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All I needed to know for the moment is the average, eyepiece, focus point with any two flat mirrors in place. The Porsa framework was mounted on the B&D workbench with props under the front legs. This gave me a potential view of a leafless tree about 150 yards away silhouetted against the sky. I needed a high contrast object to ensure it was easy to find the image in the eyepiece.
The image shows first setup was with the bare, flat, shaving/makeup mirror dangling by a cord from the tilt strip. The equally pretend, second mirror
was a compact, makeup mirror. Nothing more was needed at this early
stage.
Due to the short focus I decided to move the 1st mirror forwards by propping it on its 3" deep shell. The focus was now pushed 6" away, well beyond the backplate. Hmm. So, any mirror movement, forwards or backwards, doubles the difference in the position of the focal plane. Or so it seemed in practice. Remember that we are dealing with a focused cone of light here. Not a parallel beam.
I quickly replaced the focuser and now I had some space between the EP and the extended focuser. What would happen if I cut down the 1st mirror shell? Let's assume for my present purposes that the mirror is 12mm or 1/2" in front of the shell. Removing this difference, with the proper mirror in its deep shell, would pull the focus 1" closer to the objective. Cutting an inch from the depth of the shell would move it 2" nearer the objective. 3" movement in total is not an insignificant distance!
The 2nd mirror is presently much nearer the framework than it would be in practice. It will be pushed forwards by at least 1.5" even with a cut down shell depth. Resulting in the 3" gained [from moving the 1st mirror backward] being cancelled out. Using the full depth of the second shell would bring the focus to the required point for permanent, star diagonal use. Or so I hope!
Ideally I want the infinity focus to lie somewhere around the half way point of focuser movement when the 2" star diagonal is in place. So really, I need the focus to be pushed even further beyond the focuser and should need the focal extender tubes to reach focus when not using the star diagonal. Just as everything was with the 'classical' straight steel tube in place.
Here is the second cheapo mirror crudely supported on its shell with twine and tape. With both mirrors mounted on their respective 3" deep shells I now found I could focus on objects 150 yard distant using the star diagonal and the focuser pushed fully inwards. Any more distant object would need much more inward focus movement which I just don't have. So the OTA framework really is too long even with both mirrors fully forwards. [Forward extension pushes the focus further out.]
It is just possible that one or both test mirrors is not very flat.
This would tend to push the focus in or out depending whether either
mirror was concave or convex. Mirror curvature moves the focal plane
quite a long way.
So
my next task is to exclude such errors. I must mount the precision flat
mirrors securely in their full depth shells. The backing disks will be
held to their respective tilt strips by a single central screw and nut. I
can then start collimating more precisely and rule out focus changes
due to the very cheap 'test' mirrors. It continues to rain and sleet so
working outside is impossible.
I found throwing a dark towel over the top of the OTA excluded a lot of stray light and helped to improve contrast.
Click on any image for an enlargement.
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2 comments:
Hi Chris,
I found that the best guide of all was an accurately dimensioned and folded ray trace laid onto an accurately dimensioned outline of my tube - or in your case the Porsa framework - and then with accurately dimensioned cardboard cutouts of the "cross-section" flats and mirror cells and tilt plates all placed so that the face of each flat-cutout just touches the angled fold in the ray trace. Don't neglect to model the mid-point spring bolt positions and the final right-angle external flat which precedes your eyepiece.
Provided all the components are accurately measured, the focal length of the ray cone is accurate, the ray cone starts in the middle of the object lens cell, and the framework dimensions reflect what you have built, you should get no surprises at all - or at least no surprise greater than a maximum of 10mm.
At that point you can then consider reducing the heights of the mirror cells, and reducing the end-to-end length of the Porsa framework to correspond, so that you have minimal extra weight and complexity. :)
Otherwise I fear that in 4 blog pages' time, you will have built everything for real, carefully hooked it all up, and then find that the image of a real celestial object is way beyond the intended position, or unexpectedly inside it... and that can be really frustrating!
All the best,
Andrew
I see you may have to shave off a little from the back and sides of the framework: don't let it put you into a strop or make you foam at the mouth. If it takes the edge off your fun just razor glass and reflect on the fact that things will get hairier with the real flats in place, and you may want to wrap your head in a hot towel before confronting the bald truth about the focal point. Sorting it out may be something for the weekend, but you'll beard it I'm sure, and be on the crest of a wave rather than up the pole. Then slap on some black paint, let it blow dry, and remember you had toupee far less than most folk - in fact it was a snip!
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