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 lo 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. Copyright 1997 by the American Geophysical Union.
CITATION STYLE
Bagenal, F. (1997). The ionization source near Io from Galileo wake data. Geophysical Research Letters, 24(17), 2111–2114. https://doi.org/10.1029/97GL02052
Mendeley helps you to discover research relevant for your work.