Formation of the May 1981 Solar Flare Complex and the Global Magnetic Field of the Sun (H. R. 17 644)
Abstract
The degree to which the development of the May 1981 flare complex is related to the global changes of the solar background magnetic fields is studied. It is connected with the action of magnetic active longitudes, it lasts about 10 rotations, and in its last phase it forms a coronal hole. Its fields play a role in forming two sectors in the equatorial background fields and are involved in the fast global field redistribution into regular morphological patterns. All regularities found require physical interpretation.
- Publication:
-
Bulletin of the Astronomical Institutes of Czechoslovakia
- Pub Date:
- July 1986
- Bibcode:
- 1986BAICz..37..210B
- Keywords:
-
- Magnetic Effects;
- Solar Flares;
- Solar Magnetic Field;
- Astronomical Maps;
- Coronal Holes;
- H Alpha Line;
- Solar Longitude;
- Solar Physics