What this is
- This research investigates the correlation between non-visual metrics and brightness metrics in indoor lighting systems.
- It focuses on parameters relevant for Human Centric Lighting (HCL), such as and .
- The analysis is based on a database of 884 light sources across various technologies and daylight spectra.
Essence
- High correlations exist between non-visual metrics and brightness metrics, allowing for linear transformations among them. This facilitates improved applications in lighting design.
Key takeaways
- The latest model addresses previous limitations, particularly in the transition between warm and cold white light sources.
- Three metrics from different research groups show high correlation coefficients, enabling conversions between them for practical applications in lighting.
Caveats
- The study relies on a specific dataset of 884 light sources, which may not represent all lighting technologies.
- Correlations may vary based on the type of light spectra used, particularly in different color temperature ranges.
Definitions
- Circadian Stimulus: A measure of the effectiveness of light in influencing circadian rhythms, particularly melatonin suppression.
- Melanopic Equivalent Daylight Illuminance (mEDI): A metric quantifying the daylight-like effects of artificial light on melanopsin-containing retinal cells.
AI simplified
Introduction
Lighting research and vision science have a long history, accompanied by the dynamic evolution of light source technologies from thermal radiators such as tungsten and halogen incandescent lamps, to discharge light sources such as mercury, sodium, and fluorescent lamps, to the current technology of white and colored LEDs (Light Emitting Diodes)1–6. At each stage of this historical evolution, different visual tasks and visual metrics were defined to meet specific social, visual, and industrial needs. In the early decades of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$20\textrm{th}$$\end{document}20th century, visual performance, including contrast vision, reaction time, visual acuity, and glare, was the focus of scientific and technological considerations. Thus, photometric quantities such as illuminance, luminance, uniformity, and glare index were defined using the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V(\lambda )$$\end{document}V(λ) function, the spectral luminous efficiency function for daytime vision7,8. With the development of fluorescent lamps and metal halide lamps, with more possibilities to modify the lamp spectra, several aspects of color quality such as color rendering index (CRI), correlated color temperature (CCT) and chromaticity of white light have been addressed in scientific literature and also in regulations for practical lighting9–11. With the continuous improvement of LED technology, new aspects of color quality at higher cognitive levels, such as color preference, color memory or color saturation, have been scientifically studied. These aspects have been introduced in practical applications, e.g. museum lighting12–15.
With the discovery of intrinsically photosensitive retinal ganglion cells (ipRGCs) containing melanopsin pigments16–18, two main lines of research on non-visual ipRGC-based effects have emerged. On the one hand, in lighting and sleep research, experiments have been conducted in laboratories or real-world settings (e.g., nursing homes, hospitals, schools, offices) to investigate the relationship between light intensity, spectrum, time, duration of light treatment, and non-visual outcomes (e.g., attention, sleep quality, alertness) using conventional photometric and colorimetric parameters such as vertical illuminance in lx, luminance in cd/\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$m^2$$\end{document}m2, color temperature, and spectral irradiance distributions16–24.
Since 2005, there has been a lot of research and discussion about how the receptor signals (rods, cones, and ipRGCs) combine to produce the non-visual effects of light. Section “The 2018 Circadian Stimulus (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018) model” of this article describes the circadian stimulus (CS) models in the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 versions of Rea et al.1,2,25. Melanopic Equivalent Daylight Illuminance (mEDI, in lx) has been introduced according to the CIE publication3. These two metrics, CS and mEDI, are currently proposed for scientific discussion worldwide. They are also subject to further investigation.
From a physiological point of view, these two metrics represent different opinions on how to define the quantities for non-visual effects. According to the above mentioned CIE publication, the non-visual effects should be based on the signals of the ipRGCs, which express the effect of the melanopsin pigments, so that the mEDI metric can be used for the calculation and evaluation of lighting systems regarding the aspect of their non-visual effects. The CS model of Rea et al, in the 2005 and 2018 versions1,2, is based on the idea that the non-visual effects come either from the ipRGC channel (if the opponent channel signal \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$(b - y \le 0)$$\end{document}(b-y≤0), i.e. the blue channel has a weaker signal than the (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L+M$$\end{document}L+M) or yellow channel, for example in the case of warm white light sources), or a combination of the ipRGC channel and the signals of the combinations of the (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L+M$$\end{document}L+M), S cone and rod channels if (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$b - y > 0$$\end{document}b-y>0). The cases (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$b - y \le 0$$\end{document}b-y≤0) and (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$b - y > 0$$\end{document}b-y>0) correspond to white light correlated color temperatures (CCTs) of, empirically, about (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CCT \le 3710\,K$$\end{document}CCT≤3710K) and (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CCT> 3710\,K$$\end{document}CCT>3710K), respectively.
In recent years, roughly between 2018 and 2022, numerous international scientific discussions and analyses have been conducted to specify the correct metric for the non-visual effects, using data sets from experiments by different research groups on nocturnal melatonin suppression as a validation basis. The following important research results were achieved during this period: Improvements of the CS model (versions 2005 and 2018) in the two years 2020 and 2021, taking into account the exposure time t (in hours) and the visual field, and modeling the contributions of the ipRGC channel, the S cones, the rods and the (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L + M$$\end{document}L+M) channel with improved terms, for both cases (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$b - y > 0$$\end{document}b-y>0) and (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$b - y \le 0$$\end{document}b-y≤0)2,25. This improved formulation was validated using data sets for melatonin suppression2 and is described in the present article.Publication on “Recommendations for daytime, evening, and night-time indoor light exposure to best support physiology, sleep, and wakefulness in healthy adults” by a group of sleep researchers and neurophysiologists26.Based on the analysis of experimental data on nocturnal melatonin suppression and using mEDI as an input metric for non-visual effects, Giménez et al.4 defined a formula to predict melatonin suppression with exposure time and pupil dilation as additional parameters. This new metric was found by a machine learning method and is a non-linear transformation of the mEDI metric. This formula, now called the Gimenez formula in this article, is compared to the CS metric in its 2021 version.Parallel to the dynamic and intensive development of metrics for non-visual effects of light on humans, the development of metrics for brightness and visual clarity has experienced a renaissance with the development of quasi-monochromatic and phosphor-converted white LEDs with different correlated color temperatures and chromaticity coordinates. This new discussion started at the end of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$20\textrm{th}$$\end{document}20th century by Fotios and Levermore5, with the development and analysis of new psychophysical methods in 201227, and has been continued by the authors of the present article6,28,29. This renaissance could be explained by the fact that the brightness of white LED light sources of the same luminance but different spectra (different correlated color temperatures, chromaticity and color saturation enhancements) are perceived at different brightness levels. The root of these perceptual differences can be argued as the luminance or the signal of the luminance channel (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L + M$$\end{document}L+M) is not solely responsible for the brightness perception, which includes additional contributions from rods, S cones, opponent channels5,30–32 and the ipRGC channel33,34. This argument is demonstrated in the brightness experiments of the PhD thesis of Pepler35.
With the above considerations in mind, the non-visual effects of light can be modeled either with a combination of signals from the ipRGC channel, the S cones, the (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L + M$$\end{document}L+M) channel, and the rod channel (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 model), or with the ipRGC signals alone (mEDI, CIE publication S 026:20183). Similarly, a brightness metric (denoted by M) can be constructed by using an exponential function of the (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L + M$$\end{document}L+M) signal, the ipRGC signal, and the S cone signal6. From the point of view of lighting research and engineering, the following research questions arise: Is there a reasonable and usable correlation between the melanopic equivalent daylight illuminance (mEDI) and the circadian light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA in the CS models in the 2018 and 2021 versions; as well as the equivalent luminance \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L_{eq}$$\end{document}Leq according to Eq. 1 of Fotios and Levermore5 (see section “Brightness perception and modeling” of this article) for brightness perception?Is there also a useful correlation between the values of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 metric, the Gimenez values for melatonin suppression, and the brightness perception metric according to the brightness metric in6?What is the difference between the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 metric values and the Gimenez melatonin suppression values for the same light source spectra? Is this difference acceptable for practical use of these metrics?If there is useable correlation between the different metrics and the difference between them is small enough to be in an acceptable range then a converting formula can be developed to transform one metric to the other with sufficient accuracy so that lighting researchers, sleep researchers or lighting engineers can design and evaluate a lighting system with several metrics recommended today although these metrics were established from different human physiological viewpoints. In the next sections, the brightness metric6, the model \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 of Rea et al.2 and the formula of Giménez et al.4 will be presented before the correlations and relationships between the metrics for the non-visual effects and brightness will be described based on a calculation of 884 measured light source spectra.
Brightness perception and modeling ,,, [5] [6] [36] [37]
Over the past six decades, many research studies have been conducted using colored and conventional white light luminance experiments and modeling. The most important models are those of Guth et al.38 Ikeda et al.39, Kokoschka et al.40, Nakano et al.32, Palmer41, Ware and Cowan42, which led to a summary paper of the CIE (International Commission on Illumination) in43, which tested all models until 2001. All models included in this fundamental paper considered the contributions of the opponent channels (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L - M$$\end{document}L-M) and (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S - (L + M)$$\end{document}S-(L+M)) indirectly by implementing the chromaticity x and y into a joint function with the luminance of the achromatic signal (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L + M$$\end{document}L+M). In a dissertation on photopic brightness in indoor lighting in 2017, Pepler35 varied the spectra of polychromatic white light sources and the luminances in the photopic range on a homogeneous and diffusely reflecting wall in a real room without daylight incidence and found in a comprehensive psychophysical experiment that under the defined test conditions with white light, the most consistent model corresponding to the subjective evaluations of the test subjects is a model by Fotios et al. from 19985, in which the so-called equivalent luminance (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L_{eq}$$\end{document}Leq) can be defined according to Eq. (1). This model divides the signal of the S-cones (S) by the signal of the V(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda$$\end{document}λ) function and then calculates a metric to the power of 0.24, see Eq. (1).1\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} L_{eq} = L_v \cdot (S/V)^{0.24} \end{aligned}$$\end{document}Leq=Lv·(S/V)0.24In Eq. (1), the exponent of photopic luminance (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L_v$$\end{document}Lv) remains 1.0, i.e., luminance remains uncompressed. To calculate the signals S or V, the relative spectral radiant flux of the light source must be multiplied by the spectral sensitivity function of the S-cones or by the V(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda$$\end{document}λ) function, respectively, and this product must be integrated over the visible wavelength range.
With the discovery of a new type of ganglion cells, the intrinsically photosensitive retinal ganglion cells (ipRGCs), described in several scientific publications, including Hattar et al. in44, some research has been conducted to answer the question whether ipRGC signals would also contribute to the perception of lightness in the photopic visual field. According to recent neurophysiological studies, there are some reasons to assume that ipRGCs interact with the visual channels in at least two different ways (see Zele et al.33): \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_4$$\end{document}M4-subtype ipRGCs project to the LGN and contribute to human light perception (see Brown et al.45).a group of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_1$$\end{document}M1-subtype ipRGCs establish signaling connections with upstream dopaminergic amacrine cells. Luminance signals can be transmitted to the outermost sublamina of the inner plexiform layer, influencing the state of light adaptation (see Prigge et al.46).As a result, studies by Zele et al.33 in 2018 and Yamakawa et al.34 in 2019 had found ipRGC signals in brightness perception. In 2015, Bullough et al.36 established a model for brightness that considers the contribution of the luminance channel V(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda$$\end{document}λ), S-cone S(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda$$\end{document}λ), and ipRGC (melanopsin, Mel(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda$$\end{document}λ)), which is described in Eq. (2).2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} B_2= V(\lambda )+ 0.6 \cdot g \cdot S(\lambda ) + 0.5 \cdot Mel(\lambda ) \end{aligned}$$\end{document}B2=V(λ)+0.6·g·S(λ)+0.5·Mel(λ)The S-cone contribution multiplier g in Eq. (2) depends on the level of adaptation and increases as a function of light level. In the Bullough et al.36 model in Eq. (2), the contributions of the luminance channel, S-cones, and ipRGC signals are integrated as a linear function into the brightness metric \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$B_2$$\end{document}B2. Brightness perception was analyzed and modeled in6 based on psychophysical experiments performed by the authors of the present article. For these experiments, 25 absolute spectra of multiple LED combinations (white LEDs and colored LEDs) with 5 different correlated color temperatures between 2700 and 10,000 K and 5 horizontal illuminances between 45 and 2000 lx with a relatively high color rendering index in the range \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$89 \le \text {IES TM-30-20 } R_f \le 93$$\end{document}89≤IES TM-30-20Rf≤93 were used. The resulting brightness model is shown in Eq. (3) (TUD stands for “TU Darmstadt”).3\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} M_{TUD,VT2023}=8.9974 \cdot \left[ E_v^{0.2629} \left( S^{0.074} + 0.5 \cdot G^{0.0424}\right) \right] -1.3307 \end{aligned}$$\end{document}MTUD,VT2023=8.9974·Ev0.2629S0.074+0.5·G0.0424-1.3307This model (Eq. 3) contains the combination of an illuminance term compressed with the power function \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_v^{0.2629}$$\end{document}Ev0.2629 and two terms with the compressed S-cone andipRGC signal. The optimization based on the experimental data had also shown that, from a mathematical point of view, the contribution of the S-cones and the ipRGC channel is crucial. It was the intention of the model builders to present this brightness model for lighting applications in the photopic range with white light.
| Light level reference (ref.) (lx) | Test light source (T. L. S.) | - prediction \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$B_2$$\end{document} B 2 | Predicted Brightness (P. B.) \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_{TUD,VT2023}$$\end{document} M T U D V T , 2023 | P. B \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_{TUD,VT2023}$$\end{document} M T U D V T , 2023 | Re. B. Diff.in % \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\Delta M_{TUD, VT2023}$$\end{document} Δ M T U D V T , 2023 | |
|---|---|---|---|---|---|---|
| Amber 1 as [ref. L. S.] | 108 | 94 SEM 5.7 | 98 | [] 55.32For ref. L. S. | []62.15For T. L. S. | + 12.3 |
| Amber 2 as [ref. L. S.] | 108 | 125 SEM 5.1 | 119 | [] 65.125For ref. L. S. | [] 58.27For T. L. S. | − 10.5 |
Circadian stimulus models (and) \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document} C S 2018 \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document} C S 2021 [1] [2]
The concept of Rea et al., covering the models \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2005}$$\end{document}CS2005, \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 is based on the design of a phototransduction circuit which regards the following mechanisms: The phototransduction of photoabsorption, signal generation and conversion into a frequency-coded form, and the processing of the signals of the different channels (LMS—cones, rods and ipRGCs) exhibit subadditivity. Additivity is assumed, e.g., in the definition of illuminance or luminance with the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V(\lambda )$$\end{document}V(λ) function or the mEDI metric, when the spectral sensitivity of the receptor system is multiplied by the spectral radiance or spectral irradiance of the incident radiation and all effects at each wavelength between 380 nm and 780 nm can be integrated by summation to the final effect of the total polychromatic radiation. No signal reduction is expected. In contrast, a possible subadditivity occurs when the effect at a wavelength \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda _1$$\end{document}λ1 is reduced when interacting with radiation of a certain wavelength \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\lambda _2$$\end{document}λ2. In neurobiology, subadditivity can be explained if the neural circuit for phototransduction contains a spectral opponent channel. In vision, two spectral opponent channels are known, a (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$L - M$$\end{document}L-M) channel and a (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S - (L + M)$$\end{document}S-(L+M)) channel. In the context of non-visual effects, the spectral opponent channel (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S - (L + M)$$\end{document}S-(L+M)) (also referred to as [d=TUD]\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$b - y$$\end{document}b-y\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$B - Y$$\end{document}B-Y) is taken into account. This is an important difference between the CS conception and the conception of the mEDI metric, which is defined by the CIE3 and assumes additivity of the nonvisual pathway. However, subadditivity was found to be essential in the experiments of Figuiero et al.47,48.The CS concept followed the idea that a non-visual effect consists of two components, a spectral component and a quantity component. The spectral [d=TUD]sensitivity functioncomponent, denoted by the circadian light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA which will be described later, expresses the spectral generation of a stimulus at different receptors and channel systems (LMS-cones, rods, ipRGC) at a certain state of the spectral opponent channel (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$(B - Y > 0)$$\end{document}(B-Y>0) or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$(B - Y \le 0)$$\end{document}(B-Y≤0)). The definition of the mEDI metric does not distinguish between cases.The quantity component in the models from \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2005}$$\end{document}CS2005, \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 up to the model \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 takes into account the exposure time, the characteristic of the visual field due to the spatial distribution of the ipRGC receptors on the retina, and the absolute magnitude of the circadian light value \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA.A conversion from \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA to the circadian stimulus CS in the model versions \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2005}$$\end{document}CS2005 and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 was based on the data sets of Thapan17 and Brainnard16 with quasi-monochromatic stimuli for nocturnal melatonin suppression. It has been improved and validated in 2021 by data sets from a variety of research groups. Therefore, the CS metric is also valid for lighting design processes for both evening and nighttime lighting.
The 2018 circadian stimulus () model \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document} C S 2018 [1]
This model is implemented in two steps:
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$1{\rm st}$$\end{document}1st step: Establish circadian light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA (denoted as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A\,1.0$$\end{document}CLA1):4\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} \mathrm {CL_A}={\left\{ \begin{array}{ll} 1548 \cdot \left[ \int M_{c\lambda }E_{\lambda } d\lambda + a_{b-y}\left( \int \frac{S_{\lambda }E_{\lambda } d\lambda }{mp_{\lambda }}d\lambda - k \int \frac{V_{\lambda }E_{\lambda } \cdot d\lambda }{mp_{\lambda }}\right) -a_{rod} \left( 1-e^{\frac{-\int V'_{\lambda }E_{\lambda } d\lambda }{RodSat}}\right) \right] &{} \text {if } \left( \int \frac{S_{\lambda }E_{\lambda }d\lambda }{mp_{\lambda }} - k \cdot \int \frac{V_{\lambda }E_{\lambda }d\lambda }{mp_{\lambda }}\right) > 0 \\ 1548 \cdot \left[ \int M_{c\lambda }E_{\lambda } d\lambda \right] &{} \text {if } \left( \int \frac{S_{\lambda }E_{\lambda }d\lambda }{mp_{\lambda }} - k \cdot \int \frac{V_{\lambda }E_{\lambda }d\lambda }{mp_{\lambda }}\right) \le 0 \end{array}\right. } \end{aligned}$$\end{document}CLA=1548·∫McλEλdλ+ab-y∫SλEλdλmpλdλ-k∫VλEλ·dλmpλ-arod1-e-∫Vλ′EλdλRodSatif∫SλEλdλmpλ-k·∫VλEλdλmpλ>01548·∫McλEλdλif∫SλEλdλmpλ-k·∫VλEλdλmpλ≤0In Eq. (4), the symbols have the following meanings:\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA: Circadian Light where the subscript “A” designates a numerical equivalence of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A = 1000$$\end{document}CLA=1000 (photopic) lx for CIE illuminant A.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_{\lambda }$$\end{document}Eλ: Light source spectral irradiance.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_{c\lambda }$$\end{document}Mcλ: melanopsin sensitivity (corrected for crystalline lens transmittance, after Wyszecki and Stiles49).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$k = 0.2616$$\end{document}k=0.2616.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S_{\lambda }$$\end{document}Sλ: S cone fundamental (Smith and Pokorny50).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$a_{b-y} = 0.7$$\end{document}ab-y=0.7.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$mp_{\lambda }$$\end{document}mpλ, macular pigment transmittance (after Snodderly et al.51).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$a_{rod} = 3.3$$\end{document}arod=3.3.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V_{\lambda }$$\end{document}Vλ: Photopic luminous efficiency function (Commission Internationale de l’Éclairage52]).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$RodSat = 6.5 \textrm{W m}^{-2}$$\end{document}RodSat=6.5Wm-2.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V'_{\lambda }$$\end{document}Vλ′: Scotopic luminous efficiency function (Commission Internationale de l’Éclairage52).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$2\textrm{nd}$$\end{document}2nd step: Conversion of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA value to Circadian Stimulus \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018.
The method of Rea et al., transforms the circadian effective light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA with the help of Eq. (5) into a so-called “circadian stimulus CS”, which is proportional to the melatonin suppression in %. For example, a value of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS = 0.4$$\end{document}CS=0.4 corresponds to a nocturnal melatonin suppression of 40 % compared to the pre-irradiation state.5\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} CS=0.7-\dfrac{0.7}{1+\left( \frac{CL_A}{355.7}\right) ^{1.1026}} \end{aligned}$$\end{document}CS=0.7-0.71+CLA355.71.1026From the mathematical point of view, this logistical function in Eq. (5) shows that the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS = 0.7$$\end{document}CS=0.7 or the nocturnal melatonin suppression of 70 % is reached if the Circadian Light term \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA is already very high. A higher CS value (higher than 0.7) is not possible. This is also a subject of the questions to be discussed later in relation to the formula of Giménez et al.4 in section “The formula of Giménez et al., for nocturnal melatonin suppression”. This CS value is valid for the exposure time of 1 h during the early biological night. Model values were validated by means of a dataset with 13 polychromatic light sources with the correlation coefficient of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$r^2 = 0.69$$\end{document}r2=0.692.
The 2021 circadian stimulus () model \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document} C S 2021 [2]
The CS model \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 has been used for a long time in some research groups and partly also by the US and international lighting industry with recognized advantages and clear deficits. According to the analysis of the authors of the present article, the boundary between “cool” and “warm” white polychromatic light sources in this aspect turned out to be about 3400–3710 K. According to2, the two steps for building the improved CS model 2021 were as follows:
\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$1\textrm{st}$$\end{document}1st step: Establish a new for formula for circadian light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA (denoted as \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A\,2.0$$\end{document}CLA2):6\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} \mathrm {\textit{CL}_A\,2.0}= & {} {\left\{ \begin{array}{ll} 1548 \cdot \bigg [\int M_{c\lambda }E_{\lambda } d\lambda - a_{rod1}\left( \int \frac{V'_{\lambda }E_{\lambda } d\lambda }{\int V_{c\lambda }E_{\lambda }d\lambda + g_1 \int S_{c\lambda }E_{\lambda }d\lambda }\right) \cdot \left( 1-e^{\frac{-\int V'_{\lambda }E_{\lambda } d\lambda }{RodSat}}\right) + a_{b-y} \left( \int S_{c\lambda }E_{\lambda } d\lambda -k \int \frac{V_{\lambda }E_{\lambda } \cdot d\lambda }{mp_{\lambda }}\right) \\ - a_{rod2}\left( \int \frac{V'_{\lambda }E_{\lambda } d\lambda }{\int V_{c\lambda }E_{\lambda }d\lambda + g_2 \int S_{c\lambda }E_{\lambda }d\lambda }\right) \cdot \left( 1-e^{\frac{-\int V'_{\lambda }E_{\lambda } d\lambda }{RodSat}}\right) \bigg ]&{} \text {if } (b-y) > 0\\ 1548 \cdot \bigg [\int M_{c\lambda }E_{\lambda } d\lambda - a_{rod1}\left( \int \frac{V'_{\lambda }E_{\lambda } d\lambda }{\int V_{c\lambda }E_{\lambda }d\lambda + g_1 \int S_{c\lambda }E_{\lambda }d\lambda }\right) \cdot \left( 1-e^{\frac{-\int V'_{\lambda }E_{\lambda } d\lambda }{RodSat}}\right) \bigg ] &{} \text {if } (b-y) \le 0 \end{array}\right. } \end{aligned}$$\end{document}CLA2=1548·[∫McλEλdλ-arod1∫Vλ′Eλdλ∫VcλEλdλ+g1∫ScλEλdλ·1-e-∫Vλ′EλdλRodSat+ab-y∫ScλEλdλ-k∫VλEλ·dλmpλ-arod2∫Vλ′Eλdλ∫VcλEλdλ+g2∫ScλEλdλ·1-e-∫Vλ′EλdλRodSat]if(b-y)>01548·[∫McλEλdλ-arod1∫Vλ′Eλdλ∫VcλEλdλ+g1∫ScλEλdλ·1-e-∫Vλ′EλdλRodSat]if(b-y)≤07\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} b-y= & {} \left( \int {S_{c\lambda }E_{\lambda }d\lambda } - k \cdot \int V_{c\lambda }E_{\lambda }d\lambda \right) \end{aligned}$$\end{document}b-y=∫ScλEλdλ-k·∫VcλEλdλ8\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} V_{c\lambda }= & {} \frac{\frac{V_{\lambda }}{mp_{\lambda }}}{max \left( \frac{V_{\lambda }}{mp_{\lambda }}\right) } \end{aligned}$$\end{document}Vcλ=VλmpλmaxVλmpλ9\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} S_{c\lambda }= & {} \frac{\frac{S_{\lambda }}{mp_{\lambda }}}{max \left( \frac{S_{\lambda }}{mp_{\lambda }}\right) } \end{aligned}$$\end{document}Scλ=SλmpλmaxSλmpλwith:\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$k = 0.2616$$\end{document}k=0.2616.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_{\lambda }$$\end{document}Eλ: Light source spectral irradiance.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$a_{b-y} = 0.21$$\end{document}ab-y=0.21.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_{c\lambda }$$\end{document}Mcλ: melanopsin sensitivity (corrected for crystalline lens transmittance, after Wyszecki and Stiles49).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$a_{rod1} = 2.3$$\end{document}arod1=2.3.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$S_{\lambda }$$\end{document}Sλ: S cone fundamental (Smith and Pokorny50).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$a_{rod2} = 1.60$$\end{document}arod2=1.6.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$mp_{\lambda }$$\end{document}mpλ, macular pigment transmittance (after Snodderly et al.51).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$g_1 = 1.00$$\end{document}g1=1.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V_{\lambda }$$\end{document}Vλ: Photopic luminous efficiency function (Commission Internationale de l’Éclairage52])\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$g_2 = 0.16$$\end{document}g2=0.16.\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V'_{\lambda }$$\end{document}Vλ′: Scotopic luminous efficiency function (Commission Internationale de l’Éclairage52).\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$RodSat = 6.5\,\textrm{W m}^{-2}$$\end{document}RodSat=6.5Wm-2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$2\textrm{nd}$$\end{document}2nd step: Conversion of \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A\,2.0$$\end{document}CLA2 value to Circadian Stimulus \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021.
Compared to the model version \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018, the basic structure of the version 2021 with the logistic function remains unchanged with the exponent 1.1026 and the half saturation constant 355.7 (with the CS value of 35% as half of the maximum possible melatonin suppression, 70%). Two new factors have been implemented, the exposure time t (in hours) of 0.5 and 3 h and the factor f describing the spatial distribution of the circadian light exposure.10\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} CS_{t,f}=0.7-\dfrac{0.7}{1+\left( \frac{CL_{A,2.0}\cdot t \cdot f}{355.7}\right) ^{1.1026}} \end{aligned}$$\end{document}CSt,f=0.7-0.71+CLA,2·t·f355.71.1026Regarding the factor f in three different viewing modes, Rea et al. defined three values2:For a full visual field (a Ganzfeld): \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f = 2.0$$\end{document}f=2.For a central visual field (e.g. with a light box on a desk): \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f = 1.0$$\end{document}f=1.For a superior visual field (e.g. from ceiling mounted down-light luminaires): \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$f = 0.5$$\end{document}f=0.5.However, the above definition of viewing conditions is not precise for practical lighting applications. For the purposes of numerical analysis in this article, f is set to 1.0.
The formula of Giménez et al., for nocturnal melatonin suppression [4]
The numerical study of Giménez et al.4 pursued similar intentions as the CS models with the following research conception: The authors of this study aimed to build a metric with mEDI (Melanopic Equivalent Daylight (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$D_{65}$$\end{document}D65) illuminance) as the starting parameter and extended the analysis to include the contributions of LMS cones based on a correlation analysis of 29 different data sets of nocturnal melatonin suppression published in scientific papers.The co-parameters were the exposure time and the pupil state of the subjects during the experiments (with or without pupil dilation). The metric to be found should be a metric for predicting nocturnal melatonin suppression similar to the above mentioned \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 model of Rea et al.The data analysis was based on the Random Forest (RF) method, a machine learning approach to solving classification and regression problems. The model was constructed in two steps. In the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$1\textrm{st}$$\end{document}1st step, mEDI illuminance, photopic illuminance, rhodopic EDI (for rods), L-opic EDI, M-opic EDI, and S-opic EDI were subjected to separate correlation analyses at different exposure times for narrowband and polychromatic light spectra. From 21 to 10,000 lx, the mEDI metric showed the best correlation coefficients. The S cone EDI outperformed the mEDI metric only in the range below 21 lx.
With mEDI illuminance as the initial parameter, other components such as LMS cone signals, exposure time (duration), and pupil dilation were added to the set of input parameters, and a four-parameter logistic function was constructed and compared to the available data sets. The accuracy of the regression analysis was expressed as the root mean square error (RMSE). The optimal random forest model was the model with the lowest RMSE and the least number of predictors. In addition, the coefficient \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$r^2$$\end{document}r2 was also used. The results of this analysis can be summarized as follows: Adding L and M cones did not improve the model quality compared to the combination of S cones and ipRGC alone.The combination of ipRGC and S cones resulted in a higher correlation coefficient and a lower RMSE value compared to ipRGC alone (mEDI). The difference was rather small, so the Giménez research group decided to ignore the S-signal portion in their model.The logistic function model therefore includes mEDI, exposure time and pupil dilation, see Eq. (11).11\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} Suppression_{melatonin}=\frac{0-100}{1+\frac{log_{10}(mEDI_{melanopic} \cdot 10^6)}{9.002-0.008 \cdot \Delta t_{expose} - 0.462 \cdot dil_{pupil}}} \end{aligned}$$\end{document}Suppressionmelatonin=0-1001+log10(mEDImelanopic·106)9.002-0.008·Δtexpose-0.462·dilpupilIn Eq. (11), the symbols have the following meaning:\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$suppression_{melatonin}$$\end{document}suppressionmelatonin= melatonin suppression (in %)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$mEDI_{melanopic}$$\end{document}mEDImelanopic = melanopic EDI (lx)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\Delta t_{exposure}$$\end{document}Δtexposure = exposure duration (in minutes)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$dil_{pupil}$$\end{document}dilpupil = pupil dilation applied: 0 = no, 1 = yesCompared to the CS model of Rea et al., the value of melatonin suppression is up to 100% at infinite illuminance. In the opinion of the authors of the present article, the most important difference between the CS model in the version \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 (or \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018) and the model of Giménez et al., is the aspect of value scaling. (Note that both models were built using regression methods for nocturnal melatonin suppression data. Both models have been validated using partially similar data sets from well-known research groups).
Numerical analysis of the relationship between brightness and non-visual metrics
Introduction
The brightness metrics and the nonvisual effects of light metrics described above can be grouped into the following categories: A set of linear metrics: Fotios’ model for equivalent luminance without signal compression (Eq. 1); circadian light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA for model versions 2018 and 2021; and mEDI (which is also an input parameter of the logistic function of Giménez et al.).A group of nonlinear metrics such as CS (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021); the metric according to Giménez et al. (output parameter of the logistic function in Eq. (11); and the brightness model M of the authors of the present article, see Eq. (3).Since the CS model includes the case distinction between “warm” and “cold” white light (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$B - Y > 0)$$\end{document}B-Y>0) or (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$B - Y \le 0$$\end{document}B-Y≤0), or empirically if (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CCT\,>\,3710$$\end{document}CCT>3710 K) or (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CCT\,\le \,3710$$\end{document}CCT≤3710 K), the correlation with experimental data may depend on the type of light spectra actually used.Since the CS model (in the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 version) has been used for a long time by U.S. and international lighting science and industry, it is necessary to analyze the differences and correlations between the values of the \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018 and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 versions, as well as the “warm” and “cold” light categories.
Correlation analysis method

Spectra of 884 real measured light source spectra.
| No. | Type of light sources and their parameter ranges 220117815 K; -1.467<< 1.5290.0797 << 0.4792; 80 << 100\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\le$$\end{document}≤\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\le$$\end{document}≤\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\cdot 10^{-2}$$\end{document}·10-2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\cdot 10^{-2}$$\end{document}·10-2\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CIE\,R_a$$\end{document}CIERaCCTDuvz |
|---|---|
| 1 | Conventional incandescent lamps + filtered incandescent lamps, 28 spectra |
| 2 | Fluorescent tubes + Compact fluorescent lamps, 252 spectra |
| 3 | LED lamps + LED luminaires, 419 spectra |
| 4 | Daylight (measurements), 185 spectra |
Relationship between linear brightness metrics and non-visual effect parameters
A formula was derived for the range \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$3710 K < CCT \le 17,815 K$$\end{document}3710K<CCT≤17,815K with an RMSE-value of only 11.85, see Eq. (13).13\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\begin{aligned} mEDI=0.5924 \cdot CL_{A,2021}(\thicksim CL_{A,2.0}) + 55.5 \end{aligned}$$\end{document}mEDI=0.5924·CLA,2021(∼CLA,2)+55.5From the practical point of view of lighting engineering, it must be emphasized that most buildings and rooms in the private and professional sectors will have lighting situations with CCTs higher than 3710 K during the daytime with daylight incidence (i.e. with windows), so that the conversion between mEDI and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_{A,2021}$$\end{document}CLA,2021(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA 2.0) according to Eq. (13) is of high importance.
The above results lead to the conclusion that the correlation between mEDI and the new version \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_{A,2021}$$\end{document}CLA,2021(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA 2.0) is good for the warm white range (e.g. for evening applications) and very good for the range between 3710 K and 17815 K for indoor lighting in residential and commercial buildings (e.g. for offices, schools, supermarkets) as well as for outdoor daylight. The improvement from Circadian Light \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_{A,2018}$$\end{document}CLA,2018(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA 1.0) to the new version \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_{A,2021}$$\end{document}CLA,2021(\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document}CLA 2.0) is significant.
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Correlation betweenand(2.0) for all spectra in Tablebetween 2201 and 17815 K. mEDI \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_{A,2021}$$\end{document} C L A , 2021 \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_A$$\end{document} C L A 2
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Relationship between non-linear brightness metrics and non-visual effect parameters
Table 8 shows the correlation coefficients for the case of the wide range of correlated color temperatures between 3710 and 17,815 K. All metrics for brightness and non-visual light effects express a very good correlation with each other.
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Relationship between the Giménez value andfor all spectra in Tablebetween 2201 and 17815 K. \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021,t=1h,f=1}$$\end{document} C S 2021 1 1 , = , = t h f 2
Discussion and summary
In this article, the concept of non-visual parameters such as the circadian stimulus modes of the Circadian Stimulus by Rea et. al. in the USA (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS20181, \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS20212), melanopic equivalent daylight (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$D_{65}$$\end{document}D65) illuminance, mEDI of the CIE S 026/E: 20183 and the latest formula of Giménez et al.4 for nocturnal melatonin suppression4 are briefly described to understand their structure and characteristics. Also, the equivalent luminance of Fotios et al.5 or the brightness of the TU Darmstadt6 are briefly introduced.
Then the calculations and analyses based on the databases of 884 light sources (26 conventional incandescent lamps and filtered incandescent lamps, 252 fluorescent tubes and compact fluorescent lamps, 419 LED lamps and LED luminaires, and 185 daylight from measurements) were implemented.
Summarizing the results of this article, \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 is a significant improvement over \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2018}$$\end{document}CS2018, which did not work in the warm white region (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CCT \le 3710\,K$$\end{document}CCT≤3710K). The correlation between the brightness metric \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$M_{2023,TUD}$$\end{document}M2023,TUD, the Giménez metric (based on the mEDI metric) and \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CS_{2021}$$\end{document}CS2021 based on \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$CL_{A,2021}(CLA\,2.0)$$\end{document}CLA,2021(CLA2) is good or even very high. Consequently, these three metrics can be converted by linear formulas (see the equations Eqs. (12)–(14) with acceptable accuracy from an engineering point of view.
Informed consent
All authors have read the submitted version of the manuscript.

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