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1.
The circulation of the Southern Ocean is studied in the eddy-resolving model POP (Parallel Ocean Program) by an analysis
of zonally integrated balances. The TEM formalism (Transformed Eulerian Mean) is extended to include topography and continental
boundaries, thus deviations from a zonally integrated state involve transient and standing eddies. The meridional circulation
is presented in terms of the Eulerian, eddy-induced, and residual streamfunctions. It is shown that the splitting of the meridional
circulation into Ekman and geostrophic transports and the component induced by subgrid and Reynolds stresses is identical
to a particular form of the zonally integrated balance of zonal momentum. In this balance, the eddy-induced streamfunctions
represent the interfacial form stresses by transient and standing eddies and the residual streamfunction represents the acceleration
of the zonal current by density fluxes in a zonally integrated frame. The latter acceleration term is directly related to
the surface flux of density and interior fluxes due to the resolved and unresolved eddies. The eddy-induced circulation is
extremely vigorous in POP. In the upper ocean a shallow circulation, reversed in comparison to the Deacon cell and mainly
due to standing eddies, appears to the north of Drake Passage latitudes, and in the Drake Passage belt of latitudes a deep-reaching
cell is induced by transient eddies. In the resulting residual circulation the Deacon cell is largely cancelled and the residual
advection of the zonal mean potential density is balanced by diapycnal eddy and subgrid fluxes which are strong in the upper
few hundred meters but small in the ocean interior. The balance of zonal momentum is consistent with other eddy-resolving
models; a new aspect is the clear identification of density effects in the zonally integrated balance. We show that the wind
stress and the stress induced by the residual circulation drive the eastward current, whereas both eddy species result in
a braking. Finally, we extend the Johnson–Bryden model of zonal transport to incorporate all relevant terms from the zonal
momentum balance. It is shown that wind stress and induction by the residual circulation carry an eastward transport while
bottom form stress and the stress induced by standing eddies yield westward components of transport.
Received: 26 June 2001 / Accepted: 2 November 2001 相似文献
2.
A simple box model of the circulation into and inside the ocean cavern beneath an ice shelf is used to estimate the melt rates
of Antarctic glaciers and ice shelves. The model uses simplified cavern geometries and includes a coarse parameterization
of the overturning circulation and vertical mixing. The melting/freezing physics at the ice shelf/ocean interface are those
usually implemented in high-resolution circulation models of ice shelf caverns. The model is driven by the thermohaline inflow
conditions and coupling to the heat and freshwater exchanges at the sea surface in front of the cavern. We tune the model
for Pine Island Glacier and then apply it to six other major caverns. The dependence of the melting rate on thermohaline conditions
at the ice shelf front is investigated for this set of caverns, including sensitivity studies, alternative parameterizations,
and warming scenarios. An analytical relation between the melting rate and the inflow temperature is derived for a particular
model version, showing a quadratic dependence of basal melting on small values of the temperature of the inflow, which changes
to a linear dependence for larger values. The model predicts melting at all ice shelf bases in agreement with observations,
ranging from below a meter per year for Ronne Ice Shelf to about 25 m/year for the Pine Island Glacier. In a warming scenario
with a one-degree increase of the inflow temperature, the latter glacier responds with a 1.4-fold increase of the melting
rate. Other caverns respond by more than a tenfold increase, as, e.g., Ronne Ice Shelf. The model is suitable for use as a
simple fast module izn coarse large-scale ocean models. 相似文献
3.
Ocean Dynamics - Surface windstress transfers energy to the surface mixed layer of the ocean, and this energy partly radiates as internal gravity waves with near-inertial frequencies into the... 相似文献
4.
The equations of motion of all relevant parameters of Alfvén waves propagating from the sun outwardly into the expanding interplanetary medium are discussed for the case of a quiet, ideal, isotropic, one-fluid solar wind plasma. It is found that the frequency of the wave reamains constant, while the wave vector and the amplitudes depend, in general, on the evolution of the background medium and on the angle between the wave vector and the interplanetary magnetic field. This latter dependence cancels approximately for the evolution of the amplitudes in the case of a pure, overall spiral magnetic field. It is shown that in this case the results of earlier discussions can be derived by less decisive restrictions. 相似文献
5.
The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. 相似文献
6.
The transport of the Antarctic Circumpolar Current (ACC) is influenced by a variety of processes and parameters. A proper
implementation of basin geometry, ocean topography and baroclinicity is known to be a fundamental requisite for a realistic
simulation of the circulation and transport. Other, more subtle parameters are those of eddy-induced transports and diapycnal
mixing of thermohaline tracers or buoyancy, either treated by eddy resolution or by a proper parameterization. Quite a number
of realistic numerical simulations of the circulation in the Southern Ocean have recently been published. Many concepts on
relations of the ACC transport to model parameters and forcing function are in discussion, however, without much generality
and little success. We present a series of numerical simulations of circumpolar flow with a simplified numerical model, ranging
from flat-bottom wind-driven flow to baroclinic flow with realistic topography and wind and buoyancy forcing. Analysis of
the balances of momentum, vorticity, and baroclinic potential energy enables us to develop a new transport theory, which combines
the most important mechanisms driving the circulation of the ACC and determining its zonal transport. The theory is based
on the importance of the bottom vertical velocity in generating vorticity and shaping the baroclinic potential energy of the
ACC. It explains the breaking of the -constraint by baroclinicity and brings together in one equation the wind and buoyancy forcing of the current. The theory
emphasizes the role of Ekman pumping and eddy diffusion of buoyancy to determine the transport. It also demonstrates that
eddy viscosity effects are irrelevant in the barotropic vorticity balance and that friction arises via eddy diffusion of density.
In this regime, the classical Stommel model of vorticity balance is revived where the bottom friction coefficient is replaced
by (with the Gent–McWilliams coefficient and the baroclinic Rossby radius ) and a modified wind curl forcing appears. 相似文献
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8.
Large-scale zonal flow driven across submarine topography establishes standing Rossby waves. In the presence of stratification,
the wave pattern can be represented by barotropic and baroclinic Rossby waves of mixed planetary topographic nature, which
are locked to the topography. In the balance of momentum, the wave pattern manifests itself as topographic formstress. This
wave-induced formstress has the net effect of braking the flow and reducing the zonal transport. Locally, it may lead to acceleration,
and the parts induced by the barotropic and baroclinic waves may have opposing effects. This flow regime occurs in the circumpolar
flow around Antarctica. The different roles that the wave-induced formstress plays in homogeneous and stratified flows through
a zonal channel are analyzed with the BARBI (BARotropic-Baroclinic-Interaction ocean model, Olbers and Eden, J Phys Oceanogr 33:2719–2737, 2003) model. It is used in complete form and in a low-order version to clarify the different regimes. It is shown that the barotropic
formstress arises by topographic locking due to viscous friction and the baroclinic one due to eddy-induced density advection.
For the sinusoidal topography used in this study, the transport obeys a law in which friction and wave-induced formstress
act as additive resistances, and windstress, the effect of Ekman pumping on the density stratification, and the buoyancy forcing
(diapycnal mixing of the stratified water column) of the potential energy stored in the stratification act as additive forcing
functions. The dependence of the resistance on the system parameters (lateral viscosity ε, lateral diffusivity κ of eddy density advection, Rossby radius λ, and topography height δ) as well as the dependence of transport on the forcing functions are determined. While the current intensity in a channel
with homogeneous density decreases from the viscous flat bottom case in an inverse quadratic law ~δ
–2 with increasing topography height and always depends on ε, a stratified system runs into a saturated state in which the transport becomes independent of δ and ε and is determined by the density diffusivity κ rather than the viscosity: κ/λ
2 acts as a vertical eddy viscosity, and the transport is λ
2/κ times the applied forcing. Critical values for the topographic heights in these regimes are identified. 相似文献
9.
Synoptic scale variability of the Southern Ocean wind field in the high-frequency range of barotropic Rossby waves results
in transport variations of the Antarctic Circumpolar Current (ACC), which are highly coherent with the bottom pressure field
all around the Antarctic continent. The coherence pattern, in contrast to the steady state ACC, is steered by the geostrophic
f/h contours passing through Drake Passage and circling closely around the continent. At lower frequencies, with interannual
and decadal periods, the correlation with the bottom pressure continues, but baroclinic processes gain importance. For periods
exceeding a few years, variations of the ACC transport are in geostrophic balance with the pressure field associated with
the baroclinic potential energy stored in the stratification, whereas bottom pressure plays a minor role. The low-frequency
variability of the ACC transport is correlated with the baroclinic state variable in the entire Southern Ocean, mediated by
baroclinic topographic–planetary Rossby waves that are not bound to f/h contours. To clarify the processes of wave dynamics and pattern correlation, we apply a circulation model with simplified
physics (the barotropic–baroclinic-interaction model BARBI) and use two types of wind forcing: the National Centers for Environmental
Prediction (NCEP) wind field with integrations spanning three decades and an artificial wind field constructed from the first
three empirical orthogonal functions of NCEP combined with a temporal variability according to an autoregressive process.
Experiments with this Southern Annular Mode type forcing have been performed for 1,800 years. We analyze the spin-up, trends,
and variability of the model runs. Particular emphasis is placed on coherence and correlation patterns between the ACC transport,
the wind forcing, the bottom pressure field and the pressure associated with the baroclinic potential energy. A stochastic
dynamical model is developed that describes the dominant barotropic and baroclinic processes and represents the spectral properties
for a wide range of frequencies, from monthly periods to hundreds of years. 相似文献
10.
Much of the knowledge about ocean circulation stems from rather simple analytical models. The behavior of the meridional overturning and, more specifically, the thermohaline-induced part of the global ocean circulation, under changing surface conditions, is often judged by the bifurcation structure of box models with very low (low-order) resolution. The present study proposes a new low-order model of the thermohaline-driven circulation, which is constructed by severe truncation of a spectral decomposition of the two-dimensional equations of motion (vorticity and heat/salt balances). The physical ingredients of the new model are superior to box models because it has a continuous lateral and vertical representation of the fields and finite diffusion coefficients for heat and salt. The building of the spectral model involves much mathematical labor because the structure functions must be constructed in accordance with the boundary conditions for conservation of momentum, mass, heat, and salt. Furthermore, a number of complicated coupling coefficients must be evaluated. Like the box models, the spectral model is a dynamical system with mathematical complexity, but in most of the versions that we analyze, it still can be handled by standard analytical procedures. These versions are the spectral counterparts of the classical box models of Stommel, Rooth, and Welander, adjusted to the Atlantic overturning. A detailed comparison of the model types reveals a similar bifurcation pattern of box and spectral low-order configurations under symmetric and asymmetric forcing conditions and slight perturbations thereof (we use mixed boundary conditions for heat and salt and the surface freshwater flux as a continuation parameter). Comparison of the spectral low-order models with models towards a higher resolved range, namely, the two-dimensional overturning models for the meridional plane, reveals a close resemblance as well. A major difference of box and spectral models is the appearance of parameter windows in the latter, where only unstable steady states exist. The spectral models then show limit cycles, as well as chaotic trajectories with time scales of thousands of years. 相似文献
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