期刊文献+

基于高斯光斑的相关HS波前斜率处理器 被引量:1

Implementation of the Correlating Shack-Hartmann Processor for the Point Source Based on Gaussian Reference Spot
下载PDF
导出
摘要 大规模自适应光学系统要求哈特曼-夏克波前传感器的子孔径数目巨大,这势必会增加波前斜率提取电路实现的难度。为了在大规模自适应光学系统中进行波前斜率提取,提出了一种相关算法的实现结构,以高斯光斑作为参考模板,通过两次级联滤波完成子孔径光斑之间的相关运算,并得到局部波前斜率。与多通道并行处理的实现结构相比,本文所提出的结构实现的硬件成本不会随着子孔径规模的增大而显著增加,特别适用于大规模自适应光学系统的波前斜率提取。实验结果表明:对于8×8方形排布的哈特曼-夏克波前传感器图像,本文的结构用FPGA内实现,在27MHz的工作频率下,完成一帧所有子孔径斜率计算的延迟为1.2μs,均方根误差小于0.02个像素,最大误差不超过0.04个像素。而资源消耗仅仅为925个Slices。本结构能够满足大规模自适应光学系统中波前斜率探测高速实时和高精度要求。 Adaptive optics systems with larger size require more subapertures in the Shack-Hartmann wavefront sensor, which makes it harder to compute the wavefront gradient in real time. In order to measure local gradients in large-size adaptive optics systems, an architecture based on cross correlation is proposed. Using the Gaussian spot as the reference template, the correlation between subaperture spots is calculated by means of two cascading filters, and then the local wavefront gradient of each subaperture is determined. Compared with the existing parallel processing approach in correlating-Hartmann sensor, the cost of our architecture will not increase greatly as subapertures multiplies, which makes it more suitable for adaptive optics systems of extreme size to retrieve gradients. Experimental results indicate that when implemented in Field Programmable Gate Array (FPGA) at 27 MHz, our design can obtain gradients of all subapertures in 8x8 Shack-Hartmann with latency no more than 1.2 gs, while the RMS error is less than 0.02 pixels, and the maximum error does not exceed 0.04 pixels. It can satisfy the requirements of low cost, real time and high accuracy for gradient detection in adaptive optics systems with large-size aperture.
出处 《光电工程》 CAS CSCD 北大核心 2010年第6期42-48,共7页 Opto-Electronic Engineering
基金 863高技术计划资助项目
关键词 自适应光学 波前斜率探测 相关运算 图像滤波 FPGA adaptive optics wavefront gradient detection correlation image filtering FPGA
  • 相关文献

参考文献10

  • 1Rimmele T. Recent advances in solar adaptive optics [J]. Proc. of SPIE(S0277-786X), 2004, 5490: 34-46.
  • 2Rimmele T, Richards K. First Results from the NSO/NJIT Solar Adaptive Optics System [J]. Proc. of SPIE(S0277-786X), 2004, 5171: 179-186.
  • 3Poyneer L A, LaFortune K. Correlation wavefront sensing for Shack-Hartmann-based Adaptive Optics with a point source [R]. Lawrence Livermore National Lab, 2003.
  • 4Poyneer L A. Scene-based Shack-Hartmann wave-front sensing: analysis and simulation [J]. Applied Optics(S0003-6935), 2003, 42(29): 5807-5815.
  • 5Bake K L. Iteratively weighted centroiding for Shack- Hartmann wave-front sensors [J]. Optics Express(S 1094-4087), 2007, 15(8): 5147-5159.
  • 6饶长辉,张学军,姜文汉.太阳米粒结构相关哈特曼-夏克波前传感模拟研究[J].光学学报,2002,22(3):285-289. 被引量:9
  • 7ZHOU Wei-chao, JIANG Wen-han. Real-time area correlation tracker implementation based on absolute difference algorithm [J]. Opt. Eng(S0091-3286), 2003, 42(9): 2755-2760.
  • 8彭晓峰,李梅,饶长辉.基于绝对差分算法的相关HS波前处理机设计[J].光电工程,2008,35(12):18-22. 被引量:7
  • 9张广军.机器视觉[M].北京:科学出版社,2007.
  • 10叶敏,周文晖,顾伟康.基于FPGA的实时图像滤波及边缘检测方法[J].传感技术学报,2007,20(3):623-627. 被引量:25

二级参考文献19

  • 1Rimmele T, Richards K, Hegwer S, et al. First Results from the NSO/NJIT Solar Adaptive Optics System [J]. SHE, 2004, 5171: 179-186.
  • 2Berkefeld Thomas, Soltau Dirk, vonder Luhe Oskar F H.. Seeond-generation adaptive optics for the 1.5 m solar telescope GREGOR, Tenerife [J]. SPIE, 2004, 5490: 260-267.
  • 3Rimmele Thomas R. Recent advances in solar adaptive optics [J]. SPIE, 2004, 5490: 34-46.
  • 4Goodsell S J, Fedrigo E, DipperNA, etal. FPAG developments for the SPARTA project [J]. SPIE, 2005, 5903: 148-159.
  • 5Goodsell S J, Geng D, Fedrigo E, et al. FPAG developments for the SPARTA project: Part 2 [J]. SPIE, 2006, 6272: 62741.
  • 6Rodriguez Ramos L F, Viera Teodora, Gigante Jose V, et al. FPGA adaptive optics system test bench [J]. SPIE, 2005, 5903: 120-128.
  • 7Ballesteros E, Collades M, Bonet J A et al.. Two-dimensional, high spatial resolution, solar spectroscopy using a correlation tracker, Ⅰ: Correlation tracker description. Astron. Astrophys. Suppl. Ser, 1996,115:353-365
  • 8Molodij G, Rayrole J, Madec P Y et al.. Performance analysis for T. H. E. M. I. S image stabilizer optical system. I. Asron. Astrophys. Suppl. Ser. , 1996, 118:169-179
  • 9Molodij G, Rayrole J. Performance analysis for T. H. E. M. I. S image stabilizer optical system, Ⅱ. Anisoplanatism limitations.Astron.Astron. Astrophys. Suppl. Ser., 1997, 128:229-244
  • 10von der Luhe O, Widener A L, Rimmele T et al.. Solar feature correlation tracker for grounded-based telescopes. Astron. Astrophys. Ser., 1989, 224:351-360

共引文献39

同被引文献19

引证文献1

二级引证文献6

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