Parametric Subharmonic Instability of the M2 Internal Tides in the Tokara Strait

IF 3.3 2区 地球科学 Q1 OCEANOGRAPHY
Shuya Wang, Xinyu Guo, Anzhou Cao, Eisuke Tsutsumi, Xu Chen
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Abstract

The Tokara Strait is a mixing hotspot due to the coexistence of complex bottom topographies and strong composite flow including both the Kuroshio and tidal currents. Although previous studies have revealed several mechanisms from the view of Kuroshio-Topography interaction, the role of tides in driving mixing is still not clear. Given that it is located at the M2 critical latitude (29°N), parametric subharmonic instability (PSI) is expected as an important process responsible for the mixing. Here, we study PSI of the M2 internal tides in the Tokara Strait based on a high-resolution model. Our model results indicate that intense near-inertial waves are generated via PSI, which exhibit a horizontally layered structure and have much larger vertical wavenumbers than the M2 internal tides. Energy is transferred from the M2 internal tides to the near-inertial waves around the generation sites, and most of the near-inertial energy is dissipated locally. The dissipation rates of near-inertial waves are comparable to those of the M2 internal tides. Simulations with and without the Kuroshio Current revealed the suppression of PSI along the Kuroshio path, which could be attributed to two mechanisms. First, the Kuroshio Current modifies the local minimum internal wave frequency by its horizontal and vertical shear, making the condition for PSI not satisfied. Second, the Kuroshio Current advects the near-inertial waves downstream in the Okinawa Trough, which inhibits the accumulation of near-inertial energy there. However, in most of the areas outside the Kuroshio path, PSI majorly contributes to mixing in and around the Tokara Strait.

Abstract Image

托卡拉海峡 M2 内潮的参数次谐波不稳定性
由于复杂的海底地形与包括黑潮和潮汐流在内的强大复合流共存,十卡拉海峡是一个混合热点。尽管之前的研究从黑潮与地形相互作用的角度揭示了几种机制,但潮汐在驱动混合中的作用仍不明确。鉴于黑潮位于 M2 临界纬度(29°N),参数次谐波不稳定性(PSI)有望成为造成混合的一个重要过程。在此,我们基于高分辨率模型研究了托卡拉海峡 M2 内潮的 PSI。我们的模型结果表明,强烈的近惯性波是通过 PSI 产生的,它呈现出水平分层结构,垂直波数比 M2 内潮大得多。能量从 M2 内潮传递到生成点周围的近惯性波,大部分近惯性波能量在局部消散。近惯性波的耗散率与 M2 内潮的耗散率相当。在有黑潮和没有黑潮的情况下进行的模拟显示,沿黑潮路径的 PSI 受到了抑制,这可归因于两种机制。首先,黑潮通过其水平和垂直切变改变了当地的最小内波频率,使得 PSI 的条件无法满足。其次,黑潮将冲绳海槽的近惯性波向下游平移,抑制了近惯性能量在该海槽的积累。然而,在黑潮路径以外的大部分地区,PSI 主要促成了托卡拉海峡及其周围地区的混合。
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来源期刊
Journal of Geophysical Research-Oceans
Journal of Geophysical Research-Oceans Earth and Planetary Sciences-Oceanography
CiteScore
7.00
自引率
13.90%
发文量
429
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