Gravity wave-fine structure interactions: A reservoir of small-scale and large-scale turbulence energy

被引:29
作者
Fritts, David C. [1 ]
Wang, Ling [1 ]
Werne, Joe [1 ]
机构
[1] NW Res Associates Inc, Colorado Res Associates Div, Boulder, CO 80301 USA
基金
美国国家科学基金会;
关键词
NOCTURNAL BOUNDARY-LAYER; INSTABILITY DYNAMICS; EVOLUTION; SHEAR; TEMPERATURE; ATMOSPHERE; RADAR; STATISTICS; TRANSITION; GENERATION;
D O I
10.1029/2009GL039501
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A direct numerical simulation of gravity wave-fine structure interactions is performed to evaluate the effects of such a superposition on instability and turbulence for fine structure shears and a gravity wave (GW) amplitude that are individually stable. The superposition leads to deformations of the fine structure and GW fields that exhibit Kelvin-Helmholtz (KH) shear instabilities and turbulence extending over more than 20 buoyancy periods. KH instabilities occur on multiple scales, deplete the kinetic energy of the initial fine structure, and yield a layering of the potential temperature field resembling "sheet and layer'' structures observed in the oceans and the atmosphere. The interactions have a much smaller effect on the GW amplitude. Such interactions among GWs and fine structure are likely ubiquitous throughout the atmosphere and oceans and may account for sporadic bursts of turbulence and its persistence in regions of apparent static and dynamic stability (Ri > 1/4). Citation: Fritts, D. C., L. Wang, and J. Werne (2009), Gravity wave-fine structure interactions: A reservoir of small-scale and large-scale turbulence energy, Geophys. Res. Lett., 36, L19805, doi: 10.1029/2009GL039501.
引用
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页数:6
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