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Magnetic priming of a relativistic magnetron.

机译:相对论磁控管的磁性启动。

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摘要

Experiments and simulations have been performed testing magnetic priming at the cathode and at the anode of a relativistic magnetron to study the effects on high power microwave generation. Magnetic priming consists of N/2 azimuthal magnetic perturbations applied to an N-cavity magnetron for rapid generation of N/2 of electron spokes for then-mode. Magnetic perturbations were imposed utilizing three high-permeability nickel-iron wires embedded beneath the emission region of the cathode, spaced 120 degrees apart. Magnetic priming was demonstrated to increase the percentage of pi-mode shots by up to 30% over the baseline case. In general, the shortest wire length cases (4 cm and 8 cm-long cathode wires and 10 cm-long anode wires) yielded the best pi mode performance. The start-oscillation time for the mode in the magnetically primed magnetron was reduced to as little as 57% of the unprimed case. In an unbalanced loading condition, mean peak power for pi-mode shots was found to be higher in the magnetically primed case by almost a factor of 2. Additionally, increases in mean microwave pulse width were also observed in the magnetically primed case when compared to the unprimed case (66 ns primed versus 50 ns unprimed) under unbalanced loading conditions. Under balanced loading conditions, measured power and pulse width in the magnetically primed cases were observed to be statistically the same as the unprimed baseline case, with the exception of the 4 cm cathode wire and 15 cm anode wire cases which were slightly lower. Additional experimental and simulation work was performed to study and correct vacuum side window breakdown occurring on the dielectric microwave windows used on the UM/L-3 relativistic magnetron. Simulations indicated that electrons emitted from the microwave apertures of the magnetron were striking the microwave windows in their original configuration, located 3 cm from the apertures. The microwave windows were redesigned and moved 33 cm from the apertures, resulting in the elimination of flashover and a threefold increase in measure microwave output power and pulse width.
机译:已经进行了实验和模拟,以测试相对论磁控管的阴极和阳极处的磁启动,以研究对高功率微波产生的影响。磁启动由施加到N腔磁控管的N / 2方位磁扰动组成,以快速生成N / 2电子辐条,用于模态。利用嵌入在阴极发射区下方,间隔120度的三根高磁导率镍铁丝施加磁扰动。事实证明,磁力灌注可以使pi模式拍摄的百分比比基准情况增加多达30%。通常,最短的线长情况(4厘米和8厘米长的阴极线和10厘米长的阳极线)产生最佳的pi模式性能。磁启动磁控管中该模式的启动振荡时间减少到无启动情况的57%。在不平衡负载条件下,发现在piprimed情况下pi-shot的平均峰值功率几乎提高了2倍。此外,与相比,在primed情况下,还观察到了平均微波脉冲宽度的增加。在不平衡的负载条件下,未启动的情况(启动后为66 ns,未启动后为50 ns)。在平衡负载条件下,观察到在磁力启动情况下测得的功率和脉冲宽度与未启动基线情况在统计学上是相同的,只是4 cm阴极线和15 cm阳极线情况略低。进行了额外的实验和模拟工作,以研究和纠正在UM / L-3相对论磁控管上使用的介质微波窗口上发生的真空侧窗口击穿。模拟表明,从磁控管的微波孔发出的电子以其原始结构撞击微波窗口,该微波窗口距孔的距离为3 cm。重新设计了微波窗口,并从孔口移开了33厘米,从而消除了闪络,并且测量的微波输出功率和脉冲宽度增加了三倍。

著录项

  • 作者

    Hoff, Brad Winston.;

  • 作者单位

    University of Michigan.;

  • 授予单位 University of Michigan.;
  • 学科 Engineering Electronics and Electrical.;Engineering Nuclear.
  • 学位 Ph.D.
  • 年度 2009
  • 页码 173 p.
  • 总页数 173
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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