[1] Platt B C, Shack R V. History and principles of Shack-Hartmann wavefront sensing[J]. Journal of Refractive Surgery, 2001,17(5):573-577.
[2] Cao W, Gorceix N, Coulter R, et al. Scientific instrumentation for the 1.6 m new solar telescope in Big Bear[J]. Astronomische Nachrichten, 2010,331(6):636-639.
[3] Berkefeld T, Schmidt D, Soltau D, et al. The GREGOR adaptive optics system[J]. Astronomische Nachrichten, 2012,333(9):863-871.
[4] Upton R. Optical control of the advanced technology solar telescope[J]. Applied Optics, 2006,45(23):5881-96.
[5] 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. Rao C H, Zhang X J, Jiang W H. Simulation study on correlating Hartmann-Shack Wavefront sensor for solar granulation[J]. Acta Optica Sinica, 2002,22(3):285-289.
[6] 饶长辉, 姜文汉, 凌宁, 等. 太阳表面米粒结构观测对比度分析[J]. 天文学报, 2001,42(2):134-139. Rao C H, Jiang W H, Ling N, et al. Analysis of the observed R.M.S. contrast in solar granulation[J]. Acta Astronomica Sinica, 2001,42(2):134-139.
[7] Noll R J. Zernike polynomials and atmospheric turbulence[J]. Journal of the Optical Society of America, 1976,66(3):207-211.
[8] Lane R G, Tallon M. Wave-front reconstruction using a Shack-Hartmann sensor[J]. Applied Optics, 1992,31(32):6902-6908.
[9] Qi B, Chen H, Dong N. Wavefront fitting of interferogram with Zernike polynomials[J]. Optical Engineering, 2002,41(7):1565-1569.
[10] 杨晓飞, 张晓辉, 韩昌元. Zemax软件在离轴三反射镜系统计算机辅助装调中的应用[J]. 光学精密工程, 2004,12(3):270-274. Yang X F, Zhang X H, Han C Y. Application of Zemax software in alignment of three-mirror off-axis aspherical optical system[J]. Optics and Precision Engineering, 2004,12(3):270-274.
[11] 巩盾, 田铁印, 王红. 利用Zernike系数对离轴三反射系统进行计算机辅助装调[J]. 光学精密工程, 2010,18(8):1754-1759. Gong D, Tian T Y, Wang H. Computer-aided alignment of off-axis three-mirror system by using Zernike coefficients[J]. Optics and Precision Engineering, 2010,18(8):1754-1759. |