Acta Optica Sinica, Volume. 27, Issue 8, 1414(2007)
Influence of Scene Structure and Noise on Precision of Correlating Hartmann-Shack Wavefront Sensing
[1] [1] T. R. Rimmele. Solar adaptive optics[C]. Proc. SPIE, 2000, 4007: 218~231
[2] [2] Th. R. Rimmele, O. von der Lühe, P. H. Wiborg et al.. Solar feature correlation tracker[C]. Proc. SPIE, 1991, 1542: 186~193
[4] [4] Aimin Jiang, Seng Wang, Shengzhen Jing. Simulation system for correlation tracker[C]. Proc. SPIE, 2002, 4926: 221~226
[6] [6] Lisa A. Poyneer, Kai La Fortune, Carri Chan. Scene-based wave-front sensing for remote imaging[C]. Proc. SPIE, 2003, 5162: 91~102
[7] [7] Lisa A. Poyneer, David W. Palmer, Kai N. La Fortune et al.. Experimental results for correlation-based wavefront sensing[C]. Proc. SPIE, 2005, 5894: 1~14
[8] [8] Lisa A. Poyneer. Scene-based Shack-Hartmann wave-front sensing: analysis and simulation[J]. Appl. Opt., 2003, 42(29): 5807~5815
[9] [9] Xinqi Hu, Dazun Zhao, Xin Yu et al.. Signal processing of the Hartmann-Shack wavefront sensor operated with extended targets[C]. Proc. SPIE, 2004, 5639: 78~82
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[in Chinese], [in Chinese], [in Chinese]. Influence of Scene Structure and Noise on Precision of Correlating Hartmann-Shack Wavefront Sensing[J]. Acta Optica Sinica, 2007, 27(8): 1414