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Looking at this: https://skyandtelescope.org/astronomy-blogs/imaging-foundations-richard-wright/lucky-imaging/
Reading between the lines, my bet is that it is looking for photos with less atmospheric blurring. Since it sets reference points, it can measure the delta from a good shot, add the values to detainee how close to ideal a particular photo is, then choose the overall “luckiest” photos and stack them.
I read that article, and it's very good! But it didn't explain how detect atmospheric blurring, since it's not actually blurring, it's distortion. To quote that article
Assuming all images are compared to a reference shot as you suggested, how is the reference shot selected?
I've actually got my own ideas about how it could be done, but this is coming from a background in computer science, not from astronomy, so I don't trust my solution.
Yeah, I’m guessing your ideas and mine are going to be similar then; wish I could add more!