Neural systems show fluctuating responses to repeated presentations of the same visual stimulus (
Tolhurst & Dean, 1983), while the variance is level dependent (
Roufs, 1974). To account for level dependency with a simplified assumption, we used Crozier’s law (
Crozier, 1936), which claims constancy of the ratio of standard deviation to the mean,
\(c_v\), known as variation coefficient. Constrained by linearity assumptions in the vicinity of detection thresholds,
Roufs (1974) showed that constancy of the variation coefficient implies detector operation at a constant signal-to-noise ratio for Gaussian noise. Assuming
\begin{equation}
\frac{\sigma }{\mu }=c_v=const,
\end{equation}
we set
\(\sigma _j=c_v \mu \left[\hat{E}_{j,R}\right]\), with
\(\mu \left[\hat{E}_{j,R}\right]\) the space-average energy of the
\(j\)-th FRF chain for a reference texture (see
Appendix B for the definition of
\(\hat{E}\)). Here,
\(j\) is a running index for (
\({f,\phi }\)) combinations,
\(j \in [n]\),
\([n]=\lbrace 1,\dots ,n\rbrace\),
\(n\) the number of mechanisms. The value of
\(c_v\) was chosen such that the distribution function of the noise had a slope parameter of
\(\beta =3\) if the Weibull function was used as an approximation to a Normal distribution. Setting
\(\beta =3\) results in a variation coefficient of
\(c_v=0.384\) (see
Equation 33 in
Appendix C). A value of
\(\beta =3\) is a good overall estimate for the slope parameter of psychometric curves in many psychophysical tasks (
Robson & Graham, 1981;
Watson, 1982;
Graham, 1989;
Wallis et al., 2013;
Kingdom et al., 2015). To mimic spatial noise, we added a sample
\(\xi _j(x,y)\) from a Normal distribution
\(N(0,c_v \mu _j)\) to each point of the local energy distributions for target and reference stimuli of the
\(j\)-th FRF chain. To control noise strength while maintaining a constant variation coefficient, each sample was multiplied by a spatial noise factor,
\(n_x\). The resulting energy distributions,
\begin{equation}
\tilde{E}_{j}(x,y)=\hat{E}_{j}(x,y)+n_x \xi _j(x,y),
\end{equation}
have two independent sources of random variation, one stemming from the local energy response to a spatial random signal (see subsection “Stimuli” in Method section) and the other from external Gaussian noise.
5 Since in target intervals, local energy is increased in a given spatial region while the background is generated with the same rule as for nontarget intervals (see example pictures in
Figure 12), a classical signal-to-noise ratio detector (
Green & Swets, 1966/1988) would measure the separation of energy means in units of spatial energy variation in the reference (nontarget) distribution:
\begin{equation}
z_j=\frac{\mu \left[\tilde{E}_{j,T}\right]-\mu \left[\tilde{E}_{j,R}\right]}{\sqrt{\text{VAR}\left(\hat{E}_{j,R}(x,y)\right)+n_x^2 \text{VAR}\left(\xi _j(x,y)\right)}}.
\end{equation}
The
\(z_j\) score can be considered a
\(d^{\prime }\) measure, signal-to-noise ratio, calculated by a contrast energy detector operating on the spatial energy distributions of the
\(j\)-th FRF chain. Now, since
\(\mu [\xi _j]=0\) for all
\(j \in [n]\), the numerator of (
10) reduces to the mean difference of energies, that is,
\(\mu \left[\tilde{E}_{j,T}\right]-\mu \left[\tilde{E}_{j,R}\right]=\mu \left[\hat{E}_{j,T}\right]-\mu \left[\hat{E}_{j,R}\right]\). This means that
\begin{equation}
z_j=\frac{CE_{j,T}-CE_{j,R}}{\sqrt{\text{VAR}\left(\hat{E}_{j,R}(x,y)\right)+n_x^2 \text{VAR}\left(\xi _j(x,y)\right)}}
\end{equation}
measures the signal-to-noise ratio of net contrast energy,
\(\Delta CE\), from the
\(j\)-th FRF chain.