We find that over a wide range of values
of diapycnal diffusivity and Southern Ocean winds, and with a variety of changes in surface boundary conditions, the spatial patterns of ocean temperature anomaly are nearly always determined as much or more by the existing heat reservoir redistribution than by the nearly passive uptake of temperature due to changes in the surface boundary conditions.
The great majority
of the diapycnal flux is the result of interaction with restricted regions of rough ocean - floor topography.
Not exact matches
The researchers took measurements
of small - scale temperature and velocity fluctuations, to measure the
diapycnal movements in the Antarctic Circumpolar Current (ACC) across the Drake Passage region
of the Southern Ocean.
For a rough estimate, downwelling water to the deep ocean in convection zones is about 40 Sv (10 ^ 6 m3 / s), assuming that comes in with say 2 deg C, and leaves (through upwelling, isopycnal and
diapycnal diffusion), that is a heat flux
of 320 TW, thus at least an order
of magnitude larger than the geothermal fluxes.
Quantify the magnitude, location, and physical mechanisms associated with interior
diapycnal mixing in the ocean, which contribute to the diabatic AMOC, and evaluate the realism
of current GCMs in this regard.
Woodgate, R.A., K. Aagaard, J.H. Swift, K.K. Falkner and W.M. Smethie,» Pacific Ventilation
of the Arctic Ocean's lower halocline by upwelling and
diapycnal mixing over the continental margin `, Geophysical Research Letters, 32, L18609, doi: 10.1029 / 2005GL023999, 2005.
Mugwump, you talk about the «average
diapycnal heat transfer
of the ocean», but what Douglass» revised model actually requires is the heat transfer out
of the upper mixed layer, which must (according to his ~ 5 month time scale) be very shallow.
Therefore, it is much more likely that the average
diapycnal heat transfer
of the ocean is determined by the interior than it is by the boundaries or regions
of steep topography.
Quantify the magnitude, location, and physical mechanisms associated with interior
diapycnal mixing in the ocean, which contribute to the diabatic AMOC, and evaluate the realism
of current ocean GCMs in this regard.
The numerical experiments are designed to explore the effects
of changing various properties
of the ocean (its size, geometry and
diapycnal diffusivity), the atmosphere (its water vapour content) and the forcing
of the system (the distribution
of incoming solar radiation and the rotation rate
of the planet).
The theory shows that dynamics
of the overturning circulation can be characterized by two limiting regimes, corresponding to weak and strong
diapycnal mixing.