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• W3100692445 abstract "The solar corona is a typical example of a plasma with strongly anisotropic transport processes. The main dissipative mechanisms in the solar corona acting on slow magnetoacoustic waves are the anisotropic thermal conductivity and viscosity [Ballai et al., Phys. Plasmas 5, 252 (1998)] developed the nonlinear theory of driven slow resonant waves in such a regime. In the present paper the nonlinear behavior of driven magnetohydrodynamic waves in the slow dissipative layer in plasmas with strongly anisotropic viscosity and thermal conductivity is expanded by considering dispersive effects due to Hall currents. The nonlinear governing equation describing the dynamics of nonlinear resonant slow waves is supplemented by a term which describes nonlinear dispersion and is of the same order of magnitude as nonlinearity and dissipation. The connection formulas are found to be similar to their nondispersive counterparts." @default.
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• W3100692445 date "2008-08-01" @default.
• W3100692445 modified "2023-10-05" @default.
• W3100692445 title "Nonlinear theory of resonant slow waves in anisotropic and dispersive plasmas" @default.
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• W3100692445 doi "https://doi.org/10.1063/1.2970947" @default.
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