Radioemission from planetary magnetospheres - Observations and physical processes

Details Radioemission from planetary magnetospheres - Observations and physical processes Radioemission from planetary magnetospheres - Observations and physical processes

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stia...7910747l&link_type=abstract

Deutsche Gesellschaft für Luft- und Raumfahrt, International Symposium on Exploration of the Planetary System, Munich, West Germ

Physics

Atmospheric Physics, Decametric Waves, Earth Magnetosphere, Jupiter Atmosphere, Radio Emission, Io, Jupiter Probes, Magnetohydrodynamic Stability, Periodic Variations, Polarization (Waves), Radio Bursts, Radio Spectra, Spaceborne Experiments

Scientific paper

Low-frequency Jovian radioemission (40-0.1 MHz) is characterized with attention to spectral distribution of activity, probability of occurrence, dynamic spectral properties, and polarization of emission. Topics considered in the review of physical processes include the coupling mechanism, the instability mechanism, and wave propagation in the Jovian plasmasphere. Spacecraft studies of the radioemission are surveyed.

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