Identification of the energy contributions associated with wall-attached eddies and very-large-scale motions in the near-neutral atmospheric surface layer through wind LiDAR measurements
Matteo Puccioni, Marc Calaf, Eric R. Pardyjak, Sebastian Hoch, and Travis J. Morrison, Alexei Perelet, Giacomo Valerio Iungo

TL;DR
This study uses wind LiDAR measurements to distinguish energy contributions of wall-attached eddies and VLSMs in the near-neutral atmospheric surface layer, revealing limitations of spectral analysis and estimating eddy characteristics at high Reynolds numbers.
Contribution
It introduces an analytical model for wall-attached eddy coherence spectra and compares spectral and coherence methods for eddy characterization in high Reynolds number flows.
Findings
Spectral analysis underestimates the extent and height of wall-attached eddies due to VLSM overlap.
LCS analysis effectively estimates wall-attached eddy height and extent.
Townsend-Perry constant is reliably estimated through spectral analysis.
Abstract
Recent works on wall-bounded flows have corroborated the coexistence of wall-attached eddies, whose statistical features are predicted through Townsend's attached eddy hypothesis (AEH), and very-large-scale motions (VLSMs), which are not encompassed in the AEH. Furthermore, it has been shown that the presence of wall-attached eddies within the logarithmic layer is linked to the appearance of an inverse-power-law region in the streamwise velocity energy spectra, upon significant separation between outer and viscous scales. In this work, a near-neutral atmospheric surface layer (ASL) is probed with a wind LiDAR to investigate the contributions to the streamwise velocity energy associated with wall-attached and VLSMs for a very-high Reynolds-number boundary layer. Energy and linear coherence spectra (LCS) of the streamwise velocity are interrogated to identify the spectral boundaries…
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Taxonomy
TopicsWind and Air Flow Studies · Fluid Dynamics and Turbulent Flows · Aerodynamics and Fluid Dynamics Research
