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光场相机波前传感器性能分析 被引量:3

Performance Analysis of Light Field Wave-Front Sensor
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摘要 提出了一种光场相机波前传感器的成像模拟方法,该方法将微透镜阵列等效为一个相位掩膜,考虑了微透镜之间的干涉效应。数值模拟显示,不存在波前畸变时,光场相机的波前斜率输出不为零,降低了波前重构精度;光场相机波前传感器的线性度随着微透镜尺寸的减小而提高,然而存在一个与波前畸变程度有关的最优微透镜尺寸,使波前复原精度最高;与哈特曼波前传感器相比,在国内典型大气条件下,光场相机的波前重构精度略低。 A light field wavefront sensor camera image formation solution based on modelling micro-lens array as a phase mask is proposed, which considers the interference between lenslets. Numerical simulation shows that light field wavefront sensor gradient signals are not null when the input wavefront is unaberrated, which decreases the wavefront reconstruction precision. The linearity of light field wavefront sensor improves when the size of lenslet decreases. There exists an optimal lenslet size to make the wavefront reconstruction error least. Compared with Hartmann wavefront sensor, the wavefront reconstruction precision of light field wavefront is a bit lower.
出处 《光学学报》 EI CAS CSCD 北大核心 2014年第B12期1-7,共7页 Acta Optica Sinica
关键词 测量 光场相机 波前测量 相位掩膜 哈特曼传感器 measurement light field camera wavefront sensing phase mask Hartmann sensor
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参考文献8

  • 1J W Hardy. Adaptive Optics for Astronomical Telescopes[M]. Oxford: Oxford University Press, 1998. 135--175.
  • 2R M Clare, R G Lane. Wave-front sensing from subdivision of the focal plane with a lenslet array [J]. J Opt Soc Am A, 2005, 22(1)~ 117--125.
  • 3R Ng, M Levoy, M Brfidif, et al.. Light field photography with a hand-held plenoptic camera [C]. Stanford University Computer Science Technical Report CSTR, 2005.
  • 4J M R Rodriguez, B F Castella, F P Nava, et al.. Wavefront and distance measurement using the CAFADIS camera [C]. Astronomical Telescopes and Instrumentation, Synergies Between Ground and Space, 2008, 7015(1-3): 70155Q.
  • 5J M R Rodriguez, B Femenia, I Montilla, et al.. The CAFADIS camera: A new tomographic wavefront sensor for adaptive optics [C]. 1st AO4ELT Conference, 2009. 05011.
  • 6张锐,杨金生,田雨,饶学军.焦面哈特曼传感器波前相位复原[J].光电工程,2013,40(2):32-39. 被引量:8
  • 7Y Lti, X Zhang, H Ma, et al.. Large viewing field wavefront sensing by using a lightfield system [C]. SPIE, 2013, 8905: 89052T.
  • 8A Talmi, E N Ribak. Wavefront reconstruction from its gradients [J]. J Opt Soc Am A, 2006, 23(2): 288--297.

二级参考文献19

  • 1JIANG Zhiling. Study on Characteristics and Applications of Hartmann Wavefront Sensor [D]. Wuhan: Wuhan Institute of Physics and Mathematics, Chinese Academy of Sciences, 2005.
  • 2Roddier F. Curvature sensing: a Diffraction Theory [M]. NOAO R&D Note, 1987: 87-90.
  • 3Roddier F. Curvature sensing and compensation: a new concept in adaptive optics [J]. AO(S0003-6935), 1988, 27(7): 1223-1225.
  • 4Mihnan M, Redding D, Needel L. Analysis of curvature sensing for large aperture adaptive optics systems [J]. J.Opt.Soc.Am.A(S1520-8532), 1996, 13(6): 1226-1238.
  • 5Ragazzoni R. Pupil plane wavefront sensing with an oscillating prism [J]. Mod.opt(S0950-0340), 1996, 43: 289-293.
  • 6Riccardi A, Bindi N, Ragazzoni R. Laboratory characterization ofa "Foucault-like" wavefront sensor for Adaptive Optics [J]. Proe. ofSPIE(S0277-786X), 1988, 3353: 941-951.
  • 7Costa J, Ragazzoni R, Ghedina A. Is there Need of any Modulation in the Pyramid Wavefront Sensor? [J]. Proc. of SPIE (S0277-786X), 2003, 4839: 288-298.
  • 8Costa J. Modulation effect of the atmosphere in a pyramid wave-front sensor [J]. AO(S0003-6935), 2005, 44: 60-66.
  • 9Malacara D. Optical shop testing [M]. John Wiley&Sons, Inc. New York, 1978: 105,.
  • 10Hardy J W, Lefebvre J E, Koliopoulos C L. Real-time atmospheric compensation [J]. JOSA A(S1084-7529), 1977, 67: 360-369.

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