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Proceedings Paper

Testing the pyramid truth wavefront sensor for NFIRAOS in the lab
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Paper Abstract

For today and future adaptive optics observations, sodium laser guide stars (LGSs) are crucial; however, the LGS elongation problem due to the sodium layer has to be compensated, in particular for extremely large telescopes. In this paper, we describe the concept of truth wavefront sensing as a solution and present its design using a pyramid wavefront sensor (PWFS) to improve NFIRAOS (Narrow Field InfraRed Adaptive Optics System), the first light adaptive optics system for Thirty Meter Telescope. We simulate and test the truth wavefront sensor function under a controlled environment using the HeNOS (Herzberg NFIRAOS Optical Simulator) bench, a scaled-down NFIRAOS bench at NRC-Herzberg. We also touch on alternative pyramid component options because despite recent high demands for PWFSs, we suffer from the lack of pyramid supplies due to engineering difficulties.

Paper Details

Date Published: 26 July 2016
PDF: 10 pages
Proc. SPIE 9909, Adaptive Optics Systems V, 99091J (26 July 2016); doi: 10.1117/12.2231838
Show Author Affiliations
Etsuko Mieda, Univ. of Toronto (Canada)
Matthias Rosensteiner, National Research Council Herzberg Astronomy and Astrophysics (Canada)
Maaike van Kooten, Univ. of Victoria (Canada)
Jean-Pierre Veran, National Research Council Herzberg Astronomy and Astrophysics (Canada)
Olivier Lardiere, National Research Council Herzberg Astronomy and Astrophysics (Canada)
Glen Herriot, National Research Council Herzberg Astronomy and Astrophysics (Canada)


Published in SPIE Proceedings Vol. 9909:
Adaptive Optics Systems V
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

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