A lux meter for measuring illuminances in work places
General information
Unit system
SI derived unit
Unit of
illuminance
Symbol
lx
Conversions
1 lx in ...
... is equal to ...
SAE units
0.0929 fc
CGS units
10−4 phots
The lux (symbol: lx) is the SI derived unit of illuminance and luminous emittance, measuring luminous flux per unit area.[1] It is equal to one lumen per square metre. In photometry, this is used as a measure of the intensity, as perceived by the human eye, of light that hits or passes through a surface. It is analogous to the radiometric unit watt per square metre, but with the power at each wavelength weighted according to the luminosity function, a standardized model of human visual brightness perception. In English, "lux" is used as both the singular and plural form.[2]
Contents
1Explanation
1.1Illuminance
1.2Luminous emittance
1.3Relationship between illuminance and irradiance
2Use in video-camera specifications
3Non-SI units of illuminance
4Legacy Unicode symbol
5SI photometry units
6See also
7Notes and references
8External links
Explanation
Illuminance
Luminous energy and power
Luminous exitance
Illuminance
Luminous intensity
Luminance
Illuminance is a measure of how much luminous flux is spread over a given area. One can think of luminous flux (measured in lumens) as a measure of the total "amount" of visible light present, and the illuminance as a measure of the intensity of illumination on a surface. A given amount of light will illuminate a surface more dimly if it is spread over a larger area, so illuminance is inversely proportional to area when the luminous flux is held constant.
One lux is equal to one lumen per square metre:
1 lx = 1 lm/m2 = 1 cd·sr/m2.
A flux of 1000 lumens, concentrated into an area of 1 square metre, lights up that square metre with an illuminance of 1000 lux. However, the same 1000 lumens, spread out over 10 square metres, produces a dimmer illuminance of only 100 lux.
Achieving an illuminance of 500 lux might be possible in a home kitchen with a single fluorescent light fixture with an output of 12000 lumens. To light a factory floor with dozens of times the area of the kitchen would require dozens of such fixtures. Thus, lighting a larger area to the same level of lux requires a greater number of lumens.
As with other SI units, SI prefixes can be used, for example a kilolux (klx) is 1000 lux.
Here are some examples of the illuminance provided under various conditions:
Illuminance (lux)
Surfaces illuminated by
0.0001
Moonless, overcast night sky (starlight)[3]
0.002
Moonless clear night sky with airglow[3]
0.05–0.3
Full moon on a clear night[4]
3.4
Dark limit of civil twilight under a clear sky[5]
20–50
Public areas with dark surroundings[6]
50
Family living room lights (Australia, 1998)[7]
80
Office building hallway/toilet lighting[8][9]
100
Very dark overcast day[3]
150
Train station platforms[10]
320–500
Office lighting[7][11][12][13]
400
Sunrise or sunset on a clear day.
1000
Overcast day;[3] typical TV studio lighting
10,000–25,000
Full daylight (not direct sun)[3]
32,000–100,000
Direct sunlight
The illuminance provided by a light source on a surface perpendicular to the direction to the source is a measure of the strength of that source as perceived from that location. For instance, a star of apparent magnitude 0 provides 2.08 microlux at the Earth's surface.[14] A barely perceptible magnitude 6 star provides 8 nanolux.[15] The unobscured Sun provides an illumination of up to 100 kilolux on the Earth's surface, the exact value depending on time of year and atmospheric conditions. This direct normal illuminance is related to the solar illuminance constant Esc, equal to 128000 lux (see Sunlight and Solar constant).
The illuminance on a surface depends on how the surface is tilted with respect to the source. For example, a pocket flashlight aimed at a wall will produce a given level of illumination if aimed perpendicular to the wall, but if the flashlight is aimed at increasing angles to the perpendicular (maintaining the same distance), the illuminated spot becomes larger and so is less highly illuminated. When a surface is tilted at an angle to a source, the illumination provided on the surface is reduced because the tilted surface subtends a smaller solid angle from the source, and therefore it receives less light. For a point source, the illumination on the tilted surface is reduced by a factor equal to the cosine of the angle between a ray coming from the source and the normal to the surface.[16] In practical lighting problems, given information on the way light is emitted from each source and the distance and geometry of the lighted area, a numerical calculation can be made of the illumination on a surface by adding the contributions of every point on every light source.
Luminous emittance
The lux is also a measure of luminous emittance, the number of lumens given off by a surface per square metre, regardless of how that light is distributed in terms of the directions in which it is emitted. It differs from the luminance (measured in candela per square metre or "nits"), which does depend on the angular distribution of the emission. A perfectly white surface with one lux falling on it will emit one lux.
Relationship between illuminance and irradiance
Like all photometric units, the lux has a corresponding "radiometric" unit. The difference between any photometric unit and its corresponding radiometric unit is that radiometric units are based on physical power, with all wavelengths being weighted equally, while photometric units take into account the fact that the human eye's image-forming visual system is more sensitive to some wavelengths than others, and accordingly every wavelength is given a different weight. The weighting factor is known as the luminosity function.
The lux is one lumen per square metre (lm/m2), and the corresponding radiometric unit, which measures irradiance, is the watt per square metre (W/m2). There is no single conversion factor between lux and W/m2; there is a different conversion factor for every wavelength, and it is not possible to make a conversion unless one knows the spectral composition of the light.
The peak of the luminosity function is at 555 nm (green); the eye's image-forming visual system is more sensitive to light of this wavelength than any other. For monochromatic light of this wavelength, the amount of illuminance for a given amount of irradiance is maximum: 683.002 lux per 1 W/m2; the irradiance needed to make 1 lux at this wavelength is about 1.464 mW/m2. Other wavelengths of visible light produce fewer lux per watt-per-meter-squared. The luminosity function falls to zero for wavelengths outside the visible spectrum.
For a light source with mixed wavelengths, the number of lumens per watt can be calculated by means of the luminosity function. In order to appear reasonably "white", a light source cannot consist solely of the green light to which the eye's image-forming visual photoreceptors are most sensitive, but must include a generous mixture of red and blue wavelengths, to which they are much less sensitive.
This means that white (or whitish) light sources produce far fewer lumens per watt than the theoretical maximum of 683.002 lm/W. The ratio between the actual number of lumens per watt and the theoretical maximum is expressed as a percentage known as the luminous efficiency. For example, a typical incandescent light bulb has a luminous efficiency of only about 2%.
In reality, individual eyes vary slightly in their luminosity functions. However, photometric units are precisely defined and precisely measurable. They are based on an agreed-upon standard luminosity function based on measurements of the spectral characteristics of image-forming visual photoreception in many individual human eyes.
Use in video-camera specifications
Specifications for video cameras such as camcorders and surveillance cameras often include a minimal illuminance level in lux at which the camera will record a satisfactory image.[citation needed] A camera with good low-light capability will have a lower lux rating. Still cameras do not use such a specification, since longer exposure times can generally be used to make pictures at very low illuminance levels, as opposed to the case in video cameras, where a maximal exposure time is generally set by the frame rate.
Non-SI units of illuminance
The corresponding unit in English and American traditional units is the foot-candle. One foot candle is about 10.764 lux. Since one foot-candle is the illuminance cast on a surface by a one-candela source one foot away, a lux could be thought of as a "metre-candle", although this term is discouraged because it does not conform to SI standards for unit names.
One phot (ph) equals 10 kilolux.
One nox (nx) equals 1 millilux.
In astronomy, apparent magnitude is a measure of the illuminance of a star on the Earth's atmosphere. A star with apparent magnitude 0 is 2.54 microlux outside the earth's atmosphere, and 82% of that (2.08 microlux) under clear skies.[14] A magnitude 6 star (just barely visible under good conditions) would be 8.3 nanolux. A standard candle (one candela) a kilometre away would provide an illuminance of 1 microlux—about the same as a magnitude 1 star.
Legacy Unicode symbol
Unicode has a symbol for "lx": (㏓). It is a legacy code to accommodate old code pages in some Asian languages. Use of this code is not recommended.
SI photometry units
SI photometry quantities
v
t
e
Quantity
Unit
Dimension
Notes
Name
Symbol[nb 1]
Name
Symbol
Symbol[nb 2]
Luminous energy
Qv[nb 3]
lumen second
lm⋅s
T⋅J
The lumen second is sometimes called the talbot.
Luminous flux, luminous power
Φv[nb 3]
lumen (= candela steradians)
lm (= cd⋅sr)
J
Luminous energy per unit time
Luminous intensity
Iv
candela (= lumen per steradian)
cd (= lm/sr)
J
Luminous flux per unit solid angle
Luminance
Lv
candela per square metre
cd/m2
L−2⋅J
Luminous flux per unit solid angle per unit projected source area. The candela per square metre is sometimes called the nit.
Illuminance
Ev
lux (= lumen per square metre)
lx (= lm/m2)
L−2⋅J
Luminous flux incident on a surface
Luminous exitance, luminous emittance
Mv
lux
lx
L−2⋅J
Luminous flux emitted from a surface
Luminous exposure
Hv
lux second
lx⋅s
L−2⋅T⋅J
Time-integrated illuminance
Luminous energy density
ωv
lumen second per cubic metre
lm⋅s/m3
L−3⋅T⋅J
Luminous efficacy (of radiation)
K
lumen per watt
lm/W
M−1⋅L−2⋅T3⋅J
Ratio of luminous flux to radiant flux
Luminous efficacy (of a source)
η[nb 3]
lumen per watt
lm/W
M−1⋅L−2⋅T3⋅J
Ratio of luminous flux to power consumption
Luminous efficiency, luminous coefficient
V
1
Luminous efficacy normalized by the maximum possible efficacy
See also: SI · Photometry · Radiometry
^Standards organizations recommend that photometric quantities be denoted with a subscript "v" (for "visual") to avoid confusion with radiometric or photon quantities. For example: USA Standard Letter Symbols for Illuminating Engineering USAS Z7.1-1967, Y10.18-1967
^The symbols in this column denote dimensions; "L", "T" and "J" are for length, time and luminous intensity respectively, not the symbols for the units litre, tesla and joule.
^ abcAlternative symbols sometimes seen: W for luminous energy, P or F for luminous flux, and ρ for luminous efficacy of a source.
See also
Exposure value
Notes and references
^SI Derived Units, National Institute of Standards and Technology.
^NIST Guide to SI Units. Chapter 9 – Rules and Style Conventions for Spelling Unit Names, National Institute of Standards and Technology.
^ abcdeSchlyter, Paul (1997–2009). "Radiometry and photometry in astronomy". Starlight illuminance coincides with the human eye's minimum illuminance while moonlight coincides with the human eye's minimum colour vision illuminance (IEE Reviews, 1972, page 1183).
^Kyba, Christopher C. M.; Mohar, Andrej; Posch, Thomas (1 February 2017). "How bright is moonlight?". Astronomy & Geophysics. 58 (1): 1.31–1.32. doi:10.1093/astrogeo/atx025.
^"Electro-Optics Handbook" (pdf). photonis.com. p. 63. Retrieved 2012-04-02.[dead link]
^"NOAO Commen and Recommended Light Levels Indoor" (PDF).
^ abPears, Alan (June 1998). "Chapter 7: Appliance technologies and scope for emission reduction". Strategic Study of Household Energy and Greenhouse Issues(PDF). Sustainable Solutions Pty Ltd. Department of Industry and Science, Commonwealth of Australia. p. 61. Archived from the original (pdf) on 2 March 2011. Retrieved 2008-06-26.
^Australian Greenhouse Office (May 2005). "Chapter 5: Assessing lighting savings". Working Energy Resource and Training Kit: Lighting. Archived from the original on 2007-04-15. Retrieved 2007-03-17.
^"Low-Light Performance Calculator".
^Darlington, Paul (5 December 2017). "London Underground: Keeping the lights on". Rail Engineer. Retrieved 20 December 2017.
^"How to use a lux meter (Australian recommendation)" (PDF). Sustainability Victoria (sustainability.vic.gov.au). April 2010. Archived from the original (pdf) on 7 July 2011. External link in |publisher= (help)
^"Illumination. - 1926.56". Regulations (Standards - 29 CFR). Occupational Safety and Health Administration, US Dept. of Labor. Archived from the original on 8 May 2009.
^European law UNI EN 12464
^ abSchlyter, Section 7.
^Schlyter, Section 14.
^Jack L. Lindsey, Applied Illumination Engineering, The Fairmont Press, Inc., 1997 ISBN 0881732125 page 218
External links
Radiometry and photometry FAQ Professor Jim Palmer's Radiometry FAQ page (University of Arizona).
v
t
e
SI units
Base units
ampere
candela
kelvin
kilogram
metre
mole
second
Derived units with special names
becquerel
coulomb
degree Celsius
farad
gray
henry
hertz
joule
katal
lumen
lux
newton
ohm
pascal
radian
siemens
sievert
steradian
tesla
volt
watt
weber
Other accepted units
astronomical unit
dalton
day
decibel
degree of arc
electronvolt
hectare
hour
litre
minute
minute and second of arc
neper
tonne
See also
Conversion of units
Metric prefixes
2005–2019 definition
2019 redefinition
Systems of measurement
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Category
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