  abridged: We use XSCORT, together with the hydrodynamic accretion disc wind
simulation from Proga & Kallman (2004), to calculate the impact that the
accretion disk wind has on the X-ray spectrum from a 1E8 solar mass black hole
Active Galactic Nuclei (AGN) accreting at 0.5 L/L_Edd. The properties of the
resulting spectra depend on viewing angle and clearly reflect the distinct
regions apparent in the original hydrodynamic simulation. Very equatorial
lines-of-sight (l.o.s) are dominated by Compton scattering and nearly-neutral
absorption. Polar l.o.s result in largely featureless spectra. Finally, l.o.s
that intersect the transition region between these extremes have a wide range
of absorption features imprinted on the spectrum. Both polar and transition
region l.o.s produce spectra that show highly-ionized, blue-shifted, Fe
absorption features that are qualitatively similar to features observed in the
X-ray spectra of a growing number of AGN. The spectra presented here clearly
demonstrate that current simulations of line driven AGN accretion disk winds
cannot reproduce the smooth soft X-ray excess. Furthermore, they predict that
high accretion rate (L/L_Edd) AGN are likely to be strongly affected by
obscuration, in sharp contrast to the clean picture that is generally assumed,
based on the observed relation between the opening angle of the molecular torus
and AGN luminosity.
