The mirror and ion cyclotron anisotropy instabilities

Physics – Plasma Physics

Scientific paper

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Anisotropic Media, Ion Cyclotron Radiation, Magnetohydrodynamic Stability, Plasma-Electromagnetic Interaction, Space Plasmas, Magnetic Mirrors, Magnetosheath, Plasma Physics, Vlasov Equations

Scientific paper

The linear dispersion equation for fully electromagnetic waves and instabilities at arbitrary directions of propagation relative to a background magnetic field B(0) in a homogeneous Vlasov plasma is solved numerically for bi-Maxwellian particle distributions. For isotropic plasmas the dispersion and damping of the three modes below the proton cyclotron frequency are studied as functions of Beta(i) and T(e)/T(i). The transport ratios of helicity, cross-helicity, Alfven ratio, compressibility, and parallel compressibility are defined. Under the condition that the proton temperature perpendicular to B(0) is greater than the parallel temperature, the growth rates and transport ratios of the mirror instability and the ion cyclotron anisotropy instability are examined and compared. Both the proton parallel compressibility and the proton Alfven ratio are significantly different for the two growing modes.

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