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Numerical simulation of the initial expansion process of cathode spots in high-current triggered vacuum arc

机译:大电流触发真空电弧中阴极斑点初始膨胀过程的数值模拟

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Summary form only given. The cathode spot (CS), as an intense source of inter-electrode arc plasma, plays a predominant role in maintaining the burning of vacuum arc, especially with an inactive anode. Consequently, the dynamics of CSs have a significant influence on the characteristics of the vacuum arc. Many experimental investigations have been devoted to better understanding of the motion of CSs, especially the initial expansion process of cathodes spots in high-current triggered vacuum arc. It has been indicated that the motion characteristic of cathode spots is greatly influenced by external axial magnetic field (AMF). In this work, a method is established to simulate the initial expansion process of CSs in high-current triggered vacuum arc, based on the proposed stepwise model of the motion of a single CS1. In this method, every new CS can be ignited in any direction around the old one with certain probability, which is connected with the magnetic field around the position of the old CS. With this approach, the initial expansion processes of CSs in free-burning and AMF-stabilized high-current triggered vacuum arc are simulated numerically with CSs initially uniformly distributed on a ring. The self-generated transverse magnetic field at the position of every CS is calculated by commercial software ANSYS with the current distribution in contact plate taken into account2. Simulation results agree well with relevant experiment results. Simulation results show that CSs expand faster without external AMF than that under AMF, and external AMF has significant influence on the distribution of CSs on the cathode surface, e.g., more and more CSs appear inside the ring when external AMF is present. Furthermore, the results also indicate that the expanding ring structure of CSs is unstable, and AMF can accelerate the breaking of the ring.
机译:仅提供摘要表格。阴极点(CS)作为电极间电弧等离子体的强烈来源,在维持真空电弧的燃烧方面起着主要作用,尤其是在阳极不活动的情况下。因此,CS的动力学对真空电弧的特性有重大影响。许多实验研究致力于更好地了解CS的运动,尤其是大电流触发真空电弧中阴极斑点的初始膨胀过程。已经表明,阴极斑点的运动特性在很大程度上受到外部轴向磁场(AMF)的影响。在这项工作中,基于提出的单个CS1运动的逐步模型,建立了一种方法来模拟大电流触发真空电弧中CS的初始膨胀过程。在这种方法中,每个新的CS都可以以一定的概率在旧的CS周围的任何方向上点火,这与旧CS位置周围的磁场有关。通过这种方法,以CS均匀分布在环上的方式,对自由燃烧和AMF稳定的大电流触发真空电弧中CS的初始膨胀过程进行了数值模拟。利用商用软件ANSYS计算每个CS位置处的自生横向磁场,其中要考虑接触板中的电流分布2。仿真结果与相关实验结果吻合良好。仿真结果表明,在没有外部AMF的情况下CS的膨胀比在AMF下的CS更快,并且外部AMF对CS在阴极表面的分布有显着影响,例如,当存在外部AMF时,越来越多的CS出现在环内。此外,结果还表明,CS的膨胀环结构是不稳定的,并且AMF可以加速环的断裂。

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