نتایج جستجو برای: sand dunes

تعداد نتایج: 29226  

2005
Katherine S. Brantley Melany L. Hunt C. E. Brennen

Booming dunes” are large desert sand dunes that make a loud droning or humming noise during an avalanching of sand. The phenomenon has been observed for censturies, yet it remains largely unexplained. This note demonstrates that the booming frequency does not scale with the size of the particle or with the shearing speed of the avalanching sand. Instead, the dune may act as a waveguide with a f...

2008
R. E. KOSKE

The mycorrhizal status of dune plants from the island of Hawaii was investigated. All plants, including Batis maritima, Cocos nucifer, Ipomoea brasiliensis, Pennisetum setaceum , Prosopis pallida, Scaevola taccada, and Sporobolus sp., had vesicular urbuscular mycorrhizae (VAM) . Levels of colonization by VAM fungi ranged from less than 10% to 100% of the root length and were highest in Ipomoea ...

2008
Bruno Andreotti Philippe Claudin Stéphane Douady

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 problems they rise are presented. Then, we review the dynamical mechanisms explaining the formation and the propagation of dunes. In particular a complete and or...

Journal: :Physical review letters 2006
Orencio Durán Hans J Herrmann

Vegetation is the most common and most reliable stabilizer of loose soil or sand. This ancient technique is for the first time cast into a set of equations of motion describing the competition between aeolian sand transport and vegetation growth. Our set of equations is then applied to study quantitatively the transition between barchans and parabolic dunes driven by the dimensionless fixation ...

2008
C. D. Neish R. D. Lorenz R. L. Kirk

Introduction: Recent observations by the Cassini spacecraft show widespread regions of longitudinal dunes on Saturn’s moon Titan [1]. The exact composition of the dunes is not known, but its radar and infrared return suggest an organic component [2]. Given the broad extent of the dunes (they cover 40% of Titan’s equatorial areas), they constitute an important portion of Titan’s overall organic ...

2000
Koichi Onoue Tomoyuki Nishita

This paper proposes a method for modeling and rendering realistic desert scenes. A desert terrain includes sand dunes and wind ripples. We use two types of scale models to form them. We render the dunes with the wind-ripples by bump-mapping using LODs (Levels of Detail).

Journal: :مرتع و آبخیزداری 0
طیبه مصباح زاده دانشجوی دکتری بیابان زدایی، دانشکده منابع طبیعی، دانشگاه تهران، ایران حسن احمدی استاد دانشگاه آزاد اسلامی، واحد علوم تحقیقات، تهران، ایران

sand dunes mobility is one of the serious problems in arid regions. since wind regime is one of the important factors in sand dunes formation, its frequency, direction and magnitude can be effective. amount of wind energy and its directional variability (wind regime) have significant control on the morphology and maintenance of aeolian landforms. by recognizing of morphometric and morphodynamic...

Extended abstract 1- Introduction Fluvial and aeolian processes are important factors in changing the surface of morphology in the Earth. When rivers and sand dunes meet, the transportation of sediment  between them can lead to one of the systems or both  of them change. With their connection between river sediment and wind systems there would be lots of reactions, but very little has been st...

2009
Marco C. M. de M. Luna Eric J. R. Parteli Orencio Durán Hans J. Herrmann

In the present work, we use dune modeling in order to investigate the evolution of transverse dunes in the presence of vegetation. The vegetation is allowed to grow up to a maximum height Hmax with a growth rate R that oscillates in time. We find that the presence of the vegetation establishes a maximum height for the transverse dunes. If the transverse dune is larger than this maximum size, th...

Journal: :Science 2006
R D Lorenz S Wall J Radebaugh G Boubin E Reffet M Janssen E Stofan R Lopes R Kirk C Elachi J Lunine K Mitchell F Paganelli L Soderblom C Wood L Wye H Zebker Y Anderson S Ostro M Allison R Boehmer P Callahan P Encrenaz G G Ori G Francescetti Y Gim G Hamilton S Hensley W Johnson K Kelleher D Muhleman G Picardi F Posa L Roth R Seu S Shaffer B Stiles S Vetrella E Flamini R West

The most recent Cassini RADAR images of Titan show widespread regions (up to 1500 kilometers by 200 kilometers) of near-parallel radar-dark linear features that appear to be seas of longitudinal dunes similar to those seen in the Namib desert on Earth. The Ku-band (2.17-centimeter wavelength) images show approximately 100-meter ridges consistent with duneforms and reveal flow interactions with ...

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