Choice of reference axis in ocular wave-front aberration measurement

被引:8
作者
Cui, CW
Lakshminarayanan, V
机构
[1] GretagMacbeth, New Windsor, NY 12553 USA
[2] Univ Missouri, Sch Optometry, St Louis, MO 63121 USA
[3] Univ Missouri, Dept Phys & Astron, St Louis, MO 63121 USA
来源
JOURNAL OF THE OPTICAL SOCIETY OF AMERICA A-OPTICS IMAGE SCIENCE AND VISION | 1998年 / 15卷 / 09期
关键词
D O I
10.1364/JOSAA.15.002488
中图分类号
O43 [光学];
学科分类号
070207 [光学]; 0803 [光学工程];
摘要
The geometrical center of the pupil has often been used as the reference axis in ocular wave-front aberration measurement. However, the geometrical center of the pupil may shift when the pupil size changes under different conditions. In particular, for subjective methods, defining the center of the pupil precisely during the actual measurement is not always practical. Furthermore, the geometrical center of the pupil may not define the chief ray of the ocular optics because of the Stiles-Crawford apodization effect, which has a peak location that often deviates from the geometrical center of the pupil. We present the coefficient transformation table of the Taylor polynomial up to the sixth order with respect to reference axis shift. We illustrate the effect of wave-front aberration change with reference axis shift with experimental data. This type of wavefront aberration change could be a true measurement error if there is an error in defining the reference axis. We also propose using the coaxially sighted corneal reflex as a better reference axis in aberration measurement. (C) 1998 Optical Society of America.
引用
收藏
页码:2488 / 2496
页数:9
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