用于Sunrise -3的日出色球红外分光偏振计(SCIP):偏振调制单元

M. Kubo, T. Shimizu, Y. Katsukawa, Y. Kawabata, T. Anan, K. Ichimoto, K. Shinoda, T. Tamura, Y. Nodomi, S. Nakayama, Takuya Yamada, T. Tajima, Shimpei Nakata, Yoshihito Nakajima, Kousei Okutani, A. Feller, J. C. D. T. Iniesta
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引用次数: 6

摘要

高精度的太阳色球线偏振测量是当前和未来太阳望远镜了解色球层磁场结构的关键。日出三号的日出色球红外分光偏振仪(SCIP)是一种偏振精度为0.03% (1 σ)的分光偏振仪。利用SCIP进行高精度偏振测量的关键是一个以恒定速度连续旋转波片的偏振调制单元。旋转机构为原为未来航天任务研制的直流无刷电机,其控制逻辑原为探空火箭实验CLASP研制。由于我们对旋转速度(0.512秒/旋转)的要求比CLASP快10倍,因此我们优化了控制逻辑以满足所需的更快旋转。快速极化调制对于研究与动态色球现象相关的精细磁场结构是必不可少的。通过对日出三号气球飞行环境的模拟,验证了旋转性能可以达到SCIP要求的0.03% (1 σ)的极化精度,并且在热真空条件下仍能保持这种显著的旋转性能。波片设计为石英和蓝宝石双折射片,在较宽的波长范围内实现恒定的延迟。我们已经证实,在工作温度条件下,SCIP在770 nm和850nm波长范围内的延迟几乎是恒定的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Sunrise Chromospheric Infrared spectroPolarimeter (SCIP) for SUNRISE-3: polarization modulation unit
Polarization measurements of the solar chromospheric lines at high precision are key to present and future solar telescopes for understanding magnetic field structures in the chromosphere. The Sunrise Chromospheric Infrared spectroPolarimeter (SCIP) for Sunrise III is a spectropolarimeter with a polarimetric precision of 0.03 % (1 σ). The key to high-precision polarization measurements using SCIP is a polarization modulation unit that rotates a waveplate continuously at a constant speed. The rotating mechanism is a DC brushless motor originally developed for a future space mission, and its control logic was originally developed for the sounding rocket experiment CLASP. Because of our requirement on a speed of rotation (0.512 s/rotation) that was 10 times faster than that of CLASP, we optimized the control logic for the required faster rotation. Fast polarization modulation is essential for investigating the fine-scale magnetic field structures related to the dynamical chromospheric phenomena. We have verified that the rotation performance can achieve the polarization precision of 0.03 % (1 σ) required by SCIP and such a significant rotation performance is maintained under thermal vacuum conditions by simulating the environment of the Sunrise III balloon flight. The waveplate was designed as a pair of two birefringent plates made of quartz and sapphire to achieve a constant retardation in a wide wavelength range. We have confirmed that the retardation is almost constant in the 770 nm and 850nm wavelength bands of SCIP under the operational temperature conditions.
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