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1. |
On the dissipation of internal solitons in coastal seas |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 85,
Issue 3-4,
1997,
Page 163-194
PatrickG. Timko,
GordonE. Swaters,
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摘要:
Previous descriptions of the turbulent decay of an internal soliton have been based on an adiabatic assumption in which the soliton parameters continuously change in time in response to the dissipation. A complete leading order description of a decaying internal soliton including both horizontal and vertical dissipation is given. It is shown that the adiabatic ansatz fails to fully describe a decaying internal soliton under the influence of weak dissipation. Physically, the breakdown is the consequence of the fact that an adiabatically decaying internal soliton is unable to simultaneously satisfy averaged energyandmass balance relations. An extended region with vertical momentum flux develops behind the decaying soliton in order to compensate for the additional mass lost in the adiabatically decaying internal soliton. The leading order evolution of this extended region is described as is its connection to the stream function field associated with the internal soliton. The magnitude of the vertical flux associated with this region scales linearly with the dissipation parameters. The transition of this extended region back to zero is accomplished through the formation of a spatially decaying packet of linear internal gravity waves.
ISSN:0309-1929
DOI:10.1080/03091929708208988
出版商:Taylor & Francis Group
年代:1997
数据来源: Taylor
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2. |
Temporal variability of the wind-driven quasi-geostrophic double gyre ocean circulation: Basic bifurcation diagrams |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 85,
Issue 3-4,
1997,
Page 195-232
HenkA. Dijkstra,
CarolineA. Katsman,
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摘要:
In this paper we explore how temporal variability arises through successive bifurcations of the symmetric wind-driven double gyre circulation as lateral friction is decreased in 1.5-layer and 2-layer quasi geostrophic models. In the 1.5-layer model, the symmetric double gyre flow becomes unstable to symmetry breaking stationary instabilities, leading to asymmetric flows. These asymmetric solutions subsequently destabilize to two sets of barotropic oscillatory modes, introducing an intermonthly and interannual time scale, respectively. In the 2-layer model, the symmetric double gyre solution becomes unstable to baroclinic oscillatory instabilities, giving rise to near annual temporal variability. The asymmetric solutions which appear through symmetry breaking at smaller lateral friction, are in this case all unstable.
ISSN:0309-1929
DOI:10.1080/03091929708208989
出版商:Taylor & Francis Group
年代:1997
数据来源: Taylor
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3. |
On dimensions of attractive sets of viscous fluids on a sphere under quasi-periodic forcing |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 85,
Issue 3-4,
1997,
Page 233-242
YuriN. Skiba,
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摘要:
Simple attractive sets of a viscous incompressible fluid on a sphere under quasi-periodic polynomial forcing are considered. Each set is the vorticity equation (VE) quasi-periodic solution of the complex (2n+ 1)-dimensional subspaceHnof homogeneous spherical polynomials of degreen. The Hausdorff dimension of its path being an open spiral densely wound around a2n-dimensional torus inHn, equals to 2n. As the generalized Grashof numbGbecomes small enough then the basin of attraction of such spiral solution is expanded fromHnto the entire VE phase space. It is shown that for givenG, there exists an integernGsuch that each spiral solution generated by a forcing ofHnwithn≥nGis globally asymptotically stable. Thus, whereas the dimension of the fluid attractor under a stationary forcing is limited above byG, the dimension of the spiral attractive solution (equal to 2n) may, for a fixedG, become arbitrarily large as the degreenof the quasi-periodic polynomial forcing grows. Since the small scale quasi-periodic functions, unlike the stationary ones, more adequately depict the barotropic atmosphere forcing, this result is of meteorological interest and shows that the dimension of attractive sets depends not only on the forcing amplitude, but also on its spatial and temporal structure.
ISSN:0309-1929
DOI:10.1080/03091929708208990
出版商:Taylor & Francis Group
年代:1997
数据来源: Taylor
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4. |
Hopf-Hopf and Hopf-Steady mode interactions with O(2) symmetry in Langmuir circulations |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 85,
Issue 3-4,
1997,
Page 243-278
T. Allen,
I.M. Moroz,
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摘要:
In this paper the nonlinear stability of two-dimensional Langmuir circulations in a fluid layer, stratified by vertical thermal and salinity gradients, is investigated when two distinct wavenumbers become simultaneously unstable. These instabilities take the form of O(2) symmetric Hopf-Hopf and Hopf-Steady bifurcations when the lateral boundary conditions are assumed to be periodic. In the analysis of the Hopf-Hopf bifurcation a disagreement with the group theoretic work of Chossatet al.(1986) is found. This difference is resolved by correcting the lattice of Isotropy subgroups presented by Chossatet al.(1986) and by considering the effects of the higher order terms in the amplitude evolution equations.
ISSN:0309-1929
DOI:10.1080/03091929708208991
出版商:Taylor & Francis Group
年代:1997
数据来源: Taylor
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5. |
A fast dynamo of αω-type |
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Geophysical & Astrophysical Fluid Dynamics,
Volume 85,
Issue 3-4,
1997,
Page 279-314
A.D. Gilbert,
A.M. Soward,
S. Childress,
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ISSN:0309-1929
DOI:10.1080/03091929708208992
出版商:Taylor & Francis Group
年代:1997
数据来源: Taylor
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