Modeling and analysis for the image mapping spectrometer

doi:10.1088/1674-1056/26/4/040701

中国物理B ›› 2017, Vol. 26 ›› Issue (4): 40701-040701.doi: 10.1088/1674-1056/26/4/040701

Modeling and analysis for the image mapping spectrometer

Yan Yuan(袁艳), Xiao-Ming Ding(丁晓铭), Li-Juan Su(苏丽娟), Wan-Yue Wang(王婉悦)

Key Laboratory of Precision Opto-Mechatronics Technology, Ministry of Education, Beihang University, Beijing 100191, China

收稿日期:2016-11-06 修回日期:2017-01-17 出版日期:2017-04-05 发布日期:2017-04-05
通讯作者: Yan Yuan E-mail:yuanyan@buaa.edu.cn
基金资助:
Project supported by the National Natural Science Foundation of China (Grant Nos. 61635002 and 61307020) and the Changjiang Scholars and Innovative Research Team in University (PCSIRT) Program, China.

Modeling and analysis for the image mapping spectrometer

Yan Yuan(袁艳), Xiao-Ming Ding(丁晓铭), Li-Juan Su(苏丽娟), Wan-Yue Wang(王婉悦)

Key Laboratory of Precision Opto-Mechatronics Technology, Ministry of Education, Beihang University, Beijing 100191, China

Received:2016-11-06 Revised:2017-01-17 Online:2017-04-05 Published:2017-04-05
Contact: Yan Yuan E-mail:yuanyan@buaa.edu.cn
Supported by:
Project supported by the National Natural Science Foundation of China (Grant Nos. 61635002 and 61307020) and the Changjiang Scholars and Innovative Research Team in University (PCSIRT) Program, China.

摘要/Abstract

摘要： The snapshot image mapping spectrometer (IMS) has advantages such as high temporal resolution, high throughput, compact structure and simple reconstructed algorithm. In recent years, it has been utilized in biomedicine, remote sensing, etc. However, the system errors and various factors can cause cross talk, image degradation and spectral distortion in the system. In this research, a theoretical model is presented along with the point response function (PRF) for the IMS, and the influence of the mirror tilt angle error of the image mapper and the prism apex angle error are analyzed based on the model. The results indicate that the tilt angle error causes loss of light throughput and the prism apex angle error causes spectral mixing between adjacent sub-images. The light intensity on the image plane is reduced to 95% when the mirror tilt angle error is increased to ±100" (≈0.028°). The prism apex error should be controlled within the range of 0-36" (0.01°) to ensure the designed number of spectral bands, and avoid spectral mixing between adjacent images.

关键词: imaging spectrometers, snapshot imaging spectrometer, imaging model, image mapper

Abstract: The snapshot image mapping spectrometer (IMS) has advantages such as high temporal resolution, high throughput, compact structure and simple reconstructed algorithm. In recent years, it has been utilized in biomedicine, remote sensing, etc. However, the system errors and various factors can cause cross talk, image degradation and spectral distortion in the system. In this research, a theoretical model is presented along with the point response function (PRF) for the IMS, and the influence of the mirror tilt angle error of the image mapper and the prism apex angle error are analyzed based on the model. The results indicate that the tilt angle error causes loss of light throughput and the prism apex angle error causes spectral mixing between adjacent sub-images. The light intensity on the image plane is reduced to 95% when the mirror tilt angle error is increased to ±100" (≈0.028°). The prism apex error should be controlled within the range of 0-36" (0.01°) to ensure the designed number of spectral bands, and avoid spectral mixing between adjacent images.

Key words: imaging spectrometers, snapshot imaging spectrometer, imaging model, image mapper

中图分类号: (Visible and ultraviolet spectrometers)

07.60.Rd

07.05.Tp (Computer modeling and simulation) 42.30.-d (Imaging and optical processing)

袁艳, 丁晓铭, 苏丽娟, 王婉悦. Modeling and analysis for the image mapping spectrometer[J]. 中国物理B, 2017, 26(4): 40701-040701.

Yan Yuan(袁艳), Xiao-Ming Ding(丁晓铭), Li-Juan Su(苏丽娟), Wan-Yue Wang(王婉悦). Modeling and analysis for the image mapping spectrometer[J]. Chin. Phys. B, 2017, 26(4): 40701-040701.

参考文献 40

[1]	Vane G, Goetz A F H and Wellman J B 1984 IEEE Trans. Geosci. Remote Sens. 22 546
[2]	Xiang Li B, Yuan Y and Lu Q B 2009 Acta Phys. Sin. 58 5399 (in Chinese)
[3]	Li S P, Wang L Y, Yan B, Li L and Liu Y J 2012 Chin. Phys. B 21 108703
[4]	Zhang H M, Wang L Y, Yan B, Li L, Xi X Q and Lu L Z 2013 Chin. Phys. B 22 078701
[5]	Qian L L, Lv Q B, Huang W and Xiang Li B 2015 Chin. Phys. B 24 080703
[6]	Gao L, Wang L V 2016 Phys. Rep. 616 1
[7]	Gao L, Kester R T and Tkaczyk T S 2009 Opt. Express 17 12293
[8]	Weitzel L, Krabbe A, Kroker H, Thatte N, Tacconi-Garman L E, Cameron M and Genzel R 1996 Astron. Astrophys. Suppl. Ser. 119 531
[9]	Murphy T W, Soifer B T 1999 Publ. Astron. Soc. Pac. 111 1176
[10]	Cook T A, Gsell V J, Golub J and Chakrabarti S 2003 Astrophys. J. 585 1177
[11]	Henault F, Bacon R, Content R, Lantz B, Laurent F, Lemonnier J and Morris S 2004 Proc. SPIE 5249 134
[12]	Tecza M, Thatte N, Clarke F, Goodsall T, Freeman D and Salaun Y 2006 Proc. SPIE 6273 62732L
[13]	Antichi J, Dohlen K, Gratton R G, Mesa D, Claudi R U, Giro E, Boccaletti A, Mouillet D, Puget P and Beuzit J L 2009 Astrophys. J. 695 1042
[14]	Zhang J J, Cheng X M, Song J Y and Bai J M 2011 Astronomical Research & Technology 8 139 (in Chinese)
[15]	Gao D Y, Zhao F, Qiu P and Jiang X J 2012 Astronomical Research & Technology 9 143 (in Chinese)
[16]	Zhang T Y, Ji H X, Hou Y H, Hu Z W and Wang L 2015 J. Appl. Opt. 36 531
[17]	Kester R T, Gao L, Hagen N and Tkaczyk T S 2010 Opt. Express 18 14330
[18]	Kester R T, Bedard N, Gao L and Tkaczyk T S 2011 J. Biomed. Opt. 16 056005
[19]	Kester R T, Bedard N and Tkaczyk T S 2011 Proc. SPIE 8048 289
[20]	Gao L, Kester R T and Tkaczyk T S 2010 Biomedical Optics and 3-D Imaging, April 11-14, 2010, Miami, USA, p. BMD8
[21]	Gao L, Elliott A D, Kester R T, Bedard N, Hagen N, Piston D W and Tkaczyk T S 2010 Frontiers in Optics, October 24-28, 2010, Rochester, USA, p. FML2
[22]	Bedard N, Schwarz R A, Hu A, Bhattar V, Howe J, Williams M D, Gillenwater A M, Kortum R R and Tkaczyk T S 2013 Biomed. Opt. Express 4 938
[23]	Kester R T, Gao L, Bedard N and Tkaczyk T S 2010 Proc. SPIE 7555 75550A
[24]	Gao L, Smith R T and Tkaczyk T S 2012 Biomed. Opt. Express 3 48
[25]	Hagen N, Kester R T and Walker C 2012 Proc. SPIE 8358 43
[26]	Gao L, Bedard N, Hagen N, Kester R T and Tkaczyk T S 2011 Opt. Express 19 17439
[27]	Nguyen T, Pierce M C, Higgins L and Tkaczyk T S 2013 Opt. Express 21 13758
[28]	Gao L and Smith R T. 2015 J. Biophotonics 8 441
[29]	Bedard N, Hagen N, Gao L and Tkaczyk T S 2012 Opt. Eng. 51 111711
[30]	Gao L and Tkaczyk T S 2012 Opt. Eng. 51 043203
[31]	Kester R T, Gao L and Tkaczyk T S 2010 Appl. Opt. 49 1886
[32]	Goodman J W 2005 Introduction to Fourier Optics, 3rd edn. (New York: Roberts and Company Publishers) p. 23
[33]	Eismann M T 2012 Hyperspectral Remote Sensing (Washington: SPIE) p. 314
[34]	Voelz D 2011 Computational Fourier Optics: a MATLAB tutorial (Washington: SPIE) p. 29
[35]	Bass M 2010 Handbook of Optics, Vol. 4, 3rd edn. (New York: McGraw-Hill) p. 2.21
[36]	Shao H, Wang J Y and Xue Y Q 1998 J. Remote Sens. 2 251
[37]	Bai X, Zhang C M, Jing C Y, Guan X W, Cao F, Li Y N and Xie L L 2011 Acta Phys. Sin. 60 070703 (in Chinese)
[38]	Zhang C M, Huang W J and Zhao B C 2010 Acta Phys. Sin. 59 5486 (in Chinese)
[39]	Ding X M, Yuan Y and Su L J 2016 Frontiers in Optics, October 17-21, 2016, Rochester, SUA, p. JTh2A.73
[40]	Shamir J 2006 Optical Systems and Processes (Washington: SPIE) p. 106

Modeling and analysis for the image mapping spectrometer

Modeling and analysis for the image mapping spectrometer

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