A new tool for analyzing microinstabilities in space plasmas modeled by a generalized Lorentzian (kappa) distribution

Physics

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Lorentz Transformations, Magnetohydrodynamic Stability, Maxwell Equation, Plasma Currents, Space Plasmas, Planetary Magnetospheres, Solar Wind

Scientific paper

The modified plasma dispersion function Z* sub kappa (xi) based on the generalized Lorentzian distribution, which was introduced by Summers and Thorne (1991), is used to analyze three classical problems of plasma physics. These include the Landau damping of Langmuir waves, the ion acoustic instability in a current-carrying plasma, and the cyclotron resonant instability of electromagnetic R mode waves propagating parallel to an ambient magnetic field. It was found that, in each case, the results for a generalized Lorentzian plasma can differ significantly from those for a Maxwellian plasma. It is suggested that previous calculations based on a Maxwellian plasma distribution function Z(xi) have to be reexamined.

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