The equilibrium shape of a slender flux tube in the stratified solar atmosphere is studied. The path is determined by a balance between the downwards magnetic tension, which depends on the curvature of the loop, and the upwards buoyancy force. Previous results for untwisted slender tubes are extende
Non-equilibrium of Magnetic Flux Tubes emerging into the Solar Corona
โ Scribed by V. D. Kuznetsov; A. W. Hood
- Book ID
- 110217185
- Publisher
- Springer
- Year
- 1997
- Tongue
- English
- Weight
- 170 KB
- Volume
- 171
- Category
- Article
- ISSN
- 0038-0938
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