Quote:
Originally Posted by g__day
You know what I’d like?
<?xml:namespace prefix = o ns = "urn:schemas-microsoft-com http://www.iceinspace.com.au/forum/ ...<P><FONT face=A digital polar alignment scope that works from GPS and compass bearings to allow you to very precisely polar align your scope on a German equatorial mount, without having to look for any stars.
I'm not so much lazy, but I don't have views South or straight up where my scope is mounted, so drift alignment is alot tougher and I'd like a (rentable) digital technology solution!
|
Gary Kopff here from Wildcard Innovations.
As has been noted by "Vermin", magnetic compass technology, whether
electronic or otherwise, is not terriby accurate for these purposes.
As you are also probably aware, a stationary GPS reading will determine
your location but not establish a bearing.
Furthermore, such a hypothetical system, even if it were possinble, is
far from the ideal as it does not take into account the geometric and
flexure errors within your mount/OTA.
What many of the professional observatories do is after having pointed
the telescope through surveying techniques, then perform a star pointing
test and error analysis to determine the polar alignment corrections
necessary. The polar misalignment in azimuth and elevation for the
mount are just two "errors" out of a whole range of possible
errors that impact upon the scope's pointing performance.
Our Argo Navis system employs a similar approach. You devote one
evening and perform a star pointing test on perhaps 50 bright stars
scattered over the whole sky. The system helps you locate them.
You then fit use a feature within the system that alows you to compute
a pointing 'model'. This model consists of the various geometric and
flexure terms within the mount/OTA as well as the two polar
misalignment terms. You then tell the computer to apply
all the terms within the model except the two polar misalignment
terms. You then use the computer to guide you to a familiar bright star.
The star may not be centered in the eypiece but the pointing residual
will be in fact just the polar mis-alignment. You then adjust the scope
in Az and Alt until the star is centered. You mount is now polar aligned.
If your mount is on a pier, you are done.
If the mount is portable, on subsequent nights, you simply set the mount
down and perform a short pointing run on perhaps 4 to 6 stars and have the
system re-compute your polar mis-alignment. You guide to a star and adjust
the mount as before to center the star and you are polar aligned.
As a rule of thumb, the resolution of the fitted encoders dicates the
ultimate resolution by which the mount can be polar aligned.
The beauty of this approach is that it is faster than a drift test, it allows
you to use any bright stars you can observe and unlike a drift test, takes
the other geometric, harmonic and flexure errors into account.
I hope you found the above an interesting insight into the state-of-the-art
in polar alignment assistance. As I mentioned, most large professional
observatories with equatorial mounts employ a similar technique. Howver,
it is also possible to do this within your own back-yard.
Best Regards
Gary Kopff
Managing Director
Wildcard Innovations Pty. Ltd.
20 Kilmory Place
Mount Kuring-Gai NSW 2080
Australia
Phone +61-2-9457-9049
Fax +61-2-9457-9593
sales@wildcard-innovations.com.au
http://www.wildcard-innovations.com.au