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Here are some methods which function either inside of, or outside of, the radius of curvature.

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Spot Grid test

 Next I'll show photographs I made of my 22" f/4.5 paraboloid Newtonian telescope mirror. These images were made using a blue led shining through a pinhole about 0.005" diameter. The first two images show the result of placing a 71 spi spot grid inside the roc. One shows six zones, the other shows eight. The rows and columns on the grid itself are straight, the aspherical nature of the mirror causes the lines to bend outward in the picture. The amount of bending can be measured, and so the mirror's shape can be figured out. These two images seem much more useful than the several corresponding images below them.

 This next image shows a 90 lpi Ronchi grating in front of the same 22" mirror, similar to the setup above. If you look at the left and right edges you can see that there is an interference effect happening between the lines. This interference breaks up the image of the lines, so that you can't count exactly how many lines are showing, or know exactly where they are, or even know exactly where the edge of the mirror is.     The Spot Grid image above has a lot more zones showing, yet it is less damaged by interference effects. (By zones, I mean the number of data points between the center of the mirror and the edge, be they lines or spots.) Compared to a Ronchi grating, the Spot grid suffers much less from diffraction interference problems, because it has a greater percentage of clear aperture.     A spot grid provides a single aperture with lots of little obstructions, while the Ronchi grating actually breaks the light beam up into lots of skinny apertures. The Ronchigram can only be used perpendicular to the lines. The Spot grid photo works in two dimensions, it can be measured horizontally, vertically and diagonally.     On the right is the same Ronchi grating used outside the roc. Now the lines want to bend in the opposite direction. The center third of this mirror has a big hill (relative to the perfect parabola) which shows up in this Ronchi image and the one above. Again, you see the interference effects near the left and right edges.     Below left is a 150 lpi Ronchi grating. The interference effects become more severe. Next to it is the 71 spi Spot grid, also shown outside the roc. These images really are not very useful.

The Lateral Spot test

 The biggest problem with the Ronchi grating is that the lines have severe diffraction interference problems. One of the tests described by Léon Foucault uses the two edges of a single wire. The Kent Wire test shown on page 2, with the Phi symbol, is done at the roc. Here I show a single wire used inside or outside the roc, the same as you'd use a Ronchi grating. The big advantage of a single wire is that its diffraction effects don't have the other lines to interfere with. So the line assumes the correct shape and is much easier to interpret.      Although I am doing this differently than Foucault described, the result is similar. What I am doing is similar to the Lower test, done in reverse. The shape of the line is determined by the shape of the mirror at that point. If the mirror was a perfect sphere you could hold the line anywhere and it would appear perfectly straight. The lines should display smooth curves for a parabola, not that waviness like you see in these photos. This demonstrates how far from a parabola this particular mirror is.      So we can look at the curve in the line and see the nature of the beast. In the left image the wire is inside the roc, and in the right image the wire is outside the roc. Both positions easily show the 8" diameter hill in the center of my mirror. The image on the right shows the bad turned-down edge as well.

 John Francis showed us a way to use the caustic test to quantify a single-wire test. He calls it the Lateral Wire Test (LWT). The red led with it's diffraction is also good for this test, and that is the light source used for this set of photos. Once again it provides a nice central bright division to mark the zones with.     The LWT uses the single wire well inside the roc, and scans it from left to right across the mirror. Every time you reach a zone notch you record the readings. These two pictures show the line in the 4" zone on the left and the 8" zone on the right half. It is fairly easy to build a tester for the LWT, it is very easy to use, and it is the best way I have found to get data from near-spherical central zones.

Happy telescope making!!

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