Use Case:  Offset Guide Probe on star (Field Stab or Autoguiding  loop closed)

Description This use case is used to make small modifications to the tilt angles of the light beam arriving in the interferometric Laboratory while still being stabilised by the Field Stabilisation (or autoguiding) loop. The offsets shall be given as fixed offsets in the U-V-W site co-ordinate system. They shall be defined as tilt_around_U and tilt_around_W at the output of the M11 (i.e. they are not given in RA,dec and they are not subject to field rotation).
The Guide Probe (FAS guide window or FSS X-Y Table) is moved with a given offset step to a X-Y position while the loop is closed with M6 using the guide star light.
A Combined Offset is not suited for this purpose, because it implies too high time overhead and while it takes place the beam is not stabilized anymore.
This Use Case will be extensively used during VLTI operation (e.g. to optimise the flux injected in the Instrument fibre after each preset.

Role(s)/Actor(s):
Primary: Operator, Maintenance, VLTI-ISS
Secondary:  FSS subsystems,  FAS.

Priority: Major

Performance: Shall be limited by the guide-probe hardware. As a consequence the basic performance requirements are:

Frequency: Asynchronous, maximum 1 per second

[Design Description
  Entry]

Package Assignment Auto Guiding.

Preconditions:

Basic Course:


Exception Course: Command failed

Postconditions:
 

Issues to be Determined or Resolved:

Notes:
Since the FSS is moved with the loop closed, it may be necessary to limit the speed/acceleration of the trajectory to avoid that the loop open. It means that a specific "Set FSS Translation Stage" may be required.

Last modified: Thu Feb 28 10:19:16 UTC 2002