphi (\xi) = \arg \left( \hat f(\xi) \right), }[/math]
is the phase (see arg function).
Then the inverse transform can be written:
 [math]\displaystyle{ f(x) = \int _{\infty}^\infty A(\xi)\ e^{ i\bigl(2\pi \xi x +\varphi (\xi)\bigr)}\,d\xi, }[/math]
which is a recombination of all the frequency components of f(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 may be thought of as a mapping on function spaces. This mapping is here denoted F and F(f) is used to denote the Fourier transform of the function f. This mapping is linear, which means that 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 F f instead of 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 F f(ξ) or as (F f)(ξ). Notice that in the former case, it is implicitly understood that 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 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,
 [math]\displaystyle{ \mathcal F\bigl( \operatorname{rect}(x) \bigr) = \operatorname{sinc}(\xi) }[/math]
is sometimes used to express that the Fourier transform of a rectangular function is a sinc function, or
 [math]\displaystyle{ \mathcal F\bigl(f(x + x_0)\bigr) = \mathcal F\bigl(f(x)\bigr)\cdot e^{2\pi i \xi x_0} }[/math]
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 x_{0}.
Other conventions
The Fourier transform can also be written in terms of angular frequency:
 [math]\displaystyle{ \omega = 2\pi \xi, }[/math]
whose units are radians per second.
The substitution ξ = ω/2π into the formulas above produces this convention:
 [math]\displaystyle{ \hat{f_3}(\omega) = \int_{\mathbb R^n} f(x) e^{i\omega\cdot x}\, dx. }[/math]
Under this convention, the inverse transform becomes:
 [math]\displaystyle{ f(x) = \frac{1}{(2\pi)^n} \int_{\mathbb R^n} \hat{f_3}(\omega)e^{i\omega \cdot x}\, d\omega. }[/math]
Unlike the convention followed in this article, when the Fourier transform is defined this way, it is no longer a unitary transformation on L^{2}(R^{n}). There is also less symmetry between the formulas for the Fourier transform and its inverse.
Another convention is to split the factor of (2π)^{n} evenly between the Fourier transform and its inverse, which leads to definitions:
 [math]\displaystyle{ \begin{align} \hat{f_2}(\omega) &= \frac{1}{(2\pi)^\frac{n}{2}} \int_{\mathbb{R}^n} f(x) e^{ i\omega\cdot x}\, dx, \\ f(x) &= \frac{1}{(2\pi)^\frac{n}{2}} \int_{\mathbb{R}^n} \hat{f_2}(\omega) e^{ i\omega \cdot x}\, d\omega. \end{align} }[/math]
Under this convention, the Fourier transform is again a unitary transformation on L^{2}(R^{n}). It also restores the symmetry between the Fourier transform and its inverse.
Variations of all three conventions can be created by conjugating the complexexponential 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.
ordinary frequency ξ (Hz)  unitary  [math]\displaystyle{ \begin{align} \hat{f}_1(\xi)\ &\stackrel{\mathrm{def}}{=}\ \int_{\infty}^{\infty} f(x)\cdot e^{2 \pi i x\cdot\xi}\, dx = \sqrt{2 \pi}\cdot \hat{f}_2(2 \pi \xi) = \hat{f}_3(2 \pi \xi) \\ f(x) &= \int_{\infty}^{\infty} \hat{f}_1(\xi)\cdot e^{2 \pi i x\cdot \xi}\, d\xi \end{align} }[/math] 

angular frequency ω (rad/s)  unitary  [math]\displaystyle{ \begin{align} \hat{f}_2(\omega)\ &\stackrel{\mathrm{def}}{=}\ \frac{1}{\sqrt{2 \pi}} \int_{\infty}^{\infty} f(x)\cdot e^{i \omega\cdot x}\, dx = \frac{1}{\sqrt{2 \pi}}\cdot \hat{f}_1 \! \left(\frac{\omega}{2 \pi}\right) = \frac{1}{\sqrt{2 \pi}}\cdot \hat{f}_3(\omega) \\ f(x) &= \frac{1}{\sqrt{2 \pi}} \int_{\infty}^{\infty} \hat{f}_2(\omega)\cdot e^{i \omega\cdot x}\, d\omega \end{align} }[/math] 
nonunitary  [math]\displaystyle{ \begin{align} \hat{f}_3(\omega) \ &\stackrel{\mathrm{def}}{=}\ \int_{\infty}^{\infty} f(x)\cdot e^{i\omega\cdot x}\, dx = \hat{f}_1 \left(\frac{\omega}{2 \pi}\right) = \sqrt{2 \pi}\cdot \hat{f}_2(\omega) \\ f(x) &= \frac{1}{2 \pi} \int_{\infty}^{\infty} \hat{f}_3(\omega)\cdot e^{i \omega\cdot x}\, d\omega \end{align} }[/math] 
ordinary frequency ξ (Hz)  unitary  [math]\displaystyle{ \begin{align} \hat{f}_1(\xi)\ &\stackrel{\mathrm{def}}{=}\ \int_{\mathbb{R}^n} f(x) e^{2 \pi i x\cdot\xi}\, dx = (2 \pi)^\frac{n}{2}\hat{f}_2(2 \pi \xi) = \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 \end{align} }[/math] 

angular frequency ω (rad/s)  unitary  [math]\displaystyle{ \begin{align} \hat{f}_2(\omega)\ &\stackrel{\mathrm{def}}{=}\ \frac{1}{(2 \pi)^\frac{n}{2}} \int_{\mathbb{R}^n} f(x) e^{i \omega\cdot x}\, dx = \frac{1}{(2 \pi)^\frac{n}{2}} \hat{f}_1 \! \left(\frac{\omega}{2 \pi}\right) = \frac{1}{(2 \pi)^\frac{n}{2}} \hat{f}_3(\omega) \\ f(x) &= \frac{1}{(2 \pi)^\frac{n}{2}} \int_{\mathbb{R}^n} \hat{f}_2(\omega)e^{i \omega\cdot x}\, d\omega \end{align} }[/math] 
nonunitary  [math]\displaystyle{ \begin{align} \hat{f}_3(\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)^\frac{n}{2} \hat{f}_2(\omega) \\ f(x) &= \frac{1}{(2 \pi)^n} \int_{\mathbb{R}^n} \hat{f}_3(\omega) e^{i \omega\cdot x}\, d\omega \end{align} }[/math] 
As discussed above, the characteristic function of a random variable is the same as the Fourier–Stieltjes transform of its distribution measure, but in this context it is typical to take a different convention for the constants. Typically characteristic function is defined
 [math]\displaystyle{ E\left(e^{it\cdot X}\right)=\int e^{it\cdot x} \, d\mu_X(x). }[/math]
As in the case of the "nonunitary angular frequency" convention above, the factor of 2π appears in neither the normalizing constant nor the exponent. Unlike any of the conventions appearing above, this convention takes the opposite sign in the exponent.
Computation methods
The appropriate computation method largely depends how the original mathematical function is represented and the desired form of the output function.
Since the fundamental definition of a Fourier transform is an integral, functions that can be expressed as closedform expressions are commonly computed by working the integral analytically to yield a closedform expression in the Fourier transform conjugate variable as the result. This is the method used to generate tables of Fourier transforms,^{[48]} including those found in the table below (Fourier transform).
Many computer algebra systems such as Matlab and Mathematica that are capable of symbolic integration are capable of computing Fourier transforms analytically. For example, to compute the Fourier transform of f(t) = cos(6πt) e^{−πt2} one might enter the command integrate cos(6*pi*t) exp(−pi*t^2) exp(i*2*pi*f*t) from inf to inf
into Wolfram Alpha.^{[note 5]}
Numerical integration of closedform functions
If the input function is in closedform and the desired output function is a series of ordered pairs (for example a table of values from which a graph can be generated) over a specified domain, then the Fourier transform can be generated by numerical integration at each value of the Fourier conjugate variable (frequency, for example) for which a value of the output variable is desired.^{[49]} Note that this method requires computing a separate numerical integration for each value of frequency for which a value of the Fourier transform is desired.^{[50]}^{[51]} The numerical integration approach works on a much broader class of functions than the analytic approach, because it yields results for functions that do not have closed form Fourier transform integrals.
Numerical integration of a series of ordered pairs
If the input function is a series of ordered pairs (for example, a time series from measuring an output variable repeatedly over a time interval) then the output function must also be a series of ordered pairs (for example, a complex number vs. frequency over a specified domain of frequencies), unless certain assumptions and approximations are made allowing the output function to be approximated by a closedform expression. In the general case where the available input series of ordered pairs are assumed be samples representing a continuous function over an interval (amplitude vs. time, for example), the series of ordered pairs representing the desired output function can be obtained by numerical integration of the input data over the available interval at each value of the Fourier conjugate variable (frequency, for example) for which the value of the Fourier transform is desired.^{[52]}
Explicit numerical integration over the ordered pairs can yield the Fourier transform output value for any desired value of the conjugate Fourier transform variable (frequency, for example), so that a spectrum can be produced at any desired step size and over any desired variable range for accurate determination of amplitudes, frequencies, and phases corresponding to isolated peaks. Unlike limitations in DFT and FFT methods, explicit numerical integration can have any desired step size and compute the Fourier transform over any desired range of the conjugate Fourier transform variable (for example, frequency).
Discrete Fourier transforms and fast Fourier transforms
If the ordered pairs representing the original input function are equally spaced in their input variable (for example, equal time steps), then the Fourier transform is known as a discrete Fourier transform (DFT), which can be computed either by explicit numerical integration, by explicit evaluation of the DFT definition, or by fast Fourier transform (FFT) methods. In contrast to explicit integration of input data, use of the DFT and FFT methods produces Fourier transforms described by ordered pairs of step size equal to the reciprocal of the original sampling interval. For example, if the input data is sampled every 10 seconds, the output of DFT and FFT methods will have a 0.1 Hz frequency spacing.
Tables of important Fourier transforms
The following tables record some closedform Fourier transforms. For functions f(x), g(x) and h(x) denote their Fourier transforms by f̂, ĝ, and ĥ respectively. Only the three most common conventions are included. It may be useful to notice that entry 105 gives a relationship between the Fourier transform of a function and the original function, which can be seen as relating the Fourier transform and its inverse.
Functional relationships, onedimensional
The Fourier transforms in this table may be found in (Erdélyi 1954) or (Kammler 2000).
Function  Fourier transform unitary, ordinary frequency 
Fourier transform unitary, angular frequency 
Fourier transform nonunitary, angular frequency 
Remarks  

[math]\displaystyle{ f(x)\, }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\xi) \\&= \int_{\infty}^\infty f(x) e^{2\pi i x\xi}\, dx \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\omega) \\&= \frac{1}{\sqrt{2 \pi}} \int_{\infty}^\infty f(x) e^{i \omega x}\, dx \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\nu) \\&= \int_{\infty}^\infty f(x) e^{i \nu x}\, dx \end{align} }[/math]  Definition  
101  [math]\displaystyle{ a\cdot f(x) + b\cdot g(x)\, }[/math]  [math]\displaystyle{ a\cdot \hat{f}(\xi) + b\cdot \hat{g}(\xi)\, }[/math]  [math]\displaystyle{ a\cdot \hat{f}(\omega) + b\cdot \hat{g}(\omega)\, }[/math]  [math]\displaystyle{ a\cdot \hat{f}(\nu) + b\cdot \hat{g}(\nu)\, }[/math]  Linearity 
102  [math]\displaystyle{ f(x  a)\, }[/math]  [math]\displaystyle{ e^{2\pi i a \xi} \hat{f}(\xi)\, }[/math]  [math]\displaystyle{ e^{ i a \omega} \hat{f}(\omega)\, }[/math]  [math]\displaystyle{ e^{ i a \nu} \hat{f}(\nu)\, }[/math]  Shift in time domain 
103  [math]\displaystyle{ f(x)e^{iax}\, }[/math]  [math]\displaystyle{ \hat{f} \left(\xi  \frac{a}{2\pi}\right)\, }[/math]  [math]\displaystyle{ \hat{f}(\omega  a)\, }[/math]  [math]\displaystyle{ \hat{f}(\nu  a)\, }[/math]  Shift in frequency domain, dual of 102 
104  [math]\displaystyle{ f(a x)\, }[/math]  [math]\displaystyle{ \frac{1}{a} \hat{f}\left( \frac{\xi}{a} \right)\, }[/math]  [math]\displaystyle{ \frac{1}{a} \hat{f}\left( \frac{\omega}{a} \right)\, }[/math]  [math]\displaystyle{ \frac{1}{a} \hat{f}\left( \frac{\nu}{a} \right)\, }[/math]  Scaling in the time domain. If a is large, then f(ax) is concentrated around 0 and [math]\displaystyle{ \frac{1}{a}\hat{f} \left( \frac{\omega}{a} \right)\, }[/math] spreads out and flattens. 
105  [math]\displaystyle{ \hat{f}(x)\, }[/math]  [math]\displaystyle{ f(\xi)\, }[/math]  [math]\displaystyle{ f(\omega)\, }[/math]  [math]\displaystyle{ 2\pi f(\nu)\, }[/math]  Duality. Here f̂ needs to be calculated using the same method as Fourier transform column. Results from swapping "dummy" variables of x and ξ or ω or ν. 
106  [math]\displaystyle{ \frac{d^n f(x)}{dx^n}\, }[/math]  [math]\displaystyle{ (2\pi i\xi)^n \hat{f}(\xi)\, }[/math]  [math]\displaystyle{ (i\omega)^n \hat{f}(\omega)\, }[/math]  [math]\displaystyle{ (i\nu)^n \hat{f}(\nu)\, }[/math]  as f is a Schwartz function 
107  [math]\displaystyle{ x^n f(x)\, }[/math]  [math]\displaystyle{ \left (\frac{i}{2\pi}\right)^n \frac{d^n \hat{f}(\xi)}{d\xi^n}\, }[/math]  [math]\displaystyle{ i^n \frac{d^n \hat{f}(\omega)}{d\omega^n} }[/math]  [math]\displaystyle{ i^n \frac{d^n \hat{f}(\nu)}{d\nu^n} }[/math]  This is the dual of 106 
108  [math]\displaystyle{ (f * g)(x)\, }[/math]  [math]\displaystyle{ \hat{f}(\xi) \hat{g}(\xi)\, }[/math]  [math]\displaystyle{ \sqrt{2\pi} \hat{f}(\omega) \hat{g}(\omega)\, }[/math]  [math]\displaystyle{ \hat{f}(\nu) \hat{g}(\nu)\, }[/math]  The notation f ∗ g denotes the convolution of f and g — this rule is the convolution theorem 
109  [math]\displaystyle{ f(x) g(x)\, }[/math]  [math]\displaystyle{ \left(\hat{f} * \hat{g}\right)(\xi)\, }[/math]  [math]\displaystyle{ \frac{1}\sqrt{2\pi}\left(\hat{f} * \hat{g}\right)(\omega)\, }[/math]  [math]\displaystyle{ \frac{1}{2\pi}\left(\hat{f} * \hat{g}\right)(\nu)\, }[/math]  This is the dual of 108 
110  For f(x) purely real  [math]\displaystyle{ \hat{f}(\xi) = \overline{\hat{f}(\xi)}\, }[/math]  [math]\displaystyle{ \hat{f}(\omega) = \overline{\hat{f}(\omega)}\, }[/math]  [math]\displaystyle{ \hat{f}(\nu) = \overline{\hat{f}(\nu)}\, }[/math]  Hermitian symmetry. z indicates the complex conjugate. 
111  For f(x) purely real and even  f̂(ξ), f̂(ω) and f̂(ν) are purely real even functions.  
112  For f(x) purely real and odd  f̂(ξ), f̂(ω) and f̂(ν) are purely imaginary odd functions.  
113  For f(x) purely imaginary  [math]\displaystyle{ \hat{f}(\xi) = \overline{\hat{f}(\xi)}\, }[/math]  [math]\displaystyle{ \hat{f}(\omega) = \overline{\hat{f}(\omega)}\, }[/math]  [math]\displaystyle{ \hat{f}(\nu) = \overline{\hat{f}(\nu)}\, }[/math]  z indicates the complex conjugate. 
114  [math]\displaystyle{ \overline{f(x)} }[/math]  [math]\displaystyle{ \overline{\hat{f}(\xi)} }[/math]  [math]\displaystyle{ \overline{\hat{f}(\omega)} }[/math]  [math]\displaystyle{ \overline{\hat{f}(\nu)} }[/math]  Complex conjugation, generalization of 110 and 113 
115  [math]\displaystyle{ f(x) \cos (a x) }[/math]  [math]\displaystyle{ \frac{ \hat{f}\left(\xi  \frac{a}{2\pi}\right)+\hat{f}\left(\xi+\frac{a}{2\pi}\right)}{2} }[/math]  [math]\displaystyle{ \frac{\hat{f}(\omegaa)+\hat{f}(\omega+a)}{2}\, }[/math]  [math]\displaystyle{ \frac{\hat{f}(\nua)+\hat{f}(\nu+a)}{2} }[/math]  This follows from rules 101 and 103 using Euler's formula: [math]\displaystyle{ \cos(a x) = \frac{e^{i a x} + e^{i a x}}{2}. }[/math] 
116  [math]\displaystyle{ f(x)\sin( ax) }[/math]  [math]\displaystyle{ \frac{\hat{f}\left(\xi\frac{a}{2\pi}\right)\hat{f}\left(\xi+\frac{a}{2\pi}\right)}{2i} }[/math]  [math]\displaystyle{ \frac{\hat{f}(\omegaa)\hat{f}(\omega+a)}{2i} }[/math]  [math]\displaystyle{ \frac{\hat{f}(\nua)\hat{f}(\nu+a)}{2i} }[/math]  This follows from 101 and 103 using Euler's formula: [math]\displaystyle{ \sin(a x) = \frac{e^{i a x}  e^{i a x}}{2i}. }[/math] 
Squareintegrable functions, onedimensional
The Fourier transforms in this table may be found in (Campbell Foster), (Erdélyi 1954), or (Kammler 2000).
Function  Fourier transform unitary, ordinary frequency 
Fourier transform unitary, angular frequency 
Fourier transform nonunitary, angular frequency 
Remarks  

[math]\displaystyle{ f(x)\, }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\xi) \\&= \int_{\infty}^\infty f(x) e^{2\pi i x\xi}\, dx \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\omega) \\&= \frac{1}{\sqrt{2 \pi}} \int_{\infty}^\infty f(x) e^{i \omega x}\, dx \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\nu) \\&= \int_{\infty}^\infty f(x) e^{i \nu x}\, dx \end{align} }[/math]  
201  [math]\displaystyle{ \operatorname{rect}(a x) \, }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{sinc}\left(\frac{\xi}{a}\right) }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2 \pi a^2}}\cdot \operatorname{sinc}\left(\frac{\omega}{2\pi a}\right) }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{sinc}\left(\frac{\nu}{2\pi a}\right) }[/math]  The rectangular pulse and the normalized sinc function, here defined as sinc(x) = sin(πx)/πx 
202  [math]\displaystyle{ \operatorname{sinc}(a x)\, }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{rect}\left(\frac{\xi}{a} \right)\, }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2\pi a^2}}\cdot \operatorname{rect}\left(\frac{\omega}{2 \pi a}\right) }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{rect}\left(\frac{\nu}{2 \pi a}\right) }[/math]  Dual of rule 201. The rectangular function is an ideal lowpass filter, and the sinc function is the noncausal impulse response of such a filter. The sinc function is defined here as sinc(x) = sin(πx)/πx 
203  [math]\displaystyle{ \operatorname{sinc}^2 (a x) }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{tri} \left( \frac{\xi}{a} \right) }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2\pi a^2}}\cdot \operatorname{tri} \left( \frac{\omega}{2\pi a} \right) }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{tri} \left( \frac{\nu}{2\pi a} \right) }[/math]  The function tri(x) is the triangular function 
204  [math]\displaystyle{ \operatorname{tri} (a x) }[/math]  [math]\displaystyle{ \frac{1}{a}\cdot \operatorname{sinc}^2 \left( \frac{\xi}{a} \right) \, }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2\pi a^2}} \cdot \operatorname{sinc}^2 \left( \frac{\omega}{2\pi a} \right) }[/math]  [math]\displaystyle{ \frac{1}{a} \cdot \operatorname{sinc}^2 \left( \frac{\nu}{2\pi a} \right) }[/math]  Dual of rule 203. 
205  [math]\displaystyle{ e^{ a x} u(x) \, }[/math]  [math]\displaystyle{ \frac{1}{a + 2 \pi i \xi} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2 \pi} (a + i \omega)} }[/math]  [math]\displaystyle{ \frac{1}{a + i \nu} }[/math]  The function u(x) is the Heaviside unit step function and a > 0. 
206  [math]\displaystyle{ e^{\alpha x^2}\, }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{\alpha}}\cdot e^{\frac{(\pi \xi)^2}{\alpha}} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2 \alpha}}\cdot e^{\frac{\omega^2}{4 \alpha}} }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{\alpha}}\cdot e^{\frac{\nu^2}{4 \alpha}} }[/math]  This shows that, for the unitary Fourier transforms, the Gaussian function e^{−αx2} is its own Fourier transform for some choice of α. For this to be integrable we must have Re(α) > 0. 
207  [math]\displaystyle{ e^{i\alpha x^2}\, }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{\alpha}}\cdot e^{i(\frac{(\pi \xi)^2}{\alpha}  \frac{\pi}{4})} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2 \alpha}}\cdot e^{i(\frac{\omega^2}{4 \alpha}  \frac{\pi}{4})} }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{\alpha}}\cdot e^{i(\frac{\nu^2}{4 \alpha}  \frac{\pi}{4})} }[/math]  This is known as the complex quadraticphase sinusoid, or the "chirp" function.^{[53]} 
208  [math]\displaystyle{ e^{ax} \, }[/math]  [math]\displaystyle{ \frac{2 a}{a^2 + 4 \pi^2 \xi^2} }[/math]  [math]\displaystyle{ \sqrt{\frac{2}{\pi}} \cdot \frac{a}{a^2 + \omega^2} }[/math]  [math]\displaystyle{ \frac{2a}{a^2 + \nu^{2}} }[/math]  For Re(a) > 0. That is, the Fourier transform of a twosided decaying exponential function is a Lorentzian function. 
209  [math]\displaystyle{ \operatorname{sech}(a x) \, }[/math]  [math]\displaystyle{ \frac{\pi}{a} \operatorname{sech} \left( \frac{\pi^2}{ a} \xi \right) }[/math]  [math]\displaystyle{ \frac{1}{a}\sqrt{\frac{\pi}{2}} \operatorname{sech}\left( \frac{\pi}{2 a} \omega \right) }[/math]  [math]\displaystyle{ \frac{\pi}{a}\operatorname{sech}\left( \frac{\pi}{2 a} \nu \right) }[/math]  Hyperbolic secant is its own Fourier transform 
210  [math]\displaystyle{ e^{\frac{a^2 x^2}2} H_n(a x)\, }[/math]  [math]\displaystyle{ \frac{\sqrt{2\pi}(i)^n}{a} e^{\frac{2\pi^2\xi^2}{a^2}} H_n\left(\frac{2\pi\xi}a\right) }[/math]  [math]\displaystyle{ \frac{(i)^n}{a} e^{\frac{\omega^2}{2 a^2}} H_n\left(\frac \omega a\right) }[/math]  [math]\displaystyle{ \frac{(i)^n \sqrt{2\pi}}{a} e^{\frac{\nu^2}{2 a^2}} H_n\left(\frac \nu a \right) }[/math]  H_{n} is the nthorder Hermite polynomial. If a = 1 then the Gauss–Hermite functions are eigenfunctions of the Fourier transform operator. For a derivation, see Hermite polynomial. The formula reduces to 206 for n = 0. 
Distributions, onedimensional
The Fourier transforms in this table may be found in (Erdélyi 1954) or (Kammler 2000).
Function  Fourier transform unitary, ordinary frequency 
Fourier transform unitary, angular frequency 
Fourier transform nonunitary, angular frequency 
Remarks  

[math]\displaystyle{ f(x)\, }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\xi) \\&= \int_{\infty}^\infty f(x) e^{2\pi i x\xi}\, dx \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\omega) \\&= \frac{1}{\sqrt{2 \pi}} \int_{\infty}^\infty f(x) e^{i \omega x}\, dx \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\nu) \\&= \int_{\infty}^\infty f(x) e^{i \nu x}\, dx \end{align} }[/math]  
301  [math]\displaystyle{ 1 }[/math]  [math]\displaystyle{ \delta(\xi) }[/math]  [math]\displaystyle{ \sqrt{2\pi}\cdot \delta(\omega) }[/math]  [math]\displaystyle{ 2\pi\delta(\nu) }[/math]  The distribution δ(ξ) denotes the Dirac delta function. 
302  [math]\displaystyle{ \delta(x)\, }[/math]  [math]\displaystyle{ 1 }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2\pi}}\, }[/math]  [math]\displaystyle{ 1 }[/math]  Dual of rule 301. 
303  [math]\displaystyle{ e^{i a x} }[/math]  [math]\displaystyle{ \delta\left(\xi  \frac{a}{2\pi}\right) }[/math]  [math]\displaystyle{ \sqrt{2 \pi}\cdot \delta(\omega  a) }[/math]  [math]\displaystyle{ 2 \pi\delta(\nu  a) }[/math]  This follows from 103 and 301. 
304  [math]\displaystyle{ \cos (a x) }[/math]  [math]\displaystyle{ \frac{ \delta\left(\xi  \frac{a}{2\pi}\right)+\delta\left(\xi+\frac{a}{2\pi}\right)}{2} }[/math]  [math]\displaystyle{ \sqrt{2 \pi}\cdot\frac{\delta(\omegaa)+\delta(\omega+a)}{2} }[/math]  [math]\displaystyle{ \pi\left(\delta(\nua)+\delta(\nu+a)\right) }[/math]  This follows from rules 101 and 303 using Euler's formula: [math]\displaystyle{ \cos(a x) = \frac{e^{i a x} + e^{i a x}}{2}. }[/math] 
305  [math]\displaystyle{ \sin( ax) }[/math]  [math]\displaystyle{ \frac{\delta\left(\xi\frac{a}{2\pi}\right)\delta\left(\xi+\frac{a}{2\pi}\right)}{2i} }[/math]  [math]\displaystyle{ \sqrt{2 \pi}\cdot\frac{\delta(\omegaa)\delta(\omega+a)}{2i} }[/math]  [math]\displaystyle{ i\pi\bigl(\delta(\nua)\delta(\nu+a)\bigr) }[/math]  This follows from 101 and 303 using [math]\displaystyle{ \sin(a x) = \frac{e^{i a x}  e^{i a x}}{2i}. }[/math] 
306  [math]\displaystyle{ \cos \left( a x^2 \right) }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{a}} \cos \left( \frac{\pi^2 \xi^2}{a}  \frac{\pi}{4} \right) }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2 a}} \cos \left( \frac{\omega^2}{4 a}  \frac{\pi}{4} \right) }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{a}} \cos \left( \frac{\nu^2}{4a}  \frac{\pi}{4} \right) }[/math]  This follows from 101 and 207 using [math]\displaystyle{ \cos(a x^2) = \frac{e^{i a x^2} + e^{i a x^2}}{2}. }[/math] 
307  [math]\displaystyle{ \sin \left( a x^2 \right) }[/math]  [math]\displaystyle{  \sqrt{\frac{\pi}{a}} \sin \left( \frac{\pi^2 \xi^2}{a}  \frac{\pi}{4} \right) }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{2 a}} \sin \left( \frac{\omega^2}{4 a}  \frac{\pi}{4} \right) }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{a}}\sin \left( \frac{\nu^2}{4a}  \frac{\pi}{4} \right) }[/math]  This follows from 101 and 207 using [math]\displaystyle{ \sin(a x^2) = \frac{e^{i a x^2}  e^{i a x^2}}{2i}. }[/math] 
308  [math]\displaystyle{ x^n\, }[/math]  [math]\displaystyle{ \left(\frac{i}{2\pi}\right)^n \delta^{(n)} (\xi) }[/math]  [math]\displaystyle{ i^n \sqrt{2\pi} \delta^{(n)} (\omega) }[/math]  [math]\displaystyle{ 2\pi i^n\delta^{(n)} (\nu) }[/math]  Here, n is a natural number and δ^{(n)}(ξ) is the nth distribution derivative of the Dirac delta function. This rule follows from rules 107 and 301. Combining this rule with 101, we can transform all polynomials. 
[math]\displaystyle{ \delta^{(n)}(x) }[/math]  [math]\displaystyle{ (2\pi i\xi)^n }[/math]  [math]\displaystyle{ \frac{(i\omega)^n}{\sqrt{2\pi}} }[/math]  [math]\displaystyle{ (i\nu)^n }[/math]  Dual of rule 308. δ^{(n)}(ξ) is the nth distribution derivative of the Dirac delta function. This rule follows from 106 and 302.  
309  [math]\displaystyle{ \frac{1}{x} }[/math]  [math]\displaystyle{ i\pi\sgn(\xi) }[/math]  [math]\displaystyle{ i\sqrt{\frac{\pi}{2}}\sgn(\omega) }[/math]  [math]\displaystyle{ i\pi\sgn(\nu) }[/math]  Here sgn(ξ) is the sign function. Note that 1/x is not a distribution. It is necessary to use the Cauchy principal value when testing against Schwartz functions. This rule is useful in studying the Hilbert transform. 
310  [math]\displaystyle{ \begin{align} &\frac{1}{x^n} \\ &:= \frac{(1)^{n1}}{(n1)!}\frac{d^n}{dx^n}\log x \end{align} }[/math]  [math]\displaystyle{ i\pi \frac{(2\pi i\xi)^{n1}}{(n1)!} \sgn(\xi) }[/math]  [math]\displaystyle{ i\sqrt{\frac{\pi}{2}}\cdot \frac{(i\omega)^{n1}}{(n1)!}\sgn(\omega) }[/math]  [math]\displaystyle{ i\pi \frac{(i\nu)^{n1}}{(n1)!}\sgn(\nu) }[/math]  1/x^{n} is the homogeneous distribution defined by the distributional derivative [math]\displaystyle{ \frac{(1)^{n1}}{(n1)!}\frac{d^n}{dx^n}\logx }[/math] 
311  [math]\displaystyle{ x^\alpha }[/math]  [math]\displaystyle{ \frac{2\sin\left(\frac{\pi\alpha}{2}\right)\Gamma(\alpha+1)}{2\pi\xi^{\alpha+1}} }[/math]  [math]\displaystyle{ \frac{2}{\sqrt{2\pi}}\cdot \frac{\sin\left(\frac{\pi\alpha}{2}\right)\Gamma(\alpha+1)}{\omega^{\alpha+1}} }[/math]  [math]\displaystyle{ \frac{2\sin\left(\frac{\pi\alpha}{2}\right)\Gamma(\alpha+1)}{\nu^{\alpha+1}} }[/math]  This formula is valid for 0 > α > −1. For α > 0 some singular terms arise at the origin that can be found by differentiating 318. If Re α > −1, then x^{α} is a locally integrable function, and so a tempered distribution. The function α ↦ x^{α} is a holomorphic function from the right halfplane to the space of tempered distributions. It admits a unique meromorphic extension to a tempered distribution, also denoted x^{α} for α ≠ −1, −3, ... (See homogeneous distribution.) 
[math]\displaystyle{ \frac{1}{\sqrt{x}} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{\xi}} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{\omega}} }[/math]  [math]\displaystyle{ \frac{\sqrt{2\pi}}{\sqrt{\nu}} }[/math]  Special case of 311.  
312  [math]\displaystyle{ \sgn(x) }[/math]  [math]\displaystyle{ \frac{1}{i\pi \xi} }[/math]  [math]\displaystyle{ \sqrt{\frac{2}{\pi}} \frac{1}{i\omega } }[/math]  [math]\displaystyle{ \frac{2}{i\nu } }[/math]  The dual of rule 309. This time the Fourier transforms need to be considered as a Cauchy principal value. 
313  [math]\displaystyle{ u(x) }[/math]  [math]\displaystyle{ \frac{1}{2}\left(\frac{1}{i \pi \xi} + \delta(\xi)\right) }[/math]  [math]\displaystyle{ \sqrt{\frac{\pi}{2}} \left( \frac{1}{i \pi \omega} + \delta(\omega)\right) }[/math]  [math]\displaystyle{ \pi\left( \frac{1}{i \pi \nu} + \delta(\nu)\right) }[/math]  The function u(x) is the Heaviside unit step function; this follows from rules 101, 301, and 312. 
314  [math]\displaystyle{ \sum_{n=\infty}^{\infty} \delta (x  n T) }[/math]  [math]\displaystyle{ \frac{1}{T} \sum_{k=\infty}^{\infty} \delta \left( \xi \frac{k }{T}\right) }[/math]  [math]\displaystyle{ \frac{\sqrt{2\pi }}{T}\sum_{k=\infty}^{\infty} \delta \left( \omega \frac{2\pi k}{T}\right) }[/math]  [math]\displaystyle{ \frac{2\pi}{T}\sum_{k=\infty}^{\infty} \delta \left( \nu \frac{2\pi k}{T}\right) }[/math]  This function is known as the Dirac comb function. This result can be derived from 302 and 102, together with the fact that [math]\displaystyle{ \begin{align} & \sum_{n=\infty}^{\infty} e^{inx} \\ = {}& 2\pi\sum_{k=\infty}^{\infty} \delta(x+2\pi k) \end{align} }[/math] as distributions. 
315  [math]\displaystyle{ J_0 (x) }[/math]  [math]\displaystyle{ \frac{2\, \operatorname{rect}(\pi\xi)}{\sqrt{1  4 \pi^2 \xi^2}} }[/math]  [math]\displaystyle{ \sqrt{\frac{2}{\pi}} \cdot \frac{\operatorname{rect}\left( \frac{\omega}{2} \right)}{\sqrt{1  \omega^2}} }[/math]  [math]\displaystyle{ \frac{2\,\operatorname{rect}\left(\frac{\nu}{2} \right)}{\sqrt{1  \nu^2}} }[/math]  The function J_{0}(x) is the zeroth order Bessel function of first kind. 
316  [math]\displaystyle{ J_n (x) }[/math]  [math]\displaystyle{ \frac{2 (i)^n T_n (2 \pi \xi) \operatorname{rect}(\pi \xi)}{\sqrt{1  4 \pi^2 \xi^2}} }[/math]  [math]\displaystyle{ \sqrt{\frac{2}{\pi}} \frac{ (i)^n T_n (\omega) \operatorname{rect} \left( \frac{\omega}{2} \right)}{\sqrt{1  \omega^2}} }[/math]  [math]\displaystyle{ \frac{2(i)^n T_n (\nu) \operatorname{rect} \left( \frac{\nu}{2} \right)}{\sqrt{1  \nu^2}} }[/math]  This is a generalization of 315. The function J_{n}(x) is the nth order Bessel function of first kind. The function T_{n}(x) is the Chebyshev polynomial of the first kind. 
317  [math]\displaystyle{ \log \left x \right }[/math]  [math]\displaystyle{ \frac{1}{2} \frac{1}{\left \xi \right}  \gamma \delta \left( \xi \right) }[/math]  [math]\displaystyle{ \frac{\sqrt\frac{\pi}{2}}{\left \omega \right}  \sqrt{2 \pi} \gamma \delta \left( \omega \right) }[/math]  [math]\displaystyle{ \frac{\pi}{\left \nu \right}  2 \pi \gamma \delta \left( \nu \right) }[/math]  γ is the Euler–Mascheroni constant. It is necessary to use a finite part integral when testing 1/ξ,1/ω,1/ν against Schwartz functions. The details of this might change the coefficient of the delta function. 
318  [math]\displaystyle{ \left( \mp ix \right)^{\alpha} }[/math]  [math]\displaystyle{ \frac{\left(2\pi\right)^\alpha}{\Gamma\left(\alpha\right)}u\left(\pm \xi \right)\left(\pm \xi \right)^{\alpha1} }[/math]  [math]\displaystyle{ \frac{\sqrt{2\pi}}{\Gamma\left(\alpha\right)}u\left(\pm\omega\right)\left(\pm\omega\right)^{\alpha1} }[/math]  [math]\displaystyle{ \frac{2\pi}{\Gamma\left(\alpha\right)}u\left(\pm\nu\right)\left(\pm\nu\right)^{\alpha1} }[/math]  This formula is valid for 1 > α > 0. Use differentiation to derive formula for higher exponents. u is the Heaviside function. 
Twodimensional functions
Function  Fourier transform unitary, ordinary frequency 
Fourier transform unitary, angular frequency 
Fourier transform nonunitary, angular frequency 
Remarks  

400  [math]\displaystyle{ f(x,y) }[/math]  [math]\displaystyle{ \begin{align}& \hat{f}(\xi_x, \xi_y) \\ &= \iint f(x,y) e^{2\pi i(\xi_x x+\xi_y y)}\,dx\,dy \end{align} }[/math]  [math]\displaystyle{ \begin{align}& \hat{f}(\omega_x,\omega_y) \\ &= \frac{1}{2 \pi} \iint f(x,y) e^{i (\omega_x x +\omega_y y)}\, dx\,dy \end{align} }[/math]  [math]\displaystyle{ \begin{align}& \hat{f}(\nu_x,\nu_y) \\ &= \iint f(x,y) e^{i(\nu_x x+\nu_y y)}\, dx\,dy \end{align} }[/math]  The variables ξ_{x}, ξ_{y}, ω_{x}, ω_{y}, ν_{x}, ν_{y} are real numbers. The integrals are taken over the entire plane. 
401  [math]\displaystyle{ e^{\pi\left(a^2x^2+b^2y^2\right)} }[/math]  [math]\displaystyle{ \frac{1}{ab} e^{\pi\left(\frac{\xi_x^2}{a^2} + \frac{\xi_y^2}{b^2}\right)} }[/math]  [math]\displaystyle{ \frac{1}{2\pi\cdotab} e^{\frac{1}{4\pi}\left(\frac{\omega_x^2}{a^2} + \frac{\omega_y^2}{b^2}\right)} }[/math]  [math]\displaystyle{ \frac{1}{ab} e^{\frac{1}{4\pi}\left(\frac{\nu_x^2}{a^2} + \frac{\nu_y^2}{b^2}\right)} }[/math]  Both functions are Gaussians, which may not have unit volume. 
402  [math]\displaystyle{ \operatorname{circ}\left(\sqrt{x^2+y^2}\right) }[/math]  [math]\displaystyle{ \frac{J_1\left(2 \pi \sqrt{\xi_x^2+\xi_y^2}\right)}{\sqrt{\xi_x^2+\xi_y^2}} }[/math]  [math]\displaystyle{ \frac{J_1\left(\sqrt{\omega_x^2+\omega_y^2}\right)}{\sqrt{\omega_x^2+\omega_y^2}} }[/math]  [math]\displaystyle{ \frac{2\pi J_1\left(\sqrt{\nu_x^2+\nu_y^2}\right)}{\sqrt{\nu_x^2+\nu_y^2}} }[/math]  The function is defined by circ(r) = 1 for 0 ≤ r ≤ 1, and is 0 otherwise. The result is the amplitude distribution of the Airy disk, and is expressed using J_{1} (the order1 Bessel function of the first kind).^{[54]} 
403  [math]\displaystyle{ \frac{1}{\sqrt{x^2+y^2}} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{\xi_x^2+\xi_y^2}} }[/math]  [math]\displaystyle{ \frac{1}{\sqrt{\omega_x^2+\omega_y^2}} }[/math]  [math]\displaystyle{ \frac{2\pi}{\sqrt{\nu_x^2+\nu_y^2}} }[/math]  This is the Hankel transform of r^{−1}, a 2D Fourier "selftransform".^{[53]} 
404  [math]\displaystyle{ \frac{i}{x+i y} }[/math]  [math]\displaystyle{ \frac{1}{\xi_x+i\xi_y} }[/math]  [math]\displaystyle{ \frac{1}{\omega_x+i\omega_y} }[/math]  [math]\displaystyle{ \frac{2\pi}{\nu_x+i\nu_y} }[/math] 
Formulas for general ndimensional functions
Function  Fourier transform unitary, ordinary frequency 
Fourier transform unitary, angular frequency 
Fourier transform nonunitary, angular frequency 
Remarks  

500  [math]\displaystyle{ f(\mathbf x)\, }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\boldsymbol \xi) = \\ &\int_{\mathbb{R}^n}f(\mathbf x) e^{2\pi i \mathbf x \cdot \boldsymbol \xi }\, d \mathbf x \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\boldsymbol \omega) = \\ &\frac{1}{{(2 \pi)}^\frac{n}{2}} \int_{\mathbb{R}^n} f(\mathbf x) e^{i \boldsymbol \omega \cdot \mathbf x}\, d \mathbf x \end{align} }[/math]  [math]\displaystyle{ \begin{align} &\hat{f}(\boldsymbol \nu) = \\ &\int_{\mathbb{R}^n}f(\mathbf x) e^{i \mathbf x \cdot \boldsymbol \nu }\, d \mathbf x \end{align} }[/math]  
501  [math]\displaystyle{ \chi_{[0,1]}(\mathbf x)\left(1\mathbf x^2\right)^\delta }[/math]  [math]\displaystyle{ \frac{\Gamma(\delta+1)}{\pi^\delta\,\boldsymbol \xi^{\frac{n}{2} + \delta}} J_{\frac{n}{2}+\delta}(2\pi\boldsymbol \xi) }[/math]  [math]\displaystyle{ 2^\delta \, \frac{\Gamma(\delta+1)}{\left\boldsymbol \omega\right^{\frac{n}{2}+\delta}} J_{\frac{n}{2}+\delta}(\boldsymbol \omega) }[/math]  [math]\displaystyle{ \frac{\Gamma(\delta+1)}{\pi^\delta} \left\frac{\boldsymbol \nu}{2\pi}\right^{\frac{n}{2}\delta} J_{\frac{n}{2}+\delta}(\!\boldsymbol \nu\!) }[/math]  The function χ_{[0, 1]} is the indicator function of the interval [0, 1]. The function Γ(x) is the gamma function. The function J_{n/2 + δ} is a Bessel function of the first kind, with order n/2 + δ. Taking n = 2 and δ = 0 produces 402.^{[55]} 
502  [math]\displaystyle{ \mathbf x^{\alpha}, \quad 0 \lt \operatorname{Re} \alpha \lt n. }[/math]  [math]\displaystyle{ \frac{(2\pi)^{\alpha}}{c_{n, \alpha}} \boldsymbol \xi^{(n  \alpha)} }[/math]  [math]\displaystyle{ \frac{(2\pi)^{\frac{n}{2}}}{c_{n, \alpha}} \boldsymbol \omega^{(n  \alpha)} }[/math]  [math]\displaystyle{ \frac{(2\pi)^{n}}{c_{n, \alpha}} \boldsymbol \nu^{(n  \alpha)} }[/math]  See Riesz potential where the constant is given by [math]\displaystyle{ c_{n, \alpha} = \pi^\frac{n}{2} 2^\alpha \frac{\Gamma\left(\frac{\alpha}{2}\right)}{\Gamma\left(\frac{n  \alpha}{2}\right)}. }[/math] The formula also holds for all α ≠ n, n + 2, ... by analytic continuation, but then the function and its Fourier transforms need to be understood as suitably regularized tempered distributions. See homogeneous distribution.^{[note 6]} 
503  [math]\displaystyle{ \frac{1}{\left\boldsymbol \sigma\right\left(2\pi\right)^\frac{n}{2}} e^{\frac{1}{2} \mathbf x^{\mathrm T} \boldsymbol \sigma^{\mathrm T} \boldsymbol \sigma^{1} \mathbf x} }[/math]  [math]\displaystyle{ e^{2\pi^2 \boldsymbol \xi^{\mathrm T} \boldsymbol \sigma \boldsymbol \sigma^{\mathrm T} \boldsymbol \xi} }[/math]  [math]\displaystyle{ (2\pi)^{\frac{n}{2}} e^{\frac{1}{2} \boldsymbol \omega^{\mathrm T} \boldsymbol \sigma \boldsymbol \sigma^{\mathrm T} \boldsymbol \omega} }[/math]  [math]\displaystyle{ e^{\frac{1}{2} \boldsymbol \nu^{\mathrm T} \boldsymbol \sigma \boldsymbol \sigma^{\mathrm T} \boldsymbol \nu} }[/math]  This is the formula for a multivariate normal distribution normalized to 1 with a mean of 0. Bold variables are vectors or matrices. Following the notation of the aforementioned page, Σ = σ σ^{T} and Σ^{−1} = σ^{−T} σ^{−1} 
504  [math]\displaystyle{ e^{2\pi\alpha\mathbf x} }[/math]  [math]\displaystyle{ \frac{c_n\alpha}{\left(\alpha^2+\boldsymbol{\xi}^2\right)^\frac{n+1}{2}} }[/math]  [math]\displaystyle{ \frac{c_n (2\pi)^{\frac{n+2}{2}} \alpha}{\left(4\pi^2\alpha^2+\boldsymbol{\omega}^2\right)^\frac{n+1}{2}} }[/math]  [math]\displaystyle{ \frac{c_n (2\pi)^{n+1} \alpha}{\left(4\pi^2\alpha^2+\boldsymbol{\nu}^2\right)^\frac{n+1}{2}} }[/math]  Here^{[56]} [math]\displaystyle{ c_n=\frac{\Gamma\left(\frac{n+1}{2}\right)}{\pi^\frac{n+1}{2}}, }[/math] Re(α) > 0 
See also
 Analog signal processing
 Beevers–Lipson strip
 ConstantQ transform
 Discrete Fourier transform
 Fast Fourier transform
 Fourier integral operator
 Fourier inversion theorem
 Fourier multiplier
 Fourier series
 Fourier sine transform
 Fourier–Deligne transform
 Fourier–Mukai transform
 Fractional Fourier transform
 Indirect Fourier transform
 Integral transform
 Laplace transform
 Leastsquares spectral analysis
 Linear canonical transform
 Mellin transform
 Multidimensional transform
 NGC 4622, especially the image NGC 4622 Fourier transform m = 2.
 Nonlocal operator
 Quantum Fourier transform
 Shorttime Fourier transform
 Spectral density
 Symbolic integration
 Time stretch dispersive Fourier transform
 Transform (mathematics)
Notes
 ↑ Depending on the application a Lebesgue integral, distributional, or other approach may be most appropriate.
 ↑ (Vretblad 2000) provides solid justification for these formal procedures without going too deeply into functional analysis or the theory of distributions.
 ↑ In relativistic quantum mechanics one encounters vectorvalued Fourier transforms of multicomponent wave functions. In quantum field theory, operatorvalued Fourier transforms of operatorvalued functions of spacetime are in frequent use, see for example (Greiner Reinhardt).
 ↑ Up to an imaginary constant factor whose magnitude depends on what Fourier transform convention is used.
 ↑ The direct command
fourier transform of cos(6*pi*t) exp(−pi*t^2)
would also work for Wolfram Alpha.  ↑ In Gelfand & Shilov 1964, p. 363, with the nonunitary conventions of this table, the transform of [math]\displaystyle{ \mathbf x^\lambda }[/math] is given to be
[math]\displaystyle{ 2^{\lambda+n}\pi^{\tfrac12 n}\frac{\Gamma\left(\frac{\lambda+n}{2}\right)}{\Gamma\left(\frac{\lambda}{2}\right)}\boldsymbol\nu^{\lambdan} }[/math]
from which this follows, with [math]\displaystyle{ \lambda=\alpha }[/math].
Citations
 ↑ Kaiser 1994, p. 29.
 ↑ Rahman 2011, p. 11.
 ↑ Fourier 1822, p. 525.
 ↑ Fourier 1878, p. 408.
 ↑ (Jordan 1883) proves on pp. 216–226 the Fourier integral theorem before studying Fourier series.
 ↑ Titchmarsh 1986, p. 1.
 ↑ Rahman 2011, p. 10.
 ↑ Oppenheim 1999, p. 58
 ↑ Folland 1989.
 ↑ Fourier 1822.
 ↑ Taneja 2008, p. 192.
 ↑ Lyons, Richard (November 2001). "Understanding Digital Signal Processing's Frequency Domain". https://www.researchgate.net/publication/261779218.
 ↑ ^{13.0} ^{13.1} Stein & Shakarchi 2003.
 ↑ ^{14.0} ^{14.1} ^{14.2} ^{14.3} ^{14.4} Pinsky 2002.
 ↑ ^{15.0} ^{15.1} ^{15.2} ^{15.3} ^{15.4} Katznelson 1976.
 ↑ ^{16.0} ^{16.1} ^{16.2} ^{16.3} ^{16.4} ^{16.5} Stein & Weiss 1971.
 ↑ Rudin 1987, p. 187.
 ↑ Rudin 1987, p. 186.
 ↑ ^{19.0} ^{19.1} Duoandikoetxea 2001.
 ↑ ^{20.0} ^{20.1} Boashash 2003.
 ↑ Condon 1937.
 ↑ Howe 1980.
 ↑ Paley & Wiener 1934.
 ↑ Gelfand & Vilenkin 1964.
 ↑ Kirillov & Gvishiani 1982.
 ↑ Clozel & Delorme 1985, pp. 331–333.
 ↑ de Groot & Mazur 1984, p. 146.
 ↑ Champeney 1987, p. 80.
 ↑ ^{29.0} ^{29.1} ^{29.2} Kolmogorov & Fomin 1999.
 ↑ Wiener 1949.
 ↑ Champeney 1987, p. 63.
 ↑ Widder & Wiener 1938, p. 537.
 ↑ Pinsky 2002, p. 131.
 ↑ Stein & Shakarchi 2003, p. 158.
 ↑ Chatfield 2004, p. 113.
 ↑ Fourier 1822, p. 441.
 ↑ Poincaré 1895, p. 102.
 ↑ Whittaker & Watson 1927, p. 188.
 ↑ Grafakos 2004.
 ↑ Grafakos & Teschl 2013.
 ↑ "Applied Fourier Analysis and Elements of Modern Signal Processing Lecture 3". January 12, 2016. https://statweb.stanford.edu/~candes/teaching/math262/Lectures/Lecture03.pdf.
 ↑ Stein & Weiss 1971, Thm. 2.3.
 ↑ Pinsky 2002, p. 256.
 ↑ Scarfone, A.M. (2017). "κ deformed Fourier transform" (in en). Physica A: Statistical Mechanics and Its Applications 480: 63–78. doi:10.1016/j.physa.2017.03.036. https://linkinghub.elsevier.com/retrieve/pii/S0378437117302881.
 ↑ Scarfone, Antonio (20150504). "On the κDeformed Cyclic Functions and the Generalized Fourier Series in the Framework of the κAlgebra" (in en). Entropy 17 (5): 2812–2833. doi:10.3390/e17052812. ISSN 10994300.
 ↑ Hewitt & Ross 1970, Chapter 8.
 ↑ Knapp 2001.
 ↑ Gradshteyn et al. 2015.
 ↑ Press et al. 1992.
 ↑ Bailey & Swarztrauber 1994.
 ↑ Lado 1971.
 ↑ Simonen & Olkkonen 1985.
 ↑ ^{53.0} ^{53.1} Jr, Roger L. Easton (2010) (in en). Fourier Methods in Imaging. John Wiley & Sons. ISBN 9780470689837. https://books.google.com/books?id=wCoDDQAAQBAJ. Retrieved 26 May 2020.
 ↑ Stein & Weiss 1971, Thm. IV.3.3.
 ↑ Stein & Weiss 1971, Thm. 4.15.
 ↑ Stein & Weiss 1971, p. 6.
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External links
 Encyclopedia of Mathematics
 Weisstein, Eric W.. "Fourier Transform". http://mathworld.wolfram.com/FourierTransform.html.
Original source: https://en.wikipedia.org/wiki/Fourier transform.
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