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Re: [ATM] Baffling a Gregorian and corrector plate fabrication.
Hi Doug,
The Gregorian optical system was once the favored type for terrestrial
telescopes during the 18th century. The only baffle used was a stop
located at the exit pupil of the eyepiece. Properly sized and located,
this is very effective. I don't know where you will find further info on
this though.
Jarvis Krumbein
On Tue, 23 May 2006 15:10:38 -0400 Douglas S Angle
<Douglas.S.Angle@can.dupont.com> writes:
> I'm contemplating building a Gregorian, and I've been looking at
> different
> design considerations. I've browsed through the archives, read
> Rutten &
> van Venrooij on the subject. One thing I can't figure out is how to
>
> baffle such that stray light can't get from the entrance aperture to
> the
> eyepiece. There's an article in ATM about a newt-cass-gregorian
> telescope, but the article doesn't address baffling at all, and the
>
> pictures don't look like there's any attempt to baffle. I did a
> full size
> drawing, and I can't see how to catch more than about 1/2 the stray
> light.
> For reference, my design was:
> primary diameter 16"
> primary focal length 64 f/4
> secondary diameter 4"
> distance of focus behind primary 15"
>
> I would be interested in hearing from anyone who has built a
> gregorian, or
> advice on how to solve the baffling problem.
>
> I also considered a shorter focal length primary combined with a
> corrector
> plate. I understand the principle of the Schmidt camera, where the
>
> corrector is placed at the center of curvature, and can be made
> using the
> vacuum pan method. If I were to move the corrector plate towards
> the
> primary, is it true that the I can't use the vacuum pan method
> anymore,
> because the shape is now different? For that matter, is there any
> difference between a corrector plate as used in a schmidt camera, vs
> one
> used in a compound telescope so that the primary can be left
> spherical?
>
> Thanks all.
> -Doug
>
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