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Re: [ATM] Flexed Mirrors
The recent posts by Bill Kelley and others have got me interested again
in my own flexed mirror project. Some time ago, I investigated making a
light weight 12" telescope. I procurred a 12" x 1" plate glass disc and
proceeded to grind and polish for a f/5.6 mirror. So far, it is almost
fully polished. The back has also been fine ground to a 135" radius with
a maximum wedge of .0011". The required tension for a paraboloid figure
is 69.7 lbs. or 0.62 psi.
The main problem with a thin 12" flexed mirror is the varying slump with
altitude which compromises its otherwise perfect figure. I decided to
apply air pressure to the back while polishing and polish back to a
sphere. But, how to pressurize the back? First, we need an airtight
enclosure attached to the mirror back that does not distort the glass in
any way. Since air pressure must be maintained over the entire mirror
back, and the mirror front must remain available for polishing, this
leaves only the mirror edge for attaching the enclosure. For discussion
purposes only, consider a shallow tin can with the same inside diameter
as the mirror, slipped over the back of the mirror and cemented to its
edge with silicone rubber ( RTV). Adler’s Flex.exe program can be used
to calculate the shear forces in the silicone rubber between the mirror
and enclosure, which are surprisingly low in a 12" mirror. In this
instance, the 0.62 psi air pressure results in a shear force of 2.46
lbs./sq. in, well below the yield strength of RTV. Air pressure to this
enclosure can be introduced through a small barbed nipple, soldered to
the can bottom, for connecting an air hose. This air pressure is the
same value as vacuum applied to the back for flexing the mirror into a
parabolic shape and will bulge the front surface an equal amount. It
just remains to polish about 12.6 wavelengths off the front surface back
to a sphere while maintaining air pressure. I contemplated doing this
using a water column 16.97" high with a small PVC tank and some clear
plastic tubing. Testing for a sphere while maintaining air pressure can
be done by the usual Foucault method. Releasing the air pressure should
result in a perfect paraboloid and the mirror can now be supported with
a proper mirror cell. Voila! no more slumping with altitude!
As soon as my current project, adding 'goto' to my 12.25" truss dob
telescope is finished, I'll have to find time to get back to the flex
mirror. Meanwhile, I hope this correspondence will stimulate some more
thinking on flexed mirrors.
Clear skies,
Gil Gagne
Port Orange, FL
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