Standard illuminant

Relativespectral power distributions(SPDs) of CIE illuminants A, B, and C from380 nmto780 nm.

Astandard illuminantis a theoretical source ofvisible lightwith aspectral power distributionthat is published. Standard illuminants provide a basis for comparing images or colors recorded under different lighting.

CIE illuminants

TheInternational Commission on Illumination(usually abbreviatedCIEfor 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 (1967) represent variations of daylight, illuminant E is the equal-energy illuminant, while illuminants F (2004) 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:

At present no artificial source is recommended to realize CIE standard illuminant D65 or any other illuminant D of different CCT. It is hoped that new developments in light sources and filters will eventually offer sufficient basis for a CIE recommendation.

— CIE, Technical Report (2004) Colorimetry, 3rd ed., Publication 15:2004, CIE Central Bureau, Vienna

Nevertheless, they do provide a measure, called themetamerism index,to assess the quality of daylight simulators.TheMetamerismIndex tests how well five sets of metameric samples match under the test and reference illuminant. In a manner similar to thecolor rendering index,the average difference between the metamers is calculated.

Illuminant A

The CIE defines illuminant A in these terms:

CIE standard illuminant A is intended to represent typical, domestic, tungsten-filament lighting. Its relative spectral power distribution is that of a Planckian radiator at a temperature of approximately 2856 K. CIE standard illuminant A should be used in all applications of colorimetry involving the use of incandescent lighting, unless there are specific reasons for using a different illuminant.

— CIE,CIE Standard Illuminants for Colorimetry

Thespectral radiant exitanceof ablack bodyfollowsPlanck's law:

$M_{e,\lambda }(\lambda,T)={\frac {c_{1}\lambda ^{-5}}{\exp \left({\frac {c_{2}}{\lambda T}}\right)-1}}.$

At the time of standardizing illuminant A, both$c_{1}=2\pi \cdot h\cdot c^{2}$(which does not affect the relative SPD) and$c_{2}=h\cdot c/k$were different. In 1968, the estimate of c₂was revised from 0.01438 m·K to 0.014388 m·K (and before that, it was 0.01435 m·K when illuminant A was standardized). This difference shifted thePlanckian locus,changing the color temperature of the illuminant from its nominal 2848 K to 2856 K:

$T_{new}=T_{old}\times {\frac {1.4388}{1.435}}=2848\ {\text{K}}\times 1.002648=2855.54\ {\text{K}}.$

In order to avoid further possible changes in the color temperature, the CIE now specifies the SPD directly, based on the original (1931) value of c₂:

$S_{A}(\lambda )=100\left({\frac {560}{\lambda }}\right)^{5}{\frac {\exp {\frac {1.435\times 10^{7}}{2848\times 560}}-1}{\exp {\frac {1.435\times 10^{7}}{2848\lambda }}-1}}.$

The coefficients have been selected to achieve a normalized SPD of100at560 nm.The tristimulus values are(X,Y,Z) = (109.85, 100.00, 35.58),and the chromaticity coordinates using the standard observer are(x,y) = (0.44758, 0.40745).

Illuminants B and C

Illuminants B and C are easily achieved daylight simulations. They modify illuminant A by using liquid filters. B served as a representative of noon sunlight, with acorrelated color temperature(CCT) of 4874 K, while C represented average day light with a CCT of 6774 K. Unfortunately, they are poor approximations of any phase of natural daylight, particularly in the short-wave visible and in the ultraviolet spectral ranges. Once more realistic simulations were achievable, illuminants B and C were deprecated in favor of the D series.

Illuminant C does not have the status of CIE standard illuminants but its relative spectral power distribution, tristimulus values and chromaticity coordinates are given in Table T.1 and Table T.3, as many practical measurement instruments and calculations still use this illuminant.

— CIE, Publication 15:2004

Illuminant B was not so honored in 2004.

The liquid filters, designed byRaymond Davis, Jr.and Kasson S. Gibson in 1931,have a relatively high absorbance at the red end of the spectrum, effectively increasing the CCT of theincandescent lampto daylight levels. This is similar in function to a CTBcolor gelthat photographers and cinematographers use today, albeit much less convenient.

Each filter uses a pair of solutions, comprising specific amounts of distilled water,copper sulfate,mannite,pyridine,sulfuric acid,cobalt,andammonium sulfate.The solutions are separated by a sheet of uncolored glass. The amounts of the ingredients are carefully chosen so that their combination yields a color temperature conversion filter; that is, the filtered light is still white.

Illuminant series D

Relative spectral power distribution of illuminant D and a black body of the same correlated color temperature (in red), normalized about560 nm.

TheDseries of illuminants are designed to represent natural daylight and lie along thedaylight locus.They are difficult to produce artificially, but are easy to characterize mathematically.

By 1964, several spectral power distributions (SPDs) of daylight had been measured independently by H. W. Budde of theNational Research Council of CanadainOttawa,H. R. Condit and F. Grum of theEastman Kodak CompanyinRochester, New York,and S. T. Henderson and D. Hodgkiss ofThorn Electrical IndustriesinEnfield (north London),totaling among them 622 samples.Deane B. Judd,David MacAdam,andGünter Wyszeckianalyzed these samples and found that the(x,y) chromaticity coordinatesfollowed a simple,quadraticrelation, later known as the daylight locus:

$y=2.870x-3.000x^{2}-0.275.$

Characteristic vector analysisrevealed that the SPDs could be satisfactorily approximated by using the mean (S₀) and first two characteristic vectors (S₁and S₂):

$S_{D}(\lambda )=S_{0}(\lambda )+M_{1}S_{1}(\lambda )+M_{2}S_{2}(\lambda ).$

Characteristic vectors of illuminant D; component SPDs S₀(blue), S₁(green), S₂(red).

In simpler terms, the SPD of the studied daylight samples can be expressed as thelinear combinationof three, fixed SPDs. The first vector (S₀) is the mean of all the SPD samples, which is the best reconstituted SPD that can be formed with only a fixed vector. The second vector (S₁) corresponds to yellow–blue variation (along the locus), accounting for changes in thecorrelated color temperaturedue to proportion of indirect to direct sunlight.The third vector (S₂) corresponds to pink–green variation (across the locus) caused by the presence of water in the form of vapor and haze.

ThePlanckian locusis depicted on theCIE 1960 UCS,along with isotherms (lines of constantcorrelated color temperature) and representative illuminant coordinates

By the time the D-series was formalized by the CIE,a computation of the chromaticity$(x,y)$for a particular isotherm was included.Juddet al.then extended the reconstituted SPDs to300 nm–330 nmand700 nm–830 nmby using Moon's spectral absorbance data of the Earth's atmosphere.The tabulated SPDs presented by the CIE today are derived bylinear interpolationof the10 nmdata set down to5 nm.However, there is a proposal to usespline interpolationinstead.

Similar studies have been undertaken in other parts of the world, or repeating Juddet al.'s analysis with modern computational methods. In several of these studies, the daylight locus is notably closer to the Planckian locus than in Juddet al.

The CIE positions D65 as the standard daylight illuminant:

[D65] is intended to represent average daylight and has a correlated colour temperature of approximately 6500 K. CIE standard illuminant D65 should be used in all colorimetric calculations requiring representative daylight, unless there are specific reasons for using a different illuminant. Variations in the relative spectral power distribution of daylight are known to occur, particularly in the ultraviolet spectral region, as a function of season, time of day, and geographic location.

— ISO 10526:1999/CIE S005/E-1998, CIE Standard Illuminants for Colorimetry

Daylight locus in the CIE 1960 UCS. The isotherms are perpendicular to the Planckian locus. The two sections of the daylight locus, from 4000–7000 K and 7000–25000 K, are color-coded. Note that the two loci are separated by a fairly even distance, of around$\Delta _{uv}=0.003$.

Computation

The relativespectral power distribution(SPD)$S_{D}(\lambda )$of a D series illuminant can be derived from itschromaticity coordinatesin theCIE 1931 color space,$(x_{D},y_{D})$.First, the chromaticity coordinates must be determined:

$x_{D}={\begin{cases}0.244063+0.09911{\frac {10^{3}}{T}}+2.9678{\frac {10^{6}}{T^{2}}}-4.6070{\frac {10^{9}}{T^{3}}}&4000\ \mathrm {K} \leq T\leq 7000\ \ \mathrm {K} \\0.237040+0.24748{\frac {10^{3}}{T}}+1.9018{\frac {10^{6}}{T^{2}}}-2.0064{\frac {10^{9}}{T^{3}}}&7000\ \mathrm {K} <T\leq 25000\ \mathrm {K} \end{cases}}$

$y_{D}=-3.000x_{D}^{2}+2.870x_{D}-0.275$

whereTis the illuminant's CCT. Note that the CCTs of the canonical illuminants, D₅₀,D₅₅,D₆₅,and D₇₅,differ slightly from what their names suggest. For example, D50 has a CCT of 5003 K ( "horizon" light), whileD65has a CCT of 6504 K (noon light). This is because the value of the constants in Planck's law have been slightly changed since the definition of these canonical illuminants, whose SPDs are based on the original values in Planck's law.The same discrepancy applies to all illuminants in the D series—D₅₀,D₅₅,D₆₅,D₇₅—and can be "rectified" by multiplying the nominal color temperature by${\frac {c_{2}}{1.4380}}$;for example$6500\ {\text{K}}\times {\frac {1.438776877\dots }{1.4380}}=6503.51\ {\text{K}}$for D₆₅.

To determine the D-series SPD (S_D) that corresponds to those coordinates, the coefficients M₁and M₂of the characteristic vectors S₁and S₂are determined:

$S_{D}(\lambda )=S_{0}(\lambda )+M_{1}S_{1}(\lambda )+M_{2}S_{2}(\lambda ),$

$M_{1}=(-1.3515-1.7703x_{D}+5.9114y_{D})/M,$

$M_{2}=(0.0300-31.4424x_{D}+30.0717y_{D})/M,$

$M=0.0241+0.2562x_{D}-0.7341y_{D}$

where$S_{0}(\lambda ),S_{1}(\lambda ),S_{2}(\lambda )$are the mean and first twoeigenvectorSPDs, depicted in figure.The characteristic vectors both have a zero at560 nm,since all the relative SPDs have been normalized about this point. In order to match all significant digits of the published data of the canonical illuminants the values of M₁and M₂have to be rounded to three decimal places before calculation ofS_D.

D65 values

Using thestandard 2° observer,theCIE 1931 color spacechromaticity coordinatesof D65 are

$${\begin{aligned}x&=0.31272\\y&=0.32903\end{aligned}}$$

and theXYZ tristimulus values(normalized toY= 100), are

$${\begin{alignedat}{2}X&={}&95.047\\Y&={}&100{\phantom {.000}}\\Z&={}&108.883\end{alignedat}}$$

For thesupplementary 10° observer,

$${\begin{aligned}x&=0.31382\\y&=0.33100\end{aligned}}$$ and the corresponding XYZ tristimulus values are

$${\begin{alignedat}{2}X&={}&94.811\\Y&={}&100{\phantom {.000}}\\Z&={}&107.304\end{alignedat}}$$

Since D65 representswhitelight, its coordinates are also awhite point,corresponding to acorrelated color temperatureof 6504 K.Rec. 709,used inHDTVsystems, truncates the CIE 1931 coordinates to x=0.3127, y=0.329.

Daylight simulator

There are no actual daylight light sources, only simulators. Constructing a practical light source that emulates a D-series illuminant is a difficult problem. The chromaticity can be replicated simply by taking a well known light source and applying filters, such as the Spectralight III, that used filtered incandescent lamps.However, the SPDs of these sources deviate from the D-series SPD, leading to bad performance on the CIEmetamerism index.Better sources were achieved in the 2010s withphosphor-coated white LEDsthat can easily emulate the A, D, and E illuminants with high CRI.

Illuminant E

Illuminant E is beneath thePlanckian locus,and roughly at theCCTof D₅₅.

Illuminant E is an equal-energy radiator; it has a constant SPD inside thevisible spectrum.It is useful as a theoretical reference; an illuminant that gives equal weight to all wavelengths. It also has equalCIE XYZtristimulus values, thus its chromaticity coordinates are (x,y)=(1/3,1/3). This is by design; the XYZ color matching functions are normalized such that their integrals over the visible spectrum are the same.

Illuminant E is not a black body, so it does not have a color temperature, but it can be approximated by a D series illuminant with a CCT of 5455 K. (Of the canonical illuminants, D₅₅is the closest.) Manufacturers sometimes compare light sources against illuminant E to calculate theexcitation purity.

Illuminant series F

TheFseries of illuminants represent various types offluorescent lighting.

F1–F6 "standard" fluorescent lamps consist of two semi-broadband emissions ofantimonyandmanganeseactivations in calcium halophosphatephosphor.F4 is of particular interest since it was used for calibrating the CIEcolor rendering index(the CRI formula was chosen such that F4 would have a CRI of 51). F7–F9 are "broadband" (full-spectrum light) fluorescent lamps with multiple phosphors, and higher CRIs. Finally, F10–F12 are narrow triband illuminants consisting of three "narrowband" emissions (caused by ternary compositions of rare-earth phosphors) in the R,G,B regions of the visible spectrum. The phosphor weights can be tuned to achieve the desired CCT.

The spectra of these illuminants are published in Publication 15:2004.

• 
  FL 1–6:Standard
• 
  FL 7–9:Broadband
• 
  FL 10–12:Narrowband

Illuminant series LED

Publication 15:2018 introduces new illuminants for differentwhite LEDtypes with CCTs ranging from approx. 2700 K to 6600 K.

LED-B1 through B5 defines LEDs with phosphor-converted blue light. LED-BH1 defines a blend of phosphor-converted blue and a red LED. LED-RGB1 defines the white light produced by a tricolor LED mix. LED-V1 and V2 define LEDs with phosphor-converted violet light.

White point

Main article:White point

The spectrum of a standard illuminant, like any other profile of light, can be converted intotristimulus values.The set of three tristimulus coordinates of an illuminant is called awhite point.If the profile isnormalized,then the white point can equivalently be expressed as a pair ofchromaticity coordinates.

If an image is recorded in tristimulus coordinates (or in values which can be converted to and from them), then the white point of the illuminant used gives the maximum value of the tristimulus coordinates that will be recorded at any point in the image, in the absence offluorescence.It is called the white point of the image.

The process of calculating the white point discards a great deal of information about the profile of the illuminant, and so although it is true that for every illuminant the exact white point can be calculated, it is not the case that knowing the white point of an image alone tells you a great deal about the illuminant that was used to record it.

White points of standard illuminants

A list of standardized illuminants, their CIE chromaticity coordinates (x,y) of a perfectly reflecting (or transmitting) diffuser, and theircorrelated color temperatures(CCTs) are given below. The CIE chromaticity coordinates are given for both the 2 degree field of view (1931) and the 10 degree field of view (1964).The color swatches represent the color of each white point, automatically calculated by Wikipedia using theColor temperature template.

White points of standard illuminants

Name	CIE 1931 2°		CIE 196410°		CCT(K)	Color	Note
	x2°	y2°	x10°	y10°
A	0.44758	0.40745	0.45117	0.40594	2856		incandescent / tungsten
B	0.34842	0.35161	0.34980	0.35270	4874		obsolete, direct sunlight at noon
C	0.31006	0.31616	0.31039	0.31905	6774		obsolete, average / North sky daylight NTSC 1953,PAL-M
D50	0.34567	0.35850	0.34773	0.35952	5003		horizon light,ICC profilePCS
D55	0.33242	0.34743	0.33411	0.34877	5503		mid-morning / mid-afternoon daylight
D65	0.31272	0.32903	0.31382	0.33100	6504		noon daylight:television,sRGB color space
D75	0.29902	0.31485	0.29968	0.31740	7504		North sky daylight
D93	0.28315	0.29711	0.28327	0.30043	9305		high-efficiency blue phosphor monitors,BT.2035
E	0.33333	0.33333	0.33333	0.33333	5454		equal energy
F1	0.31310	0.33727	0.31811	0.33559	6430		daylight fluorescent
F2	0.37208	0.37529	0.37925	0.36733	4230		cool white fluorescent
F3	0.40910	0.39430	0.41761	0.38324	3450		white fluorescent
F4	0.44018	0.40329	0.44920	0.39074	2940		warm white fluorescent
F5	0.31379	0.34531	0.31975	0.34246	6350		daylight fluorescent
F6	0.37790	0.38835	0.38660	0.37847	4150		light white fluorescent
F7	0.31292	0.32933	0.31569	0.32960	6500		D65simulator, daylight simulator
F8	0.34588	0.35875	0.34902	0.35939	5000		D50 simulator, Sylvania F40 Design 50
F9	0.37417	0.37281	0.37829	0.37045	4150		cool white deluxe fluorescent
F10	0.34609	0.35986	0.35090	0.35444	5000		Philips TL85, Ultralume 50
F11	0.38052	0.37713	0.38541	0.37123	4000		Philips TL84, Ultralume 40
F12	0.43695	0.40441	0.44256	0.39717	3000		Philips TL83, Ultralume 30
LED-B1	0.4560	0.4078			2733		phosphor-converted blue
LED-B2	0.4357	0.4012			2998		phosphor-converted blue
LED-B3	0.3756	0.3723			4103		phosphor-converted blue
LED-B4	0.3422	0.3502			5109		phosphor-converted blue
LED-B5	0.3118	0.3236			6598		phosphor-converted blue
LED-BH1	0.4474	0.4066			2851		mixing of phosphor-converted blue LED and red LED (blue-hybrid)
LED-RGB1	0.4557	0.4211			2840		mixing of red, green, and blue LEDs
LED-V1	0.4560	0.4548			2724		phosphor-converted violet
LED-V2	0.3781	0.3775			4070		phosphor-converted violet

External links

• Selected colorimetric tables in Excel,as published inCIE 15:2004
• Konica Minolta Sensing:Light sources & Illuminants