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Related papers: Formation of aeolian ripples and sand sorting

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When wind blows over water, ripples are generated on the water surface. These ripples can be regarded as perturbations of the wind field, which is modelled as a parallel inviscid flow. For a given wavenumber $k$, the perturbed…

Fluid Dynamics · Physics 2022-06-28 A. F. Bonfils , Dhrubaditya Mitra , W. Moon , J. S. Wettlaufer

This article presents direct numerical simulations of the growth of turbulent spots in the transitional regime of plane Couette flow. A quantitative description of the growth process and of the detail of the quadrupolar flow around the spot…

Fluid Dynamics · Physics 2014-01-16 Joran Rolland

The saturation length of aeolian sand transport ($L_s$), characterizing the distance needed by wind-blown sand to adapt to changes in the wind shear, is essential for accurate modeling of the morphodynamics of Earth's sandy landscapes and…

Atmospheric and Oceanic Physics · Physics 2015-08-19 Thomas Pähtz , Amir Omeradžić , Marcus V. Carneiro , Nuno A. M. Araújo , Hans J. Herrmann

Many small bodies in the solar system are believed to be rubble piles, a collection of smaller elements separated by voids. We propose a model for the structure of a self-gravitating rubble pile. Static friction prevents its elements from…

Astrophysics · Physics 2009-02-12 Peter Goldreich , Re'em Sari

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…

Statistical Mechanics · Physics 2007-05-23 J. H. Lee , A. O. Sousa , E. J. R. Parteli , H. J. Herrmann

Solar wind is probably the best laboratory to study turbulence in astrophysical plasmas. In addition to the presence of magnetic field, the differences with neutral fluid isotropic turbulence are: weakness of collisional dissipation and…

Solar and Stellar Astrophysics · Physics 2015-06-16 Olga Alexandrova , Christopher H. K. Chen , Luca Sorriso-Valvo , Timothy S. Horbury , Stuart D. Bale

In this paper, we describe how we can precisely produce complex and various dynamic morphological features such as structured and chaotic features which occur in sand pilings (piles, avalanches, internal collapses, arches) , in flowing…

Graphics · Computer Science 2010-05-31 Annie Luciani

This second paper of the series (see the first one in [1]) models the dynamics and structure of upper hurricane layer in adiabatic approximation. Formulation of simplified aerodynamic model allows analytically express the radial…

Atmospheric and Oceanic Physics · Physics 2008-12-18 Arkady I. Leonov

We introduce and investigate a simple model to describe recent experiments by Douady and Daerr on flowing sand. The model reproduces experimentally observed compact avalanches, whose opening angle decreases linearly as a threshold is…

Statistical Mechanics · Physics 2009-10-31 Haye Hinrichsen , Andrea Jimenez-Dalmaroni , Yadin Rozov , Eytan Domany

Evolution of mixing of granular solids in a slowly rotated 2D drum is considered as a discrete mapping. The rotation is around the axis of the upright drum which is filled partially, and the mixing occurs only at a free surface of a…

Condensed Matter · Physics 2007-05-23 S. N. Dorogovtsev

Dense granular flows are often unstable and form inhomogeneous structures. Although significant advances have been recently made in understanding simple flows, instabilities of such flows are often not understood. We present experimental…

Soft Condensed Matter · Physics 2009-10-02 Tamas Borzsonyi , Robert E. Ecke , Jim N. McElwaine

When submitted to the repeated passages of vehicles unpaved roads made of sand or gravel can develop a ripply pattern known as washboard or corrugated road. We propose a stability analysis based on experimental measurements of the force…

Soft Condensed Matter · Physics 2013-01-21 Baptiste Percier , Sébastien Manneville , Nicolas Taberlet

We consider the Clairaut theory of the equilibrium ellipsoidal figures for differentiated non-homogeneous bodies in non-synchronous rotation adding to it a tidal deformation due to the presence of an external gravitational force. We assume…

Earth and Planetary Astrophysics · Physics 2015-05-21 Hugo Folonier , Sylvio Ferraz-Mello , Konstantin V. Kholshevnikov

Differential growth processes play a prominent role in shaping leaves and biological tissues. Using both analytical and numerical calculations, we consider the shapes of closed, elastic strips which have been subjected to an inhomogeneous…

Materials Science · Physics 2011-01-19 Bryan Gin-ge Chen , Christian D. Santangelo

We present a phenomenological theory of phase transitions in achiral lipid membranes in terms of two coupled order parameters -- a scalar order parameter describing lipid chain melting, and a vector order parameter describing the tilt of…

Soft Condensed Matter · Physics 2010-11-16 Md. Arif Kamal , Antara Pal , V. A. Raghunathan , Madan Rao

Sand traps are used to measure Aeolian flux. Since they modify the surrounding wind velocity field their gauging represents an important challenge. We use numerical simulations under the assumption of homogeneous turbulence based on FLUENT…

Fluid Dynamics · Physics 2008-08-21 A. D. Araújo , J. S. Andrade , L. P. Maia , H. J. Herrmann

We obtain simple generating sets for various mapping class groups of a nonorientable surface with punctures and/or boundary. We also compute the abelianizations of these mapping class groups.

Geometric Topology · Mathematics 2014-02-18 Michal Stukow

The evolution of surface gravity waves is driven by nonlinear interactions that trigger an energy cascade similarly to the one observed in hydrodynamic turbulence. This process, known as wave turbulence, has been found to display anomalous…

We calculate the tidal torque on a uniformly rotating 1 Msun star at various stages of core hydrogen burning by an orbiting companion. We apply the `traditional approximation' and solve the radial part of the tidal perturbations by matrix…

Astrophysics · Physics 2009-11-07 G. J. Savonije , M. G. Witte

The torsional oscillation is a well established observational fact and there are theoretical attempts for its description but no final solution has yet been accepted. One of the possible candidates for its cause is the presence of sunspots…

Solar and Stellar Astrophysics · Physics 2014-01-13 J. Muraközy , A. Ludmány
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