首页> 外文会议>International conference on port and ocean engineering under arctic conditions >MECHANISMS OF INTERACTION BETWEEN MESOSCALE OCEAN EDDIES AND SEA ICE IN HIGH-RESOLUTION ICE-OCEAN COUPLED MODEL OF THE LAPTEV SEA IN SUMMER
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MECHANISMS OF INTERACTION BETWEEN MESOSCALE OCEAN EDDIES AND SEA ICE IN HIGH-RESOLUTION ICE-OCEAN COUPLED MODEL OF THE LAPTEV SEA IN SUMMER

机译:夏季Laptev海高分辨率冰-海耦合模型中尺度海洋污染物与海冰相互作用的机理。

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Precise ice distribution prediction is one of key issues to realize safe and efficient navigation in the Northern Sea Route (NSR). Results of high-resolution (2.5km) hindcast computation (De Silva, 2015) have shown good agreement with observational ice distribution, which has motivated us to search for possible factors driving the sea ice variability in NSR using numerical model. We have found that mesoscale eddy production is one of the main factors responsible for sea ice variability in the Laptev Sea marginal ice zones. A three-dimensional high-resolution ice-ocean coupled model is used to investigate the eddy generation mechanisms. The model is designed to represent a typical condition for the summertime Laptev Sea mixed layer. Eddy generation due to ice-ocean interaction is discussed in details; a wind stress is larger over the ice than that on open water and induces Ekman pumping and suction, which produce dipole eddy motions. Vertical motions associated with the dipole eddies lead to deep vertical mixing and the subsequent melting of the ice. The dipole eddies generated by barotropic instability is further enhanced by vertical mixing and freshwater input due to sea ice melt. Those eddies are important to exchange the heat across the ice edge and to meandering of ice edge. Numerical sensitivity experiments suggest that the horizontal scale of generated eddies depends on the surface forcing. Also, these small-scale features are not modeled well with horizontal grids coarser than approximately 5 km.
机译:精确的冰分布预测是在北海航线(NSR)中实现安全,高效导航的关键问题之一。高分辨率(2.5 km)后预报计算的结果(De Silva,2015)与观测冰的分布显示出良好的一致性,这促使我们使用数值模型寻找驱动NSR中海冰变化的可能因素。我们发现中尺度涡旋产生是拉普捷夫海边缘冰区海冰变化的主要因素之一。三维高分辨率冰洋耦合模型用于研究涡旋产生机理。该模型旨在代表夏季Laptev Sea混合层的典型条件。详细讨论了由于冰洋相互作用而产生的涡流。冰上的风应力大于开阔水上的风应力,并引起埃克曼抽水和吸水,从而产生偶极涡旋运动。与偶极涡流相关的垂直运动会导致深度垂直混合,进而导致冰融化。由于海冰融化,垂直混合和淡水输入进一步增加了由正压不稳定性产生的偶极涡流。这些涡流对于跨冰边缘进行热交换以及使冰边缘弯曲非常重要。数值敏感性实验表明,所产生涡流的水平尺度取决于表面力。同样,这些小尺度特征在水平网格粗于大约5 km时也无法很好地建模。

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