In this paper, we briefly describe the principle of analytical modelization of the adaptive optics (AO) corrected point spread function in the spatial frequency domain, both for the turbulent and the telescope static aberrations, and demonstrate how this can be used for simulating AO corrected phase screens on extremely large hexagonal segmented telescopes, required for performance analysis of diffraction limited coronagraphs.
Titre
Spatial frequency analytical modeling of adaptive optics for diffraction limited coronagraphs studies on extremely large segmented telescopes
Date
2006-10
Publié dans
EAS Publications Series
Volume
2006, vol. 22, pp. 151-164
Pagination
14 p.
ISSN
1633-4760
Type d'article
scientifique
Domaine
Ingénierie et Architecture
Ecole
HEIG-VD
Institut
iAi-Institut d'Automatisation Industrielle
Note
JOLISSAINT, Laurent est chercheur à la HES-SO, HEIG-VD, depuis 2013.