An extended plasma model for Saturn

Details An extended plasma model for Saturn An extended plasma model for Saturn

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995georl..22.1177r&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 22, no. 10, p. 1177-1180

Physics

Plasma Physics

43

Planetary Magnetic Fields, Planetary Magnetospheres, Plasma Dynamics, Plasma Physics, Saturn (Planet), Static Models, Data Correlation, Electron Density (Concentration), Ion Density (Concentration), Magnetopause, Voyager Project, Wave-Particle Interactions

Scientific paper

The Saturn magnetosphere model of Richardson and Sittler (1990) is extended to include the outer magnetosphere. The inner magnetospheric portion of this model is updated based on a recent reanalysis of the plasma data near the Voyager 2 ring plane crossing. The result is an axially symmetric model of the plasma parameters which is designed to provide accurate input for models needing either in situ or line-of-sight data and to be a useful tool for Cassini planning.

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