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窄带可调谐滤光器在太阳磁场测量中的应用
Application of the tunable narrowband filter in measurements of solar magnetic fields

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王远方舟 1,2,3,4   金振宇 1,5   王希群 1,2,5   戴懿纯 1,5 *  
文摘 磁场测量是太阳科学观测中最重要的一部分,围绕磁场展开的相关研究是太阳物理的研究热点.磁像仪是一种可以进行高分辨磁场观测的精密测量器件,在地基和空间太阳观测中得到了广泛的应用.窄带可调谐滤光器是磁像仪获得窄带光的核心光学部件,其特性会对磁像仪的性能产生影响.滤光器分为两大类,具体可包括4种结构,不同结构具有不同的性能特征,可根据磁像仪的需求进行选择.本文调研了国内外著名地基、球载、空间太阳磁场望远镜,总结了太阳磁像仪中常用的各种窄带可调谐滤光系统的实现方式,滤光器的结构、原理、轮廓特性以及在磁像仪中的应用场景,归纳了不同太阳磁像仪滤光系统的设计特点和关键技术,以期为未来太阳磁像仪滤光系统的研制提供参考.
其他语种文摘 Solar magnetic field observations achieve a precise understanding of the solar activity. Imaging spectropolarimetry obtains the magnetic field strength for the entire field of view simultaneously and spectral samples sequentially. By employing highresolution reconstruction methods, ground-based solar imaging spectropolarimeters are suitable for magnetic field measurements with a high spatial and temporal resolution. The space-borne solar imaging spectropolarimeter has a compact optical path, stable performance, and convenient data processing. Furthermore, it can be used for deep space exploration. Narrowband tunable filters are the primary spectroscopic components of imaging spectropolarimeters for obtaining narrowband light, with various structural forms for different application scenarios from ground to space. Tunable narrowband filters are classified into two categories according to different principles: The Fabry-Perot filter (F-P filter) and the polarization interference filter. The Fabry-Perot filter is divided into two types based on wavelength adjustment methods: Air cavity and lithium niobate. Polarization interference filters are divided into Lyot filters and solid Michelson interferometers according to different beam-splitting structures. Magnetic field measurement using solar imaging spectropolarimetry is a high-precision measurement with strong noise and weak signal. The performance of the narrowband tunable filter determines the accuracy of the spectral transmittance curve, and the filter instability will increase the noise and affect the accuracy of the magnetic field intensity. The narrowband tunable filter, as the most complex component in the optical path of imaging spectropolarimeters, must solve different technical problems in various application scenarios, and the key technology directly affects whether the magnetic image can be obtained. Therefore, how to design the filter system based on different application scenarios is a problem that must be solved for imaging spectropolarimetry to achieve high-precision observation. This paper investigates famous solar spectropolarimeters of ground-based, balloon-borne, and space-borne. Two or three types of filters are used to meet the requirements of different application scenarios. Air-gap F-P filters are characterized by high transmittance, high spectral resolution, and low sidelobe, and they can be applied in the near-infrared band. Its most remarkable advantage is that larger apertures can be manufactured as production technology advances. The stability of this filter is the toughest problem. The filter relies on a calibrated optical path to achieve accurate adjustment even when used on the Coude platform. As a result, the F-P filter requires a relatively stable platform with a large space. It could have a sizable aperture, making it suitable for the next generation of large-aperture ground-based telescopes with a Coude platform. LiNbO_3 F-P filter, solid Michelson interferometer, and Lyot filter have the advantage of stable performance. They are suitable for space-borne, balloon-borne, and other systems with poor mechanical stability. The Lyot filter has excellent stability. Temperature is the only factor that needs to be considered. The surface precision requirements of the Lyot filter are low, whereas those of the solid Michelson and LiNbO_3 F-P filters are high. The LiNbO_3 F-P filter needs to consider the influence of high voltage. The Lyot filter is made of natural crystal, which makes achieving a large aperture difficult. The artificial glass or crystal used in the solid Michelson interferometer and LiNbO_3 F-P filter allows for a larger aperture but places high demands on processing technology. One of China’s 8 m CGST’s scientific goals is to achieve high-precision and high-resolution vector magnetic field measurements in NIR, which requires further development of a large-aperture air-gap F-P filter in NIR.
来源 科学通报 ,2023,68(15):1927-1940 【核心库】
DOI 10.1360/TB-2022-1173
关键词 磁像仪 ; 法珀滤光器 ; 偏振干涉滤光器 ; 太阳望远镜 ; 太阳磁场测量
地址

1. 中国科学院云南天文台, 昆明, 650216  

2. 中国科学院大学, 天文与空间科学学院, 北京, 100049  

3. 云南师范大学, 物理与电子信息学院, 昆明, 650500  

4. 云南省光电信息技术重点实验室, 云南省光电信息技术重点实验室, 昆明, 650500  

5. 云南省太阳物理与空间目标监测重点实验室, 云南省太阳物理与空间目标监测重点实验室, 昆明, 650216

语种 中文
文献类型 研究性论文
ISSN 0023-074X
学科 天文学
基金 国家自然科学基金 ;  云南省科技计划项目
文献收藏号 CSCD:7491110

参考文献 共 106 共6页

1.  季凯帆. 太阳局部高分辨观测像的日球坐标自动标定. 科学通报,2019,64:1738-1746 CSCD被引 1 次    
2.  刘辉. 机器学习在太阳物理中的应用. 中国科学:物理学力学天文学,2019,49:109601 CSCD被引 2 次    
3.  Iglesias F A. Instrumentation for solar spectropolarimetry: State of the art and prospects. Opt Eng,2019,58:1-2 CSCD被引 1 次    
4.  Hale G E. On the probable existence of a magnetic field in sun-spots. J Geophys Res,1908,13:159-160 CSCD被引 4 次    
5.  Hagyard M J. The MSFC vector magnetograph. Sol Phys,1982,80:33-51 CSCD被引 1 次    
6.  Ai G X. Principles of a solar magnetic field telescope. Acta Astron Sin,1986,27:173-180 CSCD被引 9 次    
7.  Ramsay J V. A new tunable filter with a very narrow pass-band. Sol Phys,1970,12:492-501 CSCD被引 1 次    
8.  Denker C. Imaging magnetographs for high-resolution solar observations in the visible and near-infrared wavelength region. Astron Nachr,2003,324:332-333 CSCD被引 4 次    
9.  Rust D M. Vector magnetography. Proceedings of the 11th Sacramento Peak Summper Workshop,1991:74-95 CSCD被引 1 次    
10.  Yang D. A pneumatic axial support prototype of the primary mirror of a 2 m solar telescope. Proceedings Volume 10700, Groundbased and Airborne Telescopes VII,2018:107003U CSCD被引 1 次    
11.  Liu Z. Science cases in the integrated modeling of Chinese giant solar telescope. Proceedings Volume 10012, Integrated Modeling of Complex Optomechanical Systems II,2016:1001204 CSCD被引 1 次    
12.  Dai Y C. Analysis of wavefront reconstruction in 8 meter ring solar telescope. Proceedings Volume 9909, Adaptive Optics Systems V,2016:990940 CSCD被引 1 次    
13.  刘忠. 中国巨型太阳望远镜. 中国科学:物理学力学天文学,2019,49:059604 CSCD被引 4 次    
14.  Liu Y. Progress of site survey for large solar telescopes in western China. Proceedings of the International Astronomical Union,2016:447-449 CSCD被引 1 次    
15.  刘忠. 中国地基大太阳望远镜. 中国科学:物理学力学天文学,2012,42:1282-1291 CSCD被引 9 次    
16.  林元章. 太阳物理导论,2000:70 CSCD被引 3 次    
17.  邓元勇. 太阳磁场探测现状与展望. 红外与激光工程,2020,49:230-236 CSCD被引 2 次    
18.  Stenflo J O. Solar magnetic fields as revealed by Stokes polarimetry. Astron Astrophys Rev,2013,21:66 CSCD被引 6 次    
19.  Wang X. Calibration of a full-disc longitudinal magnetogram at the Huairou Solar Observing Station. Mon Not Roy Astron Soc,2010,402:1166-1176 CSCD被引 2 次    
20.  Jefferies J. Transfer of line radiation in a magnetic field. Astrophys J,1989,343:920-935 CSCD被引 5 次    
引证文献 2 篇

1 王远方舟 基于Lyot滤光器的NVST磁像仪光学系统设计 天文研究与技术,2023,20(5):445-452
CSCD被引 0 次

2 王希群 快速可调谐Lyot滤光器研制及其在一米新真空太阳望远镜上观测 光学学报,2023,43(24):2423001
CSCD被引 0 次

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