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Enhancement of fronts by vertical mixing

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Field Value
Title Enhancement of fronts by vertical mixing
Names Dewey, Richard K. (creator)
Moum, James N. (creator)
Date Issued 1990-06-15 (iso8601)
Note Copyrighted by American Geophysical Union.
Abstract Microstructure observations near upwelled fronts indicate considerable variation in the structure of
vertical mixing across the frontal region. Observations of cool filaments off northern California
indicate that within the cool (dense) core of filaments the raised pycnocline inhibits the penetration to
middepths of surface-generated mixing. The microstructure profiles are used to estimate the available
wind energy for mixing as a function of pycnocline, or mixed layer depth. A greater portion of energy
input at the surface is available for entrainment of dense fluid through the pycnocline and into the
surface mixed layer where the pycnocline is shallow. Hence surface-forced mixing may cause a more
rapid increase in mixed layer density within the cool filament than outside the filament, resulting in an
enhanced horizontal density gradient in the mixed layer. Assuming the flow adjusts towards
geostrophy, the enhanced horizontal density gradient at the front could result in an accelerated mixed
layer in the direction of the preexisting geostrophic flow. Proportions relating the gain in potential
energy to the wind energy vary with pycnocline depth and differ by as much as an order of magnitude
from the findings of Denman and Miyake (1973) and Davis et al. (1981). Horizontal variability of
pycnocline erosion may not be properly taken into account in some models and should more
realistically be parameterized by including dependence on pycnocline depth.
Genre Article
Identifier Citation: Dewey, R., and J. Moum (1990), Enhancement of Fronts by Vertical Mixing, J. Geophys. Res., 95(C6), 9433-9445, doi:10.1029/JC095iC06p09433.

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