合成孔径光学成像系统研究
|
摘要
合成孔径光学成像技术是一种提高光学系统空间分辨率的新型成像技术。其利用多个孔径较小的光学系统便可得到与单大孔径系统相当的空间分辨率及成像质量，解决了单大孔径系统所带来的体积重量大、加工检测难和成本高等问题。合成孔径光学成像技术是实现超大孔径光学系统的有效手段和发展方向，其必将极大的促进光学空间遥感技术和天文光学技术的进一步发展。
本文对合成孔径光学技术中的孔径优化、像差等理论进行了研究；分析了合成孔径系统的设计方法，具体设计了三种合成孔径光学成像系统；并对合成孔径技术进行了实验室原理验证实验，对填充因子和孔径排布对系统性能的影响进行了验证。论文共七章，具体可分为如下部分：
1.从空间域和频率域两个方面对合成孔径光学成像系统提高光学系统空间分辨率的原理进行了分析，建立了合成孔径光学成像系统的成像模型，设计了基于Matlab和ZEMAX的合成孔径成像模拟分析程序。对典型的合成孔径光瞳结构进行了分析，并给出了一种由九个子望远镜组成的新型合成孔径光瞳结构，该结构具有MTF分布均匀，截止频率高等特点。
2.分析了合成孔径系统的像差性质，建立了合成孔径系统的像差模型，着重对两子镜系统中两个子镜含有不同性质和不同量值的像差的情况进行了分析。将基于遗传算法的相位差法波前传感技术应用于合成孔径系统的波前误差传感，并对含有三个子镜的系统进行了活塞误差传感模拟。
3.对合成孔径成像系统的设计方法进行了分析，给出了多望远镜型合成孔径系统的基本设计流程，并对合成孔径系统中的黄金准则等问题进行了分析。设计了一种折反式多望远镜型合成孔径系统和两种反射式合成孔径系统，对系统中无焦子望远镜、光束合成镜以及系统的集成与优化等进行了详细介绍，并对系统中的部分细节进行了分析，采用点列图、MTF和斯特列尔值等评价函数对系统成像性能进行了评估。
4.对合成孔径光学成像技术进行了实验验证。采用有限距离合成孔径系统实验验证装置对填充因子和孔径排布形式对系统的性能影响进行了实验验证，实验结果与理论分析结果相一致，证明了理论分析和计算机仿真的正确性。
Optical synthetic aperture imaging technique is a new imaging technology toachieve higher spatial resolution of the optical system. It uses several of thesmall-aperture optical system to get the spatial resolution and image quality of asingle large-aperture optical system. This can solve the heavy weight, testingdifficulties and high cost problem of making a single large aperture system. Opticalsynthetic aperture system is a effective means to make large optical system. So it willpromote the optical space remote sensing technology and the further development ofastronomical optical technology.
This dissertation derives and demonstrates the aperture optimization, aberrationanalysis, design method and three design examples. The main research contents are asfollows:
1. The principle of the optical synthetic aperture system's improvement in spatialresolution of the optical system is analyzed from space domain and frequency domain,and the system's imaging model is designed in Matlab and ZEMAX software. Thetypical entrance aperture configurations of the optical synthetic system are analyzedby the imaging model. A new aperture configuration including9sub-apertures isgiven and analyzed in the dissertation.
2. The aberration of the optical synthetic aperture is analyzed and its imagingmodel with aberration is designed. Aberration effect in two-aperture system isanalyzed by adding different aberration type and different aberration value to eachaperture. The phase diversity based on genetic algorithm is used to sense the measurethe wavefront error of the system. As an example, this method is used in athree-aperture system to measure the piston error of each aperture. The results showsthat the method is of high precision and stabilization.
3. design method of two kinds of optical synthetic aperture system is analyzedand the design process of the multiple-telescope system is given. Three opticalsynthetic aperture systems are designed based on the design process. One is acatadioptric system and the rest are reflective system. The sub-telescope, beamcombiner and the system's integration and optimization are described in detail. Spotdiagram, MTF and strehl ratio are used to evaluate the performance of the system.
4. An experiment is carried out to validate the imaging principle of the optical synthetic aperture system. The effects of the fill factor and aperture configuration tothe system are analyzed. The experiment results and the theory simulation results areanalyzed, and the two results are consistent. This shows the theoretical analysis andsimulation are correct.
本文对合成孔径光学技术中的孔径优化、像差等理论进行了研究；分析了合成孔径系统的设计方法，具体设计了三种合成孔径光学成像系统；并对合成孔径技术进行了实验室原理验证实验，对填充因子和孔径排布对系统性能的影响进行了验证。论文共七章，具体可分为如下部分：
1.从空间域和频率域两个方面对合成孔径光学成像系统提高光学系统空间分辨率的原理进行了分析，建立了合成孔径光学成像系统的成像模型，设计了基于Matlab和ZEMAX的合成孔径成像模拟分析程序。对典型的合成孔径光瞳结构进行了分析，并给出了一种由九个子望远镜组成的新型合成孔径光瞳结构，该结构具有MTF分布均匀，截止频率高等特点。
2.分析了合成孔径系统的像差性质，建立了合成孔径系统的像差模型，着重对两子镜系统中两个子镜含有不同性质和不同量值的像差的情况进行了分析。将基于遗传算法的相位差法波前传感技术应用于合成孔径系统的波前误差传感，并对含有三个子镜的系统进行了活塞误差传感模拟。
3.对合成孔径成像系统的设计方法进行了分析，给出了多望远镜型合成孔径系统的基本设计流程，并对合成孔径系统中的黄金准则等问题进行了分析。设计了一种折反式多望远镜型合成孔径系统和两种反射式合成孔径系统，对系统中无焦子望远镜、光束合成镜以及系统的集成与优化等进行了详细介绍，并对系统中的部分细节进行了分析，采用点列图、MTF和斯特列尔值等评价函数对系统成像性能进行了评估。
4.对合成孔径光学成像技术进行了实验验证。采用有限距离合成孔径系统实验验证装置对填充因子和孔径排布形式对系统的性能影响进行了实验验证，实验结果与理论分析结果相一致，证明了理论分析和计算机仿真的正确性。
Optical synthetic aperture imaging technique is a new imaging technology toachieve higher spatial resolution of the optical system. It uses several of thesmall-aperture optical system to get the spatial resolution and image quality of asingle large-aperture optical system. This can solve the heavy weight, testingdifficulties and high cost problem of making a single large aperture system. Opticalsynthetic aperture system is a effective means to make large optical system. So it willpromote the optical space remote sensing technology and the further development ofastronomical optical technology.
This dissertation derives and demonstrates the aperture optimization, aberrationanalysis, design method and three design examples. The main research contents are asfollows:
1. The principle of the optical synthetic aperture system's improvement in spatialresolution of the optical system is analyzed from space domain and frequency domain,and the system's imaging model is designed in Matlab and ZEMAX software. Thetypical entrance aperture configurations of the optical synthetic system are analyzedby the imaging model. A new aperture configuration including9sub-apertures isgiven and analyzed in the dissertation.
2. The aberration of the optical synthetic aperture is analyzed and its imagingmodel with aberration is designed. Aberration effect in two-aperture system isanalyzed by adding different aberration type and different aberration value to eachaperture. The phase diversity based on genetic algorithm is used to sense the measurethe wavefront error of the system. As an example, this method is used in athree-aperture system to measure the piston error of each aperture. The results showsthat the method is of high precision and stabilization.
3. design method of two kinds of optical synthetic aperture system is analyzedand the design process of the multiple-telescope system is given. Three opticalsynthetic aperture systems are designed based on the design process. One is acatadioptric system and the rest are reflective system. The sub-telescope, beamcombiner and the system's integration and optimization are described in detail. Spotdiagram, MTF and strehl ratio are used to evaluate the performance of the system.
4. An experiment is carried out to validate the imaging principle of the optical synthetic aperture system. The effects of the fill factor and aperture configuration tothe system are analyzed. The experiment results and the theory simulation results areanalyzed, and the two results are consistent. This shows the theoretical analysis andsimulation are correct.
引文
[1] http://en.wikipedia.org/wiki/KH-12
[2] http://en.wikipedia.org/wiki/KH-11
[3]杨秉新.美国IKONOS和QuickBird2卫星相机的主要性能和特点分析及看法[J].航天返回与遥感,2002,23(4): l4~16
[4] http://en.wikipedia.org/wiki/QuickBird
[5]吴玉石.高分辨率传输型侦察卫星技术的发展[J].航天器工程,2003,12(1):64~73
[6]郭今昌.商用高分辨率光学遥感卫星及平台技术分析[J].航天器工程,2009,18(2):83~89
[7]王金堂,乌崇德.国外几种星载光学遥感器的发展情况简介[J].航天返回与遥感,2002,23(2):15~20
[8]顾先冰,司群英.国内外遥感卫星发展现状[J].航天返回与遥感,2000,21(2):29~33
[9]玻恩,沃尔夫.光学原理（第七版）[M].北京:电子工业出版社,2005
[10] http://en.wikipedia.org/wiki/Hubble
[11] D. Schroeder. Astronomical optics(2nd)[M].California:Academic Press,2000
[12] A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt.,1970,9(11):2501~2504
[13] E. K. Hege, J. M. Beckers, P. A. Strittmatter, et al.. Multiple mirror telescope asa phased array telescope[J]. Appl. Opt.,1985,24(16):2565~2576
[14] W. A. Traub. Combining beams from separated telescopes[J]. Appl. Opt.,1986,25(4):528~532
[15] J. S. Fender. Phase array optical system[J]. SPIE,1986, Vol.643:122~128
[16] Fizeau, H.1868C. R. Hebd. Seanc. Acad. Sci. Paris66,932
[17] Advisory Committee To The Air Force Systems Command. Synthetic-apertureoptics Vol.1[C]. Washington D C: Defense Technical Information Center,1967
[18] Advisory Committee To The Air Force Systems Command. Synthetic-apertureoptics Vol.2[C]. Washington D C: Defense Technical Information Center,1967
[19] M. J. E. Golay. Point arrays having compact, nonredundant autocorrelations[J].JOSA,1971,61(2):272~273
[20] R. B. Hooker. The effects of aberrations in synthetic aperture systems[D].Arizona: University of Arizona,1974
[21] J. E. Harvey, C. Ftaclas. Field-of-view limitations of phased telescope arrays[J].Appl. Opt.,1995,34(25):5787~5798
[22] J. E. Harvey, C. Ftaclas. Fundamental limitations on off-axis performance ofphased telescope arrays[J]. SPIE,1990,Vol.1236
[23] Gonsalves. Phase retrieval and diversity in adaptive optics[J]. Opt. Eng.,1982,21(5):829~832
[24] R. G. Paxman, J. R. Fienup. Optical misalignment sensing and imagereconstruction using phase diversity[J]. JOSA,1988,5(6):914~923
[25] R. G. Paxman, T. J. Schulz, J, R. Fienup. Joint estimation of object andaberrations by using phase diversity[J].JOSA,1992,9(7):1072~1085
[26] J. Fienup.MTF and integration time versus fill factor for sparse-apertureimaging systems[J]. SPIE,2000, Vol.4091:43~47
[27] R. D. Fiete, J. A. Mooney, T. A. Tantalo, et al.. Image quality assessment ofsparse-aperture designs with decreasing fill factors[J]. SPIE,2000,4091:64~73
[28] R. D. Fiete, T. A. Tantalo, J. R. Calus,et al.. Image quality of sparse-aperturedesigns for remote sensing[J]. Opt. Eng.,2002,41(8):1957-1969
[29] T. W. Stuhlinger. All-reflective phased array imaging telescopes[J]. SPIE,1991,Vol.1354:438~446
[30] C. H. Miao, R. R. Shannon. Design of wide-field arrays[J]. SPIE,1990, Vol.1236:372~378
[31] C. H. Miao. The design of phased synthetic aperture imaging systems using aminimum number of elements[D]. Arizona: University of Arizona,1991
[32] M. S. Erin. Fundamentals of the optical design of mulitiple aperture telescopeswith wide fields of view[D]. Arizona: University of Arizona,2002
[33] R. E. Introne. Enhanced spectral modeling of sparse aperture imagingsystems[D]. New York: Rochester Institute of Technology,2004
[34] N. R. Block. A sensitivity study of a polychromatic sparse-aperture system[D].New York: Rochester Institute of Technology,2005
[35] E. K. Hege, J. M. Beckers, P. A. Strittmatter, et al.. Multiple mirror telescope asa phased array telescope[J]. Appl. Opt.,1985,24(16):2565~2576
[36] A. C. Gary, S. M. Terry, E. N. Jerry, et al.. Phasing the mirror segments of theW.M. Keck telescope[J]. SPIE,1994,2199:622~637
[37] G. Chanan, C. Ohara, M. Troy. Phasing the mirror segments of the Kecktelescopes II: the narrow-band phasing algorithm[J]. Appl. Opt.,2000,39(25):4706~4714
[38] E. N. Jerry, R. G. Peter. Overview of the performance of the W.M. KeckObservatory[J]. SPIE,1994,2199:82~93
[39] E. E. Sabatke, J. H. Burge, P. Hinz.Optical design of interferometric telescopeswith wide fields of view[J]. Appl. Opt.,2006,45(31):8026~8035
[40] J. M. Hill, R. F. Green, J. H. Slagle.The large binocular telescope[J].SPIE,2006,Vol.6267:62670Y-1~15
[41] J. M. Beckers. VLT Interferometer: III. Factors affecting wide field-of-viewoperation[J]. SPIE,1990, Vol.1236:379~389
[42] V. Zarifis, R. M. Bell, L. R. Benson,et al.. The multi aperture imaging array[J].Proc. from ASP Conference Vol.194,1999
[43] R. L. Kendrick, J.-N. Aubrun, R. Bell,et al. Wide-field Fizeau imagingtelescope: experimental results[J].Appl. Opt.,2006,45(18):4235~4240
[44] K. D. Bell, R. L. Moser, M. K. Powers, et al.. Deployable optical telescopeground demonstration[J]. SPIE,2000,4013:559~567
[45] C. Soon-Jo, W. M. David, L. d. W. Olivier.ARGOS testbed: study ofmultidisciplinary challenges of future spaceborne interferometric arrays[J]. Opt.Eng.,2004,43(9):2156~2167
[46] G. Rousset, L. Mugnier. Imaging with multi aperture optical telescopes and anapplication[J]. Comptes Rendusdel Academie des Sciences Series IV Physucs,2001,2(1):17~25
[47] L. M. Mugnier, F. Cassaing, G. Rousset, et al.. Earth observation from a highorbit: pushing the limits with synthetic aperture optics[R].P228010,2000
[48] M. Mesrine, E. Thomas, S. Garin, et al.. High resolution earth observation fromgeostationary orbit by optical aperture synthesys[C]. Proc.6th Internat. Conf.on Space Optics,2006
[49]王海涛,周必方.天文光干涉技术[J].光学精密工程,2003,11(4):320-325
[50]吴泉英.稀疏孔径光学系统成像研究[D].苏州:苏州大学,2006
[51] Wang Zhile, Zhang Wei, Deng Jian, et al..Image evaluation for optical syntheticaperture imaging system[J]. SPIE,2005, Vol.5638:967~975
[52]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[53]梁士通,杨建峰,薛彬.新型九子镜稀疏孔径结构成像研究[J].光学学报,2009,29(s2):216～220
[54] W. Y. Wang, Z. G. Chen, G. Y. Zhang. Study on optical system based onsynthetic aperture technology[J].Journal of Physics: Conference Series48,(2006):976~982
[1]玻恩,沃尔夫.光学原理（第七版）[M].北京:电子工业出版社,2005
[2]古德曼.傅里叶光学导论（第三版）[M].北京:电子工业出版社,2006
[3]王之江,伍树东.成像光学[M].北京:科学出版社,1991
[4]李晓彤,岑兆丰.几何光学像差光学设计（第二版）[M].杭州:浙江大学出版社,2007
[5] R. D. Fiete, J. A. Mooney, T. A. Tantalo, et al..Image quality assessment ofsparse-aperture designs with decreasing fill factors[J]. SPIE,2000, Vol.4091:64~73
[6] R. D. Fiete, T. A. Tantalo, J. R. Calus, et al..Image quality of sparse-aperturedesigns for remote sensing[J].Opt. Eng.,2002,41(8):1957~1969
[7] J. Fienup. MTF and integration time versus fill factor for sparse-apertureimaging systems[J]. SPIE,2000,Vol.4091:43~47
[8]梁士通,杨建峰,薛彬.新型九子镜稀疏孔径结构成像研究[J].光学学报,2009,29(s2):216～220
[9]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[10] R. E. Introne. Enhanced spectral modeling of sparse aperture imagingsystems[D]. New York: Rochester Institute of Technology,2004
[11] N. R. Block. A sensitivity study of a polychromatic sparse-aperture system[D].New York: Rochester Institute of Technology,2005
[12]阮秋琦.数字图像处理学[M].北京:电子工业出版社.2002
[13]吴泉英,钱霖,沈为民.稀疏孔径系统的成像和图像复原[J].激光杂志,2005,26(6):40~42
[14]李显宏.MATLAB7.x界面设计与编译技巧[M].北京:电子工业出版社,2006
[15] ZEMAX Development Corporation. Optical design program user's guide,2008
[16] N. J. Miller, M. P. Dierking, B. D. Duncan. Optical sparse aperture imaging[J].Appl. Opt.,2007,46(23):5933~5943
[17] B. Richard. Dilute aperture diffraction imagery and object reconstruction[J].Opt. Eng.,1990,29(2):131~139
[18] J. E. Harvey, A. KothaR. L. Phillips.Image characteristics in applicationsutilizing dilute subaperture arrays[J]. Appl. Opt.,1995,34(16):2983~2992
[19]易红伟,李英才,樊超.稀疏孔径等边六孔径结构研究[J].光子学报,2007,36(11):2062~2065
[20] W. Jianguo, J. Shengzhen, N. Shunian.Optimum linear array of an opticalaperture synthesis telescope[J].Chinese Science Bulletin,2002,47(23):1964~1968
[21]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[22] D. Schroeder. Astronomical optics(2nd)[M]. California: Academic Press,2000
[23]吴泉英.稀疏孔径光学系统成像研究[D].苏州:苏州大学,2006
[24] R. D. Fiete, T. A. Tantalo, J. R. Calus, et al..Image quality of sparse-aperturedesigns for remote sensing[J]. Opt. Eng.,2002,41(8):1957~1969
[25] M. J. E. Golay. Point arrays having compact, nonredundant autocorrelations[J].JOSA,1971,61(2):272~273
[1] L. M. Mugnier, G.. Rousset, F. Cassaing. Aperture configuration optimalitycriterion for phased arrays of optical telescopes[J]. JOSA,1996,13(12):2367~2374
[2] M. M. Laurent, R. Gerard.Pupil configuration optimality criterion in syntheticaperture optics[J].SPIE,1995, Vol.2477:124~131
[3] I. Tcherniavski, M. Kahrizi. Optimization of the optical sparse arrayconfiguration[J]. Opt. Eng.,2005,44(10):1032-01~1032-10
[4]陈宝林.最优化理论与算法(第2版)[M].北京:清华大学出版社,2005
[5]李庆扬,王能超,易大义.数值分析(第五版)[M].北京:清华大学出版社,2008
[6] T. J. Cornwell. A novel principle for optimization of the instantaneous fourierplane coverage of correlation arrays[J]. IEEE Trans., Antennas Propag. AP-36,1165~1167(1988)
[7] M. J. E. Golay. Point arrays having compact, nonredundant autocorrelations[J].JOSA,1971,61(2):272~273
[8]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[9]张文修,梁怡.遗传算法的数学基础[M].西安:西安交通大学出版社,2000
[10]龚纯,王正林.精通Matlab最优化计算[M].北京:电子工业出版社,2009
[11]梁士通,杨建峰,李湘眷等.一种新型稀疏孔径结构的研究[J].光子学报,2010,39(1):148~152
[12]梁士通,杨建峰,薛彬.新型九子镜稀疏孔径结构成像研究[J].光学学报,2009,29(s2):216～220
[13]冈萨雷斯,阮秋琦.数字图像处理(MATLAB版)[M].北京:电子工业出版社,2007
[14]吴泉英,钱霖,沈为民.稀疏孔径系统的成像和图像复原研究[J].激光杂志,2005.26(6):40~42
[15]吴泉英,钱霖,沈为民.两种稀疏孔径系统的成像研究[J].光学精密工程,2006.14(01):26~33
[1]李晓彤,岑兆丰.几何光学像差光学设计（第二版）[M].杭州:浙江大学出版社,2007
[2]张以谟.应用光学(第三版)[M].北京:电子工业出版社,2008
[3] W. J. Smith. Modern optical engineering (4th ed.)[M].New York: McGraw-HillCompanies,2008
[4] H. H. Hopkins. Wave theory of aberrations[M].New York: Oxford UniversityPress,1950
[5]古德曼.傅里叶光学导论（第三版）[M].北京:电子工业出版社,2006
[6] R. B. Hooker. The Effects of aberrations in synthetic aperture systems[D].Arizona: University of Arizona,1974
[7]郑君里,应启珩,杨为理.信号与系统(第二版)[M].北京:高等教育出版社,2000
[8] V. N. Mahajan. Strehl ratio for primary aberrations: some analytical results forcircular and annular pupils[J].JOSA,1982,72(9):1258~1266
[9] V. N. Mahajan. Strehl ratio for primary aberrations in terms of their aberrationvariance[J]. JOSA,1983,73(6):860~861
[10] W. T. Welford. Aberrations of optical system[M]. London: Taylor&FrancisGroup,1986
[11] J. L. Flores, M. Strojnik, G. Paez,et al..Effects of misalignment errors on theoptical transfer functions of synthetic aperture telescopes[J].Appl. Opt.,2004,43(32):5926-5932
[12] E. E. Sabatke, J. H. Burge, P. Hinz.Optical design of interferometric telescopeswith wide fields of view[J].Appl. Opt.,2006,45(31):8026~8035
[13] D. Malacara. Optical shop testing(3rd ed.)[M].New Jersey: John Wiley&SonsInc.,2007
[14] D. Malacara, M. Servin, Z. Malacara. Interferogram analysis for optical testing(2nd ed.)[M]. CRC Press.2005
[15] R. R. Butts.Effects of piston and tilt errors on the performance of multiplemirror telescope[J]. SPIE,1981,Vol.293:85~89
[16] G. M. Sanger. The techniques and tolerancing required for phasing hexagonallyconfigured synthetic aperture imaging systems[D].Arizona: University ofArizona,1976
[17] L. D. Barr. An update on the15-m national new technology telescope[J]. SPIE,1986, Vol.643:234~243
[18]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[19] J. E. Harvey, C. Ftaclas. Field-of-view limitations of phased telescope arrays[J].Appl. Opt.,1995,34(25):5787~5798
[20]周仁忠主编.自适应光学[M].北京:国防工业出版社,1996
[21] J. Q. Cheng. The principles of astronomical telescope design[M].New York:Springer,2009
[22] J. R. Fienup.Phase retrieval algorithms: a comparison[J].Appl. Opt.,1982,21(15):2758-2769
[23] R. G. Paxman, B. J. Thelen, R. J. Murphy,et al.. Phase-diverse adaptive opticsfor future telescopes[J]. SPIE,2007,Vol.6711:671103~671115
[24] Gonsalves. Phase retrieval and diversity in adaptive optics[J]. Opt. Eng.,1982,21(5):829~832
[25] R. G. Paxman, J. R. Fienup. Optical misalignment sensing and imagereconstruction using phase diversity[J]. JOSA,1988,5(6):914~923
[26] R. G. Paxman, T. J. Schulz, J, R. Fienup. Joint estimation of object andaberrations by using phase diversity[J].JOSA,1992,9(7):1072~1085
[27] R. L. Kendrick, D. S. Acton, A. L. Duncan. Phase-diversity wave-front sensorfor imaging systems[J].Appl. Opt.,1994,33(27):6533~6546
[28] J. R. Fienup. Phase retrieval for undersampled broadband images[J]. JOSA,1999.16(7):1831~1837.
[29] R. L. Kendrick, D. S. Acton, A. L. Duncan. Experimental results from theLockheed Phase Diversity Test Facility[J].SPIE,1994,Vol.2302:312~322
[30] A. Blanc, L. M. Mugnier, J. Idier. Marginal estimation of aberrations and imagerestoration by use of phase diversity[J].JOSA,2003,20(6):1035~1045
[31] L. Meynadier, V. Michau, M. T. Velluet, et al.. Noise propagation in wave frontsensing with phase diversity[J]. Appl. Opt.,1999,38(23):4967~4979
[32] Ellerbroek, Rafanelli, et al.. Piston error estimation method for segmentedaperture optical systems while observing arbitrary unknown extended scenes[P].US Patent:5128530,1992-07-07
[33] B. H. Dean,C. W. Bowers.Diversity selection for phase-diverse phaseretrieval[J]. JOSA,2003,20(8):1490-1504
[34] J. H. Seldin, R. G. Paxman, V. G. Zarifis, et al.. Closed-loop wavefront sensingfor a sparse-aperture multitelescope array using broadband phase diversity[J].SPIE,2000, Vol.4091:48~63
[35] H. I. Campbell, S. Zhang, A. H. Greenaway, et al..Generalized phase diversityfor wave-front sensing[J].Optics Letters,2004,29(23):2707~2709
[36]张文修,梁怡.遗传算法的数学基础[M].西安:西安交通大学出版社,2000
[37]冈萨雷斯,阮秋琦.数字图像处理(MATLAB版)[M].北京:电子工业出版社,2007
[38] W. A. Traub. Combining beams from separated telescopes[J]. Appl. Opt.,1986,25(4):528~532
[39] L. D. Weaver, J. S. Fender, C. R. De Hainaut. Design considerations formultiple telescope imaging arrays[J]. Opt. Eng.1988,27(9):730~735
[40] C. M. Lampkin, G.W. Flint, M. J. MacFarlane. Optical and mechanical designaspects of a four-telescope array for combined imaging[J]. Opt. Eng.1988,27(9):749~754
[1] F. Cassaing, B. Sorrente, B. Fleury,et al..Optical design of a Michelsonwide-field multiple-aperture telescope[J].SPIE,2004,Vol.5249:220~229
[2] A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt.,1970,9(11):2501~2504
[3] R.N. Wilson. Reflecting telescope optics I[M].New York:Springer,2007
[4] K. D. Bell, R. L. Moser, M. K. Powers, et al.. Deployable optical telescopeground demonstration[J]. SPIE,2000,4013:559~567
[5] J. Q. Cheng. The Principles of astronomical telescope design[M].New York:Springer,2009
[6] L. D. Weaver, J. S. Fender, C. R. De Hainaut. Design considerations formultiple telescope imaging arrays[J]. Opt. Eng.1988,27(9):730~735
[7] E. N. JerryR. G. Peter. Overview of the performance of the W.M. KeckObservatory[J]. SPIE,1994, Vol.2199:82~93
[8] http://www.jwst.nasa.gov
[9] T. W. Stuhlinger. All-reflective phased array imaging telescopes[J]. SPIE,1991,Vol.1354:438~446
[10] C. H. Miao, R. R. Shannon. Design of wide-field arrays[J]. SPIE,1990, Vol.1236:372~373
[11] C. H. Miao. The design of phased synthetic aperture imaging systems using aminimum number of elements[D]. Arizona: University of Arizona,1991
[12] P. W. Scott.Some design considerations for a synthetic aperture opticaltelescope array[J].SPIE,1983, Vol.440:126~129
[13] M. Bass. Handbook of optics Vol.1(3rd ed.)[M].New York, McGraw-HillCompanies,2010
[14] W. J. Smith. Modern optical engineering (4th ed.)[M].New York, McGraw-HillCompanies,2008
[15]潘君骅.光学非球面的设计、加工与检验[M].苏州:苏州大学出版社,2004
[16] X. Z. Ding, X. Wang, W. H. Lan, et al. Design of four-mirror reflective anasti-gmat optic system[J].Infrared and Laser Engineering,2008,37(2):319~321
[17] J. M. Howard, B. D. Stone, Imaging with four spherical mirrors[J]. Appl. Opt.,2000,39(19):3232~3242
[18] A. B. Meinel. Four-mirror spherical-primary submillimeter telescope design[J].Appl. Opt.,1984,23(17):3020~3023
[19] L. G. Cook. Compact four-mirror anastigmat telescope[P]. US Patent,6767103B2,2004
[1] A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt.,1970,9(11):2501~2504
[2] E. K. Hege, J. M. Beckers, P. A. Strittmatter, et al.. Multiple mirror telescope asa phased array telescope[J]. Appl. Opt.,1985,24(16):2565~2576
[3] R. B. Hooker. The effects of aberrations in synthetic aperture systems[D].Arizona: University of Arizona,1974
[4] M. S. Erin. Fundamentals of the optical design of mulitiple aperture telescopeswith wide fields of view[D]. Arizona: University of Arizona,2002
[5]朱瑶.光学系统的星点检验方法[J].红外,2004(9):31~37
[6]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[7]吴泉英.稀疏孔径光学系统成像研究[D].苏州:苏州大学,2006
[8]李兰芳.光学综合孔径成像技术的实验研究[D].南京:南京理工大学,2004
[9] R. A. Carreras, S. J. Cusumano, M. G.Andrews, et al.. Overview of a phasedarray experiment[J]. SPIE,1983, Vol.440:168~172
[10] V. Zarifis, R. M. Bell, L. R. Benson,et al.. The multi aperture imaging array[J].Proc. from ASP Conference,1999, Vol.194
[11] R. L. Kendrick, J.N. Aubrun, R. Bell,et al. Wide-field Fizeau imaging telescope:experimental results[J]. Appl. Opt.,2006,45(18):4235~4240
[12] C. Soon-Jo, W. M. David, L. d. W. Olivier.ARGOS testbed: study ofmultidisciplinary challenges of future spaceborne interferometric arrays[J]. Opt.Eng.,2004,43(9):2156~2167
[13] B. D. O'Neil, C. R. DeHainaut, P. Menicucci, et al.. Four-telescope phased arrayoptical simulation[J]. SPIE,1990, Vol.1236:406~423
[2] http://en.wikipedia.org/wiki/KH-11
[3]杨秉新.美国IKONOS和QuickBird2卫星相机的主要性能和特点分析及看法[J].航天返回与遥感,2002,23(4): l4~16
[4] http://en.wikipedia.org/wiki/QuickBird
[5]吴玉石.高分辨率传输型侦察卫星技术的发展[J].航天器工程,2003,12(1):64~73
[6]郭今昌.商用高分辨率光学遥感卫星及平台技术分析[J].航天器工程,2009,18(2):83~89
[7]王金堂,乌崇德.国外几种星载光学遥感器的发展情况简介[J].航天返回与遥感,2002,23(2):15~20
[8]顾先冰,司群英.国内外遥感卫星发展现状[J].航天返回与遥感,2000,21(2):29~33
[9]玻恩,沃尔夫.光学原理（第七版）[M].北京:电子工业出版社,2005
[10] http://en.wikipedia.org/wiki/Hubble
[11] D. Schroeder. Astronomical optics(2nd)[M].California:Academic Press,2000
[12] A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt.,1970,9(11):2501~2504
[13] E. K. Hege, J. M. Beckers, P. A. Strittmatter, et al.. Multiple mirror telescope asa phased array telescope[J]. Appl. Opt.,1985,24(16):2565~2576
[14] W. A. Traub. Combining beams from separated telescopes[J]. Appl. Opt.,1986,25(4):528~532
[15] J. S. Fender. Phase array optical system[J]. SPIE,1986, Vol.643:122~128
[16] Fizeau, H.1868C. R. Hebd. Seanc. Acad. Sci. Paris66,932
[17] Advisory Committee To The Air Force Systems Command. Synthetic-apertureoptics Vol.1[C]. Washington D C: Defense Technical Information Center,1967
[18] Advisory Committee To The Air Force Systems Command. Synthetic-apertureoptics Vol.2[C]. Washington D C: Defense Technical Information Center,1967
[19] M. J. E. Golay. Point arrays having compact, nonredundant autocorrelations[J].JOSA,1971,61(2):272~273
[20] R. B. Hooker. The effects of aberrations in synthetic aperture systems[D].Arizona: University of Arizona,1974
[21] J. E. Harvey, C. Ftaclas. Field-of-view limitations of phased telescope arrays[J].Appl. Opt.,1995,34(25):5787~5798
[22] J. E. Harvey, C. Ftaclas. Fundamental limitations on off-axis performance ofphased telescope arrays[J]. SPIE,1990,Vol.1236
[23] Gonsalves. Phase retrieval and diversity in adaptive optics[J]. Opt. Eng.,1982,21(5):829~832
[24] R. G. Paxman, J. R. Fienup. Optical misalignment sensing and imagereconstruction using phase diversity[J]. JOSA,1988,5(6):914~923
[25] R. G. Paxman, T. J. Schulz, J, R. Fienup. Joint estimation of object andaberrations by using phase diversity[J].JOSA,1992,9(7):1072~1085
[26] J. Fienup.MTF and integration time versus fill factor for sparse-apertureimaging systems[J]. SPIE,2000, Vol.4091:43~47
[27] R. D. Fiete, J. A. Mooney, T. A. Tantalo, et al.. Image quality assessment ofsparse-aperture designs with decreasing fill factors[J]. SPIE,2000,4091:64~73
[28] R. D. Fiete, T. A. Tantalo, J. R. Calus,et al.. Image quality of sparse-aperturedesigns for remote sensing[J]. Opt. Eng.,2002,41(8):1957-1969
[29] T. W. Stuhlinger. All-reflective phased array imaging telescopes[J]. SPIE,1991,Vol.1354:438~446
[30] C. H. Miao, R. R. Shannon. Design of wide-field arrays[J]. SPIE,1990, Vol.1236:372~378
[31] C. H. Miao. The design of phased synthetic aperture imaging systems using aminimum number of elements[D]. Arizona: University of Arizona,1991
[32] M. S. Erin. Fundamentals of the optical design of mulitiple aperture telescopeswith wide fields of view[D]. Arizona: University of Arizona,2002
[33] R. E. Introne. Enhanced spectral modeling of sparse aperture imagingsystems[D]. New York: Rochester Institute of Technology,2004
[34] N. R. Block. A sensitivity study of a polychromatic sparse-aperture system[D].New York: Rochester Institute of Technology,2005
[35] E. K. Hege, J. M. Beckers, P. A. Strittmatter, et al.. Multiple mirror telescope asa phased array telescope[J]. Appl. Opt.,1985,24(16):2565~2576
[36] A. C. Gary, S. M. Terry, E. N. Jerry, et al.. Phasing the mirror segments of theW.M. Keck telescope[J]. SPIE,1994,2199:622~637
[37] G. Chanan, C. Ohara, M. Troy. Phasing the mirror segments of the Kecktelescopes II: the narrow-band phasing algorithm[J]. Appl. Opt.,2000,39(25):4706~4714
[38] E. N. Jerry, R. G. Peter. Overview of the performance of the W.M. KeckObservatory[J]. SPIE,1994,2199:82~93
[39] E. E. Sabatke, J. H. Burge, P. Hinz.Optical design of interferometric telescopeswith wide fields of view[J]. Appl. Opt.,2006,45(31):8026~8035
[40] J. M. Hill, R. F. Green, J. H. Slagle.The large binocular telescope[J].SPIE,2006,Vol.6267:62670Y-1~15
[41] J. M. Beckers. VLT Interferometer: III. Factors affecting wide field-of-viewoperation[J]. SPIE,1990, Vol.1236:379~389
[42] V. Zarifis, R. M. Bell, L. R. Benson,et al.. The multi aperture imaging array[J].Proc. from ASP Conference Vol.194,1999
[43] R. L. Kendrick, J.-N. Aubrun, R. Bell,et al. Wide-field Fizeau imagingtelescope: experimental results[J].Appl. Opt.,2006,45(18):4235~4240
[44] K. D. Bell, R. L. Moser, M. K. Powers, et al.. Deployable optical telescopeground demonstration[J]. SPIE,2000,4013:559~567
[45] C. Soon-Jo, W. M. David, L. d. W. Olivier.ARGOS testbed: study ofmultidisciplinary challenges of future spaceborne interferometric arrays[J]. Opt.Eng.,2004,43(9):2156~2167
[46] G. Rousset, L. Mugnier. Imaging with multi aperture optical telescopes and anapplication[J]. Comptes Rendusdel Academie des Sciences Series IV Physucs,2001,2(1):17~25
[47] L. M. Mugnier, F. Cassaing, G. Rousset, et al.. Earth observation from a highorbit: pushing the limits with synthetic aperture optics[R].P228010,2000
[48] M. Mesrine, E. Thomas, S. Garin, et al.. High resolution earth observation fromgeostationary orbit by optical aperture synthesys[C]. Proc.6th Internat. Conf.on Space Optics,2006
[49]王海涛,周必方.天文光干涉技术[J].光学精密工程,2003,11(4):320-325
[50]吴泉英.稀疏孔径光学系统成像研究[D].苏州:苏州大学,2006
[51] Wang Zhile, Zhang Wei, Deng Jian, et al..Image evaluation for optical syntheticaperture imaging system[J]. SPIE,2005, Vol.5638:967~975
[52]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[53]梁士通,杨建峰,薛彬.新型九子镜稀疏孔径结构成像研究[J].光学学报,2009,29(s2):216～220
[54] W. Y. Wang, Z. G. Chen, G. Y. Zhang. Study on optical system based onsynthetic aperture technology[J].Journal of Physics: Conference Series48,(2006):976~982
[1]玻恩,沃尔夫.光学原理（第七版）[M].北京:电子工业出版社,2005
[2]古德曼.傅里叶光学导论（第三版）[M].北京:电子工业出版社,2006
[3]王之江,伍树东.成像光学[M].北京:科学出版社,1991
[4]李晓彤,岑兆丰.几何光学像差光学设计（第二版）[M].杭州:浙江大学出版社,2007
[5] R. D. Fiete, J. A. Mooney, T. A. Tantalo, et al..Image quality assessment ofsparse-aperture designs with decreasing fill factors[J]. SPIE,2000, Vol.4091:64~73
[6] R. D. Fiete, T. A. Tantalo, J. R. Calus, et al..Image quality of sparse-aperturedesigns for remote sensing[J].Opt. Eng.,2002,41(8):1957~1969
[7] J. Fienup. MTF and integration time versus fill factor for sparse-apertureimaging systems[J]. SPIE,2000,Vol.4091:43~47
[8]梁士通,杨建峰,薛彬.新型九子镜稀疏孔径结构成像研究[J].光学学报,2009,29(s2):216～220
[9]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[10] R. E. Introne. Enhanced spectral modeling of sparse aperture imagingsystems[D]. New York: Rochester Institute of Technology,2004
[11] N. R. Block. A sensitivity study of a polychromatic sparse-aperture system[D].New York: Rochester Institute of Technology,2005
[12]阮秋琦.数字图像处理学[M].北京:电子工业出版社.2002
[13]吴泉英,钱霖,沈为民.稀疏孔径系统的成像和图像复原[J].激光杂志,2005,26(6):40~42
[14]李显宏.MATLAB7.x界面设计与编译技巧[M].北京:电子工业出版社,2006
[15] ZEMAX Development Corporation. Optical design program user's guide,2008
[16] N. J. Miller, M. P. Dierking, B. D. Duncan. Optical sparse aperture imaging[J].Appl. Opt.,2007,46(23):5933~5943
[17] B. Richard. Dilute aperture diffraction imagery and object reconstruction[J].Opt. Eng.,1990,29(2):131~139
[18] J. E. Harvey, A. KothaR. L. Phillips.Image characteristics in applicationsutilizing dilute subaperture arrays[J]. Appl. Opt.,1995,34(16):2983~2992
[19]易红伟,李英才,樊超.稀疏孔径等边六孔径结构研究[J].光子学报,2007,36(11):2062~2065
[20] W. Jianguo, J. Shengzhen, N. Shunian.Optimum linear array of an opticalaperture synthesis telescope[J].Chinese Science Bulletin,2002,47(23):1964~1968
[21]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[22] D. Schroeder. Astronomical optics(2nd)[M]. California: Academic Press,2000
[23]吴泉英.稀疏孔径光学系统成像研究[D].苏州:苏州大学,2006
[24] R. D. Fiete, T. A. Tantalo, J. R. Calus, et al..Image quality of sparse-aperturedesigns for remote sensing[J]. Opt. Eng.,2002,41(8):1957~1969
[25] M. J. E. Golay. Point arrays having compact, nonredundant autocorrelations[J].JOSA,1971,61(2):272~273
[1] L. M. Mugnier, G.. Rousset, F. Cassaing. Aperture configuration optimalitycriterion for phased arrays of optical telescopes[J]. JOSA,1996,13(12):2367~2374
[2] M. M. Laurent, R. Gerard.Pupil configuration optimality criterion in syntheticaperture optics[J].SPIE,1995, Vol.2477:124~131
[3] I. Tcherniavski, M. Kahrizi. Optimization of the optical sparse arrayconfiguration[J]. Opt. Eng.,2005,44(10):1032-01~1032-10
[4]陈宝林.最优化理论与算法(第2版)[M].北京:清华大学出版社,2005
[5]李庆扬,王能超,易大义.数值分析(第五版)[M].北京:清华大学出版社,2008
[6] T. J. Cornwell. A novel principle for optimization of the instantaneous fourierplane coverage of correlation arrays[J]. IEEE Trans., Antennas Propag. AP-36,1165~1167(1988)
[7] M. J. E. Golay. Point arrays having compact, nonredundant autocorrelations[J].JOSA,1971,61(2):272~273
[8]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[9]张文修,梁怡.遗传算法的数学基础[M].西安:西安交通大学出版社,2000
[10]龚纯,王正林.精通Matlab最优化计算[M].北京:电子工业出版社,2009
[11]梁士通,杨建峰,李湘眷等.一种新型稀疏孔径结构的研究[J].光子学报,2010,39(1):148~152
[12]梁士通,杨建峰,薛彬.新型九子镜稀疏孔径结构成像研究[J].光学学报,2009,29(s2):216～220
[13]冈萨雷斯,阮秋琦.数字图像处理(MATLAB版)[M].北京:电子工业出版社,2007
[14]吴泉英,钱霖,沈为民.稀疏孔径系统的成像和图像复原研究[J].激光杂志,2005.26(6):40~42
[15]吴泉英,钱霖,沈为民.两种稀疏孔径系统的成像研究[J].光学精密工程,2006.14(01):26~33
[1]李晓彤,岑兆丰.几何光学像差光学设计（第二版）[M].杭州:浙江大学出版社,2007
[2]张以谟.应用光学(第三版)[M].北京:电子工业出版社,2008
[3] W. J. Smith. Modern optical engineering (4th ed.)[M].New York: McGraw-HillCompanies,2008
[4] H. H. Hopkins. Wave theory of aberrations[M].New York: Oxford UniversityPress,1950
[5]古德曼.傅里叶光学导论（第三版）[M].北京:电子工业出版社,2006
[6] R. B. Hooker. The Effects of aberrations in synthetic aperture systems[D].Arizona: University of Arizona,1974
[7]郑君里,应启珩,杨为理.信号与系统(第二版)[M].北京:高等教育出版社,2000
[8] V. N. Mahajan. Strehl ratio for primary aberrations: some analytical results forcircular and annular pupils[J].JOSA,1982,72(9):1258~1266
[9] V. N. Mahajan. Strehl ratio for primary aberrations in terms of their aberrationvariance[J]. JOSA,1983,73(6):860~861
[10] W. T. Welford. Aberrations of optical system[M]. London: Taylor&FrancisGroup,1986
[11] J. L. Flores, M. Strojnik, G. Paez,et al..Effects of misalignment errors on theoptical transfer functions of synthetic aperture telescopes[J].Appl. Opt.,2004,43(32):5926-5932
[12] E. E. Sabatke, J. H. Burge, P. Hinz.Optical design of interferometric telescopeswith wide fields of view[J].Appl. Opt.,2006,45(31):8026~8035
[13] D. Malacara. Optical shop testing(3rd ed.)[M].New Jersey: John Wiley&SonsInc.,2007
[14] D. Malacara, M. Servin, Z. Malacara. Interferogram analysis for optical testing(2nd ed.)[M]. CRC Press.2005
[15] R. R. Butts.Effects of piston and tilt errors on the performance of multiplemirror telescope[J]. SPIE,1981,Vol.293:85~89
[16] G. M. Sanger. The techniques and tolerancing required for phasing hexagonallyconfigured synthetic aperture imaging systems[D].Arizona: University ofArizona,1976
[17] L. D. Barr. An update on the15-m national new technology telescope[J]. SPIE,1986, Vol.643:234~243
[18]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[19] J. E. Harvey, C. Ftaclas. Field-of-view limitations of phased telescope arrays[J].Appl. Opt.,1995,34(25):5787~5798
[20]周仁忠主编.自适应光学[M].北京:国防工业出版社,1996
[21] J. Q. Cheng. The principles of astronomical telescope design[M].New York:Springer,2009
[22] J. R. Fienup.Phase retrieval algorithms: a comparison[J].Appl. Opt.,1982,21(15):2758-2769
[23] R. G. Paxman, B. J. Thelen, R. J. Murphy,et al.. Phase-diverse adaptive opticsfor future telescopes[J]. SPIE,2007,Vol.6711:671103~671115
[24] Gonsalves. Phase retrieval and diversity in adaptive optics[J]. Opt. Eng.,1982,21(5):829~832
[25] R. G. Paxman, J. R. Fienup. Optical misalignment sensing and imagereconstruction using phase diversity[J]. JOSA,1988,5(6):914~923
[26] R. G. Paxman, T. J. Schulz, J, R. Fienup. Joint estimation of object andaberrations by using phase diversity[J].JOSA,1992,9(7):1072~1085
[27] R. L. Kendrick, D. S. Acton, A. L. Duncan. Phase-diversity wave-front sensorfor imaging systems[J].Appl. Opt.,1994,33(27):6533~6546
[28] J. R. Fienup. Phase retrieval for undersampled broadband images[J]. JOSA,1999.16(7):1831~1837.
[29] R. L. Kendrick, D. S. Acton, A. L. Duncan. Experimental results from theLockheed Phase Diversity Test Facility[J].SPIE,1994,Vol.2302:312~322
[30] A. Blanc, L. M. Mugnier, J. Idier. Marginal estimation of aberrations and imagerestoration by use of phase diversity[J].JOSA,2003,20(6):1035~1045
[31] L. Meynadier, V. Michau, M. T. Velluet, et al.. Noise propagation in wave frontsensing with phase diversity[J]. Appl. Opt.,1999,38(23):4967~4979
[32] Ellerbroek, Rafanelli, et al.. Piston error estimation method for segmentedaperture optical systems while observing arbitrary unknown extended scenes[P].US Patent:5128530,1992-07-07
[33] B. H. Dean,C. W. Bowers.Diversity selection for phase-diverse phaseretrieval[J]. JOSA,2003,20(8):1490-1504
[34] J. H. Seldin, R. G. Paxman, V. G. Zarifis, et al.. Closed-loop wavefront sensingfor a sparse-aperture multitelescope array using broadband phase diversity[J].SPIE,2000, Vol.4091:48~63
[35] H. I. Campbell, S. Zhang, A. H. Greenaway, et al..Generalized phase diversityfor wave-front sensing[J].Optics Letters,2004,29(23):2707~2709
[36]张文修,梁怡.遗传算法的数学基础[M].西安:西安交通大学出版社,2000
[37]冈萨雷斯,阮秋琦.数字图像处理(MATLAB版)[M].北京:电子工业出版社,2007
[38] W. A. Traub. Combining beams from separated telescopes[J]. Appl. Opt.,1986,25(4):528~532
[39] L. D. Weaver, J. S. Fender, C. R. De Hainaut. Design considerations formultiple telescope imaging arrays[J]. Opt. Eng.1988,27(9):730~735
[40] C. M. Lampkin, G.W. Flint, M. J. MacFarlane. Optical and mechanical designaspects of a four-telescope array for combined imaging[J]. Opt. Eng.1988,27(9):749~754
[1] F. Cassaing, B. Sorrente, B. Fleury,et al..Optical design of a Michelsonwide-field multiple-aperture telescope[J].SPIE,2004,Vol.5249:220~229
[2] A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt.,1970,9(11):2501~2504
[3] R.N. Wilson. Reflecting telescope optics I[M].New York:Springer,2007
[4] K. D. Bell, R. L. Moser, M. K. Powers, et al.. Deployable optical telescopeground demonstration[J]. SPIE,2000,4013:559~567
[5] J. Q. Cheng. The Principles of astronomical telescope design[M].New York:Springer,2009
[6] L. D. Weaver, J. S. Fender, C. R. De Hainaut. Design considerations formultiple telescope imaging arrays[J]. Opt. Eng.1988,27(9):730~735
[7] E. N. JerryR. G. Peter. Overview of the performance of the W.M. KeckObservatory[J]. SPIE,1994, Vol.2199:82~93
[8] http://www.jwst.nasa.gov
[9] T. W. Stuhlinger. All-reflective phased array imaging telescopes[J]. SPIE,1991,Vol.1354:438~446
[10] C. H. Miao, R. R. Shannon. Design of wide-field arrays[J]. SPIE,1990, Vol.1236:372~373
[11] C. H. Miao. The design of phased synthetic aperture imaging systems using aminimum number of elements[D]. Arizona: University of Arizona,1991
[12] P. W. Scott.Some design considerations for a synthetic aperture opticaltelescope array[J].SPIE,1983, Vol.440:126~129
[13] M. Bass. Handbook of optics Vol.1(3rd ed.)[M].New York, McGraw-HillCompanies,2010
[14] W. J. Smith. Modern optical engineering (4th ed.)[M].New York, McGraw-HillCompanies,2008
[15]潘君骅.光学非球面的设计、加工与检验[M].苏州:苏州大学出版社,2004
[16] X. Z. Ding, X. Wang, W. H. Lan, et al. Design of four-mirror reflective anasti-gmat optic system[J].Infrared and Laser Engineering,2008,37(2):319~321
[17] J. M. Howard, B. D. Stone, Imaging with four spherical mirrors[J]. Appl. Opt.,2000,39(19):3232~3242
[18] A. B. Meinel. Four-mirror spherical-primary submillimeter telescope design[J].Appl. Opt.,1984,23(17):3020~3023
[19] L. G. Cook. Compact four-mirror anastigmat telescope[P]. US Patent,6767103B2,2004
[1] A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt.,1970,9(11):2501~2504
[2] E. K. Hege, J. M. Beckers, P. A. Strittmatter, et al.. Multiple mirror telescope asa phased array telescope[J]. Appl. Opt.,1985,24(16):2565~2576
[3] R. B. Hooker. The effects of aberrations in synthetic aperture systems[D].Arizona: University of Arizona,1974
[4] M. S. Erin. Fundamentals of the optical design of mulitiple aperture telescopeswith wide fields of view[D]. Arizona: University of Arizona,2002
[5]朱瑶.光学系统的星点检验方法[J].红外,2004(9):31~37
[6]易红伟.光学稀疏孔径成像系统关键问题研究[D].西安:中国科学院西安光学精密机械研究所,2007
[7]吴泉英.稀疏孔径光学系统成像研究[D].苏州:苏州大学,2006
[8]李兰芳.光学综合孔径成像技术的实验研究[D].南京:南京理工大学,2004
[9] R. A. Carreras, S. J. Cusumano, M. G.Andrews, et al.. Overview of a phasedarray experiment[J]. SPIE,1983, Vol.440:168~172
[10] V. Zarifis, R. M. Bell, L. R. Benson,et al.. The multi aperture imaging array[J].Proc. from ASP Conference,1999, Vol.194
[11] R. L. Kendrick, J.N. Aubrun, R. Bell,et al. Wide-field Fizeau imaging telescope:experimental results[J]. Appl. Opt.,2006,45(18):4235~4240
[12] C. Soon-Jo, W. M. David, L. d. W. Olivier.ARGOS testbed: study ofmultidisciplinary challenges of future spaceborne interferometric arrays[J]. Opt.Eng.,2004,43(9):2156~2167
[13] B. D. O'Neil, C. R. DeHainaut, P. Menicucci, et al.. Four-telescope phased arrayoptical simulation[J]. SPIE,1990, Vol.1236:406~423