天文学进展2024，Vol.42Issue(4)：594-617,24.DOI:10.3969/j.issn.1000-8349.2024.04.03
大气对望远镜像质影响的测量和计算方法进展
Progress in Measurement and Calculation Methods of Atmospheric Effects on Telescope Image Quality
摘要
Abstract
The degradation of telescope image quality caused by atmospheric turbulence is currently an important factor restricting the high-resolution observation capability of ground-based astronomical telescopes.Measuring and calculating the effect of the atmo-sphere on telescope image quality is an important research direction in the field of astro-nomical technology.Firstly,the theoretical basis for measuring the effect of the atmosphere on image quality using optical and non-optical methods was elaborated,and representative technical routes,measurement results,and research progress of the two measurement meth-ods were presented.The advantages and disadvantages of these measurement methods were analyzed in depth.Then,the basic principles and applicable ranges of three methods for calculating the effect of the telescope's internal airflow on the image quality of telescopes were summarized,and the advantages and disadvantages of these calculation methods were analyzed in depth.Finally,the technical characteristics of optical and non-optical measure-ment methods and computational methods were summarized,and an outlook on the future development direction of calculation methods was provided.关键词
地基天文望远镜/视宁度/Kolmogorov湍流/波前像差Key words
ground-based astronomical telescope/seeing/kolmogorov turbulence/wave-front error分类
天文与地球科学引用本文复制引用
黄善杰,赵劲松,许方宇,王岭雪,宋腾飞,蔡毅..大气对望远镜像质影响的测量和计算方法进展[J].天文学进展,2024,42(4):594-617,24.基金项目
国家自然科学基金(U1931124) （U1931124）
云南省自然科学基金(202401AT070140) （202401AT070140）
