Cassini discovered a plethora of neutral and ionised molecules in Titan’s ionosphere including, surprisingly, anions and negatively charged molecules extending up to 13,800 u/q. In this letter we forward model the Cassini electron spectrometer response function to this unexpected ionospheric component to achieve an increased mass resolving capability for negatively charged species observed at Titan altitudes of 950-1300 km.
We report on detections consistently centered between 25.8-26.0 u/q and between 49.0-50.1 u/q which are identified as belonging to the carbon chain anions, CN−/C3N− and/or C2H−/C4H−, in agreement with chemical model predictions. At higher ionospheric altitudes, detections at 73-74 u/q could be attributed to the further carbon chain anions C5N−/C6H− but at lower altitudes and during further encounters, extend over a higher mass/charge range. This, as well as further intermediary anions detected at >100 u, provide the first evidence for efficient anion chemistry in space involving structures other than linear chains.
Furthermore, at altitudes below ∼1100 km, the low mass anions (
R. T. Desai, A. J. Coates, A. Wellbrock, V. Vuitton, F. J. Crary, D. González-Caniulef, O. Shebanits, G. H. Jones, G. R. Lewis, J. H. Waite, S. A. Taylor, D. O. Kataria, J. -E. Wahlund, N. J. T. Edberg, E. C. Sittler
(Submitted on 6 Jun 2017)
Comments: 8 pages, 3 figures, 1 table, Astrophysical Journal Letter accepted June 01 2017
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:1706.01610 [astro-ph.EP] (or arXiv:1706.01610v1 [astro-ph.EP] for this version)
From: Ravindra Desai Mr
[v1] Tue, 6 Jun 2017 05:58:55 GMT (2804kb,D)
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