Deformable mirrors for open-loop adaptive optics

被引：8

作者：

Kellerer, A. ^{[1
]}

Vidal, F. ^{[1
]}

Gendron, E. ^{[1
]}

Hubert, Z. ^{[1
]}

Perret, D. ^{[1
]}

Rousset, G. ^{[1
]}

机构：

[1] Univ Paris Diderot, UPMC, CNRS, LESIA,Observ Paris, F-92190 Meudon, France

来源：

ADAPTIVE OPTICS SYSTEMS III | 2012年 / 8447卷

关键词：

adaptive optics; deformable mirrors; open-loop command;

D O I：

10.1117/12.925555

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

We characterize the performance of deformable mirrors for use in open-loop regimes. This is especially relevant for Multi Object Adaptive Optics (MOAO), or for closed-loop schemes that require improved accuracies. Deformable mirrors are usually characterized by standard parameters, such as influence functions, linearity, hysteresis, etc. We show that these parameters are insufficient for characterizing open-loop performance and that a deeper analysis of the mirror's behavior is then required. The measurements on the deformable mirrors were performed in 2007 on the AO test bench of the Meudon observatory, SESAME.

引用

页数：12

共 10 条

[1]

Andersen D. R., 2008, P SPIE, V7015

[2]

Cuby J., 2010, P SPIE, V7735

[3] MOAO first on-sky demonstration with CANARY [J].

Gendron, E. ;

Vidal, F. ;

Brangier, M. ;

Morris, T. ;

Hubert, Z. ;

Basden, A. ;

Rousset, G. ;

Myers, R. ;

Chemla, F. ;

Longmore, A. ;

Butterley, T. ;

Dipper, N. ;

Dunlop, C. ;

Geng, D. ;

Gratadour, D. ;

Henry, D. ;

Laporte, P. ;

Looker, N. ;

Perret, D. ;

Sevin, A. ;

Talbot, G. ;

Younger, E. .

ASTRONOMY & ASTROPHYSICS, 2011, 529

[4]

Gendron E., 2010, P SPIE, P7736

[5]

GUZMAN D, 2008, P SPIE, V7015

[6] ZERNIKE POLYNOMIALS AND ATMOSPHERIC-TURBULENCE [J].

NOLL, RJ .

JOURNAL OF THE OPTICAL SOCIETY OF AMERICA, 1976, 66 (03) :207-211

[7]

PUECH M, 2005, P SOC PHOTO-OPT INS, V5903, P272

[8]

Sechaud M., 1999, ADAPTIVE OPTICS ASTR

[9]

ZAMKOTSIAN F, 2007, P SPIE, V6467

[10]

Zamkotsian F., 2006, P SPIE, V6272

← 1 →