Physics
Scientific paper
Dec 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jgra..107.1464h&link_type=abstract
Journal of Geophysical Research (Space Physics), Volume 107, Issue A12, pp. SMP 27-1, CiteID 1464, DOI 10.1029/2002JA009514
Physics
9
Magnetospheric Physics: Auroral Phenomena (2407), Magnetospheric Physics: Planetary Magnetospheres (5443, 5737, 6030), Magnetospheric Physics: Magnetosphere Interactions With Satellites And Rings, Magnetospheric Physics: Magnetosphere/Ionosphere Interactions
Scientific paper
Auroral images of Jupiter reveal a distinctive signature of the downstream corotational wake of Io, as well as of Io itself. The wake signature can be understood as a product of the plasma current that accelerates Io's mass-loaded flux tube up to (almost) corotation with Jupiter. The radially directed acceleration current in the magnetosphere is linked by Birkeland (magnetic field aligned) currents to Jupiter's ionosphere where closure is provided by a meridional Pedersen current. The Pedersen current is proportional to the velocity of the plasma relative to the corotating frame, while the acceleration current is proportional to (minus) the time rate of change of that velocity. Thus the requirement of current closure implies a simple exponential decay of the relative velocity, with a time constant that is proportional to the ratio of flux-tube mass content to ionospheric Pedersen conductance. For expected values of these parameters, the time constant is ~ 0.5 hours, implying a length scale ~ 1 RJ (= Jupiter's radius) for the variation of velocity with downstream distance in the wake, or ~12° of longitude. This length scale is remarkably close to that of the observed brightness of the wake auroral signature.
Hill Thomas W.
Vasyliūnas Vytenis M.
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