The average change in aberrations from the fovea (0°) to the periphery (10° and 20°) is shown in
Table 2. As an illustrative example,
Figure 3 shows point spread functions computed from one subject's measured wavefront aberrations. As stated previously, sphere and cylinder were only corrected in the fovea. Therefore, subsequent peripheral wavefronts include the foveal spherocylindrical correction, similar to habitual viewing conditions.
MTF values of horizontal and vertical gratings for all retinal eccentricities are shown in
Figures 4a and
4b, for 2 and and 4 cyc/deg, respectively. MTF values for 0°, 10°, and 20° eccentricities are denoted by square, circle, and triangle symbols respectively. Data points above the dashed equality line indicate optical anisotropy, wherein horizontal grating contrast is higher than vertical grating contrast. Conversely, data points below the dashed line indicate higher contrast for vertical gratings as compared to horizontal gratings.
At 2 cyc/deg, average horizontal MTF was 0.89 ± 0.05, 0.86 ± 0.07, and 0.79 ± 0.18 at 0°, 10°, and 20° eccentricities, respectively, whereas vertical MTF was 0.91 ± 0.04, 0.71 ± 0.16, and 0.52 ± 0.20. At 4 cyc/deg, average horizontal MTF was 0.69 ± 0.15, 0.63 ± 0.15, and 0.57 ± 0.19 at 0°, 10°, and 20° eccentricities, respectively, whereas vertical MTF was 0.74 ± 0.11, 0.49 ± 0.21, and 0.32 ± 0.17.
The inequality in horizontal and vertical MTFs increased with eccentricity for both spatial frequencies. The MTF ratios (
Figure 5) of horizontal to vertical 2 cyc/deg gratings at 0°, 10°, and 20° were 0.98 ± 0.06, 1.27 ± 0.30, and 1.73 ± 0.62, respectively. The MTF ratios at 4 cyc/deg were 0.94 ± 0.19, 1.54 ± 0.70, and 2.57 ± 1.8.
A two-way, repeated-measures ANOVA on the MTF ratios showed a significant main effect of eccentricity, F(2, 18) = 11.82, p = 0.0005, but no significant main effect of spatial frequency, F(1, 9) = 3.15, p = 0.11. There was a marginal eccentricity-x-spatial frequency interaction, F(2, 18) = 3.00, p = 0.075. At 2 cyc/deg, the MTF ratios were significantly higher than the equality line (ratio = 1) at 10° and 20° [0°: t(1, 9) = −1.05, p = 0.319; 10°: t(1, 9) = 2.90, p = 0.0176; 20°: t(1, 9) = 3.73, p = 0.0047], and were different from each other [10° vs. 0°: t(1, 9) = 3.37, p = 0.008; 20° vs. 10°: t(1,9) = 2.80, p = 0.0206; 20° vs. 0°: t(1, 9) = 3.93, p = 0.0035]. Similarly, at 4 cyc/deg, the MTF ratios were significantly above the equality line at 10° and 20° [0°: t(1, 9) = −0.93, p = 0.375; 10°: t(1, 9) = 2.43, p = 0.038; 20°: t(1, 9) = 2.76, p = 0.022], and differed from each other [10° vs. 0°: t(1, 9) = 3.00, p = 0.015; 20° vs. 10°: t(1, 9) = 2.65, p = 0.0266; 20° vs. 0°: t(1, 9) = 2.95, p = 0.0163].
In addition, we found that the MTF ratios were not well-correlated with foveal refractive error across eccentricities. The correlation coefficient between refractive error and MTF ratios at 0°, 10°, and 20° was r = 0.16, 0.15, and 0.48 at 2 cyc/deg and 0.20, 0.17, and −0.10 at 4 cyc/deg.