Model of Convective Taylor Columns in Rotating Rayleigh-Benard Convection

被引:67
|
作者
Grooms, Ian [1 ]
Julien, Keith [1 ]
Weiss, Jeffrey B. [2 ]
Knobloch, Edgar [3 ]
机构
[1] Univ Colorado, Dept Appl Math, Boulder, CO 80309 USA
[2] Univ Colorado, Dept Atmospher & Ocean Sci, Boulder, CO 80309 USA
[3] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
基金
美国国家科学基金会;
关键词
OPEN-OCEAN CONVECTION; SPREADING PHASE; DEEP CONVECTION; FLUID LAYER; TURBULENCE; DYNAMICS; CELLS;
D O I
10.1103/PhysRevLett.104.224501
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Observations, and laboratory and numerical studies, of fluid flows with strong rotation and thermal forcing often show long-lived convective Taylor columns (CTCs) which carry a large portion of the vertical heat and mass fluxes. However, owing to experimental and numerical challenges, these structures remain poorly understood. Here we present a nonlinear, analytical multiscale model of CTCs in the context of rotating Rayleigh-Benard convection that successfully matches numerical simulations and provides a new multiscale interpretation of the Taylor-Proudman constraint.
引用
收藏
页数:4
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