16 July 2008 Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing
Author Affiliations +
Proceedings Volume 7015, Adaptive Optics Systems; 70154S (2008); doi: 10.1117/12.787469
Event: SPIE Astronomical Telescopes + Instrumentation, 2008, Marseille, France
Abstract
The Adaptive Optics Laboratory of the University of Victoria has build a LGS SH-WFS test bench for the Thirty-Meter-Telescope project and its AO system, NFIRAOS. The UVic AOLab has recently shown the ability to track Na profile induced aberrations while correcting for turbulence aberrations. The UVic AOLab has started the second phase of development of its LGS SH-WFS test bench. This next step consists in adding the Truth WFSs into the current bench design and in modeling and implementing the algorithms which blends the data coming from the variousWFSs. This paper shows the various components of the control architecture of NFIRAOS LGS wavefront sensing process. A first simulation shows the stability of the proposed control architecture and demonstrates that the DM is kept away from reproducing the LGS aberrations.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rodolphe Conan, Olivier Lardière, Colin Bradley, Glen Herriot, Kate Jackson, "Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing", Proc. SPIE 7015, Adaptive Optics Systems, 70154S (16 July 2008); doi: 10.1117/12.787469; https://doi.org/10.1117/12.787469
PROCEEDINGS
10 PAGES


SHARE
KEYWORDS
Sodium

Wavefront sensors

Adaptive optics

Charge-coupled devices

Telescopes

Image filtering

Lithium

Back to Top