Wavelet Denoising¶

This numerical tour uses wavelets to perform non-linear image denoising. $\newcommand{\dotp}[2]{\langle #1, #2 \rangle}$ $\newcommand{\qandq}{\quad\text{and}\quad}$ $\newcommand{\qwhereq}{\quad\text{where}\quad}$ $\newcommand{\qifq}{ \quad \text{if} \quad }$ $\newcommand{\ZZ}{\mathbb{Z}}$ $\newcommand{\RR}{\mathbb{R}}$ $\newcommand{\pa}[1]{\left(#1\right)}$ $\newcommand{\si}{\sigma}$ $\newcommand{\Nn}{\mathcal{N}}$ $\newcommand{\Bb}{\mathcal{B}}$ $\newcommand{\EE}{\mathbb{E}}$ $\newcommand{\norm}[1]{\|#1\|}$ $\newcommand{\abs}[1]{\left|#1\right|}$ $\newcommand{\choice}[1]{ \left\{ \begin{array}{l} #1 \end{array} \right. }$ $\newcommand{\al}{\alpha}$ $\newcommand{\la}{\lambda}$ $\newcommand{\ga}{\gamma}$ $\newcommand{\Ga}{\Gamma}$ $\newcommand{\La}{\Lambda}$ $\newcommand{\si}{\sigma}$ $\newcommand{\Si}{\Sigma}$ $\newcommand{\be}{\beta}$ $\newcommand{\de}{\delta}$ $\newcommand{\De}{\Delta}$ $\newcommand{\phi}{\varphi}$ $\newcommand{\th}{\theta}$ $\newcommand{\om}{\omega}$ $\newcommand{\Om}{\Omega}$

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Image Denoising¶

We consider a simple generative model of noisy images $F = f_0+W$ where $f_0 \in \RR^N$ is a deterministic image of $N$ pixels, and $W$ is a Gaussian white noise distributed according to $\Nn(0,\si^2 \text{Id}_N)$, where $\si^2$ is the variance of noise.

The goal of denoising is to define an estimator $\tilde F$ of $f_0$ that depends only on $F$, i.e. $\tilde F = \phi(F)$ where $\phi : \RR^N \rightarrow \RR^N$ is a potentially non-linear mapping.

Note that while $f_0$ is a deterministic image, both $F$ and $\tilde F$ are random variables (hence the capital letters).

The goal of denoising is to reduce as much as possible the denoising error given some prior knowledge on the (unknown) image $f_0$. A mathematical way to measure this error is to bound the quadratic risk $\EE_w(\norm{\tilde F - f_0}^2)$, where the expectation is computed with respect to the distribution of the noise $W$.

Image loading and adding Gaussian Noise For real life applications, one does not have access to the underlying image $f_0$. In this tour, we however assume that $f_0$ is known, and $f = f_0 + w\in \RR^N$ is generated using a single realization of the noise $w$ that is drawn from $W$. We define the estimated deterministic image as $\tilde f = \phi(f)$ which is a realization of the random vector $\tilde F$.

First we load an image $f_0 \in \RR^N$ where $N=n \times n$ is the number of pixels, and then display it.

Standard deviation $\si$ of the noise.

Then we add Gaussian noise $w$ to obtain $f=f_0+w$.

Display the noisy image.

Hard Thresholding in Wavelet Bases¶

A simple but efficient non-linear denoising estimator is obtained by thresholding the coefficients of $f$ in a well chosen orthogonal basis $\Bb = \{\psi_m\}_m$ of $\RR^N$.

In the following, we will focuss on a wavelet basis, which is efficient to denoise piecewise regular images.

The hard thresholding operator with threshold $T \geq 0$ applied to some image $f$ is defined as $$ S_T^0(f) = \sum_{\abs{\dotp{f}{\psi_m}}>T} \dotp{f}{\psi_m} \psi_m = \sum_m s_T^0(\dotp{f}{\psi_m}) \psi_m $$ where the hard thresholding operator is $$ s_T^0(\alpha) = \choice{ \alpha \qifq \abs{\al}>T, \\ 0 \quad\text{otherwise}. }$ $$

The denoising estimator is then defined as $$ \tilde f = S_T^0(f). $$

Display the function $s_T^0(\al)$ for $T=1$.

Parameters for the orthogonal wavelet transform.

First we compute the wavelet coefficients $a$
of the noisy image $f$.

Display the noisy coefficients.