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

The spectral radiant exitance of a black body follows Planck's law:

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

At the time of standardizing illuminant A, both ${\displaystyle c_{1}=2\pi \cdot h\cdot c^{2}}$ (which does not affect the relative SPD) and ${\displaystyle c_{2}=h\cdot c/k}$ were different. In 1968, the estimate of c₂ was 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 the Planckian locus, changing the color temperature of the illuminant from its nominal 2848 K to 2856 K:

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

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:^[1]

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

The coefficients have been selected to achieve a normalized SPD of 100 at 560 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 a correlated 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:.^[1] Lighting cabinets, such as the Spectralight III, that use filtered incandescent lamps have better fits to the D illuminants in the 400 nm to 700 nm range than do the fluorescent daylight simulators.^[5]

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^[6]

Illuminant B was not so honored in 2004.

The liquid filters, designed by Raymond Davis, Jr. and Kasson S. Gibson in 1931,^[7] have a relatively high absorbance at the red end of the spectrum, effectively increasing the CCT of the incandescent lamp to daylight levels. This is similar in function to a CTO color gel that 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, and ammonium 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 about 560 nm.

Derived by Judd, MacAdam, and Wyszecki,^[8] the D series of illuminants are constructed to represent natural daylight. They are difficult to produce artificially, but are easy to characterize mathematically.

H. W. Budde of the National Research Council of Canada in Ottawa, H. R. Condit and F. Grum of the Eastman Kodak Company in Rochester, New York,^[9] and S. T. Henderson and D. Hodgkiss of Thorn Electrical Industries in Enfield^[10] had independently measured the spectral power distribution (SPD) of daylight from 330 nm to 700 nm, totaling among them 622 samples. Judd et al. analyzed these samples and found that the (x, y) chromaticity coordinates had a simple, quadratic relation:

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

Simonds supervised the characteristic vector analysis of the SPDs.^[11][12] Application of his method revealed that the SPDs could be satisfactorily approximated by using the mean (S₀) and first two characteristic vectors (S₁ and S₂):

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

In simpler terms, the SPD of the studied daylight samples can be expressed as the linear combination of 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, accounting for changes in the correlated color temperature due to presence or absence of clouds or direct sunlight.^[8] The third vector (S₂) corresponds to pink–green variation caused by the presence of water in the form of vapor and haze.^[8]

To construct a daylight simulator of a particular correlated color temperature one merely needs to know the coefficients M₁ and M₂ of the characteristic vectors S₁ and S₂.

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

Expressing the chromaticities x and y as:

${\displaystyle x={\frac {X_{0}+M_{1}X_{1}+M_{2}X_{2}}{S_{0}+M_{1}S_{1}+M_{2}S_{2}}},}$

${\displaystyle y={\frac {Y_{0}+M_{1}Y_{1}+M_{2}Y_{2}}{S_{0}+M_{1}S_{1}+M_{2}S_{2}}}}$

and making use of known tristimulus values for the mean vectors, they were able to express M₁ and M₂ as follows:

Kelly's figures depicted the lines of constant correlated color temperature in uv space on the CIE 1960 UCS, as shown here, as well as on the familiar xy diagram.

${\displaystyle M_{1}={\frac {-1.3515-1.7703x+5.9114y}{0.0241+0.2562x-0.7341y}},}$

${\displaystyle M_{2}={\frac {0.0300-31.4424x+30.0717y}{0.0241+0.2562x-0.7341y}}.}$

The only problem is that this left unsolved the computation of the coordinate ${\displaystyle (x,y)}$ for a particular phase of daylight. Judd et al. simply tabulated the values of certain chromaticity coordinates, corresponding to commonly used correlated color temperatures, such as 5500 K, 6500 K, and 7500 K. For other color temperatures, one could consult figures made by Kelly.^[13] This problem was addressed in the CIE report that formalized illuminant D, with an approximation of the x coordinate in terms of the reciprocal color temperature, valid from 4000 K to 25000 K.^[14] The y coordinate trivially followed from Judd's quadratic relation.

Judd et al. then extended the reconstituted SPDs to 300 nm–330 nm and 700 nm–830 nm by using Moon's spectral absorbance data of the Earth's atmosphere.^[15]

The tabulated SPDs presented by the CIE today are derived by linear interpolation of the 10 nm data set down to 5 nm.^[16]

Similar studies have been undertaken in other parts of the world, or repeating Judd et al.'s analysis with modern computational methods. In several of these studies, the daylight locus is notably closer to the Planckian locus than in Judd et al.^{[17] [18]}

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 ${\displaystyle \Delta _{uv}=0.003}$.

Computation

The relative spectral power distribution (SPD) ${\displaystyle S_{D}(\lambda )}$ of a D series illuminant can be derived from its chromaticity coordinates in the CIE 1931 color space, ${\displaystyle (x_{D},y_{D})}$:^[19]

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

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

where T is the illuminant's CCT. The chromaticity coordinates of the illuminants D are said to form the CIE daylight locus. The relative SPD is given by:

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

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

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

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

where ${\displaystyle S_{0}(\lambda ),S_{1}(\lambda ),S_{2}(\lambda )}$ are the mean and first two eigenvector SPDs, depicted above.^[19] The characteristic vectors both have a zero at 560 nm, since all the relative SPDs have been normalized about this point.

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), while D65 has a CCT of 6504 K (noon light). As explained in a previous section, 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. In order to match all significant digits of the published data of the canonical illuminants the values of M₁ and M₂ have to be rounded to three decimal places before calculation of S_D.^[1]

Illuminant E

Illuminant E is beneath the Planckian locus, and roughly at the CCT of D₅₅.

Illuminant E is an equal-energy radiator; it has a constant SPD inside the visible spectrum. It is useful as a theoretical reference; an illuminant that gives equal weight to all wavelengths. It also has equal CIE XYZ tristimulus 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.^[1]

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, D₅₅ is the closest.) Manufacturers sometimes compare light sources against illuminant E to calculate the excitation purity.^[20]

Illuminant series F

The F series of illuminants represent various types of fluorescent lighting.

F1–F6 "standard" fluorescent lamps consist of two semi-broadband emissions of antimony and manganese activations in calcium halophosphate phosphor.^[21] F4 is of particular interest since it was used for calibrating the CIE color 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.^[6][22]

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

Illuminant series LED

Publication 15:2018 introduces new illuminants for different LED types with CCTs ranging from approx. 2700 K to 6600 K.

White points of standard illuminants

A list of standardized illuminants, their CIE chromaticity coordinates (x,y) of a perfectly reflecting (or transmitting) diffuser, and their correlated 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).^[23]The color swatches represent the color of each white point, automatically calculated by Wikipedia using the Color temperature template.