Illuminants. The four columns in this figure correspond to the four kinds of illuminants: natural (first column), fluorescent (second), random spline (third), and monochromatic (last column). The
x- and
y-axes in the first (panels a through d) and second (panels e through h) rows correspond to wavelength (in nm) and relative spectral power, respectively. Panel a illustrates examples of daylight illuminants, with red, green, and blue curves corresponding to five examples from the Grenada database (Romero et al.,
1997), the Maryland forest illuminants (Chiao et al.,
2000), and the simulated daylight spectra (Judd et al.,
1964), respectively. Panel b shows the 12 illuminants F, where the red curves correspond to the semibroadbent illuminants F1 through F6, the green curves correspond to the broadbent illuminants F7 through F9, and the blue curves correspond to the narrow triband illuminants F10 through F12. Panels c and d illustrate 12 examples of random-spline and monochromatic spectra, respectively. The three curves in the graphs of the second row (panels e through h) show the first three principal components of the illuminants (red = first component, blue = third component). The principal components were calculated for the complete set of each kind of illuminants (i.e., not only for the few examples shown in the first row). The R
2 in the top right corner indicates how much of the variance of the spectra the first three principal components explain. The third row (panels i through l) illustrates the differences between the reflected LMS signal when calculated with the exact formula (black circles) and when approximated based on the respective matrix A (red dots). The format in this row is the same as that in
Figure 1a. As an example, the reflectance of
Figure 3a was used, and the reflected signal for the sample illuminants in the first row of this figure (panels a through d, respectively) are shown here. The R
2 in the top right corner indicates how much of the variance of the reflected signal for this reflectance and the respective set of illuminants is explained by the approximation (the average across all reflectances is given in the text). The last row (panels m through p) illustrates the singularity indices across Munsell chips for the different types of illuminants. The format of the panels in this row is the same as that in
Figure 4c. For comparison, panel m shows again the singularity indices for the natural illuminants as in
Figure 4c. Panels n through p show those for the fluorescent, random-spline, and monochromatic illuminants, respectively. Although the spectra differ strongly across the four sets of illuminants (first row), and although random-spline and monochromatic spectra cannot be represented by three principal components (second row), the linear approximation is extremely accurate for all four types of illuminants (third row), and the patterns of singularities are very similar between these sets of illuminants (fourth row).