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Re: Re[2]: ATM Airy disk frustrations
Dwight wrote:
<snip>
> Now an infinite mirror, would have no edge. It would
> produce an infinitely small disk or an impulse spot.
> Well in reality, we should be able to measure the size
> of the stars disk. Something like a f/.000000000001 mirror
> would be interesting. <snip>
Stellar diameters have been measured by making the effective aperture large by
the use of two widely spaced auxiliary mirrors in a phase interferometer
configuration, similar to the two-slit Young interference experiment. As I
recall (from memory) Michelson was the first to do this using the 100" Mount
Wilson scope with auxiliary mirrors some 5 meters apart. He was able to
measure the approximate diameter of a few red giant stars in this manner in
the twenties. Since then more sophisticated interference methods have been
employed but I no longer recall the details. These initial efforts must have
been truly heroic in nature.
A wonderful, easily readable little book on the wave nature of matter and
light is Feynman's "QED, The strange Theory of Light and Matter." I very
highly recommend it. It is FUN, fascinating, and wholly accurate yet non-
mathematical. After reading it one should understand the origin of the Airy
diffraction pattern.
Dave Rowe
Torrance, CA