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

机译:锚定在一端而另一端自由的通量绳的扭结不稳定性

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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(助焊绳)的扭折不稳定性是在实验室和天然等离子体中观察到的基本过程。先前的理论,实验和观察工作都集中在周期性(无限)绳索(与环形系统相关)的情况下,或在两端都绑到指定边界的有限绳索(与在光层绑扎的冠状绳索有关)上。但是,在太阳的日冕和天体系统中,存在大量的有限通量绳,它们的一端绑在一起,而另一端则自由。受最近在RSX装置上进行的实验(Furno等,2006)和最新的理论工作(Ryutov等,2006)的启发,本文通过仿真研究了自由端磁链的线性和非线性演化。该方法基于比较周期磁链的经典情况与一端绑紧而另一端自由的情况。在线性阶段,周期性绳索和自由绳索的行为截然不同。线性相的仿真分析证实了与自由绳不稳定性增加有关的实验和现象学发现:新的稳定性极限仅显示为定期绳经典极限的一半。在非线性阶段,重新连接被视为达到最终稳态的基本推动力。研究了通量绳的饱和机理,并将其与Rosenbluth等人的经典理论(所谓的气泡状态模型)进行了比较。 (1976)。对于经典的定期案例,发现了一个惊人的协议。自由绳索的情况也大不相同。观察到饱和状态呈现出向外螺旋形的配置,等离子体柱的位移从连接端到自由端逐渐单调增加。在自由端观察到最大位移,该最大位移与定期绳索中观察到的位移一致。关键区别在于,在定期绳索中,在整个绳索中都观察到相同的位移,从而形成半径恒定的螺旋线。

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