Flux and magnetized plasma compression driven by Shiva Star

J. Degnan, D. Amdahl, M. Domonkos, C. Grabowski, E. Ruden, W. White, G. Wurden, T. Intrator, J. Sears, T. Weber, W. Waganaar, M. Frese, S. Frese, J. F. Camacho, S. Coffey, V. Makhin, N. Roderick, D. Gale, M. Kostora, A. Lerma, C. Roth, W. Sommars, G. Kiuttu, B. Bauer, S. Fuelling, A. Lynn, P. Turchi
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引用次数: 4

Abstract

The AFRL Shiva Star capacitor bank (1300 microfarads, up to 120 kilovolts) operated typically with 4 to 5 megajoules of electrically stored energy, with axial discharge currents of 10 to 15 megamps, and current rise times of approximately 10 microseconds, has been used to drive metal shell (solid liner) implosions in several geometries, including long cylindrical designs, which are suitable for compression of axial magnetic fields to multi-megagauss levels. Such imploding liners are also suitable for compressing magnetized plasmas to magneto-inertial fusion conditions. Magneto-Inertial Fusion (MIF) approaches take advantage of embedded magnetic field to improve plasma energy confinement by reducing thermal conduction relative to conventional inertial confinement fusion (ICF). MIF reduces required implosion speed and convergence ratio relative to ICF. AFRL, its contractors and collaborating institutions LANL, UNM, and UNR have developed one version of magnetized plasmas at pre-compression densities, temperatures, and magnetic fields that may be suitable for such compression. These are Field Reversed Configurations (FRCs). This effort reliably formed, translated, and captured FRCs in magnetic mirrors inside10 cm diameter, 30 cm long, mm thick metal shells or liners in preparation for subsequent compression by liner implosion; imploded a liner with an interior magnetic mirror field, obtaining evidence for compression of 1.36 T field to approximately 500 T; performed a full system experiment of FRC formation, translation, capture, and imploding liner compression operation; identified by comparison of 2D-MHD simulation and FRC capture experiments factors limiting the closed- field lifetime of FRCs to about half that required for good liner compression of FRCs to multi-keV, 1019 ion/cm3, high energy density plasma (HEDP) conditions; and designed and prepared hardware to increase that closed field FRC lifetime to the required amount. Those lifetime extension experiments have obtained imaging evidence of FRC rotation (which is a phenomenon that limits such closed field lifetimes), and of initial rotation control measures slowing and stopping such rotation. These and the results of subsequent closed field plasma lifetime and compression experiments and related simulations will be discussed.
湿婆星驱动的磁通量和磁化等离子体压缩
AFRL Shiva Star电容器组(1300微法拉,高达120千伏)通常以4至5兆焦耳的电能存储,轴向放电电流为10至15兆gamps,电流上升时间约为10微秒,已用于驱动多种几何形状的金属外壳(固体衬里)内爆,包括长圆柱形设计,适合将轴向磁场压缩到数兆aguss水平。这种内爆衬垫也适用于将磁化等离子体压缩到磁-惯性聚变条件。磁惯性聚变(MIF)方法利用嵌入磁场的优势,相对于传统的惯性约束聚变(ICF),通过减少热传导来改善等离子体能量约束。相对于ICF, MIF降低了所需的内爆速度和收敛比。AFRL及其承包商和合作机构LANL, UNM和UNR已经开发出一种适合这种压缩的预压缩密度,温度和磁场的磁化等离子体。这些都是场反转配置(FRCs)。这项工作在直径10厘米、长30厘米、厚1毫米的金属外壳或衬里内的磁镜中可靠地形成、转化和捕获FRCs,为随后的衬里内爆压缩做准备;内爆带有内部磁镜场的衬管,获得了1.36 T磁场压缩到约500 T的证据;进行了FRC形成、平移、捕获和内爆尾管压缩作业的完整系统实验;通过2D-MHD模拟和FRC捕获实验的比较,确定了限制FRC闭场寿命的因素,这些因素约为FRC在多kev、1019离子/cm3、高能量密度等离子体(HEDP)条件下良好的线性压缩所需的一半;并设计和准备硬件,以将封闭现场FRC寿命增加到所需的数量。这些延长寿命的实验已经获得了FRC旋转的成像证据(这是一种限制这种封闭油田寿命的现象),以及初始旋转控制措施减缓和停止这种旋转。这些结果以及随后的闭合场等离子体寿命和压缩实验以及相关模拟的结果将被讨论。
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