We present a method for simultaneous measurement of the vertical distributi
on of the optical turbulence strength C-N(2)(h) and wind velocity V(h) in t
he Earth's atmosphere, based on an analysis of spatio-temporal based on an
analysis of spatio-temporal correlations of stellar scintillation images ob
tained with generalized scidar. A statistical comparison of V(h) obtained w
ith this method and instrumented balloons supports the use of this method.
The algorithm used allows for the identification of dome seeing, which can
be subtracted from C-N(2)(h), to obtain a turbulence profile free of dome c
ontribution. Examples of simultaneous C-N(2)(h) and V(h) monitorings are pr
esented.