Mass-loading and diffusion-loss rates of the Io plasma torus

Details Mass-loading and diffusion-loss rates of the Io plasma torus Mass-loading and diffusion-loss rates of the Io plasma torus

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...242.1266s&link_type=abstract

Astrophysical Journal, Part 1, vol. 242, Dec. 15, 1980, p. 1266-1277.

Astronomy and Astrophysics

Astrophysics

62

Cosmic Plasma, Io, Planetary Mass, Plasma Diffusion, Satellite Atmospheres, Ion Density (Concentration), Mass Distribution, Planetary Magnetic Fields, Toroidal Plasmas

Scientific paper

Limits to the mass-loading and diffusion-loss rates of ions in the Io plasma torus have been calculated on the assumption that observed optical emissions are controlled by electron-ion collisions. Calculations of the yield of emission from the vicinity of Io limit the mass-loading rate to the order of 10 to the 27th per s for S II or O II, on the grounds that electron-excited emissions associated with the location of Io have not been observed in the optical spectrum. This mass-loading limit is dependent on the assumptions that Io is the source of torus particles and that most of the neutral atoms are converted to ions within 1 R(J) of Io. According to the calculations presented below, the observed partitioning of sulfur ion species in the hot torus at the time of Voyager 1 encounter indicates that the diffusion-loss time of the ions is of the order of 1/D = 100 days. The two results limiting the mass-loading and diffusion-loss rates are compatible and suggest that the energy required to maintain the observed radiated power cannot be supplied by acceleration of ions formed at Io in Jupiter's rotating magnetic field.

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