Energy Characteristics of the Marmara Sea Water Circulation in 2008

IF 0.7 Q4 OCEANOGRAPHY Physical Oceanography Pub Date : 2019-07-01 DOI:10.22449/0233-7584-2019-4-307-321
S. Demyshev, S. V. Dovgaya, M. Shokurov
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引用次数: 1

Abstract

Purpose. The main objectives of the study consisted in analyzing the Marmara Sea energy and in identifying the basic reasons for formation of its circulation features in 2008. Methods and Results. The numerical experiment on modeling the Marmara Sea circulation and evaluating its energy characteristics on the example of 2008 was carried out based on the eddyresolving nonlinear hydrodynamic model of Marine Hydrophysical Institute, RAS. The horizontal resolution of the model was 1.22 × 0.83 km, 18 horizons were used over vertical and the time step was 0.5 min. Temperature, salinity and water discharge through the Bosporus and the Dardanelles were preset according to the available measurement data. The applied fields of atmospheric forcing were obtained from the calculation by the regional atmospheric model MM5. The volume-integrated and year-averaged contributions of the terms in the equations of the kinetic and potential energy budgets were analyzed. The basic factors of change in the Marmara Sea kinetic energy consisted in the buoyancy force action, wind, and vertical and horizontal mixing. Having been analyzed, the volume-average summands in the equation of rate of the kinetic energy change have shown that the wind-induced energy influx was compensated mainly by vertical friction, and the buoyancy force action – by horizontal friction. On the average, in course of a year the potential energy changed mainly due to its horizontal transport conditioned by the effect of the currents located in front of the straits, vertical diffusion and the buoyancy force impact. The results of analysis of the energy transitions permitted to reveal that in the upper sea layer, the mesoscale vortices were formed directly under the wind influence and as a result of the currents’ baroclinic instability. Generation of the submesoscale vortices in the coastal regions was affected predominantly by the processes of baroclinic instability. In the region near the Bosporus, increase of the horizontal gradients in the density field and, consequently, intensification of dynamic processes are the results of inflow of the Black Sea waters with lower density. Conclusions. Study of the energy characteristics of the Marmara Sea water circulation permitted to conclude that baroclinic instability and wind are two of the basic sources of eddy formation in this basin.
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2008年马尔马拉海水环流的能量特征
目的。研究的主要目的是分析马尔马拉海的能量,并确定其2008年环流特征形成的基本原因。方法与结果。以2008年为例,基于英国科学院海洋水物理研究所的涡流解析非线性水动力模型,对马尔马拉海环流进行了数值模拟和能量特性评价。模式的水平分辨率为1.22 × 0.83 km,垂直上使用18层,时间步长为0.5 min。根据现有的测量数据预置博斯普鲁斯海峡和达达尼尔海峡的温度、盐度和水量。利用区域大气模式MM5计算得到了大气强迫的作用场。分析了动力学和势能收支方程中各项的体积积分贡献和年平均贡献。马尔马拉海动能变化的基本因素是浮力作用、风、垂直和水平混合。经分析,动能变化率方程的体积-平均总和表明,风致能量流入主要由垂直摩擦补偿,浮力主要由水平摩擦补偿。平均来看,在一年的过程中,势能的变化主要是受海峡前气流的作用、垂直扩散和浮力的影响下的水平输送。能量转换分析结果表明,在上层,中尺度涡旋是在风的直接影响下形成的,是气流斜压不稳定的结果。沿海地区亚中尺度涡的产生主要受斜压不稳定过程的影响。在博斯普鲁斯海峡附近区域,密度场水平梯度的增大,从而导致动力过程的加剧,是低密度黑海海水流入的结果。结论。通过对马尔马拉海水环流能量特征的研究,得出斜压不稳定性和风是该盆地涡旋形成的两个基本来源的结论。
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来源期刊
Physical Oceanography
Physical Oceanography OCEANOGRAPHY-
CiteScore
1.80
自引率
25.00%
发文量
8
审稿时长
24 weeks
期刊最新文献
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