The magnetic non-equilibrium of buoyant
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P. K. Browning; E. R. Priest
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Article
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1984
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Springer
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English
โ 678 KB
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