Correlation studies between solar wind parameters and the decimetric radio emission from Jupiter

Details Correlation studies between solar wind parameters and the decimetric radio emission from Jupiter Correlation studies between solar wind parameters and the decimetric radio emission from Jupiter

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94..121b&link_type=abstract

(Chapman Conference on Plasma Waves and Instabilities in Magnetospheres and at Comets, Sendai, Japan, Oct. 12-16, 1987) Journal

Physics

42

Jupiter Atmosphere, Planetary Radiation, Plasma Dynamics, Radio Emission, Solar Wind, Correlation Coefficients, Decametric Waves, Long Term Effects, Solar Planetary Interactions, Synchrotron Radiation, Twenty-Seven Day Variation, Jupiter, Solar Wind, Parameters, Decimeter Waves, Radio Waves, Emissions, Intensity, Radiation Belts, Pressure, Thermal Effects, Time Scale, Electrons, Magnetosphere, Earth-Based Observations, Microwave Methods, Solar Flux, Density

Scientific paper

Results of a study comparing long-term time variations in Jupiter's synchrotron radio emission with a variety of solar wind parameters and the 10.7 cm solar flux are reported. Data from 1963 through 1985 were analyzed, and the results suggest that many solar wind parameters are correlated with the intensity of the synchrotron emission produced by the relativistic electrons in the Jovian Van Allen radiation belts. Significant nonzero correlation coefficients appear to be associated with solar wind ion density, ram pressure, thermal pressure, flow velocity, momentum, and ion temperature. The implication of these results is that the solar wind is influencing the supply and/or loss of electrons to Jupiter's inner magnetosphere.

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