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Posterior corneal astigmatism: a review article

机译:角膜后散光:评论文章

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Most human eyes show at least a small degree of corneal astigmatism and it can arise from both surfaces of the cornea. The shape of the anterior corneal surface provides no definitive basis for knowing the toricity of the posterior surface. In the previous studies, average astigmatism of the posterior corneal surface was ?0.26 to ?0.78 diopter. The radius of the posterior corneal surface is less than the radius of the anterior corneal surface. Most studies have found a clear correlation between the anterior and posterior corneal asphericities and the asphericity of the posterior surface is independent of the vertex radius of curvature, refractive error and gender. In contrast to the anterior corneal surface, the asphericity of the posterior corneal surface varies significantly between meridians. The anterior and posterior corneal surface would have approximately parallel principal meridians and both of these surfaces are often flatter in the horizontal meridian than the vertical one. This is especially true in the higher degrees of corneal astigmatism, and then about 10% of any anterior corneal astigmatism is neutralized by an astigmatism arising from the posterior corneal surface. Although the second corneal surface only contributes to about 10% of the total refractive power of the eye, a precise knowledge of its morphology is needed for the correct diagnosis and monitoring the corneal diseases or the surgical interventions and in many eyes neglecting the posterior corneal surface measurement may lead to significant deviations from the corneal astigmatism estimation. In this article, we have reviewed the shape and the toricity of the posterior corneal surface and also the effect of age on it. We investigated the contribution of posterior corneal astigmatism to the total corneal astigmatism and evaluated the accuracy of corneal astigmatism estimation by neglecting the posterior corneal surface measurement.
机译:大多数人眼至少表现出少量的角膜散光,它可能来自角膜的两个表面。角膜前表面的形状不为确定后表面的复曲面提供确定的基础。在以前的研究中,角膜后表面的平均散光度约为0.26至0.78屈光度。角膜后表面的半径小于角膜前表面的半径。多数研究发现,角膜前和后角非球面度之间存在明显的相关性,而后表面的非球面度与顶点曲率半径,屈光不正和性别无关。与前角膜表面相反,在子午线之间,后角膜表面的非球面性明显不同。角膜前表面和后表面将具有近似平行的主子午线,并且这两个表面在水平子午线上通常比垂直子午线上更平坦。在较高程度的角膜散光中尤其如此,然后任何约10%的前角膜散光被后角膜表面产生的象散中和。尽管第二个角膜表面仅占眼睛总屈光力的10%,但需要正确了解其形态才能正确诊断和监测角膜疾病或手术干预,并且在许多眼睛中忽略了后角膜表面测量可能会导致与角膜散光估计值的明显偏差。在本文中,我们回顾了角膜后表面的形状和曲面以及年龄对其的影响。我们调查了角膜后散光对总角膜散光的贡献,并通过忽略角膜后表面的测量来评估角膜散光估计的准确性。

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