Magnetic field configuration of a 1N/M1.1 flare in AR 7321.
Abstract
The paper presents the comparison between the magnetic connectivity of patterns, or magnetic loops, and the multi-waveband observations of AR NOAA 7321 on October 27, 1992 in order to recover a comprehensive configuration from the photosphere up to the corona. The authors obtain that a 1N/M1.1 flare may be triggered by the interaction between two sheared loops.
- Publication:
-
JOSO Annu. Rep., 1997
- Pub Date:
- 1998
- Bibcode:
- 1998joso.proc..134W
- Keywords:
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- Solar Active Regions: Solar Magnetic Fields;
- Solar Active Regions: Solar Flares