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Sirius 角膜地形仪检测的高阶像差及其与不同屈光不正的关系。

Corneal higher order aberrations by Sirius topography and their relation to different refractive errors.

机构信息

Department of Ophthalmology, Tishreen University, Latakia, Syria.

Department of Ophthalmology, King's College Hospital NHS Foundation Trust, London, UK.

出版信息

BMC Ophthalmol. 2023 Mar 16;23(1):104. doi: 10.1186/s12886-023-02841-4.

Abstract

PURPOSE

To compare the root mean square (RMS) of anterior corneal higher-order aberrations (HOAs) in ametropic and emmetropic eyes.

METHODS

This retrospective observational study was conducted at the Department of Ophthalmology, Tishreen University Hospital, Latakia, Syria. Study eyes were divided into four groups based on refractive error: mild-to-moderate myopia, hypermetropia, myopic astigmatism, and emmetropic eyes as controls. The following anterior corneal HOAs were evaluated using the Scheimpflug-Placido Sirius (CSO, Italy) tomographer over 6 mm pupil: Root mean square (RMS) total corneal HOAs, RMS trefoil, RMS coma and RMS spherical aberrations.

RESULTS

RMS values of total HOAs, trefoil and coma showed statistically significant differences in all four groups (P < 0.05, all). HOAs were noted to be lowest in the control group (0.18 ± 0.09, 011 ± 0.08 and 0.09 ± 0.08 μm, respectively) and highest in the myopic astigmatism group (0.31 ± 0.16, 0.15 ± 0.12, 0.17 ± 0.14 μm, respectively). RMS spherical aberration was lowest in the astigmatism group (0.00 ± 0.16 μm) with a statistically significant difference from that in the control group (0.05 ± 0.07 μm, P = 0.049).

CONCLUSION

The mean RMS values of total HOAs, trefoil and coma were highest in the astigmatism group and lowest in the control group. However, spherical aberration was minimal in the astigmatism group. A better understanding and targeted treatment of higher-order aberrations in ametropic human eyes, and in particular eyes with astigmatism, may enhance visual quality and performance in the treatment of refractive errors. Recognising atypical HOAs may also assist in the early detection of pathological conditions such as keratoconus.

摘要

目的

比较屈光不正和正视眼中前角膜高阶像差(HOA)的均方根(RMS)。

方法

本回顾性观察研究在叙利亚拉塔基亚的提什林大学医院眼科进行。研究眼根据屈光不正分为四组:轻度至中度近视、远视、近视散光和正视眼作为对照组。使用 Scheimpflug-Placido Sirius(CSO,意大利)断层扫描仪在 6mm 瞳孔下评估以下前角膜 HOA:RMS 总角膜 HOA、RMS 三叶形、RMS 彗差和 RMS 球差。

结果

在所有四组中,RMS 总 HOAs、三叶形和彗差值均存在统计学差异(P<0.05,均)。对照组的 HOA 值最低(分别为 0.18±0.09、0.11±0.08 和 0.09±0.08μm),近视散光组最高(分别为 0.31±0.16、0.15±0.12 和 0.17±0.14μm)。在散光组中,RMS 球差最低(0.00±0.16μm),与对照组相比差异具有统计学意义(0.05±0.07μm,P=0.049)。

结论

在散光组中,总 HOAs、三叶形和彗差的 RMS 值平均值最高,而在对照组中 RMS 值平均值最低。然而,在散光组中球差最小。更好地理解和针对性治疗屈光不正患者,特别是散光患者的高阶像差,可以提高治疗屈光不正的视觉质量和性能。识别非典型的高阶像差也可能有助于早期发现如圆锥角膜等病理情况。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ab50/10018888/117081665bf8/12886_2023_2841_Fig1_HTML.jpg

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