  We collate active galactic nuclei (AGN) with reported detections of both
relativistic reflection and ultra-fast outflows. By comparing the inclination
of the inner disc from reflection with the line-of-sight velocity of the
outflow, we show that it is possible to meaningfully constrain the geometry of
the absorbing material. We find a clear relation between the velocity and
inclination, and demonstrate that it can potentially be explained either by
simple wind geometries or by absorption from the disc surface. Due to
systematic errors and a shortage of high- quality simultaneous measurements our
conclusions are tentative, but this study represents a proof-of-concept that
has great potential.
