Yu Liu, Xuefei Zhang, Tengfei Song, Mingzhe Sun, Dayang Liu, Jingxing Wang, M. Zhao, Tao Zhang, Fang-Wei Xu, Honglin Fu, Xiao-ping Pi, Shan Huang, Yan Li, Yu Fu, Jian-Bin Fan, Shun-Fang Liu, Yuandeng Shen, Fei Sha, Yuqiang Li, Zhen-yu Jin, Zhong Liu, L. Xia, Hongxin Zhang, Min Huang, Yang Liu, Min Wang, Sha-Sha Li, Jun Lin
{"title":"近空工程50毫米气球日冕仪地面试验","authors":"Yu Liu, Xuefei Zhang, Tengfei Song, Mingzhe Sun, Dayang Liu, Jingxing Wang, M. Zhao, Tao Zhang, Fang-Wei Xu, Honglin Fu, Xiao-ping Pi, Shan Huang, Yan Li, Yu Fu, Jian-Bin Fan, Shun-Fang Liu, Yuandeng Shen, Fei Sha, Yuqiang Li, Zhen-yu Jin, Zhong Liu, L. Xia, Hongxin Zhang, Min Huang, Yang Liu, Min Wang, Sha-Sha Li, Jun Lin","doi":"10.1117/12.2605310","DOIUrl":null,"url":null,"abstract":"We briefly report on the development of a 50 mm balloon-borne coronagraph and its recent ground experiment results made at the high altitude (4800 m above the sea level) site of Mt. Wumingshan in Daocheng, Sichuan of China. The main scientific purpose for developing this coronagraph is to investigate the morphology and dynamics of low-layer coronal structures before and during solar eruptions by observing at a float altitude of about 30 km from 1.08 Rsun to 1.5 Rsun at white light wavelength (centered at 550.0 nm, bandwidth 5 nm). The instrument is an internally occulted Lyot coronagraph developed by Yunnan Observatories in collaboration with Shangdong University (in Weihai) and Changchun Institute of Optics, Fine Mechanics and Physics. The coronagraph was designed with scattered light intensity level of better than 1×10-5 Isun in the inner field of view. A filter wheel system with linear polarizers and an sCMOS camera provided polarization and total brightness images of size 2048 x 2048 pixels. The first successful results were taken on February 27, 2021 in the Daocheng site. This coronagraph experiment obtained coronal images only showing obvious coronal structures very near limb. Furthermore, during the end of March and early April, after improving the polarizer filter system, higher-quality coronal images with pB coronal structures appeared in the full field of view were obtained in our ground-based experiments. Comparison between our results and the other coronal data in the world are discussed. The success of the 50 mm coronagraph in ground experiments is a milestone for us to develop the next-generation large-aperture coronagraph, as well as for future near space projects.","PeriodicalId":236529,"journal":{"name":"International Symposium on Advanced Optical Manufacturing and Testing Technologies (AOMATT)","volume":"30 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Ground experiment of a 50 mm balloon-borne coronagraph for near space project\",\"authors\":\"Yu Liu, Xuefei Zhang, Tengfei Song, Mingzhe Sun, Dayang Liu, Jingxing Wang, M. Zhao, Tao Zhang, Fang-Wei Xu, Honglin Fu, Xiao-ping Pi, Shan Huang, Yan Li, Yu Fu, Jian-Bin Fan, Shun-Fang Liu, Yuandeng Shen, Fei Sha, Yuqiang Li, Zhen-yu Jin, Zhong Liu, L. 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引用次数: 0
摘要
本文简要介绍了50毫米气球日冕仪的研制及其最近在中国四川稻城武明山高海拔(海拔4800米)站点进行的地面试验结果。研制该日冕仪的主要科学目的是通过在白光波长(中心550.0 nm,带宽5 nm)的1.08 ~ 1.5 Rsun范围内约30 km的浮子高度观测,研究太阳爆发前和爆发期间低层日冕结构的形态和动力学。该仪器是由云南天文台与山东大学(威海)和长春光学精密机械与物理研究所合作开发的内掩Lyot日冕仪。日冕仪内部视场散射光强水平优于1×10-5 Isun。采用线性偏光镜和sCMOS相机组成的滤光轮系统,可获得2048 x 2048像素的偏振和总亮度图像。第一次成功的结果于2021年2月27日在稻城站点进行。本实验获得的冠状图像仅显示非常接近肢体的明显冠状结构。此外,在3月底和4月初,在我们的地面实验中,通过改进偏光滤光系统,获得了全视场中出现pB日冕结构的更高质量的日冕图像。并与世界上其他日冕资料进行了比较。50毫米日冕仪在地面实验中的成功,对我们开发下一代大口径日冕仪以及未来的近空间项目具有里程碑式的意义。
Ground experiment of a 50 mm balloon-borne coronagraph for near space project
We briefly report on the development of a 50 mm balloon-borne coronagraph and its recent ground experiment results made at the high altitude (4800 m above the sea level) site of Mt. Wumingshan in Daocheng, Sichuan of China. The main scientific purpose for developing this coronagraph is to investigate the morphology and dynamics of low-layer coronal structures before and during solar eruptions by observing at a float altitude of about 30 km from 1.08 Rsun to 1.5 Rsun at white light wavelength (centered at 550.0 nm, bandwidth 5 nm). The instrument is an internally occulted Lyot coronagraph developed by Yunnan Observatories in collaboration with Shangdong University (in Weihai) and Changchun Institute of Optics, Fine Mechanics and Physics. The coronagraph was designed with scattered light intensity level of better than 1×10-5 Isun in the inner field of view. A filter wheel system with linear polarizers and an sCMOS camera provided polarization and total brightness images of size 2048 x 2048 pixels. The first successful results were taken on February 27, 2021 in the Daocheng site. This coronagraph experiment obtained coronal images only showing obvious coronal structures very near limb. Furthermore, during the end of March and early April, after improving the polarizer filter system, higher-quality coronal images with pB coronal structures appeared in the full field of view were obtained in our ground-based experiments. Comparison between our results and the other coronal data in the world are discussed. The success of the 50 mm coronagraph in ground experiments is a milestone for us to develop the next-generation large-aperture coronagraph, as well as for future near space projects.