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- W136656166 abstract "We review the main characteristics and the inferred properties of the hectometric (HOM) radiation which was observed by IMP-6, RAE-1 and Voyager spacecraft. This includes the occurrence of HOM in Jovian longitude, the strong beaming in latitude, the polarization properties, the local time effect, and the solar wind control of the emission. Like many radio emissions observed at the other magnetized planets, the hectometric component is likely to be generated in the R-X mode from sources in the northern and southern auroral zones. The emission is beamed along the surface of hollow cones and is possibly produced by the cyclotron maser mechanism. The HOM sources extend up to 7 R J (Jovian radii) along field lines near L=20 in the auroral zone ; they are distinct from the Io-controlled decametric (DAM) sources but are probably the extension of the non-Io DAM sources. Finally, we discuss certain questions of still unresolved problems that could be answered when Ulysses passes around Jupiter" @default.
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- W136656166 date "1991-12-01" @default.
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- W136656166 title "The Jovian hectometric radiation : an overview after the Voyager mission" @default.
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