Adaptive optics at Lick Observatory: System architecture and operations
- and others
We will describe an adaptive optics system developed for the 1 meter Nickel and 3 meter Shane telescopes at Lick Observatory. Observing wavelengths will be in the visible for the 1 meter telescope and in the near IR on the 3 meter. The adaptive optics system design is based on a 69 actuator continuous surface deformable mirror and a Hartmann wavefront sensor equipped with an intensified CCD framing camera. The system has been tested at the Cassegrain focus of the 1 meter telescope where the subaperture size is 12.5 cm. The wavefront control calculations are performed on a four processor single board computer controlled by a Unix-based system. We will describe the optical system and give details of the wavefront control system design. We will present predictions of the system performance and initial test results.
- Research Organization:
- Lawrence Livermore National Lab., CA (United States)
- Sponsoring Organization:
- USDOE, Washington, DC (United States)
- DOE Contract Number:
- W-7405-ENG-48
- OSTI ID:
- 10154688
- Report Number(s):
- UCRL-JC-115106; CONF-940391-8; ON: DE94012387
- Resource Relation:
- Conference: Society of Photo-Optical Instrumentation Engineers (SPIE) conference,Kona Beach, HI (United States),13-18 Mar 1994; Other Information: PBD: Mar 1994
- Country of Publication:
- United States
- Language:
- English
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