A schematic outline of the experiments is shown in
Figure 1. Two vertical lines are presented on a gray background. During each run, the separation Δ
x (i.e., the distance between the inner edges of the two lines) remained constant and the temporal offset Δ
t (i.e., the time interval between the onset of the two lines) varied randomly from trial to trial.
In
Figure 2, the proportion of correct responses is plotted as a function of the temporal offset (Δ
t) for the two line stimuli shown in the insets. In the top panel, line separation (Δ
x) is 0 arcmin; that is, for a line width of 2 arcmin, the line edges touch. For both conditions (see insets), proportion correct is at about chance value (0.5) for Δ
t = 0. For equal contrast polarity, proportion correct increases with increasing Δ
t, but for opposite contrast polarity, proportion correct decreases to below 0.25 for temporal offsets between 8.3 and 25 ms and only increases again between 33 and 50 ms. Thus, for the shorter temporal offsets, perceived direction is veridical for two black lines flashed in succession but is reversed in most cases, if one black line and one white line are presented. This confirms and extends earlier results (Anstis,
1970; Chubb & Sperling,
1989).
If line separation Δ
x is 18 arcmin (
Figure 2, bottom panel), the perceived direction of motion elicited by the line pairs and that of the stimuli is the same, independent of the polarity of line pairs, although the two proportion correct functions obtained for equal and opposite contrast stimuli differ slightly. The transition between the situations described in the two panels of
Figure 2 is gradual (data not shown), indicating that the influence of the presumed short-range mechanism is strong for a separation of 0 arcmin (top panel) but weakened or absent at 18 arcmin (bottom panel).
Figure 3 shows the proportion correct for stimuli with opposite contrast polarity in Observer 2. Here, temporal and spatial offsets used are almost twice as large as those in the previous experiment. I note that at a separation of 0 min and temporal offsets of 17 and 33 ms, the white–black line pair yields significantly reversed responses. At a temporal offset of 50 ms, values are still below 0.5. At 67 ms, the proportion correct is back to 0.5 with a significant increase to 0.74 (correct perception of direction is reasonably certain) at 100 ms. For a stimulus of two white lines at a separation of 0 arcmin, perception in this observer is veridical. At the larger separation (30 arcmin), the white–black line pair yields veridical responses. For the larger spatiotemporal offsets required in this observer, this corresponds to the results shown in
Figure 2.
If reversed perception of direction due to opposite contrast stimuli is generated by the short-range mechanism, it should depend on eccentricity in a way similar to short-range motion (Foster, Thorson, McIlwain, & Biederman-Thorson
1981; Thorson, Lange, & Biederman-Thorson,
1969; Westheimer,
1983). This was tested in the next experiment presenting equal and opposite contrast stimuli in the parafovea at an eccentricity of 4 deg. Stimulus dimensions and line separation (12 arcmin) match those presented in the fovea, assuming that cortical magnification factor predicts the respective spatial parameters (Westheimer,
1983). The data show that perceived direction is reversed when a white line and a black line are presented (top panel). For identical line parameters with both lines being white, a rapid increase into saturation is observed.
For a distance of 48 arcmin, long-range motion seems to dominate: Proportion correct responses to both equal and opposite contrast stimuli increase with increasing temporal offset in a very similar way.
For the stimuli used in this study, I have quantified the “reversed phi” phenomenon first described by Anstis (
1970) and reproduced later by other groups (e.g., Chubb & Sperling,
1989). Moreover, with these stimuli, I am able to delineate the transition between the conditions where strong reversed phi is observed (small separations) and those where this is not the case (large separations). On the basis of the arguments laid out in the
Discussion section, I propose that this is equivalent to the parameters constraining the short-range system. As can be seen when comparing
Figure 2 with
Figures 3 and
4, the temporal offset is much larger in Observer 2 as compared with Observer 1. The results from Observer 3 to the conditions of
Figures 2,
5, and
6 are shown as an
auxiliary file. They are very similar in all other respects to those of Observer 1. The range of spatial separations within which reversed phi is observed is similar among all three observers.
The curves in
Figures 2,
3, and
4 are based on about 1,000 trials. I obtained the data represented in such curves in two observers for six line separations, each with dark → bright, bright → dark, bright → bright, and dark → dark sequences. Following the convention introduced by Adelson and Bergen (
1985), the results are presented as space–time diagrams. In
Figure 5, the proportions of correct responses are shown as squares whose color represents the perceived direction and whose areas indicate the proportion of correct choices.
For this and the other two observers, the range of the space–time diagram in which dark → bright and bright → dark stimuli elicit inverted direction of motion is surrounded on both sides by a region in which this is not the case. The black squares indicating perception in a direction opposite to the stimulus are oriented along a diagonal tilted to the left. This is consistent with predictions arising from the energy model (Adelson & Bergen,
1985; Emerson, Bergen, & Adelson,
1992).
As a control, the space–time plot of proportions correct for stimuli of equal contrast polarity is shown in
Figure 6 (same observer as in
Figure 5). As expected, equal contrast polarity sequences are perceived to correspond to the direction of the stimulus throughout. I note that for both the smallest and largest separation, proportions correct increase more slowly with increasing temporal offset.
More data for Observer 1 and a whole set for yet another observer show that the phenomena described here are independent of whether pairs of black lines or pairs of white lines are shown. Reversed phi is reliably obtained irrespective of whether the white line or the dark line is presented first (see
auxiliary data).