Multi-Conjugate Adaptive Optics with Two Deformable Mirrors – Requirements and Performance

被引:1
作者
Thomas Berkefeld
Andreas Glindemann
Stefan Hippler
机构
[1] Kiepenheuer-Institut für Sonnenphysik,
[2] European Southern Observatory,undefined
[3] Max-Planck-Institut für Astronomie,undefined
来源
Experimental Astronomy | 2001年 / 11卷
关键词
adaptive optics; laser guide stars; multi-conjugate adaptive optics; turbulent layers;
D O I
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中图分类号
学科分类号
摘要
In order to increase the corrected field of view of an adaptive optics (AO) system, several deformable mirrors (DM) have to be placed in the conjugate planes of the dominant turbulent layers (multi-conjugate adaptive optics,MCAO (Beckers, 1988)).The performance of MCAO systems depends on the quality of thewavefront sensing ofthe individual layers and on the number of corrected modes in eachindividual layer as in single layer AO systems. In addition, the increase in corrected field of view depends on the number of guide stars providing information about theturbulence over a sufficiently large area in each turbulent layer. In this article, we investigate these points and provide formulae for calculating the increased field of view with a new approach using the spatial correlation functions of the appliedpolynomials (e.g. Zernike). We also present a new scheme of measuring the individual wavefront distortion of each of the dominantlayers with a Shack-Hartmann-Curvature Sensor using gradientinformation as well as scintillation. An example for the performance of a two layer MCAO system is given for the 3.5-m telescope of the Calar Alto Observatory, Spain, using ameasured Cn2-profile. The corrected field of view in K-band(2.2 μm) can be as large as 3 arcmin with a Strehl ratio above 60%.
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页码:1 / 21
页数:20
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