| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1777024 | Journal of Atmospheric and Solar-Terrestrial Physics | 2011 | 9 Pages |
Abstract
⺠The rolling motion of the erupting filament is away from a neighboring coronal hole. ⺠The non-radial motion of the associated CME is away from a neighboring coronal hole. ⺠The erupting filaments were all more non-radial than the CMEs but in the same general direction. ⺠The rolling motion depends on the level of force imbalances inside the filament arcade. ⺠The non-radial motion of the CME is related to global magnetic configuration force imbalances.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Olga Panasenco, Sara Martin, Anand D. Joshi, Nandita Srivastava,