2. The adjustment principle is self-collimation, which is determined by the structural design of the instrument. It can be called semi-tuning or semi-tuning.
3. No problem. Adjusting the optical axis of the telescope does not mean that the stage is horizontal. If the flat mirror is placed in different positions on the stage, the returned image may not be consistent with the adjusted alignment line.
But there is no problem with the telescope at this time.