  Many studies have considered the roles of clouds, outflows, and turbulence in
producing the broad emission and absorption lines in the spectra of active
galactic nuclei (AGNs). However, these are often treated as separate or even
competing models. Here, we consider the possibility that AGN clouds are
condensations formed within the thermally unstable zones of outflows and then
compare the typical sizes of such condensations with the injection scale
$k_0^{-1} \sim L_0$ of turbulence, where $L_0$ is assumed to be the scale
height of a representative global outflow model. We find that for broad line
region (BLR) parameters, clouds are many orders of magnitude smaller than $L_0$
and this has the following implication: BLR cloud dynamics can be modeled using
a local approximation through the use of multiphase turbulence simulations of
X-ray irradiated plasmas. We present the first such 3D local clumpy turbulent
outflow simulations. We show that the condensations share the same type of
selection effects characterizing the locally optimally emitting cloud (LOC)
scenario, thereby offering a physical interpretation for the LOC model and
accounting for its almost uncanny successes. The ubiquitous presence of
emission line regions in AGNs can be simply explained as the natural outcome of
there being a multiphase interval of $k$-space within the inertial range of a
turbulent cascade.
