Physics
Scientific paper
Apr 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.338..267n&link_type=abstract
In ESA, Symposium on Titan p 267-272 (SEE N92-32348 23-91)
Physics
Magnetohydrodynamic Flow, Planetary Magnetospheres, Planetary Magnetotails, Plasma-Electromagnetic Interaction, Satellite Atmospheres, Titan, Cassini Mission, Plasma Dynamics, Plasmas (Physics), Voyager 1 Spacecraft
Scientific paper
Interaction between Titan and the surrounding magnetospheric plasma is considered, emphasizing the aspects of the global plasma dynamics of Titan's environment. The physical picture of the magnetospheric interaction is then developed from the theoretical point of view. Voyager 1 observations are presented to quantify the physical picture. An important aspect of Titan's induced magnetosphere, i.e., its tail with four lobes, is stressed and the Cassini Mission is briefly addressed.
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