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首页> 外文期刊>Climate of the past >Paleoceanography and ice sheet variability offshore Wilkes Land, Antarctica – Part 1: Insights from late Oligocene astronomically paced contourite sedimentation
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Paleoceanography and ice sheet variability offshore Wilkes Land, Antarctica – Part 1: Insights from late Oligocene astronomically paced contourite sedimentation

机译:南极威尔克斯地区近海的古海洋学和冰盖变化–第1部分:晚渐新世天文步速轮廓岩沉积的见解

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Antarctic ice sheet and Southern Ocean paleoceanographic configurations during the late Oligocene are not well resolved. They are however important to understand the influence of high-latitude Southern Hemisphere feedbacks on global climate under COsub2/sub scenarios (between 400 and 750 ppm) projected by the IPCC for this century, assuming unabated COsub2/sub emissions. Sediments recovered by the Integrated Ocean Drilling Program (IODP) at Site U1356, offshore of the Wilkes Land margin in East Antarctica, provide an opportunity to study ice sheet and paleoceanographic configurations during the late Oligocene (26–25 Ma). Our study, based on a combination of sediment facies analysis, magnetic susceptibility, density, and X-ray fluorescence geochemical data, shows that glacial and interglacial sediments are continuously reworked by bottom currents, with maximum velocities occurring during the interglacial periods. Glacial sediments record poorly ventilated, low-oxygenation bottom water conditions, interpreted as resulting from a northward shift of westerly winds and surface oceanic fronts. Interglacial sediments record more oxygenated and ventilated bottom water conditions and strong current velocities, which suggests enhanced mixing of the water masses as a result of a southward shift of the polar front. Intervals with preserved carbonated nannofossils within some of the interglacial facies are interpreted as forming under warmer paleoclimatic conditions when less corrosive warmer northern component water (e.g., North Atlantic sourced deep water) had a greater influence on the site. Spectral analysis on the late Oligocene sediment interval shows that the glacial–interglacial cyclicity and related displacements of the Southern Ocean frontal systems between 26 and 25 Ma were forced mainly by obliquity. The paucity of iceberg-rafted debris (IRD) throughout the studied interval contrasts with earlier Oligocene and post-Miocene Climate Optimum sections from Site U1356 and with late Oligocene strata from the Ross Sea, which contain IRD and evidence for coastal glaciers and sea ice. These observations, supported by elevated sea surface paleotemperatures, the absence of sea ice, and reconstructions of fossil pollen between 26 and 25 Ma at Site U1356, suggest that open-ocean water conditions prevailed. Combined, this evidence suggests that glaciers or ice caps likely occupied the topographic highs and lowlands of the now marine Wilkes Subglacial Basin (WSB). Unlike today, the continental shelf was not overdeepened and thus ice sheets in the WSB were likely land-based, and marine-based ice sheet expansion was likely limited to coastal regions.
机译:渐新世晚期的南极冰盖和南大洋古海洋构造尚未得到很好的解决。但是,它们对于理解IPCC预测的本世纪CO 2 情景(400至750 ppm)下高纬度南半球反馈对全球气候的影响非常重要(假定CO 2 排放。在南渐新世晚期(26-25 Ma),由南极洲东部威尔克斯陆地边缘的U1356站点的综合海洋钻探计划(IODP)回收的沉积物提供了研究冰盖和古海洋构造的机会。我们的研究基于沉积相分析,磁化率,密度和X射线荧光地球化学数据的结合,表明冰川和冰川间沉积物通过底流不断地进行返修,而最大速度发生在冰川间期。冰川沉积物记录了通风不良,低氧的底水状况,这被解释为是西风和海面北风向北移动的结果。冰川间沉积物记录了更多的含氧和通风的底水情况,以及强劲的流速,这表明由于极地锋的南移,水体的混合性增强了。在某些冰川间相中保留有碳酸盐化的纳米化石的时间间隔被解释为在较温暖的古气候条件下形成的,而腐蚀性较弱的北部组分水(例如,北大西洋来源的深水)对该地点的影响更大。渐新世沉积后期的频谱分析表明,南大西洋额叶系统在26Ma和25Ma之间的冰川-冰川间的周期性和相关的位移主要是由倾斜引起的。在整个研究间隔中,冰山泛滥碎片(IRD)的匮乏与U1356站点的早渐新世和中新世后的气候最佳断面以及罗斯海的晚渐新世地层形成对比,后者包含了IRD以及沿海冰川和海冰的证据。这些观测结果受到海面古温度升高,海冰不存在以及U1356站点26至25 Ma之间化石花粉重建的支持,表明海洋环境普遍存在。综合起来,这些证据表明,冰川或冰帽很可能占据了现在的海洋威尔克斯次冰川盆地(WSB)的地形高地和低地。与今天不同,大陆架并没有加深,因此WSB的冰盖很可能是陆基的,而海洋冰盖的扩张很可能仅限于沿海地区。

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