TALK ABSTRACT:
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The Cassini spacecraft with Huygens Probe went into orbit around
Saturn on July 1, 2004. The Huygens Probe entered Titan's atmosphere
and safely landed on its surface on January 12, 2005. On the Cassini
orbiter there is a plasma instrument called Cassini Plasma Spectrometer
(CAPS). This instrument is composed of an Ion Mass Spectrometer (IMS),
Electron Spectrometer (ELS) and Ion Beam Spectrometer (IBS). The IMS and
IBS cover the energy range from 1 V < E/Q < 50 kV, and the ELS covers the
energy range from 1 eV < E < 30 keV. The IMS, using time-of-flight (TOF)
technology is able to separate ions in M/Q with the ability to distinguish
between some ion species of the same M/Q. For this talk I will primarily
be presenting results from the CAPS instrument. I will focus the talk on
Saturn Orbit Insertion (SOI) data for the inner magnetosphere of Saturn,
the numerous flybys with Saturn's moon Titan, and the most recent flyby
with its icy moon Enceladus.