Please wait a minute...
Chin. Phys. B, 2017, Vol. 26(8): 089501    DOI: 10.1088/1674-1056/26/8/089501
GEOPHYSICS, ASTRONOMY, AND ASTROPHYSICS Prev  

Error analysis and optimal design of polarization calibration unit for solar telescope

Jun-Feng Hou(侯俊峰), Dong-Guang Wang(王东光), Yuan-Yong Deng(邓元勇), Ying-Zi Sun(孙英姿), Zhi-Yong Zhang(张志勇)
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Abstract  

Polarization calibration unit (PCU) has become an indispensable element for solar telescopes to remove the instrumental polarization; the polarimetric accuracy of calibration depends strongly on the properties of PCU. In the paper, we analyze the measurement errors induced by PCU based on polarized light theory and find that the imperfections of the waveplate generate the main calibration errors. An optimized calibration method is proposed to avoid the effects from waveplate imperfections, and a numerical simulation is given to evaluate the polarization accuracy by analyzing the relation between calibration error and intensity instability. The work is very important for solar telescopes with high polarization precision up to 10-4 Ic.

Keywords:  solar telescope      polarization calibration  
Received:  13 March 2017      Revised:  04 April 2017      Accepted manuscript online: 
PACS:  95.55.Cs (Ground-based ultraviolet, optical and infrared telescopes)  
  95.55.Ev (Solar instruments)  
  95.75.Hi (Polarimetry)  
Fund: 

Project supported by the National Natural Science Foundation of China (Grant Nos. 11403047, 11427901, 11178005, 11373044, 11273034, and 11373042).

Corresponding Authors:  Jun-Feng Hou     E-mail:  jfhou@bao.ac.cn
About author:  0.1088/1674-1056/26/8/

Cite this article: 

Jun-Feng Hou(侯俊峰), Dong-Guang Wang(王东光), Yuan-Yong Deng(邓元勇), Ying-Zi Sun(孙英姿), Zhi-Yong Zhang(张志勇) Error analysis and optimal design of polarization calibration unit for solar telescope 2017 Chin. Phys. B 26 089501

[1] Hale G E 1908 ApJ 28 315
[2] Unno W 1956 PASJ 8 108
[3] Li K W, Wang Z B, Li S W, et al. 2015 Acta Phys. Sin. 64 140702 (in Chinese)
[4] Zhang Z G, Deng F L, Zhang Q C, et al. 2014 Acta Phys. Sin. 63 184204 (in Chinese)
[5] Keil S, Rimmele T, Keller C, et al. 2003 Astron. Nachr. 324 303
[6] Bettonvil F C M, Collados M, Feller A, et al. 2010 Proc. SPIE Ground-based and Airborne Instrumentation for Astronomy III, July 20, 2010, San Diego, California, USA, p. 77356
[7] Liu Z h, Deng Y Y, Ji H S h, et al. 2012 Sci. Sin.-Phys. Mech. Astron. 42 1282
[8] Elmore D 2010 Astron. Nachr. 331 655
[9] Hector S N 2005 J. Opt. Soc. Am. A 22 539
[10] Hector S N 2005 J. Opt. Soc. Am. A 22 907
[11] Yuan S 2014 Solar Polarization 7, September 9-13, 2013, Kunming, China, p. 297
[12] Goode P R, Coulter R, Gorceix N, et al. 2010 Astron. Nachr. 331 620
[13] Beck C, Schmidt W, Kentischer T, et al. 2005 A & A 437 1159
[14] Skumanich A, Lites B W, Pillet V M, et al. 1997 ApJ 110 357
[15] Ichimoto K, Shinoda K, Yamamoto T, et al. 2006 Publ. Natl. Astron. Obs. Japan 8 11
[16] Ichimoto K, Lites B, Elmore D, et al. 2008 Solar Phys. 249 223
[17] Clarke D 2004 J. Opt. A: Pure Appl. Opt. 6 1036
[18] Boulbry B, Jeune B, et al. 2001 Opt. Exp. 9 225
[19] Hou J F, Wang D G, Deng Y Y, et al. 2015 Acta Phys. Sin. 64 060701 (in Chinese)
[1] Irradiation study of liquid crystal variable retarder for Full-disk Magneto-Graph payload onboard ASO-S mission
Jun-Feng Hou(侯俊峰), Hai-Feng Wang(王海峰), Gang Wang(王刚), Yong-Quan Luo(骆永全), Hong-Wei Li(李宏伟), Zhen-Long Zhang(张振龙), Dong-Guang Wang(王东光), Yuan-Yong Deng(邓元勇). Chin. Phys. B, 2020, 29(7): 074208.
No Suggested Reading articles found!