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角膜地形图和像差的昼夜变化。

The diurnal variation of corneal topography and aberrations.

作者信息

Read Scott A, Collins Michael J, Carney Leo G

机构信息

School of Optometry, Queensland University of Technology, Room B547, O Block, Victoria Park Road, Kelvin Grove, 4059 Brisbane, Queensland, Australia.

出版信息

Cornea. 2005 Aug;24(6):678-87. doi: 10.1097/01.ico.0000154385.43732.6e.

DOI:10.1097/01.ico.0000154385.43732.6e
PMID:16015086
Abstract

PURPOSE

To investigate if diurnal variation occurs in corneal topography.

METHODS

Seventeen young subjects had corneal topography measured 3 times a day (around 9 AM, 1 PM, and 5 PM) on 3 days of the week (Monday, Tuesday, and Friday). Corneal tangential and refractive power were analyzed. To investigate diurnal variation in corneal aberrations, the corneal height data were converted into corneal wavefront error and expressed as Zernike wavefront coefficients.

RESULTS

A significant diurnal change in corneal tangential power maps was found in 15 of the 17 subjects. This change typically consisted of a horizontal band of distortion in the superior and, to a lesser extent, inferior cornea, increasing throughout the day. Corneal refractive power showed small but significant diurnal changes occurring in the best fit sphere. Corneal wavefront error analysis revealed significant diurnal changes occurring in astigmatism 90/180 degrees and astigmatism 45/135 degrees. Two higher-order aberrations, primary vertical coma and trefoil along 30 degrees, also showed significant diurnal change. The combination of these 2 aberrations represents a "wavelike" distortion increasing throughout the day and returning to baseline the next morning.

CONCLUSION

We have shown that significant diurnal change occurs in certain corneal aberrations. The changes appear to be related to forces from the eyelids on the anterior cornea. These findings may have important implications for customized refractive corrections and refractive error development.

摘要

目的

研究角膜地形图是否存在日变化。

方法

17名年轻受试者在一周中的3天(周一、周二和周五)每天测量3次角膜地形图(上午9点左右、下午1点和下午5点)。分析角膜切线和屈光力。为了研究角膜像差的日变化,将角膜高度数据转换为角膜波前误差并表示为泽尼克波前系数。

结果

17名受试者中有15名发现角膜切线力图存在显著的日变化。这种变化通常包括上方角膜以及程度较轻的下方角膜的水平扭曲带,全天逐渐增加。角膜屈光力在最佳拟合球镜中显示出微小但显著的日变化。角膜波前误差分析显示,90/180度散光和45/135度散光存在显著的日变化。两种高阶像差,即原发性垂直彗差和沿30度的三叶草像差,也显示出显著的日变化。这两种像差的组合代表了一种“波浪状”扭曲,全天逐渐增加,第二天早晨恢复到基线水平。

结论

我们已经表明,某些角膜像差存在显著的日变化。这些变化似乎与眼睑对角膜前部的作用力有关。这些发现可能对定制屈光矫正和屈光不正的发展具有重要意义。

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