Barchans are crescent-shaped dunes that form in areas where unidirectional winds predominate and where the availability of sand is insufficient to completely cover the bedrock surface. Barchans can exist in any region where granular or powdered sediments interact with moving fluids, such as air or water. They occur not only in sand deserts, but in environments such as the deep-sea floor, snowfields, and Martian surfaces. Although barchans have been extensively researched, previous studies have examined only the discrete formation of isolated barchans. Here, we present an overview of studies on barchan development focusing on the interaction dynamics of multiple barchans, based on recent research combining flume experiments and quantitative coarse-grained cell modeling. Both the numerical modeling and the flume experiments show three types of collisions between adjacent barchans, depending on the mass ratio and the locations of the dunes.
Coalescence is a type of collision in which two barchans merge to form a single dune.
Ejection represents the formation a new, small barchan from a larger “parent” barchan. A third type, called a
split barchan, represents the division of a single barchan into two smaller dunes. These results contribute to a basic understanding of not only inter-barchan interactions, but the variety of dynamics involved in dune formation; e.g., the formation of barchan corridors and the birth of barchans from transverse dunes. A synergistic research program involving a combination of well-controlled experiments and corresponding mathematical models is critical if dune research is to evolve from a qualitative to a quantitative science.
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