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使用两枚后房型有晶体眼人工晶状体使极短眼轴实现正视化

Achieving emmetropia in extremely short eyes with two piggyback posterior chamber intraocular lenses.

作者信息

Holladay J T, Gills J P, Leidlein J, Cherchio M

机构信息

Department of Ophthalmology, University of Texas Medical School, Houston, USA.

出版信息

Ophthalmology. 1996 Jul;103(7):1118-23. doi: 10.1016/s0161-6420(96)30558-7.

Abstract

PURPOSE

To examine the refractive results and limitations of current intraocular lens power formulas when implanting two posterior chamber lenses in-the-bag to achieve emmetropia in extremely short eyes.

METHODS

Preoperative measurements (corneal diameter, axial length, keratometry, anterior chamber depth, and lens thickness) and postoperative measurements (refraction, corneal vertex to iris depth, and iris to front anterior lens surface) were taken in six eyes from three patients, with axial lengths ranging from 15.09 to 19.95 mm. These data were used to calculate the prediction error for three current third-generation formulas (Holladay, Hoffer Q, SRK/T) and two older formulas (SRK2 and SRK1).

RESULTS

None of the formulas accurately predicted the refractions using the optimized lens constants for normal eyes. The third-generation formulas were not different (P > or = 0.602) and averaged 5 diopters (D) of absolute error (Hoffer Q = 4.64 +/- 1.57 D; Holladay = 5.07 +/- 1.28 D; SRK/T = 5.12 +/- 1.43 D). The older formulas were significantly worse (P = 0.0006), with average mean absolute errors of 10.93 +/- 5.09 D for the SRK2 and 13.33 +/- 5.09 D for the SRK1. When the formulas were optimized for these six eyes, the mean absolute errors were Holladay = 1.33 +/- 1.25 D; SRK/T = 2.10 +/- 1.31 D; Hoffer Q = 4.54 +/- 2.00 D; SRK2 = 4.71 +/- 1.94 D; and SRK1 = 4.71 +/- 1.94 D. The Holladay and SRK/T formulas were statistically better (P = 0.0068) than the Hoffer Q and the two older formulas.

CONCLUSION

Current third-generation formulas are better than older formulas for extremely short eyes, but still are not acceptable for the desired clinical accuracy. Newer formulas that will use additional anterior segment measurements (corneal diameter, anterior chamber depth, and lens thickness) will be required for improved accuracy, because the anterior segment often is not proportional to the axial length.

摘要

目的

研究在极短眼内植入两枚后房型人工晶状体于囊袋内以达到正视化时,当前人工晶状体屈光力计算公式的屈光结果及局限性。

方法

对3例患者的6只眼进行术前测量(角膜直径、眼轴长度、角膜曲率、前房深度及晶状体厚度)及术后测量(屈光、角膜顶点至虹膜深度及虹膜至晶状体前表面),眼轴长度范围为15.09至19.95毫米。这些数据用于计算三种当前第三代公式(霍拉迪公式、霍弗Q公式、SRK/T公式)及两种较老公式(SRK2公式和SRK1公式)的预测误差。

结果

使用针对正常眼优化的晶状体常数时,没有一种公式能准确预测屈光情况。第三代公式之间无差异(P≥0.602),绝对误差平均为5屈光度(D)(霍弗Q公式=4.64±1.57 D;霍拉迪公式=5.07±1.28 D;SRK/T公式=5.12±1.43 D)。较老的公式明显更差(P=0.0006),SRK2公式的平均绝对误差为10.93±5.09 D,SRK1公式为13.33±5.09 D。当针对这6只眼优化公式时,平均绝对误差为:霍拉迪公式=1.33±1.25 D;SRK/T公式=2.10±1.31 D;霍弗Q公式=4.54±2.00 D;SRK2公式=4.71±1.94 D;SRK1公式=4.71±1.94 D。霍拉迪公式和SRK/T公式在统计学上优于霍弗Q公式及两种较老的公式(P=0.0068)。

结论

对于极短眼,当前的第三代公式比老公式更好,但对于期望的临床准确性仍不可接受。由于眼前节通常与眼轴长度不成比例,需要使用额外眼前节测量值(角膜直径、前房深度及晶状体厚度)的更新公式以提高准确性。

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