Observations of molecular oxygen ions in Saturn's inner magnetosphere

Hilary R. Martens, Daniel B. Reisenfeld, John D. Williams, Robert E. Johnson, H. Todd Smith

Research output: Contribution to journalArticlepeer-review

Abstract

We present an analysis of molecular oxygen ion (O2+) abundance in Saturn's inner magnetosphere based on observations made with the Cassini Plasma Spectrometer (CAPS). Using data summed over 23 orbits, we resolve and isolate O2+counts from the tail of the water group ion mass distribution (W+ [O+, OH+, H2O+, H3O+]) and from background sources. O2+ was initially estimated at ∼ 1-2% of the total ion population in the inner magnetosphere based on CAPS data from the Saturn orbital insertion pass. Through refined analysis techniques, we have found O2+ to account for just above 0.3% of all W+ ions at L = 4.5, with only minor fluctuations in relative density out to L = 7.5 - 8.0. Beyond L = 7.5, the relative O2+/ W+ abundance exhibits a statistically significant increase through L = 10.5, which may indicate a neutral O2 source in the vicinity of Rhea.

Original languageEnglish
Article numberL20103
JournalGeophysical Research Letters
Volume35
Issue number20
DOIs
StatePublished - Oct 28 2008

Fingerprint

Dive into the research topics of 'Observations of molecular oxygen ions in Saturn's inner magnetosphere'. Together they form a unique fingerprint.

Cite this