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Luminance

Not to be confused withLuma (video),Luminescence, orIlluminance.
For other uses, seeLuminance (disambiguation).
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Luminance is aphotometric measure of theluminous intensity perunit area oflight travelling in a given direction.[1] It describes the amount of light that passes through, is emitted from, or is reflected from a particular area, and falls within a givensolid angle.

Atea light-type candle, imaged with a luminance camera;false colors indicate luminance levels per the bar on the right (cd/m2)

The procedure for conversion from spectralradiance to luminance is standardized by theCIE andISO.[2]

Brightness is theterm for thesubjective impression of theobjective luminance measurement standard (seeObjectivity (science) § Objectivity in measurement for the importance of this contrast).

TheSI unit for luminance iscandela per square metre (cd/m2). A non-SI term for the same unit is thenit. The unit in theCentimetre–gram–second system of units (CGS) (which predated the SI system) is thestilb, which is equal to one candela per square centimetre or 10 kcd/m2.

Description

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Luminance is often used to characterize emission or reflection from flat,diffuse surfaces. Luminance levels indicate how muchluminous power could be detected by thehuman eye looking at a particular surface from a particularangle of view. Luminance is thus an indicator of howbright the surface will appear. In this case, the solid angle of interest is the solid angle subtended by the eye'spupil.

Luminance is used in the video industry to characterize the brightness of displays. A typical computer display emits between50 and 300 cd/m2. The sun has a luminance of about1.6×109 cd/m2 at noon.[3]

Luminance isinvariant ingeometric optics.[4] This means that for an ideal optical system, the luminance at the output is the same as the input luminance.

For real, passive optical systems, the output luminance isat most equal to the input. As an example, if one uses a lens to form an image that is smaller than the source object, the luminous power is concentrated into a smaller area, meaning that theilluminance is higher at the image. The light at the image plane, however, fills a larger solid angle so the luminance comes out to be the same assuming there is no loss at the lens. The image can never be "brighter" than the source.

Health effects

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Further information:Laser safety

Retinal damage can occur when the eye is exposed to high luminance. Damage can occur because of local heating of the retina. Photochemical effects can also cause damage, especially at short wavelengths.[5]

The IEC 60825 series gives guidance on safety relating to exposure of the eye to lasers, which are high luminance sources. The IEC 62471 series gives guidance for evaluating the photobiological safety of lamps and lamp systems including luminaires. Specifically it specifies the exposure limits, reference measurement technique and classification scheme for the evaluation and control of photobiological hazards from all electrically powered incoherent broadband sources of optical radiation, including LEDs but excluding lasers, in the wavelength range from200 nm through3000 nm. This standard was prepared as Standard CIE S 009:2002 by the International Commission on Illumination.

Luminance meter

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Aluminance meter is a device used inphotometry that can measure the luminance in a particular direction and with a particularsolid angle. The simplest devices measure the luminance in a single direction while imaging luminance meters measure luminance in a way similar to the way adigital camera records color images.[6]

Formulation

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Parameters for defining the luminance

The luminance of a specified point of a light source, in a specified direction, is defined by themixed partial derivativeLv=d2ΦvdΣdΩΣcosθΣ{\displaystyle L_{\mathrm {v} }={\frac {\mathrm {d} ^{2}\Phi _{\mathrm {v} }}{\mathrm {d} \Sigma \,\mathrm {d} \Omega _{\Sigma }\cos \theta _{\Sigma }}}} where

  • Lv is the luminance (cd/m2);
  • d2Φv is theluminous flux (lm) leaving the area in any direction contained inside the solid angleΣ;
  • is aninfinitesimal area (m2) of the source containing the specified point;
  • Σ is an infinitesimalsolid angle (sr) containing the specified direction; and
  • θΣ is theangle between thenormalnΣ to the surface and the specified direction.[7]

If light travels through a lossless medium, the luminance does not change along a givenlight ray. As the ray crosses an arbitrary surfaceS, the luminance is given byLv=d2ΦvdSdΩScosθS{\displaystyle L_{\mathrm {v} }={\frac {\mathrm {d} ^{2}\Phi _{\mathrm {v} }}{\mathrm {d} S\,\mathrm {d} \Omega _{S}\cos \theta _{S}}}} where

  • dS is the infinitesimal area ofS seen from the source inside the solid angleΣ;
  • S is the infinitesimal solid anglesubtended by as seen fromdS; and
  • θS is the angle between the normalnS todS and the direction of the light.

More generally, the luminance along a light ray can be defined asLv=n2dΦvdG{\displaystyle L_{\mathrm {v} }=n^{2}{\frac {\mathrm {d} \Phi _{\mathrm {v} }}{\mathrm {d} G}}} where

  • dG is theetendue of an infinitesimally narrow beam containing the specified ray;
  • v is the luminous flux carried by this beam; and
  • n is theindex of refraction of the medium.

Relation to illuminance

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Comparison of photometric and radiometric quantities

The luminance of a reflecting surface is related to theilluminance it receives:ΩΣLvdΩΣcosθΣ=Mv=EvR,{\displaystyle \int _{\Omega _{\Sigma }}L_{\text{v}}\mathrm {d} \Omega _{\Sigma }\cos \theta _{\Sigma }=M_{\text{v}}=E_{\text{v}}R,} where the integral covers all the directions of emissionΩΣ,

In the case of a perfectlydiffuse reflector (also called aLambertian reflector), the luminance is isotropic, perLambert's cosine law. Then the relationship is simplyLv=EvRπ.{\displaystyle L_{\text{v}}={\frac {E_{\text{v}}R}{\pi }}.} 

Units

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A variety of units have been used for luminance, besides the candela per square metre. Luminance is essentially the same assurface brightness, the term used in astronomy. This is measured with a logarithmic scale, magnitudes per square arcsecond (MPSAS).

Units of luminance
cd/m2(SI unit)
≡ nit≡ lm/m2/sr
stilb (sb)(CGS unit)
≡ cd/cm2
apostilb (asb)
≡ blondel
brilskot (sk)lambert (L)foot-lambert (fL)
= 1 ⁄π cd/ft2
1 cd/m2=110−4π
≈ 3.142
107π
≈ 3.142×107
103π
≈ 3.142×103
10−4π
≈ 3.142×10−4
0.30482π
≈ 0.2919
1 sb=1041104π
≈ 3.142×104
1011π
≈ 3.142×1011
107π
≈ 3.142×107
π
≈ 3.142
30.482π
≈ 2919
1 asb=1 ⁄π
≈ 0.3183
10−4π
≈ 3.183×10−5
110710310−40.30482
≈ 0.09290
1 bril=10−7π
≈ 3.183×10−8
10−11π
≈ 3.183×10−12
10−7110−410−110.30482×10−7
≈ 9.290×10−9
1 sk=10−3π
≈ 3.183×10−4
10−7π
≈ 3.183×10−8
10−3104110−70.30482×10−3
≈ 9.290×10−5
1 L=104π
≈ 3183
1 ⁄π
≈ 0.3183
104101110710.30482×104
≈ 929.0
1 fL=1 ⁄ 0.30482π
≈ 3.426
1 ⁄ 30.482π
≈ 3.426×10−4
1 ⁄ 0.30482
≈ 10.76
107 ⁄ 0.30482
≈ 1.076×108
103 ⁄ 0.30482
≈ 1.076×104
10−4 ⁄ 0.30482
≈ 1.076×10−3
1

See also

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Table of SI light-related units

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SI photometry quantities
QuantityUnitDimension
[nb 1]
Notes
NameSymbol[nb 2]NameSymbol
Luminous energyQv[nb 3]lumen secondlm⋅sTJThe lumen second is sometimes called thetalbot.
Luminous flux, luminous powerΦv[nb 3]lumen (= candelasteradian)lm (= cd⋅sr)JLuminous energy per unit time
Luminous intensityIvcandela (= lumen per steradian)cd (= lm/sr)JLuminous flux per unitsolid angle
LuminanceLvcandela per square metrecd/m2 (= lm/(sr⋅m2))L−2JLuminous flux per unit solid angle per unitprojected source area. The candela per square metre is sometimes called thenit.
IlluminanceEvlux (= lumen per square metre)lx (= lm/m2)L−2JLuminous fluxincident on a surface
Luminous exitance, luminous emittanceMvlumen per square metrelm/m2L−2JLuminous fluxemitted from a surface
Luminous exposureHvlux secondlx⋅sL−2TJTime-integrated illuminance
Luminous energy densityωvlumen second per cubic metrelm⋅s/m3L−3TJ
Luminous efficacy (of radiation)Klumen perwattlm/WM−1L−2T3JRatio of luminous flux toradiant flux
Luminous efficacy (of a source)η[nb 3]lumen perwattlm/WM−1L−2T3JRatio of luminous flux to power consumption
Luminous efficiency, luminous coefficientV1Luminous efficacy normalized by the maximum possible efficacy
See also:
  1. ^The symbols in this column denotedimensions; "L", "T" and "J" are for length, time and luminous intensity respectively, not the symbols for theunits litre, tesla and joule.
  2. ^Standards organizations recommend that photometric quantities be denoted with a subscript "v" (for "visual") to avoid confusion with radiometric orphoton quantities. For example:USA Standard Letter Symbols for Illuminating Engineering USAS Z7.1-1967, Y10.18-1967
  3. ^abcAlternative symbols sometimes seen:W for luminous energy,P orF for luminous flux, andρ for luminous efficacy of a source.

References

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  1. ^"luminance, 17-21-050".CIE S 017:2020 ILV: International Lighting Vocabulary, 2nd edition. CIE - International Commission on Illumination. 2020. Retrieved20 April 2023.
  2. ^ISO/CIE 23539:2023 CIE TC 2-93 Photometry — The CIE system of physical photometry. ISO/CIE. 2023.doi:10.25039/IS0.CIE.23539.2023.
  3. ^"Luminance".Lighting Design Glossary. RetrievedApr 13, 2009.
  4. ^Dörband, Bernd; Gross, Herbert; Müller, Henriette (2012). Gross, Herbert (ed.).Handbook of Optical Systems. Vol. 5, Metrology of Optical Components and Systems.Wiley. p. 326.ISBN 978-3-527-40381-3.
  5. ^IEC 60825-1:2014Safety of laser products - Part 1: Equipment classification and requirements (in English, French, and Spanish) (3rd ed.).International Electrotechnical Commission. 2014-05-15. p. 220. -TC 76 - Optical radiation safety and laser equipment
  6. ^"e-ILV : Luminance meter". CIE. Archived fromthe original on 16 September 2017. Retrieved20 February 2013.
  7. ^Chaves, Julio (2015).Introduction to Nonimaging Optics, Second Edition.CRC Press. p. 679.ISBN 978-1482206739.Archived from the original on 2016-02-18.

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