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- W1488755512 abstract "Numerical simulation of global formation of auroral arcs is performed for a three-dimensional coupled ionosphere-magnetosphere system. Under the presence of the stationary convection electric field, the field-aligned current driven by the polarization and drift of the ionospheric conductivity enhancement is shown to be responsible for the feedback instability (Sato, 1978) of the shear Alfvén wave. The simulation result demonstrates the dynamic process of auroral arc formation, in which an ionospheric perturbation nearly resonant with the magnetospheric Alfvén wave (toroidal mode) can grow eventually into auroral arcs. Many of the important characteristics of quiet auroral arcs are demonstrated, and the overall distribution of auroras is shown to depend critically on the stationary state of the auroral oval characterized by the large-scale Birkeland current, the electric field, and the electron density distribution." @default.
- W1488755512 created "2016-06-24" @default.
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- W1488755512 date "2013-03-26" @default.
- W1488755512 modified "2023-09-23" @default.
- W1488755512 title "Global Simulation of Auroral Arcs" @default.
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- W1488755512 doi "https://doi.org/10.1029/gm025p0321" @default.
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