We present SCIDAR measurements made at the Pic du Midi Observatory with PIS
CO. A series of vertical profiles of the refractive-index structure constan
t C-N(2)(h) was obtained with the observations of the binary stars gamma an
d gamma Ari, with 30 second time sampling. In the free atmosphere, the turb
ulence was dominated by the contribution of a few well-separated atmospheri
c layers at altitudes in the range 8-20 km, with significant changes within
a few minutes. We describe a new method based on the CLEAN algorithm appli
ed on the 2-D covariance function of the irradiance fluctuations in the pup
il plane and compare it with the widely-used Maximum Entropy Method applied
on a slice of this 2-D function. Our method is much less sensitive to the
noise. Vertical profiles of the wind velocity and direction were obtained w
ith an automatic procedure working on the mean cross-correlation function o
f consecutive frames. Furthermore, we validate a model for the SCIDAR detec
tivity threshold in terms of distance to the turbulent layers.