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
β¦ LIBER β¦
Non-ideal MHD Properties of Magnetic Flux Tubes in the Solar Photosphere
β Scribed by Jens Kleimann; Gunnar Hornig
- Book ID
- 110289341
- Publisher
- Springer
- Year
- 2001
- Tongue
- English
- Weight
- 458 KB
- Volume
- 200
- Category
- Article
- ISSN
- 0038-0938
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## Abstract We present recent 3βD MHD numerical simulations of the nonβlinear dynamical evolution of magnetic flux tubes in an adiabatically stratified convection zone in spherical geometry, using the anelastic spherical harmonic (ASH) code.We seek to understand the mechanism of emergence of strong