Exposure value

In photography, exposure value (EV) is a number that represents a combination of a camera's shutter speed and f-number, such that all combinations that yield the same exposure have the same EV (for any fixed scene luminance). Exposure value is also used to indicate an interval on the photographic exposure scale, with a difference of 1 EV corresponding to a standard power-of-2 exposure step, commonly referred to as a stop.

The EV concept was developed by the German shutter manufacturer Friedrich Deckel in the 1950s (Gebele 1958; Ray 2000, 318). Its intent was to simplify choosing among equivalent camera exposure settings by replacing combinations of shutter speed and f-number (e.g., 1/125 s at ) with a single number (e.g., 15).

On some lenses with leaf shutters, the process was further simplified by allowing the shutter and aperture controls to be linked such that, when one was changed, the other was automatically adjusted to maintain the same exposure. This was especially helpful to beginners with limited understanding of the effects of shutter speed and aperture and the relationship between them. But it was also useful for experienced photographers who might choose a shutter speed to stop motion or an f-number for depth of field, because it allowed for faster adjustment—without the need for mental calculations—and reduced the chance of error when making the adjustment.

The concept became known as the Light Value System (LVS) in Europe; it was generally known as the Exposure Value System (EVS) when the features became available on cameras in the United States (Desfor 1957).

Because of mechanical considerations, the coupling of shutter and aperture was limited to lenses with leaf shutters; however, various automatic exposure modes now work to somewhat the same effect in cameras with focal-plane shutters.

The proper EV was determined by the scene luminance and film speed; it was intended that the system also include adjustment for filters, exposure compensation, and other variables. With all of these elements included, the camera would be set by transferring the single number thus determined.

Exposure value has been indicated in various ways. The ASA and ANSI standards used the quantity symbol Ev, with the subscript v indicating the logarithmic value; this symbol continues to be used in ISO standards, but the acronym EV is more common elsewhere. The Exif standard uses Ev (CIPA 2016).

Although all camera settings with the same EV nominally give the same exposure, they do not necessarily give the same picture. The f-number (relative aperture) determines the depth of field, and the shutter speed (exposure time) determines the amount of motion blur, as illustrated by the two images at the right (and at long exposure times, as a second-order effect, the light-sensitive medium may exhibit reciprocity failure, which is a change of light sensitivity dependent on the irradiance at the film).

Formal definition


Exposure value is a base-2 logarithmic scale defined by (Ray 2000, 318):


 * $$\mathrm {EV} = \log_2 {\frac {N^2} {t} } \,,$$

where


 * N is the f-number
 * t is the exposure time ("shutter speed") in seconds

EV 0 corresponds to an exposure time of 1 s and an aperture of. If the EV is known, it can be used to select combinations of exposure time and f-number, as shown in Table 1.

Each increment of 1 in exposure value corresponds to a change of one "step" (or, more commonly, one "stop") in exposure, i.e., half as much exposure, either by halving the exposure time or halving the aperture area, or a combination of such changes. Greater exposure values are appropriate for photography in more brightly lit situations, or for lower ISO speeds.

Alternate form:

$$EV=2\log_2(N)-\log_2(t)$$

Camera settings vs. luminous exposure


"Exposure value" indicates combinations of camera settings rather than the luminous exposure (aka photometric exposure), which is given by (Ray 2000, 310)


 * $$H = E t \,,$$

where


 * H is the luminous/photometric exposure (lux seconds)
 * E is the image-plane illuminance (lux or lumens/m²)
 * t is the exposure time ("shutter speed") (seconds)

The illuminance E is controlled by the f-number but also depends on the scene luminance. To avoid confusion, some authors (Ray 2000, 310) have used camera exposure to refer to combinations of camera settings. The 1964 ASA standard for automatic exposure controls for cameras, ASA PH2.15-1964, took the same approach, and also used the more descriptive term camera exposure settings.

Common practice among photographers is nonetheless to use "exposure" to refer to camera settings as well as to photometric exposure.

Relationship of camera settings to luminous exposure
The image-plane illuminance is directly proportional to the area of the aperture, and hence inversely proportional to the square of the lens f-number; thus


 * $$H \propto \frac {t} {N^2}\,;$$

for constant lighting conditions, the exposure is constant as long as the ratio t/N2 is constant. If, for example, the f-number is changed, an equivalent exposure time can be determined from


 * $$\frac {t_2} {t_1} = \frac {N_2^2} {N_1^2}\,.$$

Performing this calculation mentally is tedious for most photographers, but the equation is easily solved with a calculator dial on an exposure meter (Ray 2000, 318) or a similar dial on a standalone calculator. If the camera controls have detents, constant exposure can be maintained by counting the steps as one control is adjusted and counting an equivalent number of steps when adjusting the other control.

Representing camera settings: EV
The ratio t/N2 could be used to represent equivalent combinations of exposure time and f-number in a single value. But for many such combinations used in general photography, the ratio gives a fractional value with a large denominator; this is notationally inconvenient as well as difficult to remember. Inverting this ratio and taking the base-2 logarithm allows defining a quantity Ev such that


 * $$E_\mathrm v = \log_2 \frac {N^2} {t}\,,$$

resulting in a value that progresses in a linear sequence as camera exposure is changed in power-of-2 steps. For example, beginning with 1 s and, decreasing exposure

gives the simple sequence


 * 0, 1, 2, 3, ..., 14, 15, ...

The last two values shown frequently apply when using ISO 100 speed imaging media in outdoor photography.

This system provides its greatest benefit when using an exposure meter (or table) calibrated in EV with a camera that allows settings to be made in EV, especially with coupled shutter and aperture; the appropriate exposure is easily set on the camera, and choosing among equivalent settings is made by adjusting one control.

Current cameras do not allow direct setting of EV, and cameras with automatic exposure control generally obviate the need for it. EV can nonetheless be helpful when used to transfer recommended exposure settings from an exposure meter (or table of recommended exposures) to an exposure calculator (or table of camera settings).

EV as an indicator of camera settings
Used as an indicator of camera settings, EV corresponds to actual combinations of shutter speed and aperture setting. When the actual EV matches that recommended by the light level and the ISO speed, these settings should result in the "correct" exposure.



Relationship of EV to lighting conditions
"Correct" exposure is obtained when the f-number and exposure time match those "recommended" for given lighting conditions and ISO speed; the relationship is given by the exposure equation prescribed by ISO 2720:1974:

\frac {N^2} {t} = \frac {L S} {K} \,, $$

where


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

Applied to the right-hand side of the exposure equation, exposure value is


 * $$\mathrm {EV} = \log_2 {\frac {L S} {K} } \,.$$

If the common value of K = 12.5 (unit: cd s/m2 ISO) is used, an EV of zero (e.g., an aperture of and a shutter time of 1 sec) for ISO = 100 corresponds to a luminance of 0.125 cd/m2 (0.01 cd/ft2). At EV = 15 (the "sunny sixteen" amount of light) the luminance is 4096 cd/m2 (380 cd/ft2).

Camera settings also can be determined from incident-light measurements, for which the exposure equation is



\frac {N^2} {t} = \frac {E S} {C} \,, $$

where


 * E is the illuminance in lux or lumens/m²
 * C is the incident-light meter calibration constant

In terms of exposure value, the right-hand side becomes


 * $$\mathrm {EV} = \log_2 {\frac {E S} {C} } \,.$$

When applied to the left-hand side of the exposure equation, EV denotes actual combinations of camera settings; when applied to the right-hand side, EV denotes combinations of camera settings required to give the nominally "correct" exposure. The formal relationship of EV to luminance or illuminance has limitations. Although it usually works well for typical outdoor scenes in daylight, it is less applicable to scenes with highly atypical luminance distributions, such as city skylines at night. In such situations, the EV that will result in the best picture often is better determined by subjective evaluation of photographs than by formal consideration of luminance or illuminance.

For a given luminance and film speed, a greater EV results in less exposure, and for fixed exposure (i.e., fixed camera settings), a greater EV corresponds to greater luminance or illuminance.

Illuminance is measured using a flat sensor; if the common value of C = 250 (unit: lux s ISO=lm s/m2 ISO) is used, an EV of zero (e.g., an aperture of and a shutter time of 1 sec) for ISO = 100 corresponds to an illuminance of  2.5 lux (0.23 fc). At EV = 15 (the "sunny sixteen" amount of light) the illuminance is 82,000 lux (7600 fc). For general photography, incident-light measurements are usually taken with a hemispherical sensor; the readings cannot be meaningfully related to illuminance.

Tabulated exposure values
An exposure meter may not always be available, and using a meter to determine exposure for some scenes with unusual lighting distribution may be difficult. However, natural light, as well as many scenes with artificial lighting, is predictable, so that exposure often can be determined with reasonable accuracy from tabulated values.




 * Table 2 . Exposure values (ISO 100) for various lighting conditions'''
 * {| class="wikitable" style="padding: 0.1em 0.5em; text-align: left"

! Lighting condition || EV100 ! colspan="2" | Daylight ! colspan="2" | Outdoor, natural light ! colspan="2" | Outdoor, artificial light ! colspan="2" | Indoor, artificial light
 * | Light sand or snow in full or slightly hazy sunlight (distinct shadows)a
 * style="text-align: center;" | 16
 * | Typical scene in full or slightly hazy sunlight (distinct shadows)a, b
 * style="text-align: center;" | 15
 * | Typical scene in hazy sunlight (soft shadows)
 * style="text-align: center;" | 14
 * | Typical scene, cloudy bright (no shadows)
 * style="text-align: center;" | 13
 * | Typical scene, heavy overcast
 * style="text-align: center;" | 12
 * | Areas in open shade, clear sunlight
 * style="text-align: center;" | 12
 * | Typical scene, heavy overcast
 * style="text-align: center;" | 12
 * | Areas in open shade, clear sunlight
 * style="text-align: center;" | 12
 * | Areas in open shade, clear sunlight
 * style="text-align: center;" | 12
 * colspan="2" | Rainbows
 * style="padding: 0.1em 1.5em;" | Clear sky background
 * style="text-align: center;" | 15
 * style="padding: 0.1em 1.5em;" | Cloudy sky background
 * style="text-align: center;" | 14
 * colspan="2" | Sunsets and skylines
 * style="padding: 0.1em 1.5em;" | Just before sunset
 * style="text-align: center;" | 12–14
 * style="padding: 0.1em 1.5em;" | At sunset
 * style="text-align: center;" | 12
 * style="padding: 0.1em 1.5em;" | Just after sunset
 * style="text-align: center;" | 9–11
 * colspan="2" | The Moon,c altitude > 40°
 * style="padding: 0.1em 1.5em;" | Full
 * style="text-align: center;" | 15
 * style="padding: 0.1em 1.5em;" | Gibbous
 * style="text-align: center;" | 14
 * style="padding: 0.1em 1.5em;" | Quarter
 * style="text-align: center;" | 13
 * style="padding: 0.1em 1.5em;" | Crescent
 * style="text-align: center;" | 12
 * style="padding: 0.1em 1.5em;" | Blood
 * style="text-align: center;" | 0 to 3
 * colspan="2" | Moonlight, Moon altitude > 40°
 * style="padding: 0.1em 1.5em;" | Full
 * style="text-align: center;" | &minus;3 to &minus;2
 * style="padding: 0.1em 1.5em;" | Gibbous
 * style="text-align: center;" | &minus;4
 * style="padding: 0.1em 1.5em;" | Quarter
 * style="text-align: center;" | &minus;6
 * colspan="2" | Aurora borealis and australis
 * style="padding: 0.1em 1.5em;" | Bright
 * style="text-align: center;" | &minus;4 to &minus;3
 * style="padding: 0.1em 1.5em;" | Medium
 * style="text-align: center;" | &minus;6 to &minus;5
 * | Milky Way galactic center
 * style="text-align: center;" | &minus;11 to &minus;9
 * colspan="2" | Moonlight, Moon altitude > 40°
 * style="padding: 0.1em 1.5em;" | Full
 * style="text-align: center;" | &minus;3 to &minus;2
 * style="padding: 0.1em 1.5em;" | Gibbous
 * style="text-align: center;" | &minus;4
 * style="padding: 0.1em 1.5em;" | Quarter
 * style="text-align: center;" | &minus;6
 * colspan="2" | Aurora borealis and australis
 * style="padding: 0.1em 1.5em;" | Bright
 * style="text-align: center;" | &minus;4 to &minus;3
 * style="padding: 0.1em 1.5em;" | Medium
 * style="text-align: center;" | &minus;6 to &minus;5
 * | Milky Way galactic center
 * style="text-align: center;" | &minus;11 to &minus;9
 * style="text-align: center;" | &minus;4 to &minus;3
 * style="padding: 0.1em 1.5em;" | Medium
 * style="text-align: center;" | &minus;6 to &minus;5
 * | Milky Way galactic center
 * style="text-align: center;" | &minus;11 to &minus;9
 * | Milky Way galactic center
 * style="text-align: center;" | &minus;11 to &minus;9
 * | Neon and other bright signs
 * style="text-align: center;" | 9–10
 * | Night sports
 * style="text-align: center;" | 9
 * | Fires and burning buildings
 * style="text-align: center;" | 9
 * | Bright street scenes
 * style="text-align: center;" | 8
 * | Night street scenes and window displays
 * style="text-align: center;" | 7–8
 * | Night vehicle traffic
 * style="text-align: center;" | 5
 * | Fairs and amusement parks
 * style="text-align: center;" | 7
 * | Christmas tree lights
 * style="text-align: center;" | 4–5
 * | Floodlit buildings, monuments, and fountains
 * style="text-align: center;" | 3–5
 * | Distant views of lighted buildings
 * style="text-align: center;" | 2
 * style="text-align: center;" | 7
 * | Christmas tree lights
 * style="text-align: center;" | 4–5
 * | Floodlit buildings, monuments, and fountains
 * style="text-align: center;" | 3–5
 * | Distant views of lighted buildings
 * style="text-align: center;" | 2
 * | Distant views of lighted buildings
 * style="text-align: center;" | 2
 * style="text-align: center;" | 2
 * | Galleries
 * style="text-align: center;" | 8–11
 * | Sports events, stage shows, and the like
 * style="text-align: center;" | 8–9
 * | Circuses, floodlit
 * style="text-align: center;" | 8
 * | Ice shows, floodlit
 * style="text-align: center;" | 9
 * | Offices and work areas
 * style="text-align: center;" | 7–8
 * | Home interiors
 * style="text-align: center;" | 5–7
 * | Christmas tree lights
 * style="text-align: center;" | 4–5
 * }
 * | Home interiors
 * style="text-align: center;" | 5–7
 * | Christmas tree lights
 * style="text-align: center;" | 4–5
 * }
 * style="text-align: center;" | 4–5
 * }

Values for direct sunlight apply between approximately two hours after sunrise and two hours before sunset, and assume front lighting. As a rough general rule, decrease EV by 1 for side lighting, and decrease EV by 2 for back lighting. This is approximately the value given by the sunny 16 rule. These values are appropriate for pictures of the Moon taken at night with a long lens or telescope, and will render the Moon as a medium tone. They will not, in general, be suitable for landscape pictures that include the Moon. In a landscape photograph, the Moon typically is near the horizon, where its luminance changes considerably with altitude. Moreover, a landscape photograph usually must take account of the sky and foreground as well as the Moon. Consequently, it is nearly impossible to give a single correct exposure value for such a situation. 

Exposure values in Table 2 are reasonable general guidelines, but they should be used with caution. For simplicity, they are rounded to the nearest integer, and they omit numerous considerations described in the ANSI exposure guides from which they are derived. Moreover, they take no account of color shifts or reciprocity failure. Proper use of tabulated exposure values is explained in detail in the ANSI exposure guide, ANSI PH2.7-1986.

The exposure values in Table 2 are for ISO 100 speed ("EV100"). For a different ISO speed $$S$$, increase the exposure values (decrease the exposures) by the number of exposure steps by which that speed is greater than ISO 100, formally


 * $$\mathrm{EV}_{S} = \mathrm{EV}_{100} + \log_2 \frac {S} {100} \,.$$

For example, ISO 400 speed is two steps greater than ISO 100:


 * $$\mathrm{EV}_{400} = \mathrm{EV}_{100} + \log_2 \frac {400} {100}

= \mathrm{EV}_{100} + 2 \,.$$

To photograph outdoor night sports with an ISO 400–speed imaging medium, search Table 2 for "Night sports" (which has an EV of 9 for ISO 100), and add 2 to get EV400 = 11.

For lower ISO speed, decrease the exposure values (increase the exposures) by the number of exposure steps by which the speed is less than ISO 100. For example, ISO 50 speed is one step less than ISO 100:


 * $$\mathrm{EV}_{50} = \mathrm{EV}_{100} + \log_2 \frac {50} {100}

= \mathrm{EV}_{100} - 1 \,.$$

To photograph a rainbow against a cloudy sky with an ISO 50–speed imaging medium, search Table 2 for "Rainbows-Cloudy sky background" (which has an EV of 14), and subtract 1 to get EV50 = 13.

The equation for correcting for ISO speed can also be solved for EV100:


 * $$\mathrm{EV}_{100} = \mathrm{EV}_{S} - \log_2 \frac {S} {100} \,.$$

For example, using ISO 400 film and setting the camera for EV 11 allows shooting night sports at a light level of EV100 = 9, in agreement with the example done the other way around above. An online calculator that implemented this calculation was available at dpreview.com.

Setting EV on a camera


On most cameras, there is no direct way to transfer an EV to camera settings; however, a few cameras, such as some Voigtländer and Braun models or the Kodak Pony II shown in the photo, allowed direct setting of exposure value. Some medium-format cameras from Rollei (Rolleiflex, Rolleicord models) and Hasselblad allowed EV to be set on the lenses. The set EV could be locked, coupling shutter and aperture settings, such that adjusting either the shutter speed or aperture made a corresponding adjustment in the other to maintain a constant exposure (Ray 2000, 318). On some lenses the locking was optional, so that the photographer could choose the preferred method of working depending on the situation. Use of EV on some meters and cameras is discussed briefly by Adams (1981, 39). He notes that, in some cases, the EV indication from the meter may need to be adjusted for film speed.

Exposure compensation in EV
Many current cameras allow for exposure compensation, and usually state it in terms of EV (Ray 2000, 316). In this context, EV refers to the difference between the indicated and set exposures. For example, an exposure compensation of +1 EV (or +1 step) means to increase exposure, by using either a longer exposure time or a smaller f-number.

The sense of exposure compensation is opposite that of the EV scale itself. An increase in exposure corresponds to a decrease in EV, so an exposure compensation of +1 EV results in a smaller EV; conversely, an exposure compensation of −1 EV results in a greater EV. For example, if a meter reading of a lighter-than-normal subject indicates EV 16, and an exposure compensation of +1 EV is applied to render the subject appropriately, the final camera settings will correspond to EV 15.

Meter indication in EV
Some light meters (e.g., Pentax spot meters) indicate directly in EV at ISO 100. Some other meters, especially digital models, can indicate EV for the selected ISO speed. In most cases, this difference is irrelevant; with the Pentax meters, camera settings usually are determined using the exposure calculator, and most digital meters directly display shutter speeds and f-numbers.

Recently, articles on many web sites have used light value (LV) to denote EV at ISO 100. However, this term does not derive from a standards body, and has had several conflicting definitions.

EV and APEX
The Additive system of Photographic EXposure (APEX) proposed in the 1960 ASA standard for monochrome film speed, ASA PH2.5-1960, extended the concept of exposure value to all quantities in the exposure equation by taking base-2 logarithms, reducing application of the equation to simple addition and subtraction. In terms of exposure value, the left-hand side of the exposure equation became


 * $$E_v = A_v + T_v \,,$$

where Av (aperture value) and Tv (time value) were defined as:


 * $$A_v = \log_2 A^2$$

and


 * $$T_v = \log_2 (1/T) \,,$$

with


 * A the relative aperture (f-number)
 * T the exposure time ("shutter speed") in seconds

Av and Tv represent the numbers of stops from and 1 second, respectively.

Use of APEX required logarithmic markings on aperture and shutter controls, however, and these never were incorporated in consumer cameras. With the inclusion of built-in exposure meters in most cameras shortly after APEX was proposed, the need to use the exposure equation was eliminated, and APEX saw little actual use.

Though it remains of little interest to the end user, APEX has seen a partial resurrection in the Exif standard, which calls for storing exposure data using APEX values. See Use of APEX values in Exif for additional discussion.

EV as a measure of luminance and illuminance
For a given ISO speed and meter calibration constant, there is a direct relationship between exposure value and luminance (or illuminance). Strictly, EV is not a measure of luminance or illuminance; rather, an EV corresponds to a luminance (or illuminance) for which a camera with a given ISO speed would use the indicated EV to obtain the nominally correct exposure. Nonetheless, it is common practice among photographic equipment manufacturers to express luminance in EV for ISO 100 speed, as when specifying metering range (Ray 2000, 318) or autofocus sensitivity. And the practice is long established; (Ray 2002, 592) cites Ulffers (1968) as an early example. Properly, the meter calibration constant as well as the ISO speed should be stated, but this seldom is done.

Values for the reflected-light calibration constant K vary slightly among manufacturers; a common choice is 12.5 (Canon, Nikon, and Sekonic ). Using K = 12.5, the relationship between EV at ISO 100 and luminance L is then


 * $$L = 2^{\mathrm {EV} - 3} \,.$$

Values of luminance at various values of EV based on this relationship are shown in Table 3. Using this relationship, a reflected-light exposure meter that indicates in EV can be used to determine luminance.

As with luminance, common practice among photographic equipment manufacturers is to express illuminance in EV for ISO 100 speed when specifying metering range.

The situation with incident-light meters is more complicated than that for reflected-light meters, because the calibration constant C depends on the sensor type. Two sensor types are common: flat (cosine-responding) and hemispherical (cardioid-responding). Illuminance is measured with a flat sensor; a typical value for C is 250 with illuminance in lux. Using C = 250, the relationship between EV at ISO 100 and illuminance E is then


 * $$E = 2.5 \times 2^{\mathrm {EV}} \,.$$

Values of illuminance at various values of EV based on this relationship are shown in the table to the right. Using this relationship, an incident-light exposure meter that indicates in EV can be used to determine illuminance.

Although illuminance measurements may indicate appropriate exposure for a flat subject, they are less useful for a typical scene in which many elements are not flat and are at various orientations to the camera. For determining practical photographic exposure, a hemispherical sensor has proven more effective. With a hemispherical sensor, typical values for C are between 320 (Minolta) and 340 (Sekonic) with illuminance in lux. If illuminance is interpreted loosely, measurements with a hemispherical sensor indicate "scene illuminance".

Exposure meter calibration is discussed in detail in the Light meter article.