Detection of the hydroxyl radical in the Saturn magnetosphere

Details Detection of the hydroxyl radical in the Saturn magnetosphere Detection of the hydroxyl radical in the Saturn magnetosphere

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993natur.363..329s&link_type=abstract

Nature (ISSN 0028-0836), vol. 363, no. 6427, p. 329-331.

Computer Science

89

Atmospheric Composition, Hydroxyl Radicals, Planetary Magnetospheres, Saturn Atmosphere, Neutral Gases, Plasma Density, Saturn, Magnetosphere, Hydroxyl Radical, Oh Radical, Plasma, Electrons, Temperature, Cooling, Satellites, Tethys, Origin, Source, Comparison, Positon (Location), Satellite Observations, Hst Satellite, Abundance, Fos Instrument, Neutral Particles, Bombardment, Micrometeorites, Density, Hypotheses, Spectroscopy, Quenching, Gases

Scientific paper

The detection of neutral OH molecules near the orbit of Tethys is reported. The findings suggest that neutral OH is one of the dominant species in Saturn's inner magnetosphere, implying a source rate for H2O 20 times greater than current theoretical estimates. One possible explanation is that the micrometeorite erosion rates of the inner satellites are significantly higher than expected.

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