Effects of Wind Velocity and Nebkha Geometry on Shadow Dune Formation

• Published in: Journal of geophysical research. Earth surface 2019-11, Vol.124 (11), p.2579-2601
• Main Authors: Zhao, Yongcheng, Gao, Xin, Lei, Jiaqiang, Li, Shengyu, Cai, Dongxu, Song, Qin
• Format: Article
• Language: English
• Subjects: Aspect ratio; Computational fluid dynamics; computational modeling; Computer applications; Computer simulation; Dune formation; Dunes; Elongated structure; Elongation; Experiments; Fluid dynamics; Height; Hydrodynamics; Lakes; Local winds; nebkha; Playas; Radar; Sand; Sand transport; sedimentary structure; Sedimentary structures; shadow dune; Shadows; Simulation; Surveys; Velocity; Width; Wind effects; Wind regime; Wind shear; Wind speed; wind tunnel simulation; Wind tunnel testing; Wind tunnels
• ISSN: 2169-9003; 2169-9011
• DOI: 10.1029/2019JF005199

Flow dynamics and sand deposition processes over nebkhas were investigated using computational fluid dynamics simulations, wind tunnel experiments, and field measurements. The computational fluid dynamics simulations showed that nebkha width affects both the elongation and broadening of the wind shadows. The length of the wind shadows decreased as the wind shear velocity increased, following a power function, irrespective of the width and height of the nebkha. There are some uncertainties about the effect of the aspect ratio of the nebkha on the formation of wind shadows as a result of the omission of the transport of sand in the simulations. It is suggested that the length of wind shadows is dependent on the absolute values of nebkha width and height rather than the nebkha aspect ratio. Although the numerical results were consistent with the results of the wind tunnel experiments, the wind tunnel experiments showed that the height of the nebkha had a negative effect on the elongation of the shadow dunes. The sedimentary structures revealed by ground‐penetrating radar surveys of the dunes in the Taitema Dry Lake, in the eastern Taklimakan Desert, China, showed that the formation of shadow dunes can be divided into three phases. Shadow dunes are initially controlled by horizontal separation flow and then elongate following the same growth mechanisms as linear dunes, eventually breaking up into isolated barchans or short, temporary linear dunes. However, the formation of shadow dunes does not necessarily call for the three phases depending on the local wind regime and sediment supply. Key Points Shadow dune length increases with nebkha width for low incident wind velocities and decreases with nebkha height Shadow dune length decreases with wind velocity following a power function Formation of shadow dunes is dominantly dependent on the absolute values of nebkha width and height rather than the nebkha aspect ratio