Physics
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jgr....87.1395g&link_type=abstract
Journal of Geophysical Research, vol. 87, Mar. 1, 1982, p. 1395-1403. Navy-supported research;
Physics
44
Electron Density (Concentration), Plasma Waves, Titan, Wakes, Field Strength, Low Frequencies, Neutral Sheets, Plasma Temperature, Voyager 1 Spacecraft, Saturn, Satellites, Titan, Plasmas, Waves, Plasma Wave Instrument, Emissions, Electric Fields, Turbulence, Characteristics, Magnetosheath, Ionosphere, Comparisons, Ions, Corotation, Magnetotail, Resonance, Electrons, Density, Magnetic Fields, Magnetosphere, Interactions, Rotation, Pressure, Temperatures, Origin, Source, Plumes, Data, Intensity, Frequencies,
Scientific paper
The electron density profile inferred from plasma wave emissions detected during the Voyager 1 flyby of Titan exhibits three distinct peaks with densities of about 40/cu cm, the first peak corresponding to the entry into the magnetic tail, the second corresponding to the neutral sheet crossing from the northern to the southern tail lobe, and the third corresponding to the outbound exit from the tail. Large depressions in the magnetic field strength are observed coincident with each of the density peaks, indicating that a dense plume of plasma is being carried downstream of Titan by the interaction with the rapidly rotating magnetosphere of Saturn. The 8600 K plasma temperature estimated suggests that the plasma originates from the ionosphere of Titan, probably forming a plasma plume with a theta or H cross section extending downstream from Titan.
Gurnett Donald A.
Kurth Willaim S.
Scarf Frederick L.
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