Solar Prominence Eruptions and CMEs at the Start of Cycle 24
Abstract
We present the analysis of prominence eruptions and CMEs during the rising phase of cycle 24. We combine data from the two STEREO and SDO spacecraft (that are near quadrature) to observe simultaneously the region where a CME originates and the CME moving outward in the plane-of-the-sky. This allows us to compute trajectories for the CME and the associated eruptive prominence and, at the same time, to study the on-disk CME manifestations such as flares, dimming regions, and coronal waves with high spatial and temporal resolution.
- Publication:
-
Solar Heliospheric and INterplanetary Environment (SHINE 2011)
- Pub Date:
- July 2011
- Bibcode:
- 2011shin.confE.147D