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    Observations of the Tasman Sea Internal Tide Beam

    Source: Journal of Physical Oceanography:;2018:;volume 048:;issue 006::page 1283
    Author:
    Waterhouse, Amy F.
    ,
    Kelly, Samuel M.
    ,
    Zhao, Zhongxiang
    ,
    MacKinnon, Jennifer A.
    ,
    Nash, Jonathan D.
    ,
    Simmons, Harper
    ,
    Brahznikov, Dmitry
    ,
    Rainville, Luc
    ,
    Alford, Matthew
    ,
    Pinkel, Rob
    DOI: 10.1175/JPO-D-17-0116.1
    Publisher: American Meteorological Society
    Abstract: AbstractLow-mode internal tides, a dominant part of the internal wave spectrum, carry energy over large distances, yet the ultimate fate of this energy is unknown. Internal tides in the Tasman Sea are generated at Macquarie Ridge, south of New Zealand, and propagate northwest as a focused beam before impinging on the Tasmanian continental slope. In situ observations from the Tasman Sea capture synoptic measurements of the incident semidiurnal mode-1 internal-tide, which has an observed wavelength of 183 km and surface displacement of approximately 1 cm. Plane-wave fits to in situ and altimetric estimates of surface displacement agree to within a measurement uncertainty of 0.3 cm, which is the same order of magnitude as the nonstationary (not phase locked) mode-1 tide observed over a 40-day mooring deployment. Stationary energy flux, estimated from a plane-wave fit to the in situ observations, is directed toward Tasmania with a magnitude of 3.4 ± 1.4 kW m?1, consistent with a satellite estimate of 3.9 ± 2.2 kW m?1. Approximately 90% of the time-mean energy flux is due to the stationary tide. However, nonstationary velocity and pressure, which are typically 1/4 the amplitude of the stationary components, sometimes lead to instantaneous energy fluxes that are double or half of the stationary energy flux, overwhelming any spring?neap variability. Despite strong winds and intermittent near-inertial currents, the parameterized turbulent-kinetic-energy dissipation rate is small (i.e., 10?10 W kg?1) below the near surface and observations of mode-1 internal tide energy-flux convergence are indistinguishable from zero (i.e., the confidence intervals include zero), indicating little decay of the mode-1 internal tide within the Tasman Sea.
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      Observations of the Tasman Sea Internal Tide Beam

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    contributor authorWaterhouse, Amy F.
    contributor authorKelly, Samuel M.
    contributor authorZhao, Zhongxiang
    contributor authorMacKinnon, Jennifer A.
    contributor authorNash, Jonathan D.
    contributor authorSimmons, Harper
    contributor authorBrahznikov, Dmitry
    contributor authorRainville, Luc
    contributor authorAlford, Matthew
    contributor authorPinkel, Rob
    date accessioned2019-09-19T10:02:25Z
    date available2019-09-19T10:02:25Z
    date copyright4/4/2018 12:00:00 AM
    date issued2018
    identifier otherjpo-d-17-0116.1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl1/handle/yetl/4260868
    description abstractAbstractLow-mode internal tides, a dominant part of the internal wave spectrum, carry energy over large distances, yet the ultimate fate of this energy is unknown. Internal tides in the Tasman Sea are generated at Macquarie Ridge, south of New Zealand, and propagate northwest as a focused beam before impinging on the Tasmanian continental slope. In situ observations from the Tasman Sea capture synoptic measurements of the incident semidiurnal mode-1 internal-tide, which has an observed wavelength of 183 km and surface displacement of approximately 1 cm. Plane-wave fits to in situ and altimetric estimates of surface displacement agree to within a measurement uncertainty of 0.3 cm, which is the same order of magnitude as the nonstationary (not phase locked) mode-1 tide observed over a 40-day mooring deployment. Stationary energy flux, estimated from a plane-wave fit to the in situ observations, is directed toward Tasmania with a magnitude of 3.4 ± 1.4 kW m?1, consistent with a satellite estimate of 3.9 ± 2.2 kW m?1. Approximately 90% of the time-mean energy flux is due to the stationary tide. However, nonstationary velocity and pressure, which are typically 1/4 the amplitude of the stationary components, sometimes lead to instantaneous energy fluxes that are double or half of the stationary energy flux, overwhelming any spring?neap variability. Despite strong winds and intermittent near-inertial currents, the parameterized turbulent-kinetic-energy dissipation rate is small (i.e., 10?10 W kg?1) below the near surface and observations of mode-1 internal tide energy-flux convergence are indistinguishable from zero (i.e., the confidence intervals include zero), indicating little decay of the mode-1 internal tide within the Tasman Sea.
    publisherAmerican Meteorological Society
    titleObservations of the Tasman Sea Internal Tide Beam
    typeJournal Paper
    journal volume48
    journal issue6
    journal titleJournal of Physical Oceanography
    identifier doi10.1175/JPO-D-17-0116.1
    journal fristpage1283
    journal lastpage1297
    treeJournal of Physical Oceanography:;2018:;volume 048:;issue 006
    contenttypeFulltext
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    DSpace software copyright © 2002-2015  DuraSpace
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