J Bessel function of the rst kind of order
The Bessel function J n(x), n2N, called the Bessel function of the rst kind of order n, is de ned by the absolutely convergent in nite series J n(x) = xn X m 0 ( 21)mxm 22m+nm(n+ m) for all x2R: (1) It satis es the Bessel di erential equation x2 J00 n (x) + xJ0 n (x) + (x2 n2)J n(x) = 0: (2) The Bessel functions most relevant to this course are J
Radial Separation
Figure 23 1: The zeroth spherical Bessel function { this gives the radial wavefunction for a free particle in spherical coordinates (for ‘= 0) Spherical Bessel Functions We quoted the result above, the di erential equation (23 4) has solu-tions that look like u ‘(r) = rj ‘(kr) ( nite at the origin) But how
Representation of signals as series of orthogonal functions
Series expansions involving Bessel functions : Neumann series Fourier-Bessel series (can be generalized to real indexes Jν) A reference book about Bessel functions (800 pages) α np is the nth positive root of J p Convenient for expansions on [-∞,+∞] Convenient for expansions on [0,1] with boundary condition atx=1
LECTURE 5: Fluid jets 51 The shape of a falling fluid jet - MIT
Eliminating Z(r) and P(r) yields a differential equation for R(r): r2 d2R dr2 +r dR dr − 1+(kr)2 R = 0 (18) This corresponds to modified Bessel Equation of order 1, whose solutions may be written in terms of the modified Bessel functions of the first and second kind, respectively, I 1(kr) and K 1(kr) We note that K
Calcul stochastique et modèles de diffusions
12 7 Carré de processus de Bessel 258 12 8 Dépendance en la condition initiale 259 12 9 Équation différentielle stochastique de Tanaka 261 CHAPITRE 13 • DIFFUSIONS ET OPÉRATEURS AUX DÉRIVÉES PARTIELLES, EXERCICES 13 1 Compléments de cours 265 13 2 Passages successifs de barrières pour un mouvement brownien réel 267
Course notes
where no convergence condition is imposed, and de ne asymptoticity by the following De nition 1 2 A function f is asymptotic to the formal series f~ as tt 0 (once more, the approach of t 0 may have to be restricted to a generally complex curve) if f(t) XM k=0 f k(t) = o(f M(t)) (8M2N or 8M6 M 0 2N)(1 3)
Differential Equations I
A differential equation (de) is an equation involving a function and its deriva-tives Differential equations are called partial differential equations (pde) or or-dinary differential equations (ode) according to whether or not they contain partial derivatives The order of a differential equation is the highest order derivative occurring
Differential Equations
Chapter 0 A short mathematical review A basic understanding of calculus is required to undertake a study of differential equations This zero chapter presents a short review
Electrodynamique II S´erie 1 - Boston University: Physics
La fonction de Green joue le rˆole d’une fonction d’influence : 4πG(x − x′) d´etermine le potentiel au point x duˆ a une unit´e de charge ponctuelle plac´ee au point x′ Exercice 2 : Fonction de Green de l’´equation d’onde `a trois plus une dimensions (voir cours)
[PDF] multiple de 12
[PDF] multiple de 19
[PDF] fonction de bessel j0
[PDF] table de 13
[PDF] fonction de bessel pdf
[PDF] fonction de bessel modifiée
[PDF] introduction ? la microéconomie varian pdf
[PDF] cours microeconomie 1 pdf
[PDF] cours de microéconomie licence 1 pdf
[PDF] corrélation multiple
[PDF] correlation multiple r
[PDF] exercice fonction cout de production
[PDF] corrélation multiple définition
[PDF] corrélation multiple spss
1/66
Representation of signals
as series of orthogonal functionsEric Aristidi
Laboratoire Lagrange - UMR 7293 UNS/CNRS/OCA
1. Fourier Series
2. Legendre polynomials
3. Spherical harmonics
4. Bessel functions
Ecole BasMatIBases mathématiques pour l'instrumentation et le traitement du signal en astronomieNice - Porquerolles, 1 - 5 Juin 2015
1 2/66Fourier Series
Théorie analytique de la chaleur, 1822
Solutions to the heat equation (diffusion PDE) as trigonometric series 3/66For a signal with periodT
-N max N max frequencyn/T Approching a periodic signal by a sum of trigonometric functionsFourier Series
4/66Partial Fourier seriesIndividual terms
Frequencies: 0 , ±1/Tn=1
5/66Partial Fourier seriesIndividual terms
Frequencies :0 , ±1/T , ±2/T, ±3/Tn=1
n=3 n=2 6/66Partial Fourier seriesIndividual terms
7/66Partial Fourier seriesIndividual terms
8/66Partial Fourier seriesIndividual terms
9/66Two representations of the signal
Ensemble of discrete sampled values{f(t
k )}Ensemble of Fourier coefficients{c n 10/66Fourier Series
Complex form :
for a signal f(t)of periodTEven functions : sum of cosines
Odd functions : sum of sines
General case ; real form :
periodT/n 11/66 uniform convergenceCalculating the coefficientsc
n weighting function " Key » relation : nul ifpnThen :
Calculate the integral
12/66Fourier series and scalar product
Vectors (3D)
Functions
Orthogonality :Orthonormal base :
Decomposition :with
(bilinear, for u and v)Scalar product :
2 vectors...1 number
Norm :
(positive) fandgare orthogonal iifOrthonormal base :
Decomposition :
= Fourier seriesScalar product :
Norm :
(suited to Fourier series) 13/66Fourier series and Differential Equations
Harmonic oscillator equation
2 independent solutions are
andwithAny solution is the superposition
Fourier base functions are associated with harmonic differential equation(trigonometric series were introduced from Fourier work on PDE heat equation)
14/66Essential ideas on Fourier Series
Periodic signal
Can be expressed as a series of
trigonometric base functions (exp, cos, sin) Base functions are orthonormal, with respect to an appropriate scalar product Coefs. of the series calculated as a scalar product between the signal and each base function Base functions are solutions of a differential Eq. 15/66Representation of signals
as series of orthogonal functionsEric Aristidi
Laboratoire Lagrange - UMR 7293 UNS/CNRS/OCA
1. Fourier Series
2. Legendre polynomials
3. Spherical harmonics
4. Bessel functions
Ecole BasMatIBases mathématiques pour l'instrumentation et le traitement du signal en astronomieNice - Porquerolles, 1 - 5 Juin 2015
16/66Legendre Polynomials
Introduced by A.M. Legendre, 1784, " Recherches sur la figure des planètes », mém. de l'académie royale des sciences de Paris xyz R r'Gravitational potential at
R mass M with:Introducing
andGenerating function of Legendre Polynomials
O 17/66Taylor expansion atr=0:with
Degree :n
Recurrence relation :
Parity :n
ndistinct roots in the interval [1-,1] 18/66Fourier-Legendre series
Scalar product :
Orthogonality :
Not orthonormal !
Coefficient determination :
Fourier-Legendre series (for a functionf(x)square-summable on [-1,1]) : (suited to Legendre polynomials) 19/66Partial Fourier-Legendre seriesIndividual term
Signal :
a=0.3c 0 P 0 (x)Example of Fourier-Legendre reconstruction
20/66Partial Fourier-Legendre seriesIndividual terms
c 0 P 0 (x) andc 2 P 2 (x) (c 1 =0 for an even signal) 21/66Partial Fourier-Legendre seriesIndividual terms
c 0 P 0 (x) c 4 P 4 (x) c 2 P 2 (x) 22/66Partial Fourier-Legendre seriesIndividual terms
c 0 P 0 (x) c 4 P 4 (x) c 2 P 2 (x)c 6 P 6 (x) 23/66Partial Fourier-Legendre seriesIndividual terms
c 0 P 0 (x) c 4 P 4 (x) c 2 P 2 (x)c 6 P 6 (x) c 8 P 8 (x) 24/66For an even signal : all oddc
n vanish In this example, 8 coefficients seem enough to reconstruct the signal 25/66Error on the reconstruction :
Euclidean distance
26/66Another example : f(x)=tan(x)
Comparison with Fourier series
-11The signal is periodized (period 2)
xAdvantage to Fourier-Legendre (for this case)
signal N max =1 N max =3 27/66Example in physics : gravitational potential of a uniform bar P rL/2 r'
Gravitational
potential : =linear mass density Using the generating function of Legendre polynomials:One finds easily :
with -L/2 This is a Fourier-Legendre expansion of the potential (a.k.a. multipolar expansion) 28/66Fourier-Legendre series of the potential
r=0.75 L 29/66Polar plotIndividual terms Potential (partial sums)Polar plot c 0 P 0 (cos c 2 P 2 (cos c 4 P 4 (cos 30/66
Essential ideas on Fourier-Legendre Series
Signal defined on interval [-1,1]
Can be expressed as a series of
Legendre polynomials (base functions)
Legendre poly's are orthogonal, with respect to an appropriate scalar product Coefs. of the series calculated as a scalar product between the signal and each polynom Polynoms are solutions of Legendre differential Eq.Legendre polynomials are defined by Taylor expansion of a characteristic function 31/66Representation of signals
as series of orthogonal functions1. Fourier Series
2. Legendre polynomials
3. Spherical harmonics
4. Bessel functions
Ecole BasMatIBases mathématiques pour l'instrumentation et le traitement du signal en astronomieNice - Porquerolles, 1 - 5 Juin 2015
32/66Towards the Spherical Harmonics :
associated Legendre functions :P lmDefinition :
Orthogonality (same scalar product asP
n )ĺgeneralisation of Legendre polynomials ifm=0:Fixedm, differentl:Fixedl, differentm:(for m>0)
33/66l=2: 5 "polynoms"l=1: 3 "polynoms"l=0: 1 polynom
For a givenl
there are 2l+1 possible P lm 34/66Spherical Harmonics
Back to the Newtonial potential :
If azimuthal symmetry, the potential is a
function of r andand can be developped as a Fourier-Legendre series :What if no azimuthal symmetry ?The potential depends on the 3
spherical coordinates(r,). Laplace (1785) showed that a similar series expansion canbemade: P r r' function of r alonefunction ofalone 35/66Spherical Harmonics
To find the functionsC
lm (r)andY lm say that the potential obey Laplace's equation (Solutions are "harmonicfunctions») andfind:SphericalHarmonics
The potential at the surface of a sphere (fixed r) is a 2D functionf( )which can be developped as a series of spherical harmonics :l: degree, m: order; -l m l 36/66Orthogonality and series expansion
Scalar product :
Orthogonality :
orthonormal baseSeries expansion for a functionf(
)on a sphere :Coefficient determination :
(suited to Spherical harmonics) 37/66Comparison : 1D (polar) and 2D (spherical)
xyFunctionf(
)with values on a circler=C te2periodic in
Fourier expansionFunctionf(
)with values on a spherer=C te2periodic in and
Spherical harmonic expansionIn the plane : polar coordinates(r, )In space : spherical coordinates(r, 38/66First spherical harmonic
(uniform) zzz x y 39/66l=1 m=-1 m=0m=1 indep. of: azimuthal symmetry 40/66
Different representation
l=1, m=0 l=1, m=1 41/66l=2 m=-2 m=-1m=0 for positive m, use : 42/66
Symmetries of the spherical harmonics
m=0: azimuthal symmetryParity in
cos( l+m even : symmetry planez=0l+modd: anti-symmetry planez=0 Spherical harmonic expansion becomes a Fourier-Legendre series ofcos(Adapted for series expansion of functions
having a symmetry planeAdapted for series expansion of functions having a anti-symmetry plane 43/66HarmonicY
lm mperiods in directionterme im n - mnode lines (Y lm =0) in directionLarge mor (l-m)
= small details 44/66Application to wide-field imagery : WMAP images
Source : B. Terzic,
http://www.nicadd.niu.edu/~bterzic/Decomposition of the CMB signal on theY
lmPlot of coefficients |c
l 2 (averaged overm), i.e. "angular power spectrum» 45/66Cumulative image of the WMAP sky as incresing l numbers are summed (For each l, all orders m are accumulated)
Application to wide-field imagery : WMAP images
46/66Cumulative image of the WMAP sky as incresing l numbers are summed (For each l, all orders m are accumulated)