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| subject: | Fwd: RE: ATM Why am I so edgy? |
To: atm{at}shore.net
From: "Matthew L. Brown"
Reply-To: "Matthew L. Brown"
Mark,
I think we are working in parallel. My little 4.25" f9 is at the same
spot: center 90% is nice and spherical, with a 3/16" TDE. Ronchi is
hard to read with the overlapping images, so what I see matches your
description quite well. TDE is very clear under Foucault, with a ROC about
0.5" longer than the central region. Under Foucault, the TDE gives me
a darker region right along the knife-edge side of the mirror when the
knife is nulling the central region. It doesn't look flat all the way out.
I really know its a TDE because I can null that region by pulling the
knife back 0.5".
My computer setup is a little in disarray, but I'll try to put up matching
Ronchi and Foucault test images on my web page. Anyone else have example
images on their web pages?
=Matt
>Mark:
>
> I'm a stickler for edges and find that the Ronchi test can be
> difficult to
>read at the exact edge. The grating causes diffraction of the light and
>creates overlapping images of the mirror. The Ronchi bands seen in these
>overlapping images at the edge create a confusing image, looking like an
>outward flare and hook.
>
> I suggest you take real close care in looking at the edge, and
> see if this
>overlapping image effect is what you're looking at.
>
> Varying the grating spacing may make it less of a problem. I
> prefer 50lpi,
>and careful observation.
>
> Also, it makes sense to use the KE to determine the hooking of
> the band at
>the edge. Put it a half inch inside focus and cut the shadow 1/4 the way
>into the lightpath. If you see the distortion at the edge, it's real.
>
> While at a sphere, try the star test using a bright pinhole or
> underpowered
>laser pointer with its collimating lens removed. Use diffract or Suiter's
>book on star testing to verify you have a sphere and a good edge.
>
> Using the Ronchi with a monochromatic source makes for
> interesting ronchi
>bands which I think are worth looking at.
>
>Colin
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