Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing

Details Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing

Aug 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008spie.7093e...3c&link_type=abstract

Advanced Wavefront Control: Methods, Devices, and Applications VI. Edited by Gonglewski, John D.; Carreras, Richard A.; Rhoadar

Statistics

Applications

Scientific paper

The Adaptive Optics Laboratory of the University of Victoria has built 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 of adding the Truth WFSs into the current bench design and of modeling and implementing the algorithms which blend 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.

Affiliated with

Also associated with

No associations

Rating

Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling of the Thirty-Meter-Telescope matched-filter-based LGS wavefront sensing will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1064033