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Concepts and Algorithms of Scientific and Visual Computing Wavelets CS448J, Autumn 2015, Stanford University Dominik L. Michels Wavelets Wavelet functions can be seen as an analog to window functions in the context of the wavelet


  1. Concepts and Algorithms of Scientific and Visual Computing –Wavelets– CS448J, Autumn 2015, Stanford University Dominik L. Michels

  2. Wavelets Wavelet functions can be seen as an analog to window functions in the context of the wavelet transformation. The term “wavelet” derives from the French “ondelette” meaning “little wave”. Among other, fundamental contributions to wavelet theory were made by Ingrid Daubechies, see [Daubechies 1988] which can be seen as the foundation of the fast wavelet transform, and the multiresolution analysis later developed in [Mallat 1989] and [Meyer 1992].

  3. Wavelets Our derivations will lead to the continuous-time wavelet transform (CTWT), which can be considered in comparison to the WFT, in which instead of a window function g ∈ L 2 ( R ), a so-called mother wavelet ψ ∈ L 2 ( R ) is employed. Whereas the (musical) notes g ω, t : u �→ g ( u − t )exp(2 π i ω u ) of the WFT take a frequency modulation ω ∈ R and a time shift t ∈ R into account, the notes ψ s , t : u �→ | s | − 1 / 2 ψ (( u − t ) / s ) of the CTWT contain a scaling factor s ∈ R \ { 0 } and a time shift t ∈ R . Whereas the WFT notes are of identical duration because of T ( g ω, t ) = T ( g ) and Ω ( g ω, t ) = Ω ( g ), the CTWT notes are scaled in dependence of s : Ω ( ψ s , t ) = | s | − 1 Ω ( ψ ) . T ( ψ s , t ) = | s | T ( ψ ) , Furthermore t 0 ( ψ s , t ) = s t 0 ( ψ ) + t and ω 0 ( ψ s , t ) = s − 1 ω 0 ( ψ ).

  4. Wavelets A wavelet is a function ψ ∈ L 2 ( R ) satisfying the wavelet condition � 2 � � ˆ � ψ ( ω ) � � � 0 < c ψ := < ∞ . | ω | R We will show, that the set Ψ ⊂ L 2 ( R ) of all wavelets is dense in L 2 ( R ), i.e. every function f ∈ L 2 ( R ) can be approximated with a wavelet ψ ∈ Ψ with arbitrary accuracy. For that, we consider such a function f ∈ L 2 ( R ) and its Fourier transform ˆ f ∈ L 2 ( R ). We define � ˆ f ( ω ) , if | ω | ≥ ǫ ˆ f ǫ ( ω ) := , 0 , else � ˆ � � which fulfills the wavelet condition. With � f � = � , we obtain f � � � ǫ 2 = 2 d ω → 0 � f − f ǫ � 2 = � � ˆ f − ˆ � � ˆ � � f ( ω ) f ǫ � � � � � � − ǫ for ǫ → 0, which proves the statement.

  5. Wavelets It can be shown easily, that if φ ∈ L 2 ( R ) is differentiable with 0 � ψ := φ ′ ∈ L 2 ( R ), then ψ is a wavelet. This can be used to construct wavelets as in the case of the famous Mexican hat function given by ψ MH ( t ) := − d 2 t exp( − t 2 / 2) = (1 − t 2 )exp( − t 2 / 2) . Moreover, it can be shown, that for all wavelets in L 1 ( R ) the mean value � R ψ ( t )d t = ˆ ψ (0) = 0 vanishes and that for functions ψ ∈ L 1 ( R ) ∩ L 2 ( R ) with compact support the following equivalence holds: � ψ is a wavelet, iff ψ ( t )d t = 0 , R for which reason the famous Haar wavelet ψ Haar satisfies the wavelet condition;  1 , if t ∈ [0 , 1 / 2)    ψ Haar := − 1 , if t ∈ [1 / 2 , 1) .    0 , else  

  6. Continuous-time Wavelet Transform (CTWT) As in the case of the WFT, the continuous-time wavelet transform (CTWT) of a signal is defined as a inner product of the signal itself and musical notes. As already mentioned, starting from a mother wavelet ψ these notes are given by � u − t � ψ s , t : u �→ | s | − 1 / 2 ψ , s in which s ∈ R \ { 0 } denotes a scaling factor and t ∈ R a time shift. Let ψ ∈ L 2 ( R ) be a wavelet. For a given signal f ∈ L 2 ( R ), � � u − t � ˜ f ( s , t ) := � f | ψ s , t � = | s | − 1 / 2 f ( u ) ¯ d u ψ s R with s , t ∈ R , s � 0, defines the CTWT L 2 ( R ) ∋ f �→ ˜ f ∈ H of f with respect to ψ .

  7. Continuous-time Wavelet Transform (CTWT) More precisely, the Hilbert space H is defined by � � H := L 2 ( R 2 − , d s d t / s 2 ) := F : R 2 − → C | F measurable and � F � H < ∞ , − := { ( s , t ) ∈ R 2 | s � 0 } denotes the divided real plane, and inner product in which R 2 and norm are defined by � � F ( s , t )¯ G ( s , t )d s d t / s 2 , � F | G � H := � F � H := � F | F � H R 2 − for F , G ∈ H .

  8. Continuous-time Wavelet Transform (CTWT) Furthermore, for a wavelet ψ ∈ L 2 ( R ) and a signal f ∈ L 2 ( R ) the normalized CTWT is given by � � 1 W ψ := ( f �→ c − 1 / 2 ˜ � f | ψ s , t � ) f ) = f �→ (( s , t ) �→ , √ c ψ ψ which is an isometry, i.e. an injective linear mapping between Hilbert spaces preserving the inner product. Its adjoint operator W ∗ ψ : H → L 2 ( R ) given by � � � u − t � | s | − 1 / 2 ψ ψ [˜ f ]( u ) := c − 1 / 2 ˜ W ∗ f ( s , t )d s d t / s 2 ψ s s ∈ R ∗ t ∈ R inverts the normalized CTWT W ψ on its image. In particular, for f ∈ L 2 ( R ), the following reconstruction formula holds: f = 1 � ˜ f ( s , t ) ψ s , t ( · )d s d t / s 2 . c ψ

  9. Haar’s Theorem According to the reconstruction formula � f = 1 ˜ f ( s , t ) ψ s , t ( · )d s d t / s 2 c ψ f can be reconstructed using appropriate linear combinations from the uncountably infinite wavelet family ( ψ s , t ) ( s , t ) ∈ R 2 − . The classical result from [Haar 1910] shows, that this can even be done with a significant smaller amount of basis functions. In particular, it states that the wavelet family ( Ψ r , k ) r , k ∈ Z defined by � u − k 2 r � r , k ( u ) := ψ 2 r , k 2 r Haar ( u ) = 2 − r / 2 ψ Haar Ψ 2 r is a Hilbert basis of L 2 ( R ).

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