Ten-stop daylight exposure
A metered 1/30-second exposure multiplied by 2¹⁰ becomes about 34.1 seconds. That is a mathematical starting point; make a test and inspect highlights, color, leakage, and movement.
Created by: Ethan Brooks
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Convert ND stops, optical density, or filter factor into an adjusted shutter time with setting-change scenarios.
Translate one ND marking convention into stops, factor, density, and time.
A Neutral Density Filter Exposure Calculator converts ND stops, optical density, or filter factor into a longer modeled shutter time and shows comparable filter-strength scenarios.
Photography settings describe several different physical and perceptual relationships. Exposure arithmetic controls recorded light under a stated model. Focus geometry describes acceptable blur for one chosen criterion. Motion estimates compare a projected displacement with an allowed sensor-plane blur. None of these calculations can see the actual scene, lens sample, camera processing, photographer technique, or final presentation.
The tool treats stops as the common internal language while keeping the selected marking convention visible. It does not assume that an “ND number” uses one universal naming system, so users must select the convention shown by the exact maker. This tool therefore keeps every important assumption visible and provides scenarios rather than hiding uncertainty behind a single authoritative-looking number. Values such as circle of confusion, stabilization performance, filter density, and bellows factor should come from a current product source or a repeatable test whenever the result matters.
Use the result to prepare a first frame, compare alternatives, or understand which input dominates. Then verify with the camera histogram, magnified review, a calibrated meter where appropriate, and a test at the intended print or display size. Recording the successful real setting is more valuable than treating a general default as permanent truth.
Stops convert to a multiplier with two raised to the stop count. Optical density converts to stops by dividing by 0.3, while a filter factor converts with log base two. Only one convention is accepted at a time to prevent ambiguous double counting.
A positive aperture stop-change field represents additional exposure time needed after closing the aperture. A positive ISO change represents sensitivity added elsewhere and therefore reduces the time compensation. The output reports both the filter-only factor and the combined adjustment.
Very long calculated times deserve a test bracket. Actual density can differ from the label, stacked filters can cause flare or vignetting, and film or specialized capture processes may need a separately sourced reciprocity correction.
filter factor = 2^(ND stops)
ND stops = optical density ÷ 0.3
adjusted time = metered time × 2^(total stops)
A metered 1/30-second exposure multiplied by 2¹⁰ becomes about 34.1 seconds. That is a mathematical starting point; make a test and inspect highlights, color, leakage, and movement.
An optical density of 0.9 converts to three stops and a factor of eight. A two-second baseline therefore becomes sixteen seconds if aperture and ISO do not change.
A six-stop filter combined with a one-stop ISO increase produces five stops of net time compensation. A 1/4-second baseline becomes eight seconds, while the higher ISO may alter noise and highlight headroom.
The strongest workflow is comparative: change one input, observe the model response, make the frame, and log whether the assumption matched the intended result. That method turns a calculator into a repeatable testing aid instead of a substitute for field judgment.
Cover optical viewfinders when the camera maker recommends it, use a stable support, and disable or configure stabilization according to the support and lens instructions.
Confirm whether the product label is stops, optical density, or filter factor. Similar-looking ND labels are not universal across every photographic and cinema-filter system.
It applies a documented photographic model to the settings you enter and exposes the assumptions behind the result. It converts one selected ND convention into stops and multiplies the metered time by the corresponding power of two. The arithmetic is useful for planning and comparison, but it cannot inspect lens transmission, camera processing, focus calibration, subject movement, support technique, or final viewing conditions.
Defaults are worked examples that make the form usable on first load. Replace sensor dimensions, circle of confusion, stabilization, filter strength, focal length, aperture, file specifications, and other product-dependent values with the exact manual, label, metadata, or test result for your equipment. Named format families can contain different dimensions.
Equal calculated exposure does not mean equal pictures. Aperture changes depth of field and diffraction; shutter time changes motion rendering; ISO can change noise, highlight headroom, and camera processing. Filters can introduce color shifts or reflections. Treat equivalence as one controlled relationship while reviewing every visual consequence separately.
No. Sharpness depends on focus accuracy, subject and camera movement, stabilization behavior, lens performance, diffraction, atmospheric effects, sampling, processing, output size, viewing distance, and the viewer. Depth-of-field limits are acceptable-blur conventions rather than physical walls. Make test frames and inspect them at the intended output size.
Use the camera histogram and highlight warnings for exposure, magnified playback or tethered review for focus and motion, and the exact filter or lens documentation for marked specifications. Bracket when the scene is not repeatable. Record actual results so later estimates use measurements from the same camera, lens, support, subject, and output workflow.
Those values make the acceptable-blur assumption visible. A traditional circle of confusion is tied to an assumed enlargement and viewing condition, while pixel pitch supports a sensor-plane blur comparison. Neither value independently defines perceived sharpness. A demanding large print or close crop may justify a tighter criterion than a small screen image.
The result is a base-2 exposure calculation, not a guarantee. Filter transmission, spectral response, reciprocity behavior, flare, leakage, temperature, sensor processing, and changing scene light can require a different real exposure.