| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701595 | Icarus | 2013 | 18 Pages |
Abstract
⺠We assess the electron density in Titan's dayside ionosphere using a model driven by Cassini data. ⺠We obtain a factor of about 2 higher densities than observed by the Langmuir probe. ⺠We discuss possible reasons for the discrepancy found. ⺠Dissociative recombination is probably not the only important electron loss process.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
E. Vigren, M. Galand, R.V. Yelle, J. Cui, J.-E. Wahlund, K. Ã
gren, P.P. Lavvas, I.C.F. Mueller-Wodarg, D.F. Strobel, V. Vuitton, A. Bazin,