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青少年近视眼角膜高阶像差与屈光度关系的相关性

珺玥,王利华,马鲁新   

  1. 山东大学附属省立医院眼科, 济南 250021
  • 收稿日期:1900-01-01 修回日期:1900-01-01 出版日期:2008-07-16 发布日期:2008-07-16
  • 通讯作者: 曲珺玥

Changes of corneal higher-order wavefront aberrations as a function of the degree of myopia in adolescents

QU Jun-yue, WANG Li-hua, MA Lu-xin   

  1. Department of Opthalmology, Provincial Hospital Affiliated to Shandong University, Jinan 250021,China

  • Received:1900-01-01 Revised:1900-01-01 Online:2008-07-16 Published:2008-07-16
  • Contact: QU Jun-yue

摘要:

目的〓〖HTK〗了解青少年近视患者角膜高阶像差的分布规律,探讨近视程度对角膜高阶像差的影响。〖HTW〗方法〓〖HTK〗应用Ray Tracing原理设计的iTrace视功能分析仪检测104例104只青少年近视眼,等效球镜为[(-3.98±2.50)D]的角膜像差。在6mm瞳孔直径下测量3~6阶Zernike系数,计算各阶均方根(RMS)值、3~6阶总RMS值、球差(Z04,Z06)及彗差(Z-13,Z13,Z-15,Z15)RMS值,并分别与屈光度进行相关分析。〖HTW〗结果〓〖HTK〗受试者球镜平均为(-3.72±2.36)D,柱镜平均为(-0.77±0.62)D,角膜总高阶像差(3~6阶)的RMS值平均为(0.413±0.134)μm,3阶至6阶的各项Zernike系数大致呈递减趋势(4阶球差Z04除外),所有角膜的Z04(4阶球差)值均为正值,平均(0.272±0.086)μm。近视屈光度大小与角膜总高阶像差、各阶像差的RMS值无相关性,但水平彗差(Z13)与等效球镜呈负相关(P<0.01)。彗差作为主导像差的频率在高度近视组略增加,而球差是角膜像差中最主要的像差(约占80%),且不随屈光度的变化而变化。〖HTW〗结论〓〖HTK〗在青少年近视中,角膜高阶像差的个体差异较大,仅个别Zernike系数与近视程度有相关性,球差是角膜像差中最主要的像差。

关键词: 波前像差, 青少年, 角膜, 近视

Abstract:

Objective〓〖WTBZ〗To investigate the distribution of corneal high-order aberrations (HOAs, 3rd to 6th orders) myopic eyes of adolescent, and study the changes as a function of the degree of myopia. 〖WTHZ〗Methods〓〖WTBZ〗Using the iTrace Visual Function Analyzer, root mean square(RMS)of total corneal HOAs, 3rd-,4th-,5th-,6th-order aberrations, coma and SA were determined from the central 6.0mm zone of 104 eyes of 104 subjects mean 19.9±1.34 years old, ranging from 16 to 24 years; mean manifest spherical equivalent was (-3.98±2.50)D. Correlation between corneal HOAs and refractive power was analyzed. 〖WTHZ〗Results〓〖WTBZ〗The mean refractive error was sphere (-3.72±2.36)D and cylinder (-0.77±0.62)D, and the mean RMS of corneal total high order(3rd to 6th) was (0.413±0.134)μm. Values of Zernike coefficients progressively decreased from the 3rd-order to the 6th-order (except Z04). The mean coefficient of the 4th-order SAs(Z04) was (0.272±0.086)μm and was positive in all corneas. No correlation was found between total corneal high order RMS and myopia. However, horizonal primary coma(Z13) statistically correlate with spherical equivalent (SE) (P<0.01). Coma was more frequent in high myopia as a dominant aberration, and SA occurred equally around 80%. 〖WTHZ〗Conclusions〓〖WTBZ〗Corneal wavefront aberrations greatly vary among adolescents, while horizontal primary coma(Z13) slightly decreases with an increase of SE. All corneas have positive 4th-order SAs, and the values are negatively correlated with SE in median myopia. Coma is more frequent in high myopia, and SA is the most influential one in cornea aberrations.

Key words: Myopia, Cornea, Wavefront aberration, Adolescence

中图分类号: 

  • R778.1
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