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Formation and variability of the Lofoten basin vortex in a high-resolution ocean model

机译:高分辨率海洋模型中罗弗敦海盆涡的形成和变化

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The Lofoten Basin of the Norwegian Sea is characterized by a local maximum of eddy kinetic energy and it is an important transit region for the warm and saline Atlantic waters on their way towards the Arctic Ocean. Eddies are generated by the Norwegian Atlantic Current and propagate anticlockwise around the center of the basin. In situ and satellite observations have discovered a rather small (with a radius of a few tens of km), but strong quasi-permanent anticyclonic vortex that resides in the center of the Lofoten Basin near 3 degrees E, 69.8 degrees N. The objective of this paper is to understand how and why the vortex is formed and to investigate what processes support its stability and drive its variability. To achieve this objective, we have conducted three high-resolution numerical experiments with the mean horizontal grid spacing of 18 km, 9 km, and 4 km. The Lofoten Vortex did not form in the 18-km experiment. The most realistic (compared to available observations) simulation of the vortex is provided by the 4-km experiment, which better reproduces eddy variability in the region. The experiments thus provide experimental evidence of the importance of eddies in the formation and stability of the vortex. We demonstrate how anticyclonic eddies, that are usually stronger and more numerous in the basin than cyclonic eddies, contribute to the intensification of the Lofoten Vortex. The Lofoten Vortex itself is not stationary and drifts cyclonically within the area bounded by approximately the 3250 m isobath. The analysis of the barotropic vorticity budget in the 4-km experiment shows that the advection of the relative vorticity gradient by eddies is the main mechanism that drives the variability of the Lofoten Vortex. The direct impact of wind/buoyancy forcing is found to be small to negligible. (C) 2015 Elsevier Ltd. All rights reserved.
机译:挪威海的罗弗敦海域以涡动能局部最大为特征,它是温暖和咸的大西洋水向北冰洋航行的重要过境区。涡流是由挪威大西洋洋流产生的,并沿盆地中心逆时针传播。实地和卫星观测发现了一个很小的半径(半径为几十公里),但是强的准永久性反气旋涡流位于罗弗敦盆地的中部,东经3度,北纬69.8度。本文旨在了解涡流的形成方式和原因,并研究哪些过程支持其稳定性并驱动其可变性。为了实现这一目标,我们进行了三个高分辨率数值实验,平均水平网格间距为18 km,9 km和4 km。在18公里的实验中并未形成Lofoten涡流。 4 km实验提供了最现实的涡流模拟(与可用的观测值相比),该模拟可以更好地再现该区域的涡流变异性。因此,实验提供了涡旋形成和稳定性中涡旋重要性的实验证据。我们展示了通常比盆地中的旋风涡旋更强,数量更多的反旋风涡旋对罗弗敦涡流的强化作用。 Lofoten涡流本身不是静止的,而是在大约3250 m等深线所包围的区域内旋流漂移。对4 km实验中正压涡度预算的分析表明,涡旋对流的相对涡度是推动Lofoten涡旋变化的主要机制。发现风/浮力的直接影响很小甚至可以忽略不计。 (C)2015 Elsevier Ltd.保留所有权利。

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