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使用眼前节光学相干断层扫描仪评估近视和正视眼的前巩膜厚度。

Assessment of anterior scleral thickness in myopes and emmetropes using anterior segment optical coherence tomography.

机构信息

Department of Orthopedics, Renmin Hospital of Wuhan University, Wuhan, China.

Department of Ophthalmology, Zhongshan Hospital of Wuhan University, Wuhan, China.

出版信息

Mol Vis. 2024 Apr 22;30:229-238. eCollection 2024.

Abstract

PURPOSE

To investigate the differences in anterior scleral thickness (AST) among the refractive statuses of Chinese adults aged 18-35.

METHODS

This study recruited 170 Chinese participants (mean age, 24.06 ± 2.78 years), including myopes (spherical equivalent refraction [SER] -1.00 to -12.75 diopters [D]; n = 134), emmetropes (SER ± 0.75 D; n = 36), and AST (superior, inferior, nasal, and temporal), which were investigated via swept-source optical coherence tomography. Semiautomated custom-designed software measured the scleral thickness from the scleral spur to 5 mm along four meridians.

RESULTS

The mean axial length and spherical equivalent refractive error were 25.12 ± 1.44 mm and -3.93 ± 3.09 D, respectively. The anterior sclera was thickest in the inferior region and thinnest in the superior region (753.9 ± 88.7 μm versus 613.6 ± 58.4; p < 0.001). The AST in the temporal meridian was significantly thicker than that in the nasal meridian (727.5 ± 60.8, 690.9 ± 55 μm; p < 0.001). There were no significant variations in AST in the myopes and emmetropes along the five latitude lines. AST along the inferior meridian at the 4-mm (r 2 = 0.0992; p < 0.001) and 5-mm (r 2 = 0.0888; p < 0.001) locations decreased significantly with increasing myopia.

CONCLUSION

With increased myopia, AST at the 4-mm and 5-mm locations showed significant thinning in the inferior meridian. The results indicate that AST, especially along the inferior meridian, may act as a biologic marker to monitor the progression of myopia.

摘要

目的

研究 18-35 岁中国成年人不同屈光状态下的前巩膜厚度(AST)差异。

方法

本研究纳入了 170 名中国参与者(平均年龄 24.06±2.78 岁),包括近视者(等效球镜屈光度 [SER] -1.00 至-12.75 屈光度 [D];n=134)、正视者(SER ± 0.75 D;n=36)以及通过扫频源光相干断层扫描测量的 AST(上、下、鼻、颞)。半自动化定制软件在四条子午线上从巩膜突测量到 5mm 处的巩膜厚度。

结果

平均眼轴长度和等效球镜屈光度误差分别为 25.12±1.44mm 和-3.93±3.09D。前巩膜在下方区域最厚,在上方区域最薄(753.9±88.7μm 比 613.6±58.4;p<0.001)。颞子午线的 AST 明显比鼻子午线厚(727.5±60.8,690.9±55μm;p<0.001)。近视者和正视者在五条纬线上的 AST 没有明显变化。下子午线 4mm(r 2 =0.0992;p<0.001)和 5mm(r 2 =0.0888;p<0.001)位置的 AST 随近视程度的增加而显著减小。

结论

随着近视程度的增加,下子午线 4mm 和 5mm 位置的 AST 明显变薄。结果表明,AST,尤其是下子午线,可能作为监测近视进展的生物标志物。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/75d5/11575840/0cd56af363cb/mv-v30-229-f1.jpg

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