A. J. Ahumada, Jr., Bettina L. Beard
NASA Ames Research Center
Moffett Field, CA, USA
Robert Eriksson
Optics Research Institute
Stockholm, Sweden
Abstract
Ahumada & Beard (Perception 26, ECVP Suppl., 34) calibrated an image sequence discrimination model to masking conditions where the target and masker were the same spatially. Masking was based on local contrast energy so that compound grating masking is greater than that of either component alone, and masking is nearly independent of mask frequency.
Detection thresholds were measured for a 12 msec target in the presence of a 700 msec mask. Targets were 1, 3 or 9 c/deg sine wave gratings. Masks were one grating or two gratings combined in peaks-subtract phase. The target was presented in 17 temporal positions, before, during and after the mask. Peak masking was found near mask onset and offset for 1 and 3 c/deg targets, while masking was more uniform during the mask for the 9 c/deg target. In general, combination maskers were not significantly more effective than the more effective single component mask. Also there was much less masking when the mask frequency differed from that of the target.
By altering the model so that much of the masking is caused by a point nonlinearity rather than local contrast energy, the model can predict the results without the complexity of spatial frequency channels.
This image sequence discrimination model features different masking rules in its sustained and transient systems.
The model differs from that in Ahumada, Beard, and Eriksson (1998 SPIE/IS&T) only in that the combination rule for the transient and sustained systems is additive in difference contrast energy.
Here we compare predictions of this model for grating masking experiments where the test spatial frequency can be the same or different from that of the mask.
Test stimulus:
Sinusoidal grating
Duration: 12 msec (single frame)
Spatial frequency: 1, 3, or 9 c/deg
Sine phase
Circular window diameter: 5 deg
Mask stimulus:
Single or compound grating
Component contrast amplitude: 15%
Duration: 700 msec
Abrupt onset and offset
Spatial frequency: 1, 3, or 9 c/deg
Sine phase
Circular window diameter: 5 deg
Mean luminance: 4.2 cd/m2
16 SOA values: -300 to 1200 msec
3 observers (only BLB data shown)
2IFC staircase
The following graphs show the measured thresholds and the model predictions using the following model parameters.
spatial blur spreads, arc min cone, 1.7 horizontal, 8.5 magno, 4.8 magno masking energy, 25.
integration times, msec cone, 4.8 horizontal, 32. parvo, 27. magno masking energy, 27.
masking thresholds, % contrast parvo masking, 8. magno masking, 0.8
contrast energy thresholds, deg^2 sec parvo, 0.008 magno, 0.0007
Conclusions
Model can predict masking by different frequencies without cortical filters.
Model cannot predict masking which could be duration discrimination.
Foley's result that masking orientation bandwidth is narrower for 500 msec targets than for 100 msec targets is predicted from increased spatio-temporal masking spread in the transient system.
Perceived brightness is spatially integrated at a transient system scale and then applied to sustained system spatial details. The same may be true of perceived contrast.