The equilibrium and non-equilibrium properties of a coronal loop embedded in a stratified isothermal atmosphere are investigated. The shape of the loop is determined by a balance between magnetic tension, buoyancy, and external pressure gradients. The footpoints of the loop are anchored in the photo
โฆ LIBER โฆ
The Effect of Twisted Magnetic Field on the Resonant Absorption of MHD Waves in Coronal Loops
โ Scribed by K. Karami; K. Bahari
- Publisher
- Springer
- Year
- 2010
- Tongue
- English
- Weight
- 775 KB
- Volume
- 263
- Category
- Article
- ISSN
- 0038-0938
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