A combined wind tunnel and computational study of grid-generated turbulence
along the centreline shows that the close to −5/3 power law signature of energy
spectra in the frequency domain originates relatively close to the grid not only where
the velocity derivative statistics become quite suddenly isotropic but also where
the turbulent fluctuating velocities are very intermittent and non-Gaussian. As the
inlet flow velocity increases, these power laws are increasingly well defined and
increasingly close to −5/3 over an increasing range of frequencies. However, this
range continuously decreases with streamwise distance from the grid even though the
local Reynolds number first increases and then decreases along the same streamwise
extent. The intermittency at the point of origin of the close to −5/3 power spectra
consists of alternations between intense vortex tube clusters with shallow broad-band
spectra and quiescent regions where the velocity fluctuations are smooth with steep
energy spectra
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