Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jgr....86.8564l&link_type=abstract
Journal of Geophysical Research, vol. 86, Sept. 30, 1981, p. 8564-8568. Research supported by the Centre National d'Etudes Spat
Astronomy and Astrophysics
Astronomy
31
Decametric Waves, Jupiter (Planet), Planetary Radiation, Radio Sources (Astronomy), Arcs, Bursts, High Resolution, Io, Time Response, Jupiter, S Bursts, Source Medium, Observations, Emissions, Patterns, Planetary Radio Astronomy Experiment, Arcs, Satellites, Models, Pra, Data, Io
Scientific paper
By using the high resolution observations of the Nancay observatory, the S burst emission on the planetary radio astronomy records of Voyager have been identified. It is shown that the S bursts occur in two regions of the Phi(Io)-CML plane (S-IoB and S-IoA-prime C regions). In these regions, the S burst emission is arranged into a pattern of repetitive features, drifting negatively. These features could be incomplete vertex late arcs. It is shown that the S burst pattern is distinct from the pattern of the Io-controlled emission. These results are discussed in the frame of Goldstein and Thieman's arc model (1980).
Genova Francoise
Leblanc Yolanda
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