Spatial variations of low mass negative ions in Titan's upper atmosphere
Teodora Mihailescu, Ravindra Desai, Oleg Shebanits, Richard, Haythornthwaite, Anne Wellbrock, Andrew Coates, Jonathan Eastwood, J. Hunter, Waite

TL;DR
This study maps the spatial distribution of low mass negative ions in Titan's upper atmosphere, revealing day-night variations and linking ion densities to electron populations and photochemical processes.
Contribution
It provides the first detailed analysis of the spatial variation of specific low mass negative ions in Titan's ionosphere and their relation to electron densities and photochemistry.
Findings
Lower ion densities on the night side.
Ion densities proportional to electron densities on the day side.
Stable ratio of certain ions on the day side with variability at night.
Abstract
Observations with Cassini's Electron Spectrometer discovered negative ions in Titan's ionosphere, at altitudes between 1400 and 950 km. Within the broad mass distribution extending up to several thousand amu, two distinct peaks were identified at 25.8-26.0 and 49.0-50.1 amu/q, corresponding to the carbon chain anions and/or for the first peak and and/or for the second peak. In this study we present the spatial distribution of these low mass negative ions from 28 Titan flybys with favourable observations between 26 October 2004 and 22 May 2012. We report a trend of lower densities on the night side and increased densities up to twice as high on the day side at small solar zenith angles. To further understand this trend, we compare the negative ion densities to the total electron density measured by Cassini's Langmuir Probe. We find the low mass negative…
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