Color Spaces and Planckian Loci: Understanding All Those Crazy Color Metrics
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Review of Measures for Light-Source Color Rendition and Considerations for a Two-Measure System for Characterizing Color Rendition
Review of measures for light-source color rendition and considerations for a two-measure system for characterizing color rendition Kevin W. Houser,1,* Minchen Wei,1 Aurélien David,2 Michael R. Krames,2 and Xiangyou Sharon Shen3 1Department of Architectural Engineering, The Pennsylvania State University, University Park, PA, 16802, USA 2Soraa, Inc., Fremont, CA 94555, USA 3Inno-Solution Research LLC, 913 Ringneck Road, State College, PA 16801, USA *[email protected] Abstract: Twenty-two measures of color rendition have been reviewed and summarized. Each measure was computed for 401 illuminants comprising incandescent, light-emitting diode (LED) -phosphor, LED-mixed, fluorescent, high-intensity discharge (HID), and theoretical illuminants. A multidimensional scaling analysis (Matrix Stress = 0.0731, R2 = 0.976) illustrates that the 22 measures cluster into three neighborhoods in a two- dimensional space, where the dimensions relate to color discrimination and color preference. When just two measures are used to characterize overall color rendition, the most information can be conveyed if one is a reference- based measure that is consistent with the concept of color fidelity or quality (e.g., Qa) and the other is a measure of relative gamut (e.g., Qg). ©2013 Optical Society of America OCIS codes: (330.1690) Color; (330.1715) Color, rendering and metamerism; (230.3670) Light-emitting diodes. References and links 1. CIE, “Methods of measuring and specifying colour rendering properties of light sources,” in CIE 13 (CIE, Vienna, Austria, 1965). 2. W. Walter, “How meaningful is the CIE color rendering index?” Light Design Appl. 11(2), 13–15 (1981). 3. T. Seim, “In search of an improved method for assessing the colour rendering properties of light sources,” Lighting Res. -
Calculation of CCT and Duv and Practical Conversion Formulae
CORM 2011 Conference, Gaithersburg, MD, May 3-5, 2011 Calculation of CCT and Duv and Practical Conversion Formulae Yoshi Ohno Group Leader, NIST Fellow Optical Technology Division National Institute of Standards and Technology Gaithersburg, Maryland USA CORM 2011 1 White Light Chromaticity Duv CCT CORM 2011 2 Duv often missing Lighting Facts Label CCT and CRI do not tell the whole story of color quality CORM 2011 3 CCT and CRI do not tell the whole story Triphosphor FL simulation Not acceptable Not preferred Neodymium (Duv=-0.005) Duv is another important dimension of chromaticity. CORM 2011 4 Duv defined in ANSI standard Closest distance from the Planckian locus on the (u', 2/3 v') diagram, with + sign for above and - sign for below the Planckian locus. (ANSI C78.377-2008) Symbol: Duv CCT and Duv can specify + Duv the chromaticity of light sources just like (x, y). - Duv The two numbers (CCT, Duv) provides color information intuitively. (x, y) does not. Duv needs to be defined by CIE. CORM 2011 5 ANSI C78.377-2008 Specifications for the chromaticity of SSL products CORM 2011 6 CCT- Duv chart 5000 K 3000 K 4000 K 6500 K 2700 K 3500 K 4500 K 5700 K ANSI 7-step MacAdam C78.377 ellipses quadrangles (CCT in log scale) CORM 2011 7 Correlated Color Temperature (CCT) Temperature [K] of a Planckian radiator whose chromaticity is closest to that of a given stimulus on the CIE (u’,2/3 v’) coordinate. (CIE 15:2004) CCT is based on the CIE 1960 (u, v) diagram, which is now obsolete. -
Comparing Measures of Gamut Area
Comparing Measures of Gamut Area Michael P Royer1 1Pacific Northwest National Laboratory 620 SW 5th Avenue, Suite 810 Portland, OR 97204 [email protected] This is an archival copy of an article published in LEUKOS. Please cite as: Royer MP. 2018. Comparing Measures of Gamut Area. LEUKOS. Online Before Print. DOI: 10.1080/15502724.2018.1500485. PNNL-SA-132222 ▪ November 2018 COMPARING MEASURES OF GAMUT AREA Abstract This article examines how the color sample set, color space, and other calculation elements influence the quantification of gamut area. The IES TM-30-18 Gamut Index (Rg) serves as a baseline, with comparisons made to several other measures documented in scientific literature and 12 new measures formulated for this analysis using various components of existing measures. The results demonstrate that changes in the color sample set, color space, and calculation procedure can all lead to substantial differences in light source performance characterizations. It is impossible to determine the relative “accuracy” of any given measure outright, because gamut area is not directly correlated with any subjective quality of an illuminated environment. However, the utility of different approaches was considered based on the merits of individual components of the gamut area calculation and based on the ability of a measure to provide useful information within a complete system for evaluating color rendition. For gamut area measures, it is important to have a reasonably uniform distribution of color samples (or averaged coordinates) across hue angle—avoiding exclusive use of high-chroma samples—with sufficient quantity to ensure robustness but enough difference to avoid incidents of the hue-angle order of the samples varying between the test and reference conditions. -
E GE Enhanced Color Lamps
e GE Enhanced Color Lamps TRANSFORM YOUR BUSINESS... WITH THE CHANGE OF A LIGHT BULB GE enhanced GE ENHANCED color lighting can... ■ Render colors in a natural way. COLOR LIGHTING ■ Highlight and accent objects as never before. ■ Allow you to choose light sources that enhance colors, giving furnishings, merchandise and even people a rich, vibrant look. CAN TRANSFORM ■ Give your surroundings a “warm” or “cool” tone, or somewhere in between. ■ Provide a pleasing light that improves visual A FACILITY FROM appeal, enhances productivity and overall satisfaction of the occupants of the space. ■ Permit more accurate determination of THE ORDINARY color differences. In addition to color enhancement, many of these GE products can also significantly reduce your energy costs and save lamp INTO THE replacement and labor costs. Evaluating light source color. EXTRAORDINARY. Two common ways of specifying light source color are: color temperature and color rendering index. Color Temperature indicates the atmosphere created WITH THE SIMPLE by the light source. • The higher the color temperature, the “cooler” the color. • Color temperatures... – Of 2000K-3000K create a “warm” atmosphere. CHANGE OF A – Above 4000K are “cool” appearance. – Between 3000K and 4000K are considered intermediate and tend to be preferred. LIGHT BULB, YOUR Color Rendering Index (CRI) rates a light source’s ability to render colors in a natural and normal way, based on a scale from 0 to 100. • In general, light sources with high CRI (80-100) BUSINESS CAN will make people and things look better than those with lower CRIs. TAKE ON A VIBRANT NEW LOOK. Color Rendering and 7000K Overcast C75 Sky Color Temperature Starcoat™ The chart at right shows both dimensions of light source SP65 SP65 color—color temperature and color rendering—for the most popular light sources. -
Calculating Correlated Color Temperatures Across the Entire Gamut of Daylight and Skylight Chromaticities
Calculating correlated color temperatures across the entire gamut of daylight and skylight chromaticities Javier Herna´ ndez-Andre´ s, Raymond L. Lee, Jr., and Javier Romero Natural outdoor illumination daily undergoes large changes in its correlated color temperature ͑CCT͒, yet existing equations for calculating CCT from chromaticity coordinates span only part of this range. To improve both the gamut and accuracy of these CCT calculations, we use chromaticities calculated from our measurements of nearly 7000 daylight and skylight spectra to test an equation that accurately maps CIE 1931 chromaticities x and y into CCT. We extend the work of McCamy ͓Color Res. Appl. 12, 285–287 ͑1992͔͒ by using a chromaticity epicenter for CCT and the inverse slope of the line that connects it to x and y. With two epicenters for different CCT ranges, our simple equation is accurate across wide chromaticity and CCT ranges ͑3000–106 K͒ spanned by daylight and skylight. © 1999 Optical Society of America OCIS codes: 010.1290, 330.1710, 330.1730. 1. Introduction term correlated color temperature ͑CCT͒ instead of A colorimetric landmark often included in the Com- color temperature to describe its appearance. Sup- mission Internationale de l’Eclairage ͑CIE͒ 1931 pose that x1, y1 is the chromaticity of such an off-locus chromaticity diagram is the locus of chromaticity co- light source. By definition, the CCT of x1, y1 is the ordinates defined by blackbody radiators ͑see Fig. 1, temperature of the Planckian radiator whose chro- inset͒. One can calculate this Planckian ͑or black- maticity is nearest to x1, y1. The colorimetric body͒ locus by colorimetrically integrating the Planck minimum-distance calculations that determine CCT function at many different temperatures, with each must be done within the color space of the CIE 1960 temperature specifying a unique pair of 1931 x, y uniformity chromaticity scale ͑UCS͒ diagram. -
Cooledge Light Quality Metrics Fabricated
COOLEDGE LIGHT QUALITY METRICS: FABRICATED LUMINAIRES - 3500K NOTES ABOUT LIGHT QUALITY METRICS DATA: ― Values shown are TYPICAL – actual performance of individual units may vary ― The data presented has been generated in accordance with LM-79-08 ― A complete summary of LM-79-08 data is provided for nominal 4x8 (1200x2400) FABRICated Luminaire models only; however, spectral and color rendering data is applicable to all luminaire sizes, models, and flux levels including: ― Spectral Power Distribution (SPD) ― Nominal CCT ― Chromaticity ― Rf and Rg (TM-30-15) ― CRI (Ra) and R-values ― Duv SELECTED DEFINITIONS ― Candlepower: As presented in this document it is the same as “candela” the SI unit of measurement for light intensity. ― CRI (Ra): The general Color Rendering Index based on 8 CIE reference pastel color samples. ― Duv: The American National Standards Institute (ANSI) references Duv, a metric based on the CIE 1976 color space that quantifies the distance between the chromaticity of a given light source and a blackbody radiator of equal CCT. A negative Duv indicates that the source is “below” the Planckian locus (blackbody curve), potentially having a red/ blue tint, whereas a positive Duv indicates that the source is “above” the curve, potentially exhibiting a green tint. ― Nominal CCT Quadrangles: ANSI has defined acceptable chromaticity quadrangles for LED binning in relation to the blackbody curve within CIE color space. The data presented shows the typical chromaticity coordinate within the relevant quadrangle. ― R-value (Ri): The R-value is a mathematical calculation measuring how similar a light source renders a particular color compared to a reference blackbody source of the same CCT. -
A Correlated Color Temperature for Illuminants
. (R P 365) A CORRELATED COLOR TEMPERATURE FOR ILLUMINANTS By Raymond Davis ABSTRACT As has long been known, most of the artificial and natural illuminants do not match exactly any one of the Planckian colors. Therefore, strictly speaking, they can not be assigned a color temperature. A color of this type may, however, be correlated with a representative Planckian color. The method of determining correlated color temperature described in this paper consists in comparing the relative luminosities of each of the three primary red, green, and blue components of the source with similar values for the Planckian series. With such a comparison three component temperatures are obtained; that is, the red component of the source corresponds with that of the Planckian radiator at one temperature, its green component with that of the Planckian radiator at a second temperature, and its blue component with that of the Planckian radiator at a third temperature. The average of these three component temperatures is designated as the correlated color temperature of the source. The mean devia- tion of the component temperatures from the average temperature is used as a basis for specifying the color (chromaticity) departure of the source from that of the Planckian radiator at the correlated color temperature. The conjunctive wave length indicates the kind of color departure. CONTENTS Page I. Introduction 659 II. The proposed method 662 III. Procedure 665 1. The Planckian radiator evaluated in terms of relative lumi- nosity of the primary components 665 2. Computation of the correlated color temperature 670 3. Calculation of color departure in terms of sensation steps 672 4. -
Calculating Color Temperature and Illuminance Using the TAOS TCS3414CS Digital Color Sensor Contributed by Joe Smith February 27, 2009 Rev C
TAOS Inc. is now ams AG The technical content of this TAOS document is still valid. Contact information: Headquarters: ams AG Tobelbader Strasse 30 8141 Premstaetten, Austria Tel: +43 (0) 3136 500 0 e-Mail: [email protected] Please visit our website at www.ams.com NUMBER 25 INTELLIGENT OPTO SENSOR DESIGNER’S NOTEBOOK Calculating Color Temperature and Illuminance using the TAOS TCS3414CS Digital Color Sensor contributed by Joe Smith February 27, 2009 Rev C ABSTRACT The Color Temperature and Illuminance of a broad band light source can be determined with the TAOS TCS3414CS red, green and blue digital color sensor with IR blocking filter built in to the package. This paper will examine Color Temperature and discuss how to calculate the Color Temperature and Illuminance of a given light source. Color Temperature information could be useful in feedback control and quality control systems. COLOR TEMPERATURE Color temperature has long been used as a metric to characterize broad band light sources. It is a means to characterize the spectral properties of a near-white light source. Color temperature, measured in degrees Kelvin (K), refers to the temperature to which one would have to heat a blackbody (or planckian) radiator to produce light of a particular color. A blackbody radiator is defined as a theoretical object that is a perfect radiator of visible light. As the blackbody radiator is heated it radiates energy first in the infrared spectrum and then in the visible spectrum as red, orange, white and finally bluish white light. Incandescent lights are good models of blackbody radiators, because most of the light emitted from them is due to the heating of their filaments. -
Estimation of Illuminants from Projections on the Planckian Locus Baptiste Mazin, Julie Delon, Yann Gousseau
Estimation of Illuminants From Projections on the Planckian Locus Baptiste Mazin, Julie Delon, Yann Gousseau To cite this version: Baptiste Mazin, Julie Delon, Yann Gousseau. Estimation of Illuminants From Projections on the Planckian Locus. IEEE Transactions on Image Processing, Institute of Electrical and Electronics Engineers, 2015, 24 (6), pp. 1944 - 1955. 10.1109/TIP.2015.2405414. hal-00915853v3 HAL Id: hal-00915853 https://hal.archives-ouvertes.fr/hal-00915853v3 Submitted on 9 Oct 2014 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 Estimation of Illuminants From Projections on the Planckian Locus Baptiste Mazin, Julie Delon and Yann Gousseau Abstract—This paper introduces a new approach for the have been proposed, restraining the hypothesis to well chosen automatic estimation of illuminants in a digital color image. surfaces of the scene, that are assumed to be grey [41]. Let The method relies on two assumptions. First, the image is us mention the work [54], which makes use of an invariant supposed to contain at least a small set of achromatic pixels. The second assumption is physical and concerns the set of color coordinate [20] that depends only on surface reflectance possible illuminants, assumed to be well approximated by black and not on the scene illuminant. -
Optimizing Color Rendering Index Using Standard Object Color Spectra Database and CIECAM02
Optimizing Color Rendering Index Using Standard Object Color Spectra Database and CIECAM02 Pei-Li Sun Department of Information Management, Shih Hsin University, Taiwan Abstract is an idea reference for developing new CRIs. On the As CIE general color rending index (CRI) still uses other hand, CIE TC8-01 recommended CIECAM02 obsolete color space and color difference formula, it color appearance model for cross-media color 3 should be updated for new spaces and new formulae. reproduction. As chromatic adaptation plays an * * * The aim of this study is to optimize the CRI using ISO important role on visual perception, U V W should standard object color spectra database (SOCS) and be replaced by CIECAM02. However, CIE has not yet CIECAM02. In this paper, proposed CRIs were recommended any color difference formula for 3 optimized to evaluate light sources for four types of CIECAM02 applications. The aim of this study is object colors: synthetic dyes for textiles, flowers, paint therefore to evaluate the performance of proposed (not for art) and human skin. The optimization was CRI based on the SOCS and CIECAM02. How to based on polynomial fitting between mean color evaluate its performance also is a difficult question. variations (ΔEs) and visual image differences (ΔVs). The answer of this study is to create series of virtual TM The former was calculated by the color differences on scene using Autodesk 3ds Max to simulate the color SOCS’s typical/difference sets between test and appearance of real-world objects under test reference illuminants. The latter was obtained by a illuminants and their CCT (correlated color visual experiment based on four virtual scenes under temperature) corresponding reference lighting 15 different illuminants created by Autodesk 3ds Max. -
Standard Illuminant
Standard illuminant From Wikipedia, the free encyclopedia A standard illuminant is a profile or spectrum of visible light which is published in order to allow images or colors recorded under different lighting to be compared. Contents 1 CIE illuminants 1.1 Illuminant A 1.2 Illuminants B and C 1.3 Illuminant series D 1.4 Illuminant E Relative spectral power distributions (SPDs) of CIE 1.5 Illuminant series F illuminants A, B, and C from 380nm to 780nm. 2 White point 2.1 White points of standard illuminants 3 References 4 External links CIE illuminants The International Commission on Illumination (usually abbreviated CIE for its French name) is the body responsible for publishing all of the well-known standard illuminants. Each of these is known by a letter or by a letter-number combination. Illuminants A, B, and C were introduced in 1931, with the intention of respectively representing average incandescent light, direct sunlight, and average daylight. Illuminants D represent phases of daylight, Illuminant E is the equal-energy illuminant, while Illuminants F represent fluorescent lamps of various composition. There are instructions on how to experimentally produce light sources ("standard sources") corresponding to the older illuminants. For the relatively newer ones (such as series D), experimenters are left to measure to profiles of their sources and compare them to the published spectra:[1] At present no artificial source is recommended to realize CIE standard illuminant D65 or any other illuminant D of different CCT. It is hoped that new developments in light sources and filters will eventually offer sufficient basis for a CIE recommendation. -
Better Colour Rendering Offers Many Benefits
TYRI CASE STUDY BETTER COLOUR RENDERING OFFERS MANY BENEFITS Caravan Mill provides its environment. The result was both customers with gravel and better working conditions and sand which they refine “ increased productivity. ...Drivers have a hard time dealing from blasted stone. A job with the big differences between that requires precision and “For us, good lighting is primarily a white bright light from the headlights work environment and safety issue. powerful machines. The work and the dark environment next to the We work long days and for large environment is dusty and often machine. parts of the year it is dark both in dark so the lighting on their the morning and in the afternoons. machines is crucial for both the ...With TYRI´s new work lights, it Drivers have a hard time dealing with employee’s health and safety the big differences between white has become much better. Today, we as well as the productivity at bright light from the headlights have significantly better lighting that work. and the dark environment next makes our drivers feel better and to the machine. When the eye is To meet the challenges of with that, safety and productivity forced to switch between white light reflections, color rendering and increases.” and darkness for many hours, the a safe work environment for the consequence is often headaches - Pierre Jakobsson, Caravan Mill. operators, TYRI has spent four and fatigue. With TYRI´s new work years developing a LED work light lights, it has become much better. that now measures 90-95 CRI Today, we have significantly better (color rendering index).