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Alfvén wings at Earth's magnetosphere under strong interplanetary magnetic fields

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Academic year: 2021

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Figure

Fig. 1. BATSRUS simulation of sub-Alfv´enic flow at the Earth (B z = − 100 nT). (Top) The block adaptive mesh used in the simu-lation with red lines indicating boundaries between different res-olutions
Fig. 2. The magnetospheric electric and magnetic fields in the Y = 0 plane as a function of interplanetary magnetic field B z
Fig. 4. Field-aligned current (left) in µA/m 2 and potential (right) in kV for the nominal (top) and sub-Alfv´enic (bottom) cases
Fig. 5. A plot of the ionospheric cross polar cap potential as a func- func-tion of IMF B z
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