Color Engineering: Colorimetry
Dr. Wayne Cheng http://color.di.nctu.edu.tw
Reference Books
R. G. Kuehni, Kuehni, Color: An Introduction to Practice and Principles, 2nd Ed., WileyWiley-Interscience, Interscience, 2005. M. D. Fairchild, Color Appearance Models, WileyWileyIS&T, 2005 G. Wyszecki and W. S. Stiles, Color Science, John Wiley & Sons, 1982. R. G. W. Hunt, The Reproduction of Colour, Colour, 5th Ed., England: Fountain Press, 1995. Billmeyer and Saltzman, Saltzman, Principles of Color Technology, 3rd Ed., WileyWiley-Interscience, Interscience, 2000. Fundamentals of Color and Appearance, GretagMacbeth. GretagMacbeth.
Available online
Color appearance phenomena and models
Comprehensive data
Outline
Colorimetry
Chromaticity Photometry Color
diagram
spaces Color difference
Color appearance
Color
appearance terminology Color appearance phenomena
Chromaticity Diagram
CIE
International Commission on Illlumination Commision Internationale de IEclairage
CIEXYZ
CIEXYZ Chromaticity Diagram
(x,y) x,y) in CIEXYZ Visible spectrum Nominal scales Spectral locus Purple line White point Dominant wavelength Complement Mixture rules Black body curve Color temperature
Spectral Locus
Purple Line
Purples and magentas Mixture of red and blue Cannot be mixed from white and a single spectral color Non-spectral color Complement of green 550C
Dominant Wavelength
Line passing C, white, and spectral locus Polar coordinates (geometrical coordinates) Purple line: complement
Purity
Ratio of CW and CL How to mixture
Imaginary Color Stimuli
CIEXYZ Chromaticit y Diagram
(x,y) x,y) in CIEXYZ Visible spectrum Nominal scales Spectral locus Purple line White point Dominant wavelength Complement Mixture rules Black body curve Color temperature
Luminous efficiency functions
Photometry
Radiometry
Energy Power Radiant Intensity Irradiance Radiance
Color Science, Wyszechi & Stiles
Steradian: solid angle
Color Science, Wyszechi & Stiles
Photometry
Luminous Intensity
Photometry Example
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Luminous efficiency functions
CIE 1924
System of Photometry
A spectral weighting function that could be used to describe the perception of brightness matches Convert radiometry into photometry
Irradiance ~ illuminance Radiance ~ luminance Reflectance factor ~ luminance factor
Photopic: Photopic: cones Scotopic: Scotopic: rods
How about colors?
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Colorimetry
Basic Colorimetry
A tool used to make a prediction on whether two lights of different spectral power distributions will match in color for certain given conditions of observation.
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Three Parties in Colorimetry
Objects
Viewing geometries
Observers
Standard observers
Illuminants
Light sources
BlackBlack-body
radiators CIE illuminants
Viewing Geometry
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CIE Viewing geometry: D/0, 0/D
Diffuse/Normal
The sample is illuminated from all angles Viewed at an angle near the normal
Normal/Diffuse
Sphere at ITRI
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CIE Viewing geometry: 45/0, 0/45
Normal/45 45/Normal
CIE Standard Illuminants
D65
Daylight at 6500K
D50
Daylight at 5000K
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CIE Standard Illuminants
A: A gas-filled coiled-tungsten filament lamp operating at a correlated color temperature of 2856K B, C: filtered A E: uniform distribution F2: fluorescent source
Popular Light Sources
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Standard Observer
Luminous efficiency functions From radiometry to photometry
CIE 1924
System of Photometry
A spectral weighting function that could be used to describe the perception of brightness matches Convert radiometry into photometry
Irradiance ~ illuminance Radiance ~ luminance Reflectance factor ~ luminance factor
CIE 1988
Photopic: Photopic: cones Scotopic: Scotopic: rods
Spectral luminous efficiency function VM()
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Photopic, Mesopic, and Scotopic
Rod and Cone
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Color Vision
Prof. Lance Williams @ cs.unm.edu
Color Spaces
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Color Spaces
CIERGB CIEXYZ NTSC YIQ CIELab CIELuv
Newtons Hue Circle
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Color Matching Functions
Two CIE standard observers
CIE 1931 2 deg RGB CIE 1931 2 deg XYZ CIE 1964 10 deg
Two individuals with different visions
Color Matching
C: color to match W: reference white P1, P2, P3: R, G, B
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Axioms of Color Matching
Any color can be matched by a mixture of no more than three colored lights A color match at one radiance level holds over a wide range of levels Components of a mixture of colored lights cannot be resolved by the human eye The luminance of a color mixture is equal to the sum of the luminance of its components
Trichromatic Generalization
Grassmans three laws of additive color mixture Binary relation of color matching = ::= color matching Symmetry law Transitivity law
a=b => b=a a=b; b=c => a=c a=b => s*a=s*b s*a=s*b
Proportionality law Additivity law
a=b; c=d => a+c= a+c=b+d
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CIERGB 1931
R = ( ) r ( ) d
G = ( ) g ( )d
B = ( )b ( )d
Plane of x+y+z=1
x=X/(X+Y+Z) y=Y/(X+Y+Z) z=Z/(X+Y+Z) x+y+z=1
cs.rit.edu
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White point?
x = y = z = 1/3 CIE Illuminant C
CIERGB chromaticity diagram
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CIEXYZ 1931
X = k ( ) x ( ) d
Y = k ( ) y ( ) d
Z = k ( ) z ( ) d
CIERGB vs. CIEXYZ
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CIEXYZ 1931 Standard Observer
Using a visual field of 2 deg 2 deg color matching functions (2 deg observer) Not representative
Fewer than 20 observers
CIE 1964 Standard Observer
Using a larger visual field of 10 deg 49 observers 10 deg color matching functions (10 deg observer) Excluded central fovea
macular absorption
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Why So Many Color Spaces?
From CIERGB to CIEXYZ
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CIERGB and CIEXYZ
YIQ NTSC
National Television Systems Committee Y=luminance; for black-and-white TV sets (I,Q)=(hue, saturation)
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NTSC YIQ decomposition
Just Noticeable Color Difference (JNCD)
Why different color spaces? A unit of sensation difference Any given luminance x = 0 Increase x until x is just-noticeably brighter than x; x=1 x = 2
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JNCD in XYZ
MacAdams ellipses Just noticeable color difference in XYZ
CIEUCS UVW 1976
Uniform Chromaticity Scale (UCS)
Equal change in chromaticity coordinates results in equal just noticeable changes in the perceived hue and saturation of a color UVW: V=luminance
u = 4x / ((-2x+12y+3) v = 6y / ((-2x+12y+3) x = 3u / (2u(2u-8v8v-4) y = 2v / (2u(2u-8v8v-4)
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UVW decomposition
JNCD in UVW
Just noticeable color difference in UVW
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Nonlinear Transform in XYZ
Opponent Colors
Red Green Yellow - Blue
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CIELAB 1976
For computational simple measure of color L* = brightness
0-100
a* = redness-greenness
+/-
L * = 116 (
Y 13 ) 16 Yn
b* = yellowness-blueness
+/-
X 13 Y 13 ( ) a * = 500 ( X ) Y n n
Y 13 Z 13 b * = 200 ) ( (Y ) Zn n
Xn,Yn,Zn: reference white
CIELab decomposition
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CIELUV 1976
From CIELab and U*V*W* Cartesian
L*: lightness u*: rednessredness-greenness v*: yellownessyellowness-blueness
Y 13 ) 16 Yn u * = 13 L* (u 'u 'n ) L* = 116(
Cylindrical
L*: lightness C*uv: chroma Huv: Huv: hue
v* = 13L* (v 'v 'n )
* Cuv =
(u
*2
+ v*2
CIELCh
Polar coordinates of CIELab L*: lightness
0 100
C*: chroma
Distance from the neutral axis
h: hue
0 - 360
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CMC (l:c)
Color Measurement Committee
Of the Society of Dyers and Colorists
Intensity, Hue, and Saturation
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Munsell Color Space
Color Difference
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Color Difference
Goal: color differences be perceptually uniform throughout the space One unit difference in red is perceived to be equal in magnitude to a unit difference in gray Based on CIELAB Eab*, LCabHab
CIELAB Eab*
Based on CIELAB Euclidean distance E * = (L* 2 + a * 2 + b* 2 ) ab between two coordinates In terms of lightness, red-green, yellow-blue In terms of lightness, chroma, and hue differences
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CIE94 LCabHab
CIE94 Eab*=LCabHab kL, kC, kH,: adjust relative weighting
Other Color Differences
Delta E DRG
Delta Red/Green
DYB
Delta Yellow/Blue
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Black-body Radiators
Black-body radiators (Planckian radiators) Plancks Law
Wiens Law
Color Temperature
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