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近视眼的高阶像差

Higher-order aberrations in myopic eyes.

作者信息

Karimian Farid, Feizi Sepehr, Doozande Azade

机构信息

Labbafinejad Medical Center, Shahid Beheshti University of Medical Sciences, Tehran, Iran.

出版信息

J Ophthalmic Vis Res. 2010 Jan;5(1):3-9.

Abstract

PURPOSE

To evaluate the correlation between refractive error and higher-order aberrations (HOAs) in patients with myopic astigmatism.

METHODS

HOAs were measured using the Zywave II aberrometer over a 6 mm pupil. Correlations between HOAs and myopia, astigmatism, and age were analyzed.

RESULTS

One hundred and twenty-six eyes of 63 subjects with mean age of 26.4±5.9 years were studied. Mean spherical equivalent refractive error and refractive astigmatism were -4.94±1.63 D and 0.96±1.06 D, respectively. The most common higher-order aberration was primary horizontal trefoil with mean value of 0.069±0.152 μm followed by spherical aberration (-0.064±0.130 μm) and primary vertical coma (-0.038±0.148 μm). As the order of aberration increased from third to fifth, its contribution to total HOA decreased: 53.9% for third order, 31.9% for fourth order, and 14.2% for fifth order aberrations. Significant correlations were observed between spherical equivalent refractive error and primary horizontal coma (R=0.231, P=0.022), and root mean square (RMS) of spherical aberration (R=0.213, P=0.031); between astigmatism and RMS of total HOA (R=0.251, P=0.032), RMS of fourth order aberration (R=0.35, P<0.001), and primary horizontal coma (R=0.314, P=0.004). Spherical aberration (R=0.214, P=0.034) and secondary vertical coma (R=0.203, P=0.031) significantly increased with age.

CONCLUSION

Primary horizontal trefoil, spherical aberration and primary vertical coma are the predominant higher-order aberrations in eyes with myopic astigmatism.

摘要

目的

评估近视散光患者屈光不正与高阶像差(HOAs)之间的相关性。

方法

使用Zywave II像差仪在6mm瞳孔直径下测量高阶像差。分析高阶像差与近视、散光和年龄之间的相关性。

结果

研究了63名受试者的126只眼睛,平均年龄为26.4±5.9岁。平均球镜等效屈光不正和屈光性散光分别为-4.94±1.63D和0.96±1.06D。最常见的高阶像差是初级水平三叶草像差,平均值为0.069±0.152μm,其次是球差(-0.064±0.130μm)和初级垂直彗差(-0.038±0.148μm)。随着像差阶数从三阶增加到五阶,其对总高阶像差的贡献降低:三阶像差为53.9%,四阶像差为31.9%,五阶像差为14.2%。在球镜等效屈光不正与初级水平彗差(R=0.231,P=0.022)以及球差的均方根(RMS)(R=0.213,P=0.031)之间观察到显著相关性;在散光与总高阶像差的RMS(R=0.251,P=0.032)、四阶像差的RMS(R=0.35,P<0.001)和初级水平彗差(R=0.314,P=0.004)之间观察到显著相关性。球差(R=0.214,P=0.034)和二级垂直彗差(R=0.203,P=0.031)随年龄显著增加。

结论

初级水平三叶草像差、球差和初级垂直彗差是近视散光眼中主要的高阶像差。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/9716/3380664/7528602dd599/jovr-5-1-167-700-2-pbf1.jpg

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