Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19...83w&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 19, Jan. 24, 1992, p. 83-86. Research supported by Southwest Research Instit
Astronomy and Astrophysics
Astronomy
8
Auroral Ionization, Bremsstrahlung, Electron Energy, Jupiter Atmosphere, Ulysses Mission, X Ray Astronomy, Electron Precipitation, Hubble Space Telescope, Ultraviolet Emission
Scientific paper
Modeling results reported here show that precipitating auroral electrons with sufficient energy to be consistent with the Voyager UVS observations produce bremsstrahlung X-rays with sufficient energy and intensity to be detected by the Solar Flare X-ray and Cosmic-Ray-Burst Instrument on board the Ulysses spacecraft. The detection of such bremsstrahlung X-rays at Jupiter would provide strong evidence for the electron-precipitation mechanism, although it does not rule out the possibility of some heavy ion involvement, and thus makes a significant contribution toward solving the mystery of the Jovian aurora.
Alan Stern S.
Boice Daniel C.
Hurley Kevin Christopher
Sommer Matthias
Waite H. Jr. J..
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