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New type of sand wedge polygons in the salt cemented soils of the hyper-arid Atacama Desert

机译:新型砂楔多边形在超干旱的阿塔卡马沙漠的盐泥土土壤中

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摘要

Polygonal grounds are landscape features commonly associated with periglacial environments originating from freeze-thawing cycles or frost-related processes. However, such a genesis is unlikely for polygonal grounds on alluvial surfaces in the warm and hyper-arid Atacama Desert due to the lack of enduring sub-zero temperatures and limited water availability, whereas a cracking mechanism based on thermal contraction and/or desiccation is more plausible. To differentiate between those mechanisms, we performed a quantitative morphometric terrain characterization in combination with a geochemical and sedimentological analysis on three polygonal networks located in the Yungay area of the Atacama Desert, Chile. Our data show that these sand wedge polygons differ from other polygonal features in the Yungay area such as salt polygons and mud crack polygons from playa environments in regard to composition, morphometry and topographical setting. The investigated polygonal soils are composed of siliciclastic sediment that is mainly cemented by sulfates (gypsum & anhydrite) in the shallow ground (similar to 0-50 cm) and by nitrates and chlorides in the deeper ground (similar to 50-100 cm) while being separated by about 1 m deep, salt-poor and V-shaped sand wedges. The low clay content (similar to 2 wt%) makes an exclusive desiccation origin less relevant whereas the high salt content (63 wt%) and the high surface temperature variations make thermal contraction origin more likely. Morphometric data indicate a link between topography and polygon geometry, as the flat-centered polygons (mean size 3.9 to 4.7 m) are aligned either in slope direction or perpendicular to it, while being more elongated on steeper slopes, which is common to thermal contraction polygons. Although we cannot exclude that desiccation cracking plays a minor role for the formation of the here described polygons, we conclude that their genesis is dominated by thermal contraction. (c) 2020 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
机译:多边形地面是与源自冻融循环或霜冻相关过程的蠕虫环境常见的景观特征。然而,由于缺乏持久的亚零温度和有限的水可用性,这种成因不太可能在温暖和超干旱的阿塔奇拉岛沙漠中的较温暖和超级干旱的阿塔奇拉山沙漠中的造成的多边形场。基于热收缩和/或干燥的裂缝机构是更合理的。为了区分这些机制,我们与位于智利阿塔卡马沙漠的Yungay地区的三个多边形网络的地球化学和沉积学分析组合进行了定量的形态学地形特征。我们的数据表明,这些砂楔多边形与Yungay区域中的其他多边形特征不同,例如来自Playa环境的盐多边形和泥裂色多边形,关于组成,形态学和地形设置。研究的多边形土壤由硅淤积沉积物组成,该沉积物主要由浅地(类似于0-50cm)和硝酸盐和氯化物在更深的地面(类似于50-100厘米)的情况下被约1米深,盐差和V形砂楔分开。低粘土含量(类似于2wt%)使得具有较少相关的独占性干燥原点,而高盐含量(63wt%)和高表面温度变化使热收缩起源更有可能。形态测量数据表示地形和多边形几何形状之间的链路,因为平面居中的多边形(平均尺寸3.9至4.7m)在倾斜方向上或垂直于其对准,同时在陡峭的斜坡上更伸长,这与热收缩是共同的多边形。尽管我们不能排除干燥裂缝,但是对于在这里描述的多边形的形成起着次要作用,我们得出结论,它们的成因是通过热收缩来支配。 (c)2020提交人。由elsevier b.v发布。这是CC By-NC-ND许可下的开放式访问文章(http://creativecommons.org/licenses/by-nc-nd/4.0/)。

著录项

  • 来源
    《Geomorphology 》 |2021年第15期| 107481.1-107481.14| 共14页
  • 作者单位

    Tech Univ Berlin Zentrum Astron & Astrophys Astrobiol Res Grp D-10623 Berlin Germany;

    Tech Univ Berlin Zentrum Astron & Astrophys Astrobiol Res Grp D-10623 Berlin Germany;

    Tech Univ Berlin Zentrum Astron & Astrophys Astrobiol Res Grp D-10623 Berlin Germany;

    Tech Univ Berlin Zentrum Astron & Astrophys Astrobiol Res Grp D-10623 Berlin Germany|German Res Ctr Geosci GFZ Sect Geomicrobiol D-14473 Potsdam Germany|Leibniz Inst Freshwater Ecol & Inland Fisheries I Dept Expt Limnol D-12587 Stechlin Germany;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Patterned ground; Sand wedge polygon; Atacama Desert; Hyper-arid;

    机译:图案地面;沙楔多边形;阿塔卡马沙漠;超干旱;

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