| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5487142 | Icarus | 2017 | 20 Pages |
Abstract
Our study reveals that a fraction of the aurora is due to very low energy electrons (<1Â keV). Even in this case, comparisons between observed and modeled spectra show that 100Â eV is a suitable value to represent the average energy of the secondary electrons.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
J. Gustin, D. Grodent, A. Radioti, W. Pryor, L. Lamy, J. Ajello,