偏振风成像干涉仪多波长探测理论研究

朱化春; 张淳民

doi:10.7498/aps.60.074211

摘要

简述了偏振风成像干涉仪(PAMI)探测高层大气风场的基本原理;研究得出了多波长探测时偏振风成像干涉仪干涉强度、仪器调制度与位相延迟片的延迟位相之间的理论表达式;得出了偏振风成像干涉仪的干涉强度和仪器调制度受所探测谱线波长调制的重要结论;采用计算机模拟分析了使用偏振风成像干涉仪(设计谱线为高层大气氧原子跃迁时辐射的630nm的极光谱线)探测高层大气时各目标谱线的干涉强度和仪器调制度,给出了干涉强度和仪器调制度与探测谱线波长之间的关系,得出了732nm的极光谱线不适合用作探测目标的结论. 本文为高层大气风场探

关键词:

Abstract

The basic principle of measuring the upper atmosphere using the polarization atmosphere Michelson interferometer (PAMI) is briefly described. The relationships between the intensity and the visibility of the PAMI and the Delayed phase of the wave plate are presented. The visibility and the intensity of the PAMI are dependent on the wavelength of spectral line, showing that the 732nm line is inapplicable for measuring spectral line if the PAMI is designed specifically for the 630 nm line. The research provides a theoretical basis and practical guidance both for the theoretical study of polarization atmosphere Michelson interferometer and for the design and development of the new polarization atmosphere Michelson interferometer.

Keywords:

upper atmosphere measurement /
polarization atmosphere Michelson interferometer /
visibility /
measurement with multi wavelength

作者及机构信息

1.
西安交通大学理学院,非平衡物质结构及量子调控教育部重点实验室,西安 710049

基金项目: 国家自然科学基金重点项目(批准号:40537031),国家高技术研究发展计划863项目(批准号:2006AA12Z152),国防基础科学研究项目(批准号:A1420080187)和国家自然科学基金(批准号:40875013,40375010,60278019)资助的课题.

Authors and contacts

1.
School of Science, Xi'an Jiaotong University, Non-equilibrium Condensed Matter andQuantum Engineering Laboratory, the Key Laboratory of Ministry of Education, Xi'an 710049, China

参考文献

[1]	Zhang C M, Zhao B C, Xiang L B 2004 Appl. Opt. 33 6090
[2]	Zhang C M, Xiang L B, Zhao B C 2004 J. Opt. A: Pure Appl. Opt .8 815
[3]	Zhang C M, Xiang L B, Zhao B C 2002 Opt. Commun. 1-2 21
[4]	Zhang C M, Zhao B C, Xiang L B 2003 Opt. Commun. 4-6 221
[5]	Wu L, Zhang C M, Zhao B C 2007 Opt. Commun. 1 67
[6]	Jian X H, Zhang C M, Zhao B C 2007 Acta Phys. Sin. 56 824(in Chinese) [简小华、张淳民、赵葆常 2007 56 824]
[7]	Yuan Z L, Zhang C M, Zhao B C 2007 Acta Phys. Sin. 12 6413(in Chinese) [袁志林、张淳民、赵葆常 2007 56 6413]
[8]	Peng Z H, Zhang C M Zhao B C, Li Y C, Wu F Q 2006 Acta Phys. Sin. 55 6374(in Chinese) [彭志红、张淳民、赵葆常、李英才、吴福全 2006 55 6374]
[9]	Jian X H, Zhang C M, Zhu B H, Zhao B C, Du J 2008 Acta Phys. Sin. 57 7565(in Chinese) [简小华、张淳民、祝宝辉、赵葆常、杜娟 2008 57 7565]
[10]	Wu H Y, Zhang C M, Zhao B C 2009 Acta Phys. Sin. 58 930(in Chinese) [吴海英、张淳民、赵葆常 2009 58 930]
[11]	Wu H Y, Zhang C M, Zhao B C, Li Y C 2009 Acta Phys. Sin. 58 1642(in Chinese) [吴海英、张淳民、赵葆常、李英才 2009 58 1642]
[12]	Zhang C M, Mu T K, 2010, Opt. Eng. 49 043002
[13]	Zhang C M, Yan X G, Zhao B C 2008 Opt. Commun. 281 221
[14]	Bu Z C, Zhang C M, Zhao B C, Zhu H C 2009 Acta Phys. Sin. 58 2415(in Chinese) [步志超、张淳民、赵葆常、朱化春 2009 58 2415]
[15]	Zhang C M, Jian X H 2010 Optics Letters 35 366
[16]	Zhang C M,Zhao B C,Yuan Y 2006 SPIE 6032 6032T
[17]	Wang Jin-Chan, Zhang C M, Zhao B C, Liu Ning 2010 Acta Phys. Sin. 59 1631(in Chinese) [王金婵、张淳民、赵葆常、刘宁2010 Acta Phys. Sin. 59 1631]
[18]	Gault W A, Shepherd G G 1983 Adv. Space Re .2 111
[19]	Shepherd G G 1985 Appl. Opt. 24 1571
[20]	RochonY J, Rahnama P, McDade I C, Scott A, Gault W A, Lukovich J V 2004 Barcelona, Spain Proceedings of SPIE 5234 335
[21]	Gault W A, McDade I C, Rochon Y, Scott A 2003 Agia Pelagia, Crete, Greece Proceedings of SPIE 4881 60
[22]	McDade I C, Shepherd G G, Gault W A, Rochon Y J McLandress C, Scott A, Rowlands N, Butter G 2001 IEEE 1344
[23]	Gault W A, Ward W E, Shepherd G G, Rowlands N 1999 IEEE 1612
[24]	Shimoda H 2003 Agia Pelagia, Crete, Greece Proceedings of SPIE 4881 52
[25]	Bird J C, Facheng Liang, Solheim B H, Shepherd G G 1995 Meas. Sci. Technol. 6 1368
[26]	Gault W A, Brown S, Moise A, Liang D, Seller G, Shepherd G G, Wimperis 1996 Appl . Opt . 35 2913
[27]	Ward W E, Gault W A, Rowlands N, Wang S, Shepherd G G, McDaded I C, McConnelld J C Michelangelid D, CaldWelle J 2002 Quebec Canada Proceedings of SPIE 4833 226
[28]	Zhang C M, Wang W, Xiang L B, Zhao B C 2000 Acta Opt. Sin. 20 234 (in Chinese) [张淳民、王炜、相里斌 2000光学学报 20 234]
[29]	Zhang C M, He J 2006 Optics Express 14 12561
[30]	Zhang C M, Zhao B C, Xiang L B, Li Y C 2006 Optik 117 265
[31]	He J, Zhang C M, Zhang G Q 2007 Spectroscopy and Spectral Analysis 27 423 (in Chinese) [贺健、张淳民、张庆国 2007 光谱学与光谱分析 27 423]
[32]	He J, Zhang C M 2005 J. Opt. A:Pure Appl . Opt . 7 613
[33]	Jian X H, Zhang C M, Zhang L, Zhao B C 2010, Optics Express, 18:5674
[34]	Ye J Y, Zhang C M, Zhao B C 2007 Acta Phys. Sin . 57 67 (in Chinese) [叶健勇、张淳民、赵葆常 2007 57 67]
[35]	Wang L, Zhao B C, Xiang L B, Zhang C M 2007 Acta Photonica Sinca 36 1697 (in Chinese)[汪丽、赵葆常、相里斌、张淳民 2007 光子学报 36 1697]
[36]	Zhang C M, Zhao B C, Li Y C, Ye J Y 2007 Xi'an China Proc. SPIE 6279 62791D1-8
[37]	Ruan K, Zhang C M, Zhao B C 2008 Acta Phys. Sin. 57 9 (in China)[阮凯、张淳民、赵葆常 2008 57 9]
[38]	Du J, Zhang C M, Zhao B C, Sun Y 2008 Acta Phys. Sin. 57 10 (in China)[杜鹃、张淳民、赵褒常、孙尧 2008 57 10]
[39]	Liu N, Zhang C M, Wang J C, Mu T K 2010 Acta Phys. Sin. 59 385 (in China) [刘宁、张淳民、王金婵、穆廷魁 2010 59 385]
[40]	Zhang L, Zhang C M, Jian X H 2010 Acta Phys. Sin. 59 899 (in China)[张霖、张淳民、简小华 2010 59 899]
[41]	Zhu H C, Zhang C M, Jian X H 2010 Acta Phys. Sin. 59 893 (in China) [朱化春、张淳民、简小华 2010 59 893] 〖42] Title A M, Ramsey H E 1980 Appl .Opt. 19 2047
[42]	Jones R C 1941 J. Opt. Soc. Am. 31 488
[43]	Bell, Robert John 1972 Introductory Fourier transform spectroscopy(New York: Academic) p37
[44]	Thuillier G, Herse M 1991 Appl. Opt. 24 1599

施引文献

[1]	Zhang C M, Zhao B C, Xiang L B 2004 Appl. Opt. 33 6090
[2]	Zhang C M, Xiang L B, Zhao B C 2004 J. Opt. A: Pure Appl. Opt .8 815
[3]	Zhang C M, Xiang L B, Zhao B C 2002 Opt. Commun. 1-2 21
[4]	Zhang C M, Zhao B C, Xiang L B 2003 Opt. Commun. 4-6 221
[5]	Wu L, Zhang C M, Zhao B C 2007 Opt. Commun. 1 67
[6]	Jian X H, Zhang C M, Zhao B C 2007 Acta Phys. Sin. 56 824(in Chinese) [简小华、张淳民、赵葆常 2007 56 824]
[7]	Yuan Z L, Zhang C M, Zhao B C 2007 Acta Phys. Sin. 12 6413(in Chinese) [袁志林、张淳民、赵葆常 2007 56 6413]
[8]	Peng Z H, Zhang C M Zhao B C, Li Y C, Wu F Q 2006 Acta Phys. Sin. 55 6374(in Chinese) [彭志红、张淳民、赵葆常、李英才、吴福全 2006 55 6374]
[9]	Jian X H, Zhang C M, Zhu B H, Zhao B C, Du J 2008 Acta Phys. Sin. 57 7565(in Chinese) [简小华、张淳民、祝宝辉、赵葆常、杜娟 2008 57 7565]
[10]	Wu H Y, Zhang C M, Zhao B C 2009 Acta Phys. Sin. 58 930(in Chinese) [吴海英、张淳民、赵葆常 2009 58 930]
[11]	Wu H Y, Zhang C M, Zhao B C, Li Y C 2009 Acta Phys. Sin. 58 1642(in Chinese) [吴海英、张淳民、赵葆常、李英才 2009 58 1642]
[12]	Zhang C M, Mu T K, 2010, Opt. Eng. 49 043002
[13]	Zhang C M, Yan X G, Zhao B C 2008 Opt. Commun. 281 221
[14]	Bu Z C, Zhang C M, Zhao B C, Zhu H C 2009 Acta Phys. Sin. 58 2415(in Chinese) [步志超、张淳民、赵葆常、朱化春 2009 58 2415]
[15]	Zhang C M, Jian X H 2010 Optics Letters 35 366
[16]	Zhang C M,Zhao B C,Yuan Y 2006 SPIE 6032 6032T
[17]	Wang Jin-Chan, Zhang C M, Zhao B C, Liu Ning 2010 Acta Phys. Sin. 59 1631(in Chinese) [王金婵、张淳民、赵葆常、刘宁2010 Acta Phys. Sin. 59 1631]
[18]	Gault W A, Shepherd G G 1983 Adv. Space Re .2 111
[19]	Shepherd G G 1985 Appl. Opt. 24 1571
[20]	RochonY J, Rahnama P, McDade I C, Scott A, Gault W A, Lukovich J V 2004 Barcelona, Spain Proceedings of SPIE 5234 335
[21]	Gault W A, McDade I C, Rochon Y, Scott A 2003 Agia Pelagia, Crete, Greece Proceedings of SPIE 4881 60
[22]	McDade I C, Shepherd G G, Gault W A, Rochon Y J McLandress C, Scott A, Rowlands N, Butter G 2001 IEEE 1344
[23]	Gault W A, Ward W E, Shepherd G G, Rowlands N 1999 IEEE 1612
[24]	Shimoda H 2003 Agia Pelagia, Crete, Greece Proceedings of SPIE 4881 52
[25]	Bird J C, Facheng Liang, Solheim B H, Shepherd G G 1995 Meas. Sci. Technol. 6 1368
[26]	Gault W A, Brown S, Moise A, Liang D, Seller G, Shepherd G G, Wimperis 1996 Appl . Opt . 35 2913
[27]	Ward W E, Gault W A, Rowlands N, Wang S, Shepherd G G, McDaded I C, McConnelld J C Michelangelid D, CaldWelle J 2002 Quebec Canada Proceedings of SPIE 4833 226
[28]	Zhang C M, Wang W, Xiang L B, Zhao B C 2000 Acta Opt. Sin. 20 234 (in Chinese) [张淳民、王炜、相里斌 2000光学学报 20 234]
[29]	Zhang C M, He J 2006 Optics Express 14 12561
[30]	Zhang C M, Zhao B C, Xiang L B, Li Y C 2006 Optik 117 265
[31]	He J, Zhang C M, Zhang G Q 2007 Spectroscopy and Spectral Analysis 27 423 (in Chinese) [贺健、张淳民、张庆国 2007 光谱学与光谱分析 27 423]
[32]	He J, Zhang C M 2005 J. Opt. A:Pure Appl . Opt . 7 613
[33]	Jian X H, Zhang C M, Zhang L, Zhao B C 2010, Optics Express, 18:5674
[34]	Ye J Y, Zhang C M, Zhao B C 2007 Acta Phys. Sin . 57 67 (in Chinese) [叶健勇、张淳民、赵葆常 2007 57 67]
[35]	Wang L, Zhao B C, Xiang L B, Zhang C M 2007 Acta Photonica Sinca 36 1697 (in Chinese)[汪丽、赵葆常、相里斌、张淳民 2007 光子学报 36 1697]
[36]	Zhang C M, Zhao B C, Li Y C, Ye J Y 2007 Xi'an China Proc. SPIE 6279 62791D1-8
[37]	Ruan K, Zhang C M, Zhao B C 2008 Acta Phys. Sin. 57 9 (in China)[阮凯、张淳民、赵葆常 2008 57 9]
[38]	Du J, Zhang C M, Zhao B C, Sun Y 2008 Acta Phys. Sin. 57 10 (in China)[杜鹃、张淳民、赵褒常、孙尧 2008 57 10]
[39]	Liu N, Zhang C M, Wang J C, Mu T K 2010 Acta Phys. Sin. 59 385 (in China) [刘宁、张淳民、王金婵、穆廷魁 2010 59 385]
[40]	Zhang L, Zhang C M, Jian X H 2010 Acta Phys. Sin. 59 899 (in China)[张霖、张淳民、简小华 2010 59 899]
[41]	Zhu H C, Zhang C M, Jian X H 2010 Acta Phys. Sin. 59 893 (in China) [朱化春、张淳民、简小华 2010 59 893] 〖42] Title A M, Ramsey H E 1980 Appl .Opt. 19 2047
[42]	Jones R C 1941 J. Opt. Soc. Am. 31 488
[43]	Bell, Robert John 1972 Introductory Fourier transform spectroscopy(New York: Academic) p37
[44]	Thuillier G, Herse M 1991 Appl. Opt. 24 1599

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