Roquet Fabien, Ferreira David, Caneill Romain, Schlesinger Daniel, Madec Gurvan
Department of Marine Sciences, University of Gothenburg, 40530 Gothenburg, Sweden.
Department of Meteorology, University of Reading, Reading RG66ET, UK.
Sci Adv. 2022 Nov 18;8(46):eabq0793. doi: 10.1126/sciadv.abq0793. Epub 2022 Nov 16.
The formation of sea ice in polar regions is possible because a salinity gradient or halocline keeps the water column stable despite intense cooling. Here, we demonstrate that a unique water property is central to the maintenance of the polar halocline, namely, that the thermal expansion coefficient (TEC) of seawater increases by one order of magnitude between polar and tropical regions. Using a fully coupled climate model, it is shown that, even with excess precipitations, sea ice would not form at all if the near-freezing temperature TEC was not well below its ocean average value. The leading order dependence of the TEC on temperature is essential to the coexistence of the mid/low-latitude thermally stratified and the high-latitude sea ice-covered oceans that characterize our planet. A key implication is that nonlinearities of water properties have a first-order impact on the global climate of Earth and possibly exoplanets.
极地地区海冰的形成是可能的,因为盐度梯度或盐跃层使水柱保持稳定,尽管冷却强烈。在这里,我们证明了一种独特的水特性对于极地盐跃层的维持至关重要,即海水的热膨胀系数(TEC)在极地和热带地区之间增加了一个数量级。使用一个完全耦合的气候模型表明,即使有过量降水,如果接近冰点温度下的热膨胀系数没有远低于其海洋平均值,海冰根本不会形成。热膨胀系数对温度的主要阶次依赖性对于中/低纬度热分层和高纬度海冰覆盖的海洋共存至关重要,而这正是我们星球的特征。一个关键的含义是,水特性的非线性对地球乃至可能的系外行星的全球气候有一阶影响。