Astronomical Adaptive Optics

doi:10.1086/684512

2015-12-01

PRE

Rigaut, Francois *

DOI：10.1086/684512

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摘要

En 中文

Adaptive optics is now a fully mature technique to improve the angular resolution of observations taken with ground-based astronomical telescopes. It is available at most of the major optical/IR observatories, and is planned as an integral part of the Extremely Large Telescope next generation facilities. In this mini-review aimed at non-AO specialists, we recall the history, the principle of operation, the major components, the performance, and the future of nighttime astronomical adaptive optics.

Keyword:

LASER-GUIDE-STAR

GROUND-LAYER

BLACK-HOLE

HR 8799

TELESCOPE

SYSTEM

PERFORMANCE

RECONSTRUCTION

IMPROVEMENT

CLUSTER

期刊

Publications of the Astronomical Society of the Pacific

IF:

7.7

论文数:

4.0K

被引数:

1.8W

机构

Australian National University

学者数:

2.1W

论文数: 2.3W

被引数: 3.9W

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