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contributor authorThomson, Jim
contributor authorSchwendeman, Michael S.
contributor authorZippel, Seth F.
contributor authorMoghimi, Saeed
contributor authorGemmrich, Johannes
contributor authorRogers, W. Erick
date accessioned2017-06-09T17:21:37Z
date available2017-06-09T17:21:37Z
date copyright2016/06/01
date issued2016
identifier issn0022-3670
identifier otherams-83799.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4227063
description abstractbservations of winds, waves, and turbulence at the ocean surface are compared with several analytic formulations and a numerical model for the input of turbulent kinetic energy by wave breaking and the subsequent dissipation. The observations are generally consistent with all of the formulations, although some differences are notable at winds greater than 15 m s?1. The depth dependence of the turbulent dissipation rate beneath the waves is fit to a decay scale, which is sensitive to the choice of vertical reference frame. In the surface-following reference frame, the strongest turbulence is isolated within a shallow region of depths much less than one significant wave height. In a fixed reference frame, the strong turbulence penetrates to depths that are at least half of the significant wave height. This occurs because the turbulence of individual breakers persists longer than the dominant period of the waves and thus the strong surface turbulence is carried from crest to trough with the wave orbital motion.
publisherAmerican Meteorological Society
titleWave-Breaking Turbulence in the Ocean Surface Layer
typeJournal Paper
journal volume46
journal issue6
journal titleJournal of Physical Oceanography
identifier doi10.1175/JPO-D-15-0130.1
journal fristpage1857
journal lastpage1870
treeJournal of Physical Oceanography:;2016:;Volume( 046 ):;issue: 006
contenttypeFulltext


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