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Incompressible Magnetohydrodynamic Kelvin–Helmholtz Instability with Continuous Profiles |
| ZHAO Kai-Ge1, WANG Li-Feng2,3, YE Wen-Hua2,3,4, WU Jun-Feng2**, LI Ying-Jun1** |
1State Key Laboratory for Geomechanics and Deep Underground Engineering, China University of Mining and Technology, Beijing 100083
2Institute of Applied Physics and Computational Mathematics, Beijing 100094
3HEDPS, Center for Applied Physics and Technology, Peking University, Beijing 100871
4Department of Physic, Zhejiang University, Hangzhou 310027
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| Cite this article: |
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ZHAO Kai-Ge, WANG Li-Feng, YE Wen-Hua et al 2014 Chin. Phys. Lett. 31 030401 |
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Abstract Effects of a continuous magnetic field in the direction of streaming on the incompressible Kelvin–Helmholtz instability (KHI) are investigated by solving the linear ideal magnetohydrodynamic equations. It is found that the frequency of the KHI is not influenced by the magnetic field. The magnetic field strength effect decreases the linear growth of the KHI, while the magnetic field gradient scale length effect increases its linear growth. The KHI can even be completely suppressed when the magnetic field is strong enough. The linear growth rate approaches a maximum when the magnetic field gradient scale length is large enough.
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Received: 12 August 2013
Published: 28 February 2014
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| PACS: |
04.30.Tv
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(Gravitational-wave astrophysics)
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47.20.Ft
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(Instability of shear flows (e.g., Kelvin-Helmholtz))
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52.30.Cv
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(Magnetohydrodynamics (including electron magnetohydrodynamics))
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