prima star separators françoise delplancke, frédéric derie tno-tpd team (jan niejenhuis)
Post on 21-Dec-2015
216 views
TRANSCRIPT
PRIMAStar Separators
Françoise Delplancke, Frédéric Derie
TNO-TPD team (Jan Niejenhuis)
Specifications UT and AT• 2’ diameter FoV, unlimited access• 2x 2” sub-fields• 80 mm output beams• Symmetry
– Full symmetry for the ATs, including w.r.t. light ducts– Inherent slight dissymmetry for the UTs
• Integrated metrology end-point (AT)• Independent control of image and pupil positions at 10 Hz • Chopping in pupil plane• Pupil relay• No OPD introduced when tracking• No transmissive element (10µm)• High eigen-frequencies
STS for the ATs: constraints
• Very limited volume (cylinder of ø ~1m)
• Low thermal dissipation
• Good thermal stability (0 to 15ºC)
• Complex interface with the AT:– Has to mimic the current one (electrical/mechanical I/F)– Has to be transparent for the current software– Exchange of single-feed / dual-feed ROS has to be:
• Simple (limited manned operation)
• Reproducible (within 0.1mm / 1’)
• Without need of a significative STS realignment (automatic alignment check and correction is foreseen)
STS for the ATs: concept (1)
STS for the ATs: concept (2)
STS for the UTs: constraints
• No derotator but full sky coverage
• Mechanical interface – with existing supporting towers – without affecting MACAO
• Possibility of using the currently installed single-feed facility– without affecting the alignment– with a minimum of manned operations
• Adapted to alignment tools
• As similar as possible to the STS-AT concept
STS for the UTs: concept (1)
STS for UTs: concept (2)
Tip-tilt mechanisms
• In pupil / in focal plane• Rotation around vertex =>
no OPD introduced• Hinge mechanism• Fast response time:
– 100Hz first eigenfrequency
– 10ms to send command (could be improved if needed)
– 10ms to reach position
– => 50Hz actuation frequency
QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.
Mechanism performances