Physics 
        of Color 
       
        The colors of the visible light spectrum. 
      color wavelength interval frequency interval  
        red ~ 625-740 nm ~ 480-405 THz  
        orange ~ 590-625 nm ~ 510-480 THz  
        yellow ~ 565-590 nm ~ 530-510 THz  
        green ~ 500-565 nm ~ 600-530 THz  
        cyan ~ 485-500 nm ~ 620-600 THz  
        blue ~ 440-485 nm ~ 680-620 THz  
        violet ~ 380-440 nm ~ 790-680 THz  
        Continuous optical spectrum 
      Designed for monitors with gamma 1.5. 
         
        Computer "spectrum" 
      The bars below show the relative intensities of the three 
        colors mixed to make the color immediately above. 
         
        Color, frequency, and energy of light. 
       
        Color /nm /1014 Hz /104 cm-1 /eV /kJ mol-1  
        Infrared >1000 <3.00 <1.00 <1.24 <120  
        Red 700 4.28 1.43 1.77 171  
        Orange 620 4.84 1.61 2.00 193  
        Yellow 580 5.17 1.72 2.14 206  
        Green 530 5.66 1.89 2.34 226  
        Blue 470 6.38 2.13 2.64 254  
        Violet 420 7.14 2.38 2.95 285  
        Near ultraviolet 300 10.0 3.33 4.15 400  
        Far ultraviolet <200 >15.0 >5.00 >6.20 >598  
        Electromagnetic radiation is a mixture of radiation of different wavelengths 
        and intensities. When this radiation has a wavelength inside the human 
        visibility range (approximately from 380 nm to 740 nm), it is called light. 
        The light's spectrum records each wavelength's intensity. The full spectrum 
        of the incoming radiation from an object determines the visual appearance 
        of that object, including its perceived color. As we will see, there are 
        many more spectra than color sensations; in fact one may formally define 
        a color to be the whole class of spectra which give rise to the same color 
        sensation, although any such definition would vary widely among different 
        species and also somewhat among individuals intraspecifically. 
      A surface that diffusely reflects all wavelengths equally is perceived 
        as white, while a dull black surface absorbs all wavelengths and does 
        not reflect (for mirror reflection this is different: a proper mirror 
        also reflects all wavelengths equally, but is not perceived as white, 
        while shiny black objects do reflect). 
      The familiar colors of the rainbow in the spectrum—named from the 
        Latin word for appearance or apparition by Isaac Newton in 1671—contains 
        all those colors that consist of visible light of a single wavelength 
        only, the pure spectral or monochromatic colors. 
      The frequencies are approximations and given in terahertz (THz). The 
        wavelengths, valid in vacuum, are given in nanometers (nm). A list of 
        other objects of similar size is available. 
       
        Important note 
        The color table should not be interpreted as a definite list—the 
        pure spectral colors form a continuous spectrum, and how it is divided 
        into distinct colors is a matter of taste and culture; for example, Isaac 
        Newton identified the seven colors red, orange, yellow, green, blue, indigo, 
        and violet, remembered by many school children using mnemonics such as 
        Roy G. Biv, Richard Of York Gave Battle In Vain and VIBGYOR. Similarly, 
        the intensity of a spectral color may alter its perception considerably; 
        for example, a low-intensity orange-yellow is brown, and a low-intensity 
        yellow-green is olive-green. 
       
        Spectral versus non-spectral colors 
        Most light sources are not pure spectral sources; rather they are created 
        from mixtures of various wavelengths and intensities of light. To the 
        human eye, however, there is a wide class of mixed-spectrum light that 
        is perceived the same as a pure spectral color. In the table above, for 
        instance, when your computer screen is displaying the "orange" 
        patch, it is not emitting pure light at a fixed wavelength of around 600 
        nm (which is in fact not a thing most computer screens are even able to 
        do). Rather, it is emitting a mixture of about two parts red to one part 
        green light. Were you to print this page on a color printer, the orange 
        patch on the paper, when lit with white light, would reflect yet another, 
        more continuous spectrum. We cannot see those differences (although many 
        animals can), and the reason has to do with the pigments that make up 
        our color vision cells (see below). 
      A useful quantification of this property is the dominant wavelength, 
        which matches a wavelength of spectral light to a non-spectral source 
        that evokes the same color perception. Dominant wavelength is the formal 
        background for the popular concept of hue. 
      In addition to the many light sources that can appear to be pure spectral 
        colors but are actually mixtures, there are many color perceptions that 
        by definition cannot be pure spectral colors due to desaturation or because 
        they are purples (which do not appear in the Newtonian pure spectrum). 
        Some examples of necessarily non-spectral colors are the achromatic colors 
        (black, gray and white) and other colors such as pink, tan and magenta. 
        See metamerism (color) for a basic intro to why color matching challenges 
        exist. 
        
       Color in 
        the wave equation 
        The wave equation describes the behavior of light and so we should be 
        able to describe color spectra in terms of the mathematical properties 
        of the solutions of the wave equation. However, to understand which particular 
        color perception will arise from a particular physical spectrum requires 
        knowledge of the specific retinal physiology of the observer. For completeness, 
        we include a simple equation for light traveling in a vacuum: 
      utt=c2(uxx+uyy+uzz)  
        where the subscripts denote partial derivatives and c is the speed of 
        light. If we fix (x,y,z) a point in space and look at the solution u(x,y,z,t) 
        as a function of t, we obtain a signal. If we take the Fourier transform 
        of this signal, we obtain a frequency decomposition as described above. 
        Each frequency has an amplitude and phase. The frequency multiplied by 
        Planck's constant h determines the energy of a photon of the relevant 
        component. The square of the amplitude represents the intensity, which 
        is the amount of energy transmitted per second through a unit area of 
        a surface perpendicular to the light propagation. The phase information 
        is much more mysterious because it is difficult to measure and observe. 
        Humans cannot perceive phase effects of light except in special cases 
        of interference (e.g. see thin-film optics) where phase effects lead to 
        perceptible amplitude changes. Most light has randomly distributed phases, 
        but lasers are more efficient when the photons all have the same phase. 
       
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