Paper
27 September 2007 MCAO: a case study
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Abstract
Quantifying the results for a multi-conjugate adaptive optics (MCAO) system is more complex than a traditional adaptive optics (AO) system. The complexity of analyzing a MCAO system stems from using multiple deformable mirrors (DMs) and quantifying the influence functions at the wavefront sensor (WFS). In this paper, analysis tools are developed to quantify MCAO performance. Influence functions from two deformable mirrors are propagated to a WFS using CODEV to simulate an MCAO design comparable to the Dunn Solar Telescope (DST). Using MATLAB, the propagated influence functions are mapped to the appropriate field positions, and reconstructor matrices are built using the mapped influence functions. Next, a correctability analysis was performed using theoretical random phase screens. The developed tools are versatile and useful as a system design tool and in a laboratory setting.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jacqueline Roche, Patrick Reardon, Ken Pitalo, Thomas Rimmele, and Kit Richards "MCAO: a case study", Proc. SPIE 6711, Advanced Wavefront Control: Methods, Devices, and Applications V, 67110O (27 September 2007); https://doi.org/10.1117/12.740986
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KEYWORDS
Wavefronts

Adaptive optics

Iterated function systems

Wave propagation

Actuators

Atmospheric propagation

Space telescopes

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