Quote:
Originally Posted by lhansen
So I got one vote for slipping gears - i can check that out. Any other suggestions?
|
Hi Lars,
You can discount slipping gears. It is not that. Otherwise it would have betrayed itself
before the flip.
Have you been sampling stars on both sides of the meridian? Doing a meridian
flip and sampling on the "other" side is absolutely essential.
When you examine the pointing data in the spread sheet interface, you will
see a column for the star's RA and a column for its Dec as well as a column
for the scope's RA and a column for its Dec.
Examine the Dec pointing data for the scope.
Are the
absolute values of the Dec data always in the range 0 to 90 or do
you see some that are in the range 90 to 180 as well?
Once you create a model, you should not be re-syncing on anything as you will
invalidate the model.
Quote:
Originally Posted by Astro_Bot
Cone error ought to be corrected for with 3-star alignment.
|
Alas, life would be simpler if this were true, but it is not.
By the way, "cone error" is a term Chinese mount makers coined in their instruction
manuals. On professional observatories, the preferred description for the Hour Angle
component of any Dec to Optical axes non-perpendicularity is usually Collimation
error in Hour Angle or CH for short. This is also the expression TPoint uses.
GEM's notoriously tend to suffer from CH and it is among the terms that
reverses its direction during a meridian flip. Hence my question to first check that the
pointing data being supplied to TPoint is correctly denoting when the mount
is flipped by the absolute range of Dec values going from 0 to 180 not just
0 to 90.
Once you can confirm that, there are several reasons why CH can commonly occur
but we can pick up the thread from there.