Turbulence and jet-driven zonal flows: Secondary circulation in rotating fluids due to asymmetric forcing

被引:3
|
作者
Burin, M. J. [1 ]
Caspary, K. J. [2 ]
Edlund, E. M. [3 ]
Ezeta, R. [4 ,5 ]
Gilson, E. P. [2 ]
Ji, H. [2 ,6 ]
McNulty, M. [7 ]
Squire, J. [8 ,9 ]
Tynan, G. R. [10 ,11 ]
机构
[1] Calif State Univ San Marcos, Dept Phys, San Marcos, CA 92096 USA
[2] Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ 08544 USA
[3] SUNY Coll Cortland, Dept Phys, Cortland, NY 13045 USA
[4] Univ Twente, Mesa Inst, Max Planck Ctr Complex Fluid Dynam, POB 217, NL-7500 AE Enschede, Netherlands
[5] Univ Twente, JM Burgers Ctr Fluid Dynam, POB 217, NL-7500 AE Enschede, Netherlands
[6] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
[7] Univ Calif Riverside, Dept Math, Riverside, CA 92521 USA
[8] Univ Otago, Dept Phys, Dunedin 9016, New Zealand
[9] CALTECH, Theoret Astrophys, Pasadena, CA 91125 USA
[10] Univ Calif San Diego, Jacobs Sch Engn, Dept Mech Engn, San Diego, CA 92093 USA
[11] Univ Calif San Diego, Jacobs Sch Engn, Ctr Energy Res, San Diego, CA 92093 USA
关键词
GENERATION; INSTABILITY; DYNAMICS; ROSSBY;
D O I
10.1103/PhysRevE.99.023108
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We report on experiments and modeling on a rotating confined liquid that is forced by circumferential jets coaxial with the rotation axis, wherein system-scale secondary flows are observed to emerge. The jets are evenly divided in number between inlets and outlets and have zero net mass transport. For low forcing strengths the sign of this flow depends on the sign of a sloped end cap, which simulates a planetary f plane. For increased forcing strengths the secondary flow direction is insensitive to the slope sign, and instead appears to be dominated by an asymmetry in the forcing mechanism, namely, the difference in radial divergence between the inlet and outlet jet profiles. This asymmetry yields a net radial velocity that is affected by the Coriolis force, inducing secondary zonal flow.
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收藏
页数:7
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