Carvalho L Alberto V, Castro J C, Carvalho L Antonio V
Grupo de Optica, Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, SP, Brasil.
Braz J Med Biol Res. 2002 Nov;35(11):1395-406. doi: 10.1590/s0100-879x2002001100019.
In the present paper we discuss the development of "wave-front", an instrument for determining the lower and higher optical aberrations of the human eye. We also discuss the advantages that such instrumentation and techniques might bring to the ophthalmology professional of the 21st century. By shining a small light spot on the retina of subjects and observing the light that is reflected back from within the eye, we are able to quantitatively determine the amount of lower order aberrations (astigmatism, myopia, hyperopia) and higher order aberrations (coma, spherical aberration, etc.). We have measured artificial eyes with calibrated ametropia ranging from +5 to -5 D, with and without 2 D astigmatism with axis at 45 degrees and 90 degrees. We used a device known as the Hartmann-Shack (HS) sensor, originally developed for measuring the optical aberrations of optical instruments and general refracting surfaces in astronomical telescopes. The HS sensor sends information to a computer software for decomposition of wave-front aberrations into a set of Zernike polynomials. These polynomials have special mathematical properties and are more suitable in this case than the traditional Seidel polynomials. We have demonstrated that this technique is more precise than conventional autorefraction, with a root mean square error (RMSE) of less than 0.1 micro m for a 4-mm diameter pupil. In terms of dioptric power this represents an RMSE error of less than 0.04 D and 5 degrees for the axis. This precision is sufficient for customized corneal ablations, among other applications.
在本文中,我们讨论了“波前”仪器的研发,该仪器用于测定人眼的低阶和高阶光学像差。我们还讨论了此类仪器和技术可能给21世纪眼科专业人员带来的优势。通过将一个小光斑投射到受试者的视网膜上,并观察从眼内反射回来的光,我们能够定量测定低阶像差(散光、近视、远视)和高阶像差(彗差、球差等)的量。我们测量了人工眼,其校准屈光不正范围从+5到-5 D,有和没有2 D散光,轴位分别在45度和90度。我们使用了一种称为哈特曼-夏克(HS)传感器的设备,该设备最初是为测量光学仪器和天文望远镜中一般折射面的光学像差而开发的。HS传感器将信息发送到计算机软件,以便将波前像差分解为一组泽尼克多项式。这些多项式具有特殊的数学性质,在这种情况下比传统的赛德尔多项式更适用。我们已经证明,这种技术比传统的自动验光更精确,对于直径4毫米的瞳孔,均方根误差(RMSE)小于0.1微米。就屈光力而言,这代表轴位的RMSE误差小于0.04 D和5度。这种精度足以用于定制角膜消融等应用。