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    Direct evidence for solar wind control of Jupiter's hectometer-wavelength radio emission (1984)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: Observations of the solar wind close to Jupiter, by the Voyager 1 and Voyager 2 spacecraft in 1978 and 1979, are compared with the hectometer wavelength radio emission from the planet. A significant positive correlation is found between variations in the solar wind plasma density at Jupiter and the level of Jovian radio emission output. During the 173-day interval studied for the Voyager 2 data, the radio emission displayed a long term periodicity of about 13 days, identical to that shown by the solar wind density at Jupiter and consistent with the magnetic sector structure association already proposed for groundbased observations of the decameter wavelength emission.
    Keywords: LUNAR AND PLANETARY EXPLORATION
    Type: NASA-TM-86073 , NAS 1.15:86073
    Format: application/pdf
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