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Origins and genesis of loess deposits in central Spain, as indicated by heavy mineral compositions and grain-size variability

机译:黄土沉积物在中部沉积物的起源和创世纪,如重型矿物组合物和晶粒尺寸变异性所示

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The formation of loess deposits strongly depends on the availability of deflatable dust-sized material. Identification of source areas and mechanisms of dust production is essential for an appropriate characterization of related palaeoenvironmental conditions. So far, little research has been done on loess deposits in the Mediterranean region and information about mechanisms of dust production is very rare. In this context, it is not clear from where the loess deposits from the upper Tagus Basin in central Spain originated. The main objective of this study was to find out whether these loess deposits were formed primarily by mountain processes and fluvial comminution, or whether they have their origin in the weathering of Tertiary marls in the centre of the Madrid Basin. A further concern was to link the determined source areas with loess formation mechanisms and concomitant environmental contexts. Following a comprehensive approach using heavy minerals and grain-size data, together with information on stratigraphic features and geomorphic positions, different local loess sources could be identified. This study shows that during the last 35 kyr a major proportion of the Tagus loess deposits was deflated from river floodplains, while the mountain region of the Iberian Range was identified as a significant source of respective floodplain sediments. Based on heavy mineral compositions and dating results, it was found that during Heinrich Stadial 3, sediment supply from the Iberian Range strongly increased, suggesting an environmental shift from initially warmer towards colder temperatures in late Marine Isotope Stage 3. Furthermore, it was found that grain-size patterns clearly indicate maximum wind strengths during Heinrich Stadial 3, followed by Heinrich Stadial 2 and Heinrich Stadial 1. These results demonstrate that the formation of dust-sized particles in this part of the Mediterranean operated similar to many other places in temperate and continental regions, and
机译:黄土沉积物的形成强烈取决于可可折叠的粉尘尺寸材料的可用性。鉴定源区和粉尘生产机制对于相关占间环境条件的适当表征至关重要。到目前为止,在地中海地区的黄土沉积物中已经完成了很少的研究,以及有关粉尘生产机制的信息非常罕见。在这种情况下,目前尚不清楚黄土沉积在西班牙中部的上层塔卢斯源的地方起源于此。本研究的主要目标是找出这些黄土沉积物是主要由山地过程和河流粉碎形成,还是它们是否在马德里盆地中心的高等教育沼泽的风化中具有它们的起源。进一步关注的是将所确定的源区与黄土形成机制联系起来和伴随的环境背景。在使用重型矿物和晶粒尺寸数据的综合方法之后,以及关于地层特征和地貌位置的信息,可以识别不同的局部黄土源。本研究表明,在过去的35 KYR期间,Tagus黄土沉积物的主要比例从河洪泛区放气,而伊伯利亚范围的山区被确定为各种洪泛区沉积物的重要来源。基于重型矿物组合物和约会结果,发现在海因里氏三级3期间,伊伯利安范围的沉积物大规模增加,表明早期海洋同位素第3阶段的较冷温度较冷的温度。此外,它发现了晶粒尺寸图案清楚地表明了海因里氏三级3期间的最大风力优势,其次是海因里奇2和海因里氏二级的1.这些结果表明,在地中海的这一部分中形成了粉尘粒度的形成类似于温带的许多其他地方大陆地区,和

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