The high degree of symmetry often assumed in studies of the structure and stability of coronal magnetic field configurations is restrictive and can yield misleading results. We have therefore developed fully three-dimensional numerical methods for constructing force-free equilibria and for examining
The Strength and Structure of the Coronal Magnetic Field
โ Scribed by Steven R. Spangler
- Publisher
- Springer Netherlands
- Year
- 2005
- Tongue
- English
- Weight
- 194 KB
- Volume
- 121
- Category
- Article
- ISSN
- 0038-6308
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