Stewart Stephen, Yeo Tun Kuan, Moutari Salissou, McNeely Richard N, Moore Jonathan E
Cathedral Eye Clinic, Belfast, UK.
Centre for Public Health, Queen's University Belfast, Belfast, UK.
Clin Ophthalmol. 2025 Jan 6;19:35-43. doi: 10.2147/OPTH.S488571. eCollection 2025.
To determine whether accounting for posterior corneal surgically induced astigmatism (SIA) would improve toric intraocular lens power calculation prediction error.
A total of 189 eyes of 148 patients undergoing routine cataract surgery were included in the study. Standard and posterior keratometry were measured pre- and postoperatively. Centroid SIA with standard keratometry and posterior keratometry were calculated separately. Prediction errors for postoperative refractive astigmatism at 4 weeks postoperatively were compared for Barrett Toric with predicted posterior corneal astigmatism (PPCA); Barrett Toric with preoperative measured posterior corneal astigmatism (MPCA); Barrett Toric with postoperative MPCA, which accounts for posterior corneal SIA.
There was a significant increase in PCA magnitude postoperatively (p < 0.001), although a change of >0.3D occurred in only 3% of eyes. There was a postoperative rotation in the steep meridian of >10° in 32% of eyes. The Barrett Toric formula with PPCA yielded a significantly smaller refractive astigmatism prediction error compared to when a postoperative MPCA value was used (p < 0.01). Postoperative MPCA had a lower proportion of eyes within 0.50, 0.75 and 1.00D of predicted refractive astigmatism than PPCA or preoperative MPCA, although this was not statistically significant.
This study demonstrated postoperative changes in posterior corneal astigmatism magnitude and the orientation of the steep meridian. However, accounting for posterior keratometric SIA in the Barrett Toric formula does not improve refractive astigmatism prediction accuracy.
确定将角膜手术诱导的后表面散光(SIA)纳入考量是否会改善散光型人工晶状体屈光力计算的预测误差。
本研究纳入了148例行常规白内障手术患者的189只眼。术前和术后分别测量标准角膜曲率和后表面角膜曲率。分别计算标准角膜曲率和后表面角膜曲率的质心SIA。比较Barrett Toric公式在预测后表面角膜散光(PPCA);术前测量的后表面角膜散光(MPCA);考虑后表面角膜SIA的术后MPCA情况下,术后4周时术后屈光性散光的预测误差。
术后PCA大小显著增加(p < 0.001),尽管仅3%的眼变化>0.3D。32%的眼角膜陡峭子午线术后旋转>10°。与使用术后MPCA值相比,带有PPCA的Barrett Toric公式产生的屈光性散光预测误差显著更小(p < 0.01)。与PPCA或术前MPCA相比,术后MPCA在预测屈光性散光的0.50、0.75和1.00D范围内的眼比例更低,尽管这无统计学意义。
本研究证明了后表面角膜散光大小和角膜陡峭子午线方向的术后变化。然而,在Barrett Toric公式中考虑后表面角膜SIA并不能提高屈光性散光预测准确性。