The DOI matches its Crossref record; 3 of the 3 references it cites were found in a registry or an index.
Nonlinear standing Alfvén wave current system at Io: Theory
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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Cites
The Jupiter System Through the Eyes of Voyager 1
Smith, B. A., Soderblom, L. A., Johnson, T. V., Ingersoll, A. P., Collins, S. A., Shoemaker, E. M., Hunt, G. E., Masursky, H., Carr, M. H., Davies, M. E., et al. (1979) · Science · doi:10.1126/science.204.4396.951 · Cited by 780
Extreme Ultraviolet Observations from Voyager 1 Encounter with Jupiter
Broadfoot, A. L., Belton, M. J. S., Takacs, P. Z., Sandel, B. R., Shemansky, D. E., Holberg, J. B., Ajello, J. M., Atreya, S. K., Donahue, T. M., Moos, H. W., et al. (1979) · Science · doi:10.1126/science.204.4396.979 · Cited by 761
Io, a jovian unipolar inductor
Goldreich, P., & Lynden-Bell, D. (1969) · The Astrophysical Journal · doi:10.1086/149947 · Cited by 513
Cited by
Galileo Magnetometer Measurements: A Stronger Case for a Subsurface Ocean at Europa
Kivelson, M. G., Khurana, K. K., Russell, C. T., Volwerk, M., Walker, R. J., & Zimmer, C. (2000) · Science · doi:10.1126/science.289.5483.1340 · Cited by 724
Stellar wind regimes of close-in extrasolar planets
Preusse, S., Kopp, A., Büchner, J., & Motschmann, U. (2005) · Astronomy & Astrophysics · doi:10.1051/0004-6361:20041680 · Cited by 76
Metadata
- Authors
- Neubauer, F. M.
- Venue
- Journal of Geophysical Research: Space Physics
- Publisher
- American Geophysical Union (AGU)
- 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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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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