  We present a survey of OVI 1032 emission in the Milky Way using data from the
Far Ultraviolet Spectroscopic Explorer (FUSE) satellite. The observations span
the period from launch in 1999 to July 2003. Our survey contains 112 sight
lines, 23 of which show measurable OVI 1032 emission. The OVI 1032 emission
feature was detected at all latitudes and exhibits intensities of 1900-8600
photons/s/cm^2/sr. Combined with values from the literature, these emission
measurements are consistent with the picture derived from recent OVI absorption
surveys: high-latitude sight lines probe OVI-emitting gas in a clumpy, thick
disk or halo, while low-latitude sight lines sample mixing layers and
interfaces in the thin disk of the Galaxy.
