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近视激光手术后的人工晶状体计算:已发表方法的临床比较。

Intraocular lens power calculation after myopic excimer laser surgery: clinical comparison of published methods.

机构信息

GB Bietti Eye Foundation-IRCCS, Rome, Italy.

出版信息

J Cataract Refract Surg. 2010 Sep;36(9):1455-65. doi: 10.1016/j.jcrs.2010.02.029.

Abstract

PURPOSE

To compare results of intraocular lens (IOL) power calculation methods after myopic excimer laser surgery.

SETTING

Private practice.

METHODS

In this prospective study, eyes having phacoemulsification after myopic excimer laser surgery were classified into Group 1 (preoperative corneal power available, refractive change known), Group 2 (preoperative corneal power available, refractive change uncertain), and Group 3 (preoperative corneal power unavailable, refractive change known even if uncertain). The IOL power was calculated using the following methods: clinical history, Awwad, Camellin/Calossi, Diehl, Feiz, Ferrara, Latkany, Masket, Rosa, Savini, Shammas, Seitz/Speicher, and Seitz/Speicher/Savini.

RESULTS

The lowest mean absolute errors (MAEs) in IOL power prediction in Group 1 (n = 12) and Group 2 (n = 11), respectively, were with the methods of Seitz/Speicher/Savini (0.51 diopter [D] +/- 0.44 [SD] and 0.55 +/- 0.50 D), Seitz/Speicher (0.58 +/- 0.47 D and 0.54 +/- 0.45 D), Savini (0.60 +/- 0.44 D and 0.65 +/- 0.63 D), Masket (0.82 +/- 0.49 D and 0.69 +/- 0.51 D), and Shammas (0.77 +/- 0.43 D and 1.11 +/- 0.50 D). In Group 3 (n = 5), the lowest MAEs were with the methods of Masket (0.23 +/- 0.27 D), Savini (0.49 +/- 0.86 D), Seitz/Speicher/Savini (0.68 +/- 0.36 D), Shammas (0.84 +/- 0.98 D), and Camellin/Calossi (0.91 +/- 0.84 D).

CONCLUSIONS

When corneal power is known, the Seitz/Speicher method (with or without Savini adjustment) seems the best solution to obtain an accurate IOL power prediction. Otherwise, the Masket method may be the most reliable option.

摘要

目的

比较近视激光手术后人工晶状体(IOL)屈光力计算方法的结果。

背景

私人诊所。

方法

在这项前瞻性研究中,将行白内障超声乳化术的近视激光手术后的眼分为 3 组:第 1 组(术前角膜屈光力可获得,屈光变化已知)、第 2 组(术前角膜屈光力可获得,屈光变化不确定)和第 3 组(术前角膜屈光力不可获得,即使屈光变化不确定也已知)。使用以下方法计算 IOL 屈光力:临床病史、Awwad、Camellin/Calossi、Diehl、Feiz、Ferrara、Latkany、Masket、Rosa、Savini、Shammas、Seitz/Speicher 和 Seitz/Speicher/Savini。

结果

在第 1 组(n = 12)和第 2 组(n = 11)中,IOL 屈光力预测的平均绝对误差(MAE)最低的分别是 Seitz/Speicher/Savini(0.51 屈光度[D] +/- 0.44 [SD] 和 0.55 +/- 0.50 D)、Seitz/Speicher(0.58 +/- 0.47 D 和 0.54 +/- 0.45 D)、Savini(0.60 +/- 0.44 D 和 0.65 +/- 0.63 D)、Masket(0.82 +/- 0.49 D 和 0.69 +/- 0.51 D)和 Shammas(0.77 +/- 0.43 D 和 1.11 +/- 0.50 D)方法。在第 3 组(n = 5)中,MAE 最低的是 Masket(0.23 +/- 0.27 D)、Savini(0.49 +/- 0.86 D)、Seitz/Speicher/Savini(0.68 +/- 0.36 D)、Shammas(0.84 +/- 0.98 D)和 Camellin/Calossi(0.91 +/- 0.84 D)方法。

结论

当角膜屈光力已知时,Seitz/Speicher 方法(带或不带 Savini 校正)似乎是获得准确 IOL 屈光力预测的最佳方法。否则,Masket 方法可能是最可靠的选择。

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