首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Origin and formation of methane in groundwater of glacial origin from the Cambrian-Vendian aquifer system in Estonia
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Origin and formation of methane in groundwater of glacial origin from the Cambrian-Vendian aquifer system in Estonia

机译:爱沙尼亚寒武纪 - Vendian含水层系统的冰川起源地下水中甲烷的起源和形成

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摘要

Groundwater in the Cambrian-Vendian aquifer system in Estonia is characterised by the most depleted isotopic composition known in Europe (delta O-18 down to -23 parts per thousand). The water most likely originates from glacial meltwater recharge from the Fennoscandian Ice Sheet in the Pleistocene. The aquifer system is characterised by relative high methane concentrations (up to 50% of dissolved gases, estimated absolute concentration up to 1600 mu mol L-1), the origin of which has so far remained unclear. In this paper, we focus on the origin of methane, the factors controlling its spatial distribution and its isotope geochemistry in the aquifer system. The data reveal a large spatial variability in methane concentration, delta(13) C-CH4 and delta(2)H(CH4 )values (from -6 to -105 parts per thousand and from -220 to -420 parts per thousand, respectively). We show that local oxidation processes rather than different pathways of methane formation, have affected the initial isotopic composition of methane. Using the least modified delta C-13(CH4) values (from -85 to -105 parts per thousand), we conclude that methane most likely originates from the organic material overridden by the Fennoscandian Ice Shield during the Late Weichselian glaciation, that was carried into the aquifer system with infiltrating glacial meltwater. The estimated delta O-18 values of the water, where the methane was formed, are -17 +/- 1.5%e supporting the inference that the methane was formed during the Middle Weichselian interstadial. The study shows that groundwater of glacial origin in the Cambrian-Vendian aquifer system can serve as an alternative palaeoenvironmental archive to be used for studying the variations in climatic and environmental conditions in Northern Europe during glacial-interglacial cycles of the Pleistocene. (C) 2019 Elsevier Ltd. All rights reserved.
机译:在爱沙尼亚寒武纪 - Vendian含水层系统的地下水的特征在于欧洲已知的最耗尽的同位素组合物(Delta O-18降至-23份/份)。水最有可能源于冰川玻璃冰盖中的冰川熔融补给。含水层体系的特征在于相对高的甲烷浓度(高达50%的溶解气体,估计绝对浓度高达1600μmL-1),其来源仍不清楚。本文重点关注甲烷的起源,控制其空间分布及其在含水层系统中的同位素地球化学的因素。数据显示甲烷浓度,δ(13)C-CH4和Delta(2)H(CH 4)值(从-6至-105分,分别为-220至-420份每千次) )。我们表明局部氧化过程而不是甲烷形成的不同途径,影响了甲烷的初始同位素组成。使用最少修改的ΔC-13(CH4)值(从-85到-105份),我们得出结论,甲烷最有可能源于携带后期Weichselian冰川期间Fennoscandand冰盾的有机材料进入具有渗透冰川熔融水的含水层系统。甲烷形成的水的估计的ΔO-18值为-17 +/- 1.5%E,其支持在中间卫生间内形成甲烷的推理。该研究表明,寒武纪 - Vendian含水层系统中的冰川起源地下水可以作为替代古环境存档,用于研究北欧北欧期间北欧的气候和环境条件的变化。 (c)2019年elestvier有限公司保留所有权利。

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