| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701423 | Icarus | 2012 | 19 Pages |
Abstract
⺠We perform a wavelet analysis on 31 Cassini electron density profiles. ⺠Virtually all profiles at all latitudes show variability at 250-450 km scale. ⺠Overall the most often observed vertical scale is 300 km. ⺠The observed variability is consistent with forcing by atmospheric gravity waves.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Katia I. Matcheva, Daniel J. Barrow,