Detrended Structure-Function in Fully Developed Turbulence
arXiv:1402.0371 · doi:10.1080/14685248.2014.891739
Abstract
The classical structure-function (SF) method in fully developed turbulence or for scaling processes in general is influenced by large-scale energetic structures, known as infrared effect. Therefore, the extracted scaling exponents might be biased due to this effect. In this paper, a detrended structure-function (DSF) method is proposed to extract scaling exponents by constraining the influence of large-scale structures. This is accomplished by removing a st-order polynomial fitting within a window size before calculating the velocity increment. By doing so, the scales larger than , i.e., , are expected to be removed or constrained. The detrending process is equivalent to be a high-pass filter in physical domain. Meanwhile the intermittency nature is retained. We first validate the DSF method by using a synthesized fractional Brownian motion for mono-fractal processes and a lognormal process for multifractal random walk processes. The numerical results show comparable scaling exponents and singularity spectra for the original SFs and DSFs. When applying the DSF to a turbulent velocity obtained from a high Reynolds number wind tunnel experiment with , the 3rd-order DSF demonstrates a clear inertial range with on the range , corresponding to a wavenumber range . This inertial range is consistent with the one predicted by the Fourier power spectrum. The directly measured scaling exponents (resp. singularity spectrum ) agree very well with a lognormal model with an intermittent parameter . Due to large-scale effects, the results provided by the SFs are biased.
11 pages with 5 figures, accepted by Journal of Turbulence
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