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DigitalVideoAndHDTVAlgorithmsAndInterfaces.pdf

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Luminous efficiency, relative<br />

1.0<br />

0.5<br />

0.0<br />

V(λ),<br />

Scotopic<br />

I presented a brief introduction to<br />

Lightness terminology on page 11.<br />

Publication CIE 15.2, Colorimetry,<br />

Second Edition (Vienna, Austria:<br />

Commission Internationale de<br />

L’Éclairage, 1986); reprinted with<br />

corrections in 1996.<br />

Y(λ),<br />

Photopic<br />

400 500 600 700<br />

Wavelength, λ, nm<br />

Figure 20.1 Luminous efficiency functions. The solid line indicates the luminance response of the<br />

cone photoreceptors – that is, the CIE photopic response. A monochrome scanner or camera must<br />

have this spectral response in order to correctly reproduce lightness. The peak occurs at about<br />

555 nm, the wavelength of the brightest possible monochromatic 1 mW source. (The lightly<br />

shaded curve shows the scotopic response of the rod cells – loosely, the response of night vision.<br />

The increased relative luminance of blue wavelengths in scotopic vision is called the Purkinje shift.)<br />

Until 2000, Y(λ) had the symbol<br />

y _ , pronounced WYE-bar. The<br />

luminous efficiency function has<br />

also been denoted V(λ),<br />

pronounced VEE-lambda.<br />

Luminance<br />

The Commission Internationale de L’Éclairage (CIE, or<br />

International Commission on Illumination) is the international<br />

body responsible for standards in the area of<br />

color. The CIE defines brightness as the attribute of<br />

a visual sensation according to which an area appears to<br />

exhibit more or less light. Brightness is, by the CIE’s definition,<br />

a subjective quantity: It cannot be measured.<br />

The CIE has defined an objective quantity that is related<br />

to brightness. Luminance is defined as radiance<br />

weighted by the spectral sensitivity function – the sensitivity<br />

to power at different wavelengths – that is characteristic<br />

of vision. The luminous efficiency of the CIE<br />

Standard Observer, denoted Y(λ), is graphed as the<br />

black line of Figure 20.1 above. It is defined numerically,<br />

is everywhere positive, and peaks at about<br />

555 nm. When a spectral power distribution (SPD) is<br />

integrated using this weighting function, the result is<br />

luminance, denoted Y. In continuous terms, luminance<br />

is an integral of spectral radiance across the spectrum.<br />

In discrete terms, it is a dot product. The magnitude of<br />

CHAPTER 20 LUMINANCE AND LIGHTNESS 205

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