Mean vection magnitude as a function of viewing condition (binocular or monocular), disparity modulation type, and stimulus speed is shown in
Figure 4. The manipulation of most interest in this experiment was viewing condition.
Figure 4 shows that binocular viewing of disparate moving stimuli produced stronger mean vection ratings than monocular viewing for all conditions. Consistent with the results of
Experiment 1, vection magnitude estimates increased with increased stimulus speed, but there was little indication of an effect of stimulus pattern (disparity modulation type). The latter finding is expected in the monocular conditions because the disparity modulation would not be visible without stereopsis. For the binocular conditions it suggests that the particular pattern of disparity-defined features was not critical for the vection enhancement with binocular viewing.
A repeated-measures ANOVA (with Greenhouse-Geisser correction where appropriate) indicated a significant main effect of stimulus speed, with higher speeds producing stronger vection ratings, F(1, 14) = 30.35, p < 0.001, η2p = 0.684. There was also a main effect of viewing condition, F(1, 14) = 4.75, p = 0.047, η2p = 0.253, and an interaction between disparity waveform type and viewing condition, F(2.22, 31.07) = 4.512, p = 0.016, η2p = 0.244. The main effects of disparity waveform and fixation were not significant—F(2.76, 38.69) = 0.37, p = 0.762, η2p = 0.025 and F(1, 14) = 0.45, p = 0.513, η2p = 0.031, respectively—nor were there any other significant interactions. One subject reported much smaller vection magnitude under monocular conditions than other subjects; the analyses repeated with this subject removed yielded the same pattern of results as with the full data set.
The interaction of disparity waveform and viewing type was analyzed by looking at the simple main effects of viewing for each waveform. This interaction was expected since the waveform was defined by cyclopean features—hence invisible monocularly—so if there was an effect of waveform it should be apparent only under binocular viewing. Binocular viewing increased vection magnitudes, but this increase was significant only for the sine and square waveforms. Binocular viewing on average generated 8.2 (±3.49 SEM) and 9.3 (±3.49) increases in vection magnitude ratings, respectively—F(1, 14) = 5.93, p = 0.033, η2p = 0.285 and F(1, 14) = 7.11, p = 0.018, η2p = 0.337, respectively—with smaller effects for the sawtooth and triangle waveforms—mean rating increases of 7.1 (±3.79) and 4.6 (±3.00), respectively; F(1, 14) = 3.50, p = 0.083, η2p = 0.200 and F(1, 14) = 2.34, p = 0.148, η2p = 0.143, respectively. Thus, while binocular viewing generally increased vection magnitudes, the effect depended on the type of disparity waveform.