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Ripples in intertidal mud—a conceptual explanation

机译:潮间带泥浆中的涟漪—概念解释

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On protected mudflats and along sheltered tidal channel margins, wave- and current-generated ripples are frequently observed on surficial and subsurface mud beds, although such bedforms are generally not thought to occur in cohesive sediments. In this paper, examples of such ripple marks in the German Wadden Sea (back-barrier tidal flats of Spiekeroog island) and also along the west coast of Korea (Baeksu tidal flats) are documented and analyzed. The mud ripples are 5–8 cm in spacing and 0.3–0.8 cm in height, and are composed of slightly sandy to virtually pure mud (80–98% mud content). For the Spiekeroog study area, a comparison of in situ particle-size measurements of suspended matter and of dispersed mud collected from the ripples shows that the former consists of low-density flocs which are considerably larger than the constituent grains of the latter. To assess local wave effects, near-bed orbital velocities and orbital diameters were calculated on the basis of standard wave theory using estimated wave parameters at the time of the study (June 2004) as well as wave data recorded nearby within the back-barrier tidal basin. The relationships between grain size, morphometric ripple parameters, and the near-bed orbital diameter show the wave-generated mud ripples to be of the orbital post-vortex type. It is demonstrated that only short-period shoaling (intermediate water depth) waves with periods of 1.5–2.5 s and heights of 0.1–0.5 m are able to generate and maintain such ripples. Corresponding near-bed orbital velocities range from 8–32 cm s–1 and near-bed orbital diameters from 6.25–10 cm. It can be anticipated that increased current shear and turbulence associated with higher and longer waves prevent ripple formation due to the resuspension of settled mud, and the breakdown of suspended flocs and aggregates into smaller particles which then tend to remain in suspension. The most plausible explanation for the formation of the mud ripples is that mud flocs and aggregates deposited from suspension around high-water slack tide under moderate weather conditions initially respond as single (non-cohesive) particles which are hydraulically equivalent to ambient very fine sands. During exposure at low tide, gradual loss of water transforms the rippled mud into increasingly more cohesive mud drapes which are more resistant to erosion. Unless destroyed during high-energy events, the mud ripples may remain intact long enough to become buried and thereby preserved. Indeed, occasional but persistent observations of ripples in sub-Recent to ancient mudrocks document their preservation potential.
机译:在受保护的滩涂和沿潮汐河道边缘,虽然在地表和地下泥浆床中经常观察到波浪和电流产生的波纹,尽管一般认为这种床形不发生在粘性沉积物中。在本文中,记录并分析了在德国瓦登海(施皮克罗格岛的后屏障潮汐滩)以及韩国西海岸(百色潮滩)出现此类波纹痕迹的示例。泥浆波纹的间距为5-8厘米,高度为0.3-0.8厘米,由细沙状到几乎纯净的泥浆组成(泥浆含量为80-98%)。对于Spiekeroog研究区,对悬浮物和从波纹收集的分散泥进行原位粒度测量的比较表明,前者由低密度絮凝物组成,后者明显大于后者的组成颗粒。为了评估局部波浪效应,根据标准波浪理论,使用研究时(2004年6月)的估计波浪参数以及后屏障潮汐附近记录的波浪数据,根据标准波浪理论计算了近床轨道速度和轨道直径盆地。晶粒尺寸,形态波纹参数和近床轨道直径之间的关系表明,波浪产生的泥浆波纹属于轨道涡旋后类型。结果表明,只有周期为1.5-2.5 s,高度为0.1-0.5 m的短周期浅滩波(中间水深)才能产生并保持这种波纹。相应的近床轨道速度范围为8–32 cm s-1,近床轨道直径范围为6.25–10 cm。可以预见,与更高和更长的波浪有关的增加的电流剪切和湍流可防止由于沉降的泥浆的再悬浮而导致的波纹形成,以及悬浮的絮凝物和聚集体分解成较小的颗粒,然后倾向于保持悬浮状态。关于泥浆波纹形成的最合理的解释是,在中等天气条件下,泥浆絮凝物和悬浮物在高水松弛潮汐附近悬浮形成,最初起的作用是单个(非粘性)颗粒,这些颗粒在水力上等同于周围的非常细的沙子。在退潮期间,水分的逐渐流失将波纹状的泥浆转变成越来越粘的泥浆单,更能抵抗侵蚀。除非在高能事件中被破坏,否则泥浆涟漪可能会保持完整无缺的时间,足以被掩埋并保存下来。确实,在近古的泥岩中偶尔但持续地观察到的涟漪记录了它们的保存潜力。

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  • 来源
    《Geo-Marine Letters》 |2013年第6期|449-461|共13页
  • 作者单位

    Korea Institute of Geoscience Mineral Resources">(1);

    Senckenberg Institute">(2);

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  • 正文语种 eng
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