Keratoscope photograph negatives of one normal cornea and calibration
steel spheres were digitized by a CCD video camera connected to a fram
e grabber. The centroid of the innermost reflected mire was determined
and used for conversion of the image to polar coordinates. The distan
ce to each reflected ring was computed. Calculations of the radius of
curvature describing the reflecting surface locally were performed by
an iterative procedure based on differential equations. The calculated
mean radius for steel spheres in the range of 5.5 to 11 mm in diamete
r conformed with the known values. The average difference between obse
rved and expected values was 0.2% and the average coefficient of varia
tion was 0.1%. The standard deviations on observed ring means decrease
d inversely with ring number with an average coefficient of variation
of 0.2%. Likewise, on a corneal surface SD also decreased inversely wi
th ring number from 0.080 to 0.032 mm. In terms of refractive power th
is meant, that outwards from the third ring 95% of observations were w
ithin +/-0.4 diopters from the average value.