Scaling Exponents of Turbulent Static Pressure Structure Function in the Inertial Subrange
The measured variations in the turbulent static pressure structure function (Formula presented.) with scale (Formula presented.) in the roughness sublayer above a subarctic forest are empirically shown to exhibit exponents that are smaller than (Formula presented.) predicted for the inertial subrange (ISR). Three hypotheses are offered to explain these deviations. The first is based on conventional intermittency correction to the averaged turbulent kinetic energy dissipation rate, the second is based on shearing introducing deviations from locally isotropic state that must be sensed by both velocity and pressure structure functions, and the third is based on large and inertial scale pressure interactions that persist at values of (Formula presented.) within the resolvable ISR. The third hypothesis is shown to yield superior results, which allows a new formulation for (Formula presented.) to be derived that accommodates such finite interactions.
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Published In
DOI
EISSN
ISSN
Publication Date
Volume
Issue
Related Subject Headings
- Meteorology & Atmospheric Sciences