Collaborative Research: Three-Dimensional Numerical Investigation of Density Currents

合作研究：密度流的三维数值研究

• 批准号: 0209309
• 负责人: Traian Iliescu
• 金额: $ 9.48万
• 依托单位: Virginia Polytechnic Institute and State University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2002
• 资助国家: 美国
• 起止时间: 2002-09-01 至 2006-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0209309&HistoricalAwards=false
• 关键词: Collaborative; Research; Three; Dimensional; Numerical

The oceanic thermohaline circulation is strongly affected by localizeddense-water formation in high-latitude oceans. Such dense water massesare released into the large-scale circulation in the form of ocean bottomdensity currents mostly from localized regions (e.g., Denmark Strait,Strait of Gibraltar for the Mediterranean overflow, Bab el Mandep Straitfor the Red Sea overflow). Because of the small space and time scalesrequired to resolve their dynamics, such density currents form the``bottle neck'' of the thermohaline circulation investigation. Despite theirimportance, we have a limited understanding of the dynamics of bottomdensity currents, and at present, the oceanic density currents are poorlyrepresented in global climate simulations. The main goal of this proposalis to enhance the understanding of the dynamics of ocean bottom densitycurrents from laboratory scale, to geophysical scale, through three-dimensional,nonhydrostatic numerical simulations. The investigators accomplish thisin three stages. First, benchmark a parallel high-order spectral elementNavier-Stokes solver, Nek5000, by reproducing existing laboratory resultsof bottom density currents by direct numerical simulations. Second,explore dynamics for which there are few or no laboratory results, inparticular dynamics of bottom density currents protruding into a stratifiedfluid, and in a rotating environment. Third, bridge the gap betweenlaboratory scale and geophysical scale by using large eddy simulations.Geophysical scale calculations are configured for the Red Sea overflow,and confirmed with data from the Red Sea Overflow Experiment. Variousmetrics are used to quantify density current dynamics.Variation of solar heating with latitude, and other factors, drive theso-called ``thermohaline'' circulation in the ocean, which is closelylinked to the role that the ocean plays in climate dynamics. This complexgeophysical problem, with its range of scales, physical, mathematical andcomputational constraints can only be approached through an orchestratedeffort involving cross-disciplinary expertise. The investigators conductphysically-guided numerical simulations, quantify dynamical behavior ofocean density currents, and describe the impact of density currents onthe climate. The investigators integrate this research project witheducation of three graduate students and contribute to the training ofUS technical workforce for the 21st century. This research projectenhances the scientific understanding of oceanic density currents, andhelps improve the representation of ocean density currents in globalclimate simulations and contribute to the climate change research.

海洋温盐环流受高纬海洋局部密水形成的强烈影响。这种密集的水团以海底密度流的形式被释放到大尺度环流中，大部分来自局部区域（例如，丹麦海峡、直布罗陀海峡为地中海溢流口、曼德海峡为红海溢流口）。由于解决其动力学所需的空间和时间尺度很小，这种密度流形成了温盐环流调查的“瓶颈”。尽管它们的重要性，我们有一个有限的了解底层密度流的动力学，目前，海洋密度流是在全球气候模拟中表现不佳。该提案的主要目标是通过三维非流体静力数值模拟，从实验室尺度到地球物理尺度，加强对海底密度流动力学的理解。调查人员分三个阶段完成这一任务。首先，基准并行高阶谱元素Navier-Stokes求解器，Nek 5000，通过复制现有的实验室结果的底部密度流的直接数值模拟。第二，探索动力学，有很少或没有实验室结果，特别是底层密度流的动力学突出到分层流体，并在旋转环境。第三，通过大涡模拟弥合实验室尺度和地球物理尺度之间的差距。密度流动力学的量化使用了各种度量标准。太阳加热随纬度和其他因素的变化，驱动了海洋中所谓的“温盐”环流，这与海洋在气候动力学中所扮演的角色密切相关。这个复杂的地球物理问题，其范围的规模，物理，数学和计算的限制，只能通过一个协调的deffort涉及跨学科的专业知识来处理。研究人员进行物理引导的数值模拟，量化海洋密度流的动力学行为，并描述密度流对气候的影响。研究人员将这一研究项目与三名研究生的教育结合起来，为21世纪美国技术劳动力的培训做出贡献。该研究项目的开展有助于加深对海洋密度流的科学认识，提高海洋密度流在全球气候模拟中的代表性，为气候变化研究做出贡献。