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首页> 外文期刊>Organic Geochemistry: A Publication of the International Association of Geochemistry and Cosmochemistry >The geochemical characteristics of the hydrate-bound gases from the Nyegga pockmark field, Norwegian Sea
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The geochemical characteristics of the hydrate-bound gases from the Nyegga pockmark field, Norwegian Sea

机译:来自Nyegga pockmark油田,挪威海的水合物结合气体的地球化学特征

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The Nyegga pockmark field located south east of the Voring Plateau, Norwegian Sea, was investigated on the UoB Cruises GS07-148 (2007) and GS08-155 (2008). Remotely operated vehicle (ROV) monitoring and successful recovery of gas hydrate give insights to the origin of the hydrocarbon gases in the complex pockmark feature named G11. Isotope values of methane (delta C-13 ranging from -72.4 to -66.2 parts per thousand and delta D from -202.0 to -198.0 parts per thousand) in the hydrate bound gas suggest that the methane is microbially produced and originates from CO2 reduction. It is proposed that the ethane from the gas hydrate has mixed thermogenic and microbial contributions, which is supported by the fact that the gas hydrate also contains propane and isobutane. The composition of the hydrate bound gas thus leads to small inclusions of structure II (sII) in the hydrate while the major part is structure I (sI). The isotope data and gas composition together with the geological setting suggest that the hydrate bound gas originated predominantly from a free gas system located beneath the gas hydrate stability zone and accumulated under glaciated debris formations. The free gas system is mainly microbial methane from in situ production. However, a contribution of thermogenic gas from deeper polygonal faults to the free gas system seems evident from the composition of the gas. The ROV monitoring strengthens previous suggestions that the fauna in the complex pockmark G11 are supported by ongoing micro-seepage. (C) 2010 Elsevier Ltd. All rights reserved.
机译:在UoB Cruises GS07-148(2007)和GS08-155(2008)上对位于挪威海Voring高原东南部的Nyegga麻袋区进行了调查。远程控制车辆(ROV)的监视和成功回收天然气水合物,从而使人们深入了解了名为G11的复杂痘痕特征中烃类气体的来源。水合物结合气体中甲烷的同位素值(δC-13为千分之-72.4至-66.2份,δD为千分之2.02.0至-198.0份)表明甲烷是微生物产生的,起源于CO2的还原。有人提出,来自天然气水合物的乙烷具有热和微生物的混合作用,这是因为天然气水合物还含有丙烷和异丁烷。因此,与水合物结合的气体的组成导致在水合物中少量包含结构II(sII),而主要部分是结构I(sI)。同位素数据和气体组成以及地质背景表明,与水合物结合的气体主要起源于位于天然气水合物稳定区下方的自由气体系统,并在冰屑残渣层中积累。自由气体系统主要是原位生产的微生物甲烷。然而,从气体的组成看,更深的多边形断层对热气体的贡献似乎很明显。 ROV监测加强了先前的建议,即复杂的痘痕G11中的动物群受到正在进行的微渗流的支持。 (C)2010 Elsevier Ltd.保留所有权利。

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