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
【24h】

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海的高分辨率冰海耦合模型中迈空海洋漩涡与海冰之间的互动机制

获取原文

摘要

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路线(NSR)中实现安全有效的导航的关键问题之一。高分辨率(2.5公里)的Hindcast计算结果(De Silva,2015)表现出与观察冰分布的良好一致,这激发了我们在使用数值模型中寻找促进NSR中海冰变异性的可能因素。我们发现Mesoscale Eddy Production是Laptev海洋边缘冰区的海冰变异性的主要因素之一。使用三维高分辨率冰海耦合模型来研究涡流机制。该模型旨在表示夏季Laptev海洋混合层的典型条件。详细讨论了由于冰海洋互动导致的涡流;在冰上,风力胁迫比开放式水在冰上更大,并诱导ekman泵送和吸力,从而产生偶极涡流运动。与偶极铸造的垂直运动导致深垂直混合和随后的冰熔化。由于海冰熔体,通过垂直混合和淡水输入进一步增强了通过波衡量不稳定性产生的偶极涡流。这些漩涡非常重要,可以在冰边上交换热量并蜿蜒冰缘。数值敏感性实验表明产生的漩涡的水平规模取决于表面强制。此外,这些小规模特征不会与水平网格粗糙,比约5公里更粗糙。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号