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Fourier series

From Wikipedia, the free encyclopedia
Decomposition of periodic functions
"Fourier's theorem" redirects here. For the number of real roots of a polynomial, seeBudan's theorem § Fourier's theorem.
Fourier transforms

AFourier series (/ˈfʊri,-iər/[1]) is aseries expansion of aperiodic function into a sum oftrigonometric functions. The Fourier series is an example of atrigonometric series.[2] By expressing a function as a sum of sines and cosines, many problems involving the function become easier to analyze because trigonometric functions are well understood. For example, Fourier series were first used byJoseph Fourier to find solutions to theheat equation. This application is possible because the derivatives of trigonometric functions fall into simple patterns. Fourier series cannot be used to approximate arbitrary functions, because most functions have infinitely many terms in their Fourier series, and the series do not alwaysconverge. Well-behaved functions, for examplesmooth functions, have Fourier series that converge to the original function. The coefficients of the Fourier series are determined byintegrals of the function multiplied by trigonometric functions, described inFourier series § Definition.

The study of theconvergence of Fourier series focus on the behaviors of thepartial sums, which means studying the behavior of the sum as more and more terms from the series are summed. The figures below illustrate some partial Fourier series results for the components of asquare wave.

  • A square wave (represented as the blue dot) is approximated by its sixth partial sum (represented as the purple dot), formed by summing the first six terms (represented as arrows) of the square wave's Fourier series. Each arrow starts at the vertical sum of all the arrows to its left (i.e. the previous partial sum).
    A square wave (represented as the blue dot) is approximated by its sixth partial sum (represented as the purple dot), formed by summing the first six terms (represented as arrows) of the square wave's Fourier series. Each arrow starts at the vertical sum of all the arrows to its left (i.e. the previous partial sum).
  • The first four partial sums of the Fourier series for a square wave. As more harmonics are added, the partial sums converge to (become more and more like) the square wave.
    The first four partial sums of the Fourier series for asquare wave. As more harmonics are added, the partial sumsconverge to (become more and more like) the square wave.
  • Function '"`UNIQ--postMath-00000001-QINU`"' (in red) is a Fourier series sum of 6 harmonically related sine waves (in blue). Its Fourier transform '"`UNIQ--postMath-00000002-QINU`"' is a frequency-domain representation that reveals the amplitudes of the summed sine waves.
    Functions6(x){\displaystyle s_{6}(x)} (in red) is a Fourier series sum of 6 harmonically related sine waves (in blue). Its Fourier transformS(f){\displaystyle S(f)} is a frequency-domain representation that reveals the amplitudes of the summed sine waves.

Fourier series are closely related to theFourier transform, a more general tool that can even find the frequency information for functions that arenot periodic. Periodic functions can be identified with functions on a circle; for this reason Fourier series are the subject ofFourier analysis on thecircle group, denoted byT{\displaystyle \mathbb {T} } orS1{\displaystyle S_{1}}. The Fourier transform is also part ofFourier analysis, but is defined for functions onRn{\displaystyle \mathbb {R} ^{n}}.

Since Fourier's time, many different approaches to defining and understanding the concept of Fourier series have been discovered, all of which are consistent with one another, but each of which emphasizes different aspects of the topic. Some of the more powerful and elegant approaches are based on mathematical ideas and tools that were not available in Fourier's time. Fourier originally defined the Fourier series forreal-valued functions of real arguments, and used thesine and cosine functions in the decomposition. Many otherFourier-related transforms have since been defined, extending his initial idea to many applications and birthing anarea of mathematics calledFourier analysis.

History

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See also:Fourier analysis § History

The Fourier series is named in honor ofJean-Baptiste Joseph Fourier (1768–1830), who made important contributions to the study oftrigonometric series, after preliminary investigations byLeonhard Euler,Jean le Rond d'Alembert, andDaniel Bernoulli.[A] Fourier introduced the series for the purpose of solving theheat equation in a metal plate, publishing his initial results in his 1807Mémoire sur la propagation de la chaleur dans les corps solides (Treatise on the propagation of heat in solid bodies), and publishing hisThéorie analytique de la chaleur (Analytical theory of heat) in 1822. TheMémoire introduced Fourier analysis, specifically Fourier series. Through Fourier's research the fact was established that an arbitrary (at first, continuous[3] and later generalized to anypiecewise-smooth[4]) function can be represented by a trigonometric series. The first announcement of this great discovery was made by Fourier in 1807, before theFrench Academy.[5] Early ideas of decomposing a periodic function into the sum of simple oscillating functions date back to the 3rd century BC, when ancient astronomers proposed an empiric model of planetary motions, based ondeferents and epicycles.

Independently of Fourier, astronomerFriedrich Wilhelm Bessel introduced Fourier series to solveKepler's equation. His work was published in 1819, unaware of Fourier's work which remained unpublished until 1822.[6]

Theheat equation is apartial differential equation. Prior to Fourier's work, no solution to the heat equation was known in the general case, although particular solutions were known if the heat source behaved in a simple way, in particular, if the heat source was asine orcosine wave. These simple solutions are now sometimes calledeigensolutions. Fourier's idea was to model a complicated heat source as a superposition (orlinear combination) of simple sine and cosine waves, and to write thesolution as a superposition of the correspondingeigensolutions. This superposition or linear combination is called the Fourier series.

From a modern point of view, Fourier's results are somewhat informal, due to the lack of a precise notion offunction andintegral in the early nineteenth century. Later,Peter Gustav Lejeune Dirichlet[7] andBernhard Riemann[8][9][10] expressed Fourier's results with greater precision and formality.

Although the original motivation was to solve the heat equation, it later became obvious that the same techniques could be applied to a wide array of mathematical and physical problems, and especially those involving linear differential equations with constant coefficients, for which the eigensolutions aresinusoids. The Fourier series has many such applications inelectrical engineering,vibration analysis,acoustics,optics,signal processing,image processing,quantum mechanics,econometrics,[11]shell theory,[12] etc.

Beginnings

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Joseph Fourier wrote[13]

φ(y)=a0cosπy2+a1cos3πy2+a2cos5πy2+.{\displaystyle \varphi (y)=a_{0}\cos {\frac {\pi y}{2}}+a_{1}\cos 3{\frac {\pi y}{2}}+a_{2}\cos 5{\frac {\pi y}{2}}+\cdots .}

Multiplying both sides bycos(2k+1)πy2{\displaystyle \cos(2k+1){\frac {\pi y}{2}}}, and then integrating fromy=1{\displaystyle y=-1} toy=+1{\displaystyle y=+1} yields:

ak=11φ(y)cos(2k+1)πy2dy.{\displaystyle a_{k}=\int _{-1}^{1}\varphi (y)\cos(2k+1){\frac {\pi y}{2}}\,dy.}

— Joseph Fourier,Mémoire sur la propagation de la chaleur dans les corps solides (1807).

This immediately gives any coefficientak of thetrigonometric series for φ(y) for any function which has such an expansion. It works because if φ has such an expansion, then (under suitable convergence assumptions) the integral11φ(y)cos(2k+1)πy2dy=11(acosπy2cos(2k+1)πy2+acos3πy2cos(2k+1)πy2+)dy{\displaystyle {\begin{aligned}&\int _{-1}^{1}\varphi (y)\cos(2k+1){\frac {\pi y}{2}}\,dy\\&=\int _{-1}^{1}\left(a\cos {\frac {\pi y}{2}}\cos(2k+1){\frac {\pi y}{2}}+a'\cos 3{\frac {\pi y}{2}}\cos(2k+1){\frac {\pi y}{2}}+\cdots \right)\,dy\end{aligned}}}can be carried out term-by-term. But all terms involvingcos(2j+1)πy2cos(2k+1)πy2{\displaystyle \cos(2j+1){\frac {\pi y}{2}}\cos(2k+1){\frac {\pi y}{2}}} forjk vanish when integrated from −1 to 1, leaving only thekth{\displaystyle k^{\text{th}}} term, which is1.

In these few lines, which are close to the modernformalism used in Fourier series, Fourier revolutionized both mathematics and physics. Although similar trigonometric series were previously used byEuler,d'Alembert,Daniel Bernoulli andGauss, Fourier believed that such trigonometric series could represent any arbitrary function. In what sense that is actually true is a somewhat subtle issue and the attempts over many years to clarify this idea have led to important discoveries in the theories ofconvergence,function spaces, andharmonic analysis.

When Fourier submitted a later competition essay in 1811, the committee (which includedLagrange,Laplace,Malus andLegendre, among others) concluded: "...the manner in which the author arrives at these equations is not exempt of difficulties and...his analysis to integrate them still leaves something to be desired on the score of generality and evenrigour".[14]

Fourier's motivation

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This resulting heat distribution in a metal plate is easily solved using Fourier's method

The Fourier series expansion of the sawtooth function (below) looks more complicated than the simple formulas(x)=xπ{\displaystyle s(x)={\tfrac {x}{\pi }}}, so it is not immediately apparent why one would need the Fourier series. While there are many applications, Fourier's motivation was in solving theheat equation. For example, consider a metal plate in the shape of a square whose sides measureπ{\displaystyle \pi } meters, with coordinates(x,y)[0,π]×[0,π]{\displaystyle (x,y)\in [0,\pi ]\times [0,\pi ]}. If there is no heat source within the plate, and if three of the four sides are held at 0 degrees Celsius, while the fourth side, given byy=π{\displaystyle y=\pi }, is maintained at the temperature gradientT(x,π)=x{\displaystyle T(x,\pi )=x} degrees Celsius, forx{\displaystyle x} in(0,π){\displaystyle (0,\pi )}, then one can show that the stationary heat distribution (or the heat distribution after a long time has elapsed) is given by

T(x,y)=2n=1(1)n+1nsin(nx)sinh(ny)sinh(nπ).{\displaystyle T(x,y)=2\sum _{n=1}^{\infty }{\frac {(-1)^{n+1}}{n}}\sin(nx){\sinh(ny) \over \sinh(n\pi )}.}

Here, sinh is thehyperbolic sine function. This solution of the heat equation is obtained by multiplying each term of the equation fromAnalysis § Example bysinh(ny)/sinh(nπ){\displaystyle \sinh(ny)/\sinh(n\pi )}. While our example functions(x){\displaystyle s(x)} seems to have a needlessly complicated Fourier series, the heat distributionT(x,y){\displaystyle T(x,y)} is nontrivial. The functionT{\displaystyle T} cannot be written as aclosed-form expression. This method of solving the heat problem was made possible by Fourier's work.

Other applications

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Another application is to solve theBasel problem by usingParseval's theorem. The example generalizes and one may computeζ(2n), for any positive integern.

Definition

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The Fourier series of a complex-valuedP-periodic functions(x){\displaystyle s(x)}, integrable over the interval[0,P]{\displaystyle [0,P]} on the real line, is defined as atrigonometric series of the formn=cnei2πnPx,{\displaystyle \sum _{n=-\infty }^{\infty }c_{n}e^{i2\pi {\tfrac {n}{P}}x},}such that theFourier coefficientscn{\displaystyle c_{n}} are complex numbers defined by the integral[15][16]cn=1P0Ps(x) ei2πnPxdx.{\displaystyle c_{n}={\frac {1}{P}}\int _{0}^{P}s(x)\ e^{-i2\pi {\tfrac {n}{P}}x}\,dx.}The series does not necessarily converge (in thepointwise sense) and, even if it does, it is not necessarily equal tos(x){\displaystyle s(x)}. Only when certain conditions are satisfied (e.g. ifs(x){\displaystyle s(x)} is continuously differentiable) does the Fourier series converge tos(x){\displaystyle s(x)}, i.e.,s(x)=n=cnei2πnPx.{\displaystyle s(x)=\sum _{n=-\infty }^{\infty }c_{n}e^{i2\pi {\tfrac {n}{P}}x}.}For functions satisfying theDirichlet sufficiency conditions, pointwise convergence holds.[17] However, these are notnecessary conditions and there are many theorems about different types ofconvergence of Fourier series (e.g.uniform convergence ormean convergence).[18] The definition naturally extends to the Fourier series of a (periodic)distributions{\displaystyle s} (also calledFourier-Schwartz series).[19] Then the Fourier series converges tos(x){\displaystyle s(x)} in the distribution sense.[20]

The process of determining the Fourier coefficients of a given function or signal is calledanalysis, while forming the associated trigonometric series (or its various approximations) is calledsynthesis.

Synthesis

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A Fourier series can be written in several equivalent forms, shown here as theNth{\displaystyle N^{\text{th}}}partial sumssN(x){\displaystyle s_{N}(x)} of the Fourier series ofs(x){\displaystyle s(x)}:[21]

Fig 1. The top graph shows a non-periodic functions(x){\displaystyle s(x)} in blue defined only over the red interval from 0 toP. The function can be analyzed over this interval to produce the Fourier series in the bottom graph. The Fourier series is always a periodic function, even if original functions(x){\displaystyle s(x)} is not.
Sine-cosine form
sN(x)=a0+n=1N(ancos(2πnPx)+bnsin(2πnPx)){\displaystyle s_{N}(x)=a_{0}+\sum _{n=1}^{N}\left(a_{n}\cos \left(2\pi {\tfrac {n}{P}}x\right)+b_{n}\sin \left(2\pi {\tfrac {n}{P}}x\right)\right)}    Eq.1


Exponential form
sN(x)=n=NNcn ei2πnPx{\displaystyle s_{N}(x)=\sum _{n=-N}^{N}c_{n}\ e^{i2\pi {\tfrac {n}{P}}x}}    Eq.2

The harmonics are indexed by an integer,n,{\displaystyle n,} which is also the number of cycles the corresponding sinusoids make in intervalP{\displaystyle P}. Therefore, the sinusoids have:

These series can represent functions that are just a sum of one or more frequencies in theharmonic spectrum. In the limitN{\displaystyle N\to \infty }, a trigonometric series can also represent the intermediate frequencies or non-sinusoidal functions because of the infinite number of terms.

Analysis

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The coefficients can be given/assumed, such as a music synthesizer or time samples of a waveform. In the latter case, the exponential form of Fourier series synthesizes adiscrete-time Fourier transform where variablex{\displaystyle x} represents frequency instead of time. In general, the coefficients are determined byanalysis of a given functions(x){\displaystyle s(x)} whosedomain of definition is an interval of lengthP{\displaystyle P}.[B][22]

Fourier coefficients
a0=1PPs(x)dxan=2PPs(x)cos(2πnPx)dx, for n1bn=2PPs(x)sin(2πnPx)dx, for n1{\displaystyle {\begin{aligned}&a_{0}={\frac {1}{P}}\int _{P}s(x)\,dx&\\&a_{n}={\frac {2}{P}}\int _{P}s(x)\cos \left(2\pi {\tfrac {n}{P}}x\right)\,dx,\ &{\textrm {for}}~n\geq 1\\&b_{n}={\frac {2}{P}}\int _{P}s(x)\sin \left(2\pi {\tfrac {n}{P}}x\right)\,dx,\ &{\text{for}}~n\geq 1\\\end{aligned}}}    Eq.3

The2P{\displaystyle {\tfrac {2}{P}}} scale factor follows from substitutingEq.1 intoEq.3 and utilizing theorthogonality of the trigonometric system.[23] The equivalence ofEq.1 andEq.2 follows fromEuler's formulacosx=eix+eix2,sinx=eixeix2i,{\displaystyle \cos x={\frac {e^{ix}+e^{-ix}}{2}},\quad \sin x={\frac {e^{ix}-e^{-ix}}{2i}},}resulting in:

Exponential form coefficients

cn={12(anibn)if n>0,anif n=0,12(an+ibn)if n<0,{\displaystyle c_{n}={\begin{cases}{\tfrac {1}{2}}(a_{n}-ib_{n})&{\text{if }}n>0,\\a_{n}&{\text{if }}n=0,\\{\tfrac {1}{2}}(a_{-n}+ib_{-n})&{\text{if }}n<0,\\\end{cases}}}

withc0{\displaystyle c_{0}} being themean value ofs{\displaystyle s} on the intervalP{\displaystyle P}.[24] Conversely:

Inverse relationships

a0=c0an=cn+cnfor n>0bn=i(cncn)for n>0{\displaystyle {\begin{aligned}a_{0}&=c_{0}&\\a_{n}&=c_{n}+c_{-n}\qquad &{\textrm {for}}~n>0\\b_{n}&=i(c_{n}-c_{-n})\qquad &{\textrm {for}}~n>0\end{aligned}}}

Example

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Plot of thesawtooth wave, a periodic continuation of the linear functions(x)=x/π{\displaystyle s(x)=x/\pi } on the interval(π,π]{\displaystyle (-\pi ,\pi ]}
Animated plot of the first five successive partial Fourier series

Consider a sawtooth function:s(x)=s(x+2πk)=xπ,forπ<x<π, and kZ.{\displaystyle s(x)=s(x+2\pi k)={\frac {x}{\pi }},\quad \mathrm {for} -\pi <x<\pi ,{\text{ and }}k\in \mathbb {Z} .}In this case, the Fourier coefficients are given bya0=0.an=1πππs(x)cos(nx)dx=0,n1.bn=1πππs(x)sin(nx)dx=2πncos(nπ)+2π2n2sin(nπ)=2(1)n+1πn,n1.{\displaystyle {\begin{aligned}a_{0}&=0.\\a_{n}&={\frac {1}{\pi }}\int _{-\pi }^{\pi }s(x)\cos(nx)\,dx=0,\quad n\geq 1.\\b_{n}&={\frac {1}{\pi }}\int _{-\pi }^{\pi }s(x)\sin(nx)\,dx\\&=-{\frac {2}{\pi n}}\cos(n\pi )+{\frac {2}{\pi ^{2}n^{2}}}\sin(n\pi )\\&={\frac {2\,(-1)^{n+1}}{\pi n}},\quad n\geq 1.\end{aligned}}}It can be shown that the Fourier series converges tos(x){\displaystyle s(x)} at every pointx{\displaystyle x} wheres{\displaystyle s} is differentiable, and therefore:s(x)=a0+n=1[ancos(nx)+bnsin(nx)]=2πn=1(1)n+1nsin(nx),for (xπ) is not a multiple of 2π.{\displaystyle {\begin{aligned}s(x)&=a_{0}+\sum _{n=1}^{\infty }\left[a_{n}\cos \left(nx\right)+b_{n}sin\left(nx\right)\right]\\[4pt]&={\frac {2}{\pi }}\sum _{n=1}^{\infty }{\frac {(-1)^{n+1}}{n}}\sin(nx),\quad \mathrm {for} \ (x-\pi )\ {\text{is not a multiple of}}\ 2\pi .\end{aligned}}}Whenx=π{\displaystyle x=\pi }, the Fourier series converges to 0, which is the half-sum of the left- and right-limit ofs{\displaystyle s} atx=π{\displaystyle x=\pi }. This is a particular instance of theDirichlet theorem for Fourier series.

This example leads to a solution of theBasel problem.

Amplitude-phase form

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If the functions(x){\displaystyle s(x)} is real-valued then the Fourier series can also be represented as[25]

Amplitude-phase form
sN(x)=A0+n=1NAncos(2πnPxφn){\displaystyle s_{N}(x)=A_{0}+\sum _{n=1}^{N}A_{n}\cos \left(2\pi {\tfrac {n}{P}}x-\varphi _{n}\right)}    Eq.4

whereAn{\displaystyle A_{n}} is theamplitude andφn{\displaystyle \varphi _{n}} is thephase shift of thenth{\displaystyle n^{th}} harmonic.

The equivalence ofEq.4 andEq.1 follows from thetrigonometric identity:cos(2πnPxφn)=cos(φn)cos(2πnPx)+sin(φn)sin(2πnPx),{\displaystyle \cos \left(2\pi {\tfrac {n}{P}}x-\varphi _{n}\right)=\cos(\varphi _{n})\cos \left(2\pi {\tfrac {n}{P}}x\right)+\sin(\varphi _{n})\sin \left(2\pi {\tfrac {n}{P}}x\right),}which implies[26]an=Ancos(φn)andbn=Ansin(φn){\displaystyle a_{n}=A_{n}\cos(\varphi _{n})\quad {\text{and}}\quad b_{n}=A_{n}\sin(\varphi _{n})}

Fig 2. The blue curve is the cross-correlation of a square wave and a cosine template, as the phase lag of the template varies over one cycle. The amplitude and phase at the maximum value are the polar coordinates of one harmonic in the Fourier series expansion of the square wave. The corresponding rectangular coordinates can be determined by evaluating the correlation at just two samples separated by 90°.

are therectangular coordinates of a vector withpolar coordinatesAn{\displaystyle A_{n}} andφn{\displaystyle \varphi _{n}} given byAn=an2+bn2andφn=Arg(cn)=atan2(bn,an){\displaystyle A_{n}={\sqrt {a_{n}^{2}+b_{n}^{2}}}\quad {\text{and}}\quad \varphi _{n}=\operatorname {Arg} (c_{n})=\operatorname {atan2} (b_{n},a_{n})} whereArg(cn){\displaystyle \operatorname {Arg} (c_{n})} is theargument ofcn{\displaystyle c_{n}}.

An example of determining the parameterφn{\displaystyle \varphi _{n}} for one value ofn{\displaystyle n} is shown in Figure 2. It is the value ofφ{\displaystyle \varphi } at the maximum correlation betweens(x){\displaystyle s(x)} and a cosinetemplate,cos(2πnPxφ){\displaystyle \cos(2\pi {\tfrac {n}{P}}x-\varphi )}. The blue graph is thecross-correlation function, also known as amatched filter:

X(φ)=Ps(x)cos(2πnPxφ)dxφ[0,2π]=cos(φ)Ps(x)cos(2πnPx)dxX(0)+sin(φ)Ps(x)sin(2πnPx)dxX(π/2){\displaystyle {\begin{aligned}\mathrm {X} (\varphi )&=\int _{P}s(x)\cdot \cos \left(2\pi {\tfrac {n}{P}}x-\varphi \right)\,dx\quad \varphi \in \left[0,2\pi \right]\\&=\cos(\varphi )\underbrace {\int _{P}s(x)\cdot \cos \left(2\pi {\tfrac {n}{P}}x\right)dx} _{X(0)}+\sin(\varphi )\underbrace {\int _{P}s(x)\cdot \sin \left(2\pi {\tfrac {n}{P}}x\right)dx} _{X(\pi /2)}\end{aligned}}}

Fortunately, it is not necessary to evaluate this entire function, because its derivative is zero at the maximum:X(φ)=sin(φ)X(0)cos(φ)X(π/2)=0,at φ=φn.{\displaystyle X'(\varphi )=\sin(\varphi )\cdot X(0)-\cos(\varphi )\cdot X(\pi /2)=0,\quad {\textrm {at}}\ \varphi =\varphi _{n}.} Henceφnarctan(bn/an)=arctan(X(π/2)/X(0)).{\displaystyle \varphi _{n}\equiv \arctan(b_{n}/a_{n})=\arctan(X(\pi /2)/X(0)).}

Common notations

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The notationcn{\displaystyle c_{n}} is inadequate for discussing the Fourier coefficients of several different functions. Therefore, it is customarily replaced by a modified form of the function (s,{\displaystyle s,} in this case), such ass^(n){\displaystyle {\widehat {s}}(n)} orS[n],{\displaystyle S[n],} and functional notation often replaces subscripting:

s(x)=n=s^(n)ei2πnPxcommon mathematics notation=n=S[n]ei2πnPxcommon engineering notation{\displaystyle {\begin{aligned}s(x)&=\sum _{n=-\infty }^{\infty }{\widehat {s}}(n)\cdot e^{i2\pi {\tfrac {n}{P}}x}&&\scriptstyle {\text{common mathematics notation}}\\&=\sum _{n=-\infty }^{\infty }S[n]\cdot e^{i2\pi {\tfrac {n}{P}}x}&&\scriptstyle {\text{common engineering notation}}\end{aligned}}}

In engineering, particularly when the variablex{\displaystyle x} represents time, the coefficient sequence is called afrequency domain representation. Square brackets are often used to emphasize that the domain of this function is a discrete set of frequencies.

Another commonly used frequency domain representation uses the Fourier series coefficients tomodulate aDirac comb:

S(f)  n=S[n]δ(fnP),{\displaystyle S(f)\ \triangleq \ \sum _{n=-\infty }^{\infty }S[n]\cdot \delta \left(f-{\frac {n}{P}}\right),}

wheref{\displaystyle f} represents a continuous frequency domain. When variablex{\displaystyle x} has units of seconds,f{\displaystyle f} has units ofhertz. The "teeth" of the comb are spaced at multiples (i.e.harmonics) of1P{\displaystyle {\tfrac {1}{P}}}, which is called thefundamental frequency.s(x){\displaystyle s(x)} can be recovered from this representation by aninverse Fourier transform:

F1{S(f)}=(n=S[n]δ(fnP))ei2πfxdf,=n=S[n]δ(fnP)ei2πfxdf,=n=S[n]ei2πnPx   s(x).{\displaystyle {\begin{aligned}{\mathcal {F}}^{-1}\{S(f)\}&=\int _{-\infty }^{\infty }\left(\sum _{n=-\infty }^{\infty }S[n]\cdot \delta \left(f-{\frac {n}{P}}\right)\right)e^{i2\pi fx}\,df,\\[6pt]&=\sum _{n=-\infty }^{\infty }S[n]\cdot \int _{-\infty }^{\infty }\delta \left(f-{\frac {n}{P}}\right)e^{i2\pi fx}\,df,\\[6pt]&=\sum _{n=-\infty }^{\infty }S[n]\cdot e^{i2\pi {\tfrac {n}{P}}x}\ \ \triangleq \ s(x).\end{aligned}}}

The constructed functionS(f){\displaystyle S(f)} is therefore commonly referred to as aFourier transform, even though the Fourier integral of a periodic function is not convergent at the harmonic frequencies.[C]

Table of common Fourier series

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Some common pairs of periodic functions and their Fourier series coefficients are shown in the table below.

Time domain

s(x){\displaystyle s(x)}

PlotFrequency domain (sine-cosine form)

a0anfor n1bnfor n1{\displaystyle {\begin{aligned}&a_{0}\\&a_{n}\quad {\text{for }}n\geq 1\\&b_{n}\quad {\text{for }}n\geq 1\end{aligned}}}

RemarksReference
s(x)=A|sin(2πPx)|for 0x<P{\displaystyle s(x)=A\left|\sin \left({\frac {2\pi }{P}}x\right)\right|\quad {\text{for }}0\leq x<P}
a0=2Aπan={4Aπ1n21n even0n oddbn=0{\displaystyle {\begin{aligned}a_{0}=&{\frac {2A}{\pi }}\\a_{n}=&{\begin{cases}{\frac {-4A}{\pi }}{\frac {1}{n^{2}-1}}&\quad n{\text{ even}}\\0&\quad n{\text{ odd}}\end{cases}}\\b_{n}=&0\\\end{aligned}}}Full-wave rectified sine[27]: p. 193 
s(x)={Asin(2πPx)for 0x<P/20for P/2x<P{\displaystyle s(x)={\begin{cases}A\sin \left({\frac {2\pi }{P}}x\right)&\quad {\text{for }}0\leq x<P/2\\0&\quad {\text{for }}P/2\leq x<P\\\end{cases}}}
a0=Aπan={2Aπ1n21n even0n oddbn={A2n=10n>1{\displaystyle {\begin{aligned}a_{0}=&{\frac {A}{\pi }}\\a_{n}=&{\begin{cases}{\frac {-2A}{\pi }}{\frac {1}{n^{2}-1}}&\quad n{\text{ even}}\\0&\quad n{\text{ odd}}\end{cases}}\\b_{n}=&{\begin{cases}{\frac {A}{2}}&\quad n=1\\0&\quad n>1\end{cases}}\\\end{aligned}}}Half-wave rectified sine[27]: p.193 
s(x)={Afor 0x<DP0for DPx<P{\displaystyle s(x)={\begin{cases}A&\quad {\text{for }}0\leq x<D\cdot P\\0&\quad {\text{for }}D\cdot P\leq x<P\\\end{cases}}}
a0=ADan=Anπsin(2πnD)bn=2Anπ(sin(πnD))2{\displaystyle {\begin{aligned}a_{0}=&AD\\a_{n}=&{\frac {A}{n\pi }}\sin \left(2\pi nD\right)\\b_{n}=&{\frac {2A}{n\pi }}\left(\sin \left(\pi nD\right)\right)^{2}\\\end{aligned}}}0D1{\displaystyle 0\leq D\leq 1}
s(x)=AxPfor 0x<P{\displaystyle s(x)={\frac {Ax}{P}}\quad {\text{for }}0\leq x<P}
a0=A2an=0bn=Anπ{\displaystyle {\begin{aligned}a_{0}=&{\frac {A}{2}}\\a_{n}=&0\\b_{n}=&{\frac {-A}{n\pi }}\\\end{aligned}}}[27]: p.192 
s(x)=AAxPfor 0x<P{\displaystyle s(x)=A-{\frac {Ax}{P}}\quad {\text{for }}0\leq x<P}
a0=A2an=0bn=Anπ{\displaystyle {\begin{aligned}a_{0}=&{\frac {A}{2}}\\a_{n}=&0\\b_{n}=&{\frac {A}{n\pi }}\\\end{aligned}}}[27]: p.192 
s(x)=4AP2(xP2)2for 0x<P{\displaystyle s(x)={\frac {4A}{P^{2}}}\left(x-{\frac {P}{2}}\right)^{2}\quad {\text{for }}0\leq x<P}
a0=A3an=4Aπ2n2bn=0{\displaystyle {\begin{aligned}a_{0}=&{\frac {A}{3}}\\a_{n}=&{\frac {4A}{\pi ^{2}n^{2}}}\\b_{n}=&0\\\end{aligned}}}[27]: p.193 

Table of basic transformation rules

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See also:Fourier transform § Basic properties

This table shows some mathematical operations in the time domain and the corresponding effect in the Fourier series coefficients. Notation:

PropertyTime domainFrequency domain (exponential form)RemarksReference
Linearityas(x)+br(x){\displaystyle a\cdot s(x)+b\cdot r(x)}aS[n]+bR[n]{\displaystyle a\cdot S[n]+b\cdot R[n]}a,bC{\displaystyle a,b\in \mathbb {C} }
Time reversal / Frequency reversals(x){\displaystyle s(-x)}S[n]{\displaystyle S[-n]}[28]: p. 610 
Time conjugations(x){\displaystyle s^{*}(x)}S[n]{\displaystyle S^{*}[-n]}[28]: p. 610 
Time reversal & conjugations(x){\displaystyle s^{*}(-x)}S[n]{\displaystyle S^{*}[n]}
Real part in timeRe(s(x)){\displaystyle \operatorname {Re} {(s(x))}}12(S[n]+S[n]){\displaystyle {\frac {1}{2}}(S[n]+S^{*}[-n])}
Imaginary part in timeIm(s(x)){\displaystyle \operatorname {Im} {(s(x))}}12i(S[n]S[n]){\displaystyle {\frac {1}{2i}}(S[n]-S^{*}[-n])}
Real part in frequency12(s(x)+s(x)){\displaystyle {\frac {1}{2}}(s(x)+s^{*}(-x))}Re(S[n]){\displaystyle \operatorname {Re} {(S[n])}}
Imaginary part in frequency12i(s(x)s(x)){\displaystyle {\frac {1}{2i}}(s(x)-s^{*}(-x))}Im(S[n]){\displaystyle \operatorname {Im} {(S[n])}}
Shift in time / Modulation in frequencys(xx0){\displaystyle s(x-x_{0})}S[n]ei2πx0Pn{\displaystyle S[n]\cdot e^{-i2\pi {\tfrac {x_{0}}{P}}n}}x0R{\displaystyle x_{0}\in \mathbb {R} }[28]: p.610 
Shift in frequency / Modulation in times(x)ei2πn0Px{\displaystyle s(x)\cdot e^{i2\pi {\frac {n_{0}}{P}}x}}S[nn0]{\displaystyle S[n-n_{0}]\!}n0Z{\displaystyle n_{0}\in \mathbb {Z} }[28]: p. 610 

Properties

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Symmetry relations

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When the real and imaginary parts of a complex function are decomposed into theireven and odd parts, there are four components, denoted below by the subscriptsRE, RO, IE, and IO. And there is a one-to-one mapping between the four components of a complex time function and the four components of its complex frequency transform:[29][30]

Time domains=sRE+sRO+i sIE+i sIOFF  F  F  FFrequency domainS=SRE+i SIO+i SIE+SRO{\displaystyle {\begin{array}{rlcccccccc}{\mathsf {Time\ domain}}&s&=&s_{\mathrm {RE} }&+&s_{\mathrm {RO} }&+&i\ s_{\mathrm {IE} }&+&i\ s_{\mathrm {IO} }\\&{\Bigg \Updownarrow }{\mathcal {F}}&&{\Bigg \Updownarrow }{\mathcal {F}}&&\ \ {\Bigg \Updownarrow }{\mathcal {F}}&&\ \ {\Bigg \Updownarrow }{\mathcal {F}}&&\ \ {\Bigg \Updownarrow }{\mathcal {F}}\\{\mathsf {Frequency\ domain}}&S&=&S_{\mathrm {RE} }&+&i\ S_{\mathrm {IO} }\,&+&i\ S_{\mathrm {IE} }&+&S_{\mathrm {RO} }\end{array}}}

From this, various relationships are apparent, for example:

Riemann–Lebesgue lemma

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Main article:Riemann–Lebesgue lemma

IfS{\displaystyle S} isintegrable,lim|n|S[n]=0{\textstyle \lim _{|n|\to \infty }S[n]=0},limn+an=0{\textstyle \lim _{n\to +\infty }a_{n}=0} andlimn+bn=0.{\textstyle \lim _{n\to +\infty }b_{n}=0.}

Parseval's theorem

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Main article:Parseval's theorem

Ifs{\displaystyle s} belongs toL2(P){\displaystyle L^{2}(P)} (periodic over an interval of lengthP{\displaystyle P}) then:1PP|s(x)|2dx=n=|S[n]|2.{\displaystyle {\frac {1}{P}}\int _{P}|s(x)|^{2}\,dx=\sum _{n=-\infty }^{\infty }{\Bigl |}S[n]{\Bigr |}^{2}.}

Plancherel's theorem

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Main article:Plancherel theorem

Ifc0,c±1,c±2,{\displaystyle c_{0},\,c_{\pm 1},\,c_{\pm 2},\ldots } are coefficients andn=|cn|2<{\textstyle \sum _{n=-\infty }^{\infty }|c_{n}|^{2}<\infty } then there is a unique functionsL2(P){\displaystyle s\in L^{2}(P)} such thatS[n]=cn{\displaystyle S[n]=c_{n}} for everyn{\displaystyle n}.

Convolution theorems

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Main article:Convolution theorem § Periodic convolution (Fourier series coefficients)

GivenP{\displaystyle P}-periodic functions,sP{\displaystyle s_{P}} andrP{\displaystyle r_{P}} with Fourier series coefficientsS[n]{\displaystyle S[n]} andR[n],{\displaystyle R[n],}nZ,{\displaystyle n\in \mathbb {Z} ,}

Derivative property

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Ifs{\displaystyle s} is a 2π-periodic function onR{\displaystyle \mathbb {R} } which isk{\displaystyle k} times differentiable, and itskth{\displaystyle k^{\text{th}}} derivative is continuous, thens{\displaystyle s} belongs to thefunction spaceCk(R){\displaystyle C^{k}(\mathbb {R} )}.

Compact groups

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Main articles:Compact group,Lie group, andPeter–Weyl theorem

One of the interesting properties of the Fourier transform which we have mentioned, is that it carries convolutions to pointwise products. If that is the property which we seek to preserve, one can produce Fourier series on anycompact group. Typical examples include thoseclassical groups that are compact. This generalizes the Fourier transform to all spaces of the formL2(G), whereG is a compact group, in such a way that the Fourier transform carriesconvolutions to pointwise products. The Fourier series exists and converges in similar ways to the[−π,π] case.

An alternative extension to compact groups is thePeter–Weyl theorem, which proves results about representations of compact groups analogous to those about finite groups.

Theatomic orbitals ofchemistry are partially described byspherical harmonics, which can be used to produce Fourier series on thesphere.

Riemannian manifolds

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Main articles:Laplace operator andRiemannian manifold

If the domain is not a group, then there is no intrinsically defined convolution. However, ifX{\displaystyle X} is acompactRiemannian manifold, it has aLaplace–Beltrami operator. The Laplace–Beltrami operator is the differential operator that corresponds toLaplace operator for the Riemannian manifoldX{\displaystyle X}. Then, by analogy, one can consider heat equations onX{\displaystyle X}. Since Fourier arrived at his basis by attempting to solve the heat equation, the natural generalization is to use the eigensolutions of the Laplace–Beltrami operator as a basis. This generalizes Fourier series to spaces of the typeL2(X){\displaystyle L^{2}(X)}, whereX{\displaystyle X} is a Riemannian manifold. The Fourier series converges in ways similar to the[π,π]{\displaystyle [-\pi ,\pi ]} case. A typical example is to takeX{\displaystyle X} to be the sphere with the usual metric, in which case the Fourier basis consists ofspherical harmonics.

Locally compact Abelian groups

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Main article:Pontryagin duality

The generalization to compact groups discussed above does not generalize to noncompact,nonabelian groups. However, there is a straightforward generalization toLocally Compact Abelian (LCA) groups.

This generalizes the Fourier transform toL1(G){\displaystyle L^{1}(G)} orL2(G){\displaystyle L^{2}(G)}, whereG{\displaystyle G} is an LCA group. IfG{\displaystyle G} is compact, one also obtains a Fourier series, which converges similarly to the[π,π]{\displaystyle [-\pi ,\pi ]} case, but ifG{\displaystyle G} is noncompact, one obtains instead aFourier integral. This generalization yields the usualFourier transform when the underlying locally compact Abelian group isR{\displaystyle \mathbb {R} }.

Extensions

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Fourier-Stieltjes series

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See also:Bochner's theorem § Special cases, andWiener's lemma

Formally, the Fourier-Stieltjes series can be defined as the Fourier series whose coefficients are given bycn=μ^(n)=1P0P ei2πnPxdμ(x),nZ,{\displaystyle c_{n}={\hat {\mu }}(n)={\frac {1}{P}}\int _{0}^{P}\ e^{-i2\pi {\tfrac {n}{P}}x}\,d\mu (x),\quad \forall n\in \mathbb {Z} ,}for anyμM{\displaystyle \mu \in M}, whereM{\displaystyle M} is the spacefiniteBorel measures on the interval[0,P]{\displaystyle [0,P]}. As such, whenμM{\displaystyle \mu \in M}, the functionμ^(n){\displaystyle {\hat {\mu }}(n)} is also referred to as aFourier-Stieltjes transform.[32][33]

This follows from an earlier and more concrete representation of aRadon measure (i.e. alocally finiteBorel measure) onR{\displaystyle \mathbb {R} }, given byF. Riesz. That is, ifF{\displaystyle F} is function ofbounded variation on the interval[0,P]{\displaystyle [0,P]} then the Fourier coefficients can be expressed by theRiemann-Stieltjes integralcn=1P0P ei2πnPxdF(x),nZ,{\displaystyle c_{n}={\frac {1}{P}}\int _{0}^{P}\ e^{-i2\pi {\tfrac {n}{P}}x}\,dF(x),\quad \forall n\in \mathbb {Z} ,}called theFourier-Stieltjes coefficients ofF{\displaystyle F}.[34] As the distributional derivative ofF{\displaystyle F} is a Radon measure, it is subject to theLebesgue decomposition and can be expressed asdF=Fdx+dFs{\displaystyle dF=F'dx+dF_{s}}.[35][36] IfdFs=0{\displaystyle dF_{s}=0} the expression reduces to the original definition of the Fourier coefficients, hence a Fourier series is a Fourier-Stieltjes series.

The question whether or notμ{\displaystyle \mu } exists for a given sequence ofcn{\displaystyle c_{n}} forms the basis of thetrigonometric moment problem.[37]

The Fourier series can be generalized still further from measures todistributions. If the Fourier coefficients are determined by a distributionFD{\displaystyle F\in {\mathcal {D}}'} then the series is sometimes described as aFourier-Schwartz series.[38]

While it is often extremely difficult to decide whether a given series is a Fourier or a Fourier-Stieltjes series, deciding whether or not it is a Fourier-Schwartz series is relatively trivial.[39]

Fourier series on a square

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We can also define the Fourier series for functions of two variablesx{\displaystyle x} andy{\displaystyle y} in the square[π,π]×[π,π]{\displaystyle [-\pi ,\pi ]\times [-\pi ,\pi ]}:f(x,y)=j,kZcj,keijxeiky,cj,k=14π2ππππf(x,y)eijxeikydxdy.{\displaystyle {\begin{aligned}f(x,y)&=\sum _{j,k\in \mathbb {Z} }c_{j,k}e^{ijx}e^{iky},\\[5pt]c_{j,k}&={\frac {1}{4\pi ^{2}}}\int _{-\pi }^{\pi }\int _{-\pi }^{\pi }f(x,y)e^{-ijx}e^{-iky}\,dx\,dy.\end{aligned}}}

Aside from being useful for solving partial differential equations such as the heat equation, one notable application of Fourier series on the square is inimage compression. In particular, theJPEG image compression standard uses the two-dimensionaldiscrete cosine transform, a discrete form of theFourier cosine transform, which uses only cosine as the basis function.

For two-dimensional arrays with a staggered appearance, half of the Fourier series coefficients disappear, due to additional symmetry.[40]

Fourier series of a Bravais-lattice-periodic function

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A three-dimensionalBravais lattice is defined as the set of vectors of the formR=n1a1+n2a2+n3a3{\displaystyle \mathbf {R} =n_{1}\mathbf {a} _{1}+n_{2}\mathbf {a} _{2}+n_{3}\mathbf {a} _{3}}whereni{\displaystyle n_{i}} are integers andai{\displaystyle \mathbf {a} _{i}} are three linearly independent but not necessarily orthogonal vectors. Let us consider some functionf(r){\displaystyle f(\mathbf {r} )} with the same periodicity as the Bravais lattice,i.e.f(r)=f(R+r){\displaystyle f(\mathbf {r} )=f(\mathbf {R} +\mathbf {r} )} for any lattice vectorR{\displaystyle \mathbf {R} }. This situation frequently occurs insolid-state physics wheref(r){\displaystyle f(\mathbf {r} )} might, for example, represent the effective potential that an electron "feels" inside a periodic crystal. In presence of such a periodic potential, the quantum-mechanical description of the electron results in a periodically modulated plane-wave commonly known asBloch state.

In order to developf(r){\displaystyle f(\mathbf {r} )} in a Fourier series, it is convenient to introduce an auxiliary functiong(x1,x2,x3)f(r)=f(x1a1a1+x2a2a2+x3a3a3).{\displaystyle g(x_{1},x_{2},x_{3})\triangleq f(\mathbf {r} )=f\left(x_{1}{\frac {\mathbf {a} _{1}}{a_{1}}}+x_{2}{\frac {\mathbf {a} _{2}}{a_{2}}}+x_{3}{\frac {\mathbf {a} _{3}}{a_{3}}}\right).} Bothf(r){\displaystyle f(\mathbf {r} )} andg(x1,x2,x3){\displaystyle g(x_{1},x_{2},x_{3})} contain essentially the same information. However, instead of the position vectorr{\displaystyle \mathbf {r} }, the arguments ofg{\displaystyle g} are coordinatesx1,2,3{\displaystyle x_{1,2,3}} along the unit vectorsai/ai{\displaystyle \mathbf {a} _{i}/{a_{i}}} of the Bravais lattice, such thatg{\displaystyle g} is an ordinary periodic function in these variables,g(x1,x2,x3)=g(x1+a1,x2,x3)=g(x1,x2+a2,x3)=g(x1,x2,x3+a3)x1,x2,x3.{\displaystyle g(x_{1},x_{2},x_{3})=g(x_{1}+a_{1},x_{2},x_{3})=g(x_{1},x_{2}+a_{2},x_{3})=g(x_{1},x_{2},x_{3}+a_{3})\quad \forall \;x_{1},x_{2},x_{3}.} This trick allows us to developg{\displaystyle g} as a multi-dimensional Fourier series, in complete analogy with the square-periodic function discussed in the previous section. Its Fourier coefficients arec(m1,m2,m3)=1a30a3dx31a20a2dx21a10a1dx1g(x1,x2,x3)ei2π(m1a1x1+m2a2x2+m3a3x3),{\displaystyle {\begin{aligned}c(m_{1},m_{2},m_{3})={\frac {1}{a_{3}}}\int _{0}^{a_{3}}dx_{3}{\frac {1}{a_{2}}}\int _{0}^{a_{2}}dx_{2}{\frac {1}{a_{1}}}\int _{0}^{a_{1}}dx_{1}\,g(x_{1},x_{2},x_{3})\,e^{-i2\pi \left({\tfrac {m_{1}}{a_{1}}}x_{1}+{\tfrac {m_{2}}{a_{2}}}x_{2}+{\tfrac {m_{3}}{a_{3}}}x_{3}\right)}\end{aligned}},} wherem1,m2,m3{\displaystyle m_{1},m_{2},m_{3}} are all integers.c(m1,m2,m3){\displaystyle c(m_{1},m_{2},m_{3})} plays the same role as the coefficientscj,k{\displaystyle c_{j,k}} in the previous section but in order to avoid double subscripts we note them as a function.

Once we have these coefficients, the functiong{\displaystyle g} can be recovered via the Fourier seriesg(x1,x2,x3)=m1,m2,m3Zc(m1,m2,m3)ei2π(m1a1x1+m2a2x2+m3a3x3).{\displaystyle g(x_{1},x_{2},x_{3})=\sum _{m_{1},m_{2},m_{3}\in \mathbb {Z} }\,c(m_{1},m_{2},m_{3})\,e^{i2\pi \left({\tfrac {m_{1}}{a_{1}}}x_{1}+{\tfrac {m_{2}}{a_{2}}}x_{2}+{\tfrac {m_{3}}{a_{3}}}x_{3}\right)}.} We would now like to abandon the auxiliary coordinatesx1,2,3{\displaystyle x_{1,2,3}} and to return to the original position vectorr{\displaystyle \mathbf {r} }. This can be achieved by means of thereciprocal lattice whose vectorsb1,2,3{\displaystyle \mathbf {b} _{1,2,3}} are defined such that they are orthonormal (up to a factor2π{\displaystyle 2\pi }) to the original Bravais vectorsa1,2,3{\displaystyle \mathbf {a} _{1,2,3}},aibj=2πδij,{\displaystyle \mathbf {a} _{i}\cdot \mathbf {b_{j}} =2\pi \delta _{ij},}withδij{\displaystyle \delta _{ij}} theKronecker delta. With this, the scalar product between a reciprocal lattice vectorQ{\displaystyle \mathbf {Q} } and an arbitrary position vectorr{\displaystyle \mathbf {r} } written in the Bravais lattice basis becomesQr=(m1b1+m2b2+m3b3)(x1a1a1+x2a2a2+x3a3a3)=2π(x1m1a1+x2m2a2+x3m3a3),{\displaystyle \mathbf {Q} \cdot \mathbf {r} =\left(m_{1}\mathbf {b} _{1}+m_{2}\mathbf {b} _{2}+m_{3}\mathbf {b} _{3}\right)\cdot \left(x_{1}{\frac {\mathbf {a} _{1}}{a_{1}}}+x_{2}{\frac {\mathbf {a} _{2}}{a_{2}}}+x_{3}{\frac {\mathbf {a} _{3}}{a_{3}}}\right)=2\pi \left(x_{1}{\frac {m_{1}}{a_{1}}}+x_{2}{\frac {m_{2}}{a_{2}}}+x_{3}{\frac {m_{3}}{a_{3}}}\right),}which is exactly the expression occurring in the Fourier exponents. The Fourier series forf(r)=g(x1,x2,x3){\displaystyle f(\mathbf {r} )=g(x_{1},x_{2},x_{3})} can therefore be rewritten as a sum over the all reciprocal lattice vectorsQ=m1b1+m2b2+m3b3{\displaystyle \mathbf {Q} =m_{1}\mathbf {b} _{1}+m_{2}\mathbf {b} _{2}+m_{3}\mathbf {b} _{3}},f(r)=Qc(Q)eiQr,{\displaystyle f(\mathbf {r} )=\sum _{\mathbf {Q} }c(\mathbf {Q} )\,e^{i\mathbf {Q} \cdot \mathbf {r} },} and the coefficients arec(Q)=1a30a3dx31a20a2dx21a10a1dx1f(x1a1a1+x2a2a2+x3a3a3)eiQr.{\displaystyle c(\mathbf {Q} )={\frac {1}{a_{3}}}\int _{0}^{a_{3}}dx_{3}\,{\frac {1}{a_{2}}}\int _{0}^{a_{2}}dx_{2}\,{\frac {1}{a_{1}}}\int _{0}^{a_{1}}dx_{1}\,f\left(x_{1}{\frac {\mathbf {a} _{1}}{a_{1}}}+x_{2}{\frac {\mathbf {a} _{2}}{a_{2}}}+x_{3}{\frac {\mathbf {a} _{3}}{a_{3}}}\right)e^{-i\mathbf {Q} \cdot \mathbf {r} }.} The remaining task will be to convert this integral over lattice coordinates back into a volume integral. The relation between the lattice coordinatesx1,2,3{\displaystyle x_{1,2,3}} and the original cartesian coordinatesr=(x,y,z){\displaystyle \mathbf {r} =(x,y,z)} is a linear system of equations,r=x1a1a1+x2a2a2+x3a3a3,{\displaystyle \mathbf {r} =x_{1}{\frac {\mathbf {a} _{1}}{a_{1}}}+x_{2}{\frac {\mathbf {a} _{2}}{a_{2}}}+x_{3}{\frac {\mathbf {a} _{3}}{a_{3}}},}which, when written in matrix form,[xyz]=J[x1x2x3]=[a1a1,a2a2,a3a3][x1x2x3],{\displaystyle {\begin{bmatrix}x\\y\\z\end{bmatrix}}=\mathbf {J} {\begin{bmatrix}x_{1}\\x_{2}\\x_{3}\end{bmatrix}}={\begin{bmatrix}{\frac {\mathbf {a} _{1}}{a_{1}}},{\frac {\mathbf {a} _{2}}{a_{2}}},{\frac {\mathbf {a} _{3}}{a_{3}}}\end{bmatrix}}{\begin{bmatrix}x_{1}\\x_{2}\\x_{3}\end{bmatrix}}\,,}involves a constant matrixJ{\displaystyle \mathbf {J} } whose columns are the unit vectorsaj/aj{\displaystyle \mathbf {a} _{j}/a_{j}} of the Bravais lattice. When changing variables fromr{\displaystyle \mathbf {r} } to(x1,x2,x3){\displaystyle (x_{1},x_{2},x_{3})} in an integral, the same matrixJ{\displaystyle \mathbf {J} } appears as aJacobian matrixJ=[xx1xx2xx3yx1yx2yx3zx1zx2zx3].{\displaystyle \mathbf {J} ={\begin{bmatrix}{\dfrac {\partial x}{\partial x_{1}}}&{\dfrac {\partial x}{\partial x_{2}}}&{\dfrac {\partial x}{\partial x_{3}}}\\[12pt]{\dfrac {\partial y}{\partial x_{1}}}&{\dfrac {\partial y}{\partial x_{2}}}&{\dfrac {\partial y}{\partial x_{3}}}\\[12pt]{\dfrac {\partial z}{\partial x_{1}}}&{\dfrac {\partial z}{\partial x_{2}}}&{\dfrac {\partial z}{\partial x_{3}}}\end{bmatrix}}\,.}

Its determinantJ{\displaystyle J} is therefore also constant and can be inferred from any integral over any domain; here we choose to calculate the volume of the primitive unit cellΓ{\displaystyle \Gamma } in both coordinate systems:VΓ=Γd3r=J0a1dx10a2dx20a3dx3=Ja1a2a3{\displaystyle V_{\Gamma }=\int _{\Gamma }d^{3}r=J\int _{0}^{a_{1}}dx_{1}\int _{0}^{a_{2}}dx_{2}\int _{0}^{a_{3}}dx_{3}=J\,a_{1}a_{2}a_{3}} The unit cell being aparallelepiped, we haveVΓ=a1(a2×a3){\displaystyle V_{\Gamma }=\mathbf {a} _{1}\cdot (\mathbf {a} _{2}\times \mathbf {a} _{3})} and thusd3r=Jdx1dx2dx3=a1(a2×a3)a1a2a3dx1dx2dx3.{\displaystyle d^{3}r=Jdx_{1}dx_{2}dx_{3}={\frac {\mathbf {a} _{1}\cdot (\mathbf {a} _{2}\times \mathbf {a} _{3})}{a_{1}a_{2}a_{3}}}dx_{1}dx_{2}dx_{3}.} This allows us to writec(Q){\displaystyle c(\mathbf {Q} )} as the desired volume integral over the primitive unit cellΓ{\displaystyle \Gamma } in ordinary cartesian coordinates:c(Q)=1a1(a2×a3)Γd3rf(r)eiQr.{\displaystyle c(\mathbf {Q} )={\frac {1}{\mathbf {a} _{1}\cdot (\mathbf {a} _{2}\times \mathbf {a} _{3})}}\int _{\Gamma }d^{3}r\,f(\mathbf {r} )\cdot e^{-i\mathbf {Q} \cdot \mathbf {r} }\,.}

Hilbert space

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See also:Riesz–Fischer theorem

As the trigonometric series is a special class oforthogonal system, Fourier series can naturally be defined in the context ofHilbert spaces. For example, the space ofsquare-integrable functions on[π,π]{\displaystyle [-\pi ,\pi ]} forms the Hilbert spaceL2([π,π]){\displaystyle L^{2}([-\pi ,\pi ])}. Itsinner product, defined for any two elementsf{\displaystyle f} andg{\displaystyle g}, is given by:f,g=12πππf(x)g(x)¯dx.{\displaystyle \langle f,g\rangle ={\frac {1}{2\pi }}\int _{-\pi }^{\pi }f(x){\overline {g(x)}}\,dx.}This space is equipped with theorthonormal basis{en=einx:nZ}{\displaystyle \left\{e_{n}=e^{inx}:n\in \mathbb {Z} \right\}}.Then the(generalized) Fourier series expansion offL2([π,π]){\displaystyle f\in L^{2}([-\pi ,\pi ])}, given byf(x)=n=cneinx,{\displaystyle f(x)=\sum _{n=-\infty }^{\infty }c_{n}e^{inx},}can be written as[41]f=n=f,enen.{\displaystyle f=\sum _{n=-\infty }^{\infty }\langle f,e_{n}\rangle \,e_{n}.}

Sines and cosines form an orthogonal set, as illustrated above. The integral of sine, cosine and their product is zero (green and red areas are equal, and cancel out) whenm{\displaystyle m},n{\displaystyle n} or the functions are different, and π only ifm{\displaystyle m} andn{\displaystyle n} are equal, and the function used is the same. They would form an orthonormal set, if the integral equaled 1 (that is, each function would need to be scaled by1/π{\displaystyle 1/{\sqrt {\pi }}}).

The sine-cosine form follows in a similar fashion. Indeed, the sines and cosines form anorthogonal set:ππcos(mx)cos(nx)dx=12ππcos((nm)x)+cos((n+m)x)dx=πδmn,m,n1,{\displaystyle \int _{-\pi }^{\pi }\cos(mx)\,\cos(nx)\,dx={\frac {1}{2}}\int _{-\pi }^{\pi }\cos((n-m)x)+\cos((n+m)x)\,dx=\pi \delta _{mn},\quad m,n\geq 1,}ππsin(mx)sin(nx)dx=12ππcos((nm)x)cos((n+m)x)dx=πδmn,m,n1{\displaystyle \int _{-\pi }^{\pi }\sin(mx)\,\sin(nx)\,dx={\frac {1}{2}}\int _{-\pi }^{\pi }\cos((n-m)x)-\cos((n+m)x)\,dx=\pi \delta _{mn},\quad m,n\geq 1}(whereδmn is theKronecker delta), andππcos(mx)sin(nx)dx=12ππsin((n+m)x)+sin((nm)x)dx=0;{\displaystyle \int _{-\pi }^{\pi }\cos(mx)\,\sin(nx)\,dx={\frac {1}{2}}\int _{-\pi }^{\pi }\sin((n+m)x)+\sin((n-m)x)\,dx=0;}Hence, the set{12,cosx2,sinx2,,cos(nx)2,sin(nx)2,},{\displaystyle \left\{{\frac {1}{\sqrt {2}}},{\frac {\cos x}{\sqrt {2}}},{\frac {\sin x}{\sqrt {2}}},\dots ,{\frac {\cos(nx)}{\sqrt {2}}},{\frac {\sin(nx)}{\sqrt {2}}},\dots \right\},}also forms an orthonormal basis forL2([π,π]){\displaystyle L^{2}([-\pi ,\pi ])}. The density of their span is a consequence of theStone–Weierstrass theorem, but follows also from the properties of classical kernels like theFejér kernel.

Fourier theorem proving convergence of Fourier series

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Main article:Convergence of Fourier series

Inengineering, the Fourier series is generally assumed to converge except at jump discontinuities since the functions encountered in engineering are usually better-behaved than those in other disciplines. In particular, ifs{\displaystyle s} is continuous and the derivative ofs(x){\displaystyle s(x)} (which may not exist everywhere) is square integrable, then the Fourier series ofs{\displaystyle s} converges absolutely and uniformly tos(x){\displaystyle s(x)}.[42] If a function issquare-integrable on the interval[x0,x0+P]{\displaystyle [x_{0},x_{0}+P]}, then the Fourier seriesconverges to the functionalmost everywhere. It is possible to define Fourier coefficients for more general functions or distributions, in which casepointwise convergence often fails, and convergence in norm orweak convergence is usually studied.

  • Four partial sums (Fourier series) of lengths 1, 2, 3, and 4 terms, showing how the approximation to a square wave improves as the number of terms increases (animation)
    Four partial sums (Fourier series) of lengths 1, 2, 3, and 4 terms, showing how the approximation to a square wave improves as the number of terms increases(animation)
  • Four partial sums (Fourier series) of lengths 1, 2, 3, and 4 terms, showing how the approximation to a sawtooth wave improves as the number of terms increases (animation)
    Four partial sums (Fourier series) of lengths 1, 2, 3, and 4 terms, showing how the approximation to a sawtooth wave improves as the number of terms increases(animation)
  • Example of convergence to a somewhat arbitrary function. Note the development of the "ringing" (Gibbs phenomenon) at the transitions to/from the vertical sections.
    Example of convergence to a somewhat arbitrary function. Note the development of the "ringing" (Gibbs phenomenon) at the transitions to/from the vertical sections.

The theorems proving that a Fourier series is a valid representation of any periodic function (that satisfies theDirichlet conditions), and informal variations of them that do not specify the convergence conditions, are sometimes referred to generically asFourier's theorem orthe Fourier theorem.[43][44][45][46]

Least squares property

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The earlierEq.2:

sN(x)=n=NNS[n] ei2πnPx,{\displaystyle s_{N}(x)=\sum _{n=-N}^{N}S[n]\ e^{i2\pi {\tfrac {n}{P}}x},}

is atrigonometric polynomial of degreeN{\displaystyle N} that can be generally expressed as:

pN(x)=n=NNp[n] ei2πnPx.{\displaystyle p_{N}(x)=\sum _{n=-N}^{N}p[n]\ e^{i2\pi {\tfrac {n}{P}}x}.}

Parseval's theorem implies that:

TheoremThe trigonometric polynomialsN{\displaystyle s_{N}} is the unique best trigonometric polynomial of degreeN{\displaystyle N} approximatings(x){\displaystyle s(x)}, in the sense that, for any trigonometric polynomialpNsN{\displaystyle p_{N}\neq s_{N}} of degreeN{\displaystyle N}, we have:sNs2<pNs2,{\displaystyle \|s_{N}-s\|_{2}<\|p_{N}-s\|_{2},}where the Hilbert space norm is defined as:g2=1PP|g(x)|2dx.{\displaystyle \|g\|_{2}={\sqrt {{1 \over P}\int _{P}|g(x)|^{2}\,dx}}.}

Convergence theorems

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See also:Gibbs phenomenon

Because of the least squares property, and because of the completeness of the Fourier basis, we obtain an elementary convergence result.

TheoremIfs{\displaystyle s} belongs toL2(P){\displaystyle L^{2}(P)}, thensN{\displaystyle s_{N}} converges tos{\displaystyle s} inL2(P){\displaystyle L^{2}(P)} asN{\displaystyle N\to \infty }, that is:limNsNs2=0.{\displaystyle \lim _{N\to \infty }\|s_{N}-s\|_{2}=0.}

Ifs{\displaystyle s} is continuously differentiable, then(in)S[n]{\displaystyle (in)S[n]} is thenth{\displaystyle n^{\text{th}}} Fourier coefficient of the first derivatives{\displaystyle s'}. Sinces{\displaystyle s'} is continuous, and therefore bounded, it issquare-integrable and its Fourier coefficients are square-summable. Then, by theCauchy–Schwarz inequality,

(n0|S[n]|)2n01n2n0|nS[n]|2.{\displaystyle \left(\sum _{n\neq 0}|S[n]|\right)^{2}\leq \sum _{n\neq 0}{\frac {1}{n^{2}}}\cdot \sum _{n\neq 0}|nS[n]|^{2}.}

This means thats{\displaystyle s} isabsolutely summable. The sum of this series is a continuous function, equal tos{\displaystyle s}, since the Fourier series converges inL1{\displaystyle L^{1}} tos{\displaystyle s}:

TheoremIfsC1(R){\displaystyle s\in C^{1}(\mathbb {R} )}, thensN{\displaystyle s_{N}} converges tos{\displaystyle s}uniformly.

This result can be proven easily ifs{\displaystyle s} is further assumed to beC2{\displaystyle C^{2}}, since in that casen2S[n]{\displaystyle n^{2}S[n]} tends to zero asn{\displaystyle n\rightarrow \infty }. More generally, the Fourier series is absolutely summable, thus converges uniformly tos{\displaystyle s}, provided thats{\displaystyle s} satisfies aHölder condition of orderα>1/2{\displaystyle \alpha >1/2}. In the absolutely summable case, the inequality:

supx|s(x)sN(x)||n|>N|S[n]|{\displaystyle \sup _{x}|s(x)-s_{N}(x)|\leq \sum _{|n|>N}|S[n]|}

proves uniform convergence.

Many other results concerning the convergence of Fourier series are known, ranging from the moderately simple result that the series converges atx{\displaystyle x} ifs{\displaystyle s} is differentiable atx{\displaystyle x}, to more sophisticated results such asCarleson's theorem which states that the Fourier series of anL2{\displaystyle L^{2}} function convergesalmost everywhere.

Divergence

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Since Fourier series have such good convergence properties, many are often surprised by some of the negative results. For example, the Fourier series of a continuousT-periodic function need not converge pointwise. Theuniform boundedness principle yields a simple non-constructive proof of this fact.

In 1922,Andrey Kolmogorov published an article titledUne série de Fourier-Lebesgue divergente presque partout in which he gave an example of a Lebesgue-integrable function whose Fourier series diverges almost everywhere. He later constructed an example of an integrable function whose Fourier series diverges everywhere.[47]

It is possible to give explicit examples of a continuous function whose Fourier series diverges at 0: for instance, the even and 2π-periodic functionf defined for allx in [0,π] by[48]

f(x)=n=11n2sin[(2n3+1)x2].{\displaystyle f(x)=\sum _{n=1}^{\infty }{\frac {1}{n^{2}}}\sin \left[\left(2^{n^{3}}+1\right){\frac {x}{2}}\right].}

Because the function is even the Fourier series contains only cosines:

m=0Cmcos(mx).{\displaystyle \sum _{m=0}^{\infty }C_{m}\cos(mx).}

The coefficients are:

Cm=1πn=11n2{22n3+12m+22n3+1+2m}{\displaystyle C_{m}={\frac {1}{\pi }}\sum _{n=1}^{\infty }{\frac {1}{n^{2}}}\left\{{\frac {2}{2^{n^{3}}+1-2m}}+{\frac {2}{2^{n^{3}}+1+2m}}\right\}}

Asm increases, the coefficients will be positive and increasing until they reach a value of aboutCm2/(n2π){\displaystyle C_{m}\approx 2/(n^{2}\pi )} atm=2n3/2{\displaystyle m=2^{n^{3}}/2} for somen and then become negative (starting with a value around2/(n2π){\displaystyle -2/(n^{2}\pi )}) and getting smaller, before starting a new such wave. Atx=0{\displaystyle x=0} the Fourier series is simply the running sum ofCm,{\displaystyle C_{m},} and this builds up to around

1n2πk=02n3/222k+11n2πln2n3=nπln2{\displaystyle {\frac {1}{n^{2}\pi }}\sum _{k=0}^{2^{n^{3}}/2}{\frac {2}{2k+1}}\sim {\frac {1}{n^{2}\pi }}\ln 2^{n^{3}}={\frac {n}{\pi }}\ln 2}

in thenth wave before returning to around zero, showing that the series does not converge at zero but reaches higher and higher peaks. Note that though the function is continuous, it is not differentiable.

See also

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Notes

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  1. ^These three did someimportant early work on the wave equation, especially D'Alembert. Euler's work in this area was mostlycomtemporaneous/ in collaboration with Bernoulli, although the latter made some independent contributions to the theory of waves and vibrations. (SeeFetter & Walecka 2003, pp. 209–210).
  2. ^Typically[P/2,P/2]{\displaystyle [-P/2,P/2]} or[0,P]{\displaystyle [0,P]}. Some authors defineP2π{\displaystyle P\triangleq 2\pi } because it simplifies the arguments of the sinusoid functions, at the expense of generality.
  3. ^Since the integral defining the Fourier transform of a periodic function is not convergent, it is necessary to view the periodic function and its transform asdistributions. In this senseF{ei2πnPx}{\displaystyle {\mathcal {F}}\{e^{i2\pi {\tfrac {n}{P}}x}\}} is aDirac delta function, which is an example of a distribution.

References

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  1. ^"Fourier".Dictionary.com Unabridged (Online). n.d.
  2. ^Zygmund 2002, p. 1-8.
  3. ^Stillwell, John (2013)."Logic and the philosophy of mathematics in the nineteenth century". In Ten, C. L. (ed.).Routledge History of Philosophy. Vol. VII: The Nineteenth Century. Routledge. p. 204.ISBN 978-1-134-92880-4.
  4. ^Fasshauer, Greg (2015)."Fourier Series and Boundary Value Problems"(PDF).Math 461 Course Notes, Ch 3. Department of Applied Mathematics, Illinois Institute of Technology. Retrieved6 November 2020.
  5. ^Cajori, Florian (1893).A History of Mathematics. Macmillan. p. 283.
  6. ^Dutka, Jacques (1995). "On the early history of Bessel functions".Archive for History of Exact Sciences.49 (2):105–134.doi:10.1007/BF00376544.
  7. ^Lejeune-Dirichlet, Peter Gustav (1829)."Sur la convergence des séries trigonométriques qui servent à représenter une fonction arbitraire entre des limites données" [On the convergence of trigonometric series which serve to represent an arbitrary function between two given limits].Journal für die reine und angewandte Mathematik (in French).4:157–169.arXiv:0806.1294.
  8. ^"Ueber die Darstellbarkeit einer Function durch eine trigonometrische Reihe" [About the representability of a function by a trigonometric series].Habilitationsschrift,Göttingen; 1854. Abhandlungen derKöniglichen Gesellschaft der Wissenschaften zu Göttingen, vol. 13, 1867. Published posthumously for Riemann byRichard Dedekind (in German).Archived from the original on 20 May 2008. Retrieved19 May 2008.
  9. ^Mascre, D.; Riemann, Bernhard (2005) [1867], "Posthumous Thesis on the Representation of Functions by Trigonometric Series", in Grattan-Guinness, Ivor (ed.),Landmark Writings in Western Mathematics 1640–1940, Elsevier, p. 49,ISBN 9780080457444
  10. ^Remmert, Reinhold (1991).Theory of Complex Functions: Readings in Mathematics. Springer. p. 29.ISBN 9780387971957.
  11. ^Nerlove, Marc; Grether, David M.; Carvalho, Jose L. (1995).Analysis of Economic Time Series. Economic Theory, Econometrics, and Mathematical Economics. Elsevier.ISBN 0-12-515751-7.
  12. ^Wilhelm Flügge,Stresses in Shells (1973) 2nd edition.ISBN 978-3-642-88291-3. Originally published in German asStatik und Dynamik der Schalen (1937).
  13. ^Fourier, Jean-Baptiste-Joseph (2014) [1890]. "Mémoire sur la propagation de la chaleur dans les corps solides, présenté le 21 Décembre 1807 à l'Institut national" [Report on the propagation of heat in solid bodies, presented on December 21, 1807 to the National Institute]. In Darboux, Gaston (ed.).Oeuvres de Fourier [The Works of Fourier] (in French). Vol. 2. Paris: Gauthier-Villars et Fils. pp. 218–219.doi:10.1017/CBO9781139568159.009.ISBN 9781139568159.
    Whilst the cited article does list the author as Fourier, a footnote on page 215 indicates that the article was actually written byPoisson and that it is, "for reasons of historical interest", presented as though it were Fourier's original memoire.
  14. ^Fourier, Jean-Baptiste-Joseph (2013) [1888]. "Avant-propos des oevres de Fourier" [Foreword]. In Gaston Darboux (ed.).Oeuvres de Fourier [The Works of Fourier] (in French). Vol. 1. Paris: Gauthier-Villars et Fils. pp. VII–VIII.doi:10.1017/cbo9781139568081.001.ISBN 978-1-108-05938-1.
  15. ^Folland 1992, pp. 18–25.
  16. ^Hardy & Rogosinski 1999, pp. 2–4.
  17. ^Lion 1986.
  18. ^Edwards 1979, pp. 8–9.
  19. ^Edwards 1982, pp. 57, 67.
  20. ^Schwartz 1966, pp. 152–158.
  21. ^Strang, Gilbert (2008),"4.1"(PDF),Fourier Series And Integrals (2 ed.), Wellesley-Cambridge Press, p. 323 (eq 19)
  22. ^Stade 2005, p. 6.
  23. ^Zygmund, Antoni (1935)."Trigonometrical series".EUDML. p. 6. Retrieved2024-12-14.
  24. ^Folland 1992, pp. 21.
  25. ^Stade 2005, pp. 59–64.
  26. ^Kassam, Saleem A. (2004)."Fourier Series (Part II)"(PDF). Retrieved2024-12-11.The phase relationships are important because they correspond to having different amounts of "time shifts" or "delays" for each of the sinusoidal waveforms relative to a zero-phase waveform.
  27. ^abcdePapula, Lothar (2009).Mathematische Formelsammlung: für Ingenieure und Naturwissenschaftler [Mathematical Functions for Engineers and Physicists] (in German). Vieweg+Teubner Verlag.ISBN 978-3834807571.
  28. ^abcdShmaliy, Y.S. (2007).Continuous-Time Signals. Springer.ISBN 978-1402062711.
  29. ^Proakis & Manolakis 1996, p. 291.
  30. ^Oppenheim & Schafer 2010, p. 55.
  31. ^"Characterizations of a linear subspace associated with Fourier series". MathOverflow. 2010-11-19. Retrieved2014-08-08.
  32. ^Edwards 1982, p. 67.
  33. ^Katznelson 2004, p. 164.
  34. ^Zygmund 2002, p. 11.
  35. ^Edwards 1982, pp. 53, 72–73.
  36. ^Katznelson 2004, p. 40.
  37. ^Akhiezer 1965, pp. 180–181.
  38. ^Charpentier, Lesne & Nikolski 2007, p. 11.
  39. ^Edwards 1982, pp. 48, 67–68.
  40. ^Vanishing of Half the Fourier Coefficients in Staggered Arrays
  41. ^Rudin 1987, p. 82.
  42. ^Tolstov, Georgi P. (1976).Fourier Series. Courier-Dover.ISBN 0-486-63317-9.
  43. ^Siebert, William McC. (1985).Circuits, signals, and systems. MIT Press. p. 402.ISBN 978-0-262-19229-3.
  44. ^Marton, L.; Marton, Claire (1990).Advances in Electronics and Electron Physics. Academic Press. p. 369.ISBN 978-0-12-014650-5.
  45. ^Kuzmany, Hans (1998).Solid-state spectroscopy. Springer. p. 14.ISBN 978-3-540-63913-8.
  46. ^Pribram, Karl H.; Yasue, Kunio; Jibu, Mari (1991).Brain and perception. Lawrence Erlbaum Associates. p. 26.ISBN 978-0-89859-995-4.
  47. ^Katznelson 2004.
  48. ^Gourdon, Xavier (2009).Les maths en tête. Analyse (2ème édition) (in French). Ellipses. p. 264.ISBN 978-2729837594.

Bibliography

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External links

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