  (abridged) We present a semianalytic model of steady-state magnetically and
radiatively driven disk outflows in Active Galactic Nuclei (AGNs) consisting of
a continuous wind with embedded clouds. The continuous outflow is launched from
the disk surface as a centrifugally driven wind, whereas the clouds are
uplifted from the disk by the ram pressure of the continuous outflow. In
addition, the continuous wind and clouds are subject to both line and continuum
radiative acceleration. We describe this model in detail, outline the tests
used to verify its accuracy, and compare it to other outflow models, showing
possible difficulties with some past line-driven models. We then perform a
comprehensive parameter study to explore the dependence of the continuous wind
on the relevant physical parameters. We find that clouds have a significant
impact on the geometry, density, and velocity in the continuous wind, changing
the terminal velocity by up to 50%. Furthermore, line driving is the dominant
acceleration mechanism for clouds; continuum driving can also become important
for dusty clouds. We find that radiative acceleration can have a significant
impact on the velocities in the continuous wind and note that the radiative
acceleration comes largely from continuum opacities, not from line driving as
in some previous models. When the continuous winds are dusty, their terminal
velocities change by approximately 20% to 30% (depending on the type of dust).
