Wavefront sensing and control for a segmented primary mirror

Dong Bing*, Yu Xina, Zhang Xiaofang, Guo Baiwei, Zhao Lei

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

1 Citation (Scopus)

Abstract

Large-aperture segmented primary mirror has been widely used in high-resolution space telescopes. In this paper, we concentrate on the wavefront sensing and control (WFS&C) methods for a segmented primary mirror comprising a central octagon and eight surrounding petals. As the wavefront errors have a wide dynamic range in amplitude and spatial frequency, a multistage wavefront control algorithm is proposed. The control process is divided to five steps to reduce the wavefront errors gradually. A simulation toolbox integrating multi-disciplinary software has been developed to verify our WFS&C algorithms. Simulation results give a good demonstration of the feasibility of our algorithms.

Original languageEnglish
Title of host publicationAdaptive Optics Systems
DOIs
Publication statusPublished - 2008
EventAdaptive Optics Systems - Marseille, France
Duration: 23 Jun 200826 Jun 2008

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume7015
ISSN (Print)0277-786X

Conference

ConferenceAdaptive Optics Systems
Country/TerritoryFrance
CityMarseille
Period23/06/0826/06/08

Keywords

  • Adaptive optics
  • High-resolution space telescope
  • Integrated analysis
  • Segmented primary mirror
  • Simulation
  • Spatial frequency
  • Wavefront sensing and control

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