Despite prior strabismus surgery in many cases, orbital MRI was considered to provide a reasonable reflection of the sizes and positions of the rectus EOM bellies, since surgery is largely confined to the region of the insertional tendons. All subjects with CFEOM1 showed profound hypoplasia of the SR and LPS muscles, as illustrated in subject 7 in the coronal plane in
Figure 2and in the quasisagittal plane in
Figure 3 . It was often possible to detect the presence of these EOMs only in the quasisagittal MRI plane that had optimal resolution along the EOM paths, as the residual EOMs were markedly attenuated.
We computed rectus EOM volumes for subjects with CFEOM1, beginning with quantitative analysis of the largest and most homogeneous CFEOM1 subject group with the R954W amino acid substitution. These volumes included a total of contiguous six image planes beginning with the image plane that included the globe–ON junction and extending five image planes posteriorly. The volume computations thus did not include the region of the orbital apex, which was generally deep in relation to the field of imaging. Statistical analysis was performed in subjects with the R954W substitution, where a meaningful sample size was available
(Table 2) . The reduction from normal in SR volume computed from quasicoronal plane MRI ranged from 28% to 81% and averaged approximately 60% over all 11 of these subjects (
P < 0.000001;
Table 2 ). The medial rectus (MR) showed a 33% reduction in size from normal (
P < 0.000001). There were smaller, insignificant volume reductions in the IR and LR muscles averaging 13% and 14%, respectively. At least some of these small IR and LR reductions may have resulted from prior surgeries to weaken these EOMs (such as the tenotomy that thinned the anterior portion of the IR in subject 7;
Fig. 4 ), causing segmental shift of the volume of the contracted IR to the orbital apex outside the field of imaging). Comparing the data from pedigrees A and AA using
t-tests for each of the rectus EOMs, we detected no significant interfamilial differences (
P ≥ 0.15). Recognizing the availability of only one representative of each pedigree having the remaining substitutions, we cautiously compared the data of pedigree AA with those obtained from subject 14 with the R954W substitution and subjects 15, 17, and 19 with the rarer KIF21A substitutions—R954Q, M356T, and M947R—respectively. Inspection of MRI images of these subjects exhibited the same qualitative pattern of rectus EOM size reduction as did subjects with the more common R954W substitution. After adjustment for multiple comparisons, the only significant difference in subjects 14, 15, 17, and 19 was that the SR of subject 17 was significantly larger at 200 mm
3 (
P < 0.05). No other EOM volumes of the subjects with rarer substitutions differed significantly from those of the AA pedigree.
Structural abnormalities of the LR muscle were found unilaterally in one and bilaterally in six subjects with the R954W amino acid substitution. Abnormalities typically consisted of a longitudinal fissure in the deep LR belly, dividing it into superior and inferior portions
(Fig. 4) , as well as an abnormal C-shaped configuration convex to the orbital side, and irregular internal regions of bright signal. Abnormal bright signal was also observed in multiple other EOMs, as illustrated in the MRI in
Figure 5 . Subject 15 with the R954Q substitution exhibited irregular internal regions of bright signal in the horizontal rectus EOMs. The origin of this abnormal bright signal is unknown, but it would not have influenced EOM size determinations because it was distinguishable from surrounding tissues. Subject 19 with the M947R substitution had bilaterally hypoplastic LR muscles. Splitting of the LR was not observed in subject 19 or 17.