  We report the detection with FUSE of strong, highly blue-shifted absorption
features appearing in the absorption troughs of practically all major P Cygni
profiles in the presumably single Wolf-Rayet star WR135. These features also
appear in the shock-sensitive OVI 1032/38 \AA doublet, coincident both in time
and velocity space with the rest of the lower-ionization species. Choosing
between two alternative interpretations: large-scale, coherent structures vs.
localized, random shocks, we favor the latter. The absolute value of velocity,
as well as velocity dispersion in the shocked region, the density of the
shocked gas, and the time scales of the observed variability allow us to relate
the observed shocks to the incidence of numerous over-dense clumps (blobs) in
the wind of a hot, massive star.
