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Re: [ATM] Corrector/reducer for a fast Newtonian
At 06:13 10/15/05, David Whysong wrote:
>SURFACE RADIUS THICKNESS APERTURE RADIUS GLASS SPECIAL
>OBJ -- 5.6743e+19 8.4186e+17 AIR
>
>AST -5.8830e+3 -2.7197e+03 361.897150 A REFLECT *
>2 -320.748335 V -6.878973 70.000000 BK7 C
>3 -202.021812 V -70.677574 70.000000 AIR
>4 -310.258760 V -14.475886 65.000000 F6 C
>5 4.3789e+03 V -50.665601 65.000000 AIR
>6 -443.950052 V -18.094858 53.000000 BK7 C
>7 1.7508e+03 V -5.066560 53.000000 SF11 C
>8 -144.758860 V -14.475886 53.000000 LAFN28 C
>9 -2.8344e+03 V -49.830000 53.000000 AIR
>10 -- -- 36.000000 BK7 C
>11 -- -- 36.000000 AIR
>IMS -- -0.001395 35.780712 S
>
>(I don't understand why the size of the primary is 28.4" rather than 1
>meter - this differs from the other examples in the paper. And I don't
>understand surfaces #10 and #11; I guess that just defines the focal
>plane.)
Are you sure this is specified right? As shown this has a BK7 window
of zero thickness, which obviously would perform no optical function.
In OSLO putting a dummy surface at the Gaussian focus will make it
extend ray diagrams to the focal plane - otherwise they get truncated
just past the last real surface. That's the only purpose for surface
11 as far as I know.
If I entered this design correctly it looks not so good to me. It's
producing geometric spot sizes around 20 microns and is short of
diffraction limited by about an order of magnitude.
Go to the searchable ATM list archives at
<http://astro.umsystem.edu/atm/search.html> and try a search on
"hyperbolic astrograph". If the primary can be made somewhat
hyperboloidal a much simpler field corrector can be designed. In fact
Dave Rowe posted one for a similar sized telescope just a couple months ago.
As for focal reduction, why not save for a larger format camera instead?
_________________
Michael Peck
email mpeck1@ix.netcom.com
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