Charged particles moving in a spiral trajectory along magnetic lines of force in extended gravitational fields, and plasma capture by the peaks of the lines of force

Physics

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Charged Particles, Gravitational Fields, Lines Of Force, Magnetically Trapped Particles, Particle Trajectories, Plasma Interactions, Auroras, Earth Magnetosphere, Magnetic Fields, Plasma Dynamics, Radiation Belts, Solar Wind

Scientific paper

Formulas obtained for energetic charged particles moving in spiral trajectories in combined magnetic and gravitational fields can be applied to the case of the solar wind-magnetospheric interaction and the formation of radiation belts, auroras, and various polar cap phenomena. It is shown that the motionless plasma can be trapped by the peaks of the magnetic lines of force only if the velocity of its particles is greater than approximately half the drift velocity.

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