首页> 外文期刊>Ocean Dynamics >Simulations of a Line W-based observing system for the Atlantic meridional overturning circulation
【24h】

Simulations of a Line W-based observing system for the Atlantic meridional overturning circulation

机译:基于W线的大西洋子午倾覆环流观测系统的仿真

获取原文
获取原文并翻译 | 示例
           

摘要

In a series of observing system simulations, we test whether the Atlantic meridional overturning circulation (AMOC) can be observed based on the existing Line W deep western boundary array. We simulate a Line W array, which is extended to the surface and to the east to cover the basin to the Bermuda Rise. In the analyzed ocean circulation model ORCA025, such an extended Line W array captures the main characteristics of the western boundary current. Potential trans-basin observing systems for the AMOC are tested by combining the extended Line W array with a mid-ocean transport estimate obtained from thermal wind “measurements” and Ekman transport to the total AMOC (similarly to Hirschi et al., Geophys Res Lett 30(7):1413, 2003). First, we close Line W zonally supplementing the western boundary array with several “moorings” in the basin (Line W-32°N). Second, we supplement the western boundary array with a combination of observations at Bermuda and the eastern part of the RAPID array at 26°N (Line W-B-RAPID). Both, a small number of density profiles across the basin and also only sampling the eastern and western boundary, capture the variability of the AMOC at Line W-32°N and Line W-B-RAPID. In the analyzed model, the AMOC variability at both Line W-32°N and Line W-B-RAPID is dominated by the western boundary current variability. Away from the western boundary, the mid-ocean transport (east of Bermuda) shows no significant relation between the two Line W-based sections and 26°N. Hence, a Line W-based AMOC estimate could yield an estimate of the meridional transport that is independent of the 26°N RAPID estimate. The model-based observing system simulations presented here provide support for the use of Line W as a cornerstone for a trans-basin AMOC observing system.
机译:在一系列观测系统模拟中,我们基于现有的W线深西部边界阵列,测试是否可以观测到大西洋子午倾覆环流(AMOC)。我们模拟了一个Line W数组,该数组延伸到表面和东部,以覆盖盆地至百慕大上升。在分析的海洋环流模型ORCA025中,这样的扩展W线阵列捕获了西部边界流的主要特征。通过将扩展的Line W阵列与热风“测量”和Ekman输运到总AMOC的中洋输运估计值相结合,测试了AMOC的潜在跨盆地观测系统(类似于Hirschi等,Geophys Res Lett 30(7):1413,2003)。首先,我们关闭W线,在盆地中向西部边界阵列纬向补充一些“系泊设备”(W-32°N线)。其次,我们结合在百慕大和26°N处RAPID阵列东部(W-B-RAPID线)的观测资料对西部边界阵列进行补充。既有整个盆地的少量密度分布图,也仅是东西边界的采样,捕获了W-32°N线和W-B-RAPID线AMOC的变化。在分析的模型中,W-32°N线和W-B-RAPID线的AMOC变异性主要由西方边界电流变异性决定。远离西边界,中海运输(百慕大东部)显示出两个基于W线的断面与26°N的区域之间没有显着关系。因此,基于W线的AMOC估算值可以得出与26°N RAPID估算值无关的子午线传输估算值。此处介绍的基于模型的观测系统模拟为使用Line W作为跨盆地AMOC观测系统的基石提供了支持。

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