Internal gravity wave dynamics in a rotating and stratified fluid

旋转分层流体中的内部重力波动力学

• 批准号: 0755114
• 负责人: Harry Swinney
• 金额: $ 29.58万
• 依托单位: University of Texas at Austin
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2008
• 资助国家: 美国
• 起止时间: 2008-09-01 至 2012-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0755114&HistoricalAwards=false
• 关键词: Internal; gravity; wave; dynamics; rotating

CBET-0755114Swinney Internal gravity waves are ubiquitous in lakes, oceans and the atmosphere, due to the density stratification present in these environmental fluid bodies. Internal gravity waves affect acoustic transmission, sediment transport and off-shore platforms. These waves are also a major driving mechanism for the general circulation of the ocean. The goal of this research is to use laboratory experiments and numerical simulations is to better understand the fundamental fluid dynamics underlying the generation, interaction and breaking of internal gravity waves. The experiments will be conducted in a stratified and rotating fluid using Particle Image Velocimetry, a conductivity probe, and fluorescent dye visualization. Pseudo-spectral numerical experiments will complement the laboratory experiments. Specifically, the PIs will study harmonic wave generation by internal gravity wave-wave interactions, internal wave generation and mixing over a sloping boundary, and latitudinal dependence of the parametric subharmonic instability. Detailed spatiotemporal data will be obtained in regimes where appropriate theoretical models do not exist and field observations provide sparse data. Systematic variation of parameters in the experiments and simulations will help reveal the underlying physics. Experiments on nonresonant wave-wave interactions will improve the current picture of energy exchange between waves. Experiments on internal wave generation will quantify a new mechanism that can produce strong boundary flow and turbulent mixing in lakes and continental margins. Experiments on the parametric subharmonic instability will help to understand the global internal gravity wave dissipation in oceans. Understanding of the fundamental physics revealed by this research will enhance the ability to quantify the role of internal gravity waves in lake, oceanic and atmospheric dynamics. Besides the environmental applications, experiments on nonresonant wave-wave interactions may also have impact on the understanding of waves in strongly magnetized plasmas, where there exist waves (e.g., in tokamaks) with the same dispersion relation as internal gravity waves. Further, this type of wave plays an important role in the dynamics of White Dwarfs and Neutron Stars.

CBET-0755114 Swinney内部重力波在湖泊、海洋和大气中普遍存在，这是由于这些环境流体中存在密度分层。重力内波影响声波传输、沉积物输运和海上平台。这些波浪也是海洋环流的主要驱动机制。本研究的目标是使用实验室实验和数值模拟，以更好地了解内部重力波的产生，相互作用和破碎的基本流体动力学。实验将在分层和旋转的流体中进行，使用粒子图像测速仪，电导率探针和荧光染料可视化。伪谱数值实验将补充实验室实验。具体而言，PI将研究谐波产生的内部重力波波相互作用，内波产生和混合的倾斜边界，和纬度依赖的参数次谐波不稳定性。在不存在适当理论模型且实地观察提供稀疏数据的情况下，将获得详细的时空数据。在实验和模拟中系统地改变参数将有助于揭示潜在的物理现象。关于非共振波-波相互作用的实验将改善目前波之间能量交换的情况。内波生成实验将量化一种新的机制，这种机制可以在湖泊和大陆边缘产生强烈的边界流和湍流混合。参数亚谐不稳定性的实验研究将有助于理解全球海洋重力内波的耗散。了解这项研究揭示的基础物理学将提高量化湖泊，海洋和大气动力学中内部重力波作用的能力。除了环境应用外，非共振波-波相互作用的实验也可能对理解强磁化等离子体中的波产生影响，在强磁化等离子体中存在波（例如，在托卡马克中）具有与内部重力波相同的色散关系。此外，这种类型的波在白色矮星和中子星的动力学中起着重要的作用。