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Eastern Mediterranean Sea circulation inferred from the conditions of S1 sapropel deposition

机译:从S1腐殖质沉积条件推断地中海东部环流

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Holocene eastern Mediterranean Sea sediments contain an organic-rich sapropelS1 layer that was formed in oxygen-depleted waters. The spatial distributionof this layer revealed that during S1 deposition, deep waters were anoxicbelow a depth of 1800 m. However, whether this boundary permanently existedfrom the early to the mid-Holocene has not been examined yet. To answer thisquestion, a multi-proxy approach was applied to a core retrieved close to the1800 m boundary (at 1780 m). We measured the bulk sediment elementalcomposition, the stable isotopic composition of the planktonic foraminiferGlobigerinoides ruber and the abundance of benthic foraminiferasince the last deglaciation. The result indicates that authigenic U and Moaccumulation began around 13–12 cal ka BP, in concert with surface waterfreshening estimated from the G. ruber δ18O record. Theonset of bottom and pore water oxygen depletion occurred prior to S1deposition inferred from barium enrichment. In the middle of the S1deposition period, reduced authigenic V, Fe and As contents and theBr/Cl ratio indicated short-term bottom-water re-oxygenation. A sharpMn peak and maximal abundance for benthic foraminifera marked a totalrecovery for circulation at approximately 7 cal ka BP. Based on ourresults and existing data, we suggest that S1 formation within the upper1780 m of the eastern Mediterranean Sea was preconditioned by reducedventilation, resulting from excess freshwater inputs due to insolationchanges under deglacial conditions that initiated between 15 and12 cal ka BP within the upper1780 m. Short-term re-oxygenation in the Levantine Basin is estimated tohave affected bottom water at least as deep as 1780 m in response to coolingand/or the reduction of freshwater inputs. We tentatively propose thatcomplete ventilation recovery at the S1 termination was depth-dependent, withearlier oxygenation within the upper 1780 m. Our results provide newconstraints on vertical water column structure in the eastern MediterraneanSea since the last deglaciation.
机译:全新世的地中海东部沉积物含有富含有机物的腐殖质S1层,该层是在贫氧水中形成的。该层的空间分布表明,在S1沉积过程中,深水在1800 m以下缺氧。但是,还没有研究从全新世早期到中期永久存在的边界。为了回答这个问题,对接近1800 m边界(在1780 m处)取回的岩心采用了多代理方法。我们测量了浮游有孔虫 Globigerinoides ruber 的总体沉积物元素组成,稳定同位素组成以及最近一次冰消作用下底栖有孔虫的丰度。结果表明,自生U和Moaccumulation开始于约13–12 cal ka BP,与根据 G估计的地表水淡化相一致。 ruber δ 18 O记录。从钡富集推断出S1沉积之前,开始发生底部和孔隙水耗氧的现象。在S1沉积期的中间,自生的V,Fe和As含量降低,Br / Cl比降低,表明短期底水再充氧。底栖有孔虫的一个尖锐的Mn峰和最大丰度标志着在大约7 cal ka BP循环的总回收率。根据我们的结果和现有数据,我们认为东地中海上部1780 m内的S1形成是通过减少通风来预先调节的,这是由于冰消条件下日照变化导致的淡水输入过量而导致的,淡水输入在上部1780 m内在15至12 cal BP之间开始。据估计,由于冷却和/或淡水输入的减少,黎凡特盆地的短期再充氧作用对底部水至少影响了1780m。我们初步建议S1终端的完全通风恢复取决于深度,在上部1780 m内氧合较早。自上次冰消以来,我们的结果对地中海东部的垂直水柱结构提供了新的约束。

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