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Cited by 567

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Nonlinear standing Alfvén wave current system at Io: Theory

Neubauer, F.M.·1980·Journal of Geophysical Research: Space Physics

Abstract

We present a nonlinear analytical model of the Alfvén current tubes continuing the currents through Io (or rather its ionosphere) generated by the unipolar inductor effect due to Io's motion relative to the magnetospheric plasma. We thereby extend the linear work by Drell et al. (1965) to the fully nonlinear, sub‐Alfvénic situation also including flow which is not perpendicular to the background magnetic field. The following principal results have been obtained: (1) The portion of the currents feeding Io is aligned with the Alfvén characteristics at an angle θA = tan−1 M A to the magnetic field for the special case of perpendicular flow where M A is the Alfvén Mach number. (2) The Alfvén tubes act like an external conductance ΣA = 1/(µ 0V A(1 + M A² + 2 M A sin θ)1/2) where V A is the Alfvén speed and θ the angular deviation from perpendicular flow towards the direction of Alfvén wave propagation. Hence the Jovian ionospheric conductivity is not necessary for current closure. (3) In addition, the Alfvén tubes may be reflected from either the torus boundary or the Jovian ionosphere. The efficiency of the resulting interaction with these boundaries varies with Io position. The interaction is particularly strong at extreme magnetic latitudes, thereby suggesting a mechanism for the Io control of decametric emissions. (4) The reflected Alfvén waves may heat both the torus plasma and the Jovian ionosphere as well as produce increased diffusion of high‐energy particles in the torus. (5) From the point of view of the electrodynamic interaction, Io is unique among the Jovian satellites for several reasons: these include its ionosphere arising from ionized volcanic gases, a high external Alfvénic conductance ΣA, and a high corotational voltage in addition to the interaction phenomenon with a boundary. (6) We find that Amalthea is probably strongly coupled to Jupiter's ionosphere while the outer Galilean satellites may occasionally experience super‐Alfvénic conditions.

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Metadata

Authors
Neubauer, F. M.
Venue
Journal of Geophysical Research: Space Physics
Published
1980-03
Volume
85
Issue
A3
Pages
1171-1178
ISSN
0148-0227 (ISSN-L)
OpenAlex
W2058990725
Cited by
567
References
3
FWCI
21.10
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Nonlinear standing Alfvén wave current system at Io: Theory. https://app.cochat.ai/papers/10.1029/ja085ia03p01171
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Neubauer, F. M. (1980). Nonlinear standing Alfvén wave current system at Io: Theory. Journal of Geophysical Research: Space Physics. https://doi.org/10.1029/ja085ia03p01171

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