The Atmosphere of Io: Abundances and Sources of Sulfur Dioxide and Atomic Hydrogen

Details The Atmosphere of Io: Abundances and Sources of Sulfur Dioxide and Atomic Hydrogen The Atmosphere of Io: Abundances and Sources of Sulfur Dioxide and Atomic Hydrogen

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.277..271s&link_type=abstract

Astrophysics and Space Science, v. 277, Issue 1/2, p. 271-287 (2001).

Astronomy and Astrophysics

Astrophysics

24

Scientific paper

An analysis and interpretation of reflected solar Lyman α intensity data acquired with the Hubble Space Telescope (HST) implies an equatorially confined atmosphere with SO2 column densities ˜ 1 2 × 1016 cm-2. Poleward of 30° the SO2 density must decrease sharply reaching an asymptotic polar value of < 1015 cm-2 at 45° to achieve the observed 2 kR intensity peaks. The corresponding surface reflectivities must be either a constant 0.047 for higher equatorial SO2 or a variable reflectivity of 0.027 with lower SO2 densities at the equator increasing to a polar value of ˜ 0.05. The average residence time for an atmospheric SO2 molecule is ˜ 2 3 days for the canonical mass loading rate of the Io plasma torus = 1030 amu s-1. With atomic hydrogen in the atmosphere and corona constrained by the HST observations, it is estimated that a pickup proton density ratio of 0.25 0.4% can be sustained by a supply of Io plasma torus protons neutralized in Io's atmosphere/exosphere, if protons constitute 7% of the total torus ion density, which is close to the Chust et al. (1999) pickup proton density ratio and under the widely quoted 10% proton content of the torus.

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