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[术中屈光状态下光学计算眼轴长度及预测屈光度的特征]

[The characteristics of the optically calculated axial length and the predicted refraction when using the intraoperative refraction].

作者信息

Iwami S, Senoh K

机构信息

Department of Ophthalmology, Iwate Prefectural Kitakami Hospital, 3-15-36 Kunenbashi, Kitakami 024-0063, Japan.

出版信息

Nippon Ganka Gakkai Zasshi. 2001 Mar;105(3):155-60.

PMID:11280873
Abstract

PURPOSE

To understand the effect of the error in corneal refractive power on the optically calculated axial length (AXO) and the postoperative predicted refraction (Q'gl) calculated from the aphakic refraction (Qaph).

METHOD

We used the Gullstrand's schematic eye, in which the intraocular lens (+20 D) was inserted at a depth of 5 mm, and calculated Qaph and postoperative refraction (Qgl) geometrically when the corneal radius of the anterior surface (Rfc) changed from 7 mm to 9 mm. AXO was calculated using the calculation formula from a previous report, and then Q'gl was calculated from the AXO and the true axial length (AXT) using the theoretical calculation formula (regarding the fictitious corneal refractive index as 1.3315).

RESULTS

When the measured corneal radius of the anterior surface (K) was equal to Rfc, the error of the AXO was largest (AXO/AXT = 101.512) when K was 9 mm. The error in power prediction (Qgl-Q'gl) of the AXT was 7.7 times larger than that of AXO.

CONCLUSION

If K is exact, AXO is useful to predict the intraocular lens depth because the error of AXO is small. The error in power prediction of AXO is smaller than that of AXT.

摘要

目的

了解角膜屈光力误差对光学计算眼轴长度(AXO)以及根据无晶状体眼屈光不正(Qaph)计算的术后预测屈光不正(Q'gl)的影响。

方法

我们使用了Gullstrand简化眼模型,其中人工晶状体(+20 D)植入深度为5 mm,当前表面角膜半径(Rfc)从7 mm变化到9 mm时,通过几何方法计算Qaph和术后屈光不正(Qgl)。使用先前报告中的计算公式计算AXO,然后使用理论计算公式(将虚拟角膜折射率视为1.3315)从AXO和真实眼轴长度(AXT)计算Q'gl。

结果

当前表面测量的角膜半径(K)等于Rfc时,当K为9 mm时AXO的误差最大(AXO/AXT = 101.512)。AXT的屈光力预测误差(Qgl - Q'gl)比AXO的大7.7倍。

结论

如果K准确,AXO可用于预测人工晶状体植入深度,因为AXO的误差较小。AXO的屈光力预测误差小于AXT的。

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