Some Characteristics of Large Solar Flares- Towards Solar Flare Forecasting
Abstract
Solar flares are the result of strong magnetic field lines reconfiguring and undergoing magnetic reconnection. This reconfiguration releases >10^{20}
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2019
- Bibcode:
- 2019AGUFMSH31D3329A
- Keywords:
-
- 7519 Flares;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7524 Magnetic fields;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7924 Forecasting;
- SPACE WEATHER;
- 7959 Models;
- SPACE WEATHER