期刊文献+

四棱锥波前传感技术数值仿真和重构研究 被引量:1

Numerical simulation and reconstruction of pyramid wave-front sensor
原文传递
导出
摘要 介绍了四棱锥传感技术的基本原理和数学模型。当以调制模式工作时,可计算复原矩阵或梯度矩阵。分析了调制半径在不同像差条件下对复原速度和精度的影响,对无调制模式采用复原矩阵进行了仿真,并与调制模式进行了对比。实验结果表明:无调制状态下,经过校正,残差RMS可减至0.05,调制状态下,梯度矩阵重构效果较好,残差RMS可减至0.02;对大像差的输入信号,调制模式的精度和速度都优于无调制模式。结果表明,四棱锥波前传感技术具有高速度、高精度和灵活的工作模式,是一种先进的波前传感技术。 Two reconstruction matrixes based on Zernike Polynomials and their gradient are compared respectively in reconstruction of modulation pyramid wave-front sensor (PWFS), the effect of modulation radius on the reconstruction speed and precision is analyzed, and non-modulation PWFS is simulated as a comparison. The results show that the residual RMS of non-modulation PWFS is 0. 05, and the residual RMS of modulation PWFS with a gradient matrix is 0. 02. For big aberration, modulation PWFS works faster and more precise than non-modulation PWFS. The numerical simulation proves that PWFS as a new wave-front sensor is both precise and flexible.
出处 《光学技术》 CAS CSCD 北大核心 2015年第2期101-105,共5页 Optical Technique
关键词 自适应光学 波前重构 四棱锥传感技术 调制模式 adapting optics wave-front reconstruction pyramid wave-front sensor modulation
  • 相关文献

参考文献16

  • 1Ragazzoni R. Pupil plane wavefront sensing with an oscillating prism[J]. Journal of Modern Optics,1996, 43(2): 289 -293.
  • 2Ragazzoni R, Farinato J. Sensitivity of a pyramidic wave front sensor in closed loop adaptive optics[-J]. Astronomy and Astro- physics, 1999,350 : 23-26.
  • 3Ragazzoni R, Ghedina A, Baruffolo A, et al. Testing the pyra- mid wavefront sensor on the sky[J]. Proceedings of SHE, 2000, 4007.
  • 4Ragazzoni R, Diolaiti E. A pyramid wavefront sensor with no dynamic modulation[J]. Optics Communications, 2002, 208: 51 -60.
  • 5Richard M C, Richard G L. Comparison of wavefront sensing with the Shack-Hartmann and pyramid sensors[J]. Astronomy and Astrophysics, 1999,350 : 23-26.
  • 6Peter D, Baumeister H, Bizenberger P, et al. Pyramir: con- struction and implementation of the world's first infrared pyra- mid sensor[-J]. Proceedings of SPIE,2006, 6276.
  • 7Esposito S, Riccardi A. Pyramid wavefront sensor behavior in partial adaptive optic systems[J]. Astronomy and Astrophys- ics, 2001,369 : 9-12.
  • 8Tozzi A, Stefanini P, Pinna E, et al. The double pyramid wave- front sensor for LBT[J]. Proceedings of SHE,2008, 7015.
  • 9Wang Jianxin, Bai Fuzhong, Ning Yu, et al. Comparison be- tween non-modulation four-side and two-side pyramid wave{ront sensor[-J]. Optics Express, 2010, 18(26).
  • 10王建新,白福忠,宁禹,黄林海,姜文汉.无调制两面锥波前传感器的衍射理论分析和数值仿真[J].物理学报,2011,60(2):840-846. 被引量:8

二级参考文献13

  • 1李超宏,鲜浩,姜文汉,饶长辉.用于白天自适应光学的波前探测方法分析[J].物理学报,2007,56(7):4289-4296. 被引量:14
  • 2张逸新 迟泽英.光波在大气中的传输与成像[M].北京:国防工业出版社,1996..
  • 3沈忙作.斑点干涉术在天文学中的应用.光学工程,1982,(4):49-62.
  • 4Benjamin L.McGlamery.Computer simulation studies of compensation of turbulence degraded images[J].SPIE,1976,74:225-233.
  • 5Robert J.Noll.Zernike polynomials and atmospheric turbulence[J].J.Opt.Soc.Am,1976,66(3):207-211.
  • 6Nicolas Roddier.Atmospheric wavefront simulation using Zernike polynomials[J].Opt.Eng,1990,29(10):1174-1180.
  • 7E.M.Johansson,D.T.Gavel.Simulation of stellar speckle imaging[J].SPIE,1994,2200:372-383.
  • 8S.E.Troxel,B.M.Welsh,M.C.Roggemann.Off-axis optical transfer function calculations in an adaptive-optics system by means of a diffraction calculation for weak index fluctuations[J].J.Opt.Soc.Am,1994,11:2100-2111.
  • 9M.C.Roggemann,B.M.Welsh.Imaging through turbulence[M].New York:CRC Press,1995.
  • 10魏宏刚 沈忙作 廖胜.扩展目标克服大气湍流成像的实验室模拟.光电工程,2005,32(2):40-44.

共引文献36

同被引文献8

引证文献1

二级引证文献1

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