Calibration of NAOS and CONICA static aberrations - Application of the phase diversity technique

被引:65
作者
Blanc, A
Fusco, T
Hartung, M
Mugnier, LM
Rousset, G
机构
[1] Off Natl Etud & Rech Aerosp, Dept Opt Theor & Appl, F-92322 Chatillon, France
[2] Ecole Super Elect, Signaux & Syst Lab, F-91192 Gif Sur Yvette, France
[3] Max Planck Inst Astron, D-69117 Heidelberg, Germany
来源
ASTRONOMY & ASTROPHYSICS | 2003年 / 399卷 / 01期
关键词
instrumentation : adaptive optics;
D O I
10.1051/0004-6361:20021655
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe and evaluate the performance of a phase diversity wavefront sensor used to measure the static aberrations of the VLT instrument NAOS-CONICA. The main limitations of this phase diversity technique are compiled. We investigate the systematic errors due to the experimental implementation and the design restrictions. Further error sources stem from the imperfect knowledge of the system, and from limitations of the algorithm. The influence of these errors on the wavefront estimation is evaluated on numerical and experimental data. This study highlights the essential verifications and calibrations needed to obtain accurate results and gives a practical guideline for the application of a phase diversity wavefront sensor. The comprehensive calibration results and the final gain in optical performance are presented and discussed in a complementary paper (Hartung et al. 2003).
引用
收藏
页码:373 / 383
页数:11
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