Figure 1: A rendering of the Wolf scene under environment lighting using (left) our physically-based double cylinder fur reflectance model with parameters from our database of animal fur samples, and (right) energy conserving Marschner model [Marschner et al. 2003; d'Eon et al. 2011] with best-fit parameters. Insets showing detailed comparisons from top to bottom using our model, Marschner model and Kajiya-Kay model. Since the Marschner model consists of only specular lobes, it often produces dark regions (limbs and tail). Furthermore, since the T T lobe is extremely strong in the Marschner model, especially for light colored fur fibers, it completely fails in heterogeneous regions (head) where dark colored fur is covered by light colored fur. The Kajiya-Kay model produces empirically plausible but hard-and-solid appearance, and it doesn't fit the measured reflectance data in Sec. 6.