The statistical objects characterizing turbulence in real turbulent flows d
iffer from those of the ideal homogeneous isotropic model. They contain con
tributions from various two- and three-dimensional aspects, and from the su
perposition of inhomogeneous and anisotropic contributions. We employ the r
ecently introduced decomposition of statistical tensor objects into irreduc
ible representations of the SO(3) symmetry group (characterized by j and m
indices, where j = 0... infinity, -j less than or equal to m less than or e
qual to j) to disentangle some of these contributions, separating the unive
rsal and the asymptotic from the specific aspects of the how. The different
j contributions transform differently under rotations, and so form a compl
ete basis in which to represent the tensor objects under study. The experim
ental data are recorded with hot-wire probes placed at various heights in t
he atmospheric surface layer. Time series data from single probes and from
pairs of probes are analyzed to compute the amplitudes and exponents of dif
ferent contributions to the second order statistical objects characterized
by j = 0, 1, and 2. The analysis shows the need to make a careful distincti
on between long-lived quasi-two-dimensional turbulent motions (close to the
ground) and relatively short-lived three-dimensional motions. We demonstra
te that the leading scaling exponents in the three leading sectors (j = 0,
1, and 2) appear to be different but universal, independent of the position
s of the probe, the tensorial component considered, and the large scale pro
perties. The measured values of the scaling exponent are xi 2((j = 0)) = 0.
68+/-0.01, xi(2)((j = 1)) = 1.0 +/-0.15, and xi(2)((j = 2)) = 1.38+/-0.10.
We present theoretical arguments for the values of these exponents using th
e Clebsch representation of the Euler equations; neglecting anomalous corre
ctions, the values obtained are 2/3, 1, and 4/3, respectively. Some enigmas
and questions for the future are sketched. PACS number(s): 47.27.Gs, 47.27
.Jv, 05.40.-a.