Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-05T14:49:42.286Z Has data issue: false hasContentIssue false

Stationary ideal flow on a free surface of a given shape

Published online by Cambridge University Press:  13 March 2013

L. Tophøj
Affiliation:
Physics Department & Center for Fluid Dynamics, The Technical University of Denmark, Kgs. Lyngby, DK-2800, Denmark
T. Bohr*
Affiliation:
Physics Department & Center for Fluid Dynamics, The Technical University of Denmark, Kgs. Lyngby, DK-2800, Denmark
*
Email address for correspondence: [email protected]

Abstract

We study the stationary, ideal flow on a free fluid surface with a prescribed shape. It is demonstrated that the flow is governed by a self-contained set of equations for the surface flow field without any reference to the bulk flow. To write down these equations for arbitrary surfaces, we apply a covariant formulation using Riemannian geometry and we show how to include surface tension and velocity-dependent forces such as the Coriolis force. We write down explicitly the equations for cases where the surface elevation can be written as function of either Cartesian or polar coordinates in the plane, and we obtain solutions for the important case of rotational symmetry and the perturbed flow when this symmetry is slightly broken. To understand the general character and solubility of the equations, we introduce the associated dynamical system describing the motion along the streamlines. The existence of orbits with transversal intersections, as well as quasi-periodic and chaotic solutions, show that not all boundary value problems are well-posed. In the particular case of unforced motion the streamlines are geodesic curves and in this case the existence of a non-trivial surface velocity field requires that the surface can be foliated by a family of non-intersecting geodesic curves.

Type
Papers
Copyright
©2013 Cambridge University Press

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Aris, R. 1962 Vectors, Tensors and the Basic Equations of Fluid Mechanics. Prentice Hall.Google Scholar
Arnold, V. I. 1978 Mathematical Methods of Classical Mechanics. Springer.Google Scholar
Bergmann, R., Tophøj, L., Homan, T. A. M., Hersen, P., Andersen, A. & Bohr, T. 2011 Polygon formation and surface flow on a rotating fluid surface. J. Fluid Mech. 679, 415431.Google Scholar
do Carmo, M. P. 1976 Differential Geometry of Curves and Surfaces. Prentice-Hall.Google Scholar
Carroll, S. 2003 Spacetime and Geometry: An Introduction to General Relativity. Pearson.Google Scholar
Courant, R. & Hilbert, D. 1989 Methods of Mathematical Physics. Wiley.Google Scholar
Ilin, A. A. 1991 The Navier–Stokes and Euler equations of two-dimensional closed manifolds. Math. USSR Sb. 69, 559579.CrossRefGoogle Scholar
Lebedev, L. P., Cloud, M. J. & Eremeyev, V. A. 2010 Tensor Analysis with Applications in Mechanics. World Scientific.Google Scholar
Ott, E. 1993 Chaos in Dynamical Systems. Cambridge University Press.Google Scholar
Ray, R. D. 2001 Inversion of oceanic tidal currents from measured elevations. J. Mar. Syst. 28 (1–2), 118.Google Scholar
Stoker, J. J. 1969 Differential Geometry. Wiley.Google Scholar