A high-speed and high-efficiency imaging polarimeter based on ferroelectric liquid crystal retarders: Design and test

被引:0
|
作者
Guo, Jing [1 ,2 ]
Ren, Deqing [3 ]
Zhu, Yongtian [1 ,2 ,4 ]
Zhang, Xi [1 ,2 ]
机构
[1] Chinese Acad Sci, Nanjing Inst Astron Opt & Technol, Natl Astron Observ, Nanjing 210042, Peoples R China
[2] Nanjing Inst Astron Opt & Technol, CAS Key Lab Astron Opt & Technol, Nanjing 210042, Peoples R China
[3] Calif State Univ Northridge, Phys & Astron Dept, Northridge, CA 91330 USA
[4] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
基金
中国国家自然科学基金;
关键词
instrumentation: polarimeters; methods: miscellaneous; Sun: chromosphere; techniques: polarimetric; MAGNETIC-FIELD; SOLAR POLARIMETRY; TELESCOPE; MAGNETOGRAPH;
D O I
10.1093/pasj/psab007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Polarimeters play a key role in investigating solar magnetic fields. In this paper, a High speed and high efficiency Imaging POlarimeter (HIPO) is proposed based on a pair of ferroelectric liquid crystal retarders (FLCs), with the ultimate goal of measuring magnetic fields of prominences and filaments from the ground. A unique feature of the HIPO is that it enables high cadence polarization measurements covering a wide field of view (FOV); the modulation frequency of the HIPO is able to achieve similar to 100 Hz, which greatly suppresses the seeing-induced crosstalk, and the maximum FOV can reach 62 '' x 525 ''. Additionally, FLC retardances under low and high states were calibrated individually and found to have a slight discrepancy, which is neglected in most works. Based on FLC calibration results, an optimization was performed using a constrained nonlinear minimization approach to obtain the maximum polarimetric efficiency. Specifically, optimized efficiencies of the Stokes Q, U, and V are well balanced and determined as (xi(Q), xi(U), xi(V)) = (0.5957, 0.5534, 0.5777), yielding a total efficiency of 0.9974. Their practical efficiencies are measured as (xi(Q)', xi(U)', xi(V)') = (0.5934, 0.5385, 0.5747), slightly below the optimized values but still resulting in a high total efficiency of 0.9861. The HIPO shows advantages in terms of modulation frequency and polarimetric efficiency compared with most other representative ground-based solar polarimeters. In the observations, measurement accuracy is found to be better than 2.7 x 10(-3) by evaluating full Stokes Ha polarimetry results of the chromosphere. This work lays a foundation for the development of high-speed and high-accuracy polarimeters for our next-generation solar instruments.
引用
收藏
页码:405 / 416
页数:12
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