解码活动构造对喜马拉雅流域沉积预算的控制:从河床沉积物的钍和钕同位素组成(87Sr/86Sr,εNd)中获得的启示

IF 2.6 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Satyabrata Das , Santosh K. Rai , Waliur Rahaman , Saurabh Singhal , Sandeep Panda , Shushanta Sarangi
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引用次数: 0

摘要

在构造活跃的喜马拉雅山系中,气候与构造之间的相互作用主要影响着侵蚀和沉积作用。在本研究中,利用河床沉积物的钍和钕同位素组成(87Sr/86Sr、εNd),对喜马拉雅山各岩石构造单元对蒂斯塔河水系(TRS)(雅鲁藏布江水系的一条主要支流)沉积预算的相对贡献进行了解密。此外,还对观测到的这种沉积来源的可能控制因素进行了评估。排放加权沉积物迁移量已转化为流域侵蚀率的量化。河床沉积物硅酸盐部分的 87Sr/86Sr 和 εNd 值范围分别为 0.74867 至 0.90529 和 - 24.3 至 -13.9。在 Teesta 主河道,87Sr/86Sr 和 εNd 在整个河道中的变化范围很大,分别为 0.74867 至 0.82288 和 -21.8 至 -13.9。这种巨大的变化表明了沉积物来源的变化,即高喜马拉雅山和小喜马拉雅山的变化。这些数据集显示,60% 的 TRS 沉积物来自小喜马拉雅山,表明小喜马拉雅山流域的物理侵蚀程度较高。我们的评估结果表明,蒂埃斯塔盆地的沉积预算主要受研究区域小喜马拉雅地区较高的掘起和垂直抬升率(由于 Rangeet 双峰的存在)以及集中降水的影响。根据沉积物排放法,我们估计蒂埃斯塔盆地的侵蚀速率为 1.7 ± 0.5 毫米/年,由此得出的年沉积物通量总量为 ~41.4 ± 12.4 兆吨。这一估计值与恒河流域等其他喜马拉雅河流域相当,但低于雅鲁藏布江流域(纳木错巴瓦和东综合区)和印度河流域(西综合区)等侵蚀热点地区。泰斯特河流域的侵蚀率似乎是喜马拉雅山脉锡金段活跃的构造运动造成的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Decoding the control of active tectonics on the sedimentary budget of a Himalayan River basin: Insights from Sr and Nd isotopic compositions (87Sr/86Sr, εNd) of bed sediments

The interaction between climate and tectonics chiefly governs the erosion and sedimentary budget in the tectonically active Himalayan Mountain chain. In the present study, the relative contribution from the various litho-tectonic units of the Himalaya to the sedimentary budget of the Teesta River System (TRS) (a major tributary of the Brahmaputra system) has been deciphered using the Sr and Nd isotopic compositions (87Sr/86Sr, εNd) of bed sediments. The possible controlling factors for such observed sedimentary provenance have also been assessed. The discharge-weighted sediment transport amount has been translated into the quantification of the erosion rate in the basin. The 87Sr/86Sr and εNd values in the silicate fraction of bed sediments range from 0.74867 to 0.90529 and − 24.3 to −13.9, respectively. In the Teesta main channel, 87Sr/86Sr and εNd show large variability ranging from 0.74867 to 0.82288 and −21.8 to −13.9, respectively along its entire course. This large variability indicates changes in sediment sources i.e., Higher Himalaya and Lesser Himalaya. These data sets show that >60 % of TRS sediments are derived from the Lesser Himalaya, indicating a higher physical erosion over the catchments in the Lesser Himalaya. Our assessment suggests that the sedimentary budget of the Teesta Basin is chiefly governed by higher exhumation as well as the vertical uplift rate of the lesser Himalaya sector of the study area (due to the presence of Rangeet duplex) coupled with focused precipitations. Based on the sediment discharge method, we estimate the erosion rate in the Teesta basin to be 1.7 ± 0.5 mm/yr, which yields a total annual sediment flux of ~41.4 ± 12.4 Mtons. This estimate is comparable to other Himalayan River basins like the Ganga basin, however, lower than the erosion hotspots such as the Brahmaputra basin (Namche Barwa and eastern Syntaxis region) and Indus basin (western Syntaxis region). The obtained erosion rate of the Teesta basin seems to result from the active tectonics in the Sikkim sector of the Himalaya.

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来源期刊
Chemie Der Erde-Geochemistry
Chemie Der Erde-Geochemistry 地学-地球化学与地球物理
CiteScore
7.10
自引率
0.00%
发文量
40
审稿时长
3.0 months
期刊介绍: GEOCHEMISTRY was founded as Chemie der Erde 1914 in Jena, and, hence, is one of the oldest journals for geochemistry-related topics. GEOCHEMISTRY (formerly Chemie der Erde / Geochemistry) publishes original research papers, short communications, reviews of selected topics, and high-class invited review articles addressed at broad geosciences audience. Publications dealing with interdisciplinary questions are particularly welcome. Young scientists are especially encouraged to submit their work. Contributions will be published exclusively in English. The journal, through very personalized consultation and its worldwide distribution, offers entry into the world of international scientific communication, and promotes interdisciplinary discussion on chemical problems in a broad spectrum of geosciences. The following topics are covered by the expertise of the members of the editorial board (see below): -cosmochemistry, meteoritics- igneous, metamorphic, and sedimentary petrology- volcanology- low & high temperature geochemistry- experimental - theoretical - field related studies- mineralogy - crystallography- environmental geosciences- archaeometry
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