Analysis of chorus emissions at Jupiter

Details Analysis of chorus emissions at Jupiter Analysis of chorus emissions at Jupiter

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.3801c&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, June 1, 1984, p. 3801-3820.

Physics

19

Dawn Chorus, Jupiter Atmosphere, Planetary Radiation, Broadband, Planetary Magnetospheres, Plasma Waves, Spatial Distribution, Voyager 1 Spacecraft, Whistlers, Jupiter, Emissions, Analysis, Voyager 1, Magnetosphere, Waves, Bands, Plasma Wave Instrument, Frequencies, Satellites, Io, Plasma Torus, Density, Power, Spectra, Bursts, Whistlers, Electrostatic Properties, Resonance, Distribution, Anisotropy, Electromagnetic Properties, Hypotheses, Absorption, Electrons

Scientific paper

The emissions in the chorus frequency band which were detected on the Voyager 1 inbound pass between about ten and six Jupiter radii are surveyed. An overview of the plasma and wave observations during the inbound pass is presented and the spatial regions in which chorus band signals were observed are discussed. A series of wide-band frequency-time frames which characterize the onset of two observed intervals of chorus band activity is displayed. A detailed examination is made of the spectra for rising chorus which sweeps upward in frequency from 0.2 to 0.5 times the electron cyclotron frequency f(c). Two temporally successive wide-band frames in which several types of chorus band emissions were observed are discussed. The spatial morphology of chorus is discussed in terms of the electron energies which resonate with whistler mode waves. A recent theory of chorus generation is reviewed along with theories and a model explaining the narrow-band emissions above f(c)/2.

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