Use
Case: Prepare for Image Alignment
Description:
Prepare the AT subsystems so that they are ready for the VLTI ISS to perform
the VLTI Image Alignment. The main options are:
- use FAS or use FSS,
- use Nasmyth beacon or use Lab source.
Role(s)/Actor(s):
Primary: User (Operator, Maintenance, VLTI-ISS)
Secondary: Coude Beam Switching Device, Nasmyth wheel, FSS Filter Wheel,
Nasmyth Beacon, M6, FSS detector FAS detector
Priority:
Major
Performance:
10
to 15 seconds
Frequency:
Asynchronous,
at least once a day before starting observations and up to once per hour
in worst case, or any time for maintenance/test purpose
Preconditions:
-
Coude Beam switching device is switched On and ONLINE
-
Nasmyth sub-system is switched On and ONLINE
-
FAS sub-system is ONLINE (if selected)
-
FSS sub-system is ONLINE (if selected)
-
M6 is ONLINE
-
ROS shutter is open
Basic
Course:Using Nasmyth Beacon Light Source
-
Send command PREPIAL to prepare for Optical Image Alignment using Nasmyth Beacon Light Source
Exception Course: Command failed
-
ATCS Sets
FSS Filter Wheel to the appropriate ND filter (depending on Beacon
intensity level)
Exception Course: Command failed
-
ATCS Sets
Coude Beam switching device to the free hole (if FSS selected) or to
mirror (if FAS is selected)
Exception Course: Command failed
-
ATCS Sets
Nasmyth Wheel to the position for Nasmyth Beacon
Exception Course: Command failed
-
ATCS Centers
M6
Alternate course: set M6 to "VLTI Coude pointing reference
point"
Exception Course: Command failed
-
ATCS Prepares
FSS Strap for exposures in Closed loop on artificial beacon
Alternate Course: Prepares
FAS Setup to configure FAS exposure (typ. 5s)
Exception Course: Command failed
-
ATCS sets Nasmyth Beacon level
Exception Course: Command failed
-
ATCS switches
On Nasmyth Beacon Light Source
Exception Course: Command failed
-
ATCS returns OK reply
Alternate
Course:Using an external source located inside the VLTI Lab and
the retro-reflecting mirror on the Nasmyth Wheel
-
Send command PREPIAL to prepare for Optical Image Alignment using the retro-reflecting mirror on the Nasmyth Wheel
Exception Course: Command failed
-
ATCS Sets
FSS Filter Wheel to the appropriate ND filter (given by VLTI ISS)
Exception Course: Command failed
-
ATCS Sets
Coude Beam switching device to the free hole (if FSS selected) or to
mirror (if FAS is selected)
Exception Course: Command failed
-
ATCS Sets
Nasmyth Wheel to the Flat Retro-Reflecting Mirror position
Exception Course: Command failed
-
ATCS Centers
M6
Alternate course: set M6 to "VLTI Coude pointing reference
point"
Exception Course: Command failed
-
ATCS Prepares
FSS Strap for exposures in Closed loop on artificial beacon
Alternate Course: Prepares
FAS Setup to configure FAS exposure (typ. 5s)
Exception Course: Command failed
-
ATCS returns OK reply
Exception
Course: Command failed
Postconditions:
-
Devices in appropriate position for Image Alignment
-
ATCS ready to receive Offset Guide Probe Command
Issues
to be Determined or Resolved:
Notes:The Telescope Optical Alignment Configuration could be
a file containing all the settings of the various devices used for the
alignment such as: the ND filter to be used, the light source to be used,
the Nasmyth wheel position, The Coude Beam Switching Device position, etc.
The actual setting of the device shall then be executed in the proper predefined
sequence. It's anyway a good idea to define the parts and their respective
position in a kind of configuration (if it's a file or something else,
implementation issue) Actually similar to the CCD setup files associated
to dedicated commands such as FLAT or STARTAG.
The Alternate course: set M6 to "VLTI Coude pointing reference
point" should indeed be the default (instead of Center M6).
If the reference does not exist, then center M6 should be
used. This command should do the following: i) this retreives the existing
reference point stored in the DB, ii) computes the M6.
What is the position of the Nasmyth wheel for the nasmyth beacon
(tool1, tool2, retro, free)?
Last modified: Thu Jun 28 13:39:43 UTC 2001