View source for Light meter

{{short description|Device used to measure the amount of light}}
{{more citations needed|date=September 2012}}
[[File:Erkan Umut shoots Sibel Can.jpg|thumb|Use of a light meter for portrait cinematography in a Turkish music video set]]

A '''light meter''' (or '''illuminometer''') is a device used to measure the amount of light. In [[photography]], an '''exposure meter''' is a light meter coupled to either a [[Digital data|digital]] or analog calculator which displays the correct [[shutter speed]] and [[f-number]] for optimum [[exposure (photography)|exposure]], given a certain lighting situation and [[film speed]]. Similarly, exposure meters are also used in the fields of [[cinematography]] and [[scenic design]], in order to determine the optimum light level for a scene.

Light meters also are used in the general field of [[architectural lighting design]] to verify proper installation and performance of a building lighting system, and in assessing the light levels for growing plants.

If a light meter is giving its indications in [[lux]]es, it is called a "'''luxmeter'''".<ref>[https://www.merriam-webster.com/dictionary/luxmeter Merriam-Webster Dictionary - luxmeter]</ref>

== Evolution ==
<gallery mode="packed" heights="120px" widths="160px" caption="Photographic exposure meters">
File:Watkins Bee Meter.jpg|Watkins Bee Meter - a type of actinometer
File:Leudi extinction meter.jpg|Leudi extinction meter<ref>{{cite web |url=http://www.earlyphotography.co.uk/site/entry_E20.html |title=Leudi, 1934 |website=Early Photography |access-date=8 September 2023}}</ref>
File:METROPHOT.jpg|Metrophot
Norwood Director IMG20240628134530.jpg|Norwood Director <br />Model No. 56646
Norwood Director Pat56646 IMG20240628134530.jpg|Norwood Director<br /> Pat. 2,214,238
File:SEKONIC TWINMATE L208.jpg|Sekonic "Twinmate" L208
File:KODALUX.jpg|Kodalux
File:TESSINA METER.jpg|Tessina Meter
File:Voigtlander VC METER.jpg|Voigtlander VC Meter
File:LEICA IIIC WITH VOIGTLANDER VC METER II.jpg|Leica IIIC with Voigtlander VC Meter II
File:Sekonic L-358 Flash Master.jpg|alt=A handheld digital light meter showing an exposure of {{frac|200}}th at an aperture of {{f/|11}}, at ISO 100. The light sensor is on top, under the white diffusing hemisphere|Sekonic L-358 "Flash Master"
</gallery>

===Actinometers===
[[File:Watkins Standard Exposure Meter.jpg|thumb|Watkins Standard Exposure Meter - a type of actinometer]]
The earliest exposure meters were called ''actinometers'' (not to be confused with the [[Actinometer|scientific instrument with the same name]]), described as early as 1840<ref name=Clerc70>{{cite book |url=https://archive.org/details/photographytheor0000cler |title=Photography: Theory and Practice |last1=Clerc |first1=Louis-Philippe |last2=Mannheim |first2=L.A. |editor1-last=Spencer |editor1-first=D.A. |volume=3: Films {{!}} Subject and Exposure |date=1970 |publisher=Focal Press |edition=Completely revised |isbn=0-240-50706-1 |url-access=registration}}</ref>{{rp|415}} but developed in the late 1800s after commercial [[photographic plate]]s became available with consistent sensitivity. These photographic actinometers used light-sensitive paper; the photographer would measure the time required for the paper to darken to a control value, providing an input to a mechanical calculation of shutter speed and aperture for a given plate number.<ref name=Secret-Exposure/>{{rp|69}} They were popular between approximately 1890 and 1920.<ref name=EP-meters/>

===Extinction types===
[[File:Dremo Light Meter (1931) (15494003563).jpg|thumb|right|upright|Dremo extinction meter<ref>{{cite web |url=http://www.earlyphotography.co.uk/site/entry_E277.html |title=Dremo, 1931 |website=Early Photography |access-date=8 September 2023}}</ref>]]
The next exposure meters, developed at about the same time<ref name=Clerc70/>{{rp|415}} but not displacing actinometers in popularity until the 1920s and 1930s, are known as ''[[Complex index of refraction|extinction]] meters'', evaluating the correct exposure settings by variable attenuation.<ref name=EP-meters>{{cite web |url=http://www.earlyphotography.co.uk/site/meters.html |title=Exposure Meters |website=Early Photography |access-date=8 September 2023}}</ref> One type of extinction meter contained a numbered or lettered row of [[neutral density filter]]s of increasing density. The photographer would position the meter in front of their subject and note the filter with the greatest density that still allowed incident light to pass through. In another example, sold as Heyde's Aktino-Photometer starting from the early 1900s, the photographer views the scene through an [[eyepiece]] and turns the meter to vary the effective density until the scene can no longer be seen.<ref>{{cite web |url=http://www.earlyphotography.co.uk/site/entry_E3.html |title=Heyde Aktino-Photometer, 1904 |website=Early Photography |access-date=8 September 2023}}</ref> The letter or number corresponding to the filter strength causing the "extinction" of the scene was used as an index into a chart of appropriate aperture and shutter speed combinations for a given [[film speed]].<ref name=Secret-Exposure>{{cite book |url=https://archive.org/details/secretofexposure00fraprich/page/72/mode/2up |title=The Secret of Exposure |series=Practical Photography |volume=1 |editor=Fraprie, Frank R. |date=1915 |publisher=American Photographic Publishing Company |location=Boston, Massachusetts |quote=In [the Heyde] instrument, blue-glass prisms are used to cut out the light reflected from the object. One looks through the eyepiece and turns the thicker portion of the prisms (one or both, according to the luminosity of the object) into position until the shadow details are suppressed. By reference to Tables, the necessary exposure may readily be found. |access-date=8 September 2023}}</ref>{{rp|72}}

Extinction meters tended to provide inconsistent results because they depended on subjective interpretation and the [[Luminosity function|light sensitivity of the human eye]], which can vary from person to person.<ref>{{cite book |url=https://archive.org/details/exposuremanual0000dunn/ |title=Exposure Manual |chapter-url=https://archive.org/details/exposuremanual0000dunn/page/82/mode/2up |chapter=3: Extinction Meters |author1=Dunn, Jack F. |author2=Wakefield, George L. |edition=Third |date=1974 |publisher=Fountain Press |location=Hertfordshire, England |isbn=0-85242-361-6 |pages=82–86 |url-access=registration |access-date=8 September 2023}}</ref>

===Photoelectric types===
[[File:Gossen Lunasix 3 front.jpg|thumb|upright|Gossen Lunasix 3 (in US: Luna Pro S) using {{chem|Cd|S|link=Cadmium sulfide}} photoresistor with analog readout; available from 1961 to 1977]]
Starting in 1932,<ref>{{cite book |url=https://archive.org/details/guideperfectexpo0000unse/page/20/mode/2up |title=Guide to Perfect Exposure |first1=George B. |last1=Wright |first2=Cora |last2=Wright |edition=Fourth |publisher=Chilton Book Company |location=Philadelphia |date=1967 |url-access=registration |lccn=67-17795}}</ref>{{rp|20}} electronic light meters removed the human element and relied on technologies incorporating (in chronological order) [[selenium]], [[Cadmium sulfide|CdS]] (1960s), and silicon ([[semiconductor]], 1970s) [[photodetector]]s.<ref name=Dunn-Wakefield-ch4>{{cite book |url=https://archive.org/details/exposuremanual0000dunn/ |title=Exposure Manual |chapter-url=https://archive.org/details/exposuremanual0000dunn/page/86/mode/2up |chapter=4: Photoelectric Reflected-light Meters |author1=Dunn, Jack F. |author2=Wakefield, George L. |edition=Third |date=1974 |publisher=Fountain Press |location=Hertfordshire, England |isbn=0-85242-361-6 |pages=87–121 |url-access=registration |access-date=8 September 2023}}</ref> Most modern light meters use silicon sensors.<ref name=Hicks99>{{cite book |url=https://archive.org/details/perfectexposuref0000hick/ |chapter-url=https://archive.org/details/perfectexposuref0000hick/page/88/mode/2up |title=Perfect exposure: from theory to practice |chapter=7: Exposure Meters |last1=Hicks |first1=Roger |last2=Schultz |first2=Frances |date=1999 |pages=88–103 |publisher=David & Charles |isbn=0-7153-0814-9 |url-access=registration}}</ref>{{rp|91}} They indicate the exposure either with a needle [[galvanometer]] or on an [[LCD]] screen.

Selenium light meters use sensors that are [[photovoltaic]]: they ''generate'' a voltage proportional to light exposure. Selenium sensors generate enough voltage for direct connection to a meter; they need no battery to operate and this made them very convenient in completely mechanical cameras.<ref name=Clerc70/>{{rp|416}}<ref name=Dunn-Wakefield-ch4/>{{rp|87–88}} Selenium sensors however cannot measure low light accurately (ordinary lightbulbs can take them close to their limits) and are altogether unable to measure very low light, such as candlelight, moonlight, starlight etc.<ref name=Focal78/>{{rp|56}}

CdS light meters use a [[photoresistor]] sensor whose electrical resistance decreases proportionately to the intensity of light exposure. These require a battery to operate,<ref name=Dunn-Wakefield-ch4/>{{rp|89–90}} but are significantly more sensitive to low light, able to detect lighting levels approximately {{frac|100}} of the lower sensitivity limit of selenium cells.<ref name=Clerc70/>{{rp|417}} However, CdS sensors fell out of favor due to their slower response and extended sensitivity to red and infrared wavelengths.<ref name=Clerc70/>{{rp|417}}<ref name=Focal78/>{{rp|58}}

Semiconductor sensors are also photovoltaic, but the voltage generated is much weaker than selenium cells and semiconductor-based light meters need an amplification circuit and therefore require a power source such as [[battery (electricity)|batteries]] to operate. These are usually named after the materials and filtration used to ensure the spectral response is similar to the human eye or [[photographic film]], such as '[[Silicon]] Blue Cell' (SBC) or '{{chem|Ga|As|link=Gallium arsenide}}'.<ref name=Focal78>{{cite book |url=https://archive.org/details/focalguidetoexpo0000lync/ |title=The Focalguide to exposure |first=David |last=Lynch |date=1978 |publisher=Focal Press |isbn=0-8038-2364-9 |url-access=registration}}</ref>{{rp|59}}

[[File:Autoexpmeter.JPG|thumb|left|An automatic light meter/exposure unit from an [[8mm film|8 mm]] [[movie camera]], based on a galvanometer mechanism (center) and a [[Cadmium sulfide|CdS]] [[photoresistor]], in opening at left.]]
Many modern consumer still and video [[camera]]s include a built-in meter that measures a scene-wide light level and are able to make an approximate measure of appropriate exposure based on that. Photographers working with controlled lighting and [[cinematographer]]s use handheld light meters to precisely measure the light falling on various parts of their subjects and use suitable lighting to produce the desired exposure levels.

===Reflected and incident measurements===
Exposure meters generally are sorted into reflected-light or incident-light types, depending on the method used to measure the scene.

'''Reflected-light meters''' measure the light ''reflected by the scene'' to be photographed.<ref name=Dunn-Wakefield-ch4/> All in-camera meters are reflected-light meters. Reflected-light meters are calibrated to show the appropriate exposure for "average" scenes.<ref name=Focal78/>{{rp|74}} An unusual scene with a preponderance of light colors or specular highlights would have a higher reflectance; a reflected-light meter taking a reading would incorrectly compensate for the difference in [[reflectance]] and lead to underexposure.  Badly underexposed sunset photos are common exactly because of this effect: the brightness of the setting sun fools the camera's light meter and, unless the in-camera logic or the photographer take care to compensate, the picture will be grossly underexposed and dull.

[[File:Sekonic L 398.jpg|thumb|left|upright|Sekonic L-398, with opalescent incident light-integrating dome]]
This pitfall (but not in the setting-sun case) is avoided by '''incident-light meters''' which measure the amount of light ''falling on the subject'' using a diffuser with a flat or (more commonly) hemispherical field of view placed on top of the light sensor.<ref name=Dunn-Wakefield-ch5>{{cite book |url=https://archive.org/details/exposuremanual0000dunn/ |title=Exposure Manual |chapter-url=https://archive.org/details/exposuremanual0000dunn/page/122/mode/2up |chapter=5: Photoelectric Incident-light Meters and Attachments |author1=Dunn, Jack F. |author2=Wakefield, George L. |edition=Third |date=1974 |publisher=Fountain Press |location=Hertfordshire, England |isbn=0-85242-361-6 |pages=122–140 |url-access=registration |access-date=8 September 2023}}</ref> Because the incident-light reading is independent of the subject's reflectance, it is less likely to lead to incorrect exposures for subjects with unusual average reflectance. Taking an incident-light reading requires placing the meter at the subject's position and pointing it in the general direction of the camera, something not always achievable in practice, e.g., in [[landscape photography]] where the subject distance approaches infinity.

[[File:Asahi Pentax Digital Spotmeter, against color chart (Pcs34560).jpg|thumb|right|upright|Pentax Digital Spotmeter]]
Another way to avoid under- or over-exposure for subjects with unusual reflectance is to use a '''spot meter''': a specialized reflected-light meter that measures light in a very tight [[Elliptical cone|cone]], typically with a one degree circular [[Angle of view#Calculating a camera's angle of view|angle of view]].<ref name=Dunn-Wakefield-ch6>{{cite book |url=https://archive.org/details/exposuremanual0000dunn/ |title=Exposure Manual |chapter-url=https://archive.org/details/exposuremanual0000dunn/page/140/mode/2up |chapter=6: Exposure Photometers |author1=Dunn, Jack F. |author2=Wakefield, George L. |edition=Third |date=1974 |publisher=Fountain Press |location=Hertfordshire, England |isbn=0-85242-361-6 |pages=141–177 |url-access=registration |access-date=8 September 2023}}</ref> An experienced photographer can take multiple readings over the shadows, midrange, and highlights of the scene to determine optimal exposure, using systems like the [[Zone System]].<ref name=Hicks99/>{{rp|102;126}}

Many modern cameras include sophisticated [[Metering mode#Multi-zone metering|multi-segment metering]] systems that measure the [[luminance]] of different parts of the scene to determine the optimal exposure.<ref name=Hicks99/>{{rp|102}} When using a film whose spectral sensitivity is not a good match to that of the light meter, for example [[orthochromatic]] [[Black and White Photography|black-and-white]] or infrared film, the meter may require special filters and re-calibration to match the sensitivity of the film.<ref name=Hicks99/>{{rp|89–92}}

[[File:Gossen-variosix hg.jpg|thumb|left|upright|Gossen Variosix (Luna-Star) F, capable of reflected, incident, and flash measurements]]
There are other types of specialized photographic light meters. Flash meters are used in flash photography to verify correct exposure. Color meters are used where high fidelity in color reproduction is required. [[Densitometer]]s are used in photographic reproduction.

==Exposure meter calibration==

In most cases, an incident-light meter will cause a medium tone to be recorded as a medium tone, and a reflected-light meter will cause ''whatever is metered'' to be recorded as a medium tone.  What constitutes a "medium tone" depends on meter calibration and several other factors, including film processing or [[digital image]] conversion.

Meter calibration establishes the relationship between subject lighting and recommended camera settings. The calibration of photographic light meters is covered by [[#CITEREF ISO2720:1974|ISO 2720:1974]].

===Exposure equations===

For reflected-light meters, camera settings are related to ISO speed and subject luminance by the reflected-light exposure equation:

<math>
\frac {N^2} {t} = \frac {L S} {K}
</math>

where

* <math>N</math> is the relative [[aperture]] ([[f-number]])
* <math>t</math> is the exposure time ("[[shutter speed]]") in seconds
* <math>L</math> is the average scene [[luminance]]
* <math>S</math> is the ISO arithmetic [[film speed|speed]]
* <math>K</math> is the reflected-light meter calibration constant

For incident-light meters, camera settings are related to ISO speed and subject illuminance by the incident-light exposure equation:

:<math>
\frac {N^2} {t} = \frac {E S} {C}
</math>

where

* <math>E</math> is the [[illuminance]]
* <math>C</math> is the incident-light meter calibration constant

===Calibration constants===<!-- This section is linked from [[Exposure value]] -->

Determination of calibration constants has been largely subjective; [[#CITEREF ISO2720:1974|ISO 2720:1974]] states that

<blockquote>
The constants <math>K</math> and <math>C</math> shall be chosen by statistical analysis of the results of a large number of tests carried out to determine the acceptability to a large number of observers, of a number
of photographs, for which the exposure was known, obtained under various conditions of subject manner and over a range of luminances.
</blockquote>

In practice, the variation of the calibration constants among manufacturers is considerably less than this statement might imply, and values have changed little since the early 1970s.

[[#CITEREF ISO2720:1974|ISO 2720:1974]] recommends a range for <math>K</math> of 10.6 to 13.4 with
luminance in cd/m<sup>2</sup>.  Two values for <math>K</math> are in common use: 12.5 ([[Canon Inc.|Canon]], [[Nikon]], and
[[Sekonic]]<ref>Specifications for Sekonic light meters are available on the [http://www.sekonic.com/ Sekonic] web site under "Products."</ref>) and 14 ([[Minolta]],<ref name="KM_2006" /> [[Kenko (company)|Kenko]],<ref name="KM_2006">[[Konica Minolta]] Photo Imaging, Inc. left the camera business on March 31, 2006. Rights and tooling for Minolta exposure meters were acquired by Kenko Co, Ltd. in 2007.
Specifications for the Kenko meters are essentially the same as for the equivalent Minolta meters.</ref> and [[Pentax]]); the difference between the two values is approximately {{frac|6}} [[Exposure value|EV]].

The earliest calibration standards were developed for use with wide-angle averaging reflected-light meters
([[#CITEREF JonesCondit1941|Jones and Condit 1941]]).  Although wide-angle average metering has largely given way to other metering sensitivity patterns (e.g., spot, center-weighted, and multi-segment), the values for <math>K</math> determined for wide-angle averaging meters have remained.

The incident-light calibration constant depends on the type of light receptor.  Two receptor types are common: flat ([[cosine]]-responding) and hemispherical ([[cardioid]]-responding).  With a flat receptor, [[#CITEREF ISO2720:1974|ISO 2720:1974]] recommends a range for <math>C</math> of 240 to 400 with illuminance in [[lux]]; a value of 250 is commonly used.  A flat receptor typically is used for measurement of lighting ratios, for measurement of illuminance, and occasionally, for determining exposure for a flat subject.

For determining practical photographic exposure, a hemispherical receptor has proven more effective. [[Don Norwood]], inventor of incident-light exposure meter with a hemispherical receptor, thought that a sphere was a reasonable representation of a photographic subject. According to his patent ([[#CITEREF Norwood1938|Norwood 1938]]), the objective was

<blockquote>
to provide an exposure meter which is substantially uniformly responsive to light incident upon the photographic subject from practically all directions which would result in the reflection of light to the camera or other photographic register.
</blockquote>

and the meter provided for "measurement of the effective illumination obtaining at the position of the subject."

With a hemispherical receptor, [[#CITEREF ISO2720:1974|ISO 2720:1974]] recommends a range for <math>C</math> of 320 to 540 with illuminance in lux; in practice, values typically are between 320 (Minolta) and 340 (Sekonic).  The relative responses of flat and hemispherical receptors depend upon the number and type of light sources; when each receptor is pointed at a small light source, a hemispherical receptor with <math>C</math> = 330 will indicate an exposure approximately 0.40 step greater than that indicated by a flat receptor with <math>C</math> = 250.  With a slightly revised definition of illuminance, measurements with a hemispherical receptor indicate "effective scene illuminance."

===Calibrated reflectance===

It is commonly stated that reflected-light meters are calibrated to an 18% reflectance,<ref> Some authors ([[#CITEREF Ctein1997|Ctein 1997]], 29) have argued that the calibrated reflectance is closer to 12% than to 18%. </ref> but the calibration has nothing to do with reflectance, as should be evident from the exposure formulas.  However, some notion of reflectance is implied by a comparison of incident- and reflected-light meter calibration.

Combining the reflected-light and incident-light exposure equations and rearranging gives

:<math>\frac {L} {E} = \frac {K} {C}</math>

[[Reflectance]] <math>R</math> is defined as

:<math>R = \frac {\mbox {flux emitted from surface}} {\mbox {flux incident upon surface}}</math>

A uniform perfect diffuser (one following [[Lambert's cosine law]]) of luminance <math>L</math> emits a flux density of <math>\pi</math><math>L</math>; reflectance then is

:<math>R = \frac {\pi L} {E} = \frac {\pi K} {C}</math>

Illuminance is measured with a flat receptor.  It is straightforward to compare an incident-light measurement using a flat receptor with a reflected-light measurement of a uniformly illuminated flat surface of constant reflectance.  Using values of 12.5 for <math>K</math> and 250 for <math>C</math> gives

:<math>R = \frac {\pi \times 12.5} {250} \approx 15.7\%</math>

With a <math>K</math> of 14, the reflectance would be 17.6%, close to that of a standard 18% neutral test card.  In theory, an incident-light measurement should agree with a reflected-light measurement of a test card of suitable reflectance that is perpendicular to the direction to the meter.  However, a test card seldom is a uniform diffuser, so incident- and reflected-light measurements might differ slightly.

In a typical scene, many elements are not flat and are at various orientations to the camera, so that for practical photography, a hemispherical receptor usually has proven more effective for determining exposure.  Using values of 12.5 for <math>K</math> and 330 for <math>C</math> gives

:<math>R = \frac {\pi \times 12.5} {330} \approx 11.9\%</math>

With a slightly revised definition of reflectance, this result can be taken as indicating that the average scene reflectance is approximately 12%.  A typical scene includes shaded areas as well as areas that receive direct illumination, and a wide-angle averaging reflected-light meter responds to these differences in illumination as well as differing reflectances of various scene elements. Average scene reflectance then would be

:<math>\mbox{average scene reflectance} =
\frac {\mbox {average scene luminance} } {\mbox {effective scene illuminance }}
</math>

where "effective scene illuminance" is that measured by a meter with a hemispherical receptor.

[[#CITEREF ISO2720:1974|ISO 2720:1974]] calls for reflected-light calibration to be measured by aiming the receptor at a transilluminated diffuse surface, and for incident-light calibration to be measured by aiming the receptor at a point source in a darkened room.  For a perfectly diffusing test card and perfectly diffusing flat receptor, the comparison between a reflected-light measurement and an incident-light measurement is valid for any position of the light source.  However, the response of a hemispherical receptor to an off-axis light source is approximately that of a [[cardioid]] rather than a [[cosine]], so the 12% "reflectance" determined for an incident-light meter with a hemispherical receptor is valid only when the light source is on the receptor axis.

===Cameras with internal meters===

Calibration of cameras with internal meters is covered by [[#CITEREF ISO2721:1982|ISO 2721:1982]]; nonetheless, many manufacturers specify (though seldom state) exposure calibration in terms of <math>K</math>, and many calibration instruments (e.g., Kyoritsu-Arrowin multi-function camera testers<ref>Specifications for Kyoritsu testers are available on the [http://www.criscam.com/ C.R.I.S. Camera Services] web site under "kyoritsu test equipment."</ref> ) use the specified <math>K</math> to set the test parameters.

==Exposure determination with a neutral test card==

If a scene differs considerably from a statistically average scene, a wide-angle averaging reflected-light measurement may not indicate the correct exposure.  To simulate an average scene, a substitute measurement sometimes is made of a neutral test card, or ''[[gray card]]''.

At best, a flat card is an approximation to a three-dimensional scene, and measurement of a test card may lead to underexposure unless adjustment is made. The instructions for a Kodak neutral test card recommend that the indicated exposure be increased by {{frac|1|2}} step for a frontlighted scene in sunlight.  The instructions also recommend that the test card be held vertically and faced in a direction midway between the Sun and the camera; similar directions are also given in the ''Kodak Professional Photoguide''. The combination of exposure increase and the card orientation gives recommended exposures that are reasonably close to those given by an incident-light meter with a hemispherical receptor when metering with an off-axis light source.

In practice, additional complications may arise.  Many neutral test cards are far from perfectly diffuse reflectors, and specular reflections can cause increased reflected-light meter readings that, if followed, would result in underexposure.  It is possible that the neutral test card instructions include a correction for specular reflections.

==Use in illumination==

Light meters or light detectors are also used in [[Lighting|illumination]]. Their purpose is to measure the illumination level in the interior and to switch off or reduce the output level of [[luminaire]]s. This can greatly reduce the energy burden of the building by significantly increasing the efficiency of its lighting system. It is therefore recommended to use light meters in lighting systems, especially in rooms where one cannot expect users to pay attention to manually switching off the lights. Examples include hallways, stairs, and big halls.

There are, however, significant obstacles to overcome in order to achieve a successful implementation of light meters in lighting systems, of which user acceptance is by far the most formidable. Unexpected or too frequent switching and too bright or too dark rooms are very annoying and disturbing for users of the rooms. Therefore, different switching algorithms have been developed:
*difference algorithm, where lights are switched on at a lower light level than they switch off, thus taking ensuring the difference between the light level of the 'on' state and 'off' state is not too big
*time delay algorithms:
**a certain amount of time must pass since the last switch
**a certain amount of time at a sufficient illumination level must pass.

== Other uses ==

In Scientific Research & Development uses, a light meter consists of a [[radiometer]] (the electronics/readout), a photo-diode or sensor (generates an output when exposed to electromagnetic radiation/light) a filter (used to modify the incoming light so only the desired portion of incoming radiation reaches the sensor) and a cosine correcting input optic (assures the sensor can see the light coming in from all directions accurately).

When the word light meter or photometer is used in place of radiometer or optometer, or it is often assumed the system was configured to see only visible light. Visible light sensors are often called illuminance or photometric sensors because they have been filtered to be sensitive only to 400-700 nanometers (nm) mimicking the human eyes' sensitivity to light. How accurately the meter measures often depends on how well the filtration matches the human eyes' response.

The sensor will send a signal to the meter that is proportional to the amount of light that reaches the sensor after being collected by the optics and passing through the filter. The meter then converts the incoming signal (typically current or voltage) from the sensor into a reading of calibrated units such as Foot-Candles (fc) or Lux (lm/m^2). Calibration in fc or lux, is the second most important feature of a light meter. It not only converts the signal from V or mA, but it also provides accuracy and unit to unit repeatability. [[National Institute of Standards and Technology]] (NIST) traceability and [[ISO/IEC 17025]] accreditation are two well known terms that verify the system includes a valid calibration.

The meter/radiometer/photometer portion may have many features including:

'''Zero:''' subtracts ambient/background light levels, or stabilize the meter to the working environment

'''Hold:''' freezes the value on the display.

'''Range:''' for systems that are not linear and auto ranging this function allows the user to select the portion of the meter electronics that best handles the signal level in use.

'''Units:''' For illuminance the units are typically only lux and foot-candles but many light meters can also be used for UV, VIS and IR applications so the readout could change to W/cm^2, candela, Watts etc.

'''Integrate:''' sums up the values into a dose or exposure level i.e. lux*sec or J/cm^2.

Along with having a variety of features, a light meter may also be usable for a variety of applications. These may include the measurement of other bands of light such UVA, UVB, UVC and Near IR.  For example, UVA and UVB light meters are used for phototherapy or treatment of skin conditions, germicidal radiometers are used for measuring the UVC level from lamps used for disinfection and sterilization, luminance meters are used to measure the brightness of a sign, display or exit sign, PAR quantum sensors are used to measure how much of a given light source's emission will help plants grow, and UV-curing radiometers test how much of the lights emission is effective for hardening a glue, plastic, or protective coating.
  
Some light meters also have the ability to provide a readout in many different units.  Lux and footcandles are the common units for visible light, but so are Candelas, Lumens, and Candela per square meter.  In the realm of disinfection, UVC is typically measured in watts per square centimeter, or watts for a given individual lamp assembly, whereas systems used in the context of the curing of coatings often provide readouts in Joules per Square centimeter.  Regular measurements of UVC light intensity thus can serve to provide assurance of proper disinfection of water and food-preparation surfaces, or reliable coating hardness in painted products.
  
Although a light meter can take the form of a very simple handheld tool with one-button operation, there are also many advanced light-measurement systems available for use in numerous different applications.  These can be incorporated into automated systems that can, for example, wipe lamps clean when a certain reduction in output is detected, or that can trigger an alarm when lamp-failure occurs.

==See also==
{{Commons category|Light meters}}
* [[Selenium meter]]
* [[Photometer]] | [[Photodetector]]
* [[Colorimetry]] | [[Photometry (optics)|Photometry]] | [[Radiometry]]
* [[Light value]]
* [[Photomultiplier]] tubes for detecting light at very low levels.
* [[PIN diode]] solid state electronic devices for detecting incident light.

==References==

{{reflist}}

===Bibliography===

* <span id="CITEREF_Ctein1997">Ctein. 1997. ''Post Exposure: Advanced Techniques for the Photographic Printer''. Boston: [http://www.focalpress.com Focal Press]</span>. {{ISBN|0-240-80299-3}}.
* Eastman Kodak Company. Instructions for Kodak Neutral Test Card, 453-1-78-ABX. Rochester: Eastman Kodak Company.
* Eastman Kodak Company. 1992. ''Kodak Professional Photoguide''. Kodak publication no. R-28. Rochester: Eastman Kodak Company.
* <span id="CITEREF_ISO2720:1974"> [http://www.iso.org/iso/en/CatalogueDetailPage.CatalogueDetail?CSNUMBER=7690 ISO 2720:1974]. ''General Purpose Photographic Exposure Meters (Photoelectric Type) — Guide to Product Specification''. International Organization for Standardization</span>.
* <span id="CITEREF_ISO2721:2013"> [http://www.iso.org/iso/home/store/catalogue_tc/catalogue_detail.htm?csnumber=62742 ISO 2721:2013]. ''Photography&nbsp;—&nbsp;Film-based cameras&nbsp;—&nbsp;Automatic controls of exposure''. International Organization for Standardization</span>.
* <span id="CITEREF_JonesCondit1941">Jones, Loyd A., and H. R. Condit. 1941. The Brightness Scale of Exterior Scenes and the Correct Computation of Photographic Exposure. ''Journal of the Optical Society of America''. 31:651–678</span>.
* <span id="CITEREF_Norwood1938">{{cite patent |country=US |number=2214283 |status=Patent |inventor=Donald W. Norwood |title=Exposure Meter |fdate=14 November 1938 |pubdate=10 September 1940}}</span>.

==External links==
* [http://www.otc.co.uk/Problem_With_Lux_Meters.php The Problem with Lux Meters] An article suggesting that Lux meter may read incorrectly when measuring light not from a tungsten source (i.e. fluorescent, metal halide, sodium, LED and other types).
* [http://www.largeformatphotography.info/articles/conrad-meter-cal.pdf Exposure Metering: Relating Subject Lighting to Film Exposure] ([[PDF]]) A discussion of meter calibration and its practical effects.
* [http://jimsphoto.yolasite.com/resources/Using%20a%20Gray%20Card.pdf Estimating Luminance and Illuminance] ([[PDF]]) A Kodak guide to using a camera's exposure meter.
* [https://www.intl-lighttech.com/basic-light-measurement-principles-chapter-6-light-measurement-tutorial Basic Light Measurement Principles] An article from International Light Technologies on basic principles

[[Category:Photography equipment]]
[[Category:Electromagnetic radiation meters]]
[[Category:Lighting]]