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We investigate the emission of active galactic nucleus (AGN) dusty tori in infrared domain.
Following theoretical predictions derived from hydrodynamical simulations, we model the dusty torus as a 3D two-phase medium with high-density clumps and low-density medium filling the space between the clumps.
Spectral energy distributions (SEDs) and images of the torus at different wavelengths are obtained using the 3D Monte Carlo radiative transfer code .
Our approach of generating clumpy structure allows us to model the tori with single clumps, complex structures of merged clumps or interconnected sponge-like structure.
A corresponding set of clumps-only models and models with smooth dust distribution is calculated for comparison.