11 September 1998 UnISIS: a laser-guided adaptive optics system for the Mt. Wilson 2.5-m telescope
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Abstract
Final design details are given for UnISIS, the University of Illinois Seeing Improvement System. The principle components include a 50 Watt Excimer laser working at 351 nm which produces a pulsed Rayleigh laser guide star at 333 Hz and 18 km altitude, a 177-actuator deformable mirror, an atmospheric dispersion correction system, and a science camera configuration with both visual and near-IR cameras that can be used simultaneously. Two high-speed CCD cameras are used to feed dual quad C40 DSP-based reconstructor to close the feedback loop with the deformable mirror. The adaptive optics system is situated on a large optics table that rests above the old Coude spectrograph of the Mt. Wilson 2.5-m telescope and the Excimer laser is located in a basement Coude room.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Laird A. Thompson, Laird A. Thompson, Richard M. Castle, Richard M. Castle, Scott W. Teare, Scott W. Teare, Peter R. McCullough, Peter R. McCullough, Samuel L. Crawford, Samuel L. Crawford, } "UnISIS: a laser-guided adaptive optics system for the Mt. Wilson 2.5-m telescope", Proc. SPIE 3353, Adaptive Optical System Technologies, (11 September 1998); doi: 10.1117/12.321707; https://doi.org/10.1117/12.321707
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