Kinetic Theory of the Inner Magnetospheric Plasma
The inner magnetosphere plasma is a very unique composition of different plasma particles and waves. It covers a huge energy plasma range with spatial and time variations of many orders of magnitude. In such a situation, the kinetic approach is the key element, and the starting point of the theoretical description of this plasma phenomena which requires a dedicated book to this particular area of research.
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Alfve´n altitude approximation auroral beam bounce-averaged calculated cmÀ3 collision integral collisional collisionless components convection Coulomb collisions cyclotron ð Þ decrease dependence drift Earth’s effects electric field electron temperature EMIC waves energy distribution field-aligned frequency geomagnetic field Geophys growth rate heat flux Heþ Heþ-mode hydrodynamic inelastic collisions injection inner magnetosphere instability interaction ionization ionosphere ionospheric plasma isotropic Khazanov kinetic equation Konikov Kozyra Landau damping Liemohn loss cone Loto’aniu magnetic field observed obtained oscillations parameters peak perpendicular photoelectron pitch pitch-angle plasma density plasma oscillations plasmapause plasmasphere polar wind potential energy precipitating presented processes region relativistic electron resonance ring current scattering Schunk secondary electrons self-consistent simulation solar solution Space Sci spatial spectra spectrum storm superthermal electrons temperature anisotropy tensor thermal electrons thermal plasma timescale tion trapped zone values velocity wave normal angle wave packet wave power wave vector