Eruption of a helically twisted prominence

被引:0
|
作者
P. Romano
L. Contarino
F. Zuccarello
机构
[1] Città Universitaria,Dipartimento di Fisica e Astronomia
来源
Solar Physics | 2003年 / 214卷
关键词
Magnetic Field; Geometrical Parameter; Field Line; Flux Tube; Magnetic Field Line;
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学科分类号
摘要
In this paper we analyze the eruption of a prominence, characterized by a helical-like structure and by a non-linear rising motion. We approximated the prominence as a cylindrical curved flux tube and estimated the behaviour of several geometrical parameters during the activation and the eruption phases. We determined that, at the onset of the activation, the number N of turns of a magnetic field line over the whole length of the prominence was ∼5.0, while the value of the ratio P/r0 between the pitch of the magnetic field lines and the prominence width was ∼0.45. These values are in good agreement with those predicted by the kink-mode instability. Moreover, we found a decrease of the total twist of one helical thread from Φ∼10π to Φ∼2π during the prominence eruption, indicating a relaxation of the magnetic field towards a less twisted configuration. We conclude that the prominence was initially destabilized by the kink-mode instability and, not succeeding in finding a new equilibrium configuration, it erupted.
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页码:313 / 323
页数:10
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