Figure 5 shows within-observer averages (circles) and inter-observer averages (bars) for all 16 participants. The ordinate represents angular mislocalization, where the positive shifts denote the CCW direction.
For the interobserver averages, we performed one-sample t-tests to determine whether the FGE shift (i.e., the angular mislocalization in the direction of the FGE prediction) was >0° to confirm the occurrence of FGE. In the sync condition with the filled-in inducer, the FGE shift was >0° in the top-CCW (t(15) = 2.16, p = 0.047), top-CW (t(15) = 6.17, p < 0.001) and bottom-CCW (t(15) = 11.45, p < 0.001) conditions, although the shift in the top-CCW condition was not significant after the adjustment of significance level using the Holm method. In the sync condition with the occluded inducer, the FGE shift was >0° in the top-CCW (t(15) = 2.86, p = 0.012), top-CW (t(15) = 6.00, p < 0.001), and bottom-CCW (t(15) = 7.68, p < 0.001) conditions. In the async condition with the filled-in inducer, the FGE shift was >0° in the top-CW (t(15) = 6.45, p < 0.001) and bottom-CCW (t(15) = 7.80, p < 0.001) conditions. In the async condition with the occluded inducer, the FGE shift was >0° in the top-CW (t(15) = 6.08, p < 0.001) and bottom-CCW (t(15) = 7.94, p < 0.001) conditions. Thus, in all combinations of inducer type (filled-in and occluded) and flash onset time (sync and async), the FGE significantly occurred at least in the critical conditions in which the FGE prediction was within the blind-spot region. In all conditions with the physical inducer, the FGE shift was >0° (the async and top-CCW, p = 0.011; the async and bottom-CCW, p = 0.038; otherwise, ps < 0.001).
As mentioned in the above individual data analysis, the FGE prediction under the bottom-CCW and top-CW conditions fell inside the blind-spot region. To examine whether the FGE indeed delivered the flash inside the blind-spot region in the critical conditions of bottom-CCW and top-CW, we performed a one-sample two-tailed t-test to determine whether the FGE shift was >5°, i.e., the distance between the flash and the ellipse border, for the inter-observer average in each condition. The results were as follows.
To compare the FGE shifts across conditions, we additionally performed a four-way repeated-measures analysis of variance (ANOVA) with inducer type (filled-in, occluded, and physical), flash onset time (sync and async), flash position (top and bottom), and rotation direction after the reversal (CW and CCW) as factors. The main effect of flash onset time (
F(1,15) = 47.44,
p < 0.001,
\(\eta^{2}_{\rm{p}}\) = 0.76) was significant, confirming that the FGE shift indeed depended on the synchronicity between the flash and the directional reversal of the inducer, consistent with previous studies (
Cavanagh & Anstis, 2013). The main effect of inducer type (
F(2,30) = 26.89,
p < 0.001,
\(\eta^{2}_{\rm{p}}\) = 0.64) was significant. Because there was no significant four-way interaction (
p = 0.75), we further analyzed the sync and async conditions separately using a three-way ANOVA for each, with completion type, target position, and rotation direction as the factors. In the sync condition, in which an optimal FGE was expected to occur, the main effect of completion type was significant (
F(2,30) = 32.07,
p < 0.001,
\(\eta^{2}_{\rm{p}}\) = 0.68). The statistical results for other conditions including the async condition are detailed in
Tables 1 and
2. In the results of the post-hoc pairwise multiple comparisons with the Tukey-Kramer method, the illusion amplitude for the filled-in inducer was significantly smaller than that for the physical inducer in the
top-CCW condition (
t(15) = 5.03,
p < 0.001,
r = 0.79). In the top-CW condition, the filled-in (
t(15) = 4.65,
p < 0.001,
r = 0.77) and occluded (
t(15) = 4.94,
p < 0.001,
r = 0.79) inducers exhibited significantly smaller illusion amplitudes than the physical inducer.