  We produce radiation hydrodynamics models of an AGN 'torus' plus outflow on
1-100 pc scales. This large scale permits direct comparison with observations,
provides justification for configurations used in radiation transfer models,
and tests the sensitivity of results of smaller scale dynamical models. We find
that anisotropic radiation from an AGN accretion disk can cause an outflow to
evolve to become more polar, agreeing with the ubiquity of polar extended
mid-IR emission, and the general geometry predicted by radiative transfer
models. We also find the velocity maps can reproduce many features of
observations, including apparent 'counter-rotation'.
