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Telescope Characteristics |
The characteristics of the
telescope mount and control system are, in general, yet to be established definitively.
The values given here are the requirements and goals
taken from the Science Requirements Document 3.0.
Absolute pointing (driven by the desire to acquire a guide star within the ~5 arcsec instantaneous field of view of the peripheral wavefront sensor):
Recent measurements have produced values of less than 1 arcsec rms (see the results from a recent pointing test).
Open loop tracking is required to be consistent with pointing and sufficiently stable for guide star acquisition.
Slow correction (e.g. of flexure using OIWFS):
Fast correction (e.g. with image motion compensation using PWFS or OIWFS):
Open loop:
Closed loop (e.g. loop closed around peripheral wavefront sensor):
Slewing times:
Last update August 31, 2000; Phil Puxley