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
β¦ LIBER β¦
The loop prominence of 1984 February 18 and its velocity field
β Scribed by Xiao-ma Gu; Qiu-sha Li
- Publisher
- Elsevier Science
- Year
- 1988
- Tongue
- English
- Weight
- 573 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0275-1062
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