Carvalho Luis Alberto, Chamon Wallace, Schor Paulo, Castro Jarbas Caiado de
Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, SP, Brazil.
Arq Bras Oftalmol. 2006 Mar-Apr;69(2):239-47. doi: 10.1590/s0004-27492006000200019. Epub 2006 May 8.
There is a general acceptance among the scientific community of Cartesian symmetry wavefront sensors (such as the Hartmann-Shack (HS) sensor) as a standard in the field of optics and vision science. In this study it is shown that sensors of different symmetries and/or configurations should also be tested and analyzed in order to quantify and compare their effectiveness when applied to visual optics. Three types of wave-aberration sensors were developed and tested here. Each sensor has a very different configuration and/or symmetry (dodecagonal (DOD), cylindrical (CYL) and conventional Hartmann-Shack (HS)).
All sensors were designed and developed in the Physics Department of the Universidade de São Paulo--São Carlos. Each sensor was mounted on a laboratory optical bench used in a previous study. A commercial mechanical eye was used as control. This mechanical eye has a rotating mechanism that allows the retinal plane to be positioned at different axial distances. Ten different defocus aberrations were generated: 5 cases of myopia from -1D to -5D and 5 cases of hyperopia, from +1D to +5D, in steps of 1D following the scale printed on the mechanical eye. For each wavefront sensor a specific image-processing and fitting algorithm was implemented. For all three cases, the wavefront information was fit using the first 36 VSIA standard Zernike polynomials. Results for the mechanical eye were also compared to the absolute Zernike surface generated from coefficients associated with the theoretical sphere-cylinder aberration value.
Precision was analyzed using two different methods: first, a theoretical approach was used by generating synthetic Zernike coefficients from the known sphere-cylinder aberrations, simply by applying sphere-cylinder equations in the backward direction. Then comparisons were made of these coefficients with the ones obtained in practice. Results for DOD, HS and CYL sensors were, respectively, as follows: mean of root mean square (RMSE) for all aberrations, when theoretical Zernike coefficients were used as control, was 0.22, 0.66 and 0.26 microns; RMSE of sphere-cylinder values when compared to autorefractor measurements was 0.18D, 0.22D and 0.35D for sphere, 0.14D, 0.24D and 0.17D for cylinder, 34.36 degrees, 35.16 degrees and 26.36 degrees for axis; RMSE of sphere-cylinder values when theoretical values were used as control was 0.11D, 0.29D and 0.46D for sphere, 0.15D, 0.28D and 0.17D for cylinder, 19.71 degrees, 25.56 degrees and 18.56 degrees for axis.
The main conclusion is that the symmetry of an optical sensor is not an important consideration when measuring typical eye aberrations such as defocus (myopic and hyperopic), but there are differences. In this sense, the polar symmetry sensors render results that are equivalent to the traditional Cartesian Hartmann-Shack sensor, but furnish an easier method for determining the optical center.
科学界普遍认可笛卡尔对称波前传感器(如哈特曼-夏克(HS)传感器)为光学和视觉科学领域的标准。本研究表明,不同对称性和/或配置的传感器也应进行测试和分析,以便在应用于视觉光学时量化和比较它们的有效性。这里开发并测试了三种类型的波像差传感器。每个传感器都有非常不同的配置和/或对称性(十二边形(DOD)、圆柱形(CYL)和传统的哈特曼-夏克(HS))。
所有传感器均在圣保罗大学圣卡洛斯分校物理系设计和开发。每个传感器都安装在先前研究中使用的实验室光学平台上。使用商用机械眼作为对照。该机械眼具有旋转机构,可使视网膜平面位于不同的轴向距离处。产生了十种不同的离焦像差:5例近视,从-1D到-5D,以及5例远视,从+1D到+5D,按照机械眼上印刷的刻度以1D为步长。针对每个波前传感器实施了特定的图像处理和拟合算法。对于所有三种情况,使用前36个VSIA标准泽尼克多项式拟合波前信息。还将机械眼的结果与根据与理论球柱面像差值相关的系数生成的绝对泽尼克曲面进行了比较。
使用两种不同方法分析精度:首先,采用理论方法,通过简单地向后应用球柱面方程,从已知的球柱面像差生成合成泽尼克系数。然后将这些系数与实际获得的系数进行比较。DOD、HS和CYL传感器的结果分别如下:当使用理论泽尼克系数作为对照时,所有像差的均方根误差(RMSE)平均值分别为0.22、0.66和0.26微米;与自动验光仪测量值相比,球镜的球柱面值RMSE分别为0.18D、0.22D和0.35D,柱镜为0.14D、0.24D和0.17D,轴位为34.36度、35.16度和26.36度;当使用理论值作为对照时,球镜的球柱面值RMSE分别为0.11D、0.29D和0.46D,柱镜为0.15D、0.28D和0.17D,轴位为19.71度、25.56度和18.56度。
主要结论是,在测量典型的眼像差如离焦(近视和远视)时,光学传感器的对称性不是一个重要考虑因素,但存在差异。从这个意义上说,极对称传感器给出的结果与传统的笛卡尔哈特曼-夏克传感器相当,但提供了一种更简便的确定光心的方法。