The images can belong to very different types. In particular, there are images that are highly “graphic” comprised of clear lines, and images that are much more “natural” comprised of many gradients of colours.
Each compression algorithm uses its own data representation. For example, the compression via wavelets separates the image into successive sub-images with frequency transformations, while certain codecs, in particular developed by the applicant take the differences between the numerical values of the image.
The invention therefore proposes to define a codec that automatically selects at encoding the best representation of the data using the type of image data, and carries out the inverse transform at decompression using information contained in the file header.
Each one of the types of algorithms is more or less adapted to certain types of images. In particular, frequency representations model low-contrast images very well while representations via differences model graphic or highly contrasted images well.
Each one of the methods (Differences/Wavelets) can be used in loss or lossless mode. The transformation is applied to each one of the layers separately. On the other hand, the choice of the type of transformation is taken on the layer considered to be the most representative, for example the layer Y in the case of an image that has been subjected beforehand to a YCbCr transform, or the layer that best represents the light intensity of an image in the case of a lossless colorimetric transformation.
When the algorithm used is a transformation via wavelets, this transformation can be carried out by a specific implementation of wavelets and binary encoding, or using standard formats such as Jpeg2000 or PGF. In the following example, and in a non-limiting manner, the wavelet formats used will be Jpeg2000 and PGF.
When the algorithm used is a transformation via differences, the transformation via differences consists in taking the difference between the values of two adjacent pixels over the same layer, then in quantifying this difference by a predefined factor Q. In order to not propagate the error, the difference is taken with respect to a decompressed value defined hereinbelow. In the same way, if two directions of differences are possible, the direction that would generate the lowest difference, using decompressed values, is determined. The difference at compression and decompression is then calculated.
In a more detailed manner, this method of encoding is carried out in the following way:
A matrix to be transformed is considered, representing a layer of an image in 2 dimensions. The following nomenclature is adopted:
Vij is an initial value of the matrix, for which i represents the line number and j the column number. Cij represents the corresponding compressed value, and Dij the corresponding decompressed value. As such, for a 5×5 matrix, the following is the distribution of the values:
Take a numerical example with the following numerical values for each Vij, as well as a quantification coefficient Q=3:
The differences are taken line by line, from the first to the last, from left to right. The first value V11 is retained as is.
In the first horizontal line, for each value V1j, the difference is taken with respect to the decompressed value located to the left thereof D1j−1, then it is quantified and rounded. As such:
D11=C11=V11=0;
C12=ROUND((V12−D11)/Q)=ROUND((0−0)/3)=0
D12=ROUND(D11+(C12*Q))=ROUND(0+0*3)=0
And so on until the end of the line.
For each one of the following lines, the compressed value Ci1 of the first box of said line is calculated by taking a difference between the current value Vi1 and the decompressed value of the line immediately above Di-11:
This will therefore yield, for example for the 2nd line:
C21=ROUND((V21−D11)/Q)=ROUND((0−0)/3)=0
D21=ROUND(D11+(C21*Q))=ROUND(0+(0*3))=0
For each one of the following values of the line, for each value Vij the difference horizontally is calculated if (Di-1 j−D i−1 j−1) is less as an absolute value than (Di j−1−D i−1 j−1), and the difference is calculated vertically in the opposite case.
As such, for the value V22:
As such, for the value V23:
As such, for the value V24:
Through iteration, the following compressed and decompressed values are obtained for this matrix:
When Q=1, this transformation is lossless. When Q>1, it is with losses.
This transformation of data is called “APE”
Once this “APE” transformation has been carried out, an RLE (Run-Length Encoding) transformation is applied then a compression using the Bzip2 algorithm on the data obtained. The compression chain is then as follows, for each one of the layers of the image: APE, RLE, Bzip
In an embodiment, two methods of compression via wavelets are applied, for example Jpeg2000 and PGF, as well as the compression chain APE, RLE, Bzip, described hereinabove, over 3 different images:
The effectiveness of each one of the methods (APE/RLE/Bzip, Jpeg2000, PGF) is represented using a so-called PSNR curve, which represents the quality of the restored image after compression then decompression. Each encoding parameter corresponds to a file size and a value of quality referred to as PSNR, between 0 and 100. The PSNR is a standard measurement, here calculated over the layer Y, with 100 being the best quality possible and corresponds to a lossless compression. It is considered that a compression has better performance than another when, at the equivalent size, it has a better PSNR, or when with an equivalent PSNR, the size is less.
It is therefore observed that:
In a first embodiment of the invention, the choice of the algorithm is taken after the colorimetric transformation, YCbCr in the examples shown.
In order to choose the algorithm, the following is carried out:
In a second embodiment, the number of unique RGB colour triplets of the image is counted, which is reduced to the size of the image, preferably by dividing it by a coefficient according to the number of pixels of the image. When the number of unique RGB colour triplets of the image, reduced to the size of the image, is below a predefined threshold, the image is considered to be a graphics image; when it is above a second threshold, higher than the first, the image is considered to be a low contrast image. Between these two thresholds, the image is considered to be highly contrasted.
The same transformations are then applied as in the first embodiment:
More generally:
A method for compressing an image is therefore proposed, characterised in that:
Advantageously, the calculation is carried out over all of a layer that is most representative of the image (for example the layer Y)
Advantageously, these steps can be preceded by a colorimetric transformation, with loss or lossless, on the input data. For example, a YCbCr transformation can be applied on the RGB input data.
In order to classify the image, with each hue corresponding to a hue value (preferably k=0-255 in the case of 8-bit layers), for each hue the number n(k) of pixels having this hue is calculated; then, an indicator of the concentration of the hues of the image around the value k is calculated, for example:
E(k)=n(k)−0.4(n(k−1)+n(k+1))−0.1(n(k−2)+n(k+2)),
by taking the difference between the number of pixels n(k) of the hue (k) considered and a proportion of those of its neighbours, preferably of its first-row (k−1 and k+1) and second-row (k−2 and k+2) neighbours, with the respective proportion being more reduced for the neighbours of the highest row, for example a proportion of 80% for each one of the first-row neighbours, i.e. the immediate neighbours of the hue (k) considered and of 20% for each one of the second-row neighbours, i.e. the immediate neighbours of the first-row neighbours.
Preferably, the sum of the proportions of the neighbouring values is equal to one. In the example shown, the sum of the proportions is effectively equal to 1 (0.4+0.4+0.1+0.1=1).
The indicator of the concentration of the hues around values k (E(k)) is then maintained higher than a certain threshold, preferably the positive indicators of concentration, i.e. Max(E(k),0), and each one of the indicators of concentration is reduced to the size of the image, for example to the total number (N) of pixels of the image.
Preferably, for better discrimination between the types of images, i.e. in order to facilitate classification, the result Max(E(k))/N is then raised to a power strictly greater than 1, preferably equal to 2.
A metric (FD) is then obtained by compiling these results for all of the layer, preferably by taking the sum of the results obtained as such for all of the hues of the layer. As such, in the example shown:
FD2=Σ(Max(E(k))/N)2,
Number | Date | Country | Kind |
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14 01695 | Jul 2014 | FR | national |
Filing Document | Filing Date | Country | Kind |
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PCT/FR2015/000142 | 7/9/2015 | WO | 00 |
Publishing Document | Publishing Date | Country | Kind |
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WO2016/012667 | 1/28/2016 | WO | A |
Number | Name | Date | Kind |
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7457360 | Otsuka | Nov 2008 | B2 |
20040179742 | Li | Sep 2004 | A1 |
20070133017 | Kobayashi | Jun 2007 | A1 |
20110147457 | Cha | Jun 2011 | A1 |
20130003086 | Mebane | Jan 2013 | A1 |
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Number | Date | Country | |
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20170213107 A1 | Jul 2017 | US |