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首页> 外文期刊>Catena: An Interdisciplinary Journal of Soil Science Hydrology-Geomorphology Focusing on Geoecology and Landscape Evolution >Meteoric Be-10, clay, and extractable iron depth profiles in the Colorado Front Range: Implications for understanding soil mixing and erosion
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Meteoric Be-10, clay, and extractable iron depth profiles in the Colorado Front Range: Implications for understanding soil mixing and erosion

机译:科罗拉多前锋范围内的Be-10陨石,粘土和可提取铁的深度剖面:对理解土壤混合和侵蚀的意义

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Analyzing meteoric Be-10 in soil profiles along with soil measurements such as pedogenic Fe and clay content permits better understanding of meteoric Be-10 transport in soils, soil formation, and hillslope geomorphology. This study presents meteoric Be-10 depth profiles from saprolite-derived soil catenas sampled in the Gordon Gulch catchment, Colorado Front Range and from nearby c. 130 and 15 ka glacial moraines. We compare meteoric Be-10 data with more classically used soil analyses of clay and extractable iron (Fed) content. Meteoric Be-10 and Fed do not show consistent trends in the hillslope profiles. Meteoric Be-10 and clay concentrations, however, generally decrease with depth and highest concentrations of Be-10 in horizons coincide with highest clay concentrations. Soils at moraine sites are better developed than those on hillslopes, and correlations of Be-10, Fed, and clay are stronger. In Gordon Gulch, south-facing hillslopes display meteoric Be-10 bulges at depth and lower near-surface concentrations compared to the declining profiles and higher near-surface concentrations of north-facing hillslopes. The aspect differences imply that south-facing hillslopes experience greater vertical mixing than north-facing hillslopes, and that greater lateral transport and erosion has occurred over the last 15-20 ka on south-facing hillslopes relative to north-facing hillslopes. Meteoric Be-10 depth profiles at moraine sites display bulge profiles with highest meteoric Be-10 concentrations in B-horizons, reflecting landform stability and pedogenic processes. Overall, our data demonstrate that signatures of chemical weathering in soils (Fed and clay) may or may not correlate to the meteoric Be-10 added through atmospheric deposition, and that profile shape of meteoric Be-10 can provide insight into the relative contribution of vertical mixing and surface erosion in relation to catena location and aspect during hillslope evolution. (C) 2014 Elsevier B.V. All rights reserved.
机译:分析土壤剖面中的Be-10陨石以及土壤测量(例如成岩铁和粘土含量)可以更好地了解Be-10的陨石在土壤中的运输,土壤形成和山坡地貌。这项研究提出了从腐泥土来源的土壤链中Be-10深度的流变图,这些土在戈登峡谷集水区,科罗拉多州前山脉和附近c采样。 130和15 ka冰川冰rain。我们将Be-10的流星数据与更传统的粘土和可提取铁(Fed)含量的土壤分析进行了比较。流星Be-10和美联储在山坡剖面上没有显示出一致的趋势。但是,流星的Be-10和黏土浓度通常随深度而降低,地平线上Be-10的最高浓度与黏土的最高浓度一致。冰m地区的土壤比山坡上的土壤发育更好,Be-10,美联储和粘土的相关性更强。在戈登峡谷,朝南的山坡在深度处呈现出Be-10隆起,近地表浓度较低,而朝北的山坡剖面下降且近地表浓度较高。坡度差异意味着,朝南的山坡比朝北的山坡经历了更大的垂直混合,并且相对于朝北的山坡,在朝南的山坡上的最后15-20 ka发生了更大的横向运输和侵蚀。冰m地区的流星Be-10深度剖面显示出B型地平线中Be-10浓度最高的凸起剖面,反映了地形的稳定性和成岩作用。总体而言,我们的数据表明,土壤(美联储和粘土)中化学风化的特征可能与通过大气沉积而添加的流星型Be-10相关,也可能不相关,并且流星型Be-10的轮廓形状可以洞察土壤中的相对贡献垂直混合和地表侵蚀与山坡演化过程中链的位置和纵横比有关。 (C)2014 Elsevier B.V.保留所有权利。

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