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This module describes compressible signals, i.e., signals that can be well-approximated by sparse signals.

Compressibility and K -term approximation

An important assumption used in the context of compressive sensing (CS) is that signals exhibit a degree of structure. So far the only structure we have considered is sparsity , i.e., the number of non-zero values the signal has when representation in an orthonormal basis Ψ . The signal is considered sparse if it has only a few nonzero values in comparison with its overall length.

Few structured signals are truly sparse; rather they are compressible. A signal is compressible if its sorted coefficient magnitudes in Ψ decay rapidly. To consider this mathematically, let x be a signal which is compressible in the basis Ψ :

x = Ψ α ,

where α are the coefficients of x in the basis Ψ . If x is compressible, then the magnitudes of the sorted coefficients α s observe a power law decay:

| α s | C 1 s - q , s = 1 , 2 , . . . .

We define a signal as being compressible if it obeys this power law decay. The larger q is, the faster the magnitudes decay, and the more compressible a signal is. [link] shows images that are compressible in different bases.

The image in the upper left is a signal that is compressible in space. When the pixel values are sorted from largest to smallest, there is a sharp descent. The image in the lower left is not compressible in space, but it is compressible in wavelets since its wavelet coefficients exhibit a power law decay.

Because the magnitudes of their coefficients decay so rapidly, compressible signals can be represented well by K N coefficients. The best K -term approximation of a signal is the one in which the K largest coefficients are kept, with the rest being zero. The error between the true signal and its K term approximation is denoted the K -term approximation error σ K ( x ) , defined as

σ K ( x ) = arg min α Σ K x - Ψ α 2 .

For compressible signals, we can establish a bound with power law decay as follows:

σ K ( x ) C 2 K 1 / 2 - s .

In fact, one can show that σ K ( x ) 2 will decay as K - r if and only if the sorted coefficients α i decay as i - r + 1 / 2   [link] . [link] shows an image and its K -term approximation.

Sparse approximation of a natural image. (a) Original image. (b) Approximation of image obtained by keeping only the largest 10% of the wavelet coefficients. Because natural images are compressible in a wavelet domain, approximating this image it in terms of its largest wavelet coefficients maintains good fidelity.

Compressibility and p Spaces

A signal's compressibility is related to the p space to which the signal belongs. An infinite sequence x ( n ) is an element of an p space for a particular value of p if and only if its p norm is finite:

x p = i | x i | p 1 p < .

The smaller p is, the faster the sequence's values must decay in order to converge so that the norm is bounded. In the limiting case of p = 0 , the “norm” is actually a pseudo-norm and counts the number of non-zero values. As p decreases, the size of its corresponding p space also decreases. [link] shows various p unit balls (all sequences whose p norm is 1) in 3 dimensions.

As the value of p decreases, the size of the corresponding p space also decreases. This can be seen visually when comparing the the size of the spaces of signals, in three dimensions, for which the p norm is less than or equal to one. The volume of these p “balls” decreases with p .

Suppose that a signal is sampled infinitely finely, and call it x [ n ] . In order for this sequence to have a bounded p norm, its coefficients must have a power-law rate of decay with q > 1 / p . Therefore a signal which is in an p space with p 1 obeys a power law decay, and is therefore compressible.

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Source:  OpenStax, An introduction to compressive sensing. OpenStax CNX. Apr 02, 2011 Download for free at http://legacy.cnx.org/content/col11133/1.5
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