Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsm11a..06h&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SM11A-06
Physics
5737 Magnetospheres (2756), 6275 Saturn
Scientific paper
The Charge-Energy-Mass Spectrometer (CHEMS), one of three sensors comprising the MIMI investigation on Cassini, measures the mass and charge state of ions in the energy per charge range 3--220 keV/e. The suprathermal ion composition determined by CHEMS has been generally consistent during the first four passes through Saturn's magnetosphere. The observed heavy ions are largely water products (O+, OH+, H2O+, and O2+) with a near absence of N+ ions. Nonetheless, both spatial and temporal variations have been observed in the heavy ion composition and in the ratio of heavy to light ions (H+, H2+, He+, and He++). We will discuss those variations and their causes and compare the average composition at Saturn with CHEMS' measurements during the flybys of Earth and Jupiter.
Armstrong Tom
Dandouras Jannis
Hamilton Dave
Hill Michael
Krimigis Stamatios
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