ISO and Exposure Value Are One Relationship: A Worked Guide
It's easy to treat ISO and exposure value (EV) as two unrelated numbers you happen to need for historical process work — one describing a material, the other describing a lighting condition. They're actually a single relationship: EV at a target ISO equals EV at a reference ISO, plus log base 2 of the ratio between the two ISOs. Once that's clear, converting between any two ISOs — whether they're two stops apart or nine — becomes a matter of plugging numbers into one formula, which is exactly what our ISO↔EV Converter does. This guide works through that single relationship across a range of realistic conversions.
The one formula behind every conversion
Every result the converter produces comes from exactly the same calculation: stop difference equals log base 2 of (target ISO divided by reference ISO), and target EV equals reference EV plus that stop difference. There's no separate case for "converting down" versus "converting up," and no special handling for large gaps versus small ones — it's one continuous relationship across the entire range of possible ISOs, which is part of why it's genuinely useful rather than a lookup table of special cases.
A daylight reading, converted to three different process speeds
Start with a single metered reading: EV 12 at ISO 100, a plausible reading for open shade on a clear day. Converting that reading to an ISO 3 process — a reasonable estimate for some wet-plate collodion work — gives a stop difference of −5.06 and a target EV of 6.94. Converting the same EV 12 reading to an ISO 1 process instead, closer to a daguerreotype's estimated speed, widens the stop difference to −6.64 and drops the target EV to 5.36. Notice that both conversions started from the exact same metered reading; the only thing that changed was the target ISO, and the relationship scaled the answer accordingly, continuously, rather than jumping between fixed brackets.
A dimmer reading at a different reference ISO
The formula works identically regardless of which ISO the original reading was taken at. Metering at EV 10 with a reference ISO of 400 (a common daylight film speed) and converting to an ISO 3 process gives a stop difference of −7.06 and a target EV of 2.94 — over seven stops of correction, even though the starting EV here (10) was lower than the EV 12 examples above, because the reference ISO (400) was itself four stops faster than the ISO 100 used in those earlier conversions. This is exactly why quoting an EV number without its reference ISO is close to meaningless: EV 10 at ISO 400 and EV 10 at ISO 100 describe two different actual light levels, even though the number "10" is identical in both cases.
A conversion that barely moves the needle
Not every historical-adjacent conversion produces a dramatic stop difference. Converting an EV 14 reading at ISO 100 down to ISO 25 — representative of an early orthochromatic dry-plate film rather than a daguerreotype or wet-plate process — gives a stop difference of exactly −2 and a target EV of 12. Two stops is a real, meaningful adjustment, but it's a fraction of the five-to-seven-stop corrections the daguerreotype and wet-plate examples above required. This is the same single relationship at work, just applied across a much smaller ISO gap; the formula doesn't change, only the size of the ratio you feed into it.
Two more points along the same line
A couple of additional conversions round out the picture. EV 13 at ISO 100, converted to an ISO 6 process, gives a stop difference of −4.06 and a target EV of 8.94. EV 15 at ISO 400, converted to an ISO 2 process, gives a stop difference of −7.64 and a target EV of 7.36. Plot all six of this guide's conversions on a single axis of "stops between reference and target ISO," and they fall on exactly one straight line — because that's what the log base 2 relationship actually is: a straight line in stop-space, however curved the raw ISO numbers might look when you write them out as 1, 2, 3, 6, 25, 100, 400.
When the stop difference flips sign
All six conversions above moved from a faster reference ISO to a slower target ISO, which is the direction that matters for historical process work and always produces a negative stop difference, meaning the target EV drops below the reference EV. The same formula works identically in the opposite direction: converting from a slow ISO to a faster one produces a positive stop difference and a higher target EV, exactly mirroring the historical-process case. A photographer converting from a process ISO back to a modern camera's ISO — useful for comparing a planned historical shot against what an equivalent modern exposure would look like — would see the same magnitude of stop difference, just with the opposite sign. The relationship doesn't care which direction you're converting; it only cares about the ratio between the two ISOs involved.
A caution about precision that isn't really there
It's worth being honest about what these conversions actually represent. The formula itself is exact arithmetic — log base 2 of a ratio is a precise mathematical operation with no room for interpretation. What's approximate is the historical ISO figure you feed into it. A daguerreotype's "ISO 1" and wet-plate collodion's "ISO 1 to 3" are retroactive estimates built from modern reproductions and historical accounts, not measurements the original processes were ever rated against using a standardized modern test. That means a target EV of 6.94 or 5.36, calculated to two decimal places, carries far more apparent precision than the underlying ISO estimate actually supports. Treat the calculated stop difference as directionally and roughly quantitatively correct — genuinely useful for knowing you need "about five stops more" rather than "about two stops more" — without assuming the second decimal place reflects anything more precise than the historical ISO estimate that went into it.
Chaining the conversion into a full exposure plan
A brief second worked example shows the full pipeline end to end, using a different starting point than the ones already covered in our combined-corrections coverage elsewhere on the site. Suppose a handheld meter set to ISO 400 reads EV 11 in a moderately lit interior. Converting that to an ISO 2 process (a plausible wet-plate ambrotype estimate) gives a stop difference of log base 2 of (2/400), which comes out to roughly −7.64, for a target EV near 3.36. That's a very low EV, implying a wide aperture, a long shutter time, or some mix of both. If the resulting shutter time you settle on turns out to be, say, 45 seconds at your chosen aperture, that figure then becomes the input to a reciprocity check, since a metered exposure that long is well within the range where reciprocity failure meaningfully changes the real exposure needed — a separate correction layered on top of, not instead of, the ISO conversion covered here.
Why "stops" is the unit that makes this click
The reason this single relationship covers ISO, aperture, and shutter speed all at once is that all three are defined the same way: a "stop" is always a doubling or halving of light, whether that doubling comes from twice the film sensitivity, twice the lens opening's light-gathering area, or twice the exposure time. Once you're thinking in stops rather than raw ISO numbers, aperture f-numbers, or shutter fractions, an ISO conversion, an aperture change, and a shutter speed change all become interchangeable currency — five stops lost to a slower ISO can be recovered by five stops gained somewhere else in the exposure triangle, in any combination that adds up. That's the deeper reason ISO and EV aren't two separate things to memorize: they're two views of the same underlying stop-based accounting system that runs through the entire exposure calculation, historical or modern.
Putting the relationship to work
In practice, the workflow is simple once the relationship clicks: meter the scene normally, at whatever ISO your camera or handheld meter is set to, then convert that EV to your process's estimated true ISO using this single formula. The resulting target EV tells you, in the same stop-based units as everything else in the exposure triangle, how much additional light the process actually needs relative to what the meter reported. From there, translating that target EV into an actual aperture and shutter-speed combination is a separate step, and if the combination you land on involves a long shutter time, it's worth checking that time against our Reciprocity & Exposure Calculator as well, since a long enough exposure needs a second, independent correction on top of the ISO conversion covered here.
Run your own reference EV, reference ISO, and target ISO through the ISO↔EV Converter, and see Reading ISO, EV, and Exposure in Historical vs Modern Photography for more on where these historical ISO estimates come from in the first place. Our Exposure & Print Planning Reference runs several lighting scenarios against a full set of process speeds at once, all from this same converter function.