Ion distributions upstream of earthward propagating dipolarization fronts

Physics – Plasma Physics

Scientific paper

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[2736] Magnetospheric Physics / Magnetosphere/Ionosphere Interactions, [2744] Magnetospheric Physics / Magnetotail, [2764] Magnetospheric Physics / Plasma Sheet, [7807] Space Plasma Physics / Charged Particle Motion And Acceleration

Scientific paper

We present case studies of THEMIS multi-point observations on ion distributions in the magnetotail plasma sheet at various locations upstream of earthward propagating dipolarization fronts. Gradual enhancements of earthward-moving ion fluxes have been observed in the central plasma sheet ~ 30 seconds before front arrivals, a characteristic signature well explained in previous studies as front-reflected ions coexisting with the ambient population in a confined region characterized by their gyroradii over background Bz field. In the plasma sheet boundary layer, observations have shown the appearances of earthward moving ions a few more minutes earlier than their appearances in the central plasma sheet, indicating a larger accessibility region of front-reflected ions. As the magnetic field lines are predominantly in the x direction in the plasma sheet boundary layer, the reflected ions could move along the field lines and eventually result in auroral activities in the ionosphere. Numerical simulations, as well as theoretical analysis of ion dynamics, have been carried out to interpret the observed patterns of ion distributions, and to improve our understandings of interactions between earthward propagating fronts and the ambient plasma in the near-Earth magnetotail.

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