On the mother bodies of steady polygonal uniform vortices. Part I: numerical experiments

IF 1.1 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
G. Riccardi
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引用次数: 0

Abstract

ABSTRACT The existence of an integral relation between self-induced velocity of a uniform, planar vortex and Schwarz function of its boundary opens the way to understand the kinematics of the vortex by analysing the internal singularities of that function. In general, they are branch cuts and form the so-called “mother body” of the vortex, because they generate the same external velocities of the vortex, by means of a relation identical to the Biot–Savart law for a vortex sheet. The jump of the Schwarz function across the cuts plays the role of the (complex) density of circulation. This paper investigates the singularities of polygonal vortices, which are highly nontrivial steady vortices widely present in Nature, and having fascinating properties, some of them still not well understood. By means of the equation of the dynamics of the Schwarz function specialised for steady vortices, a numerical tool based on elementary properties of the holomorphic functions is used for detecting the internal singularities and evaluating their strengths. In this way, it is shown that an nagonal vortex possesses n internal branch cuts. In a reference system having origin on the centre of vorticity of the vortex and real axis crossing one of its vertices, these cuts start from the origin and are directed along the n roots of the unity, so that they are aligned with the vertices. The positions of the branch points and the values assumed by the Schwarz function in these points are calculated by evaluating this function just outside the vortex boundary. Once the conditions on the branch points are defined, a power series representation of the Schwarz function is proposed, that is able to explain the behaviour of its real and imaginary parts in neighbourhoods of these points. Some conjectures about the external singularities are also discussed.
在稳定多边形均匀涡的母体上。第一部分:数值实验
均匀平面涡的自激速度与其边界的Schwarz函数之间的积分关系的存在,为通过分析该函数的内部奇点来理解涡的运动学开辟了道路。一般来说,它们是分支,形成所谓的涡旋“母体”,因为它们产生相同的涡旋外部速度,其关系与涡旋片的比奥-萨瓦定律相同。施瓦兹函数在切口上的跳跃起着循环(复)密度的作用。本文研究了自然界中广泛存在的高度非平凡的稳定涡旋的奇异性,它们具有令人着迷的性质,其中一些还没有被很好地理解。利用稳定涡专用的Schwarz函数的动力学方程,利用全纯函数的初等性质,利用数值工具检测内部奇异性并评价其强度。由此可见,一个非涡旋具有n个内部分支切割。在一个原点在漩涡涡度中心的参考系中,实轴穿过它的一个顶点,这些切割从原点开始,沿着单位的n根方向,这样它们就与顶点对齐了。分支点的位置和Schwarz函数在这些点上的假设值是通过在涡边界外计算该函数来计算的。一旦定义了分支点上的条件,就提出了Schwarz函数的幂级数表示,它能够解释其实部和虚部在这些点的邻域内的行为。讨论了关于外部奇异性的一些猜想。
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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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