Optical investigation of constricted vacuum arcs

M. Abplanalp, K. Menzel, T. Delachaux, R. Sutterlin, F. Kassubek
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引用次数: 1

Abstract

The optical investigation of arcs in transverse magnetic field (TMF) vacuum interrupters is difficult due to the strong motion of the constricted arc in the magnetic field. In order to determine a first estimate of temperature and pressure distribution in such arcs, a non-moving constricted arc is created in a dedicated test geometry with two pin electrodes. Dimensions and currents in this setup are very similar to the TMF case; the arc is mostly cylinder symmetric. The plasma temperature for a plane inside the cathode jet is deduced from spatially resolved optical emission spectroscopy: Using an in-house code the expected spectrum from an arc of given profile is computed taking into account known emission lines in the observation window and (self) absorption. With this the arc profile can be fitted to the experimental spectrum. We find typical peak temperatures around 25 kK, the pressure depends on the current (e.g. 7 bar for 30 kA peak). Furthermore, spatial profiles of temperature and pressure are given.
压缩真空弧的光学研究
由于压缩电弧在磁场中的强烈运动,给横向磁场真空灭弧的光学研究带来了困难。为了确定这种弧线中的温度和压力分布的初步估计,在专用的测试几何形状中使用两个引脚电极创建一个不移动的收缩弧线。这种情况下的尺寸和电流与TMF情况非常相似;圆弧基本上是圆柱对称的。从空间分辨的光学发射光谱中推导出阴极射流内平面的等离子体温度:使用内部代码计算给定剖面弧线的预期光谱,并考虑到观测窗口和(自)吸收中的已知发射线。这样就可以将弧廓线拟合到实验光谱中。我们发现典型的峰值温度约为25 kK,压力取决于电流(例如30 kA峰值为7 bar)。此外,还给出了温度和压力的空间分布。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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