  We present 3-dimensional radiative transfer models for clumpy dust tori
around AGN. Our method combines Monte Carlo simulations of individual dust
clouds with the actual 3-dimensional distribution of clouds in the torus. The
model has been applied to NIR and MIR photometric and interferometric
observations of NGC 1068. For the first time, it is possible to simultaneously
reproduce both photometric and interferometric observations in the NIR and MIR.
We infer a luminosity L=2*10^45 erg/s and an inclination of i=70deg for NGC
1068 from our model.
