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Methane in shallow subsurface sediments at the landward limit of the gas hydrate stability zone offshore western Svalbard

机译:在svalbard西部海域天然气水合物稳定带的陆地上的浅层地下沉积物中的甲烷

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摘要

Offshore western Svalbard plumes of gas bubbles rise from the seafloor at the landward limit of the gas hydrate stability zone (LLGHSZ; ∼400 m water depth). It is hypothesized that this methane may, in part, come from dissociation of gas hydrate in the underlying sediments in response to recent warming of ocean bottom waters. To evaluate the potential role of gas hydrate in the supply of methane to the shallow subsurface sediments, and the role of anaerobic oxidation in regulating methane fluxes across the sediment–seawater interface, we have characterised the chemical and isotopic compositions of the gases and sediment pore waters. The molecular and isotopic signatures of gas in the bubble plumes (C/C = 1 × 10; δC-CH = −55 to −51‰; δD-CH = −187 to −184‰) are similar to gas hydrate recovered from within sediments ∼30 km away from the LLGHSZ. Modelling of pore water sulphate profiles indicates that subsurface methane fluxes are largely at steady state in the vicinity of the LLGHSZ, providing no evidence for any recent change in methane supply due to gas hydrate dissociation. However, at greater water depths, within the GHSZ, there is some evidence that the supply of methane to the shallow sediments has recently increased, which is consistent with downslope retreat of the GHSZ due to bottom water warming although other explanations are possible. We estimate that the upward diffusive methane flux into shallow subsurface sediments close to the LLGHSZ is 30,550 mmol m yr, but it is <20 mmol m yr in sediments further away from the seafloor bubble plumes. While anaerobic oxidation within the sediments prevents significant transport of dissolved methane into ocean bottom waters this amounts to less than 10% of the total methane flux (dissolved + gas) into the shallow subsurface sediments, most of which escapes AOM as it is transported in the gas phase.
机译:斯瓦尔巴群岛西部的近海气泡从海底上升到天然气水合物稳定区的陆地极限(LLGHSZ;水深约400 m)。据推测,这种甲烷可能部分是由于响应于近期海洋底水的变暖而使下层沉积物中的气体水合物解离。为了评估天然气水合物在向浅层地下沉积物供应甲烷中的潜在作用,以及厌氧氧化在调节沉积物-海水界面中甲烷通量中的作用,我们表征了气体和沉积物孔隙的化学和同位素组成水域。气泡羽流中气体的分子和同位素特征(C / C = 1×10;δC-CH= -55至-51‰;δD-CH= -187至-184‰)与从内部回收的天然气水合物相似距LLGHSZ约30公里的沉积物。孔隙水硫酸盐剖面的模型表明,在LLGHSZ附近,地下甲烷通量在很大程度上处于稳定状态,没有证据表明由于天然气水合物的分解而导致甲烷供应的近期变化。然而,在GHSZ内较大的水深处,有证据表明,最近对浅层沉积物的甲烷供应有所增加,这与由于底部水变暖导致GHSZ的下坡后退是一致的,尽管还有其他解释可能。我们估计,进入靠近LLGHSZ的浅层地下沉积物中的向上扩散甲烷通量为30,550 mmol·myr,但在距海底气泡羽流较远的沉积物中,其<20 mmol·myr。虽然沉积物中的厌氧氧化阻止了溶解的甲烷大量转移到海底水中,但这不到进入浅层地下沉积物中的甲烷总通量(溶解的+气体)的10%,其中大部分在通过AOM运移时逃逸了AOM。气相。

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