透镜状反气旋在线性分层旋转流体中的聚合

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Geophysical and Astrophysical Fluid Dynamics Pub Date : 2020-03-18 DOI:10.1080/03091929.2020.1734199
A. Orozco Estrada, R. C. Cruz Gómez, A. Cros, P. Le Gal
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引用次数: 4

摘要

本研究致力于线性分层旋转流体中两个透镜状反气旋合并的实验室实验。这些反气旋是通过在旋转槽的中心注入小体积的流体来产生的,在旋转槽的中心,先前用盐制备了线性分层层。利用可视化和粒子图像测速(PIV)技术研究了涡旋间初始分离距离、旋转台科里奥利参数和Brünt-Väisälä密度分层频率对涡旋间相互作用特性的影响。我们的结果表明,合并的临界距离很大程度上取决于涡的变形的罗斯比半径,并与以前的涡合并的数值模拟完全一致。我们还观察到,合并涉及三维过程,因为涡旋缠绕在一起,可能是因为椭圆不稳定性的存在使涡旋核心倾斜。它们还伴随着涡度细丝和内部重力波辐射的发射,尽管我们无法证明在我们的实验中这些波仅仅是由于合并过程。
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Coalescence of lenticular anticyclones in a linearly stratified rotating fluid
This study is devoted to laboratory experiments on the coalescence of two lenticular anticyclones in a linearly stratified rotating fluid. These anticyclones are generated by injecting small volumes of fluid at the centre of a rotating tank where a linearly stratified layer was previously prepared with salt. The characteristics of the interaction between the vortices are studied by visualisation and Particle Image Velocimetry (PIV) as a function of the initial separation distance between the vortices, the Coriolis parameter of the rotating table and the Brünt-Väisälä frequency of the density stratification. Our results show that the merging critical distance depends drastically on the Rossby radius of deformation of the vortices and are in complete agreement with previous numerical modelling of vortex coalescence. We have also observed that mergers involve three-dimensional processes as the vortices intertwine together possibly because of the presence of an elliptic instability that tilts the vortex cores. They are also accompanied by the emission of vorticity filaments and internal gravity waves radiation although we cannot prove that in our experiments these waves are solely due to the merging process.
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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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