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Detection of SO in Io's exosphere
1Institute of Geophysics and Planetary Physics, 3845 Slichter Hall, University of California Los Angeles, Los Angeles, CA 90095-1567, USA.
Summary
Galileo
Area of Science:
- Planetary Science
- Space Physics
- Plasma Physics
Background:
- Jupiter's moon Io possesses a tenuous atmosphere, or exosphere, primarily composed of sulfur dioxide (SO2).
- This exosphere is known to interact with Jupiter's magnetosphere, leading to plasma torus mass loading.
- Previous Galileo flybys provided initial evidence of this interaction.
Purpose of the Study:
- To investigate the spatial and temporal variability of Io's exosphere.
- To analyze the composition and distribution of ions produced from Io's volcanic outgassing.
- To understand the mass loading processes in Jupiter's plasma torus.
Main Methods:
- Analysis of ion cyclotron wave data from the Galileo orbiter during close flybys of Io.
- Comparison of wave spectra and ion signatures from different flyby trajectories and times.
- Mapping the spatial extent of ion pickup regions relative to Io and Jupiter's magnetosphere.
Main Results:
- Direct detection of sulfur dioxide ions (SO2+) and sulfur monoxide ions (SO+) via ion cyclotron waves.
- SO+ emissions were observed closer to Io than SO2+ emissions, indicating an inhomogeneous exosphere.
- A fan-shaped ion pickup region was identified extending in the anti-Jupiter direction.
- Differences in wave spectra between 1995 and 1999 flybys suggest temporal variability in Io's exosphere.
Conclusions:
- Io's exosphere is spatially inhomogeneous, with distinct regions for different ion species.
- The interaction between Io's volcanic activity and Jupiter's magnetosphere is a dynamic process.
- Temporal variations in Io's exosphere significantly influence plasma torus composition and dynamics.
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