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首页> 外文期刊>Izvestiya Atmospheric and Oceanic Physics >The Structure of the Tidal Mixing Front in the Region of Shantar Islands (Sea of Okhotsk) According to Data of Satellite Observations
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The Structure of the Tidal Mixing Front in the Region of Shantar Islands (Sea of Okhotsk) According to Data of Satellite Observations

机译:根据卫星观测数据,在Santar群岛(鄂霍次克海)地区的潮汐混合锋面结构

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摘要

The location and seasonal variability of the tidal mixing front in the region of Shantar Islands are studied based on an analysis of satellite data. The Shantar tidal mixing front is related to the main features of the oceanographic structure of the northwestern shelf of the Sea of Okhotsk in summer. This front separates the coastal waters mixed by tidal currents and the stratified part of the shelf. The temperature tidal mixing front forms in July after the melting ice cover and disappears in the end of October when the stratification is broken. The mean position of the front changes insignificantly and is determined by the critical value of the Simpson—Hunter parameter (logh/u3 = 2.5); the front is located over the isobath of 50 m. The temperature tidal mixing front corresponds to the front in the distribution of chlorophyll a determined from SeaWiFS and MODIS satellite imagery. High (when compared to the stratified part of the shelf) concentrations of chlorophyll a were observed within the zone of intense tidal mixing. Satellite images in the IR range of the spectrum (Landsat-5 TM) demonstrated that the front is dynamically unstable. Mixing effects connected with frontal submesoscale baroclinic eddies have an influence on the structure of the stratified part of the shelf.
机译:在分析卫星数据的基础上,研究了香塔尔群岛地区潮汐混合锋的位置和季节变化。 Shantar潮汐混合前沿与夏季鄂霍次克海西北陆架海洋结构的主要特征有关。这条前沿将潮汐混合的沿海水域和架子的分层部分分开。温度潮汐混合前沿在融化的冰层覆盖后的七月形成,并在十月底分层破裂时消失。前沿的平均位置变化不大,由Simpson-Hunter参数的临界值确定(logh / u3 = 2.5);正面位于等高线50 m上方。潮汐温度混合前沿对应于从SeaWiFS和MODIS卫星图像确定的叶绿素a分布的前沿。在强烈的潮汐混合区域内观察到了较高的叶绿素a浓度(与货架的分层部分相比)。红外光谱范围内的卫星图像(Landsat-5 TM)表明,前缘是动态不稳定的。与额中亚尺度斜斜涡旋相关的混合效应对架子分层部分的结构有影响。

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