Solar wind control of Jupiter's decametric radio emission

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

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...165..244b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 165, no. 1-2, Sept. 1986, p. 244-250.

Astronomy and Astrophysics

Astrophysics

28

Decametric Waves, Jupiter Atmosphere, Planetary Radiation, Radio Emission, Solar Wind, Interplanetary Magnetic Fields, Planetary Magnetospheres, Voyager Project

Scientific paper

Observations of the solar wind close to Jupiter are compared with the decametric radio emission (DAM), using data recorded by Voyager 1 and Voyager 2 during 1979. The Non-Io DAM, recorded by both spacecraft and combined using the superposed epoch technique, is found to correlate with the solar wind density and velocity, as well as with the interplanetary magnetic field (IMF) magnitude. In agreement with earlier work using ground-based observations, there are indications that the Non-Io DAM is somehow associated with magnetic sector structure although the precise details of the relationship are still not known and it is not clear if this is a fundamental effect or some secondary effect of intercorrelation.

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