Physics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981m%26p....24...45w&link_type=abstract
Moon and the Planets, vol. 24, Feb. 1981, p. 45-52.
Physics
2
Ionospheric Ion Density, Planetary Atmospheres, Planetary Ionospheres, Europa, Jupiter (Planet), Lunar Atmosphere, Mercury (Planet), Solar Radiation, Space Exploration
Scientific paper
It is noted that negative ions may be formed in the ionospheres of Mercury, the moon, and Jupiter's satellites with densities of a few percent of the ionospheric electron density. Negative ions result from three mechanisms at the planetary surface: charge inversion during energetic proton scattering, with simultaneous secondary negative ion emission, and micrometeorite impacts. The density and distribution of negative ions around planetary bodies depends primarily on the negative ion lifetimes determined through photodetachment by solar radiation.
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