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| subject: | Re: ATM An Old TMs Simple Query |
From: "mommoteandcoyote" To: "George Anderson" Cc: Reply-To: "mommoteandcoyote" George, HEAR, HEAR! or is that, HERE, HERE!!! Well, in either case, well spoken! Then, we can speak of the venerable Snider-Enfield Coyot‚ ----- Original Message ----- From: "George Anderson" To: "Richard Schwartz" Cc: Sent: Thursday, January 23, 2003 8:14 PM Subject: Re: ATM An Old TMs Simple Query > > Believers in Schmidt's should have a read of Robert Reeves "Widefield > Astro-Photography". > You will mortgage your paid off house and sell your first born after you > are infected with Schmidt envy. > > George Anderson > Montreal Canada > > Clear skies and good health > > Richard Schwartz wrote: > > > > OK, I have a few schmidt questions... > > > > If I have a schmidt, I will end up with a lot of little round pieces of > > film. What is a good way to cut the film to the requires shape and size? > > What is a good way to identify the films, index them, and store them? What > > is a good way to take measurements off of them? What is a good way to warp > > the film to match the curved focal plane? If a field flattener lens is > > used, what is a good way to remove distortion from the image, and to correct > > measurements on the distorted image (assuming the exact center of the image > > is not located). > > > > I think the science value is greatly enhanced when the images can be located > > in time and space, and stored in a non-destructive way. There is more to > > working with schmidts than just building the optics. > > > > What I really would like is (1) some kind of field flattener lens, and (2) > > something like a Hasselblad camera back that automatically records date, > > time, and approximate RA and Dec. > > > > . . . Richard > > > > ----- Original Message ----- > > From: "Jerry Hudson" > > To: > > Sent: Wednesday, January 22, 2003 11:16 AM > > Subject: Re:ATM An Old TMs Simple Query > > > > > > > > To ol' Coyote - > > > > > > Your formula, > > > > a*rho^2+b*rho^+b*rho^4... > > > giving the shape of the Schmidt plate, is > > > exactly opposite in sign to the wavefront > > > aberration describing an uncorrected spherical > > > mirror. The glass introduces just enough extra > > > path length where it is thicker to compensate. > > > > > > A straightforward way to see how this all works > > > out, if you have the patience and either a > > > good calculator or BASIC, is to start > > > at the desired focal point of the sphere and > > > trace a ray, bouncing it off the sphere, and > > > taking it out to where it intersects a plane > > > positioned where you want the plate to go. > > > Figure out the path distance along that ray, > > > and subtract off the path distance for the > > > central ray. THat's your "wavefront aberration." > > > If you plot this against radial distance of > > > the ray from the axis, you will get a 4th order > > > looking curve. > > > > > > Note that adding the rho^2 term simply re-focuses > > > the wavefront - you have this degree of freedom > > > to try to make the overall power of the plate > > > to be zero (avoiding all but a trace of color). > > > > > > I hope this helps. > > > > > > BTW, I'd enjoy a direct off-list exchange with > > > you about Schmidts - an interest of mine. I've > > > only made one: a Wright-type Newtonian. And, yes, > > > Edgar Everhart's articles were a great help to me! > > > He was a smart guy and a great glass-pusher! > > > > > > - Jerry Hudson > > > > > > > > > > > --- 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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