Interacting vorticity waves as an instability mechanism for magnetohydrodynamic shear instabilities

被引:25
作者
Heifetz, E. [1 ,2 ]
Mak, J. [1 ]
Nycander, J. [2 ]
Umurhan, O. M. [3 ,4 ]
机构
[1] Tel Aviv Univ, Dept Geophys & Planetary Sci, IL-69978 Tel Aviv, Israel
[2] Stockholm Univ, Dept Meteorol MISU, SE-10691 Stockholm, Sweden
[3] NASA Ames Res, Div Space Sci, Mountain View, CA 94043 USA
[4] SETI Inst, Mountain View, CA 94043 USA
关键词
instability; magnetic fluids; MUD and electrohydrodynamics; BAROCLINIC INSTABILITY; JOINT INSTABILITY; FLOW; PERSPECTIVE; STABILITY; DYNAMICS; FIELDS;
D O I
10.1017/jfm.2015.47
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
The interacting vorticity wave formalism for shear flow instabilities is extended here to the magnetohydrodynamic (MUD) setting, to provide a mechanistic description for stabilising and destabilising shear instabilities by the presence of a background magnetic field. The interpretation relies on local vorticity anomalies inducing a non-local velocity field, resulting in action at a distance. It is shown here that the waves supported by the system are able to propagate vorticity via the Lorentz force, and waves may interact. The existence of instability then rests upon whether the choice of basic state allows for phase locking and constructive interference of the vorticity waves via mutual interaction. To substantiate this claim, we solve the instability problem of two representative basic states, one where a background magnetic field stabilises an unstable flow and the other where the field destabilises a stable flow, and perform relevant analyses to show how this mechanism operates in MHD.
引用
收藏
页码:199 / 225
页数:27
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