A CSO SUBMILLIMETER ACTIVE OPTICS SYSTEM |
Dish Surface Optimization System | |
URSI 2005 Jan. 6, 2005 | |
Melanie Leong |
DSOS Agenda |
Preliminary Specifications | |
99 Channel Dish Surface Optimization System | |
Engineering Challenges / Major Milestones | |
Performance | |
Summary | |
Acknowledgements |
DSOS Preliminary Specifications |
Desired Performance Specifications | ||
+/- 25 micron length change for most of the dish | ||
Reduce RMS surface error from 25 micron RMS to 15 micron RMS | ||
Improve aperture efficiency by a factor of 2, integration time by a factor of 4 | ||
Single Channel Prototype | ||
Determined +/- 25 micron feasibility | ||
Determined design, parts, and materials | ||
3 Toothpick Controller/Driver Prototype demonstrated that desired length changes can be achieved | ||
99 Channel Dish Surface Optimization System requested to build in January 2001 |
DSOS System Diagram |
DSOS Simplified Block Diagram |
DSOS Toothpick Assembly |
DSOS Dish Wiring & Plumbing |
DSOS System Racks |
DSOS 99 Channel Controller Unit |
DSOS 99 Channel Controller Unit (cont.) |
DSOS 25 Channel Driver Unit |
DSOS 25 Channel Driver Unit (cont.) |
DSOS Length Change Capability |
DSOS Performance |
The +/- 25 micron desired capability has been achieved | ||
Power Consumption | ||
Power Draw At Start Up = 4kWatts | ||
Quiescent Power Draw = 840 Watts | ||
Added Weight to Dish - 268 lbs | ||
Approximate Weight of System on 3rd Floor - 1,994 lbs |
DSOS Performance - Feb. 2003 |
DSOS SHARCII - April 2003 |
DSOS - Holography Sept 2002 vs Aug 2003 |
DSOS Holography - April 2004 |
DSOS SHARCII - April 2004 |
DSOS Summary |
The DSOS consistently improves the aperture efficiency of the 10.4-meter Leighton Telescope in the 350 micron wavelength range | |
New detections of weak and/or distant objects with SHARCII and 850 GHz Receiver have been obtained with the help of the DSOS | |
It is a unique active optics system for a unique telescope | |
The DSOS has been in operation since Feb. 2003 | |