It is widely accepted that, regardless of their very different observational characteristics, Seyfert galaxies of types I and II are made of the same building blocks: a central accretion-driven, radiation-generating engine, and a surrounding dust torus, that processes this radiation and re-emits it in the infrared. I will describe our group's ansatz to model the characteristics of the IR radiation emerging from these dusty, clumpy tori. Special emphasis will be placed on localizing the origin of the IR emission within the torus.