Yes, I had played with this sort of thing with one of our Gokosha autocollimators (I forget the fl). These had a threaded collar that allowed fine (and precise) adjustment of the objective lens so that different distances could be mimicked, looking into the front of the collector. With the collar set at zero it was an infinity target, and could be verified via a flat mirror in front of the autocollimator. If the film position changes one simply rotates the autocollimator barrel until focus is again achieved (via the autocollimator eyepiece). Then read the distance off the barrel. Using the classic formula 1/f = 1/u + 1/v one can figure how far the film surface moved. Note: f = autocollimator fl, u and f are the conjugate distances of the lens.
As a note the autocollimator is mainly looking only at a small area near the center of the film.
I wonder what kind of glass plate is it used, it would be very handy to know the parallelism is well set with the autocolimator.
From the Edmund Optics technical documents archive linked above:
https://www.edmundoptics.com/ViewDocument/CollimatorsCollimation.pdf
https://www.edmundoptics.com/ViewDocument/Collimating Systems.pdf
Note that photographers and camera technicians tend to use "collimating" to mean setting the focus distance accurately (so that infinity matches a parallel bundle of rays). While telescope users often use "collimate" to mean aligning an optical system so that the optical axes match, for example getting the optical axes of the primary mirror, secondary mirror, and eyepiece of a telescope lined up in position and angle. Both of these uses are correct, but there is sometimes confusion. They reflect (haha) the different alignment needs of typical photographic vs telescopic systems.
I'm currently building a DIY autocollimator. It's a WIP and I'll make a thread when it's done.
I think plain glass would work (although maybe with some flatness certification). In the setup illustrated above you would see the main reflection from the mirror at the film rails, as well as fainter reflection(s) from the glass surface(s) lying on top of the flange mount. If the planes are parallel, the reflections will be co-axial. If not, they will be shifted.
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