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用于预测可植入 Collamer 透镜后房房水型人工晶状体术后拱高的新尺寸参数和模型。

New Sizing Parameters and Model for Predicting Postoperative Vault for the Implantable Collamer Lens Posterior Chamber Phakic Intraocular Lens.

出版信息

J Refract Surg. 2022 May;38(5):272-279. doi: 10.3928/1081597X-20220302-01. Epub 2022 May 1.

Abstract

PURPOSE

To identify parameters influencing the postoperative vault of the Implantable Collamer Lens (ICL) (STAAR Surgical) using the Artemis Insight 100 very high-frequency (VHF) digital ultrasound robotic scanner (ArcScan, Inc) and develop a model to improve lens vault prediction.

METHODS

This was a retrospective analysis of 147 consecutive V4c EVO and EVO+ ICL implantation procedures performed over three phases in myopic eyes. In the initial phase, lens size was defined by published sulcus-to-sulcus and crystalline lens rise measurements (Kojima formula) from VHF digital ultrasound biometry. From these data, a stepwise multivariate regression analysis was performed to develop a model for predicting central vault including the following variables: ICL size, ICL power, sulcus-to-sulcus (STS), ciliary body inner diameter (CBID), zonule-to-zonule, STS lens rise (STSL), ACD, anterior chamber angle, scotopic pupil diameter (SPD), angle-to-angle, and white-to-white diameter. The resulting regression model was used in coordination with the Kojima formula to select the lens size for the next series of eyes. The regression analysis was then repeated and a further series were treated. The postoperative achieved vault at 1 month was compared to the target vault predicted by the formula. A comparison analysis of the new model was made to previously published lens sizing formulas.

RESULTS

Statistically significant variables were ICL size, ICL power, CBID, STSL, and SPD. The primary 42 eyes (Kojima formula) achieved a mean vault of 506 ± 233 µm, a range of 810 µm (114 to 924 µm), and an interquartile range (IQR) of 391 µm. Using the Reinstein formula v1.0 for the next 36 eyes, the mean vault relative to target was +7 ± 123 µm, range of 569 µm (-278 to +291 µm), and IQR of 169 µm. Using the Reinstein formula v2.0 for the next 69 eyes, the mean vault relative to target was +67 ± 121 µm, range of 573 µm (-219 to +354 µm), and IQR of 131 µm. The achieved vault was within ±100, ±200, and ±300 µm of target in 33%, 50%, and 74% of eyes, respectively, for the training group, 58%, 89%, and 100% for the Reinstein formula v1.0 group, and 62%, 84%, and 94% for the Reinstein formula v2.0 group.

CONCLUSIONS

This is the first report describing the ciliary body inner diameter, which proved to be more highly correlated with vault than STS, and thus CIBD supersedes STS from the previous widely accepted improvement over WTW sizing. The new model also found scotopic pupil size to be a significant predictor, which has not been a part of any previously published model. The significant improvement in vault predictability afforded by these parameters and the new model enables charting attempted versus achieved vault outcomes for the first time. .

摘要

目的

使用 Artemis Insight 100 超高频率(VHF)数字超声机器人扫描仪(ArcScan,Inc)识别植入式可折叠人工晶状体(ICL)(STAAR Surgical)术后拱顶的影响参数,并开发一种模型以提高晶状体拱顶预测能力。

方法

这是一项回顾性分析,共纳入 147 例连续进行的近视眼中的 V4c EVO 和 EVO+ ICL 植入手术。在初始阶段,晶状体尺寸通过 VHF 数字超声生物测量法中公布的巩膜沟到巩膜沟和晶状体上升测量值(Kojima 公式)来定义。根据这些数据,进行了逐步多元回归分析,以建立一个包括以下变量的预测中央拱顶的模型:ICL 尺寸、ICL 功率、巩膜沟到巩膜沟(STS)、睫状体内部直径(CBID)、晶状体赤道到晶状体赤道、STS 晶状体上升(STSL)、ACD、前房角、暗瞳直径(SPD)、角到角、白到白直径。根据 Kojima 公式选择下一系列眼的晶状体尺寸,使用所得回归模型。然后重复回归分析并进行进一步的系列治疗。将术后 1 个月时的实际拱顶与公式预测的目标拱顶进行比较。对新模型与以前发表的晶状体尺寸公式进行了比较分析。

结果

具有统计学意义的变量为 ICL 尺寸、ICL 功率、CBID、STSL 和 SPD。主要的 42 只眼(Kojima 公式)的平均拱顶为 506 ± 233 µm,范围为 810 µm(114 至 924 µm),四分位距(IQR)为 391 µm。对于接下来的 36 只眼,使用 Reinstein 公式 v1.0,相对于目标的平均拱顶为 +7 ± 123 µm,范围为 569 µm(-278 至 +291 µm),IQR 为 169 µm。对于接下来的 69 只眼,使用 Reinstein 公式 v2.0,相对于目标的平均拱顶为 +67 ± 121 µm,范围为 573 µm(-219 至 +354 µm),IQR 为 131 µm。在训练组中,33%、50%和 74%的眼实际拱顶分别在目标值的±100 µm、±200 µm 和±300 µm 范围内,Reinstein 公式 v1.0 组为 58%、89%和 100%,Reinstein 公式 v2.0 组为 62%、84%和 94%。

结论

这是第一个描述睫状体内部直径的报告,该直径证明与 STS 相比,与拱顶的相关性更高,因此,与之前广泛接受的 WTW 尺寸相比,CBID 取代了 STS。新模型还发现暗瞳大小是一个重要的预测因子,这在以前的任何模型中都没有涉及。这些参数和新模型显著提高了拱顶预测能力,首次实现了试图与实际拱顶结果的图表绘制。

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