Boundary-layer turbulence in experiments on quasi-Keplerian flows

被引:25
|
作者
Lopez, Jose M. [1 ,2 ,3 ]
Avila, Marc [1 ,4 ]
机构
[1] Friedrich Alexander Univ Erlangen Nurnburg, Inst Fluid Mech, D-91058 Erlangen, Germany
[2] Univ Politecn Cataluna, Dept Fis Aplicada, Barcelona 08034, Spain
[3] Inst Sci & Technol, D-3400 Kolsterneuburg, Germany
[4] Univ Bremen, Ctr Appl Space Tech & Micrograv, D-28359 Bremen, Germany
关键词
rotating flows; Taylor-Couette flow; turbulent boundary layers; TAYLOR-COUETTE FLOW; ANGULAR-MOMENTUM TRANSPORT; ACCRETION DISKS; PROTOPLANETARY DISKS; SHEAR INSTABILITY; STRATIFIED DISKS; STABILITY; ROTATION; STARS; DISCS;
D O I
10.1017/jfm.2017.109
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Most flows in nature and engineering are turbulent because of their large velocities and spatial scales. Laboratory experiments on rotating quasi-Keplerian flows, for which the angular velocity decreases radially but the angular momentum increases, are however laminar at Reynolds numbers exceeding one million. This is in apparent contradiction to direct numerical simulations showing that in these experiments turbulence transition is triggered by the axial boundaries. We here show numerically that as the Reynolds number increases, turbulence becomes progressively confined to the boundary layers and the flow in the bulk fully relaminarizes. Our findings support that turbulence is unlikely to occur in isothermal constant-density quasi-Keplerian flows.
引用
收藏
页码:21 / 34
页数:14
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