Forbush decrease caused by interacting and non-interacting passing CME
Abstract
On 5-6 Aug. 2011 two short-time consecutive M-class solar flares led to profile of multiple Forbush Decreases showing the possible interaction of long-time passing of ICME.
- Publication:
-
Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles
- Pub Date:
- February 2018
- DOI:
- 10.1017/S1743921318001552
- Bibcode:
- 2018IAUS..340..151I
- Keywords:
-
- cosmic rays;
- flares;
- coronal mass ejections (CMEs);
- Solar-stellar connection