天文自适应光学:综述

IF 15.7 Q1 OPTICS
Changhui Rao, Libo Zhong, Youming Guo, Min Li, Lanqiang Zhang, Kai Wei
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引用次数: 0

摘要

自 1953 年提出自适应光学(AO)概念以来,AO 已成为以高分辨率观测为目标的大口径地面光学望远镜不可或缺的技术。本文全面回顾了大口径天文光学望远镜(包括夜用和日用太阳光学望远镜)的自适应光学技术进展。重点介绍了激光导星、可变形二次反射镜、极端自动光学观测和多共轭自动光学观测等最新自动光学观测技术的进展。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Astronomical adaptive optics: a review

Astronomical adaptive optics: a review

Since the concept of adaptive optics(AO) was proposed in 1953, AO has become an indispensable technology for large aperture ground-based optical telescopes aimed at high resolution observations. This paper provides a comprehensive review of AO progress for large aperture astronomical optical telescopes including both night-time and day-time solar optical telescopes. The recent AO technological advances, such as Laser Guide Star, Deformable Secondary Mirror, Extreme AO, and Multi-Conjugate AO are focused.

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来源期刊
CiteScore
25.70
自引率
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审稿时长
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