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| subject: | Re: ATM Astroscan Houghton |
From: "Bob May" To: "atmlist" Reply-To: "Bob May" Actually, Bill, the difference in surfaces is indeed important. A parabolic mirror has a center of rotation and that is only at one point and angle. That center of rotation must go through the center of the eyepiece for best operation of the surface in the scope. A spherical surface has no unique center of rotation and thus it can be merely put into the tube and crudely alligned to somewhere near the appropiate direction. The corrector plate will reform the wavefront which will then be reflected back to the center of that center of rotation of the surface of the corrector and that will be where the light is picked off and sent to the side for the eyepiece. The full symetric image may not be present if the spherical mirror is really off of collimation but the image presented to the eyepiece will still be on-axis as the important part is where the focus is relative to the corrector plate, not the primary mirror. Bob May http://nav.to/bobmay bobmay{at}nethere.com NEW! http://bobmay.astronomy.net --- BBBS/NT v4.00 MP* Origin: Email Gate (1:379/1.100) SEEN-BY: 633/267 270 @PATH: 379/1 633/267 |
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