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Re: [ATM] Tracking Systems for Astrophotography
The original question posed open loop guiding against closed loop guiding
with no internal tracking model. The discussion is being turned more
towards the latter having a straightforward practical implementation. It's
an interesting question because if solvable in a simple inexpensive manner
might be significant.
Open loop guiding consists of some sort of internal tracking model, be it
mechanical with an equatorial mount, or, computed as in an altazimuth mount.
Some sort of predictive error correction is added. One can achieve unguided
tracking to sub arcsecond accuracy from 30 seconds to 10 minutes this way.
The latter was reached recently by someone using my freeware software with
careful attention to the mechanics.
Closed loop with no internal tracking model in the proposed scenario
consists of a quadrant detector feeding back on/off signals to a motor
controller. Others and I have thought about how to make this work easily,
but I don't have any breakthrough thoughts. There's the issue of
sensitivity of the detector, a tremendous problem in not only getting the
feedback loop to work at a high enough frequency, but also simply in finding
bright enough guide stars next to the desired object to track on. Then
there's the issue of simple on/off feedback loop: no proportional, and no
derivative is available. All you know is that the guide star is either on
one side of the divider or on the other. You don't know how far. So the
control loop has to be stable enough to handle large deviations to either
side but yet stable enough to keep the guide star basically sitting on the
divider, half the time on and half the time off. Remember that perfect
guiding to a certain threshold is required - not even a single deviation out
of bounds is allowable. I think that's hard but maybe someone can point me
to a successful high precision system using simple on/off feedback and the
theory behind its control loop.
Mel Bartels
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