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  • 1
    Online-Ressource
    Online-Ressource
    American Meteorological Society ; 2016
    In:  Journal of Physical Oceanography Vol. 46, No. 3 ( 2016-03), p. 827-840
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 46, No. 3 ( 2016-03), p. 827-840
    Kurzfassung: The dominant processes governing ocean mixing during an active phase of the Madden–Julian oscillation are identified. Air–sea fluxes and upper-ocean currents and hydrography, measured aboard the R/V Revelle during boreal fall 2011 in the Indian Ocean at 0°, 80.5°E, are integrated by means of a large-eddy simulation (LES) to infer mixing mechanisms and quantify the resulting vertical property fluxes. In the simulation, wind accelerates the mixed layer, and shear mixes the momentum downward, causing the mixed layer base to descend. Turbulent kinetic energy gains due to shear production and Langmuir circulations are opposed by stirring gravity and frictional losses. The strongest stirring of buoyancy follows precipitation events and penetrates to the base of the mixed layer. The focus here is on the initial 24 h of an unusually strong wind burst that began on 24 November 2011. The model shows that Langmuir turbulence influences only the uppermost few meters of the ocean. Below the wave-energized region, shear instability responds to the integrated momentum flux into the mixed layer, lagging the initial onset of the storm. Shear below the mixed layer persists after the storm has weakened and decelerates the surface jet slowly (compared with the acceleration at the peak of the storm). Slow loss of momentum from the mixed layer extends the effect of the surface wind burst by energizing the fluid at the base of the mixed layer, thereby prolonging heat uptake due to the storm. Ocean turbulence and air–sea fluxes contribute to the cooling of the mixed layer approximately in the ratio 1:3, consistent with observations.
    Materialart: Online-Ressource
    ISSN: 0022-3670 , 1520-0485
    Sprache: Unbekannt
    Verlag: American Meteorological Society
    Publikationsdatum: 2016
    ZDB Id: 2042184-9
    ZDB Id: 184162-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    Springer Science and Business Media LLC ; 2002
    In:  Ocean Dynamics Vol. 52, No. 3 ( 2002-7-1), p. 104-115
    In: Ocean Dynamics, Springer Science and Business Media LLC, Vol. 52, No. 3 ( 2002-7-1), p. 104-115
    Materialart: Online-Ressource
    ISSN: 1616-7341 , 1616-7228
    Sprache: Unbekannt
    Verlag: Springer Science and Business Media LLC
    Publikationsdatum: 2002
    ZDB Id: 2063267-8
    ZDB Id: 201122-0
    SSG: 14
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 3
    Online-Ressource
    Online-Ressource
    American Meteorological Society ; 2023
    In:  Journal of Physical Oceanography Vol. 53, No. 8 ( 2023-08), p. 1821-1833
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 53, No. 8 ( 2023-08), p. 1821-1833
    Kurzfassung: Along with boundary layer turbulence, downward radiation of near-inertial waves (NIWs) damps inertial oscillations (IOs) in the surface ocean; however, the latter can also energize abyssal mixing. Here we present observations made from a dipole vortex in the Iceland Basin where, after the period of direct wind forcing, IOs lost over half their kinetic energy (KE) in two inertial periods to radiation of NIWs with minimal turbulent dissipation of KE. The dipole’s vorticity gradient led to a rapid reduction in the NIW’s lateral wavelength via ζ refraction that was accompanied by isopycnal undulations below the surface mixed layer. Pressure anomalies associated with the undulations were correlated with the NIW’s velocity yielding an energy flux of 310 mW m −2 pointed antiparallel to the vorticity gradient and a downward flux of 1 mW m −2 capable of driving the observed drop in KE. The minimal role of turbulence in the energetics after the IOs had been generated by the winds was confirmed using a large-eddy simulation driven by the observed winds. Significance Statement We report direct observational estimates of the vector wave energy flux of a near-inertial wave. The energy flux points from high to low vorticity in the horizontal, consistent with the theory of ζ refraction. The downward energy flux dominates the observed damping of inertial motions over turbulent dissipation and mixing.
    Materialart: Online-Ressource
    ISSN: 0022-3670 , 1520-0485
    Sprache: Unbekannt
    Verlag: American Meteorological Society
    Publikationsdatum: 2023
    ZDB Id: 2042184-9
    ZDB Id: 184162-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 4
    Online-Ressource
    Online-Ressource
    American Meteorological Society ; 2017
    In:  Journal of Physical Oceanography Vol. 47, No. 10 ( 2017-10), p. 2429-2454
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 47, No. 10 ( 2017-10), p. 2429-2454
    Kurzfassung: Generation of ocean surface boundary layer turbulence and coherent roll structures is examined in the context of wind-driven and geostrophic shear associated with horizontal density gradients using a large-eddy simulation model. Numerical experiments over a range of surface wind forcing and horizontal density gradient strengths, combined with linear stability analysis, indicate that the dominant instability mechanism supporting coherent roll development in these simulations is a mixed instability combining shear instability of the ageostrophic, wind-driven flow with symmetric instability of the frontal geostrophic shear. Disruption of geostrophic balance by vertical mixing induces an inertially rotating ageostrophic current, not forced directly by the wind, that initially strengthens the stratification, damps the instabilities, and reduces vertical mixing, but instability and mixing return when the inertial buoyancy advection reverses. The resulting rolls and instabilities are not aligned with the frontal zone, with an oblique orientation controlled by the Ekman-like instability. Mean turbulence is enhanced when the winds are destabilizing relative to the frontal orientation, but mean Ekman buoyancy advection is found to be relatively unimportant in these simulations. Instead, the mean turbulent kinetic energy balance is dominated by mechanical shear production that is enhanced when the wind-driven shear augments the geostrophic shear, while the resulting vertical mixing nearly eliminates any effective surface buoyancy flux from near-surface, cold-to-warm, Ekman buoyancy advection.
    Materialart: Online-Ressource
    ISSN: 0022-3670 , 1520-0485
    Sprache: Unbekannt
    Verlag: American Meteorological Society
    Publikationsdatum: 2017
    ZDB Id: 2042184-9
    ZDB Id: 184162-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 5
    Online-Ressource
    Online-Ressource
    American Meteorological Society ; 2020
    In:  Journal of Physical Oceanography Vol. 50, No. 9 ( 2020-09-01), p. 2781-2796
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 50, No. 9 ( 2020-09-01), p. 2781-2796
    Kurzfassung: A simple, isolated front is modeled using a turbulence resolving, large-eddy simulation (LES) to examine the generation of instabilities and inertial oscillations by surface fluxes. Both surface cooling and surface wind stress are considered. Coherent roll instabilities with 200–300-m horizontal scale form rapidly within the front after the onset of surface forcing. With weak surface cooling and no wind, the roll axis aligns with the front, yielding results that are equivalent to previous constant gradient symmetric instability cases. After ~1 day, the symmetric modes transform into baroclinic mixed modes with an off-axis orientation. Traditional baroclinic instability develops by day 2 and thereafter dominates the overall circulation. Addition of destabilizing wind forcing produces a similar behavior, but with off-axis symmetric-Ekman shear modes at the onset of instability. In all cases, imbalance of the geostrophic shear by vertical mixing leads to an inertial oscillation in the frontal currents. Analysis of the energy budget indicates an exchange between kinetic energy linked to the inertial currents and potential energy associated with restratification as the front oscillates in response to the vertically sheared inertial current. Inertial kinetic energy decreases from enhanced mixed layer turbulence dissipation and vertical propagation of inertial wave energy into the pycnocline.
    Materialart: Online-Ressource
    ISSN: 0022-3670 , 1520-0485
    Sprache: Unbekannt
    Verlag: American Meteorological Society
    Publikationsdatum: 2020
    ZDB Id: 2042184-9
    ZDB Id: 184162-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 6
    Online-Ressource
    Online-Ressource
    American Meteorological Society ; 2023
    In:  Journal of Physical Oceanography Vol. 53, No. 8 ( 2023-08), p. 1887-1900
    In: Journal of Physical Oceanography, American Meteorological Society, Vol. 53, No. 8 ( 2023-08), p. 1887-1900
    Kurzfassung: The observed development of deep mixed layers and the dependence of intense, deep-mixing events on wind and wave conditions are studied using an ocean LES model with and without an imposed Stokes-drift wave forcing. Model results are compared to glider measurements of the ocean vertical temperature, salinity, and turbulence kinetic energy (TKE) dissipation rate structure collected in the Icelandic Basin. Observed wind stress reached 0.8 N m −2 with significant wave height of 4–6 m, while boundary layer depths reached 180 m. We find that wave forcing, via the commonly used Stokes drift vortex force parameterization, is crucial for accurate prediction of boundary layer depth as characterized by measured and predicted TKE dissipation rate profiles. Analysis of the boundary layer kinetic energy (KE) budget using a modified total Lagrangian-mean energy equation, derived for the wave-averaged Boussinesq equations by requiring that the rotational inertial terms vanish identically as in the standard energy budget without Stokes forcing, suggests that wind work should be calculated using both the surface current and surface Stokes drift. A large percentage of total wind energy is transferred to model TKE via regular and Stokes drift shear production and dissipated. However, resonance by clockwise rotation of the winds can greatly enhance the generation of inertial current mean KE (MKE). Without resonance, TKE production is about 5 times greater than MKE generation, whereas with resonance this ratio decreases to roughly 2. The results have implications for the problem of estimating the global kinetic energy budget of the ocean.
    Materialart: Online-Ressource
    ISSN: 0022-3670 , 1520-0485
    Sprache: Unbekannt
    Verlag: American Meteorological Society
    Publikationsdatum: 2023
    ZDB Id: 2042184-9
    ZDB Id: 184162-2
    Standort Signatur Einschränkungen Verfügbarkeit
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