Z mode radiation in Jupiter's magnetosphere

Details Z mode radiation in Jupiter's magnetosphere Z mode radiation in Jupiter's magnetosphere

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....92.9978k&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 92, Sept. 1, 1987, p. 9978-9996.

Physics

11

Jupiter Atmosphere, Planetary Magnetospheres, Planetary Radiation, Plasma Waves, Voyager Project, Cyclotron Frequency, Magnetic Dipoles, Narrowband, Plasma Frequencies, Spatial Distribution, Jupiter, Radiation, Magnetosphere, Plasma Waves, Spacecraft Observations, Voyager 1 Mission, Voyager 2 Mission, Emissions, Intensity, Frequencies, Electromagnetism, Hypotheses, Plasma, Pws Instrument, Energy, Density, Calculations, Diagrams, Spectra, Distribution, Source, Plasma Sheets

Scientific paper

Results of a survey of the Voyager plasma wave instrument wide-band frames that exhibit a narrow-band emission below the low-frequency cutoff of the continuum band are discussed. The analysis of these waves made it possible to identify them as the slow branch of the X mode, the so-called Z mode. As the Voyager 1 spacecraft approached the plasma sheet on March 8, 1979, the Z mode intensified and then disappeared on plasma sheet entry. This observation is interpreted as evidence of local Z mode generation.

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