Outer satellite atmospheres: Their extended nature and planetary interactions

Details Outer satellite atmospheres: Their extended nature and planetary interactions Outer satellite atmospheres: Their extended nature and planetary interactions

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aeri.reptt....s&link_type=abstract

Interim Report, Sep. - Nov. 1983 Atmospheric and Environmental Research, Inc., Cambridge, MA.

Mathematics

Comets, Earth Magnetosphere, Mathematical Models, Satellite Atmospheres, Saturn (Planet), Titan, Gravitational Effects, Particle Trajectories, Radiation Pressure, Solar Radiation, Space-Time Functions, Spatial Distribution

Scientific paper

Model calculations for the spatial morphology of the Region B sodium cloud are presented that include both the oscillating plasma torus sink and solar radiation pressure in the D-lines. These calculations exhibit the qualitative behavior observed in the sodium cloud and have diagnostic capabilities to probe more deeply the atom ejection characteristics of the sodium source. Significant progress in specifying the plasma properties of Saturn's magnetosphere for use in the Titan hydrogen torus model is reported. Efforts to apply the AER comet model to calculations of the spatial distribution of the H atoms in cometary atmospheres are also discussed.

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