Spectra in the inertial subrange

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Short definition of Spectra in the inertial subrange
In the inertial subrange, the three-dimensional velocity spectrum follows a power-law behaviour and this makes it possible to easily derive the one-dimensional spectra, in this range

This is the common definition for Spectra in the inertial subrange, but other definitions maybe discussed within the wiki.

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In the inertial subrange, the three-dimensional velocity spectrum follows a power-law behaviour and this makes it possible to easily derive the one-dimensional spectra, in this range. Using ( ?) within the inertial subrange gives

F~11(κ^1)=κ^1F(κ^)κ^(1κ^12κ^2)dκ^=1855Cκ^15/3=C1κ^15/3

where C1=18C/5527/55 is frequently called the one-dimensional Kolmogorov constant, and the tilde is used to indicate these equations apply only in the inertial subrange. It is not possible to measure the three-dimensional spectrum and, thus, it is not possible to estimate C directly. Consequently, there is research interest in estimating </math>C_1</math> because it is the only practical way to determine the three-dimensional Kolmogorov constant C. Sreenivasa (1995)[1] compiled the values of the one-dimensional Kolmogorov constant reported from a wide range of measurements in the atmosphere, ocean, wind tunnels and pipes. The mean value (excluding low Reynolds number measurements) is 0.53 and the standard deviation is 0.055 (Figure 1). A crude estimate of the 95% confidence interval is C1=0.53±0.03.

Figure 1. Figure 3 from Sreenivasa (1995)[1] for the estimates of the one-dimensional Kolmogorov constant, C1, derived from experimental measurements of along-stream velocity measurements and/or the rate of strain.

Using F~22=43F~11, the one-dimensional spectrum for the velocity components that are orthogonal to the direction of profiling is

F~22(κ^1)=43C1κ^15/3

The gradient spectra in the inertial subrange are

Failed to parse (unknown function "\begin{equation}"): {\displaystyle \begin{equation} \tilde{G}_{11} (\hat{\kappa}_1) = C_1 \hat{\kappa}_1^{1/3} \end{equation} }

and

Failed to parse (unknown function "\begin{equation}"): {\displaystyle \begin{equation} \tilde{G}_{22} (\hat{\kappa}_1) = \frac{4}{3} C_1 \hat{\kappa}_1^{1/3} \end{equation} }

You want more? Go to Spectral integration

  1. 1.0 1.1 Sreenivasan, K. R. (1995). On the universality of the Kolmogorov constant. Physics of Fluids, 7(11), 2778-2784.