Up to now only a few numerical or experimental simulations of atmosphe
ric turbulent layers have been performed in the laboratory. These are
devoted mainly to show the validity of Kolmogorov behavior but are not
suitable to implement in an optical bench to test light propagation.
Here we present a small size experimental simulation of an optical tur
bulent layer. With optical and in situ measurements, we managed to det
ermine its characteristics: the mean variance of the refractive-index
fluctuations integrated over the thickness of the turbulent flow and l
ongitudinal and transverse structure functions of angles of arrival. F
rom these measurements we found that the power spectrum of the refract
ive index is well fitted by a Von Karman function with an outer scale
of 91 mm and an inner scale of 4.7 mm. Moreover, the temporal stationa
rity of these parameters indicates the reproducibility of this simulat
ed turbulent flow. (C) 1996 Optical Society of America