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G. Rowe, E. Firing, G. Johnson (2000)
Pacific Equatorial Subsurface Countercurrent Velocity, Transport, and Potential VorticityJournal of Physical Oceanography, 30
B. Basu (2019)
Some numerical investigations into a nonlinear three-dimensional model of the Pacific equatorial ocean flowsDeep Sea Research Part II: Topical Studies in Oceanography
B. Basu (2018)
On a Three-Dimensional Nonlinear Model of Pacific Equatorial Ocean Dynamics: Velocities and Flow PathsOceanography
A. Constantin, R. Johnson (2016)
An Exact, Steady, Purely Azimuthal Equatorial Flow with a Free SurfaceJournal of Physical Oceanography, 46
A. Constantin, R. Johnson (2017)
A nonlinear, three-dimensional model for ocean flows, motivated by some observations of the Pacific Equatorial Undercurrent and thermoclinePhysics of Fluids, 29
G. Johnson, M. Mcphaden, E. Firing (2001)
Equatorial Pacific Ocean Horizontal Velocity, Divergence, and Upwelling*Journal of Physical Oceanography, 31
D. Henry (2016)
Equatorially trapped nonlinear water waves in a $\unicode[STIX]{x1D6FD}$ -plane approximation with centripetal forcesJournal of Fluid Mechanics, 804
A. Constantin (2014)
Some Nonlinear, Equatorially Trapped, Nonhydrostatic Internal Geophysical WavesJournal of Physical Oceanography, 44
D. Henry (2018)
Nonlinear Features of Equatorial Ocean FlowsOceanography
W. Kessler, G. Johnson, D. Moore (2003)
Sverdrup and Nonlinear Dynamics of the Pacific Equatorial CurrentsJournal of Physical Oceanography, 33
Robin Johnson (2018)
The Value of Asymptotic Theories in Physical OceanographyOceanography
A. Constantin (2012)
An exact solution for equatorially trapped wavesJournal of Geophysical Research, 117
Adrian Constantin, R. Johnson (2019)
Ekman-type solutions for shallow-water flows on a rotating sphere: A new perspective on a classical problemPhysics of Fluids
J. Boyd (2017)
Dynamics of the Equatorial OceanDynamics of the Equatorial Ocean
AbstractA systematic development, based on the construction of an asymptotic solution of the Euler equation, written in rotating, spherical coordinates (φ,θ,r), is used to investigate the flows of the type seen in the neighborhood of the Pacific equator. First, it is shown that the observed poleward surface-flow structure away from the line of the equator is possible only if the flow evolves (changes) in the azimuthal direction. Then, allowing for variations in the azimuthal direction, the shallow-water, small-Rossby-number version of the problem, approximated close to the equator, leads to an asymptotic formulation that admits any prescribed azimuthal velocity profile u(θ,r) at some fixed longitude φ. The maximum extent of the flow region inside which we can describe in detail the velocity field is restricted by the size of the Rossby number. The analysis demonstrates that the meridional υ and vertical w velocity components are nonlinearly connected to u, and that all three velocity components appear at the same order in the leading (scaled) equations, even though the physical size of w is very much smaller than that of the other two components. An appropriate choice is made for u, at a given φ, and the corresponding complete three-dimensional flow field, which emerges from the interlinkage of the velocity components, is described; the thermocline is also added to the flow configuration. We compare these results with the available field data, demonstrating that this formulation captures all the main structures of the flow field, but also allows for many choices to be made that can be used to adjust the details of the flow and to model other, similar flows.
Journal of Physical Oceanography – American Meteorological Society
Published: Aug 31, 2019
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