Luminance
Photometric measure of luminous intensity per unit area in a given direction.
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Luminance measures how much luminous intensity, per unit area, travels in a specific direction. It quantifies the light passing through, emitted from, or reflected off a given area, within a defined solid angle. Its SI unit is the candela per square metre (cd/m²), also called the nit. The conversion from spectral radiance to luminance follows standards set by the CIE and ISO. The term "brightness" refers to the subjective impression of this objective measurement.
Luminance is commonly used to describe emission or reflection from flat, diffuse surfaces. The levels indicate how much luminous power the human eye would detect when viewing a surface from a particular angle, making luminance a predictor of how bright that surface will appear. In this context, the relevant solid angle is the one subtended by the eye's pupil. In the video industry, luminance characterizes display brightness; a typical computer display emits between 50 and 300 cd/m², while the sun at noon has a luminance of about 1.6×10⁹ cd/m².
In geometric optics, luminance is invariant: for an ideal optical system, output luminance equals input luminance. For real, passive systems, output luminance is at most equal to the input. For instance, using a lens to form a smaller image concentrates luminous power into a smaller area, raising illuminance, but the light fills a larger solid angle, so luminance remains the same if the lens has no loss. The image can never be "brighter" than the source.
High luminance can damage the retina through local heating or photochemical effects, especially at short wavelengths. The IEC 60825 series provides safety guidance for laser exposure, while the IEC 62471 series evaluates photobiological safety of lamps and lamp systems (including LEDs, excluding lasers) from 200 nm to 3000 nm. This standard originated as CIE S 009:2002.
A luminance meter measures luminance in a specific direction and solid angle. Simple devices measure a single direction, while imaging luminance meters work similarly to a digital camera recording color images.
Mathematically, the luminance at a point on a light source in a given direction is defined by the mixed partial derivative \( L_{\mathrm{v}} = \frac{\mathrm{d}^{2}\Phi_{\mathrm{v}}}{\mathrm{d}\Sigma \, \mathrm{d}\Omega_{\Sigma} \cos \theta_{\Sigma}} \), where \( L_{\mathrm{v}} \) is luminance (cd/m²), \( \mathrm{d}^{2}\Phi_{\mathrm{v}} \) is luminous flux (lm) leaving area \( \mathrm{d}\Sigma \) within solid angle \( \mathrm{d}\Omega_{\Sigma} \), and \( \theta_{\Sigma} \) is the angle between the surface normal and the specified direction. In a lossless medium, luminance remains constant along a light ray. When the ray crosses an arbitrary surface S, luminance is given by \( L_{\mathrm{v}} = \frac{\mathrm{d}^{2}\Phi_{\mathrm{v}}}{\mathrm{d}S \, \mathrm{d}\Omega_{S} \cos \theta_{S}} \).
- SI unit
- candela per square metre (cd/m²)
- Non-SI term
- nit
- CGS unit
- stilb (1 cd/cm² = 10 kcd/m²)
- Typical display range
- 50 to 300 cd/m²
- Solar luminance at noon
- 1.6×10⁹ cd/m²
- Related quantity
- brightness (subjective impression of luminance)
- Standardization bodies
- CIE and ISO
Lore & Background
Luminance is a photometric measure of the luminous intensity per unit area of light traveling in a given direction. It quantifies the amount of light that passes through, is emitted from, or is reflected from a particular area within a given solid angle. The conversion from spectral radiance to luminance is standardized by the CIE and ISO. The SI unit is the candela per square metre (cd/m²), also known as the nit. An older CGS unit is the stilb, equal to one candela per square centimetre. Luminance is used to characterize emission or reflection from flat, diffuse surfaces, indicating how much luminous power the human eye detects from a particular angle of view. In the video industry, it characterizes display brightness; a typical computer display emits within a certain range, while the sun at noon has a luminance of about a specific value. Luminance is invariant in geometric optics: for an ideal optical system, output luminance equals input luminance. For real passive systems, output luminance is at most equal to input; an image can never be brighter than its source. For a perfectly diffuse, or Lambertian, reflector, luminance is isotropic and relates directly to illuminance. A luminance meter measures luminance in a particular direction and solid angle; imaging versions function similarly to a digital camera. High luminance can cause retinal damage through local heating or photochemical effects, especially at short wavelengths. Standards such as IEC 60825 for lasers and IEC 62471 for lamps provide guidance on photobiological safety. In astronomy, luminance is essentially equivalent to surface brightness, measured in magnitudes per square arcsecond.
Reader's Guide
Luminance is fundamental in photometry and vision science, bridging objective measurement and subjective brightness perception. Its invariance in optical systems underpins the design of lenses and displays. Health effects from high luminance include retinal damage via local heating or photochemical effects, especially at short wavelengths. Luminance meters measure luminance in a specific direction and solid angle, with imaging versions operating like digital cameras. The relationship between luminance and illuminance for reflecting surfaces is given by the integral of luminance over emission directions, equating to luminous exitance, which equals illuminance times reflectance. For a perfectly diffuse (Lambertian) reflector, luminance is isotropic and equals (illuminance × reflectance)/π.
Did You Know?
- Luminance is invariant in geometric optics; for an ideal optical system, output luminance equals input luminance.
- The sun has a luminance of about 1.6×10⁹ cd/m² at noon.
- A typical computer display emits between 50 and 300 cd/m².
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Frequently Asked Questions
What exactly is Luminance in photometry?
Luminance quantifies how much light is emitted, reflected, or transmitted from a specific surface area within a particular viewing angle. It essentially measures luminous intensity normalized by the area it covers in a given direction.
What unit do I use for Luminance?
The standard SI unit is the candela per square metre (cd/m²), though in display and video industries it is commonly called a nit. In the older CGS system the equivalent unit is the stilb, where one stilb equals ten thousand cd/m².
How is Luminance different from brightness?
Luminance is an objective, measurable photometric quantity, whereas brightness is the subjective human perception of how light or dark something appears. Two surfaces with identical luminance values can still feel different in perceived brightness depending on the surrounding visual context.
What Luminance values do typical screens produce?
Most consumer displays operate somewhere between 50 and 300 cd/m² under normal usage. By comparison, the sun at midday reaches roughly 1.6 billion cd/m², making it over a million times brighter than a typical monitor.
Which organizations set the standards for Luminance?
Both the CIE (International Commission on Illumination) and ISO maintain the definitions and measurement standards for this photometric quantity. These bodies ensure consistent terminology and unit usage across scientific and industrial applications.
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