Internal Wave Induced Sub-inertial Currents (IWISC)

内波感应次惯性电流 (IWISC)

• 批准号: 0551371
• 负责人: Douglas Luther
• 金额: $ 28.89万
• 依托单位: University of Hawaii
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2006
• 资助国家: 美国
• 起止时间: 2006-03-15 至 2010-02-28
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0551371&HistoricalAwards=false
• 关键词: Internal; Wave; Induced; Sub; inertial

The flow of energy from the winds and tides through the ocean's internal gravity wave field may have far-reaching consequences, impacting even the qualitative nature of the abyssal ocean's circulation, with attendant implications for global climate fluctuations. Consequently, understanding the pathways of this energy flow is more than just an esoteric exercise in geophysical fluid dynamics. Until now, there has been little evidence for the proposition that an important pathway for energy leaving the internal wave band in the open ocean might be by the direct generation of non-resonant, non-propogating, sub-inertial motions.In this study, a researcher at the University of Hawaii will further explore the observational evidence for such a process acting on inertial and semi-diurnal internal waves. For simplicity, the process is referred to as "Internal Wave Induced Sub-inertial Currents" or IWISC. He proposes that a non-linear interaction between the semi-diurnal internal tide (nominally at the M2 frequency) and the inertial oscillations (at frequency f) results in the generation of these sub-inertial motions which exist around the frequency of M2 minus f. Preliminary analytical modeling and numerical simulations with a primitive equation model support this conjecture, but more work is needed to define the dynamics of its generics. Most importantly, this observation of the M2-f interaction may presage the existence of a whole class of interactions that pump energy out of the internal wave field and into sub-inertial motions in the open ocean. To explore this IWISC phenomenon analysis of historical datasets, simulations with a primitive equation numerical model, and theoretical analysis will be used. The results from this work significantly impact the estimates of the mount of internal wave energy that is available for mixing the abyssal ocean. In addition to the intellectual merit of the work, this research will support a graduate student as he conducts much of the proposed work under the close supervision of his advisor.

来自风和潮汐的能量流通过海洋内部重力波场可能会产生深远的影响，甚至影响深海环流的性质，从而对全球气候波动产生影响。 因此，了解这种能量流的路径不仅仅是地球物理流体动力学中的深奥练习。 到目前为止，几乎没有证据表明能量离开公海内波段的重要途径可能是直接产生非共振、非传播、亚惯性运动。在这项研究中，夏威夷大学的一位研究人员将进一步探索作用于惯性和半日内波的这一过程的观测证据。 为简单起见，该过程称为“内波感应亚惯性流”或 IWISC。 他提出，半日内潮汐（名义上在 M2 频率）和惯性振荡（在频率 f）之间的非线性相互作用导致了这些亚惯性运动的产生，这些运动存在于 M2 减去 f 的频率附近。 初步分析建模和使用原始方程模型的数值模拟支持了这一猜想，但需要更多的工作来定义其泛型的动力学。 最重要的是，对 M2-f 相互作用的观察可能预示着一整类相互作用的存在，这些相互作用将能量从内波场泵出并进入公海的亚惯性运动。 为了探索历史数据集的 IWISC 现象分析，将使用原始方程数值模型进行模拟，并进行理论分析。 这项工作的结果极大地影响了可用于混合深海海洋的内波能量的估计。 除了这项工作的智力价值之外，这项研究还将支持研究生，因为他在导师的密切监督下开展了大部分拟议的工作。