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高度近视人群正常眼中高阶像差对对比敏感度的影响。

Effects of higher-order aberrations on contrast sensitivity in normal eyes of a large myopic population.

作者信息

Zhao Peng-Fei, Li Shi-Ming, Lu Jing, Song Hong-Min, Zhang Jing, Zhou Yue-Hua, Wang Ning-Li

机构信息

Ophthalmic Center, Beijing Tongren Hospital, Capital Medical University, Beijing Ophthalmology and Visual Sciences Key Lab, Beijing 100730, China.

Department of Ophthalmology, Affiliated Hospital of Hebei Medical University, Baoding 100730, Hebei Province, China.

出版信息

Int J Ophthalmol. 2017 Sep 18;10(9):1407-1411. doi: 10.18240/ijo.2017.09.13. eCollection 2017.

Abstract

AIM

To study the relation between higher-order aberrations (HOAs) and contrast sensitivity (CS) in normal eyes among a population of laser keratomileusis (LASIK) candidates.

METHODS

In 6629 eyes of 3315 LASIK candidates, CS were measured under dark environment at the spatial frequencies of 1.5, 3, 6, 12 and 18 cycles per degree (c/d), respectively, using an Optec 6500 visual function tester. Meanwhile, ocular HOAs were measured for a 6.0 mm pupil with a Hartmann-Shack wavefront analyzer.

RESULTS

In the study, the subjects with an average spherical equivalent of -4.86±2.07 D were included. HOAs decreased from the third to the sixth order aberrations with predominant aberrations of third-order coma, trefoil and fourth-order spherical aberration. At low and moderate spatial frequencies, CS was negatively correlated with the third-order coma and trefoil aberrations, and decreased with increasing Z, but increased with increasing Z and Z. At high spatial frequencies, CS decreased with increasing Z and increased with increasing Z.

CONCLUSION

At a large pupil size of 6.0 mm, the third-order aberrations, but not the total aberrations, are the main factors affecting CS. Vertical coma is negatively correlated with CS.

摘要

目的

研究准分子激光原位角膜磨镶术(LASIK)候选人群中正常眼高阶像差(HOAs)与对比敏感度(CS)之间的关系。

方法

使用Optec 6500视觉功能测试仪,在暗环境下分别于空间频率为1.5、3、6、12和18周/度(c/d)时,对3315例LASIK候选者的6629只眼进行CS测量。同时,使用Hartmann-Shack波前分析仪测量6.0mm瞳孔直径下的眼HOAs。

结果

本研究纳入平均等效球镜度为-4.86±2.07D的受试者。HOAs从三阶像差到六阶像差逐渐降低,主要像差为三阶彗差、三叶草像差和四阶球差。在低、中等空间频率下,CS与三阶彗差和三叶草像差呈负相关,并随Z3增加而降低,但随Z4和Z6增加而升高。在高空间频率下,CS随Z6增加而降低,随Z4增加而升高。

结论

在6.0mm的大瞳孔直径下,影响CS的主要因素是三阶像差而非总像差。垂直彗差与CS呈负相关。

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