Observations of the Tasman Sea Internal Tide BeamSource: Journal of Physical Oceanography:;2018:;volume 048:;issue 006::page 1283Author: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-17-0116.1Publisher: 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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contributor author | Waterhouse, Amy F. | |
contributor author | Kelly, Samuel M. | |
contributor author | Zhao, Zhongxiang | |
contributor author | MacKinnon, Jennifer A. | |
contributor author | Nash, Jonathan D. | |
contributor author | Simmons, Harper | |
contributor author | Brahznikov, Dmitry | |
contributor author | Rainville, Luc | |
contributor author | Alford, Matthew | |
contributor author | Pinkel, Rob | |
date accessioned | 2019-09-19T10:02:25Z | |
date available | 2019-09-19T10:02:25Z | |
date copyright | 4/4/2018 12:00:00 AM | |
date issued | 2018 | |
identifier other | jpo-d-17-0116.1.pdf | |
identifier uri | http://yetl.yabesh.ir/yetl1/handle/yetl/4260868 | |
description 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. | |
publisher | American Meteorological Society | |
title | Observations of the Tasman Sea Internal Tide Beam | |
type | Journal Paper | |
journal volume | 48 | |
journal issue | 6 | |
journal title | Journal of Physical Oceanography | |
identifier doi | 10.1175/JPO-D-17-0116.1 | |
journal fristpage | 1283 | |
journal lastpage | 1297 | |
tree | Journal of Physical Oceanography:;2018:;volume 048:;issue 006 | |
contenttype | Fulltext |