Description: Author Posting. © American Meteorological Society, 2012. This article is posted here by permission of American Meteorological Society for personal use, not for redistribution. The definitive version was published in Journal of Climate 25 (2012): 343–349, doi:10.1175/JCLI-D-11-00059.1.

Description: The Equatorial Undercurrent (EUC) is a major component of the tropical Pacific Ocean circulation. EUC velocity in most global climate models is sluggish relative to observations. Insufficient ocean resolution slows the EUC in the eastern Pacific where nonlinear terms should dominate the zonal momentum balance. A slow EUC in the east creates a bottleneck for the EUC to the west. However, this bottleneck does not impair other major components of the tropical circulation, including upwelling and poleward transport. In most models, upwelling velocity and poleward transport divergence fall within directly estimated uncertainties. Both of these transports play a critical role in a theory for how the tropical Pacific may change under increased radiative forcing, that is, the ocean dynamical thermostat mechanism. These findings suggest that, in the mean, global climate models may not underrepresent the role of equatorial ocean circulation, nor perhaps bias the balance between competing mechanisms for how the tropical Pacific might change in the future. Implications for model improvement under higher resolution are also discussed.

Description: KBK gratefully acknowledges the J. Lamar Worzel Assistant Scientist Fund. GCJ is supported by NOAA’s Office of Oceanic and Atmospheric Research. RM gratefully acknowledges the generous support and hospitality of the Divecha Centre for Climate Change and CAOS at IISc, Bangalore, and partial support by NASA PO grants.

Description: 2012-07-01

Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 1990

Description: Theory and observations of deep circulation in the near-equatorial Atlantic, Indian and Pacific Oceans are reviewed. Flow of deep and bottom water in the near-equatorial Indian and Pacific oceans, the two oceans with only a southern source of bottom water, is described through analysis of recent CTD data. Zero-velocity surfaces are chosen through use of water-mass properties and transports are estimated. Effects of basin geometry, bottom bathymetry and vertical diffusivity as well as a model meridional inertial current on a sloping bottom near the equator are all discussed in conjunction with the flow patterns inferred from observations. In the western equatorial Indian Ocean, repeat CTD surveys in the Somali Basin at the height of subsequent northeast and southwest monsoons show only small differences in the strength of the circulation of the bottom water (potential temperature θ ≤1.2°C). A deep western boundary current (DWBC) carrying about 4x106 m3 s-1 of this water is observed moving north along the continental rise of Africa at 3°S. The cross-equatorial sections suggest that the current turns eastward at the equator. The northern sections show a large mass of the coldest water in the interior east of the Chain Ridge, augmenting the evidence that the DWBC observed south of the equator turns east at the equator rather than remaining on the boundary, and feeds the interior circulation in the northern part of the basin from the equator. The circulation of deep water (1.2°C〈 θ ≤ 1.7°C) in the Somali and Arabian Basins is also analyzed. A DWBC flowing southward along the Carlsberg ridge in the Arabian Basin is described. In the central equatorial Pacific Ocean a recent zonal CTD section at 10°N, allows estimation that 5.0x106 m3 s-1 of Lower Circumpolar Water (LCPW, θ ≤ 1.2°C) moves northward as a DWBC along the Caroline Seamounts in the East Mariana Basin. In the Central Pacific Basin, 8.1x106 m3 s-1 of LCPW is estimated to move northward along the Marshal Seamounts as a DWBC at this latitude. An estimated 4.7x106 m3 s-1 of the LCPW moves back southward across 10°N in the Northeast Pacific Basin along the western flank of the East Pacific Rise and an equatorial jet is observed to flow westward from 138°W to 148°W shifting south of the Line Islands at 2.5°S, 159°W. The net northward flow of LCPW across 10°N in the Pacific Ocean is estimated at 8.4x106 m3 s-I. The net southward flow of the silica-rich North Pacific Deep Water (NPDW, 1.2 〈 θ ≤ 2.0°C) in the central Pacific Ocean estimated at 2.7x106 m3 s-1 is also discussed. In the Indian Ocean, the eastward equatorial flow in the the bottom water of the Somali Basin differs from the prediction of a flat-bottom uniform-upwelling Stommel-Arons calculation with realistic basin geometry and source location. The behavior of a uniform potential vorticity meridional jet on a sloping bottom is examined in an attempt to explain the observed behavior at the equator. The inertial jet does not cross the equator in a physically plausible fashion owing to the constraint of conservation of potential vorticity. Mass and heat budgets for the bottom water of the Somali Basin are of interest with respect to the equatorial feature. Upwelling through the θ = 1.2°C surface is estimated at 12±4x10-5 cm s-1 and a rough heat budget for the deep Somali Basin results in an estimate of vertical diffusivity of 9±5 cm2 s-1 at 3800 m. Numerical model results indicate that large vertical diffusivities result in eastward jets in the bottom water at the equator. In the Pacific Ocean the DWBC observed flowing northward south of the equator crosses the equator with transport nearly intact, albeit split into two at 10°N by the tortuous bathymetry. However the southward flow along the East Pacific Rise in the Northeast Pacific Basin and the westward equatorial jet this flow feeds are puzzling. The basin depth decreases equatorward and eastward, which may allow some southeastward flow in the Stommel-Arons framework. However, the equatorial jet is still unexplained. The estimated vertical velocity and diffusivity at 3600 db of 2±2x10-5 cm s-1 and 4±3 cm2 s-1 for the area between 12°8 and 10°N are much smaller than estimates in the Somali Basin. Thus the two oceans, similar in their single southern source of bottom water, have DWBC's which behave remarkably differently near the equator. In the Somali Basin of the Indian Ocean the DWBC appears to turn eastward at the equator, with large vertical upwelling velocity and large vertical diffusivity estimates for the bottom water of the basin. In the Pacific Ocean the DWBC appears to cross the equator, but there is a puzzling westward flowing equatorial jet in the bottom water of the Northeast Pacific Basin.

Description: The author began this research in the M.I.T.-W.H.O.I Joint Program while supported by the U. S. Offce of Naval Research through a Secretary of the Navy Graduate Fellowship in Oceanography. Support for collection and analysis of the data taken during R.R.S. Charles Darwin cruises 86-19 and 87-25 was provided by the U. S. National Science Foundation under grants OCE8800135 and OCE8513825 to D. B. Olson at the University of Miami and by the U. S. Offce of Naval Research under contract N00014-87-K-0001, NR083-004 and grant N00014-89-J-1076 to B. A. Warren at W.H.O.I. Collection of data taken during R.Y. Moana Wave cruise 89- 3 was supp6rted by the U. S. National Science Foundation under grant OCE881691O to H. L. Bryden and J. M. Toole at W.H.O.I. Collection of data taken during the U.S.-P.R.C. Toga cruises was supported by N.O.A.A. under grant NA85AA-DACU7.

Description: Author Posting. © The Author(s), 2009. This is the author's version of the work. It is posted here by permission of Elsevier B.V. for personal use, not for redistribution. The definitive version was published in Progress In Oceanography 82 (2009): 281-325, doi:10.1016/j.pocean.2009.08.002.

Description: To address questions concerning the intensity and spatial structure of the 3–dimensional circulation within the Pacific Ocean and the associated advective and diffusive property flux divergences, data from approximately 3000 high–quality hydrographic stations collected on 40 zonal and meridional cruises have been merged into a physically consistent model. The majority of the stations were occupied as part of the World Ocean Circulation Experiment (WOCE), which took place in the 1990s. These data are supplemented by a few pre–WOCE surveys of similar quality, and time–averaged direct–velocity and historical hydrographic measurements about the equator. An inverse box model formalism is employed to estimate the absolute along–isopycnal velocity field, the magnitude and spatial distribution of the associated diapycnal flow and the corresponding diapycnal advective and diffusive property flux divergences. The resulting large–scale WOCE Pacific circulation can be described as two shallow overturning cells at mid– to low latitudes, one in each hemisphere, and a single deep cell which brings abyssal waters from the Southern Ocean into the Pacific where they upwell across isopycnals and are returned south as deep waters. Upwelling is seen to occur throughout most of the basin with generally larger dianeutral transport and greater mixing occurring at depth. The derived pattern of ocean heat transport divergence is compared to published results based on air–sea flux estimates. The synthesis suggests a strongly east/west oriented pattern of air–sea heat flux with heat loss to the atmosphere throughout most of the western basins, and a gain of heat throughout the tropics extending poleward through the eastern basins. The calculated meridional heat transport agrees well with previous hydrographic estimates. Consistent with many of the climatologies at a variety of latitudes as well, our meridional heat transport estimates tend toward lower values in both hemispheres.

Description: This work was funded by National Science Foundation grants OCE–9710102, OCE– 9712209 and OCE–0079383, and also benefited from work on closely related projects funded by NSF grants OCE–0223421 and OCE–0623261, and NOAA grant NA17RJ1223 funded through CICOR. For G.C.J. NASA funding came under Order W–19,314.