论文标题
太阳能磁性活性研究望远镜在HIDA天文台的串联仪表板的极化校准
Polarization calibration of the Tandem Etalon Magnetograph of the Solar Magnetic Activity Research Telescope at Hida Observatory
论文作者
论文摘要
串联eTalon磁力仪(TEM)是HIDA天文台的太阳能磁性活性研究望远镜的工具之一。 TEM是部分磁盘(320“ x240”)滤光片,该滤光片在6303 Angstrom处的Fe I线周围扫描波长,并且对于每个波长而言,占地敏感性<5x10^-4。为了获得仪器的偏振计响应矩阵,我们进行了仪器的端到端极化校准。我们还测量了极化束分离器(PBS)的极化特性,该特性是该仪器的关键组成部分。由于端到端校准的结果,我们发现整个视野响应矩阵的显着空间变化。通过实验室测试,我们发现PBS圆形扭曲的幅度的1%是由于立方体中的压力和膜的线性扭曲引起的延迟。尽管整个视野的空间变化大于十倍以上,以达到偏振灵敏度<5x10^-4,但可以通过PBS的极化特征很好地解释,并使用端到端校准中获得的响应矩阵进行校正。此外,我们还获得了TEM的极化特性的每日变化。我们发现,从Stokes Q到V的串扰会改变与一天的公差相当的数量。在当前的配置中,我们需要每100分钟进行像素校准的像素校准,以满足准确性要求。
The Tandem Etalon Magnetograph (TEM) is one of the instruments of the Solar Magnetic Activity Research Telescope of Hida Observatory. The TEM is a partial disk (320" x240") filter magnetograph which scans the wavelength around a Fe I line at 6303 angstrom and achieves polarimetric sensitivity of < 5x10^-4 for each wavelength. To obtain the polarimeter response matrix of the instrument, we have carried out end-to-end polarization calibrations of the instrument. We have also measured the polarization characteristics of the polarization beam splitter (PBS), which is a crucial component of the instrument. As a result of end-to-end calibration, we found significant spatial variation in the response matrix across the field of view. From a laboratory test, we found that 1% of the magnitude of a circular diattenuation of the PBS was due to the retardation caused by the stress in the cube and the linear diattenuation of the film. Although the spatial variation across the field of view is more than ten times larger, to achieve the polarimetric sensitivity of < 5x10^-4, this can be well explained by the polarization characteristic of the PBS and corrected by using the response matrix obtained in the end-to-end calibration. In addition, we also obtained the daily variation of the polarization property of the TEM. We found that the crosstalk from Stokes Q to V changes an amount comparable to the tolerance through a day. In the present configuration, we require a pixel-by-pixel calibration every 100 minutes to meet the accuracy requirement.