Physics – Plasma Physics
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...289..392b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 289, Feb. 1, 1985, p. 392-408.
Physics
Plasma Physics
24
Io, Plasma Heating, Plasma Waves, Plasma-Particle Interactions, Toroidal Plasmas, Electric Fields, Electrical Measurement, Heat Transfer, Jupiter Satellites, Planetology, Plasma Physics, Voyager 1 Spacecraft, Jupiter, Satellites, Io, Voyager Missions, Observations, Plasma Torus, Heating, Electric Fields, Plasma Wave Instrument, Analysis, Spectra, Noise, Sulfur, Oxygen, Waves, Intensity, Doppler Observations, Ions, Theoretical Studies, Distribution, Models, Density, Electrons
Scientific paper
A study of Voyager 1 electric field measurements obtained by the plasma wave instrument in the Io plasma torus has been carried out. A survey of the data has revealed the presence of persistent peaks in electric field spectra in the frequency range 100-600 Hz consistent with their identification as lower hybrid noise for a heavy-ion plasma of sulfur and oxygen. Typical wave intensities are 0.1 mV/m, and the spectra also show significant Doppler broadening, Delta omega/omega approximately 1. A theoretical analysis of lower hybrid wave generation by a bump-on-tail ring distribution of ions is given. The model is appropriate for plasmas with a superthermal pickup ion population present. A general methodology is used to demonstrate that the maximum plasma heating rate possible through anomalous wave-particle heat exchange is less than approximately 10 to the -14th ergs per cu cm per s. Although insufficient to meet the power requirement of the EUV-emitting warm torus, the heating rate is large enough to maintain a low-density (0.01-0.1 percent) superthermal electron population of keV electrons, which may lead to a small but significant anomalous ionization effect.
Barbosa Domingos
Coroniti Ferdinan V.
Kurth Willaim S.
Scarf Frederick L.
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