25 October 2004 Design of ground-layer turbulence compensation with a Rayleigh beacon
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The adaptive optics instrument for the SOAR 4.1-m telescope will improve the spatial resolution by 2-3 times at visible wavelengths, over a field of 3 arcmin, by sensing and correcting low-altitude turbulence selectively. We will use a Rayleigh laser guide star to accomplish this. We present the laser guide star design with predictions of system performance based on real turbulence statistics and telescope properties, sky coverage and some opto-mechanical aspects of the AO module. Various design trade-offs are discussed.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrei Tokovinin, Andrei Tokovinin, Sandrine Thomas, Sandrine Thomas, Brooke Gregory, Brooke Gregory, Nicole van der Bliek, Nicole van der Bliek, Patricio Schurter, Patricio Schurter, Rolando Cantarutti, Rolando Cantarutti, Eduardo Mondaca, Eduardo Mondaca, } "Design of ground-layer turbulence compensation with a Rayleigh beacon", Proc. SPIE 5490, Advancements in Adaptive Optics, (25 October 2004); doi: 10.1117/12.550053; https://doi.org/10.1117/12.550053


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