Helmholtz instability in stratified shear flows with magnetic fields

1983 ◽  
Vol 95 (2) ◽  
pp. 277-282 ◽  
Author(s):  
A. Satya Narayanan
2013 ◽  
Vol 31 (9) ◽  
pp. 1535-1541 ◽  
Author(s):  
K.-I. Nishikawa ◽  
P. Hardee ◽  
B. Zhang ◽  
I. Duţan ◽  
M. Medvedev ◽  
...  

Abstract. We have investigated the generation of magnetic fields associated with velocity shear between an unmagnetized relativistic jet and an unmagnetized sheath plasma. We have examined the strong magnetic fields generated by kinetic shear (Kelvin–Helmholtz) instabilities. Compared to the previous studies using counter-streaming performed by Alves et al. (2012), the structure of the kinetic Kelvin–Helmholtz instability (KKHI) of our jet-sheath configuration is slightly different, even for the global evolution of the strong transverse magnetic field. In our simulations the major components of growing modes are the electric field Ez, perpendicular to the flow boundary, and the magnetic field By, transverse to the flow direction. After the By component is excited, an induced electric field Ex, parallel to the flow direction, becomes significant. However, other field components remain small. We find that the structure and growth rate of KKHI with mass ratios mi/me = 1836 and mi/me = 20 are similar. In our simulations saturation in the nonlinear stage is not as clear as in counter-streaming cases. The growth rate for a mildly-relativistic jet case (γj = 1.5) is larger than for a relativistic jet case (γj = 15).


2018 ◽  
Vol 30 (9) ◽  
pp. 092002 ◽  
Author(s):  
Md Rifat Hassan ◽  
Jie Zhang ◽  
Cheng Wang

2020 ◽  
Vol 32 (7) ◽  
pp. 073306 ◽  
Author(s):  
L. H. P. Cunha ◽  
I. R. Siqueira ◽  
F. R. Cunha ◽  
T. F. Oliveira
Keyword(s):  

1959 ◽  
Vol 6 (4) ◽  
pp. 583-598 ◽  
Author(s):  
John W. Miles

The Kelvin-Helmholtz model for the formation of surface waves at the interface between two fluids in relative motion is generalized for parallel shear flows. It is assumed that phase changes across the flow are negligible and hence that the aerodynamic pressure on the wave is in phase with its displacement (rather than its slope). A variational formulation is established and leads to the determination of appropriately weighted means for the velocity profiles. The principal application is to flow of a light inviscid fluid over a viscous liquid; it is shown that the principle of exchange of stabilities is applicable to such a configuration, and a critical wind speed in satisfactory agreement with observation is predicted for an air-oil interface. The results also are applied to an air-water interface and lead to the conclusion that Kelvin-Helmholtz instability of such an interface is unlikely at commonly observed wind speeds. A more general formulation of the Kelvin-Helmholtz boundary-value problem and variational principle, allowing for variations in both velocity and density, is given in two appendices.


2011 ◽  
Vol 23 (9) ◽  
pp. 094107 ◽  
Author(s):  
Amey S. Joshi ◽  
M. C. Radhakrishna ◽  
N. Rudraiah

2018 ◽  
Vol 30 (4) ◽  
pp. 044102 ◽  
Author(s):  
Y. Liu ◽  
Z. H. Chen ◽  
H. H. Zhang ◽  
Z. Y. Lin

2010 ◽  
Vol 712 (2) ◽  
pp. 875-882 ◽  
Author(s):  
R. Soler ◽  
J. Terradas ◽  
R. Oliver ◽  
J. L. Ballester ◽  
M. Goossens

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