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屈光手术科室中轴性、角膜性及复合性屈光不正的分布情况。

Distribution of axial, corneal, and combined ametropia in a refractive surgery unit.

作者信息

Barcsay Gy, Nagy Z Zs, Németh J

机构信息

First Dept. of Ophthalmology, Semmelweis University, Budapest, Hungary.

出版信息

Eur J Ophthalmol. 2003 Nov-Dec;13(9-10):739-44. doi: 10.1177/1120672103013009-1001.

DOI:10.1177/1120672103013009-1001
PMID:14700092
Abstract

PURPOSE

To group eyes in our refractive surgery unit on the basis of the origin of their ametropia and to assess the percentage of eyes in the different groups.

METHODS

Refractive parameters and the axial eye length (AL) of 131 eyes of 131 persons with different refraction were measured. The eyes were initially classified into five groups on the basis of the grade of their ametropia: hypermetropic (> +0.5 D, n = 35), emmetropic (between +/- 0.5 D, n = 24), low myopic (between -0.75 and -4.0 D, n = 24), medium myopic (between -4.25 and -8.0 D, n = 24), and high myopic (over -8.0 D, n = 24). Then a classification scheme was made to group the origin of the ametropia on the basis of AL and corneal refractive power.

RESULTS

In the hypermetropic group pure corneal origin was found in 8.6%, pure axial origin in 62.8%, and combined origin in 28.6% of the eyes. In the low myopic group these values were 20.9%, 29.2%, and 45.8%, respectively. In the medium and high myopic groups no pure corneal myopia was found, while axial myopia was found in 16.7% and combined myopia in 83.3% of the eyes.

CONCLUSIONS

With the help of the classification scheme, an objective decision could be made as to whether the ametropia of a particular eye had axial, corneal, or mixed origin. The most interesting result was that in 83% of medium and high myopic eyes not only AL but also corneal refractive power contributed to the refractive error instead of the eyes being purely axially myopic.

摘要

目的

根据屈光不正的起源对我们屈光手术科室的眼睛进行分组,并评估不同组中眼睛的百分比。

方法

测量了131例不同屈光状态患者的131只眼睛的屈光参数和眼轴长度(AL)。这些眼睛最初根据屈光不正的程度分为五组:远视(>+0.5D,n = 35)、正视(±0.5D之间,n = 24)、低度近视(-0.75至-4.0D之间,n = 24)、中度近视(-4.25至-8.0D之间,n = 24)和高度近视(>-8.0D,n = 24)。然后制定了一种分类方案,根据眼轴长度和角膜屈光力对屈光不正的起源进行分组。

结果

在远视组中,8.6%的眼睛为单纯角膜起源,62.8%为单纯眼轴起源,28.6%为混合起源。在低度近视组中,这些值分别为20.9%、29.2%和45.8%。在中度和高度近视组中,未发现单纯角膜性近视,而16.7%的眼睛为眼轴性近视,83.3%的眼睛为混合性近视。

结论

借助该分类方案,可以客观地确定某只眼睛的屈光不正的起源是眼轴性、角膜性还是混合性。最有趣的结果是,在83%的中度和高度近视眼中,不仅眼轴长度,而且角膜屈光力也对屈光不正有影响,而不是眼睛纯粹为眼轴性近视。

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