  Signs of turbulence have been observed at the relativistic heavy ion
collision at high collision energies. We study the signatures of turbulence in
this system and find that there are significant departures from isotropic
turbulence in the initial stages of the collision. Since the anisotropic
fluctuations are sub leading to the isotropic fluctuations, the Kolmogorov
spectrum can usually be obtained even for the initial stages. However, the
energy spectrum and the temperature fluctuations indicate deviations from
isotropic turbulence. Since a strong momentum anisotropy exists between the
transverse and the longitudinal plane, we study the energy density spectrum in
these two planes. The geometrical anisotropy is reflected in the anisotropic
turbulence generated in the rotating plasma and we find that the scaling
exponent is different in the two planes. We find that the scaling exponents in
the longitudinal plane are independent of centrality while the scaling exponent
in the transverse plane depends on the centrality range. We also obtain the
temperature spectrum in the initial stages. The spectrum deviates from the
Gaussian spectra expected for an isotropic turbulence. All these seem to
indicate that the large scale momentum anisotropy persists in the smaller
length scales for the relativistic heavy ion collisions.
