This paper presents results about atmospheric turbulence in the form o
f power spectral density of the w-wind component. Such results are rar
ely presented in the international literature because of the difficult
y that these systems have in order to derive atmospheric turbulence pa
rameters, as explained in the text. The data for the analysis was gath
ered during CLEOPATRA experimental campaign around Munich area in the
period May-July 1992. The power spectral densities derived seem to fol
low the-5/3 law.