Abstract

Sand flux is the key factor to determine the migration of sand dunes and the erosion to the surrounding environment. There are crescent-shaped sand dunes of various scales in the desert, and there are significant differences in spatial wind field and sand flux among them. However, due to the difficulty of monitoring, it is difficult to continuously observe the spatial wind field and sand flux around the larger crescentic dunes. On the basis of the Reynolds-Average Navier–Stokes (RA-NS) equation and the stress and sand flux model, the distribution of wind field and sand flux of a circular dune with a height of 4.2 m and a length of about 100 m during the four evolutionary periods of the evolution into a crescentic dune was simulated in this study. By comparing with the measured results, we verified that the closer to the leeward side, the more the simulated values of the velocity in wind field and sand flux were in line with the measured results. In order to further analyze the influence of the height of dune and other relevant parameters on sand flux, we simulated the influence on wind field and sand flux by changing the air viscosity and wind velocity of upper boundary. We found that the air viscosity mainly affected the amount of deposited sand on the leeward side of sand dune, while the increase of wind velocity would undoubtedly increase the sand flux of the whole sand dune. In addition, the simulation results also showed that the influence of changes in height of dune on the turbulent intensity of leeward side was very significant, and the turbulent intensity increased with the height of dune. The height changes of tall dunes gradually affected the transport of sand caused by wind flow behind the leeward side because that the rotation of the wind flow would form new vortexes at the large pores behind the leeward side, which would increase the turbulent energy in space and thus would increase the distance of migration of the lifting sand. While the low sand dunes could not form extra small vortexes at the bottom of the leeward side, so the wind velocity was small and the eddy currents behind the leeward side were more stable. The simulation results indicated that wind velocity was not the only reason for increasing the amount of sand flux, and the fluctuation of wind flow caused by turbulence could also stimulate the movement of sand particles on the ground.

Highlights

  • Larger-scaled observations of crescentic dunes greatly increase the work load of field monitoring

  • Three problems were analyzed by numerical simulation in this study: (1) Changes of wind field and sand flux around the sand dune during evolution; (2) Influence of different heights of sand dune and turbulences behind the leeward side on sand flux; (3) Variation in the amount of sand flux caused by the height of dune and wind velocity of boundary

  • It could be seen that under the combined action of uneven spatial wind velocity and air viscous ­force[5], a large number of irregular turbulence appeared behind the leeward side of sand dune, which was close to the result of ­Zhang[51]

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Summary

Introduction

Larger-scaled observations of crescentic dunes greatly increase the work load of field monitoring. Althoughmany scholars have used more convenient methods and means to carry out researches on migration and deposition of sand dunes, such as wind tunnel e­ xperiments[17,18,19,20], remote sensing ­survey[21,22,23] and so on, it is still difficult to continuously show the variation of wind field and sand flux at different positions and heights of sand dunes of different scale, and it is difficult to give the detailed structure of wind flow field and the distribution of shear stress in continuous space To compensate for this defect, many scholars began to use numerical simulation to analyze the changes of wind flow field in sand ­dunes[13,24,25,26,27,28]. The results of this study could provide a theoretical reference for the researches on surface erosion and migration of crescentic sand dunes of different scale

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