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DOI | 10.1029/2020JC016502 |
The Three-Dimensional Internal Tide Radiation and Dissipation in the Mariana Arc-Trench System | |
Zhao C.; Xu Z.; Robertson R.; Li Q.; Wang Y.; Yin B. | |
发表日期 | 2021 |
ISSN | 21699275 |
卷号 | 126期号:5 |
英文摘要 | Internal tides are energetic in the Mariana arc, but their three-dimensional radiation and dissipation remain unexplored, particularly the trench-arc-basin impacts. Here, the generation, propagation and dissipation of M2 internal tides over the Mariana area are examined using a series of observation-supported high-resolution simulations. The M2 barotropic to baroclinic conversion rate amounts to 8.35 GW, of which two arc-shaped ridges contribute ∼81% of the generated energy. The contributions to generation by the Mariana basin and deep trench are weak. Nevertheless, they are important in modulating the energy radiation and dissipation, since tidal beams can spread to these areas. The Mariana ridges radiate the westward-focused and eastward-spreading tidal beams. This is very consistent with the altimetric measurements. The resonance in the ridge center enhances the westward converging beam, which can travel across the Palau Ridge, 800 km away. In contrast, the eastward beams propagate over a limited lateral range, but can radiate and dissipate significant energy in the deep water column, reaching even to the abyssal Mariana trench. The direct estimation from the model results reveals the dissipation's multilayer vertical profile in the entire water column, and is well consistent with the finescale parameterization estimate based on vertical strain. However, the estimate of an oft-used energy balance method, which typically assumes an exponentially decaying vertical structure function for the dissipation rate based on distance above the seafloor, is largely inconsistent with the measurements. Our findings highlight the complexity of three-dimensional radiation paths and dissipation map of internal tides in the Mariana area. © 2021. American Geophysical Union. All Rights Reserved. |
英文关键词 | Abyssal Ocean; energy; internal tide; Mariana Arc; numerical |
语种 | 英语 |
来源期刊 | Journal of Geophysical Research: Oceans
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文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/186329 |
作者单位 | CAS Key Laboratory of Ocean Circulation and Waves, Institute of Oceanology Chinese Academy of Sciences, Qingdao, China; Pilot National Laboratory for Marine Science and Technology, Qingdao, China; Center for Ocean Mega-Science, Chinese Academy of Sciences, Qingdao, China; College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing, China; CAS Engineering Laboratory for Marine Ranching, Institute of Oceanology, Chinese Academy of Sciences, Qingdao, China; China-Asean College of Marine Science, Xiamen University Malaysia, Sepang, Malaysia; Polar Research Institute of China, Shanghai, China |
推荐引用方式 GB/T 7714 | Zhao C.,Xu Z.,Robertson R.,et al. The Three-Dimensional Internal Tide Radiation and Dissipation in the Mariana Arc-Trench System[J],2021,126(5). |
APA | Zhao C.,Xu Z.,Robertson R.,Li Q.,Wang Y.,&Yin B..(2021).The Three-Dimensional Internal Tide Radiation and Dissipation in the Mariana Arc-Trench System.Journal of Geophysical Research: Oceans,126(5). |
MLA | Zhao C.,et al."The Three-Dimensional Internal Tide Radiation and Dissipation in the Mariana Arc-Trench System".Journal of Geophysical Research: Oceans 126.5(2021). |
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