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Standard illuminant : ウィキペディア英語版
Standard illuminant

A standard illuminant is a theoretical source of visible light with a profile (its spectral power distribution) which is published. Standard illuminants provide a basis for comparing images or colors recorded under different lighting.
==CIE illuminants==

The International Commission on Illumination (usually abbreviated CIE for its French name) is the body responsible for publishing all of the well-known standard illuminants. Each of these is known by a letter or by a letter-number combination.
Illuminants A, B, and C were introduced in 1931, with the intention of respectively representing average incandescent light, direct sunlight, and average daylight. Illuminants D represent phases of daylight, Illuminant E is the equal-energy illuminant, while Illuminants F represent fluorescent lamps of various composition.
There are instructions on how to experimentally produce light sources ("standard sources") corresponding to the older illuminants. For the relatively newer ones (such as series D), experimenters are left to measure to profiles of their sources and compare them to the published spectra:〔
Nevertheless, they do provide a measure, called the Metamerism Index, to assess the quality of daylight simulators.〔 Prepared by TC 1-53 "A Standard Method for Assessing the Quality of Daylight Simulators". (ISO Standard 23603:2005(E) ).〕 The Metamerism Index tests how well five sets of metameric samples match under the test and reference illuminant. In a manner similar to the color rendering index, the average difference between the metamers is calculated.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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