{"title":"Polarization Optical Design of 8-meter Chinese Giant Solar Telescope","authors":"FU Yu , YUAN Shu , JIN Zhen-yu , LIU Zhong","doi":"10.1016/j.chinastron.2023.09.010","DOIUrl":null,"url":null,"abstract":"<div><p><span><span>Instrumental polarization is a vital factor for the accurate measurements of the solar magnetic field. It is necessary to optimize the optical design of the large </span>solar telescope<span><span> to obtain high accuracy solar magnetic field information. In this paper, an optimal design scheme based on four-mirror polarization compensation optics<span> for the 8-meter giant solar telescope is presented. The polarization effect of pupil and field of view are analyzed by the polarization ray tracing programming, the telescope motion and wavelength properties of the field-effect are investigated detailedly. The result shows that, in the </span></span>near infrared<span> waveband which includes the magnetic sensitive spectral lines of He I 1.083 </span></span></span><span><math><mi>μ</mi></math></span>m and Fe I 1.565 <span><math><mi>μ</mi></math></span>m, the polarization-free field size is 0.91<span><math><msup><mrow></mrow><mo>′</mo></msup></math></span>, and the polarization-free field size in the visible band is 0.5<span><math><msup><mrow></mrow><mo>′</mo></msup></math></span>, in which the instrumental polarization of telescope is smaller than <span><math><mrow><mn>2</mn><mo>×</mo><msup><mn>10</mn><mrow><mo>−</mo><mn>4</mn></mrow></msup></mrow></math></span>.</p></div>","PeriodicalId":35730,"journal":{"name":"Chinese Astronomy and Astrophysics","volume":"47 3","pages":"Pages 659-677"},"PeriodicalIF":0.0000,"publicationDate":"2023-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0275106223000619","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
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Abstract
Instrumental polarization is a vital factor for the accurate measurements of the solar magnetic field. It is necessary to optimize the optical design of the large solar telescope to obtain high accuracy solar magnetic field information. In this paper, an optimal design scheme based on four-mirror polarization compensation optics for the 8-meter giant solar telescope is presented. The polarization effect of pupil and field of view are analyzed by the polarization ray tracing programming, the telescope motion and wavelength properties of the field-effect are investigated detailedly. The result shows that, in the near infrared waveband which includes the magnetic sensitive spectral lines of He I 1.083 m and Fe I 1.565 m, the polarization-free field size is 0.91, and the polarization-free field size in the visible band is 0.5, in which the instrumental polarization of telescope is smaller than .
仪器极化是精确测量太阳磁场的重要因素。为了获得高精度的太阳磁场信息,有必要对大型太阳望远镜的光学设计进行优化。本文提出了一种基于四镜偏振补偿光学器件的8米巨型太阳望远镜优化设计方案。利用偏振光线跟踪程序分析了光瞳和视场的偏振效应,详细研究了场效应的望远镜运动和波长特性。结果表明,在包括He I 1.083μm和Fe I 1.565μm磁敏谱线的近红外波段,偏振自由场尺寸为0.91′,可见光波段偏振自由场大小为0.5′,其中望远镜的仪器偏振小于2×10−4。
期刊介绍:
The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.