Evolution of Turbulence in the Diurnal Warm LayerSource: Journal of Physical Oceanography:;2017:;volume 048:;issue 002::page 383DOI: 10.1175/JPO-D-17-0170.1Publisher: American Meteorological Society
Abstract: AbstractThe daily evolution of temperature, stratification, and turbulence in the diurnal warm layer is described from time series measurements at low to moderate winds and strong insolation in the equatorial Indian Ocean. At 2.0-m depth, turbulence dissipation rates (ε) decreased by two orders of magnitude over 1?2 h immediately after sunrise, initiated by stratification caused by penetrating solar radiation prior to the change in sign of net surface heat flux from cooling to warming. Decaying turbulence preceded a period of rapid growth, in which ε increased by two orders of magnitude over a few hours, and following which ε approached a daytime period of near-steady state. Decay and growth rates predicted by a simplified turbulence model are consistent with those observed. During the daytime period of near-steady state, asymmetric temperature ramps were associated with enhanced ε, supporting the interpretation that this period represents a balance between buoyancy and shear production associated with a shear-driven response to trapping of momentum within the diurnal warm layer.
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contributor author | Moulin, Aurélie J. | |
contributor author | Moum, James N. | |
contributor author | Shroyer, Emily L. | |
date accessioned | 2019-09-19T10:02:38Z | |
date available | 2019-09-19T10:02:38Z | |
date copyright | 12/28/2017 12:00:00 AM | |
date issued | 2017 | |
identifier other | jpo-d-17-0170.1.pdf | |
identifier uri | http://yetl.yabesh.ir/yetl1/handle/yetl/4260907 | |
description abstract | AbstractThe daily evolution of temperature, stratification, and turbulence in the diurnal warm layer is described from time series measurements at low to moderate winds and strong insolation in the equatorial Indian Ocean. At 2.0-m depth, turbulence dissipation rates (ε) decreased by two orders of magnitude over 1?2 h immediately after sunrise, initiated by stratification caused by penetrating solar radiation prior to the change in sign of net surface heat flux from cooling to warming. Decaying turbulence preceded a period of rapid growth, in which ε increased by two orders of magnitude over a few hours, and following which ε approached a daytime period of near-steady state. Decay and growth rates predicted by a simplified turbulence model are consistent with those observed. During the daytime period of near-steady state, asymmetric temperature ramps were associated with enhanced ε, supporting the interpretation that this period represents a balance between buoyancy and shear production associated with a shear-driven response to trapping of momentum within the diurnal warm layer. | |
publisher | American Meteorological Society | |
title | Evolution of Turbulence in the Diurnal Warm Layer | |
type | Journal Paper | |
journal volume | 48 | |
journal issue | 2 | |
journal title | Journal of Physical Oceanography | |
identifier doi | 10.1175/JPO-D-17-0170.1 | |
journal fristpage | 383 | |
journal lastpage | 396 | |
tree | Journal of Physical Oceanography:;2017:;volume 048:;issue 002 | |
contenttype | Fulltext |