Inverse cascades in rotating stratified turbulence: Fast growth of large scales

被引:72
|
作者
Marino, R. [1 ]
Mininni, P. D. [1 ,2 ,3 ]
Rosenberg, D. [4 ]
Pouquet, A. [1 ,5 ]
机构
[1] Natl Ctr Atmospher Res, Boulder, CO 80307 USA
[2] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Fis, RA-1428 Buenos Aires, DF, Argentina
[3] Consejo Nacl Invest Cient & Tecn, IFIBA, RA-1428 Buenos Aires, DF, Argentina
[4] Oak Ridge Natl Lab, Natl Ctr Computat Sci, Oak Ridge, TN 37831 USA
[5] Univ Colorado, Dept Appl Math, Boulder, CO 80309 USA
基金
美国国家科学基金会;
关键词
2-DIMENSIONAL TURBULENCE; GEOSTROPHIC TURBULENCE; SOLAR-WIND; ENERGY; FLOWS;
D O I
10.1209/0295-5075/102/44006
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We examine the inverse cascade of kinetic energy to large scales in rotating stratified turbulence as occurs in the oceans and in the atmosphere, while varying the relative frequency of gravity to inertial waves, N/f. Using direct numerical simulations with grid resolutions up to 1024(3) points, we find that the transfer of energy from three-dimensional to two-dimensional modes is most efficient in the range 1/2 <= N/f <= 2, in which resonances disappear. In this range, the cascade is faster than in the purely rotating case, and thus the interplay between rotation and stratification helps creating large-scale structures. The ensuing inverse cascade follows a - 5/3 spectral law with an approximately constant flux. This inverse cascade becomes negligible when stratification is dominant. Copyright (c) EPLA, 2013
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页数:6
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