Paper
11 July 2018 Design of a laser guide star wavefront sensor system for NFIRAOS
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Abstract
The application of phase diversity is first invested in simulation to characterize ideal parameters to GPI with faithfully simulated calibration source data. The best working simulation parameters are applied to real GPI data and shown to recover an injected astigmatism. The estimated GPI NCPA are then corrected and the Strehl ratio is improve by ⇠ 5%, although the application is rudimentary and a more thorough correction will be applied in the near future.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jeffrey Crane, Jenny Atwood, David Andersen, Peter Byrnes, Glen Herriot, and Jean-Pierre Véran "Design of a laser guide star wavefront sensor system for NFIRAOS", Proc. SPIE 10703, Adaptive Optics Systems VI, 107033L (11 July 2018); https://doi.org/10.1117/12.2314312
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Interfaces

Mirrors

Sodium

Laser guide stars

Telescopes

Wavefront sensors

Adaptive optics

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