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  • 1
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 1996
    In:  Journal of Fluid Mechanics Vol. 312 ( 1996-04-10), p. 107-124
    In: Journal of Fluid Mechanics, Cambridge University Press (CUP), Vol. 312 ( 1996-04-10), p. 107-124
    Abstract: We describe a mechanistic picture of the essential dynamical processes in the growing Tollmien-Schlichting wave in a Blasius boundary layer and similar flows. This picture depends on the interaction between two component parts of a disturbance (denoted ‘partial modes’), each of which is a complete linear solution in some idealization of the system. The first component is an inviscid mode propagating on the vorticity gradient of the velocity profile with the free-slip boundary condition, and the second, damped free viscous modes in infinite uniform shear with the no-slip condition. There are two families of these viscous modes, delineated by whether the phase lines of the vorticity at the wall are oriented with or against the shear, and they are manifested as resonances in a forced system. The interaction occurs because an initial ‘inviscid’ disturbance forces a viscous response via the no-slip condition at the wall. This viscous response is large near the resonance associated with the most weakly damped viscous mode, and in the unstable parameter range it has suitable phase at the outer part of the boundary layer to increase the amplitude of the inviscid partial mode by advection.
    Type of Medium: Online Resource
    ISSN: 0022-1120 , 1469-7645
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1996
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  • 2
    Online Resource
    Online Resource
    Springer Science and Business Media LLC ; 1997
    In:  Nature Vol. 388, No. 6642 ( 1997-8), p. 518-519
    In: Nature, Springer Science and Business Media LLC, Vol. 388, No. 6642 ( 1997-8), p. 518-519
    Type of Medium: Online Resource
    ISSN: 0028-0836 , 1476-4687
    RVK:
    RVK:
    RVK:
    Language: English
    Publisher: Springer Science and Business Media LLC
    Publication Date: 1997
    detail.hit.zdb_id: 120714-3
    detail.hit.zdb_id: 1413423-8
    SSG: 11
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  • 3
    Online Resource
    Online Resource
    American Meteorological Society ; 1999
    In:  Journal of Climate Vol. 12, No. 10 ( 1999-10), p. 3087-3104
    In: Journal of Climate, American Meteorological Society, Vol. 12, No. 10 ( 1999-10), p. 3087-3104
    Type of Medium: Online Resource
    ISSN: 0894-8755 , 1520-0442
    RVK:
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 1999
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    detail.hit.zdb_id: 2021723-7
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  • 4
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 1999
    In:  The Mathematical Gazette Vol. 83, No. 496 ( 1999-03), p. 187-
    In: The Mathematical Gazette, Cambridge University Press (CUP), Vol. 83, No. 496 ( 1999-03), p. 187-
    Type of Medium: Online Resource
    ISSN: 0025-5572
    Language: Unknown
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1999
    detail.hit.zdb_id: 2262088-6
    SSG: 17,1
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1996
    In:  Journal of Geophysical Research: Oceans Vol. 101, No. C6 ( 1996-06-15), p. 14073-14093
    In: Journal of Geophysical Research: Oceans, American Geophysical Union (AGU), Vol. 101, No. C6 ( 1996-06-15), p. 14073-14093
    Abstract: We present an analysis of the interaction between wind‐driven and thermohaline‐driven circulations in a coarse‐resolution global ocean general circulation model of the Bryan‐Cox code. A series of experiments is described in which the flow is driven by wind forcing only, thermohaline forcing only, or both. In a global ocean with topography, the circulation driven by wind alone is strongly influenced by contours of constant potential vorticity, which limit the barotropic transport to relatively small values. With the same geometry, the flow driven by relaxing to observed surface temperature and salinity fields alone contains deep overturning circulation (producing North Atlantic Deep Water and Antarctic Bottom Water (AABW)) and a large barotropic Antarctic Circumpolar Current (ACC) generated by bottom form stress. The ACC is dependent on the overturning circulation, the deep density field and the bottom form stress and increases with A TV , the vertical mixing coefficient. If wind is added to this flow, the additional circulation is also dependent on the baroclinic structure but decreases with increasing A TV . This applies especially to the ACC, where wind‐induced additions are much larger than when the wind acts alone in a homogeneous ocean. An analysis of the dynamic balance of the ACC in the model shows that it is governed by lateral friction, bottom form stress, and wind. The mechanism for driving the ACC by deep convection and bottom topography is revealed in special experiments with simplified topography. In these runs, all topography is removed except for all or part of a submarine ridge across the Drake Passage; this topography alone causes an ACC with barotropic transport of 80 Sv, driven by a deep density difference and pressure gradient across the ridge. This ridge channels AABW formed in the Weddell Sea northward into the South Atlantic, and the ACC is driven by angular momentum conservation across these latitudes of the compensating southward flowing shallower flow (or, equivalently, by the Coriolis force acting on it) above the ridge. In most other parts of the model ocean, bottom form stress acts as a net drag on the zonal current.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1996
    detail.hit.zdb_id: 2033040-6
    detail.hit.zdb_id: 3094104-0
    detail.hit.zdb_id: 2130824-X
    detail.hit.zdb_id: 2016813-5
    detail.hit.zdb_id: 2016810-X
    detail.hit.zdb_id: 2403298-0
    detail.hit.zdb_id: 2016800-7
    detail.hit.zdb_id: 161666-3
    detail.hit.zdb_id: 161667-5
    detail.hit.zdb_id: 2969341-X
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094268-8
    detail.hit.zdb_id: 710256-2
    detail.hit.zdb_id: 2016804-4
    detail.hit.zdb_id: 3094181-7
    detail.hit.zdb_id: 3094219-6
    detail.hit.zdb_id: 3094167-2
    detail.hit.zdb_id: 2220777-6
    detail.hit.zdb_id: 3094197-0
    SSG: 16,13
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  • 6
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 1998
    In:  Journal of Fluid Mechanics Vol. 363 ( 1998-05-25), p. 229-252
    In: Journal of Fluid Mechanics, Cambridge University Press (CUP), Vol. 363 ( 1998-05-25), p. 229-252
    Abstract: Properties of the flow generated by a continuous source of dense fluid on a slope in a rotating system are investigated with a variety of laboratory experiments. The dense fluid may initially flow down the slope but it turns (under the influence of rotation) to flow along the slope, and initial geostrophic adjustment gives it an anticyclonic velocity profile. Some of the dense fluid drains downslope in a viscous Ekman layer, which may become unstable to growing waves. Provided that the viscous draining is not too strong, cyclonic vortices form periodically in the upper layer and the dense flow breaks up into a series of domes. Three processes may contribute to the formation of these eddies. First, initial downslope flow of the dense current may stretch columns of ambient fluid by the ‘Taylor column’ process (which we term ‘capture’). Secondly, the initial geostrophic adjustment implies lower-layer collapse which may stretch the fluid column, and thirdly, viscous drainage will progressively stretch and spin up a captured water column. Overall this last process may be the most significant, but viscous drainage has contradictory effects, in that it progressively removes dense lower-layer fluid which terminates the process when the layer thickness approaches that of the Ekman layer. The eddies produced propagate along the slope owing to the combined effects of buoyancy–Coriolis balance and ‘beta-gyres’. This removes fluid from the vicinity of the source and causes the cycle to repeat. The vorticity of the upper-layer cyclones increases linearly with Γ = L α/ D (where L is the Rossby deformation radius, α the bottom slope and D the total depth), reaching approximately 2 f in the experiments presented here. The frequency at which the eddy/dome structures are produced also increases with Γ , while the speed at which the structures propagate along the slope is reduced by viscous effects. The flow of dense fluid on slopes is a very important part of the global ocean circulation system and the implications of the laboratory experiments for oceanographic flows are discussed.
    Type of Medium: Online Resource
    ISSN: 0022-1120 , 1469-7645
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1998
    detail.hit.zdb_id: 1472346-3
    detail.hit.zdb_id: 218334-1
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  • 7
    Online Resource
    Online Resource
    American Meteorological Society ; 1996
    In:  Journal of Physical Oceanography Vol. 26, No. 12 ( 1996-12), p. 2576-2588
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 26, No. 12 ( 1996-12), p. 2576-2588
    Type of Medium: Online Resource
    ISSN: 0022-3670 , 1520-0485
    Language: English
    Publisher: American Meteorological Society
    Publication Date: 1996
    detail.hit.zdb_id: 2042184-9
    detail.hit.zdb_id: 184162-2
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