Physics
Scientific paper
Aug 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004georl..3115703k&link_type=abstract
Geophysical Research Letters, Volume 31, Issue 15, CiteID L15703
Physics
28
Magnetospheric Physics: Magnetosphere Interactions With Satellites And Rings, Magnetospheric Physics: Planetary Magnetospheres (5443, 5737, 6030), Magnetospheric Physics: Numerical Modeling, Ionosphere: Ionosphere/Magnetosphere Interactions (2736)
Scientific paper
The Titan-Saturn plasma interaction is studied using a global numerical kinetic model. The developed self-consistent three-dimensional quasi-neutral hybrid model is used to study Titan's interaction with supersonic and subsonic plasma flow. The subsonic flow case represents Titan in the Kronian magnetosphere during the Voyager-1 flyby. The supersonic and weakly supermagnetosonic flow cases are used to study a disturbed magnetospheric plasma flow event. In both cases the magnetic field is found to pile up against Titan and forming a magnetotail on the wake side. The subsonic flow case does not produce a bow shock in front of Titan, in contrast to the supersonic case. The magnetic field is found to have a Saturn facing side-anti Saturn facing side asymmetry in both cases. The subsonic case resulted in a twisting of the magnetotail toward Saturn that is qualitatively in agreement with the magnetic field observations made by Voyager 1.
Janhunen Pekka
Kallio Esa
Sillanpää I.
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