I. Definition
The CIE luminous efficiency function $V(\lambda)$ is a standard response function established by the International Commission on Illumination (CIE) to describe the relative visual sensitivity of the standard observer to visible light of different wavelengths under specific photometric conditions.
Strict Definition:Under specific photometric conditions, if radiant flux $\Phi_{e,\lambda}$ at wavelength $\lambda$ and radiant flux $\Phi_{e,\lambda_m}$ at the peak sensitivity wavelength $\lambda_m$ produce an identical visual sensation of brightness, the ratio of these two fluxes, $\Phi_{e,\lambda_m}/\Phi_{e,\lambda}$, defines the spectral luminous efficiency $V(\lambda)$.
II. Unit
Spectral luminous efficiency is a dimensionless quantity with a unit of 1. It represents only the relative ratio of radiant flux and has no physical dimension.
III. Luminous Efficiency Functions
Human spectral sensitivity depends on visual adaptation, field of view (FOV), and the angle of incidence. The CIE defines several standard functions for different photometric conditions:
Photopic Vision \(V(\lambda)\)
Figure 1: Schematic Diagram of Cone Cells
Source: https://en.wikipedia.org/wiki/Cone_cell#media/File:Cone_cell_eng.svg
Scotopic Vision \(V'(\lambda)\)
Figure 2:Schematic Diagram of Rod Cells
Source: https://en.wikipedia.org/wiki/Rod_cell#/media/File:Rod_Cell.svg
Mesopic Vision \(V_{\text{mes},m}(\lambda)\)
Comparison of Spectral Luminous Efficiency Functions
(Image source: https://commons.wikimedia.org/wiki/File:LuminosityCurve1.svg)
The figure clearly shows the spectral sensitivity differences between photopic and scotopic vision. Scotopic vision is more sensitive to blue - green light (507 nm), while photopic vision is most sensitive to green light (555 nm). The horizontal axis represents wavelength, with units of nanometers (nm).
IV. Photometric calculations based on the luminous efficiency function
The primary application of the luminous efficiency function is to convert radiometric quantities into photometric quantities. The general calculation model is:
$$\varPhi_{\text{v}} = K_{\text{m}} \int_{0}^{\infty} \varPhi_{\text{e},\lambda}(\lambda) \cdot V(\lambda) \, d\lambda$$
where:
As an example, under photopic conditions, the spectral luminous efficiency of the human eye at $480\ \mathrm{nm}$ is approximately $20\%$ of that at $555\ \mathrm{nm}$. Therefore, a monochromatic source at $480\ \mathrm{nm}$ with five times the radiant power of a $555\ \mathrm{nm}$ source would yield identical luminous flux. Under identical viewing conditions (same emitting area, field of view and observation distance), the two sources produce the same perceived brightness.