Sulfur and oxygen escape from Io and a lower limit to atmospheric SO2 at Voyager 1 encounter

Details Sulfur and oxygen escape from Io and a lower limit to atmospheric SO2 at Voyager 1 encounter Sulfur and oxygen escape from Io and a lower limit to atmospheric SO2 at Voyager 1 encounter

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.7399k&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, Sept. 1, 1984, p. 7399-7406.

Physics

37

Atmospheric Composition, Gas Transport, Io, Satellite Atmospheres, Space Plasmas, Sulfur Dioxides, Escape, Outgassing, Oxygen Ions, Sulfur, Toroidal Plasmas, Voyager 1 Spacecraft, Jupiter, Satellites, Io, Sulfur, Oxygen, Atmosphere, Sulfur Dioxide, Voyager 1, Transport, Plasma Torus, Escape, Volcanism, Sputtering, Surface, Frost, Ions, Corotation, Magnetosphere, Flux, Energy, Thickness, Photochemistry, Models, Pressure, Density

Scientific paper

Estimates of the abundance of sulfur, sodium and oxygen ions and neutrals observed by Voyager 1 in the plasma torus and neutral cloud associated with the Jovian satellite Io are used to investigate the physical characteristics of the Io atmosphere. Specific attention is given to two questions about the Io atmosphere: the necessity of an atmosphere to account for the supply of sulfur and oxygen observed in the plasma torus, and, if an atmosphere is necessary, the lower limit to such atmosphere. It is found that an SO2 atmosphere is most likely needed on Io as an intermediate buffer so that the sulfur and oxygen can be transported to the plasma torus. The minimum atmosphere needed for this process is calculated to be 1.4 x 10 to the -10th bar with an SO2 column density of about 10 to the 16th per sq cm and an SO2 surface density of about 1.2 x 10 to the 10th per cu cm. A complete list of all the atmospheric escape fluxes for Io is provided.

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