The dependence of Jupiter's decametric emissions on the Jovian magnetic latitude of Io |
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| Authors: | H.R. Miller A.G. Smith |
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| Affiliation: | Department of Physics, Georgia State University, Atlanta, Georgia 30303, USA;Department of Physics and Astronomy, University of Florida, Gainesville, Florida 32602, USA |
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| Abstract: | ![]()
The present analysis confirms the contention that the majority of Jupiter's decametric radio emissions occur when Io is above the northern magnetic hemisphere of Jupiter. However, a substantial portion of the non-Io-related component of source A was found to occur when Io was above southern magnetic latitudes of Jupiter. |
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