Solar adaptive optics systems for the New Vacuum Solar Telescope at the Fuxian Lake Solar Observatory

作者： Lanqiang Zhang ^1,2,3 Xuejun Rao ^1,2 Hua Bao ^1,2 Youming Guo ^1,2,3 Jinsheng Yang ^1,2 Nanfei Yan ^1,2,3 Xian Ran ^1,2,3 Dingkang Tong ^1,2 Xinlong Fan ^1,2 Zhongyi Feng ^1,2 Changhui Rao ^1,2,3
作者单位：

1. National Laboratory on Adaptive Optics, Chengdu 610209, China

2. The Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China

3. University of Chinese Academy of Sciences, Beijing 100049, China
通讯作者： Changhui Rao Email:chrao@ioe.ac.cn
提交时间：2024-04-18 09:18:15

Abstract: Adaptive optics (AO) is essential for high-quality ground-based observations with large telescopes because it counters the impact of wavefront aberrations caused by atmospheric turbulence. The new vacuum solar telescope（NVST） is one of the most important high-resolution solar observation instruments in the world. Three sets of solar adaptive optics systems have been developed and installed on this telescope: conventional adaptive optics, ground layer adaptive optics, and multi- conjugate adaptive optics. These have been in operation from 2018 to 2023. This paper details the development and application of solar adaptive optics on the NVST and discusses the newest instrumentation.

Solar observation Adaptive optics Multi-conjugate adaptive optics

分类： 天文学 >> 天文仪器与技术
投稿状态： 已在期刊出版
引用： ChinaXiv:202404.00382 (或此版本 ChinaXiv:202404.00382V1)
DOI:https://doi.org/10.61977/ ati2024014
CSTR:32003.36.ChinaXiv.202404.00382.V1
推荐引用方式： Lanqiang Zhang,Xuejun Rao,Hua Bao,Youming Guo,Jinsheng Yang,Nanfei Yan,Xian Ran,Dingkang Tong,Xinlong Fan,Zhongyi Feng,Changhui Rao.(2024).Solar adaptive optics systems for the New Vacuum Solar Telescope at the Fuxian Lake Solar Observatory.天文技术与仪器（英文）.doi:https://doi.org/10.61977/ ati2024014 (点此复制)

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2024-04-18 09:18:15

ChinaXiv:202404.00382V1

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