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