Computer Science – Sound
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.263...11f&link_type=abstract
In ESA Proceedings of an International Symposium on New Insights in Astrophysics. Eight Years of UV Astronomy with IUE p 11-16
Computer Science
Sound
Astronomical Spectroscopy, Io, Iue, Jupiter Atmosphere, Planetary Magnetospheres, Toruses, Atmospheric Sounding, Auroras, Emission Spectra, Magnetospheric Electron Density, Temperature Distribution, Ultraviolet Astronomy, Voyager 1977 Mission
Scientific paper
The IUE has been used since 1979 to remotely monitor the physical conditions in the Jovian magnetospheric system using the in situ Voyager measurements as a basis for comparison. Both the Io plasma torus, observable in emission of S+, S++ and S+3, and the Jovian H2 polar aurorae are accessible to the IUE short wavelength spectrograph. Despite significant short-term variations sometimes observed, the electron density and temperature structure of the torus has not changed appreciably in the seven years since the Voyager encounters. Similarly, the total radiated power from the polar aurorae has remained relatively constant during this period.
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