In order to compare chromatic and luminance adaptation effects to each other, both data sets were converted into constancy indices (
Arend, Reeves, Schirillo, & Goldstein, 1991;
Foster, 2011). The constancy index (CI) captures constancy by seeing where on the scale a data point falls, with one extreme being no adaptation and the other extreme total adaptation. If complete adaptation occurs, the constancy index will be 1. If no, or little, adaptation occurs, the constancy index will be close to zero. The current study quantified the constancy index using the following equation:
\begin{eqnarray*}
CI = 1 - \frac{{\rm{baseline}} - {\rm{test}}}{{\rm{baseline}} - {\rm{no}}\, {\rm{adapt}}}
\end{eqnarray*}
where “baseline” refers to the preliminary measure, “test” refers to a given filter measure (t0, t30, or t60), and “no adapt” refers to the filtered prediction if no adaptation occurred. For achromatic settings, the “no adapt” prediction chromaticity used was (u′, v′) = [0.44,0.51], which corresponds to the black “P” drawn on
Figure 3. For HFP, “no adapt” refers to the filtered luminance predictions derived from each individual participant’s baseline setting (data used to calculate the gray lines in
Figures 6A and
6B). For the HFP data, the constancy indices were calculated separately for the two conditions and averaged together.
The CI will be close to zero if the fraction term is close to 1, which would happen if the test value is close to the “no adapt” prediction. A negative constancy index (which occurred sometimes for luminance) implies that participant matches with the filter were more extremely shifted than predictions derived from their baseline measures. The CI will be 1 if there is no difference between the baseline and test.
The results of the constancy index analysis are plotted in
Figure 8. The left graph in
Figure 8 shows the black and right graph the cockpit background, and orange bars represent chromatic and blue bars luminance. A three-way, repeated-measures ANOVA was done with
adaptation type (luminance or chromatic),
background, and
time as factors. There was a significant interaction between
adaptation type and
background (
F(1, 18) = 18.9,
p < 0.001, η
p2 = 0.51), driven by the constancy index being greater for cockpit than black background for chromatic adaptation but not luminance. There was also a significant interaction between
adaptation type and
time (
F(2, 36) = 4.02,
p = 0.027, η
p2 = 0.18), driven by constancy index increasing with time for chromatic adaptation but not luminance. While
time and
background significantly influenced chromatic adaptation, they did not significantly affect luminance adaptation, which hovered around zero (one-sample
t tests for luminance were not significantly different from zero;
p > 0.18 for all tests). Results also showed a significant main effect of
adaptation type with chromatic having greater adaptation than luminance (
F(1, 18) = 245.57,
p < 0.001, η
p2 = 0.91), as well as a significant effect of
background (
F(1, 18) = 17.58,
p < 0.001, η
p2 = 0.49), although this effect was driven by the chromatic adaptation data. The main effect of
time did not reach significance (
F(2, 36) = 2.92,
p = 0.07).