Audited ·Last updated 28 Jul 2026·6 citations·Tier 1·0 uses

Exposure Value (EV) Calculator

Free exposure value calculator. Get EV and EV100 from aperture, shutter speed and ISO, or solve for the shutter speed or f-number a light level needs.

Exposure Value (EV) Calculator

What do you want to work out?
Type 8 for f/8, 1.4 for f/1.4. Ignored when you are solving for the aperture. Always the real f-number on the lens, never a format-equivalent one.
f/
Read together with the unit below: type 250 with "fraction of a second" for 1/250 s, or 30 with "whole seconds" for a 30-second exposure. Ignored when you are solving for the shutter speed.
Shutter speed unit
The ISO arithmetic (ASA) speed set on the camera. Used for the Sv term and to refer the light level back to ISO 100. Required in all three directions.
Used only when solving for shutter speed or aperture. Roughly 15 in bright sun, 12 under heavy overcast, 7 in a well-lit room, 3 at street-light level, and negative at night.
EV
Exposure value (EV)
13.9658
Ev = Av + Tv, the exposure value of the settings themselves. Every combination of aperture and shutter speed with the same EV admits the same total light, which is what makes equivalent exposures possible.
Light level (EV at ISO 100)
11.9658
Shutter speed
1/250 s
Shutter speed in seconds
0.004 s
Aperture
f/8
Av — aperture value
6
Tv — shutter speed value
7.9658
Sv — sensitivity value
7

Background.

Exposure value is the single number that collapses aperture and shutter speed into one measure of how much light a photograph is being given. This calculator returns it from the three settings you actually set — f-number, shutter speed and ISO — and will also run backwards, solving for the shutter speed or the f-number a stated light level demands.

It implements the APEX system exactly as the industry standard defines it, with nothing invented in between. CIPA DC-008 — the Exif specification every camera on the market writes its files to — sets out the whole system in five lines: the aperture value Av is 2·log₂(f-number), the shutter speed value Tv is −log₂(exposure time), the sensitivity value Sv is log₂(ISO ÷ 3.125), and the exposure value is simply Ev = Av + Tv = Bv + Sv. Every number this page returns is one of those four quantities or a difference between them, which is why it reports Av, Tv and Sv alongside the EV rather than hiding them.

The reason the system is additive is the reason photographers think in stops at all. Because each quantity is a base-2 logarithm, one unit of Av, Tv or Sv is exactly one stop — one doubling or halving of light. f/2 to f/2.8 is one unit of Av. 1/125 s to 1/250 s is one unit of Tv. ISO 400 to ISO 800 is one unit of Sv. Adding and subtracting these small integers is arithmetic you can do in your head on a windy hillside, which is precisely what the system was designed for in the 1960s and why it survives inside every Exif header written today.

The page reports two exposure values, and the distinction matters. The plain EV describes the settings: f/8 at 1/250 s is EV 13.97 whatever ISO you have set, because ISO is not part of Av + Tv. The EV100 figure describes the light: it takes the same exposure and asks what EV would have produced it at ISO 100, which is the convention every published light-level table uses. Shooting f/8 and 1/250 s at ISO 400 gives EV 13.97 in settings terms but only EV 11.97 of actual light — bright overcast, not sunshine. Confusing the two is why people find published EV charts disagree with their cameras.

Run in reverse, the page does the job a light meter does. Give it a light level in EV at ISO 100 along with an ISO and one of the two exposure settings, and it solves for the other: t = 2^(Av − Ev) for shutter speed, N = 2^(Av/2) for aperture. The answers will not land on a marked stop, because marked stops are themselves rounded — f/11 is really f/11.314, and 1/250 s is really 1/256 s in the ideal scale — so the page hands you the exact figure and tells you which way to round.

One thing is deliberately missing, and the reason is worth stating plainly. This page does not convert EV into lux or candelas per square metre. The standard's own brightness definition is Bv = log₂(B ÷ NK) with the note "N, K: constant" — the calibration constants are named but not valued, because ISO 2720 lets each meter manufacturer choose K within a range, and different makers do. Guessing one would put a systematic bias of up to a sixth of a stop into every light figure on the page. Instead the calculator stays inside what the standard defines exactly, and says so.

Below the widget you will find the full APEX derivation, three worked examples computed by hand, the standard's own aperture and shutter tables, why the sunny-16 rule is EV 14.64 rather than the EV 15 everyone quotes, and the metering ranges real cameras publish.

What is exposure value (ev) calculator?

Exposure value (EV) is a base-2 logarithmic measure of photographic exposure: one EV is one stop, a doubling or halving of the light reaching the sensor. It belongs to the APEX system — the Additive System of Photographic Exposure — which CIPA DC-008, the Exif standard, defines in Annex C as follows: ApertureValue Av = 2·log₂(f-number); ShutterSpeedValue Tv = −log₂(exposure time in seconds); BrightnessValue Bv = log₂(B ÷ NK); film sensitivity Sv = log₂(ASA ÷ 3.125); and Ev = Av + Tv = Bv + Sv. The left-hand equality is what the camera is doing, the right-hand equality is what the scene is doing, and a correct exposure is the statement that the two are equal. Because every term is a logarithm, the whole system is additive: open up one stop and add 1 to Av, halve the shutter speed and add 1 to Tv, double the ISO and add 1 to Sv. Note that EV as defined by Av + Tv contains no ISO term at all — f/8 at 1/250 s is the same EV on ISO 100 and ISO 6400. That is deliberate, because EV describes a camera setting, not a light level. To describe light you need a reference sensitivity, and the universal convention is ISO 100, giving EV100 = EV − log₂(ISO ÷ 100). Since Sv at ISO 100 is log₂(32) = 5 exactly, EV100 is simply Bv + 5. What EV cannot tell you on its own is the absolute light level in lux or cd/m², because that conversion requires the meter calibration constant K, which the standard names but does not fix and which varies between manufacturers by around a sixth of a stop.

How to use this calculator.

  1. Pick the direction. "The EV of these settings" is the measuring direction — you have an exposure and want to know its value. The other two are the metering directions — you know the light and want the missing setting.
  2. Enter the aperture as a plain f-number: 8 for f/8, 1.4 for f/1.4. It must be the real f-number of the lens, never a format-equivalent one, because equivalent apertures describe depth of field and not exposure.
  3. Enter the shutter speed together with its unit. Type 250 with "fraction of a second" for 1/250 s, or 30 with "whole seconds" for a half-minute exposure. The unit selector is purely a typing convenience; it changes nothing in the maths.
  4. Enter the ISO speed actually set on the camera. It never affects the plain EV, but it sets Sv and it is what converts the settings EV into the ISO 100 light level.
  5. When solving for a setting, enter the scene light level as EV at ISO 100 — around 15 in bright sun, 12 under heavy overcast, 7 in a well-lit room, and negative outdoors at night. This is the figure published EV tables quote.
  6. Read the EV and the EV100 as a pair. The first is what your settings are doing; the second is what the light is doing. If they differ, the difference is exactly log₂(ISO ÷ 100) — two stops at ISO 400, six at ISO 6400.
  7. Round solved settings towards more exposure, not less, unless you are protecting highlights. A solved f/16.19 means f/16 rather than f/22; a solved 1/541.6 s means 1/500 s rather than 1/640 s. Digital sensors recover shadows far better than blown highlights, so the direction of the rounding is a real decision.
  8. Use Av, Tv and Sv to plan changes in your head. Every unit is one stop, so trading two stops of shutter for two of aperture leaves the EV untouched — the whole point of the additive system, and the arithmetic behind every equivalent exposure.

The formula.

Av = 2·log₂N · Tv = −log₂t · Sv = log₂(ISO ⁄ 3.125) · Ev = Av + Tv = Bv + Sv · EV₁₀₀ = Ev − log₂(ISO ⁄ 100)

The whole system is four definitions and one identity, and CIPA DC-008 Annex C states them in exactly this form:

a) Av = 2·log₂(f-number) b) Tv = −log₂(exposure time) c) Bv = log₂(B ÷ NK) with B in cd/cm², N and K constants d) Sv = log₂(ASA ÷ 3.125) e) Ev = Av + Tv = Bv + Sv

Why 2·log₂ for the aperture? Because light gathered scales with the area of the entrance pupil, and the pupil diameter is f ÷ N, so illuminance goes as 1/N². Taking the base-2 log of 1/N² and flipping the sign gives 2·log₂N, which makes one unit of Av one stop. That is why the familiar aperture series runs in steps of √2: f/1, f/1.4, f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16 — Av 0 through 8, exactly as tabulated in the standard.

Shutter speed is simpler because exposure is directly proportional to time, so a single log suffices, negated so that shorter exposures score higher. The standard's own table maps Tv −5 to 30 s, Tv 0 to 1 s, Tv 3 to 1/8 s, Tv 8 to 1/250 s and Tv 11 to 1/2000 s. Note the marked speeds are rounded: Tv 8 is really 1/256 s, not 1/250 s, and Tv 7 is 1/128 s rather than 1/125 s. This calculator uses the number you actually type, so an entry of 1/250 s returns Tv 7.9658 rather than 8. That is not an error; it is the difference between the engraved scale and the ideal one.

Sensitivity uses the divisor 3.125 so that ISO 100 lands on Sv 5 exactly: 100 ÷ 3.125 = 32, and log₂32 = 5. ISO 400 gives Sv 7, ISO 51200 gives Sv 14.

The identity Ev = Av + Tv = Bv + Sv is the statement of correct exposure. The left side is what the camera does; the right side is what the scene and the film or sensor do. From it, the ISO-100 reference falls out with no further assumptions: for a fixed scene brightness Bv, two ISO speeds differ only in Sv, so

EV₁₀₀ = Ev − log₂(ISO ÷ 100)

Solving backwards is then algebra. Given a light level and an aperture,

Tv = Ev − Av t = 2^(Av − Ev)

and given a light level and a shutter speed,

Av = Ev − Tv N = 2^(Av ÷ 2)

One thing the identity cannot give you is an absolute light level. Line (c) contains the constants N and K, which the standard names and does not value. ISO 2720:1974, the standard governing exposure meters, permits each manufacturer to pick K within a range, and the values in common use differ by about a sixth of a stop. A calculator that prints a lux figure has silently chosen one of them for you. This page does not, and instead confines itself to the quantities the standard pins down exactly.

Finally, a note on sunny 16, which is usually quoted as EV 15. The rule states that in bright sun you shoot f/16 at a shutter speed of 1/ISO. At ISO 100 that is f/16 and 1/100 s, giving Av 8 and Tv 6.644, so Ev = 14.64 — not 15. The round number comes from rounding 1/100 s up to the tabulated 1/128 s. This page returns 14.64 because that is what the settings compute to, and reports the rounding rather than absorbing it.

A worked example.

Example

A shot at f/8 and 1/250 s on ISO 400 — a typical daylight action setting. The aperture value is Av = 2·log₂(8) = 6 exactly, which is the value CIPA's own Table 52 lists against f/8. The shutter speed value is Tv = −log₂(1/250) = log₂(250) = 7.9658; the standard tabulates f/250 at Tv 8, and the 0.034 shortfall is precisely the gap between the engraved "1/250" and the ideal 1/256 s. The exposure value is therefore Ev = 6 + 7.9658 = 13.97. The sensitivity value is Sv = log₂(400 ÷ 3.125) = log₂(128) = 7 exactly. Now the part that trips people up: the light level. EV100 = 13.97 − log₂(400 ÷ 100) = 13.97 − 2 = 11.97. So although the settings are EV 13.97, the scene itself is only EV 11.97 — heavy overcast, not sunshine. If you had metered EV 15 sunlight with these settings you would be three stops overexposed. Run the page the other way to see the metering direction. Take bright sun at EV100 15, ISO 200 and f/11. Then Ev = 15 + log₂(2) = 16 exactly, Av = 2·log₂(11) = 6.9189, so Tv = 16 − 6.9189 = 9.0811 and t = 2^(Av − Ev) = 121 ÷ 65536 = 0.0018463 s, which is 1/541.6 s. Set 1/500 s and you are a sixth of a stop generous, which is the right way to round. Do it once more for the aperture: EV100 15, ISO 100, 1/125 s. Ev = 15, Tv = log₂(125) = 6.9658, Av = 8.0342, and N = 2^(8.0342 ÷ 2) = √(32768 ÷ 125) = 16.19. That is f/16 — the sunny-16 rule dropping out of the standard rather than being asserted, and a useful reminder that the rule is a rounding of 16.19 rather than an exact result.

target Exposure Value10015
aperture8
shutter Speed Value250
iso Speed400
shutter Unitfraction
solve ForexposureValue

Frequently asked questions.

Does EV include ISO or not?
Not in the strict definition, and this is the single most common source of confusion. CIPA DC-008 Annex C defines Ev = Av + Tv, and neither Av nor Tv contains a sensitivity term, so f/8 at 1/250 s is EV 13.97 whether you shoot it at ISO 100 or ISO 6400. What changes with ISO is which EV correctly exposes a given scene, through the other half of the identity, Ev = Bv + Sv. That is why this page returns two numbers: the plain EV describes your settings, and EV100 describes the light by asking what EV would have produced the same result at ISO 100. Published EV tables — EV 15 for bright sun, EV 7 for a lit room — are always EV100 figures, so compare them against the second number, never the first.
Why is Av twice the log of the f-number?
Because illuminance at the sensor scales with the area of the entrance pupil while the f-number describes its diameter. The pupil diameter is focal length ÷ f-number, so light gathered goes as 1/N². Taking log₂ of that and negating gives 2·log₂N, and the factor of two is what makes one unit of Av equal one stop rather than half of one. It is also why the aperture scale advances in steps of √2 ≈ 1.414: f/1, f/1.4, f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16, f/22, f/32 correspond to Av 0 to 10, exactly as tabulated in CIPA DC-008 Annex C, Table 52. The marked numbers are rounded — f/11 is really 2^3.5 = 11.314 and f/22 is 22.627 — which is why a calculator working from the number you type will disagree very slightly with the tabulated integer.
Why does the calculator say 1/250 s is Tv 7.9658 when the standard's table says 8?
Because the standard's table lists marked shutter speeds against their nearest APEX integer, and the marked scale is itself a rounding. Tv 8 means exactly 1/2⁸ = 1/256 s; camera dials print "1/250" because it is a friendlier number, and the difference is 0.034 EV — about a thirtieth of a stop, far below anything you could see or any shutter could hold to. This calculator takes the number you type at face value, so entering 250 returns Tv = log₂(250) = 7.9658. If you would rather work in exact APEX steps, enter the true power of two: 256 for Tv 8, 128 for Tv 7, 1024 for Tv 10. The same applies to marked apertures.
Why is there no lux or candela output?
Because computing one honestly requires a constant that no accessible primary source fixes. CIPA DC-008's own brightness definition is Bv = log₂(B ÷ NK) with the note "B: cd/cm², N, K: constant" — the constants are named but never valued. The document that governs them, ISO 2720:1974 on general purpose photographic exposure meters, permits each manufacturer to choose the reflected-light constant K within a range, and different makers genuinely choose differently; the values in common use differ by roughly a sixth of a stop. Any calculator that shows you a lux figure has quietly picked one of them on your behalf, and its number will disagree with a meter calibrated to the other. Rather than bake in an unsourced bias, this page confines itself to the quantities APEX defines exactly and states the limitation instead of hiding it.
What are equivalent exposures, and how do I find them here?
Two settings are equivalent when they share an EV, because the identity Ev = Av + Tv is additive: subtract one from Av and add one to Tv and the sum is unchanged. So at EV 14, f/8 at 1/256 s (Av 6 + Tv 8), f/5.6 at 1/512 s (Av 5 + Tv 9), f/4 at 1/1024 s (Av 4 + Tv 10) and f/11 at 1/128 s (Av 7 + Tv 7) all admit the same total light. To use this page for that, compute the EV of the settings you have, then switch to "the aperture this light level needs" or "the shutter speed this light level needs" and enter the EV100 it reported. What changes between equivalent exposures is not the brightness of the file but everything else: depth of field, motion blur, and diffraction at very small apertures. That is the whole craft of choosing between them.
Is bright sunlight really EV 15?
It is the number everyone quotes, but it is a rounding rather than a computed result. The sunny-16 rule says use f/16 at a shutter speed of 1 ÷ ISO, so at ISO 100 that is f/16 and 1/100 s. Av is 2·log₂16 = 8 and Tv is log₂100 = 6.644, giving EV 14.64. The tidy "EV 15" comes from rounding 1/100 s up to the tabulated 1/128 s, which is a third of a stop. This calculator returns 14.64 because that is what the settings compute to, and the difference is small enough not to matter in the field but large enough to explain why your camera's meter and a printed EV chart never quite agree. Use EV 15 as a mental anchor and the calculator for anything you intend to act on.
What EV range can a real camera actually meter?
Narrower than you might expect, and the manufacturers publish it. Nikon quotes the D7500's metering range as 0 to 20 EV for matrix, centre-weighted and highlight-weighted metering, and 2 to 20 EV for spot, all measured at ISO 100 with an f/1.4 lens at 20 °C. Canon quotes the EOS R7 at EV −2 to 20 for stills and EV 0 to 20 for movies. Below the bottom of that range — deep dusk, moonlight, the night sky — the meter stops being able to help and you are into calculated or trial exposures, which is exactly the situation this calculator is most useful in. The shutter and ISO limits bound the other end: both bodies run 1/8000 to 30 seconds mechanically, the R7 reaching 1/16000 electronically, and both reach ISO 51200 at the top.
My lens does not have f/16.19. What do I set?
Round to the nearest marked stop, and prefer the direction that gives more exposure unless you are protecting highlights. Modern lenses click in third stops, so f/16.19 rounds to f/16 and costs you 0.03 of a stop — invisible. A solved 1/541.6 s rounds to 1/500 s, giving a sixth of a stop more light, or to 1/640 s for a sixth less. Digital sensors recover detail from underexposed shadows far more gracefully than from clipped highlights, so in a high-contrast scene round towards the shorter exposure; in flat light, round towards the longer one. If your camera offers third-stop increments, the residual error after rounding is never more than a sixth of a stop, which is inside the tolerance the meter itself is built to.
How does EV relate to exposure compensation?
Exposure compensation is measured in exactly the same units, which is why the dial is marked in EV. Dialling +1 EV asks the camera to give one stop more light than its meter thinks correct, which it achieves by moving Av, Tv or Sv by one unit depending on the mode you are in. Exif even stores it as ExposureBiasValue in APEX units. So if this page tells you a scene is EV100 12 and you want to render it a stop brighter than a mid-tone meter would, work to EV100 11 instead. The additivity is the point: everything in the system — aperture, shutter, ISO, compensation, flash compensation, even filter factors — is expressed in the same stops and can simply be added.
Does a neutral density filter change the EV?
It changes the exposure you must set, not the exposure value of the scene, and keeping those separate avoids a lot of confusion. An ND filter is rated in stops: a 10-stop filter, often sold as ND1000, cuts the light by a factor of 2¹⁰ ≈ 1000. The scene is still whatever EV100 it was, but the light arriving at the sensor is 10 EV lower, so you must add 10 to the exposure you would otherwise use. In practice: meter the scene, read the EV100 here, subtract the filter's stop rating from it, then re-run the calculator in "shutter speed this light level needs" mode with the reduced figure. A sunlit EV100 15 scene behind a 10-stop filter behaves like EV100 5, which at f/11 and ISO 100 works out at t = 11² ÷ 2⁵ = 121 ÷ 32 = 3.78 seconds — call it four.

References& sources.

  1. [1]Camera & Imaging Products Association / JEITA. CIPA DC-008-2012 (JEITA CP-3451C), 'Exchangeable image file format for digital still cameras: Exif Version 2.3', Annex C — APEX Units. The source for every equation on this page: 'a) ApertureValue (Av) = 2 log 2 (F number); b) ShutterSpeedValue (Tv) = - log 2 (exposure time); c) BrightnessValue (Bv) = log2 ( B/NK ) Note that: B:cd/cm2, N,K: constant; d) Film sensitivity (Sv) = log2 ( ASA / 3.125 ); e) Ev = Av + Tv = Bv + Sv.' Annex C also carries Table 52, 'Typical APEX Values', mapping Av 0–10 to f/1–f/32 and Tv −5–11 to 30 s–1/2000 s.
  2. [2]Nikon Corporation. D7500 Online Manual, Technical Notes — Specifications. Gives the exposure metering range as '0 – 20 EV' for matrix, centre-weighted and highlight-weighted metering and '2 – 20 EV' for spot metering, qualified 'at ISO 100, f/1.4 lens, 20 °C/68 °F'; the shutter range as '1/8000–30 s in steps of 1/3 or 1/2 EV, bulb, time, X250'; and sensitivity as 'ISO 100–51200 in steps of 1/3 or 1/2 EV'.
  3. [3]Canon Inc. EOS R7 Product Manual, Specifications. Gives the metering range as 'EV –2 to 20' for still photo shooting and 'EV 0 to 20' for movie recording; shutter speeds of '1/8000–30 sec., Bulb' with the mechanical shutter and '1/16000, 1/8000–30 sec., Bulb' with the electronic shutter; and 'ISO 100–32000' with an expanded 'H (equivalent to ISO 51200)'.
  4. [4]Canon Inc. EOS R6 Product Manual, Specifications — Image Sensor. Gives the full-frame sensor size as 'Approx. 35.9×23.9 mm'. Cited here in support of the point that exposure value is a property of the settings and the light and not of the sensor format: the same f-number and shutter speed give the same EV on any sensor size.
  5. [5]International Organization for Standardization. ISO 2720:1974, 'Photography — General purpose photographic exposure meters (photoelectric type) — Guide to product specification'. The standard governing the calibration constant K that CIPA DC-008 Annex C refers to but does not value. It permits manufacturers to select K within a range, which is why this calculator publishes no luminance or illuminance figure. Cited without a link: the ISO catalogue entry returned HTTP 403 when fetched, and the standard itself is paywalled.
  6. [6]Nasse, H. H. (2010). 'Depth of Field and Bokeh.' Carl Zeiss Camera Lens Division. Source for the warning that a sensor-format-converted f-number 'would be incorrect as an exposure parameter' — the reason this page insists on real f-numbers rather than 35 mm-equivalent ones in the aperture field.

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