Saitoh Kahori, Yoshida Kenji, Hamatsu Yasuhiro, Tazawa Yutaka
Department of Ophthalmology, Iwate Medical University School of Medicine, Morioka, Japan.
J Cataract Refract Surg. 2004 May;30(5):1024-30. doi: 10.1016/j.jcrs.2003.10.040.
To evaluate changes in the anterior and posterior corneal shape, corneal thickness, and anterior chamber depth (ACD) caused by mydriasis or miosis using scanning-slit corneal topography.
Department of Ophthalmology, Iwate Medical University School of Medicine, Iwate, Morioka, Japan.
Twenty-eight eyes of 28 healthy volunteers with refractive errors of -6.00 to +0.25 diopters were studied. One eye of each subject had instillation of tropicamide-phenylephrine hydrochloride (Mydrin P) to obtain mydriasis and of pilocarpine hydrochloride 2% (Sanpilo) to obtain miosis. To assess the corneal shape, the best-fit sphere (BFS), axial power, and tangential power were measured for the anterior and posterior corneal surfaces before and after mydriasis and before and after miosis using scanning-slit corneal topography (Orbscan version 3.0, Orbtek, Inc.). The pupil size, corneal thickness, and ACD were also examined before and after mydriasis and before and after miosis.
The mean age of the patients was 31.1 years +/- 5.6 (SD) (range 20 to 46 years). The anterior BFS changed from a mean of 8.04 +/- 0.3 mm at the time of mydriasis to a mean of 8.00 +/- 0.3 mm at the time of miosis. The posterior BFS changed from 6.53 +/- 0.3 mm to 6.46 +/- 0.3 mm, respectively. Thus, the anterior and posterior cornea became significantly steeper after miosis (P<.01). The ACD was significantly more shallow after miosis than after mydriasis. However, there was no significant difference in corneal thickness after mydriasis or miosis.
The anterior and posterior corneal shapes changed as a result of mydriasis and miosis, and the refractive power of the cornea significantly increased after miosis. To date, changes in refractive power from changes in pupil size have been attributed to a change in the refractive power of the crystalline lens; however, it is now thought that changes in corneal refractive power also occur.
使用扫描裂隙角膜地形图评估散瞳或缩瞳引起的角膜前后表面形状、角膜厚度和前房深度(ACD)的变化。
日本盛冈市岩手医科大学医学院眼科。
对28名屈光不正度数在-6.00至+0.25屈光度之间的健康志愿者的28只眼睛进行研究。每位受试者的一只眼睛滴入托吡卡胺-盐酸去氧肾上腺素(美多丽P)以散瞳,另一只眼睛滴入2%盐酸毛果芸香碱(喜保灵)以缩瞳。为评估角膜形状,使用扫描裂隙角膜地形图(Orbscan 3.0版本,Orbtek公司)在散瞳前后和缩瞳前后测量角膜前、后表面的最佳拟合球镜(BFS)、轴向屈光力和切向屈光力。还在散瞳前后和缩瞳前后检查瞳孔大小、角膜厚度和ACD。
患者的平均年龄为31.1岁±5.6(标准差)(范围20至46岁)。散瞳时前表面BFS的平均值为8.04±0.3 mm,缩瞳时变为8.00±0.3 mm。后表面BFS分别从6.53±0.3 mm变为6.46±0.3 mm。因此,缩瞳后角膜前、后表面明显变陡(P<0.01)。缩瞳后的ACD明显比散瞳后浅。然而,散瞳或缩瞳后角膜厚度没有显著差异。
散瞳和缩瞳导致角膜前后表面形状发生变化,缩瞳后角膜屈光力显著增加。迄今为止,瞳孔大小变化引起的屈光力变化一直归因于晶状体屈光力的改变;然而,现在认为角膜屈光力也会发生变化。