Bennett
31 derived an equation for a conic section, which can be written
\[r_{\mathrm{a}}^{2}\ {=}\ r_{\mathrm{o}}^{2}\ {+}\ ({-}Q)y^{2},\]
where
r o,
Q,
r a, and
y refer to the apical radius of curvature, corneal asphericity, the axial radius of curvature, and perpendicular distance from the corneal apex, respectively. Both
r a and
y are provided by the TMS-1 in the .DIO (
r a = 0.3375/.DIO) and .RAD files, respectively. Assuming the TMS-1 measures axial radius of curvature, we graphed data for each corneal position as axial radius of curvature squared,
r a 2, versus perpendicular distance from the corneal apex squared (
y 2). When the best-fitting line is plotted to this graph by the method of least squares, the square root of the
y-intercept equals apical radius of curvature (
r o), and the negative slope equals corneal asphericity (
Q).
32 When data obtained from the TMS-1 are used, this graphical method has been found to be very accurate when measuring aspheric surfaces near
Q = −0.2 as demonstrated on calibrated conicoid surfaces.
33 A demonstration of the graphical method for one topography reading of a subject included in the study can be found in
Figure 2 . Corneal asphericity and
r o obtained using the graphical method can be considered particularly useful in comparative studies, considering the high repeatability of the TMS-1.
33 34 35 The
Q and
r o found for the videokeratoscopic images were averaged for each child. Corneal asphericity data obtained in this study are reported as global asphericity, representing the cornea as a whole and encompassing all meridians. Children with ≥1.50 D of refractive astigmatism were excluded from the study as a stringent cutoff, since individuals with no more than 2 D of refractive astigmatism are known to exhibit little meridional variation in corneal asphericity.
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