Fourier Analysis

Total Page:16

File Type:pdf, Size:1020Kb

Fourier Analysis Fourier Analysis Hilary Weller <[email protected]> 19th October 2015 This is brief introduction to Fourier analysis and how it is used in atmospheric and oceanic science, for: Analysing data (eg climate data) • Numerical methods • Numerical analysis of methods • 1 1 Fourier Series Any periodic, integrable function, f (x) (defined on [ π,π]), can be expressed as a Fourier − series; an infinite sum of sines and cosines: ∞ ∞ a0 f (x) = + ∑ ak coskx + ∑ bk sinkx (1) 2 k=1 k=1 The a and b are the Fourier coefficients. • k k The sines and cosines are the Fourier modes. • k is the wavenumber - number of complete waves that fit in the interval [ π,π] • − sinkx for different values of k 1.0 k =1 k =2 k =4 0.5 0.0 0.5 1.0 π π/2 0 π/2 π − − x The wavelength is λ = 2π/k • The more Fourier modes that are included, the closer their sum will get to the function. • 2 Sum of First 4 Fourier Modes of a Periodic Function 1.0 Fourier Modes Original function 4 Sum of first 4 Fourier modes 0.5 2 0.0 0 2 0.5 4 1.0 π π/2 0 π/2 π π π/2 0 π/2 π − − − − x x 3 The first four Fourier modes of a square wave. The additional oscillations are “spectral ringing” Each mode can be represented by motion around a circle. ↓ The motion around each circle has a speed and a radius. These represent the wavenumber and the Fourier coefficients. Which is which? speed is wavenumber, radius is coefficient 4 Equivalently, equation (1) can be expressed as an infinite sum of exponentials using the relation eiθ = cosθ + isinθ where i = √ 1: − ∞ ∞ ∞ a0 ikx f (x) = + ∑ ak coskx + ∑ bk sinkx = ∑ Ake . (2) 2 k=1 k=1 k= ∞ − Exercise Evaluate the Aks in terms of the aks and bks. 5 2 Fourier Transform The Fourier Transform transforms a function f which is defined over space (or time) into • the frequency domain, so that it is defined in terms of Fourier coefficients. The Fourier transform calculates the Fourier coefficients as: • 1 π 1 π ak = f (x)cos(kx)dx , bk = f (x)sin(kx)dx π ˆ π π ˆ π − − 3 Discrete Fourier Transform A discrete Fourier Transform converts a list of 2N + 1 equally spaced samples of a real valued, periodic function, fn, to the list of the first 2N + 1 complex valued Fourier coefficients: N 1 iπnkx/N Ak = ∑ fn e− . N n= N − The truncated Fourier series: N ikx f (x) ∑ Ake ≈ k= N − is an approximation to the function f which fits the sampled points, fn, exactly. On a computer this is done with a Fast Fourier Transform (or fft). The inverse Fourier transform (sometimes called ifft) transforms the Fourier coefficients back to the f values (transforming from spectral back to real space): fft f0, f1, f2, f2N A0,A1, A2N ··· −−−→ifft ··· A ,A , A f , f , f , f 0 1 ··· 2N −−−→ 0 1 2 ··· 2N 6 4 Differentiation and Interpolation If we know the Fourier coefficients, Ak, of a function f then we can calculate the gradient of f at any point, x: If ∞ ∞ ∞ ikx f (x) = ∑ ak coskx + ∑ bk sinkx = ∑ Ake (3) k=0 k=0 k= ∞ − then ∞ ∞ ∞ ikx f 0(x) = ∑ kak sinkx + ∑ kbk coskx = ∑ i k Ake . (4) k=0 − k=0 k= ∞ − and the second derivative: ∞ ∞ ∞ 2 2 2 ikx f 00(x) = ∑ k ak coskx ∑ k bk sinkx = ∑ k Ake . (5) k=0 − − k=0 k= ∞ − − These have spectral accuracy; the order of accuracy is as high as the number of points. Similarly equation 1 or 2 can be used directly to interpolate f onto an undefined point, x. Again, the order of accuracy is spectral. 5 Spectral Models ECMWF use a spectral model. • The prognostic variables are transformed between physical and spectral space using ffts • and iffts. Gradients are calculated very accurately in spectral space • 6 Wave Power and Frequency If a function, f , has Fourier coefficients, a and b , then wavenumber k has power a2 + b2. • k k k k A plot of wave frequency versus power is referred to as the power spectrum. Before we • learn how power spectra are used, we will have some revision questions... 7 7 Recap Questions 1. In the Fourier decomposition ∞ ∞ a0 f (x) = + ∑ ak coskx + ∑ bk sinkx 2 k=1 k=1 what are: (a) the Fourier coefficients (the ak and the bk) (b) the Fourier modes (the sines and cosines) (c) the wavenumbers (or frequencies) (the ks) 2 2 (d) the power of a given wavenumber (ak + bk) 2. How would you describe the operation: 1 π 1 π ak = f (x)cos(kx)dx , bk = f (x)sin(kx)dx π ˆ π π ˆ π − − (a Fourier transform) 3. Given a list of 2N + 1 equally spaced samples of a real valued, periodic function, fn, how would you describe the following operation to convert this into a a list of N + 1 values: N 1 iπknx/N Ak = ∑ fn e− N n= N − (a discrete Fourier transform) 4. What is the wavelength of a wave described by sin4x (2π/4) 8 8 Analysing Power Spectra Daily rainfall at a station in the Middle East for 21 years 60 daily rainfall Fourier filtered using 40 wave numbers Obervations about the 50 Truncated Fourier 40 filtered rainfall: 30 very smooth (only low 20 rainfall (mm) • wavenumbers included) 10 includes negative values 0 • – “spectral ringing” 0 5 10 15 20 years Power Spectrum of Middle East Rainfall 100 10-1 Observations 10-2 10-3 dominant frequency at one year power • 10-4 (annual cycle) -5 power at high frequencies (ie 10 • 10-6 daily variability) 10-1 100 101 102 Number per year number per year = wavenumber 365/total number of days × 9 Time Series of the Nino 3 sea surface temperature (SST) The SST in the Nino 3 region of the equatorial Pacific is a diagnostic of El Nino 30 raw 2 years and slower 29 annual cycle How were the dashed lines generated? 28 Annual cycle is the • 27 Fourier mode at 1 year 26 The “two years and SST (deg C) • slower” filtered data is 25 the sum of all the 24 Fourier modes of these frequencies. 23 1990 1995 2000 2005 2010 Power Spectrum of Nino 3 SST 1 Observations 0.1 Dominant frequency at 1 year (annual 0.01 • cycle) 0.001 power Less power at high frequencies (SST • 0.0001 varies slowly) 1e−05 Power at 1-10 years (El Nino every 3-7 • 1e−06 years) 0.01 0.1 1 10 Frequency (per year) 10 Time Series of the Quasi-Biennial Oscillation (QBO) The QBO is an oscillation of the equatorial zonal wind between easterlies and westerlies in the tropical stratosphere which has a mean period of 28 to 29 months: Power Spectrum of QBO 8 10 Observations 107 6 Dominant frequency at 10 • 105 close to 2 years 4 power 10 Less power at high 3 • 10 frequencies 102 Less power at long 101 • time-scales 10-2 10-1 100 101 frequency (per year) 11.
Recommended publications
  • The Fast Fourier Transform
    The Fast Fourier Transform Derek L. Smith SIAM Seminar on Algorithms - Fall 2014 University of California, Santa Barbara October 15, 2014 Table of Contents History of the FFT The Discrete Fourier Transform The Fast Fourier Transform MP3 Compression via the DFT The Fourier Transform in Mathematics Table of Contents History of the FFT The Discrete Fourier Transform The Fast Fourier Transform MP3 Compression via the DFT The Fourier Transform in Mathematics Navigating the Origins of the FFT The Royal Observatory, Greenwich, in London has a stainless steel strip on the ground marking the original location of the prime meridian. There's also a plaque stating that the GPS reference meridian is now 100m to the east. This photo is the culmination of hundreds of years of mathematical tricks which answer the question: How to construct a more accurate clock? Or map? Or star chart? Time, Location and the Stars The answer involves a naturally occurring reference system. Throughout history, humans have measured their location on earth, in order to more accurately describe the position of astronomical bodies, in order to build better time-keeping devices, to more successfully navigate the earth, to more accurately record the stars... and so on... and so on... Time, Location and the Stars Transoceanic exploration previously required a vessel stocked with maps, star charts and a highly accurate clock. Institutions such as the Royal Observatory primarily existed to improve a nations' navigation capabilities. The current state-of-the-art includes atomic clocks, GPS and computerized maps, as well as a whole constellation of government organizations.
    [Show full text]
  • B1. Fourier Analysis of Discrete Time Signals
    B1. Fourier Analysis of Discrete Time Signals Objectives • Introduce discrete time periodic signals • Define the Discrete Fourier Series (DFS) expansion of periodic signals • Define the Discrete Fourier Transform (DFT) of signals with finite length • Determine the Discrete Fourier Transform of a complex exponential 1. Introduction In the previous chapter we defined the concept of a signal both in continuous time (analog) and discrete time (digital). Although the time domain is the most natural, since everything (including our own lives) evolves in time, it is not the only possible representation. In this chapter we introduce the concept of expanding a generic signal in terms of elementary signals, such as complex exponentials and sinusoids. This leads to the frequency domain representation of a signal in terms of its Fourier Transform and the concept of frequency spectrum so that we characterize a signal in terms of its frequency components. First we begin with the introduction of periodic signals, which keep repeating in time. For these signals it is fairly easy to determine an expansion in terms of sinusoids and complex exponentials, since these are just particular cases of periodic signals. This is extended to signals of a finite duration which becomes the Discrete Fourier Transform (DFT), one of the most widely used algorithms in Signal Processing. The concepts introduced in this chapter are at the basis of spectral estimation of signals addressed in the next two chapters. 2. Periodic Signals VIDEO: Periodic Signals (19:45) http://faculty.nps.edu/rcristi/eo3404/b-discrete-fourier-transform/videos/chapter1-seg1_media/chapter1-seg1- 0.wmv http://faculty.nps.edu/rcristi/eo3404/b-discrete-fourier-transform/videos/b1_02_periodicSignals.mp4 In this section we define a class of discrete time signals called Periodic Signals.
    [Show full text]
  • Fourier Series
    Academic Press Encyclopedia of Physical Science and Technology Fourier Series James S. Walker Department of Mathematics University of Wisconsin–Eau Claire Eau Claire, WI 54702–4004 Phone: 715–836–3301 Fax: 715–836–2924 e-mail: [email protected] 1 2 Encyclopedia of Physical Science and Technology I. Introduction II. Historical background III. Definition of Fourier series IV. Convergence of Fourier series V. Convergence in norm VI. Summability of Fourier series VII. Generalized Fourier series VIII. Discrete Fourier series IX. Conclusion GLOSSARY ¢¤£¦¥¨§ Bounded variation: A function has bounded variation on a closed interval ¡ ¢ if there exists a positive constant © such that, for all finite sets of points "! "! $#&% (' #*) © ¥ , the inequality is satisfied. Jordan proved that a function has bounded variation if and only if it can be expressed as the difference of two non-decreasing functions. Countably infinite set: A set is countably infinite if it can be put into one-to-one £0/"£ correspondence with the set of natural numbers ( +,£¦-.£ ). Examples: The integers and the rational numbers are countably infinite sets. "! "!;: # # 123547698 Continuous function: If , then the function is continuous at the point : . Such a point is called a continuity point for . A function which is continuous at all points is simply referred to as continuous. Lebesgue measure zero: A set < of real numbers is said to have Lebesgue measure ! $#¨CED B ¢ £¦¥ zero if, for each =?>A@ , there exists a collection of open intervals such ! ! D D J# K% $#L) ¢ £¦¥ ¥ ¢ = that <GFIH and . Examples: All finite sets, and all countably infinite sets, have Lebesgue measure zero. "! "! % # % # Odd and even functions: A function is odd if for all in its "! "! % # # domain.
    [Show full text]
  • FOURIER TRANSFORM Very Broadly Speaking, the Fourier Transform Is a Systematic Way to Decompose “Generic” Functions Into
    FOURIER TRANSFORM TERENCE TAO Very broadly speaking, the Fourier transform is a systematic way to decompose “generic” functions into a superposition of “symmetric” functions. These symmetric functions are usually quite explicit (such as a trigonometric function sin(nx) or cos(nx)), and are often associated with physical concepts such as frequency or energy. What “symmetric” means here will be left vague, but it will usually be associated with some sort of group G, which is usually (though not always) abelian. Indeed, the Fourier transform is a fundamental tool in the study of groups (and more precisely in the representation theory of groups, which roughly speaking describes how a group can define a notion of symmetry). The Fourier transform is also related to topics in linear algebra, such as the representation of a vector as linear combinations of an orthonormal basis, or as linear combinations of eigenvectors of a matrix (or a linear operator). To give a very simple prototype of the Fourier transform, consider a real-valued function f : R → R. Recall that such a function f(x) is even if f(−x) = f(x) for all x ∈ R, and is odd if f(−x) = −f(x) for all x ∈ R. A typical function f, such as f(x) = x3 + 3x2 + 3x + 1, will be neither even nor odd. However, one can always write f as the superposition f = fe + fo of an even function fe and an odd function fo by the formulae f(x) + f(−x) f(x) − f(−x) f (x) := ; f (x) := . e 2 o 2 3 2 2 3 For instance, if f(x) = x + 3x + 3x + 1, then fe(x) = 3x + 1 and fo(x) = x + 3x.
    [Show full text]
  • An Introduction to Fourier Analysis Fourier Series, Partial Differential Equations and Fourier Transforms
    An Introduction to Fourier Analysis Fourier Series, Partial Differential Equations and Fourier Transforms Notes prepared for MA3139 Arthur L. Schoenstadt Department of Applied Mathematics Naval Postgraduate School Code MA/Zh Monterey, California 93943 August 18, 2005 c 1992 - Professor Arthur L. Schoenstadt 1 Contents 1 Infinite Sequences, Infinite Series and Improper Integrals 1 1.1Introduction.................................... 1 1.2FunctionsandSequences............................. 2 1.3Limits....................................... 5 1.4TheOrderNotation................................ 8 1.5 Infinite Series . ................................ 11 1.6ConvergenceTests................................ 13 1.7ErrorEstimates.................................. 15 1.8SequencesofFunctions.............................. 18 2 Fourier Series 25 2.1Introduction.................................... 25 2.2DerivationoftheFourierSeriesCoefficients.................. 26 2.3OddandEvenFunctions............................. 35 2.4ConvergencePropertiesofFourierSeries.................... 40 2.5InterpretationoftheFourierCoefficients.................... 48 2.6TheComplexFormoftheFourierSeries.................... 53 2.7FourierSeriesandOrdinaryDifferentialEquations............... 56 2.8FourierSeriesandDigitalDataTransmission.................. 60 3 The One-Dimensional Wave Equation 70 3.1Introduction.................................... 70 3.2TheOne-DimensionalWaveEquation...................... 70 3.3 Boundary Conditions ............................... 76 3.4InitialConditions................................
    [Show full text]
  • Fourier Transforms & the Convolution Theorem
    Convolution, Correlation, & Fourier Transforms James R. Graham 11/25/2009 Introduction • A large class of signal processing techniques fall under the category of Fourier transform methods – These methods fall into two broad categories • Efficient method for accomplishing common data manipulations • Problems related to the Fourier transform or the power spectrum Time & Frequency Domains • A physical process can be described in two ways – In the time domain, by h as a function of time t, that is h(t), -∞ < t < ∞ – In the frequency domain, by H that gives its amplitude and phase as a function of frequency f, that is H(f), with -∞ < f < ∞ • In general h and H are complex numbers • It is useful to think of h(t) and H(f) as two different representations of the same function – One goes back and forth between these two representations by Fourier transforms Fourier Transforms ∞ H( f )= ∫ h(t)e−2πift dt −∞ ∞ h(t)= ∫ H ( f )e2πift df −∞ • If t is measured in seconds, then f is in cycles per second or Hz • Other units – E.g, if h=h(x) and x is in meters, then H is a function of spatial frequency measured in cycles per meter Fourier Transforms • The Fourier transform is a linear operator – The transform of the sum of two functions is the sum of the transforms h12 = h1 + h2 ∞ H ( f ) h e−2πift dt 12 = ∫ 12 −∞ ∞ ∞ ∞ h h e−2πift dt h e−2πift dt h e−2πift dt = ∫ ( 1 + 2 ) = ∫ 1 + ∫ 2 −∞ −∞ −∞ = H1 + H 2 Fourier Transforms • h(t) may have some special properties – Real, imaginary – Even: h(t) = h(-t) – Odd: h(t) = -h(-t) • In the frequency domain these
    [Show full text]
  • Fourier Analysis
    Chapter 1 Fourier analysis In this chapter we review some basic results from signal analysis and processing. We shall not go into detail and assume the reader has some basic background in signal analysis and processing. As basis for signal analysis, we use the Fourier transform. We start with the continuous Fourier transformation. But in applications on the computer we deal with a discrete Fourier transformation, which introduces the special effect known as aliasing. We use the Fourier transformation for processes such as convolution, correlation and filtering. Some special attention is given to deconvolution, the inverse process of convolution, since it is needed in later chapters of these lecture notes. 1.1 Continuous Fourier Transform. The Fourier transformation is a special case of an integral transformation: the transforma- tion decomposes the signal in weigthed basis functions. In our case these basis functions are the cosine and sine (remember exp(iφ) = cos(φ) + i sin(φ)). The result will be the weight functions of each basis function. When we have a function which is a function of the independent variable t, then we can transform this independent variable to the independent variable frequency f via: +1 A(f) = a(t) exp( 2πift)dt (1.1) −∞ − Z In order to go back to the independent variable t, we define the inverse transform as: +1 a(t) = A(f) exp(2πift)df (1.2) Z−∞ Notice that for the function in the time domain, we use lower-case letters, while for the frequency-domain expression the corresponding uppercase letters are used. A(f) is called the spectrum of a(t).
    [Show full text]
  • STATISTICAL FOURIER ANALYSIS: CLARIFICATIONS and INTERPRETATIONS by DSG Pollock
    STATISTICAL FOURIER ANALYSIS: CLARIFICATIONS AND INTERPRETATIONS by D.S.G. Pollock (University of Leicester) Email: stephen [email protected] This paper expounds some of the results of Fourier theory that are es- sential to the statistical analysis of time series. It employs the algebra of circulant matrices to expose the structure of the discrete Fourier transform and to elucidate the filtering operations that may be applied to finite data sequences. An ideal filter with a gain of unity throughout the pass band and a gain of zero throughout the stop band is commonly regarded as incapable of being realised in finite samples. It is shown here that, to the contrary, such a filter can be realised both in the time domain and in the frequency domain. The algebra of circulant matrices is also helpful in revealing the nature of statistical processes that are band limited in the frequency domain. In order to apply the conventional techniques of autoregressive moving-average modelling, the data generated by such processes must be subjected to anti- aliasing filtering and sub sampling. These techniques are also described. It is argued that band-limited processes are more prevalent in statis- tical and econometric time series than is commonly recognised. 1 D.S.G. POLLOCK: Statistical Fourier Analysis 1. Introduction Statistical Fourier analysis is an important part of modern time-series analysis, yet it frequently poses an impediment that prevents a full understanding of temporal stochastic processes and of the manipulations to which their data are amenable. This paper provides a survey of the theory that is not overburdened by inessential complications, and it addresses some enduring misapprehensions.
    [Show full text]
  • Fourier Transform, Convolution Theorem, and Linear Dynamical Systems April 28, 2016
    Mathematical Tools for Neuroscience (NEU 314) Princeton University, Spring 2016 Jonathan Pillow Lecture 23: Fourier Transform, Convolution Theorem, and Linear Dynamical Systems April 28, 2016. Discrete Fourier Transform (DFT) We will focus on the discrete Fourier transform, which applies to discretely sampled signals (i.e., vectors). Linear algebra provides a simple way to think about the Fourier transform: it is simply a change of basis, specifically a mapping from the time domain to a representation in terms of a weighted combination of sinusoids of different frequencies. The discrete Fourier transform is therefore equiv- alent to multiplying by an orthogonal (or \unitary", which is the same concept when the entries are complex-valued) matrix1. For a vector of length N, the matrix that performs the DFT (i.e., that maps it to a basis of sinusoids) is an N × N matrix. The k'th row of this matrix is given by exp(−2πikt), for k 2 [0; :::; N − 1] (where we assume indexing starts at 0 instead of 1), and t is a row vector t=0:N-1;. Recall that exp(iθ) = cos(θ) + i sin(θ), so this gives us a compact way to represent the signal with a linear superposition of sines and cosines. The first row of the DFT matrix is all ones (since exp(0) = 1), and so the first element of the DFT corresponds to the sum of the elements of the signal. It is often known as the \DC component". The next row is a complex sinusoid that completes one cycle over the length of the signal, and each subsequent row has a frequency that is an integer multiple of this \fundamental" frequency.
    [Show full text]
  • A Hilbert Space Theory of Generalized Graph Signal Processing
    1 A Hilbert Space Theory of Generalized Graph Signal Processing Feng Ji and Wee Peng Tay, Senior Member, IEEE Abstract Graph signal processing (GSP) has become an important tool in many areas such as image pro- cessing, networking learning and analysis of social network data. In this paper, we propose a broader framework that not only encompasses traditional GSP as a special case, but also includes a hybrid framework of graph and classical signal processing over a continuous domain. Our framework relies extensively on concepts and tools from functional analysis to generalize traditional GSP to graph signals in a separable Hilbert space with infinite dimensions. We develop a concept analogous to Fourier transform for generalized GSP and the theory of filtering and sampling such signals. Index Terms Graph signal proceesing, Hilbert space, generalized graph signals, F-transform, filtering, sampling I. INTRODUCTION Since its emergence, the theory and applications of graph signal processing (GSP) have rapidly developed (see for example, [1]–[10]). Traditional GSP theory is essentially based on a change of orthonormal basis in a finite dimensional vector space. Suppose G = (V; E) is a weighted, arXiv:1904.11655v2 [eess.SP] 16 Sep 2019 undirected graph with V the vertex set of size n and E the set of edges. Recall that a graph signal f assigns a complex number to each vertex, and hence f can be regarded as an element of n C , where C is the set of complex numbers. The heart of the theory is a shift operator AG that is usually defined using a property of the graph.
    [Show full text]
  • 20. the Fourier Transform in Optics, II Parseval’S Theorem
    20. The Fourier Transform in optics, II Parseval’s Theorem The Shift theorem Convolutions and the Convolution Theorem Autocorrelations and the Autocorrelation Theorem The Shah Function in optics The Fourier Transform of a train of pulses The spectrum of a light wave The spectrum of a light wave is defined as: 2 SFEt {()} where F{E(t)} denotes E(), the Fourier transform of E(t). The Fourier transform of E(t) contains the same information as the original function E(t). The Fourier transform is just a different way of representing a signal (in the frequency domain rather than in the time domain). But the spectrum contains less information, because we take the magnitude of E(), therefore losing the phase information. Parseval’s Theorem Parseval’s Theorem* says that the 221 energy in a function is the same, whether f ()tdt F ( ) d 2 you integrate over time or frequency: Proof: f ()tdt2 f ()t f *()tdt 11 F( exp(j td ) F *( exp(j td ) dt 22 11 FF() *(') exp([j '])tdtd ' d 22 11 FF( ) * ( ') [2 ')] dd ' 22 112 FF() *() d F () d * also known as 22Rayleigh’s Identity. The Fourier Transform of a sum of two f(t) F() functions t g(t) G() Faft() bgt () aF ft() bFgt () t The FT of a sum is the F() + sum of the FT’s. f(t)+g(t) G() Also, constants factor out. t This property reflects the fact that the Fourier transform is a linear operation. Shift Theorem The Fourier transform of a shifted function, f ():ta Ffta ( ) exp( jaF ) ( ) Proof : This theorem is F ft a ft( a )exp( jtdt ) important in optics, because we often encounter functions Change variables : uta that are shifting (continuously) along fu( )exp( j [ u a ]) du the time axis – they are called waves! exp(ja ) fu ( )exp( judu ) exp(jaF ) ( ) QED An example of the Shift Theorem in optics Suppose that we’re measuring the spectrum of a light wave, E(t), but a small fraction of the irradiance of this light, say , takes a different path that also leads to the spectrometer.
    [Show full text]
  • The Fourier Transform
    The Fourier Transform CS/CME/BIOPHYS/BMI 279 Fall 2015 Ron Dror The Fourier transform is a mathematical method that expresses a function as the sum of sinusoidal functions (sine waves). Fourier transforms are widely used in many fields of sciences and engineering, including image processing, quantum mechanics, crystallography, geoscience, etc. Here we will use, as examples, functions with finite, discrete domains (i.e., functions defined at a finite number of regularly spaced points), as typically encountered in computational problems. However the concept of Fourier transform can be readily applied to functions with infinite or continuous domains. (We won’t differentiate between “Fourier series” and “Fourier transform.”) A graphical example ! ! Suppose we have a function � � defined in the range − < � < on 2� + 1 discrete points such that ! ! ! � = �. By a Fourier transform we aim to express it as: ! !!!! � �! = �! + �! cos 2��!� + �! + �! cos 2��!� + �! + ⋯ (1) We first demonstrate graphically how a function may be described by its Fourier components. Fig. 1 shows a function defined on 101 discrete data points integer � = −50, −49, … , 49, 50. In fig. 2, the first Fig. 1. The function to be Fourier transformed few Fourier components are plotted separately (left) and added together (right) to form an approximation to the original function. Finally, fig. 3 demonstrates that by including the components up to � = 50, a faithful representation of the original function can be obtained. � ��, �� & �� Single components Summing over components up to m 0 �! = 0.6 �! = 0 �! = 0 1 �! = 1.9 �! = 0.01 �! = 2.2 2 �! = 0.27 �! = 0.02 �! = −1.3 3 �! = 0.39 �! = 0.03 �! = 0.4 Fig.2.
    [Show full text]