Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9821145l&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A12, p. 21,145-21,149
Astronomy and Astrophysics
Astronomy
8
Abundance, Hydrogen, Jupiter (Planet), Jupiter Atmosphere, Molecular Ions, Planetary Ionospheres, Planetary Magnetospheres, Power Spectra, Spaceborne Astronomy, Astronomical Spectroscopy, Atmospheric Composition, Energetic Particles, Helium Isotopes, Space Plasmas, Ulysses Mission
Scientific paper
The Voyager 2 measurements of energetic (approximately 1 MeV/nucleon) H3 molecules in Jupiter's magnetosphere provided strong evidence that the planet's ionosphere is an important plasma source in the Jovian environment (Hamilton et al., 1980). During the Ulysses spacecraft encounter with Jupiter in February 1992 the Heliosphere Instrument for Spectra, Composition, and Anisotropy at Low Energies (HI-SCALE) on this satellite also detected significant fluxes of energetic H3 molecules. These molecules were measured throughout the dayside inbound pass (near the plasma sheet) as well as during the outbound pass at high Jovian latitudes on the duskside. The spectral shapes of the energetic He-4 and the H3 are found to be similar over the range approximately 0.6 - 1.6 MeV/nucleon, with a power law spectral slope of n approximately 3. The abundance ratio R (H3/He-4) is found to be approximately 0.1 over this energy range for the inbound pass and to vary from approximately 0.2 at approximately 0.6 MeV/nucleon to approximately 0.1 at approximately 1.6 MeV/nucleon at dusk side high latitudes. These observations, especially those from high latitudes, confirm that the energetic molecules must be accelerated out of the Jovian topside ionosphere into the magnetosphere.
Feldman D. M.
Lanzerotti Louis J.
Maclennan Carol G.
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