Xu Chenglin, Qu Zhongquan, Zhang Xiaoyu, Jin Chunlan, Yan Xiaoli
National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming, 650011 Yunnan, China.
Appl Opt. 2006 Nov 20;45(33):8428-33. doi: 10.1364/ao.45.008428.
A polarimeter to be mounted on the Yunnan solar tower is described. It features the ability to simultaneously measure the magnetic fields of the solar photosphere and chromosphere by analyzing the Stokes spectra of those magnetosensitive lines forming in the two regions with very high efficiency of polarization measurement. The polarimeter consists of two ferroelectric liquid crystals and one lambda/4 wave plate before a polarizing beam splitter. The achromatism of the design is emphasized to get the maximum combination efficiency over a spectral range from 5000 to 6000 A. For the used solar absorption lines MgI517.27, FeI525.06, FeI630.15, and FeI630.25 nm, the design gives theoretical efficiencies of polarization measurements, which are 0.999, 1.0, 0.943, and 0.943, respectively. A comparison with other reference polarimeters, such as the Synoptic Optical Long-term Investigation of the Sun, the Tenerife infrared polarimeter, and the La Palma Stokes Polarimeter, is carried out.
本文描述了一种将安装在云南太阳塔上的偏振计。它能够通过分析在太阳光球层和色球层形成的那些磁敏线的斯托克斯光谱,以非常高的偏振测量效率同时测量这两个区域的磁场。该偏振计由两块铁电液晶和一块位于偏振分束器之前的λ/4波片组成。设计强调了消色差特性,以便在5000至6000埃的光谱范围内获得最大的组合效率。对于所使用的太阳吸收线MgI517.27、FeI525.06、FeI630.15和FeI630.25纳米,该设计给出的偏振测量理论效率分别为0.999、1.0、0.943和0.943。还与其他参考偏振计进行了比较,如太阳的综合光学长期观测、特内里费岛红外偏振计和拉帕尔马岛斯托克斯偏振计。