Modelling of Cassini charging and wake formation in Saturn's Magnetosphere

Details Modelling of Cassini charging and wake formation in Saturn's Magnetosphere Modelling of Cassini charging and wake formation in Saturn's Magnetosphere

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..871y&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.871

Physics

Scientific paper

A self-consistent three-dimensional particle-in-cell code has been employed to explore modifications of the spacecraft (SC) potential and the resultant wake structure in a wide range of distances from the planet (for the dipole shell in the range L~ 4 -10). The plasma parameters derived from the Cassini plasma spectrometer (CAPS) measurements during the Saturn orbit insertion (SOI) period on June 30, 2004 [1], and CAPS data obtained in the inner equatorial magnetosphere in 2005 on Oct. 11 and 29, Nov. 27 and Dec. 24 [2] have been used as input data.

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