大口径光学合成孔径成像技术发展现状

周程灏; 王治乐; 朱峰

doi:10.3788/CO.20171001.0025

大口径光学合成孔径成像技术发展现状

doi: 10.3788/CO.20171001.0025

cstr: 32171.14.CO.20171001.0025

周程灏^1,,
王治乐^1, ,,
朱峰²

1.
哈尔滨工业大学航天学院, 黑龙江哈尔滨 150001
2.
中国工程物理研究院, 四川绵阳 621900

基金项目:

航天五院CAST创新基金重点项目 CASTHCKJ

详细信息

作者简介:
周程灏(1989-), 男, 河南洛阳人, 博士研究生, 主要从事图像复原和光学合成孔径方面的研究。E-mail:jokerzch@163.com

通讯作者:
王治乐, E-mail:wangzhile@hit.edu.cn

中图分类号: O436
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- 被引次数: 0
出版历程
- 收稿日期: 2016-08-12
- 修回日期: 2016-09-29
- 刊出日期: 2017-02-01

Review on optical synthetic aperture imaging technique

1.
School of Astronautics, Harbin Institute of technology, Harbin 150001, China
2.
China Academy of Engineering Physics, Mianyang 621900, China

Funds:

Innovation Foundation Project of CAST CASTHCKJ

More Information

Corresponding author: WANG Zhi-le, E-mail:wangzhile@hit.edu.cn

摘要

摘要: 简明介绍了光学合成孔径的两种成像方式和光学波段合成孔径的发展概况。全面介绍镜面拼接、稀疏孔径和位相阵列3种合成孔径结构系统国内外发展现状。归纳出了目前光学合成孔径技术在天基和地基观测系统的发展趋势及技术难题。与传统单一口径的光学系统相比，光学合成孔径系统具有更高的分辨率、镜面加工难度低、易折叠、重量轻等特点，是实现高分辨率光学成像系统的一种重要且有效途径。
- 合成孔径成像 /
- 镜面拼接 /
- 稀疏孔径 /
- 阵列望远镜
Abstract: Two imaging modes and development of optical synthetic aperture are presented briefly in this paper. The current development situation of three kinds of optical synthetic aperture: segmented mirror, sparse aperture and phased array are introduced comprehensively. This paper also summarized the development trend of ground-based and space-based optical synthetic aperture system and the technical problems. Comparing with traditional single aperture optical system, optical synthetic aperture system has higher resolution, low processing difficulty of mirror, easy folding, light weight, and some other characteristics. So it is an important and effective way to realize high resolution optical imaging system.
- synthetic aperture /
- segmented mirror /
- sparse aperture /
- phased array

HTML全文

图 1 单孔径、合成孔径直接成像与间接成像示意图

Figure 1. Imaging diagram of single aperture and synthetic aperture system

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图 2 迈克尔逊型和斐索型合成孔径成像系统示意图

Figure 2. Schematic diagram of two types of synthetic aperture:(a) Michelson type, (b) Fizeau type

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图 3 Keck望远镜

Figure 3. Keck telescope

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图 4 TMT设计图

Figure 4. Design diagram of TMT

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图 5 GCT望远镜

Figure 5. GCT telescope

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图 6 HET望远镜

Figure 6. HET telescope

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图 7 SALT望远镜

Figure 7. SALT telescope

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图 8 E-ELT望远镜

Figure 8. E-ELT telescope

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图 9 OWL设计图及光路图

Figure 9. Design and optical path diagrams of OWL telescope

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图 10 GMT太空望远镜

Figure 10. GMT telescope

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图 11 GMT太空望远镜

Figure 11. GMT telescope

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图 12 GMT太空望远镜

Figure 12. GMT telescope

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图 13 ESA光学稀疏孔径设计图

Figure 13. Design diagram of ESA sparse aperture system

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图 14 MMT与MMTT望远镜

Figure 14. MMT and MMTT telescope

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图 15 LBT望远镜

Figure 15. LBT telescope

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图 16 VLT及其光路图

Figure 16. VLT telescope

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图 17 ARGOS样机与结构图

Figure 17. Protype and structure diagram of ARGOS telescope

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图 18 洛-马公司样机

Figure 18. Protype of L-M telescope

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图 19 SIM光学样图

Figure 19. Optical sample of SIM telescope

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图 20 TPF-I概念图

Figure 20. Concept diagram of TPF-I telescope

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图 21 Darwin概念图

Figure 21. Concept diagram of Darwin telescope

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图 22 法国与俄罗斯望远镜的系统图

Figure 22. System diagrams of synthetic aperture of France and Russia

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图 23 LAMOST结构图及主镜

Figure 23. Structure diagram and primary mirror of LAMOST telescope

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图 24 CFGT设计方案

Figure 24. Design scheme of CFGT telescope

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图 25 哈工大原理样机

Figure 25. Protype of HIT telescope

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图 26 光电研究所实验结果

Figure 26. Experimental result from IOE

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参考文献(34)

[1]	BORN M E. Wolf principles of optics[J]. Pergamon Press, 1980, 6:188-189.
[2]	ROUSSET G, MUGNIER L M, CASSAING F, et al. Imaging with multi-aperture optical telescopes and an application[J]. Comptes Rendus de l'Acad mie des Sciences-Series IV-Physics, 2001, 2(1):17-25. http://www.ingentaconnect.com/content/els/12962147/2001/00000002/00000001/art01158
[3]	MERMELSTEIN M. Optical synthetic aperture array:US, 6548820 B1[P]. 2003-04-15.
[4]	CASSAING F, SORRENTE B, FLEURY B, et al.. Optical design of a Michelson wide-field multiple-aperture telescope[J]. SPIE, 2004, 5249:220-229. doi: 10.1117/12.515215
[5]	KNIGHT J S, LIGHTSEY P, BARTO A. Predicted JWST imaging performance[J]. SPIE, 2012, 8442:84422G. https://www.researchgate.net/publication/258718427_Predicted_JWST_imaging_performance
[6]	CHANAN G, OHARA C, TROY M. Phasing the mirror segments of the Keck telescopes Ⅱ:the narrow-band phasing algorithm[J]. Applied Optics, 2000, 39(25):4706-4714. doi: 10.1364/AO.39.004706
[7]	CHANAN G, TROY M, DEKENS F, et al.. Phasing the mirror segments of the Keck telescopes:the broadband phasing algorithm[J]. Applied Optics, 1998, 37(1):140-155. doi: 10.1364/AO.37.000140
[8]	MACINTOSH B, TROY M, DOYON R, et al.. Extreme adaptive optics for the Thirty Meter Telescope[J]. SPIE, 2006, 6272:62720N-15. http://adsabs.harvard.edu/abs/2006SPIE.6272E..0NM
[9]	BROWN A M, ARMSTRONG T, CHADWICK P M, et al.. Flasher and muon-based calibration of the GCT telescopes proposed for the cherenkov telescope array[J]. Research in Astronomy & Astrophysics, 2015, 15(8):1095-1124. http://www.oalib.com/paper/3708931
[10]	HORNSCHEMEIER A E, BRANDT W N, GARMIRE G P, et al.. The Chandra Deep Survey of the Hubble Deep Field-North Area[J]. The Astrophysical J., 2001, 554(2):742. doi: 10.1086/apj.2001.554.issue-2
[11]	BUCKLEY D A H, BARNES S I, BURGH E B, et al.. Commissioning of the Southern African Large Telescopes (SALT) first-generation instruments[J]. SPIE, 2008, 7014:701407-15. https://www.researchgate.net/profile/Andrew_Sheinis/publication/252818340_Commissioning_of_the_Southern_African_Large_Telescope_(SALT)_First-Generation_Instruments/links/54eba5a20cf2082851be4d06.pdf?inViewer=true&pdfJsDownload=true&disableCoverPage=true&origin=publication_detail
[12]	GILMOZZI R, SPYROMILIO J. The european extremely large telescope (E-ELT)[J]. The Messenger, 2007, 127(11):3. https://www.eso.org/sci/publications/messenger/archive/no.127-mar07/messenger-no127-11-19.pdf
[13]	DIERICKX P, GILMOZZI R. Progress of the OWL 100-m telescope conceptual design[C]. Astronomical Telescopes and Instrumentation. International Society for Optics and Photonics, Munich, Germany, 2000:290-299.
[14]	LENZEN R, BRANDL B, BRANDNER W. The science case for exoplanets and star formation using mid-IR instrumentation at the OWL telescope[C]. The Scientific Requirements for Extremely Large Telescopes, 2005, 1(232):329-333.
[15]	LAJOIE C P, SOUMMER R, PUEYO L, et al.. Planning and developing JWST CORONAGRAPHS OPerations[J]. Iau General Assembly, 2015:22. http://adsabs.harvard.edu/abs/2015IAUGA..2257743L
[16]	JOHNS M, ANGEL J R P, SHECTMAN S, et al.. Status of the giant magellan telescope (GMT) project[J]. SPIE, 2004, 5489:441-453. https://www.researchgate.net/publication/247647325_Status_of_the_Giant_Magellan_Telescope_GMT_Project?_sg=7CMQlENRA73-BdrPKQFckugloqXHmXqJ3vhWjEBe_5wv9lbMZx988Fa1nv2epKvczOYXVqo-IA4YraEwYm7Uug
[17]	RUTTEN R J, HAMMERSCHLAG R H, BETTONVIL F C M, et al.. DOT tomography of the solar atmosphere-I. Telescope summary and program definition[J]. Astronomy & Astrophysics, 2004, 413(3):1183-1189. http://citeseerx.ist.psu.edu/viewdoc/bookmark?doi=10.1.1.494.1692&site=connotea
[18]	朱仁璋, 丛云天, 王鸿芳, 等.全球高分光学量概述(二):欧洲[J].航天器工程, 2016, 25(1):95-118. http://www.cnki.com.cn/Article/CJFDTOTAL-HTGC201601015.htm
[19]	BECKERS J M, ULICH B L, WILLIAMS J T. Performance of The Multiple Mirror Telescope (MMT) I. MMT-the first of the advanced technology telescopes[C]. 1982 Astronomy Conferences. International Society for Optics and Photonics, Muich, Germany, 1982:2-8.
[20]	HILL J M, ASHBY D S, BRYNNEL J G, et al.. The large binocular telescope:binocular all the time[J]. SPIE, 2014, 9145:914502.
[21]	BONANOS A Z, STANEK K A. Reanalysis of very large telescope data for M83 with image subtraction-nicefold increase in number of cepheids[J]. Astrophysical J., 2003, 591(2):L111-L114 doi: 10.1086/377073
[22]	CHUNG S J, MILLER D W, WECK O L D. ARGOS testbed:study of multidisciplinary challenges of future spaceborne interferometric arrays[J]. Optical Engineering, 2004, 43(43):2156-2167. https://www.researchgate.net/publication/268571251_Multidisciplinary_Control_of_a_Sparse_Interferometric_Array_Satellite_Testbed
[23]	PITMAN J T, DUNCAN A, STUBBS D, et al. Remote sensing space science enabled by the multiple instrument distributed aperture sensor (MIDAS) concept[J]. SPIE, 2004, 5555:301-310. https://www.researchgate.net/publication/260077353_Remote_sensing_space_science_enabled_by_the_Multiple_Instrument_Distributed_Aperture_Sensor_MIDAS_concept
[24]	FRINK S, QUIRRENBACH A, FISCHER D, et al.. A strategy for identifying the grid stars for the Space Interferometry Mission (SIM)[J]. Publications of the Astronomical Society of the Pacific, 2001, 113(780):173-187. doi: 10.1086/pasp.2001.113.issue-780
[25]	KALTENEGGER L, FRIDLUND M. Characteristics of proposed 3 and 4 telescope configurations for Darwin and TPF-I[J]. Proceedings of the International Astronomical Union, 2005, 1(C200):255-258. doi: 10.1017/S1743921306009410
[26]	HILL J M. The large binocular telescope[J]. Applied Optics, 2010, 49(16):D115-D122. doi: 10.1364/AO.49.00D115
[27]	TRAUB W A. Combining beams from separated telescopes[J]. Applied Optics, 1986, 25(4):528-532. doi: 10.1364/AO.25.000528
[28]	MATHER J, STOCKMAN H S, GREENBEL T. Next generation space telescope[J]. SPIE, 2000, 4013:2~16 http://www.nasa.gov/news/budget/image_jwst.html
[29]	LEVOY M, CHEN B, VAISH V, et al.. Synthetic aperture confocal imaging[J]. Acm Transactions on Graphics, 2004, 23(3):825-834. doi: 10.1145/1015706
[30]	ZHAO Y. Large sky area multi-object fiber spectroscopic telescope[J]. Bulletin of the Chinese Academy of Sciences, 2011(3):231-232. http://www.docin.com/p-1544731231.html
[31]	ZHOU Z, WANG D, WANG Y. Effect of noise on the performance of image restoration in an optical sparse aperture system[J]. J. Optics, 2011, 13(7):075502. doi: 10.1088/2040-8978/13/7/075502
[32]	魏小峰, 耿则勋, 宋向.光学合成孔径复原图像的振铃探测与消除[J].光学精密工程, 2014, 22(11):3091-3099. http://www.cnki.com.cn/Article/CJFDTOTAL-GXJM201411029.htm WEI X F, GENG Z X, SONG X. Detection and removal of ringing artifact for optical synthetic aperture restoration image[J]. Optics & Precision Engineering, 2014, 22(11):3091-3099.(in Chinese) http://www.cnki.com.cn/Article/CJFDTOTAL-GXJM201411029.htm
[33]	刘政, 王胜千, 饶长辉.一种基于远场图像的稀疏光学合成孔径系统共相探测新方法的仿真研究[J].物理学报, 2012, 61(3):0390501. http://www.cnki.com.cn/Article/CJFDTOTAL-WLXB201203082.htm LIU ZH, WANG SH Q, RAO CH H, et al.. Analysis of an Co-phasing detecting method based on far-field images of sparse-optical-synthetic-aperture system[J]. Acta Physica Sinica, 2012, 61(3):0390501.(in Chinese) http://www.cnki.com.cn/Article/CJFDTOTAL-WLXB201203082.htm
[34]	中国科学院光电技术研究所.光电所在分离镜面光学合成孔径关键技术研究上取得重要进展[EB/OL].[2016-03-29].