Raphael said:
No, the worst problem is the highly folded optical path
and the tiny, short-focal-length lenses used on flatbeds,
as compared to dedicated 35mm or MF scanners.
Compare the imaging lens on an LS-9000 to the one
on a 4990, or compare the optical paths on the two
-- it's like comparing Palomar to a Questar.
Hmmm 200 inch/3.5 inch = 57 times the aperture.
I have taken apart some flatbeds and in the better ones,
lens aperture is ~3/4 inch or so. I haven't checked
a 4990, of dedicated film scanner. You're saying
a dedicated scanner has lenses much larger than 3/4 inch
(0.75 * 57 = 42-inch aperture lens ;-)?
That layer of glass that your negative sits on is really
only a minor part of the problem.
If the aperture, f/ratio and sensor deliver the MTF, then
the optical system is not the issue. There are quite large
linear arrays available at low cost these days, so matching
the linear sensor to a lens system is not that hard.
I've worked enough with CCDs and scanner firmware to
hazard a guess that anything beyond 11-12 bits of real
S/N from a CCD is a pipe dream.
To get 12-bits of S/N one needs to collect over 16 million
photons (with zero read noise), so I'll agree with you
here. With read noise of 4 electrons, you would need to
collect over 65 million photons/pixel! No CCD or CMOS
sensor can do that, unless the pixel is mm in diameter.
Are you referring to dynamic range?
Then with image stacking (multiple sampling in scanner),
one can beat down the noise and get well above 12-bits dynamic range.
This is done even with 8-bit web cams by amateur astronomers
imaging the planets! Multisampling scanners are no big deal.
Film doesn't have 12-bits of S/N, not even 200 (perhaps if you
average large areas with special controlled development).
I think you mean dynamic range.
Roger