Topographic instability of flow in a rotating fluid

Here are presented the results of experimental and theoretical studies on a stability of zonal geostrophic flows in the rotating layer of the shallow water. In the experiments, a special apparatus by Abastumani Astrophysical Observatory Georgian Academy of Science was used. This apparatus represents...

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Main Authors: K. I. Patarashvili, Z. J. Tsakadze, M. V. Kalashnik, V. O. Kakhiani, R. J. Chanishvili, J. I. Nanobashvili, M. A. Zhvania
Format: Article
Language:English
Published: Copernicus Publications 2006-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/13/231/2006/npg-13-231-2006.pdf
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spelling doaj-1be6a989354b4a94845809ecb3051c4b2020-11-25T01:27:26ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462006-01-01132231235Topographic instability of flow in a rotating fluidK. I. PatarashviliZ. J. TsakadzeZ. J. TsakadzeM. V. KalashnikV. O. KakhianiR. J. ChanishviliJ. I. NanobashviliM. A. ZhvaniaHere are presented the results of experimental and theoretical studies on a stability of zonal geostrophic flows in the rotating layer of the shallow water. In the experiments, a special apparatus by Abastumani Astrophysical Observatory Georgian Academy of Science was used. This apparatus represents a paraboloid of rotation, which can be set in a regulable rotation around the vertical axis. Maximal diameter of the paraboloid is 1.2 m, radius of curvature in the pole is 0.698 m. In the paraboloid, water spreads on walls as a layer uniform on height under the period of rotation 1.677 s. Against a background of the rotating fluid, the zonal flows are formed by the source-sink system. It consists of two concentric circular perforations on the paraboloid bottom (width is 0.3 cm, radiuses are 8.4 and 57.3 cm, respectively); water can be pumped through them with various velocities and in all directions. It has been established that under constant vertical depth of the rotating fluid the zonal flows are stable. There are given the measurements of the radial profiles for the water level and velocity in the stationary regime. It has been found that zonal flows may lose stability under the presence of the radial gradient of full depth formed by a change of angular velocity of paraboloid rotation. An instability origin results in the loss of flow axial symmetry and in the appearance of self-excited oscillations in the zonal flow. At the given angular velocity of rotation, instability is observed only in the definite range of intensities of the source-sink system. The theoretical estimations are performed in the framework of the equations of the shallow water theory, including the terms describing the bottom friction. It has been shown that the instability of zonal flows found experimentally has a topographical nature and is related with non-monotone dependence of the potential vorticity on radius.http://www.nonlin-processes-geophys.net/13/231/2006/npg-13-231-2006.pdf
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language English
format Article
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author K. I. Patarashvili
Z. J. Tsakadze
Z. J. Tsakadze
M. V. Kalashnik
V. O. Kakhiani
R. J. Chanishvili
J. I. Nanobashvili
M. A. Zhvania
spellingShingle K. I. Patarashvili
Z. J. Tsakadze
Z. J. Tsakadze
M. V. Kalashnik
V. O. Kakhiani
R. J. Chanishvili
J. I. Nanobashvili
M. A. Zhvania
Topographic instability of flow in a rotating fluid
Nonlinear Processes in Geophysics
author_facet K. I. Patarashvili
Z. J. Tsakadze
Z. J. Tsakadze
M. V. Kalashnik
V. O. Kakhiani
R. J. Chanishvili
J. I. Nanobashvili
M. A. Zhvania
author_sort K. I. Patarashvili
title Topographic instability of flow in a rotating fluid
title_short Topographic instability of flow in a rotating fluid
title_full Topographic instability of flow in a rotating fluid
title_fullStr Topographic instability of flow in a rotating fluid
title_full_unstemmed Topographic instability of flow in a rotating fluid
title_sort topographic instability of flow in a rotating fluid
publisher Copernicus Publications
series Nonlinear Processes in Geophysics
issn 1023-5809
1607-7946
publishDate 2006-01-01
description Here are presented the results of experimental and theoretical studies on a stability of zonal geostrophic flows in the rotating layer of the shallow water. In the experiments, a special apparatus by Abastumani Astrophysical Observatory Georgian Academy of Science was used. This apparatus represents a paraboloid of rotation, which can be set in a regulable rotation around the vertical axis. Maximal diameter of the paraboloid is 1.2 m, radius of curvature in the pole is 0.698 m. In the paraboloid, water spreads on walls as a layer uniform on height under the period of rotation 1.677 s. Against a background of the rotating fluid, the zonal flows are formed by the source-sink system. It consists of two concentric circular perforations on the paraboloid bottom (width is 0.3 cm, radiuses are 8.4 and 57.3 cm, respectively); water can be pumped through them with various velocities and in all directions. It has been established that under constant vertical depth of the rotating fluid the zonal flows are stable. There are given the measurements of the radial profiles for the water level and velocity in the stationary regime. It has been found that zonal flows may lose stability under the presence of the radial gradient of full depth formed by a change of angular velocity of paraboloid rotation. An instability origin results in the loss of flow axial symmetry and in the appearance of self-excited oscillations in the zonal flow. At the given angular velocity of rotation, instability is observed only in the definite range of intensities of the source-sink system. The theoretical estimations are performed in the framework of the equations of the shallow water theory, including the terms describing the bottom friction. It has been shown that the instability of zonal flows found experimentally has a topographical nature and is related with non-monotone dependence of the potential vorticity on radius.
url http://www.nonlin-processes-geophys.net/13/231/2006/npg-13-231-2006.pdf
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