To provide direct comparisons to previous
studies,
18 19 the mean sphere cycloplegic refractive error
at grade 3 was evaluated
(Table 2) as a predictor of myopia, producing a sensitivity of 86.7% and a
specificity of 73.3%. Of course, some of the nonmyopic children in the
right column of
Table 2 may go on to develop myopia, so this analysis
will be ongoing. The cut point of at least +0.75 D of hyperopia
depicted in
Table 2 was chosen so as to maximize the –2 log likelihood
in a proportional hazards analysis. (For details, see Klein and
Moeschberger, 1997.
26 ) Shifting this cut point just 0.25 D
in the myopic direction changes the sensitivity of this analysis to
68.9% and the specificity to 87.2%, illustrating the trade-off
between sensitivity and specificity with a change in predictive
criterion. Previous investigators demonstrated the predictive value of
the ratio of axial length to corneal radius of curvature (AL/CR ratio)
with a sensitivity of 88% and specificity of 57% for a cutoff of 3.02
for the AL/CR ratio
23 ; we find a much lower sensitivity
and only slightly higher specificity, even though the children in the
previous study were similar in age distribution to our sample
(Table 3) .
The ROC curves are presented in
Figures 1 and 2 . The point estimates, θ̂, and SEs for the area under the curve
are presented in
Table 4 . An MCB analysis comparing each of the individual components’ ROC
curves and the mean sphere ROC curve reveals that corneal power,
Gullstrand lens power, and axial length are each inferior to mean
sphere at the α = 0.0001 level. Therefore, the mean sphere is
the best single predictor for myopia of all the variables tested. We
wanted to examine whether the other variables in combination with the
mean sphere would improve the predictive model over that using the mean
sphere alone. A separate MCB analysis comparing the mean sphere, the
canonical, the logistic, the canonical without Gullstrand lens power,
and the logistic without Gullstrand lens power ROC curves, give the
following 95% MCB simultaneous confidence intervals:
\[{\theta}_{\mathrm{mean\ sphere}}{-}\mathrm{max}{\{}{\theta}_{\mathrm{canonical}},\ {\theta}_{\mathrm{logistic}},\ {\theta}_{\mathrm{canonical-GLP}},\ {\theta}_{\mathrm{logistic-GLP}}{\}}{=}\mathrm{{[}{-}0.042,\ 0.0000}{]}\]
\[{\theta}_{\mathrm{canonical}}{-}\mathrm{max}{\{}{\theta}_{\mathrm{mean\ sphere,}}\ {\theta}_{\mathrm{logistic}},\ {\theta}_{\mathrm{canonical-GLP}},\ {\theta}_{\mathrm{logistic-GLP}}{\}}{=}\mathrm{{[}{-}0.0099,\ }0.0083{]}\]
\[{\theta}_{\mathrm{logistic}}{-}\mathrm{max}{\{}{\theta}_{\mathrm{mean\ sphere}},\ {\theta}_{\mathrm{canonical}},\ {\theta}_{\mathrm{canonical-GLP}},\ {\theta}_{\mathrm{logistic-GLP}}{\}}{=}\mathrm{{[}{-}0.0083,}\ 0.0099{]}\]
\[{\theta}_{\mathrm{canonical-GLP}}{-}\mathrm{max}{\{}{\theta}_{\mathrm{mean\ sphere}},\ {\theta}_{\mathrm{canonical}},\ {\theta}_{\mathrm{logistic}},\ {\theta}_{\mathrm{logistic-GLP}}{\}}{=}\mathrm{{[}{-}0.0197,}\ 0.0009{]}\]
\[{\theta}_{\mathrm{logistic-GLP}}{-}\mathrm{max}{\{}{\theta}_{\mathrm{mean\ sphere}},\ {\theta}_{\mathrm{canonical}},\ {\theta}_{\mathrm{logistic}},\ {\theta}_{\mathrm{canonical-GLP}}{\}}{=}\mathrm{{[}{-}0.0203,}\ 0.0010{]}\]
The first confidence interval has zero as its upper bound,
indicating that the mean sphere (alone) model is not the best model
compared to the other four at α = 0.05. Other confidence
intervals imply that the canonical model is either the best or is
within 0.0099 of the best model, the logistic model is either the best
or is within 0.0083 of the best model, the canonical without GLP model
is either the best or is within 0.0197 of the best model, and the
logistic without GLP model is either the best or is within 0.0203 of
the best model. As these four models are indistinguishable, the
logistic model can be chosen with confidence as the best model for
practical usage, but given the difficulty in assessing Gullstrand lens
power,
25 the logistic model without Gullstrand lens power
included would be an acceptable substitute. The increment of improved
performance of the logistic model without Gullstrand lens power may be
seen in the ROC curve depicted in
Figure 2 .
Figures 3 and 4 apply the mean sphere and logistic without Gullstrand lens power models
to the prediction of future myopia in an individual child. These
figures extend the models arrived at in the ROC analysis for the
purpose of prediction. For example, the arrow in
Figure 3 corresponds
to a child with a mean sphere of –0.25 D at baseline, translating to a
chance of that child becoming myopic of 60%. Likewise, on
Figure 4a child with the logistic without GLP index of 0.456, e.g., with −0.15 D
mean sphere at baseline, a corneal power in the vertical meridian of
42.25 D, and an axial length of 24.94 mm at baseline, has a 61% chance
of developing myopia sometime in grades 4 through 8.