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Modeling the barrier-layer formation in the southeastern Arabian Sea

机译:模拟阿拉伯海东南部的障碍层形成

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摘要

The effect of salinity on the formation of the barrier layer (BL) in the southeastern Arabian Sea (SEAS) is investigated using an ocean general circulation model. In accordance with previous studies, the runoff distribution and the India–Sri Lanka passage have a strong impact on the realism of the salinity simulated in the area at seasonal time scales. The model simulates a BL pattern in fairly good agreement with available observations. Eulerian and Lagrangian approaches show that the BL is formed by two complementary processes, the arrival of low-salinity surface waters that are cooled en route to the SEAS and downwelling of waters mostly local to the SEAS in the subsurface layers. The surface waters are partly of Bay of Bengal origin and are partly from the SEAS, but are cooled east and south of Sri Lanka in the model. That the downwelled subsurface waters are warm and are not cooled leads to temperature inversions in the BL. The main forcing for this appears to be remotely forced planetary waves.
机译:使用海洋总环流模型研究了盐度对阿拉伯东南海(SEAS)屏障层(BL)形成的影响。根据先前的研究,径流分布和印度-斯里兰卡通道对季节性时标对该地区模拟的盐度的真实性有很大影响。该模型模拟的BL模式与可用的观测值相当吻合。欧拉和拉格朗日方法表明,BL是由两个互补过程形成的:低盐度地表水的到达,这些地表水在进入SEAS的途中被冷却,而下层地层的水大多位于SEAS下方。地表水部分来自孟加拉湾,部分来自SEAS,但在模型中被冷却至斯里兰卡的东部和南部。下涌的地下水是温暖的,而不是被冷却的,这导致BL中的温度反转。造成这种现象的主要因素似乎是遥远强迫的行星波。

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