  We present a self-consistent, semi-analytical dynamical model of disk driven
outflows in AGNs that are accelerated by a combination of magnetic stresses and
radiation pressure. This model will make it possible to examine scenarios in
which the wind is homogeneous as well as cases where it consists of dense
clouds embedded in a more tenuous, magnetized medium. The various ingredients
of this model will be tested through quantitative predictions from both
multiwavelength spectral observations and reverberation mapping of AGNs.
