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Bagenal 1997
Bagenal, F. (1997). The ionization source near Io from Galileo wake data. Geophysical Research Letters 24: doi: 10.1029/97GL02052. issn: 0094-8276.

From measurements of plasma fluxes obtained along the Galileo trajectory through the wake of Io we estimate the source of ions within 5 RIo of the satellite to be 0.5 to 1.7¿1028 s-1 (18 to 58% of the canonical 3¿1028 s-1 torus supply rate). This source of ionization close to Io can supply 0.3 to 0.8¿1012 watts to the torus plasma (15 to 28% of the canonical 3¿1012 watts of EUV emissions from the torus). Modeling the energy flux at the spacecraft with local ionization matches the observations reasonably well, which we interpret as evidence against extensive additional charge exchange reactions occurring near Io.¿ 1997 American Geophysical Union

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Abstract

Keywords
Planetology, Comets and Small Bodies, Interactions with solar wind plasma and fields, Magnetospheric Physics, Planetary magnetospheres (5443, 5737, 6030), Magnetospheric Physics, Magnetosphere interactions with satellites and rings, Space Plasma Physics, Ionization processes
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
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