From the Ruiz Department of Ophthalmology and Visual Science, McGovern Medical School, The University of Texas Health Science Center at Houston (Bruner, Skanchy, Wooten, Chuang, Kim), and Robert Cizik Eye Clinic (Kim), Houston, Texas, USA.
J Cataract Refract Surg. 2020 Jan;46(1):95-101. doi: 10.1016/j.jcrs.2019.08.043.
To determine the most accurate method of estimating scleral-spur-to-scleral-spur (STS) distance for ophthalmologists without access to an anterior chamber optical coherence tomography (AS-OCT) instrument when selecting an anterior chamber intraocular lens (AC IOL).
Robert Cizik Eye Clinic, Houston, TX.
Prospective cohort study.
The eyes of 65 participants aged 18 years or older were imaged by the Lenstar LS 900 optical biometer and CASIA SS-1000 swept-source Fourier-domain AS-OCT. Eyes were excluded if the anterior segment anatomy was significantly altered and the angle could not be visualized. When both eyes were eligible, 1 eye was randomly selected. The white-to-white (WTW) distance, STS distance, and axial length were recorded and compared. The difference between STS and horizontal WTW was calculated for each meridian. The mean (±SD) differences, 95% limits of agreement, and Bland-Altman agreement were computed for each pair of STS and WTW measurements.
The study comprised 65 eyes of 65 participants. In nearly every case, WTW + 0.5 and WTW + 1 overestimated STS. The horizontal WTW without adjustment was the best predictor of STS. The WTW best corresponded to the vertical STS meridian (6 to 12 o'clock) and not the horizontal meridian (3 to 9 o'clock), along which AC IOLs are traditionally placed.
The horizontal WTW method without an adjustment factor most accurately estimated STS distance and should be used to select AC IOL size when AS-OCT is not available. If AS-OCT is available, it should be used instead. In addition, AC IOLs should be placed in a vertical orientation rather than the traditional horizontal orientation to minimize sizing errors.
当选择前房人工晶状体 (AC IOL) 时,为无法使用前房光学相干断层扫描 (AS-OCT) 仪器的眼科医生确定最准确的巩膜嵴 - 巩膜嵴 (STS) 距离估计方法。
德克萨斯州休斯顿的罗伯特·西泽克眼科诊所。
前瞻性队列研究。
使用 Lenstar LS 900 光学生物测量仪和 CASIA SS-1000 扫频源傅里叶域 AS-OCT 对 65 名年龄在 18 岁或以上的参与者的眼睛进行成像。如果前段解剖结构明显改变且无法观察到角度,则排除该眼。当双眼都符合条件时,随机选择一只眼。记录并比较了白到白 (WTW) 距离、STS 距离和眼轴长度。计算了每条子午线 STS 和水平 WTW 之间的差值。计算了每对 STS 和 WTW 测量值的平均值 (±SD) 差值、95%一致性界限和 Bland-Altman 一致性。
该研究包括 65 名参与者的 65 只眼睛。在几乎所有情况下,WTW + 0.5 和 WTW + 1 均高估了 STS。未经调整的水平 WTW 是 STS 的最佳预测指标。WTW 最符合垂直 STS 子午线 (6 至 12 点),而不是传统上放置 AC IOL 的水平子午线 (3 至 9 点)。
未经调整的水平 WTW 方法最准确地估计了 STS 距离,如果无法获得 AS-OCT,则应使用该方法选择 AC IOL 尺寸。如果可以获得 AS-OCT,则应使用它。此外,应将 AC IOL 放置在垂直方向,而不是传统的水平方向,以最大程度地减少尺寸误差。