
Originally Posted by
Glenn NK
George:
Specular highlights (the sun's reflections off water or a vehicle windshield) cannot be captured without some very heavy underexposure. Even the human eye/brain combination cannot discern any detail from specular highlights. Well maybe with a 10 stop ND
Non-specular highlights can be captured, and these are what one would "push" to the right end of the histogram using ETTR.
I don't understand what you mean by "not of high quality especially how he deals with the binary values".
Could you explain please? Thanks.
Glenn
So if one attempted to use ETTR on a scene with specular highlights, and tried to keep the specular highlights from blowing out, it would be a fool's errand.
I don't mean the spectacular highlights of water but just a scene which has a white house by example and not real dark in it. This histogram wil be closed at the right site and open at the left site, and the DR of the scene is smaller than that of the sensor.
Reichmans is using an argument for his theory which I see often. I think, am sure, this is false.
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A typical consumer DSLR recording 12 bits per sensel is able to record up to 4,098 separate tonal values.
If we assume a 10 stop dynamic range this is how this data is distributed...
The brightest stop = 2048 tonal values
The next brightest stop = 1024 tonal values
The next brightest stop = 512 tonal values
The next brightest stop = 256 tonal values
The next brightest stop = 128 tonal values
The next brightest stop = 64 tonal values
The darkest stop = 32 tonal values
As can be seen, each stop from the brightest to the darkest contains half of the data of the one preceding it.
The camera doesn't record a 12 bits value or an x bit value. It's recordibng an analogue signal. Upper in this article he states that to but I think he forgot that.
In the quote above he is mixing the DR and the tonal value. That are two complete different things.
A DR of 10 doesn't give 2048 tonal values. It can be any number or binary any 2^x.
He is insinuating here that an image is the summation of individual stops. A stop is a halve or double of the light and has influence over the whole recorded value, not a part of it.
George