Nonideal momentum coupling between Iogenic plasma and the Jovian ionosphere

Physics

Scientific paper

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2756 Planetary Magnetospheres (5443, 5737, 6030), 5737 Magnetospheres (2756)

Scientific paper

The interaction between Io and Jupiter was dramatically illustrated by recent ultraviolet and infrared imaging of the Io-induced Jovian aurora. Bright auroral emissions were observed at the base of Io's flux tube with emissions at the footprint of Io's wake extending large distances downstream (roughly 180 deg around Jupiter). The extended emission trail is poorly understood. We propose as a possible explanation for the persisting wake emissions a nonideal plasma interaction between Iogenic plasma and the Jovian ionosphere that is caused by field-aligned electric fields. The fundamental problem is the transfer of momentum from the corotating torus/Jovian ionosphere to the subcorotating Iogenic plasma via the Alfvenic interaction. Intense field-aligned currents associated with the Alfvenic disturbance can lead to the formation of parallel electric fields. By comparing the field-aligned current density of the initial Alfvenic disturbance to that of a one-dimensional, steady-state Vlasov calculation for the Io flux tube, we infer a current limitation, or momentum decoupling, caused by a high latitude field-aligned potential drop. The resulting nonideal plasma flow allows decoupling between a subcorotating flux tube and the Jovian ionosphere and hence the persistence of auroral emissions for large distances downstream of the initial Io-disturbed flux tube.

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