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Michael Fallwell's projects:Drought Reduction * Glider powered windmill * Folded Newtonian Design * The secret of Brown Adipose Tissue (BAT) |
Folded Newtonian Design
*) a friction drive equatorial table has low periodic error.
Advantages of large secondariesProfessional Cassegrains rarely have secondaries smaller than 33% and there are some real advantages to larger secondaries: So the only real advantage of a small diagonal in a large telescope is a tiny improvement in contrast/resolution that can easily be recaptured with image processing.
A few comments in response to threads on the web (slashdot)It took me many years to realize that secondary size is of much less importance than the quality of the primaries figure in 2 hours I can put a nearly perfect figure on a f:8 mirror. Its just not possible to achieve the same quality in a week of work on an f:4 . But because on some objects a small secondary may be useful, a longer upper cage can be used. In this case the trunions are used in their extended position to eliminate the need for massive counter weight. My binoviewer is better in at least one respect than the $1000 model. It gives a 100 degree field of view. I used a split field, not a beam splitter. If you place your fist on your forehead, you can study the effect of the transitions from one field to the other and each eye has twice the light to work with. The binoviewer is the reason for this telescope. Collimation of the primary is fixed - no adjustments possible. But the secondary has 4 degrees of freedom; all collimation adjustments are made at the secondary. The secondary can be stored without disturbing the adjustments. Setup does not require collimation. The tracking table has low periodic error for CCD work, but it is not designed for film photography. However, an autoguider driving servos on the secondary would meet even this need. I find little use for the star diagonal - even at the zenith you are not looking straight up.
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Please contact me by email: mike_fallwell@yahoo.com