首页> 外文期刊>Journal of sedimentary research >Eolian topography as a control on deposition incorporating lessons from modern dune seas: Permian Cedar Mesa Sandstone, SE Utah, USA
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Eolian topography as a control on deposition incorporating lessons from modern dune seas: Permian Cedar Mesa Sandstone, SE Utah, USA

机译:结合现代沙丘海洋的经验,以风沙地形作为沉积控制:美国犹他州二叠纪雪松梅萨砂岩

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The dominant current model for the accumulation of eolian strata in the rock record emphasizes translation and climb of bedforms and the preservation of continuous beds. Studies of modern dune fields, however, show that, when large dunes form, they create a topographically irregular surface; later episodes of eolian activity commonly fill the low-lying areas between the older dunes, resulting in beds that are laterally discontinuous. Strata in part of the Permian Cedar Mesa Sandstone in southeastern Utah require this model. In this new model, inherited eolian topography influences subsequent deposition. Detailed GPS mapping of an 8 km(2) area was used to trace eolian strata through a 20-25-m-thick unit in the Cedar Mesa Sandstone. The unit is bounded above and below by subparallel erosion surfaces that have up to 5 to of relief. Within the unit, large transverse draa (or megadune) deposits, are spaced 1 km apart. Locally (over 0.5 km wide areas), the draa deposits fill the entire 25 m thickness of the unit, only to be completely replaced by interdraa deposits a few hundred meters away. The draa surfaces were eroded and exposed prior to the filling of the intervening lows with alternations of barchanoid dune deposits, sand sheets, and ponds, which formed in the topographic lows. The Cedar Mesa Sandstone illustrates aggradation wherein the important factor is the preserved eolian topography. The draas formed an undulating stable surface, from which subsequent deposition filled the interdraa low. Large eolian dunes that influenced subsequent deposition are also observed in several Pleistocene to Recent dune seas. This mechanism offers an alternative to the existing models that require continuous migration of large dunes.
机译:岩石记录中风积层形成的主要潮流模型强调地层的平移和爬升以及连续床的保存。然而,对现代沙丘场的研究表明,形成大沙丘时,它们会形成地形上不规则的表面。以后的风沙活动通常填充较老的沙丘之间的低洼区域,从而导致床层横向不连续。犹他州东南部的二叠纪Cedar Mesa砂岩部分地层需要此模型。在这个新模型中,继承的风积地形会影响随后的沉积。 8 km(2)区域的详细GPS映射用于通过Cedar Mesa砂岩中20-25米厚的单元追踪风成岩层。该单元的上方和下方由亚平行的腐蚀表面界定,这些腐蚀表面具有最多5到8的浮雕。在单元内,大型横向draa(或megadune)沉积物相距1 km。就局部而言(超过0.5 km宽的区域),draa沉积物填充了该单元的整个25 m厚度,只是被数百米外的interdraa沉积物完全替代。在用低垂的沙丘沉积物,砂岩和池塘交替填充中间低谷之前,对draa表面进行腐蚀和暴露,在地势低谷中形成。雪松台地砂岩说明了沉积,其中重要因素是保存的风积地形。 draas形成起伏的稳定表面,随后的沉积从该表面上充满了dradra的下部。在几个更新世至最近的沙丘海中也观察到了影响随后沉积的大型风沙丘。该机制为需要连续迁移大型沙丘的现有模型提供了替代方法。

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