| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8135595 | Icarus | 2016 | 27 Pages |
Abstract
Lyman and Werner H2 emission profiles, resulting from secondary electrons produced by precipitation of heavy ions in the 1-2Â MeV/u range, have been applied to our model. The low CR obtained from this emission suggests that heavy ions, presumably the main source of the X-ray aurora, do not significantly contribute to typical UV high latitude emission.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
J. Gustin, D. Grodent, L.C. Ray, B. Bonfond, E.J. Bunce, J.D. Nichols, N. Ozak,