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Barchans are isolated mobile dunes often organized in large dune fields. Dune fields seem to present a characteristic dune size and spacing, which suggests a cooperative behavior based on dune interaction. In Duran et al. (2009), we propose…

软凝聚态物质 · 物理学 2011-05-20 Orencio Durán , Veit Schwämmle , Pedro G. Lind , Hans J. Herrmann

Barchans are crescentic dunes propagating on a solid ground. They form dune fields in the shape of elongated corridors in which the size and spacing between dunes are rather well selected. We show that even very realistic models for…

凝聚态物理 · 物理学 2009-11-10 P. Hersen , K. H. Andersen , H. Elbelrhiti , B. Andreotti , P. Claudin , S. Douady

In nature, barchan dunes typically exist as members of larger fields that display striking, enigmatic structures that cannot be readily explained by examining the dynamics at the scale of single dunes, or by appealing to patterns in…

软凝聚态物质 · 物理学 2013-07-15 S. Worman , A. B. Murray , R. Littlewood , B. Andreotti , P. Claudin

The collision processes of two crescentic dunes called barchans are systematically studied using a simple computer simulation model. The simulated processes, coalescence, ejection and reorganization, qualitatively correspond to those…

软凝聚态物质 · 物理学 2009-11-10 Atsunari Katsuki , Hiraku Nishimori , Noritaka Endo , Keisuke Taniguchi

Barchan dunes emerge as a collective phenomena involving the generation of thousands of them in so called barchan dune fields. By measuring the size and position of dunes in Moroccan barchan dune fields, we find that these dunes tend to…

软凝聚态物质 · 物理学 2011-03-29 Orencio Durán , Veit Schwämmle , Pedro G. Lind , Hans J. Herrmann

Barchan dunes, or simply barchans, are crescent-shaped dunes found in diverse environments such as the bottom of rivers, Earth's deserts and the surface of Mars. In a recent paper [Phys. Rev. E 101, 012905 (2020)], we investigated the…

地球物理 · 物理学 2021-01-26 Carlos Azael Alvarez Zambrano , Erick de Moraes Franklin

Beautiful dune patterns can be found in deserts and along coasts due to the instability of a plain sheet of sand under the action of the wind. Barchan dunes are highly mobile aeolian dunes found in areas of low sand availability and…

其他凝聚态物理 · 物理学 2009-11-10 O. Duran , V. Schwaemmle , H. Herrmann

Aeolian sand dunes originate from wind flow and sand bed interactions. According to wind properties and sand availability, they can adopt different shapes, ranging from huge motion-less star dunes to small and mobile barchan dunes. The…

软凝聚态物质 · 物理学 2009-11-10 P. Hersen

The dune skeleton model is a reduced model to describe the formation process and dynamics of characteristic types of dunes emerging under unidirectional steady wind. Using this model, we study the dependency of the morphodynamics of…

斑图形成与孤子 · 物理学 2016-09-09 H. Niiya , A. Awazu , H. Nishimori

Three dimensional dunes of crescentic shape, called barchans, are commonly found on Earth and other planetary environments. In the great majority of cases, barchans are organized in large fields in which corridors of size-selected barchans…

地球物理 · 物理学 2021-12-03 Willian Righi Assis , Fernando David Cúñez , Erick de Moraes Franklin

Corridors of size-selected crescent-shaped dunes, known as barchans, are commonly found in water, air, and other planetary environments. The growth of barchans results from the interplay between a fluid flow and a granular bed, but their…

地球物理 · 物理学 2021-08-24 Willian Righi Assis , Erick de Moraes Franklin

Barchans are eolian dunes of crescent shape found on Earth, Mars and other celestial bodies. Among the different types of barchan-barchan interaction, there is one, known as chasing, in which the dunes remain close but without touching each…

Almost fifty years of investigations of barchan dunes morphology and dynamics is reviewed, with emphasis on the physical understanding of these objects. The characteristics measured on the field (shape, size, velocity) and the physical…

凝聚态物理 · 物理学 2009-11-07 Bruno Andreotti , Philippe Claudin , Stéphane Douady

Barchan dunes --- crescent-shaped dunes that form in areas of unidirectional winds and low sand availability --- commonly display an asymmetric shape, with one limb extended downwind. Several factors have been identified as potential causes…

软凝聚态物质 · 物理学 2013-12-03 Eric J. R. Parteli , Orencio Durán , Mary C. Bourke , Haim Tsoar , Thorsten Poeschel , Hans J. Herrmann

Barchan dunes were found to transform into parabolic dunes and vice versa when the amount of vegetation on and around them changes. This work presents the first numerical simulation of this effect. We propose a continuum model for the…

其他凝聚态物理 · 物理学 2007-05-23 O. Duran , V. Schatz , H. J. Herrmann , H. Tsoar

To analyze theoretically the stability of the shape and the migration process of transverse dunes and barchans, we propose a {\it skeleton model} of 3D dunes described with coupled dynamics of 2D cross-sections. First, 2D cross-sections of…

斑图形成与孤子 · 物理学 2012-01-05 Hirofumi Niiya , Akinori Awazu , Hiraku Nishimori

We model formation and evolution of transverse dune fields. In the model, only the cross section of the dune is simulated. The only physical variable of relevance is the dune height, from which the dune width and velocity are determined, as…

统计力学 · 物理学 2007-05-23 J. H. Lee , A. O. Sousa , E. J. R. Parteli , H. J. Herrmann

Barchans are crescent-shaped sand dunes forming in aride regions with unidirectional wind and limited sand supply. We report analytical and numerical results for dune shapes under different environmental conditions as obtained from the…

软凝聚态物质 · 物理学 2009-11-11 Klaus Kroy , Sebastian Fischer , Benedikt Obermayer

Barchans are dunes of crescentic shape found on Earth, Mars and other celestial bodies, growing usually on polydisperse granular beds. In this Letter, we investigate experimentally the growth of subaqueous barchans consisting of bidisperse…

Sand dunes are ubiquitous in nature, and are found in abundance on Earth and other planetary environments. One of the most common types are crescent-shaped dunes known as barchans, whose mid-line could be assumed to behave as 2D dunes. In…

地球物理 · 物理学 2025-05-13 Willian Righi Assis , Erick de Moraes Franklin , Nathalie Vriend
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