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Abstract
Working within the domain of inviscid incompressible MHD theory, we found that a tangential discontinuity (TD) separating two uniform regions of different density, velocity and magnetic field may be Kelvin-Helmholtz (KH) stable and yet a study of a transition between the same constant regions given by a continuous velocity profile shows the presence of the instability with significant growth rates. Since the cause of the instability stems from the velocity gradient, and since a TD may be considered as the ultimate limit of such gradient, the statement comes as a surprise. In fact, a long wavelength (lambda) boundary for the KH instability does not exist in ordinary liquids being instead a consequence of the presence of magnetic shear, a possibility that has passed unnoticed in the literature. It is shown that KH modes of a magnetic field configuration with constant direction do not have the long lambda boundary. A theoretical explanation of this feature and examples of the violation of the TD stability condition are given using a model that can be solved in closed form. Stability diagrams in the (kd, MA) plane are given (where kd = 2pid/lambda, 2d is the velocity gradient length scale, and MA is the Alfvénic Mach number) that show both the well-known limit at small lambdas and the boundary for large but finite lambdas noted here. Consequences of this issue are relevant for stability studies of the dayside magnetopause as the stability condition for a TD should be used with care in data analysis work.
Publication Date
12-1-2004
Journal Title
Brazilian Journal of Physics
Publisher
Scielo
Digital Object Identifier (DOI)
Document Type
Article
Recommended Citation
Gratton, FT; Gnavi, G; Farrugia, CJ; Bender, L (2004). On the MHD boundary of Kelvin-Helmholtz stability diagram at large wavelengths, BRAZILIAN JOURNAL OF PHYSICS. Vol. 34, No. 4B, 1804-1813. DOI: 10.1590/S0103-97332004000800053
Comments
This is an article published by Scielo in Brazilian Journal of Physics in 2004, available online: https://dx.doi.org/10.1590/S0103-97332004000800053