Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88..455r&link_type=abstract
Journal of Geophysical Research, vol. 88, Jan. 1, 1983, p. 455-458. Research supported by Narrabri Enterprises, Inc.;
Astronomy and Astrophysics
Astronomy
13
Io, Jupiter (Planet), Radio Astronomy, Radio Emission, Decametric Waves, Planetary Magnetic Fields, Jupiter, Satellites, Io, Radio Emissions, Flux Tube, Decameter Waves, Theoretical Studies, Observations, Comparisons, Mapping, Longitudes, Pra, Planetary Radio Astronomy Experiment, Voyager, Features, Diagrams, Characteristics, Intensity, Models, Data
Scientific paper
The identification of a specific Jovian decametric emission with the particular flux tube near the orbit of Io giving rise to it would substantially improve theoretical understandings of the relation of the Io flux tubes with the arc-like structures seen on time vs. frequency plots of decametric emissions observed by the Voyager spacecraft. The present paper shows how the instantaneous Io flux tube may be identified with particular emission features. It is demonstrated that the emissions designated Io caused emission (ICE) may be interpreted as representing sections of arc structures emitted by the interaction of Io with successive flux tubes. The model is capable of accounting for the change of displacement angle of the ICE structures as the sub-observed Jovian longitude changes. The identification permits the mapping of emissions onto the causative flux tubes for Jovian longitudes from 240 to 360 deg.
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