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Here is an actual tl;dr for what I was saying:
These are from this lovely article here: https://www.edmundoptics.com/knowle...sensor-limitations-on-collecting-information/
Yes, I think that is a big part of what you were saying earlier. You weren't talking about diffraction in the visible to the naked eye sort of way that old times photographers talk about it, but you were talk about diffraction between microscopic photo sites that are at the sub pixel level, since it may only effect one or two colours at a time. Even with lens projectors, blowing up a chart pattern into a 2meter area, that kind of diffraction will still read as "sharp" to the eye, but perhaps be just enough diffraction to reduce moiré.
Reason I found the your comments fascinating, is that I never realized that a good lens at F2, a lens might resolve sharper than F5.6, if that is what you are getting at.
Zeiss supremes (not the same as Arri Signature, which have nothing to do with Zeiss) are nice, but they aren’t perfect. They have some visible chromatic aberation, even more so than sigma or canon likely.
One more thing I wanted to mention about using 2.5x pixel width for diffraction. The calculators online and what I have been using is based on light being at green (usually 550nm) since that is right in the middle of the spectrum. But just using green doesn't tell the whole picture.
Violet light (just at the edge of UV) is around 400nm, which means it actually creates a smaller Airy Disk at every f stop. So, using that 2.5x number on the 12K (a width of 5.5um) but with 400nm light, we get violet light diffraction right at f5.6. That's a much deeper f stop than the f4.1 you get when running the math at 550nm. [The math, once again, is 5.5um = 2.44 * 400nm * f stop. OR f stop = 5.5um / 2.44 / .4um]
Far red light is around 700nm, which means it creates a larger Airy Disk at every f stop. The 2.5x math puts far red light diffraction at f3.2.
Warmer tones are going to experience diffraction before cooler tones do. That's just the physics of light.
For comparison at 2.5x width:
400nm = f5.64
550nm = f4.10
700nm = f3.22
For comparison at 1.5x width:
400nm = f3.38
550nm = f2.46
700nm = f1.93
For comparison at 1x width:
400nm = f2.25
550nm = f1.64
700nm = f1.29
Is this helpful? Maybe not to everyone, but I certainly find it absolutely fascinating. It also again shows why that 2.5x defacto standard for diffraction is just a simplistic number like any other rule.
Oops! Yes, I know the difference, I just misspoke.
@ Josh and John Brawley I understand the connection between the limits in size of the Airy disk and photosite size, an am aware of the 2.5 constant for calculations. But why does the physics decide on a 2.5 constant? What does it mean, where does it come from?
I’m reluctant to continue post here on this topic. My responses are being voted as not helpful.
I’m reluctant to continue post here on this topic. My responses are being voted as not helpful.
It’s getting into some very esoteric ideas. And once you actually go out and shoot enough tests you can get a feel for how much in reality it will affect you in the way you shoot with the cameras you have.
There’s a lot of things that affect the real world usefulness of these calculations. No one for example has brought up how fill factor affects these calculations. This is the active size of a pixel Vs it’s physical size. Things like microlens arrays can factor here too.
Lens performance as well. An airy desk in a physics model is a perfect circle, but most lenses have some kind of aberrations that means it’s rarely uniform across the airy disk diameter interns of field flatness. (It’s darker often in the middle or the edges depending on the lens)
The general accepted consensus is 2.5x is a good compromise for all these factors.

Here is a visual example of lens aberration vs. diffraction (the lines are a little wonky - but you get the idea):
View attachment 141015
You can see that there is a point - a specific f stop - where resolution is maximized. Before that point, in this case f4.2, aberration is limiting the lens from delivering maximum resolution for the sensor. After that point, diffraction is steadily bringing the resolution down.
But, if you don't need all the resolution a lens and sensor combination can give, then it might not matter to you. In the illustration it shows a yellow required resolution line (for our case, let's say it's a 4K delivery). For the illustration purposes, you could go up to f13.5 and still get the required resolution you need.
If you move that yellow line up (let's say an 8K delivery or a 2k punch in) you are going to more quickly reach an f stop where you no longer have that much total resolution and things will start to look blurry at the viewing resolution.
Also, for the lens in the example, as the target resolution increases (as the yellow line moves up) you have to stop down more to reach it - the f stop window for the target resolution narrows. If you wanted to hit 15 lp/mm, for instance, you could only do so in between about f4 and f5.6.
This chart is just an example, though - don't get too caught up in the exact numbers. Different lens and sensor combinations are going to look different, but they will be similar to this.
[The chart came from here: https://www.edmundoptics.com/knowle...d-detection/choosing-the-correct-test-target/ . (The rest of the article is not that helpful for what we are talking about.)]



Is that for 4K raw, or 4K final from a 6K raw supersample?