The adiabatic motion of charged dust grains in rotating magnetospheres

Physics

Scientific paper

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Adiabatic Equations, Charged Particles, Earth Magnetosphere, Jupiter Rings, Particle Motion, Saturn Rings, Celestial Mechanics, Equations Of Motion, Interplanetary Dust, Planetary Atmospheres, Planetary Magnetic Fields, Planetary Rotation, Plasma-Particle Interactions, Rotating Plasmas

Scientific paper

Adiabatic equations of motion are derived for the micrometer-sized dust grains detected in the Jovian and Saturn magnetospheres by the Pioneer 10 and 11 spacecraft. The adiabatic theory of charged particle motion is extended to the case of variable grain charge. Attention is focused on the innermost and outermost limits to the grain orbit evolution, with all orbits tending to become circular with time. The parameters such as the center equation of motion, the drift velocity, and the parallel equation of motion are obtained for grains in a rotating magnetosphere. Consideration is given to the effects of periodic grain charge-discharge, which are affected by the ambient plasma properties and the grain plasma velocity. The charge-discharge process at the gyrofrequency is determined to eliminate the invariance of the magnetic moment and cause the grain to exhibit radial movement. The magnetic moment increases or decreases as a function of the gyrophase of the charge variation.

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