Kashiwagi T
Kashiwagi Eye Clinic, Sakai-city, Japan.
Nippon Ganka Gakkai Zasshi. 1993 Apr;97(4):519-25.
Postoperative lens location was expressed as a linear regression formula of axial length and corneal curvature. Using the formula, the IOL power of a convexplano, biconvex, and planoconvex lens was calculated by Ray Tracing Error Correction (RTEC). The calculated power of a convexplano lens coincides with Sanders, Retzlaff, Kraff (SRK) II in axial length less than 28 mm and corneal curvature between 7 to 9 mm. Varying regression coefficients changes lens power continuously and simulates the theoretical formulas SRK II and SRK. RTEC predicted that formula SRK II is valid only for a convexplano lens and needs correction in a biconvex or planconvex lens and in corneal curvature less than 7.0 mm. IOL power determination requires a learning process based on the postoperative refraction. The difference of learning between SRK and RTEC is also discussed.
术后晶状体位置用眼轴长度和角膜曲率的线性回归公式表示。利用该公式,通过光线追踪误差校正(RTEC)计算出凸平、双凸和平凸透镜的人工晶状体屈光度。在眼轴长度小于28mm且角膜曲率在7至9mm之间时,凸平晶状体的计算屈光度与桑德斯、雷茨拉夫、克拉夫(SRK)II公式相符。改变回归系数可连续改变晶状体屈光度,并模拟SRK II和SRK的理论公式。RTEC预测,SRK II公式仅对凸平晶状体有效,在双凸或平凸透镜以及角膜曲率小于7.0mm时需要校正。人工晶状体屈光度的确定需要基于术后验光的学习过程。还讨论了SRK和RTEC在学习方面的差异。