We measured the impact of overall light level on temporal processing in the visual system by taking advantage of both the reverse and classic Pulfrich effects. Two experiments were run. The first experiment assessed how changes in overall light level changed the strength of the reverse Pulfrich effect, which is induced by interocular differences in focus error. The second experiment assessed how changes in overall light level changed the strength of the classic Pulfrich effect, which is induced by interocular differences in the amount of light entering each eye. In both experiments, pupil size was either fixed to one of three diameters (2 mm, 4 mm, and 6 mm), or it was measured as it varied naturally during the experiments (see
Methods). Across the four overall light levels (i.e., display luminances) used in the experiment, the natural pupil sizes ranged from between 4 mm to 6 mm (see
Supplementary Figure S1). In total, there were 16 distinct retinal illuminance levels ranging from between 0.6 to 360 trolands.
Subjects viewed four horizontally drifting strips textured with vertical bars, that were stereoscopically specified to be in front of, in line with, or behind the plane of the screen. The task, in an adjustment procedure, was to adjust the apparent depth until all strips appeared to be moving in the plane of the screen. Neighboring strips always drifted at the same speed in opposite directions (left vs. right), and the onscreen disparity associated with adjacent strips was always equal in magnitude and opposite in sign. The task was intuitive and easy for subjects to perform.
In the reverse Pulfrich experiment, for each overall light level, data was collected in each of the two conditions. In one condition, the left-eye image was more defocused (ΔF = −3.0 D) and, hence, blurrier than the right-eye image; in the other condition, the right-eye image was more defocused than the left-eye image (ΔF = 3.0 D).
Figure 4A shows the onscreen delay for the 12 adjustment runs (6 runs × 2 conditions) from one observer at a particular overall light level and pupil size (0.2 cd/m
2 and 4 mm). (This data is representative of the raw data in other conditions.) The average across the final settings of all six runs in a given condition provides an estimate of the critical onscreen delay that was required to make the drifting bars appear to move in the plane of the screen. This critical onscreen delay should be equal in magnitude and opposite in sign to the neural delay caused by the interocular difference in light level. When the left eye was blurry, the critical onscreen delay was −11.4 ± 4.9 ms (ΔF = −3.0 D). When the right eye was blurry, the critical onscreen delay was 11.7 ± 3.6 ms (ΔF = 3.0 D). These results indicate that the image in the manipulated (blurrier) eye was neurally processed more quickly. These results are consistent with previously reported results (
Burge et al., 2019;
Rodriguez-Lopez et al., 2020). Thus, blurring an image speeds up how quickly that image is processed by the visual system.
Figure 4B shows the impact of overall light level on the strength of the reverse Pulfrich effect, one panel for each observer. Each data point is the (average) magnitude of the critical onscreen delays in the two defocus conditions at a given light level and pupil size (see
Figure 4A). Larger interocular delays are associated with lower light levels, smaller interocular delays are associated with higher light levels, and the change in interocular delay with light level is approximately linear on a log-log scale. For S1 (
Figure 4B, left panel), the slope of the linear regression in the log-log space reflects the power of the power function, which is −0.08 ms/td (68% confidence interval = [−0.09, −0.04], which is essentially equivalent to the standard error of the reported statistic) for natural, 4 mm and 6 mm pupil sizes and −0.01 ms/td (68% confidence interval = [−0.05, 0.01]) for 2 mm pupil size. For S2 (
Figure 4B, middle panel), the slopes are −0.06 ms/td (68% confidence interval = [−0.09, −0.04]) for natural, 4 mm and 6 mm pupil sizes and −0.06 ms/td (68% confidence interval = [−0.09, −0.03]) for 2 mm pupil size. For S3 (
Figure 4B, right panel), the slopes are −0.07 ms/td (68% confidence interval = [−0.21 0.15]) for natural pupil and −0.03 ms/td (68% confidence interval = [−0.07, −0.002]) for 2 mm pupil size.
Note that the interocular delays associated with fixed 2 mm pupils are quite a bit smaller than the interocular delays associated with larger pupil sizes. This is to be expected. A given focus error (e.g., 3.0 D) produces less retinal blur when pupil sizes are small (
Equation 4), so the difference in retinal blur between the eyes and, hence, the interocular delay is expected to be smaller.
In fact, theoretical predictions based on geometric optics (
Equation 4) and previous empirical results showing a linear relationship between defocus blur and delay (
Burge et al., 2019;
Rodriguez-Lopez et al., 2020), both predict that delays in the 2 mm pupil-size conditions should be 0.5× the delays in the 4 mm pupil-size conditions. This is precisely what we observe: The prediction (
Figure 4B, lower dashed line) aligns with the 2 mm data (
Figure 4B, symbols). However, it is a bit surprising that there are no clear differences among interocular delays associated with the 4 mm pupils, 6 mm pupils, and natural pupil sizes which ranged from 4 mm to 6 mm. By the same reasoning as above, the delays in 6 mm pupil size conditions should be 1.5× the delay in the 4 mm pupil-size conditions. However, we did not observe this: The prediction (
Figure 4B, upper dashed lines) does not align with the data (
Figure 4B, symbols). We speculate that this pattern in the data can be accounted for by the presence of higher-order aberrations in the human eye. We discuss this possibility in the Discussion section below.
In the classic Pulfrich experiment, for each overall light level, there were again two conditions. In one condition, the left-eye image was dimmer and received only 25% of the light that the right eye did (ΔO = −0.6 OD). In the other condition, the right-eye image was dimmer than the left eye (ΔO = 0.6 OD). Six adjustment runs were completed for each condition. (Note that an optical density of 0.6 corresponds to a 25% transmittance, which is equivalent to a 75% light loss).
Figure 5A shows all 12 adjustment runs (6 runs × 2 conditions) from one observer at another overall light level and pupil size (3.2 cd/m
2 and 6 mm). This data is representative of the raw data in other conditions. At this light level, when the left eye was dark (ΔO = −0.6 OD) the critical onscreen delay was 12.6 ± 1.0 ms, indicating that the dark left-eye image had to be advanced onscreen to counteract the fact that it was neurally delayed. When the right eye was dark (ΔO = 0.6 OD), the critical onscreen delay was −12.4 ± 0.9 ms, indicating that the left-eye image had to be delayed onscreen to compensate for the fact that the dark right-eye image was neurally delayed (
Figure 5A). Unlike in the previous experiment in which the manipulated (blurrier) image was neurally processed more quickly, in this experiment the image in the manipulated (dimmer) eye was neurally processed more slowly.
Figure 5B shows the impact of overall light level on the strength of the classic Pulfrich effect, with one panel for each observer. Clearly, larger interocular delays are associated with lower light levels, and smaller interocular delays are associated with higher light levels. For S1 (
Figure 5B, left panel), the slope of the linear regression in the log-log space reflects the power of the power function, which is −0.14 ms/td (68% confidence interval = [−0.16, −0.11]) for all pupil sizes. For S2 (
Figure 5B, middle panel) the slope is −0.10 ms/td (68% confidence interval = [−0.15, −0.04]) for all pupil sizes. For S3 (
Figure 5B, right subplot) the slope is −0.10 ms/td (68% confidence interval = [−0.13, −0.08]). These results replicate findings reported by
Lit (1949) and
Prestrude (1971) (see
Supplementary Figure S2). Similarly, for S1, the y-intercept of the linear regression in the log-log space is 19.24 ms (68% confidence interval = [17.85, 20.62]). For S2, the y-intercept is 16.3 ms (68% confidence interval = [12.4, 20.06]). For S3, the y-intercept is 52.3 ms (68% confidence interval = [50.13, 56.7]).
Overall light level has a similar impact on the strengths of the reverse and classic Pulfrich effect (see
Figures 4 and
5). The most evident difference between the two experiments is that pupil size does not affect the classic Pulfrich effect, whereas it has a systematic effect on the reverse Pulfrich effect. These issues are discussed below.