HARMONI at ELT: a telescope simulator for laser tomographic AO

被引:0
|
作者
Salyy, G. De Saint [1 ]
Dohlen, K. [1 ]
Jouye, P. [1 ]
Costale, A. [1 ]
El Hadi, K. [1 ]
Neichel, B. [1 ]
机构
[1] Aix Marseille Univ, CNRS, CNES, Lab Astrophys Marseille,UMR 7326, F-13388 Marseille, France
来源
ADAPTIVE OPTICS SYSTEMS VIII | 2022年 / 12185卷
基金
欧盟地平线“2020”;
关键词
ELT; Adaptive Optics; Telescope Simulator; SLM;
D O I
10.1117/12.2629301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450nm to 2450nm with resolving powers from 3500 to 18000 and spatial sampling from 60mas to 4mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The project is preparing for Final Design Reviews. The AO wavefront sensor modules are assembled and tested in Marseille, requiring a large telescope simulator for realistic projection of various guide objects into the system. This is particularly challenging for the six laser guide stars, whose partially overlapping beams converge to a focus several meters behind the instrument entrance focus. To avoid building a well-corrected, meter-sized, optical system for this task, a single large lens is employed, associated with source modules individually equipped with spatial light modulators (SLM) capable both of simulating the atmosphere and the telescope's deformable mirror (M4) and of compensating the aberrations inherent to the simple simulator optics. In this paper, we present preliminary optical designs for the telescope simulator and the source units. We also describe prototype work, associated with theoretical analysis, to demonstrate the SLM's capabilities for generating sufficiently large aberrations.
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页数:11
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