2016
DOI: 10.1175/jpo-d-15-0008.1
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Symmetric Instability, Inertial Oscillations, and Turbulence at the Gulf Stream Front

Abstract: The passage of a winter storm over the Gulf Stream observed with a Lagrangian float and hydrographic and velocity surveys provided a unique opportunity to study how the interaction of inertial oscillations, the front, and symmetric instability (SI) shapes the stratification, shear, and turbulence in the upper ocean under unsteady forcing. During the storm, the rapid rise and rotation of the winds excited inertial motions. Acting on the front, these sheared motions modulate the stratification in the surface bou… Show more

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Cited by 91 publications
(138 citation statements)
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“…When Q is multiplied by the Coriolis parameter ( f = 2Ω sin ϕ), we theoretically expect negative values to appear in regions where symmetric instabilities could be at play, corresponding as well to areas where the gradient Richardson number ( Ri ) is <1. Ri can be defined as follows (Thomas et al, ): Ri=N2S2 where N 2 = bz and S 2 = uz2 + vz2. N 2 is the stratification and S 2 is the squared shear.…”
Section: Methodsmentioning
confidence: 99%
“…When Q is multiplied by the Coriolis parameter ( f = 2Ω sin ϕ), we theoretically expect negative values to appear in regions where symmetric instabilities could be at play, corresponding as well to areas where the gradient Richardson number ( Ri ) is <1. Ri can be defined as follows (Thomas et al, ): Ri=N2S2 where N 2 = bz and S 2 = uz2 + vz2. N 2 is the stratification and S 2 is the squared shear.…”
Section: Methodsmentioning
confidence: 99%
“…Periods of down‐front wind, reduce the surface buoyancy in the front, deepen the SXL, and drive entrainment (Figure ), whereas periods of up‐front wind (when the winds are opposite to the geostrophic frontal jet) increase the surface buoyancy in the front, shoal the SXL, and drive detrainment. In the real ocean, the EBF sometimes vacillates in time between positive and negative values, primarily due to variations in the wind stress direction and amplitude, but also due to variations in the horizontal buoyancy gradient in the ocean hb [e.g., Thomas et al ., ; Thompson et al ., ]. Hence, a question arises: what is the time‐integrated effect of these vacillations in the EBF (and wind stress more generally) on SXL depths, SXL nutrient budgets, and plankton ecosystems at a front?…”
Section: Introductionmentioning
confidence: 99%
“…Here, a two‐dimensional PV section (e.g., Ramachandran et al, ; Thomas et al, ) is evaluated from the objective field, assuming that along‐stream variations of quantities are negligible. However, these gradients could be significant, refuting the approximation of two‐dimensional PV (see details in Thomas et al, ; Ramachandran et al, ). The Ertel PV is given by q=false(.2emftruek^+×boldufalse)·b, where f is the planetary vorticity, truek^ is the unit vector, and boldu=false(u,v,wfalse) is the 3‐D velocity vector.…”
Section: The Mesoscale Fieldmentioning
confidence: 99%
“…According to Thomas et al (), is expressed by a sum of two constituents that emphasizes the contrasting roles of vertical vorticity/stratification and baroclinicity. The scaled PV, q][)(f+vxN2vzbxftruef2N2, where the overbar denotes spatial averaging, is outlined in Figure .…”
Section: The Mesoscale Fieldmentioning
confidence: 99%