双强度调制静态傅里叶变换偏振成像光谱系统测量原理及仿真
|
摘要
为了抑制背景噪声,获得高信噪比的纯干涉条纹并实现图像、光谱和全偏振信息的同时测量,提出了一种基于双强度调制的静态傅里叶变换偏振成像光谱技术新方案.系统由前置望远系统、两个相位延迟器构成的偏振来谱调制模块、Wollaston棱镜构成的偏振.分束器、Savart偏光镜和线偏振器构成的干涉糢块以及CCD面阵探测器组成,可在单一探测器上同时获取两幅经过不同强度调制的全偏振干涉图,通过对两幅全偏振干涉图的简单加减运算,便可获得探测目标清晰的纯图像和高信噪比的纯干涉条纹.对该系统的图像和光谱偏振复原过程进行了理论分析和数值摸拟,结果表明该系统可有效分离探测目标的背景图像和干涉图像,实现高精度的光谱复原和全偏振信息的有效提取,具有髙稳定性、高光谱、高灵敏度、高信噪比、信息复原精度高及数据处理复杂度低等优点,为偏振干涉成像光谱技术的发展提供了新思路.
Traditional imaging spectropolarimetry generally requires slit,moving parts,electrically tunable devices,or the use of micropolarized arrays.Furthermore,the acquired raw data are a physical superposition of interferogram and image.Given their complicated structure,poor seismic capacity,low detection sensitivity,and heavy computations with approximation in spectral reconstruction,meeting the needs for applications in aviation,remote sensing,and field detection is difficult.To overcome these drawbacks,a new spectropolarimetric imaging technique based on static dual intensity-modulated Fourier transform is presented.The system consists of a front telescopic system,two phase retarders,a linear polarizer,a Wollaston prism,a Savart polariscope,a linear analyzer,a reimaging system,and a charge-coupled device(CCD) array detector.The incident light is modulated through a module of polarization spectrum modulation,which consists of the retarders and the polarizer.The Wollaston prism splits the modulated incident light into two equal intensities,orthogonally polarized components with a small divergent angle.After passing through the interference module,which is composed of the Savart polariscope and the analyzer,then the reimaging system,two full-polarization interferograms,which are the superposition of background images and interference fringes,are recorded simultaneously on a single CCD.The pure target image and the pure interference fringes can be simply achieved from the summation or the difference of the two interferograms.Spectral and complete polarization information can be acquired by using the Fourier transform of the pure interference fringes.The principle and the configuration of the system are described here in this paper.The reconstruction processes of the target image and the full Stokes polarization spectra are theoretically analyzed and mathematically simulated.The results show that the system can availably separate background image from interference fringes of the target,achieving high-precision spectral reconstruction and effective extraction of the complete polarization information.Compared with the features of existing instruments,one of the salient features of the described model is to use the dual-intensity modulation,which can avoid mutual interference between the image and the fringes from the hardware and is conducive to the extraction of pure interference fringes with high signal-tonoise ratio(SNR).With this feature,the inadequacies on traditional spectral reconstruction,such as large computation,heavy data processing,and low accuracy of acquired information,are overcome.Moreover,the entrance slit in the front telescopic system is removed,which greatly increases the transmittance and flux of the incident light and improves the SNR of the interferogram.The modified Savart polariscope is used in the interference module.Its transverse shearsplitting principle further enlarges the field of view and increases the spectral resolution of the straight fringes.Thus,this design has the advantages of good stability,high spectrum,high sensitivity,large SNR,high-precision information reconstruction,and low-complexity data processing,as well as simultaneous detection of image,spectrum,and complete polarization information.This work will provide an important theoretical basis and practical instruction for developing new spectropolarimetric imaging technique and its engineering applications.
Traditional imaging spectropolarimetry generally requires slit,moving parts,electrically tunable devices,or the use of micropolarized arrays.Furthermore,the acquired raw data are a physical superposition of interferogram and image.Given their complicated structure,poor seismic capacity,low detection sensitivity,and heavy computations with approximation in spectral reconstruction,meeting the needs for applications in aviation,remote sensing,and field detection is difficult.To overcome these drawbacks,a new spectropolarimetric imaging technique based on static dual intensity-modulated Fourier transform is presented.The system consists of a front telescopic system,two phase retarders,a linear polarizer,a Wollaston prism,a Savart polariscope,a linear analyzer,a reimaging system,and a charge-coupled device(CCD) array detector.The incident light is modulated through a module of polarization spectrum modulation,which consists of the retarders and the polarizer.The Wollaston prism splits the modulated incident light into two equal intensities,orthogonally polarized components with a small divergent angle.After passing through the interference module,which is composed of the Savart polariscope and the analyzer,then the reimaging system,two full-polarization interferograms,which are the superposition of background images and interference fringes,are recorded simultaneously on a single CCD.The pure target image and the pure interference fringes can be simply achieved from the summation or the difference of the two interferograms.Spectral and complete polarization information can be acquired by using the Fourier transform of the pure interference fringes.The principle and the configuration of the system are described here in this paper.The reconstruction processes of the target image and the full Stokes polarization spectra are theoretically analyzed and mathematically simulated.The results show that the system can availably separate background image from interference fringes of the target,achieving high-precision spectral reconstruction and effective extraction of the complete polarization information.Compared with the features of existing instruments,one of the salient features of the described model is to use the dual-intensity modulation,which can avoid mutual interference between the image and the fringes from the hardware and is conducive to the extraction of pure interference fringes with high signal-tonoise ratio(SNR).With this feature,the inadequacies on traditional spectral reconstruction,such as large computation,heavy data processing,and low accuracy of acquired information,are overcome.Moreover,the entrance slit in the front telescopic system is removed,which greatly increases the transmittance and flux of the incident light and improves the SNR of the interferogram.The modified Savart polariscope is used in the interference module.Its transverse shearsplitting principle further enlarges the field of view and increases the spectral resolution of the straight fringes.Thus,this design has the advantages of good stability,high spectrum,high sensitivity,large SNR,high-precision information reconstruction,and low-complexity data processing,as well as simultaneous detection of image,spectrum,and complete polarization information.This work will provide an important theoretical basis and practical instruction for developing new spectropolarimetric imaging technique and its engineering applications.
引文
[1]Persky M J 1995 Rev.Sci.Instrum.66 4763
[2]Denes L J,Gottlieb M S,Kaminsky B 1998 Opt.Eng.37 1262
[3]Oka K,Kato T 1999 Opt.Lett 24 1475
[4]Tyo J S,Theodore S,Turner J 1999 Proc.SPIE 3753214
[5]Dereniak E L,Hagen N A,Johnson W R 2003 Proc.SPIE 5074 272
[6]Miles B H,Kim L B 2004 Proc.SPIE 5432 155
[7]Stephen H J,Frank J I,Chris H 2006 NASA Earth Science Technology Conference Proceeding
[8]Tyo J S,Goldstein D L,Chenault D B,Shaw J A 2006Appl.Opt.45 5453
[9]Kudenov M W,Hagen N A,Dereniak E L,Gerhart G R2007 Opt.Express 15 12792
[10]Gupta N 2008 Proc.SPIE 6972 69720C
[11]Gerhart G R 2008 Opt.Eng.47 0160011
[12]Corrie V,Sampson R,Carven J 2008 Proc.SPIE 7086708604
[13]Aumiller R W,Vandervlugt C,Dereniak E L 2008 Proc.SPIE 6972 69720D
[14]Gendre L,Foulonneau A,Bigue L 2010 Appl.Opt.494687
[15]Li J,Zhu J P,Wu H Y 2010 Opt.Lett.35 3784
[16]Hyde M W,Schmidt J D,Havrilla M J,Cain S C 2010Opt.Lett.35 3601
[17]Jones J C,Kudenov M W,Stapelbroe M G,Dereniak E L 2011 Appl Opt.50 1170
[18]Mu T K,Zhang C M,Jia C L,Ren W Y 2012 Opt.Express 20 18194
[19]Meng X,Li G,Liu D 2013 Opt.Lett.38 778
[20]Meng X,Li J,Liu D,Xu T,Liu D,Zhu R 2013 Opt.Express 21 32071
[21]Li J,Zhu J P,Qi C,Zheng C L,Gao B,Zhang Y Y,Hou X 2013 Acta Phys.Sin.62 044206(in Chinese)[李杰,朱京平,齐春,郑传林,高博,张云尧,侯洵2013物理学报62 044206]
[22]Li J,Zhu J P,Qi C,Zheng C L,Gao B,Zhang Y Y,Hou X 2014 Infrared Laser Eng.43 574(in Chinese)[李杰,朱京平,齐春,郑传林,高博,张云亮,侯洵2014红外与激光工程43 574]
[23]Mu T K,Zhang C M,Li Q W,Wei Y T,Chen Q Y,Jia C L 2014 Acta Phys.Sin.63 110704(in Chinese)[穆廷魁,张淳民,李祺伟,魏宇童,陈清颖,贾辰凌2014物理学报63 110704]
[24]Liu Y,Lo Y,Li C,Liao C 2015 Opt.Commun.336 295
[25]Zhang R,Chen Y H,Li K W,Wang Z B,Li S W,Wang nese)[张瑞,陈友华,李克武,王志斌,李世伟,王耀利,张敏娟2016光学学报36 1011001]
[26]Kohzo H,Hirokimi S,Hiromichi Y 2005 Proc.SPIE5655 407
[27]Zhao Y Q,Pan Q,Zhang H C 2006 Proc.SPIE 6240624007
[28]Scharmer G B,Narayan G,Hillberg T 2008 Astrophys.J.689 169
[29]Nathan J P,Andrew R D,Michael J,Joseph A 2011Opt.Express 19 18602
[30]Zhao Y Q,Pan Q,Cheng Y M 2011 Imaging Spectropolarimetric Remote Sensing and Application(Beijng:National Defense Industry Press)pp16-19(in Chinese)[赵永强,潘泉,程咏梅2011成像偏振光谱遥感及应用(北京:国防工业出版社)第16—19页]
[31]Li Y N,Sun X B,Mao Y N 2012 Infrared Laser Eng.41205
[32]Lou M J,Xing Q G,Shi P 2013 Remote Sensing Technology and Application 28 627
[33]Zhao J,Zhou F,Li H 2014 Spacecraft Recovery and Remote Sensing 35 39
[34]Xue Q S 2014 Chin.J.Lasers 41 0316003
[35]Liao Y B 2003 Polarization Optics(Beijing:Science Press)p322(in Chinese)[廖延彪2003偏振光学(北京:科学出版社)第322页]
[36]Wang X Q 2011 Ph.D.Dissertation(Taiyuan:Shanxi University)(in Chinese)[王新全2011博士学位论文(西安:中国科学院西安光学精密机械研究所)]
[37]Zhang C M,Jian X H 2010 Opt.Lett.35 366
[2]Denes L J,Gottlieb M S,Kaminsky B 1998 Opt.Eng.37 1262
[3]Oka K,Kato T 1999 Opt.Lett 24 1475
[4]Tyo J S,Theodore S,Turner J 1999 Proc.SPIE 3753214
[5]Dereniak E L,Hagen N A,Johnson W R 2003 Proc.SPIE 5074 272
[6]Miles B H,Kim L B 2004 Proc.SPIE 5432 155
[7]Stephen H J,Frank J I,Chris H 2006 NASA Earth Science Technology Conference Proceeding
[8]Tyo J S,Goldstein D L,Chenault D B,Shaw J A 2006Appl.Opt.45 5453
[9]Kudenov M W,Hagen N A,Dereniak E L,Gerhart G R2007 Opt.Express 15 12792
[10]Gupta N 2008 Proc.SPIE 6972 69720C
[11]Gerhart G R 2008 Opt.Eng.47 0160011
[12]Corrie V,Sampson R,Carven J 2008 Proc.SPIE 7086708604
[13]Aumiller R W,Vandervlugt C,Dereniak E L 2008 Proc.SPIE 6972 69720D
[14]Gendre L,Foulonneau A,Bigue L 2010 Appl.Opt.494687
[15]Li J,Zhu J P,Wu H Y 2010 Opt.Lett.35 3784
[16]Hyde M W,Schmidt J D,Havrilla M J,Cain S C 2010Opt.Lett.35 3601
[17]Jones J C,Kudenov M W,Stapelbroe M G,Dereniak E L 2011 Appl Opt.50 1170
[18]Mu T K,Zhang C M,Jia C L,Ren W Y 2012 Opt.Express 20 18194
[19]Meng X,Li G,Liu D 2013 Opt.Lett.38 778
[20]Meng X,Li J,Liu D,Xu T,Liu D,Zhu R 2013 Opt.Express 21 32071
[21]Li J,Zhu J P,Qi C,Zheng C L,Gao B,Zhang Y Y,Hou X 2013 Acta Phys.Sin.62 044206(in Chinese)[李杰,朱京平,齐春,郑传林,高博,张云尧,侯洵2013物理学报62 044206]
[22]Li J,Zhu J P,Qi C,Zheng C L,Gao B,Zhang Y Y,Hou X 2014 Infrared Laser Eng.43 574(in Chinese)[李杰,朱京平,齐春,郑传林,高博,张云亮,侯洵2014红外与激光工程43 574]
[23]Mu T K,Zhang C M,Li Q W,Wei Y T,Chen Q Y,Jia C L 2014 Acta Phys.Sin.63 110704(in Chinese)[穆廷魁,张淳民,李祺伟,魏宇童,陈清颖,贾辰凌2014物理学报63 110704]
[24]Liu Y,Lo Y,Li C,Liao C 2015 Opt.Commun.336 295
[25]Zhang R,Chen Y H,Li K W,Wang Z B,Li S W,Wang nese)[张瑞,陈友华,李克武,王志斌,李世伟,王耀利,张敏娟2016光学学报36 1011001]
[26]Kohzo H,Hirokimi S,Hiromichi Y 2005 Proc.SPIE5655 407
[27]Zhao Y Q,Pan Q,Zhang H C 2006 Proc.SPIE 6240624007
[28]Scharmer G B,Narayan G,Hillberg T 2008 Astrophys.J.689 169
[29]Nathan J P,Andrew R D,Michael J,Joseph A 2011Opt.Express 19 18602
[30]Zhao Y Q,Pan Q,Cheng Y M 2011 Imaging Spectropolarimetric Remote Sensing and Application(Beijng:National Defense Industry Press)pp16-19(in Chinese)[赵永强,潘泉,程咏梅2011成像偏振光谱遥感及应用(北京:国防工业出版社)第16—19页]
[31]Li Y N,Sun X B,Mao Y N 2012 Infrared Laser Eng.41205
[32]Lou M J,Xing Q G,Shi P 2013 Remote Sensing Technology and Application 28 627
[33]Zhao J,Zhou F,Li H 2014 Spacecraft Recovery and Remote Sensing 35 39
[34]Xue Q S 2014 Chin.J.Lasers 41 0316003
[35]Liao Y B 2003 Polarization Optics(Beijing:Science Press)p322(in Chinese)[廖延彪2003偏振光学(北京:科学出版社)第322页]
[36]Wang X Q 2011 Ph.D.Dissertation(Taiyuan:Shanxi University)(in Chinese)[王新全2011博士学位论文(西安:中国科学院西安光学精密机械研究所)]
[37]Zhang C M,Jian X H 2010 Opt.Lett.35 366
© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号 地址：北京市海淀区学院路29号 邮编：100083 电话：办公室：(+86 10)66554848；文献借阅、咨询服务、科技查新：66554700 |