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Observational evidence for non-equilibrium ionization in the solar corona

โœ Scribed by D. Spadaro; P. Leto; S. K. Antiochos


Publisher
Springer Netherlands
Year
1994
Tongue
English
Weight
187 KB
Volume
70
Category
Article
ISSN
0038-6308

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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