Figure 6From: Analysis of colour constancy algorithms using the knowledge of variation of correlated colour temperature of daylight with solar elevation Typical feature space formed by the model-based algorithm when illuminating a pair of Munsell samples (Munsell samples: 2.5R 9/2 and 5Y 7/1) by daylight spectra measured between 5.00 and 20.00 GMT (daylight set 1). A Mahalanobis distance boundary is drawn for each Munsell sample (shown in thick solid black line). A cross and a small circle show the feature obtained using model-based algorithm by illuminating the Munsell samples: 2.5R 9/2 and 5Y 7/1 illuminated by one of the CIE standard illuminant, respectively.Back to article page