Solar wind control of Jupiter's hectometric radio emission

Details Solar wind control of Jupiter's hectometric radio emission Solar wind control of Jupiter's hectometric radio emission

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...213..495b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 213, no. 1-2, April 1989, p. 495-501.

Astronomy and Astrophysics

Astrophysics

29

Planetary Radiation, Radio Emission, Solar Planetary Interactions, Solar Wind, Interplanetary Magnetic Fields, Io, Voyager 1 Spacecraft, Voyager 2 Spacecraft, Jupiter, Solar Wind, Radio Emissions, Hectometer Waves, Voyager Missions, Magnetic Fields, Density, Pressure, Comparisons, Frequencies, Energy, Pra Instrument, Spacecraft Observations

Scientific paper

Radio, plasma, and magnetic field data obtained by Voyager 1 and Voyager 2 were used to examine the manner in which the Jovian hectometric radio emission (HOM) is controlled by the solar wind. Using the method of superposed epochs, it was found that the higher energy HOM is correlated with the IMF as well as with the solar wind density and pressure. However, unlike the Io-independent decametric radio emission (Non-Io DAM), the HOM displayed no correlation with the solar wind velocity, although this radio component appear to be also influenced by the IMF. The results suggest separate HOM amd Non-Io DAM sources.

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