用有限尺寸Lyapunov指数分析亚得里亚海的混合结构

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2021-08-27 DOI:10.1080/03091929.2021.1962851
S. Hariri
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引用次数: 2

摘要

本文报道了2006年10月至2011年12月亚得里亚海作为地中海半封闭海盆的混合结构和输运性质。拉格朗日输运模式用于模拟由麻省理工学院亚得里亚海通用环流模式得到的平均流场的合成轨迹。我们通过计算亚得里亚海每年选定月份的时间平均有限尺寸李雅普诺夫指数(FSLEs)来研究数值对粒子的色散特性。结果表明,河流径流和风强迫,特别是Bora风场,通过涡的产生对数值对粒子的混合活动有显著影响,涡在FSLE图上表现为缠结的细丝。包含高FSLEs值的拉伸/压缩线作为坚固的运输屏障,大多数在亚得里亚海东侧和西侧的边界流中被检测到,特别是在冬季。数值实验表明,每年6月和9月,亚得里亚海北部出现稳定的流动,混合活动较少,而南部亚得里亚海坑受来自爱奥尼亚海的风和高能流的影响,季节性波动较大,涡流动能值较高。
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Analysis of mixing structures in the Adriatic Sea using finite-size Lyapunov exponents
In this paper, we report on the mixing structures and transport properties of the Adriatic Sea surface, as a semi-enclosed basin of the Mediterranean Sea, from October 2006 until December 2011. Lagrangian transport models were used to simulate synthetic trajectories from the mean flow fields obtained by the Massachusetts Institute of Technology general circulation model implemented for the Adriatic. We examine the dispersion properties of numerical pair particles, through the calculation of time-averaged finite-size Lyapunov exponents (FSLEs) in the Adriatic Sea during selected months in each year. The results show the significant effects of river runoff and wind forcing, especially the Bora wind field, on the mixing activities of numerical pair particles by the generation of vortices, which appear as a tangle of filaments on the FSLE maps. The stretch/compression lines, which contain high values of the FSLEs, work as robust transport barriers, most having been detected along boundary currents on the eastern and western flanks of the Adriatic, particularly during winter. Numerical experiments have indicated that stable flows, with less mixing activity, occur in the northern part of the Adriatic in June and September of each year, while the Southern Adriatic Pit has flows with larger seasonal fluctuations and high values of eddy kinetic energy because of the influence of wind and energetic currents entering from the Ionian Sea.
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来源期刊
Geophysical and Astrophysical Fluid Dynamics
Geophysical and Astrophysical Fluid Dynamics 地学天文-地球化学与地球物理
CiteScore
3.10
自引率
0.00%
发文量
14
审稿时长
>12 weeks
期刊介绍: Geophysical and Astrophysical Fluid Dynamics exists for the publication of original research papers and short communications, occasional survey articles and conference reports on the fluid mechanics of the earth and planets, including oceans, atmospheres and interiors, and the fluid mechanics of the sun, stars and other astrophysical objects. In addition, their magnetohydrodynamic behaviours are investigated. Experimental, theoretical and numerical studies of rotating, stratified and convecting fluids of general interest to geophysicists and astrophysicists appear. Properly interpreted observational results are also published.
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