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Kink instability of flux ropes anchored at one end and free at the other

机译:扭结通量绳一端固定不稳定和自由

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The kink instability of a magnetized plasma column (flux rope) is a fundamental process observed in laboratory and in natural plasmas. Previous theoretical, experimental, and observational work has focused either on the case of periodic (infinite) ropes (relevant to toroidal systems) or on finite ropes with both ends tied to a specified boundary (relevant to coronal ropes tied at the photosphere). However, in the Sun's corona and in astrophysical systems there is an abundant presence of finite flux ropes tied at one end but free at the other. Motivated by recent experiments conducted on the RSX device (Furno et al., 2006) and by recent theoretical work (Ryutov et al., 2006), the present paper investigates by simulation the linear and nonlinear evolution of free-ended flux ropes. The approach is based on comparing the classic case of a periodic flux rope with the case of a rope tied at one end and free at the other. In the linear phase, periodic and free ropes behave radically differently. A simulation analysis of the linear phase confirms the experimental and phenomenological findings relative to an increased instability of a free rope: the new stability limit is shown to be just half of the classic limit for periodic ropes. In the nonlinear phase, reconnection is observed to be a fundamental enabler to reach the eventual steady state. The mechanism for saturation of a flux rope is investigated and compared with the classic theory (the so-called bubble state model) by Rosenbluth et al. (1976). A remarkable agreement is found for the classic periodic case. The case of a free rope is again very different. The saturated state is observed to present a outwardly spiraling configuration with the displacement of the plasma column increasing progressively and monotonically from the tied end to the free end. The maximum displacement is observed at the free end where it is consistent with the displacement observed in a periodic rope. The key distinction is that in a periodic rope the same displacement is observed throughout the whole rope to form a helix with constant radius.
机译:磁化等离子体柱的扭结不稳定(通量绳)是一个基本的过程中观察到实验室和自然的等离子体。理论、实验和观测工作都集中在周期性的情况吗(无限)绳索(环形相关系统)或在有限的绳索绑在两端指定的边界(相关冠状绳索在光球层)。有一个日冕和天体物理系统丰富的通量绳绑在有限的存在但一端自由。最近的实验RSX设备上进行(Furno et al ., 2006)和最近的理论工作(Ryutov et al ., 2006),摘要通过模拟线性和调查非线性演化的自由端通量绳。方法是基于比较的经典案例一个周期的通量绳一根绳子的情况下系和自由在另一端。线性相位、周期和自由绳索的行为从根本上是不同的。证实了实验和线性阶段相对于一个现象学的研究结果不稳定性的增加一个免费的绳子:新只是显示了稳定极限的一半经典限制定期绳索。非线性阶段,重新连接被观察到基本推动者达到最终稳定状态。绳子是调查和比较经典理论(所谓的泡沫状态模型)Rosenbluth et al。(1976)。协议是发现对于经典的周期情况。免费的绳子的情况下再次非常不同。饱和状态的观察提出表面上螺旋配置的等离子体柱的位移增加逐步和单调的自由端。观察到自由端是一致的位移观测的一个周期绳子。绳子也遵循同样的位移整个绳,形成一个螺旋与常数半径。

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