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• W2017795103 abstract "[1] The near-equatorial region is importantly different from other ocean areas: it acts as a barrier for large-scale meridional circulation, because the strongest currents are directed East-West, and it shows weak interior mixing despite large internal wave shear. All seems related to a change in importance of the vertical ‘inertial’ component of the earth's rotation. As rotational effects dominate large-scale ocean motions through a geostrophic balance, they become negligible at the equator. Here, deep-ocean observational evidence is presented of hitherto neglected rotational effects. It is demonstrated that when the equator is approached near-inertial internal wave motions very suddenly rather than smoothly change polarization from near-circular to near-rectilinear within half a degree across latitudes ∣φ∣ = 1.5 ± 0.5°. At the same latitudes sudden transitions are observed of large-scale kinetic energy and small-scale density stratification variations. Understanding the above requires a non-traditional approach in which the horizontal component of earth's rotation is considered." @default.
• W2017795103 created "2016-06-24" @default.
• W2017795103 creator A5001194458 @default.
• W2017795103 date "2005-01-01" @default.
• W2017795103 modified "2023-09-27" @default.
• W2017795103 title "Sharp near-equatorial transitions in inertial motions and deep-ocean step-formation" @default.
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• W2017795103 doi "https://doi.org/10.1029/2004gl021630" @default.
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