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01 / 06   Light & perception

Application note

Light, Cones, and Color Perception

Separate the spectrum of light from the visual response it produces.

A color specification connects a physical light stimulus with a visual response under stated conditions. Wavelength alone cannot describe the color of a coating, display, or illuminated part: the spectrum, viewing level, adaptation, and surrounding scene all matter. Separating these quantities is the first step toward a useful measurement.

Begin with the light

A monochromatic stimulus contains one wavelength in the ideal limit; practical sources have finite bandwidth. Most familiar light is a mixture of wavelengths. A spectral power distribution describes how radiant power is distributed with wavelength, commonly per nanometer. Its integral gives radiant power over the stated band.

A photon at vacuum wavelength λ\lambda carries energy:

E=hcλ,E [eV]≈1239.84λ [nm]E=\frac{hc}{\lambda},\qquad E\,[\mathrm{eV}]\approx\frac{1239.84}{\lambda\,[\mathrm{nm}]}

Shorter wavelengths carry more energy per photon. A 450 nm photon carries approximately 2.76 eV; a 650 nm photon carries approximately 1.91 eV. Neither photon energy nor photon count alone predicts a visual color or brightness. The visual system weights wavelengths differently.

Three overlapping cone responses

Under photopic viewing conditions, three cone classes contribute to human color matching: long-, medium-, and short-wavelength sensitive cones, abbreviated L, M, and S. Their broad, overlapping sensitivities allow one wavelength to stimulate several classes. They are not separate red, green, and blue detectors. Rods support vision at lower light levels but do not provide the same trichromatic discrimination.

Schematic overlapping L, M, and S sensitivity curves show why one wavelength can excite multiple cone classes. Each curve has its own normalized peak.

View diagram at full size

For energy-based cone sensitivities l,m,sl,m,s and a compatible spectral stimulus PλP_\lambda:

(L,M,S)=∫Pλ(λ) [l(λ),m(λ),s(λ)] dλ(L,M,S)=\int P_\lambda(\lambda)\,[l(\lambda),m(\lambda),s(\lambda)]\,d\lambda

A photon-based stimulus requires sensitivities defined on the same basis. Peak normalization makes curve shapes easier to compare; it does not establish equal absolute sensitivity, cone population, or signal strength. Real cone fundamentals include physiological and viewing-condition effects. Symmetric bell curves are useful sketches, not calibrated replacements.

What normalization and a bell-shaped approximation mean

For a specified cone sensitivity l(λ)l(\lambda), peak normalization gives:

lnorm(λ)=l(λ)max⁡λl(λ)l_{\mathrm{norm}}(\lambda)=\frac{l(\lambda)}{\max_\lambda l(\lambda)}

Each channel can be normalized separately, so the three unit peaks do not retain their original relative amplitudes. The schematic curves use the form:

g(λ)=exp⁡ ⁣[−(λ−μ)22σ2]g(\lambda)=\exp\!\left[-\frac{(\lambda-\mu)^2}{2\sigma^2}\right]

Here μ\mu locates a peak and σ\sigma controls its width. This is a shape illustration, not a probability distribution over colors or a calibrated cone model. Real sensitivities are not symmetric Gaussians; use the appropriate tabulated functions for quantitative work.

Distinguish luminance from brightness

Luminance is a photometric quantity in cd/m². It weights spectral radiance Le,λL_{e,\lambda} with the photopic luminous-efficiency function V(λ)V(\lambda):

Lv≈683∫Le,λ(λ)V(λ) dλL_v\approx683\int L_{e,\lambda}(\lambda)V(\lambda)\,d\lambda

The factor is approximately 683 lm/W, with compatible spectral units. For monochromatic radiation, luminous efficacy is approximately 683V(λ)683V(\lambda) lm/W of radiant power; electrical efficiency is a separate quantity. Equal radiant power at different wavelengths therefore need not give equal luminance.

Brightness describes visual appearance and depends on adaptation and context. Luminance is not a count of photons per unit area, and equal luminance does not guarantee equal apparent brightness.

A spectrum does not contain every color category

Some cyan stimuli are monochromatic. Purple and magenta require spectral mixtures; there is no single purple wavelength. Pink combines a reddish stimulus with a lighter appearance. White is an adapted neutral reference, not a universal maximum of all three cone signals.

The same brown-orange sRGB patch appears against light and dark surrounds. Identical code values demonstrate the importance of context without constituting a calibrated visual experiment.

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Black can describe a low-luminance region relative to its surroundings even when it returns some light. Brown commonly describes an orange or yellow appearance at low lightness relative to a brighter context. Consequently, a measurement intended to track appearance should define the viewing background and illumination along with the sample.

Explore the model

Photon energy and rate

Separate the energy of one photon from the number of photons in a beam.

Change the values to update the results and visualization.

Photon energy
2.2339 eV
Photon energy
3.5792e-19 J
Frequency
540.17 THz
Photon rate
2.7939e+15 s⁻¹

The plot shows 360–830 nm; the energy calculation also supports wavelengths outside this interval.

Photon energy and rate: interactive plotPhoton energy / eV against Vacuum wavelength / nm. Curves: E = hc/λ. Input: 555, 2.233936004540.85481.66422.47363.28304InputVacuum wavelength / nmPhoton energy / eV
E = hc/λ
Formula & assumptions

E = hc/λ; ν = c/λ; photon rate = P/E.

Vacuum wavelength and monochromatic radiant power. Photon rate is emitted or incident beam rate, not detected photoelectrons. Quantum efficiency and collection losses are not included.

Explore the model

Monochromatic luminous flux

Compare equal radiant power at different wavelengths through photopic weighting.

Change the values to update the results and visualization.

Photopic V(λ)
1
Luminous efficacy of radiation
683 lm/W
Luminous flux
0.683 lm
Monochromatic luminous flux: interactive plotPhotopic V(λ) against Wavelength in standard air / nm. Curves: Photopic weighting. Input: 555, 136004540.25480.46420.67360.88301InputWavelength in standard air / nmPhotopic V(λ)
Photopic weighting
Formula & assumptions

Φv = 683 V(λ) Φe; K(λ) = 683 V(λ) lm/W.

CIE 1931 2° ȳ equals the CIE photopic V(λ) table here. Wavelength in standard air, 360–830 nm; linear interpolation between 1 nm values. These are lumens, not luminance in cd/m², perceived brightness, or LED electrical efficiency.

Reference data: CIE 1931 2° observer and Illuminant D65. Numeric tables © CIE, used under CC BY-SA 4.0; derived data plots share this license. Tables retained at 1 nm on the common 360–830 nm interval. Figures and calculations by Iris Optics.

From estimate to application

Define what your color measurement needs to capture.

Source spectrum, viewing conditions, and detector response determine what a color result can tell you. Connect those choices to your inspection task.

Discuss your color measurement