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Introduction to Plasma Instabilities
MicroinstabilitiesInstabilities Due to Velocity Space Nonequi
MacroinstabilitiesInstabilities Due to Coordinate Space Non
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Alfven wave amplitude anisotropic assume beam becomes Buneman co/k coci cold electrons cold plasma collision frequency consider coupling cyclotron frequency density gradient derive dielectric constant diffusion direction discussed dispersion relation drift speed drift wave instability dynamics effect electric field electromagnetic electron stream electrons and ions electrostatic energy density envelope example expression field energy field line finite fluid flux Fourier Geophys given growth rate Hasegawa hence humped instability condition instability occurs integral interaction ion acoustic wave ion cyclotron wave ionosphere Kelvin-Helmholtz instability kinetic energy Landau damping magnetic field magnetic mirror magnetosphere mode Necessary condition negative dissipation nonlinear nonuniformity number density obtained from Eq oscillation parallel particle perpendicular phase velocity Phys plasma instabilities proton Section shown in Fig solar wind soliton solution stability stationary stream instability Subsection temperature term thermal speed three wave trapped unperturbed vector velocity space Vlasov equation wave number wave propagating wavelength