School of Mathematics and Statistics, University of New South Wales, Sydney, New South Wales 2052, Australia.
LOCEAN Laboratory, Sorbonne Universités (Université Pierre et Marie Curie Paris 6)-CNRS-IRD-MNHN, F-75005 Paris, France.
Nature. 2017 Nov 8;551(7679):181-186. doi: 10.1038/nature24472.
The abyssal ocean is broadly characterized by northward flow of the densest waters and southward flow of less-dense waters above them. Understanding what controls the strength and structure of these interhemispheric flows-referred to as the abyssal overturning circulation-is key to quantifying the ocean's ability to store carbon and heat on timescales exceeding a century. Here we show that, north of 32° S, the depth distribution of the seafloor compels dense southern-origin waters to flow northward below a depth of about 4 kilometres and to return southward predominantly at depths greater than 2.5 kilometres. Unless ventilated from the north, the overlying mid-depths (1 to 2.5 kilometres deep) host comparatively weak mean meridional flow. Backed by analysis of historical radiocarbon measurements, the findings imply that the geometry of the Pacific, Indian and Atlantic basins places a major external constraint on the overturning structure.
深渊海洋的一个显著特征是,密度较大的水向北流动,密度较小的水在其上方向南流动。了解控制这些半球间流(即深海翻转环流)强度和结构的因素,对于量化海洋在超过一个世纪的时间尺度上储存碳和热量的能力至关重要。在这里,我们表明,在南纬 32°以北,海底的深度分布迫使源自南方的高密度水在大约 4 公里深的地方向北流动,并主要在大于 2.5 公里深的地方向南回流。除非从北方通风,否则覆盖的中层(1 至 2.5 公里深)的平均经向流相对较弱。历史放射性碳测量的分析结果支持了这一发现,这意味着太平洋、印度洋和大西洋盆地的几何形状对翻转结构构成了重大的外部限制。