Image::Leptonica::Func::colorspace
version 0.04
colorspace.c
colorspace.c Colorspace conversion between RGB and HSV PIX *pixConvertRGBToHSV() PIX *pixConvertHSVToRGB() l_int32 convertRGBToHSV() l_int32 convertHSVToRGB() l_int32 pixcmapConvertRGBToHSV() l_int32 pixcmapConvertHSVToRGB() PIX *pixConvertRGBToHue() PIX *pixConvertRGBToSaturation() PIX *pixConvertRGBToValue() Selection and display of range of colors in HSV space PIX *pixMakeRangeMaskHS() PIX *pixMakeRangeMaskHV() PIX *pixMakeRangeMaskSV() PIX *pixMakeHistoHS() PIX *pixMakeHistoHV() PIX *pixMakeHistoSV() PIX *pixFindHistoPeaksHSV() PIX *displayHSVColorRange() Colorspace conversion between RGB and YUV PIX *pixConvertRGBToYUV() PIX *pixConvertYUVToRGB() l_int32 convertRGBToYUV() l_int32 convertYUVToRGB() l_int32 pixcmapConvertRGBToYUV() l_int32 pixcmapConvertYUVToRGB()
l_int32 convertHSVToRGB ( l_int32 hval, l_int32 sval, l_int32 vval, l_int32 *prval, l_int32 *pgval, l_int32 *pbval )
convertHSVToRGB() Input: hval, sval, vval &rval, &gval, &bval (<return> RGB values) Return: 0 if OK, 1 on error Notes: (1) See convertRGBToHSV() for valid input range of HSV values and their interpretation in color space.
l_int32 convertRGBToHSV ( l_int32 rval, l_int32 gval, l_int32 bval, l_int32 *phval, l_int32 *psval, l_int32 *pvval )
convertRGBToHSV() Input: rval, gval, bval (RGB input) &hval, &sval, &vval (<return> HSV values) Return: 0 if OK, 1 on error Notes: (1) The range of returned values is: h [0 ... 239] s [0 ... 255] v [0 ... 255] (2) If r = g = b, the pixel is gray (s = 0), and we define h = 0. (3) h wraps around, so that h = 0 and h = 240 are equivalent in hue space. (4) h has the following correspondence to color: h = 0 magenta h = 40 red h = 80 yellow h = 120 green h = 160 cyan h = 200 blue
l_int32 convertRGBToYUV ( l_int32 rval, l_int32 gval, l_int32 bval, l_int32 *pyval, l_int32 *puval, l_int32 *pvval )
convertRGBToYUV() Input: rval, gval, bval (RGB input) &yval, &uval, &vval (<return> YUV values) Return: 0 if OK, 1 on error Notes: (1) The range of returned values is: Y [16 ... 235] U [16 ... 240] V [16 ... 240]
l_int32 convertYUVToRGB ( l_int32 yval, l_int32 uval, l_int32 vval, l_int32 *prval, l_int32 *pgval, l_int32 *pbval )
convertYUVToRGB() Input: yval, uval, vval &rval, &gval, &bval (<return> RGB values) Return: 0 if OK, 1 on error Notes: (1) The range of valid input values is: Y [16 ... 235] U [16 ... 240] V [16 ... 240] (2) Conversion of RGB --> YUV --> RGB leaves the image unchanged. (3) The YUV gamut is larger than the RBG gamut; many YUV values will result in an invalid RGB value. We clip individual r,g,b components to the range [0, 255], and do not test input.
PIX * displayHSVColorRange ( l_int32 hval, l_int32 sval, l_int32 vval, l_int32 huehw, l_int32 sathw, l_int32 nsamp, l_int32 factor )
displayHSVColorRange() Input: hval (hue center value; in range [0 ... 240] sval (saturation center value; in range [0 ... 255] vval (max intensity value; in range [0 ... 255] huehw (half-width of hue range; > 0) sathw (half-width of saturation range; > 0) nsamp (number of samplings in each half-width in hue and sat) factor (linear size of each color square, in pixels; > 3) Return: pixd (32 bpp set of color squares over input range), or null on error Notes: (1) The total number of color samplings in each of the hue and saturation directions is 2 * nsamp + 1.
PIX * pixConvertHSVToRGB ( PIX *pixd, PIX *pixs )
pixConvertHSVToRGB() Input: pixd (can be NULL; if not NULL, must == pixs) pixs Return: pixd always Notes: (1) For pixs = pixd, this is in-place; otherwise pixd must be NULL. (2) The user takes responsibility for making sure that pixs is in our HSV space. The definition of our HSV space is given in convertRGBToHSV(). (3) The h, s and v values are stored in the same places as the r, g and b values, respectively. Here, they are explicitly placed in the 3 MS bytes in the pixel.
PIX * pixConvertRGBToHSV ( PIX *pixd, PIX *pixs )
pixConvertRGBToHSV() Input: pixd (can be NULL; if not NULL, must == pixs) pixs Return: pixd always Notes: (1) For pixs = pixd, this is in-place; otherwise pixd must be NULL. (2) The definition of our HSV space is given in convertRGBToHSV(). (3) The h, s and v values are stored in the same places as the r, g and b values, respectively. Here, they are explicitly placed in the 3 MS bytes in the pixel. (4) Normalizing to 1 and considering the r,g,b components, a simple way to understand the HSV space is: - v = max(r,g,b) - s = (max - min) / max - h ~ (mid - min) / (max - min) [apart from signs and constants] (5) Normalizing to 1, some properties of the HSV space are: - For gray values (r = g = b) along the continuum between black and white: s = 0 (becoming undefined as you approach black) h is undefined everywhere - Where one component is saturated and the others are zero: v = 1 s = 1 h = 0 (r = max), 1/3 (g = max), 2/3 (b = max) - Where two components are saturated and the other is zero: v = 1 s = 1 h = 1/2 (if r = 0), 5/6 (if g = 0), 1/6 (if b = 0)
PIX * pixConvertRGBToHue ( PIX *pixs )
pixConvertRGBToHue() Input: pixs (32 bpp RGB or 8 bpp with colormap) Return: pixd (8 bpp hue of HSV), or null on error Notes: (1) The conversion to HSV hue is in-lined here. (2) If there is a colormap, it is removed. (3) If you just want the hue component, this does it at about 10 Mpixels/sec/GHz, which is about 2x faster than using pixConvertRGBToHSV()
PIX * pixConvertRGBToSaturation ( PIX *pixs )
pixConvertRGBToSaturation() Input: pixs (32 bpp RGB or 8 bpp with colormap) Return: pixd (8 bpp sat of HSV), or null on error Notes: (1) The conversion to HSV sat is in-lined here. (2) If there is a colormap, it is removed. (3) If you just want the saturation component, this does it at about 12 Mpixels/sec/GHz.
PIX * pixConvertRGBToValue ( PIX *pixs )
pixConvertRGBToValue() Input: pixs (32 bpp RGB or 8 bpp with colormap) Return: pixd (8 bpp max component intensity of HSV), or null on error Notes: (1) The conversion to HSV sat is in-lined here. (2) If there is a colormap, it is removed. (3) If you just want the value component, this does it at about 35 Mpixels/sec/GHz.
PIX * pixConvertRGBToYUV ( PIX *pixd, PIX *pixs )
pixConvertRGBToYUV() Input: pixd (can be NULL; if not NULL, must == pixs) pixs Return: pixd always Notes: (1) For pixs = pixd, this is in-place; otherwise pixd must be NULL. (2) The Y, U and V values are stored in the same places as the r, g and b values, respectively. Here, they are explicitly placed in the 3 MS bytes in the pixel. (3) Normalizing to 1 and considering the r,g,b components, a simple way to understand the YUV space is: - Y = weighted sum of (r,g,b) - U = weighted difference between Y and B - V = weighted difference between Y and R (4) Following video conventions, Y, U and V are in the range: Y: [16, 235] U: [16, 240] V: [16, 240] (5) For the coefficients in the transform matrices, see eq. 4 in "Frequently Asked Questions about Color" by Charles Poynton, http://www.poynton.com/notes/colour_and_gamma/ColorFAQ.html
PIX * pixConvertYUVToRGB ( PIX *pixd, PIX *pixs )
pixConvertYUVToRGB() Input: pixd (can be NULL; if not NULL, must == pixs) pixs Return: pixd always Notes: (1) For pixs = pixd, this is in-place; otherwise pixd must be NULL. (2) The user takes responsibility for making sure that pixs is in YUV space. (3) The Y, U and V values are stored in the same places as the r, g and b values, respectively. Here, they are explicitly placed in the 3 MS bytes in the pixel.
l_int32 pixFindHistoPeaksHSV ( PIX *pixs, l_int32 type, l_int32 width, l_int32 height, l_int32 npeaks, l_float32 erasefactor, PTA **ppta, NUMA **pnatot, PIXA **ppixa )
pixFindHistoPeaksHSV() Input: pixs (32 bpp; HS, HV or SV histogram; not changed) type (L_HS_HISTO, L_HV_HISTO or L_SV_HISTO) width (half width of sliding window) height (half height of sliding window) npeaks (number of peaks to look for) erasefactor (ratio of erase window size to sliding window size) &pta (locations of maximum for each integrated peak area) &natot (integrated peak areas) &pixa (<optional return> pixa for debugging; NULL to skip) Return: 0 if OK, 1 on error Notes: (1) pixs is a 32 bpp histogram in a pair of HSV colorspace. It should be thought of as a single sample with 32 bps (bits/sample). (2) After each peak is found, the peak is erased with a window that is centered on the peak and scaled from the sliding window by @erasefactor. Typically, @erasefactor is chosen to be > 1.0. (3) Data for a maximum of @npeaks is returned in @pta and @natot. (4) For debugging, after the pixa is returned, display with: pixd = pixaDisplayTiledInRows(pixa, 32, 1000, 1.0, 0, 30, 2);
PIX * pixMakeHistoHS ( PIX *pixs, l_int32 factor, NUMA **pnahue, NUMA **pnasat )
pixMakeHistoHS() Input: pixs (HSV colorspace) factor (subsampling factor; integer) &nahue (<optional return> hue histogram) &nasat (<optional return> saturation histogram) Return: pixd (32 bpp histogram in hue and saturation), or null on error Notes: (1) pixs is a 32 bpp image in HSV colorspace; hue is in the "red" byte, saturation is in the "green" byte. (2) In pixd, hue is displayed vertically; saturation horizontally. The dimensions of pixd are w = 256, h = 240, and the depth is 32 bpp. The value at each point is simply the number of pixels found at that value of hue and saturation.
PIX * pixMakeHistoHV ( PIX *pixs, l_int32 factor, NUMA **pnahue, NUMA **pnaval )
pixMakeHistoHV() Input: pixs (HSV colorspace) factor (subsampling factor; integer) &nahue (<optional return> hue histogram) &naval (<optional return> max intensity (value) histogram) Return: pixd (32 bpp histogram in hue and value), or null on error Notes: (1) pixs is a 32 bpp image in HSV colorspace; hue is in the "red" byte, max intensity ("value") is in the "blue" byte. (2) In pixd, hue is displayed vertically; intensity horizontally. The dimensions of pixd are w = 256, h = 240, and the depth is 32 bpp. The value at each point is simply the number of pixels found at that value of hue and intensity.
PIX * pixMakeHistoSV ( PIX *pixs, l_int32 factor, NUMA **pnasat, NUMA **pnaval )
pixMakeHistoSV() Input: pixs (HSV colorspace) factor (subsampling factor; integer) &nasat (<optional return> sat histogram) &naval (<optional return> max intensity (value) histogram) Return: pixd (32 bpp histogram in sat and value), or null on error Notes: (1) pixs is a 32 bpp image in HSV colorspace; sat is in the "green" byte, max intensity ("value") is in the "blue" byte. (2) In pixd, sat is displayed vertically; intensity horizontally. The dimensions of pixd are w = 256, h = 256, and the depth is 32 bpp. The value at each point is simply the number of pixels found at that value of saturation and intensity.
PIX * pixMakeRangeMaskHS ( PIX *pixs, l_int32 huecenter, l_int32 huehw, l_int32 satcenter, l_int32 sathw, l_int32 regionflag )
pixMakeRangeMaskHS() Input: pixs (32 bpp rgb) huecenter (center value of hue range) huehw (half-width of hue range) satcenter (center value of saturation range) sathw (half-width of saturation range) regionflag (L_INCLUDE_REGION, L_EXCLUDE_REGION) Return: pixd (1 bpp mask over selected pixels), or null on error Notes: (1) The pixels are selected based on the specified ranges of hue and saturation. For selection or exclusion, the pixel HS component values must be within both ranges. Care must be taken in finding the hue range because of wrap-around. (2) Use @regionflag == L_INCLUDE_REGION to take only those pixels within the rectangular region specified in HS space. Use @regionflag == L_EXCLUDE_REGION to take all pixels except those within the rectangular region specified in HS space.
PIX * pixMakeRangeMaskHV ( PIX *pixs, l_int32 huecenter, l_int32 huehw, l_int32 valcenter, l_int32 valhw, l_int32 regionflag )
pixMakeRangeMaskHV() Input: pixs (32 bpp rgb) huecenter (center value of hue range) huehw (half-width of hue range) valcenter (center value of max intensity range) valhw (half-width of max intensity range) regionflag (L_INCLUDE_REGION, L_EXCLUDE_REGION) Return: pixd (1 bpp mask over selected pixels), or null on error Notes: (1) The pixels are selected based on the specified ranges of hue and max intensity values. For selection or exclusion, the pixel HV component values must be within both ranges. Care must be taken in finding the hue range because of wrap-around. (2) Use @regionflag == L_INCLUDE_REGION to take only those pixels within the rectangular region specified in HV space. Use @regionflag == L_EXCLUDE_REGION to take all pixels except those within the rectangular region specified in HV space.
PIX * pixMakeRangeMaskSV ( PIX *pixs, l_int32 satcenter, l_int32 sathw, l_int32 valcenter, l_int32 valhw, l_int32 regionflag )
pixMakeRangeMaskSV() Input: pixs (32 bpp rgb) satcenter (center value of saturation range) sathw (half-width of saturation range) valcenter (center value of max intensity range) valhw (half-width of max intensity range) regionflag (L_INCLUDE_REGION, L_EXCLUDE_REGION) Return: pixd (1 bpp mask over selected pixels), or null on error Notes: (1) The pixels are selected based on the specified ranges of saturation and max intensity (val). For selection or exclusion, the pixel SV component values must be within both ranges. (2) Use @regionflag == L_INCLUDE_REGION to take only those pixels within the rectangular region specified in SV space. Use @regionflag == L_EXCLUDE_REGION to take all pixels except those within the rectangular region specified in SV space.
l_int32 pixcmapConvertHSVToRGB ( PIXCMAP *cmap )
pixcmapConvertHSVToRGB() Input: colormap Return: 0 if OK; 1 on error Notes: - in-place transform - See convertRGBToHSV() for def'n of HSV space. - replaces: h --> r, s --> g, v --> b
l_int32 pixcmapConvertRGBToHSV ( PIXCMAP *cmap )
pixcmapConvertRGBToHSV() Input: colormap Return: 0 if OK; 1 on error Notes: - in-place transform - See convertRGBToHSV() for def'n of HSV space. - replaces: r --> h, g --> s, b --> v
l_int32 pixcmapConvertRGBToYUV ( PIXCMAP *cmap )
pixcmapConvertRGBToYUV() Input: colormap Return: 0 if OK; 1 on error Notes: - in-place transform - See convertRGBToYUV() for def'n of YUV space. - replaces: r --> y, g --> u, b --> v
l_int32 pixcmapConvertYUVToRGB ( PIXCMAP *cmap )
pixcmapConvertYUVToRGB() Input: colormap Return: 0 if OK; 1 on error Notes: - in-place transform - See convertRGBToYUV() for def'n of YUV space. - replaces: y --> r, u --> g, v --> b
Zakariyya Mughal <zmughal@cpan.org>
This software is copyright (c) 2014 by Zakariyya Mughal.
This is free software; you can redistribute it and/or modify it under the same terms as the Perl 5 programming language system itself.
To install Image::Leptonica, copy and paste the appropriate command in to your terminal.
cpanm
cpanm Image::Leptonica
CPAN shell
perl -MCPAN -e shell install Image::Leptonica
For more information on module installation, please visit the detailed CPAN module installation guide.