New Vacuum Solar Telescope Achieves Narrowband Infrared Solar Imaging Observation at He I 10830 A

作     者：Wei-Jie Meng Fang-Yu Xu Zhen-Yu Jin Wei-Jie Meng;Fang-Yu Xu;Zhen-Yu Jin

作者机构：Yunnan ObservatoriesChinese Academy of SciencesKunming 650011China Yunnan Key Laboratory of Solar Physics and Space ScienceKunming 650216China University of Chinese Academy of SciencesBeijing 100049China 

出 版 物：《Research in Astronomy and Astrophysics》 (天文和天体物理学研究（英文版）)

年 卷 期：2024年第24卷第5期

页      面：76-84页

核心收录：

学科分类：07[理学] 070401[理学-天体物理] 0704[理学-天文学] 

基　　金：supported by Yunnan Revitalization Talent Support Program(202305AS350029 and 202305AT350005) Yunnan Key Laboratory of Solar Physics and Space Science(202205AG070009) 

主　　题：instrumentation detectors-instrumentation high angular resolution-Sun chromosphere-Sun infrared 

摘      要：The near-infrared imaging channel constitutes a crucial component of the multichannel high-resolution imaging system of the New Vacuum Solar Telescope(NVST). We have successfully achieved high-resolution, narrowband imaging of the chromosphere using He I 10830 A triplet within this channel, which significantly enhances the imaging observation capabilities of NVST. This paper provides a concise overview of the optical system associated with the near-infrared imaging channel, detailing data processing procedures and presenting several observed images. Leveraging a high-resolution image reconstruction algorithm, we were able to generate a narrowband image near the diffraction limit at 10830 A with a temporal resolution of less than 10 s.