Collaboration Case: Autoguider Offset

Description Offsets the telescope position of the given (alpha,delta) step, but without updating the (alpha,delta) values of the actual telescope position as set at the last preset (or rather the last position), i.e. the telescope is moved to the new position but without any update of pointing coordinates: the new physical position is a corrected value for the previous coordinates.
This offset is internally used to correct for telescope pointing errors.
In particular the guiding systems (autoguiding and field stabilization) use this command to correct pointing errors dynamically measured and typically due to wind and athmospheric effects and to minor imperfections in the installed telescope pointing model.
An offset step is always relative to the current position of the telescope (i.e. consecutive steps are accumulated). To issue a new offset, it is not necessary to wait until a previous offset has completed. Consecutive offsets are therefore not lost if one does not exceed the defined performance limits.

Role(s)/Actor(s)
Secondary: Alt/Az Axis

Priority Major

Performance0.5 second

FrequencyAsynchronous, up to 10 Hz

[Design Description
  Entry]

Package Assignment Tracking.

Preconditions

Basic Course

Exception CourseCommand failed

Postconditions

Issues to be Determined or Resolved

Notes:

Last modified: Thu Jun 28 13:59:59 UTC 2001