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Re: ATM A cage as secondary holder
Things that make us go hmmm.....:
Why not use steppers to control all the optical and mechanical adjustments?
Just think, push a button, and the scope collimates and boresites all by
itself. Just a few lines of code....
ran@netgate.net wrote:
> In <199807210159.TAA13795@intergate.pvtnetworks.net>, on 07/20/98
> at 07:59 PM, iss@pvtnetworks.net said:
>
> >Re the (re)movable secondary cages, one of the problems with building
> >accurate telescopes/mounts (in terms of tracking and finding things) in
> >amateur class systems is the need to have the telescope axes orthogonal
> >(ra/dec or alt/az), and have the optical axis also orthogonal to the
> >alt/dec axis. It's
> >not that hard to build the mount accurately and, once built
> >and aligned, it usually stays that way.
>
> I would guess that "usually" it doesn't: i.e., that most mounts get
> moved frequently as they're hauled from observing site to site, and back
> home to be "parked" between sessions.
>
> The axes will stayed aligned *with each other*, but not with the rest of
> the universe. So any control system needs provisions to compensate for
> that. And the compensation factors need to be recalculated every time the
> mount is set up.
>
> Meanwhile, unless you can rotate the tube (which is common, I know), the
> error added by collimation movements is constant (for the observing
> session), and can be compensated for by the same system that handles
> errors in polar alignment. If you do rotate the tube, a fairly quick
> recalibration should cancel out the new error constant.
>
> Ran
>
> --
> -----------------------------------------------------------
> ran@netgate.net
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