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Turbulence variability at the equator in the central Pacific at the beginning of the 1991-1993 El Nino

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Title Turbulence variability at the equator in the central Pacific at the beginning of the 1991-1993 El Nino
Names Lien, R.-C. (creator)
Caldwell, Douglas R. (creator)
Gregg, M.C. (creator)
Moum, James N. (creator)
Date Issued 1995-04-15 (iso8601)
Abstract A 38-day, 5990-cast microstructure study on the equator performed
during the onset of the 1991-1993 El Nino shows the effect on small-scale activity
at 140°W of an equatorial Kelvin wave. By using two ships, data were taken
continuously from November 4 to December 12, 1991, near the National Oceanic
and Atmospheric Administration Pacific Marine Environmental Laboratory mooring
at 0°N, 140°W. The ships occupied the station sequentially with a 3.5-day overlap
for intercalibration. Variability in currents was observed on tidal periods, and
periods of 4 days (presumably equatorially trapped internal gravity waves), 8 days
(cause unknown), 20 days (tropical instability waves), and longer (Kelvin waves).
Variation in water structure occurred most prominently on the timescale of Kelvin
waves. The diurnal cycle typical of that location was observed: nocturnal deepening
of the surface mixed layer was accompanied by a "deep cycle," bursts of turbulence
penetrating into the stratified region below the nighttime mixed layer. During the
observational period, one Kelvin wave trough and one crest passed through the site.
Changes accompanying the phase change in the Kelvin wave included a reversal
of the near-surface current, a deepening of the thermocline, and a change of water
mass. Changes in small-scale activity included a tenfold decrease of the thermal
dissipation rate and a fourfold decrease of the rate of heat transport downward
from the mixed layer. The nighttime mixed layer deepened from 30 to 60 m. The
thickness of the stratified region in which nocturnal turbulence bursts occurred,
the deep cycle region, thinned from 40 to 20 m because it was confined between
the bottom of the nighttime mixed layer and the low-shear region near the core of
the undercurrent. The decrease in downward heat flux observed at this passage of
the downwelling Kelvin wave front could explain the rapid sea surface temperature
(SST) increase seen at El Nino onsets. The magnitude of the change in vertical
flux is similar to the magnitude of the change in horizontal advection. This process
would produce a warmer SST much more quickly than could the advection of warm
waters eastward.
Genre Article
Identifier Lien, R. C., Caldwell, D. R., Gregg, M. C., & Moum, J. N. (1995). Turbulence variability at the equator in the central Pacific at the beginning of the 1991-1993 El Nino. Journal of Geophysical Research, 100(C4), 6881-6898.

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