Incorporating Magnetogram Data into Time-Dependent Coronal Field Models
Abstract
We briefly review our efforts to incorporate sequences of photospheric vector magnetograms into MHD simulations of coronal evolution, in an effort to create data-driven models of the coronal magnetic field. Such models should improve our understanding of flares and coronal mass ejections (CMEs), and might eventually lead to predictive capabilities.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2009
- Bibcode:
- 2009AGUFMSM51A1340F
- Keywords:
-
- 7513 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY / Coronal mass ejections;
- 7519 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY / Flares;
- 7524 SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY / Magnetic fields