When there is a significant polar alignment error, dec drift can have a
substantial effect on calibration.
During RA calibration, the camera angle is off since the motion of the star has
a component in the N/S direction in addition to the W motion due to the guide
pulses.
During Dec calibration, the Dec guide rate is off since the motion of the star
has an additional motion in the N/S direction beyond the motion caused by the
guide pulses.
We can correct both of these errors by measuring the N/S displacement at the
end of the W-E calibration and determining the Dec drift rate (px/sec).
For RA, we can use the elapsed time for the W calibration to find the Dec drift
during the W calibration. The camera angle correction, a, we get from sin(a) =
dec_drift/RA_cal_distance.
For Sec, we would use the elapsed time for the N calibration and the measured
drift rate to determine the drift distance. The corrected dec rate is
(dec_distance_pixels + drift_distance) / sum_dec_pulses.
Original issue reported on code.google.com by andy.gal...@gmail.com on 22 Apr 2015 at 3:56
Original issue reported on code.google.com by
andy.gal...@gmail.com
on 22 Apr 2015 at 3:56