Rivalry alternations produce fluctuations in amplitude and thus SNR.
The real-time detector requires that the VEP amplitude be above the EEG
noise level at least some of the time. We computed average interocular
correlations for three progressively more stringent SNR criteria. The
first criterion included all the data. The second two criteria required
that the average SNR in the eye with the lowest SNR exceed either 2:1
or 3:1, with SNR defined on the basis of amplitudes at the response
frequency, relative to adjacent EEG frequencies that were free of
driven activity. Previous work has indicated that a SNR of 3:1 places
an individual bin reliably above the EEG noise level.
11 Beginning with the most inclusive criterion (all data), the infant
correlations were both significantly positive (0.24 ± 0.05;
P < 0.05 and 0.31 ± 0.06) for the cardinal and
oblique configurations, respectively. The adult values were both
negative (−0.10 ± 0.04;
P < 0.05 and−
0.09 ± 0.05;
P < 0.10) for the corresponding
conditions. The SNR > 2:1 criterion resulted in significantly
positive average correlations for the infants of 0.28 ± 0.06;
P < 0.01 and 0.36 ± 0.06;
P <
0.01 for the cardinal and oblique configurations, respectively.
Comparable values for the adults were both significantly negative
(−0.13 ± 0.05;
P < 0.05 and −0.17 ±
0.07;
P < 0.05). Infant correlations remained
significantly positive for the 3:1 criterion (0.31 ± 0.07;
P < 0.01; 0.47 ± 0.05;
P <
0.01) for the cardinal and oblique configurations, respectively.
Comparable values for the adults were −0.29 ± 0.04
(
P < 0.02) and −0.17 ± 0.12 (
P < 0.20). Nonparametric testing of the distribution of the signs of the
correlations indicated that the adult correlations were significantly
negative in the cardinal condition for the “all data included”
criterion (9/12 negative:
P < 0.05; sign test) and 2:1
SNR criterion (8/9 negative:
P < 0.01). In the oblique
condition, the adult correlations were significantly negative for the
2:1 criterion (9/11 negative:
P < 0.02). All three
adult observers showed negative correlations in the cardinal axis
condition under the 3:1 SNR criterion. However, the sign test is not
applicable with this sample size, so no significance values can be
reported. The other nonparametric comparisons were not significant at
the 0.05 level. Each distribution of infant correlations was
significantly skewed to positive correlations (
P <
0.01) due to the fact that only one interocular correlation was
negative in each of the two cross-oriented conditions. These two
negative correlations occurred at less than the 2:1 criterion and were
small enough to be individually not significantly different from 0.
Therefore, while the adults showed physiological alternations
characteristic of binocular rivalry in the cross-oriented conditions,
infants did not. This led us to ask whether the apparent lack of
binocular rivalry could be attributed to a general immaturity of
binocular interactions under our stimulus conditions.