Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...234.1148s&link_type=abstract
Astrophysical Journal, Part 1, vol. 234, Dec. 15, 1979, p. 1148-1153.
Astronomy and Astrophysics
Astrophysics
13
Atmospheric Composition, D Lines, Io, Sodium Vapor, Spatial Distribution, Asymmetry, Emission Spectra, Light Scattering, Pressure Effects, Radiation Pressure, Solar Radiation
Scientific paper
An explanation of the east-west asymmetries of Io's sodium clouds is suggested based upon the force experienced by sodium atoms as they resonantly scatter sunlight and upon the ability of this force to alter the cloud atom orbits, as determined by the gravitational fields of Io and Jupiter. Orbit calculations illustrating the time-dependent changes in the sodium atom trajectories produced by the solar radiation force as a function of Io's orbital location are presented in support of this explanation. This theory agrees with the idea that sodium atoms are emitted from the satellite nonisotropically and at a constant rate. These conclusions may be important in studying the global effects of active volcanoes and the intense satellite plasma torus discovered for Io from Voyager I spacecraft measurements.
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