Show that the energy spectrum ( E(\kappa) \sim \varepsilon^2/3 \kappa^-5/3 ) in the inertial subrange.
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6.1
The allure of the solution manual is obvious: Turbulence is hard. The subject involves statistical tools, correlation tensors, and the infamous "closure problem." When stuck on a derivation involving the Kolmogorov microscales or the energy cascade, seeing the solution provides a lifeline. Show that the energy spectrum ( E(\kappa) \sim
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