期刊文献+

直线阵光学综合孔径成像中的子孔径尺寸效应 被引量:14

Size Effects of Sub-Aperture on Imaging of Linear Array of Optical Synthetic Aperture
原文传递
导出
摘要 光学综合孔径阵列中的子孔径的位置和直径的大小对成像质量有着重要的影响。详细分析了几种不同优化排列的光学综合孔径直线阵列的无像差点扩展函数、光学传递函数和衍射成像特性,结果表明,子孔径的位置不同,光学传递函数的空间频率覆盖有很大的差异。增大子孔径的直径可以增大空间频率覆盖程度,但子孔径直径过大时又会产生空间频率冗余度和增加制造成本。直线阵光学综合孔径的衍射成像是多重像,子孔径直径的增大还可以减小重影的程度,提高成像质量。结果说明,在进行光学综合孔径阵列优化排列时必须考虑子孔径的直径大小这个重要的因素。 Positions and diameters of sub-aperture in optical synthetic aperture array are two important factor for imaging. The characteristics of point spread function, optical transfer function and diffraction image of several different optimized linear array configuration of optical aperture synthesis with aberration-free are discussed by using an approach based on ratio of diameter of sub-aperture to length of arrays. The results of simulated computation show that cover of spatial frequencies for optical transfer function are very different for different position of sub-aperture.The bigger the diameter of sub-aperture is, the more complete the spatial frequency covers. But when the ratio exceeds some extent, the spatial frequencies will be redundant and cost of system construction will increase. Besides,increase of sub-aperture can decrease the intensity of the ghost images and intensified the quality of imaging. The results show that the factors of diameter of sub-aperture and total length of arrays must be taken into account in the optimizations.
作者 江月松
出处 《光学学报》 EI CAS CSCD 北大核心 2005年第8期1042-1047,共6页 Acta Optica Sinica
基金 国防预研基金(6140434)资助课题。
关键词 成像系统 光学综合孔径 空间频率覆盖 子孔径尺寸 imaging systems optical synthetic aperture space frequency cover size of sub-aperture
  • 相关文献

参考文献13

  • 1A. B. Meinel. Aperture synthesis using independent telescopes[J]. Appl. Opt., 1970, 9(11): 2501-2504.
  • 2V. N. Sintsov, A. F. Zapryagaev. Aperture synthesis in optics[J]. Soy. Phys. Usp. 1975, 17(6):931-941.
  • 3C. A. Haniff, C. D. Mackay, D. J. Titterington et al.. The first images from optical aperture synthesis[J]. Nature, 1987,328(6132): 694-696.
  • 4王海涛,周必方.光学综合孔径干涉成像技术[J].光学精密工程,2002,10(5):434-442. 被引量:19
  • 5J. E. Baldwin, M. G. Beckett, R. C. Boyson et al.. The first images from an optical aperture synthesis array: mapping of capella with COAST at two epochs [J ]. Astronomy and Astrophysics, 1996, 306:L13-L16.
  • 6王海涛,周必方.光学综合孔径望远镜阵的光束组合器[J].光学学报,2002,22(9):1109-1115. 被引量:24
  • 7范伟军,周必方,王海涛,夏良正.光学综合孔径成像中的傅里叶相位研究[J].光学学报,2004,24(3):408-412. 被引量:11
  • 8范伟军,夏良正,周必方.光学综合孔径像面干涉数学模型与计算机仿真[J].红外与毫米波学报,2004,23(2):143-147. 被引量:3
  • 9Richard Barakat. Dilute aperture dlffraclion imagery and object reconstruction[J]. Opt. Engng.. 1990. 29(2): 131-139.
  • 10J. T. Armstrong, D. Mozurkewich. L. J. Rickard et al.. The Navy prototype optical interferometer[J].The Astrophysical J..1998. 496(1):550-571.

二级参考文献12

  • 1Zhao Peiqian Zhou Bifang 等.-[J].光学学报,1994,14(7):784-751.
  • 2Zhou Bifang Zhao Peiqing.-[J].天文学报,1992,33(2):212-219.
  • 3Zhou Bifang Mao Weijun.天文仪器与技术[M].-,1998.34-49.
  • 4Liang Quanting.物理光学[M].-,1980.101-112.
  • 5李继陶.统计光学基础[M].四川:四川大学出版社,1998..
  • 6陶纯堪 陶纯匡.光子信息论[M].北京:科学出版社,1999.187-208.
  • 7Schoeller M. Fizeau beam combination with optical interferometers-some ideas for second generation VLTI instrumentation[J]. SPIE, 2000, 4006:116-123
  • 8Hege E K, Agel J R P, Cheslka M. et al. Simulation of aperture synthesis with the large binocular telescope [ J ].SPIE, 1995, 2566:144-155
  • 9Crokett G A, Strange D A. Computer model for evaluating synthetic aperture propagation[ J]. SPIE, 1983, 440: 77-84
  • 10邱耀辉,刘忠,卢汝为,楼柯.CLEAN算法在天文图像空域重建中的应用[J].云南天文台台刊,2000(2):1-9. 被引量:9

共引文献44

同被引文献108

引证文献14

二级引证文献71

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部