EV100
11.9
vs Sunny 16
-3.1 EV
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The Exposure Value (EV) Calculator quantifies the total amount of light in a photographic exposure using a single numerical scale that combines aperture, shutter speed, and ISO sensitivity into one comparable number. EV was originally defined at ISO 100 (EV100) and is formally standardized by the American National Standards Institute in ANSI PH2.7-1973. An EV of 0 corresponds to one second exposure at f/1.0 (at ISO 100), and each increment of 1 EV represents a doubling of the light (equivalent to 1 stop). The EV scale allows photographers to express scene brightness independently of the specific camera settings used. A sunny day at noon in mid-latitudes is approximately EV 15, while a candlelit room is around EV 2–4. When you know the EV for a scene, you can choose any combination of aperture, shutter speed, and ISO that produces the same total exposure. This is the exposure triangle — the fundamental concept that underlies all photographic exposure decisions. EV calculations are also used in flash photography, where guide numbers quantify flash output in EV units, and in metering systems, where incident light meters and reflected light meters output EV readings that camera exposure systems interpret. Photographers use EV values to compare scene brightness across lighting conditions, to understand automatic exposure shifts made by the camera, to set exposure compensation in fraction-stop increments, and to communicate lighting requirements to assistants and cinematographers. The EV system elegantly unifies the exposure triangle into a single number, enabling precise, systematic exposure control.
EV = log2(N² / t) at ISO 100, where N = f-number, t = shutter speed in seconds EV (at any ISO) = EV100 - log2(ISO / 100) For EV at ISO S: EV_S = log2(N² × S / (t × 100)) Alternatively: EV = log2(f² / t) + log2(ISO/100) Scene EV (reflected): EV = log2(L × S / K), L = luminance (cd/m²), K = reflected light meter constant (~12.5)
- 1Step 1: Note your camera settings: aperture (f-number), shutter speed (seconds), and ISO.
- 2Step 2: Calculate EV100 = log2(f² / t). For f/8 and 1/125 s: f² = 64, t = 0.008 s. EV100 = log2(64/0.008) = log2(8000) = 12.97 ≈ 13.
- 3Step 3: If ISO differs from 100, adjust: EV_actual = EV100 + log2(ISO/100). At ISO 400: +2 stops adjustment.
- 4Step 4: Compare to scene brightness tables (e.g., EV 15 = bright sun, EV 12 = overcast, EV 6 = indoor fluorescent).
- 5Step 5: Use the EV to find equivalent exposures: any combination of N and t satisfying log2(N²/t) = target EV produces the same exposure.
- 6Step 6: Apply exposure compensation (+/- EV) for high-key or low-key subjects where the meter would otherwise give incorrect readings.
f² = 64, t = 0.004 s. EV = log2(64/0.004) = log2(16000) = 13.97 ≈ EV 14. This matches the 'sunny 16' rule — a sunny day is EV 14–16.
EV100 = log2(1.8²/0.0167) = log2(3.24/0.0167) = log2(194) = 7.6. ISO boost: log2(1600/100) = 4 stops. EV_scene ≈ 7.6 (indoor tungsten).
EV100 = log2(7.84/30) = log2(0.26) = -1.9. ISO adjustment: +5 stops. Effective EV ≈ 0. Night sky without moon is EV -1 to 1.
f-number = GN / distance = 58 / 3 = f/19.3. At 1/200 s (flash sync): EV = log2(19.3²/0.005) = log2(74,650) = 16.2.
Photographers setting manual exposure on film cameras without in-body metering.
Cinematographers calculating exposure for mixed lighting scenes across multiple setups.
Light meter calibration and verification against known EV reference standards.
Understanding and setting exposure compensation for challenging metering situations.
EV at non-standard ISOs
EV100 is the reference, but any ISO can be used. To find the scene EV: EV_scene = EV100 + log2(ISO/100). At ISO 800, your camera's EV100 equivalent is 3 stops higher — a reading of EV 5 at ISO 800 represents an EV 8 scene.
Video exposure and EV
In video, EV is fixed by the 180° shutter rule (shutter = 2× frame rate) and aperture choice; ISO is adjusted to match the resulting EV to the scene brightness. Video cameras often display exposure using IRE levels or waveform monitors rather than EV, but the underlying EV math is identical.
When input values approach zero or become negative, the Exposure Ev Calculator
When input values approach zero or become negative, the Exposure Ev Calculator calculation may produce undefined or misleading results. Always validate that inputs fall within the model's valid range before interpreting outputs. Extreme values should be flagged for manual review.
| Lighting Condition | EV (ISO 100) | Example Exposure |
|---|---|---|
| Direct sun, white sand/snow | 16–17 | f/16, 1/125 s |
| Bright sun, clear sky | 15 | f/16, 1/100 s |
| Slightly overcast | 13–14 | f/8, 1/250 s |
| Open shade / heavy overcast | 11–12 | f/5.6, 1/250 s |
| Sunset (sun near horizon) | 9–10 | f/4, 1/125 s |
| Office fluorescent / window light | 7–8 | f/2.8, 1/60 s |
| Home interior (tungsten lamps) | 5–6 | f/1.8, 1/30 s |
| Candlelight | 3–4 | f/1.4, 1/4 s |
| Night street with lights | 2–3 | f/1.8, 1 s |
| Milky Way / starry sky | -1 to 1 | f/2.8, 20–30 s |
What does EV 0 mean in practical terms?
EV 0 at ISO 100 is achieved with an exposure of 1 second at f/1.0. This is an extremely dim light level — approximately the brightness of a single candle at 1 meter. Most modern cameras can meter and expose correctly down to EV -2 or below using electronic front curtain shutters and high-ISO capabilities.
How is EV related to the exposure triangle?
EV mathematically combines all three exposure triangle elements. Every full stop of aperture change (e.g., f/2.8 to f/4), shutter speed change (1/125 to 1/250), or ISO change (ISO 200 to ISO 100) shifts EV by exactly 1.0. Understanding EV makes it easy to see why equivalent exposures work: you can trade one variable for another as long as the total EV stays constant.
What is the Sunny 16 rule and how does it relate to EV?
The Sunny 16 rule states that in direct sunlight, correct exposure at ISO 100 is f/16 at 1/100 s (approximately 1/ISO seconds). EV for f/16 at 1/100 s = log2(256/0.01) = log2(25,600) = 14.6 ≈ EV 15. This is why direct sunlight is defined as EV 15 at ISO 100 — the Sunny 16 rule and EV scale are perfectly consistent.
Can I use EV to set exposure on a camera without a built-in meter?
Yes. Measure scene EV with an incident light meter (measures EV directly) or calculate it from a reference (Sunny 16, published tables). Then use an EV lookup table to find any combination of aperture and shutter speed at your working ISO that matches the target EV. This is exactly how photographers used Ansel Adams' Zone System with manual cameras.
What is exposure compensation and how does it relate to EV?
Exposure compensation (EC) adds or subtracts EV from the camera's metered exposure. +1 EV doubles the exposure (opens aperture 1 stop, slows shutter 1 stop, or doubles ISO). Negative EC reduces exposure. Use +EC for snow, white walls, and bright backgrounds; use -EC for dark subjects on dark backgrounds where the meter overexposes to achieve 'middle gray.'
How do luminance meters display EV?
Incident and spot luminance meters (Sekonic, Gossen) measure scene luminance in EV units, typically at a reference ISO. The meter displays an EV reading that corresponds to a specific combination of aperture and shutter speed shown on its calculator dial. Digital meters show recommended aperture/shutter combinations directly. The relationship is: EV = log2(L × S / K), where L is luminance, S is ISO, and K is the reflected meter calibration constant (12.5 for Sekonic meters).
How does HDR photography relate to EV?
HDR (High Dynamic Range) photography merges multiple exposures at different EV settings (typically ±2 EV, ±1 EV brackets) to capture scenes whose dynamic range exceeds the sensor's single-shot capability. A typical scene may have a dynamic range of 12–16 EV from deepest shadow to brightest highlight. A camera sensor captures 12–15 EV of dynamic range, and post-processing software tone-maps the merged HDR to fit this into the display range.
プロのヒント
Carry an EV reference card or use a metering app on your phone when shooting manual on film or digital cameras without reliable metering. Sekonic's Light Meter University online provides downloadable EV reference tables covering sunrise to midnight.
ご存知でしたか？
The APEX (Additive system of Photographic EXposure) system, introduced in 1960, extended EV mathematics to include film speed and luminance as additive logarithmic values on the same scale — enabling simple arithmetic exposure calculations, a predecessor to the digital camera's automatic exposure algorithms.
参考文献
- ›ANSI PH2.7-1973 – American National Standard for Photography: Exposure Value Scale
- ›Sekonic Light Metering: Understanding EV and Luminance
- ›Adams, Ansel: The Negative (Zone System and Exposure)
- ›ISO 2720:1974 – Photography: General purpose photographic exposure meters
- ›Cambridge in Colour: Exposure Triangle and EV
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