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Fine structure, microstructure, and vertical mixing processes in the upper ocean in the western Weddell Sea

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Title Fine structure, microstructure, and vertical mixing processes in the upper ocean in the western Weddell Sea
Names Robertson, Robin (creator)
Padman, Laurie (creator)
Levine, Murray D. (creator)
Date Issued 1995-09-15 (iso8601)
Note Copyrighted by American Geophysical Union.
Abstract The upward flux of heat from the subsurface core of Warm Deep Water
(WDW) to the perennially ice-covered sea surface over the continental slope in the
western Weddell Sea is estimated using data obtained during February-June 1992
from a drifting ice station. Through the permanent pycnocline the diapycnal heat
flux is estimated to be about 3 W m⁻², predominantly because of double-diffusive
convection. There is no evidence that shear-driven mixing is important in the
pycnocline. The estimated mean rate of heat transfer from the mixed layer to the
ice is 1.7 W m⁻², although peak heat fluxes of up to 15 W m⁻² are found during
storms. It is hypothesized that isopycnal mixing along sloping intrusions also
contributes to the loss of heat from the WDW in this region; however, we are unable
to quantify the fluxes associated with this process. Intrusions occur intermittently
throughout this experiment but are most commonly found near the boundary of
the warm-core current and the shelf-modified water to the east. These heat fluxes
are significantly lower than the basin-averaged value of 19 W m⁻² (Fahrbach et
al., 1994) that is required to balance the heat budget of the Weddell Gyre. Other
studies suggest that shelf processes to the west of the ice station drift track and
more energetic double-diffusive convection in the midgyre to the east could account
for the difference between our flux estimates for this region and those based on the
basin-scale heat budget.
Genre Article
Identifier Robertson, R., L. Padman, and M. Levine (1995), Fine structure, microstructure, and vertical mixing processes in the upper ocean in the western Weddell Sea, J. Geophys. Res., 100(C9), 18517-18535.

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