The evolution of a localized nonlinear wave of the Kelvin―Helmholtz instability with gravity
At the interface between two fluids of different density and in the presence of gravity, there are well known periodic surface waves which can propagate for long distances with little attenuation, as it is for instance the case at the surface of the sea. If wind is present, these waves progressively...
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Published in | Physics of fluids (1994) Vol. 24; no. 11 |
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Main Authors | , |
Format | Journal Article |
Language | English |
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Melville, NY
American Institute of Physics
01.11.2012
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Abstract | At the interface between two fluids of different density and in the presence of gravity, there are well known periodic surface waves which can propagate for long distances with little attenuation, as it is for instance the case at the surface of the sea. If wind is present, these waves progressively accumulate energy as they propagate and grow to large sizes-this is the Kelvin-Helmholtz instability. On the other hand, we show in this paper that for a given wind strength, there is potential for the growth of a localized nonlinear wave. This wave can reach a size such that the hydrostatic pressure drop from top to bottom equals the stagnation pressure of the wind. This process for the disruption of the flat interface is localized and nonlinear. We study the properties of this wave using numerical simulations of the Navier-Stokes equations. |
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AbstractList | At the interface between two fluids of different density and in the presence of gravity, there are well known periodic surface waves which can propagate for long distances with little attenuation, as it is for instance the case at the surface of the sea. If wind is present, these waves progressively accumulate energy as they propagate and grow to large sizes-this is the Kelvin-Helmholtz instability. On the other hand, we show in this paper that for a given wind strength, there is potential for the growth of a localized nonlinear wave. This wave can reach a size such that the hydrostatic pressure drop from top to bottom equals the stagnation pressure of the wind. This process for the disruption of the flat interface is localized and nonlinear. We study the properties of this wave using numerical simulations of the Navier-Stokes equations. |
Author | ORAZZO, Annagrazia HOEPFFNER, Jérôme |
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Cites_doi | 10.1017/S0022112057000567 10.1098/rspa.1979.0009 10.1017/S0022112078002189 10.1017/S002211207400190X 10.1098/rspa.1931.0115 10.1146/annurev.fl.11.010179.000523 10.1017/S0022112067000941 10.1615/AtomizSpr.2012004148 10.1146/annurev.fl.16.010184.002053 10.1016/S0167-2789(97)00045-6 10.1063/1.1693419 10.1017/S0022112071000557 10.1063/1.1693456 10.1017/S0022112076001353 10.1146/annurev.fl.22.010190.002353 10.1017/S0022112001003652 10.1098/rsta.1979.0019 10.1080/14786447108640585 10.1016/j.jcp.2009.04.042 10.1017/S0022112069002023 10.1017/S0022112074001121 10.1017/S0022112000002706 10.1103/PhysRevLett.106.104502 10.1016/0167-2789(89)90150-4 10.1080/14786446808640073 10.1017/S0022112086001842 10.1017/S0022112059000842 10.1007/BF02079924 10.1088/0034-4885/71/3/036601 |
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Phys. doi: 10.1088/0034-4885/71/3/036601 |
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SubjectTerms | Computational fluid dynamics Density Earth, ocean, space Exact sciences and technology External geophysics Fluid flow Fluids Gravitation Mathematical analysis Navier-Stokes equations Nonlinearity Physics of the oceans Sea-air exchange processes |
Title | The evolution of a localized nonlinear wave of the Kelvin―Helmholtz instability with gravity |
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