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LAST UPDATED: 24 Oct, 2022
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The Munsell tools (Munsell Color System description) enable you to: • convert RGB to Munsell Hue Value/Chroma (select within 24 predefined RGB spaces plus a Custom space); • convert L * a*b * to Munsell HVC (select within 15 predefined illuminants plus a Custom illuminant); • convert Munsell to RGB and L * a*b *; • measure a sample, in reflectance, with one of the ...
https://www.babelcolor.com/cta_munsell.htmPantone certified RIPs have Pantone's defined CIE L * a*b * values included to aid in the conversion of spot into process. Here are Pantone's values for the colors you requested: PANTONE 5483 C 55.09 -18.65 -11.81. PANTONE 417 C 46.86 -1.9 5.77. PANTONE 452 C 72.12 -2.74 16.72.
https://printplanet.com/threads/l-a-b-values-for-pantone-colors.15436/For this, I use images of skin spots in the RGB color space. The code below I can get the colors of each pixel and convert to HSV using color .rgb2lab. But as I want to convert to L * a*b *, because it is closer to human vision, in the python library there is no conversion to L * a*b *.
https://stackoverflow.com/questions/52767317/how-to-convert-rgb-image-pixels-to-labI suppose that the L channel is the first layer of the 3d array due to the shape (3, w, h) img_ l = np.asarray(img_ l , dtype=np.float32) img_ l = torch.from_numpy(img_ l ) # Convert from numpy array to torch tensor.
https://discuss.pytorch.org/t/cie-l-a-b-color-channels-extraction-using-numpy-and-pytorch/80091Is there a way to convert color specifications defined by N. B .S. units in x, y, Y color space under illuminant C, 2° Standard Observer to delta E* values in CIE L * a*b * color space under D65, 10
https://www.researchgate.net/post/Converting_color_specifications_from_x_y_Y_to_CIELab_with_a_twistThe L value for each scale therefore indicates the level of light or dark, the a value redness or greenness, and the b value yellowness or blueness. All three values are required to completely describe an object‘s color. A three-dimensional representation of L, a, b color space is shown below. Hunter l a b
Use the rgb2lab and lab2rgb functions to convert between the RGB and L*a*b* color spaces. The toolbox supports several related color space specifications that are better suited to some purposes than XYZ.
The Lightness value (L*) indicates how light or dark the color is. The a* value indicates the position on the red-green axis, b* is the position on the yellow-blue axis. Once the L*a*b* position of a standard color is determined a rectangular tolerance “box” can be drawn around the standard.
If instead you want the input color space to be linearized Adobe RGB (1998), then you can use the lin2rgb function. For example, to convert linearized Adobe RGB (1998) image RGBlinadobe to the CIE 1976 L*a*b* color space, perform the conversion in two steps:
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