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不同屈光不正组离轴高阶像差的特征及其随时间的变化

Profile of off-axis higher order aberrations and its variation with time among various refractive error groups.

作者信息

Philip Krupa, Sankaridurg Padmaja R, Ale Jit B, Naduvilath Thomas J, Mitchell Paul

机构信息

School of Optometry and Vision Science, University of New South Wales, Sydney, Australia.

Brien Holden Vision Institute, Sydney, Australia; The Vision Cooperative Research Centre, Sydney, Australia; School of Optometry and Vision Science, University of New South Wales, Sydney, Australia.

出版信息

Vision Res. 2018 Dec;153:111-123. doi: 10.1016/j.visres.2018.07.005. Epub 2018 Sep 29.

Abstract

Peripheral higher order aberrations (HOA) of 646 children at 30° temporal, nasal and inferior visual field were measured under cycloplegia (5 mm pupil diameter) using a commercially available Shack-Hartmann aberrometer in the Sydney Myopia Study [age, 12.7 ± 0.4 years (mean ± standard deviation)] and five years later in the Sydney Adolescent Vascular and Eye Study. At baseline, 176 eyes were emmetropic, 95 were myopic and 375 were hyperopic. Coma, 3rd order and RMS of coma increased with eccentricity for all eyes and no difference was observed for 4th order and RMS of C(4,0) among refractive error groups. More positive C(4,0) was observed for hyperopic eyes at periphery. At follow up, 26% had 'myopic change' and 70% had 'no change' in refractive error. At follow-up, horizontal coma became more negative at nasal field and more positive at temporal field for all eyes. More positive C(4,0) for hyperopic eyes at baseline may indicate variation in optical characteristics of peripheral cornea and crystalline lens. An increase in horizontal coma with time, irrespective of refractive error change, may be attributed to variation in the shape factor of peripheral cornea and crystalline lens and/or misalignment of optical surfaces/components relative to the visual axis (angle kappa) as the eye grows in axial length.

摘要

在悉尼近视研究中(年龄为12.7±0.4岁,均值±标准差),使用市售的Shack - Hartmann像差仪,在睫状肌麻痹状态下(瞳孔直径5毫米)测量了646名儿童在颞侧、鼻侧和下方30°视野的周边高阶像差(HOA),并在五年后的悉尼青少年血管与眼研究中再次进行测量。基线时,176只眼为正视眼,95只为近视眼,375只为远视眼。所有眼睛的彗差、三阶彗差以及彗差的均方根随偏心率增加,屈光不正组之间的四阶和C(4,0)的均方根未观察到差异。周边远视眼观察到更正向的C(4,0)。随访时,26%的人屈光不正有“近视变化”,70%的人“无变化”。随访时,所有眼睛的水平彗差在鼻侧视野变得更负,在颞侧视野变得更正。基线时远视眼更正向的C(4,0)可能表明周边角膜和晶状体光学特性的差异。随着时间推移水平彗差增加,无论屈光不正如何变化,可能归因于周边角膜和晶状体形状因子的变化和/或随着眼轴长度增加光学表面/组件相对于视轴(kappa角)的错位。

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