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  2. CIE 1931 color space - Wikipedia

    en.wikipedia.org/wiki/CIE_1931_color_space

    A comparison between a typical normalized M cone's spectral sensitivity and the CIE 1931 luminosity function for a standard observer in photopic vision. In the CIE 1931 model, Y is the luminance, Z is quasi-equal to blue (of CIE RGB), and X is a mix of the three CIE RGB curves chosen to be nonnegative (see § Definition of the CIE XYZ color space).

  3. Interference colour chart - Wikipedia

    en.wikipedia.org/wiki/Interference_colour_chart

    As polarised light passes through a birefringent sample, the phase difference between the fast and slow directions varies with the thickness, and wavelength of light used. The optical path difference (o.p.d.) is defined as o . p . d . = Δ n ⋅ t {\displaystyle {o.p.d.}=\Delta \,n\cdot t} , where t is the thickness of the sample.

  4. Color–color diagram - Wikipedia

    en.wikipedia.org/wiki/Colorcolor_diagram

    The typical axes for infrared colorcolor diagrams have (H–K) on the horizontal axis and (J–H) on the vertical axis (see infrared astronomy for information on band color designations). On a diagram with these axes, stars which fall to the right of the main sequence and the reddening bands drawn are significantly brighter in the K band ...

  5. Template:Spectral colors simple table - Wikipedia

    en.wikipedia.org/wiki/Template:Spectral_colors...

    will display the same table except that the British spelling "colour" is used instead of the American spelling "color". sRGB rendering of the spectrum of visible light Colour

  6. CIELAB color space - Wikipedia

    en.wikipedia.org/wiki/CIELAB_color_space

    The "CIELCh" or "CIEHLC" space is a color space based on CIELAB, which uses the polar coordinates C* (chroma, relative saturation) and h° (hue angle, angle of the hue in the CIELAB color wheel) instead of the Cartesian coordinates a* and b*. The CIELAB lightness L* remains unchanged. The conversion of a* and b* to C* and h° is performed as ...

  7. Dispersion staining - Wikipedia

    en.wikipedia.org/wiki/Dispersion_staining

    These wavelengths combine to produce a single color that can be used to indicate which band of wavelengths are missing (see Chart 2). Examples of this type of dispersion staining and the colors shown for different λo's can be seen at the microlabgallery.com site for Darkfield Dispersion Staining .

  8. Dominant wavelength - Wikipedia

    en.wikipedia.org/wiki/Dominant_wavelength

    In color science, the dominant wavelength is a method of approximating a color's hue. Along with purity , it makes up one half of the Helmholtz coordinates. A color's dominant wavelength is the wavelength of monochromatic spectral light that, if plotted in a chromaticity diagram, the straight line that passes through the color in question and ...

  9. Color space - Wikipedia

    en.wikipedia.org/wiki/Color_space

    Color space conversion is the translation of the representation of a color from one basis to another. This typically occurs in the context of converting an image that is represented in one color space to another color space, the goal being to make the translated image look as similar as possible to the original.