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[ATM] Lurie-Houghton Newtonian collimation revised



Now that I have more experience, I've found a way to collimate all three of the corrector, primary mirror, and secondary mirror. You'll need some sort of pinhole eyepiece. I use a 35mm film canister with the bottom cut off and a small hole cut in the cap.

1) Center the image of the primary mirror in the secondary mirror, just as you would in a regular Newtonian while using the pinhole eyepiece.

2) Continue to use the pinhole eyepiece. Find the reflection of the corrector cell in the primary mirror. You should be able to see this as your primary mirror should be oversized relative to the corrector cell. Use the collimation screws in the primary mirror mount to center the image of the corrector cell in the primary mirror.

3) Perform a star test. Determine if there is any coma present in the star image by racking it through focus. If there is coma, use the collimation bolts in your corrector cell to move the star in the direction that the coma points. Note that this is opposite what you would do for a normal Newtonian. The coma points to the center of field in a normal Newtonian and you would move opposite the direction the coma points to center the optical axis. Not so with a Lurie-Houghton Newtonian. Keep going until there is no more coma.

4) You have now messed up the secondary mirror collimation performed in step #1 since your corrector supports the secondary. Repeat steps #1 and #3 until satisfied. The primary mirror collimation in step #2 should only have to be performed once but you can recheck it if you wish.

5) At this point, I had to square my focuser to get the focal plane parallel to my CCD chip. Once I was done I found that the field was properly centered on the CCD chip. However, if you find that the center of field is not centered on your CCD or eyepiece, use the secondary collimation bolts to center it. The center of field is indicated by where the astigmatism points off axis when out of focus.

I still have not had to mess with the centering of the two corrector lenses relative to each other. It seems that what looks good (within 1/32") is good enough.

The reason that I messed with the corrector collimation is that I found I had coma that flared to one side of the star image inside focus and then flared to the opposite side of the star image on the other side of focus. I surmise that this is what happens when you try to compensate for the corrector's collimation with the primary mirror collimation only. The result on axis at focus seemed like astigmatism. Properly collimating the corrector eliminated this.

The pictures that I am getting are pinpoint edge to edge. I still do not get nearly the same performance in the eyepiece as I do on my CCD.

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