Laser guide star simulations for 8-m class telescopes

被引：4

作者：

Delplancke, F ^{[1
]}

Carbillet, M ^{[1
]}

Hubin, N ^{[1
]}

Esposito, S ^{[1
]}

Rigaut, F ^{[1
]}

Marchetti, E ^{[1
]}

Riccardi, A ^{[1
]}

Viard, E ^{[1
]}

Ragazzoni, R ^{[1
]}

Le Louarn, M ^{[1
]}

Fini, L ^{[1
]}

机构：

[1] ESO, D-85748 Garching, Germany

来源：

ADAPTIVE OPTICAL SYSTEM TECHNOLOGIES, PARTS 1 AND 2 | 1998年 / 3353卷

关键词：

adaptive optics; laser guide star; atmospheric perturbations; wavefront sensing; cone effect; atmospheric tomography;

D O I：

10.1117/12.321625

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

We describe in this paper the development of a simulation tool for modeling any kind of adaptive optic system with laser guide star within the framework of the European network Laser Guide Star for 8-m Class Telescopes. This is intended to support investigations about laser guide stars problems like cone effect and tip-tilt determination. The different kind of software modules to be developed are listed and the libraries already distributed among the network are described: phase screen generation (with fast Fourier transform and Zernike methods), downward propagation (for natural and laser guide stars), wavefront sensing and reconstruction (with Shack-Hartmann and curvature sensor of various geometries). The future studies for serving the cone effect are also presented.

引用

页码：371 / 382

页数：12

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