Particle-image velocimetry measurements of flow over interacting barchan dunes

• Published in: Experiments in fluids Vol. 52; no. 3; pp. 809 - 829
• Main Authors: Palmer, Jessica A., Mejia-Alvarez, Ricardo, Best, James L., Christensen, Kenneth T.
• Format: Journal Article
• Language: English
• Published: Berlin/Heidelberg Springer-Verlag 01-03-2012; Springer
• Subjects: Computational fluid dynamics; Cosmochemistry. Extraterrestrial geology; Dunes; Earth sciences; Earth, ocean, space; Engineering; Engineering Fluid Dynamics; Engineering Thermodynamics; Exact sciences and technology; Extraterrestrial geology; Fluid flow; Fluid- and Aerodynamics; Heat and Mass Transfer; Marine and continental quaternary; Research Article; Shear layers; Surficial geology; Turbulence; Turbulent flow; Upstream; Velocimetry; Proper Orthogonal Decomposition; Proper Orthogonal Decomposition Mode; Turbulent Kinetic Energy; Shear Layer; Reynolds Shear Stress; experimental studies; particulate matters; models; Mars; shear stress; dunes; wind transport; barchans; contour maps; global; velocity; landform evolution
• ISSN: 0723-4864; 1432-1114
• DOI: 10.1007/s00348-011-1104-4

Barchan dunes are crescentic planform-shaped dunes that are present in many natural environments, and may occur either in isolation or in groups. This study uses high-resolution particle-image velocimetry (PIV) experiments using fixed-bed models to examine the effects of barchan dune interaction upon the flow field structure. The barchan dune models were created from an idealized contour map, the shape and dimensions of which were based upon previous empirical studies of dune morphology. The experimental setup comprised two, co-axially aligned, barchan dune models that were spaced at different distances apart. In this paper, two volumetric ratios (
V
r
, upstream dune: downstream dune) of 1.0 and 0.175 were examined. Models were placed in a boundary-layer wind tunnel and flow quantification was achieved via PIV measurements of the mean and turbulent flow field in the streamwise–wall-normal plane, along the centerline of the barchan(s), at an average flow Reynolds number of 59,000. The presence of an upstream barchan dune induces a “sheltering effect” on the flow. Flow on the stoss side of the downstream dune is controlled by the developing internal boundary layer from the upstream dune, as well as by the turbulent flow structures shed from the free shear layer of the upstream dune leeside. At both volumetric ratios, enhanced turbulence is present over the downstream barchan dune leeside, which is proposed to be caused by the interaction of shear layers from the upstream and downstream dunes. Both the size and magnitude of the shear layer formed in the leeside of the upstream dune control this interaction, together with the proximity of this shear layer to the stoss side of the downstream dune. Proper orthogonal decomposition (POD) analysis shows that the distribution of turbulent kinetic energy is shifted to higher modes (i.e., smaller spatial scales) over interacting barchan dunes, which also reflects the role of the leeside free shear layer in dominating the flow field by generation, or redistribution, of TKE to smaller scales.